WorldWideScience

Sample records for survey classroom observations

  1. Observing Classroom Practice

    Science.gov (United States)

    Danielson, Charlotte

    2012-01-01

    Classroom observation is a crucial aspect of any system of teacher evaluation. No matter how skilled a teacher is in other aspects of teaching--such as careful planning, working well with colleagues, and communicating with parents--if classroom practice is deficient, that individual cannot be considered a good teacher. Classroom observations can…

  2. Classroom Observation Criteria and Techniques.

    Science.gov (United States)

    Peters, Richard O.

    Classroom observation is an integral part of teacher preparation. The observer must enter the classroom with a frame-of-reference: knowledge of the teacher's goals and objectives, awareness of the climate of the classroom, and knowledge of the discipline. Observation forms to objectively record classroom interaction, assess the learning climate,…

  3. THE VALUE OF CLASSROOM OBSERVATION

    Institute of Scientific and Technical Information of China (English)

    1998-01-01

    An analysis of the value of classroom observation for both the teacher being observed and the observer. 1. Introduction I have been a teacher for nearly two years. I did not like classroom observation until a week before. It hasbeen teaching practice on an advanced teacher training course that has made me change my mind. Now I want to be observed when I have difficulties or want to try something new. Here I shall discuss the value

  4. Trends in Classroom Observation Scores

    Science.gov (United States)

    Casabianca, Jodi M.; Lockwood, J. R.; McCaffrey, Daniel F.

    2015-01-01

    Observations and ratings of classroom teaching and interactions collected over time are susceptible to trends in both the quality of instruction and rater behavior. These trends have potential implications for inferences about teaching and for study design. We use scores on the Classroom Assessment Scoring System-Secondary (CLASS-S) protocol from…

  5. Guidance for Technology Decisions from Classroom Observation

    Science.gov (United States)

    Bielefeldt, Talbot

    2012-01-01

    Correlational analysis of two years of classroom observation indicates relationships between technology use and various classroom characteristics, including teacher roles and instructional strategies. Three observers used the ISTE Classroom Observation Tool (ICOT) to record 144 observations of classrooms participating in a variety of educational…

  6. Classroom Observation Techniques. IDEA Paper No. 4.

    Science.gov (United States)

    Acheson, Keith A.

    Techniques for observing the classroom behavior of teachers and students are examined. These techniques provide a framework for analyzing and understanding classroom interaction, for making decisions about what should be happening, and for changing instructional behavior when it is necessary. The observation methods allow collection, analysis, and…

  7. Classroom Observation of Potential Special Education Children.

    Science.gov (United States)

    Forness, Steven R.

    The present study is a portion of a larger study dealing with early identification of children with potential learning or behavioral difficulties. Specifically, the purpose of this phase of the project was (1) to refine classroom observation techniques and procedures and (2) to collect classroom observation data on children in regular classes who…

  8. A Critical Examination of Classroom Communication Observation Techniques.

    Science.gov (United States)

    Babich, Roger M.; Scafe, Marla

    More than 100 classroom communication observation instruments are surveyed and assessed from a communication-based perspective in this paper. In an overview, a schema designating three main types of approaches is established; they include behavioral descriptive, message functional, and cognitive/affective inferential observational categories.…

  9. Communication in the Classroom: Research and Observation. ERIC Report.

    Science.gov (United States)

    Boileau, Don M.

    1981-01-01

    Presents an annotated bibliography of ERIC resources on the following topics: teacher communication; research on classroom interaction; using systematic observations to improve teaching; different systems of classroom observations; and research on classroom observation techniques. (PD)

  10. Procedures for Classroom Observations: 1973-1974. Technical Report #19.

    Science.gov (United States)

    Miley, Alan

    This report describes classroom observation techniques used to record the behavior of educational specialists (teachers) and students in a kindergarten and a first grade classroom of the Kamehameha Early Education Program (KEEP). Classroom behavior was observed and recorded daily during the 1973-1974 school year. Each student was observed three…

  11. Corrective Feedback in L2 Latvian Classrooms: Teacher Perceptions versus the Observed Actualities of Practice

    Science.gov (United States)

    Dilans, Gatis

    2016-01-01

    This two-part study aims to investigate teacher perceptions about providing oral corrective feedback (CF) to minority students of Latvian as a second language and compare the perceptions to the actual provision of CF in L2 Latvian classrooms. The survey sample represents sixty-six L2 Latvian teachers while the classroom observations involved 13…

  12. Complex language encounters: Observations from linguistically diverse South African classrooms

    National Research Council Canada - National Science Library

    Rinelle Evans; Ailie Cleghorn

    2010-01-01

    .... Observations during teaching practice visits to linguistically and culturally diverse South African urban classrooms yielded several vignettes that illustrate the need for teachers to be provided...

  13. Rater Drift and Time Trends in Classroom Observations

    Science.gov (United States)

    Casabianca, Jodi M.; Lockwood, J. R.

    2013-01-01

    Classroom observation protocols, in which observers rate multiple dimensions of teaching according to established protocols (either live in the classroom, or post-hoc from lesson videos), are increasingly being used in both research and policy contexts. However, scores generated from these protocols have many sources of error. Day to day variation…

  14. Classroom Observation on Developing Students’Competence in SEIB

    Institute of Scientific and Technical Information of China (English)

    王蓓

    2012-01-01

      China’s entry to WTO and China’s 2008 Olympic Games have widely opened the door to the outside world. Tal⁃ents with business knowledge and excellent oral English are urgently needed. For students in English major, we give the course of Spoken English for International Business (SEIB) to improve their abilities in SEIB. The author aims to use the methods like classroom observation, interview, questionnaire survey to observe and compare two classes and two teachers to explore the rela⁃tions between students’competence development and teachers’with different levels and teaching practice, and to gain some enlightenment on students’competence developing in SEIB from the study.

  15. Emotional Bias in Classroom Observations: Within-Rater Positive Emotion Predicts Favorable Assessments of Classroom Quality

    Science.gov (United States)

    Floman, James L.; Hagelskamp, Carolin; Brackett, Marc A.; Rivers, Susan E.

    2017-01-01

    Classroom observations increasingly inform high-stakes decisions and research in education, including the allocation of school funding and the evaluation of school-based interventions. However, trends in rater scoring tendencies over time may undermine the reliability of classroom observations. Accordingly, the present investigations, grounded in…

  16. Classroom "Cupcake" Celebrations: Observations of Foods Offered and Consumed

    Science.gov (United States)

    Isoldi, Kathy K.; Dalton, Sharron; Rodriguez, Desiree P.; Nestle, Marion

    2012-01-01

    Objective: To describe food and beverage types offered and consumed during classroom celebrations at an elementary school in a low-income, urban community. In addition, to report student intake of fresh fruit provided alongside other party foods. Methods: Observations held during 4 classroom celebrations. Food and beverage items were measured and…

  17. The sign language skills classroom observation: a process for describing sign language proficiency in classroom settings.

    Science.gov (United States)

    Reeves, J B; Newell, W; Holcomb, B R; Stinson, M

    2000-10-01

    In collaboration with teachers and students at the National Technical Institute for the Deaf (NTID), the Sign Language Skills Classroom Observation (SLSCO) was designed to provide feedback to teachers on their sign language communication skills in the classroom. In the present article, the impetus and rationale for development of the SLSCO is discussed. Previous studies related to classroom signing and observation methodology are reviewed. The procedure for developing the SLSCO is then described. This procedure included (a) interviews with faculty and students at NTID, (b) identification of linguistic features of sign language important for conveying content to deaf students, (c) development of forms for recording observations of classroom signing, (d) analysis of use of the forms, (e) development of a protocol for conducting the SLSCO, and (f) piloting of the SLSCO in classrooms. The results of use of the SLSCO with NTID faculty during a trial year are summarized.

  18. Geodetic Survey Water Level Observations

    Data.gov (United States)

    National Oceanic and Atmospheric Administration, Department of Commerce — Over one million images of National Coast & Geodetic Survey (now NOAA's National Geodetic Survey/NGS) forms captured from microfiche. Tabular forms and charts...

  19. Developing and Validating a New Classroom Climate Observation Assessment Tool.

    Science.gov (United States)

    Leff, Stephen S; Thomas, Duane E; Shapiro, Edward S; Paskewich, Brooke; Wilson, Kim; Necowitz-Hoffman, Beth; Jawad, Abbas F

    2011-01-01

    The climate of school classrooms, shaped by a combination of teacher practices and peer processes, is an important determinant for children's psychosocial functioning and is a primary factor affecting bullying and victimization. Given that there are relatively few theoretically-grounded and validated assessment tools designed to measure the social climate of classrooms, our research team developed an observation tool through participatory action research (PAR). This article details how the assessment tool was designed and preliminarily validated in 18 third-, fourth-, and fifth-grade classrooms in a large urban public school district. The goals of this study are to illustrate the feasibility of a PAR paradigm in measurement development, ascertain the psychometric properties of the assessment tool, and determine associations with different indices of classroom levels of relational and physical aggression.

  20. Aspects on Learner-Biased Classroom Observational Techniques

    Science.gov (United States)

    Chen, Linhan

    2012-01-01

    This paper was designed to explore the means in the field of observing classroom teaching/learning from both a general, and an "English as a Foreign Language" (EFL), viewpoint. The aim was to browse the relevant literature, and lead to consider observation tools which might serve to research in EFL. This paper summarizes the reading by…

  1. Spatial Mapping as a Method for Observing Classroom Art Instruction.

    Science.gov (United States)

    Susi, Frank D.

    1985-01-01

    Spatial mapping is a category system for directly observing instruction in art classrooms. A rationale for studying the spatial dimensions of teaching is presented, how to train observers is explained, procedures involved in a mapping episode are described, methods for analyzing data are suggested, and examples of instruments are presented.…

  2. Teacher's Approaches in Teaching Literature: Observations of ESL Classroom

    Science.gov (United States)

    Mustakim, Siti Salina; Mustapha, Ramlee; Lebar, Othman

    2014-01-01

    This study aimed to identify the approaches employed by teachers in teaching Contemporary Children's Literature Program to upper primary school. Using classroom observations and interview as research instruments, this paper evaluates the approaches of five ESL teachers teaching Year 5 students and examines the various challenges faced by them in…

  3. Teaching the Teachers: Peer Observations in Elementary Classrooms

    Science.gov (United States)

    Schenk, Matthew D.

    2016-01-01

    The United States is facing an unprecedented teacher shortage. With many studies estimating that 17-33% of teachers leave the profession within their first five years of starting a career, something needs to change to keep new teachers in the classroom. This study evaluates the effectiveness of peer observation as a learning tool to supplement the…

  4. Learning about Classroom Management through Guided Observation and Analysis. R&D Report No. 6026.

    Science.gov (United States)

    Sanford, Julie P.; Emmer, Edmund T.

    A development and field-testing effort explored ways of helping preservice teachers learn classroom management knowledge and skills during field-based preservice courses. An observation guide, "Learning the Classroom Environment, An Observer's Guide to Classroom Management" (Sanford & Emmer, 1985), has four general areas: the classroom setting;…

  5. Classroom Assessment Practices: A Survey of Botswana Primary and Secondary School Teachers

    Science.gov (United States)

    Koloi-Keaikitse, Setlhomo

    2012-01-01

    The Classroom Assessment Practices and Skills (CAPS) questionnaire was administered to a sample of 691 primary and secondary school teachers in Botswana, Southern Africa to survey their thoughts about classroom assessment and identify classroom assessment practices teachers perceive to be skilled and those that they used most. The study examined…

  6. Classroom Technology in Business Schools: A Survey of Installations and Attitudes toward Teaching and Learning

    Science.gov (United States)

    Parker, Betty; Burnie, David

    2009-01-01

    A survey of administrators and faculty of AACSB-accredited business schools provided insights into current classroom technology infrastructure, attitudes towards technology and learning, and the use of web course tools in business school classrooms. The results of the survey provided four major findings: business schools are utilizing high levels…

  7. Classroom Technology in Business Schools: A Survey of Installations and Attitudes toward Teaching and Learning

    Science.gov (United States)

    Parker, Betty; Burnie, David

    2009-01-01

    A survey of administrators and faculty of AACSB-accredited business schools provided insights into current classroom technology infrastructure, attitudes towards technology and learning, and the use of web course tools in business school classrooms. The results of the survey provided four major findings: business schools are utilizing high levels…

  8. Uncovering Multivariate Structure in Classroom Observations in the Presence of Rater Errors

    Science.gov (United States)

    McCaffrey, Daniel F.; Yuan, Kun; Savitsky, Terrance D.; Lockwood, J. R.; Edelen, Maria O.

    2015-01-01

    We examine the factor structure of scores from the CLASS-S protocol obtained from observations of middle school classroom teaching. Factor analysis has been used to support both interpretations of scores from classroom observation protocols, like CLASS-S, and the theories about teaching that underlie them. However, classroom observations contain…

  9. Observation of Classroom Performance Using Therapy Balls as a Substitute for Chairs in Elementary School Children

    Science.gov (United States)

    Burgoyne, Molly E.; Ketcham, Caroline J.

    2015-01-01

    Many classrooms are beginning to substitute standard chairs with therapy balls, which help to improve students' focus and classroom performance, according to teacher and student reports. Researchers conducted an observational study in a classroom at a local elementary school that implemented therapy balls. For each hour-long observation, three…

  10. All Sky Survey Mission Observing Scenario Strategy

    CERN Document Server

    Spangelo, Sara C; Unwin, Stephen C; Bock, Jamie J

    2014-01-01

    This paper develops a general observing strategy for missions performing all-sky surveys, where a single spacecraft maps the celestial sphere subject to realistic constraints. The strategy is flexible such that targeted observations and variable coverage requirements can be achieved. This paper focuses on missions operating in Low Earth Orbit, where the thermal and stray-light constraints due to the Sun, Earth, and Moon result in interacting and dynamic constraints. The approach is applicable to broader mission classes, such as those that operate in different orbits or that survey the Earth. First, the instrument and spacecraft configuration is optimized to enable visibility of the targeted observations throughout the year. Second, a constraint-based high-level strategy is presented for scheduling throughout the year subject to a simplified subset of the constraints. Third, a heuristic-based scheduling algorithm is developed to assign the all-sky observations over short planning horizons. The constraint-based...

  11. The Classroom Learning Activities Checklist: Validity Evidence of an Observation Tool in Preschool

    Science.gov (United States)

    Candee, Allyson Joelle

    2016-01-01

    In this paper, the Classroom Learning Activities Checklist (CLAC) is proposed as a classroom observation measure that effectively captures the classroom environments and strategies that support self-regulation via task-oriented learning in young students. The CLAC's dimensionality, reliability, and concurrent and predictive validity evidence are…

  12. The ISI Classroom Observation System: Examining the Literacy Instruction Provided to Individual Students

    Science.gov (United States)

    Connor, Carol McDonald; Morrison, Frederick J.; Fishman, Barry J.; Ponitz, Claire Cameron; Glasney, Stephanie; Underwood, Phyllis S.; Piasta, Shayne B.; Crowe, Elizabeth Coyne; Schatschneider, Christopher

    2009-01-01

    The Individualizing Student Instruction (ISI) classroom observation and coding system is designed to provide a detailed picture of the classroom environment at the level of the individual student. Using a multidimensional conceptualization of the classroom environment, foundational elements (teacher warmth and responsiveness to students, classroom…

  13. Refining MARGINS Mini-Lessons Using Classroom Observations

    Science.gov (United States)

    Iverson, E. A.; Manduca, C. A.; McDaris, J. R.; Lee, S.

    2009-12-01

    One of the challenges that we face in developing teaching materials or activities from research findings is testing the materials to determine that they work as intended. Traditionally faculty develop material for their own class, notice what worked and didn’t, and improve them the next year. However, as we move to a community process of creating and sharing teaching materials, a community-based process for testing materials is appropriate. The MARGINS project has piloted such a process for testing teaching materials and activities developed as part of its mini-lesson project (http://serc.carleton.edu/margins/index.html). Building on prior work developing mechanisms for community review of teaching resources (e.g. Kastens, 2002; Hancock and Manduca, 2005; Mayhew and Hall, 2007), the MARGINS evaluation team developed a structured classroom observation protocol. The goals of field testing are to a) gather structured, consistent feedback for the lesson authors based on classroom use; b) guide reviewers of these lessons to reflect on research-based educational practice as a framework for their comments; c) collect information on the data and observations that the reviewer used to underpin their review; d) determine which mini-lessons are ready to be made widely available on the website. The protocol guides faculty observations on why they used the activity, the effectiveness of the activity in their classroom, the success of the activity in leading to the desired learning, and what other faculty need to successfully use the activity. Available online (http://serc.carleton.edu/margins/protocol.html), the protocol can be downloaded and completed during instruction with the activity. In order to encourage review of mini-lessons using the protocol, a workshop focused on review and revision of activities was held in May 2009. In preparation for the workshop, 13 of the 28 participants chose to field test a mini-lesson prior to the workshop and reported that they found this

  14. The Classroom Observation Protocol for Undergraduate STEM (COPUS): a new instrument to characterize university STEM classroom practices.

    Science.gov (United States)

    Smith, Michelle K; Jones, Francis H M; Gilbert, Sarah L; Wieman, Carl E

    2013-01-01

    Instructors and the teaching practices they employ play a critical role in improving student learning in college science, technology, engineering, and mathematics (STEM) courses. Consequently, there is increasing interest in collecting information on the range and frequency of teaching practices at department-wide and institution-wide scales. To help facilitate this process, we present a new classroom observation protocol known as the Classroom Observation Protocol for Undergraduate STEM or COPUS. This protocol allows STEM faculty, after a short 1.5-hour training period, to reliably characterize how faculty and students are spending their time in the classroom. We present the protocol, discuss how it differs from existing classroom observation protocols, and describe the process by which it was developed and validated. We also discuss how the observation data can be used to guide individual and institutional change.

  15. Classroom observation data and instruction in primary mathematics education: improving design and rigour

    Science.gov (United States)

    Thompson, Carla J.; Davis, Sandra B.

    2014-06-01

    The use of formal observation in primary mathematics classrooms is supported in the literature as a viable method of determining effective teaching strategies and appropriate tasks for inclusion in the early years of mathematics learning. The twofold aim of this study was to (a) investigate predictive relationships between primary mathematics classroom observational data and student achievement data, and (b) to examine the impact of providing periodic classroom observational data feedback to teachers using a Relational-Feedback-Intervention (RFI) Database Model. This observational research effort focused on an empirical examination of student engagement levels in time spent on specific learning activities observed in primary mathematics classrooms as predictors of student competency outcomes in mathematics. Data were collected from more than 2,000 primary classroom observations in 17 primary schools during 2009-2011 and from standardised end-of-year tests for mathematics achievement. Results revealed predictive relationships among several types of teaching and learning tasks with student achievement. Specifically, the use of mathematics concepts, technology and hands-on materials in primary mathematics classrooms was found to produce substantive predictors of increased student mathematics achievement. Additional findings supported the use of periodic classroom observation data reporting as a positive influence on teachers' decisions in determining instructional tasks for inclusion in primary mathematics classrooms. Study results indicate classroom observational research involving a RFI Database Model is a productive tool for improving teaching and learning in primary mathematics classrooms.

  16. Classroom Writing Environments and Children's Early Writing Skills: An Observational Study in Head Start Classrooms

    Science.gov (United States)

    Zhang, Chenyi; Hur, Jinhee; Diamond, Karen E.; Powell, Douglas

    2015-01-01

    This study examined the classroom writing environment in 31 Head Start classrooms, and explored the relations between the writing environment, children's (N = 262) name-writing, and children's letter knowledge using pathway analysis. Our analyses showed that Head Start classrooms provided opportunities (i.e., writing materials and teachers'…

  17. Classroom Writing Environments and Children's Early Writing Skills: An Observational Study in Head Start Classrooms

    Science.gov (United States)

    Zhang, Chenyi; Hur, Jinhee; Diamond, Karen E.; Powell, Douglas

    2015-01-01

    This study examined the classroom writing environment in 31 Head Start classrooms, and explored the relations between the writing environment, children's (N = 262) name-writing, and children's letter knowledge using pathway analysis. Our analyses showed that Head Start classrooms provided opportunities (i.e., writing materials and teachers'…

  18. Standardized Observational Assessment of Attention Deficit Hyperactivity Disorder Combined and Predominantly Inattentive Subtypes. II. Classroom Observations.

    Science.gov (United States)

    McConaughy, Stephanie H; Ivanova, Masha Y; Antshel, Kevin; Eiraldi, Ricardo B; Dumenci, Levent

    2009-07-01

    Trained classroom observers used the Direct Observation Form (DOF; McConaughy & Achenbach, 2009) to rate observations of 163 6- to 11-year-old children in their school classrooms. Participants were assigned to four groups based on a parent diagnostic interview and parent and teacher rating scales: Attention Deficit Hyperactivity Disorder (ADHD)-Combined type (n = 64); ADHD-Inattentive type (n = 22); clinically referred without ADHD (n = 51); and nonreferred control children (n = 26). The ADHD-Combined group scored significantly higher than the referred without ADHD group and controls on the DOF Intrusive and Oppositional syndromes, Attention Deficit Hyperactivity Problems scale, Hyperactivity-Impulsivity subscale, and Total Problems; and significantly lower on the DOF On-Task score. The ADHD-Inattentive group scored significantly higher than controls on the DOF Sluggish Cognitive Tempo and Attention Problems syndromes, Inattention subscale, and Total Problems; and significantly lower on the DOF On-Task score. Implications are discussed regarding the discriminative validity of standardized classroom observations for identifying children with ADHD and differentiating between the two ADHD subtypes.

  19. Once is not enough : Establishing reliability criteria for teacher evaluation based on classroom observations

    NARCIS (Netherlands)

    van der Lans, Rikkert; van de Grift, Wim; van Veen, Klaas

    2016-01-01

    Classroom observation is the most implemented method to evaluate teaching. To ensure reliability, researchers often train observers extensively. However, schools have limited resources to train observers and often lesson observation is performed by limitedly trained or untrained colleagues. In this

  20. The VISTA Deep Extragalactic Observations (VIDEO) Survey

    CERN Document Server

    Jarvis, Matt J; Bruce, V A; Geach, J E; McAlpine, K; McLure, R J; Gonzalez-Solares, E; Irwin, M; Lewis, J; Yoldas, A Kupcu; Andreon, S; Cross, N J G; Emerson, J P; Dalton, G; Dunlop, J S; Hodgkin, S T; Fevre, O Le; Karouzos, M; Meisenheimer, K; Oliver, S; Rawlings, S; Simpson, C; Smail, I; Smith, D J B; Sullivan, M; Sutherland, W; White, S V; Zwart, J T L

    2012-01-01

    In this paper we describe the first data release of the the Visible and Infrared Survey Telescope for Astronomy (VISTA) Deep Extragalactic Observations (VIDEO) survey. VIDEO is a ~12degree^2 survey in the near-infrared Z,Y,J,H and K_s bands, specifically designed to enable the evolution of galaxies and large structures to be traced as a function of both epoch and environment from the present day out to z=4, and active galactic nuclei (AGN) and the most massive galaxies up to and into the epoch of reionization. With its depth and area, VIDEO will be able to fully explore the period in the Universe where AGN and starburst activity were at their peak and the first galaxy clusters were beginning to virialize. VIDEO therefore offers a unique data set with which to investigate the interplay between AGN, starbursts and environment, and the role of feedback at a time when it was potentially most crucial. We provide data over the VIDEO-XMM3 tile, which also covers the Canada-France-Hawaii-Telescope Legacy Survey Deep-...

  1. Live versus Video Observations: Comparing the Reliability and Validity of Two Methods of Assessing Classroom Quality

    Science.gov (United States)

    Curby, Timothy W.; Johnson, Price; Mashburn, Andrew J.; Carlis, Lydia

    2016-01-01

    When conducting classroom observations, researchers are often confronted with the decision of whether to conduct observations live or by using pre-recorded video. The present study focuses on comparing and contrasting observations of live and video administrations of the Classroom Assessment Scoring System-PreK (CLASS-PreK). Associations between…

  2. Teachers' Characteristics and Science Teachers' Classroom Behaviour: Evidence from Science Classroom Surveys

    Science.gov (United States)

    Ajaja, Patrick O.; Eravwoke, Urhievwejire Ochuko

    2013-01-01

    The major purpose of this study was to find out if there is any influence of teachers' characteristics on science teacher's classroom behaviours and determine the kind of relationship between teachers' characteristics and classroom behaviours. To guide this study, five research questions and hypotheses were raised, stated, answered, and tested at…

  3. Improving Method-in-Use through Classroom Observation

    Science.gov (United States)

    Nunn, Roger

    2011-01-01

    Method-in-use (Nunn, Describing classroom interaction in intercultural curricular research and development, University of Reading, 1996, International Review of Applied Linguistics in Language Teaching 37: 23-42, 1999) is a description of the method actually being enacted through classroom interaction in a particular context. The description is…

  4. Evaluating the Validity of Classroom Observations in the Head Start Designation Renewal System

    Science.gov (United States)

    Mashburn, Andrew J.

    2017-01-01

    Classroom observations are increasingly common in education policies as a means to assess the quality of teachers and/or education programs for purposes of making high-stakes decisions. This article considers one policy, the Head Start Designation Renewal System (DRS), which involves classroom observations to assess the quality of Head Start…

  5. Mirrors for the Classroom: A Guide to Observation Techniques for Teachers and Supervisors.

    Science.gov (United States)

    Mitsakos, Charles L.

    This guide is designed to present a variety of techniques that can be used in conducting classroom observations. Observation techniques are clustered under four major teaching/learning variables: time on task, teacher talk, classroom interaction, and organization and management. Techniques are presented with an overview that details the rationale…

  6. Classroom Observation Data: Is It Valid? Is It Generalizable? A Compendium of Methodological Papers.

    Science.gov (United States)

    Borich, Gary; And Others

    The issues discussed in these four papers concern the validity and generalizability of classroom observation instruments. These issues have been studied and are reported here in an attempt to better define the limits to which classroom observation instruments can be used in researching relationships between teacher behavior and student outcome.…

  7. Bringing Real-time Astronomical Observations into the Classroom

    Science.gov (United States)

    Cominsky, L.

    2006-12-01

    The Sonoma State University Education and Public Outreach group (SSU E/PO) coordinates the Global Telescope Network (GTN) - an informal association of scientists, students, individuals and observatories interested in supporting NASA's Gamma-ray Large Area Space Telescope (GLAST) and Swift missions, as well as the joint ESA/NASA XMM-Newton mission. Partners and associates in the GTN obtain and reduce ground based observations for objects related to the primary science goals for these missions and work together with NASA mission scientists to conduct multi-wavelength studies of exotic objects such as monstrous black holes, and highly-magnetized neutron stars and white dwarfs. The Global Telescope Network provides hands-on classroom activities and engaging instructional materials for a range of levels and interests, including Cookie Cutter Photometry and Jelly Bean Spectroscopy. We also provide mentoring in research practices, telescope use, data analysis and other educational resources. Examples of ongoing research projects will be presented, and the educational resources available through the GTN will be discussed.

  8. Practice teaching: An inquiry into the experiences in developing an evaluation tool used in classroom observations

    Directory of Open Access Journals (Sweden)

    Wen-Lin Wang

    2016-01-01

    Full Text Available Proper preparation prior to practice teachers’ actual internship is deemed as an important part of the teacher development program. This presentation depicts the summary and findings of a semester-long action research study with 19 practice teachers (PT undertaken in the fall semester of 2013. After finishing all their required credits, PTs needed to prepare themselves for their upcoming internship. In order to help make their internship fruitful and be able to learn as much as possible from their teacher mentor, an internship preparation course designed as an action research was created to support PTs in being able to determine specific classroom observation skills. Within the course, PTs were separated into 4 groups and tasked with organizing all the previous theories learned from other courses in order to determine the key features of a good classroom teacher. Afterwards, the researchers oriented the PTs with the problem-based learning (PBL approach in creating a list of key features of a good classroom teacher. After a month of preparation, PTs were then assigned to undergo two months of classroom observations in a nearby elementary school. In addition, the PTs needed to do two practice teaching sessions before the end of the observation period. During the classroom observations and practice teaching, the PTs used their list of key features of a good classroom teacher to evaluate each other. Pre-post conferences were accomplished before and after each practice teaching session. Researcher observations, interview, and PTs’ reflection logs were later collected and analyzed. Results indicate that PTs claimed that they are able to learn more within a PBL approach in developing an evaluation tool used in classroom observation as compared to the typical classroom discussion type setup. In sum, the process of classroom lectures presented in tandem with actual classroom observations and practice teaching has led to the enrichment of their

  9. Observations of Effective Teacher-Student Interactions in Secondary School Classrooms: Predicting Student Achievement with the Classroom Assessment Scoring System--Secondary

    Science.gov (United States)

    Allen, Joseph; Gregory, Anne; Mikami, Amori; Lun, Janetta; Hamre, Bridget; Pianta, Robert

    2013-01-01

    Multilevel modeling techniques were used with a sample of 643 students enrolled in 37 secondary school classrooms to predict future student achievement (controlling for baseline achievement) from observed teacher interactions with students in the classroom, coded using the Classroom Assessment Scoring System--Secondary. After accounting for prior…

  10. Executive control goes to school: Implications of preschool executive performance for observed elementary classroom learning engagement.

    Science.gov (United States)

    Nelson, Timothy D; Nelson, Jennifer Mize; James, Tiffany D; Clark, Caron A C; Kidwell, Katherine M; Espy, Kimberly Andrews

    2017-05-01

    The transition to elementary school is accompanied by increasing demands for children to regulate their attention and behavior within the classroom setting. Executive control (EC) may be critical for meeting these demands; however, few studies have rigorously examined the association between EC and observed classroom behavior. This study examined EC in preschool (age 5 years 3 months) as a predictor of classroom learning engagement behaviors in first grade, using a battery of performance-based EC tasks and live classroom observations in a longitudinal sample of 313 children. Multilevel modeling results indicated that stronger EC predicted more focused engagement and fewer task management and competing responses, controlling for socioeconomic status, child sex, and age at observations. Results suggest that early EC may support subsequent classroom engagement behaviors that are critical for successful transition to elementary school and long-term learning trajectories. (PsycINFO Database Record (c) 2017 APA, all rights reserved).

  11. Concurrent Validity of the Classroom Strategies Scale for Elementary School--Observer Form

    Science.gov (United States)

    Reddy, Linda A.; Fabiano, Gregory A.; Dudek, Christopher M.

    2013-01-01

    The present study is an initial investigation of the concurrent validity of a new assessment, the Classroom Strategies Scale (CSS version 2.0) for Elementary School--Observer Form. The CSS assesses teachers' use of instructional and behavioral management strategies. In the present study, the CSS is compared to the Classroom Assessment Scoring…

  12. The Use of Classroom Observation Techniques in the Evaluation of Educational Programs. TM Report 49.

    Science.gov (United States)

    Brown, Bob Burton; Webb, Jeaninne N.

    Systematic observations of classroom behavior of both teachers and pupils are effective measures of process in education. Until a few years ago, the classroom process--what actually does and does not happen as a result of instituting a new program--went unmeasured for want of tools and techniques to do that job. In this article, examples of…

  13. Comparing Vignette Instruction and Assessment Tasks to Classroom Observations and Reflections

    Science.gov (United States)

    Jeffries, Carolyn; Maeder, Dale W.

    2011-01-01

    The growing body of research on the use of vignettes in teacher education courses suggests that vignette-based instruction and assessment tasks may represent a viable alternative to traditional forms of scaffolded instruction and reflective essays following classroom observations, thereby creating a bridge between college and K-12 classrooms for…

  14. Initiating round robins in the L2 classroom - preliminary observations

    DEFF Research Database (Denmark)

    Mortensen, Kristian; Hazel, Spencer

    2011-01-01

    position in which round robins are initiated and how this is talked and embodied into being by the participants as well as the design of the turn that initiates the round robin activity. Relevant to the initiation and further development of the round robin are the physical arrangement of the classroom......Complementing recent interactional research on the contingent operation of online task accomplishment, this paper deals with a specific way of organizing and managing tasks in plenary L2 classrooms – namely the round robin. This may seem like a “traditional” and rigid form of classroom organization...... that reduces students’ contributions to responses to the teacher’s elicitations. This paper shows that although the round robin puts certain interactional features out of play, it is nonetheless done in and through participants’ mutual orientation to the ongoing activity. The paper describes the sequential...

  15. Clowning and improvisation in the ESL classroom : observations and suggestions

    OpenAIRE

    Sigríður Friðriksdóttir 1976

    2012-01-01

    This thesis examines how clowning and improvisation can help students in the ESL classroom. Clowning and improvisation was taught in a 6th grade ESL classroom and its effectiveness discussed. This thesis discusses the basics of clowning and why it is helpful when helping students feel at ease with speaking English. I also describe how it can be used and suggest drama-related games that are helpful. The conclusion is that drama-related games help students have fun while learning a new langu...

  16. An Observational Study of Social Behavior in Microcomputer Classrooms.

    Science.gov (United States)

    Feldmann, Shirley C.; And Others

    1991-01-01

    This study examined the effects of five variables--student grouping at the computer, keyboarding status, academic discipline, student gender, and gender of partner--on student social behavior, both verbal and affective, in microcomputer classrooms in a public business high school. The effect of these variables on teacher behavior was also…

  17. Student Observations: Introducing iPads into University Classrooms

    Science.gov (United States)

    Wardley, Leslie J.; Mang, Colin F.

    2016-01-01

    This paper explores the growing trend of using mobile technology in university classrooms, exploring the use of tablets in particular, to identify learning benefits faced by students. Students, acting on their efficacy beliefs, make decisions regarding technology's influence in improving their education. We construct a theoretical model in which…

  18. Mathematical Observations: The Genesis of Mathematical Discovery in the Classroom

    Science.gov (United States)

    Beaugris, Louis M.

    2013-01-01

    In his "Proofs and Refutations," Lakatos identifies the "Primitive Conjecture" as the first stage in the pattern of mathematical discovery. In this article, I am interested in ways of reaching the "Primitive Conjecture" stage in an undergraduate classroom. I adapted Realistic Mathematics Education methods in an…

  19. A survey of acoustic conditions in semi-open plan classrooms in the United Kingdom.

    Science.gov (United States)

    Greenland, Emma E; Shield, Bridget M

    2011-09-01

    This paper reports the results of a large scale, detailed acoustic survey of 42 open plan classrooms of varying design in the UK each of which contained between 2 and 14 teaching areas or classbases. The objective survey procedure, which was designed specifically for use in open plan classrooms, is described. The acoustic measurements relating to speech intelligibility within a classbase, including ambient noise level, intrusive noise level, speech to noise ratio, speech transmission index, and reverberation time, are presented. The effects on speech intelligibility of critical physical design variables, such as the number of classbases within an open plan unit and the selection of acoustic finishes for control of reverberation, are examined. This analysis enables limitations of open plan classrooms to be discussed and acoustic design guidelines to be developed to ensure good listening conditions. The types of teaching activity to provide adequate acoustic conditions, plus the speech intelligibility requirements of younger children, are also discussed.

  20. Research for the Classroom: Analyzing Classroom Literacy Events--What Observing Classroom Conversations about Popular Culture Can Reveal about Reading

    Science.gov (United States)

    Garland, Kathy

    2012-01-01

    Ms. Mayer, a recently retired English language arts teacher, frequently used strategies described in John Golden's book "Reading in the Dark: Using Film as a Tool in the English Classroom." In this book, Golden suggests that ELA teachers "reverse the order: use a film clip to practice the reading and analytical skills that we want our students to…

  1. The 21st Century Physics Classroom: What Students, Teachers, and Classroom Observers Report

    Science.gov (United States)

    Sunal, Dennis W.; Dantzler, John A.; Sunal, Cynthia Szymanski; Turner, Donna P.; Harrell, James W.; Simon, Marsha; Aggarwal, Mohan D.

    2016-01-01

    Before we can effectively apply specific interventions through professional development, it is important to determine what is occurring in our high school physics classrooms. This study investigated common professional practices in physics teaching among a representative sample group of schools and teachers from a diverse, geographically large…

  2. Live Video Classroom Observation: An Effective Approach to Reducing Reactivity in Collecting Observational Information for Teacher Professional Development

    Science.gov (United States)

    Liang, Jiwen

    2015-01-01

    This paper examines the significance of live video classroom observations of teaching practice to reduce reactivity (the observer effect) so as to obtain more credible observational information for teacher professional development in a secondary school in the largest city in southern China. Although much has been discussed regarding the use of…

  3. Live Video Classroom Observation: An Effective Approach to Reducing Reactivity in Collecting Observational Information for Teacher Professional Development

    Science.gov (United States)

    Liang, Jiwen

    2015-01-01

    This paper examines the significance of live video classroom observations of teaching practice to reduce reactivity (the observer effect) so as to obtain more credible observational information for teacher professional development in a secondary school in the largest city in southern China. Although much has been discussed regarding the use of…

  4. The ESSENCE Supernova Survey: Survey Optimization, Observations, and Supernova Photometry

    Energy Technology Data Exchange (ETDEWEB)

    Miknaitis, Gajus; Pignata, G.; Rest, A.; Wood-Vasey, W.M.; Blondin, S.; Challis, P.; Smith, R.C.; Stubbs, C.W.; Suntzeff, N.B.; Foley, R.J.; Matheson, T.; Tonry, J.L.; Aguilera, C.; Blackman, J.W.; Becker, A.C.; Clocchiatti, A.; Covarrubias, R.; Davis, T.M.; Filippenko, A.V.; Garg, A.; Garnavich, P.M.; /Fermilab /Chile U., Catolica /Cerro-Tololo

    2007-01-08

    We describe the implementation and optimization of the ESSENCE supernova survey, which we have undertaken to measure the equation of state parameter of the dark energy. We present a method for optimizing the survey exposure times and cadence to maximize our sensitivity to the dark energy equation of state parameter w = P/{rho}c{sup 2} for a given fixed amount of telescope time. For our survey on the CTIO 4m telescope, measuring the luminosity distances and redshifts for supernovae at modest redshifts (z {approx} 0.5 {+-} 0.2) is optimal for determining w. We describe the data analysis pipeline based on using reliable and robust image subtraction to find supernovae automatically and in near real-time. Since making cosmological inferences with supernovae relies crucially on accurate measurement of their brightnesses, we describe our efforts to establish a thorough calibration of the CTIO 4m natural photometric system. In its first four years, ESSENCE has discovered and spectroscopically confirmed 102 type Ia SNe, at redshifts from 0.10 to 0.78, identified through an impartial, effective methodology for spectroscopic classification and redshift determination. We present the resulting light curves for the all type Ia supernovae found by ESSENCE and used in our measurement of w, presented in Wood-Vasey et al. (2007).

  5. How Junior High School English Teachers in Bengkulu City Utilise Published Textbooks in the Classroom: A Classroom Observation Study

    Directory of Open Access Journals (Sweden)

    Safnil Safnil

    2003-01-01

    Full Text Available The purpose of the study was to find out: (1 how the junior high school English teachers in Bengkulu city exploited the commercially published textbooks for classroom use; (2 if there was a difference in the way the experienced and the inexperienced English language teachers exploited the commercially published textbooks in the classroom; and (3 whether the teachers adapted textbooks or produced their own materials for classroom use. Twelve English teachers (6 experienced and 6 inexperienced teachers from four different junior high schools or SMPs (2 favourite and 2 non-favourite in Bengkulu city were the participants in this study. Data were obtained through a questionnaire, classroom observations, and sample lesson plans. The results of the study revealed that: first, the junior high school English language teachers (ET and IT; (1 used the commercially prescribed textbooks to a large extent; (2 there was not much difference between the way experienced teachers and inexperienced teachers exploited the textbooks; (3 both groups of teachers adapted the textbooks or produced their own teaching materials.

  6. Talking about Chemistry Classroom Observation Class%刍议化学课堂观察课

    Institute of Scientific and Technical Information of China (English)

    吴晓红; 张建琴

    2012-01-01

    Classroom observation by observing the status of the classroom, to record, analyze and research, in order to improve teachers' teaching to enhance students' learning. The principle of classroom observation, classroom observation of the implementation of steps to do a preliminary study. Ninth-grade chemistry chemical equations simple calculation of this lesson as an example, analyze and discuss of a real classroom observation.%课堂观察是通过观察对课堂的运行状况进行记录、分析和研究,以此改善教师的教学,促进学生的学习。本文从课堂观察的原则、课堂观察的实施步骤等方面做了初步探讨。以九年级化学"化学方程式的简单计算"这节课为例进行了真实的课堂观察与分析讨论。

  7. Commentary on two classroom observation systems: moving toward a shared understanding of effective teaching.

    Science.gov (United States)

    Connor, Carol McDonald

    2013-12-01

    In this commentary, I make five points: that designing observation systems that actually predict students' outcomes is challenging; second that systems that capture the complex and dynamic nature of the classroom learning environment are more likely to be able to meet this challenge; three, that observation tools are most useful when developed to serve a particular purpose and are put to that purpose; four that technology can help; and five, there are policy implications for valid and reliable classroom observation tools. The two observation systems presented in this special issue represent an important step forward and a move toward policy that promises to make a true difference in what is defined as high quality and effective teaching, what it looks like in the classroom, and how these practices can be more widely disseminated so that all children, including those attending under-resourced schools, can experience effective instruction, academic success and the lifelong accomplishment that follows.

  8. THE ROLE OF AND APPROACHES TOENGLISH CLASSROOM OBSERVATION

    Institute of Scientific and Technical Information of China (English)

    XiaZhanghong

    2004-01-01

    English teaching observation, which has long been a common practice in different levels of schools,is beneficial to both observers (visiting teachers) and the instructor (the visited teacher). This paper covers the benefits and importance to both parties, especially those to the observers. Carrying out observation properly and effectively, we must master some techniques, ways and steps. There are two broad approaches to class visiting, qualitative and quantitative. Among qualitative approaches the “limited or selected ethnography or recording” seems tobe more practical; among qualitative ones, the SCORE method is focused on in this paper. Of the three observation ways, peer observation is described in detail: regarding observation, detailed descriptions are given of the three stages-preobservation, observation and postobservation. Some points to be paid attention to also are discussed in this paper.

  9. Culture Orientation and Sociometry of the Classroom: A Possible Relationship.

    Science.gov (United States)

    Epp, Juanita Ross; Hajnal, Vivian

    Findings of a study that examined the relationship between classroom orientation and sociometric patterns within the classroom are presented in this paper. Methodology involved observation of 12 classrooms in Ontario and administration of two survey instruments to 20 fourth-year students. Classroom orientations were categorized as cooperative,…

  10. All Together Now: Measuring Staff Cohesion in Special Education Classrooms

    Science.gov (United States)

    Kratz, Hilary E.; Locke, Jill; Piotrowski, Zinnia; Ouellette, Rachel R.; Xie, Ming; Stahmer, Aubyn C.; Mandell, David S.

    2015-01-01

    This study sought to validate a new measure, the Classroom Cohesion Survey (CCS), designed to examine the relationship between teachers and classroom assistants in autism support classrooms. Teachers, classroom assistants, and external observers showed good inter-rater agreement on the CCS and good internal consistency for all scales. Simple…

  11. Observational Research in a Marketing Classroom: A Guidebook

    OpenAIRE

    Winterton, Kristen

    2012-01-01

    Qualitative research plays an integral part in marketing research (Denzin and Lincoln, 1998). In fact, a search of the website for the American Marketing Association for the term “qualitative research” reveals literally hundreds of documents (white papers, case studies, etc) discussing methods of conducting observational research, examples of observational research studies, and the importance of observational research in marketing. Interestingly, though qualitative methods are used frequently...

  12. Observations of Children with Disabilities in Four Elementary Music Classrooms

    Science.gov (United States)

    Draper, Ellary A.

    2017-01-01

    Much of what we know about music classes comes from observing students without disabilities; there is little empirical research that informs music education practices for students with disabilities in inclusive music settings. The purpose of this study was to systematically observe and describe opportunities for nine students with disabilities to…

  13. Observing Teaching Practice: Assessing Competence in the Classroom

    Science.gov (United States)

    Mansell, Ray

    2013-01-01

    In this article, I draw on my experiences as a Teaching Practice Observer for various Colleges of Further Education and Adult Education establishments across South West England from 1994-2002. I discuss the essential lesson components that observers need to attend to when evaluating candidates. These include the candidate's diversity of teaching…

  14. A classroom observation tool for scaffolding reading comprehension

    NARCIS (Netherlands)

    Smit, Nienke; van de Grift, Wim; de Bot, Kees; Jansen, Ellen

    An important goal of educational research is to find out which teaching practices are effective in promoting students' learning. In order to assess these practices, adequate observation instruments are needed. Existing observation schemes for language teaching are not suitable to gauge which

  15. Classroom Observation Data and Instruction in Primary Mathematics Education: Improving Design and Rigour

    Science.gov (United States)

    Thompson, Carla J.; Davis, Sandra B.

    2014-01-01

    The use of formal observation in primary mathematics classrooms is supported in the literature as a viable method of determining effective teaching strategies and appropriate tasks for inclusion in the early years of mathematics learning. The twofold aim of this study was to (a) investigate predictive relationships between primary mathematics…

  16. Classroom Composition and Measured Teacher Performance: What Do Teacher Observation Scores Really Measure?

    Science.gov (United States)

    Steinberg, Matthew P.; Garrett, Rachel

    2016-01-01

    As states and districts implement more rigorous teacher evaluation systems, measures of teacher performance are increasingly being used to support instruction and inform retention decisions. Classroom observations take a central role in these systems, accounting for the majority of teacher ratings upon which accountability decisions are based.…

  17. Observations of Children’s Interactions with Teachers, Peers, and Tasks across Preschool Classroom Activity Settings

    Science.gov (United States)

    Booren, Leslie M.; Downer, Jason T.; Vitiello, Virginia E.

    2014-01-01

    This descriptive study examined classroom activity settings in relation to children’s observed behavior during classroom interactions, child gender, and basic teacher behavior within the preschool classroom. 145 children were observed for an average of 80 minutes during 8 occasions across 2 days using the inCLASS, an observational measure that conceptualizes behavior into teacher, peer, task, and conflict interactions. Findings indicated that on average children’s interactions with teachers were higher in teacher-structured settings, such as large group. On average, children’s interactions with peers and tasks were more positive in child-directed settings, such as free choice. Children experienced more conflict during recess and routines/transitions. Finally, gender differences were observed within small group and meals. The implications of these findings might encourage teachers to be thoughtful and intentional about what types of support and resources are provided so children can successfully navigate the demands of particular settings. These findings are not meant to discourage certain teacher behaviors or imply value of certain classroom settings; instead, by providing an evidenced-based picture of the conditions under which children display the most positive interactions, teachers can be more aware of choices within these settings and have a powerful way to assist in professional development and interventions. PMID:25717282

  18. Teacher Interviews, Student Interviews, and Classroom Observations in Combinatorics: Four Analyses

    Science.gov (United States)

    Caddle, Mary C.

    2012-01-01

    This research consists of teacher interviews, student interviews, and classroom observations, all based around the mathematical content area of combinatorics. Combinatorics is a part of discrete mathematics concerning the ordering and grouping of distinct elements. The data are used in four separate analyses. The first provides evidence that…

  19. Teacher and TA Ratings of Preschoolers' Externalizing Behavior: Agreement and Associations with Observed Classroom Behavior

    Science.gov (United States)

    Wolcott, Catherine Sanger; Williford, Amanda P.

    2015-01-01

    The present study investigated teachers' and teacher aides' (TAs) agreement in their ratings of preschoolers' externalizing behavior and their associations with observed classroom behavior for a sample of children at risk of developing a disruptive behavior disorder. One hundred twenty-two teachers rated 360 students' externalizing behavior in the…

  20. Building a More Complete Understanding of Teacher Evaluation Using Classroom Observations

    Science.gov (United States)

    Cohen, Julie; Goldhaber, Dan

    2016-01-01

    Improving teacher evaluation is one of the most pressing but also contested areas of educational policy. Value-added measures have received much of the attention in new evaluation systems, but they can only be used to evaluate a fraction of teachers. Classroom observations are almost universally used to assess teachers, yet their statistical…

  1. Theoretical and Methodological Challenges in Measuring Instructional Quality in Mathematics Education Using Classroom Observations

    Science.gov (United States)

    Schlesinger, Lena; Jentsch, Armin

    2016-01-01

    In this article, we analyze theoretical as well as methodological challenges in measuring instructional quality in mathematics classrooms by examining standardized observational instruments. At the beginning, we describe the results of a systematic literature review for determining subject-specific aspects measured in recent lesson studies in…

  2. Generalizability and decision studies to inform observational and experimental research in classroom settings.

    Science.gov (United States)

    Bottema-Beutel, Kristen; Lloyd, Blair; Carter, Erik W; Asmus, Jennifer M

    2014-11-01

    Attaining reliable estimates of observational measures can be challenging in school and classroom settings, as behavior can be influenced by multiple contextual factors. Generalizability (G) studies can enable researchers to estimate the reliability of observational data, and decision (D) studies can inform how many observation sessions are necessary to achieve a criterion level of reliability. We conducted G and D studies using observational data from a randomized control trial focusing on social and academic participation of students with severe disabilities in inclusive secondary classrooms. Results highlight the importance of anchoring observational decisions to reliability estimates from existing or pilot data sets. We outline steps for conducting G and D studies and address options when reliability estimates are lower than desired.

  3. Using Classroom Observations to Measure Teacher Effectiveness: Q&A with Rob Ramsdell. REL Mid-Atlantic Webinar

    Science.gov (United States)

    Regional Educational Laboratory Mid-Atlantic, 2013

    2013-01-01

    In this webinar, Mr. Rob Ramsdell, Vice President, Cambridge Education, discussed the use of classroom observations as one measure of teacher effectiveness in a comprehensive educator support system. Mr. Ramsdell presented research-based recommendations for improving the quality and rigor of classroom observations. This Q&A addressed the…

  4. Understanding Teachers' Conceptions of Classroom Inquiry With a Teaching Scenario Survey Instrument

    Science.gov (United States)

    Kang, Nam-Hwa; Orgill, Marykay; Crippen, Kent J.

    2008-08-01

    A survey instrument using everyday teaching scenarios was developed to measure teacher conceptions of inquiry. Validity of the instrument was established by comparing responses for a group of secondary teachers to narrative writing and group discussion. Participating teachers used only three of the five essential features of inquiry detailed in the standards documents (NRC 2000) when expressing their ideas of classroom inquiry. The features of ‘evaluating explanations in connection with scientific knowledge’ and ‘communicating explanations’ were rarely mentioned. These missing components indicate a gap between the teachers’ conceptions of inquiry and the ideals of the reform movement.

  5. Development and construct validity of the Classroom Strategies Scale-Observer Form.

    Science.gov (United States)

    Reddy, Linda A; Fabiano, Gregory; Dudek, Christopher M; Hsu, Louis

    2013-12-01

    Research on progress monitoring has almost exclusively focused on student behavior and not on teacher practices. This article presents the development and validation of a new teacher observational assessment (Classroom Strategies Scale) of classroom instructional and behavioral management practices. The theoretical underpinnings and empirical basis for the instructional and behavioral management scales are presented. The Classroom Strategies Scale (CSS) evidenced overall good reliability estimates including internal consistency, interrater reliability, test-retest reliability, and freedom from item bias on important teacher demographics (age, educational degree, years of teaching experience). Confirmatory factor analyses (CFAs) of CSS data from 317 classrooms were carried out to assess the level of empirical support for (a) a 4 first-order factor theory concerning teachers' instructional practices, and (b) a 4 first-order factor theory concerning teachers' behavior management practice. Several fit indices indicated acceptable fit of the (a) and (b) CFA models to the data, as well as acceptable fit of less parsimonious alternative CFA models that included 1 or 2 second-order factors. Information-theory-based indices generally suggested that the (a) and (b) CFA models fit better than some more parsimonious alternative CFA models that included constraints on relations of first-order factors. Overall, CFA first-order and higher order factor results support the CSS-Observer Total, Composite, and subscales. Suggestions for future measurement development efforts are outlined.

  6. The Individualized Classroom Assessment Scoring System (inCLASS): Preliminary Reliability and Validity of a System for Observing Preschoolers' Competence in Classroom Interactions.

    Science.gov (United States)

    Downer, Jason T; Booren, Leslie M; Lima, Olivia K; Luckner, Amy E; Pianta, Robert C

    2010-01-01

    This paper introduces the Individualized Classroom Assessment Scoring System (inCLASS), an observation tool that targets children's interactions in preschool classrooms with teachers, peers, and tasks. In particular, initial evidence is reported of the extent to which the inCLASS meets the following psychometric criteria: inter-rater reliability, normal distributions and adequate range, construct validity, and criterion-related validity. These initial findings suggest that the inCLASS has the potential to provide an authentic, contextualized assessment of young children's classroom behaviors. Future directions for research with the inCLASS are discussed.

  7. The Classroom Observation Schedule to Measure Intentional Communication (COSMIC): an observational measure of the intentional communication of children with autism in an unstructured classroom setting.

    Science.gov (United States)

    Pasco, Greg; Gordon, Rosanna K; Howlin, Patricia; Charman, Tony

    2008-11-01

    The Classroom Observation Schedule to Measure Intentional Communication (COSMIC) was devised to provide ecologically valid outcome measures for a communication-focused intervention trial. Ninety-one children with autism spectrum disorder aged 6 years 10 months (SD 16 months) were videoed during their everyday snack, teaching and free play activities. Inter-rater reliability was high and relevant items showed significant associations with comparable items from concurrent Autism Diagnostic Observation Schedule-Generic (Lord et al. 2000, J Autism Dev Disord 30(3):205-223) assessments. In a subsample of 28 children initial differences in rates of initiations, initiated speech/vocalisation and commenting were predictive of language and communication competence 15 months later. Results suggest that the use of observational measures of intentional communication in natural settings is a valuable assessment strategy for research and clinical practice.

  8. How Are They Really Doing? Observation of Inclusionary Classroom Participation for Children with Mild-to-Moderate Deafness

    Science.gov (United States)

    Borders, Christina M.; Barnett, David; Bauer, Anne M.

    2010-01-01

    Direct observation was utilized to study how 5 children with mild-to-moderate deafness participated within inclusive classroom settings. Responses to practice and prompt opportunities, levels of prompting required to follow classroom directions, and engagement were analyzed across students with mild-to-moderate deafness and were compared to…

  9. A Study of the Relationship between Observed and Reported Use of a Cappella Singing in the Elementary General Music Classroom

    Science.gov (United States)

    Baker, Valerie Anne

    2010-01-01

    The purpose of this study was to investigate any relationship between observed and reported use of a cappella singing in the elementary general music classroom. A secondary purpose of this study was to examine teachers' practical perspectives influencing the use of a cappella singing in the elementary general music classroom. From a total of 50…

  10. A hybrid double-observer sightability model for aerial surveys

    Science.gov (United States)

    Griffin, Paul C.; Lubow, Bruce C.; Jenkins, Kurt J.; Vales, David J.; Moeller, Barbara J.; Reid, Mason; Happe, Patricia J.; Mccorquodale, Scott M.; Tirhi, Michelle J.; Schaberi, Jim P.; Beirne, Katherine

    2013-01-01

    Raw counts from aerial surveys make no correction for undetected animals and provide no estimate of precision with which to judge the utility of the counts. Sightability modeling and double-observer (DO) modeling are 2 commonly used approaches to account for detection bias and to estimate precision in aerial surveys. We developed a hybrid DO sightability model (model MH) that uses the strength of each approach to overcome the weakness in the other, for aerial surveys of elk (Cervus elaphus). The hybrid approach uses detection patterns of 2 independent observer pairs in a helicopter and telemetry-based detections of collared elk groups. Candidate MH models reflected hypotheses about effects of recorded covariates and unmodeled heterogeneity on the separate front-seat observer pair and back-seat observer pair detection probabilities. Group size and concealing vegetation cover strongly influenced detection probabilities. The pilot's previous experience participating in aerial surveys influenced detection by the front pair of observers if the elk group was on the pilot's side of the helicopter flight path. In 9 surveys in Mount Rainier National Park, the raw number of elk counted was approximately 80–93% of the abundance estimated by model MH. Uncorrected ratios of bulls per 100 cows generally were low compared to estimates adjusted for detection bias, but ratios of calves per 100 cows were comparable whether based on raw survey counts or adjusted estimates. The hybrid method was an improvement over commonly used alternatives, with improved precision compared to sightability modeling and reduced bias compared to DO modeling.

  11. Observed classroom behavior of children with ADHD: relationship to gender and comorbidity.

    Science.gov (United States)

    Abikoff, Howard B; Jensen, Peter S; Arnold, L L Eugene; Hoza, Betsy; Hechtman, Lily; Pollack, Simcha; Martin, Diane; Alvir, Jose; March, John S; Hinshaw, Stephen; Vitiello, Benedetto; Newcorn, Jeffrey; Greiner, Andrew; Cantwell, Dennis P; Conners, C Keith; Elliott, Glen; Greenhill, Laurence L; Kraemer, Helena; Pelham, William E; Severe, Joanne B; Swanson, James M; Wells, Karen; Wigal, Tim

    2002-08-01

    Examined hypothesized gender and comorbidity differences in the observed classroom behavior of children with attention deficit hyperactivity disorder (ADHD). The behavior of 403 boys and 99 girls with ADHD, ages 7-10, was compared (a) to observed, sex-specific classroom behavior norms, (b) by sex, and (c) by comorbid subgroups. Boys and girls with ADHD deviated significantly from classroom norms on 15/16 and 13/16 categories, respectively. Compared to comparison girls, girls with ADHD had relatively high rates of verbal aggression to children. Boys with ADHD engaged in more rule-breaking and externalizing behaviors than did girls with ADHD, but the sexes did not differ on more "neutral," unobtrusive behaviors. The sex differences are consistent with notions of why girls with ADHD are identified and referred later than boys. Contrary to hypothesis, the presence of comorbid anxiety disorder (ANX) was not associated with behavioral suppression; yet, as hypothesized, children with a comorbid disruptive behavior disorder (DBD) had higher rates of rule-breaking, and impulsive and aggressive behavior, than did children with ADHD alone and those with ADHD+ANX. Elevated rates of ADHD behaviors were also observed in children with comorbid DBD, indicating that these behaviors are truly present and suggesting that reports of higher ADHD ratings in this subgroup are not simply a consequence of negative halo effects and rater biases.

  12. ASPECT: A Survey to Assess Student Perspective of Engagement in an Active-Learning Classroom.

    Science.gov (United States)

    Wiggins, Benjamin L; Eddy, Sarah L; Wener-Fligner, Leah; Freisem, Karen; Grunspan, Daniel Z; Theobald, Elli J; Timbrook, Jerry; Crowe, Alison J

    2017-01-01

    The primary measure used to determine relative effectiveness of in-class activities has been student performance on pre/posttests. However, in today's active-learning classrooms, learning is a social activity, requiring students to interact and learn from their peers. To develop effective active-learning exercises that engage students, it is important to gain a more holistic view of the student experience in an active-learning classroom. We have taken a mixed-methods approach to iteratively develop and validate a 16-item survey to measure multiple facets of the student experience during active-learning exercises. The instrument, which we call Assessing Student Perspective of Engagement in Class Tool (ASPECT), was administered to a large introductory biology class, and student responses were subjected to exploratory factor analysis. The 16 items loaded onto three factors that cumulatively explained 52% of the variation in student response: 1) value of activity, 2) personal effort, and 3) instructor contribution. ASPECT provides a rapid, easily administered means to measure student perception of engagement in an active-learning classroom. Gaining a better understanding of students' level of engagement will help inform instructor best practices and provide an additional measure for comprehensively assessing the impact of different active-learning strategies. © 2017 B. L. Wiggins, S. L. Eddy, et al. CBE—Life Sciences Education © 2017 The American Society for Cell Biology. This article is distributed by The American Society for Cell Biology under license from the author(s). It is available to the public under an Attribution–Noncommercial–Share Alike 3.0 Unported Creative Commons License (http://creativecommons.org/licenses/by-nc-sa/3.0).

  13. Exploring Researchers in Dialogue: Linguistic and Educational Perspectives on Observational Data from a Sixth Grade Classroom

    Directory of Open Access Journals (Sweden)

    Helg Fottland

    2004-09-01

    Full Text Available This article reflects on a collaborative process between two researchers from different backgrounds conducting a joint-venture classroom observation project focusing on language, communication and special education. Focusing on the connection between explorative learning situations and dialogue in relation to children's learning and identity development, the researchers cooperate on all levels in the research process. The article compares findings when approaching data from two different professional traditions, linguistics and education. The main focus is how each of the researchers approaches the data analysis. The combining of approaches in interpreting and writing is also discussed. Narratives and spoken dialogues are vital in this work; transcripts of video material from a primary school classroom are used as illustrations.

  14. The Westerbork Hydrogen Accretion in Local Galaxies (HALOGAS) Survey I. Survey Description and Pilot Observations

    CERN Document Server

    Heald, George; Serra, Paolo; Zschaechner, Laura; Rand, Richard; Fraternali, Filippo; Oosterloo, Tom; Walterbos, Rene; Juette, Eva; Gentile, Gianfranco

    2010-01-01

    We introduce a new, very deep neutral hydrogen (HI) survey being performed with the Westerbork Synthesis Radio Telescope (WSRT). The Westerbork Hydrogen Accretion in LOcal GAlaxieS (HALOGAS) Survey is producing an archive of some of the most sensitive HI observations available, on the angular scales which are most useful for studying faint, diffuse gas in and around nearby galaxies. The survey data are being used to perform careful modeling of the galaxies, characterizing their gas content, morphology, and kinematics, with the primary goal of revealing the global characteristics of cold gas accretion onto spiral galaxies in the local Universe. In this paper, we describe the survey sample selection, the data acquisition, reduction, and analysis, and present the data products obtained during our pilot program, which consists of UGC 2082, NGC 672, NGC 925, and NGC 4565. The observations reveal a first glimpse of the picture that the full HALOGAS project aims to illuminate: the properties of accreting HI in diffe...

  15. Energy Education in the Schools. Results of a Survey of the Penetration of Energy Education into the Classroom.

    Science.gov (United States)

    White, Janet A.; Fowler, John M.

    Nine years after the 1973 oil embargo and the outpouring of educational materials and strategies developed in response to the energy crisis, the extent and content of energy education in the classroom were assessed. Seven thousand randomly selected teachers and principals were surveyed at the end of the 1981-82 school year (1000 each of elementary…

  16. Preservice Teachers' Classroom Management Training: A Survey of Self-Reported Training Experiences, Content Coverage, and Preparedness

    Science.gov (United States)

    Christofferson, Michael; Sullivan, Amanda L.

    2015-01-01

    Many teachers report that their preservice training in classroom management was inadequate or ineffective, but little is known about the types of training they receive. In this exploratory study, 157 preservice teachers from throughout the United States were surveyed about the training sources through which they obtained knowledge and skills in…

  17. A Survey of Exemplar Teachers' Perceptions, Use, and Access of Computer-Based Games and Technology for Classroom Instruction

    Science.gov (United States)

    Proctor, Michael D.; Marks, Yaela

    2013-01-01

    This research reports and analyzes for archival purposes surveyed perceptions, use, and access by 259 United States based exemplar Primary and Secondary educators of computer-based games and technology for classroom instruction. Participating respondents were considered exemplary as they each won the Milken Educator Award during the 1996-2009…

  18. Technology Use and Acceptance in the Classroom: Results from an Exploratory Survey Study among Secondary Education Teachers in the USA

    Science.gov (United States)

    Holden, Heather; Ozok, Ant; Rada, Roy

    2008-01-01

    Purpose: The purpose of this study is to explore the current usage and acceptance of classroom technologies by secondary math/science education teachers in one community. Design/methodology/approach: Forty-seven secondary education math and science teachers in one American city responded to a survey about their use and perceptions of technology in…

  19. Preservice Teachers' Classroom Management Training: A Survey of Self-Reported Training Experiences, Content Coverage, and Preparedness

    Science.gov (United States)

    Christofferson, Michael; Sullivan, Amanda L.

    2015-01-01

    Many teachers report that their preservice training in classroom management was inadequate or ineffective, but little is known about the types of training they receive. In this exploratory study, 157 preservice teachers from throughout the United States were surveyed about the training sources through which they obtained knowledge and skills in…

  20. Mercury's Plasma Mantle – a survey of MESSENGER observations

    Science.gov (United States)

    Jasinski, Jamie Matthew; Slavin, James A.; Raines, Jim; DiBraccio, Gina

    2016-10-01

    The plasma mantle is a region of solar wind plasma entry into the nightside high-latitude magnetosphere. We present a survey of plasma mantles identified in particle and magnetic field measurements from four years of MESSENGER spacecraft observations of Mercury's magnetosphere. The two common observational signatures of this region are ion energy latitude dispersions as well as diamagnetic depressions. From these observations we estimate the contribution of plasma from the solar wind via the mantle and infer magnitude and variability in the cross-magnetospheric electric fields present at Mercury's dynamic magnetosphere.

  1. Science Teacher Beliefs and Classroom Practice Related to Constructivism in Different School Settings

    Science.gov (United States)

    Savasci, Funda; Berlin, Donna F.

    2012-01-01

    Science teacher beliefs and classroom practice related to constructivism and factors that may influence classroom practice were examined in this cross-case study. Data from four science teachers in two schools included interviews, demographic questionnaire, Classroom Learning Environment Survey (preferred/perceived), and classroom observations and…

  2. Science Teacher Beliefs and Classroom Practice Related to Constructivism in Different School Settings

    Science.gov (United States)

    Savasci, Funda; Berlin, Donna F.

    2012-01-01

    Science teacher beliefs and classroom practice related to constructivism and factors that may influence classroom practice were examined in this cross-case study. Data from four science teachers in two schools included interviews, demographic questionnaire, Classroom Learning Environment Survey (preferred/perceived), and classroom observations and…

  3. The GALAH Survey: Observational Overview and Gaia DR1 companion

    CERN Document Server

    Martell, Sarah; Buder, Sven; Duong, Ly; Schlesinger, Katharine; Simpson, Jeffrey; Lind, Karin; Ness, Melissa; Marshall, Jonathan; Asplund, Martin; Bland-Hawthorn, Joss; Casey, Andrew; De Silva, Gayandhi; Freeman, Ken; Kos, Janez; Lin, Jane; Zucker, Daniel; Zwitter, Tomaz; Anguiano, Borja; Bacigalupo, Carlos; Carollo, Daniela; Casagrande, Luca; Da Costa, Gary; Horner, Jonathan; Huber, Daniel; Hyde, Elaina; Kafle, Prajwal; Lewis, Geraint; Nataf, David; Stello, Dennis; Tinney, Chris; Watson, Fred; Wittenmyer, Rob

    2016-01-01

    The Galactic Archaeology with HERMES (GALAH) Survey is a massive observational project to trace the Milky Way's history of star formation, chemical enrichment, stellar migration and minor mergers. Using high-resolution (R$\\simeq$28,000) spectra taken with the High Efficiency and Resolution Multi-Element Spectrograph (HERMES) instrument at the Anglo-Australian Telescope (AAT), GALAH will determine stellar parameters and abundances of up to 29 elements for up to one million stars. Selecting targets from a colour-unbiased catalogue built from 2MASS, APASS and UCAC4 data, we expect to observe dwarfs at 0.3 to 3 kpc and giants at 1 to 10 kpc. This enables a thorough local chemical inventory of the Galactic thin and thick disks, and also captures smaller samples of the bulge and halo. In this paper we present the plan, process and progress as of early 2016 for GALAH survey observations. In our first two years of survey observing we have accumulated the largest high-quality spectroscopic data set at this resolution,...

  4. Modern Cosmology: Interactive Computer Simulations that use Recent Observational Surveys

    CERN Document Server

    Moldenhauer, Jacob; Stone, Keenan; Shuler, Ezekiel

    2013-01-01

    We present a collection of new, open-source computational tools for numerically modeling recent large-scale observational data sets using modern cosmology theory. Specifically, these tools will allow both students and researchers to constrain the parameter values in competitive cosmological models, thereby discovering both the accelerated expansion of the universe and its composition (e.g., dark matter and dark energy). These programs have several features to help the non-cosmologist build an understanding of cosmological models and their relation to observational data: a built-in collection of several real observational data sets; sliders to vary the values of the parameters that define different cosmological models; real-time plotting of simulated data; and $\\chi^2$ calculations of the goodness of fit for each choice of parameters (theory) and observational data (experiment). The current list of built-in observations includes several recent supernovae Type Ia surveys, baryon acoustic oscillations, the cosmi...

  5. Experimental investigation of observation error in anuran call surveys

    Science.gov (United States)

    McClintock, B.T.; Bailey, L.L.; Pollock, K.H.; Simons, T.R.

    2010-01-01

    Occupancy models that account for imperfect detection are often used to monitor anuran and songbird species occurrence. However, presenceabsence data arising from auditory detections may be more prone to observation error (e.g., false-positive detections) than are sampling approaches utilizing physical captures or sightings of individuals. We conducted realistic, replicated field experiments using a remote broadcasting system to simulate simple anuran call surveys and to investigate potential factors affecting observation error in these studies. Distance, time, ambient noise, and observer abilities were the most important factors explaining false-negative detections. Distance and observer ability were the best overall predictors of false-positive errors, but ambient noise and competing species also affected error rates for some species. False-positive errors made up 5 of all positive detections, with individual observers exhibiting false-positive rates between 0.5 and 14. Previous research suggests false-positive errors of these magnitudes would induce substantial positive biases in standard estimators of species occurrence, and we recommend practices to mitigate for false positives when developing occupancy monitoring protocols that rely on auditory detections. These recommendations include additional observer training, limiting the number of target species, and establishing distance and ambient noise thresholds during surveys. ?? 2010 The Wildlife Society.

  6. Characterisation of false-positive observations in botanical surveys

    Directory of Open Access Journals (Sweden)

    Quentin J. Groom

    2017-05-01

    Full Text Available Errors in botanical surveying are a common problem. The presence of a species is easily overlooked, leading to false-absences; while misidentifications and other mistakes lead to false-positive observations. While it is common knowledge that these errors occur, there are few data that can be used to quantify and describe these errors. Here we characterise false-positive errors for a controlled set of surveys conducted as part of a field identification test of botanical skill. Surveys were conducted at sites with a verified list of vascular plant species. The candidates were asked to list all the species they could identify in a defined botanically rich area. They were told beforehand that their final score would be the sum of the correct species they listed, but false-positive errors counted against their overall grade. The number of errors varied considerably between people, some people create a high proportion of false-positive errors, but these are scattered across all skill levels. Therefore, a person’s ability to correctly identify a large number of species is not a safeguard against the generation of false-positive errors. There was no phylogenetic pattern to falsely observed species; however, rare species are more likely to be false-positive as are species from species rich genera. Raising the threshold for the acceptance of an observation reduced false-positive observations dramatically, but at the expense of more false negative errors. False-positive errors are higher in field surveying of plants than many people may appreciate. Greater stringency is required before accepting species as present at a site, particularly for rare species. Combining multiple surveys resolves the problem, but requires a considerable increase in effort to achieve the same sensitivity as a single survey. Therefore, other methods should be used to raise the threshold for the acceptance of a species. For example, digital data input systems that can verify

  7. The sloan digital sky Survey-II supernova survey: search algorithm and follow-up observations

    Energy Technology Data Exchange (ETDEWEB)

    Sako, Masao [Department of Physics and Astronomy, University of Pennsylvania, 209 South 33rd Street, Philadelphia, PA 19104 (United States); Bassett, Bruce [Department of Mathematics and Applied Mathematics, University of Cape Town, Rondebosch 7701 (South Africa); Becker, Andrew; Hogan, Craig J. [Department of Astronomy, University of Washington, Box 351580, Seattle, WA 98195 (United States); Cinabro, David [Department of Physics, Wayne State University, Detroit, MI 48202 (United States); DeJongh, Fritz; Frieman, Joshua A.; Marriner, John; Miknaitis, Gajus [Center for Particle Astrophysics, Fermi National Accelerator Laboratory, P.O. Box 500, Batavia, IL 60510 (United States); Depoy, D. L.; Prieto, Jose Luis [Department of Astronomy, Ohio State University, 140 West 18th Avenue, Columbus, OH 43210-1173 (United States); Dilday, Ben; Kessler, Richard [Kavli Institute for Cosmological Physics, The University of Chicago, 5640 South Ellis Avenue Chicago, IL 60637 (United States); Doi, Mamoru [Institute of Astronomy, Graduate School of Science, University of Tokyo 2-21-1, Osawa, Mitaka, Tokyo 181-0015 (Japan); Garnavich, Peter M. [University of Notre Dame, 225 Nieuwland Science, Notre Dame, IN 46556-5670 (United States); Holtzman, Jon [Department of Astronomy, MSC 4500, New Mexico State University, P.O. Box 30001, Las Cruces, NM 88003 (United States); Jha, Saurabh [Kavli Institute for Particle Astrophysics and Cosmology, Stanford University, P.O. Box 20450, MS29, Stanford, CA 94309 (United States); Konishi, Kohki [Institute for Cosmic Ray Research, University of Tokyo, 5-1-5, Kashiwanoha, Kashiwa, Chiba, 277-8582 (Japan); Lampeitl, Hubert [Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218 (United States); Nichol, Robert C. [Institute of Cosmology and Gravitation, Mercantile House, Hampshire Terrace, University of Portsmouth, Portsmouth PO1 2EG (United Kingdom); and others

    2008-01-01

    The Sloan Digital Sky Survey-II Supernova Survey has identified a large number of new transient sources in a 300 deg{sup 2} region along the celestial equator during its first two seasons of a three-season campaign. Multi-band (ugriz) light curves were measured for most of the sources, which include solar system objects, galactic variable stars, active galactic nuclei, supernovae (SNe), and other astronomical transients. The imaging survey is augmented by an extensive spectroscopic follow-up program to identify SNe, measure their redshifts, and study the physical conditions of the explosions and their environment through spectroscopic diagnostics. During the survey, light curves are rapidly evaluated to provide an initial photometric type of the SNe, and a selected sample of sources are targeted for spectroscopic observations. In the first two seasons, 476 sources were selected for spectroscopic observations, of which 403 were identified as SNe. For the type Ia SNe, the main driver for the survey, our photometric typing and targeting efficiency is 90%. Only 6% of the photometric SN Ia candidates were spectroscopically classified as non-SN Ia instead, and the remaining 4% resulted in low signal-to-noise, unclassified spectra. This paper describes the search algorithm and the software, and the real-time processing of the SDSS imaging data. We also present the details of the supernova candidate selection procedures and strategies for follow-up spectroscopic and imaging observations of the discovered sources.

  8. New Quasar Surveys With WIRO: Planning and Depth of Observations

    Science.gov (United States)

    Bassett, Neil; Deam, Sophie; Dixon, Don; Griffith, Emily; Harvey, William; Lee, Daniel; Lyke, Bradley; Haze Nunez, Evan; Parziale, Ryan; Witherspoon, Catherine; Myers, Adam D.; Findlay, Joseph; Kobulnicky, Henry A.; Dale, Daniel A.

    2017-01-01

    The Wyoming Infrared Observatory (WIRO) 2.3-meter telescope is used to observe a section of sky behind the outer regions of the galaxy M33 with the goal of identifying previously undiscovered quasar candidates. We choose the regions based on visibility during the time of year the observations are taken as well as regions in which few quasars have been detected by previous surveys. DS9 and Python are used to determine the coordinates of our desired field centers for photometric observations in the u, g, r, and i Sloan filters. Exposure times are chosen such that the depth in each filter is greater than an apparent magnitude of 21. This depth allows us to identify quasar candidates which are fainter than other quasar surveys in the same vicinity. Future spectroscopic observations will be able to confirm if the candidates are indeed quasars and spectra of the confirmed quasars can be used to study the extended gaseous region of M33. This work is supported by the National Science Foundation under REU grant AST 1560461.

  9. From Texts to Pictures in Teaching Civics. Participant Observation in Mark’s Classroom

    Directory of Open Access Journals (Sweden)

    Per-Olof Erixon

    2010-11-01

    Full Text Available We are now living in a “new media age”, with a dramatic shift from the linguistic to the visual, from books and book pages to screens and windows (Kress, 2003. This article offsets out to explore what happens to educational activities in schools when electronic media and pictures replace written texts. The article draws on interviews and classroom observations of a particular Swedish vocational upper secondary programme, where the social studies teacher observes that students are finding it increasingly difficult to benefit from written texts. Theoretically, the study draws on Meyrowitz (1985/1986 theories concerning the relationship among media, situations and behaviour and the effect of a shift from “print situations” to “electronic situations” on a broad range of social role and Bernstein’s (1996/2000 notions of ‘recontextualisation’, ‘framing’ and ‘classification’. The study shows that classroom relations are changing; hierarchies between students and teachers are being broken down, and classification of subjects is affected in the sense that the students’ own interpretations and references are beginning to govern teaching when pictures and electronic media enter the educational discourse.

  10. DUst Around NEarby Stars. The survey observational results

    CERN Document Server

    Eiroa, C; Mora, A; Montesinos, B; Absil, O; Augereau, J Ch; Bayo, A; Bryden, G; Danchi, W; del Burgo, C; Ertel, S; Fridlund, M; Heras, A M; Krivov, A V; Launhardt, R; Liseau, R; Löhne, T; Maldonado, J; Pilbratt, G L; Roberge, A; Rodmann, J; Sanz-Forcada, J; Solano, E; Stapelfeldt, K; Thébault, P; Wolf, S; Ardila, D; Arévalo, M; Beichmann, C; Faramaz, V; González-García, B M; Gutiérrez, R; Lebreton, J; Martínez-Arnáiz, R; Meeus, G; Montes, D; Olofsson, G; Su, K Y L; White, G J; Barrado, D; Fukagawa, M; Grün, E; Kamp, I; Lorente, R; Morbidelli, A; Müller, S; Mutschke, H; Nakagawa, T; Ribas, I; Walker, H

    2013-01-01

    Debris discs are a consequence of the planet formation process and constitute the fingerprints of planetesimal systems. Their solar system's counterparts are the asteroid and Edgeworth-Kuiper belts. The DUNES survey aims at detecting extra-solar analogues to the Edgeworth-Kuiper belt around solar-type stars, putting in this way the solar system into context. The survey allows us to address some questions related to the prevalence and properties of planetesimal systems. We used {\\it Herschel}/PACS to observe a sample of nearby FGK stars. Data at 100 and 160 $\\mu$m were obtained, complemented in some cases with observations at 70 $\\mu$m, and at 250, 350 and 500 $\\mu$m using SPIRE. The observing strategy was to integrate as deep as possible at 100 $\\mu$m to detect the stellar photosphere. Debris discs have been detected at a fractional luminosity level down to several times that of the Edgeworth-Kuiper belt. The incidence rate of discs around the DUNES stars is increased from a rate of $\\sim$ 12.1% $\\pm$ 5% befo...

  11. The Identity, Second Language, and the Classroom Dynamic: Participant Observation in a Beginning Korean as a Second Language Classroom

    Science.gov (United States)

    Diamond, Joel S.

    2010-01-01

    The goal of this qualitative study was to explore the nexus between second language acquisition, identity, and the beginning second language classroom. Using a social constructionist framework, the study utilizes ethnographic methodology incorporating both narrative and autoethnographic elements. Specifically the author acted as a participant…

  12. Examination of Classroom Observations and Educator Perceptions of Classroom Interventions of Middle School Gifted Students Exhibiting Unhealthy Perfectionist Tendencies

    Science.gov (United States)

    Drawdy, LaTease

    2013-01-01

    Unhealthy perfectionist tendencies plague many gifted middle school students, and this type of perfectionism can lead to a lack of classroom success. Identifying effective interventions that educators can utilize is important in assisting middle school gifted students who demonstrate these maladaptive tendencies in their achievement in the…

  13. Evaluating teaching and learning from students’ perspectives in their classroom through easy-to-use online surveys

    Directory of Open Access Journals (Sweden)

    LIP Paul Chi Hong

    2008-06-01

    Full Text Available The aim of this article is to help technophobic teachers to use a free and easy-to-use online survey to investigate their students’ opinions and beliefs about the learning and teaching in the classroom. This article would also help technophobic teachers who were used to analyzing the results manually by counting the students’ responses from the traditional paper-based questionnaires/surveys to instantly and conveniently use online surveys to get qualitative and quantitative data from their students’ responses with just a few clicks. In this article, the researcher will share the following aspects: 1 the need to use online surveys at secondary and postsecondary level; 2 the definition of technophobia and the need to train technophobic teachers to use technology; 3 the definition of an online survey; 4 and a sharing of how to create an online surv

  14. Observing physical education teachers' need-supportive interactions in classroom settings.

    Science.gov (United States)

    Haerens, Leen; Aelterman, Nathalie; Van den Berghe, Lynn; De Meyer, Jotie; Soenens, Bart; Vansteenkiste, Maarten

    2013-02-01

    According to self-determination theory, teachers can motivate students by supporting their psychological needs for relatedness, competence, and autonomy. The present study complements extant research (most of which relied on self-report measures) by relying on observations of need-supportive teaching in the domain of physical education (PE), which allows for the identification of concrete, real-life examples of how teacher need support manifests in the classroom. Seventy-four different PE lessons were coded for 5-min intervals to assess the occurrence of 21 need-supportive teaching behaviors. Factor analyses provided evidence for four interpretable factors, namely, relatedness support, autonomy support, and two components of structure (structure before and during the activity). Reasonable evidence was obtained for convergence between observed and student perceived need support. Yet, the low interrater reliability for two of the four scales indicates that these scales need further improvement.

  15. Very metal-poor stars observed by the RAVE survey

    Science.gov (United States)

    Matijevič, G.; Chiappini, C.; Grebel, E. K.; Wyse, R. F. G.; Zwitter, T.; Bienaymé, O.; Bland-Hawthorn, J.; Freeman, K. C.; Gibson, B. K.; Gilmore, G.; Helmi, A.; Kordopatis, G.; Kunder, A.; Munari, U.; Navarro, J. F.; Parker, Q. A.; Reid, W.; Seabroke, G.; Siviero, A.; Steinmetz, M.; Watson, F.

    2017-07-01

    Metal-poor stars trace the earliest phases in the chemical enrichment of the Universe. They give clues about the early assembly of the Galaxy as well as on the nature of the first stellar generations. Multi-object spectroscopic surveys play a key role in finding these fossil records in large volumes. Here we present a novel analysis of the metal-poor star sample in the complete Radial Velocity Experiment (RAVE) Data Release 5 catalog with the goal of identifying and characterizing all very metal-poor stars observed by the survey. Using a three-stage method, we first identified the candidate stars using only their spectra as input information. We employed an algorithm called t-SNE to construct a low-dimensional projection of the spectrum space and isolate the region containing metal-poor stars. Following this step, we measured the equivalent widths of the near-infrared Ca ii triplet lines with a method based on flexible Gaussian processes to model the correlated noise present in the spectra. In the last step, we constructed a calibration relation that converts the measured equivalent widths and the color information coming from the 2MASS and WISE surveys into metallicity and temperature estimates. We identified 877 stars with at least a 50% probability of being very metal-poor ([Fe/H] < -2 dex), out of which 43 are likely extremely metal-poor ([Fe/H] < -3 dex). The comparison of the derived values to a small subsample of stars with literature metallicity values shows that our method works reliably and correctly estimates the uncertainties, which typically have valuesσ[Fe/H] ≈ 0.2 dex. In addition, when compared to the metallicity results derived using the RAVE DR5 pipeline, it is evident that we achieve better accuracy than the pipeline and therefore more reliably evaluate the very metal-poor subsample. Based on the repeated observations of the same stars, our method gives very consistent results. We intend to study the identified sample further by acquiring high

  16. Observing the interactive qualities of L2 instructional practices in ESL and FSL classrooms

    Directory of Open Access Journals (Sweden)

    Michael Zuniga

    2016-03-01

    Full Text Available Discourse features that promote the generation of interactionally modified input and output, such as negotiation for meaning, have been shown to significantly enhance second language acquisition. Research has also identified several characteristics of instructional practices that render them more or less propitious to the generation of these discourse features. While various classroom observation studies have successfully measured the communicative orientation of classroom environments, most of the indicators of interactivity analyzed in those studies were obtained through micro-level discourse analyses and not through macro-level analyses of task-related factors shown to directly influence the interactivity of instructional practices. Such a macro-level scale has potential practical implications for teachers and administrators seeking an efficient tool for assessing and improving the interactivity afforded by a given curriculum. The objective of the present study was therefore to develop macro-level scale to determine the extent to which teachers of French and English as a second language use interaction-friendly instructional practices. Using an observation scheme designed to code data on factors shown to influence interactivity, 63 hours of FSL and ESL classes from secondary schools in the Montreal area were observed and analyzed. Results indicate clear differences between the two groups. While both ESL and FSL classes were less teacher-centered than those observed in previous studies, they were still rated as not-very-interactive. Target language differences showed that the FSL classes were more teacher-centered and characterized by fewer interaction-friendly tasks and activities than the ESL classes. Task characteristics, reasons for ESL and FSL differences and recommendations for improvement are discussed.

  17. Survey and Chase: A New Method of Observations For The Michigan Orbital Debris Survey Telescope (MODEST)

    Science.gov (United States)

    Abercromby, Kira J.; Seitzer, Patrick; Rodriquez, Heather M.; Barker, Edwin S.; Matney, Mark J.

    2006-01-01

    For more than 40 years astronauts have been observing Earth, taking photographs or digital images from their spacecraft. Today, a robust program of observation from the International Space Station (ISS) has yielded hundreds of thousands of images of the Earth s surface collected since 2001. Seeing Earth through the eyes of an astronaut is exciting to the general public, and the images are popular in classrooms. Because the ISS has an orbital inclination of 51.6 degrees (the north-south limits of the orbit are at 51.6 degrees latitude), high latitude observations are common. Some of the most striking images collected include views of polar phenomena. Astronauts routinely pass above brilliant red and green aurora; view high, wispy clouds at the top of the atmosphere; or look down on glaciers and floating ice rafts. These images, framed and captured by humans, are easily interpreted by students and teachers. Astronaut observations provide a way to visualize complicated polar phenomena and communicate about them to students of all ages. Over the next two years, astronauts aboard the ISS will formally focus their observations on polar phenomena as participants in the International Polar Year (IPY). Imagery acquisition from the ISS will be coordinated with other IPY scientists staging studies and field campaigns on the ground. The imagery collected from the ISS will be cataloged and served on NASA s web-based database of images, http://eol.jsc.nasa.gov . The website allows investigators, students and teachers to search through the imagery, assemble image datasets, and download the imagery and the metadata. We display some of the most spectacular examples of polar imagery and demonstrate NASA s database of astronaut images of Earth.

  18. DUst around NEarby Stars. The Survey Observational Results

    Science.gov (United States)

    Eiroa, C.; Marshall, J. P.; Mora, A.; Montesinos, B.; Absil, O.; Augereau, J. Ch.; Bayo, A.; Bryden, G.; Danchi, W.; delBurgo, C.; Ertel, S..; Fridlund, M.; Heras, A. M.; Krivov, A. V.; Launhardt, R.; Liseau, R.; Lohne, T.; Maldonado, J.; Pilbratt, G. L.; Roberge, A.; Rodman, J.; Sanz-Forcada, J.; Stapelfeldt, K.; Ardila, D.; Beichmann, C.

    2013-01-01

    Context. Debris discs are a consequence of the planet formation process and constitute the fingerprints of planetesimal systems. Their solar system counterparts are the asteroid and Edgeworth-Kuiper belts.Aims. The DUNES survey aims at detecting extra-solar analogues to the Edgeworth-Kuiper belt around solar-type stars, putting in this way the solar system into context. The survey allows us to address some questions related to the prevalence and properties of planetesimal systems.Methods. We used Herschel PACS to observe a sample of nearby FGK stars. Data at 100 and 160 micron were obtained, complemented in some cases with observations at 70 micron, and at 250, 350 and 500 micron using SPIRE. The observing strategy was to integrate as deep as possible at 100 micron to detect the stellar photosphere. Results. Debris discs have been detected at a fractional luminosity level down to several times that of the Edgeworth-Kuiper belt. The incidence rate of discs around the DUNES stars is increased from a rate of approx. 12.1% +/- 5% before Herschel to approx 20.2 % +/- % 2. A significant fraction (approx. 52%) of the discs are resolved, which represents an enormous step ahead from the previously known resolved discs. Some stars are associated with faint far-IR excesses attributed to a new class of cold discs. Although it cannot be excluded that these excesses are produced by coincidental alignment of background galaxies, statistical arguments suggest that at least some of them are true debris discs. Some discs display peculiar SEDs with spectral indexes in the 70-160 micron range steeper than the Rayleigh-Jeans one. An analysis of the debris disc parameters suggests that a decrease might exist of the mean black body radius from the F-type to the K-type stars. In addition, a weak trend is suggested for a correlation of disc sizes and an anticorrelation of disc temperatures with the stellar age.

  19. Initial Validation of the Prekindergarten Classroom Observation Tool and Goal Setting System for Data-Based Coaching

    Science.gov (United States)

    Crawford, April D.; Zucker, Tricia A.; Williams, Jeffrey M.; Bhavsar, Vibhuti; Landry, Susan H.

    2013-01-01

    Although coaching is a popular approach for enhancing the quality of Tier 1 instruction, limited research has addressed observational measures specifically designed to focus coaching on evidence-based practices. This study explains the development of the prekindergarten (pre-k) Classroom Observation Tool (COT) designed for use in a data-based…

  20. Preparing for the WFIRST Microlensing Survey: Simulations, Requirements, Survey Strategies, and Precursor Observations

    Science.gov (United States)

    Gaudi, Bernard

    As one of the four primary investigations of the Wide Field Infrared Survey Telescope (WFIRST) mission, the microlensing survey will monitor several square degrees of the Galactic bulge for a total of roughly one year. Its primary science goal is to "Complete the statistical census of planetary systems in the Galaxy, from the outer habitable zone to free floating planets, including analogs of all of the planets in our Solar System with the mass of Mars or greater.'' WFIRST will therefore (a) measure the mass function of cold bound planets with masses greater than that of roughly twice the mass of the moon, including providing an estimate of the frequency of sub-Mars-mass embryos, (b) determine the frequency of free-floating planets with masses down to the Earth and below, (c) inform the frequency and habitability of potentially habitable worlds, and (d) revolutionize our understanding of the demographics of cold planets with its exquisite sensitivity to, and large expected yield of, planets in a broad and unexplored region of parameter space. In order for the microlensing survey to be successful, we must develop a plan to go from actual survey observations obtained by the WFIRST telescope and hardware to the final science products. This plan will involve many steps, the development of software, data reduction, and analysis tools at each step, and a list of requirements for each of these components. The overarching goal of this proposal is thus to develop a complete flowdown from the science goals of the microlensing survey to the mission design and hardware components. We have assembled a team of scientists with the breadth of expertise to achieve this primary goal. Our specific subgoals are as follows. Goal 1: We will refine the input Galactic models in order to provide improved microlensing event rates in the WFIRST fields. Goal 2: We will use the improved event rate estimates, along with improvements in our simulation methodology, to provide higher

  1. An Observation of Classroom Assessment Practices among Lecturers in Selected Malaysian Higher Learning Institutions

    Science.gov (United States)

    Singh, Charanjit Kaur Swaran; Lebar, Othman; Kepol, Napisah; Rahman, Rafiah Abdul; Mukhtar, Kurotol Aini Muhammad

    2017-01-01

    Purpose: The study was aimed at exploring and analysing the current assessment practices of lecturers in selected Malaysian higher learning institution classrooms. The focus was the different modes of assessment used in the classroom and to make recommendations on using a variety of assessment modes that would be well-aligned with the intended…

  2. Participate or Observe? Effects of Economic Classroom Experiments on Students' Economic Literacy

    Science.gov (United States)

    Grol, Roel; Sent, Esther-Mirjam; de Vries, Bregje

    2017-01-01

    Economic classroom experiments are controlled interactive learning exercises targeting the comprehension of economic concepts in an inductive way. Aiming at increasing students' knowledge of economic concepts, two types of economic classroom experiments are examined in a sample of 134 secondary school students. In the interactive research…

  3. Who Is Granted Authority in the Mathematics Classroom? An Analysis of the Observed and Perceived Distribution of Authority

    Science.gov (United States)

    Depaepe, Fien; De Corte, Erik; Verschaffel, Lieven

    2012-01-01

    The article deals with the way in which authority was established and interpreted by teachers and students in two Flemish sixth-grade mathematics classrooms. Problem-solving lessons during a seven-month observation period were analysed regarding three aspects of teacher-student interactions that explicitly or implicitly reflect who bears…

  4. The Development and Implementation of a Planned Program of Classroom Observation at the Elementary School Level. Maxi II Practicum Report.

    Science.gov (United States)

    Williams, Samuel L.

    This report describes the development, implementation, and evaluation of a model for classroom observation designed to improve instructional supervisory skills and enhance teaching and learning. The project was carried out in 10 (Broward County, Florida) elementary schools with the principals and six teachers from each school involved. The aims of…

  5. 77 FR 20550 - Uniform Criteria for State Observational Surveys of Seat Belt Use

    Science.gov (United States)

    2012-04-05

    ... State Observational Surveys of Seat Belt Use AGENCY: National Highway Traffic Safety Administration... implementation date for use of the revised uniform criteria for State Observational Surveys of Seat Belt Use... Observational Surveys of Seat Belt Use.'' 76 FR 18042. That final rule amended the regulation...

  6. Predicting Student Achievement in University-Level Business and Economics Classes: Peer Observation of Classroom Instruction and Student Ratings of Teaching Effectiveness

    Science.gov (United States)

    Galbraith, Craig S.; Merrill, Gregory B.

    2012-01-01

    We examine the validity of peer observation of classroom instruction for purposes of faculty evaluation. Using both a multi-section course sample and a sample of different courses across a university's School of Business and Economics we find that the results of annual classroom observations of faculty teaching are significantly and positively…

  7. The role of children's ethnicity in the relationship between teacher ratings of attention-deficit/hyperactivity disorder and observed classroom behavior.

    Science.gov (United States)

    Epstein, Jeffrey N; Willoughby, Michael; Valencia, Elvia Y; Tonev, Simon T; Abikoff, Howard B; Arnold, L Eugene; Hinshaw, Stephen P

    2005-06-01

    Significant ethnic differences have been consistently documented on attention-deficit/hyperactivity disorder (ADHD) teacher rating scales. Whether these ethnic differences result from a teacher rating bias or reflect actual classroom behavior patterns is unknown. Ethnic differences between Caucasian and African American (AA) elementary schoolchildren on teacher ratings and codings of observed classroom behavior were examined with latent variables. In structural equation models, correlations between teacher ratings and observed classroom behavior suggested nonbiased teacher ratings of AA schoolchildren with diagnosed ADHD. Ethnic differences were documented for both teacher ratings of ADHD and classroom behavior. Differences in classroom behavior were attenuated when the behavior of an average child in the classroom was taken into account. Multiple explanations for this pattern of results are discussed.

  8. Survey of Galileo Plasma Observations in Jupiter's Plasma Sheet

    Science.gov (United States)

    Bagenal, Fran; Wilson, Robert J.; Siler, Scott; Paterson, William R.; Kurth, William S.

    2016-01-01

    The plasma science (PLS) Instrument on the Galileo spacecraft (orbiting Jupiter from December 1995 to September 2003) measured properties of the ions that were trapped in the magnetic field. The PLS data provide a survey of the plasma properties between approx. 5 and 30 Jupiter radii [R(sub J)] in the equatorial region. We present plasma properties derived via two analysis methods: numerical moments and forward modeling. We find that the density decreases with radial distance by nearly 5 orders of magnitude from approx. 2 to 3000 cm(exp.-3) at 6R(sub j) to approx. 0.05cm(sub -3) at 30 R(sub j). The density profile did not show major changes from orbit to orbit, suggesting that the plasma production and transport remained constant within about a factor of 2. The radial profile of ion temperature increased with distance which implied that contrary to the concept of adiabatic cooling on expansion, the plasma heats up as it expands out from Io's orbit (where TI is approx.60-80 eV) at approx. 6R(sub j) to a few keV at 30R(sub j).There does not seem to be a long-term, systematic variation in ion temperature with either local time or longitude. This latter finding differs from earlier analysis of Galileo PLS data from a selection of orbits. Further examination of all data from all Galileo orbits suggests that System Ill variations are transitory on timescales of weeks, consistent with the modeling of Cassini Ultraviolet Imaging Spectrograph observations. The plasma flow is dominated by azimuthal flow that is between 80% and 100% of corotation out to 25 R(sub j).

  9. Airborne Magnetic Trackline and Survey Data (Vector and Scalar Observations)

    Data.gov (United States)

    National Oceanic and Atmospheric Administration, Department of Commerce — The NOAA National Centers for Environmental Information (formerly National Geophysical Data Center) receive airborne magnetic survey data from US and non-US...

  10. Manifestations of Differential Cultural Capital in a University Classroom: Views from Classroom Observations and Focus Group Discussions in a South African University

    Directory of Open Access Journals (Sweden)

    Edmore Mutekwe

    2014-11-01

    Full Text Available Based predominantly on Pierre Bourdieu’s social and cultural reproduction theory, particularly his notions of cultural capital and symbolic violence, this paper explores how first year post graduate Diploma in Higher Education (PGDHE university students from diverse socio-linguistic backgrounds differ in the levels at which they understand and express themselves in classroom activities. The paper’s thesis is that the diverse nature of South African classrooms presents a number of challenges not only for students but also for educators in terms of the use of English as a medium of instruction or the language for learning and teaching (LOLT. Owing to the fact that the South African Language in Education Policy (LiEP of 1997 empowers both learners and educators in schools to use any of the eleven South African official languages as a LOLT wherever that is reasonably possible, students whose English backgrounds were deficient in enculturating them in the use of English as a learning tool often encounter challenges in expressing their ideas in the classroom, whether in writing or in oral presentations. The discussion is anchored in the data elicited through two data collection methods, lesson observations in a Diploma in Higher Education, Research class composed of students from diverse racial and ethnic backgrounds and through focus group discussion sessions with 40 multi-ethnic Diploma in Higher Education students from the same classroom. The data management and analysis for this study was done thematically, with views emerging from the observations and focus group discussions being clustered into superordinate themes for convenience of the discussion of the findings. The findings of this study were that students from affluent socio-economic backgrounds who enter university with a rich and relevant English linguistic capital, values and attitudes enjoy an enormous advantage compared to their counterparts whose social class and linguistic

  11. Further Insight into the Effectiveness of a Behavioral Teacher Program Targeting ADHD Symptoms Using Actigraphy, Classroom Observations and Peer Ratings

    Directory of Open Access Journals (Sweden)

    Betty Veenman

    2017-07-01

    Full Text Available Objective: The Positivity and Rules program (PR program, a low-level behavioral teacher program targeting symptoms of attention-deficit/hyperactivity disorder (ADHD, has shown positive effects on teacher-rated ADHD symptoms and social functioning. This study aimed to assess whether program effects could be confirmed by instruments assessing classroom behavior other than teacher-ratings, given teachers’ involvement with the training.Methods: Participants were 114 primary school children (age = 6–13 displaying ADHD symptoms in the classroom, who were randomly assigned to the treatment (n = 58 or control group (n = 65. ADHD symptoms were measured using classroom observations and actigraphy, and peer acceptance was measured using peer ratings. Intention-to-treat multilevel analyses were conducted to assess program effects.Results: No beneficial program effects were found for any of the measures.Conclusion: The earlier beneficial program effects on both ADHD symptoms and social functioning reported by teachers, may be explained by a change in the perception of teachers rather than changes in the child’s behavior. Other methodological explanations are also discussed, such as differences between instruments in the sensitivity to program-related changes. The current study underlines the importance of using different measures of classroom behavior to study program effects.ClinicalTrials.gov registration number: NCT02518711

  12. DUst around NEarby Stars. The survey observational results

    NARCIS (Netherlands)

    Eiroa, C.; Marshall, J. P.; Mora, A.; Montesinos, B.; Absil, O.; Augereau, J. Ch.; Bayo, A.; Bryden, G.; Danchi, W.; del Burgo, C.; Ertel, S.; Fridlund, M.; Heras, A. M.; Krivov, A. V.; Launhardt, R.; Liseau, R.; Loehne, T.; Maldonado, J.; Pilbratt, G. L.; Roberge, A.; Rodmann, J.; Sanz-Forcada, J.; Solano, E.; Stapelfeldt, K.; Thebault, P.; Wolf, S.; Ardila, D.; Arevalo, M.; Beichmann, C.; Faramaz, V.; Gonzalez-Garcia, B. M.; Gutierrez, R.; Lebreton, J.; Martinez-Arnaiz, R.; Meeus, G.; Montes, D.; Olofsson, G.; Su, K. Y. L.; White, G. J.; Barrado, D.; Fukagawa, M.; Gruen, E.; Kamp, I.; Lorente, R.; Morbidelli, A.; Mueller, S.; Mutschke, H.; Nakagawa, T.; Ribas, I.; Walker, H.

    2013-01-01

    Context. Debris discs are a consequence of the planet formation process and constitute the fingerprints of planetesimal systems. Their solar system counterparts are the asteroid and Edgeworth-Kuiper belts. Aims: The DUNES survey aims at detecting extra-solar analogues to the Edgeworth-Kuiper belt ar

  13. Advancing the discussion about systematic classroom behavioral observation, a product review of Tenny, J. (2010). eCOVE observation software. Pacific City, OR: eCOVE Software, LLC.

    Science.gov (United States)

    Froiland, John Mark; Smith, Liana

    2014-05-01

    Applied child psychologists and behavioral consultants often use systematic behavioral observations to inform the psychological assessment and intervention development process for children referred for attention and hyperactivity problems. This article provides a review of the 2010 version of the eCOVE classroom observation software in terms of its utility in tracking the progress of children with attention and hyperactive behaviors and its use in evaluating teacher behaviors that may impede or promote children's attention and positive behavior. The eCOVE shows promise as an efficient tool for psychologists and behavioral consultants who want to evaluate the effects of interventions for children with symptoms of ADHD, ODD, mood disorders and learning disorders; however, some research-based improvements for future models are suggested. The reviewers also share their firsthand experience in using eCOVE to evaluate teacher and student behavior exhibited on a television show about teaching urban high school students and during a movie about an eccentric new kindergarten teacher. Rich examples are provided of using strategic behavioral observations to reveal how to improve the classroom environment so as to facilitate attention, motivation and positive behavior among youth. Broader implications for enhancing the use of systematic behavioral observations in the assessment of children and adolescents with attention disorders and related behavioral problems are discussed. Key issues are examined such as the use of behavioral observations during psychological consultation to prevent the previously found gender bias in referrals for ADHD. Using behavioral observations to enhance differential diagnosis is also discussed.

  14. Subaru Deep Survey I. Near-Infrared Observations

    CERN Document Server

    Maihara, T; Tanabe, H; Taguchi, T; Hata, R; Oya, S; Kashikawa, N; Iye, M; Miyazaki, S; Karoji, H; Yoshida, M; Totani, T; Yoshii, Y; Okamura, S; Shimasaku, K; Saitô, Y; Ando, H; Goto, M; Hayashi, M; Kaifu, N; Kobayashi, N; Kosugi, G; Motohara, K; Nishimura, T; Noumaru, J; Ogasawara, R; Sasaki, T; Sekiguchi, K; Takata, T; Terada, H; Yamashita, T; Usuda, T; Tokunaga, A T

    2000-01-01

    Deep near-infrared images of a blank 2'x2' section of sky near the Galactic north pole taken by Subaru Telescope are presented. The total integration times of the J and K' bands are 12.1 hours and 9.7 hours, resulting in 5-sigma limiting magnitudes of 25.1 and 23.5 mag, respectively. The numbers of sources within these limiting magnitudes found with an automated detection procedure are 385 in the J band and 350 in K'. Based on photometric measurements of these sources, we present number count vs. magnitude relations, color vs. magnitude diagrams, size vs. color relationships, etc. The slope of the galaxy number count plotted against the AB magnitude scale is about 0.23 in the 22 to 26 AB magnitude range of both bands. The spatial number density of galaxies as well as the slopes in the faint-end region given by the Subaru Deep Field (SDF) survey is consistent with those given by HST-NICMOS surveys as expressed on the AB magnitude diagram. Several sources having very large J-K' color are found including a few K...

  15. DA WHITE DWARFS OBSERVED IN THE LAMOST PILOT SURVEY

    Energy Technology Data Exchange (ETDEWEB)

    Zhang Yueyang; Deng Licai; Liu Chao; Carrell, Kenneth; Yang Fan; Gao Shuang; Xu Yan; Li Jing; Zhang Haotong; Zhao Yongheng; Luo Ali; Bai Zhongrui; Yuan Hailong [Key Lab for Optical Astronomy, National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100012 (China); Lepine, Sebastien [Department of Astrophysics, Division of Physical Sciences, American Museum of Natural History, Central Park West at 79th Street, New York, NY (United States); Newberg, Heidi Jo; Carlin, Jeffrey L. [Department of Physics, Applied Physics and Astronomy, Rensselaer Polytechnic Institute, 110 8th Street, Troy, NY 12180 (United States); Jin Ge [University of Science and Technology of China, Hefei 230026 (China)

    2013-08-01

    A total of {approx}640, 000 objects from the LAMOST pilot survey have been publicly released. In this work, we present a catalog of DA white dwarfs (DAWDs) from the entire pilot survey. We outline a new algorithm for the selection of white dwarfs (WDs) by fitting Sersic profiles to the Balmer H{beta}, H{gamma}, and H{delta} lines of the spectra, and calculating the equivalent width of the Ca II K line. Two thousand nine hundred sixty-four candidates are selected by constraining the fitting parameters and the equivalent width of the Ca II K line. All the spectra of candidates are visually inspected. We identify 230 DAWDs (59 of which are already included in the Villanova and SDSS WD catalogs), 20 of which are DAWDs with non-degenerate companions. In addition, 128 candidates are classified as DAWDs/subdwarfs, which means the classifications are ambiguous. The result is consistent with the expected DAWD number estimated based on the LEGUE target selection algorithm.

  16. PROBING THE EARLY UNIVERSE WITH DEEP OBSERVATIONS AND LARGE SURVEYS

    Institute of Scientific and Technical Information of China (English)

    Zheng Wei

    2001-01-01

    Recent advances in astronomy have enabled scientists to reach the early universe to an unprecedented depth. With the new telescopes such as the Chandra, FUSE, and with the Sloan Digital Sky Survey (SDSS), we have gained critical insights into the “Origin of our Universe”, i.e. how the intergalactic medium evolves to form galaxies and quasars. SDSS has broken a ten-year barrier of z = 5 to reach the very early universe, with the discovery of five quasars at z ≥ 5. 0. The survey will find more than ten thousands of quasars, enabling us to carry out the most comprehensive classification of quasars. FUSE finds traces of the primordial matter at z ~ 3, which corresponds to hydrogen column density as low as 10-11 cm-2 and cannot be detected even with the largest optical telescope. The finding suggests that the intergalactic medium is an evolving and complex entity, and it is ionized mainly by the accumulated radiation from quasars. The Chandra telescope has taken a million second deep exposure of a selected region,reaching about twenty times deeper than ROSAT to a limiting flux of 5 × 1 0-17 ergs s-1 cm-2 in the 0. 5-2 keV band. The sources found so far can account for up to 90 % of the hard X-ray background field, and they consist of Seyfert-2 and normal galaxies at z < 1 and quasars at z < 4.5. In the near future, the Next Generation Space Telescope and others will reveal the first generation of baryonic objects after the Big Bang.

  17. A Survey of Attitudes on the Use of Calculators in the College Classroom.

    Science.gov (United States)

    Bukowski, Joseph E.

    This study focused on faculty and student attitudes toward the use of calculators in college accounting and business mathematics courses. Two different surveys were used; one was administered to thirty-five full-time and part-time faculty in the accounting and business mathematics areas at one college, while a second survey was administered to a…

  18. The DEEP2 Galaxy Redshift Survey: Design, Observations, Data Reduction, and Redshifts

    OpenAIRE

    Newman, Jeffrey A.; Kassin, Susan A.; Noeske, K. G.; Lotz, Jennifer M.

    2013-01-01

    We describe the design and data analysis of the DEEP2 Galaxy Redshift Survey, the densest and largest high-precision redshift survey of galaxies at z ~ 1 completed to date. The survey was designed to conduct a comprehensive census of massive galaxies, their properties, environments, and large-scale structure down to absolute magnitude M_B = −20 at z ~ 1 via ~90 nights of observation on the Keck telescope. The survey covers an area of 2.8 deg^2 divided into four separate fields observed to a l...

  19. The Sloan Digital Sky Survey-II Supernova Survey:Search Algorithm and Follow-up Observations

    Energy Technology Data Exchange (ETDEWEB)

    Sako, Masao; /Pennsylvania U. /KIPAC, Menlo Park; Bassett, Bruce; /Cape Town U. /South African Astron. Observ.; Becker, Andrew; /Washington U., Seattle, Astron. Dept.; Cinabro, David; /Wayne State U.; DeJongh, Don Frederic; /Fermilab; Depoy, D.L.; /Ohio State U.; Doi, Mamoru; /Tokyo U.; Garnavich, Peter M.; /Notre Dame U.; Craig, Hogan, J.; /Washington U., Seattle, Astron. Dept.; Holtzman, Jon; /New Mexico State U.; Jha, Saurabh; /Stanford U., Phys. Dept.; Konishi, Kohki; /Tokyo U.; Lampeitl, Hubert; /Baltimore, Space; Marriner, John; /Fermilab; Miknaitis, Gajus; /Fermilab; Nichol, Robert C.; /Portsmouth U.; Prieto, Jose Luis; /Ohio State U.; Richmond, Michael W.; /Rochester Inst.; Schneider, Donald P.; /Penn State U., Astron. Astrophys.; Smith, Mathew; /Portsmouth U.; SubbaRao, Mark; /Chicago U. /Tokyo U. /Tokyo U. /South African Astron. Observ. /Tokyo

    2007-09-14

    The Sloan Digital Sky Survey-II Supernova Survey has identified a large number of new transient sources in a 300 deg2 region along the celestial equator during its first two seasons of a three-season campaign. Multi-band (ugriz) light curves were measured for most of the sources, which include solar system objects, Galactic variable stars, active galactic nuclei, supernovae (SNe), and other astronomical transients. The imaging survey is augmented by an extensive spectroscopic follow-up program to identify SNe, measure their redshifts, and study the physical conditions of the explosions and their environment through spectroscopic diagnostics. During the survey, light curves are rapidly evaluated to provide an initial photometric type of the SNe, and a selected sample of sources are targeted for spectroscopic observations. In the first two seasons, 476 sources were selected for spectroscopic observations, of which 403 were identified as SNe. For the Type Ia SNe, the main driver for the Survey, our photometric typing and targeting efficiency is 90%. Only 6% of the photometric SN Ia candidates were spectroscopically classified as non-SN Ia instead, and the remaining 4% resulted in low signal-to-noise, unclassified spectra. This paper describes the search algorithm and the software, and the real-time processing of the SDSS imaging data. We also present the details of the supernova candidate selection procedures and strategies for follow-up spectroscopic and imaging observations of the discovered sources.

  20. Observing efl classrooms in primary or secondary schools: a research task in applied linguistics Observing efl classrooms in primary or secondary schools: a research task in applied linguistics

    Directory of Open Access Journals (Sweden)

    Viviane Heberle

    2008-04-01

    Full Text Available Neste trabalho, com base em princípios da gramática funcional de Halliday e de análise crítica do discurso, bem como minha experiência em Lingüística Aplicada, discuto questões relacionadas à observação de aulas de inglês como língua estrangeira. A análise (de cunho etnográfico surge de discussões nas minhas aulas de Lingüística Aplicada e de relatos de alunos sobre as aulas observadas. O estudo visa contribuir para uma conscientização da relevância de uma prática educacional que vai além de, por exemplo, mera listagem de pronomes pessoais com as formas do verbo to be, para uma discussão de tópicos que possam, de alguma forma, integrar perspectivas socioculturais na educação de professores de inglês como língua estrangeira. In this paper, based on principles of systemic-functional grammar and critical discourse analysis, as well as on my experience as a teacher of Applied Linguistics, I discuss issues related to the observation of EFL classes. The analysis (qualitative, ethnographically-based arises from discussions in my Applied Linguistics course and students’ reports on the classes they observed. The study aims at contributing to an awareness of the relevance of an educational practice that goes beyond the mere listing of personal pronouns with the corresponding forms of the verb to be, for instance, and suggests a discussion of topics which could somehow integrate sociocultural perspectives into EFL teacher education.

  1. 75 FR 4509 - Uniform Criteria for State Observational Surveys of Seat Belt Use

    Science.gov (United States)

    2010-01-28

    ... Observational Surveys of Seat Belt Use AGENCY: National Highway Traffic Safety Administration (NHTSA... amendments to the regulations establishing the criteria for designing and conducting State seat belt use... seat belt use rates to NHTSA. NHTSA proposes these amendments so that future surveys will give...

  2. Collaboration Between Astronomers at UT Austin and K-12 Teachers: Connecting the Experience of Observing and Research with the Classroom

    Science.gov (United States)

    Finkelstein, Keely D.; Sneden, Christopher; Hemenway, Mary Kay; Preston, Sandra; EXES Teachers Associate Program

    2015-01-01

    McDonald Observatory has a long history of providing teacher professional development (PD), and recently we have developed a new workshop model for more advanced participants. By choosing a select group of middle and high school teachers from those previously involved in our past PD programs, we have created a joint workshop / observing run program for them. After traveling to the observatory, the teachers participate in an actual observing run with a research astronomer. The teachers are trained first-hand how to take observations, operate the telescope, set up the instrument, and monitor observing conditions. The teachers are fully put in the role of observer. They are also given background information before and during the workshop related to the science and data they are helping to collect. The teachers work in teams to both perform the nightly observations with an astronomer, but to also perform new interactive classroom activities with education staff, and use other telescopes on the mountain. This is a unique experience for teachers since it allows them to take the resources and experiences directly back to their classrooms and students. They can directly relate to their students what skills for specific careers in STEM fields are needed. Evaluation from these workshops shows that there is: increased content knowledge among participants, greater impact that will be passed on to their students, and an authentic research experience that can't be replicated in other PD settings. In addition, not only is this program beneficial to the teachers, but this group is benefit to the education program of McDonald Observatory. Building on an existing PD program (with a 16 year history) we have the opportunity to test out new products and new education endeavors with this devoted group of well-trained teachers before bringing them to wider teacher and student audiences. This program is currently supported by the NSF grant AST-1211585 (PI Sneden).

  3. Counseling Instruction in the Online Classroom: A Survey of Student and Faculty Perceptions

    Science.gov (United States)

    Cicco, Gina

    2012-01-01

    This article will review the design, procedures, and results of a recent study conducted to survey the perceptions of counseling students and professionals regarding the delivery of counseling instruction in online courses. Few studies have addressed the appropriateness, effectiveness, and evaluation procedures of counseling skills instruction via…

  4. Third and Fourth Grade Teacher's Classroom Practices in Writing: A National Survey

    Science.gov (United States)

    Brindle, Mary; Graham, Steve; Harris, Karen R.; Hebert, Michael

    2016-01-01

    A random sample of teachers in grades 3 and 4 (N = 157) from across the United States were surveyed about their use of evidence-based writing practices, preparation to teach writing, and beliefs about writing. Teachers' beliefs included their efficacy to teach writing, their orientations to teach writing, their attitude about teaching writing, and…

  5. Surveying Instruments: Their History and Classroom Use. National Council of Teachers of Mathematics, Yearbook 19 [1947].

    Science.gov (United States)

    Kiely, Edmond R.

    The first four chapters trace the history of surveying instruments from beginnings in Egypt, China, and Babylonia to Greece and Rome, then Europe, Islam, and India and finally in the Renaissance in Europe. The organization of these chapters is generally by the major areas of leveling instruments, right-angle instruments, staff combinations, and…

  6. Pacific Remote Islands MNM: Initial Survey Instructions for Terrestrial Plant Observations

    Data.gov (United States)

    US Fish and Wildlife Service, Department of the Interior — The purpose of the terrestrial plant observations survey is to document vegetation species presence/absence and distribution on the island unit of the refuge. The...

  7. The Lunar Occultation Observer (LOCO) -- A Nuclear Astrophysics All-Sky Survey Mission Concept

    Science.gov (United States)

    Miller, R. S.; Bonamente, M.; Burgess, J. M.; Jenke, P.; Lawrence, D. J.; O'Brien, S.; Orr, M. R.; Paciesas, W. S.; Young, C. A.

    2009-03-01

    The Lunar Occultation Observer (LOCO) is a new γ-ray astrophysics mission concept expected to have unprecedented sensitivity in the nuclear regime. Operating in lunar orbit, LOCO will utilize lunar occultation imaging to survey and probe the cosmos.

  8. Initial validation of the prekindergarten Classroom Observation Tool and goal setting system for data-based coaching.

    Science.gov (United States)

    Crawford, April D; Zucker, Tricia A; Williams, Jeffrey M; Bhavsar, Vibhuti; Landry, Susan H

    2013-12-01

    Although coaching is a popular approach for enhancing the quality of Tier 1 instruction, limited research has addressed observational measures specifically designed to focus coaching on evidence-based practices. This study explains the development of the prekindergarten (pre-k) Classroom Observation Tool (COT) designed for use in a data-based coaching model. We examined psychometric characteristics of the COT and explored how coaches and teachers used the COT goal-setting system. The study included 193 coaches working with 3,909 pre-k teachers in a statewide professional development program. Classrooms served 3 and 4 year olds (n = 56,390) enrolled mostly in Title I, Head Start, and other need-based pre-k programs. Coaches used the COT during a 2-hr observation at the beginning of the academic year. Teachers collected progress-monitoring data on children's language, literacy, and math outcomes three times during the year. Results indicated a theoretically supported eight-factor structure of the COT across language, literacy, and math instructional domains. Overall interrater reliability among coaches was good (.75). Although correlations with an established teacher observation measure were small, significant positive relations between COT scores and children's literacy outcomes indicate promising predictive validity. Patterns of goal-setting behaviors indicate teachers and coaches set an average of 43.17 goals during the academic year, and coaches reported that 80.62% of goals were met. Both coaches and teachers reported the COT was a helpful measure for enhancing quality of Tier 1 instruction. Limitations of the current study and implications for research and data-based coaching efforts are discussed.

  9. VALIDATION OF OBSERVATIONS OBTAINED WITH A LIQUID MIRROR TELESCOPE BY COMPARISON WITH SLOAN DIGITAL SKY SURVEY OBSERVATIONS

    Energy Technology Data Exchange (ETDEWEB)

    Borra, E. F. [Centre d’Optique, Photonique et Lasers Département de Physique, Université Laval (Canada)

    2015-06-15

    The results of a search for peculiar astronomical objects using very low resolution spectra obtained with the NASA Orbital Debris Observatory (NODO) 3 m diameter liquid mirror telescope (LMT) are compared with results of spectra obtained with the Sloan Digital Sky Survey (SDSS). The main purpose of this comparison is to verify whether observations taken with this novel type of telescope are reliable. This comparison is important because LMTs are an inexpensive novel type of telescope that is very useful for astronomical surveys, particularly surveys in the time domain, and validation of the data taken with an LMT by comparison with data from a classical telescope will validate their reliability. We start from a published data analysis that classified as peculiar only 206 of the 18,000 astronomical objects observed with the NODO LMT. A total of 29 of these 206 objects were found in the SDSS. The reliability of the NODO data can be seen through the results of the detailed analysis that, in practice, incorrectly identified less than 0.3% of the 18,000 spectra as peculiar objects, most likely because they are variable stars. We conclude that the LMT gave reliable observations, comparable to those that would have been obtained with a telescope using a glass mirror.

  10. Predictive validity of the classroom strategies scale-observer form on statewide testing scores: an initial investigation.

    Science.gov (United States)

    Reddy, Linda A; Fabiano, Gregory A; Dudek, Christopher M; Hsu, Louis

    2013-12-01

    The present study examined the validity of a teacher observation measure, the Classroom Strategies Scale--Observer Form (CSS), as a predictor of student performance on statewide tests of mathematics and English language arts. The CSS is a teacher practice observational measure that assesses evidence-based instructional and behavioral management practices in elementary school. A series of two-level hierarchical generalized linear models were fitted to data of a sample of 662 third- through fifth-grade students to assess whether CSS Part 2 Instructional Strategy and Behavioral Management Strategy scale discrepancy scores (i.e., ∑ |recommended frequency--frequency ratings|) predicted statewide mathematics and English language arts proficiency scores when percentage of minority students in schools was controlled. Results indicated that the Instructional Strategy scale discrepancy scores significantly predicted mathematics and English language arts proficiency scores: Relatively larger discrepancies on observer ratings of what teachers did versus what should have been done were associated with lower proficiency scores. Results offer initial evidence of the predictive validity of the CSS Part 2 Instructional Strategy discrepancy scores on student academic outcomes.

  11. PORTAAL: A Classroom Observation Tool Assessing Evidence-Based Teaching Practices for Active Learning in Large Science, Technology, Engineering, and Mathematics Classes

    Science.gov (United States)

    Eddy, Sarah L.; Converse, Mercedes; Wenderoth, Mary Pat

    2015-01-01

    There is extensive evidence that active learning works better than a completely passive lecture. Despite this evidence, adoption of these evidence-based teaching practices remains low. In this paper, we offer one tool to help faculty members implement active learning. This tool identifies 21 readily implemented elements that have been shown to increase student outcomes related to achievement, logic development, or other relevant learning goals with college-age students. Thus, this tool both clarifies the research-supported elements of best practices for instructor implementation of active learning in the classroom setting and measures instructors’ alignment with these practices. We describe how we reviewed the discipline-based education research literature to identify best practices in active learning for adult learners in the classroom and used these results to develop an observation tool (Practical Observation Rubric To Assess Active Learning, or PORTAAL) that documents the extent to which instructors incorporate these practices into their classrooms. We then use PORTAAL to explore the classroom practices of 25 introductory biology instructors who employ some form of active learning. Overall, PORTAAL documents how well aligned classrooms are with research-supported best practices for active learning and provides specific feedback and guidance to instructors to allow them to identify what they do well and what could be improved. PMID:26033871

  12. A double-observer method to estimate detection rate during aerial waterfowl surveys

    Science.gov (United States)

    Koneff, M.D.; Royle, J. Andrew; Otto, M.C.; Wortham, J.S.; Bidwell, J.K.

    2008-01-01

    We evaluated double-observer methods for aerial surveys as a means to adjust counts of waterfowl for incomplete detection. We conducted our study in eastern Canada and the northeast United States utilizing 3 aerial-survey crews flying 3 different types of fixed-wing aircraft. We reconciled counts of front- and rear-seat observers immediately following an observation by the rear-seat observer (i.e., on-the-fly reconciliation). We evaluated 6 a priori models containing a combination of several factors thought to influence detection probability including observer, seat position, aircraft type, and group size. We analyzed data for American black ducks (Anas rubripes) and mallards (A. platyrhynchos), which are among the most abundant duck species in this region. The best-supported model for both black ducks and mallards included observer effects. Sample sizes of black ducks were sufficient to estimate observer-specific detection rates for each crew. Estimated detection rates for black ducks were 0.62 (SE = 0.10), 0.63 (SE = 0.06), and 0.74 (SE = 0.07) for pilot-observers, 0.61 (SE = 0.08), 0.62 (SE = 0.06), and 0.81 (SE = 0.07) for other front-seat observers, and 0.43 (SE = 0.05), 0.58 (SE = 0.06), and 0.73 (SE = 0.04) for rear-seat observers. For mallards, sample sizes were adequate to generate stable maximum-likelihood estimates of observer-specific detection rates for only one aerial crew. Estimated observer-specific detection rates for that crew were 0.84 (SE = 0.04) for the pilot-observer, 0.74 (SE = 0.05) for the other front-seat observer, and 0.47 (SE = 0.03) for the rear-seat observer. Estimated observer detection rates were confounded by the position of the seat occupied by an observer, because observers did not switch seats, and by land-cover because vegetation and landform varied among crew areas. Double-observer methods with on-the-fly reconciliation, although not without challenges, offer one viable option to account for detection bias in aerial waterfowl

  13. Follow-Up Discovery Channel Telescope Observations of Transients and Variables from Optical Time Domain Surveys

    Science.gov (United States)

    Gezari, Suvi; Liu, Tingting; Hung, Tiara

    2017-01-01

    We highlight the capabilities of the Discovery Channel Telescope (DCT) for follow-up observations of transients and variables discovered by optical time-domain surveys. We present two DCT programs: 1) extended-baseline imaging with the Large Monolithic Imager of periodically variable quasars from the Pan-STARRS1 survey to identify binary supermassive black hole candidates, and 2) spectroscopic classification with the DeVeny spectrograph of nuclear transients from the iPTF survey to identify tidal disruption event candidates. We demonstrate that DCT is well-matched to the magnitude ranges of the transients and variables discovered by these surveys, and has played an important role in their classification and characterization.

  14. Efficient scheduling of astronomical observations. Application to the CARMENES radial-velocity survey

    Science.gov (United States)

    Garcia-Piquer, A.; Morales, J. C.; Ribas, I.; Colomé, J.; Guàrdia, J.; Perger, M.; Caballero, J. A.; Cortés-Contreras, M.; Jeffers, S. V.; Reiners, A.; Amado, P. J.; Quirrenbach, A.; Seifert, W.

    2017-08-01

    Context. Targeted spectroscopic exoplanet surveys face the challenge of maximizing their planet detection rates by means of careful planning. For a large planet survey, the number of possible observation combinations, i.e., the sequence of observations night after night, both in total time and amount of targets, is enormous. Aims: Sophisticated scheduling tools and the improved understanding of the exoplanet population are employed to investigate an efficient and optimal way to plan the execution of observations. This is applied to the CARMENES instrument, which is an optical and infrared high-resolution spectrograph that has started a survey of about 300 M-dwarf stars in search of terrestrial exoplanets. Methods: We used evolutionary computation techniques to create an automatic scheduler that minimizes the idle periods of the telescope and distributes the observations among all the targets using configurable criteria. We simulated the case of the CARMENES survey with a realistic sample of targets, and we estimated the efficiency of the planning tool both in terms of telescope operations and planet detection. Results: Our scheduling simulations produce plans that use about 99% of the available telescope time (including overheads) and optimally distribute the observations among the different targets. Under such conditions, and using current planet statistics, the optimized plan using this tool should allow the CARMENES survey to discover about 65% of the planets with radial-velocity semi-amplitudes greater than 1 ms-1 when considering only photon noise. Conclusions: The simulations using our scheduling tool show that it is possible to optimize the survey planning by minimizing idle instrument periods and fulfilling the science objectives in an efficient manner to maximize the scientific return.

  15. At-sea aerial survey species observations in southern California, 1999-2002

    Data.gov (United States)

    U.S. Geological Survey, Department of the Interior — Broad survey lines, island radial survey lines, coastal survey lines, and focal-area (Santa Barbara Channel) survey lines were surveyed during each oceanographic...

  16. The LEGUE input catalog for dark night observing in the LAMOST pilot survey

    Institute of Scientific and Technical Information of China (English)

    Fan Yang; Jin-Liang Hou; Xiao-Wei Liu; Norbert Christlieb; Hao-Tong Zhang; Hsu-Tai Lee; Kai-Ke Pan; Zhan-Wen Han; Hong-Chi Wang; Jeffrey L.Carlin; Chao Liu; Yue-Yang Zhang; Shuang Gao; Yan Xu; Li-Cai Deng; Heidi Jo Newberg; Sébastien Lépine

    2012-01-01

    We outline the design of the dark nights portion of the LAMOST Pilot Survey,which began observations in 2011 October.In particular,we focus on Milky Way stellar candidates that are targeted for the LEGUE(LAMOST Experiment for Galactic Understanding and Exploration)survey.We discuss the regions of sky in which spectroscopic candidates were selected,and the motivations for selecting each of these sky areas.Some limitations due to the unique design of the telescope are discussed,including the requirement that a bright(V < 8)star be placed at the center of each plate for wavefront sensing and active optics corrections.The target selection categories and scientific goals motivating them are briefly discussed,followed by a detailed overview of how these selection functions were implemented.We illustrate the difference between the overall input catalog-Sloan Digital Sky Survey(SDSS)photometry-and the final targets selected for LAMOST observations.

  17. Enabling and Supporting Remote Classroom Teaching Observation: Live Video Conferencing Uses in Initial Teacher Education

    Science.gov (United States)

    Wang, Ruolan; Wiesemes, Rolf

    2012-01-01

    In this paper the authors present findings from a small-scale study in order to extend their understanding of using live video conferencing in initial teacher education. Four distinct steps, consisting of observation, contextualisation, reflection and development of personal practices, were identified based on an in-depth focus group interview.…

  18. Tale of the Tape: International Teaching Assistant Noticing during Videotaped Classroom Observations

    Science.gov (United States)

    Williams, Gwendolyn M.; Case, Rod E.

    2015-01-01

    International teaching assistants face challenges in learning the norms for teaching in American universities. In order to address this learning curve this article describes a qualitative study of twenty international teaching assistants that examined how these participants viewed observations as part of their professional development. The study…

  19. Once is not enough : Establishing reliability criteria for feedback and evaluative decsions based on classroom observation

    NARCIS (Netherlands)

    van der Lans, Rikkert M.; van de Grift, Wim J.C.M.; van Veen, Klaas; Fokkens-Bruinsma, Marjon

    2016-01-01

    Implementation of effective teacher evaluation procedures is a global challenge in which lowering the chances that teachers receive inaccurate evaluations is a pertinent goal. This study investigates the minimum number of observations required to guarantee that teachers receive feedback with modest

  20. Survey on methods of increasing the efficiency of extended state disturbance observers.

    Science.gov (United States)

    Madoński, R; Herman, P

    2015-05-01

    This survey presents various methods of improving the overall estimation quality in the class of extended state observers (ESO), which estimate not only the conventional states of the system, but the acting disturbance as well. This type of observers is crucial in forming the active disturbance rejection control structure (ADRC), where the precision of online perturbation reconstruction and cancellation directly influences the robustness of the closed-loop control system. Various aspects of the observer-based disturbance estimation/rejection loop are covered by this work and divided into three categories, related with observer: structure, tuning, and working conditions. The survey is dedicated to researchers and practitioners who are interested in increasing the efficiency of their ADRC-based governing schemes.

  1. Observations of adolescent peer resistance skills following a classroom-based healthy relationship program: a post-intervention comparison.

    Science.gov (United States)

    Wolfe, David A; Crooks, Claire V; Chiodo, Debbie; Hughes, Raymond; Ellis, Wendy

    2012-04-01

    This study examines peer resistance skills following a 21-lesson classroom-based intervention to build healthy relationships and decrease abusive and health-risk behaviors among adolescents. The Fourth R instructs students in positive relationship skills, such as negotiation and delay, for navigating challenging peer and dating scenarios. Observational data from 196 grade 9 students participating in a larger cluster randomized controlled trial were used to evaluate post-intervention acquisition of peer resistance skills. Pairs of students engaged in a role play paradigm with older student actors, where they were subjected to increasing pressure to comply with peer requests related to drugs and alcohol, bullying, and sexual behavior. Specific and global measures of change in peer resistance responses were obtained from two independent sets of observers, blinded to condition. Specific peer resistance responses (negotiation, delay, yielding to pressure, refusal, and compliance) were coded by research assistants; global peer resistance responses were rated by teachers from other schools (thinking / inquiry, application, communication, and perceived efficacy). Students who received the intervention were more likely to demonstrate negotiation skills and less likely to yield to negative pressure relative to controls. Intervention students were also more likely to use delay than controls; control girls were more likely to use refusal responses; the number of times students complied with peer requests did not differ. Teacher ratings demonstrated significant main effects favoring intervention youth on all measures. Program and research implications are highlighted.

  2. The XXL Survey: I. Scientific motivations - XMM-Newton observing plan - Follow-up observations and simulation programme

    CERN Document Server

    Pierre, M; Adami, C; Alis, S; Altieri, B; Baran, B; Benoist, C; Birkinshaw, M; Bongiorno, A; Bremer, M N; Brusa, M; Butler, A; Ciliegi, P; Chiappetti, L; Clerc, N; Corasaniti, P S; Coupon, J; De Breuck, C; Democles, J; Desai, S; Delhaize, J; Devriendt, J; Dubois, Y; Eckert, D; Elyiv, A; Ettori, S; Evrard, A; Faccioli, L; Farahi, A; Ferrari, C; Finet, F; Fotopoulou, S; Fourmanoit, N; Gandhi, P; Gastaldello, F; Gastaud, R; Georgantopoulos, I; Giles, P; Guennou, L; Guglielmo, V; Horellou, C; Husband, K; Huynh, M; Iovino, A; Kilbinger, M; Koulouridis, E; Lavoie, S; Brun, A M C Le; Fevre, J P Le; Lidman, C; Lieu, M; Lin, C A; Mantz, A; Maughan, B J; Maurogordato, S; McCarthy, I G; McGee, S; Melin, J B; Melnyk, O; Menanteau, F; Novak, M; Paltani, S; Plionis, M; Poggianti, B M; Pomarede, D; Pompei, E; Ponman, T J; Ramos-Ceja, M E; Ranalli, P; Rapetti, D; Raychaudury, S; Reiprich, T H; Rottgering, H; Rozo, E; Rykoff, E; Sadibekova, T; Santos, J; Sauvageot, J L; Schimd, C; Sereno, M; Smith, G P; Smolčić, V; Snowden, S; Spergel, D; Stanford, S; Surdej, J; Valageas, P; Valotti, A; Valtchanov, I; Vignali, C; Willis, J; Ziparo, F

    2015-01-01

    We present the XXL Survey, the largest XMM programme totaling some 6.9 Ms to date and involving an international consortium of roughly 100 members. The XXL Survey covers two extragalactic areas of 25 deg2 each at a point-source sensitivity of ~ 5E-15 erg/sec/cm2 in the [0.5-2] keV band (completeness limit). The survey's main goals are to provide constraints on the dark energy equation of state from the space-time distribution of clusters of galaxies and to serve as a pathfinder for future, wide-area X-ray missions. We review science objectives, including cluster studies, AGN evolution, and large-scale structure, that are being conducted with the support of approximately 30 follow-up programmes. We describe the 542 XMM observations along with the associated multi-lambda and numerical simulation programmes. We give a detailed account of the X-ray processing steps and describe innovative tools being developed for the cosmological analysis. The paper provides a thorough evaluation of the X-ray data, including qua...

  3. Naturalistic Observations of Nonverbal Children with Autism: A Study of Intentional Communicative Acts in the Classroom

    Directory of Open Access Journals (Sweden)

    Samantha Drain

    2013-01-01

    Full Text Available We examined evoked and spontaneous communicative acts in six nonverbal children with autism (10–15 years, M = 12.8, SD = 2.1. All participants attended the same special school for children with autism but were in different classes. Each was observed for 30 minutes during a typical school day. An observer coded the presence/absence of an antecedent, the form and function of the communicative act, and the teacher’s response to the child. One hundred and fifty-five communicative acts were observed, 41% were spontaneous and 59% were evoked. The main antecedents to evoked communicative acts were verbal prompts, and most of the evoked communicative acts were physical in nature (i.e., motor acts and gestures. However, verbalizations and the use of the Picture Exchange Communication System (PECS were higher for spontaneous communicative acts. The functions of spontaneous communicative acts were primarily requests. Results showed a substantial number of “nonresponses” from teachers, even following evoked communicative acts. These results suggest that teachers may not actively promote intentional communication as much as possible. Therefore, our findings provide information concerning ways in which educators could facilitate intentional communication in non-verbal children with autism.

  4. Detection and plant monitoring programs: lessons from an intensive survey of Asclepias meadii with five observers.

    Science.gov (United States)

    Alexander, Helen M; Reed, Aaron W; Kettle, W Dean; Slade, Norman A; Bodbyl Roels, Sarah A; Collins, Cathy D; Salisbury, Vaughn

    2012-01-01

    Monitoring programs, where numbers of individuals are followed through time, are central to conservation. Although incomplete detection is expected with wildlife surveys, this topic is rarely considered with plants. However, if plants are missed in surveys, raw count data can lead to biased estimates of population abundance and vital rates. To illustrate, we had five independent observers survey patches of the rare plant Asclepias meadii at two prairie sites. We analyzed data with two mark-recapture approaches. Using the program CAPTURE, the estimated number of patches equaled the detected number for a burned site, but exceeded detected numbers by 28% for an unburned site. Analyses of detected patches using Huggins models revealed important effects of observer, patch state (flowering/nonflowering), and patch size (number of stems) on probabilities of detection. Although some results were expected (i.e. greater detection of flowering than nonflowering patches), the importance of our approach is the ability to quantify the magnitude of detection problems. We also evaluated the degree to which increased observer numbers improved detection: smaller groups (3-4 observers) generally found 90 - 99% of the patches found by all five people, but pairs of observers or single observers had high error and detection depended on which individuals were involved. We conclude that an intensive study at the start of a long-term monitoring study provides essential information about probabilities of detection and what factors cause plants to be missed. This information can guide development of monitoring programs.

  5. The Arecibo Galaxy Environment Survey: Precursor Observations of the NGC 628 group

    CERN Document Server

    Auld, R; Davies, J I; Catinella, B; Henning, P A; Linder, S; Momjian, E; Müller, E; O'Neil, K; Sabatini, S; Schneider, S; Bothun, G; Cortese, L; Disney, M; Hoffman, G L; Putman, M; Rosenberg, J L; Baes, M; De Blok, W J G; Boselli, A; Brinks, E; Brosch, N; Irwin, J; Karachentsev, I D; Kilborn, V A; Koribalski, B; Spekkens, K

    2006-01-01

    The Arecibo Galaxy Environment Survey (AGES) is one of several HI surveys utilising the new Arecibo L-band Feed Array (ALFA) fitted to the 305m radio telescope at Arecibo. The survey is specifically designed to investigate various galactic environments to higher sensitivity, higher velocity resolution and higher spatial resolution than previous fully sampled, 21 cm multibeam surveys. The emphasis is on making detailed observations of nearby objects although the large system bandwidth (100 MHz) will allow us to quantify the HI properties over a large instantaneous velocity range. In this paper we describe the survey and its goals and present the results from the precursor observations of a 5 degree x 1 degree region containing the nearby (~10 Mpc) NGC 628 group. We have detected all the group galaxies in the region including the low mass (M{HI}~10^7Mo) dwarf, dw0137+1541 (Briggs, 1986). The fluxes and velocities for these galaxies compare well with previously published data. There is no intra-group neutral gas...

  6. X ray observations of late-type stars using the ROSAT all-sky survey

    Science.gov (United States)

    Linsky, Jeffrey L.; Fleming, Thomas A.

    1992-03-01

    The ROSAT mission made the first x ray survey of the entire sky using an imaging detector. Although ROSAT is a joint NASA/German project and involves direct American participation during its second phase of pointed observations, the all-sky survey remains the sole property of the German investigators. NASA grant represented the first use of ROSAT data analysis funds to support direct American participation in the ROSAT all-sky survey. The project involved a collaborative agreement between the Joint Institute for Laboratory Astrophysics (JILA) and the Max-Planck-Institut fur Extraterrestrische Physik (MPE) where JILA supplied MPE with a post-doctoral research associate with experience in the field of stellar (coronal) x ray emission to work within their ROSAT group. In return, members of the cool star research group at JILA were given the opportunity to collaborate on projects involving ROSAT all-sky survey data. Both sides have benefitted (and still benefit) from this arrangement since MPE suffers from a shortage of researchers who are interested in x ray emission from 'normal' stars and white dwarfs. MPE has also drawn upon experience in optical identification of x ray sources from the Einstein Extended Medium Sensitivity Survey in planning their own identification strategies for the ROSAT all-sky survey. The JILA cool stars group has benefitted since access to all-sky survey data has expanded the scope of their already extensive research programs involving multiwavelength observations of late-type stars. ROSAT was successfully launched on 1 June 1990 and conducted the bulk of the survey from 30 July 1990 to 25 January 1991. Data gaps in the survey have subsequently been made up. At the time of this writing (February 1992), the survey data have been processed once with the Standard Analysis Software System (SASS). A second processing will soon begin with improvements made to the SASS to correct errors and bugs found while carrying out scientific projects with data

  7. Application of the time-delay integration method: Survey observations of geosynchronous orbit objects and short-term variability observations

    Science.gov (United States)

    Okumura, Shin-ichiro; Yanagisawa, Toshifumi; Nakaya, Hidehiko; Tanaka, Wataru; Nishiyama, Kota; Takahashi, Noritsugu; Yoshikawa, Makoto

    2014-12-01

    "Time-Delay Integration (TDI)" readout technique has been adopted to a mosaic CCD camera equipped with four fully-depleted CCDs. Optical distortion and image deformation due to the TDI operation are discussed. The manner and advantages of the TDI method in survey observations of geosynchronous orbit objects are summarized. We propose a new TDI application method of getting short-term light curves of artificial space objects. This method of detecting a short-term variability can be applied for a variety of objects, ranging from satellites to stars. It can also be used for the light-curve observations of transient objects which might show short-term variability and of which the precise time information is needed.

  8. Brood surveys and hunter observations used to predict gobbling activity wild turkeys in Mississippi

    Science.gov (United States)

    Palumbo, Matthew D.; Vilella, Francisco; Strickland, Bronson K.; Wang, Guiming; Godwin, Dave

    2014-01-01

    The Mississippi Department of Wildlife, Fisheries, and Parks utilize data from turkey hunter observations and brood surveys from across the state to manage wild turkey Meleagris gallopavo populations. Since 1995, hunters have collected gobbling and jake observation data, while the Mississippi Department of Wildlife, Fisheries, and Parks' personnel and cooperating wildlife managers of several natural resource agencies throughout the state have collected brood survey data. Both sources of data serve to forecast poult recruitment and gobbling activity. The objective of this study was to evaluate if these data can serve as a viable predictor of gobbling activity. We used three mixed models to investigate the relationship between the number of jakes observed per hour of hunting 1 y prior and the total number of poults per hens 2 y prior (model 1), number of gobblers heard per hour of hunting and the number of jakes observed per hour of hunting 1 y prior (model 2), the number of gobblers heard per hour of hunting and the total number poults per total hens observed 2 y prior (model 3) using data from 1995 to 2008 among five wild turkey management regions encompassing the state. We incorporated region as a random effect to account for spatial variation. We found the number of jakes observed per hour of hunting 1 y prior correlated with the total number of poults per total hens observed 2 y prior. We also found the number of gobblers heard per hour of hunting correlated with the number of jakes observed per hour of hunting 1 y prior. Additionally, we found that the total poults per total hens observed 2 y prior was correlated to the number of gobblers heard per hour of hunting. Our results show promise for using indices of gobbling activity, jake observations, and brood surveys to estimate gobbling activity.

  9. Twelve thousand laser-AO observations: first results from the Robo-AO large surveys

    Science.gov (United States)

    Law, Nicholas M.; Baranec, Christoph; Riddle, Reed L.

    2014-07-01

    Robo-AO is the first AO system which can feasibly perform surveys of thousands of targets. The system has been operating in a fully robotic mode on the Palomar 1.5m telescope for almost two years. Robo-AO has completed nearly 12,000 high-angular-resolution observations in almost 20 separate science programs including exoplanet characterization, field star binarity, young star binarity and solar system observations. We summarize the Robo-AO surveys and the observations completed to date. We also describe the data-reduction pipeline we developed for Robo-AO—the first fully-automated AO data-reduction, point-spread-function subtraction and companion-search pipeline.

  10. The XXL Survey. I. Scientific motivations - XMM-Newton observing plan - Follow-up observations and simulation programme

    Science.gov (United States)

    Pierre, M.; Pacaud, F.; Adami, C.; Alis, S.; Altieri, B.; Baran, N.; Benoist, C.; Birkinshaw, M.; Bongiorno, A.; Bremer, M. N.; Brusa, M.; Butler, A.; Ciliegi, P.; Chiappetti, L.; Clerc, N.; Corasaniti, P. S.; Coupon, J.; De Breuck, C.; Democles, J.; Desai, S.; Delhaize, J.; Devriendt, J.; Dubois, Y.; Eckert, D.; Elyiv, A.; Ettori, S.; Evrard, A.; Faccioli, L.; Farahi, A.; Ferrari, C.; Finet, F.; Fotopoulou, S.; Fourmanoit, N.; Gandhi, P.; Gastaldello, F.; Gastaud, R.; Georgantopoulos, I.; Giles, P.; Guennou, L.; Guglielmo, V.; Horellou, C.; Husband, K.; Huynh, M.; Iovino, A.; Kilbinger, M.; Koulouridis, E.; Lavoie, S.; Le Brun, A. M. C.; Le Fevre, J. P.; Lidman, C.; Lieu, M.; Lin, C. A.; Mantz, A.; Maughan, B. J.; Maurogordato, S.; McCarthy, I. G.; McGee, S.; Melin, J. B.; Melnyk, O.; Menanteau, F.; Novak, M.; Paltani, S.; Plionis, M.; Poggianti, B. M.; Pomarede, D.; Pompei, E.; Ponman, T. J.; Ramos-Ceja, M. E.; Ranalli, P.; Rapetti, D.; Raychaudury, S.; Reiprich, T. H.; Rottgering, H.; Rozo, E.; Rykoff, E.; Sadibekova, T.; Santos, J.; Sauvageot, J. L.; Schimd, C.; Sereno, M.; Smith, G. P.; Smolčić, V.; Snowden, S.; Spergel, D.; Stanford, S.; Surdej, J.; Valageas, P.; Valotti, A.; Valtchanov, I.; Vignali, C.; Willis, J.; Ziparo, F.

    2016-06-01

    Context. The quest for the cosmological parameters that describe our universe continues to motivate the scientific community to undertake very large survey initiatives across the electromagnetic spectrum. Over the past two decades, the Chandra and XMM-Newton observatories have supported numerous studies of X-ray-selected clusters of galaxies, active galactic nuclei (AGNs), and the X-ray background. The present paper is the first in a series reporting results of the XXL-XMM survey; it comes at a time when the Planck mission results are being finalised. Aims: We present the XXL Survey, the largest XMM programme totaling some 6.9 Ms to date and involving an international consortium of roughly 100 members. The XXL Survey covers two extragalactic areas of 25 deg2 each at a point-source sensitivity of ~5 × 10-15 erg s-1 cm-2 in the [0.5-2] keV band (completeness limit). The survey's main goals are to provide constraints on the dark energy equation of state from the space-time distribution of clusters of galaxies and to serve as a pathfinder for future, wide-area X-ray missions. We review science objectives, including cluster studies, AGN evolution, and large-scale structure, that are being conducted with the support of approximately 30 follow-up programmes. Methods: We describe the 542 XMM observations along with the associated multi-λ and numerical simulation programmes. We give a detailed account of the X-ray processing steps and describe innovative tools being developed for the cosmological analysis. Results: The paper provides a thorough evaluation of the X-ray data, including quality controls, photon statistics, exposure and background maps, and sky coverage. Source catalogue construction and multi-λ associations are briefly described. This material will be the basis for the calculation of the cluster and AGN selection functions, critical elements of the cosmological and science analyses. Conclusions: The XXL multi-λ data set will have a unique lasting legacy

  11. Seoul National University Bright Quasar Survey in Optical (SNUQSO) I: First Phase Observations and Results

    CERN Document Server

    Lee, Induk; Kim, Minjin; Kang, Eugene; Shim, Hyunjin; Richards, Gordon T; Edge, Alastair C; Lee, Myung Gyoon; Park, Changbom; Park, Myeong-Gu

    2008-01-01

    We present results from the first phase of the Seoul National University Bright Quasar Survey in Optical (SNUQSO) as well as its basic observational setup. Previous and current large-area surveys have been successful in identifying many quasars, but they could have missed bright quasars due to their survey design. In order to help complete the census of bright quasars, we have performed spectroscopic observations of new bright quasar candidates selected from various methods based on optical colors, near-infrared colors, radio, and X-ray data. In 2005/2006, we observed 55 bright quasar candidates using the Bohyunsan Optical Echelle Spectrograph (BOES) on the 1.8 m telescope at the Bohyunsan Optical Astronomy Observatory in Korea. We identify 14 quasars/Seyferts from our observation, including an optically bright quasar with i=14.98 mag at z=0.092 (SDSS J003236.59-091026.2). Non-quasar/Seyfert objects are found to be mostly stars, among which there are five M-type stars and one cataclysmic variable. Our result ...

  12. PreCam: A Precursor Observational Campaign for Calibration of the Dark Energy Survey

    Energy Technology Data Exchange (ETDEWEB)

    Kuehn, K.; Kuhlmann, S.; Allam, S.; Annis, J. T.; Bailey, T.; Balbinot, E.; Bernstein, J. P.; Biesiadzinski, T.; Burke, D. L.; Butner, M.; Camargo, J. I. B.; da Costa, L. A. N.; DePoy, D.; Diehl, H. T.; Dietrich, J. P.; Estrada, J.; Fausti, A.; Gerke, B.; Guarino, V.; Head, H. H.; Kessler, R.; Lin, H.; Lorenzon, W.; Maia, M. A. G.; Maki, L.; Marshall, J.; Nord, B.; Neilsen, E.; Ogando, R. L. C.; Park, D.; Peoples, J.; Rastawicki, D.; Rheault, J. -P.; Santiago, B.; Schubnell, M.; Seitzer, P.; Smith, J. A.; Spinka, H.; Sypniewski, A.; Tarle, G.; Tucker, D. L.; Walker, A. R.; Wester, W.

    2013-04-01

    PreCam, a precursor observational campaign supporting the Dark Energy Survey (DES), is designed to produce a photometric and astrometric catalog of nearly a hundred thousand standard stars within the DES footprint, while the PreCam instrument also serves as a prototype testbed for the Dark Energy Camera's hardware and software. This catalog represents a potential 100-fold increase in Southern Hemisphere photometric standard stars, and therefore will be an important component in the calibration of the Dark Energy Survey. We provide details on the PreCam instrument's design, construction, and testing, as well as results from a subset of the 51 nights of PreCam survey observations on the University of Michigan Department of Astronomy's Curtis-Schmidt telescope at Cerro Tololo Inter-American Observatory (CTIO). We briefly describe the preliminary data processing pipeline that has been developed for PreCam data and the preliminary results of the instrument performance, as well as astrometry and photometry of a sample of stars previously included in other southern sky surveys.

  13. The XXL Survey XI: ATCA 2.1 GHz continuum observations

    CERN Document Server

    Smolcic, Vernesa; Huynh, Minh; Bondi, Marco; Ciliegi, Paolo; Novak, Mladen; Baran, Nikola; Birkinshaw, Mark; Bremer, Malcolm N; Chiappetti, Lucio; Ferrari, Chiara; Fotopoulou, Sotiria; Horellou, Cathy; McGee, Sean L; Pacaud, Florian; Pierre, Marguerite; Raychaudhury, Somak; Roettgering, Huub; Vignali, Cristian

    2015-01-01

    We present 2.1 GHz imaging with the Australia Telescope Compact Array (ATCA) of a 6.5 deg^2 region within the XXM-Newton XXL South field using a band of 1.1-3.1 GHz. We achieve an angular resolution of 4.7" x 4.2" in the final radio continuum map with a median rms noise level of 50 uJy/beam. We identify 1389 radio sources in the field with peak S/N >=5 and present the catalogue of observed parameters. We find that 305 sources are resolved, of which 77 consist of multiple radio components. These number counts are in agreement with those found for the COSMOS-VLA 1.4 GHz survey. We derive spectral indices by a comparison with the Sydney University Molongolo Sky Survey (SUMSS) 843MHz data. We find an average spectral index of -0.78 and a scatter of 0.28, in line with expectations. This pilot survey was conducted in preparation for a larger ATCA program to observe the full 25 deg^2 southern XXL field. When complete, the survey will provide a unique resource of sensitive, wide-field radio continuum imaging with com...

  14. The VLT-FLAMES Tarantula Survey I: Introduction and observational overview

    CERN Document Server

    Evans, C J; Henault-Brunet, V; Sana, H; de Koter, A; Simon-Diaz, S; Carraro, G; Bagnoli, T; Bastian, N; Bestenlehner, J M; Bonanos, A Z; Bressert, E; Brott, I; Campbell, M A; Cantiello, M; Clark, J S; Costa, E; Crowther, P A; de Mink, S E; Doran, E; Dufton, P L; Dunstall, P R; Friedrich, K; Garcia, M; Gieles, M; Graefener, G; Herrero, A; Howarth, I D; Izzard, R G; Langer, N; Lennon, D J; Apellaniz, J Maiz; Markova, N; Najarro, F; Puls, J; Ramirez, O H; Sabin, C; Smartt, S J; Stroud, V E; van Loon, J Th; Vink, J S; Walborn, N R

    2011-01-01

    The VLT-FLAMES Tarantula Survey (VFTS) is an ESO Large Programme that has obtained multi-epoch optical spectroscopy of over 800 massive stars in the 30 Doradus region of the Large Magellanic Cloud (LMC). Here we introduce our scientific motivations and give an overview of the survey targets, including optical and near-infrared photometry and comprehensive details of the data reduction. One of the principal objectives was to detect massive binary systems via variations in their radial velocities, thus shaping the multi-epoch observing strategy. Spectral classifications are given for the massive emission-line stars observed by the survey, including the discovery of a new Wolf-Rayet star (VFTS 682, classified as WN5h), 2' to the northeast of R136. To illustrate the diversity of objects encompassed by the survey, we investigate the spectral properties of sixteen targets identified by Gruendl & Chu from Spitzer photometry as candidate young stellar objects or stars with notable mid-infrared excesses. Detailed ...

  15. Science Teacher Beliefs and Classroom Practice Related to Constructivism in Different School Settings

    Science.gov (United States)

    Savasci, Funda; Berlin, Donna F.

    2012-02-01

    Science teacher beliefs and classroom practice related to constructivism and factors that may influence classroom practice were examined in this cross-case study. Data from four science teachers in two schools included interviews, demographic questionnaire, Classroom Learning Environment Survey (preferred/perceived), and classroom observations and documents. Using an inductive analytic approach, results suggested that the teachers embraced constructivism, but classroom observations did not confirm implementation of these beliefs for three of the four teachers. The most preferred constructivist components were personal relevance and student negotiation; the most perceived component was critical voice. Shared control was the least preferred, least perceived, and least observed constructivist component. School type, grade, student behavior/ability, curriculum/standardized testing, and parental involvement may influence classroom practice.

  16. An investigation on levels of the emphatic tendencies of classroom teachers

    Directory of Open Access Journals (Sweden)

    Emine Akbulut

    2010-12-01

    Full Text Available The purpose of this reseach study is to investigate the empathic tendencies of classroom teachers according to some certain variables.  Total field under survey is 1257 classroom teachers working in Düzce Province in 2009-2010. Samples consist of 307 classroom teachers, gathered through basic random sampling in the field under survey. Personal Information Form and Empathic Tendency Scale is used in the research. .05 statistical significance level is observed in the analysis of the data. A t-test method is applied for independent samples in order to determine whether the empathic tendencies of primary school classroom tearchers change in relation to gender, civil status, willingness to chose to become classroom teacher, satisfaction from their job. One-Way Anova analysis is applied for independent samples in order to determine whether the empathic tendencies of primary school classroom tearchers change in relation to length of service, where they live. Results show that gender has a statistically significant effect on the empathic tendencies of primary school classroom tearchers. The average point of female classroom teachers' empathic tendencies is observed higher than male teachers' empathic tendencies. Results show that civil status, willingness to chose to become classroom teacher, satisfaction from their job, length of service and where they live have no statistically significant effect on the empathic tendencies of primary school classroom tearchers.

  17. 基于人种志视角的英语课堂观察建构%Construction of English Classroom Observation Based on the Perspective of Ethnography

    Institute of Scientific and Technical Information of China (English)

    彭志斌

    2014-01-01

    Based on the perspective of ethnography ,"field work"methodology has been introduced into micro level of educa-tion research (class), playing an important role in it.The development of ethnography, combined with English classroom activities, complements the method and means in English classroom observation .English classroom observation under the perspective of eth-nography is good at local analysis and diagnosis of classroom behavior , compared with the traditional evaluation system .It not only introduces the characteristics of classroom research nature , also pays attention to the marginalized in the education object , and high-lights the significance of teachers'cooperation .%基于人种志视角的“田野工作”的方法论逐渐渗入教育研究的微观领域(课堂)发挥着重要的作用,教育人种志的深入开展提供了与英语课堂活动相结合的机会,并因此补充和发展了英语课堂观察的方法和手段。基于人种志视角下的英语课堂观察善于对课堂行为的局部的分析与诊断,相对于传统听评课,它不仅引入了课堂研究的人本性特质,还关注了教育中的边缘化对象,突出了教师合作的重要性。

  18. PORTAAL: A Classroom Observation Tool Assessing Evidence-Based Teaching Practices for Active Learning in Large Science, Technology, Engineering, and Mathematics Classes.

    Science.gov (United States)

    Eddy, Sarah L; Converse, Mercedes; Wenderoth, Mary Pat

    2015-01-01

    There is extensive evidence that active learning works better than a completely passive lecture. Despite this evidence, adoption of these evidence-based teaching practices remains low. In this paper, we offer one tool to help faculty members implement active learning. This tool identifies 21 readily implemented elements that have been shown to increase student outcomes related to achievement, logic development, or other relevant learning goals with college-age students. Thus, this tool both clarifies the research-supported elements of best practices for instructor implementation of active learning in the classroom setting and measures instructors' alignment with these practices. We describe how we reviewed the discipline-based education research literature to identify best practices in active learning for adult learners in the classroom and used these results to develop an observation tool (Practical Observation Rubric To Assess Active Learning, or PORTAAL) that documents the extent to which instructors incorporate these practices into their classrooms. We then use PORTAAL to explore the classroom practices of 25 introductory biology instructors who employ some form of active learning. Overall, PORTAAL documents how well aligned classrooms are with research-supported best practices for active learning and provides specific feedback and guidance to instructors to allow them to identify what they do well and what could be improved. © 2015 S. L. Eddy et al. CBE—Life Sciences Education © 2015 The American Society for Cell Biology. This article is distributed by The American Society for Cell Biology under license from the author(s). It is available to the public under an Attribution–Noncommercial–Share Alike 3.0 Unported Creative Commons License (http://creativecommons.org/licenses/by-nc-sa/3.0).

  19. IRAC Snapshot Imaging of Massive-Cluster Gravitational Lenses Observed by the Herschel Lensing Survey

    Science.gov (United States)

    Egami, Eiichi; Rawle, Timothy; Cava, Antonio; Clement, Benjamin; Dessauges-Zavadsky, Miroslava; Ebeling, Harald; Kneib, Jean-Paul; Perez-Gonzalez, Pablo; Richard, Johan; Rujopakarn, Wiphu; Schaerer, Daniel; Walth, Gregory

    2015-10-01

    Using the Herschel Space Observatory, our team has been conducting a large survey of the fields of massive galaxy clusters, 'The Herschel Lensing Survey (HLS)' (PI: Egami; 419 hours). The main scientific goal is to penetrate the confusion limit of Herschel by taking advantage of the strong gravitational lensing power of these massive clusters and study the population of low-luminosity and/or high-redshift dusty star-forming galaxies that are beyond the reach of field Herschel surveys. In the course of this survey, we have obtained deep PACS (100/160 um) and SPIRE (250/350/500 um) images for 54 clusters (HLS-deep) as well as shallower (but nearly confusion-limited) SPIRE images for 527 clusters (HLS-snapshot). The goal of this proposal is to obtain shallow (500 sec/band) 3.6/4.5 um images of 266 cluster fields that have been observed by the HLS-snapshot survey but do not have any corresponding IRAC data. The HLS-snapshot SPIRE images are deep enough to detect a large number of sources in the target cluster fields, many of which are distant star-forming galaxies lensed by the foreground clusters, and the large sample size of HLS-snapshot promises a great potential for making exciting discoveries. Yet, these Herschel images would be of limited use if we could not identify the counterparts of the Herschel sources accurately and efficiently. The proposed IRAC snapshot program will greatly enhance the utility of these Herschel data, and will feed powerful gound observing facilities like ALMA and NOEMA with interesting targets to follow up.

  20. On observation distributions for state space models of population survey data.

    Science.gov (United States)

    Knape, Jonas; Jonzén, Niclas; Sköld, Martin

    2011-11-01

    1. State space models are starting to replace more simple time series models in analyses of temporal dynamics of populations that are not perfectly censused. By simultaneously modelling both the dynamics and the observations, consistent estimates of population dynamical parameters may be obtained. For many data sets, the distribution of observation errors is unknown and error models typically chosen in an ad-hoc manner. 2. To investigate the influence of the choice of observation error on inferences, we analyse the dynamics of a replicated time series of red kangaroo surveys using a state space model with linear state dynamics. Surveys were performed through aerial counts and Poisson, overdispersed Poisson, normal and log-normal distributions may all be adequate for modelling observation errors for the data. We fit each of these to the data and compare them using AIC. 3. The state space models were fitted with maximum likelihood methods using a recent importance sampling technique that relies on the Kalman filter. The method relaxes the assumption of Gaussian observation errors required by the basic Kalman filter. Matlab code for fitting linear state space models with Poisson observations is provided. 4. The ability of AIC to identify the correct observation model was investigated in a small simulation study. For the parameter values used in the study, without replicated observations, the correct observation distribution could sometimes be identified but model selection was prone to misclassification. On the other hand, when observations were replicated, the correct distribution could typically be identified. 5. Our results illustrate that inferences may differ markedly depending on the observation distributions used, suggesting that choosing an adequate observation model can be critical. Model selection and simulations show that for the models and parameter values in this study, a suitable observation model can typically be identified if observations are

  1. ESO Imaging Survey. Hubble Deep Field South Optical-Infrared Observations, Data Reduction and Photometry

    CERN Document Server

    Da Costa, L N; Rengelink, R B; Zaggia, S R; Benoist, C; Erben, T; Wicenec, A; Scodeggio, M; Olsen, L F; Guarnieri, M D; Deul, E; D'Odorico, S; Hook, R N; Moorwood, A F M; Slijkhuis, R

    1998-01-01

    This paper presents ground-based data obtained from deep optical and infrared observations of the HST Hubble Deep Field South (HDF-S) field carried out at the ESO 3.5 New Technology Telescope (NTT). These data were taken as part of the ESO Imaging Survey (EIS) program, a public survey coordinated by ESO and member states, in preparation for the first year of operation of the VLT. Deep CCD images are available for five optical passbands, reaching 2 sigma limiting magnitudes of U_AB~27.0, B_AB~26.5, V_AB~26, R_AB~26, I_AB~25, covering a region of ~25 square arcmin, which includes the HST WPFC2 field. The infrared observations cover a total area of ~42 square arcmin and include both the HST WFPC2 and STIS fields. The observations of the WFPC2 region were conducted in JHKs passbands, reaching J_AB~25, and H_AB and K_AB~24.0. Due to time constraints, the adjacent field, covering the STIS field, has been observed only in R, I and JHKs, while no observations were conducted covering the NIC3 field. This paper describ...

  2. The Arecibo Legacy Fast ALFA Survey: II. Results of Precursor Observations

    CERN Document Server

    Giovanelli, R; Kent, B R; Perillat, P; Catinella, B; Hoffman, G L; Momjian, E; Rosenberg, J L; Saintonge, A; Spekkens, K; Stierwalt, S; Brosch, N; Masters, K L; Springob, C M; Karachentsev, I D; Karachentseva, V E; Koopmann, R A; Müller, E; Van Driel, W; Van Zee, L; Giovanelli, Riccardo; Haynes, Martha P.; Kent, Brian R.; Perillat, Philip; Catinella, Barbara; Momjian, Emmanuel; Rosenberg, Jessica L.; Saintonge, Amelie; Spekkens, Kristine; Stierwalt, Sabrina; Brosch, Noah; Masters, Karen L.; Springob, Christopher M.; Karachentsev, Igor D.; Karachentseva, Valentina E.; Koopmann, Rebecca A.; Muller, Erik; Driel, Wim van; Zee, Liese van

    2005-01-01

    In preparation for the full Arecibo Legacy Fast ALFA extragalactic HI survey, precursor observations were carried out in Aug--Sep 2004 with the 7-beam Arecibo L-band feed array (ALFA) receiver system and the WAPP spectral processors. While these observations were geared mainly at testing and debugging survey strategy, hardware and software, approximately 36 hours of telescope time yielded science--quality data. From those observations, an initial list of 730 tentative detections of varying degree of reliability was extracted. Ninety--eight high signal-to-noise candidates were deemed to be bona fide HI line detections. To test our ability to discriminate cosmic signals from RFI and noise, 165 candidates ranging in reliability likelihood were re--observed with the single beam L--band wide system at Arecibo in Jan--Feb 2005. Of those, 41% were confirmed as real. We present the results of both the ALFA and single beam observations for the sample of 166 confirmed HI sources, as well as our assessment of their opti...

  3. Preschool Teachers' Use of Music in the Classroom: A Survey of Park District Preschool Programs

    Science.gov (United States)

    Rajan, Rekha S.

    2017-01-01

    The purpose of this study was to explore how preschool teachers use music and identify the types of music activities available to children in their classrooms. Preschool teachers (N = 178) at park district programs throughout a large state in the American Midwest responded to an online questionnaire. Although teachers acknowledged using music…

  4. Placement of Twins and Multiples in the Classroom: A Brief Survey of School Counselors' Knowledge and Attitudes

    Science.gov (United States)

    Nilsson, Johanna; Leonard, Lynn; Barazanji, Danah; Simone, Rachel

    2010-01-01

    This study investigated 65 school counselors' perception of classroom placement of twins and multiples. The results show that most of the participants had twins and multiples in their schools, but that they were neither aware of their school district nor building's policy regarding placement. Most participants supported early separation, already…

  5. Metrics for Optimization of Large Synoptic Survey Telescope Observations of Stellar Variables and Transients

    CERN Document Server

    Lund, Michael B; Pepper, Joshua A; Stassun, Keivan G

    2015-01-01

    The Large Synoptic Survey Telescope (LSST) will be the largest time-domain photometric survey ever. In order to maximize the LSST science yield for a broad array of transient stellar phenomena, it is necessary to optimize the survey cadence, coverage, and depth via quantitative metrics that are specifically designed to characterize the time-domain behavior of various types of stellar transients. In this paper we present three such metrics built on the LSST Metric Analysis Framework (MAF) model (Jones et al. 2014). Two of the metrics quantify the ability of LSST to detect non-periodic and/or non-recurring transient events, and the ability of LSST to reliably measure periodic signals of various timescales. The third metric provides a way to quantify the range of stellar parameters in the stellar populations that LSST will probe. We provide example uses of these metrics and discuss some implications based on these metrics for optimization of the LSST survey for observations of stellar variables and transients.

  6. An extensive survey of dayside diffuse aurora based on optical observations at Yellow River Station

    CERN Document Server

    Han, De-Sheng; Liu, Jian-Jun; Qiu, Qi; Keika, K; Hu, Ze-Jun; Liu, Jun-Ming; Hu, Hong-Qiao; Yang, Hui-Gen

    2016-01-01

    By using 7 years optical auroral observations obtained at Yellow River Station (magnetic latitude $76.24\\,^{\\circ}{\\rm C}$N) at Ny-Alesund, Svalbard, we performed the first extensive survey for the dayside diffuse auroras (DDAs) and acquired observational results as follows. (1) The DDAs can be classified into two broad categories, i.e., unstructured and structured DDAs. The unstructured DDAs are mainly distributed in the morning and afternoon, but the structured DDAs predominantly occurred around the magnetic local noon (MLN). (2) The unstructured DDAs observed in morning and afternoon present obviously different properties. The afternoon ones are much stable and seldom show pulsating property. (3) The DDAs are more easily observed under geomagnetically quiet times. (4) The structured DDAsmainly show patchy, stripy, and irregular forms and are often pulsating and drifting. The drifting directions are mostly westward (with speed $\\sim$5km/s), but there are cases showing eastward or poleward drifting. (5) The ...

  7. Observing Strategy for the SDSS-IV/MaNGA IFU Galaxy Survey

    CERN Document Server

    Law, David R; Bershady, Matthew A; Bundy, Kevin; Cherinka, Brian; Drory, Niv; MacDonald, Nicholas; Sanchez-Gallego, Jose R; Weijmans, Anne-Marie; Blanton, Michael R; Klaene, Mark; Moran, Sean M; Sanchez, Sebastian F; Zhang, Kai

    2015-01-01

    MaNGA (Mapping Nearby Galaxies at Apache Point Observatory) is an integral-field spectroscopic survey of 10,000 nearby galaxies that is one of three core programs in the fourth-generation Sloan Digital Sky Survey (SDSS-IV). MaNGA's 17 pluggable optical fiber-bundle integral field units (IFUs) are deployed across a 3 deg field, they yield spectral coverage 3600-10,300 Ang at a typical resolution R ~ 2000, and sample the sky with 2" diameter fiber apertures with a total bundle fill factor of 56%. Observing over such a large field and range of wavelengths is particularly challenging for obtaining uniform and integral spatial coverage and resolution at all wavelengths and across each entire fiber array. Data quality is affected by the IFU construction technique, chromatic and field differential refraction, the adopted dithering strategy, and many other effects. We use numerical simulations to constrain the hardware design and observing strategy for the survey with the aim of ensuring consistent data quality that ...

  8. Observing Strategy for the SDSS-IV/MaNGA IFU Galaxy Survey

    Science.gov (United States)

    Law, David R.; Yan, Renbin; Bershady, Matthew A.; Bundy, Kevin; Cherinka, Brian; Drory, Niv; MacDonald, Nicholas; Sánchez-Gallego, José R.; Wake, David A.; Weijmans, Anne-Marie; Blanton, Michael R.; Klaene, Mark A.; Moran, Sean M.; Sanchez, Sebastian F.; Zhang, Kai

    2015-07-01

    Mapping Nearby Galaxies at Apache Point Observatory (MaNGA) is an integral-field spectroscopic survey that is one of three core programs in the fourth-generation Sloan Digital Sky Survey (SDSS-IV). MaNGA’s 17 pluggable optical fiber-bundle integral field units (IFUs) will observe a sample of 10,000 nearby galaxies distributed throughout the SDSS imaging footprint (focusing particularly on the North Galactic Cap). In each pointing these IFUs are deployed across a 3° field; they yield spectral coverage 3600-10300 Å at a typical resolution R ˜ 2000, and sample the sky with 2″ diameter fiber apertures with a total bundle fill factor of 56%. Observing over such a large field and range of wavelengths is particularly challenging for obtaining uniform and integral spatial coverage and resolution at all wavelengths and across each entire fiber array. Data quality is affected by the IFU construction technique, chromatic and field differential refraction, the adopted dithering strategy, and many other effects. We use numerical simulations to constrain the hardware design and observing strategy for the survey with the aim of ensuring consistent data quality that meets the survey science requirements while permitting maximum observational flexibility. We find that MaNGA science goals are best achieved with IFUs composed of a regular hexagonal grid of optical fibers with rms displacement of 5 μm or less from their nominal packing position; this goal is met by the MaNGA hardware, which achieves 3 μm rms fiber placement. We further show that MaNGA observations are best obtained in sets of three 15 minute exposures dithered along the vertices of a 1.44 arcsec equilateral triangle; these sets form the minimum observational unit, and are repeated as needed to achieve a combined signal-to-noise ratio of 5 Å-1 per fiber in the r-band continuum at a surface brightness of 23 AB arcsec-2. In order to ensure uniform coverage and delivered image quality, we require that the

  9. The DES Bright Arcs Survey: Hundreds of Candidate Strongly Lensed Galaxy Systems from the Dark Energy Survey Science Verification and Year 1 Observations

    Energy Technology Data Exchange (ETDEWEB)

    Diehl, H. T. [Fermilab

    2017-06-09

    We report the results of our searches for strong gravitational lens systems in the Dark Energy Survey (DES) Science Verication and Year 1 observations. The Science Verication data spans approximately 250 sq. deg. with median i

  10. Radio Observations of the Hubble Deep Field South region: I. Survey Description and Initial Results

    CERN Document Server

    Norris, R P; Jackson, C A; Boyle, B J; Ekers, R D; Mitchell, D A; Sault, R J; Wieringa, M H; Williams, R E; Hopkins, A M; Higdon, J; Norris, Ray P.; Huynh, Minh T.; Jackson, Carole A.; Boyle, Brian J.; Ekers, Ronald. D.; Mitchell, Daniel A.; Sault, Robert J.; Wieringa, Mark H.; Williams, Robert E.; Hopkins, Andrew M.; Higdon, James

    2005-01-01

    This paper is the first of a series describing the results of the Australia Telescope Hubble Deep Field South (ATHDFS) radio survey. The survey was conducted at four wavelengths - 20, 11, 6, and 3 cm, over a 4-year period, and achieves an rms sensitivity of about 10 microJy at each wavelength. We describe the observations and data reduction processes, and present data on radio sources close to the centre of the HDF-S. We discuss in detail the properties of a subset of these sources. The sources include both starburst galaxies and galaxies powered by an active galactic nucleus, and range in redshift from 0.1 to 2.2. Some of them are characterised by unusually high radio-to-optical luminosities, presumably caused by dust extinction.

  11. Thrust-breakthrough of asymmetric anticlines: Observational constraints from surveys in the Brooks Range, Alaska

    Science.gov (United States)

    Jadamec, Margarete A.; Wallace, Wesley K.

    2014-05-01

    To gain insights into the processes governing the thrust-truncation of anticlines, we conducted a field study of the thrust-truncated folds in the remote Brooks Range of northern Alaska, where there is a transition in fold style from symmetric detachment folds to thrust-truncated asymmetric folds. In order to document the detailed geometry of the km-scale folds exposed in cliff-forming, largely inaccessible outcrops, a new surveying technique was developed that combines data from a theodolite and laser range finder. The field observations, survey profiles, and cross section reconstructions, indicate that late-stage thrust breakthrough of the anticlines within the mechanically competent Lisburne Group carbonates accommodated continued shortening when other mechanisms became unfeasible, including fold tightening, forelimb rotation, and parasitic folding in the anticline forelimbs. These results provide constraints on the processes that govern the transition from buckle folding to thrust truncation in fold-and-thrust belts worldwide.

  12. The Green Bank Telescope 350 MHz Drift-scan Survey I: Survey Observations and the Discovery of 13 Pulsars

    CERN Document Server

    Boyles, Jason; Ransom, Scott M; Stairs, Ingrid H; Lorimer, Duncan R; McLaughlin, Maura A; Hessels, Jason W T; Kaspi, Vicky M; Kondratiev, Vlad I; Archibald, Anne; Berndsen, Aaron; Cardoso, Rogerio F; Cherry, Angus; McPhee, Christie A; Pennucci, Tim; Roberts, Mallory S E; Stovall, Kevin; van Leeuwen, Joeri

    2012-01-01

    Over the summer of 2007, we obtained 1191 hours of `drift-scan' pulsar search observations with the Green Bank Telescope at a radio frequency of 350 MHz. Here we describe the survey setup, search procedure, and the discovery and follow-up timing of thirteen pulsars. Among the new discoveries, one (PSR J1623-0841) was discovered only through its single pulses, two (PSRs J1327-0755 and J1737-0814) are millisecond pulsars, and another (PSR J2222-0137) is a mildly recycled pulsar. PSR J1327-0755 is a 2.7 ms pulsar at a DM of 27.9 pc cm^{-3} in a 8.7 day orbit with a minimum companion mass of 0.22$ solar mass. PSR J1737-0814 is a 4.2 ms pulsar at a DM of 55.3 pc cm^{-3} in a 79.3 day orbit with a minimum companion mass of 0.06 solar mass. PSR J2222$-$0137 is a 32.8 ms pulsar at a very low DM of 3.27 pc cm^{-3} in a 2.4 day orbit with a minimum companion mass of 1.11 solar mass. It is most likely a white dwarf-neutron star system or an unusual low-eccentricity double neutron star system. Ten other pulsars discovere...

  13. The DEEP2 Galaxy Redshift Survey: Design, Observations, Data Reduction, and Redshifts

    Science.gov (United States)

    Newman, Jeffrey A.; Cooper, Michael C.; Davis, Marc; Faber, S. M.; Coil, Alison L.; Guhathakurta, Puragra; Koo, David C.; Phillips, Andrew C.; Conroy, Charlie; Dutton, Aaron A.; Finkbeiner, Douglas P.; Gerke, Brian F.; Rosario, David J.; Weiner, Benjamin J.; Willmer, C. N. A.; Yan, Renbin; Harker, Justin J.; Kassin, Susan A.; Konidaris, N. P.; Lai, Kamson; Madgwick, Darren S.; Noeske, K. G.; Wirth, Gregory D.; Connolly, A. J.; Kaiser, N.; Kirby, Evan N.; Lemaux, Brian C.; Lin, Lihwai; Lotz, Jennifer M.; Luppino, G. A.; Marinoni, C.; Matthews, Daniel J.; Metevier, Anne; Schiavon, Ricardo P.

    2013-09-01

    We describe the design and data analysis of the DEEP2 Galaxy Redshift Survey, the densest and largest high-precision redshift survey of galaxies at z ~ 1 completed to date. The survey was designed to conduct a comprehensive census of massive galaxies, their properties, environments, and large-scale structure down to absolute magnitude MB = -20 at z ~ 1 via ~90 nights of observation on the Keck telescope. The survey covers an area of 2.8 deg2 divided into four separate fields observed to a limiting apparent magnitude of R AB = 24.1. Objects with z 0.7 to be targeted ~2.5 times more efficiently than in a purely magnitude-limited sample. Approximately 60% of eligible targets are chosen for spectroscopy, yielding nearly 53,000 spectra and more than 38,000 reliable redshift measurements. Most of the targets that fail to yield secure redshifts are blue objects that lie beyond z ~ 1.45, where the [O II] 3727 Å doublet lies in the infrared. The DEIMOS 1200 line mm-1 grating used for the survey delivers high spectral resolution (R ~ 6000), accurate and secure redshifts, and unique internal kinematic information. Extensive ancillary data are available in the DEEP2 fields, particularly in the Extended Groth Strip, which has evolved into one of the richest multiwavelength regions on the sky. This paper is intended as a handbook for users of the DEEP2 Data Release 4, which includes all DEEP2 spectra and redshifts, as well as for the DEEP2 DEIMOS data reduction pipelines. Extensive details are provided on object selection, mask design, biases in target selection and redshift measurements, the spec2d two-dimensional data-reduction pipeline, the spec1d automated redshift pipeline, and the zspec visual redshift verification process, along with examples of instrumental signatures or other artifacts that in some cases remain after data reduction. Redshift errors and catastrophic failure rates are assessed through more than 2000 objects with duplicate observations. Sky subtraction is

  14. Rip current evidence by hydrodynamic simulations, bathymetric surveys and UAV observation

    Science.gov (United States)

    Benassai, Guido; Aucelli, Pietro; Budillon, Giorgio; De Stefano, Massimo; Di Luccio, Diana; Di Paola, Gianluigi; Montella, Raffaele; Mucerino, Luigi; Sica, Mario; Pennetta, Micla

    2017-09-01

    The prediction of the formation, spacing and location of rip currents is a scientific challenge that can be achieved by means of different complementary methods. In this paper the analysis of numerical and experimental data, including RPAS (remotely piloted aircraft systems) observations, allowed us to detect the presence of rip currents and rip channels at the mouth of Sele River, in the Gulf of Salerno, southern Italy. The dataset used to analyze these phenomena consisted of two different bathymetric surveys, a detailed sediment analysis and a set of high-resolution wave numerical simulations, completed with Google EarthTM images and RPAS observations. The grain size trend analysis and the numerical simulations allowed us to identify the rip current occurrence, forced by topographically constrained channels incised on the seabed, which were compared with observations.

  15. Observations of Representational Practices by Indian-Descent Children in a US Preschool Classroom: Connections among People, Spaces and Artifacts

    Science.gov (United States)

    Braswell, Gregory S.

    2015-01-01

    This exploratory study examined children's experiences with producing and comprehending external representations in a preschool classroom. Data collection and analyses focused on how artifacts, spaces, adult-guided routines, and social conventions shape young children's representational development. Participants included 4- and…

  16. A Case Based Analysis Preparation Strategy for Use in a Classroom Management for Inclusive Settings Course: Preliminary Observations

    Science.gov (United States)

    Niles, William J.; Cohen, Alan

    2012-01-01

    Case based instruction (CBI) is a pedagogical option in teacher preparation growing in application but short on practical means to implement the method. This paper presents an analysis strategy and questions developed to help teacher trainees focus on classroom management issues embedded in a set of "real" cases. An analysis of teacher candidate…

  17. Information and Experience: Audio-Visual Observations of Reading Activities in Swedish Comprehensive School Classrooms 1967-1969

    Science.gov (United States)

    Dolatkhah, Mats; Hampson Lundh, Anna

    2016-01-01

    This study investigates reading activities in Swedish primary school classrooms during the late 1960s. Sound and video recordings of 223 Swedish lessons held between 1967 and 1969 are used to analyse the activity of reading as taught and performed. The results indicate that the practice of informational reading, often based on finding…

  18. The ALFA Zone of Avoidance Survey: Results from the Precursor Observations

    CERN Document Server

    Springob, C M; Catinella, B; Day, F; Minchin, R; Momjian, E; Koribalski, B; Masters, K L; Müller, E; Pantoja, C; Putman, M; Rosenberg, J L; Schneider, S; Staveley-Smith, L

    2007-01-01

    The Arecibo L-band Feed Array Zone of Avoidance Survey (ALFA ZOA) will map 1350-1800 square degrees at low Galactic latitude, providing HI spectra for galaxies in regions of the sky where our knowledge of local large scale structure remains incomplete, owing to obscuration from dust and high stellar confusion near the Galactic plane. Because of these effects, a substantial fraction of the galaxies detected in the survey will have no optical or infrared counterparts. However, near infrared follow up observations of ALFA ZOA sources found in regions of lowest obscuration could reveal whether some of these sources could be objects in which little or no star formation has taken place ("dark galaxies"). We present here the results of ALFA ZOA precursor observations on two patches of sky totaling 140 square degrees (near l=40 degrees, and l=192 degrees). We have measured HI parameters for detections from these observations, and cross-correlated with the NASA/IPAC Extragalactic Database (NED). A significant fraction...

  19. XMM-Newton Observations of the DLS Shear-Selected Cluster Survey

    Science.gov (United States)

    DellAntonio, Ian

    2005-01-01

    The goal of this project continues to be to test the selection effects in cluster surveys by investigating the X-ray properties of the first shear-selected sample of galaxy clusters, the Deep Lens Survey (DLS). Because lensing signal is only sensitive to mass (albeit with projection effects), lensing signal can be used to select a sample that is independent of its X-ray properties. If a lensing-selected sample has very different X-ray properties from an X-ray selected sample, it would have important consequences for evolutionary studies based on existing cluster samples was aimed at refining the lensing-selected sample as part of this continuing study The grant supported a KPNO run to obtain data on another region of the sky to extend the cluster sample, and also the purchase of a disk array for archiving the optical mosaic data (Two terabytes worth) from which the lensing maps are derived As a result of the grant, we have extended the lensing cluster sample to another 4-square degree patch of the sky, adding another three clusters to our sample to be observed While the sample of X-ray observed clusters is too small to derive a firm conclusion yet, our preliminary finding is that the X-ray properties of the observed sample do not differ from those of X-ray selected surveys A paper discussing the first results has been published, and a second paper on the mass differences is still in preparation (with J Hughes as first author)

  20. Monitoring greenhouse gas emissions in Australian landscapes: Comparing ground based mobile surveying data to GOSAT observations

    Science.gov (United States)

    Bashir, S.; Iverach, C.; Kelly, B. F. J.

    2016-12-01

    Climate change is threatening the health and stability of the natural world and human society. Such concerns were emphasized at COP21 conference in Paris 2015 which highlighted the global need to improve our knowledge of sources of greenhouse gas and to develop methods to mitigate the effects of their emissions. Ongoing spatial and temporal measurements of greenhouse gases at both point and regional scales is important for clarification of climate change mechanisms and accounting. The Greenhouse gas Observing SATellite (GOSAT) is designed to monitor the global distribution of carbon dioxide (CO2) and methane (CH4) from orbit. As existing ground monitoring stations are limited and still unevenly distributed, satellite observations provide important frequent, spatially extensive, but low resolution observations. Recent developments in portable laser based greenhouse gas measurement systems have enabled the rapid measurement of greenhouse gases in ppb at the ground surface. This study was conducted to map major sources of CO2 and CH4 in the eastern states of Australia at the landscape scale and to compare the results to GOSAT observations. During April 2016 we conducted a regional CH4 and CO2 mobile survey, using an LGR greenhouse gas analyzer. Measurements were made along a 4000 KM circuit through major cities, country towns, dry sclerophyll forests, coastal wetlands, coal mining regions, coal seam gas developments, dryland farming and irrigated agricultural landscapes. The ground-based survey data were then compared with the data (L2) from GOSAT. Ground-based mobile surveys showed that there are clear statistical differences in the ground level atmospheric concentration of CH4 and CO2 associated with all major changes in land use. These changes extend for kilometers, and cover one or more GOSAT pixels. In the coal mining districts the ground-level atmospheric concentration of CH4 exceeded 2 ppm for over 40 km, yet this was not discernable in the retrieved data (L2

  1. High-J CO survey of low-mass protostars observed with Herschel-HIFI

    DEFF Research Database (Denmark)

    Yıldız, U. A.; Kristensen, L. E.; van Dishoeck, E. F.

    2013-01-01

    with Herschel (WISH) key program. This is the first large spectrally resolved high-J CO survey conducted for these types of sources. Complementary lower J CO maps were observed using ground-based telescopes, such as the JCMT and APEX and convolved to matching beam sizes. Results: The 12CO 10-9 line is detected...... with science instruments provided by European-led Principal Investigator consortia and with important participation from NASA.Appendices C and D are available in electronic form at http://www.aanda.org...

  2. The EDGE-CALIFA Survey: Interferometric Observations of 126 Galaxies with CARMA

    Science.gov (United States)

    Bolatto, Alberto D.; Wong, Tony; Utomo, Dyas; Blitz, Leo; Vogel, Stuart N.; Sánchez, Sebastián F.; Barrera-Ballesteros, Jorge; Cao, Yixian; Colombo, Dario; Dannerbauer, Helmut; García-Benito, Rubén; Herrera-Camus, Rodrigo; Husemann, Bernd; Kalinova, Veselina; Leroy, Adam K.; Leung, Gigi; Levy, Rebecca C.; Mast, Damián; Ostriker, Eve; Rosolowsky, Erik; Sandstrom, Karin M.; Teuben, Peter; van de Ven, Glenn; Walter, Fabian

    2017-09-01

    We present interferometric CO observations, made with the Combined Array for Millimeter-wave Astronomy (CARMA) interferometer, of galaxies from the Extragalactic Database for Galaxy Evolution survey (EDGE). These galaxies are selected from the Calar Alto Legacy Integral Field Area (CALIFA) sample, mapped with optical integral field spectroscopy. EDGE provides good-quality CO data (3σ sensitivity {{{Σ }}}{mol}∼ 11 {M}ȯ {{pc}}-2 before inclination correction, resolution ∼1.4 kpc) for 126 galaxies, constituting the largest interferometric CO survey of galaxies in the nearby universe. We describe the survey and data characteristics and products, then present initial science results. We find that the exponential scale lengths of the molecular, stellar, and star-forming disks are approximately equal, and galaxies that are more compact in molecular gas than in stars tend to show signs of interaction. We characterize the molecular-to-stellar ratio as a function of Hubble type and stellar mass and present preliminary results on the resolved relations between the molecular gas, stars, and star-formation rate. We then discuss the dependence of the resolved molecular depletion time on stellar surface density, nebular extinction, and gas metallicity. EDGE provides a key data set to address outstanding topics regarding gas and its role in star formation and galaxy evolution, which will be publicly available on completion of the quality assessment.

  3. A fast method for quantifying observational selection effects in asteroid surveys

    Science.gov (United States)

    Jedicke, Robert; Bolin, Bryce; Granvik, Mikael; Beshore, Ed

    2016-03-01

    We present a fast method to calculate an asteroid survey's 'bias' - essentially a correction factor from the observed number of objects to the actual number in the population. The method builds upon the work of Jedicke and Metcalfe (Jedicke, R., Metcalfe, T.S. [1998]. Icaurs 131, 245-260) and Granvik et al. (Granvik, M., Vaubaillon, J., Jedicke, R. [2012]. Icarus 218, 262-277) and essentially efficiently maps out the phase space of orbit elements that can appear in a field-of-view. It does so by 'integrating' outwards in geocentric distance along a field's boresite from the topocentric location of the survey and calculating the allowable angular elements for each desired combination of semi-major axis, eccentricity and inclination. We then use a contour algorithm to map out the orbit elements that place an object at the edge of the field-of-view. We illustrate the method's application to calculate the bias correction for near Earth Objects detected with the Catalina Sky Survey (Christensen, E. et al. [2012]. AAS/Division for Planetary Sciences Meeting Abstracts, vol. 44, p. 210.13; Larson, S. et al. [1998]. Bulletin of the American Astronomical Society, vol. 30, p. 1037).

  4. THE DEEP2 GALAXY REDSHIFT SURVEY: DESIGN, OBSERVATIONS, DATA REDUCTION, AND REDSHIFTS

    Energy Technology Data Exchange (ETDEWEB)

    Newman, Jeffrey A. [Department of Physics and Astronomy, University of Pittsburgh, Pittsburgh, PA 15260 (United States); Cooper, Michael C. [Center for Galaxy Evolution, Department of Physics and Astronomy, University of California, Irvine, 4129 Frederick Reines Hall, Irvine, CA 92697 (United States); Davis, Marc [Department of Astronomy and Physics, University of California, 601 Campbell Hall, Berkeley, CA 94720 (United States); Faber, S. M.; Guhathakurta, Puragra; Koo, David C.; Phillips, Andrew C.; Conroy, Charlie; Harker, Justin J.; Lai, Kamson [UCO/Lick Observatory, University of California, 1156 High Street, Santa Cruz, CA 95064 (United States); Coil, Alison L. [Department of Physics, University of California, San Diego, La Jolla, CA 92093 (United States); Dutton, Aaron A. [Max Planck Institute for Astronomy, Koenigstuhl 17, D-69117 Heidelberg (Germany); Finkbeiner, Douglas P. [Harvard-Smithsonian Center for Astrophysics, Harvard University, 60 Garden St., Cambridge, MA 02138 (United States); Gerke, Brian F. [Lawrence Berkeley National Laboratory, 1 Cyclotron Rd., MS 90R4000, Berkeley, CA 94720 (United States); Rosario, David J. [Max-Planck-Institut fuer Extraterrestrische Physik, Giessenbachstrasse, D-85748 Garching (Germany); Weiner, Benjamin J.; Willmer, C. N. A. [Steward Observatory, University of Arizona, 933 N. Cherry Ave., Tucson, AZ 85721-0065 (United States); Yan Renbin [Department of Physics and Astronomy, University of Kentucky, 505 Rose Street, Lexington, KY 40506-0055 (United States); Kassin, Susan A. [Astrophysics Science Division, Goddard Space Flight Center, Code 665, Greenbelt, MD 20771 (United States); Konidaris, N. P., E-mail: janewman@pitt.edu, E-mail: djm70@pitt.edu, E-mail: m.cooper@uci.edu, E-mail: mdavis@berkeley.edu, E-mail: faber@ucolick.org, E-mail: koo@ucolick.org, E-mail: raja@ucolick.org, E-mail: phillips@ucolick.org [Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218 (United States); and others

    2013-09-15

    We describe the design and data analysis of the DEEP2 Galaxy Redshift Survey, the densest and largest high-precision redshift survey of galaxies at z {approx} 1 completed to date. The survey was designed to conduct a comprehensive census of massive galaxies, their properties, environments, and large-scale structure down to absolute magnitude M{sub B} = -20 at z {approx} 1 via {approx}90 nights of observation on the Keck telescope. The survey covers an area of 2.8 deg{sup 2} divided into four separate fields observed to a limiting apparent magnitude of R{sub AB} = 24.1. Objects with z {approx}< 0.7 are readily identifiable using BRI photometry and rejected in three of the four DEEP2 fields, allowing galaxies with z > 0.7 to be targeted {approx}2.5 times more efficiently than in a purely magnitude-limited sample. Approximately 60% of eligible targets are chosen for spectroscopy, yielding nearly 53,000 spectra and more than 38,000 reliable redshift measurements. Most of the targets that fail to yield secure redshifts are blue objects that lie beyond z {approx} 1.45, where the [O II] 3727 A doublet lies in the infrared. The DEIMOS 1200 line mm{sup -1} grating used for the survey delivers high spectral resolution (R {approx} 6000), accurate and secure redshifts, and unique internal kinematic information. Extensive ancillary data are available in the DEEP2 fields, particularly in the Extended Groth Strip, which has evolved into one of the richest multiwavelength regions on the sky. This paper is intended as a handbook for users of the DEEP2 Data Release 4, which includes all DEEP2 spectra and redshifts, as well as for the DEEP2 DEIMOS data reduction pipelines. Extensive details are provided on object selection, mask design, biases in target selection and redshift measurements, the spec2d two-dimensional data-reduction pipeline, the spec1d automated redshift pipeline, and the zspec visual redshift verification process, along with examples of instrumental signatures or

  5. The DEEP2 Galaxy Redshift Survey: Design, Observations, Data Reduction, and Redshifts

    Science.gov (United States)

    Newman, Jeffrey A.; Cooper, Michael C.; Davis, Marc; Faber, S. M.; Coil, Alison L; Guhathakurta, Puraga; Koo, David C.; Phillips, Andrew C.; Conroy, Charlie; Dutton, Aaron A.; Finkbeiner, Douglas P.; Gerke, Brian F.; Rosario, David J.; Weiner, Benjamin J.; Wilmer, C. N. A.; Yan, Renbin; Harker, Justin J.; Kassin, Susan A.; Konidaris, N. P.; Lai, Kamson; Madgwick, Darren S.; Noeske, K. G.; Wirth, Gregory D.; Kirby, Evan N.; Lotz, Jennifer M.

    2013-01-01

    We describe the design and data analysis of the DEEP2 Galaxy Redshift Survey, the densest and largest high-precision redshift survey of galaxies at z approx. 1 completed to date. The survey was designed to conduct a comprehensive census of massive galaxies, their properties, environments, and large-scale structure down to absolute magnitude MB = -20 at z approx. 1 via approx.90 nights of observation on the Keck telescope. The survey covers an area of 2.8 Sq. deg divided into four separate fields observed to a limiting apparent magnitude of R(sub AB) = 24.1. Objects with z approx. galaxies with z > 0.7 to be targeted approx. 2.5 times more efficiently than in a purely magnitude-limited sample. Approximately 60% of eligible targets are chosen for spectroscopy, yielding nearly 53,000 spectra and more than 38,000 reliable redshift measurements. Most of the targets that fail to yield secure redshifts are blue objects that lie beyond z approx. 1.45, where the [O ii] 3727 Ang. doublet lies in the infrared. The DEIMOS 1200 line mm(exp -1) grating used for the survey delivers high spectral resolution (R approx. 6000), accurate and secure redshifts, and unique internal kinematic information. Extensive ancillary data are available in the DEEP2 fields, particularly in the Extended Groth Strip, which has evolved into one of the richest multiwavelength regions on the sky. This paper is intended as a handbook for users of the DEEP2 Data Release 4, which includes all DEEP2 spectra and redshifts, as well as for the DEEP2 DEIMOS data reduction pipelines. Extensive details are provided on object selection, mask design, biases in target selection and redshift measurements, the spec2d two-dimensional data-reduction pipeline, the spec1d automated redshift pipeline, and the zspec visual redshift verification process, along with examples of instrumental signatures or other artifacts that in some cases remain after data reduction. Redshift errors and catastrophic failure rates are assessed

  6. Increasing Positive Interactive Classroom Behavior

    Science.gov (United States)

    Kotcher, Elaine; Doremus, Richard R.

    1973-01-01

    The question examined in this study was as follows: do teachers increase their positive classroom interactive behaviors as a result of training in systematic classroom observation techniques? (Authors/JA)

  7. Sherlock Holmes in the Classroom.

    Science.gov (United States)

    Faia, Jean E.

    1988-01-01

    Describes a three-day classroom activity combining criminal investigations and scientific skills, especially observation skills. Provides detailed classroom procedures with an illustration of eight basic fingerprint patterns and a classification chart. (YP)

  8. Sherlock Holmes in the Classroom.

    Science.gov (United States)

    Faia, Jean E.

    1988-01-01

    Describes a three-day classroom activity combining criminal investigations and scientific skills, especially observation skills. Provides detailed classroom procedures with an illustration of eight basic fingerprint patterns and a classification chart. (YP)

  9. Narrow absorption lines with two observations of Sloan Digital Sky Survey

    CERN Document Server

    Chen, Zhi-Fu; Chen, Yan-Mei; Cao, Yue

    2015-01-01

    We assemble 3524 quasars from Sloan Digital Sky Survey (SDSS) with repeated observations to search for variations of narrow C IV1548,1551 and Mg II2796,2803 absorption doublets in spectral regions shortward of 7000 Ang at the observed frame, which corresponds to time-scales of about 150 ~ 2643 days at quasar rest frame. In these quasar spectra, we detect 3580 C IV absorption systems with z_{abs} = 1.5188 ~ 3.5212, and 1809 Mg II absorption systems with z_{abs} = 0.3948 ~ 1.7167. In term of the absorber velocity (beta) distribution at quasar rest frame, we find a substantial number of C IV absorbers with beta4sigma for lambda2796 lines and >3sigma for lambda2803 lines.

  10. Selection Effects in Galaxy Cluster Surveys: What Do We Learn from Observed Scaling Relations?

    Science.gov (United States)

    Nord, Brian D.; Evrard, A. E.

    2006-12-01

    The plethora of observable quantities across multiple wave bands contains redundant information about the masses of galaxy clusters. Proper calibration across the descriptor set are crucial steps to correctly map the cosmic mass distribution, thereby constraining dark sector cosmology. Survey flux thresholds mask the X-Ray sky, and establish a selection effect that is highly dependent on the intrinsic scatter in the mass at fixed luminosity. A precise model for the L-M relation has emerged from constraints from the REFLEX catalog. We extend this model to include temperature variations, modeled via a log-normal covariance. We show how redshift characteristics of cluster surveys contain a strong degeneracy between intrinsic scatter and true scaling. Knowledge of the covariance behavior is therefore important in recovering true physical evolution of the cluster population. We apply a similar technique to the X-ray properties of optically selected clusters. Inter-comparison of cluster properties among samples selected on different, or multiple, observables will potentially break model degeneracies, providing clues to how properties, like X-ray luminosity, optical richness, velocity dispersion, are linked. Many thanks to the Michigan Space Grant Consortium for their encouragement.

  11. TIMASSS: the IRAS 16293-2422 millimeter and submillimeter spectral survey. I. Observations, calibration, and analysis of the line kinematics

    NARCIS (Netherlands)

    Caux, E.; Kahane, C.; Castets, A.; Coutens, A.; Ceccarelli, C.; Bacmann, A.; Bisschop, S.; Bottinelli, S.; Comito, C.; Helmich, F. P.; Lefloch, B.; Parise, B.; Schilke, P.; Tielens, A. G. G. M.; van Dishoeck, E.; Vastel, C.; Wakelam, V.; Walters, A.

    2011-01-01

    Context. Unbiased spectral surveys are powerful tools to study the chemistry and the physics of star forming regions, because they can provide a complete census of the molecular content and the observed lines probe the physical structure of the source. Aims: While unbiased surveys at the millimeter

  12. TIMASSS: the IRAS 16293-2422 millimeter and submillimeter spectral survey. I. Observations, calibration, and analysis of the line kinematics

    NARCIS (Netherlands)

    Caux, E.; Kahane, C.; Castets, A.; Coutens, A.; Ceccarelli, C.; Bacmann, A.; Bisschop, S.; Bottinelli, S.; Comito, C.; Helmich, F. P.; Lefloch, B.; Parise, B.; Schilke, P.; Tielens, A. G. G. M.; van Dishoeck, E.; Vastel, C.; Wakelam, V.; Walters, A.

    2011-01-01

    Context. Unbiased spectral surveys are powerful tools to study the chemistry and the physics of star forming regions, because they can provide a complete census of the molecular content and the observed lines probe the physical structure of the source. Aims. While unbiased surveys at the millimeter

  13. CARMA LARGE AREA STAR FORMATION SURVEY: OBSERVATIONAL ANALYSIS OF FILAMENTS IN THE SERPENS SOUTH MOLECULAR CLOUD

    Energy Technology Data Exchange (ETDEWEB)

    Fernández-López, M.; Looney, L.; Lee, K.; Segura-Cox, D. [Department of Astronomy, University of Illinois at Urbana—Champaign, 1002 West Green Street, Urbana, IL 61801 (United States); Arce, H. G.; Plunkett, A. [Department of Astronomy, Yale University, P.O. Box 208101, New Haven, CT 06520-8101 (United States); Mundy, L. G.; Storm, S.; Teuben, P. J.; Pound, M. [Department of Astronomy, University of Maryland, College Park, MD 20742 (United States); Isella, A.; Kauffmann, J. [Astronomy Department, California Institute of Technology, 1200 East California Boulevard, Pasadena, CA 91125 (United States); Tobin, J. J. [National Radio Astronomy Observatory, Charlottesville, VA 22903 (United States); Rosolowsky, E. [Departments of Physics and Statistics, University of British Columbia, Okanagan Campus, 3333 University Way, Kelowna, BC V1V 1V7 (Canada); Kwon, W. [SRON Netherlands Institute for Space Research, Landleven 12, 9747-AD Groningen (Netherlands); Ostriker, E. [Department of Astrophysical Sciences, Princeton University, Princeton, NJ 08544 (United States); Tassis, K. [Department of Physics and Institute of Theoretical and Computational Physics, University of Crete, P.O. Box 2208, GR-710 03 Heraklion, Crete (Greece); Shirley, Y. L., E-mail: manferna@gmail.com [Steward Observatory, 933 North Cherry Avenue, Tucson, AZ 85721 (United States)

    2014-08-01

    We present the N{sub 2}H{sup +} (J = 1 → 0) map of the Serpens South molecular cloud obtained as part of the CARMA Large Area Star Formation Survey. The observations cover 250 arcmin{sup 2} and fully sample structures from 3000 AU to 3 pc with a velocity resolution of 0.16 km s{sup –1}, and they can be used to constrain the origin and evolution of molecular cloud filaments. The spatial distribution of the N{sub 2}H{sup +} emission is characterized by long filaments that resemble those observed in the dust continuum emission by Herschel. However, the gas filaments are typically narrower such that, in some cases, two or three quasi-parallel N{sub 2}H{sup +} filaments comprise a single observed dust continuum filament. The difference between the dust and gas filament widths casts doubt on Herschel ability to resolve the Serpens South filaments. Some molecular filaments show velocity gradients along their major axis, and two are characterized by a steep velocity gradient in the direction perpendicular to the filament axis. The observed velocity gradient along one of these filaments was previously postulated as evidence for mass infall toward the central cluster, but these kind of gradients can be interpreted as projection of large-scale turbulence.

  14. The Gaia spectrophotometric standard stars survey -II. Instrumental effects of six ground-based observing campaigns

    CERN Document Server

    Altavilla, G; Pancino, E; Galleti, S; Ragaini, S; Bellazzini, M; Cocozza, G; Bragaglia, A; Carrasco, J M; Castro, A; Di Fabrizio, L; Federici, L; Figueras, F; Gebran, M; Jordi, C; Masana, E; Schuster, W; Valentini, G; Voss, H

    2015-01-01

    The Gaia SpectroPhotometric Standard Stars (SPSS) survey started in 2006, it was awarded almost 450 observing nights, and accumulated almost 100,000 raw data frames, with both photometric and spectroscopic observations. Such large observational effort requires careful, homogeneous, and automated data reduction and quality control procedures. In this paper, we quantitatively evaluate instrumental effects that might have a significant (i.e.,$\\geq$1%) impact on the Gaia SPSS flux calibration. The measurements involve six different instruments, monitored over the eight years of observations dedicated to the Gaia flux standards campaigns: DOLORES@TNG in La Palma, EFOSC2@NTT and ROSS@REM in La Silla, CAFOS@2.2m in Calar Alto, BFOSC@Cassini in Loiano, and LaRuca@1.5m in San Pedro Martir. We examine and quantitatively evaluate the following effects: CCD linearity and shutter times, calibration frames stability, lamp flexures, second order contamination, light polarization, and fringing. We present methods to correct ...

  15. Calibrating the lithium-age relation with open clusters observed with GES (Gaia-ESO Survey)

    Science.gov (United States)

    Gutiérrez Albarrán, M. L.; Montes, D.; Gómez Garrido, M.; Tabernero, H. M..; González Hernández, J. I.; GES Survey Builders

    2017-03-01

    Li depletion is strongly age-dependent but currently available data have shown a complex pattern of Li depletion on the pre- and main-sequence stars that is not yet understood. The lithium abundance observed in late-type stars depend not only of the age and the temperature but also on metallicity, mixing mechanisms, convection structure, rotation and magnetic activity. The large number of stars observed within the Gaia-ESO survey (GES - https://www.gaia-eso.eu/) for many open clusters and associations can be used to calibrate the lithium-age relation and its dependence with other parameters that can be derived from the UVES and GIRAFFE spectroscopic observations. We present here the preliminary results of the analysis of membership and Li abundance of the young clusters and associations, as well as of the intermediate-age and old open clusters, observed until now in GES (iDR4) in order to conduct a comparative study. All this information allowed us to characterize the properties of the members of these clusters and identify a series of field contaminant stars, both lithium-rich giants and non-giant outliers.

  16. CARMA Large Area Star Formation Survey: Observational Analysis of Filaments in the Serpens South Molecular Cloud

    CERN Document Server

    Fernández-López, M; Looney, L; Mundy, L G; Storm, S; Teuben, P J; Lee, K; Segura-Cox, D; Isella, A; Tobin, J J; Rosolowsky, E; Plunkett, A; Kwon, W; Kauffmann, J; Ostriker, E; Tassis, K; Shirley, Y L; Pound, M

    2014-01-01

    We present the N2H+(J=1-0) map of the Serpens South molecular cloud obtained as part of the CARMA Large Area Star Formation Survey (CLASSy). The observations cover 250 square arcminutes and fully sample structures from 3000 AU to 3 pc with a velocity resolution of 0.16 km/s, and they can be used to constrain the origin and evolution of molecular cloud filaments. The spatial distribution of the N2H+ emission is characterized by long filaments that resemble those observed in the dust continuum emission by Herschel. However, the gas filaments are typically narrower such that, in some cases, two or three quasi-parallel N2H+ filaments comprise a single observed dust continuum filament. The difference between the dust and gas filament widths casts doubt on Herschel ability to resolve the Serpens South filaments. Some molecular filaments show velocity gradients along their major axis, and two are characterized by a steep velocity gradient in the direction perpendicular to the filament axis. The observed velocity gra...

  17. Observation and Confirmation of Six Strong Lensing Systems in The Dark Energy Survey Science Verification Data

    CERN Document Server

    Nord, B; Lin, H; Diehl, H T; Helsby, J; Kuropatkin, N; Amara, A; Collett, T; Allam, S; Caminha, G; De Bom, C; Desai, S; Dúmet-Montoya, H; Pereira, M Elidaiana da S; Finley, D A; Flaugher, B; Furlanetto, C; Gaitsch, H; Gill, M; Merritt, K W; More, A; Tucker, D; Rykoff, E S; Rozo, E; Abdalla, F B; Agnello, A; Auger, M; Brunner, R J; Kind, M Carrasco; Castander, F J; Cunha, C E; da Costa, L N; Foley, R; Gerdes, D W; Glazebrook, K; Gschwend, J; Hartley, W; Kessler, R; Lagattuta, D; Lewis, G; Maia, M A G; Makler, M; Menanteau, F; Niernberg, A; Scolnic, D; Vieira, J D; Gramillano, R; Abbott, T M C; Banerji, M; Benoit-Lévy, A; Brooks, D; Burke, D L; Capozzi, D; Rosell, A Carnero; Carretero, J; D'Andrea, C B; Dietrich, J P; Doel, P; Evrard, A E; Frieman, J; Gaztanaga, E; Gruen, D; Honscheid, K; James, D J; Kuehn, K; Li, T S; Lima, M; Marshall, J L; Martini, P; Melchior, P; Miquel, R; Neilsen, E; Nichol, R C; Ogando, R; Plazas, A A; Romer, A K; Sako, M; Sanchez, E; Scarpine, V; Schubnell, M; Sevilla-Noarbe, I; Smith, R C; Soares-Santos, M; Sobreira, F; Suchyta, E; Swanson, M E C; Tarle, G; Thaler, J; Walker, A R; Wester, W; Zhang, Y

    2015-01-01

    We report the observation and confirmation of the first group- and cluster-scale strong gravitational lensing systems found in Dark Energy Survey (DES) data. Through visual inspection of data from the Science Verification (SV) season, we identified 53 candidate systems. We then obtained spectroscopic follow-up of 21 candidates using the Gemini Multi-Object Spectrograph (GMOS) at the Gemini South telescope and the Inamori-Magellan Areal Camera and Spectrograph (IMACS) at the Magellan/Baade telescope. With this follow-up, we confirmed six candidates as gravitational lenses: Three of the systems are newly discovered, and the remaining three were previously known. Of the 21 observed candidates, the remaining 15 were either not detected in spectroscopic observations, were observed and did not exhibit continuum emission (or spectral features), or were ruled out as lensing systems. The confirmed sample consists of one group-scale and five galaxy cluster-scale lenses. The lensed sources range in redshift z ~ 0.80-3.2...

  18. Observation and Confirmation of Six Strong Lensing Systems in The Dark Energy Survey Science Verification Data

    Energy Technology Data Exchange (ETDEWEB)

    Nord, B.; et al.

    2015-12-09

    We report the observation and confirmation of the first group- and cluster-scale strong gravitational lensing systems found in Dark Energy Survey (DES) data. Through visual inspection of data from the Science Verification (SV) season, we identified 53 candidate systems. We then obtained spectroscopic follow-up of 21 candidates using the Gemini Multi-Object Spectrograph (GMOS) at the Gemini South telescope and the Inamori-Magellan Areal Camera and Spectrograph (IMACS) at the Magellan/Baade telescope. With this follow-up, we confirmed six candidates as gravitational lenses: Three of the systems are newly discovered, and the remaining three were previously known. Of the 21 observed candidates, the remaining 15 were either not detected in spectroscopic observations, were observed and did not exhibit continuum emission (or spectral features), or were ruled out as lensing systems. The confirmed sample consists of one group-scale and five galaxy cluster-scale lenses. The lensed sources range in redshift z ~ 0.80-3.2, and in i-band surface brightness i_{SB} ~ 23-25 mag/sq.-arcsec. (2" aperture). For each of the six systems, we estimate the Einstein radius and the enclosed mass, which have ranges ~ 5.0 - 8.6" and ~ 7.5 x 10^{12} - 6.4 x 10^{13} solar masses, respectively.

  19. 739 observed NEAs and new 2-4m survey statistics within the EURONEAR network

    CERN Document Server

    Vaduvescu, O; Tudorica, A; Popescu, M; Colas, F; Asher, D J; Sonka, A; Suciu, O; Lacatus, D; Paraschiv, A; Badescu, T; Tercu, O; Dumitriu, A; Chirila, A; Stecklum, B; Licandro, J; Nedelcu, A; Turcu, E; Vachier, F; Beauvalet, L; Taris, F; Bouquillon, L; Nunez, F Pozo; Saavedra, J P Colque; Unda-Sanzana, E; Karami, M; Khosroshahi, H G; Toma, R; Ledo, H; Tyndall, A; Patrick, L; Fohring, D; Muelheims, D; Enzian, G; Klaes, D; Lenz, D; Mahlberg, P; Ordenes, Y; Sendlinger, K

    2013-01-01

    We report follow-up observations of 477 program Near-Earth Asteroids (NEAs) using nine telescopes of the EURONEAR network having apertures between 0.3 and 4.2 m. Adding these NEAs to our previous results we now count 739 program NEAs followed-up by the EURONEAR network since 2006. The targets were selected using EURONEAR planning tools focusing on high priority objects. Analyzing the resulting orbital improvements suggests astrometric follow-up is most important days to weeks after discovery, with recovery at a new opposition also valuable. Additionally we observed 40 survey fields spanning three nights covering 11 sq. degrees near opposition, using the Wide Field Camera on the 2.5m Isaac Newton Telescope (INT), resulting in 104 discovered main belt asteroids (MBAs) and another 626 unknown one-night objects. These fields, plus program NEA fields from the INT and from the wide field MOSAIC II camera on the Blanco 4m telescope, generated around 12,000 observations of 2,000 minor planets (mostly MBAs) observed i...

  20. The BHB stars in the Survey Fields of Rodgers et al. (1993): New Observations and Comparisons with other Recent Surveys

    CERN Document Server

    Kinman, T D

    2011-01-01

    We study blue horizontal branch (BHB) and RR Lyrae stars in the Rogers et al. (1993a) fields and compare their velocity and density distributions with other surveys in the same part of the sky. Photometric data are given for 176 early-type stars in the northern field. We identify fourteen BHB stars and four possible BHB stars, and determine the selection efficiency of the Century Survey, the HK Survey, and the SDSS survey for BHB stars. We give light curves and \\gamma -radial velocities for three type-ab RR Lyrae stars in the northern field; comparison with the nearby LONEOS Survey shows that there is likely to be an equal number of lower-amplitude type-ab RR Lyrae stars that we do not find. There are therefore at least twice as many BHB stars as type-ab RR Lyrae stars in the northern field--similar to the ratio in the solar neighborhood. The velocity distribution of the southern field shows no evidence for an anomalous thick disk that was found by Gilmore et al. (2002); the halo velocity peaks at a slightly ...

  1. Gemini Observations of Galaxies in Rich Early Environments (GOGREEN) I: survey description

    Science.gov (United States)

    Balogh, Michael L.; Gilbank, David G.; Muzzin, Adam; Rudnick, Gregory; Cooper, Michael C.; Lidman, Chris; Biviano, Andrea; Demarco, Ricardo; McGee, Sean L.; Nantais, Julie B.; Noble, Allison; Old, Lyndsay; Wilson, Gillian; Yee, Howard K. C.; Bellhouse, Callum; Cerulo, Pierluigi; Chan, Jeffrey; Pintos-Castro, Irene; Simpson, Rane; van der Burg, Remco F. J.; Zaritsky, Dennis; Ziparo, Felicia; Alonso, María Victoria; Bower, Richard G.; De Lucia, Gabriella; Finoguenov, Alexis; Lambas, Diego Garcia; Muriel, Hernan; Parker, Laura C.; Rettura, Alessandro; Valotto, Carlos; Wetzel, Andrew

    2017-10-01

    We describe a new Large Program in progress on the Gemini North and South telescopes: Gemini Observations of Galaxies in Rich Early Environments (GOGREEN). This is an imaging and deep spectroscopic survey of 21 galaxy systems at 1 10 in halo mass. The scientific objectives include measuring the role of environment in the evolution of low-mass galaxies, and measuring the dynamics and stellar contents of their host haloes. The targets are selected from the SpARCS, SPT, COSMOS, and SXDS surveys, to be the evolutionary counterparts of today's clusters and groups. The new red-sensitive Hamamatsu detectors on GMOS, coupled with the nod-and-shuffle sky subtraction, allow simultaneous wavelength coverage over λ ˜ 0.6-1.05 μm, and this enables a homogeneous and statistically complete redshift survey of galaxies of all types. The spectroscopic sample targets galaxies with AB magnitudes z΄ < 24.25 and [3.6] μm < 22.5, and is therefore statistically complete for stellar masses M* ≳ 1010.3 M⊙, for all galaxy types and over the entire redshift range. Deep, multiwavelength imaging has been acquired over larger fields for most systems, spanning u through K, in addition to deep IRAC imaging at 3.6 μm. The spectroscopy is ˜50 per cent complete as of semester 17A, and we anticipate a final sample of ˜500 new cluster members. Combined with existing spectroscopy on the brighter galaxies from GCLASS, SPT, and other sources, GOGREEN will be a large legacy cluster and field galaxy sample at this redshift that spectroscopically covers a wide range in stellar mass, halo mass, and clustercentric radius.

  2. The Parkes Galactic Meridian Survey (PGMS): observations and CMB polarization foreground analysis

    CERN Document Server

    Carretti, E; McConnell, D; Bernardi, G; McClure-Griffiths, N M; Cortiglioni, S; Poppi, S

    2009-01-01

    [abridged] We present observations, maps, polarised emission properties study, and CMB foreground analysis of the Parkes Galactic Meridian Survey (PGMS), a project to investigate the Galactic latitude behaviour of the polarized synchrotron emission at 2.3-GHz with the Parkes Radio Telescope. The survey consists of a 5-deg wide strip along the Galactic meridian l=254-deg. We identify three zones distinguished by polarized emission properties: the disc, the halo, and a transition region connecting them. The halo section lies at latitudes |b|>40-deg and is characterised by weak and smooth polarized emission with steep angular power spectra of median slope $\\beta_{\\rm med} \\sim -2.6$. The disc region covers the latitudes |b|<20-deg and shows a brighter, more complex emission with inverted spectra of mean slope $\\bar{\\beta} = -1.8$. The transition region has steep spectra as in the halo, but the emission power increases toward the Galactic plane from halo to disc levels. The change at b ~ -20-deg is sudden, ind...

  3. The JCMT Gould Belt Survey: First results from SCUBA-2 observations of the Cepheus Flare Region

    CERN Document Server

    Pattle, Kate; Kirk, Jason M; Di Francesco, James; Kirk, Helen; Mottram, Joseph C; Keown, Jared; Buckle, Jane; Beaulieu, Sylvie F; Berry, David S; Broekhoven-Fiene, Hannah; Currie, Malcolm J; Fich, Michel; Hatchell, Jenny; Jenness, Tim; Johnstone, Doug; Nutter, David; Pineda, Jaime E; Quinn, Ciera; Salji, Carl; Tisi, Sam; Walker-Smith, Samantha; Hogerheijde, Michiel R; Bastien, Pierre; Bresnahan, David; Butner, Harold; Chen, Mike; Chrysostomou, Antonio; Coudé, Simon; Davis, Chris J; Drabek-Maunder, Emily; Duarte-Cabral, Ana; Fiege, Jason; Friberg, Per; Friesen, Rachel; Fuller, Gary A; Graves, Sarah; Greaves, Jane; Gregson, Jonathan; Holland, Wayne; Joncas, Gilles; Knee, Lewis B G; Mairs, Steve; Marsh, Ken; Matthews, Brenda C; Moriarty-Schieven, Gerald; Mowat, Chris; Rawlings, Jonathan; Richer, John; Robertson, Damien; Rosolowsky, Erik; Rumble, Damian; Sadavoy, Sarah; Thomas, Holly; Tothill, Nick; Viti, Serena; White, Glenn J; Wouterloot, Jan; Yates, Jeremy; Zhu, Ming

    2016-01-01

    We present observations of the Cepheus Flare obtained as part of the James Clerk Maxwell Telescope (JCMT) Gould Belt Legacy Survey (GBLS) with the SCUBA-2 instrument. We produce a catalogue of sources found by SCUBA-2, and separate these into starless cores and protostars. We determine masses and densities for each of our sources, using source temperatures determined by the Herschel Gould Belt Survey. We compare the properties of starless cores in four different molecular clouds: L1147/58, L1172/74, L1251 and L1228. We find that the core mass functions for each region typically show shallower-than-Salpeter behaviour. We find that L1147/58 and L1228 have a high ratio of starless cores to Class II protostars, while L1251 and L1174 have a low ratio, consistent with the latter regions being more active sites of current star formation, while the former are forming stars less actively. We determine that, if modelled as thermally-supported Bonnor-Ebert spheres, most of our cores have stable configurations accessible...

  4. The VLT LBG Redshift Survey - IV. Gas and galaxies at z~3 in observations and simulations

    CERN Document Server

    Tummuangpak, P; Bielby, R; Crighton, N H M; Francke, H; Infante, L; Theuns, T

    2013-01-01

    We use observations and simulations to study the relationship between star-forming galaxies and the IGM at z~3. We use redshift data taken from the VLT LBG Redshift Survey (VLRS) and Keck surveys in fields centred on bright background QSOs, whilst the simulated data is taken from GIMIC. In the simulations, we find that the dominant peculiar velocities are in the form of large-scale coherent motions of gas and galaxies. Gravitational infall of galaxies towards each other is also seen, consistent with linear theory. Peculiar velocity pairs with separations smaller than 1Mpc have a smaller dispersion and better explain the simulated z-space correlations. Lyman-alpha auto- and cross-correlations in the simulations appear to show smaller infall than implied by the expected beta_Lyman-alpha ~ 1.3. Galaxy-wide outflows implemented in the simulations may contribute to this effect. When velocity errors are taken into account, the LBG correlation function prefers the high clustering amplitude shown by higher mass galax...

  5. Spectral Line Survey and Mapping Observations toward the HVCC CO-0.40-0.22

    Science.gov (United States)

    Oka, T.; Mizuno, R.; Miura, K.; Takekawa, S.; Tanaka, K.

    2015-12-01

    We performed a 3 mm band line survey toward CO-0.40-0.22, a small cloud with an extremely large velocity width (Δ V˜90 km s-1) in the central molecular zone of our Galaxy, using the Mopra 22 m telescope. We surveyed the frequency range between 76 GHz and 116 GHz detecting 54 lines from 32 molecules. Analyzing line profiles carefully, we concluded that CH3OH, HC3N, H2CS, SiO, and SO lines are good probes for this cloud. We also have performed deep OTF mapping observations of CO-0.40-0.22 with the NRO 45 m telescope in these probes. Spatial-velocity behaviors of these probes show that this cloud consists of an intense component with shallow velocity gradient and a less intense high-velocity wing. This kinematical structure can be explained by the gravitational kick of a molecular cloud by an invisible compact object with a mass of ˜105 M⊙.

  6. Survey Observations of a Possible Glycine Precursor, Methanimine (CH$_2$NH)

    CERN Document Server

    Suzuki, Taiki; Hirota, Tomoya; Saito, Masao; Majumdar, Liton; Wakelam, Valentine

    2016-01-01

    We conducted survey observations of a glycine precursor, methanimine or methylenimine (CH$_2$NH), with the NRO 45 m telescope and the SMT telescope towards 12 high-mass and two low-mass star-forming regions in order to increase number of CH$_2$NH sources and to better understand the characteristics of CH2NH sources. As a result of our survey, CH$_2$NH was detected in eight sources, including four new sources. The estimated fractional abundances were ~10$^8$ in Orion KL and G10.47+0.03, while they were ~10$^9$ towards the other sources. Our hydrogen recombination line and past studies suggest that CH$_2$NH-rich sources have less evolved HII regions. The less destruction rates by UV flux from the central star would be contributed to the high CH$_2$NH abundances towards CH$_2$NH-rich sources. Our gas-grain chemical simulations suggest that CH$_2$NH is mostly formed in the gas-phase by neutral-neutral reactions rather than the product of thermal evaporation from the dust surfaces.

  7. Wide-Field Infrared Survey Explorer Observations of the Evolution of Massive Star-Forming Regions

    Science.gov (United States)

    Koenig, X. P.; Leisawitz, D. T.; Benford, D. J.; Rebull, L. M.; Padgett, D. L.; Asslef, R. J.

    2012-01-01

    We present the results of a mid-infrared survey of II outer Galaxy massive star-forming regions and 3 open clusters with data from the Wide-field Infrared Survey Explorer (WISE). Using a newly developed photometric scheme to identify young stellar objects and exclude extragalactic contamination, we have studied the distribution of young stars within each region. These data tend to support the hypothesis that latter generations may be triggered by the interaction of winds and radiation from the first burst of massive star formation with the molecular cloud material leftover from that earlier generation of stars. We dub this process the "fireworks hypothesis" since star formation by this mechanism would proceed rapidly and resemble a burst of fireworks. We have also analyzed small cutout WISE images of the structures around the edges of these massive star-forming regions. We observe large (1-3 pc size) pillar and trunk-like structures of diffuse emission nebulosity tracing excited polycyclic aromatic hydrocarbon molecules and small dust grains at the perimeter of the massive star-forming regions. These structures contain small clusters of emerging Class I and Class II sources, but some are forming only a single to a few new stars.

  8. The Spitzer c2d Survey of Large, Nearby, Interstellar Clouds: VII. Ophiuchus Observed with MIPS

    CERN Document Server

    Padgett, Deborah L; Stapelfeldt, Karl R; Chapman, Nicholas L; Lai, Shih-Ping; Mundy, Lee G; Evans, Neal J; Brooke, Timothy Y; Cieza, Lucas A; Spiesman, William J; Noriega-Crespo, Alberto; McCabe, Caer-Eve; Allen, Lori E; Blake, Geoffrey A; Harvey, Paul M; Huard, Tracy L; Jorgensen, Jes K; Koerner, David W; Myers, Philip C; Sargent, Anneila I; Teuben, Peter; van Dishoeck, Ewine F; Wahhaj, Zahed; Young, Kaisa E

    2007-01-01

    We present maps of 14.4 deg^2 of the Ophiuchus dark clouds observed by the Spitzer Space Telescope Multiband Imaging Photometer for Spitzer (MIPS). These high quality maps depict both numerous point sources as well as extended dust emission within the star-forming and non-star-forming portions of these clouds. Using PSF-fitting photometry, we detect 5779 sources at 24 um and 81 sources at 70 um at the 10 sigma level of significance. Three hundred twenty-three candidate young stellar objects (YSOs) were identified according to their positions on the MIPS/2MASS K versus K$-$[24] color-magnitude diagrams as compared to 24 um detections in the SWIRE extragalactic survey. We find that more than half of the YSO candidates, and almost all the ones with protostellar Class I spectral energy distributions, are confined to the known cluster and aggregates.

  9. XMM-Newton and Optical Observations of Cataclysmic Variables from the Sloan Digital Sky Survey

    Science.gov (United States)

    Hilton, Eric J.; Szkody, Paula; Mukadam, Anjum; Henden, Arne; Dillon, William; Schmidt, Gary D.

    2009-03-01

    We report on XMM-Newton and optical results for six cataclysmic variables that were selected from Sloan Digital Sky Survey (SDSS) spectra because they showed strong He II emission lines, indicative of being candidates for containing white dwarfs with strong magnetic fields. While high X-ray background rates prevented optimum results, we are able to confirm SDSS J233325.92+152222.1 as an intermediate polar from its strong pulse signature at 21 minutes and its obscured hard X-ray spectrum. Ground-based circular polarization and photometric observations were also able to confirm SDSS J142256.31 - 022108.1 as a polar with a period near 4 hr. Photometry of SDSS J083751.00+383012.5 and SDSS J093214.82+495054.7 solidifies the orbital period of the former as 3.18 hr and confirms the latter as a high-inclination system with deep eclipses.

  10. Observation of Two New L4 Neptune Trojans in the Dark Energy Survey Supernova Fields

    CERN Document Server

    Gerdes, D W; Bernstein, G M; Sako, M; Adams, F; Goldstein, D; Kessler, R; Abbott, T; Abdalla, F B; Allam, S; Benoit-Lévy, A; Bertin, E; Brooks, D; Buckley-Geer, E; Burke, D L; Capozzi, D; Rosell, A Carnero; Kind, M Carrasco; Carretero, J; Cunha, C E; D'Andrea, C B; da Costa, L N; DePoy, D L; Desai, S; Dietrich, J P; Doel, P; Eifler, T F; Neto, A Fausti; Flaugher, B; Frieman, J; Gaztanaga, E; Gruen, D; Gruendl, R A; Gutierrez, G; Honscheid, K; James, D J; Kuehn, K; Kuropatkin, N; Lahav, O; Li, T S; Maia, M A G; March, M; Martini, P; Miller, C J; Miquel, R; Nichol, R C; Nord, B; Ogando, R; Plazas, A A; Romer, A K; Roodman, A; Sanchez, E; Santiago, B; Schubnell, M; Sevilla-Noarbe, I; Smith, R C; Soares-Santos, M; Sobreira, F; Suchyta, E; Swanson, M E C; Tarlé, G; Thaler, J; Walker, A R; Wester, W; Zhang, Y

    2015-01-01

    We report the discovery of the eighth and ninth known Trojans in stable orbits around Neptune's leading Lagrange point, L4. The objects 2014 QO$_{441}$ and 2014 QP$_{441}$ were detected in data obtained during the 2013-14 and 2014-15 observing seasons by the Dark Energy Survey, using the Dark Energy Camera (DECam) on the 4-meter Blanco telescope at Cerro Tololo Inter-American Observatory. Both are in high-inclination orbits (18.8$^{\\circ}$ and 19.4$^{\\circ}$ respectively). With an eccentricity of 0.104, 2014 QO$_{441}$ has the most eccentric orbit of the eleven known stable Neptune Trojans. Here we describe the search procedure and investigate the objects' long-term dynamical stability and physical properties.

  11. Metallicity Gradients in the Milky Way Disk as Observed by the SEGUE Survey

    CERN Document Server

    Cheng, Judy Y; Morrison, Heather L; Schönrich, Ralph A; Lee, Young Sun; Beers, Timothy C; Bizyaev, Dmitry; Pan, Kaike; Schneider, Donald P

    2011-01-01

    The observed radial and vertical metallicity distribution of old stars in the Milky Way disk provides a powerful constraint on the chemical enrichment and dynamical history of the disk. We present the radial metallicity gradient, \\Delta[Fe/H]/\\Delta R, as a function of height above the plane, |Z|, using 7010 main sequence turnoff stars observed by the Sloan Extension for Galactic Understanding and Exploration (SEGUE) survey. The sample consists of mostly old thin and thick disk stars, with a minimal contribution from the stellar halo, in the region 6 1 kpc. The median metallicity at large |Z| is consistent with the metallicities seen in outer disk open clusters, which exhibit a flat radial gradient at [Fe/H] ~ -0.5. We note that the outer disk clusters are also located at large |Z|; because the flat gradient extends to small R for our sample, there is some ambiguity in whether the observed trends for clusters are due to a change in R or |Z|. We therefore stress the importance of considering both the radial a...

  12. Spitzer 70 and 160-micron Observations of the Extragalactic First Look Survey

    CERN Document Server

    Frayer, D T; Yan, L; Marleau, F R; Choi, P I; Helou, G; Soifer, B T; Appleton, P N; Armus, L; Beck, R; Dole, H; Engelbracht, C W; Fang, F; Gordon, K D; Heinrichsen, I; Henderson, D; Hesselroth, T; Im, M; Kelly, D M; Lacy, M; Laine, S; Latter, W B; Mahoney, W; Makovoz, D; Masci, F J; Morrison, J E; Moshir, M; Noriega-Crespo, A; Padgett, D L; Pesenson, M; Shupe, D L; Squires, G K; Storrie-Lombardi, L J; Surace, J A; Teplitz, H I; Wilson, G

    2005-01-01

    We present Spitzer 70um and 160um observations of the Spitzer extragalactic First Look Survey (xFLS). The data reduction techniques and the methods for producing co-added mosaics and source catalogs are discussed. Currently, 26% of the 70um sample and 49% of the 160um-selected sources have redshifts. The majority of sources with redshifts are star-forming galaxies at z<0.5, while about 5% have infrared colors consistent with AGN. The observed infrared colors agree with the spectral energy distribution (SEDs) of local galaxies previously determined from IRAS and ISO data. The average 160um/70um color temperature for the dust is Td~= 30+/-5 K, and the average 70um/24um spectral index is alpha~= 2.4+/-0.4. The observed infrared to radio correlation varies with redshift as expected out to z~1 based on the SEDs of local galaxies. The xFLS number counts at 70um and 160um are consistent within uncertainties with the models of galaxy evolution, but there are indications that the current models may require slight m...

  13. Observations and properties of candidate high frequency GPS radio sources in the AT20G survey

    CERN Document Server

    Hancock1, Paul J; Mahony, Elizabeth K; Ricci, Roberto

    2010-01-01

    We used the Australia Telescope Compact Array (ATCA) to obtain 40 GHz and 95 GHz observations of a number of sources that were selected from the Australia Telescope Compact Array 20 GHz (AT20G) survey . The aim of the observations was to improve the spectral coverage for sources with spectral peaks near 20 GHz or inverted (rising) radio spectra between 8.6 GHz and 20 GHz. We present the radio observations of a sample of 21 such sources along with optical spectra taken from the ANU Siding Spring Observatory 2.3m telescope and the ESO-New Technology Telescope (NTT). We find that as a group the sources show the same level of variability as typical GPS sources, and that of the 21 candidate GPS sources roughly 60% appear to be genuinely young radio galaxies. Three of the 21 sources studied show evidence of being restarted radio galaxies. If these numbers are indicative of the larger population of AT20G radio sources then as many as 400 genuine GPS sources could be contained within the AT20G with up to 25% of them ...

  14. Optimal design of a lagrangian observing system for hydrodynamic surveys in coastal areas

    Science.gov (United States)

    Cucco, Andrea; Quattrocchi, Giovanni; Antognarelli, Fabio; Satta, Andrea; Maicu, Francesco; Ferrarin, Christian; Umgiesser, Georg

    2014-05-01

    The optimization of ocean observing systems is a pressing need for scientific research. In particular, the improvement of ocean short-term observing networks is achievable by reducing the cost-benefit ratio of the field campaigns and by increasing the quality of measurements. Numerical modeling is a powerful tool for determining the appropriateness of a specific observing system and for optimizing the sampling design. This is particularly true when observations are carried out in coastal areas and lagoons where, the use satellites is prohibitive due to the water shallowness. For such areas, numerical models are the most efficient tool both to provide a preliminary assess of the local physical environment and to make short -term predictions above its change. In this context, a test case experiment was carried out within an enclosed shallow water areas, the Cabras Lagoon (Sardinia, Italy). The aim of the experiment was to explore the optimal design for a field survey based on the use of coastal lagrangian buoys. A three-dimensional hydrodynamic model based on the finite element method (SHYFEM3D, Umgiesser et al., 2004) was implemented to simulate the lagoon water circulation. The model domain extent to the whole Cabras lagoon and to the whole Oristano Gulf, including the surrounding coastal area. Lateral open boundary conditions were provided by the operational ocean model system WMED and only wind forcing, provided by SKIRON atmospheric model (Kallos et al., 1997), was considered as surface boundary conditions. The model was applied to provide a number of ad hoc scenarios and to explore the efficiency of the short-term hydrodynamic survey. A first field campaign was carried out to investigate the lagrangian circulation inside the lagoon under the main wind forcing condition (Mistral wind from North-West). The trajectories followed by the lagrangian buoys and the estimated lagrangian velocities were used to calibrate the model parameters and to validate the

  15. ESO Diffuse Interstellar Bands Large Exploration Survey (EDIBLES) - Merging Observations and Laboratory Data

    Science.gov (United States)

    Salama, Farid

    2016-01-01

    laboratory facilities, MIS and COSmIC, that have been developed for this study and discuss the findings resulting from the comparison of the laboratory data with high resolution, high S/N ratio astronomical observations. MIS stands for Matrix Isolation Spectroscopy, a well-proven technique for isolating cold molecular species in inert solid environments. COSmIC stands for Cosmic Simulation Chamber. It combines a supersonic free jet expansion with discharge plasma and high-sensitivity cavity ringdown spectroscopy and time-of-flight mass spectrometry detection tools for the generation and the detection of cold, isolated gas-phase molecules and ions under experimental conditions that closely mimic interstellar conditions. The column densities of the individual neutral PAH molecules and ions probed in these surveys are derived from the comparison of these unique laboratory data with high resolution, high S/N ratio astronomical observations. The comparisons of astronomical and laboratory data lead to clear and unambiguous conclusions regarding the expected abundances for PAHs of various sizes and charge states in the interstellar environments probed in the surveys. Band profile comparisons between laboratory and astronomical spectra lead to information regarding the molecular structures and characteristics associated with the DIB carriers in the corresponding lines-of-sight. These quantitative surveys of neutral and ionized PAHs in the optical range open the way for unambiguous quantitative searches of PAHs and complex organics in a variety of interstellar and circumstellar environments.

  16. High-J CO survey of low-mass protostars observed with Herschel-HIFI

    CERN Document Server

    Yıldız, Umut A; van Dishoeck, Ewine F; Jose-Garcia, Irene San; Karska, Agata; Harsono, Daniel; Tafalla, Mario; Fuente, Asuncion; Visser, Ruud; Jørgensen, Jes K; Hogerheijde, Michiel R

    2013-01-01

    The evolution of deeply embedded young stellar objects (YSOs) has traditionally been traced through dust continuum spectral energy distributions (SEDs), but the use of CO excitation as an evolutionary probe has not yet been explored due to lack of high-J CO observations. The aim is to constrain the physical characteristics (excitation, kinematics, column density) of the warm gas toward 26 low-mass Class 0 and I YSOs using spectrally-resolved Herschel Space Observatory data of high-J lines of CO. Data are complemented by ground-based observations from APEX and the JCMT to compare those with the colder gas traced by lower-J CO lines. This is the first large spectrally resolved high-J CO survey conducted for these types of sources. The median excitation temperatures for 12CO, 13CO and C18O derived from single-temperature fits to the J_u=2-10 integrated intensities are ~70K, 48K and 37K, respectively, with no significant difference between Class 0 and I sources and no trend with M_env or L_bol. Thus, in contrast ...

  17. The Herschel Orion Protostar Survey: Constraining Protostellar Models with Near- to Far-Infrared Observations

    Science.gov (United States)

    Furlan, Elise; Ali, Babar; Fischer, Will; Tobin, John; Stutz, Amy; Megeath, Tom; Allen, Lori; HOPS Team

    2013-07-01

    During the protostellar stage of star formation, a young star is surrounded by a large infalling envelope of dust and gas; the material falls onto a circumstellar disk and is eventually accreted by the central star. The dust in the disk and envelope emits prominently at mid- to far-infrared wavelengths; at 10 micron, absorption by small silicate grains typically causes a broad absorption feature. By modeling the near- to far-IR spectral energy distributions (SEDs) of protostars, properties of their disks and envelopes can be derived. As part of the Herschel Orion Protostar Survey (HOPS; PI: S. T. Megeath), we have observed a large sample of protostars in the Orion star-forming complex at 70 and 160 micron with the PACS instrument on the Herschel Space Observatory. For most objects, we also have photometry in the near-IR (2MASS), mid-IR (Spitzer/ IRAC and MIPS), at 100 micron (PACS data from the Gould Belt Survey), sub-mm (APEX/SABOCA and LABOCA), and mid-infrared spectra (Spitzer/IRS). For the interpretation of the SEDs, we have constructed a large grid of protostellar models using a Monte Carlo radiative transfer code. Here we present our SED fitting techniques to determine the best-fit model for each object. We show the importance of including IRS spectra with appropriate weights, in addition to the constraints provided by the PACS measurements, which probe the peak of the SED. The 10 micron silicate absorption feature and the mid- to far-IR SED slope provide key constraints for the inclination angle of the object and its envelope density, with a deep absorption feature and steep SED slope for the most embedded and highly inclined objects. We show a few examples that illustrate our SED fitting method and present some preliminary results from our fits.

  18. The JCMT Gould Belt Survey: first results from SCUBA-2 observations of the Cepheus Flare region

    Science.gov (United States)

    Pattle, K.; Ward-Thompson, D.; Kirk, J. M.; Di Francesco, J.; Kirk, H.; Mottram, J. C.; Keown, J.; Buckle, J.; Beaulieu, S. F.; Berry, D. S.; Broekhoven-Fiene, H.; Currie, M. J.; Fich, M.; Hatchell, J.; Jenness, T.; Johnstone, D.; Nutter, D.; Pineda, J. E.; Quinn, C.; Salji, C.; Tisi, S.; Walker-Smith, S.; Hogerheijde, M. R.; Bastien, P.; Bresnahan, D.; Butner, H.; Chen, M.; Chrysostomou, A.; Coudé, S.; Davis, C. J.; Drabek-Maunder, E.; Duarte-Cabral, A.; Fiege, J.; Friberg, P.; Friesen, R.; Fuller, G. A.; Graves, S.; Greaves, J.; Gregson, J.; Holland, W.; Joncas, G.; Knee, L. B. G.; Mairs, S.; Marsh, K.; Matthews, B. C.; Moriarty-Schieven, G.; Mowat, C.; Rawlings, J.; Richer, J.; Robertson, D.; Rosolowsky, E.; Rumble, D.; Sadavoy, S.; Thomas, H.; Tothill, N.; Viti, S.; White, G. J.; Wouterloot, J.; Yates, J.; Zhu, M.

    2017-02-01

    We present observations of the Cepheus Flare obtained as part of the James Clerk Maxwell Telescope (JCMT) Gould Belt Legacy Survey (GBLS) with the SCUBA-2 instrument. We produce a catalogue of sources found by SCUBA-2, and separate these into starless cores and protostars. We determine masses and densities for each of our sources, using source temperatures determined by the Herschel Gould Belt Survey. We compare the properties of starless cores in four different molecular clouds: L1147/58, L1172/74, L1251 and L1228. We find that the core mass functions for each region typically show shallower-than-Salpeter behaviour. We find that L1147/58 and L1228 have a high ratio of starless cores to Class II protostars, while L1251 and L1174 have a low ratio, consistent with the latter regions being more active sites of current star formation, while the former are forming stars less actively. We determine that if modelled as thermally supported Bonnor-Ebert spheres, most of our cores have stable configurations accessible to them. We estimate the external pressures on our cores using archival 13CO velocity dispersion measurements and find that our cores are typically pressure confined, rather than gravitationally bound. We perform a virial analysis on our cores, and find that they typically cannot be supported against collapse by internal thermal energy alone, due primarily to the measured external pressures. This suggests that the dominant mode of internal support in starless cores in the Cepheus Flare is either non-thermal motions or internal magnetic fields.

  19. A deep survey of the AKARI north ecliptic pole field : I. WSRT 20 cm radio survey description, observations and data reduction

    NARCIS (Netherlands)

    White, G. J.; Pearson, C.; Braun, R.; Serjeant, S.; Matsuhara, H.; Takagi, T.; Nakagawa, T.; Shipman, R.; Barthel, P.; Hwang, N.; Lee, H. M.; Lee, M. G.; Im, M.; Wada, T.; Oyabu, S.; Pak, S.; Chun, M. -Y.; Hanami, H.; Goto, T.; Oliver, S.

    2010-01-01

    Aims. The Westerbork Radio Synthesis Telescope, WSRT, has been used to make a deep radio survey of an similar to 1.7 degree(2) field coinciding with the AKARI north ecliptic pole deep field. The observations, data reduction and source count analysis are presented, along with a description of the ove

  20. A deep survey of the AKARI north ecliptic pole field . I. WSRT 20 cm radio survey description, observations and data reduction

    NARCIS (Netherlands)

    White, G. J.; Pearson, C.; Braun, R.; Serjeant, S.; Matsuhara, H.; Takagi, T.; Nakagawa, T.; Shipman, R.; Barthel, P.; Hwang, N.; Lee, H. M.; Lee, M. G.; Im, M.; Wada, T.; Oyabu, S.; Pak, S.; Chun, M.-Y.; Hanami, H.; Goto, T.; Oliver, S.

    2010-01-01

    Aims: The Westerbork Radio Synthesis Telescope, WSRT, has been used to make a deep radio survey of an ~1.7 degree2 field coinciding with the AKARI north ecliptic pole deep field. The observations, data reduction and source count analysis are presented, along with a description of the overall scienti

  1. [Road-side observational survey on 4 unlawful acts among electric bicycle riders in Zhejiang].

    Science.gov (United States)

    Zhao, M; Yu, M; Fang, L; Wang, H; Wu, W X; Huang, G H; Duan, L L; Chen, Z X; Chen, P F

    2016-05-01

    To investigate the prevalence of key unlawful acts among electric bicycle riders and provide evidence for the development of specific interventions. A 4-day road-side survey was conducted in Jinhua, Zhejiang province, in 2013. The speed of electric bicycle was measured by speed measuring instrument and the unlawful acts of riders, such as reverse riding, running the red-light and carrying passengers, were observed with non-participatory way. A total of 3 448 running electric bicycles were observed and the average speed was 26 km/h, the proportion of electric bicycle at the speed of ≥15 km/h was 87.06%. The average speed was highest during 10 am-11 am(30 km/h). the number of observed electric bicycle riders with unlawful acts of ' running the red-light','reverse riding' and ' carrying passengers' were 1 315, 656 and 1 877 respectively, and the estimated rate was 10.01%, 4.99% and 15.22%, respectively. More ' running the red-light','reverse riding' and ' carrying passengers' occurred during 7 am-8 am(14.59%)and 13 pm-14 pm(15.25%), 13 pm-14 pm(7.33%)and 17 pm-18 pm(7.63%), 6 am-7 am(32.44%)and 12 pm-13 pm(27.90%), respectively. Overspeeding, carrying passengers, running the red-light, reverse riding were the key unlawful acts among electric bicycle riders. Targeted intervention should be carried out to reduce the prevalence of unlawful riding acts and the incidence of electric bicycle related injuries and deaths.

  2. Validation and Application of the Constructivist Learning Environment Survey in English Language Teacher Education Classrooms in Iran

    Science.gov (United States)

    Ebrahimi, Nabi. A.

    2015-01-01

    This article reports the validation and application of an English language teacher education (LTE) version of the Constructivist Learning Environment Survey (CLES). The instrument, called the CLES-LTE, was field tested with a sample of 622 Iranian English language student teachers in 28 classes. When principal components analysis led to the…

  3. Correlating student knowledge and confidence using a graded knowledge survey to assess student learning in a general microbiology classroom.

    Science.gov (United States)

    Favazzo, Lacey; Willford, John D; Watson, Rachel M

    2014-12-01

    Knowledge surveys are a type of confidence survey in which students rate their confidence in their ability to answer questions rather than answering the questions. These surveys have been discussed as a tool to evaluate student in-class or curriculum-wide learning. However, disagreement exists as to whether confidence is actually an accurate measure of knowledge. With the concomitant goals of assessing content-based learning objectives and addressing this disagreement, we present herein a pretest/posttest knowledge survey study that demonstrates a significant difference correctness on graded test questions at different levels of reported confidence in a multi-semester timeframe. Questions were organized into Bloom's taxonomy, allowing for the data collected to further provide statistical analyses on strengths and deficits in various levels of Bloom's reasoning with regard to mean correctness. Collectively, students showed increasing confidence and correctness in all levels of thought but struggled with synthesis-level questions. However, when students were only asked to rate confidence and not answer the accompanying test questions, they reported significantly higher confidence than the control group which was asked to do both. This indicates that when students do not attempt to answer questions, they have significantly greater confidence in their ability to answer those questions. Additionally, when students rate only confidence without answering the question, resolution across Bloom's levels of reasoning is lost. Based upon our findings, knowledge surveys can be an effective tool for assessment of both breadth and depth of knowledge, but may require students to answer questions in addition to rating confidence to provide the most accurate data.

  4. Incivility beyond the Classroom Walls

    Science.gov (United States)

    Bjorklund, Wendy L.; Rehling, Diana L.

    2011-01-01

    Classroom incivility has become a major concern in higher education. Faculty and students frequently interact outside of class, and the lack of civility in those interactions can influence the relationship between students and faculty and impact classroom dynamics. Based on a survey of faculty at a Midwestern public university, this study reports…

  5. The XMM Deep Survey in the CDF-S VIII. UV catalogue of the Optical Monitor observations

    CERN Document Server

    Antonucci, M; Vagnetti, F; Trevese, D; Comastri, A; Paolillo, M; Ranalli, P; Vignali, C

    2014-01-01

    The XMM-Newton X-ray observatory has performed repeated observations of the CDFS in 33 epochs (2001-2010) through the XMM-CDFS Deep Survey. During the X-ray observations, XMM-OM targeted the central 17x17 arcmin2 region of the X-ray field of view, providing simultaneous optical/UV coverage of the CDFS. The resulting set of data can be taken into account to build an XMM-OM catalogue of the CDFS, filling the UV spectral coverage between the optical surveys and GALEX observations. We present the UV catalogue of the XMM-CDFS Deep Survey. Its main purpose is to provide complementary UV average photometric measurements of known optical/UV sources in the CDFS, taking advantage of the unique characteristics of the survey. The data reduction is intended also to improve the standard source detection on individual observations, by cataloguing faint sources through the stacking of their exposure images. We reprocessed the XMM-OM data of the survey and we stacked the exposures from consecutive observations using the stand...

  6. Application of classroom observation in"surgical nursing"teaching%课堂观察法在《外科护理技术》教学中的应用

    Institute of Scientific and Technical Information of China (English)

    王博; 宫小飞

    2013-01-01

    Through the classroom observation, analysis of factors for effective teaching in classroom teaching, improve the consciousness and ability of teachers' classroom effective teaching. And found that the teachers in classroom teaching, provides objective feedback in order to seek the effective teaching methods and means, so as to further improve the level of teaching.%通过课堂观察,对课堂教学进行有效教学的因素分析,提高教师课堂有效教学的意识和能力。并发现教师课堂教学中的问题,为寻求有效的教学方式和手段提供客观的反馈,从而进一步提高教学水平。

  7. National survey of health in the tattoo industry: Observational study of 448 French tattooists

    Directory of Open Access Journals (Sweden)

    Nicolas Kluger

    2017-02-01

    Full Text Available Objectives: The data regarding the health of professional tattooists is inexistent. Tattooists are usually heavily tattooed and exposed daily to body fluids and skin-to-skin contacts with customers, tattoo inks, solvents, allergens, irritants, and work for hours often in inadequate positions using vibrating tattoo machines. We analyzed the health status of active French professional tattooists. Material and Methods: An observational self-reported Internet survey was performed among 448 tattooists who were members of the French Tattoo Union in November 2013. Results: The main physical complaints were musculoskeletal: back pain (65%, finger pain (41.5% and muscular pain (28.8%. Finger pain, back pain, muscular pain and carpal tunnel symptoms/tingling sensations on the fingers occurred among 88%, 61.5%, 68% and 84% of the cases after having started their activity (p < 0.001. Other chronic diseases, autoimmune diseases and cancers remained at a low level here. Conclusions: Professional tattooists have a high prevalence of musculoskeletal complaints about back pain due to repetitive movements, awkward postures and use of a vibrating tattoo machine. Tattooists have a unique environment that imply developing intervention and preventive strategies for them. Int J Occup Med Environ Health 2017;30(1:111–120

  8. The Spitzer c2d Survey of Large, Nearby, Interstellar Clouds VIII. Serpens Observed with MIPS

    CERN Document Server

    Harvey, Paul M; Brooke, Tim; Spiesman, William J; Chapman, Nicholas; Huard, Tracy L; Evans, Neal J; Cieza, Lucas; Lai, Shih-Ping; Allen, Lori E; Mundy, Lee G; Padgett, Deborah L; Sargent, Anneila I; Stapelfeldt, Karl R; Myers, Philip C; van Dishoeck, Ewine F; Blake, Geoffrey A; Koerner, David W

    2007-01-01

    We present maps of 1.5 square degrees of the Serpens dark cloud at 24, 70, and 160\\micron observed with the Spitzer Space Telescope MIPS Camera. More than 2400 compact sources have been extracted at 24um, nearly 100 at 70um, and 4 at 160um. We estimate completeness limits for our 24um survey from Monte Carlo tests with artificial sources inserted into the Spitzer maps. We compare source counts, colors, and magnitudes in the Serpens cloud to two reference data sets, a 0.50 deg^2 set on a low-extinction region near the dark cloud, and a 5.3 deg^2 subset of the SWIRE ELAIS N1 data that was processed through our pipeline. These results show that there is an easily identifiable population of young stellar object candidates in the Serpens Cloud that is not present in either of the reference data sets. We also show a comparison of visual extinction and cool dust emission illustrating a close correlation between the two, and find that the most embedded YSO candidates are located in the areas of highest visual extinct...

  9. National asthma observational survey of severe asthmatics in Israel: the no-air study

    Directory of Open Access Journals (Sweden)

    Izbicki Gabriel

    2012-06-01

    Full Text Available Abstract Background Asthma is considered a global public health issue requiring a significant medical expenditure as a result of its high prevalence and the low rate of disease control. Objective This is the first nationwide survey of severe asthma patients carried out in Israel. In this study we aimed to assess health resources utilization, compliance with treatment and disease-control in a subgroup of patients with severe asthma in Israel. Material and method One hundred and twenty-three patients with a diagnosis of asthma for more then one year, as well as a hospitalization during the last 12 months due to asthma exacerbation or maintenance systemic steroids therapy, were included in this non-interventional observational study. Results Asthma was uncontrolled in 43.9%, partly controlled in 50.4% and well controlled in only 5.7%. The majority of the patients (83% were compliant with drug treatment. Conclusion The fact that 83% of the asthma patients included in this study were compliant with their asthma therapy was not manifested in asthma control. Therefore concrete tools are required for achieving and maintaining asthma control, especially in the treatment of the most severe asthmatic patients.

  10. A high-resolution spectropolarimetric survey of Herbig Ae/Be stars - I. Observations and measurements

    CERN Document Server

    Alecian, E; Catala, C; Grunhut, J H; Landstreet, J D; Bagnulo, S; Böhm, T; Folsom, C P; Marsden, S; Waite, I

    2012-01-01

    This is the first in a series of papers in which we describe and report the analysis of a large survey of Herbig Ae/Be stars in circular spectropolarimetry. Using the ESPaDOnS and Narval high-resolution spectropolarimeters at the Canada-France-Hawaii and Bernard Lyot Telescopes, respectively, we have acquired 132 circularly-polarised spectra of 70 Herbig Ae/Be stars and Herbig candidates. The large majority of these spectra are characterised by a resolving power of about 65,000, and a spectral coverage from about 3700 ang to 1 micron. The peak SNR per CCD pixel ranges from below 100 (for the faintest targets) to over 1000 (for the brightest). The observations were acquired with the primary aim of searching for magnetic fields in these objects. However, our spectra are suitable for a variety of other important measurements, including rotational properties, variability, binarity, chemical abundances, circumstellar environment conditions and structure, etc. In this first paper, we describe the sample selection, ...

  11. The globular cluster system in NGC5866: optical observations from HST Advanced Camera for Surveys

    CERN Document Server

    Cantiello, Michele; Raimondo, Gabriella

    2007-01-01

    We perform a detailed study of the Globular Cluster (GC) system in the galaxy NGC5866 based on F435W, F555W, and F625W (~ B, V, and R) HST Advanced Camera for Surveys images. Adopting color, size and shape selection criteria, the final list of GC candidates comprises 109 objects, with small estimated contamination from background galaxies, and foreground stars. The color distribution of the final GC sample has a bimodal form. Adopting color to metallicity transformations derived from the Teramo--SPoT simple stellar population model, we estimate a metallicity [Fe/H]~ -1.5, and -0.6 dex for the blue and red peaks, respectively. A similar result is found if the empirical color-metallicity relations derived from Galactic GCs data are used. The two subpopulations show some of the features commonly observed in the GC system of other galaxies, like a ``blue tilt'', higher central concentrations of the red subsystem, and larger half--light radii at larger galactocentric distances. However, we do not find evidence of ...

  12. Offshore observations of eastern red bats (Lasiurus borealis in the Mid-Atlantic United States using multiple survey methods.

    Directory of Open Access Journals (Sweden)

    Shaylyn K Hatch

    Full Text Available Little is known about the migration and movements of migratory tree-roosting bat species in North America, though anecdotal observations of migrating bats over the Atlantic Ocean have been reported since at least the 1890s. Aerial surveys and boat-based surveys of wildlife off the Atlantic Seaboard detected a possible diurnal migration event of eastern red bats (Lasiurus borealis in September 2012. One bat was sighted approximately 44 km east of Rehoboth Beach, Delaware during a boat-based survey. Eleven additional bats were observed between 16.9 and 41.8 km east of New Jersey, Delaware, and Virginia in high definition video footage collected during digital aerial surveys. Observations were collected incidentally as part of a large baseline study of seabird, marine mammal, and sea turtle distributions and movements in the offshore environment. Digital survey methods also allowed for altitude estimation for several of these bats at >100 m above sea level. These observations provide new evidence of bat movements offshore, and offer insight into their flight heights above sea level and the times of day at which such migrations may occur.

  13. Loggerhead sea turtle bycatch data in artisanal fisheries within a marine protected area: fishermen surveys versus scientific observations

    Directory of Open Access Journals (Sweden)

    Lozano, M.

    2011-06-01

    Full Text Available Loggerhead sea turtles can be incidentally captured by artisanal gears but information about the impact of this fishing is inconsistent and scarce. Recent studies have observed that the bycatch, or incidental catch rate, in fishermen surveys is irregular. The aim of this study was to compare direct data (onboard observers concerning the incidental catch of loggerhead sea turtles by the artisanal vessels versus data from fishermen surveys. The study area was the Cabo de Gata-Níjar marine protected area, situated in the western Mediterranean (southeast of the Iberian peninsula. We observed two loggerhead turtles that were incidentally caught in a total of 165 fishing operations. According to fishermen surveys, a total of nine loggerheads were incidentally caught in 861 fishing operations. The differences between the loggerhead sea turtle bycatch reported by fishermen surveys and scientific observations versus random distribution (x2 = 0.3146, P = 0.575, df = 1 were not significant. We conclude that the surveys are useful but that findings should be interpreted with caution.

  14. The VLT-FLAMES Tarantula Survey: I. Introduction and observational overview

    NARCIS (Netherlands)

    Evans, C.J.; Taylor, W.D.; Hénault-Brunet, V.; Sana, H.A.A.; de Koter, A.; Simón-Díaz, S.; Carraro, G.; Bagnoli, T.; Bastian, N.; Bestenlehner, J.M.; Bonanos, A.Z.; Bressert, E.; Brott, I.; Campbell, M.A.; Cantiello, M.; Clark, J.S.; Costa, E.; Crowther, P.A.; de Mink, S.E.; Doran, E.; Dufton, P.L.; Dunstall, P.R.; Friedrich, K.; Garcia, M.; Gieles, M.; Gräfener, G.; Herrero, A.; Howarth, I.D.; Izzard, R.G.; Langer, N.; Lennon, D.J.; Maiz Apellániz, J.; Markova, N.; Najarro, F.; Puls, J.; Ramirez, O.H.; Sabín-Sanjulián, C.; Smartt, S.J.; Stroud, V.E.; van Loon, J.T.; Vink, J.S.; Walborn, N.R.

    2011-01-01

    The VLT-FLAMES Tarantula Survey (VFTS) is an ESO Large Programme that has obtained multi-epoch optical spectroscopy of over 800 massive stars in the 30 Doradus region of the Large Magellanic Cloud (LMC). Here we introduce our scientific motivations and give an overview of the survey targets, includi

  15. The VLT-FLAMES Tarantula Survey. I. Introduction and observational overview

    NARCIS (Netherlands)

    Evans, C.J.; Taylor, W.D.; de Koter, A.; Brott, I.; Walborn, N.R.

    2011-01-01

    The VLT-FLAMES Tarantula Survey (VFTS) is an ESO Large Programme that has obtained multi-epoch optical spectroscopy of over 800 massive stars in the 30 Doradus region of the Large Magellanic Cloud (LMC). Here we introduce our scientific motivations and give an overview of the survey targets, includi

  16. The Classroom Animal: Mealworms.

    Science.gov (United States)

    Kramer, David C., Ed.

    1985-01-01

    Describes appearance, longevity, and changes in each step of the mealworm life cycle. Guidelines for starting a classroom colony are given with housing and care instructions. Suggested observations, activities, and questions for students are included. (DH)

  17. Functions of Teacher and Student Code-Switching in an EFL Classroom and Pedagogical Focus: Observations and Implications

    Directory of Open Access Journals (Sweden)

    Stefan Rathert

    2012-11-01

    Full Text Available Code-switching (CS, the alternation between two or more languages within a stretch of language, is accepted as a valuable strategy of bilinguals in making linguistic choices for communicative purposes. Following different perspectives, CS can be understood either as an attempt to communicate meanings at the macro level (such as identity, solidarity etc., or to convey intended meaning to the listener within the boundaries of conversational interaction at the micro level. Accepted as a strategy of speakers in bilingual communities, CS in foreign language learning settings is still a contentious matter. However, its potential has been emphasized in recent studies. This small-scale study examines teacher and student CS occurrences in an EFL lesson at a Turkish state university. CS occurrences were transcribed and sample extracts were analyzed through conversational analysis. The results show that teachers and learners apply CS to generate access to language or as a tool in classroom management. This study also reveals that CS can be a learner strategy to avoid L2 when lesson content is of little relevance to learners. In such cases CS cannot fulfil its potential as a means in discourse strategy, and language learning is unlikely to be facilitated.

  18. Angular spectra of the intrinsic galaxy ellipticity field, their observability and their impact on lensing in tomographic surveys

    Science.gov (United States)

    Schäfer, Björn Malte; Merkel, Philipp M.

    2017-09-01

    This paper describes intrinsic ellipticity correlations between galaxies, their statistical properties, their observability with future surveys and their interference with weak gravitational lensing measurements. Using an angular-momentum-based, quadratic intrinsic alignment model we derive correlation functions of the ellipticity components and project them to yield the four non-zero angular ellipticity spectra C^ɛ _E(ℓ), C^ɛ _B(ℓ), C^ɛ _C(ℓ) and C^ɛ _S(ℓ) in their generalization to tomographic surveys. For a Euclid-like survey, these spectra would have amplitudes smaller than the weak lensing effect on non-linear structures, but would constitute an important systematics. Computing estimation biases for cosmological parameters derived from an alignment-contaminated survey suggests biases of +5σw for the dark energy equation of state parameter w, -20σ _{Ω _m} for the matter density Ωm and -12σ _{σ _8} for the spectrum normalization σ8. Intrinsic alignments yield a signal that is easily observable with a survey similar to Euclid: while not independent, significances for estimates of each of the four spectra reach values of tens of σ if weak lensing and shape noise are considered as noise sources, which suggests relative uncertainties on alignment parameters at the percent level, implying that galaxy alignment mechanisms can be investigated by future surveys.

  19. SURVEY

    DEFF Research Database (Denmark)

    SURVEY er en udbredt metode og benyttes inden for bl.a. samfundsvidenskab, humaniora, psykologi og sundhedsforskning. Også uden for forskningsverdenen er der mange organisationer som f.eks. konsulentfirmaer og offentlige institutioner samt marketingsafdelinger i private virksomheder, der arbejder...... med surveys. Denne bog gennemgår alle surveyarbejdets faser og giver en praktisk indføring i: • design af undersøgelsen og udvælgelse af stikprøver, • formulering af spørgeskemaer samt indsamling og kodning af data, • metoder til at analysere resultaterne...

  20. Incremental Validity of Test Session and Classroom Observations in a Multimethod Assessment of Attention Deficit/Hyperactivity Disorder

    Science.gov (United States)

    McConaughy, Stephanie H.; Harder, Valerie S.; Antshel, Kevin M.; Gordon, Michael; Eiraldi, Ricardo; Dumenci, Levent

    2010-01-01

    This study tested the incremental validity of behavioral observations, over and above parent and teacher reports, for assessing symptoms of Attention Deficit/Hyperactivity Disorder (ADHD) in children ages 6 to 12, using the Test Observation Form (TOF) and Direct Observation Form (DOF) from the Achenbach System of Empirically Based Assessment. The…

  1. Incremental Validity of Test Session and Classroom Observations in a Multimethod Assessment of Attention Deficit/Hyperactivity Disorder

    Science.gov (United States)

    McConaughy, Stephanie H.; Harder, Valerie S.; Antshel, Kevin M.; Gordon, Michael; Eiraldi, Ricardo; Dumenci, Levent

    2010-01-01

    This study tested the incremental validity of behavioral observations, over and above parent and teacher reports, for assessing symptoms of Attention Deficit/Hyperactivity Disorder (ADHD) in children ages 6 to 12, using the Test Observation Form (TOF) and Direct Observation Form (DOF) from the Achenbach System of Empirically Based Assessment. The…

  2. Spectroscopic observation of SN 2017pp by NUTS (NOT Un-biased Transient Survey)

    Science.gov (United States)

    Pastorello, A.; Elias-Rosa, N.; Benetti, S.; Cappellaro, E.; Terreran, G.; Tomasella, L.; Tronsgaard, R.

    2017-01-01

    The Nordic Optical Telescope (NOT) Unbiased Transient Survey (NUTS; ATel #8992) reports the spectroscopic classification of SN 2017pp in PGC 1378162. The candidate was discovered by F. Ciabattari, E. Mazzoni, S. Donati (ISSP; http://italiansupernovae.org).

  3. Observations of Whooping Cranes During Winter Aerial Surveys: 1950–2011

    Data.gov (United States)

    US Fish and Wildlife Service, Department of the Interior — The Aransas-Wood Buffalo population of whooping cranes (Grus americana) declined to near extinction by the 1940s. Starting in winter 1950–1951, annual aerial surveys...

  4. Policy implications of using a household consumption and expenditures survey versus an observed-weighed food record survey to design a food fortification program.

    Science.gov (United States)

    Lividini, Keith; Fiedler, John L; Bermudez, Odilia I

    2013-12-01

    Observed-Weighed Food Record Surveys (OWFR) are regarded as the most precise dietary assessment methodology, despite their recognized shortcomings, which include limited availability, high cost, small samples with uncertain external validity that rarely include all household members, Hawthorne effects, and using only 1 or 2 days to identify "usual intake." Although Household Consumption and Expenditures Surveys (HCES) also have significant limitations, they are increasingly being used to inform nutrition policy To investigate differences in fortification simulations based on OWFR and HCES from Bangladesh. The pre- and postfortification nutrient intake levels from the two surveys were compared. The total population-based rank orderings of oil, wheat flour, and sugar coverage were identical for the two surveys. OWFR found differences in women's and children's coverage rates and average quantities consumed for all three foods that were not detected by HCES. Guided by the Food Fortification Formulator, we found that these differences did not result in differences in recommended fortification levels. Differences were found, however, in estimated impacts: although both surveys found that oil would be effective in reducing the prevalence of inadequate vitamin A intake among both subpopulations, only OWFR also found that sugar and wheat flour fortification would significantly reduce inadequate vitamin A intake among children. Despite the less precise measure of food consumption from HCES, the two surveys provide similar guidance for designing a fortification program. The external validity of these findings is limited. With relatively minor modifications, the precision of HCES in dietary assessment and the use ofHCES in fortification programming could be strengthened.

  5. Classroom Behaviors of Asian American Students in Mathematics.

    Science.gov (United States)

    Huang, Shwu-yong L.; Waxman, Hersholt C.

    This study examines Asian American middle school students' classroom behaviors in mathematics using systematic classroom observation techniques. The study explores questions related to classroom behaviors in terms of interactions with teachers, classroom settings, activities, and manners; differences in classroom behaviors between boys and girls…

  6. [Results from the X-ray and Optical Follow-up Observations of the Swift BAT AGN Survey

    Science.gov (United States)

    Mushotzky, R.

    2008-01-01

    I will present results from the x-ray and optical follow-up observations of the Swift BAT ACN survey. I will discuss the nature of obscuration in these objects, the relationship to optical properties and the change of properties with luminosity and galaxy type and how they will influence the design of XO.

  7. Precision Analysis of Trimble Rtx Surveying Technology with Xfill Function in the Context of Obtained Conversion Observations

    Directory of Open Access Journals (Sweden)

    Krzyżek Robert

    2015-02-01

    Full Text Available As a result of traditional geodetic surveying we usually achieve observations which are then used for calculating rectangular coordinates onto a plane along with precision evaluation. In this article the surveying methods are presented in which the situation is different. Test measurements were carried out, consisting in the measurement of a fragment of detailed control network in RTK (Real Time Kinematic and RTX (Real Time Extended mode with xFill function. First, the rectangular coordinates onto a plane (through the transformation of data ellipsoidal were obtained, on the basis of which the conversion observations were determined and they were compared with each other, as well as with reference parameters - conversion observations out of detailed control network adjustment with use of the method of least squares. The results of the study allow to verify the precision and application possibilities of conversion observations obtained thanks to Trimble RTX technology with xFill function. Application of this surveying method in typical geodetic tasks is fully justifiable. Nevertheless, it is recommendable to be aware of the correlations of absolute or relative values obtained in RTX procedure to reference parameters, which in turn will enable conclusive verification of the possibilities of Trimble RTX technology application in certain geodetic surveys.

  8. Herschel observations of EXtra-Ordinary Sources (HEXOS): The present and future of spectral surveys with Herschel/HIFI

    NARCIS (Netherlands)

    Bergin, E. A.; Phillips, T. G.; Comito, C.; Crockett, N. R.; Lis, D. C.; Schilke, P.; Wang, S.; Bell, T. A.; Blake, G. A.; Bumble, B.; Caux, E.; Cabrit, S.; Ceccarelli, C.; Cernicharo, J.; Daniel, F.; de Graauw, Th.; Dubernet, M.-L.; Emprechtinger, M.; Encrenaz, P.; Falgarone, E.; Gerin, M.; Giesen, T. F.; Goicoechea, J. R.; Goldsmith, P. F.; Gupta, H.; Hartogh, P.; Helmich, F. P.; Herbst, E.; Joblin, C.; Johnstone, D.; Kawamura, J. H.; Langer, W. D.; Latter, W. B.; Lord, S. D.; Maret, S.; Martin, P. G.; Melnick, G. J.; Menten, K. M.; Morris, P.; Müller, H. S. P.; Murphy, J. A.; Neufeld, D. A.; Ossenkopf, V.; Pagani, L.; Pearson, J. C.; Pérault, M.; Plume, R.; Roelfsema, P.; Qin, S.-L.; Salez, M.; Schlemmer, S.; Stutzki, J.; Tielens, A. G. G. M.; Trappe, N.; van der Tak, F. F. S.; Vastel, C.; Yorke, H. W.; Yu, S.; Zmuidzinas, J.

    2010-01-01

    We present initial results from the Herschel GT key program: Herschel observations of EXtra-Ordinary Sources (HEXOS) and outline the promise and potential of spectral surveys with Herschel/HIFI. The HIFI instrument offers unprecedented sensitivity, as well as continuous spectral coverage across the

  9. EUVE All-Sky Survey Observations of the Dwarf Nova VW Hydri

    Science.gov (United States)

    Mauche, C. W.; Warren, J. K.; Vallerga, J. V.; Mukai, K.; Mattei, J. A.

    1993-05-01

    The dwarf nova VW Hyi was observed from 1992 November 1 to 18 and from November 20 to 23 by the Extreme Ultraviolet Explorer (EUVE) satellite during its all-sky survey. The total time on source was 22 kiloseconds. During the first part of the scan, VW Hyi was in quiescence following a superoutburst and was not detected by EUVE above background. However, the source went into a narrow outburst on November 13.8 U.T., peaked at V ~ 10 on November 14.8 U.T., started to fade on November 15.9 U.T., and returned to quiescence on November 17.8 U.T. In contrast, the source did not turn on in the EUV until November 15.0 U.T., did not peak until November 15.3 U.T., and had returned to quiescence by November 16.3 U.T. Accounting for the different sensitivities in the two wavebands, we conclude that the EUV outburst was delayed relative to the optical outburst by ~ 0.5 day and that the EUV outburst was narrower than the optical outburst by ~ 1 day. During the peak of the EUV outburst, the source was detected at the 3sigma level in the Lex/B (50--180 Angstroms ) scanner with a count rate of ~ 0.03 s(-1) and at the 4sigma level in the Al/Ti/C (160--240 Angstroms ) scanner with a count rate of ~ 0.09 s(-1) . That the Al/Ti/C count rate is significantly higher than the Lex/B count rate, whereas the effective area of the Al/Ti/C filter is smaller than that of the Lex/B filter, strongly indicates that the source was very soft when it was on. We use the count rates in these two filters to constrain the temperature and luminosity of the source of the shortest wavelength radiation in VW Hyi: the inner disk and the boundary layer between the disk and the surface of the white dwarf.

  10. Virtual Visits and Patient-Centered Care: Results of a Patient Survey and Observational Study.

    Science.gov (United States)

    McGrail, Kimberlyn Marie; Ahuja, Megan Alyssa; Leaver, Chad Andrew

    2017-05-26

    Virtual visits are clinical interactions in health care that do not involve the patient and provider being in the same room at the same time. The use of virtual visits is growing rapidly in health care. Some health systems are integrating virtual visits into primary care as a complement to existing modes of care, in part reflecting a growing focus on patient-centered care. There is, however, limited empirical evidence about how patients view this new form of care and how it affects overall health system use. Descriptive objectives were to assess users and providers of virtual visits, including the reasons patients give for use. The analytic objective was to assess empirically the influence of virtual visits on overall primary care use and costs, including whether virtual care is with a known or a new primary care physician. The study took place in British Columbia, Canada, where virtual visits have been publicly funded since October 2012. A survey of patients who used virtual visits and an observational study of users and nonusers of virtual visits were conducted. Comparison groups included two groups: (1) all other BC residents, and (2) a group matched (3:1) to the cohort. The first virtual visit was used as the intervention and the main outcome measures were total primary care visits and costs. During 2013-2014, there were 7286 virtual visit encounters, involving 5441 patients and 144 physicians. Younger patients and physicians were more likely to use and provide virtual visits (Pvirtual visit patients indicated that virtual visits were liked by patients, with 372 (93.2%) of respondents saying their virtual visit was of high quality and 364 (91.2%) reporting their virtual visit was "very" or "somewhat" helpful to resolve their health issue. Segmented regression analysis and the corresponding regression parameter estimates suggested virtual visits appear to have the potential to decrease primary care costs by approximately Can $4 per quarter (Can -$3.79, P=.12

  11. The Test Matters: The Relationship between Classroom Observation Scores and Teacher Value Added on Multiple Types of Assessment

    Science.gov (United States)

    Grossman, Pam; Cohen, Julie; Ronfeldt, Matthew; Brown, Lindsay

    2014-01-01

    In this study, we examined how the relationships between one observation protocol, the Protocol for Language Arts Teaching Observation (PLATO), and value-added measures shift when different tests are used to assess student achievement. Using data from the Measures of Effective Teaching Project, we found that PLATO was more strongly related to the…

  12. Classroom Observations and Reflections: Using Online Streaming Video as a Tool for Overcoming Barriers and Engaging in Critical Thinking

    Science.gov (United States)

    Barlow, Angela T.; McCrory, Michael R.; Blessing, Stephen

    2013-01-01

    In typical school settings, teachers are not afforded the opportunity to observe the instructional practices of their peers. Time constraints, opportunity, and willingness to participate in observational practices are just three of the factors that may limit teachers' engagement in this type of activity. To provide teachers with opportunities to…

  13. Analysing language classrooms through classroom interaction

    Directory of Open Access Journals (Sweden)

    Müge Gündüz

    2014-11-01

    Full Text Available This research study focuses on teacher-student and student-student interaction, which are considered very important aspects of classroom life. There has been a growth of interest in the analysis of teacher language and interaction in language classrooms and many (e.g. Ellis, 1994; Tsui, 2001 believe that classroom interaction is one of the major variables affecting SLA in formal settings. This study aims to give some insight into classroom interaction and how this interaction shapes L2 learning and teaching in Turkey and England. Systematic classroom observation along with the field notes taken to record observations is the main research method in this study used to describe and examine interaction patterns and to measure learner production in secondary classes in Turkey and England. The participants are foreign language teachers and non-native speaking students. Over a month, more than 50 lessons were observed in the secondary schools in both Turkey and England at two levels (13-14 and 14-15 year age group. In Turkey, English classes were observed whereas in England, the observation was conducted in German and French classes. English is taught as a foreign language in Turkey; German and French are also taught as a foreign language in England. The findings of this research study are expected to provide a better understanding of instructional practices and procedures in L2 classrooms. The results of this research study, however, should be seen as suggestive rather than conclusive since they are derived from a relatively small sample.

  14. Classroom Dimensions and Classroom Types.

    Science.gov (United States)

    Kendall, Arthur J.; Solomon, Daniel

    Although classroom "openness" has been much discussed in recent years, there has been little effort to investigate to what degree this openness occurs within a general sample of classrooms. The purpose of this study is to identify significant attributes of classroom activity and organization relevant to the concepts of "traditional" and "open" and…

  15. Deep far infrared ISOPHOT survey in "Selected Area 57" - I. Observations and source counts

    DEFF Research Database (Denmark)

    Linden-Vornle, M.J.D.; Nørgaard-Nielsen, Hans Ulrik; Jørgensen, H.E.

    2000-01-01

    We present here the results of a deep survey in a 0.4 deg(2) blank field in Selected Area 57 conducted with the ISOPHOT instrument aboard ESAs Infrared Space Observatory (ISO1) at both 60 mu m and 90 mu m. The resulting sky maps have a spatial resolution of 15 x 23 arcsrc(2) per pixel which is much...

  16. The Sloan Lens ACS Survey. VII. Elliptical galaxy scaling laws from direct observational mass measurements

    NARCIS (Netherlands)

    Bolton, Adam S.; Treu, Tommaso; Koopmans, Leon V. E.; Gavazzi, Raphael; Moustakas, Leonidas A.; Burles, Scott; Schlegel, David J.; Wayth, Randall

    2008-01-01

    We use a sample of 53 massive early-type strong gravitational lens galaxies with well-measured redshifts (ranging from z = 0.06 to 0.36) and stellar velocity dispersions (between 175 and 400 km s(-1)) from the Sloan Lens ACS (SLACS) Survey to derive numerous empirical scaling relations. The ratio be

  17. Differentiation in Classroom Practice

    DEFF Research Database (Denmark)

    Mottelson, Martha

    2015-01-01

    Differentiation in School Practice is an ongoing research project currently being carried out in UCC’s research department by myself and my coworker Christina Jørgensen. The project includes a field study of everyday life in a Danish 5th grade classroom with the aim to observe, describe and analy...... those everyday practices in the classroom that ultimately result in offering students different positions, identities and opportunities for participation....

  18. 10C Survey of Radio Sources at 15.7 GHz: I - Observing, mapping and source extraction

    OpenAIRE

    2010-01-01

    We have observed an area of approximatley 27 deg^2 to an rms noise level of less than 0.2 mJy at 15.7 GHz, using the Arcminute Microkelvin Imager Large Array. These observations constitute the most sensitive radio-source survey of any extent (greater than approximately 0.2 deg^2) above 1.4 GHz. This paper presents the techniques employed for observing, mapping and source extraction. We have used a systematic procedure for extracting information and producing source catalogues, from maps with ...

  19. Assertive classroom management strategies and students’ performance: The case of EFL classroom

    OpenAIRE

    Mohammad Aliakbari; Bafrin Bozorgmanesh

    2015-01-01

    Ample research findings support the effective role that classroom management strategies play in enhancing students’ learning. Drawing upon Iranian high school teachers’ classroom management strategies, this article is intended to examine the extent to which these teachers follow assertive classroom management strategies and if these strategies affect students’ performance. Conducting a survey including 123 female students, it was found out that Iranian teachers apply classroom management stra...

  20. 翻转课堂之《制作市场调查问卷》教学设计%Flip Classroom Teaching Design for Making Market Survey Questionnaire

    Institute of Scientific and Technical Information of China (English)

    周惠娟

    2014-01-01

    The new form of teaching, flip Classroom teaching is to reverse knowledge imparting and internalization, to realize the reform of traditional teaching. This article uses the flip classroom teaching mode, to analyze the context of Make Market Survey Questionnaire. We also conduct before class task and class teaching task design.%翻转课堂教学是将知识传授与内化进行颠倒的新型教学形式,实现了对传统教学的改革。本文使用翻转课堂的教学模式,对《制作市场调查问卷》的教学内容进行分析,并对课前任务及课堂教学进行了设计。

  1. Deformation Study of Papandayan Volcano using GPS Survey Method and Its Correlation with Seismic Data Observation

    Directory of Open Access Journals (Sweden)

    Dina A. Sarsito

    2006-11-01

    Full Text Available Papandayan volcano located in the southern part of Garut regency, around 70 km away from Bandung city, West Java. Many methods carried out to monitoring the activities of volcano, both continuously or periodically, one of the monitoring method is periodically GPS survey. Basically those surveys are carried out to understand the pattern and velocity of displacement which occurred in the volcano body, both horizontally and vertically, and also others deformation elements such as; translation, rotation and dilatation. The Mogi modeling was also used to determine the location and volume of the pressure source which caused deformation of volcano body. By comparing seismic activity and the deformation reveal from GPS measurement, before, during and after eruption, it could be understood there is a correlation between the seismicity and its deformation. These studies is hoping that GPS measurement in Papandayan volcano could be one of supported method to determine the volcano activities, at least in Papandayan volcano.

  2. Large collaboration in observational astronomy: the Gemini Planet Imager exoplanet survey case

    CERN Document Server

    Marchis, Franck; Perrin, Marshall D; Konopacky, Quinn M; Savransky, Dmitry; Macintosh, Bruce; Marois, Christian; Graham, James R

    2016-01-01

    The Gemini Planet Imager (GPI) is a next-generation high-contrast imager built for the Gemini Observatory. The GPI exoplanet survey (GPIES) consortium is made up of 102 researchers from 28 institutions in North and South America and Europe. In November 2014, we launched a search for young Jovian planets and debris disks. In this paper, we discuss how we have coordinated the work done by this large team to improve the technical and scientific productivity of the campaign, and describe lessons we have learned that could be useful for future instrumentation-based astronomical surveys. The success of GPIES lies mostly on its decentralized structure, clear definition of policies that are signed by each member, and the heavy use of modern tools for communicating, exchanging information, and processing data.

  3. Large collaboration in observational astronomy: the Gemini Planet Imager exoplanet survey case

    Science.gov (United States)

    Marchis, Franck; Kalas, Paul G.; Perrin, Marshall D.; Konopacky, Quinn M.; Savransky, Dmitry; Macintosh, Bruce; Marois, Christian; Graham, James R.

    2016-08-01

    The Gemini Planet Imager (GPI) is a next-generation high-contrast imager built for the Gemini Observatory. The GPI exoplanet survey (GPIES) consortium is made up of 102 researchers from 28 institutions in North and South America and Europe. In November 2014, we launched a search for young Jovian planets and debris disks. In this paper, we discuss how we have coordinated the work done by this large team to improve the technical and scientific productivity of the campaign, and describe lessons we have learned that could be useful for future instrumentation-based astronomical surveys. The success of GPIES lies mostly on its decentralized structure, clear definition of policies that are signed by each member, and the heavy use of modern tools for communicating, exchanging information, and processing data.

  4. The Detection of Interstellar Ethanimine (CH3CHNH) from Observations taken during the GBT PRIMOS Survey

    CERN Document Server

    Loomis, Ryan A; Steber, Amanda L; Neill, Justin L; Muckle, Matthew T; Harris, Brent J; Hollis, Jan M; Jewell, Philip R; Lattanzi, Valerio; Lovas, Frank J; Martinez,, Oscar; McCarthy, Michael C; Remijan, Anthony J; Pate, Brooks H

    2013-01-01

    We have performed reaction product screening measurements using broadband rotational spectroscopy to identify rotational transition matches between laboratory spectra and the Green Bank Telescope PRIMOS radio astronomy survey spectra in Sagittarius B2 North (Sgr B2(N)). The broadband rotational spectrum of molecules created in an electrical discharge of CH3CN and H2S contained several frequency matches to unidentified features in the PRIMOS survey that did not have molecular assignments based on standard radio astronomy spectral catalogs. Several of these transitions are assigned to the E- and Z-isomers of ethanimine. Global fits of the rotational spectra of these isomers in the range of 8 to 130 GHz have been performed for both isomers using previously published mm-wave spectroscopy measurements and the microwave measurements of the current study. Possible interstellar chemistry formation routes for E-ethanimine and Z-ethanimine are discussed. The detection of ethanimine is significant because of its possibl...

  5. The effects of methylphenidate on the classroom behavior of elementary school-age children with cerebral palsy: a preliminary observational analysis.

    Science.gov (United States)

    Symons, Frank J; Tervo, Raymond C; Kim, Ockjean; Hoch, John

    2007-01-01

    High- and low-dose methylphenidate administration was evaluated prospectively for 3 elementary school-age children with cerebral palsy, cognitive impairments, and attention-deficit hyperactivity disorder (ADHD) symptoms using single-case, randomized, double-blind, placebo-controlled designs. An observational time sampling protocol was used to directly measure and quantify classroom behavior. Summary level analysis showed that (1) low-dose (0.3 mg/kg/dose) administration was associated with clinically significant (>50%) reductions in stereotyped and disruptive behavior relative to baseline and placebo conditions, (2) high-dose (0.5 mg/kg/dose) administration was associated with exacerbated amounts of stereotyped and disruptive behavior, and (3) no changes were directly observed for task-related behavior at either dose. Results are discussed with respect to previous research with methylphenidate administration and cerebral palsy, and the suggestion is made that further work using larger, randomly selected study samples with complementary measures of behavior and performance appears warranted.

  6. ADDING CONTEXT TO JAMES WEBB SPACE TELESCOPE SURVEYS WITH CURRENT AND FUTURE 21 cm RADIO OBSERVATIONS

    Energy Technology Data Exchange (ETDEWEB)

    Beardsley, A. P.; Morales, M. F. [Department of Physics, University of Washington Seattle, WA 98195 (United States); Lidz, A.; Malloy, M. [Department of Physics and Astronomy, University of Pennsylvania, Philadelphia, PA 19104 (United States); Sutter, P. M., E-mail: beards@phys.washington.edu [INFN - National Institute for Nuclear Physics via Valerio 2, I-34127, Trieste (Italy)

    2015-02-20

    Infrared and radio observations of the Epoch of Reionization promise to revolutionize our understanding of the cosmic dawn, and major efforts with the JWST, MWA, and HERA are underway. While measurements of the ionizing sources with infrared telescopes and the effect of these sources on the intergalactic medium with radio telescopes should be complementary, to date the wildly disparate angular resolutions and survey speeds have made connecting proposed observations difficult. In this paper we develop a method to bridge the gap between radio and infrared studies. While the radio images may not have the sensitivity and resolution to identify individual bubbles with high fidelity, by leveraging knowledge of the measured power spectrum we are able to separate regions that are likely ionized from largely neutral, providing context for the JWST observations of galaxy counts and properties in each. By providing the ionization context for infrared galaxy observations, this method can significantly enhance the science returns of JWST and other infrared observations.

  7. Millimeter- and Submillimeter-Wave Observations of the OMC-2/3 Region. III. An Extensive Survey for Molecular Outflows

    CERN Document Server

    Takahashi, Satoko; Ohashi, Nagayoshi; Kusakabe, Nobuhiko; Takakuwa, Shigehisa; Shimajiri, Yoshito; Tamura, Motohide; Kawabe, Ryohei

    2008-01-01

    Using the ASTE 10 m submillimeter telescope and the 1.4 m Infrared Survey Facility (IRSF), we performed an extensive outflow survey in the Orion Molecular Cloud -2 and -3 region. Our survey, which includes 41 potential star-forming sites, has been newly compiled using multi-wavelength data based on millimeter- and submillimeter-continuum observations as well as radio continuum observations. From the CO (3-2) observations performed with the ASTE 10 m telescope, we detected 14 CO molecular outflows, seven of which were newly identified. This higher detection rate, as compared to previous CO (1-0) results in the same region, suggests that CO (3-2) may be a better outflow tracer. Physical properties of these outflows and their possible driving sources were derived. Derived parameters were compared with those of CO outflows in low- and high-mass starforming regions. We show that the CO outflow momentum correlates with the bolometric luminosity of the driving source and with the envelope mass, regardless of the mas...

  8. The Spitzer Survey of Interstellar Clouds in the Gould Belt. IV. Lupus V and VI Observed with IRAC and MIPS

    CERN Document Server

    Spezzi, Loredana; Merın, Bruno; Allen, Lori E; Evans, Neal J; Jørgensen, Jes K; Bourke, Tyler L; Cieza, Lucas A; Dunham, Michael M; Harvey, Paul M; Huard, Tracy L; Peterson, Dawn; Tothill, Nick F H

    2011-01-01

    We present Gould's Belt (GB) Spitzer IRAC and MIPS observations of the Lupus V and VI clouds and discuss them in combination with near-infrared (2MASS) data. Our observations complement those obtained for other Lupus clouds within the frame of the Spitzer "Core to Disk" (c2d) Legacy Survey. We found 43 Young Stellar Object (YSO) candidates in Lupus V and 45 in Lupus VI, including 2 transition disks, using the standard c2d/GB selection method. None of these sources was classified as a pre-main sequence star from previous optical, near-IR and X-ray surveys. A large majority of these YSO candidates appear to be surrounded by thin disks (Class III; ~79% in Lupus V and ~87% in Lupus VI). These Class III abundances differ significantly from those observed for the other Lupus clouds and c2d/GB surveyed star-forming regions, where objects with optically thick disks (Class II) dominate the young population. We investigate various scenarios that can explain this discrepancy. In particular, we show that disk photo-evapo...

  9. TIMASSS: The IRAS16293-2422 Millimeter And Submillimeter Spectral Survey. I. Observations, calibration and analysis of the line kinematics

    CERN Document Server

    Caux, E; Castets, A; Coutens, A; Ceccarelli, C; Bacmann, A; Bisshop, S; Bottinelli, S; Comito, C; Helmich, F P; Lefloch, B; Parise, B; Schilke, P; Tielens, A G G M; van Dishoeck, E; Vastel, C; Wakelam, V; Walters, A

    2011-01-01

    While unbiased surveys observable from ground-based telescopes have previously been obtained towards several high mass protostars, very little exists on low mass protostars. To fill up this gap, we carried out a complete spectral survey of the bands at 3, 2, 1 and 0.8 mm towards the solar type protostar IRAS16293-2422. The observations covered about 200\\,GHz and were obtained with the IRAM-30m and JCMT-15m telescopes. Particular attention was devoted to the inter-calibration of the obtained spectra with previous observations. All the lines detected with more than 3 sigma and free from obvious blending effects were fitted with Gaussians to estimate their basic kinematic properties. More than 4000 lines were detected (with sigma \\geq 3) and identified, yielding a line density of approximatively 20 lines per GHz, comparable to previous surveys in massive hot cores. The vast majority (~2/3) of the lines are weak and due to complex organic molecules. The analysis of the profiles of more than 1000 lines belonging 7...

  10. The relationship between classroom quality and students' engagement in secondary school

    OpenAIRE

    Virtanen, Tuomo; Lerkkanen, Marja-Kristiina; Poikkeus, Anna-Maija; Kuorelahti, Matti

    2015-01-01

    Student engagement has been identified as an influential mediator between classroom interactional quality and adolescent learning outcomes. This study examined the relationship between classroom quality and student behavioural engagement in secondary school classrooms. Three dimensions of classroom quality (emotional, organisational and instructional support) and the dimension of student engagement were observed in nine classrooms using the Classroom Assessment Scoring System. Self-ratings of...

  11. Classroom Management

    OpenAIRE

    2008-01-01

    This paper is aiming to discover the paths that enable teachers to manage their work with students in the classroom. To be an efficient teacher means to know with what and how to motivate students to learn. Teacher as an efficient classroom manager needs to have skills to plan and prepare the education process, know how to organize the teaching and how to guide the class. An efficient teacher moreover needs o establish positive classroom climate and working discipline. Also, teacher should be...

  12. Scrutinizing a Survey-Based Measure of Science and Mathematics Teacher Knowledge: Relationship to Observations of Teaching Practice

    Science.gov (United States)

    Talbot, Robert M.

    2016-12-01

    There is a clear need for valid and reliable instrumentation that measures teacher knowledge. However, the process of investigating and making a case for instrument validity is not a simple undertaking; rather, it is a complex endeavor. This paper presents the empirical case of one aspect of such an instrument validation effort. The particular instrument under scrutiny was developed in order to determine the effect of a teacher education program on novice science and mathematics teachers' strategic knowledge (SK). The relationship between novice science and mathematics teachers' SK as measured by a survey and their SK as inferred from observations of practice using a widely used observation protocol is the subject of this paper. Moderate correlations between parts of the observation-based construct and the SK construct were observed. However, the main finding of this work is that the context in which the measurement is made (in situ observations vs. ex situ survey) is an essential factor in establishing the validity of the measurement itself.

  13. Voids in the SDSS DR9: observations, simulations, and the impact of the survey mask

    CERN Document Server

    Sutter, P M; Wandelt, Benjamin D; Weinberg, David H; Warren, Michael S

    2013-01-01

    We present and study cosmic voids identified using the watershed void finder ZOBOZ in the Sloan Digital Sky Survey Data Release 9, compare these voids to ones identified in mock catalogs, and assess the impact of the survey mask on void statistics such as number functions, ellipticity distributions, and radial density profiles. The nearly 1,000 identified voids span three volume-limited samples from redshift z=0.43 to 0.7. For comparison we use 98 of the publicly available 2LPT-based mock galaxy catalogs of Manera et al. (2012), and also generate our own mock catalogs by applying a Halo Occupation Distribution model to an N-body simulation. We find that the mask reduces the number density of voids at all scales by a factor of three and slightly skews the relative size distributions. This engenders an increase in the mean ellipticity by roughly 30%. However, we find that radial density profiles are largely robust to the effects of the mask. We see excellent agreement between the data and both mock catalogs, an...

  14. Extending the limits of globule detection -- ISOPHOT Serendipity Survey Observations of interstellar clouds

    CERN Document Server

    Tóth, L V; Juvela, M; Stickel, M; Liesenfeld, U; Hotzel, S; Kiss, Cs.

    2002-01-01

    A faint $I_{\\rm 170}=4$ MJysr$^{-1}$ bipolar globule was discovered with the ISOPHOT 170 $\\mu$m Serendipity Survey (ISOSS). ISOSS J 20246+6541 is a cold ($T_{\\rm d}\\approx 14.5$ K) FIR source without an IRAS pointsource counterpart. In the Digitized Sky Survey B band it is seen as a 3\\arcmin size bipolar nebulosity with an average excess surface brightness of $\\approx 26$ mag/$\\square $\\arcsec . The CO column density distribution determined by multi-isotopic, multi-level CO measurements with the IRAM-30m telescope agrees well with the optical appearance. An average hydrogen column density of $\\approx 10^{21}$cm$^{-2}$ was derived from both the FIR and CO data. Using a kinematic distance estimate of 400 pc the NLTE modelling of the CO, HCO$^+$, and CS measurements gives a peak density of $\\approx 10^4$cm$^{-3}$. The multiwavelength data characterise ISOSS 20246+6541 as a representative of a class of globules which has not been discovered so far due to their small angular size and low 100$\\mu $m brightness. A s...

  15. Teaching and Learning about Matter in Grade 6 Classrooms: A Conceptual Change Approach

    Science.gov (United States)

    Pimthong, Pattamaporn; Yutakom, Naruemon; Roadrangka, Vantipa; Sanguanruang, Sudjid; Cowie, Bronwen; Cooper, Beverley

    2012-01-01

    The purpose of this study was to enhance the teaching and learning of matter and its properties for grade 6 students. The development of a conceptual change approach instructional unit was undertaken for this purpose. Pre- and post-concept surveys, classroom observations, and student and teacher interviews were used to collect data. The teaching…

  16. Observation and analysis of a classroom teaching and learning practice based on augmented reality and serious games on mobile platforms

    Directory of Open Access Journals (Sweden)

    Sylvie Barma

    2015-06-01

    Full Text Available This qualitative research is part of a learning effort to better understand how serious games are exploited in a science education context. The research team examined this issue by focusing on augmented reality as a technological innovation imbedded on a tablet. Given the current state of knowledge related to serious games and augmented reality, and given the fact that its use in the context of teaching/learning is not extended, this paper focuses on an initial exploration of how a new teaching practice involving a serious game based on an interactive augmented reality solution would impact on students in a physics class. A Design Based Research methodology was applied in a real‑world context within a college‑level physics class. Two conceptual tests containing ten questions on spatial notions regarding electromagnetic fields were administered to two control groups and two groups using the proposed serious game. The latter groups were administrated a game evaluation questionnaire as well. Thematic interpretation of students written responses to the evaluation questionnaire as well as the lessons and observations we derived from the in-class experimentation are provided and discussed in the paper.

  17. Physical properties of star clusters in the outer LMC as observed by the Dark Energy Survey

    CERN Document Server

    Pieres, A; Balbinot, E; Luque, E; Queiroz, A B A; da Costa, L N; Maia, M A G; Drlica-Wagner, A; Roodman, A; Abbott, C; Allam, S; Benoit-Levy, A; Bertin, E; Brooks, D; Buckley-Geer, E; Burke, D L; Rosell, A Carnero; Kind, M Carrasco; Carretero, J; Cunha, C E; Desai, S; Diehl, H T; Eifler, T F; Finley, D A; Flaugher, B; Fosalba, P; Frieman, J; Gerdes, D W; Gruen, D; Gruendl, R A; Gutierrez, G; Honscheid, K; James, D J; Kuehn, K; Kuropatkin, N; Lahav, O; Li, T S; Marshall, J L; Martini, P; Miller, C J; Miquel, R; Nichol, R C; Nord, B; Ogando, R; Plazas, A A; Romer, A K; Sanchez, E; Scarpine, V; Schubnell, M; Sevilla-Noarbe, I; Smith, R C; Soares-Santos, M; Sobreira, F; Suchyta, E; Swanson, M E C; Tarle, G; Thaler, J; Thomas, D; Tucker, D; Walker, A R

    2015-01-01

    The Large Magellanic Cloud (LMC) harbors a rich and diverse system of star clusters, whose ages, chemical abundances, and positions provide information about the LMC history of star formation. We use Science Verification imaging data from the Dark Energy Survey to increase the census of known star clusters in the outer LMC and to derive physical parameters for a large sample of such objects using a spatially and photometrically homogeneous data set. Our sample contains 255 visually identified cluster candidates, of which 109 were not listed in any previous catalog. We quantify the crowding effect for the stellar sample produced by the DES Data Management pipeline and conclude that the stellar completeness is < 10% inside typical LMC cluster cores. We therefore develop a pipeline to sample and measure stellar magnitudes and positions around the cluster candidates using DAOPHOT. We also implement a maximum-likelihood method to fit individual density profiles and colour-magnitude diagrams. For 117 (from a tot...

  18. Learning from 8 years of regional cyanobacteria observation in Brittany in view of sanitary survey improvement.

    Science.gov (United States)

    Pitois, Frédéric; Thomas, Olivier; Thoraval, Isabelle; Baurès, Estelle

    2014-01-01

    Cyanobacteria and cyanotoxins have been more and more studied during the last decades with regard to environment and health issues. More recently the consequences of climate change reinforced the need for research in view of a better management of cyanobacteria blooms. In this context the exploitation of the water quality survey of 26 recreational lakes in Brittany (north western France) between 2004 and 2011 is reported in this paper in order to encompass spatial and interannual patterns of cyanobacteria development at a regional scale. Starting from weekly data principally acquired during summertime, the links between cyanobacteria cell densities, toxin occurrences and interannual meteorological factors can give insights on the potential evolution of cyanobacterial crisis in the future. This study is part of a project aiming at a better understanding of potentially toxic cyanobacteria crisis occurrences in recreational waters, in order to improve predictive monitoring routines.

  19. Analysis of the GPS Observations of the Site Survey at Sheshan 25-m Radio Telescope in August 2008

    Science.gov (United States)

    Liu, L.; Cheng, Z. Y.; Li, J. L.

    2010-01-01

    The processing of the GPS observations of the site survey at Sheshan 25-m radio telescope in August 2008 is reported. Because each session in this survey is only about six hours, not allowing the subdaily high frequency variations in the station coordinates to be reasonably smoothed, and because there are serious cycle slips in the observations and a large volume of data would be rejected during the software automatic adjustment of slips, the ordinary solution settings of GAMIT needed to be adjusted by loosening the constraints in the a priori coordinates to 10 m, adopting the "quick" mode in the solution iteration, and combining Cview manual operation with GAMIT automatic fixing of cycle slips. The resulting coordinates of the local control polygon in ITRF2005 are then compared with conventional geodetic results. Due to large rotations and translations in the two sets of coordinates (geocentric versus quasi-topocentric), the seven transformation parameters cannot be solved for directly. With various trial solutions it is shown that with a partial pre-removal of the large parameters, high precision transformation parameters can be obtained with post-fit residuals at the millimeter level. This analysis is necessary to prepare the follow-on site and transformation survey of the VLBI and SLR telescopes at Sheshan

  20. Incivility Beyond the Classroom Walls

    Directory of Open Access Journals (Sweden)

    Wendy L. Bjorklund, PhD

    2011-08-01

    Full Text Available Classroom incivility has become a major concern in higher education. Faculty and students frequently interact outside of class, and the lack of civility in those interactions can influence the relationship between students and faculty and impact classroom dynamics. Based on a survey of faculty at a Midwestern public university, this study reports that faculty experience a fair amount of moderately inappropriate student behavior outside the classroom, including missing scheduled appointments, wearing revealing clothing, and requesting a grade change. These results can help faculty and administrators guide students toward more appropriate behavior and create better relationships between faculty and students.

  1. Investigation on Classroom Questioning, Improving the Teaching Engagement: Classroom Observation Report on Teaching Quality in Schools for Rural Migrant Children (continued)%问诊课堂提问,提高教学的参与度——上海进城务工人员随迁子女学校课堂质量观察报告(续)

    Institute of Scientific and Technical Information of China (English)

    黄忠敬; 王美玲

    2015-01-01

    经过为期三年的参与式教学培训,上海市M区进城务工人员随迁子女学校的课堂发生了较大变化.本文在对七所学校14节课堂进行观察测量的基础上,通过与三年前课堂观察结果进行对比分析,发现:学校教师对参与式教学理念已经普遍认同,教学技能得到了有效改进,课堂质量也获得了整体提升.%Great changes and improvement happened in the classrooms of schools for rural migrant children in M District'' Shanghai after the intervention of a three-year participatory teacher training.We did classroom observation analysis on 14 classrooms (Chinese, English, mathematics) in seven schools and conducted comparative analysis of the 2011 and 2014 by using data from observation protocols. Research ifndings: school teachers have widely recognized the concept of participatory teaching, improved teaching skills effectivily and enhanced the overall classroom teaching quality largely.

  2. Outdoor Classrooms

    Science.gov (United States)

    Mayes, Valynda

    2010-01-01

    An outdoor classroom is the ideal vehicle for community involvement: Parents, native plant societies, 4-H, garden clubs, and master naturalists are all resources waiting to be tapped, as are local businesses offering support. If you enlist your community in the development and maintenance of your outdoor classroom, the entire community will…

  3. The LAMOST survey of background quasars in the vicinity of the Andromeda and Triangulum galaxies. II. Results from the commissioning observations and the pilot surveys

    Energy Technology Data Exchange (ETDEWEB)

    Huo, Zhi-Ying; Bai, Zhong-Rui; Chen, Jian-Jun; Chen, Xiao-Yan; Du, Bing; Jia, Lei; Lei, Ya-Juan [Key Laboratory of Optical Astronomy, National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100012 (China); Liu, Xiao-Wei; Yuan, Hai-Bo [Kavli Institute for Astronomy and Astrophysics, Peking University, Beijing 100871 (China); Xiang, Mao-Sheng; Huang, Yang; Zhang, Hui-Hua [Department of Astronomy, Peking University, Beijing 100871 (China); Yan, Lin [Infrared Processing and Analysis Center, California Institute of Technology, MS 100-22, Pasadena, CA 91125 (United States); Chu, Jia-Ru; Chu, Yao-Quan; Hu, Hong-Zhuan [University of Science and Technology of China, Hefei 230026 (China); Cui, Xiang-Qun; Hou, Yong-Hui; Hu, Zhong-Wen; Jiang, Fang-Hua, E-mail: zhiyinghuo@bao.ac.cn [Nanjing Institute of Astronomical Optics and Technology, National Astronomical Observatories, Chinese Academy of Sciences, Nanjing 210042 (China); and others

    2013-06-01

    We present new quasars discovered in the vicinity of the Andromeda and Triangulum galaxies with the Large Sky Area Multi-Object Fiber Spectroscopic Telescope, also named the Guoshoujing Telescope, during the 2010 and 2011 observational seasons. Quasar candidates are selected based on the available Sloan Digital Sky Survey, Kitt Peak National Observatory 4 m telescope, Xuyi Schmidt Telescope Photometric Survey optical, and Wide-field Infrared Survey Explorer near-infrared photometric data. We present 509 new quasars discovered in a stripe of ∼135 deg{sup 2} from M31 to M33 along the Giant Stellar Stream in the 2011 pilot survey data sets, and also 17 new quasars discovered in an area of ∼100 deg{sup 2} that covers the central region and the southeastern halo of M31 in the 2010 commissioning data sets. These 526 new quasars have i magnitudes ranging from 15.5 to 20.0, redshifts from 0.1 to 3.2. They represent a significant increase of the number of identified quasars in the vicinity of M31 and M33. There are now 26, 62, and 139 known quasars in this region of the sky with i magnitudes brighter than 17.0, 17.5, and 18.0, respectively, of which 5, 20, and 75 are newly discovered. These bright quasars provide an invaluable collection with which to probe the kinematics and chemistry of the interstellar/intergalactic medium in the Local Group of galaxies. A total of 93 quasars are now known with locations within 2.°5 of M31, of which 73 are newly discovered. Tens of quasars are now known to be located behind the Giant Stellar Stream, and hundreds are behind the extended halo and its associated substructures of M31. The much enlarged sample of known quasars in the vicinity of M31 and M33 can potentially be utilized to construct a perfect astrometric reference frame to measure the minute proper motions (PMs) of M31 and M33, along with the PMs of substructures associated with the Local Group of galaxies. Those PMs are some of the most fundamental properties of the Local

  4. Increasing Positive Interactive Classroom Behavior.

    Science.gov (United States)

    Kotcher, Elaine; Doremus, Richard R.

    During the spring of 1972 training workshops for 88 elementary and secondary teachers of the Great Neck Public Schools held to examine four hypotheses: 1) workshops in training teachers to observe classroom behavior would significantly increase these same teachers' positive classroom interactive behaviors consisting of teacher, pupil-pupil,…

  5. EVN observations of 6.7 GHz methanol masers from Medicina survey

    CERN Document Server

    Voronkov, M A; Palagi, F; Tofani, G

    2002-01-01

    We report VLBI observations of methanol masers in the brightest 5(1)-6(0) A+ transition at 6.7 GHz in NGC 281W, 18151-1208 and 19388+2357. Using the fringe rate method absolute positions were obtained for all observed sources. A linear ordered structure with a velocity gradient was revealed in NGC 281W. Under assumption that such structure is an edge-on Keplerian disk around the central object with a mass of 30Msun located at a distance of 3.5 kpc from the Sun, we estimated that methanol masers are situated at the distance about 400 a.u. from the center of the disk. A second epoch of observations was reported for L1206, GL2789 and 20062+3550. The upper limits on the relative motions of maser spots are estimated to be 4.7 km/s and 28 km/s for L1206 and GL2789 respectively.

  6. Subaru Telescope adaptive optics observations of gravitationally lensed quasars in the Sloan Digital Sky Survey

    CERN Document Server

    Rusu, Cristian E; Minowa, Yosuke; Iye, Masanori; Inada, Naohisa; Oya, Shin; Kayo, Issha; Hayano, Yutaka; Hattori, Masayuki; Saito, Yoshihiko; Ito, Meguru; Pyo, Tae-Soo; Terada, Hiroshi; Takami, Hideki; Watanabe, Makoto

    2015-01-01

    We present the results of an imaging observation campaign conducted with the Subaru Telescope adaptive optics system (IRCS+AO188) on 26 gravitationally lensed quasars (24 doubles, 1 quad, and 1 possible triple) from the SDSS Quasar Lens Search. We develop a novel modelling technique that fits analytical and hybrid point spread functions (PSFs), while simultaneously measuring the relative astrometry, photometry, as well as the lens galaxy morphology. We account for systematics by simulating the observed systems using separately observed PSF stars. The measured relative astrometry is comparable with that typically achieved with the Hubble Space Telescope, even after marginalizing over the PSF uncertainty. We model for the first time the quasar host galaxies in 5 systems, without a-priory knowledge of the PSF, and show that their luminosities follow the known correlation with the mass of the supermassive black hole. For each system, we obtain mass models far more accurate than those previously published from low...

  7. Lightcurve Survey of V-type Asteroids. I. Observations until Spring 2004

    CERN Document Server

    Hasegawa, Sunao; Yoshizumi, Chiaki; Sekiguchi, Tomohiko; Sarugaku, Yuki; Nishihara, Setsuko; Kitazato, Kouhei; Abe, Masanao; Mito, Hiroyuki

    2012-01-01

    To examine the distribution of rotational rates for chips of asteroid 4 Vesta, lightcurve observation of seven V-type asteroids (2511 Patterson, 2640 Hallstorm, 2653 Principia, 2795 Lapage, 3307 Athabasca, 4147 Lennon, and 4977 Rauthgundis) were performed from fall 2003 to spring 2004. Distribution of spin rates of V-type main-belt asteroids from the past and our observations have three peaks. This result implies that age of catastrophic impact making Vesta family may be not as young as Karin and Iannini families but as old as Eos and Koronis families.

  8. Bridging Theory to Practice with Classroom Rounds

    Science.gov (United States)

    Bowman, Connie L.; Herrelko, Janet M.

    2014-01-01

    Pre-service candidates' perceptions of how to teach were challenged after going through the process of Classroom Rounds, the process that was used in this study. Classroom Rounds consisted of a pre-conference meeting with an inservice teacher, followed by a classroom observation of that teacher, and finally a discussion focusing on proven…

  9. The Sloan Lens ACS Survey. VII. Elliptical Galaxy Scaling Laws from Direct Observational Mass Measurements

    CERN Document Server

    Bolton, Adam S; Koopmans, Leon V E; Gavazzi, Raphael; Moustakas, Leonidas A; Burles, Scott; Schlegel, David J; Wayth, Randall

    2008-01-01

    We use a sample of 53 massive early-type strong gravitational lens galaxies with well-measured redshifts (ranging from z=0.06 to 0.36) and stellar velocity dispersions (between 175 and 400 km/s) from the Sloan Lens ACS (SLACS) Survey to derive numerous empirical scaling relations. The ratio between central stellar velocity dispersion and isothermal lens-model velocity dispersion is nearly unity within errors. The SLACS lenses define a fundamental plane (FP) that is consistent with the FP of the general population of early-type galaxies. We measure the relationship between strong-lensing mass M_lens within one-half effective radius (R_e/2) and the dimensional mass variable M_dim = G^-1 sigma_e2^2 R_e/2 to be log_10 [M_lens/10^11 M_Sun] = (1.03 +/- 0.04) log_10 [M_dim/10^11 M_Sun] + (0.54 +/- 0.02) (where sigma_e2 is the projected stellar velocity dispersion within R_e/2). The near-unity slope indicates that the mass-dynamical structure of massive elliptical galaxies is independent of mass, and that the "tilt" ...

  10. Three years of Swift/BAT Survey of AGN: Reconciling Theory and Observations?

    Energy Technology Data Exchange (ETDEWEB)

    Burlon, D.; /Garching, Max Planck Inst., MPE; Ajello, M.; /SLAC /KIPAC, Menlo Park; Greiner, J.; /Garching, Max Planck Inst., MPE; Comastri, A.; /Muenchen, Tech. U. Universe; Merloni, A.; /Garching, Max Planck Inst., MPE /Muenchen, Tech. U. Universe; Gehrels, N.; /NASA, Goddard

    2011-02-07

    It is well accepted that unabsorbed as well as absorbed AGN are needed to explain the nature and the shape of the Cosmic X-ray background, even if the fraction of highly absorbed objects (dubbed Compton-thick sources) substantially still escapes detection. We derive and analyze the absorption distribution using a complete sample of AGN detected by Swift-BAT in the first three years of the survey. The fraction of Compton-thick AGN represents only 4.6% of the total AGN population detected by Swift-BAT. However, we show that once corrected for the bias against the detection of very absorbed sources the real intrinsic fraction of Compton-thick AGN is 20{sub -6}{sup +9}%. We proved for the first time (also in the BAT band) that the anti-correlation of the fraction of absorbed AGN and luminosity it tightly connected to the different behavior of the luminosity functions (XLFs) of absorbed and unabsorbed AGN. This points towards a difference between the two subsamples of objects with absorbed AGN being, on average, intrinsically less luminous than unobscured ones. Moreover the XLFs show that the fraction of obscured AGN might also decrease at very low luminosity. This can be successfully interpreted in the framework of a disk cloud outflow scenario as the disappearance of the obscuring region below a critical luminosity. Our results are discussed in the framework of population synthesis models and the origin of the Cosmic X-ray Background.

  11. Far-infrared data for symbiotic stars. II - The IRAS survey observations

    Science.gov (United States)

    Kenyon, S. J.; Fernandez-Castro, T.; Stencel, R. E.

    1988-06-01

    IRAS survey data for all known symbiotic binaries are reported. S type systems have 25 micron excesses much larger than those of single red giant stars, suggesting that these objects lose mass more rapidly than do normal giants. D type objects have far-IR colors similar to those of Mira variables, implying mass-loss rate of about 10 to the -6th solar masses/yr. The near-IR extinctions of the D types indicate that their Mira components are enshrouded in optically thick dust shells, while their hot companions lie outside the shells. If this interpretation of the data is correct, then the very red near-IR colors of D type symbiotic stars are caused by extreme amounts of dust absorption rather than dust emission. The small group of D prime objects possesses far-IR colors resembling those of compact planetary nebulae or extreme OH/IR stars. It is speculated that these binaries are not symbiotic stars at all, but contain a hot compact star and an exasymptotic branch giant which is in the process of ejecting a planetary nebula shell.

  12. The JCMT Gould Belt Survey: SCUBA-2 observations of circumstellar disks in L 1495

    CERN Document Server

    Buckle, J V; Greaves, J; Richer, J S; Matthews, B C; Johnstone, D; Kirk, H; Beaulieu, S F; Berry, D S; Broekhoven-Fiene, H; Currie, M J; Fich, M; Hatchell, J; Jenness, T; Mottram, J C; Nutter, D; Pattle, K; Pineda, J E; Salji, C; Tisi, S; Di Francesco, J; Hogerheijde, M R; Ward-Thompson, D; Bastien, P; Butner, H; Chen, M; Chrysostomou, A; Coude, S; Davis, C J; Duarte-Cabral, A; Friberg, P; Friesen, R; Fuller, G A; Graves, S; Gregson, J; Holland, W; Joncas, G; Kirk, J M; Knee, L B G; Mairs, S; Marsh, K; Moriarty-Schieven, G; Rawlings, J; Rosolowsky, E; Rumble, D; Sadavoy, S; Thomas, H; Tothill, N; Viti, S; White, G J; Wilson, C D; Wouterloot, J; Yates, J; Zhu, M

    2015-01-01

    We present 850$\\mu$m and 450$\\mu$m data from the JCMT Gould Belt Survey obtained with SCUBA-2 and characterise the dust attributes of Class I, Class II and Class III disk sources in L1495. We detect 23% of the sample at both wavelengths, with the detection rate decreasing through the Classes from I--III. The median disk mask is 1.6$\\times 10^{-3}$M$_{\\odot}$, and only 7% of Class II sources have disk masses larger than 20 Jupiter masses. We detect a higher proportion of disks towards sources with stellar hosts of spectral type K than spectral type M. Class II disks with single stellar hosts of spectral type K have higher masses than those of spectral type M, supporting the hypothesis that higher mass stars have more massive disks. Variations in disk masses calculated at the two wavelengths suggests there may be differences in dust opacity and/or dust temperature between disks with hosts of spectral types K to those with spectral type M.

  13. Subaru Telescope adaptive optics observations of gravitationally lensed quasars in the Sloan Digital Sky Survey

    Science.gov (United States)

    Rusu, Cristian E.; Oguri, Masamune; Minowa, Yosuke; Iye, Masanori; Inada, Naohisa; Oya, Shin; Kayo, Issha; Hayano, Yutaka; Hattori, Masayuki; Saito, Yoshihiko; Ito, Meguru; Pyo, Tae-Soo; Terada, Hiroshi; Takami, Hideki; Watanabe, Makoto

    2016-05-01

    We present the results of an imaging observation campaign conducted with the Subaru Telescope adaptive optics system (IRCS+AO188) on 28 gravitationally lensed quasars and candidates (23 doubles, 1 quad, 1 possible triple, and 3 candidates) from the SDSS Quasar Lens Search. We develop a novel modelling technique that fits analytical and hybrid point spread functions (PSFs), while simultaneously measuring the relative astrometry, photometry, as well as the lens galaxy morphology. We account for systematics by simulating the observed systems using separately observed PSF stars. The measured relative astrometry is comparable with that typically achieved with the Hubble Space Telescope, even after marginalizing over the PSF uncertainty. We model for the first time the quasar host galaxies in five systems, without a priori knowledge of the PSF, and show that their luminosities follow the known correlation with the mass of the supermassive black hole. For each system, we obtain mass models far more accurate than those previously published from low-resolution data, and we show that in our sample of lensing galaxies the observed light profile is more elliptical than the mass, for ellipticity ≳0.25. We also identify eight doubles for which the sources of external and internal shear are more reliably separated, and should therefore be prioritized in monitoring campaigns aimed at measuring time delays in order to infer the Hubble constant.

  14. The Lunar Occultation Observer (LOCO) - A Nuclear Astrophysics All-Sky Survey Mission Concept

    Science.gov (United States)

    Miller, R. S.; Bonamente, M.; Burgess, J. M.; Harmon, B. A.; Jenke, P.; Lawrence, D. J.; O'Brien, S.; Orr, M. R.; Paciesas, W. S.; Young, C. A.

    2008-07-01

    The Lunar Occultation Observer (LOCO) is a new lunar-based concept to probe the nuclear astrophysics regime. It will be a pioneering mission in high-energy astrophysics: the first to employ occultation as the principle detection and imaging method.

  15. Chandra Observations of the Highest Redshift Quasars from the Sloan Digital Sky Survey

    CERN Document Server

    Shemmer, O; Brandt, W N; Brinkmann, J; Diamond-Stanic, A M; Fan, X; Gunn, J E; Richards, G T; Schneider, D P; Strauss, M A; Anderson, Scott F.; Brinkmann, Jon; Diamond-Stanic, Aleksandar M.; Fan, Xiaohui; Gunn, James E.; Richards, Gordon T.; Schneider, Donald P.; Shemmer, Ohad; Strauss, Michael A.

    2006-01-01

    We present new Chandra observations of 21 z>4 quasars, including 11 sources at z>5. These observations double the number of X-ray detected quasars at z>5, allowing investigation of the X-ray spectral properties of a substantial sample of quasars at the dawn of the modern Universe. By jointly fitting the spectra of 15 z>5 radio-quiet quasars (RQQs), including sources from the Chandra archive, with a total of 185 photons, we find a mean X-ray power-law photon index of Gamma=1.95^{+0.30}_{-0.26}, and a mean neutral intrinsic absorption column density of N_H5 RQQs, excluding broad absorption line quasars, is alpha_ox=-1.69+/-0.03, which is consistent with the value predicted from the observed relationship between alpha_ox and ultraviolet luminosity. Four of the sources in our sample are members of the rare class of weak emission-line quasars, and we detect two of them in X-rays. We discuss the implications our X-ray observations have for the nature of these mysterious sources and, in particular, whether their wea...

  16. Observing Strategies for Focused Orbital Debris Surveys Using the Magellan Telescope

    Science.gov (United States)

    Frith, James; Seitzer, Patrick; Anz-Meador, Phillip; Cowardin, Heather; Lederer, Susan; Matney, Mark; Buckalew, Brent; Barker, Ed

    2017-01-01

    A breakup of the Titan 3C-17 Transtage rocket body was reported to have occurred on June 4th, 2014 at 02:38 UT by the Space Surveillance Network (SSN). Five objects were associated with this breakup and this is the fourth breakup known for this class of object. There are likely many more objects associated with this event that are not within the Space Surveillance Network's ability to detect and have not been catalogued. Several months after the breakup, observing time was obtained on the Magellan Baade 6.5 meter telescope to be used for observations of geosynchronous (GEO) space debris targets. Using the NASA Standard Satellite Breakup Model (SSBM), a simulated debris cloud of the recent Transtage breakup was produced and propagated forward in time. This provided right ascension, declination, and tracking rate predictions for where debris associated with this breakup may be more likely to be found in the sky over Magellan for our observing run. Magellan observations were then optimized using the angles and tracking rates from the model predictions to focus the search for Transtage debris. Data were collected and analysed and preliminary comparisons made between the number of objects detected and the number expected from the model. We present our results here.

  17. Observation

    Science.gov (United States)

    Patell, Hilla

    2016-01-01

    In order to achieve the goal of observation, preparation of the adult, the observer, is necessary. This preparation, says Hilla Patell, requires us to "have an appreciation of the significance of the child's spontaneous activities and a more thorough understanding of the child's needs." She discusses the growth of both the desire to…

  18. Observation

    Science.gov (United States)

    Kripalani, Lakshmi A.

    2016-01-01

    The adult who is inexperienced in the art of observation may, even with the best intentions, react to a child's behavior in a way that hinders instead of helping the child's development. Kripalani outlines the need for training and practice in observation in order to "understand the needs of the children and...to understand how to remove…

  19. Observers, Publications, and Surveys: Astronomy in the United States in 1849

    Science.gov (United States)

    Rothenberg, Marc

    1999-01-01

    By the mid-19th century, astronomy in the United States was productive and growing. Information gathered by and at the behest of the Smithsonian Institution shows that the community consisted of approximately 50 individuals, including a significant number of military officers, and a dozen observatories. Americans were deeply involved in astronomical research, and the discipline was entrenched in the college curriculum. What the discipline lacked was an adequate publication vehicle to ensure refereed, rapid dissemination of observations.

  20. GaLactic and Extragalactic All-Sky MWA-eXtended (GLEAM-X) survey: Pilot observations

    Science.gov (United States)

    Hurley-Walker, N.; Seymour, N.; Staveley-Smith, L.; Johnston-Hollitt, M.; Kapinska, A.; McKinley, B.

    2017-01-01

    This proposal is a pilot study for the extension of the highly successful GaLactic and Extragalactic MWA (GLEAM) survey (Wayth et al. 2015). The aim is to test out new observing strategies and data reduction techniques suitable for exploiting the longer baselines of the extended phase 2 MWA array. Deeper and wide surveys at higher resolution will enable a legion of science capabilities pertaining to galaxy evolution, clusters and the cosmic web, whilst maintaining the advantages over LOFAR including larger field-of-view, wider frequency coverage and better sensitivity to extended emission. We will continue the successful drift scan mode observing to test the feasibility of a large-area survey in 2017-B and onward. We will also target a single deep area with a bright calibrator source to establish the utility of focussed deep observations. In both cases, we will be exploring calibrating and imaging strategies across 72-231 MHz with the new long baselines. The published extragalactic sky catalogue (Hurley-Walker et al. 2017) improves the prospects for good ionospheric calibration in this new regime, as well as trivialising flux calibration. The new Alternative Data Release of the TIFR GMRT Sky Survey (TGSS-ADR1; Intema et al. 2016), which has 30" resolution and covers the proposed observing area, allows us to test whether our calibration and imaging strategy correctly recovers the true structure of (high surface-brightness) resolved sources. GLEAM-X will have lower noise, higher surface brightness sensitivity, and have considerably wider bandwidth than TGSS. These properties will enable a wide range of science, such as: Detecting and characterising cluster relics and haloes beyond z=0.45; Accurately determining radio source counts at multiple frequencies; Measuring the low-v luminosity function to z 0.5; Performing Galactic plane science such as HII region detection and cosmic tomography; Determining the typical ionospheric diffractive scale at the MRO, feeding into

  1. Tsunami damages assessment: vulnerability functions on buildings based on field and earth observation survey.

    Science.gov (United States)

    Gauraz, A. L.; Valencia, N.; Koscielny, M.; Guillande, R.; Gardi, A.; Leone, F.; Salaun, T.

    2009-04-01

    The assessment of damages caused by tsunami scenarios on coastal buildings requires using vulnerability matrixes or functions to carry out a relation between the magnitude of the phenomena and the damage expected. These functions represent the probability for a building belonging to a class of vulnerability to suffer from a mean damage level. The physical vulnerability of buildings depends on two parameters: the solicitation level applied by the tsunami on buildings and their resistance capacity. According to the authors after post-tsunami observations (Reese et al. 2007; Ruangrassamee et al. 2006; Leone et al. 2006; Peiris 2006), the level of damage is clearly linked to the water elevation of the inundated areas and the type of observed buildings. Very few works propose relations based on velocity or hydrodynamic pressure of the waves. An approach developed for the estimation of the building vulnerability consists in deriving empirical damage functions starting from field observations. As part of the SCHEMA European Project on the vulnerability assessment for tsunami hazards in the Atlantic and Mediterranean area, vulnerability functions have been elaborated for different classes of buildings in order to produce vulnerability maps for exposed areas with emphasis on extraction of building characteristics using remote sensing data. The damage detection has been carried out by field data collected after the 24 December 2006 tsunami event on the southwest area of Banda Aceh (Sumatra, Thailand) completed by photo-interpretation of satellite images to get representative functions with large population of samples. The building classes consist in several categories depending mainly on the type of construction material (timber/bamboo, traditional brick, reinforced concrete …), the type of structure (beam, pillars, etc) and the number of storeys. The level of damage has been also classified in five categories, from D0 (no damage) to D5 (total destruction). Vulnerability

  2. Observation of Microlensing towards the Galactic Spiral Arms EROS II 3 year survey

    CERN Document Server

    Derue, F; Albert, J N; Andersen, J; Ansari, R; Aubourg, E; Bareyre, P; Bauer2, F; Beaulieu, J P; Blanc, G; Bouquet, A; Char, S; Charlot, X; Couchot, F; Couture, C; Ferlet, R; Glicenstein, J F; Goldman, B; Gould, A; Gros, M; Hassinski, J; Hamilton, J C; Hardin, D; deKat, J; Kim, A; Lassere, T; Lesquoy, E; Loup, C; Magneville, C; Mansoux, B; Marquette, J B; Gra, D; Maurice, E; Milsztajn, A; Moniez, M; Palanque-Delabrouille, Nathalie; Perdereau, O; Prévôt, L; Regnault, N; Rich, J; Spiro, M; Vidal-madjar, A; Vigroux, L; Zylberajch, S

    2000-01-01

    We present an analysis of the light curves of 9.1 million stars observed during three seasons by EROS (Experience de Recherche d'Objets Sombres), in the Galactic plane away from the bulge. Seven stars exhibit luminosity variations compatible with gravitational microlensing effects due to unseen objects. The corresponding optical depth, averaged over four directions, is tau = 0.45 +0.24 -0.11 x 10^-6. While this value is compatible with expectations from simple galactic models under reasonable assumptions on the target distances, we find an excess of events with short timescale towards the direction closest to the Galactic Centre.

  3. On the Use of Cell Phones and Other Electronic Devices in the Classroom: Evidence from a Survey of Faculty and Students

    Science.gov (United States)

    Baker, William M.; Lusk, Edward J.; Neuhauser, Karyn L.

    2012-01-01

    The authors investigated faculty and student perceptions regarding the use of cell phones and other electronic devices in the classroom. Students differed markedly from faculty, with students exhibiting much greater acceptance of in-class use of technology. Among students, the authors found that gender affected perceptions. Specifically, male…

  4. What Are Teenagers Reading? The Findings of a Survey of Teenagers' Reading Choices and the Implications of These for English Teachers' Classroom Practice.

    Science.gov (United States)

    Manuel, Jacqueline; Robinson, Dennis

    2002-01-01

    Reports on the findings of a pilot study investigating the reading choices and habits of adolescents between the ages of 12 and 15 years. Sets out to understand more fully what, when, where, why and how adolescents between the ages of 12 and 15 years are reading, and the implications of this information for teachers and classroom reading pedagogy.…

  5. THE PANCHROMATIC STARBURST IRREGULAR DWARF SURVEY (STARBIRDS): OBSERVATIONS AND DATA ARCHIVE

    Energy Technology Data Exchange (ETDEWEB)

    McQuinn, Kristen B. W.; Mitchell, Noah P.; Skillman, Evan D., E-mail: kmcquinn@astro.umn.edu [Institute for Astrophysics, University of Minnesota, 116 Church Street, S.E., Minneapolis, MN 55455 (United States)

    2015-06-22

    Understanding star formation in resolved low mass systems requires the integration of information obtained from observations at different wavelengths. We have combined new and archival multi-wavelength observations on a set of 20 nearby starburst and post-starburst dwarf galaxies to create a data archive of calibrated, homogeneously reduced images. Named the panchromatic “STARBurst IRregular Dwarf Survey” archive, the data are publicly accessible through the Mikulski Archive for Space Telescopes. This first release of the archive includes images from the Galaxy Evolution Explorer Telescope (GALEX), the Hubble Space Telescope (HST), and the Spitzer Space Telescope (Spitzer) Multiband Imaging Photometer instrument. The data sets include flux calibrated, background subtracted images, that are registered to the same world coordinate system. Additionally, a set of images are available that are all cropped to match the HST field of view. The GALEX and Spitzer images are available with foreground and background contamination masked. Larger GALEX images extending to 4 times the optical extent of the galaxies are also available. Finally, HST images convolved with a 5″ point spread function and rebinned to the larger pixel scale of the GALEX and Spitzer 24 μm images are provided. Future additions are planned that will include data at other wavelengths such as Spitzer IRAC, ground-based Hα, Chandra X-ray, and Green Bank Telescope H i imaging.

  6. High-J CO survey of low-mass protostars observed with Herschel-HIFI

    DEFF Research Database (Denmark)

    Yıldız, U. A.; Kristensen, L. E.; van Dishoeck, E. F.

    2013-01-01

    derived from single-temperature fits to the Ju = 2-10 integrated intensities are ~70 K, 48 K and 37 K, respectively, with no significant difference between Class 0 and Class I sources and no trend with Menv or Lbol. Thus, in contrast to the continuum SEDs, the spectral line energy distributions (SLEDs) do...... probe has not yet been explored due to the lack of high-J CO observations. Aims: The aim is to constrain the physical characteristics (excitation, kinematics, column density) of the warm gas in low-mass protostellar envelopes using spectrally resolved Herschel data of CO and compare those...... with the colder gas traced by lower excitation lines. Methods: Herschel-HIFI observations of high-J lines of 12CO, 13CO, and C18O (up to Ju = 10, Eu up to 300 K) are presented toward 26 deeply embedded low-mass Class 0 and Class I young stellar objects, obtained as part of the Water In Star-forming regions...

  7. 体育课堂观察的内涵、价值与生成策略研究%P. E. Classroom Observation:Content,Value and Generation Strategy

    Institute of Scientific and Technical Information of China (English)

    赵富学; 王发斌

    2014-01-01

    体育课堂观察是开展体育教学研究和课堂教学效果诊断的一种新型体育教学评价活动,它是开展体育教学行动研究工作和体育教学质量评价工作的有效方法,其精细化的研究风格、清晰的操作流程深受学术界和大中小学体育教师的推崇。通过课堂观察可以提高体育教师教学判断的准确性,使体育教师针对性的选取教学策略,有效提升体育课堂教学质量。有利于体育教师反思课堂教学问题,实现知识共享。体育课堂观察是体育教师促进自身专业成长,凝聚团队智慧,实现教学创新的重要路径。完整的体育课堂观察通过确定合理的观察点、选择适当的记录方式、树立有效的观察目标导向和建立常态的观察机制,使体育教师重塑教学行为,为体育课堂的预设提供了可能,为体育教师教学智慧的生成指明了方向。%P. E. classroom observation is a new type of physical education teaching evaluation activity for P. E. re-search and classroom teaching effectiveness assessment,and an effective method for action research in P. E teaching and the evaluation of the quality of teaching. With a refined style of study and clear operational process,it has been widely welcomed by the academia and primary and secondary school physical education teachers. Classroom obser-vation can improve the accuracy of the teaching judgment of physical education teachers,help them apply teaching strategies tailored for their specific class,effectively improving the quality of classroom teaching. Classroom observa-tion enables the teachers to reflect on problems in classroom teaching and share what they know. It helps promote teacher�s professional development and rally team wisdom,thus conducive to teaching innovation. A complete P. E. classroom observation entails the selection of proper observation points,appropriate ways to record,effective observa-tion targets,and a normal

  8. SHORT GMC LIFETIMES: AN OBSERVATIONAL ESTIMATE WITH THE PdBI ARCSECOND WHIRLPOOL SURVEY (PAWS)

    Energy Technology Data Exchange (ETDEWEB)

    Meidt, Sharon E.; Hughes, Annie; Schinnerer, Eva; Colombo, Dario; Querejeta, Miguel [Max-Planck-Institut für Astronomie / Königstuhl 17 D-69117 Heidelberg (Germany); Dobbs, Clare L. [School of Physics and Astronomy, University of Exeter, Stocker Road, Exeter EX4 4QL (United Kingdom); Pety, Jérôme [Institut de Radioastronomie Millimétrique, 300 Rue de la Piscine, F-38406 Saint Martin d’Hères (France); Thompson, Todd A. [Department of Astronomy, The Ohio State University, 140 W. 18th Ave., Columbus, OH 43210 (United States); García-Burillo, Santiago [Observatorio Astronómico Nacional—OAN, Observatorio de Madrid Alfonso XII, 3, E-28014 Madrid (Spain); Leroy, Adam K. [National Radio Astronomy Observatory, 520 Edgemont Road, Charlottesville, VA 22903 (United States); Kramer, Carsten [Instituto Radioastronomía Milimétrica, Av. Divina Pastora 7, Nucleo Central, E-18012 Granada (Spain); Schuster, Karl F.; Dumas, Gaëlle [Observatoire de Paris, 61 Avenue de l’Observatoire, F-75014 Paris (France)

    2015-06-10

    We describe and execute a novel approach to observationally estimate the lifetimes of giant molecular clouds (GMCs). We focus on the cloud population between the two main spiral arms in M51 (the inter-arm region) where cloud destruction via shear and star formation feedback dominates over formation processes. By monitoring the change in GMC number densities and properties across the inter-arm, we estimate the lifetime as a fraction of the inter-arm travel time. We find that GMC lifetimes in M51's inter-arm are finite and short, 20–30 Myr. Over most of the region under investigation shear appears to regulate the lifetime. As the shear timescale increases with galactocentric radius, we expect cloud destruction to switch primarily to feedback at larger radii. We identify a transition from shear- to feedback-dominated disruption, finding that shear is more efficient at dispersing clouds, whereas feedback transforms the population, e.g., by fragmenting high-mass clouds into lower mass pieces. Compared to the characteristic timescale for molecular hydrogen in M51, our short lifetimes suggest that gas can remain molecular while clouds disperse and reassemble. We propose that galaxy dynamics regulates the cycling of molecular material from diffuse to bound (and ultimately star-forming) objects, contributing to long observed molecular depletion times in normal disk galaxies. We also speculate that, in extreme environments like elliptical galaxies and concentrated galaxy centers, star formation can be suppressed when the shear timescale is short enough that some clouds will not survive to form stars.

  9. The Spitzer c2d Survey of Large, Nearby, Interstellar Clouds. III. Perseus Observed with IRAC

    CERN Document Server

    Jørgensen, J K; Evans, N J; Huard, T L; Allen, L E; Porras, A; Blake, G A; Bourke, T L; Chapman, N; Cieza, L; Körner, D W; Lai, S P; Mundy, L G; Myers, P C; Padgett, D L; Rebull, L M; Sargent, A I; Spiesman, W; Stapelfeldt, K R; Van Dishoeck, E F; Wahhaj, Z; Young, K E; Jorgensen, Jes K.; Harvey, Paul M.; II, Neal J. Evans; Huard, Tracy L.; Allen, Lori E.; Porras, Alicia; Blake, Geoffrey A.; Bourke, Tyler L.; Chapman, Nicholas; Cieza, Lucas; Koerner, David W.; Lai, Shih-Ping; Mundy, Lee G.; Myers, Philip C.; Padgett, Deborah L.; Rebull, Luisa; Sargent, Anneila I.; Spiesman, William; Stapelfeldt, Karl R.; Dishoeck, Ewine F. van; Wahhaj, Zahed; Young, Kaisa E.

    2006-01-01

    We present observations of 3.86 sq. deg. of the Perseus molecular cloud complex with the Spitzer Space Telescope Infrared Array Camera (IRAC). The maps show strong extended emission arising from shocked H2 in outflows in the region and from polycyclic aromatic hydrocarbon features. More than 120,000 sources are extracted toward the cloud. Based on their IRAC colors and comparison to off-cloud and extragalactic fields, we identify 400 candidate young stellar objects. About two thirds of these are associated with the young clusters IC348 and NGC1333, while the last third is distributed over the remaining cloud. We classify the young stellar objects according to the traditional scheme based on the slope of their spectral energy distributions. Significant differences are found for the numbers of embedded Class I objects relative to more evolved Class II objects in IC348, NGC1333 and the remaining cloud with the embedded Class I and "flat spectrum" YSOs constituting 14%, 36% and 47% of the total number of YSOs ide...

  10. The Spitzer c2d Survey of Large, Nearby, Interstellar Clouds: VI. Perseus Observed with MIPS

    CERN Document Server

    Rebull, L M; II, N J E; Jørgensen, J K; Harvey, P M; Brooke, T Y; Bourke, T L; Padgett, D L; Chapman, N L; Lai, S P; Spiesmann, W J; Noreiga-Crespo, A; Merin, B; Huard, T; Allen, L E; Blake, G A; Jarrett, T; Körner, D W; Mundy, L G; Myers, P C; Sargent, A I; Van Dishoeck, E F; Wahhaj, Z; Young, K E

    2007-01-01

    We present observations of 10.6 square degrees of the Perseus molecular cloud at 24, 70, and 160 microns with the Spitzer Space Telescope Multiband Imaging Photometer for Spitzer (MIPS). The image mosaics show prominent, complex extended emission dominated by illuminating B stars on the East side of the cloud, and by cold filaments of 160 micron emission on the West side. Of 3950 point sources identified at 24 microns, 1141 have 2MASS counterparts. A quarter of these populate regions of the Ks vs. Ks-[24] diagram that are distinct from stellar photospheres and background galaxies, and thus are likely to be cloud members with infrared excess. Nearly half (46%) of these 24 micron excess sources are distributed outside the IC 348 and NGC 1333 clusters. NGC 1333 shows the highest fraction of stars with flat or rising spectral energy distributions (28%), while Class II SEDs are most common in IC 348. These results are consistent with previous relative age determinations for the two clusters. The intercluster regio...

  11. Candidemia in the Neonatal Intensive Care Unit: A Retrospective, Observational Survey and Analysis of Literature Data.

    Science.gov (United States)

    Caggiano, Giuseppina; Lovero, Grazia; De Giglio, Osvalda; Barbuti, Giovanna; Montagna, Osvaldo; Laforgia, Nicola; Montagna, Maria Teresa

    2017-01-01

    We evaluated the epidemiology of Candida bloodstream infections in the neonatal intensive care unit (NICU) of an Italian university hospital during a 9-year period as a means of quantifying the burden of infection and identifying emerging trends. Clinical data were searched for in the microbiological laboratory database. For comparative purposes, we performed a review of NICU candidemia. Forty-one candidemia cases were reviewed (overall incidence, 3.0 per 100 admissions). Candida parapsilosis sensu stricto (58.5%) and C. albicans (34.1%) were the most common species recovered. A variable drift through years was observed; in 2015, 75% of the cases were caused by non-albicans species. The duration of NICU hospitalization of patients with non-albicans was significantly longer than in those with C. albicans (median days, 10 versus 12). Patients with non-albicans species were more likely to have parenteral nutrition than those with C. albicans (96.3% versus 71.4%). Candida albicans was the dominant species in Europe and America (median, 55% and 60%; resp.); non-albicans species predominate in Asia (75%). Significant geographic variation is evident among cases of candidemia in different parts of the world, recognizing the importance of epidemiological data to facilitate the treatment.

  12. Candidemia in the Neonatal Intensive Care Unit: A Retrospective, Observational Survey and Analysis of Literature Data

    Directory of Open Access Journals (Sweden)

    Giuseppina Caggiano

    2017-01-01

    Full Text Available We evaluated the epidemiology of Candida bloodstream infections in the neonatal intensive care unit (NICU of an Italian university hospital during a 9-year period as a means of quantifying the burden of infection and identifying emerging trends. Clinical data were searched for in the microbiological laboratory database. For comparative purposes, we performed a review of NICU candidemia. Forty-one candidemia cases were reviewed (overall incidence, 3.0 per 100 admissions. Candida parapsilosis sensu stricto (58.5% and C. albicans (34.1% were the most common species recovered. A variable drift through years was observed; in 2015, 75% of the cases were caused by non-albicans species. The duration of NICU hospitalization of patients with non-albicans was significantly longer than in those with C. albicans (median days, 10 versus 12. Patients with non-albicans species were more likely to have parenteral nutrition than those with C. albicans (96.3% versus 71.4%. Candida albicans was the dominant species in Europe and America (median, 55% and 60%; resp.; non-albicans species predominate in Asia (75%. Significant geographic variation is evident among cases of candidemia in different parts of the world, recognizing the importance of epidemiological data to facilitate the treatment.

  13. Short GMC lifetimes: an observational estimate with the PdBI Arcsecond Whirlpool Survey (PAWS)

    CERN Document Server

    Meidt, Sharon E; Dobbs, Clare L; Pety, Jerome; Thompson, Todd A; Garcia-Burillo, Santiago; Leroy, Adam K; Schinnerer, Eva; Colombo, Dario; Querejeta, Miguel; Kramer, Carsten; Schuster, Karl F; Dumas, Gaelle

    2015-01-01

    We describe and execute a novel approach to observationally estimate the lifetimes of giant molecular clouds (GMCs). We focus on the cloud population between the two main spiral arms in M51 (the inter-arm region) where cloud destruction via shear and star formation feedback dominates over formation processes. By monitoring the change in GMC number densities and properties from one side of the inter-arm to the other, we estimate the lifetime as a fraction of the inter-arm travel time. We find that GMC lifetimes in M51's inter-arm are finite and short, 20 to 30 Myr. Such short lifetimes suggest that cloud evolution is influenced by environment, in which processes can disrupt GMCs after a few free-fall times. Over most of the region under investigation shear appears to regulate the lifetime. As the shear timescale increases with galactocentric radius, we expect cloud destruction to switch primarily to star formation feedback at larger radii. We identify a transition from shear- to feedback-dominated disruption t...

  14. Exploring Anticorrelations and Light Element Variations in Northern Globular Clusters Observed by the APOGEE Survey

    CERN Document Server

    Meszaros, Szabolcs; Shetrone, Matthew; Lucatello, Sara; Troup, Nicholas W; Bovy, Jo; Cunha, Katia; Garcia-Hernandez, Domingo A; Overbeek, Jamie C; Prieto, Carlos Allende; Beers, Timothy C; Frinchaboy, Peter M; Perez, Ana E Garcia; Hearty, Fred R; Holtzman, Jon; Majewski, Steven R; Nidever, David L; Schiavon, Ricardo P; Schneider, Donald P; Sobeck, Jennifer S; Smith, Verne V; Zamora, Olga; Zasowski, Gail

    2015-01-01

    We investigate the light-element behavior of red giant stars in Northern globular clusters (GCs) observed by the SDSS-III Apache Point Observatory Galactic Evolution Experiment (APOGEE). We derive abundances of nine elements (Fe, C, N, O, Mg, Al, Si, Ca, and Ti) for 428 red giant stars in 10 globular clusters. The intrinsic abundance range relative to measurement errors is examined, and the well-known C-N and Mg-Al anticorrelations are explored using an extreme-deconvolution code for the first time in a consistent way. We find that Mg and Al drive the population membership in most clusters, except in M107 and M71, the two most metal-rich clusters in our study, where the grouping is most sensitive to N. We also find a diversity in the abundance distributions, with some clusters exhibiting clear abundance bimodalities (for example M3 and M53) while others show extended distributions. The spread of Al abundances increases significantly as cluster average metallicity decreases as previously found by other works, ...

  15. The Effects of Classroom Management on the Behaviors of Students with Disabilities in Inclusive Classrooms in Turkey

    Science.gov (United States)

    Sucuoglu, Bulbin; Akalin, Selma; Sazak-Pinar, Elif

    2010-01-01

    The purpose of this study was to determine whether the behaviors of the students with disabilities placed in general education classrooms differed according to the classroom management level of the teachers. The classroom management strategies of the 44 teachers were assessed by using The Proactive Classroom Management Observation Form. The…

  16. 英语教学中基于课堂观察的非测试性评价述评%Review on non-test assessment based on classroom observation in English teaching

    Institute of Scientific and Technical Information of China (English)

    何梦川子

    2014-01-01

    目前的教学评价多以学生考试成绩为依据的终结性评价为主,科学的教学评价不仅应该包括以标准化考试为代表的终结性评价,还应该包括注重学习过程的非测试性评价。不同于传统的终结性评价以测试为单一的评价工具,非测试性评价的工具种类繁多,包括课堂观察、档案袋、日记等。文章将重点讨论第一种评价手段,即课堂观察。通过有效的课堂观察,教师对学生反馈信息做出正确的诊断和及时的评价,从而进行课堂的有效教学。%Present teaching assessment is mainly summative assessment which is based on students’test scores. However, scientific teaching assessment should includes both summative evaluation represented by standard tests and non-test evaluation concerning the learning process. Different from traditional summative evaluation whose exclusive tool is test,non-test assess-ment has various of tools to apply in the teaching,including classroom observation,portfolio,diary,etc. This paper will be go-ing to discuss the first tool,that is classroom observation. Through effective classroom observation,teachers can make appro-priate judgment and timely assessment of students’feedback and carry out effective classroom teaching.

  17. Physical, chemical, net haul, bird surveys, and other observations (BIOMASS data) from the British Antarctic Survey FIBEX and SIBEX Projects from 01 November 1980 to 30 April 1985 (NODC Accession 9400053)

    Data.gov (United States)

    National Oceanic and Atmospheric Administration, Department of Commerce — This accession includes observations of physical, chemical, and biomass properties from three field experiments conducted by the British Antarctic Survey: the First...

  18. CLASSROOM MANAGEMENT

    Directory of Open Access Journals (Sweden)

    Jasmina Delceva – Dizdarevik

    2014-06-01

    Full Text Available This paper is aiming to discover the paths that enable teachers to manage their work with students in the classroom. To be an efficient teacher means to know with what and how to motivate students to learn. Teacher as an efficient classroom manager needs to have skills to plan and prepare the education process, know how to organize the teaching and how to guide the class. An efficient teacher moreover needs o establish positive classroom climate and working discipline. Also, teacher should be able to evaluate the progress of the students and self-evaluate his own work.In order to examine classroom management skills of teachers in Republic of Macedonia, a research has been made for teachers in primary schools in Republic of Macedonia. Instruments which will be used in order to complete the research and analyses are the following: questionnaire for teachers and educational policy analyses in our country in order to discover whether there is concrete strategy for promotion and implementation of classroom management on local and national level.Analyses of results show that there is a deficit of classroom management skills among teachers, which is due moreover to some lapses in initial education of teachers.

  19. Toward Better Classroom Teaching.

    Science.gov (United States)

    Grew, James H.

    1964-01-01

    Designed for the inexperienced language teacher, this summary of effective language teaching techniques is based on observations made in high school French classes, but is applicable also to elementary school and beginning college language programs. Consideration is given to maintaining interest and classroom control, using realia, and giving each…

  20. EXPLORING ANTICORRELATIONS AND LIGHT ELEMENT VARIATIONS IN NORTHERN GLOBULAR CLUSTERS OBSERVED BY THE APOGEE SURVEY

    Energy Technology Data Exchange (ETDEWEB)

    Mészáros, Szabolcs [ELTE Gothard Astrophysical Observatory, H-9704 Szombathely, Szent Imre Herceg st. 112 (Hungary); Martell, Sarah L. [Department of Astrophysics, School of Physics, University of New South Wales, Sydney, NSW 2052 (Australia); Shetrone, Matthew [University of Texas at Austin, McDonald Observatory, Fort Davis, TX 79734 (United States); Lucatello, Sara [INAF-Osservatorio Astronomico di Padova, vicolo dell Osservatorio 5, I-35122 Padova (Italy); Troup, Nicholas W.; Pérez, Ana E. García; Majewski, Steven R. [Department of Astronomy, University of Virginia, Charlottesville, VA 22904-4325 (United States); Bovy, Jo [Institute for Advanced Study, Einstein Drive, Princeton, NJ 08540 (United States); Cunha, Katia [University of Arizona, Tucson, AZ 85719 (United States); García-Hernández, Domingo A.; Prieto, Carlos Allende [Instituto de Astrofísica de Canarias (IAC), E-38200 La Laguna, Tenerife (Spain); Overbeek, Jamie C. [Department of Astronomy, Indiana University, Bloomington, IN 47405 (United States); Beers, Timothy C. [Department of Physics and JINA Center for the Evolution of the Elements, University of Notre Dame, Notre Dame, IN 46556 (United States); Frinchaboy, Peter M. [Texas Christian University, Fort Worth, TX 76129 (United States); Hearty, Fred R.; Schneider, Donald P. [Department of Astronomy and Astrophysics, The Pennsylvania State University, University Park, PA 16802 (United States); Holtzman, Jon [New Mexico State University, Las Cruces, NM 88003 (United States); Nidever, David L. [Department of Astronomy, University of Michigan, Ann Arbor, MI 48109 (United States); Schiavon, Ricardo P. [Astrophysics Research Institute, IC2, Liverpool Science Park, Liverpool John Moores University, 146 Brownlow Hill, Liverpool, L3 5RF (United Kingdom); and others

    2015-05-15

    We investigate the light-element behavior of red giant stars in northern globular clusters (GCs) observed by the SDSS-III Apache Point Observatory Galactic Evolution Experiment. We derive abundances of 9 elements (Fe, C, N, O, Mg, Al, Si, Ca, and Ti) for 428 red giant stars in 10 GCs. The intrinsic abundance range relative to measurement errors is examined, and the well-known C–N and Mg–Al anticorrelations are explored using an extreme-deconvolution code for the first time in a consistent way. We find that Mg and Al drive the population membership in most clusters, except in M107 and M71, the two most metal-rich clusters in our study, where the grouping is most sensitive to N. We also find a diversity in the abundance distributions, with some clusters exhibiting clear abundance bimodalities (for example M3 and M53) while others show extended distributions. The spread of Al abundances increases significantly as cluster average metallicity decreases as previously found by other works, which we take as evidence that low metallicity, intermediate mass AGB polluters were more common in the more metal-poor clusters. The statistically significant correlation of [Al/Fe] with [Si/Fe] in M15 suggests that {sup 28}Si leakage has occurred in this cluster. We also present C, N, and O abundances for stars cooler than 4500 K and examine the behavior of A(C+N+O) in each cluster as a function of temperature and [Al/Fe]. The scatter of A(C+N+O) is close to its estimated uncertainty in all clusters and independent of stellar temperature. A(C+N+O) exhibits small correlations and anticorrelations with [Al/Fe] in M3 and M13, but we cannot be certain about these relations given the size of our abundance uncertainties. Star-to-star variations of α-element (Si, Ca, Ti) abundances are comparable to our estimated errors in all clusters.

  1. Wide-bandwidth drift-scan pulsar surveys of globular clusters: application to early science observations with FAST

    Science.gov (United States)

    Zhang, Lei; Hobbs, George; Li, Di; Lorimer, Duncan; Zhang, Jie; Yu, Meng; Yue, You-Ling; Wang, Pei; Pan, Zhi-Chen; Dai, Shi

    2016-10-01

    The Five-hundred-meter Aperture Spherical Telescope (FAST) will begin its early-science operations during 2016. Drift-scan pulsar surveys will be carried out during this period using an ultra-wide-band receiver system (covering ∼ 270 to 1620 MHz). We describe a method for accounting for the changes in the telescope beam shape and the pulsar parameters when searching for pulsars over such a wide bandwidth. We applied this method to simulated data sets of pulsars in globular clusters that are visible to FAST and found that a representative observation would have a sensitivity of ∼ 40 μJy. Our results showed that a single drift-scan (lasting less than a minute) is likely to find at least one pulsar for observations of four globular clusters. Repeated observations will increase the likely number of detections. We found that pulsars in ∼16 clusters are likely to be found if the data from 100 drift-scan observations of each cluster are incoherently combined.

  2. Wide-bandwidth drift-scan pulsar surveys of globular clusters: application to early science observations with FAST

    Science.gov (United States)

    Zhang, Lei; Hobbs, George; Li, Di; Lorimer, Duncan; Zhang, Jie; Yu, Meng; Yue, You-Ling; Wang, Pei; Pan, Zhi-Chen; Dai, Shi

    2016-10-01

    The Five-hundred-meter Aperture Spherical Telescope (FAST) will begin its early-science operations during 2016. Drift-scan pulsar surveys will be carried out during this period using an ultra-wide-band receiver system (covering ˜ 270 to 1620 MHz). We describe a method for accounting for the changes in the telescope beam shape and the pulsar parameters when searching for pulsars over such a wide bandwidth. We applied this method to simulated data sets of pulsars in globular clusters that are visible to FAST and found that a representative observation would have a sensitivity of ˜ 40 μJy. Our results showed that a single drift-scan (lasting less than a minute) is likely to find at least one pulsar for observations of four globular clusters. Repeated observations will increase the likely number of detections. We found that pulsars in ˜16 clusters are likely to be found if the data from 100 drift-scan observations of each cluster are incoherently combined.

  3. Serendipity observations of far infrared cirrus emission in the Spitzer Infrared Nearby Galaxies Survey: Analysis of far-infrared correlations

    CERN Document Server

    Bot, Caroline; Boulanger, Francois; Lagache, Guilaine; Miville-Deschenes, Marc-Antoine; Draine, Bruce; Martin, Peter

    2009-01-01

    We present an analysis of far-infrared dust emission from diffuse cirrus clouds. This study is based on serendipitous observations at 160 microns at high galactic latitude with the Multiband Imaging Photometer (MIPS) onboard the Spitzer Space Telescope by the Spitzer Infrared Nearby Galaxies Survey (SINGS). These observations are complemented with IRIS data at 100 and 60 microns and constitute one of the most sensitive and unbiased samples of far infrared observations at small scale of diffuse interstellar clouds. Outside regions dominated by the cosmic infrared background fluctuations, we observe a substantial scatter in the 160/100 colors from cirrus emission. We compared the 160/100 color variations to 60/100 colors in the same fields and find a trend of decreasing 60/100 with increasing 160/100. This trend can not be accounted for by current dust models by changing solely the interstellar radiation field. It requires a significant change of dust properties such as grain size distribution or emissivity or ...

  4. Observation and Confirmation of Six Strong-lensing Systems in the Dark Energy Survey Science Verification Data

    Science.gov (United States)

    Nord, B.; Buckley-Geer, E.; Lin, H.; Diehl, H. T.; Helsby, J.; Kuropatkin, N.; Amara, A.; Collett, T.; Allam, S.; Caminha, G. B.; De Bom, C.; Desai, S.; Dúmet-Montoya, H.; Pereira, M. Elidaiana da S.; Finley, D. A.; Flaugher, B.; Furlanetto, C.; Gaitsch, H.; Gill, M.; Merritt, K. W.; More, A.; Tucker, D.; Saro, A.; Rykoff, E. S.; Rozo, E.; Birrer, S.; Abdalla, F. B.; Agnello, A.; Auger, M.; Brunner, R. J.; Carrasco Kind, M.; Castander, F. J.; Cunha, C. E.; da Costa, L. N.; Foley, R. J.; Gerdes, D. W.; Glazebrook, K.; Gschwend, J.; Hartley, W.; Kessler, R.; Lagattuta, D.; Lewis, G.; Maia, M. A. G.; Makler, M.; Menanteau, F.; Niernberg, A.; Scolnic, D.; Vieira, J. D.; Gramillano, R.; Abbott, T. M. C.; Banerji, M.; Benoit-Lévy, A.; Brooks, D.; Burke, D. L.; Capozzi, D.; Carnero Rosell, A.; Carretero, J.; D'Andrea, C. B.; Dietrich, J. P.; Doel, P.; Evrard, A. E.; Frieman, J.; Gaztanaga, E.; Gruen, D.; Honscheid, K.; James, D. J.; Kuehn, K.; Li, T. S.; Lima, M.; Marshall, J. L.; Martini, P.; Melchior, P.; Miquel, R.; Neilsen, E.; Nichol, R. C.; Ogando, R.; Plazas, A. A.; Romer, A. K.; Sako, M.; Sanchez, E.; Scarpine, V.; Schubnell, M.; Sevilla-Noarbe, I.; Smith, R. C.; Soares-Santos, M.; Sobreira, F.; Suchyta, E.; Swanson, M. E. C.; Tarle, G.; Thaler, J.; Walker, A. R.; Wester, W.; Zhang, Y.; DES Collaboration

    2016-08-01

    We report the observation and confirmation of the first group- and cluster-scale strong gravitational lensing systems found in Dark Energy Survey data. Through visual inspection of data from the Science Verification season, we identified 53 candidate systems. We then obtained spectroscopic follow-up of 21 candidates using the Gemini Multi-object Spectrograph at the Gemini South telescope and the Inamori-Magellan Areal Camera and Spectrograph at the Magellan/Baade telescope. With this follow-up, we confirmed six candidates as gravitational lenses: three of the systems are newly discovered, and the remaining three were previously known. Of the 21 observed candidates, the remaining 15 either were not detected in spectroscopic observations, were observed and did not exhibit continuum emission (or spectral features), or were ruled out as lensing systems. The confirmed sample consists of one group-scale and five galaxy-cluster-scale lenses. The lensed sources range in redshift z ˜ 0.80-3.2 and in i-band surface brightness i SB ˜ 23-25 mag arcsec-2 (2″ aperture). For each of the six systems, we estimate the Einstein radius θ E and the enclosed mass M enc, which have ranges θ E ˜ 5″-9″ and M enc ˜ 8 × 1012 to 6 × 1013 M ⊙, respectively. This paper includes data gathered with the 6.5 m Magellan Telescopes located at Las Campanas Observatory, Chile.

  5. The LAMOST Survey of Background Quasars in the Vicinity of the Andromeda and Triangulum Galaxies -- II. Results from the Commissioning Observations and the Pilot Surveys

    CERN Document Server

    Huo, Zhi-Ying; Xiang, Mao-Sheng; Yuan, Hai-Bo; Huang, Yang; Zhang, Hui-Hua; Yan, Lin; Bai, Zhong-Rui; Chen, Jian-Jun; Chen, Xiao-Yan; Chu, Jia-Ru; Chu, Yao-Quan; Cui, Xiang-Qun; Du, Bing; Hou, Yong-Hui; Hu, Hong-Zhuan; Hu, Zhong-Wen; Jia, Lei; Jiang, Fang-Hua; Lei, Ya-Juan; Li, Ai-Hua; Li, Guang-Wei; Li, Guo-Ping; Li, Jian; Li, Xin-Nan; Li, Yan; Li, Ye-Ping; Liu, Gen-Rong; Liu, Zhi-Gang; Lu, Qi-Shuai; Luo, A-Li; Luo, Yu; Men, Li; Ni, Ji-Jun; Qi, Yong-Jun; Qi, Zhao-Xiang; Shi, Jian-Rong; Shi, Huo-Ming; Sun, Shi-Wei; Tang, Zheng-Hong; Tian, Yuan; Tu, Liang-Ping; Wang, Dan; Wang, Feng-Fei; Wang, Gang; Wang, Jia-Ning; Wang, Lei; Wang, Shu-Qing; Wang, You; Wang, Yue-Fei; Wei, Ming-Zhi; Wu, Yue; Xue, Xiang-Xiang; Yao, Zheng-Qiu; Yu, Yong; Yuan, Hui; Zhai, Chao; Zhang, En-Peng; Zhang, Hao-Tong; Zhang, Jian-Nan; Zhang, Wei; Zhang, Yan-Xia; Zhang, Yong; Zhang, Zhen-Chao; Zhao, Gang; Zhao, Ming; Zhao, Yong-Heng; Zhou, Fang; Zhou, Xin-Lin; Zhu, Yong-Tian; Zou, Si-Cheng

    2013-01-01

    We present new quasars discovered in the vicinity of the Andromeda and Triangulum galaxies with the LAMOST during the 2010 and 2011 observational seasons. Quasar candidates are selected based on the available SDSS, KPNO 4 m telescope, XSTPS optical, and WISE near infrared photometric data. We present 509 new quasars discovered in a stripe of ~135 sq. deg from M31 to M33 along the Giant Stellar Stream in the 2011 pilot survey datasets, and also 17 new quasars discovered in an area of ~100 sq. deg that covers the central region and the southeastern halo of M31 in the 2010 commissioning datasets. These 526 new quasars have i magnitudes ranging from 15.5 to 20.0, redshifts from 0.1 to 3.2. They represent a significant increase of the number of identified quasars in the vicinity of M31 and M33. There are now 26, 62 and 139 known quasars in this region of the sky with i magnitudes brighter than 17.0, 17.5 and 18.0 respectively, of which 5, 20 and 75 are newly-discovered. These bright quasars provide an invaluable c...

  6. Observational Constraints on the Nature of the Dark Energy: First Cosmological Results From the ESSENCE Supernova Survey

    Energy Technology Data Exchange (ETDEWEB)

    Wood-Vasey, W.Michael; Miknaitis, G.; Stubbs, C.W.; Jha, S.; Riess, A.G.; Garnavich, P.M.; Kirshner, R.P.; Aguilera, C.; Becker, A.C.; Blackman, J.W.; Blondin, S.; Challis, P.; Clocchiatti, A.; Conley, A.; Covarrubias, R.; Davis, T.M.; Filippenko, A.V.; Foley, R.J.; Garg, A.; Hicken, M.; Krisciunas, K.; /Harvard-Smithsonian Ctr. Astrophys.

    2007-01-05

    We present constraints on the dark energy equation-of-state parameter, w = P/({rho}c{sup 2}), using 60 Type Ia supernovae (SNe Ia) from the ESSENCE supernova survey. We derive a set of constraints on the nature of the dark energy assuming a flat Universe. By including constraints on ({Omega}{sub M}, w) from baryon acoustic oscillations, we obtain a value for a static equation-of-state parameter w = -1.05{sub -0.12}{sup +0.13} (stat 1{sigma}) {+-} 0.13 (sys) and {Omega}{sub M} = 0.274{sub -0.020}{sup +0.033} (stat 1{sigma}) with a best-fit {chi}{sup 2}/DoF of 0.96. These results are consistent with those reported by the Super-Nova Legacy Survey in a similar program measuring supernova distances and redshifts. We evaluate sources of systematic error that afflict supernova observations and present Monte Carlo simulations that explore these effects. Currently, the largest systematic currently with the potential to affect our measurements is the treatment of extinction due to dust in the supernova host galaxies. Combining our set of ESSENCE SNe Ia with the SuperNova Legacy Survey SNe Ia, we obtain a joint constraint of w = -1.07{sub -0.09}{sup +0.09} (stat 1{sigma}) {+-} 0.13 (sys), {Omega}{sub M} = 0.267{sub -0.018}{sup +0.028} (stat 1{sigma}) with a best-fit {chi}{sup 2}/DoF of 0.91. The current SNe Ia data are fully consistent with a cosmological constant.

  7. Surveying the experiences and perceptions of undergraduate nursing students of a flipped classroom approach to increase understanding of drug science and its application to clinical practice.

    Science.gov (United States)

    Hanson, Julie

    2016-01-01

    Patient harm from medication error is a significant issue. Individual failures by health professionals including knowledge deficits and poor communication have been identified as increasing the likelihood of medication administration errors. In Australia, the National Strategy for Quality Use of Medicines in 2002 compels health professionals to have the knowledge and skills to use medicines safely and effectively. This paper examines nursing students' perceptions of the effectiveness of a flipped classroom approach to increase understanding of pharmacology principles and the application of this knowledge to medication practice. An internet-based self-completion questionnaire was used in 2013 (n = 26) after the flipped classroom approach was implemented, and pre- (n = 6) and post-flipping (n = 25) in 2014. Students who engaged with digitally recorded lectures (eLectures) prior to face-to-face workshops stated that they had greater understanding of the subject and enhanced critical thinking skills. The replay function of the eLecture was perceived by some students as most beneficial to independent learning. However, for some students, time constraints meant that they relied on eLectures alone, while others preferred traditional teaching methods. Although limited by sample size and potential participant bias, the results provide insights about the flipped classroom experience from a student perspective.

  8. The - - and Submm-Wave Spectrum of Allyl Isocyanide and Radioastronomical Observations in Orion KL and the Primos Line Survey

    Science.gov (United States)

    Haykal, I.; Motiyenko, R. A.; Margules, L.; Huet, T. R.; Ecija, P.; Cocinero, E. J.; Basterretxea, F.; Fernandez, J. A.; Castano, F.; Tercero, B.; Cernicharo, J.; Lesarri, A.; Guillemin, J. C.

    2013-06-01

    Last year we presented the first rotational analysis of the ground state of the two conformers of allyl isocyanide from 4 GHz to 905 GHz. The analysis of the rotational spectrum of the cis conformer of allyl isocyanide was extended. We resolved Coriolis interactions of a and b types between the excited vibrational states ν_1=1 and ν_2=1, calculated to be at 156 cm^{-1} (A^{'}) and 167 cm^{-1} (A^{''}) respectively (MP2/aug-cc-pvtz), from 150 GHz to 600 GHz. Strong perturbations were observed in the 150-310 GHz range for low values of the quantum number K_a starting from K_a = 0, 1. The anharmonicities appeared as well at higher frequencies for larger quantum numbers. The two modes were fitted together with the SPFIT/SPCAT suite of programs and a set of Coriolis parameters was accurately determined. The fit contains more than 3000 lines up to J = 99 and K_a = 12 for both modes. We did not detect these species neither in the IRAM 30-m line survey of Orion KL nor in the PRIMOS survey towards SgrB2. Nevertheless, we provided upper limits to their column density in Orion KL. This work was supported by the CNES and the Action sur Projets de l'INSU, PCMI. I. Haykal et al. manuscript in preparation H. Pickett J. Mol. Spec.{148}, 371-377, 1991.

  9. The OmegaWhite survey for Short-Period Variable Stars III: Follow-up Photometric and Spectroscopic Observations

    CERN Document Server

    Macfarlane, S A; Groot, P J; Ramsay, G; Toma, R; Motsoaledi, M; Crause, L A; Gilbank, D G; O'Donoghue, D; Potter, S B; Sickafoose, A A; van Gend, C; Worters, H L

    2016-01-01

    We present photometric and spectroscopic follow-up observations of short-period variables discovered in the OmegaWhite survey: a wide-field high-cadence g-band synoptic survey targeting the Galactic Plane. We have used fast photometry on the SAAO 1.0-m and 1.9-m telescopes to obtain light curves of 27 variables, and use these results to validate the period and amplitude estimates from the OmegaWhite processing pipeline. Furthermore, 57 sources (44 unique, 13 also with new light curves) were selected for spectroscopic follow-up using either the SAAO 1.9-m telescope or the Southern African Large Telescope. We find many of these variables have spectra which are consistent with being delta Scuti type pulsating stars. At higher amplitudes, we detect four possible pulsating white dwarf/subdwarf sources and an eclipsing cataclysmic variable. Due to their rarity, these targets are ideal candidates for detailed follow-up studies. From spectroscopy, we confirm the symbiotic binary star nature of two variables identifie...

  10. Herschel observations of EXtraordinary Sources: Analysis of the full Herschel/HIFI molecular line survey of Sagittarius B2(N)

    CERN Document Server

    Neill, Justin L; Lis, Dariusz C; Schilke, Peter; Crockett, Nathan R; Favre, Cecile; Emprechtinger, Martin; Comito, Claudia; Qin, Sheng-Li; Anderson, Dana E; Burkhardt, Andrew M; Chen, Jo-Hsin; Harris, Brent J; Lord, Steven D; McGuire, Brett A; McNeill, Trevor D; Monje, Raquel R; Phillips, Thomas G; Steber, Amanda L; Vasyunina, Tatiana; Yu, Shanshan

    2014-01-01

    A sensitive broadband molecular line survey of the Sagittarius B2(N) star-forming region has been obtained with the HIFI instrument on the Herschel Space Observatory, offering the first high-spectral resolution look at this well-studied source in a wavelength region largely inaccessible from the ground (625-157 um). From the roughly 8,000 spectral features in the survey, a total of 72 isotopologues arising from 44 different molecules have been identified, ranging from light hydrides to complex organics, and arising from a variety of environments from cold and diffuse to hot and dense gas. We present an LTE model to the spectral signatures of each molecule, constraining the source sizes for hot core species with complementary SMA interferometric observations, and assuming that molecules with related functional group composition are cospatial. For each molecule, a single model is given to fit all of the emission and absorption features of that species across the entire 480-1910 GHz spectral range, accounting fo...

  11. The OmegaWhite survey for short-period variable stars - III: follow-up photometric and spectroscopic observations

    Science.gov (United States)

    Macfarlane, S. A.; Woudt, P. A.; Groot, P. J.; Ramsay, G.; Toma, R.; Motsoaledi, M.; Crause, L. A.; Gilbank, D. G.; O'Donoghue, D.; Potter, S. B.; Sickafoose, A. A.; van Gend, C.; Worters, H. L.

    2017-02-01

    We present photometric and spectroscopic follow-up observations of short-period variables discovered in the OmegaWhite survey, a wide-field high-cadence g-band synoptic survey targeting the Galactic Plane. We have used fast photometry on the SAAO 1.0- and 1.9-m telescopes to obtain light curves of 27 variables, and use these results to validate the period and amplitude estimates from the OmegaWhite processing pipeline. Furthermore, 57 sources (44 unique, 13 with new light curves) were selected for spectroscopic follow-up using either the SAAO 1.9-m telescope or the Southern African Large Telescope. We find that many of these variables have spectra which are consistent with being δ Scuti-type pulsating stars. At higher amplitudes, we detect four possible pulsating white dwarf/subdwarf sources and an eclipsing cataclysmic variable. Due to their rarity, these targets are ideal candidates for detailed follow-up studies. From spectroscopy, we confirm the symbiotic binary star nature of two variables identified as such in the SIMBAD database. We also report what could possibly be the first detection of the `Bump Cepheid' phenomena in a δ Scuti star, with OW J175848.21-271653.7 showing a pronounced 22 per cent amplitude dip lasting 3 min during each pulsational cycle peak. However, the precise nature of this target is still uncertain as it exhibits the spectral features of a B-type star.

  12. Wide-field infrared survey explorer observations of young stellar objects in the Lynds 1509 dark cloud in Auriga

    Energy Technology Data Exchange (ETDEWEB)

    Liu, Wilson M.; McCollum, Bruce; Fajardo-Acosta, Sergio [Infrared Processing and Analysis Center, California Institute of Technology, MC 100-22, Pasadena, CA 91125 (United States); Padgett, Deborah L. [National Aeronautics and Space Administration, Goddard Space Flight Center, Code 665, Greenbelt, MD 20771 (United States); Terebey, Susan; Angione, John [Department of Physics and Astronomy, California State University, Los Angeles, CA 90032 (United States); Rebull, Luisa M. [Spitzer Science Center, California Institute of Technology, MC 314-6, Pasadena, CA 91125 (United States); Leisawitz, David, E-mail: wliu@ipac.caltech.edu [National Aeronautics and Space Administration, Goddard Space Flight Center, Code 605, Greenbelt, MD 20771 (United States)

    2014-06-01

    The Wide-Field Infrared Survey Explorer (WISE) has uncovered a striking cluster of young stellar object (YSO) candidates associated with the L1509 dark cloud in Auriga. The WISE observations, at 3.4 μm, 4.6 μm, 12 μm, and 22 μm, show a number of objects with colors consistent with YSOs, and their spectral energy distributions suggest the presence of circumstellar dust emission, including numerous Class I, flat spectrum, and Class II objects. In general, the YSOs in L1509 are much more tightly clustered than YSOs in other dark clouds in the Taurus-Auriga star forming region, with Class I and flat spectrum objects confined to the densest aggregates, and Class II objects more sparsely distributed. We estimate a most probable distance of 485-700 pc, and possibly as far as the previously estimated distance of 2 kpc.

  13. Herschel observations of extraordinary sources: Analysis of the full Herschel/HIFI molecular line survey of sagittarius B2(N)

    Energy Technology Data Exchange (ETDEWEB)

    Neill, Justin L.; Bergin, Edwin A.; Crockett, Nathan R.; Favre, Cécile; Anderson, Dana E.; Burkhardt, Andrew M.; McNeill, Trevor D. [Department of Astronomy, University of Michigan, 500 Church Street, Ann Arbor, MI 48109 (United States); Lis, Dariusz C.; Emprechtinger, Martin; Monje, Raquel R.; Phillips, Thomas G. [California Institute of Technology, Cahill Center for Astronomy and Astrophysics 301-17, Pasadena, CA 91125 (United States); Schilke, Peter; Comito, Claudia; Qin, Sheng-Li [Physikalisches Institut, Universität zu Köln, Zülpicher Str. 77, D-50937 Köln (Germany); Chen, Jo-Hsin [Jet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Drive, Pasadena, CA 91109 (United States); Harris, Brent J.; Steber, Amanda L.; Vasyunina, Tatiana [Department of Chemistry, University of Virginia, McCormick Road, Charlottesville, VA 22904 (United States); Lord, Steven D. [National Herschel Science Center, California Institute of Technology, Pasadena, CA 91125 (United States); McGuire, Brett A., E-mail: jneill@umich.edu, E-mail: ebergin@umich.edu [Division of Chemistry and Chemical Engineering, California Institute of Technology, Pasadena, CA 91125 (United States); and others

    2014-07-01

    A sensitive broadband molecular line survey of the Sagittarius B2(N) star-forming region has been obtained with the Heterodyne Instrument for the Far-Infrared (HIFI) instrument on the Herschel Space Observatory, offering the first high spectral resolution look at this well-studied source in a wavelength region largely inaccessible from the ground (625-157 μm). From the roughly 8000 spectral features in the survey, a total of 72 isotopologues arising from 44 different molecules have been identified, ranging from light hydrides to complex organics, and arising from a variety of environments from cold and diffuse to hot and dense gas. We present a local thermodynamic equilibrium (LTE) model to the spectral signatures of each molecule, constraining the source sizes for hot core species with complementary Submillimeter Array interferometric observations and assuming that molecules with related functional group composition are cospatial. For each molecule, a single model is given to fit all of the emission and absorption features of that species across the entire 480-1910 GHz spectral range, accounting for multiple temperature and velocity components when needed to describe the spectrum. As with other HIFI surveys toward massive star-forming regions, methanol is found to contribute more integrated line intensity to the spectrum than any other species. We discuss the molecular abundances derived for the hot core where the LTE approximation is generally found to describe the spectrum well, in comparison to abundances derived for the same molecules in the Orion KL region from a similar HIFI survey. Notably, we find significantly higher abundances of amine- and amide-bearing molecules (CH{sub 3}NH{sub 2}, CH{sub 2}NH, and NH{sub 2}CHO) toward Sgr B2(N) than Orion KL and lower abundances of some complex oxygen-bearing molecules (CH{sub 3}OCHO in particular). In addition to information on the chemical composition of the hot core, the strong far-infrared dust continuum allows

  14. Wide-Field Infrared Survey Explorer Observations of Young Stellar Objects in the Lynds 1509 Dark Cloud in Auriga

    Science.gov (United States)

    Liu, Wilson M.; Padgett, Deborah L.; Terebey, Susan; Angione, John; Rebull, Luisa M.; McCollum, Bruce; Fajardo-Acosta, Sergio; Leisawitz, David

    2015-01-01

    The Wide-Field Infrared Survey Explorer (WISE) has uncovered a striking cluster of young stellar object (YSO) candidates associated with the L1509 dark cloud in Auriga. The WISE observations, at 3.4, 4.6, 12, and 22 microns, show a number of objects with colors consistent with YSOs, and their spectral energy distributions suggest the presence of circumstellar dust emission, including numerous Class I, flat spectrum, and Class II objects. In general, the YSOs in L1509 are much more tightly clustered than YSOs in other dark clouds in the Taurus-Auriga star forming region, with Class I and flat spectrum objects confined to the densest aggregates, and Class II objects more sparsely distributed. We estimate a most probable distance of 485-700 pc, and possibly as far as the previously estimated distance of 2 kpc.

  15. Geocoronal Balmer-alpha Emission Observed by the Wisconsin H-Alpha Mapper During the Southern Sky Survey

    Science.gov (United States)

    Mierkiewicz, E. J.; Haffner, L. M.; Nossal, S. M.; Wilson, M. L.; Freer, C. W.; Babler, B.; Gardner, D.; Roesler, F. L.

    2015-12-01

    After a successful eleven-year run at Kitt Peak Observatory (AZ), the Wisconsin H-Alpha Mapper (WHAM) was moved to Cerro Tololo (Chile) in 2009 to complete the southern portion of the Galactic Balmer-alpha survey. Although WHAM is primarily used for making observations of the interstellar medium, the terrestrial emission present in each of WHAM's astronomical spectra offers a rich resource for studying the Earth's atmosphere. Here we present an overview of the terrestrial Balmer-alpha emission collected during WHAM's first five years of operation under southern skies. Seasonal trends and comparisons with northern hemisphere observations will be discussed. WHAM can detect Balmer-alpha emission as faint as 0.05R in a 30s exposure, covering a 200 km/s (4.4 Angstrom) spectral region with 12 km/s spectral resolution from a 1 degree beam on the sky. With this sensitivity, hundreds of spectra can be collected in a single clear night. Although not capable of fully resolving the geocoronal Balmer-alpha line profile itself, WHAM's sensitivity makes it an exceptional instrument for geocoronal Balmer-alpha intensity observations. This work is supported by NSF award AGS-1352311 and AST-1108911.

  16. First spectro-interferometric survey of Be stars I. Observations and constraints on the disks geometry and kinematics

    CERN Document Server

    Meilland, Anthony; Kanaan, Samer; Stee, Philippe; Petrov, Romain

    2011-01-01

    Context. Classical Be stars are hot non-supergiant stars surrounded by a gaseous circumstellar disk responsible for the observed infrared-excess and emission lines. The phenomena involved in the disk formation still remain highly debated. Aims. To progress in the understanding of the physical process or processes responsible for the mass-ejection and test the hypothesis that they depends on the stellar parameters, we initiate a survey on the circumstellar environment of the brightest Be stars. Methods. To achieve this goal, we used spectro-interferometry, the only technique combining high spectral (R=12000) and high spatial (\\thetamin=4mas) resolutions. Observations were carried out at Paranal observatory with the VLTI/AMBER instrument. We concentrate our observations on the Br{\\gamma} emission line to be able to study the kinematics within the circumstellar disk. Our sample is composed of eight bright classical Be stars : \\alph Col, \\kappa CMa, \\omega Car, p Car, \\delta Cen, \\mu Cen, \\alpha Ara, and o Aqr. R...

  17. Traffic Accidents Involving Cyclists Identifying Causal Factors Using Questionnaire Survey, Traffic Accident Data, and Real-World Observation.

    Science.gov (United States)

    Oikawa, Shoko; Hirose, Toshiya; Aomura, Shigeru; Matsui, Yasuhiro

    2016-11-01

    The purpose of this study is to clarify the mechanism of traffic accidents involving cyclists. The focus is on the characteristics of cyclist accidents and scenarios, because the number of traffic accidents involving cyclists in Tokyo is the highest in Japan. First, dangerous situations in traffic incidents were investigated by collecting data from 304 cyclists in one city in Tokyo using a questionnaire survey. The survey indicated that cyclists used their bicycles generally while commuting to work or school in the morning. Second, the study investigated the characteristics of 250 accident situations involving cyclists that happened in the city using real-world bicycle accident data. The results revealed that the traffic accidents occurred at intersections of local streets, where cyclists collided most often with vehicles during commute time in the morning. Third, cyclists' behavior was observed at a local street intersection in the morning in the city using video pictures. In one hour during the morning commute period, 250 bicycles passed through the intersection. The results indicated that one of the reasons for traffic accidents involving cyclists might be the combined effect of low visibility, caused by the presence of box-like building structures close to the intersections, and the cyclists' behavior in terms of their velocity and no confirming safety. It was observed that, on average, bicycle velocity was 3.1 m/s at the initial line of an intersection. The findings from this study could be useful in developing new technologies to improve cyclist safety, such as alert devices for cyclists and vehicle drivers, wireless communication systems between cyclists and vehicle drivers, or advanced vehicles with bicycle detection and collision mitigation systems.

  18. Ectoparasitism on deep-sea fishes in the western North Atlantic: In situ observations from ROV surveys.

    Science.gov (United States)

    Quattrini, Andrea M; Demopoulos, Amanda W J

    2016-12-01

    A complete understanding of how parasites influence marine ecosystem functioning requires characterizing a broad range of parasite-host interactions while determining the effects of parasitism in a variety of habitats. In deep-sea fishes, the prevalence of parasitism remains poorly understood. Knowledge of ectoparasitism, in particular, is limited because collection methods often cause dislodgment of ectoparasites from their hosts. High-definition video collected during 43 remotely operated vehicle surveys (2013-2014) provided the opportunity to examine ectoparasitism on fishes across habitats (open slope, canyon, seamount, cold seep) and depths (494-4689 m) off the northeastern U.S., while providing high-resolution images and valuable observations of fish behavior. Only 9% (n = 125 individuals) of all observed fishes (25 species) were confirmed with ectoparasites, but higher percentages (∼33%) were observed for some of the most abundant fish species (e.g., Antimora rostrata). Ectoparasites included two copepod families (Lernaeopodidae, Sphyriidae) that infected four host species, two isopod families (Cymothoidae, Aegidae) that infected three host species, and one isopod family (Gnathiidae) that infected 19 host species. Hyperparasitism was also observed. As host diversity declined with depth, ectoparasite diversity declined; only gnathiids were observed at depths down to 3260 m. Thus, gnathiids appear to be the most successful group to infect a diversity of fishes across a broad depth range in the deep sea. For three dominant fishes (A. rostrata, Nezumia bairdii, Synaphobranchus spp.), the abundance and intensity of ectoparasitism peaked in different depths and habitats depending on the host species examined. Notably, gnathiid infections were most intense on A. rostrata, particularly in submarine canyons, suggesting that these habitats may increase ectoparasite infections. Although ectoparasitism is often overlooked in deep-sea benthic communities, our

  19. Ectoparasitism on deep-sea fishes in the western North Atlantic: In situ observations from ROV surveys

    Science.gov (United States)

    Quattrini, Andrea; Demopoulos, Amanda

    2016-01-01

    A complete understanding of how parasites influence marine ecosystem functioning requires characterizing a broad range of parasite-host interactions while determining the effects of parasitism in a variety of habitats. In deep-sea fishes, the prevalence of parasitism remains poorly understood. Knowledge of ectoparasitism, in particular, is limited because collection methods often cause dislodgment of ectoparasites from their hosts. High-definition video collected during 43 remotely operated vehicle surveys (2013–2014) provided the opportunity to examine ectoparasitism on fishes across habitats (open slope, canyon, seamount, cold seep) and depths (494–4689 m) off the northeastern U.S., while providing high-resolution images and valuable observations of fish behavior. Only 9% (n = 125 individuals) of all observed fishes (25 species) were confirmed with ectoparasites, but higher percentages (∼33%) were observed for some of the most abundant fish species (e.g., Antimora rostrata). Ectoparasites included two copepod families (Lernaeopodidae, Sphyriidae) that infected four host species, two isopod families (Cymothoidae, Aegidae) that infected three host species, and one isopod family (Gnathiidae) that infected 19 host species. Hyperparasitism was also observed. As host diversity declined with depth, ectoparasite diversity declined; only gnathiids were observed at depths down to 3260 m. Thus, gnathiids appear to be the most successful group to infect a diversity of fishes across a broad depth range in the deep sea. For three dominant fishes (A. rostrata, Nezumia bairdii, Synaphobranchus spp.), the abundance and intensity of ectoparasitism peaked in different depths and habitats depending on the host species examined. Notably, gnathiid infections were most intense on A. rostrata, particularly in submarine canyons, suggesting that these habitats may increase ectoparasite infections. Although ectoparasitism is often overlooked in deep-sea benthic communities

  20. CHANDRA OBSERVATIONS OF 3C RADIO SOURCES WITH z < 0.3. II. COMPLETING THE SNAPSHOT SURVEY

    Energy Technology Data Exchange (ETDEWEB)

    Massaro, F. [SLAC National Laboratory and Kavli Institute for Particle Astrophysics and Cosmology, 2575 Sand Hill Road, Menlo Park, CA 94025 (United States); Tremblay, G. R. [European Southern Observatory, Karl-Schwarzschild-Str. 2, D-85748 Garching bei Muenchen (Germany); Harris, D. E.; O' Dea, C. P. [Smithsonian Astrophysical Observatory, 60 Garden Street, Cambridge, MA 02138 (United States); Kharb, P.; Axon, D. [Department of Physics, Rochester Institute of Technology, Carlson Center for Imaging Science 76-3144, 84 Lomb Memorial Dr., Rochester, NY 14623 (United States); Balmaverde, B.; Capetti, A. [INAF-Osservatorio Astrofisico di Torino, Strada Osservatorio 20, I-10025 Pino Torinese (Italy); Baum, S. A. [Carlson Center for Imaging Science 76-3144, 84 Lomb Memorial Dr., Rochester, NY 14623 (United States); Chiaberge, M.; Macchetto, F. D.; Sparks, W. [Space Telescope Science Institute, 3700 San Martine Drive, Baltimore, MD 21218 (United States); Gilli, R. [INAF-Osservatorio Astronomico di Bologna, Via Ranzani 1, I-40127 Bologna (Italy); Giovannini, G. [INAF-Istituto di Radioastronomia di Bologna, Via Gobetti 101, I-40129 Bologna (Italy); Grandi, P.; Torresi, E. [INAF-IASF-Istituto di Astrofisica Spaziale e fisica Cosmica di Bologna, Via P. Gobetti 101, I-40129 Bologna (Italy); Risaliti, G. [INAF-Osservatorio Astronomico di Arcetri, Largo E. Fermi 5, I-50125 Firenze (Italy)

    2012-12-15

    We report on the second round of Chandra observations of the 3C snapshot survey developed to observe the complete sample of 3C radio sources with z < 0.3 for 8 ks each. In the first paper, we illustrated the basic data reduction and analysis procedures performed for the 30 sources of the 3C sample observed during Chandra Cycle 9, while here we present the data for the remaining 27 sources observed during Cycle 12. We measured the X-ray intensity of the nuclei and of any radio hot spots and jet features with associated X-ray emission. X-ray fluxes in three energy bands, i.e., soft, medium, and hard, for all the sources analyzed are also reported. For the stronger nuclei, we also applied the standard spectral analysis, which provides the best-fit values of the X-ray spectral index and absorbing column density. In addition, a detailed analysis of bright X-ray nuclei that could be affected by pile-up has been performed. X-ray emission was detected for all the nuclei of the radio sources in our sample except for 3C 319. Among the current sample, there are two compact steep spectrum radio sources, two broad-line radio galaxies, and one wide angle tail radio galaxy, 3C 89, hosted in a cluster of galaxies clearly visible in our Chandra snapshot observation. In addition, we also detected soft X-ray emission arising from the galaxy cluster surrounding 3C 196.1. Finally, X-ray emission from hot spots has been found in three FR II radio sources and, in the case of 3C 459, we also report the detection of X-ray emission associated with the eastern radio lobe as well as X-ray emission cospatial with radio jets in 3C 29 and 3C 402.

  1. Ectoparasitism on deep-sea fishes in the western North Atlantic: In situ observations from ROV surveys

    Directory of Open Access Journals (Sweden)

    Andrea M. Quattrini

    2016-12-01

    Full Text Available A complete understanding of how parasites influence marine ecosystem functioning requires characterizing a broad range of parasite-host interactions while determining the effects of parasitism in a variety of habitats. In deep-sea fishes, the prevalence of parasitism remains poorly understood. Knowledge of ectoparasitism, in particular, is limited because collection methods often cause dislodgment of ectoparasites from their hosts. High-definition video collected during 43 remotely operated vehicle surveys (2013–2014 provided the opportunity to examine ectoparasitism on fishes across habitats (open slope, canyon, seamount, cold seep and depths (494–4689 m off the northeastern U.S., while providing high-resolution images and valuable observations of fish behavior. Only 9% (n = 125 individuals of all observed fishes (25 species were confirmed with ectoparasites, but higher percentages (∼33% were observed for some of the most abundant fish species (e.g., Antimora rostrata. Ectoparasites included two copepod families (Lernaeopodidae, Sphyriidae that infected four host species, two isopod families (Cymothoidae, Aegidae that infected three host species, and one isopod family (Gnathiidae that infected 19 host species. Hyperparasitism was also observed. As host diversity declined with depth, ectoparasite diversity declined; only gnathiids were observed at depths down to 3260 m. Thus, gnathiids appear to be the most successful group to infect a diversity of fishes across a broad depth range in the deep sea. For three dominant fishes (A. rostrata, Nezumia bairdii, Synaphobranchus spp., the abundance and intensity of ectoparasitism peaked in different depths and habitats depending on the host species examined. Notably, gnathiid infections were most intense on A. rostrata, particularly in submarine canyons, suggesting that these habitats may increase ectoparasite infections. Although ectoparasitism is often overlooked in deep-sea benthic

  2. Academic Practices to Gain and Maintain Student-Teacher Connectedness and Classroom Behavioral Management, Related to Educator Demographics

    Science.gov (United States)

    Kendall, Leslie Threadgill

    2015-01-01

    Connectedness and classroom management has been defined as the ability to relate to students and keep order and maintain successful relationships with individuals. This qualitative study utilized surveys, questionnaires, interviews, and observations to examine the best practices implemented by educators to develop and maintain connections with…

  3. Predicting High School Student Use of Learning Strategies: The Role of Preferred Learning Styles and Classroom Climate

    Science.gov (United States)

    Cheema, Jehanzeb; Kitsantas, Anastasia

    2016-01-01

    This study investigated the predictiveness of preferred learning styles (competitive and cooperative) and classroom climate (teacher support and disciplinary climate) on learning strategy use in mathematics. The student survey part of the Programme for International Student Assessment 2003 comprising of 4633 US observations was used in a weighted…

  4. Academic Practices to Gain and Maintain Student-Teacher Connectedness and Classroom Behavioral Management, Related to Educator Demographics

    Science.gov (United States)

    Kendall, Leslie Threadgill

    2015-01-01

    Connectedness and classroom management has been defined as the ability to relate to students and keep order and maintain successful relationships with individuals. This qualitative study utilized surveys, questionnaires, interviews, and observations to examine the best practices implemented by educators to develop and maintain connections with…

  5. Predicting High School Student Use of Learning Strategies: The Role of Preferred Learning Styles and Classroom Climate

    Science.gov (United States)

    Cheema, Jehanzeb; Kitsantas, Anastasia

    2016-01-01

    This study investigated the predictiveness of preferred learning styles (competitive and cooperative) and classroom climate (teacher support and disciplinary climate) on learning strategy use in mathematics. The student survey part of the Programme for International Student Assessment 2003 comprising of 4633 US observations was used in a weighted…

  6. History of surface displacements at the Yellowstone Caldera, Wyoming, from leveling surveys and InSAR observations, 1923-2008

    Science.gov (United States)

    Dzurisin, Daniel; Wicks, Charles W.; Poland, Michael P.

    2012-01-01

    Modern geodetic studies of the Yellowstone caldera, Wyoming, and its extraordinary tectonic, magmatic, and hydrothermal systems date from an initial leveling survey done throughout Yellowstone National Park in 1923 by the U.S. Coast and Geodetic Survey. A repeat park-wide survey by the U.S. Geological Survey (USGS) and the University of Utah during 1975-77 revealed that the central part of the caldera floor had risen more than 700 mm since 1923, at an average rate of 14±1 mm/yr. From 1983 to 2007, the USGS conducted 15 smaller surveys of a single level line that crosses the northeast part of the caldera, including the area where the greatest uplift had occurred from 1923 to 1975-77. The 1983 and 1984 surveys showed that uplift had continued at an average rate of 22±1 mm/yr since 1975-77, but no additional uplift occurred during 1984-85 (-2±5 mm/yr), and during 1985-95 the area subsided at an average rate of 19±1 mm/yr. The change from uplift to subsidence was accompanied by an earthquake swarm, the largest ever recorded in the Yellowstone area (as of March 2012), starting in October 1985 and located near the northwest rim of the caldera. Interferometric synthetic aperture radar (InSAR) images showed that the area of greatest subsidence migrated from the northeast part of the caldera (including the Sour Creek resurgent dome) during 1992-93 to the southwest part (including the Mallard Lake resurgent dome) during 1993-95. Thereafter, uplift resumed in the northeast part of the caldera during 1995-96, while subsidence continued in the southwest part. The onset of uplift migrated southwestward, and by mid-1997, uplift was occurring throughout the entire caldera (essentially rim to rim, including both domes). Consistent with these InSAR observations, leveling surveys indicated 24±3 mm of uplift in the northeast part of the caldera during 1995-98. The beginning of uplift was coincident with or followed shortly after an earthquake swarm near the north caldera rim

  7. Primary school teachers’ views about pupil control ideologies and classroom management styles

    Directory of Open Access Journals (Sweden)

    Kürşad Yılmaz

    2009-12-01

    Full Text Available Classroom management is a critical competency area for all teachers because classroom management skills are directly relatedto pupil achievement. In the present study, the four-category (authoritarian, authoritative, laissez-faire, indifferentclassification of Kris (1997a is used. Pupil control ideologies, conceptualized by Willover, Eidell and Hoy (1967, were developedto define teachers’ views about pupil control. Pupil control ideologies conceptualized as two poles ranging from custodialcontrol ideology to humanistic control ideology. The purpose of the present study is to determine the correlation betweenprimary school teachers’ views about pupil control ideologies and classroom management styles. The survey model studyattempts to answer the research questions. 200 primary school teachers from Kütahya province are included in the sample ofthe research. The data is collected using “Classroom Management Profile Scale” and the “Pupil Control Ideology Scale”.Descriptive statistics and Pearson correlation analysis were used in data analysis. According to the findings obtained from thestudy, primary school teachers mostly presented authoritarian classroom management style, which was respectively followedby authoritative classroom management style, laissez-faire classroom management style and indifferent classroommanagement style. The findings of the study show that primary school teachers are closer to custodial control ideology. Acustodial control ideology has certain qualities such as strict control, enforcement of orders, one way downwardcommunication, and distrust towards pupils, cruel punishments and taking undisciplined behavior as personal offences. There isa moderate, positive and significant correlation between the participants’ views about custodial control ideologies andauthoritarian classroom management styles. It could be said from the findings of the study that the more the custodial controlideology of the participants

  8. A census of dense cores in the Aquila cloud complex: SPIRE/PACS observations from the Herschel Gould Belt survey

    CERN Document Server

    Konyves, V; Men'shchikov, A; Palmeirim, P; Arzoumanian, D; Schneider, N; Roy, A; Didelon, P; Maury, A; Shimajiri, Y; Di Francesco, J; Bontemps, S; Peretto, N; Benedettini, M; Bernard, J -Ph; Elia, D; Griffin, M J; Hill, T; Kirk, J; Ladjelate, B; Marsh, K; Martin, P G; Motte, F; Luong, Q Nguyen; Pezzuto, S; Roussel, H; Rygl, K L J; Sadavoy, S I; Schisano, E; Spinoglio, L; Ward-Thompson, D; White, G J

    2015-01-01

    We present and discuss the results of the Herschel Gould Belt survey observations in a ~11 deg^2 area of the Aquila molecular cloud complex at d~260 pc, imaged with the SPIRE/PACS cameras from 70 to 500 micron. We identify a complete sample of starless dense cores and embedded protostars in this region, and analyze their global properties and spatial distributions. We find a total of 651 starless cores, ~60% of which are gravitationally bound prestellar cores, and they will likely form stars in the future. We also detect 58 protostellar cores. The core mass function (CMF) derived for the prestellar cores is very similar in shape to the stellar initial mass function (IMF), supporting the earlier view that there is a close physical link between the IMF and the CMF. The global shift in mass scale observed between the CMF and the IMF is consistent with a typical star formation efficiency of ~40%. By comparing the numbers of starless cores to the number of young stellar objects, we estimate that the lifetime of pr...

  9. BAT AGN Spectroscopic Survey - III. An observed link between AGN Eddington ratio and narrow-emission-line ratios

    Science.gov (United States)

    Oh, Kyuseok; Schawinski, Kevin; Koss, Michael; Trakhtenbrot, Benny; Lamperti, Isabella; Ricci, Claudio; Mushotzky, Richard; Veilleux, Sylvain; Berney, Simon; Crenshaw, D. Michael; Gehrels, Neil; Harrison, Fiona; Masetti, Nicola; Soto, Kurt T.; Stern, Daniel; Treister, Ezequiel; Ueda, Yoshihiro

    2017-01-01

    We investigate the observed relationship between black hole mass (MBH), bolometric luminosity (Lbol) and Eddington ratio (λEdd) with optical emission-line ratios ([N II] λ6583/Hα, [S II] λλ6716, 6731/Hα, [O I] λ6300/Hα, [O III] λ5007/Hβ, [Ne III] λ3869/Hβ and He II λ4686/Hβ) of hard X-ray-selected active galactic nuclei (AGN) from the BAT AGN Spectroscopic Survey. We show that the [N II] λ6583/Hα ratio exhibits a significant correlation with λEdd (RPear = -0.44, p-value = 3 × 10-13, σ = 0.28 dex), and the correlation is not solely driven by MBH or Lbol. The observed correlation between [N II] λ6583/Hα ratio and MBH is stronger than the correlation with Lbol, but both are weaker than the λEdd correlation. This implies that the large-scale narrow lines of AGN host galaxies carry information about the accretion state of the AGN central engine. We propose that [N II] λ6583/Hα is a useful indicator of Eddington ratio with 0.6 dex of rms scatter, and that it can be used to measure λEdd and thus MBH from the measured Lbol, even for high-redshift obscured AGN. We briefly discuss possible physical mechanisms behind this correlation, such as the mass-metallicity relation, X-ray heating, and radiatively driven outflows.

  10. The VIPERS Multi-Lambda Survey - I: UV and NIR Observations, multi-color catalogs and photometric redshifts

    CERN Document Server

    Moutard, T; Ilbert, O; Coupon, J; Hudelot, P; Vibert, D; Comte, V; Conseil, S; Davidzon, I; Guzzo, L; Llebaria, A; Martin, C; McCracken, H J; Milliard, B; Morrison, G E; Schiminovich, D; Treyer, M; Van Werbaeke, L

    2016-01-01

    We present observations collected in the CFHTLS-VIPERS region in the ultraviolet (UV) with the GALEX satellite (far and near UV channels) and the near infrared with the CFHT/WIRCam camera ($K_s$-band) over an area of 22 and 27 deg$^2$, respectively. The depth of the photometry was optimized to measure the physical properties (e.g., SFR, stellar masses) of all the galaxies in the VIPERS spectroscopic survey. The large volume explored by VIPERS will enable a unique investigation of the relationship between the galaxy properties and their environment (density field and cosmic web) at high redshift (0.5 < z < 1.2). In this paper, we present the observations, the data reductions and the build-up of the multi-color catalogs. The CFHTLS-T0007 (gri-{\\chi}^2) images are used as reference to detect and measure the $K_s$-band photometry, while the T0007 u-selected sources are used as priors to perform the GALEX photometry based on a dedicated software (EMphot). Our final sample reaches $NUV_{AB}$~25 (at 5{\\sigma})...

  11. SZ observations with AMI of the hottest galaxy clusters detected in the XMM-Newton Cluster Survey

    CERN Document Server

    :,; Rodriguez-Gonzalvez, Carmen; Feroz, Farhan; Franzen, Thomas M O; Grainge, Keith J B; Hobson, Michael P; Hurley-Walker, Natasha; Lasenby, Anthony N; Lloyd-Davies, E J; Olamaie, Malak; Perrott, Yvette C; Pooley, Guy G; Rumsey, Clare; Romer, A Kathy; Saunders, Richard D E; Scaife, Anna M M; Schammel, Michel P; Scott, Paul F; Titterington, David J; Waldram, Elizabeth M

    2013-01-01

    We have obtained deep SZ observations towards 15 of the apparently hottest XMM Cluster Survey (XCS) clusters that can be observed with the Arcminute Microkelvin Imager (AMI). We use a Bayesian analysis to quantify the significance of our SZ detections. We detect the SZ effect at high significance towards three of the clusters and at lower significance for a further two clusters. Towards the remaining ten clusters, no clear SZ signal was measured. We derive cluster parameters using the XCS mass estimates as a prior in our Bayesian analysis. For all AMI-detected clusters, we calculate large-scale mass and temperature estimates while for all undetected clusters we determine upper limits on these parameters. We find that the large- scale mean temperatures derived from our AMI SZ measurements (and the upper limits from null detections) are substantially lower than the XCS-based core-temperature estimates. For clusters detected in the SZ, the mean temperature is, on average, a factor of 1.4 lower than temperatures ...

  12. BAT AGN Spectroscopic Survey-III. An observed link between AGN Eddington ratio and narrow emission line ratios

    CERN Document Server

    Oh, Kyuseok; Koss, Michael; Trakhtenbrot, Benny; Lamperti, Isabella; Ricci, Claudio; Mushotzky, Richard; Veilleux, Sylvain; Berney, Simon; Crenshaw, D Michael; Gehrels, Neil; Harrison, Fiona; Masetti, Nicola; Soto, Kurt T; Stern, Daniel; Treister, Ezequiel; Ueda, Yoshihiro

    2016-01-01

    We investigate the observed relationship between black hole mass ($M_{\\rm BH}$), bolometric luminosity ($L_{\\rm bol}$), and Eddington ratio (${\\lambda}_{\\rm Edd}$) with optical emission line ratios ([NII] {\\lambda}6583/H{\\alpha}, [SII] {\\lambda}{\\lambda}6716,6731/H{\\alpha}, [OI] {\\lambda}6300/H{\\alpha}, [OIII] {\\lambda}5007/H{\\beta}, [NeIII] {\\lambda}3869/H{\\beta}, and HeII {\\lambda}4686/H{\\beta}) of hard X-ray-selected AGN from the BAT AGN Spectroscopic Survey (BASS). We show that the [NII] {\\lambda}6583/H{\\alpha} ratio exhibits a significant correlation with ${\\lambda}_{\\rm Edd}$ ($R_{\\rm Pear}$ = -0.44, $p$-value=$3\\times10^{-13}$, {\\sigma} = 0.28 dex), and the correlation is not solely driven by $M_{\\rm BH}$ or $L_{\\rm bol}$. The observed correlation between [NII] {\\lambda}6583/H{\\alpha} ratio and $M_{\\rm BH}$ is stronger than the correlation with $L_{\\rm bol}$, but both are weaker than the ${\\lambda}_{\\rm Edd}$ correlation. This implies that the large-scale narrow lines of AGN host galaxies carry informa...

  13. The Bolocam Galactic Plane Survey. XI. Temperatures and Substructure of Galactic Clumps Based on 350 micron Observations

    CERN Document Server

    Merello, Manuel; Shirley, Yancy L; Rosolowsky, Erik; Ginsburg, Adam; Bally, John; Battersby, Cara; Dunham, Michael M

    2015-01-01

    We present 107 maps of continuum emission at 350 microns from Galactic molecular clumps. Observed sources were mainly selected from the Bolocam Galactic Plane Survey (BGPS) catalog, with 3 additional maps covering star forming regions in the outer Galaxy. The higher resolution of the SHARC-II images (8.5'' beam) compared with the 1.1 mm images from BGPS (33'' beam) allowed us to identify a large population of smaller substructures within the clumps. A catalog is presented for the 1386 sources extracted from the 350 micron maps. The color temperature distribution of clumps based on the two wavelengths has a median of 13.3 K and mean of 16.3 +- 0.4 K, assuming an opacity law index of 1.7. For the structures with the best determined color temperatures, the mean ratio of gas temperature, determined from NH3 observations, to dust color temperature is 0.88 and the median ratio is 0.76. About half the clumps have more than two substructures and 22 clumps have more than 10. The fraction of the mass in dense substruct...

  14. Collaborative Classroom Simulation (CCS): An Innovative Pedagogy Using Simulation in Nursing Education.

    Science.gov (United States)

    Berndt, Jodi; Dinndorf-Hogenson, Georgia; Herheim, Rena; Hoover, Carrie; Lanc, Nicole; Neuwirth, Janet; Tollefson, Bethany

    2015-01-01

    Collaborative Classroom Simulation (CCS) is a pedagogy designed to provide a simulation learning experience for a classroom of students simultaneously through the use of unfolding case scenarios. The purpose of this descriptive study was to explore the effectiveness of CCS based on student perceptions. Baccalaureate nursing students (n = 98) participated in the study by completing a survey after participation in the CCS experience. Opportunities for collaboration, clinical judgment, and participation as both observer and active participant were seen as strengths of the experience. Developed as a method to overcome barriers to simulation, CCS was shown to be an effective active learning technique that may prove to be sustainable.

  15. Probability friends-of-friends (PFOF) group finder: Performance study and observational data applications on photometric surveys

    Energy Technology Data Exchange (ETDEWEB)

    Jian, Hung-Yu; Chiueh, Tzihong [Department of Physics, National Taiwan University, 106, Taipei, Taiwan (China); Lin, Lihwai; Lin, Kai-Yang; Liu, Hauyu Baobab; Chen, Chin-Wei; Foucaud, Sebastien [Institute of Astronomy and Astrophysics, Academia Sinica, 106, Taipei, Taiwan (China); Merson, Alex [Department of Physics and Astronomy, University College London, Gower Street, London WC1E 6BT (United Kingdom); Baugh, Carlton; Cole, Shaun [Institute for Computational Cosmology, Department of Physics, Durham University, South Road, Durham DH1 3LE (United Kingdom); Huang, Jia-Sheng [National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100012 (China); Murphy, David N. A. [Department of Astronomy and Astrophysics, Pontificia Universidad Católica de Chile, Vicuña Mackenna 4860, 7820436 Macul, Santiago (Chile); Burgett, William; Kaiser, Nick, E-mail: hyj@phys.ntu.edu.tw [Institute for Astronomy, University of Hawaii, 2680 Woodlawn Drive, Honolulu, HI 96822 (United States)

    2014-06-20

    In tandem with observational data sets, we utilize realistic mock catalogs, based on a semi-analytic galaxy formation model, constructed specifically for Pan-STARRS1 Medium Deep Surveys to assess the performance of the Probability Friends-of-Friends (PFOF) group finder, and aim to develop a grouping optimization method applicable to surveys like Pan-STARRS1. Producing mock PFOF group catalogs under a variety of photometric redshift accuracies (σ{sub Δz/(1+z{sub s)}}), we find that catalog purities and completenesses from 'good' (σ{sub Δz/(1+z{sub s)}}∼ 0.01) to 'poor' (σ{sub Δz/(1+z{sub s)}}∼ 0.07) photo-zs gradually degrade from 77% and 70% to 52% and 47%, respectively. A 'subset optimization' approach is developed by using spectroscopic-redshift group data from the target field to train the group finder for application to that field and demonstrated using zCOSMOS groups for PFOF searches within PS1 Medium Deep Field04 (PS1MD04) and DEEP2 EGS groups in PS1MD07. With four data sets spanning the photo-z accuracy range from 0.01 to 0.06, we find purities and completenesses agree with their mock analogs. Further tests are performed via matches to X-ray clusters. We find PFOF groups match ∼85% of X-ray clusters identified in COSMOS and PS1MD04, lending additional support to the reliability of the detection algorithm. In the end, we demonstrate, by separating red and blue group galaxies in the EGS and PS1MD07 group catalogs, that the algorithm is not biased with respect to specifically recovering galaxies by color. The analyses suggest the PFOF algorithm shows great promise as a reliable group finder for photometric galaxy surveys of varying depth and coverage.

  16. Profiles of classroom behavior in high schools: associations with teacher behavior management strategies and classroom composition.

    Science.gov (United States)

    Pas, Elise T; Cash, Anne H; O'Brennan, Lindsey; Debnam, Katrina J; Bradshaw, Catherine P

    2015-04-01

    Although there has been considerable attention to the issue of classroom management and processes in educational reform models, there has been relatively limited research on these factors in high schools. The current study utilized observational data from 1262 classrooms in 52 high schools to examine teacher classroom management strategies and ratings of student compliance, engagement, and social disruption. Latent profile analysis (LPA) was conducted to examine specific patterns of classroom-wide student behavior in relation to teachers' use of classroom management strategies and classroom composition. The LPA revealed three distinct classroom behavioral profiles where students consistently met behavioral expectations (71%), inconsistently met expectations (23%), and were noncompliant (6%). Analyses indicated a functional association between patterns of student behavior and teachers' classroom management. In classrooms where students consistently met expectations, teachers provided more opportunities to respond and less disapproval and reactive behavioral management. Classrooms with noncompliant students had teachers who used the most disapproval and reactive behavior management. In addition, classrooms characterized as consistent had fewer males and more White students than classrooms characterized by inconsistent and noncompliant behaviors. These findings highlight the link between student patterns of behavior and teacher classroom management and have important implications for screening and professional development. Copyright © 2014 Society for the Study of School Psychology. Published by Elsevier Ltd. All rights reserved.

  17. The Research on the Model of Collaborative Observing Classroom in the Background of University-School Collaboration Culture%院校协作文化背景下"协同观课模式"实践探究

    Institute of Scientific and Technical Information of China (English)

    严启英; 左璜

    2015-01-01

    The development of University-School Collaboration and the dilemma of observing classroom culture urged the birth of the Model of Collaborative Observing Classroom. Reactive to the development of teacher cooperation culture and at the basis of the situation theory of learning and cultural teaching epistemology,this model which takes the "collaboration" as purpose and means together advocates the community of cultural practice as the observing subject,proposes the system of observing objects,insists on the mixed methods including qualitative and quantitative,pursues the multiple values.%院校协作的深层推进与已有观课文化的现实困境催生了"协同观课模式". 因应教师合作文化的发展,以情景学习理论与文化教学认识论为基础,"协同观课模式"统合了协同的价值性与工具性. 它主张以文化实践共同体作为观课主体, 提倡整体与局部结合的观课内容体系, 坚持经验与研究相统一的观课方法,并最终追求多元的价值取向.

  18. Virtual Classroom

    DEFF Research Database (Denmark)

    Christensen, Ove

    2013-01-01

    In the Scandinavian countries: Sweden, Norway and Denmark, the project GNU (Grænseoverskridende Nordisk Undervisning, i.e. Transnational Nordic Teaching) is experimenting with ways of conducting teaching across the borders in the elementary schools. The cloud classes are organised with one class ...... and benefits in regard to learning and pedagogy with virtual classroom....

  19. Classroom Tech

    Science.gov (United States)

    Instructor, 2006

    2006-01-01

    This article features the latest classroom technologies namely the FLY Pentop, WriteToLearn, and a new iris scan identification system. The FLY Pentop is a computerized pen from Leapster that "magically" understands what kids write and draw on special FLY paper. WriteToLearn is an automatic grading software from Pearson Knowledge Technologies and…

  20. Classroom Tips.

    Science.gov (United States)

    Stevens, Jacqueline; And Others

    1993-01-01

    Describes five classroom activities or projects used in Canadian social studies classes. Includes discussions of the use of artifacts, a field trip to Spain, a simulation of the Earth Summit meeting, and the application of mahatma Gandhi's philosophy to current problems. (CFR)

  1. 论课堂观察LICC范式:一种专业的听评课%On the Paradigm of LICC: A New Way of Profession Classroom Observation

    Institute of Scientific and Technical Information of China (English)

    崔允漷

    2012-01-01

    The problems of traditional Chinese classroom observation can be listed as listening without cooperation, commenting without evidence and research, which reflect the loss of professionalism. Based on the practical study for more than four years, we have built up a new professional LICC paradigm of observing class which aims to promote the effective teaching. The paradigm is to resolve the current issues and to use scientific observation methods by adhering to the scientific pragmatism. LICC deconstructs the class and advocates teachers to establish different cooperation groups, to study the effectiveness of classroom teaching problems. This paradigm is good at enriching the knowledge base of classroom, improving student learning and promoting teacher development, yet still has limitations on its reliability.%传统的听评课存在听课无合作、评课无依据、听评课无研究的症状,体现了专业性的丧失。课堂观察LICC范式从当前作为一种课堂研究的听评课存在的问题出发,坚持科学实用主义,通过对课堂的解构,倡导教师组建不同的合作体,采用类似科学观察的方法,研究课堂教学的有效性问题。该范式在丰富课堂知识、改善学生课堂学习、促进教师专业发展的同时,在可靠性方面还存在一定问题。

  2. An Overview and Reflection on Classroom Observation and Evaluation in the Past Twenty Years in China%我国听评课研究二十年:回顾与反思

    Institute of Scientific and Technical Information of China (English)

    方洁

    2014-01-01

    When school-based research goes further , the practice and research of classroom observation and evaluation are heading to prosperity gradually as well . With the ongoing mature of classroom observation techniques nowadays , the contents and forms of research on classroom observation and evaluation has developed and innovated further . In the past twenty years , the researches on classroom observation and evaluation include the nature , meaning and value , types and lens , contents and standards ,models ,strategies .Through reflecting on the researches mentioned above ,we have already achieved fruitful results . However , there are still some problems , such as simplex research method , priority to theory and minor attention to practice . Therefore , multi-dimension research , practice-oriented research , subject-related research multiple research methods are seriously needed .%听评课活动的实践与研究是随着校本教研的深入而逐渐走向繁荣的。在课堂观察技术日趋成熟的今天,听评课研究的内容与形式都得以拓展与创新。近二十年来,听评课活动的研究主要包括:听评课的内涵、意义与价值、类型与视角、内容与标准、模式与路径、策略与方法以及听评课活动中存在的问题等多个方面。反思听评课研究,虽然取得了丰硕的成果,但是不难发现尚存在研究主体与方法单一、重理论轻实践等问题。因此,听评课的研究主体应该多元化、研究取向应该走向实践、研究内容应该深入学科、研究方法应该多样化。

  3. Teachers' perceptions of effective science, technology, and mathematics professional development and changes in classroom practices

    Science.gov (United States)

    Boriack, Anna Christine

    The purpose of this study is to examine teachers' perceptions of professional development and changes in classroom practice. A proposed conceptual framework for effective professional development that results in changes in classroom practices was developed. Data from two programs that provided professional development to teachers in the areas of technology, mathematics, and science was used to inform the conceptual framework. These two programs were Target Technology in Texas (T3) and Mathematics, Science, and Technology Teacher Preparation Academies (MSTTPA). This dissertation used a multiple article format to explore each program separately, yet the proposed conceptual framework allowed for comparisons to be made between the two programs. The first study investigated teachers' perceptions of technology-related professional development after their districts had received a T3 grant. An online survey was administrated to all teachers to determine their perceptions of technology-related professional development along with technology self-efficacy. Classroom observations were conducted to determine if teachers were implementing technology. The results indicated that teachers did not perceive professional development as being effective and were not implementing technology in their classrooms. Teachers did have high technology self-efficacy and perceived adequate school support, which implies that effective professional development may be a large factor in whether or not teachers implement technology in their classrooms. The second study evaluated participants' perceptions of the effectiveness of mathematics and science professional development offered through a MSTTP academy. Current and former participants completed an online survey which measured their perceptions of academy activities and school environment. Participants also self-reported classroom implementation of technology. Interviews and open-ended survey questions were used to provide further insight into

  4. Survey lines along which SEABed Observation and Sampling System (SEABOSS) data were collected by the U.S. Geological Survey within the Northern Cape Cod Bay survey area (CCB_SeabossTrackline Esri shapefile, Geographic, WGS84).

    Data.gov (United States)

    U.S. Geological Survey, Department of the Interior — These data were collected under a cooperative agreement with the Massachusetts Office of Coastal Zone Management (CZM) and the U.S. Geological Survey (USGS),...

  5. Improving Photometric Redshifts using GALEX Observations for the SDSS Stripe 82 and the Next Generation of SZ Cluster Surveys

    CERN Document Server

    Niemack, Michael D; Verde, Licia; Menanteau, Felipe; Panter, Ben; Spergel, David

    2008-01-01

    Four large-area Sunyaev-Zeldovich (SZ) experiments -- APEX-SZ, SPT, ACT, and Planck -- promise to detect clusters of galaxies through the distortion of Cosmic Microwave Background photons by hot (> 10^6 K) cluster gas (the SZ effect) over thousands of square degrees. A large observational follow-up effort to obtain redshifts for these SZ-detected clusters is under way. Given the large area covered by these surveys, most of the redshifts will be obtained via the photometric redshift (photo-z) technique. Here we demonstrate, in an application using ~3000 SDSS stripe 82 galaxies with r<20, how the addition of GALEX photometry (FUV, NUV) greatly improves the photometric redshifts of galaxies obtained with optical griz or ugriz photometry. In the case where large spectroscopic training sets are available, empirical neural-network-based techniques (e.g., ANNz) can yield a photo-z scatter of $\\sigma_z = 0.018 (1+z)$. If large spectroscopic training sets are not available, the addition of GALEX data makes possible...

  6. Herschel observations of EXtra-Ordinary Sources: the present and future of spectral surveys with Herschel/HIFI

    CERN Document Server

    Bergin, E A; Comito, C; Crockett, N R; Lis, D C; Schilke, P; Wang, S; Bell, T A; Blake, G A; Bumble, B; Caux, E; Cabrit, S; Ceccarelli, C; Cernicharo, J; Daniel, F; de Graauw, Th; Dubernet, M -L; Emprechtinger, M; Encrenaz, P; Falgarone, E; Gerin, M; Giesen, T F; Goicoechea, J R; Goldsmith, P F; Gupta, H; Hartogh, P; Helmich, F P; Herbst, E; Joblin, C; Johnstone, D; Kawamura, J H; Langer, W D; Latter, W B; Lord, S D; Maret, S; Martin, P G; Melnick, G J; Menten, K M; Morris, P; Muller, H S P; Murphy, J A; Neufeld, D A; Ossenkopf, V; Pagani, L; Pearson, J C; Perault, M; Plume, R; Roelfsema, P; Qin, S -L; Salez, M; Schlemmer, S; Stutzki, J; Tielens, A G G M; Trappe, N; van der Tak, F F S; Vastel, C; Yorke, H W; Yu, S; Zmuidzinas, J

    2010-01-01

    We present initial results from the Herschel GT key program: Herschel observations of EXtra-Ordinary Sources (HEXOS) and outline the promise and potential of spectral surveys with Herschel/HIFI. The HIFI instrument offers unprecedented sensitivity, as well as continuous spectral coverage across the gaps imposed by the atmosphere, opening up a largely unexplored wavelength regime to high-resolution spectroscopy. We show the spectrum of Orion KL between 480 and 560 GHz and from 1.06 to 1.115 THz. From these data, we confirm that HIFI separately measures the dust continuum and spectrally resolves emission lines in Orion KL. Based on this capability we demonstrate that the line contribution to the broad-band continuum in this molecule-rich source is ~20-40% below 1 THz and declines to a few percent at higher frequencies. We also tentatively identify multiple transitions of HD18O in the spectra. The first detection of this rare isotopologue in the interstellar medium suggests that HDO emission is optically thick i...

  7. VVV Survey Observations of a Microlensing Stellar Mass Black Hole Candidate in the Field of the Globular Cluster NGC 6553

    CERN Document Server

    Minniti, D; Alonso-Garcia, J; Anguita, T; Catelan, M; Gran, F; Motta, V; Muro, G; Rojas, K; Saito, R K

    2015-01-01

    We report the discovery of a large timescale candidate microlensing event of a bulge stellar source based on near-infrared observations with the VISTA Variables in the Via Lactea Survey (VVV). The new microlensing event is projected only 3.5 arcmin away from the center of the globular cluster NGC 6553. The source appears to be a bulge giant star with magnitude Ks = 13.52, based on the position in the color-magnitude diagram. The foreground lens may be located in the globular cluster, which has well-known parameters such as distance and proper motions. If the lens is a cluster member, we can directly estimate its mass simply following Paczynski et al. (1996) which is a modified version of the more general case due to Refsdal. In that case, the lens would be a massive stellar remnant, with M = 1.5-3.5 Msun. If the blending fraction of the microlensing event appears to be small, and this lens would represent a good isolated black hole (BH) candidate, that would be the oldest BH known. Alternative explanations (w...

  8. A Prospective Observational Survey on the Long-Term Effect of LDL Apheresis on Drug-Resistant Nephrotic Syndrome

    Directory of Open Access Journals (Sweden)

    Eri Muso

    2015-08-01

    Full Text Available Background/Aims: LDL apheresis (LDL-A is used for drug-resistant nephrotic syndrome (NS as an alternative therapy to induce remission by improvement of hyperlipidemia. Several clinical studies have suggested the efficacy of LDL-A for refractory NS, but the level of evidence remains insufficient. A multicenter prospective study, POLARIS (Prospective Observational Survey on the Long-Term Effects of LDL Apheresis on Drug-Resistant Nephrotic Syndrome, was conducted to evaluate its clinical efficacy with high-level evidence. Methods: Patients with NS who showed resistance to primary medication for at least 4 weeks were prospectively recruited to the study and treated with LDL-A. The long-term outcome was evaluated based on the rate of remission of NS 2 years after treatment. Factors affecting the outcome were also examined. Results: A total of 58 refractory NS patients from 40 facilities were recruited and enrolled as subjects of the POLARIS study. Of the 44 subjects followed for 2 years, 21 (47.7% showed remission of NS based on a urinary protein (UP level Conclusions: Almost half of the cases of drug-resistant NS showed remission 2 years after LDL-A. Improvement of nephrotic parameters at termination of the LDL-A treatment was a predictor of a favorable outcome.

  9. Asteroid phase curve analysis with the H, G 1, G 2 photometric phase function: application to the PTF survey observations

    Science.gov (United States)

    Penttilä, Antti; Cellino, Alberto; Lu, Xiaoping; Shevchenko, Vasilij G.; Muinonen, Karri

    2016-10-01

    Estimation of an asteroid's absolute magnitude H from its photometry is extremely important. The absolute magnitude relates the brightness of the asteroid to its size, if the geometric albedo is known. The shape of the phase curve can serve as a proxy for the taxonomic type of the asteroid in cases with no spectral information available [1,2].In 2012, the IAU adopted the H,G1,G2 function to replace the H,G function for phase curve analysis [3]. This new function improves the backscattering behavior of the curve with high- and low-albedo asteroids. The phase function (PF) can be applied to asteroids with multiple high-quality observations. If the number of observations is small, or their accuracy is low, problems may arise. The most apparent problem is that the parameter G or the parameters G1, G2 might be poorly estimated. The solution has been to fix to value of G or values of G1, G2 and estimate only the H. In our recent work [4], we offer a solution that can improve the current situation with the photometric fits with a small number of low-accuracy observations. We present a constrained nonlinear least-squares method for fitting the H,G1,G2 function that can improve the possible bias with low-accuracy data. Then, we revisit the two-parameter PF with new data and offer a new version, the H,G12* PF. Finally, we assess the problem with fixed G or G1, G2 parameters by introducing one-parameter models that relate to five taxonomic asteroid groups. We tie all the models together with three or two parameters, or a single parameter, with a statistical model selection procedure to select the best version for a particular data set.We have developed practical tools for the abovementioned algorithms. We apply the tools to a dataset of 8,900 asteroids with almost 500,000 photometric observations from the Palomar Transient Factory survey [5]. We report the effect of the revised H estimates on the geometric albedos in cases where WISE-mission size estimates are available.[1] D

  10. THE BOLOCAM GALACTIC PLANE SURVEY. XI. TEMPERATURES AND SUBSTRUCTURE OF GALACTIC CLUMPS BASED ON 350 μM OBSERVATIONS

    Energy Technology Data Exchange (ETDEWEB)

    Merello, Manuel; Evans II, Neal J. [The University of Texas at Austin, Department of Astronomy, 2515 Speedway, Stop C1400, Austin, TX 78712-1205 (United States); Shirley, Yancy L. [Steward Observatory, University of Arizona, 933 North Cherry Avenue, Tucson, AZ 85721 (United States); Rosolowsky, Erik [Department of Physics, 4-181 CCIS, University of Alberta, Edmonton, AB T6G 2E1 (Canada); Ginsburg, Adam [European Southern Observatory, ESO Headquarters, Karl-Schwarzschild-Strasse 2, D-95748 Garching bei Munchen (Germany); Bally, John [CASA, University of Colorado, 389-UCB, Boulder, CO 80309 (United States); Battersby, Cara; Dunham, Michael M., E-mail: manuel@astro.as.utexas.edu [Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, MS 78, Cambridge, MA 02138 (United States)

    2015-05-15

    We present 107 maps of continuum emission at 350 μm from Galactic molecular clumps. Observed sources were mainly selected from the Bolocam Galactic Plane Survey (BGPS) catalog, with three additional maps covering star-forming regions in the outer Galaxy. The higher resolution of the SHARC-II images (8.″5 beam) compared with the 1.1 mm images from BGPS (33″ beam) allowed us to identify a large population of smaller substructures within the clumps. A catalog is presented for the 1386 sources extracted from the 350 μm maps. The color temperature distribution of clumps based on the two wavelengths has a median of 13.3 K and mean of 16.3 ± 0.4 K, assuming an opacity law index of 1.7. For the structures with good determination of color temperatures, the mean ratio of gas temperature, determined from NH{sub 3} observations, to dust color temperature is 0.88 and the median ratio is 0.76. About half the clumps have more than 2 substructures and 22 clumps have more than 10. The fraction of the mass in dense substructures seen at 350 μm compared to the mass of their parental clump is ∼0.19, and the surface densities of these substructures are, on average, 2.2 times those seen in the clumps identified at 1.1 mm. For a well-characterized sample, 88 structures (31%) exceed a surface density of 0.2 g cm{sup −2}, and 18 (6%) exceed 1.0 g cm{sup −2}, thresholds for massive star formation suggested by theorists.

  11. U.S. Geological Survey (USGS) Earth Resources Observation and Science (EROS) Center-fiscal year 2010 annual report

    Science.gov (United States)

    Nelson, Janice S.

    2011-01-01

    The Earth Resources Observation and Science (EROS) Center is a U.S. Geological Survey (USGS) facility focused on providing science and imagery to better understand our Earth. The work of the Center is shaped by the earth sciences, the missions of our stakeholders, and implemented through strong program and project management, and application of state-of-the-art information technologies. Fundamentally, EROS contributes to the understanding of a changing Earth through 'research to operations' activities that include developing, implementing, and operating remote-sensing-based terrestrial monitoring capabilities needed to address interdisciplinary science and applications objectives at all levels-both nationally and internationally. The Center's programs and projects continually strive to meet, and where possible exceed, the changing needs of the USGS, the Department of the Interior, our Nation, and international constituents. The Center's multidisciplinary staff uses their unique expertise in remote sensing science and technologies to conduct basic and applied research, data acquisition, systems engineering, information access and management, and archive preservation to address the Nation's most critical needs. Of particular note is the role of EROS as the primary provider of Landsat data, the longest comprehensive global land Earth observation record ever collected. This report is intended to provide an overview of the scientific and engineering achievements and illustrate the range and scope of the activities and accomplishments at EROS throughout fiscal year (FY) 2010. Additional information concerning the scientific, engineering, and operational achievements can be obtained from the scientific papers and other documents published by EROS staff or by visiting our web site at http://eros.usgs.gov. We welcome comments and follow-up questions on any aspect of this Annual Report and invite any of our customers or partners to contact us at their convenience. To

  12. Dutch survey of congenital coronary artery fistulas in adults: coronary artery-left ventricular multiple micro-fistulas multi-center observational survey in the Netherlands.

    NARCIS (Netherlands)

    Said, S.A.M.; Werf, T. van der

    2006-01-01

    BACKGROUND: Congenital coronary artery-left ventricular multiple micro-fistulas (CA-LVMMFs) in adults are rare anomalies. They may cause angina pectoris and myocardial infarction in association with normal coronary arteries. METHODS AND RESULTS: From the medical databases of a Dutch Survey of corona

  13. Multilevel and Diverse Classrooms

    Science.gov (United States)

    Baurain, Bradley, Ed.; Ha, Phan Le, Ed.

    2010-01-01

    The benefits and advantages of classroom practices incorporating unity-in-diversity and diversity-in-unity are what "Multilevel and Diverse Classrooms" is all about. Multilevel classrooms--also known as mixed-ability or heterogeneous classrooms--are a fact of life in ESOL programs around the world. These classrooms are often not only multilevel…

  14. The Effects of the Flipped Model of Instruction on Student Engagement and Performance in the Secondary Mathematics Classroom

    Directory of Open Access Journals (Sweden)

    Kevin R. Clark

    2015-01-01

    Full Text Available In many of the secondary classrooms across the country, students are passively engaged in the mathematics content, and academic performance can be described, at best, as mediocre. This research study sought to bring about improvements in student engagement and performance in the secondary mathematics classroom through the implementation of the flipped model of instruction and compared student interaction in the flipped classroom with a traditional format. The flipped model of instruction is a relatively new teaching strategy attempting to improve student engagement and performance by moving the lecture outside the classroom via technology and moving homework and exercises with concepts inside the classroom via learning activities. Changes in the student participants’ perceptions and attitudes were evidenced and evaluated through the completion of a pre- and post-survey, a teacher-created unit test, random interviews, and a focus group session. In addition, the researcher documented observations, experiences, thoughts, and insights regarding the intervention in a journal on a daily basis. Quantitative results and qualitative findings revealed the student participants responded favorably to the flipped model of instruction and experienced an increase in their engagement and communication when compared to the traditional classroom experience. The student participants also recognized improvements in the quality of instruction and use of class of time with the flipped model of instruction. In terms of academic performance, no significant changes were demonstrated between the flipped model of instruction students and those taught in a traditional classroom environment.

  15. Out of Classroom Instruction in the Flipped Classroom

    DEFF Research Database (Denmark)

    Triantafyllou, Evangelia; Timcenko, Olga

    2015-01-01

    This article presents experiences and student perceptions on the introduction of the flipped classroom model in two consecutive semesters at Media Technology department of Aalborg University, Copenhagen, Denmark. We introduced the flipped instruction model to a statistics course and a mathematics...... workshop. We collected data by two online survey studies, which show support for student perceptions that out-of-classroom instruction with online resources enhances learning, by providing visual and in depth explanations, and can engage the learner. However, students stated that they miss just......-in-time explanations when learning with online resources and they questioned the quality and validity of some of them. Based on these findings and our own experience, we discuss requirements for resources and activities in flipped classrooms in order for the student to engage and learn. Finally, we present a framework...

  16. The influence of fidelity of implementation on teacher-student interaction quality in the context of a randomized controlled trial of the Responsive Classroom approach.

    Science.gov (United States)

    Abry, Tashia; Rimm-Kaufman, Sara E; Larsen, Ross A; Brewer, Alexis J

    2013-08-01

    This study examined the direct and indirect effects between training in the Responsive Classroom® (RC) approach, teachers' uptake of RC practices, and teacher-student interaction quality, using a structural equation modeling framework. A total of 24 schools were randomly assigned to experimental or control conditions. Third- and fourth-grade teachers in treatment schools (n=132) received training in the RC approach, whereas teachers in control schools (n=107) continued "business as usual." Observers rated teachers' fidelity of implementation (FOI) of RC practices 5 times throughout the year using the Classroom Practices Observation Measure. In addition, teachers completed self-report measures of FOI, the Classroom Practices Teacher Survey and Classroom Practices Frequency Survey, at the end of the school year. Teacher-student interactions were rated during classroom observations using the Classroom Assessment Scoring System. Controlling for teachers' grade level and teacher-student interaction quality at pretest, RC training was expected to predict posttest teacher-student interaction quality directly and indirectly through FOI. Results supported only a significant indirect effect, β=0.85, p=.002. Specifically, RC teachers had higher levels of FOI of RC practices, β=1.62, pteacher-student interaction quality, β=0.52, p=.001, R2=.32. Discussion highlights factors contributing to variability in FOI and school administrators roles in supporting FOI. Copyright © 2013 Society for the Study of School Psychology. Published by Elsevier Ltd. All rights reserved.

  17. First survey of Wolf-Rayet star populations over the full extension of nearby galaxies observed with CALIFA

    Science.gov (United States)

    Miralles-Caballero, D.; Díaz, A. I.; López-Sánchez, Á. R.; Rosales-Ortega, F. F.; Monreal-Ibero, A.; Pérez-Montero, E.; Kehrig, C.; García-Benito, R.; Sánchez, S. F.; Walcher, C. J.; Galbany, L.; Iglesias-Páramo, J.; Vílchez, J. M.; González Delgado, R. M.; van de Ven, G.; Barrera-Ballesteros, J.; Lyubenova, M.; Meidt, S.; Falcon-Barroso, J.; Mast, D.; Mendoza, M. A.; Califa Collaboration

    2016-08-01

    The search of extragalactic regions with conspicuous presence of Wolf-Rayet (WR) stars outside the Local Group is challenging task owing to the difficulty in detecting their faint spectral features. In this exploratory work, we develop a methodology to perform an automated search of WR signatures through a pixel-by-pixel analysis of integral field spectroscopy (IFS) data belonging to the Calar Alto Legacy Integral Field Area survey, CALIFA. This procedure has been applied to a sample of nearby galaxies spanning a wide range of physical, morphological, and environmental properties. This technique allowed us to build the first catalogue of regions rich in WR stars with spatially resolved information, and enabled us to study the properties of these complexes in a two-dimensional (2D) context. The detection technique is based on the identification of the blue WR bump (around He iiλ4686 Å, mainly associated with nitrogen-rich WR stars; WN) and the red WR bump (around C ivλ5808 Å, mainly associated with carbon-rich WR stars; WC) using a pixel-by-pixel analysis that maximizes the number of independent regions within a given galaxy. We identified 44 WR-rich regions with blue bumps distributed in 25 out of a total of 558 galaxies. The red WR bump was identified only in 5 of those regions. Most of the WR regions are located within one effective radius from the galaxy centre, and around one-third are located within ~1 kpc or less from the centre. We found that the majority of the galaxies hosting WR populations in our sample are involved in some kind of interaction process. Half of the host galaxies share some properties with gamma-ray burst (GRB) hosts where WR stars, such as potential candidates to the progenitors of GRBs, are found. We also compared the WR properties derived from the CALIFA data with stellar population synthesis models, and confirm that simple star models are generally not able to reproduce the observations. We conclude that other effects, such as

  18. Reaching the Millennial Generation in the Classroom

    Science.gov (United States)

    Kotz, Paul E.

    2016-01-01

    The millennial generation (Generation Y) is the age group of children born between 1982 and 2002. Students aged 15 to 16 were asked to answer questions regarding their classroom experience. Sixty eight students were asked to participate in the survey and 63 gave consent for their participation. A qualitative survey approach was used asking three…

  19. CANDELS: The Cosmic Assembly Near-infrared Deep Extragalactic Legacy Survey - The Hubble Space Telescope Observations, Imaging Data Products and Mosaics

    CERN Document Server

    Koekemoer, Anton M; Ferguson, Henry C; Grogin, Norman A; Kocevski, Dale D; Koo, David C; Lai, Kamson; Lotz, Jennifer M; Lucas, Ray A; McGrath, Elizabeth J; Ogaz, Sara; Rajan, Abhijith; Riess, Adam G; Rodney, Steve A; Strolger, Louis; Casertano, Stefano; Dahlen, Tomas; Dickinson, Mark; Dolch, Timothy; Fontana, Adriano; Giavalisco, Mauro; Grazian, Andrea; Guo, Yicheng; Hathi, Nimish P; Huang, Kuang-Han; van der Wel, Arjen; Yan, Hao-Jing; Acquaviva, Viviana; Almaini, David M Alexander Omar; Ashby, Matthew L N; Barden, Marco; Bell, Eric F; Bournaud, Frédéric; Brown, Thomas M; Caputi, Karina I; Cassata, Paolo; Challis, Peter; Chary, Ranga-Ram; Cheung, Edmond; Cirasuolo, Michele; Conselice, Christopher J; Cooray, Asantha Roshan; Croton, Darren J; Daddi, Emanuele; Davé, Romeel; de Mello, Duilia F; de Ravel, Loic; Dekel, Avishai; Donley, Jennifer L; Dunlop, James S; Dutton, Aaron A; Elbaz, David; Fazio, Giovanni G; Filippenko, Alex V; Finkelstein, Steven L; Frazer, Chris; Gardner, Jonathan P; Garnavich, Peter M; Gawiser, Eric; Gruetzbauch, Ruth; Hartley, Will G; Häussler, Boris; Herrington, Jessica; Hopkins, Philip F; Huang, Jia-Sheng; Jha, Saurabh; Johnson, Andrew; Kartaltepe, Jeyhan S; Khostovan, Ali Ahmad; Kirshner, Robert P; Lani, Caterina; Lee, Kyoung-Soo; Li, Weidong; Madau, Piero; McCarthy, Patrick J; McIntosh, Daniel H; McLure, Ross J; McPartland, Conor; Mobasher, Bahram; Moreira, Heidi; Mortlock, Alice; Moustakas, Leonidas A; Mozena, Mark; Nandra, Kirpal; Newman, Jeffrey A; Nielsen, Jennifer L; Niemi, Sami; Noeske, Kai G; Papovich, Casey J; Pentericci, Laura; Pope, Alexandra; Primack, Joel R; Ravindranath, Swara; Reddy, Naveen A; Renzini, Alvio; Rix, Hans-Walter; Robaina, Aday R; Rosario, David J; Rosati, Piero; Salimbeni, Sara; Scarlata, Claudia; Siana, Brian; Simard, Luc; Smidt, Joseph; Snyder, Diana; Somerville, Rachel S; Spinrad, Hyron; Straughn, Amber N; Telford, Olivia; Teplitz, Harry I; Trump, Jonathan R; Vargas, Carlos; Villforth, Carolin; Wagner, Cory R; Wandro, Pat; Wechsler, Risa H; Weiner, Benjamin J; Wiklind, Tommy; Wild, Vivienne; Wilson, Grant; Wuyts, Stijn; Yun, Min S

    2011-01-01

    This paper describes the Hubble Space Telescope imaging data products and data reduction procedures for the Cosmic Assembly Near-IR Deep Extragalactic Legacy Survey (CANDELS). This survey is designed to document the evolution of galaxies and black holes at $z\\sim1.5-8$, and to study Type Ia SNe beyond $z>1.5$. Five premier multi-wavelength sky regions are selected, each with extensive multiwavelength observations. The primary CANDELS data consist of imaging obtained in the Wide Field Camera 3 / infrared channel (WFC3/IR) and UVIS channel, along with the Advanced Camera for Surveys (ACS). The CANDELS/Deep survey covers \\sim125 square arcminutes within GOODS-N and GOODS-S, while the remainder consists of the CANDELS/Wide survey, achieving a total of \\sim800 square arcminutes across GOODS and three additional fields (EGS, COSMOS, and UDS). We summarize the observational aspects of the survey as motivated by the scientific goals and present a detailed description of the data reduction procedures and products from...

  20. Direct Observation of Cosmic Strings Via Their Strong Gravitational Lensing Effect. 1. Predictions for High Resolution Imaging Surveys

    Energy Technology Data Exchange (ETDEWEB)

    Gasparini, Maria Alice; Marshall, Phil; Treu, Tommaso; /UC, Santa Barbara; Morganson, Eric; /KIPAC, Menlo Park; Dubath, Florian; /Santa Barbara, KITP

    2007-11-14

    We use current theoretical estimates for the density of long cosmic strings to predict the number of strong gravitational lensing events in astronomical imaging surveys as a function of angular resolution and survey area. We show that angular resolution is the single most important factor, and that interesting limits on the dimensionless string tension G{mu}/c{sup 2} can be obtained by existing and planned surveys. At the resolution of the Hubble Space Telescope (0'.14), it is sufficient to survey of order a square degree -- well within reach of the current HST archive -- to probe the regime G{mu}/c{sup 2} {approx} 10{sup -8}. If lensing by cosmic strings is not detected, such a survey would improve the limit on the string tension by an order of magnitude on that available from the cosmic microwave background. At the resolution (0'.028) attainable with the next generation of large ground based instruments, both in the radio and the infra-red with adaptive optics, surveying a sky area of order ten square degrees will allow us to probe the G{mu}/c{sup 2} {approx} 10{sup -9} regime. These limits will not be improved significantly by increasing the solid angle of the survey.

  1. Informing policy on open water drowning prevention: an observational survey of life jacket use in Washington State.

    Science.gov (United States)

    Chung, Celeste; Quan, Linda; Bennett, Elizabeth; Kernic, Mary A; Ebel, Beth E

    2014-08-01

    To assess life jacket use among Washington State boaters and to examine the relationship between life jacket use and boating laws. A statewide observational survey of boaters was conducted between August 2010 and September 2010. Data collection included age, sex, life jacket use, boat type, and weather and water conditions. Among 5157 boaters, 30.7% wore life jackets. Life jacket use was highest among groups required by state law: personal watercraft users (96.8%), people being towed (eg, water-skiers) (95.3%) and children 0-12 years old (81.7%). Children and youth were more likely to use a life jacket if any adult in the boat wore a life jacket: 100% versus 87.2% for 0-5 years, 92.8% versus 76.7% for 6-12 years and 81.4% versus 36.1% for 13-17 years. Adult role modelling was particularly beneficial for adolescents aged 13-17 years, who were not covered by a life jacket law. In multivariable analysis, the presence of at least one adult wearing a life jacket was associated with a 20-fold increased likelihood that adolescents were also wearing a life jacket. Highest life jacket use was strongly associated with laws requiring use and with adult role modelling. Legislation requiring life jackets for ages 13-17 years and social marketing encouraging adult life jacket wear in the company of children and youth are promising strategies to increase life jacket use in Washington State. Published by the BMJ Publishing Group Limited. For permission to use (where not already granted under a licence) please go to http://group.bmj.com/group/rights-licensing/permissions.

  2. The JCMT Gould Belt Survey: the effect of molecular contamination in SCUBA-2 observations of Orion A

    Science.gov (United States)

    Coudé, S.; Bastien, P.; Kirk, H.; Johnstone, D.; Drabek-Maunder, E.; Graves, S.; Hatchell, J.; Chapin, E. L.; Gibb, A. G.; Matthews, B.; JCMT Gould Belt Survey Team

    2016-04-01

    Thermal emission from cold dust grains in giant molecular clouds can be used to probe the physical properties, such as density, temperature and emissivity in star-forming regions. We present the Submillimetre Common-User Bolometer Array (SCUBA-2) shared-risk observations at 450 and 850 μm of the Orion A molecular cloud complex taken at the James Clerk Maxwell Telescope (JCMT). Previous studies showed that molecular emission lines can contribute significantly to the measured fluxes in those continuum bands. We use the Heterodyne Array Receiver Programme 12CO J = 3-2 integrated intensity map for Orion A in order to evaluate the molecular line contamination and its effects on the SCUBA-2 maps. With the corrected fluxes, we have obtained a new spectral index α map for the thermal emission of dust in the well-known integral-shaped filament. Furthermore, we compare a sample of 33 sources, selected over the Orion A molecular cloud complex for their high 12CO J = 3-2 line contamination, to 27 previously identified clumps in OMC 4. This allows us to quantify the effect of line contamination on the ratio of 850-450 μm flux densities and how it modifies the deduced spectral index of emissivity β for the dust grains. We also show that at least one Spitzer-identified protostellar core in OMC 5 has a 12CO J = 3-2 contamination level of 16 per cent. Furthermore, we find the strongest contamination level (44 per cent) towards a young star with disc near OMC 2. This work is part of the JCMT Gould Belt Legacy Survey.

  3. The JCMT Gould Belt Survey: A First Look at SCUBA-2 Observations of the Lupus I Molecular Cloud

    Science.gov (United States)

    Mowat, C.; Hatchell, J.; Rumble, D.; Kirk, H.; Buckle, J.; Berry, D. S.; Broekhoven-Fiene, H.; Currie, M. J.; Jenness, T.; Johnstone, D.; Mottram, J. C.; Pattle, K.; Tisi, S.; Francesco, J. Di; Hogerheijde, M. R.; Ward-Thompson, D.; Bastien, P.; Bresnahan, D.; Butner, H.; Chen, M.; Chrysostomou, A.; Coudé, S.; Davis, C. J.; Drabek-Maunder, E.; Duarte-Cabral, A.; Fich, M.; Fiege, J.; Friberg, P.; Friesen, R.; Fuller, G. A.; Graves, S.; Greaves, J.; Holland, W.; Joncas, G.; Kirk, J. M.; Knee, L. B. G.; Mairs, S.; Marsh, K.; Matthews, B. C.; Moriarty-Schieven, G.; Rawlings, J.; Retter, B.; Richer, J.; Robertson, D.; Rosolowsky, E.; Sadavoy, S.; Thomas, H.; Tothill, N.; Viti, S.; White, G. J.; Wouterloot, J.; Yates, J.; Zhu, M.

    2017-01-01

    This paper presents observations of the Lupus I molecular cloud at 450 and 850 µm with SCUBA-2 as part of the James Clerk Maxwell Telescope Gould Belt Survey (JCMT GBS). Nine compact sources, assumed to be the disks of young stellar objects (YSOs), twelve extended protostellar, pre-stellar and starless cores, and one isolated, low luminosity protostar, are detected in the region. Spectral Energy Distributions (SEDs), including submillimetre fluxes, are produced for 15 YSOs, and each is fitted with the models of Robitaille et al. (2006). The proportion of Class 0 / I protostars is higher than that seen in other Gould Belt regions such as Ophiuchus and Serpens. Circumstellar disk masses are calculated for more evolved sources, while protostellar envelope masses are calculated for protostars. Up to four Very Low Luminosity Objects are found, a large fraction when compared to other Spitzer c2d regions. One YSO has a disk mass greater than the minimum mass solar nebula (MMSN). Twelve starless / protostellar cores are detected by SCUBA-2, and their masses are calculated. The stability of these cores is examined using both the thermal Jeans mass and a turbulent virial mass when possible. Two cores in Lupus I are super-Jeans and contain no known YSOs. One of these cores has a virial parameter of 1.1 ± 0.4, and could therefore be prestellar. The high ratio of Class 0 / I to Class III YSOs (1:1), and the presence of a prestellar core candidate, provides support for the hypothesis that a shock recently triggered star formation in Lupus I.

  4. The JCMT Gould Belt Survey: A First Look at SCUBA-2 Observations of the Lupus I Molecular Cloud

    Science.gov (United States)

    Mowat, C.; Hatchell, J.; Rumble, D.; Kirk, H.; Buckle, J.; Berry, D. S.; Broekhoven-Fiene, H.; Currie, M. J.; Jenness, T.; Johnstone, D.; Mottram, J. C.; Pattle, K.; Tisi, S.; Di Francesco, J.; Hogerheijde, M. R.; Ward-Thompson, D.; Bastien, P.; Bresnahan, D.; Butner, H.; Chen, M.; Chrysostomou, A.; Coudé, S.; Davis, C. J.; Drabek-Maunder, E.; Duarte-Cabral, A.; Fich, M.; Fiege, J.; Friberg, P.; Friesen, R.; Fuller, G. A.; Graves, S.; Greaves, J.; Holland, W.; Joncas, G.; Kirk, J. M.; Knee, L. B. G.; Mairs, S.; Marsh, K.; Matthews, B. C.; Moriarty-Schieven, G.; Rawlings, J.; Retter, B.; Richer, J.; Robertson, D.; Rosolowsky, E.; Sadavoy, S.; Thomas, H.; Tothill, N.; Viti, S.; White, G. J.; Wouterloot, J.; Yates, J.; Zhu, M.

    2017-05-01

    This paper presents observations of the Lupus I molecular cloud at 450 and 850 μm with Submillimetre Common User Bolometer Array (SCUBA-2) as part of the James Clerk Maxwell Telescope Gould Belt Survey (JCMT GBS). Nine compact sources, assumed to be the discs of young stellar objects (YSOs), 12 extended protostellar, pre-stellar and starless cores, and one isolated, low-luminosity protostar, are detected in the region. Spectral energy distributions, including submillimetre fluxes, are produced for 15 YSOs, and each is fitted with the models of Robitaille et al. The proportion of Class 0/I protostars is higher than that seen in other Gould Belt regions such as Ophiuchus and Serpens. Circumstellar disc masses are calculated for more evolved sources, while protostellar envelope masses are calculated for protostars. Up to four very low luminosity objects are found; a large fraction when compared to other Spitzer c2d regions. One YSO has a disc mass greater than the minimum mass solar nebula. 12 starless/protostellar cores are detected by SCUBA-2 and their masses are calculated. The stability of these cores is examined using both the thermal Jeans mass and a turbulent virial mass when possible. Two cores in Lupus I are super-Jeans and contain no known YSOs. One of these cores has a virial parameter of 1.1 ± 0.4, and could therefore be pre-stellar. The high ratio of Class 0/I to Class III YSOs (1:1), and the presence of a pre-stellar core candidate, provides support for the hypothesis that a shock recently triggered star formation in Lupus I.

  5. A cross sectional, observational survey to assess levels and predictors of psychological wellbeing in adults with epidermolysis bullosa

    Directory of Open Access Journals (Sweden)

    Emma Dures

    2013-01-01

    Full Text Available Epidermolysis bullosa (EB describes a cluster of genetically determined skin disorders. Symptoms can be painful, disabling and disfiguring, yet there is little research on the psychological impact of the disease. The study aim was to measure psychological wellbeing in adults with EB; and to examine the association between psychological wellbeing and self efficacy, health locus of control and adjustment to appearance in an observational, cross sectional survey. Questionnaire packs comprising the General Health Questionnaire (GHQ-12, the General Self Efficacy Scale (GSE, the Multidimensional Health Locus of Control Scale (MHLOC, and the Derriford Appearance Scale (DAS-24, were sent to approximately 385 adults with EB. The data were analysed using SPSS. Eighty-seven participants responded. Scores on the GHQ-12 showed non-problematic psychological health in 36% of the sample; levels bordering on clinical disorder in 32.1% and severe psychological distress in 31.9%. No correlations were found between demographic factors (age and sex or clinical factors (EB type and perceived severity and psychological well-being. Scores on the GSE, the internal locus of control sub-scale of the MHLOC and the DAS-24 showed them to be statistically significant correlates of psychological wellbeing (P<0.001; P<0.018; and P<0.001 respectively. In a regression analysis, adjustment to appearance and self efficacy accounted for 24% of the variation in psychological wellbeing. Adults with EB might be at risk of experiencing poor psychological health. Interventions designed to enhance disease self management, self efficacy and improve body image are likely to be beneficial in this clinical group.

  6. SweetSpot: A 3-year NOAO Survey to Observe 150 Type Ia Supernovae in the Near Infrared in the Nearby Hubble Flow

    Science.gov (United States)

    Wood-Vasey, W. M.; Weyant, A.; Allen, L.; Garnavich, P. M.; Jahan, N.; Jha, S.; Joyce, R. R.; Matheson, T.; Rest, A.

    2014-01-01

    SweetSpot is an NOAO Survey program from 2012B-2015A that will observe 150 Type Ia supernovae (SNe Ia) in the Hubble flow to obtain reliable near-infrared (NIR) luminosities free from peculiar-velocity confusion and the uncertainties of dust. A key part of the program is a focus on accurate calibration incorporating recently demonstrated techniques for characterization of telescope systems and the Earth's atmosphere. Our full SweetSpot program will (1) extend the NIR Hubble diagram past currently available samples; (2) quantitatively demonstrate the degree to which SNe Ia are robust standard candles in the NIR; (3) provide key insights about the color evolution and intrinsic properties of SNe Ia and their host galaxies; and (4) establish a well-calibrated low-redshift anchor for future NIR supernova surveys from JWST, Euclid, and WFIRST/NEW. By the end of the survey we will have measured the relative distance to a redshift of 0.05 to 1%. Nearby Type Ia supernova (SN Ia) observations such as these will test the standard nature of SNe Ia in the rest-frame NIR, allow insight into the nature of dust, and provide a critical anchor for future cosmological SN Ia surveys at higher redshift. We will present the results from our pilot survey in 2011B and discuss our first year of full observations from 2012B-2013A.

  7. The influence of a Classroom Model of Scientific Scholarship on Four Girls' Trajectories of Identification with Science

    Science.gov (United States)

    Cook, Melissa Sunshine

    This study examines the teacher's role in shaping the identity construction resources available in a classroom and the ways in which individual students take up, modify, and appropriate those resources to construct themselves as scientists through interaction with their teacher and peers. Drawing on frameworks of identity construction and social positioning, I propose that the locally-negotiated classroom-level cultural model of what it means to be a "good" science student forms the arena in which students construct a sense of their own competence at, affiliation with, and interest in science. The setting for this study was a 6th grade science class at a progressive urban elementary school whose population roughly represents the ethnic and socioeconomic diversity of the state of California. The teacher was an experienced science and math teacher interested in social justice and inquiry teaching. Drawing from naturalistic observations, video and artifact analysis, survey data, and repeated interviews with students and the teacher, I demonstrated what it meant to be a "good" science student in this particular cultural community by analyzing what was required, reinforced, and rewarded in this classroom. Next, I traced the influence of this particular classroom's conception of what it meant to be good at science on the trajectories of identification with science of four 6th grade girls selected to represent a variety of stances towards science, levels of classroom participation, and personal backgrounds. Scientific scholarship in this class had two parts: values related to science as a discipline, and a more generic set of school-related values one might see in any classroom. Different meanings of and values for science were indexed in the everyday activities of the classroom: science as a language for describing the natural world, science as a set of rhetorical values, science as an adult social community, and science as a place for mess and explosions. Among school

  8. The VIPERS Multi-Lambda Survey. I. UV and near-IR observations, multi-colour catalogues, and photometric redshifts

    Science.gov (United States)

    Moutard, T.; Arnouts, S.; Ilbert, O.; Coupon, J.; Hudelot, P.; Vibert, D.; Comte, V.; Conseil, S.; Davidzon, I.; Guzzo, L.; Llebaria, A.; Martin, C.; McCracken, H. J.; Milliard, B.; Morrison, G.; Schiminovich, D.; Treyer, M.; Van Werbaeke, L.

    2016-05-01

    We present observations collected in the CFHTLS-VIPERS region in the ultraviolet with the GALEX satellite (far- and near-ultraviolet channels) and in the near-infrared with the CFHT/WIRCam camera (Ks band) over an area of 22 and 27 deg2, respectively. The depth of the photometry was optimised to measure the physical properties (e.g., star formation rate, stellar masses) of all the galaxies in the VIPERS spectroscopic survey. The large volume explored by VIPERS will enable a unique investigation of the relationship between the galaxy properties and their environment (density field and cosmic web) at high redshift (0.5 ≤ z ≤ 1.2). In this paper, we present the observations, the data reductions, and the build-up of the multi-colour catalogues. The CFHTLS-T0007 (gri-χ2) images are used as reference to detect and measure the Ks-band photometry, while the T0007 u∗-selected sources are used as priors to perform the GALEX photometry based on a dedicated software (EMphot). Our final sample reaches NUVAB ~ 25 (at 5σ) and KAB ~ 22 (at 3σ). The large spectroscopic sample (~51 000 spectroscopic redshifts) allows us to highlight the robustness of our star/galaxy separation and the reliability of our photometric redshifts with a typical accuracy of σz ≤ 0.04 and a fraction of catastrophic failures η ≤ 2% down to i ~ 23. We present various tests on the Ks-band completeness and photometric redshift accuracy by comparing our results with existing overlapping deep photometric catalogues. Finally, we discuss the BzK sample of passive and active galaxies at high redshift and the evolution of galaxy morphology in the (NUV-r) vs. (r-Ks) diagram at low redshift (z ≤ 0.25) based on the high image quality of the CFHTLS. The catalogue is available at the CDS via anonymous ftp to http://cdsarc.u-strasbg.fr (http://130.79.128.5) or via http://cdsarc.u-strasbg.fr/viz-bin/qcat?J/A+A/590/A102The images, catalogues, and photometric redshifts for 1.5 million sources (down to NUV

  9. U.S. Geological Survey (USGS) Earth Resources Observation and Science (EROS) Center-Fiscal Year 2009 Annual Report

    Science.gov (United States)

    Nelson, Janice S.

    2010-01-01

    The Earth Resources Observation and Science (EROS) Center is a U.S. Geological Survey (USGS) facility focused on providing science and imagery to better understand our Earth. As part of the USGS Geography Discipline, EROS contributes to the Land Remote Sensing (LRS) Program, the Geographic Analysis and Monitoring (GAM) Program, and the National Geospatial Program (NGP), as well as our Federal partners and cooperators. The work of the Center is shaped by the Earth sciences, the missions of our stakeholders, and implemented through strong program and project management and application of state-of-the-art information technologies. Fundamentally, EROS contributes to the understanding of a changing Earth through 'research to operations' activities that include developing, implementing, and operating remote sensing based terrestrial monitoring capabilities needed to address interdisciplinary science and applications objectives at all levels-both nationally and internationally. The Center's programs and projects continually strive to meet and/or exceed the changing needs of the USGS, the Department of the Interior, our Nation, and international constituents. The Center's multidisciplinary staff uses their unique expertise in remote sensing science and technologies to conduct basic and applied research, data acquisition, systems engineering, information access and management, and archive preservation to address the Nation's most critical needs. Of particular note is the role of EROS as the primary provider of Landsat data, the longest comprehensive global land Earth observation record ever collected. This report is intended to provide an overview of the scientific and engineering achievements and illustrate the range and scope of the activities and accomplishments at EROS throughout fiscal year (FY) 2009. Additional information concerning the scientific, engineering, and operational achievements can be obtained from the scientific papers and other documents published by

  10. The influence of classroom aggression and classroom climate on aggressive-disruptive behavior.

    Science.gov (United States)

    Thomas, Duane E; Bierman, Karen L; Powers, C J

    2011-01-01

    Research suggests that early classroom experiences influence the socialization of aggression. Tracking changes in the aggressive behavior of 4,179 children from kindergarten to second-grade (ages 5-8), this study examined the impact of 2 important features of the classroom context--aggregate peer aggression and climates characterized by supportive teacher-student interactions. The aggregate aggression scores of children assigned to first-grade classrooms predicted the level of classroom aggression (assessed by teacher ratings) and quality of classroom climate (assessed by observers) that emerged by the end of Grade 1. Hierarchical linear model analyses revealed that first-grade classroom aggression and quality of classroom climate made independent contributions to changes in student aggression, as students moved from kindergarten to second grade. Implications for policy and practice are discussed.

  11. Streaming Seismograms into Earth-Science Classrooms

    Science.gov (United States)

    Ammon, C. J.

    2011-12-01

    Seismograms are the fundamental observations upon which seismology is based; they are central to any course in seismology and important for any discussion of earthquake-related phenomena based on seismic observations. Advances in the collection and distribution of seismic data have made the use of research-quality seismograms in any network capable classroom feasible. The development of large, deep seismogram archives place an unprecedented quantity of high-quality data within reach of the modern classroom environment. I describe and discuss several computer tools and classroom activities that I use in introductory (general education) and advanced undergraduate courses that present near real-time research-quality seismic observations in the classroom. The Earth Motion Monitor Application (EMMA), is a MacOS application that presents a visually clear seismogram display that can be projected in classrooms with internet access. Seismic signals from thousands of station are available from the IRIS data center and the bandwidth can be tailored to the particular type of signal of interest (large event, low frequencies; small event, high frequencies). In introductory classes for non-science students, the near realtime display routinely shows magnitude 4.0-5.0 earthquake-generated signals, demonstrating to students the frequency of earthquake occurrence. Over the next few minutes as the waves travel through and across the planet, their arrival on the seismogram display provides some basic data for a qualitative estimate of the event's general location. When a major or great earthquake occurs, a broad-band display of signals from nearby stations can dramatically and dynamically illuminate the frequent activity associated with the aftershock sequence. Routine use of the display (while continuing the traditional classroom activities) provides students with a significant dose of seismogram study. Students generally find all the signals, including variations in seismic

  12. Teacher and Student Perceptions on High School Science Flipped Classrooms: Educational Breakthrough or Media Hype?

    Science.gov (United States)

    Hunley, Rebecca C.

    For years educators have struggled to ensure students meet the rigors of state mandated tests. Challenges that often impede student success are student absences, school closings due to weather, and remediation for students who need additional help while advanced students can move ahead. Many educators, especially secondary math and science teachers, have responded to these issues by implementing a teaching strategy called the flipped classroom where students view lectures, power points, or podcasts outside of school and class time shifts to allow opportunities for collaborative learning. The purpose of this research was to evaluate teacher and student perceptions of high school flipped science classrooms. A qualitative phenomenological study was conducted to observe 3 high school science teachers from Georgia, North Carolina, and Tennessee selected through purposeful sampling who have used the flipped classroom method for a minimum of 2 years. Analysis of data from an online survey, direct observation, teacher interviews, and student focus groups helped to identify challenges and benefits of this teaching and learning strategy. Findings indicated that teachers find the flipped classroom beneficial to build student relationships but requires a significant amount of time to develop. Mixed student reactions revealed benefits of a flipped classroom as a successful learning tool for current and future endeavors for college or career preparation.

  13. The Moving Group Targets of the SEEDS High-contrast Imaging Survey of Exoplanets and Disks: Results and Observations from the First Three Years

    NARCIS (Netherlands)

    Brandt, T.D.; et al., [Unknown; Thalmann, C.

    2014-01-01

    We present results from the first three years of observations of moving group (MG) targets in the Strategic Exploration of Exoplanets and Disks with Subaru (SEEDS) high-contrast imaging survey of exoplanets and disks using the Subaru telescope. We achieve typical contrasts of ~105 at 1'' and ~106

  14. Herschel Observations of Extra-Ordinary Sources (hexos) : Analysis of the Hifi 1.2 Thz Wide Spectral Survey Toward Orion KL

    NARCIS (Netherlands)

    Crockett, N. R.; Bergin, E. A.; Wang, S.; Blake, G.; Emprechtinger, M.; Lis, D.; Gupta, H.; Pearson, J.; Yu, S.; Bell, T.; Cernicharo, J.; Lord, S.; Plume, R.; Schilke, P.; van der Tak, F.

    2011-01-01

    We present a full spectral survey of the Kleiman-Low nebula within the Orion Molecular Cloud (Orion KL), one of the most chemically rich regions in the galaxy, using the HIFI instrument on board the Herschel Space Observatory. These observations span a frequency range of 490 -- 1240 GHz and 1430 --

  15. Herschel Observations of EXtra-Ordinary Sources (HEXOS): Analysis of the HIFI 1.2 THz Wide Spectral Survey Toward Orion KL

    NARCIS (Netherlands)

    Crockett, N. R.; Bergin, E. A.; Bell, T. A.; Blake, G.; Cernicharo, J.; Emprechtinger, M.; Gupta, H.; Lord, S.; Pearson, J.; Plume, R.; Schilke, P.; van der Tak, F.; Wang, S.; Yu, S.

    2011-01-01

    We present a full spectral survey of the Kleiman-Low nebula within the Orion Molecular Cloud (Orion KL), one of the most chemically rich regions in the galaxy, using the HIFI instrument on board the Herschel Space Observatory. These observations, shown in the figure below, span a frequency range of

  16. Herschel Observations of Extra-Ordinary Sources (hexos): Analysis of the Hifi 1.2 Thz Wide Spectral Survey Toward Orion KL

    NARCIS (Netherlands)

    Crockett, N. R.; Bergin, E. A.; Wang, S.; Blake, G.; Emprechtinger, M.; Lis, D.; Gupta, H.; Pearson, J.; Yu, S.; Bell, T.; Cernicharo, J.; Lord, S.; Plume, R.; Schilke, P.; van der Tak, F.

    2011-01-01

    We present a full spectral survey of the Kleiman-Low nebula within the Orion Molecular Cloud (Orion KL), one of the most chemically rich regions in the galaxy, using the HIFI instrument on board the Herschel Space Observatory. These observations span a frequency range of 490 -- 1240 GHz and 1430 --

  17. The Moving Group Targets of the SEEDS High-contrast Imaging Survey of Exoplanets and Disks: Results and Observations from the First Three Years

    NARCIS (Netherlands)

    Brandt, T.D.; et al., [Unknown; Thalmann, C.

    2014-01-01

    We present results from the first three years of observations of moving group (MG) targets in the Strategic Exploration of Exoplanets and Disks with Subaru (SEEDS) high-contrast imaging survey of exoplanets and disks using the Subaru telescope. We achieve typical contrasts of ~105 at 1'' and ~106 be

  18. THOR - The HI, OH, Recombination Line Survey of the Milky Way - HI observations of the giant molecular cloud W43

    Science.gov (United States)

    Bihr, Simon; Beuther, Henrik; Johnston, Katharine; Henning, Thomas; Ott, Juergen; Brunthaler, Andreas; THOR Collaboration

    2015-08-01

    To study the atomic, molecular and ionised emission of Giant Molecular Clouds (GMCs) in the Milky Way, we have initiated a Large Program with the VLA: 'THOR - The HI, OH, Recombination Line survey of the Milky Way'. We map the 21cm HI line, 4 OH lines, 19 Hα recombination lines and the continuum from 1-2GHz of a significant fraction of the Milky Way (l=15-67°, |b|thin with properties such as the column density calculated under this assumption. While this approach gives reasonable results for regions of low-mass star-formation, it is not sufficient to describe the atomic gas in close proximity to GMCs. In my talk, I will present a method using strong continuum sources to measure the optical depth, and thus correct the HI 21cm emission for optical depth effects and weak diffuse continuum emission. Our analysis puts a lower limit of M~6.6x106 Msun on the HI mass associated with the W43 GMC, which is a factor of 2.4 larger than the mass obtained using the optically thin assumption. The HI column densities reach NHI~150 Msun pc-2 ~ 1.9x1022 cm-2, which is an order of magnitude higher than seen in low mass star formation regions. This result challenges theoretical models that predict a threshold for the HI column density of ~10 Msun pc-2, at which the formation of molecular hydrogen should set in. Furthermore, we assume an elliptical layered structure for W43 to estimate the particle density profile. The HI particle density shows a linear decrease toward the centre of W43 and the molecular hydrogen, traced via dust observations with Herschel, shows an exponential increase toward the centre. While at the cloud edge atomic and molecular hydrogen are well mixed, the centre of the cloud is dominated by H2. We do not identify a sharp transition between hydrogen in atomic and molecular form. Our results are an important characterization of the atomic to molecular hydrogen transition in an extreme environment that challenges current theoretical models.

  19. Teaching Practices and Elementary Classroom Peer Ecologies

    Science.gov (United States)

    Gest, Scott D.; Rodkin, Philip C.

    2011-01-01

    Teachers and students in 39 1st, 3rd and 5th grade classrooms participated in a study of teaching practices and classroom peer networks. Teachers reported on their attitudes towards aggression and withdrawal, provided rationales for their seating arrangements, and were observed on patterns of emotional and instructional support and classroom…

  20. Effective Management in Junior High Mathematics Classrooms.

    Science.gov (United States)

    Emmer, Edmund T.

    Reporting on part of the data collected in the Junior High Classroom Organization Study, this document focuses on the mathematics subsample. Twenty-six mathematics teachers in 11 junior high schools were observed in two classes. The major purpose of this paper is to describe the classroom procedures and behaviors of teachers identified as…

  1. Continuous Classroom Assessment at Primary Level

    Science.gov (United States)

    Ali, Imtiaz; Shah, Syed Manzoor Hussein; Gujjar, Aijaz Ahmed

    2014-01-01

    This study was designed to analyze the continuous classroom assessment at primary level in Pakistan. Findings of the study revealed that the students' achievement of single class teacher in the subject of English, General science, Urdu and mathematics were almost on average and rubric observation during continuous classroom assessment ranked…

  2. Second Language Writing in the Mainstream Classroom.

    Science.gov (United States)

    Turner, Lyn

    The case study of a Bulgarian immigrant child's literacy education in English as a Second Language (ESL) is presented. Focus is on the boy's literacy development within the context of a mainstream kindergarten/first grade classroom in Australia. The report details the teacher's observations in the classroom and particularly in the child's writing…

  3. Exclusively Visual Analysis of Classroom Group Interactions

    Science.gov (United States)

    Tucker, Laura; Scherr, Rachel E.; Zickler, Todd; Mazur, Eric

    2016-01-01

    Large-scale audiovisual data that measure group learning are time consuming to collect and analyze. As an initial step towards scaling qualitative classroom observation, we qualitatively coded classroom video using an established coding scheme with and without its audio cues. We find that interrater reliability is as high when using visual data…

  4. Classroom acoustics: Three pilot studies

    Science.gov (United States)

    Smaldino, Joseph J.

    2005-04-01

    This paper summarizes three related pilot projects designed to focus on the possible effects of classroom acoustics on fine auditory discrimination as it relates to language acquisition, especially English as a second language. The first study investigated the influence of improving the signal-to-noise ratio on the differentiation of English phonemes. The results showed better differentiation with better signal-to-noise ratio. The second studied speech perception in noise by young adults for whom English was a second language. The outcome indicated that the second language learners required a better signal-to-noise ratio to perform equally to the native language participants. The last study surveyed the acoustic conditions of preschool and day care classrooms, wherein first and second language learning occurs. The survey suggested an unfavorable acoustic environment for language learning.

  5. Effective Factors in Interactions within Japanese EFL Classrooms

    Science.gov (United States)

    Maftoon, Parviz; Ziafar, Meisam

    2013-01-01

    Classroom interactional patterns depend on some contextual, cultural and local factors in addition to the methodologies employed in the classroom. In order to delineate such factors, the focus of classroom interaction research needs to shift from the observables to the unobservables like teachers' and learners' psychological states and cultural…

  6. Observations of the Earth's magnetic field from the shuttle: Using the Spartan carrier as a magnetic survey tool

    Science.gov (United States)

    Webster, W. J., Jr.

    1986-01-01

    The shuttle-deployed and recovered Spartan shows promise as an inexpensive and simple support module for potential field measurements. The results of a preliminary engineering study on the applications of the Spartan carrier to magnetic measurements shows: (1) Extension of the mission duration to as long as 7 days is feasible but requires more reconfiguration of the internal systems; (2) On-board recording of Global Positioning System signals will provide position determination with an accuracy consistent with the most severe requirements; and (3) Making Spartan a magnetically clean spacecraft is straight forward but requires labor-intensive modifications to both the data and power systems. As a magnetic survey tool, Spartan would allow surveys at regularly spaced intervals and could make quick-reaction surveys at times of instability in the secular variation.

  7. A High Galactic Latitude HI 21 cm-line Absorption Survey using the GMRT: I. Observations and Spectra

    Indian Academy of Sciences (India)

    Rekhesh Mohan; K. S. Dwarakanath; G. Srinivasan

    2004-09-01

    We have used the Giant Meterwave Radio Telescope (GMRT) to measure the Galactic HI 21-cm line absorption towards 102 extragalactic radio continuum sources, located at high (|| > 15°) Galactic latitudes. The Declination coverage of the present survey is ≳ -45°. With a mean rms optical depth of ∼ 0.003, this is the most sensitive Galactic HI 21-cm line absorption survey to date. To supplement the absorption data, we have extracted the HI 21-cm line emission profiles towards these 102 lines of sight from the Leiden Dwingeloo Survey of Galactic neutral hydrogen. We have carried out a Gaussian fitting analysis to identify the discrete absorption and emission components in these profiles. In this paper, we present the spectra and the components. A subsequent paper will discuss the interpretation of these results.

  8. SN 2006oz: rise of a super-luminous supernova observed by the SDSS-II SN Survey

    DEFF Research Database (Denmark)

    Leloudas, Georgios; Chatzopoulos, E.; Dilday, B.;

    2012-01-01

    to contribute to a better understanding of these objects by studying SN 2006oz, a newly-recognized member of this class. Methods. We present multi-color light curves of SN 2006oz from the SDSS-II SN Survey that cover its rise time, as well as an optical spectrum that shows that the explosion occurred at z ~ 0...

  9. 高校西班牙语课堂沉默现象分析及对策%Analysis and Countermeasures of College Spanish Classroom Silence

    Institute of Scientific and Technical Information of China (English)

    张琼; 侯健

    2016-01-01

    China students' classroom silence problem has always been one of the difficulties in foreign language education. The classroom silence theory as the foundation, combined with questionnaire survey, analyzes the causes of the Spanish silence in the classroom, combined with their own classroom practice and observation gives the solution to the problem of suggestions and countermeasures.%中国学生的课堂沉默问题一向是高校外语教育面临的困境之一。本文以课堂沉默理论为基础,结合调查问卷,分析了高校西班牙语课堂沉默现象的成因,并结合笔者的课堂实践和观察给出了解决该问题的建议和对策。

  10. The Cornell High-order Adaptive Optics Survey for Brown Dwarfs in Stellar Systems-I: Observations, Data Reduction, and Detection Analysis

    CERN Document Server

    Carson, J C; Brandl, B R; Wilson, J C; Hayward, T L

    2005-01-01

    In this first of a two-paper sequence, we report techniques and results of the Cornell High-order Adaptive Optics Survey for brown dwarf companions (CHAOS). At the time of this writing, this study represents the most sensitive published population survey of brown dwarf companions to main sequence stars, for separation akin to our own outer solar system. The survey, conducted using the Palomar 200-inch Hale Telescope, consists of K-short coronagraphic observations of 80 main sequence stars out to 22 parsecs. At 1 arcsecond separations from a typical target system, the survey achieves median sensitivities 10 magnitudes fainter than the parent star. In terms of companion mass, the survey achieves typical sensitivities of 25 Jupiter masses (1 Gyr), 50 Jupiter masses (solar age), and 60 Jupiter masses (10 Gyr), using evolutionary models of Baraffe et al. (2003). Using common proper motion to distinguish companions from field stars, we find that no systems show positive evidence of a substellar companion (searchabl...

  11. Teacher perceptions of usefulness of mobile learning devices in rural secondary science classrooms

    Science.gov (United States)

    Tighe, Lisa

    The internet and easy accessibility to a wide range of digital content has created the necessity for teachers to embrace and integrate digitial media in their curriculums. Although there is a call for digital media integration in curriculum by current learning standards, rural schools continue to have access to fewer resources due to limited budgets, potentially preventing teachers from having access to the most current technology and science instructional materials. This dissertation identifies the perceptions rural secondary science teachers have on the usefulness of mobile learning devices in the science classroom. The successes and challenges in using mobile learning devices in the secondary classroom were also explored. Throughout this research, teachers generally supported the integration of mobile devices in the classroom, while harboring some concerns relating to student distractability and the time required for integrating mobile devices in exisiting curriculum. Quantitative and qualitative data collected through surveys, interviews, and classroom observations revealed that teachers perceive that mobile devices bring benefits such as ease of communication and easy access to digitial information. However, there are perceived challenges with the ability to effectively communicate complex scientific information via mobile devices, distractibility of students, and the time required to develop effective curriculum to integrate digital media into the secondary science classroom.

  12. The contribution of children's self-regulation and classroom quality to children's adaptive behaviors in the kindergarten classroom.

    Science.gov (United States)

    Rimm-Kaufman, Sara E; Curby, Tim W; Grimm, Kevin J; Nathanson, Lori; Brock, Laura L

    2009-07-01

    In this study, the authors examined the extent to which children's self-regulation upon kindergarten entrance and classroom quality in kindergarten contributed to children's adaptive classroom behavior. Children's self-regulation was assessed using a direct assessment upon entrance into kindergarten. Classroom quality was measured on the basis of multiple classroom observations during the kindergarten year. Children's adaptive classroom behavior in kindergarten was assessed through teacher report and classroom observations: Teachers rated children's cognitive and behavioral self-control and work habits during the spring of the kindergarten year; observers rated children's engagement and measured off-task behavior at 2-month intervals from November to May. Hierarchical linear models revealed that children's self-regulation upon school entry in a direct assessment related to teachers' report of behavioral self-control, cognitive self-control, and work habits in the spring of the kindergarten year. Classroom quality, particularly teachers' effective classroom management, was linked to children's greater behavioral and cognitive self-control, children's higher behavioral engagement, and less time spent off-task in the classroom. Classroom quality did not moderate the relation between children's self-regulation upon school entry and children's adaptive classroom behaviors in kindergarten. The discussion considers the implications of classroom management for supporting children's early development of behavioral skills that are important in school settings.

  13. Clasroom Observation Techniques

    OpenAIRE

    Akbayrak, Burcu

    1999-01-01

    In this article observation techniques as a data collecting tool used in social and educational research are examined and discussed. First the concepts and purposes of the observation technique are explained and later systematic and non-systematic observation techniques are described. Two research projects conducted in the classroom are then summarized. These are ‘ORACLE’ (Observational Research and Classroom Learning Evaluation Project), and ‘PRINDEP’ (Primary Needs Independent Evaluation Pr...

  14. Territoriality: Seat Preferences in Different Types of Classroom Arrangements

    Science.gov (United States)

    Kaya, Naz; Burgess, Brigitte

    2007-01-01

    Students' degree of territoriality based on gender and seat preferences in different types of classroom arrangements was studied. The types of classroom arrangements included rows of tablet-arm chairs, U-shaped, clusters, and rows of tables with individual chairs. The study was carried out through a survey at a large public institution in the…

  15. Classroom Assessment Practices of Secondary School Members of NCTM

    Science.gov (United States)

    Ohlsen, Michele T.

    2007-01-01

    In the current high-stakes educational environment, emphasis is on measurable student learning outcomes. The focus remains on single high-stakes tests, but most assessments of student learning occur in the classroom. In a survey of secondary mathematics teachers, the teachers self-reported their use of classroom assessment methods. The classroom…

  16. Classroom Environment Influence on Student Self-Efficacy in Mathematics

    Science.gov (United States)

    Croissant, Hillary P.

    2014-01-01

    This study aimed to find the characteristics of public school math classrooms and how they influence self-efficacy of students. Data were collected on math students in grades 4 through 12 in a North Texas school district. Two surveys were administered to students in the district. Within 10 days, the students completed a classroom environment…

  17. Geography Teachers' Attitudes and Beliefs Regarding Classroom Management

    Science.gov (United States)

    Dikmenli, Yurdal; Çifçi, Taner

    2016-01-01

    This study scrutinizes geography teachers' attitude and belief levels regarding classroom management. As a matter of fact, classroom management is one of the prominent areas emphasized by all educators. Descriptive correlational survey model was used in the study. Study group includes 58 geography teachers working in Sivas province during the…

  18. Persistent Classroom Management Training Needs of Experienced Teachers

    Science.gov (United States)

    Stough, Laura M.; Montague, Marcia L.; Landmark, Leena Jo; Williams-Diehm, Kendra

    2015-01-01

    Experienced special education teachers (n = 62) were surveyed on their professional preparation to become effective classroom managers. Despite having received extensive preservice training, over 83% of the sample reported being underprepared in classroom management and behavioral interventions. No statistically significant difference was found…

  19. A Large-scale Spectroscopic Survey of Methanol and OH Line Emission from the Galactic Center: Observations and Data

    Science.gov (United States)

    Cotton, W. D.; Yusef-Zadeh, F.

    2016-11-01

    Class I methanol masers are collisionally pumped and are generally correlated with outflows in star-forming sites in the Galaxy. Using the Very Large Array in its A-array configuration, we present a spectral line survey to identify methanol J={4}-1\\to {3}0E emission at 36.169 GHz. Over 900 pointings were used to cover a region 66‧ × 13‧ along the inner Galactic plane. A shallow survey of OH at 1612, 1665, 1667, and 1720 MHz was also carried out over the area covered by our methanol survey. We provide a catalog of 2240 methanol masers with narrow line-widths of ˜1 km s-1, spatial resolutions of ˜ 0\\buildrel{\\prime\\prime}\\over{.} 14× 0\\buildrel{\\prime\\prime}\\over{.} 05, and rms noises ˜20 mJy beam-1 per channel. Lower limits on the brightness temperature range from 27,000 to 10,000,000 K, showing that the emission is of non-thermal origin. We also provide a list of 23 OH (1612), 14 OH (1665), 5 OH (1667), and 5 OH (1720 MHz) masers. The origin of such a large number of methanol masers is not clear. Many methanol masers appear to be associated with infrared dark clouds, though it appears unlikely that the entire population of these masers traces the early phase of star formation in the Galactic center.

  20. An Empirical Investigation of the Dimensionality of the Physical Literacy Environment in Early Childhood Classrooms

    Science.gov (United States)

    Dynia, Jaclyn M.; Schachter, Rachel E.; Piasta, Shayne B.; Justice, Laura M.; O'Connell, Ann A.; Yeager Pelatti, Christina

    2016-01-01

    This study investigated the dimensionality of the physical literacy environment of early childhood education classrooms. Data on the classroom physical literacy environment were collected from 245 classrooms using the Classroom Literacy Observation Profile. A combination of confirmatory and exploratory factor analysis was used to identify five…

  1. The Effects of Clinical Experiences on the Understanding of Classroom Management Techniques

    Science.gov (United States)

    Cushman, Carey Anne Aycock; Kempy, Andrew

    2012-01-01

    For teacher educators, classroom management education is one of the least researched aspects of the profession. The purpose of this study was to determine if classroom management was most effectively learned through textbook analysis coupled with classroom discussion, or the experience of observing and practicing classroom management in the…

  2. Examining the Impact of Classroom Relationships on Student Engagement: A Multilevel Analysis

    Science.gov (United States)

    Kearney, W. Sean; Smith, Page A.; Maika, Sean

    2014-01-01

    This study explores the impact of classroom relationships on student engagement. To determine whether improved classroom relations lead to higher levels of student engagement, surveys were distributed to 2,340 students from 117 fourth- and fifth-grade classrooms. Respondents reported the degree to which they felt support from teachers,…

  3. The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: Observational systematics and baryon acoustic oscillations in the correlation function

    CERN Document Server

    Ross, Ashley J; Chuang, Chia-Hsun; Pellejero-Ibanez, Marcos; Seo, Hee-Jong; Vargas-Magana, Mariana; Cuesta, Antonio J; Percival, Will J; Burden, Angela; Sanchez, Ariel G; Grieb, Jan Niklas; Reid, Beth; Brownstein, Joel R; Dawson, Kyle S; Eisenstein, Daniel J; Ho, Shirley; Kitaura, Francisco-Shu; Nichol, Robert C; Olmstead, Matthew D; Prada, Francisco; Rodriguez-Torres, Sergio A; Saito, Shun; Salazar-Albornoz, Salvador; Schneider, Donald P; Thomas, Daniel; Tinker, Jeremy; Tojeiro, Rita; Wang, Yuting; White, Martin; Zhao, Gong-bo

    2016-01-01

    We present baryon acoustic oscillation (BAO) scale measurements determined from the clustering of 1.2 million massive galaxies with redshifts 0.2 < z < 0.75 distributed over 9300 square degrees, as quantified by their redshift-space correlation function. In order to facilitate these measurements, we define, describe, and motivate the selection function for galaxies in the final data release (DR12) of the SDSS III Baryon Oscillation Spectroscopic Survey (BOSS). This includes the observational footprint, masks for image quality and Galactic extinction, and weights to account for density relationships intrinsic to the imaging and spectroscopic portions of the survey. We simulate the observed systematic trends in mock galaxy samples and demonstrate that they impart no bias on baryon acoustic oscillation (BAO) scale measurements and have a minor impact on the recovered statistical uncertainty. We measure transverse and radial BAO distance measurements in 0.2 < z < 0.5, 0.5 < z < 0.75, and (overla...

  4. How Can Online Observation Support the Assessment and Feedback, on Classroom Performance, to Trainee Teachers at a Distance and in Real Time?

    Science.gov (United States)

    Dyke, Martin; Harding, Alan; Liddon, Sue

    2008-01-01

    This article reports the key findings of a project commissioned in 2005 by the UK Department for Education and Skills to consider the use of synchronous digital video for observation, feedback and assessment of teaching practice in post-compulsory education and training. A protocol for the remote observation of teaching is presented that was…

  5. Galaxy Survey On The Fly: Prospects of Rapid Galaxy Cataloging to Aid the Electromagnetic Follow-up of Gravitational-wave Observations

    CERN Document Server

    Bartos, Imre; Marka, Szabolcs

    2014-01-01

    Galaxy catalogs are essential for efficient searches of the electromagnetic counterparts of extragalactic gravitational wave (GW) signals with highly uncertain localization. We show that one can efficiently catalog galaxies within a short period of time with 1-2 meter-class telescopes such as the Palomar Transient Factory or MDM, in response to an observed GW signal from a compact binary coalescence. A rapid galaxy survey is feasible on the relevant time scale of $\\lesssim 1$ week, maximum source distance of $> 200$ Mpc and sky area of 100 deg$^2$. The catalog can be provided to other telescopes to aid electromagnetic follow-up observations to find kilonovae from binary coalescences, as well as other sources. We consider H$\\alpha$ observations, which track the star formation rate and are therefore correlated with the rate of compact binary mergers. H$\\alpha$ surveys are also able to filter out galaxies that are farther away than the maximum GW source distance. Rapid galaxy surveys that follow GW triggers coul...

  6. The LBTI Hunt for Observable Signatures of Terrestrial Systems (HOSTS) Survey: a Key NASA Science Program on the Road to Exoplanet Imaging Missions (SPIE Proceedings 2)

    Science.gov (United States)

    Danchi, William C.; Bailey, V.; Defrere, D.; Haniff, C.; Hinz, P.; Kennedy, G.; Mennesson, B.; Millan-Gabet, R.; Rieke, G.; Roberge, Aki; Serabyn, E.; Skemer, A.; Stapelfeldt, K.; Weinberger, A.; Wyatt, M.

    2014-01-01

    Telescope Interferometer (LBTI) will survey nearby stars for faint exozodiacal dust (exozodi). This warm circumstellar dust, analogous to the interplanetary dust found in the vicinity of the Earth in our own system, is produced in comet breakups and asteroid collisions. Emission and or scattered light from the exozodi will be the major source of astrophysical noise for a future space telescope aimed at direct imaging and spectroscopy of terrestrial planets (exo- Earths) around nearby stars. About 20 of nearby field stars have cold dust coming from planetesimals at large distances from the stars (Eiroa et al. 2013, AA, 555, A11; Siercho et al. 2014, ApJ, 785, 33). Much less is known about exozodi; current detection limits for individual stars are at best 500 times our solar system's level (aka. 500 zodi). LBTI-HOSTS will be the first survey capable of measuring exozodi at the 10 zodi level (3). Detections of warm dust will also reveal new information about planetary system architectures and evolution. We will describe the motivation for the survey and progress on target selection, not only the actual stars likely to be observed by such a mission but also those whose observation will enable sensible extrapolations for stars that will not be observed with LBTI. We briefly describe the detection of the debris disk around Crv, which is the first scientific result from the LBTI coming from the commissioning of the instrument in December 2013, shortly after the first time the fringes were stabilized.

  7. Raising Beetles in a Classroom.

    Science.gov (United States)

    Hackett, Erla

    This guide is designed to provide elementary school teachers with a harmless, inexpensive, clean, odorless, and easy-to-care-for insect-rearing project for the classroom. The following topics are included: (1) instructions for the care and feeding of the beetle larvae; (2) student activities for observing larval characteristics and behavior…

  8. Novice teachers’ classroom management self efficacy beliefs

    Directory of Open Access Journals (Sweden)

    Türkay Nuri Tok

    2016-12-01

    Full Text Available This study aims to determine novice teachers’ classrom management self efficacy beliefs as well as the extent to which these beliefs change according to independent variables. This research which aims to determine novice teachers’ classroom management self efficacy beliefs is a survey type research. The participants of the study are 85 novice teachers on duty in their first year in Hatay Province in Turkey. Classroom Management Self-Efficacy Convictions Scale that is internally consistent and valid in measuring classroom management self-efficacy beliefs of prospective teachers devised by Çetin (2013 was used in the study. There is not any statistically significant difference in terms of school of graduation and classroom management efficacy belief and result expectation sub-dimension. There is not any statistically significant difference in classroom management efficacy belief and result expectation sub-dimension. In terms of gender, there is not any statistically significant difference in the result expectation sub-dimension but there is a statistically significant difference in classroom management efficacy belief. Male novice teachers have higher level of classroom management efficacy beliefs than female novice teachers.

  9. Classroom discipline skills and disruption rate: A correlational study

    Science.gov (United States)

    Dropik, Melonie Jane

    Very little has been done to quantify the relationship between the frequency with which teachers use discipline skills and disruption rate in high school settings. Most of the available research that examined this relationship empirically was done in elementary schools, while a few studies examined the junior high school setting. The present research examined whether the use of ten specific discipline skills were related to the rate of disruption in suburban high school science classrooms. The ten skills were selected based on their prevalence in the theoretical literature and the strength of the relationships reported in empirical studies of elementary and junior high classrooms. Each relationship was tested directionally at alpha = .01. The maximum experimentwise Type I error rate was .10. Disruption rate was measured by trained observers over five class periods in the Fall of the school year. The frequency of performing the ten skills was assessed using a student survey developed for this study. The ten skills were: (1) beginning class on time, (2) using routines, (3) waiting for student attention before speaking, (4) giving clear directions, (5) presenting material fast enough to hold students' attention, (6) requiring students to remain seated, (7) appearing confident, (8) stopping misbehavior quickly, (9) checking for student attentiveness, and (10) teaching to the bell. Appearing confident (r = --.697, p = .004) and quickly stopping misbehavior (r = --.709, p = .003) were significantly negatively related to disruption rate. The effect sizes for the confidence and stopping misbehavior variables were .49 and .50, respectively. At least half of the variation in disruption rate was attributable to the difference in the frequency of appearing confident and stopping misbehavior quickly. The eight other relationships produced nonsignificant results. The results raise questions about whether theories developed from observational and anecdotal evidence gathered in

  10. Psychology of Language Classroom Practice

    Institute of Scientific and Technical Information of China (English)

    梁志超

    2005-01-01

    This paper is based on my personal observation and context, as well as some implications inspired trom theones, First, I shall give an evaluation of traditional language classroom practice I am familiar to. Second, relating to some implications in the theories of socialcultural psychology, I shall discuss some principled ways in which the classroom practices I have described and evaluated might be modified in order that we could enhance the effective opportunities for social and individual learning processes. I shall also provide my suggested structure of a lesson, in which some practices are implemented in this language classroom. Last but not the least, I shall give my reflection on how my own psychology of learning has been developed since I arrived at the university to begin my English teaching.

  11. Classroom Activity and Intrinsic Motivationin EFL Teaching and Learning

    Institute of Scientific and Technical Information of China (English)

    郑玉全

    2015-01-01

    The question of how to motivate language learners has been a neglected area in L2 motivation research, and even thefew available analyses lack an adequate research base. This article presents the results of an empirical survey aimed at initiatinginterviews and conducting follow-up questionnaire to obtain classroom data on motivational classroom teaching activities and theactual effect of these strategies. This current study provides new insights into English classroom teaching with further researchinvestigation and teaching implication to promote students' integrative motivation through classroom teaching activities.

  12. THE DETECTION OF INTERSTELLAR ETHANIMINE (CH{sub 3}CHNH) FROM OBSERVATIONS TAKEN DURING THE GBT PRIMOS SURVEY

    Energy Technology Data Exchange (ETDEWEB)

    Loomis, Ryan A.; Zaleski, Daniel P.; Steber, Amanda L.; Neill, Justin L.; Muckle, Matthew T.; Harris, Brent J.; Pate, Brooks H. [Department of Chemistry, University of Virginia, McCormick Road, Charlottesville, VA 22904 (United States); Hollis, Jan M. [NASA Goddard Space Flight Center, Greenbelt, MD 20771 (United States); Jewell, Philip R.; Remijan, Anthony J. [National Radio Astronomy Observatory, 520 Edgemont Road, Charlottesville, VA 22904-2475 (United States); Lattanzi, Valerio; Martinez, Oscar Jr.; McCarthy, Michael C. [Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138 (United States); Lovas, Frank J. [National Institute of Standards and Technology, Gaithersburg, MD 20899 (United States); Corby, Joanna F. [Department of Astronomy, University of Virginia, McCormick Road, Charlottesville, VA 22904 (United States)

    2013-03-01

    We have performed reaction product screening measurements using broadband rotational spectroscopy to identify rotational transition matches between laboratory spectra and the Green Bank Telescope PRIMOS radio astronomy survey spectra in Sagittarius B2 North (Sgr B2(N)). The broadband rotational spectrum of molecules created in an electrical discharge of CH{sub 3}CN and H{sub 2}S contained several frequency matches to unidentified features in the PRIMOS survey that did not have molecular assignments based on standard radio astronomy spectral catalogs. Several of these transitions are assigned to the E- and Z-isomers of ethanimine. Global fits of the rotational spectra of these isomers in the range of 8-130 GHz have been performed for both isomers using previously published mm-wave spectroscopy measurements and the microwave measurements of the current study. Possible interstellar chemistry formation routes for E-ethanimine and Z-ethanimine are discussed. The detection of ethanimine is significant because of its possible role in the formation of alanine-one of the twenty amino acids in the genetic code.

  13. Collaborative Classroom Management in a Co-Taught Primary School Classroom

    Science.gov (United States)

    Rytivaara, Anna

    2012-01-01

    The purpose of this study was to examine how teachers manage their classroom in co-taught lessons. The data were collected by observing and interviewing a pair of primary school teachers. The most important influence of collaboration on classroom management seemed to be the emotional support of another adult, and the opportunity to use different…

  14. Collaborative Classroom Management in a Co-Taught Primary School Classroom

    Science.gov (United States)

    Rytivaara, Anna

    2012-01-01

    The purpose of this study was to examine how teachers manage their classroom in co-taught lessons. The data were collected by observing and interviewing a pair of primary school teachers. The most important influence of collaboration on classroom management seemed to be the emotional support of another adult, and the opportunity to use different…

  15. Three-Year Global Survey of Coronal Null Points from Potential-Field-Source-Surface (PFSS) Modeling and Solar Dynamics Observatory (SDO) Observations

    CERN Document Server

    Freed, Michael; McKenize, David

    2014-01-01

    This article compiles and examines a comprehensive coronal magnetic-null-point survey created by potential-field-source-surface (PFSS) modeling and Solar Dynamics Observatory/Atmospheric Imaging Assembly (SDO/AIA) observations. The locations of 582 potential magnetic null points in the corona were predicted from the PFSS model between Carrington Rotations (CR) 2098 (June 2010) and 2139 (July 2013). These locations were manually inspected, using contrast-enhanced SDO/AIA images in 171 angstroms at the east and west solar limb, for structures associated with nulls. A Kolmogorov--Smirnov (K--S) test showed a statistically significant difference between observed and predicted latitudinal distributions of null points. This finding is explored further to show that the observability of null points could be affected by the Sun's asymmetric hemisphere activity. Additional K--S tests show no effect on observability related to eigenvalues associated with the fan and spine structure surrounding null points or to the orie...

  16. CARS: the CFHTLS-Archive-Research Survey. I. Five-band multi-colour data from 37 sq. deg. CFHTLS-wide observations

    Science.gov (United States)

    Erben, T.; Hildebrandt, H.; Lerchster, M.; Hudelot, P.; Benjamin, J.; van Waerbeke, L.; Schrabback, T.; Brimioulle, F.; Cordes, O.; Dietrich, J. P.; Holhjem, K.; Schirmer, M.; Schneider, P.

    2009-01-01

    catalogues reach a 5σ limiting magnitude of about i'_AB≈ 24.5. Comparisons with the SDSS indicate that most of our survey fields are photometrically calibrated to an accuracy of 0.04 mag or better. This allows us to derive photometric redshifts of homogeneous quality over the whole survey area. The accuracy of our high-confidence photo-z sample (10-15 galaxies per sq. arcmin) is estimated with external spectroscopic data to σΔ_z/(1+z)≈ 0.04-0.05 up to i'_AB outliers. In the spirit of the Legacy Survey we make our catalogues available to the astronomical community. Our products consist of multi-colour catalogues and supplementary information, such as image masks and JPEG files to visually inspect our catalogues. Interested users can obtain the data by request to the authors. Based on observations obtained with MegaPrime/MegaCam, a joint project of CFHT and CEA/DAPNIA, at the Canada-France-Hawaii Telescope (CFHT), which is operated by the National Research Council (NRC) of Canada, the Institut National des Sciences de l'Univers of the Centre National de la Recherche Scientifique (CNRS) of France, and the University of Hawaii. This work is based in part on data products produced at TERAPIX and the Canadian Astronomy Data Centre (CADC) as part of the Canada-France-Hawaii Telescope Legacy Survey, a collaborative project of NRC and CNRS.

  17. Classroom management, student-teacher relationships and quality in education

    DEFF Research Database (Denmark)

    Christensen, Mette Vedsgaard

    2017-01-01

    Knowledge about classroom management is crucial for both teachers’ and students’ well-being and educational success. Studies have indicated that teaching and learning cannot take place effectively in poorly managed classrooms (Jones & Jones, 2012; Marzano, Marzano & Pickering, 2003), and research...... management and relational competencies carried out in Denmark and Tanzania. The projects have explored and conceptualized the notions of classroom management and relational competencies in both theory and practice. Through classroom observations (in Denmark), we have identified and described constructive...... classroom management strategies and teacher-student relations, and by adjusting and applying insights from theory in pedagogical practice, we have introduced new ways of managing learning environments....

  18. Predicting prognosis in stable angina - results from the Euro heart survey of stable angina: prospective observational study

    DEFF Research Database (Denmark)

    Daly, Caroline A.; De Stavola, Bianca; Sendon, Jose L. Lopez

    2006-01-01

    -European survey in 156 outpatient cardiology clinics. Participants 3031 patients were included on the basis of a new clinical diagnosis by a cardiologist of stable angina with follow-up at one year. Main outcome measure Death or non-fatal myocardial infarction. Results The rate of death and non-fatal myocardial...... infarction in the first year was 2.3 per 100 patient years; the rate was 3.9 per 100 patient years in the subgroup (n = 994) with angiographic confirmation of coronary disease. The clinical and investigative factors most predictive of adverse outcome were comorbidity, diabetes, shorter duration of symptoms......, increasing severity of symptoms, abnormal ventricular function, resting electrocardiogaphic changes, or not having any stress test done. Results of non-invasive stress tests did not significantly predict outcome in the population who had tests done. A score was constructed using the parameters predictive...

  19. Comparing Dark Energy Survey and HST-CLASH observations of the galaxy cluster RXC J2248.7-4431: implications for stellar mass versus dark matter

    Science.gov (United States)

    Palmese, A.; Lahav, O.; Banerji, M.; Gruen, D.; Jouvel, S.; Melchior, P.; Aleksić, J.; Annis, J.; Diehl, H. T.; Hartley, W. G.; Jeltema, T.; Romer, A. K.; Rozo, E.; Rykoff, E. S.; Seitz, S.; Suchyta, E.; Zhang, Y.; Abbott, T. M. C.; Abdalla, F. B.; Allam, S.; Benoit-Lévy, A.; Bertin, E.; Brooks, D.; Buckley-Geer, E.; Burke, D. L.; Capozzi, D.; Carnero Rosell, A.; Carrasco Kind, M.; Carretero, J.; Crocce, M.; Cunha, C. E.; D'Andrea, C. B.; da Costa, L. N.; Desai, S.; Dietrich, J. P.; Doel, P.; Estrada, J.; Evrard, A. E.; Flaugher, B.; Frieman, J.; Gerdes, D. W.; Goldstein, D. A.; Gruendl, R. A.; Gutierrez, G.; Honscheid, K.; James, D. J.; Kuehn, K.; Kuropatkin, N.; Li, T. S.; Lima, M.; Maia, M. A. G.; Marshall, J. L.; Miller, C. J.; Miquel, R.; Nord, B.; Ogando, R.; Plazas, A. A.; Roodman, A.; Sanchez, E.; Scarpine, V.; Sevilla-Noarbe, I.; Smith, R. C.; Soares-Santos, M.; Sobreira, F.; Swanson, M. E. C.; Tarle, G.; Thomas, D.; Tucker, D.; Vikram, V.

    2016-12-01

    We derive the stellar mass fraction in the galaxy cluster RXC J2248.7-4431 observed with the Dark Energy Survey (DES) during the Science Verification period. We compare the stellar mass results from DES (five filters) with those from the Hubble Space Telescope Cluster Lensing And Supernova Survey (CLASH; 17 filters). When the cluster spectroscopic redshift is assumed, we show that stellar masses from DES can be estimated within 25 per cent of CLASH values. We compute the stellar mass contribution coming from red and blue galaxies, and study the relation between stellar mass and the underlying dark matter using weak lensing studies with DES and CLASH. An analysis of the radial profiles of the DES total and stellar mass yields a stellar-to-total fraction of f⋆ = (6.8 ± 1.7) × 10-3 within a radius of r200c ≃ 2 Mpc. Our analysis also includes a comparison of photometric redshifts and star/galaxy separation efficiency for both data sets. We conclude that space-based small field imaging can be used to calibrate the galaxy properties in DES for the much wider field of view. The technique developed to derive the stellar mass fraction in galaxy clusters can be applied to the ˜100 000 clusters that will be observed within this survey and yield important information about galaxy evolution.

  20. Comparing Dark Energy Survey and HST{CLASH observations of the galaxy cluster RXC J2248.7{4431: implications for stellar mass versus dark matter

    Energy Technology Data Exchange (ETDEWEB)

    Palmese, A.; Lahav, O.; Banerji, M.; Gruen, D.; Jouvel, S.; Melchior, P.; Aleksic, J.; Annis, J; Diehl, H. T.; Jeltema, T.; Vikram, Vinu

    2016-12-01

    We derive the stellar mass fraction in the galaxy cluster RXC J2248.7-4431 observed with the Dark Energy Survey (DES) during the Science Verification period. We compare the stellar mass results from DES (five filters) with those from the Hubble Space Telescope Cluster Lensing And Supernova Survey (CLASH; 17 filters). When the cluster spectroscopic redshift is assumed, we show that stellar masses from DES can be estimated within 25 per cent of CLASH values. We compute the stellar mass contribution coming from red and blue galaxies, and study the relation between stellar mass and the underlying dark matter using weak lensing studies with DES and CLASH. An analysis of the radial profiles of the DES total and stellar mass yields a stellar-to-total fraction of f(star) = (6.8 +/- 1.7) x 10(-3) within a radius of r(200c) similar or equal to 2 Mpc. Our analysis also includes a comparison of photometric redshifts and star/galaxy separation efficiency for both data sets. We conclude that space-based small field imaging can be used to calibrate the galaxy properties in DES for the much wider field of view. The technique developed to derive the stellar mass fraction in galaxy clusters can be applied to the similar to 100 000 clusters that will be observed within this survey and yield important information about galaxy evolution.

  1. Morphology of the southern African geomagnetic field derived from observatory and repeat station survey observations: 2005-2014

    Science.gov (United States)

    Kotzé, P. B.; Korte, M.

    2016-02-01

    Geomagnetic field data from four observatories and annual field surveys between 2005 and 2015 provide a detailed description of Earth's magnetic field changes over South Africa, Namibia and Botswana on time scales of less than 1 year. The southern African area is characterized by rapid changes in the secular variation pattern and lies in close proximity to the South Atlantic Anomaly (SAA) where the geomagnetic field intensity is almost 30 % weaker than in other regions at similar latitudes around the globe. Several geomagnetic secular acceleration (SA) pulses (geomagnetic jerks) around 2007, 2010 and 2012 could be identified over the last decade in southern Africa. We present a new regional field model for declination and horizontal and vertical intensity over southern Africa (Southern African REGional (SAREG)) which is based on field survey and observatory data and covering the time interval from 2005 to 2014, i.e. including the period between 2010 and 2013 when no low Earth-orbiting vector field satellite data are available. A comparative evaluation between SAREG and global field models like CHAOS-5, the CHAMP, Orsted and SAC-C model of the Earth's magnetic field and International Geomagnetic Reference Field (IGRF-12) reveals that a simple regional field model based on a relatively dense ground network is able to provide a realistic representation of the geomagnetic field in this area. We particularly note that a global field model like CHAOS-5 does not always indicate similar short-period patterns in the field components as revealed by observatory data, while representing the general secular variation reasonably well during the time interval without near-Earth satellite vector field data. This investigation further shows the inhomogeneous occurrence and distribution of secular variation impulses in the different geomagnetic field components and at different locations in southern African.

  2. Intensification of the Learning Process: Diagnostic Instruments--Visual Performance Screening Test, Observing the Learner, Questionnaire-Parent. A Series of Reports Designed for Classroom Use.

    Science.gov (United States)

    Bucks County Public Schools, Doylestown, PA.

    Instruments for screening visual performance, for observing vision behavior, the learner in general, and the student at a learning task, and a parent questionnaire are described. (See TM 001 363 for a description of the total project; for other related documents, see TM 001 160, 364-368, 370-374.) (MS)

  3. Curbing Digital Distractions in the Classroom

    Science.gov (United States)

    Seemiller, Corey

    2017-01-01

    Whether banking, communicating, watching television, or shopping, people can now do nearly anything on their personal digital devices. This digital access even extends to the college classroom where students use their personal devices for a multitude of non-class related purposes. Findings from a survey of 193 college undergraduates found that…

  4. Investigation and analysis of human body thermal comfort in classroom

    Science.gov (United States)

    Zhai, Xue

    2017-05-01

    In this survey, we selected the 11th building of North China Electric Power University as the research object. Data were measured and distributed on each floor. We record the temperature of the classroom, humidity, wind speed, average radiation temperature and other environmental parameters. And we used spare time to create a questionnaire survey of the subjective feeling of the survey, to get everyone in the classroom TSV (hot feeling vote value) and TCV (thermal comfort vote). We analyzed the test data and survey data. What's more we discuss and reflect on the thermal comfort of the human body in different indoor temperature atmospheres.

  5. Dimensions of Classroom Instruction: A Programmatic Approach to the Description of the Classroom Environment. Planning Report No. 5076.

    Science.gov (United States)

    Clements, R. O.

    An ongoing research project, Dimensions of Classroom Instruction (DCI) is described. The primary data source is a study of reading in nine second-grade classrooms using such observation techniques as categorical observation, ethnographic observation, and videotaping. Three major objectives for the project are stated: 1) developing methods of…

  6. A Survey of Magnetic Waves Excited by Newborn Interstellar He+ Observed by the ACE Spacecraft at 1 au

    Science.gov (United States)

    Fisher, Meghan K.; Argall, Matthew R.; Joyce, Colin J.; Smith, Charles W.; Isenberg, Philip A.; Vasquez, Bernard J.; Schwadron, Nathan A.; Skoug, Ruth M.; Sokół, Justyna M.; Bzowski, Maciej; Zurbuchen, Thomas H.; Gilbert, Jason A.

    2016-10-01

    We report observations of low-frequency waves at 1 au by the magnetic field instrument on the Advanced Composition Explorer (ACE/MAG) and show evidence that they arise due to newborn interstellar pickup He+. Twenty-five events are studied. They possess the generally predicted attributes: spacecraft-frame frequencies slightly greater than the He+ cyclotron frequency, left-hand polarization in the spacecraft frame, and transverse fluctuations with minimum variance directions that are quasi-parallel to the mean magnetic field. Their occurrence spans the first 18 years of ACE operations, with no more than 3 such observations in any given year. Thus, the events are relatively rare. As with past observations by the Ulysses and Voyager spacecraft, we argue that the waves are seen only when the background turbulence is sufficiently weak as to allow for the slow accumulation of wave energy over many hours.

  7. Microtremor Array Measurement Survey and Strong Ground Motion Observation Activities of The MarDiM (SATREPS) Project

    Science.gov (United States)

    Ozgur Citak, Seckin; Karagoz, Ozlem; Chimoto, Kosuke; Ozel, Oguz; Yamanaka, Hiroaki; Aksahin, Bengi; Arslan, Safa; Hatayama, Ken; Ohori, Michihiro; Hori, Muneo

    2015-04-01

    Since 1939, devastating earthquakes with magnitude greater than seven ruptured North Anatolian Fault (NAF) westward, starting from 1939 Erzincan (Ms=7.9) at the eastern Turkey and including the latest 1999 Izmit-Golcuk (Ms=7.4) and the Duzce (Ms=7.2) earthquakes in the eastern Marmara region, Turkey. On the other hand, the west of the Sea of Marmara an Mw7.4 earthquake ruptured the NAF' s Ganos segment in 1912. The only un-ruptured segments of the NAF in the last century are within the Sea of Marmara, and are identified as a "seismic gap" zone that its rupture may cause a devastating earthquake. In order to unravel the seismic risks of the Marmara region a comprehensive multidisciplinary research project The MarDiM project "Earthquake And Tsunami Disaster Mitigation in The Marmara Region and Disaster Education in Turkey", has already been started since 2003. The project is conducted in the framework of "Science and Technology Research Partnership for Sustainable Development (SATREPS)" sponsored by Japan Science and Technology Agency (JST) and Japan International Cooperation Agency (JICA). One of the main research field of the project is "Seismic characterization and damage prediction" which aims to improve the prediction accuracy of the estimation of the damages induced by strong ground motions and tsunamis based on reliable source parameters, detailed deep and shallow velocity structure and building data. As for detailed deep and shallow velocity structure microtremor array measurement surveys were conducted in Zeytinburnu district of Istanbul and Tekirdag province at about 81 sites on October 2013 and September 2014. Also in September 2014, 11 accelerometer units were installed mainly in public buildings in both Zeytinburnu and Tekirdag area and are currently in operation. Each accelerometer unit compose of a Network Sensor (CV-374A2) by Tokyo Sokushin, post processing PC for data storage and power supply unit. The Network Sensor (CV-374A2) consist of three servo

  8. Microtremor Array Measurement Survey and Strong Ground Motion observation activities of The SATREPS, MarDiM project -Part 2-

    Science.gov (United States)

    Citak, Seckin; Karagoz, Ozlem; Chimoto, Kosuke; Ozel, Oguz; Yamanaka, Hiroaki; Arslan, Safa; Aksahin, Bengi; Hatayama, Ken; Ohori, Michihiro; Hori, Muneo

    2016-04-01

    Since 1939, devastating earthquakes with magnitude greater than seven ruptured North Anatolian Fault (NAF) westward, starting from 1939 Erzincan (Ms=7.9) at the eastern Turkey and including the latest 1999 Izmit-Golcuk (Ms=7.4) and the Duzce (Ms=7.2) earthquakes in the eastern Marmara region, Turkey. On the other hand, the west of the Sea of Marmara an Mw7.4 earthquake ruptured the NAF' s Ganos segment in 1912. The only un-ruptured segments of the NAF in the last century are within the Sea of Marmara, and are identified as a "seismic gap" zone that its rupture may cause a devastating earthquake. In order to unravel the seismic risks of the Marmara region a comprehensive multidisciplinary research project The MarDiM project "Earthquake And Tsunami Disaster Mitigation in The Marmara Region and Disaster Education in Turkey", has already been started since 2003. The project is conducted in the framework of "Science and Technology Research Partnership for Sustainable Development (SATREPS)" sponsored by Japan Science and Technology Agency (JST) and Japan International Cooperation Agency (JICA). One of the main research field of the project is "Seismic characterization and damage prediction" which aims to improve the prediction accuracy of the estimation of the damages induced by strong ground motions and tsunamis based on reliable source parameters, detailed deep and shallow velocity structure and building data. As for detailed deep and shallow velocity structure microtremor array measurement surveys were conducted in Zeytinburnu district of Istanbul, Tekirdag, Canakkale and Edirne provinces at about 109 sites on October 2013, September 2014 and 2015. Also in September 2014, 11 accelerometer units were installed mainly in public buildings in both Zeytinburnu and Tekirdag area and are currently in operation. Each accelerometer unit compose of a Network Sensor (CV-374A) by Tokyo Sokushin, post processing PC for data storage and power supply unit. The Network Sensor (CV-374

  9. Microtremor Array Measurement Survey and Strong Ground Motion observation activities of The SATREPS, MarDiM project -Part 3-

    Science.gov (United States)

    Citak, Seckin; Safa Arslan, Mehmet; Karagoz, Ozlem; Chimoto, Kosuke; Ozel, Oguz; Yamanaka, Hiroaki; Behiye Aksahin, Bengi; Hatayama, Ken; Sahin, Abdurrahman; Ohori, Michihiro; Safak, Erdal; Hori, Muneo

    2017-04-01

    Since 1939, devastating earthquakes with magnitude greater than seven ruptured North Anatolian Fault (NAF) westward, starting from 1939 Erzincan (Ms=7.9) at the eastern Turkey and including the latest 1999 Izmit-Golcuk (Ms=7.4) and the Duzce (Ms=7.2) earthquakes in the eastern Marmara region, Turkey. On the other hand, the west of the Sea of Marmara an Mw7.4 earthquake ruptured the NAF' s Ganos segment in 1912. The only un-ruptured segments of the NAF in the last century are within the Sea of Marmara, and are identified as a "seismic gap" zone that its rupture may cause a devastating earthquake. In order to unravel the seismic risks of the Marmara region a comprehensive multidisciplinary research project The MarDiM project "Earthquake And Tsunami Disaster Mitigation in The Marmara Region and Disaster Education in Turkey", has already been started since 2003. The project is conducted in the framework of "Science and Technology Research Partnership for Sustainable Development (SATREPS)" sponsored by Japan Science and Technology Agency (JST) and Japan International Cooperation Agency (JICA). One of the main research field of the project is "Seismic characterization and damage prediction" which aims to improve the prediction accuracy of the estimation of the damages induced by strong ground motions and tsunamis based on reliable source parameters, detailed deep and shallow velocity structure and building data. As for detailed deep and shallow velocity structure microtremor array measurement surveys were conducted in Zeytinburnu district of Istanbul, Tekirdag, Canakkale and Edirne provinces at about 140 sites on October 2013, September 2014, 2015 and 2016. Also in September 2014, 11 accelerometer units were installed mainly in public buildings in both Zeytinburnu and Tekirdag area and are currently in operation. Each accelerometer unit compose of a Network Sensor (CV-374A) by Tokyo Sokushin, post processing PC for data storage and power supply unit. The Network Sensor

  10. Classroom Management. TESOL Classroom Practice Series

    Science.gov (United States)

    Farrell, Thomas S. C., Ed.

    2008-01-01

    This series captures the dynamics of the contemporary ESOL classroom. It showcases state-of-the-art curricula, materials, tasks, and activities reflecting emerging trends in language education and seeks to build localized language teaching and learning theories based on teachers' and students' unique experiences in and beyond the classroom. Each…

  11. First survey of Wolf-Rayet star populations over the full extension of nearby galaxies observed with CALIFA

    CERN Document Server

    Miralles-Caballero, D; López-Sánchez, Á R; Rosales-Ortega, F F; Monreal-Ibero, A; Pérez-Montero, E; Kehrig, C; García-Benito, R; Sánchez, S F; Walcher, C J; Galbany, L; Iglesias-Páramo, J; Vílchez, J M; Delgado, R M González; van de Ven, G; Barrera-Ballesteros, J; Lyubenova, M; Meidt, S; Falcon-Barroso, J; Mast, D; Mendoza, M A

    2016-01-01

    The search of extragalactic regions with conspicuous presence of Wolf-Rayet (WR) stars outside the Local Group is challenging task due to the difficulties in detecting their faint spectral features. In this exploratory work, we develop a methodology to perform an automated search of WR signatures through a pixel-by-pixel analysis of integral field spectroscopy (IFS) data belonging to the Calar Alto Legacy Integral Field Area survey, CALIFA. This technique allowed us to build the first catalogue of Wolf-Rayet rich regions with spatially-resolved information, allowing to study the properties of these complexes in a 2D context. The detection technique is based on the identification of the blue WR bump (around He II 4686 {\\AA}, mainly associated to nitrogen-rich WR stars, WN) and the red WR bump (around C IV 5808 {\\AA} and associated to carbon-rich WR stars, WC) using a pixel-by-pixel analysis. We identified 44 WR-rich regions with blue bumps distributed in 25 galaxies of a total of 558. The red WR bump was ident...

  12. The Star Formation in Radio Survey: GBT 33 GHz Observations of Nearby Galaxy Nuclei and Extranuclear Star-Forming Regions

    CERN Document Server

    Murphy, E J; Mason, B S; Condon, J J; Schinnerer, E; Aniano, G; Armus, L; Helou, G; Turner, J L; Jarrett, T H

    2012-01-01

    We present 33\\,GHz photometry of 103 galaxy nuclei and extranuclear star-forming complexes taken with the Green Bank Telescope (GBT) as part of the Star Formation in Radio Survey (SFRS). Among the sources without evidence for an AGN, and also having lower frequency radio data, we find a median thermal fraction at 33GHz of ~76% with a dispersion of ~24%. For all sources resolved on scales 90%. This suggests that the rest-frame 33GHz emission provides a sensitive measure of the ionizing photon rate from young star-forming regions, thus making it a robust star formation rate indicator. Taking the 33GHz star formation rates as a reference, we investigate other empirical calibrations relying on different combinations of warm 24\\mu m dust, total infrared (IR; 8-1000\\mu m), H\\alpha\\ line, and far-UV continuum emission. The recipes derived here generally agree with others found in the literature, albeit with a large dispersion that most likely stems from a combination of effects. Comparing the 33GHz to total IR flux ...

  13. Optical spectroscopic observations of blazars and γ-ray blazar candidates in the sloan digital sky survey data release nine

    Energy Technology Data Exchange (ETDEWEB)

    Massaro, F.; Masetti, N.; D' Abrusco, R.; Paggi, A.; Funk, S.

    2014-09-09

    We present an analysis of the optical spectra available in the Sloan Digital Sky Survey data release nine (SDSS DR9) for the blazars listed in the ROMA-BZCAT and for the γ-ray blazar candidates selected according to their IR colors. First, we adopt a statistical approach based on Monte Carlo simulations to find the optical counterparts of the blazars listed in the ROMA-BZCAT catalog. Then, we crossmatched the SDSS spectroscopic catalog with our selected samples of blazars and γ-ray blazar candidates, searching for those with optical spectra available to classify our blazar-like sources and, whenever possible, to confirm their redshifts. Our main objectives are to determine the classification of uncertain blazars listed in the ROMA-BZCAT and to discover new gamma-ray blazars. For the ROMA-BZCAT sources, we investigated a sample of 84 blazars, confirming the classification for 20 of them and obtaining 18 new redshift estimates. For the γ-ray blazars, indicated as potential counterparts of unassociated Fermi sources or with uncertain nature, we established the blazar-like nature of 8 out of the 27 sources analyzed and confirmed 14 classifications.

  14. Predicting prognosis in stable angina--results from the Euro heart survey of stable angina: prospective observational study.

    NARCIS (Netherlands)

    Daly, C.A.; Stavola, B. De; Lopez Sendon, J.L.; Tavazzi, L.; Boersma, E.; Clemens, F.; Danchin, N.; Delahaye, F.; Gitt, A.; Julian, D.; Mulcahy, D.; Ruzyllo, W.; Thygesen, K.; Verheugt, F.W.A.; Fox, K.M.

    2006-01-01

    OBJECTIVES: To investigate the prognosis associated with stable angina in a contemporary population as seen in clinical practice, to identify the key prognostic features, and from this to construct a simple score to assist risk prediction. DESIGN: Prospective observational cohort study. SETTING: Pan

  15. FIRST-based survey of Compact Steep Spectrum sources, IV. Multifrequency VLBA observations of very compact objects

    CERN Document Server

    Kunert-Bajraszewska, M; Thomasson, P; Kunert-Bajraszewska, Magdalena; Marecki, Andrzej; Thomasson, Peter

    2006-01-01

    Evidence has been mounting recently that activity in some radio loud AGNs (RLAGNs) can cease shortly after ignition and that perhaps even a majority of very compact sources may be short-lived phenomena because of a lack of stable fuelling from the black hole. Thus, they can fade out before having evolved to large, extended objects. Re-ignition of the activity in such objects is not ruled out. With the aim of finding more examples of these objects and to investigate if they could be RLAGNs switched off at very early stages of their evolution, multifrequency VLBA observations of six sources with angular sizes significantly less than an arcsecond, yet having steep spectra, have been made. Observations were initially made at 1.65 GHz using the VLBA with the inclusion of Effelsberg telescope. The sources were then re-observed with the VLBA at 5, 8.4 and 15.4 GHz. All the observations were carried out in a snapshot mode with phase referencing. One of the sources studied, 0809+404, is dominated by a compact componen...

  16. An Astronomical Misconceptions Survey

    Science.gov (United States)

    LoPresto, Michael C.; Murrell, Steven R.

    2011-01-01

    Misconceptions that students bring with them to the introductory science classroom plague every area of science and are especially prevalent in astronomy. One way to identify and possibly dispel some of these misconceptions is through the use of a misconceptions survey. The following is a report on the development, implementation, and some early…

  17. ASHA Survey of Health Curriculum Needs: Survey Results.

    Science.gov (United States)

    Schneider, Livingston S.; Thier, Herbert D.

    The results of a survey conducted by the Ad hoc Committee to Study the Needs and Problems of the Classroom Teacher in Curriculum Development are reported. Questionnaires were sent to members of the American School Health Association (ASHA). The survey was composed of four sections: (1) background information on demographic data, institutional…

  18. Research Experience for Teachers at NRAO-Green Bank: Planning for Cometary Observations with the Green Bank Telescope and Its Application to Chemistry Classroom Activities

    Science.gov (United States)

    Hynes, Christopher; Lockman, F. J.; Lovell, A.

    2010-01-01

    The NSF-funded "Research Experience for Teachers" project provides teachers an opportunity to work on a current scientific or engineering research project. This paper will describe the development of a Python program as a further expansion of a previous mathematical model3 designed to simulate cometary data collected by the Green Bank Telescope (GBT). The program allows for user interaction to change parameters such as the comet's distance from the sun, the rate of production of gaseous outflows, lifetime of these gaseous particles and maximum limit for how many gas particles are generated. Furthermore this paper will present results of how students can write their own Python programming code to manipulate these parameters to generate velocity profiles of the out gassed chemical species. Students should be enlightened that Science can be cross disciplinary. Several concepts in Chemistry: sublimation, electromagnetic spectrum, quantum mechanics, gas behavior and chemical kinetics play an important role in the formation of a comet cloud and how that cloud could be observed using radio astronomy. Chemical species such as HCN, CS and HCO+1 have been observed in cometary clouds. The chemical composition of the cloud and its size are a function of its distance from the sun and the radial location from the center of the comet cloud. High-school students at the Louisiana School for Math, Science and the Arts, LA will learn Python programming language to create a mathematical model of a cometary cloud. The students will have formulated models for rate of sublimation, rate of photo-dissociation, and velocity of gas particles as the fundamental framework to determine frequencies and intensities of the molecular spectra. The students will be able to manipulate their code to create various comet cloud scenarios as it might be observed by the GBT.

  19. Herschel observations of extraordinary sources: Analysis of the HIFI 1.2 THz wide spectral survey toward orion KL. I. method

    Energy Technology Data Exchange (ETDEWEB)

    Crockett, Nathan R.; Bergin, Edwin A.; Neill, Justin L.; Favre, Cécile [Department of Astronomy, University of Michigan, 500 Church Street, Ann Arbor, MI 48109 (United States); Schilke, Peter [Physikalisches Institut, Universität zu Köln, Zülpicher Str. 77, D-50937 Köln (Germany); Lis, Dariusz C.; Emprechtinger, Martin; Phillips, Thomas G. [Cahill Center for Astronomy and Astrophysics 301-17, California Institute of Technology, Pasadena, CA 91125 (United States); Bell, Tom A.; Cernicharo, José; Esplugues, Gisela B. [Centro de Astrobiología (CSIC/INTA), Laboratiorio de Astrofísica Molecular, Ctra. de Torrejón a Ajalvir, km 4, E-28850 Torrejón de Ardoz, Madrid (Spain); Blake, Geoffrey; Kleshcheva, Maria [Division of Geological and Planetary Sciences, California Institute of Technology, MS 150-21, Pasadena, CA 91125 (United States); Gupta, Harshal; Pearson, John [Jet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Drive, Pasadena, CA 91109 (United States); Lord, Steven [Infrared Processing and Analysis Center, California Institute of Technology, MS 100-22, Pasadena, CA 91125 (United States); Marcelino, Nuria [National Radio Astronomy Observatory, 520 Edgemont Road, Charlottesville, VA 22903 (United States); McGuire, Brett A. [Division of Chemistry and Chemical Engineering, California Institute of Technology Pasadena, CA 91125 (United States); Plume, Rene [Department of Physics and Astronomy, University of Calgary, 2500 University Drive NW, Calgary, AB T2N 1N4 (Canada); Van der Tak, Floris [SRON Netherlands Institute for Space Research, P.O. Box 800, 9700 AV Groningen (Netherlands); and others

    2014-06-01

    We present a comprehensive analysis of a broadband spectral line survey of the Orion Kleinmann-Low nebula (Orion KL), one of the most chemically rich regions in the Galaxy, using the HIFI instrument on board the Herschel Space Observatory. This survey spans a frequency range from 480 to 1907 GHz at a resolution of 1.1 MHz. These observations thus encompass the largest spectral coverage ever obtained toward this high-mass star-forming region in the submillimeter with high spectral resolution and include frequencies >1 THz, where the Earth's atmosphere prevents observations from the ground. In all, we detect emission from 39 molecules (79 isotopologues). Combining this data set with ground-based millimeter spectroscopy obtained with the IRAM 30 m telescope, we model the molecular emission from the millimeter to the far-IR using the XCLASS program, which assumes local thermodynamic equilibrium (LTE). Several molecules are also modeled with the MADEX non-LTE code. Because of the wide frequency coverage, our models are constrained by transitions over an unprecedented range in excitation energy. A reduced χ{sup 2} analysis indicates that models for most species reproduce the observed emission well. In particular, most complex organics are well fit by LTE implying gas densities are high (>10{sup 6} cm{sup –3}) and excitation temperatures and column densities are well constrained. Molecular abundances are computed using H{sub 2} column densities also derived from the HIFI survey. The distribution of rotation temperatures, T {sub rot}, for molecules detected toward the hot core is significantly wider than the compact ridge, plateau, and extended ridge T {sub rot} distributions, indicating the hot core has the most complex thermal structure.

  20. Observation as an Assessment Tool.

    Science.gov (United States)

    Nickell, Pat; Wilson, Angene

    1999-01-01

    Considers the use of observation in the classroom as a means of student assessment. Focuses on developing an observation instrument, the scoring criteria, and using progress-based rankings rather than static rankings. Provides an example teacher observation form. (CMK)

  1. Survey of ELF-VLF plasma waves in outer radiation belt observed by Cluster STAFF-SA experiment

    Directory of Open Access Journals (Sweden)

    D. Pokhotelov

    2008-10-01

    Full Text Available Various types of plasma waves have profound effects on acceleration and scattering of radiation belt particles. For the purposes of radiation belt modeling it is necessary to know statistical distributions of plasma wave parameters. This paper analyzes four years of plasma wave observations in the Earth's outer radiation belt obtained by the STAFF-SA experiment on board Cluster spacecraft. Statistical distributions of spectral density of different plasma waves observed in ELF-VLF range (chorus, plasmaspheric hiss, magnetosonic waves are presented as a function of magnetospheric coordinates and geomagnetic activity indices. Comparison with other spacecraft studies supports some earlier conclusions about the distribution of chorus and hiss waves and helps to remove the long-term controversy regarding the distribution of equatorial magnetosonic waves. This study represents a step towards the development of multi-spacecraft database of plasma wave activity in radiation belts.

  2. Bullying and Victimization Trends in Undergraduate Medical Students - A Self-Reported Cross-Sectional Observational Survey.

    Science.gov (United States)

    Kapoor, Shrea; Ajinkya, Shaunak; Jadhav, Pradeep R

    2016-02-01

    Bullying is a form of behaviour that can negatively impact a person. It can lead to several deleterious consequences like low self-confidence, drop in academic performance and depression. Studies have shown that bullying behaviour exists amongst medical students also. In the medical field, it is known to negatively impact dispensing of health care and attitudes of medical students towards becoming doctors. It is very difficult for medical students to cope with such a menace as they are already burdened with a vast curriculum and rigorous schedules. There exists paucity of studies regarding bullying amongst undergraduate medical students in Indian context. To study prevalence of peer-based bullying and victimization along with their associated factors in undergraduate medical students. Four hundred randomly chosen undergraduate medical students were included in the study. Socio-demographic and personal details including history of substance use were recorded in a self-designed case record form. Illinois Bullying Scale was used to assess bullying behaviours. Out of total 400 students, 383 completed the survey and this data was analysed. In this study, 98.69% participants self-reported to having indulged in bullying while 88.77% reported feeling victimized. Physical (pStudents of the third year of medical school indulged in significantly (p=0.034) greater severity of physical bullying than those of other years. Alcohol consumption (p=0.001) and cigarette smoking (pstudents. There is an urgent need for more detailed studies on bullying in medical students so that remedial measures can be initiated and steps to limit such behaviours can be looked at seriously.

  3. Circadian-related sleep disorders and sleep medication use in the New Zealand blind population: an observational prevalence survey.

    Directory of Open Access Journals (Sweden)

    Guy R Warman

    Full Text Available STUDY OBJECTIVES: To determine the prevalence of self-reported circadian-related sleep disorders, sleep medication and melatonin use in the New Zealand blind population. DESIGN: A telephone survey incorporating 62 questions on sleep habits and medication together with validated questionnaires on sleep quality, chronotype and seasonality. PARTICIPANTS: PARTICIPANTS WERE GROUPED INTO: (i 157 with reduced conscious perception of light (RLP; (ii 156 visually impaired with no reduction in light perception (LP matched for age, sex and socioeconomic status, and (iii 156 matched fully-sighted controls (FS. SLEEP HABITS AND DISTURBANCES: The incidence of sleep disorders, daytime somnolence, insomnia and sleep timing problems was significantly higher in RLP and LP compared to the FS controls (p<0.001. The RLP group had the highest incidence (55% of sleep timing problems, and 26% showed drifting sleep patterns (vs. 4% FS. Odds ratios for unconventional sleep timing were 2.41 (RLP and 1.63 (LP compared to FS controls. For drifting sleep patterns, they were 7.3 (RLP and 6.0 (LP. MEDICATION USE: Zopiclone was the most frequently prescribed sleep medication. Melatonin was used by only 4% in the RLP group and 2% in the LP group. CONCLUSIONS: Extrapolations from the current study suggest that 3,000 blind and visually impaired New Zealanders may suffer from circadian-related sleep problems, and that of these, fewer than 15% have been prescribed melatonin. This may represent a therapeutic gap in the treatment of circadian-related sleep disorders in New Zealand, findings that may generalize to other countries.

  4. Using medical student observers of infection prevention, hand hygiene, and injection safety in outpatient settings: A cross-sectional survey.

    Science.gov (United States)

    Thompson, Deborah; Bowdey, Lisa; Brett, Meghan; Cheek, James

    2016-04-01

    Health care-associated infection outbreaks have occurred in outpatient settings due to lapses in infection prevention. However, little is known about the overall infection prevention status in outpatient environments. A cross-sectional design was employed to assess infection prevention policies and practices at 15 outpatient sites across New Mexico in 2014 during a medical student outpatient rotation. A standardized infection prevention checklist was completed via staff interview; observations of injection safety practices and hand hygiene behavior were conducted. Aggregate data were analyzed using Excel (Microsoft, Redmond, WA) and Stata (version 12.1, Stata Corp, College Station, TX) statistical software. Medical practice staff interviews reported a mean of 92.8% (median, 96.7%; range, 75.0%-98.9%) presence of recommended policies and practices. One hundred sixty-three injection safety observations were performed that revealed medication vial rubber septums were disinfected with alcohol 78.4% (95% confidence interval [CI], 71.1%-84.7%) of the time before piercing. Three hundred thirty hand hygiene observations revealed 33.9% (95% CI, 28.8%-39.1%) use of alcohol-based handrub, 29.1% (95% CI, 24.2%-34.0%) use of soap and water, and 37.0% (95% CI, 31.8%-42.4%) use of no hand hygiene. These findings support the need for ongoing infection prevention quality improvement initiatives in outpatient settings and underscore the importance of assessing both self-report and observed behavior of infection prevention compliance. Copyright © 2016 Association for Professionals in Infection Control and Epidemiology, Inc. Published by Elsevier Inc. All rights reserved.

  5. Improving the speech intelligibility in classrooms

    Science.gov (United States)

    Lam, Choi Ling Coriolanus

    One of the major acoustical concerns in classrooms is the establishment of effective verbal communication between teachers and students. Non-optimal acoustical conditions, resulting in reduced verbal communication, can cause two main problems. First, they can lead to reduce learning efficiency. Second, they can also cause fatigue, stress, vocal strain and health problems, such as headaches and sore throats, among teachers who are forced to compensate for poor acoustical conditions by raising their voices. Besides, inadequate acoustical conditions can induce the usage of public address system. Improper usage of such amplifiers or loudspeakers can lead to impairment of students' hearing systems. The social costs of poor classroom acoustics will be large to impair the learning of children. This invisible problem has far reaching implications for learning, but is easily solved. Many researches have been carried out that they have accurately and concisely summarized the research findings on classrooms acoustics. Though, there is still a number of challenging questions remaining unanswered. Most objective indices for speech intelligibility are essentially based on studies of western languages. Even several studies of tonal languages as Mandarin have been conducted, there is much less on Cantonese. In this research, measurements have been done in unoccupied rooms to investigate the acoustical parameters and characteristics of the classrooms. The speech intelligibility tests, which based on English, Mandarin and Cantonese, and the survey were carried out on students aged from 5 years old to 22 years old. It aims to investigate the differences in intelligibility between English, Mandarin and Cantonese of the classrooms in Hong Kong. The significance on speech transmission index (STI) related to Phonetically Balanced (PB) word scores will further be developed. Together with developed empirical relationship between the speech intelligibility in classrooms with the variations

  6. XQ-100: A legacy survey of one hundred 3.5 z < 4.5 quasars observed with VLT/XSHOOTER

    CERN Document Server

    Lopez, S; Ellison, S L; Becker, G D; Christensen, L; Cupani, G; Denney, K D; Paris, I; Worseck, G; Berg, T A M; Cristiani, S; Dessauges-Zavadsky, M; Haehnelt, M; Hamann, F; Hennawi, J; Irsic, V; Kim, T -S; Lopez, P; Saust, R Lund; Menard, B; Perrotta, S; Prochaska, J X; Sanchez-Ramirez, R; Vestergaard, M; Viel, M; Wisotzki, L

    2016-01-01

    We describe the execution and data reduction of the European Southern Observatory Large Programme "Quasars and their absorption lines: a legacy survey of the high-redshift universe with VLT/XSHOOTER" (hereafter `XQ-100'). XQ-100 has produced and made publicly available an homogeneous and high-quality sample of echelle spectra of 100 QSOs at redshifts z~3.5-4.5 observed with full spectral coverage from 315 to 2500 nm at a resolving power ranging from R~4000 to 7000, depending on wavelength. The median signal-to-noise ratios are 33, 25 and 43, as measured at rest-frame wavelengths 1700, 3000 and 3600 Angstrom, respectively. This paper provides future users of XQ-100 data with the basic statistics of the survey, along with details of target selection, data acquisition and data reduction. The paper accompanies the public release of all data products, including 100 reduced spectra. XQ-100 is the largest spectroscopic survey to date of high-redshift QSOs with simultaneous rest-frame UV/optical coverage, and as such...

  7. Classroom Climate among Teacher Education Mathematics Students

    Directory of Open Access Journals (Sweden)

    Polemer M. Cuarto

    2015-11-01

    Full Text Available Classroom climate has gained prominence as recent studies revealed its potentials as an effective mediator in the various motivational factors as well as an antecedent of academic performance outcome of the students. This descriptive-correlational study determined the level of classroom climate dimensions among teacher education students specializing in Mathematics at Mindoro State College of Agriculture and Technology. Employing a self-structured questionnaire adapted to the WIHIC (What Is Happening In this Class questionnaire, the surveyed data were treated statistically using Pearson’s r. Result showed that there was high level of classroom climate among the respondents in their Mathematics classes in both teacher-directed and student-directed dimensions specifically in terms of equity, teacher support, cohesiveness, involvement, responsibility and task orientation. Also, it revealed that equity and teacher support were both positively related to the students-directed classroom climate dimensions. With these results, teachers are seen to be very significant determinants of the climate in the classroom. Relevant to this, the study recommended that faculty should develop effective measures to enhance classroom climate dimensions such as equity and teacher support to address the needs of diverse studentsdespite large size classes. Moreover, faculty should provide greater opportunitiesfor the students to achieve higher level of responsibility, involvement, cohesiveness, and task orientation as these could motivate them to develop positive learning attitude, perform to the best of their ability, as well as maximize their full potential in school.

  8. Eight New Luminous z > 6 Quasars Selected via SED Model Fitting of VISTA, WISE and Dark Energy Survey Year 1 Observations

    Energy Technology Data Exchange (ETDEWEB)

    Reed, S.L.; et al.

    2017-01-17

    We present the discovery and spectroscopic confirmation with the ESO NTT and Gemini South telescopes of eight new 6.0 < z < 6.5 quasars with z$_{AB}$ < 21.0. These quasars were photometrically selected without any star-galaxy morphological criteria from 1533 deg$^{2}$ using SED model fitting to photometric data from the Dark Energy Survey (g, r, i, z, Y), the VISTA Hemisphere Survey (J, H, K) and the Wide-Field Infrared Survey Explorer (W1, W2). The photometric data was fitted with a grid of quasar model SEDs with redshift dependent Lyman-{\\alpha} forest absorption and a range of intrinsic reddening as well as a series of low mass cool star models. Candidates were ranked using on a SED-model based $\\chi^{2}$-statistic, which is extendable to other future imaging surveys (e.g. LSST, Euclid). Our spectral confirmation success rate is 100% without the need for follow-up photometric observations as used in other studies of this type. Combined with automatic removal of the main types of non-astrophysical contaminants the method allows large data sets to be processed without human intervention and without being over run by spurious false candidates. We also present a robust parametric redshift estimating technique that gives comparable accuracy to MgII and CO based redshift estimators. We find two z $\\sim$ 6.2 quasars with HII near zone sizes < 3 proper Mpc which could indicate that these quasars may be young with ages < 10$^6$ - 10$^7$ years or lie in over dense regions of the IGM. The z = 6.5 quasar VDESJ0224-4711 has J$_{AB}$ = 19.75 is the second most luminous quasar known with z > 6.5.

  9. SIRA Model of Classroom Observation Pointed to Biology Inquiry Teaching Level%探究式教学实施程度评价的一种探索:SIRA课堂观察模式

    Institute of Scientific and Technical Information of China (English)

    黄鹤; 马云鹏

    2012-01-01

    Nowadays, new curriculum reform pays much attention to inquiry teaching. This paper, based on the practical issue, introduces a quantitative curriculum observation SIRA model which comes from biology classroom practice. In addition, this model is independently developed and has highly associated with inquiry teaching implementation at junior level. This paper talks about where this model comes from, sets up four observation dimension based on the inquiry teaching nature analysis, and the observation point according to each dimension. SIRA model is simple, practical and easy to carry out.%探究式教学作为培养学生科学素养和自主精神的有效模式之一受到我国中小学广泛重视,并开展了多方面的实践探索。但是,当前中小学探究式教学课堂教学实施情况评价却处于“无标准”、“无证据化”状态,影响了探究式教学的有效实施。本文立足于实践,以教学主体为核心将探究式课堂教学实践划分为四个维度,即探究主体(Subject)、探究互动(Intemction)、探究资源(Resource)、探究能力(Ability),构建了SIRA课堂观察模式。该模式简单、实用、易操作,可用于不同学校、不同类型的探究式教学实践中。

  10. Survey of professional ethics observance degree among managers and staff of teaching hospitals of Shiraz University of Medical Sci

    Directory of Open Access Journals (Sweden)

    FARZAD MAHMOUDIAN

    2013-01-01

    Full Text Available Introduction: Professional ethics is a very important issue for managers who are role models for students and staff. It can also be very effective in organizational activities. The main objective of this research is to describe the result of managers’ self assessment in Shiraz teaching hospitals. Methods: The present research is a cross-sectional study. The statistical society of this research includes all senior, middle and executive managers of Nemazi, Faghihi and Chamran hospitals. Regarding the small volume of statistical society and advice of a statistical counselor, the census method was used. The data were gathered using questionnaires. Results: The result of this research showed that there was a significant association between managerial ethics and education levels but there wasn’t a significant association between average score of managerial ethics and the field of study, sex and age. Also the mean for managerial ethics was the highest in Faghihi hospital. Discussion: According to research findings and positive association between managerial ethics and education levels, observance of professional ethics is essential. So we can train managers to observe professional ethics more in their organizations in order to improve organizational efficacy.

  11. The Spitzer c2d Survey of Large, Nearby, Interstellar Clouds. I. Chamaeleon II Observed with MIPS

    CERN Document Server

    Young, K E; Allen, L E; Bertoldi, F; Blake, G A; Bourke, T L; Brooke, T Y; Chapman, N; Harvey, P M; Kauffmann, J; Körner, D W; Lai, S P; Mundy, L G; Myers, P C; Padgett, D L; Salinas, A; Sargent, A I; Spiesman, W; Stapelfeldt, K R; Teuben, P; Van Dishoeck, E F; Wahhaj, Z

    2005-01-01

    We present maps of over 1.5 square degrees in Chamaeleon (Cha) II at 24, 70, and 160 micron observed with the Spitzer Space Telescope Multiband Imaging Photometer for Spitzer (MIPS) and a 1.2 square degree millimeter map from SIMBA on the Swedish-ESO Submillimetre Telescope (SEST). The c2d Spitzer Legacy Team's data reduction pipeline is described in detail. Over 1500 24 micron sources and 41 70 micron sources were detected by MIPS with fluxes greater than 10-sigma. More than 40 potential YSOs are identified with a MIPS and 2MASS color-color diagram and by their spectral indices, including two previously unknown sources with 24 micron excesses. Our new SIMBA millimeter map of Cha II shows that only a small fraction of the gas is in compact structures with high column densities. The extended emission seen by MIPS is compared with previous CO observations. Some selected interesting sources, including two detected at 1 mm, associated with Cha II are discussed in detail and their SEDs presented. The classificatio...

  12. Chandra X-ray Observations of the 0.6 < z < 1.1 Red-Sequence Cluster Survey Sample

    CERN Document Server

    Hicks, Amalia K; Bautz, Mark; Cain, Benjamin; Gilbank, David; Gladders, M D; Hoekstra, Henk; Yee, Howard; Garmire, Gordon

    2007-01-01

    We present the results of Chandra observations of 13 optically-selected clusters with 0.63; though 3 were not observed long enough to support detailed analysis. Surface brightness profiles are fit to beta-models. Integrated spectra are extracted within R(2500), and Tx and Lx information is obtained. We derive gas and total masses within R(2500) and R(500). Cosmologically corrected scaling relations are investigated, and we find the RCS clusters to be consistent with self-similar scaling expectations. However discrepancies exist between the RCS sample and lower-z X-ray selected samples for relationships involving Lx, with the higher-z RCS clusters having lower Lx for a given Tx. In addition, we find that gas mass fractions within R(2500) for the high-z RCS sample are lower than expected by a factor of ~2. This suggests that the central entropy of these high-z objects has been elevated by processes such as pre-heating, mergers, and/or AGN outbursts, that their gas is still infalling, or that they contain compar...

  13. Evidence of AGB pollution in Galactic globular clusters from the Mg-Al anticorrelations observed by the APOGEE survey

    CERN Document Server

    Ventura, P; Dell'Agli, F; D'Antona, F; Meszaros, Sz; Lucatello, S; Di Criscienzo, M; Shetrone, M; Tailo, M; Tang, Baitian; Zamora, O

    2016-01-01

    We study the formation of multiple populations in globular clusters (GC), under the hypothesis that stars in the second generation formed from the winds of intermediate-mass stars, ejected during the asymptotic giant branch (AGB) phase, possibly diluted with pristine gas, sharing the same chemical composition of first-generation stars. To this aim, we use the recent APOGEE data, which provide the surface chemistry of a large sample of giant stars, belonging to clusters that span a wide metallicity range. The APOGEE data set is particularly suitable to discriminate among the various pollution scenarios proposed so far, as it provides the surface abundances of Mg and Al, the two elements involved in a nuclear channel extremely sensitive to the temperature, hence to the metallicity of the polluters. The present analysis shows a remarkable agreement between the observations and the theoretical yields from massive AGB stars. In particular, the observed extension of the depletion of Mg and O and the increase in Al ...

  14. Evidence of AGB Pollution in Galactic Globular Clusters from the Mg-Al Anticorrelations Observed by the APOGEE Survey

    Science.gov (United States)

    Ventura, P.; García-Hernández, D. A.; Dell'Agli, F.; D'Antona, F.; Mészáros, Sz.; Lucatello, S.; Di Criscienzo, M.; Shetrone, M.; Tailo, M.; Tang, Baitian; Zamora, O.

    2016-11-01

    We study the formation of multiple populations in globular clusters (GCs), under the hypothesis that stars in the second generation formed from the winds of intermediate-mass stars, ejected during the asymptotic giant branch (AGB) phase, possibly diluted with pristine gas, sharing the same chemical composition of first-generation stars. To this aim, we use the recent Apache Point Observatory Galactic Evolution Experiment (APOGEE) data, which provide the surface chemistry of a large sample of giant stars, belonging to clusters that span a wide metallicity range. The APOGEE data set is particularly suitable to discriminate among the various pollution scenarios proposed so far, as it provides the surface abundances of Mg and Al, the two elements involved in a nuclear channel extremely sensitive to the temperature, hence to the metallicity of the polluters. The present analysis shows a remarkable agreement between the observations and the theoretical yields from massive AGB stars. In particular, the observed extension of the depletion of Mg and O and the increase in Al is well reproduced by the models and the trend with the metallicity is also fully accounted for. This study further supports the idea that AGB stars were the key players in the pollution of the intra-cluster medium, from which additional generations of stars formed in GCs.

  15. Spectroscopic survey of Kepler stars - II. FIES/NOT observations of A- and F-type stars

    Science.gov (United States)

    Niemczura, E.; Polińska, M.; Murphy, S. J.; Smalley, B.; Kołaczkowski, Z.; Jessen-Hansen, J.; Uytterhoeven, K.; Lykke, J. M.; Triviño Hage, A.; Michalska, G.

    2017-09-01

    We have analysed high-resolution spectra of 28 A and 22 F stars in the Kepler field, observed using the Fibre-Fed Échelle Spectrograph at the Nordic Optical Telescope. We provide spectral types, atmospheric parameters and chemical abundances for 50 stars. Balmer, Fe i and Fe ii lines were used to derive effective temperatures, surface gravities and microturbulent velocities. We determined chemical abundances and projected rotational velocities using a spectrum synthesis technique. Effective temperatures calculated by spectral energy distribution fitting are in good agreement with those determined from the spectral line analysis. The stars analysed include chemically peculiar stars of the Am and λ Boo types, as well as stars with approximately solar chemical abundances. The wide distribution of projected rotational velocity, vsin i, is typical for A and F stars. The microturbulence velocities obtained are typical for stars in the observed temperature and surface gravity ranges. Moreover, we affirm the results of Niemczura et al. that Am stars do not have systematically higher microturbulent velocities than normal stars of the same temperature.

  16. Improving Instruction through Teacher Observation.

    Science.gov (United States)

    Protheroe, Nancy

    2002-01-01

    Describes classroom observation techniques focusing on what the students are learning rather than how the teacher is teaching. Highlights research on effective teaching; provides examples of programs to teach principals effective classroom observation and teacher-evaluation techniques; emphasizes link between teacher evaluation and professional…

  17. XQ-100: A legacy survey of one hundred 3.5 ≲ z ≲ 4.5 quasars observed with VLT/X-shooter

    Science.gov (United States)

    López, S.; D'Odorico, V.; Ellison, S. L.; Becker, G. D.; Christensen, L.; Cupani, G.; Denney, K. D.; Pâris, I.; Worseck, G.; Berg, T. A. M.; Cristiani, S.; Dessauges-Zavadsky, M.; Haehnelt, M.; Hamann, F.; Hennawi, J.; Iršič, V.; Kim, T.-S.; López, P.; Lund Saust, R.; Ménard, B.; Perrotta, S.; Prochaska, J. X.; Sánchez-Ramírez, R.; Vestergaard, M.; Viel, M.; Wisotzki, L.

    2016-10-01

    We describe the execution and data reduction of the European Southern Observatory Large Programme "Quasars and their absorption lines: a legacy survey of the high-redshift Universe with VLT/X-shooter" (hereafter "XQ-100"). XQ-100 has produced and made publicly available a homogeneous and high-quality sample of echelle spectra of 100 quasars (QSOs) at redshifts z ≃ 3.5-4.5 observed with full spectral coverage from 315 to 2500 nm at a resolving power ranging from R ~ 4000 to 7000, depending on wavelength. The median signal-to-noise ratios are 33, 25 and 43, as measured at rest-frame wavelengths 1700, 3000 and 3600 Å, respectively. This paper provides future users of XQ-100 data with the basic statistics of the survey, along with details of target selection, data acquisition and data reduction. The paper accompanies the public release of all data products, including 100 reduced spectra. XQ-100 is the largest spectroscopic survey to date of high-redshift QSOs with simultaneous rest-frame UV/optical coverage, and as such enables a wide range of extragalactic research, from cosmology and galaxy evolution to AGN astrophysics. Based on observations made with ESO Telescopes at the La Silla Paranal Observatory under programme ID 189.A-0424.The XQ-100 raw data and the XQ-100 Science Data Products can be found at http://archive.eso.org/eso/eso_archive_main.html and http://archive.eso.org/wdb/wdb/adp/phase3_main/form, respectively.

  18. ISO deep far-infrared survey in the ``Lockman Hole''. A search for obscured objects at high redshift. I. Observations

    Science.gov (United States)

    Kawara, K.; Sato, Y.; Matsuhara, H.; Taniguchi, Y.; Okuda, H.; Sofue, Y.; Matsumoto, T.; Wakamatsu, K.; Karoji, H.; Okamura, S.; Chambers, K. C.; Cowie, L. L.; Joseph, R. D.; Sanders, D. B.

    1998-08-01

    Two 44arcmin x 44arcmin fields in the Lockman Hole were mapped at 95 mu m and 175 mu m using ISOPHOT. A simple program code combined with PIA works well to correct for drift in the detector responsivity. The number density of 175 mu m sources is 3-10 times higher than expected from the no-evolution model. Based on observations with ISO, an ESA project with instruments funded by ESA member states (especially the PI countries: France, Germany, the Netherlands, and the United Kingdom) and with the participation of ISAS and NASA. The ISOPHOT data presented in this paper was reduced using PIA, which is a joint development by the ESA Astrophysics Division and the ISOPHOT consortium led by the Max Plank Institute for Astronomy (MPIA), Heidelberg.

  19. Optical & Sunyaev-Zel'dovich Observations of a New Sample of Distant Rich Galaxy Clusters in the ROSAT All Sky Survey

    CERN Document Server

    Buddendiek, A; Greer, C H; Hoekstra, H; Sommer, M; Eifler, T; Erben, T; Erler, J; Hicks, A K; High, F W; Hildebrandt, H; Marrone, D P; Morris, R G; Muzzin, A; Reiprich, T H; Schirmer, M; Schneider, P; von der Linden, A

    2014-01-01

    Finding a sample of the most massive clusters with redshifts $z>0.6$ can provide an interesting consistency check of the $\\Lambda$CDM model. Here we present results from our search for clusters with $0.6Survey DR8. Our survey thus covers $\\approx10,000\\,\\rm{deg^2}$, much larger than previous studies. Deeper follow-up observations in three bands using the William Herrschel Telescope and the Large Binocular Telescope were performed to confirm the candidates, resulting in a sample of 44 clusters for which we present richnesses and red sequence redshifts, as well as spectroscopic redshifts for a subset. At least two of the clusters in our sample are comparable in richness to RCS2-$J$232727.7$-$020437, one of the richest systems discovered to date. We also obtained new observations with the Combined Array for Research in Millimeter Astronomy for a subs...

  20. Campaign 9 of the $K2$ Mission: Observational Parameters, Scientific Drivers, and Community Involvement for a Simultaneous Space- and Ground-based Microlensing Survey

    CERN Document Server

    Henderson, Calen B; Street, Rachel A; Bennett, David P; Hogg, David W; Poleski, R; Barclay, T; Barentsen, G; Howell, S B; Udalski, A; Szymański, M K; Skowron, J; Mróz, P; Kozłowski, S; Wyrzykowski, Ł; Pietrukowicz, P; Soszyński, I; Ulaczyk, K; Pawlak, M; Sumi, T; Abe, F; Asakura, Y; Barry, R K; Bhattacharya, A; Bond, I A; Donachie, M; Freeman, M; Fukui, A; Hirao, Y; Itow, Y; Koshimoto, N; Li, M C A; Ling, C H; Masuda, K; Matsubara, Y; Muraki, Y; Nagakane, M; Ohnishi, K; Oyokawa, H; Rattenbury, N; Saito, To; Sharan, A; Sullivan, D J; Tristram, P J; Yonehara, A; Bachelet, E; Bramich, D A; Cassan, A; Dominik, M; Jaimes, R Figuera; Horne, K; Hundertmark, M; Mao, S; Ranc, C; Schmidt, R; Snodgrass, C; Steele, I A; Tsapras, Y; Wambsganss, J; Akeson, R; Batista, V; Beaulieu, J -P; Beichman, C A; Bozza, V; Bryden, G; Ciardi, D; Cole, A; Coutures, C; Dong, S; Foreman-Mackey, D; Fouqué, P; Gaudi, B S; Kerins, E; Korhonen, H; Jørgensen, U; Lang, D; Lineweaver, C; Marquette, J -B; Mogavero, Federico; Morales, J C; Nataf, D; Pogge, R W; Santerne, A; Shvartzvald, Y; Suzuki, D; Tamura, M; Tisserand, P; Wang, D; Zhu, W

    2016-01-01

    $K2$'s Campaign 9 ($K2$C9) will conduct a $\\sim$3.4 deg$^{2}$ survey toward the Galactic bulge from 7/April through 1/July of 2016 that will leverage the spatial separation between $K2$ and the Earth to facilitate measurement of the microlens parallax $\\pi_{\\rm E}$ for $\\gtrsim$120 microlensing events, including several planetary in nature as well as many short-timescale microlensing events, which are potentially indicative of free-floating planets (FFPs). These satellite parallax measurements will in turn allow for the direct measurement of the masses of and distances to the lensing systems. In this white paper we provide an overview of the $K2$C9 space- and ground-based microlensing survey. Specifically, we detail the demographic questions that can be addressed by this program, including the frequency of FFPs and the Galactic distribution of exoplanets, the observational parameters of $K2$C9, and the array of ground-based resources dedicated to concurrent observations. Finally, we outline the avenues throug...