WorldWideScience

Sample records for jwst science working

  1. Progress by the JWST Science Working Group

    Science.gov (United States)

    Gardner, Jonathan P.

    2007-01-01

    The JWST Science Working Group recently published a comprehensive, top-level review of JWST science in the journal Space Science Reviews (Gardner et al. 2006, SSR, 123, 485). That review paper gives details of the 4 JWST science themes, and describes the design of the observatory and ground system. Since publication, the SWG, working with members of the astronomical community, has continued to develop the science case for JWST, giving more details in a series of white papers. The white paper topics include first light, galaxy surveys, AGN, supernovae, stellar populations, and exoplanets. The white papers are in various stages of completion. In this poster, I will review recent progress.

  2. Status of the JWST Science Instrument Payload

    Science.gov (United States)

    Greenhouse, Matt

    2016-01-01

    The James Webb Space Telescope (JWST) Integrated Science Instrument Module (ISIM) system consists of five sensors (4 science): Mid-Infrared Instrument (MIRI), Near Infrared Imager and Slitless Spectrograph (NIRISS), Fine Guidance Sensor (FGS), Near InfraRed Camera (NIRCam), Near InfraRed Spectrograph (NIRSpec); and nine instrument support systems: Optical metering structure system, Electrical Harness System; Harness Radiator System, ISIM Electronics Compartment, ISIM Remote Services Unit, Cryogenic Thermal Control System, Command and Data Handling System, Flight Software System, Operations Scripts System.

  3. JWST science instrument pupil alignment measurements

    Science.gov (United States)

    Kubalak, Dave; Sullivan, Joe; Ohl, Ray; Antonille, Scott; Beaton, Alexander; Coulter, Phillip; Hartig, George; Kelly, Doug; Lee, David; Maszkiewicz, Michael; Schweiger, Paul; Telfer, Randal; Te Plate, Maurice; Wells, Martyn

    2016-09-01

    NASA's James Webb Space Telescope (JWST) is a 6.5m diameter, segmented, deployable telescope for cryogenic IR space astronomy ( 40K). The JWST Observatory architecture includes the Optical Telescope Element (OTE) and the Integrated Science Instrument Module (ISIM) element that contains four science instruments (SI), including a guider. OSIM is a full field, cryogenic, optical simulator of the JWST OTE. It is the "Master Tool" for verifying the cryogenic alignment and optical performance of ISIM by providing simulated point source/star images to each of the four Science Instruments in ISIM. Included in OSIM is a Pupil Imaging Module (PIM) - a large format CCD used for measuring pupil alignment. Located at a virtual stop location within OSIM, the PIM records superimposed shadow images of pupil alignment reference (PAR) targets located in the OSIM and SI pupils. The OSIM Pupil Imaging Module was described by Brent Bos, et al, at SPIE in 2011 prior to ISIM testing. We have recently completed the third and final ISIM cryogenic performance verification test before ISIM was integrated with the OTE. In this paper, we describe PIM implementation, performance, and measurement results.

  4. The JWST science instrument payload: mission context and status

    Science.gov (United States)

    Greenhouse, Matthew A.

    2016-07-01

    The James Webb Space Telescope (JWST) is the scientific successor to the Hubble Space Telescope. It is a cryogenic infrared space observatory with a 25 m2 aperture (6 m class) telescope that will achieve diffraction limited angular resolution at a wavelength of 2 um. The science instrument payload includes four passively cooled near-infrared instruments providing broad- and narrow-band imagery, coronography, as well as multi-object and integral-field spectroscopy over the 0.6 Construction, integration and verification testing is underway in all areas of the program. The JWST is on schedule for launch during 2018.

  5. Titan Science with the James Webb Space Telescope (JWST)

    CERN Document Server

    Nixon, Conor A; Adamkovics, Mate; Bezard, Bruno; Bjoraker, Gordon L; Cornet, Thomas; Hayes, Alexander G; Lellouch, Emmanuel; Lemmon, Mark T; Lopez-Puertas, Manuel; Rodriguez, Sebastien; Sotin, Christophe; Teanby, Nicholas A; Turtle, Elizabeth P; West, Robert A

    2015-01-01

    The James Webb Space Telescope (JWST), scheduled for launch in 2018, is the successor to the Hubble Space Telescope (HST) but with a significantly larger aperture (6.5 m) and advanced instrumentation focusing on infrared science (0.6-28.0 $\\mu$m ). In this paper we examine the potential for scientific investigation of Titan using JWST, primarily with three of the four instruments: NIRSpec, NIRCam and MIRI, noting that science with NIRISS will be complementary. Five core scientific themes are identified: (i) surface (ii) tropospheric clouds (iii) tropospheric gases (iv) stratospheric composition and (v) stratospheric hazes. We discuss each theme in depth, including the scientific purpose, capabilities and limitations of the instrument suite, and suggested observing schemes. We pay particular attention to saturation, which is a problem for all three instruments, but may be alleviated for NIRCam through use of selecting small sub-arrays of the detectors - sufficient to encompass Titan, but with significantly fas...

  6. Bringing the Science of JWST to the Public

    Science.gov (United States)

    Green, Joel D.; Smith, Denise A.; Lawton, Brandon L.; Meinke, Bonnie K.; Jirdeh, Hussein

    2017-01-01

    The James Webb Space Telescope is the successor to the Hubble Space Telescope. STScI and the Office of Public Outreach are committed to bringing awareness of the technology, the excitement, and the future science potential of this great observatory to the public and to the scientific community, prior to its 2018 launch. The challenges in ensuring the high profile of JWST (understanding the infrared, the vast distance to the telescope's final position, and the unfamiliar science territory) requires us to lay the proper background, particularly in the area of spectroscopy. We currently engage the full range of the public and scientific communities using a variety of high impact, memorable initiatives, in combination with modern technologies to extend reach, linking the science goals of Webb to the ongoing discoveries being made by Hubble. Webbtelescope.org, the public hub for scientific information related to JWST, is now open. We have injected Webb-specific content into ongoing outreach programs: for example, partnering with high impact science communicators such as MinutePhysics to produce timely and concise content; partnering with musicians and artists to link science and art. Augmented reality apps showcase NASA’s telescopes in a format usable by anyone with a smartphone, and visuals from increasingly affordable 3D VR technologies.

  7. Observing Planetary Rings with JWST: Science Justification and Observation Requirements

    CERN Document Server

    Tiscareno, Matthew S; Cuzzi, Jeffrey N; de Pater, Imke; Hamilton, Douglas P; Hedman, Matthew M; Nicholson, Philip D; Showalter, Mark R; Tamayo, Daniel; Verbiscer, Anne J

    2014-01-01

    The rings that adorn the four giant planets are of prime importance as accessible natural laboratories for disk processes, as clues to the origin and evolution of planetary systems, and as shapers as well as detectors of their planetary environments. The retinue of small moons accompanying all known ring systems are intimately connected as both sources and products, as well as shepherds and perturbers, of the rings. Leading sources of data on ring systems include spacecraft such as Cassini and Voyager, but also space telescopes such as Hubble and Spitzer as well as ground-based telescopes. The James Webb Space Telescope (JWST) is being prepared for launch in 2018 to begin a planned five-year mission. JWST will have the capability to observe solar system objects as close as Mars. Although most of the hardware is already designed and under construction if not completed, work continues on the development of operations guidelines and software and the completion of calibration tasks. The purpose of this white pape...

  8. Community Targets for JWST's Early Release Science Program: Evaluation of Transiting Exoplanet WASP-63b.

    Science.gov (United States)

    Kilpatrick, Brian; Cubillos, Patricio; Bruno, Giovanni; Lewis, Nikole K.; Stevenson, Kevin B.; Wakeford, Hannah; Blecic, Jasmina; Burrows, Adam Seth; Deming, Drake; Heng, Kevin; Line, Michael R.; Madhusudhan, Nikku; Morley, Caroline; Waldmann, Ingo P.; Transiting Exoplanet Early Release Science Community (Stevenson et al. 2016)

    2017-06-01

    We present observations of the Hubble Space Telescope (HST) ``A Preparatory Program to Identify the Single Best Transiting Exoplanet for JWST Early Release Science" for WASP-63b, one of the community targets proposed for the James Webb Space Telescope (JWST) Early Release Science (ERS) program. A large collaboration of transiting exoplanet scientists identified a set of ``community targets" which meet a certain set of criteria for ecliptic latitude, period, host star brightness, well constrained orbital parameters, and strength of spectroscopic features. WASP-63b was one of the targets identified as a potential candidate for the ERS program. It is presented as an inflated planet with a large signal. It will be accessible to JWST approximately six months after the planned start of Cycle 1/ERS in April 2019 making it an ideal candidate should there be any delays in the JWST timetable. Here, we observe WASP-63b to evaluate its suitability as the best target to test the capabilities of JWST. Ideally, a clear atmosphere will be best suited for bench marking the instruments ability to detect spectroscopic features. We can use the strength of the water absorption feature at 1.4 μm as a way to determine the presence of obscuring clouds/hazes. The results of atmospheric retrieval are presented along with a discussion on the suitability of WASP-63b as the best target to be observed during the ERS Program.

  9. Cryo-vacuum testing of the JWST Integrated Science Instrument Module (SPIE)

    Science.gov (United States)

    Kimble, Randy A.; Vila, M. Begona; Van Campen, Julie; Birkmann, Stephan M.; Comber, Brian J.; Fatig, Curtis C.; Glasse, Alistair C. H.; Glazer, Stuart D.; Kelly, Douglas M.; Mann, Steven D.; Martel, Andre R.; Novo-Gradac, Kevin J.; Ohl, Raymond G.; Penanen, Konstantin; Rohrbach, Scott O.; Sullivan, Joseph F.; Zak, Dean; Zhou, Julia

    2016-01-01

    In late 2015/early 2016, a major cryo-vacuum test was carried out for the Integrated Science Instrument Module (ISIM) of the James Webb Space Telescope (JWST). This test comprised the final cryo-certification and calibration test of the ISIM, after its ambient environmental test program (vibration, acoustics, EMI/EMC), and before its delivery for integration with the rest of the JWST observatory. Over the 108-day period of the round-the-clock test program, the full complement of ISIM flight instruments, structure, harness radiator, and electronics were put through a comprehensive program of thermal, optical, electrical, and operational tests. The test verified the health and excellent performance of the instruments and ISIM systems, proving the ISIM element's readiness for integration with the telescope. We report here on the context, goals, setup, execution, and key results for this critical JWST milestone.

  10. Transiting Exoplanet Studies and Community Targets for JWST's Early Release Science Program

    CERN Document Server

    Stevenson, Kevin B; Bean, Jacob L; Beichman, Charles; Fraine, Jonathan; Kilpatrick, Brian M; Krick, J E; Lothringer, Joshua D; Mandell, Avi M; Valenti, Jeff A; Agol, Eric; Angerhausen, Daniel; Barstow, Joanna K; Birkmann, Stephan M; Burrows, Adam; Cowan, Nicolas B; Crouzet, Nicolas; Cubillos, Patricio E; Curry, S M; Dalba, Paul A; de Wit, Julien; Deming, Drake; Desert, Jean-Michel; Doyon, Rene; Dragomir, Diana; Ehrenreich, David; Fortney, Jonathan J; Munoz, Antonio Garcia; Gibson, Neale P; Gizis, John E; Greene, Thomas P; Harrington, Joseph; Heng, Kevin; Kataria, Tiffany; Kempton, Eliza M -R; Knutson, Heather; Kreidberg, Laura; Lafreniere, David; Lagage, Pierre-Olivier; Line, Michael R; Lopez-Morales, Mercedes; Madhusudhan, Nikku; Morley, Caroline V; Rocchetto, Marco; Schlawin, Everett; Shkolnik, Evgenya L; Shporer, Avi; Sing, David K; Todorov, Kamen O; Tucker, Gregory S; Wakeford, Hannah R

    2016-01-01

    The James Webb Space Telescope will revolutionize transiting exoplanet atmospheric science due to its capability for continuous, long-duration observations and its larger collecting area, spectral coverage, and spectral resolution compared to existing space-based facilities. However, it is unclear precisely how well JWST will perform and which of its myriad instruments and observing modes will be best suited for transiting exoplanet studies. In this article, we describe a prefatory JWST Early Release Science (ERS) program that focuses on testing specific observing modes to quickly give the community the data and experience it needs to plan more efficient and successful future transiting exoplanet characterization programs. We propose a multi-pronged approach wherein one aspect of the program focuses on observing transits of a single target with all of the recommended observing modes to identify and understand potential systematics, compare transmission spectra at overlapping and neighboring wavelength regions...

  11. Transiting Exoplanet Studies and Community Targets for JWST's Early Release Science Program

    Science.gov (United States)

    Stevenson, Kevin B.; "Enabling Transiting Exoplanet Science with JWST" workshop attendees

    2016-10-01

    The James Webb Space Telescope (JWST) will likely revolutionize transiting exoplanet atmospheric science; however, it is unclear precisely how well it will perform and which of its myriad instruments and observing modes will be best suited for transiting exoplanet studies. We will describe a prefatory JWST Early Release Science (ERS) Cycle 1 program that focuses on testing specific observing modes to quickly give the community the data and experience it needs to plan more efficient and successful transiting exoplanet characterization programs in later cycles. We will also present a list of "community targets" that are well suited to achieving these goals. Since most of the community targets do not have well-characterized atmospheres, we have initiated a preparatory HST + Spitzer observing program to determine the presence of obscuring clouds/hazes within their atmospheres. Measurable spectroscopic features are needed to establish the optimal resolution and wavelength regions for exoplanet characterization. We will present preliminary results from this preparatory observing program and discuss their implications on the pending JWST ERS proposal deadline in mid-2017.

  12. Transiting Exoplanet Studies and Community Targets for JWST's Early Release Science Program

    Science.gov (United States)

    Stevenson, Kevin B.; Lewis, Nikole K.; Bean, Jacob L.; Beichman, Charles A.; Fraine, Jonathan; Kilpatrick, Brian M.; Krick, J. E.; Lothringer, Joshua D.; Mandell, Avi M.; Valenti, Jeff A.; Agol, Eric; Angerhausen, Daniel; Barstow, Joanna K.; Birkmann, Stephan M.; Burrows, Adam; Charbonneau, David; Cowan, Nicolas B.; Greene, Thomas P.; Line, Michael R.; Wakeford, Hanna R.

    2016-01-01

    The James Webb Space Telescope (JWST) will likely revolutionize transiting exoplanet atmospheric science, due to a combination of its capability for continuous, long duration observations and its larger collecting area, spectral coverage, and spectral resolution compared to existing space-based facilities. However, it is unclear precisely how well JWST will perform and which of its myriad instruments and observing modes will be best suited for transiting exoplanet studies. In this article, we describe a prefatory JWST Early Release Science (ERS) Cycle 1 program that focuses on testing specific observing modes to quickly give the community the data and experience it needs to plan more efficient and successful transiting exoplanet characterization programs in later cycles. We propose a multi-pronged approach wherein one aspect of the program focuses on observing transits of a single target with all of the recommended observing modes to identify and understand potential systematics, compare transmission spectra at overlapping and neighboring wavelength regions, confirm throughputs, and determine overall performances. In our search for transiting exoplanets that are well suited to achieving these goals, we identify 12 objects (dubbed community targets'') that meet our defined criteria. Currently, the most favorable target is WASP-62b because of its large predicted signal size, relatively bright host star, and location in JWST's continuous viewing zone. Since most of the community targets do not have well-characterized atmospheres, we recommend initiating preparatory observing programs to determine the presence of obscuring clouds/hazes within their atmospheres. Measurable spectroscopic features are needed to establish the optimal resolution and wavelength regions for exoplanet characterization. Other initiatives from our proposed ERS program include testing the instrument brightness limits and performing phase-curve observations. The latter are a unique challenge

  13. Transiting Exoplanet Studies and Community Targets for JWST's Early Release Science Program

    Science.gov (United States)

    Stevenson, Kevin B.; Lewis, Nikole K.; Bean, Jacob L.; Beichman, Charles; Fraine, Jonathan; Kilpatrick, Brian M.; Krick, J. E.; Lothringer, Joshua D.; Mandell, Avi M.; Valenti, Jeff A.; Agol, Eric; Angerhausen, Daniel; Barstow, Joanna K.; Birkmann, Stephan M.; Burrows, Adam; Charbonneau, David; Cowan, Nicolas B.; Crouzet, Nicolas; Cubillos, Patricio E.; Curry, S. M.; Dalba, Paul A.; de Wit, Julien; Deming, Drake; Désert, Jean-Michel; Doyon, René; Dragomir, Diana; Ehrenreich, David; Fortney, Jonathan J.; García Muñoz, Antonio; Gibson, Neale P.; Gizis, John E.; Greene, Thomas P.; Harrington, Joseph; Heng, Kevin; Kataria, Tiffany; Kempton, Eliza M.-R.; Knutson, Heather; Kreidberg, Laura; Lafrenière, David; Lagage, Pierre-Olivier; Line, Michael R.; Lopez-Morales, Mercedes; Madhusudhan, Nikku; Morley, Caroline V.; Rocchetto, Marco; Schlawin, Everett; Shkolnik, Evgenya L.; Shporer, Avi; Sing, David K.; Todorov, Kamen O.; Tucker, Gregory S.; Wakeford, Hannah R.

    2016-09-01

    The James Webb Space Telescope (JWST) will likely revolutionize transiting exoplanet atmospheric science, due to a combination of its capability for continuous, long duration observations and its larger collecting area, spectral coverage, and spectral resolution compared to existing space-based facilities. However, it is unclear precisely how well JWST will perform and which of its myriad instruments and observing modes will be best suited for transiting exoplanet studies. In this article, we describe a prefatory JWST Early Release Science (ERS) Cycle 1 program that focuses on testing specific observing modes to quickly give the community the data and experience it needs to plan more efficient and successful transiting exoplanet characterization programs in later cycles. We propose a multi-pronged approach wherein one aspect of the program focuses on observing transits of a single target with all of the recommended observing modes to identify and understand potential systematics, compare transmission spectra at overlapping and neighboring wavelength regions, confirm throughputs, and determine overall performances. In our search for transiting exoplanets that are well suited to achieving these goals, we identify 12 objects (dubbed “community targets”) that meet our defined criteria. Currently, the most favorable target is WASP-62b because of its large predicted signal size, relatively bright host star, and location in JWST's continuous viewing zone. Since most of the community targets do not have well-characterized atmospheres, we recommend initiating preparatory observing programs to determine the presence of obscuring clouds/hazes within their atmospheres. Measurable spectroscopic features are needed to establish the optimal resolution and wavelength regions for exoplanet characterization. Other initiatives from our proposed ERS program include testing the instrument brightness limits and performing phase-curve observations. The latter are a unique challenge

  14. Cryogenic Thermal Distortion Model Validation for the JWST ISIM Structure

    Science.gov (United States)

    Johnston, John; Cofie, Emmanuel

    2011-01-01

    The James Webb Space Telescope (JWST) is a large, infrared-optimized space telescope consisting of an Optical telescope element (OTE), Integrated science instrument module (ISIM), a Spacecraft, and a Sunshield. The Integrated Science Instrument Module (ISIM) consists of the JWST science instruments (NIRCam, MIRI, NIRSpec), a fine guidance sensor (FGS), the ISIM Structure, and thermal and electrical subsystems. JWST's instruments are designed to work primarily in the infrared range of the electromagnetic spectrum, and the instruments and telescope operate at cryogenic temperatures (approximately 35 K for the instruments).

  15. Observing Outer Planet Satellites (except Titan) with JWST: Science Justification and Observational Requirements

    CERN Document Server

    Keszthelyi, Laszlo; Stansberry, John; Sivaramakrishnan, Anand; Thatte, Deepashri; Gudipati, Murthy; Tsang, Constantine; Greenbaum, Alexandra; McGruder, Chima

    2015-01-01

    The James Webb Space Telescope (JWST) will allow observations with a unique combination of spectral, spatial, and temporal resolution for the study of outer planet satellites within our Solar System. We highlight the infrared spectroscopy of icy moons and temporal changes on geologically active satellites as two particularly valuable avenues of scientific inquiry. While some care must be taken to avoid saturation issues, JWST has observation modes that should provide excellent infrared data for such studies.

  16. Observing outer planet satellites (except Titan) with JWST: Science justification and observational requirements

    Science.gov (United States)

    Kestay, Laszlo P.; Grundy, Will; Stansberry, John; Sivaramakrishnan, Anand; Thatte, Deepashri; Gudipati, Murthy; Tsang, Constantine; Greenbaum, Alexandra; McGruder, Chima

    2016-01-01

    The James Webb Space Telescope (JWST) will allow observations with a unique combination of spectral, spatial, and temporal resolution for the study of outer planet satellites within our Solar System. We highlight the infrared spectroscopy of icy moons and temporal changes on geologically active satellites as two particularly valuable avenues of scientific inquiry. While some care must be taken to avoid saturation issues, JWST has observation modes that should provide excellent infrared data for such studies.

  17. Solar System Observations with JWST

    Science.gov (United States)

    Norwood, James; Hammel, Heidi; Milam, Stefanie; Stansberry, John; Lunine, Jonathan; Chanover, Nancy; Hines, Dean; Sonneborn, George; Tiscareno, Matthew; Brown, Michael; Ferruit, Pierre

    2014-01-01

    The James Webb Space Telescope will enable a wealth of new scientific investigations in the near- and mid- infrared, with sensitivity and spatial-spectral resolution greatly surpassing its predecessors. In this paper, we focus upon Solar System science facilitated by JWST, discussing the most current information available concerning JWST instrument properties and observing techniques relevant to planetary science. We also present numerous example observing scenarios for a wide variety of Solar System targets to illustrate the potential of JWST science to the Solar System community. This paper updates and supersedes the Solar System white paper published by the JWST Project in 2010 (Lunine et al., 2010). It is based both on that paper and on a workshop held at the annual meeting of the Division for Planetary Sciences in Reno, NV in 2012.

  18. Wavefront-Error Performance Characterization for the James Webb Space Telescope (JWST) Integrated Science Instrument Module (ISIM) Science Instruments

    Science.gov (United States)

    Aronstein, David L.; Smith, J. Scott; Zielinski, Thomas P.; Telfer, Randal; Tournois, Severine C.; Moore, Dustin B.; Fienup, James R.

    2016-01-01

    The science instruments (SIs) comprising the James Webb Space Telescope (JWST) Integrated Science Instrument Module (ISIM) were tested in three cryogenic-vacuum test campaigns in the NASA Goddard Space Flight Center (GSFC)'s Space Environment Simulator (SES) test chamber. In this paper, we describe the results of optical wavefront-error performance characterization of the SIs. The wavefront error is determined using image-based wavefront sensing, and the primary data used by this process are focus sweeps, a series of images recorded by the instrument under test in its as-used configuration, in which the focal plane is systematically changed from one image to the next. High-precision determination of the wavefront error also requires several sources of secondary data, including 1) spectrum, apodization, and wavefront-error characterization of the optical ground-support equipment (OGSE) illumination module, called the OTE Simulator (OSIM), 2) F-number and pupil-distortion measurements made using a pseudo-nonredundant mask (PNRM), and 3) pupil geometry predictions as a function of SI and field point, which are complicated because of a tricontagon-shaped outer perimeter and small holes that appear in the exit pupil due to the way that different light sources are injected into the optical path by the OGSE. One set of wavefront-error tests, for the coronagraphic channel of the Near-Infrared Camera (NIRCam) Longwave instruments, was performed using data from transverse translation diversity sweeps instead of focus sweeps, in which a sub-aperture is translated and/or rotated across the exit pupil of the system. Several optical-performance requirements that were verified during this ISIM-level testing are levied on the uncertainties of various wavefront-error-related quantities rather than on the wavefront errors themselves. This paper also describes the methodology, based on Monte Carlo simulations of the wavefront-sensing analysis of focus-sweep data, used to establish

  19. James Webb Space Telescope (JWST) Integrated Science Instruments Module (ISIM) Cryo-Vacuum (CV) Test at GSFC

    Science.gov (United States)

    Yew, Calinda M.

    2014-01-01

    JWST ISIM has entered into its system-level testing program at NASA Goddard Space Flight Center (GSFC). In December 2013, ISIM successfully completed the first in a series of three cryo-vacuum tests, which included two flight science instruments. Since then, there have been full-fledged efforts towards the CV2 test scheduled to finish at the end of 2014. The complexity of the mission has generated challenging requirements that demand highly reliable system performance and capabilities from the Space Environment Simulator (SES) vacuum chamber. In order to satisfy the program requirements, GSFC had to develop unique structural and thermal hardware to test ISIM. Most noteworthy is a helium shroud structure and cooling system built in order to achieve operational temperatures below 20K (-253C). This paper: (1) provides an overview of the integrated mechanical and thermal facility systems required to achieve the objectives of JWST ISIM testing, (2) communicates the performance and challenges of the SES during the first ISIM test, and (3) summarizes the action plan to improve the system prior to the next test.

  20. EMC Testing on the Integrated Science Instrument Module (ISIM) - A Summary of the EMC Test Campaign for the Science Payload of the James Webb Space Telescope (JWST)

    Science.gov (United States)

    McCloskey, John

    2016-01-01

    This paper describes the electromagnetic compatibility (EMC) tests performed on the Integrated Science Instrument Module (ISIM), the science payload of the James Webb Space Telescope (JWST), at NASAs Goddard Space Flight Center (GSFC) in August 2015. By its very nature of being an integrated payload, it could be treated as neither a unit level test nor an integrated spacecraft/observatory test. Non-standard test criteria are described along with non-standard test methods that had to be developed in order to evaluate them. Results are presented to demonstrate that all test criteria were met in less than the time allocated.

  1. Wavefront-error performance characterization for the James Webb Space Telescope (JWST) Integrated Science Instrument Module (ISIM) science instruments

    Science.gov (United States)

    Aronstein, David L.; Smith, J. S.; Zielinski, Thomas P.; Telfer, Randal; Tournois, Severine C.; Moore, Dustin B.; Fienup, James R.

    2016-07-01

    The science instruments (SIs) comprising the James Webb Space Telescope (JWST) Integrated Science Instrument Module (ISIM) were tested in three cryogenic-vacuum test campaigns in the NASA Goddard Space Flight Center (GSFC)'s Space Environment Simulator (SES) test chamber. In this paper, we describe the results of optical wavefront-error performance characterization of the SIs. The wavefront error is determined using image-based wavefront sensing, and the primary data used by this process are focus sweeps, a series of images recorded by the instrument under test in its as-used configuration, in which the focal plane is systematically changed from one image to the next. High-precision determination of the wavefront error also requires several sources of secondary data, including 1) spectrum, apodization, and wavefront-error characterization of the optical ground-support equipment (OGSE) illumination module, called the OTE Simulator (OSIM), 2) f/# and pupil-distortion measurements made using a pseudo-nonredundant mask (PNRM), and 3) pupil-geometry predictions for each SI field point tested, which are complicated because of a tricontagon-shaped outer perimeter and small holes that appear in the exit pupil due to the way that different light sources are injected into the optical path by the OGSE. One set of wavefront-error tests, for the coronagraphic channel of the Near-Infrared Camera (NIRCam) Longwave instruments, was performed using data from transverse-translation diversity (TTD) sweeps instead of focus sweeps, in which a subaperture is translated and/or rotated across the exit pupil of the system from one image to the next. Several optical-performance requirements that were verified during this ISIM Element-level testing are levied on the uncertainties of various wavefront-error-related quantities rather than on the wavefront errors themselves. This paper also gives an overview of the methodology, based on Monte Carlo simulations of the wavefront-sensing analysis

  2. Two NIRCam Channels are Better than One: How JWST Can Do More Science with NIRCam’s Short-wavelength Dispersed Hartmann Sensor

    Science.gov (United States)

    Schlawin, E.; Rieke, M.; Leisenring, J.; Walker, L. M.; Fraine, J.; Kelly, D.; Misselt, K.; Greene, T.; Line, M.; Lewis, N.; Stansberry, J.

    2017-01-01

    The James Webb Space Telescope (JWST) offers unprecedented sensitivity, stability, and wavelength coverage for transiting exoplanet studies, opening up new avenues for measuring atmospheric abundances, structure, and temperature profiles. Taking full advantage of JWST spectroscopy of planets from 0.6 to 28 μm, however, will require many observations with a combination of the NIRISS, NIRCam, NIRSpec, and MIRI instruments. In this white paper, we discuss a new NIRCam mode (not yet approved or implemented) that can reduce the number of necessary observations to cover the 1.0-5.0 μm wavelength range. Even though NIRCam was designed primarily as an imager, it also includes several grisms for phasing and aligning JWST’s 18 hexagonal mirror segments. NIRCam’s long-wavelength channel includes grisms that cover 2.4-5.0 μm with a resolving power of R = 1200-1550 using two separate configurations. The long-wavelength grisms have already been approved for science operations, including wide field and single object (time series) slitless spectroscopy. We propose a new mode that will simultaneously measure spectra for science targets in the 1.0-2.0 μm range using NIRCam’s short-wavelength channel. This mode, if approved, would take advantage of NIRCam’s Dispersed Hartmann Sensor (DHS), which produces 10 spatially separated spectra per source at R ˜ 300. We discuss the added benefit of the DHS in constraining abundances in exoplanet atmospheres as well as its ability to observe the brightest systems. The DHS essentially comes for free (at no time cost) with any NIRCam long-wavelength grism observation, but the detector integration parameters have to be selected to ensure that the long-wavelength grism observations do not saturate and that JWST data volume downlink constraints are not violated. Combining both of NIRCam’s channels will maximize the science potential of JWST, which is a limited life observatory.

  3. Planning JWST NIRSpec MSA spectroscopy using NIRCam pre-images

    Science.gov (United States)

    Beck, Tracy L.; Ubeda, Leonardo; Kassin, Susan A.; Gilbert, Karoline; Karakla, Diane M.; Reid, I. N.; Blair, William P.; Keyes, Charles D.; Soderblom, D. R.; Peña-Guerrero, Maria A.

    2016-07-01

    The Near-Infrared Spectrograph (NIRSpec) is the work-horse spectrograph at 1-5microns for the James Webb Space Telescope (JWST). A showcase observing mode of NIRSpec is the multi-object spectroscopy with the Micro-Shutter Arrays (MSAs), which consist of a quarter million tiny configurable shutters that are 0. ''20×0. ''46 in size. The NIRSpec MSA shutters can be opened in adjacent rows to create flexible and positionable spectroscopy slits on prime science targets of interest. Because of the very small shutter width, the NIRSpec MSA spectral data quality will benefit significantly from accurate astrometric knowledge of the positions of planned science sources. Images acquired with the Hubble Space Telescope (HST) have the optimal relative astrometric accuracy for planning NIRSpec observations of 5-10 milli-arcseconds (mas). However, some science fields of interest might have no HST images, galactic fields can have moderate proper motions at the 5mas level or greater, and extragalactic images with HST may have inadequate source information at NIRSpec wavelengths beyond 2 microns. Thus, optimal NIRSpec spectroscopy planning may require pre-imaging observations with the Near-Infrared Camera (NIRCam) on JWST to accurately establish source positions for alignment with the NIRSpec MSAs. We describe operational philosophies and programmatic considerations for acquiring JWST NIRCam pre-image observations for NIRSpec MSA spectroscopic planning within the same JWST observing Cycle.

  4. The James Webb Space Telescope (JWST), The First Light Machine

    Science.gov (United States)

    Stahl, H. Philip

    2013-01-01

    Scheduled to begin its 10 year mission after 2018, the James Webb Space Telescope (JWST) will search for the first luminous objects of the Universe to help answer fundamental questions about how the Universe came to look like it does today. At 6.5 meters in diameter, JWST will be the world s largest space telescope. This talk reviews science objectives for JWST and how they drive the JWST architecture, e.g. aperture, wavelength range and operating temperature. Additionally, the talk provides an overview of the JWST primary mirror technology development and fabrication status.

  5. Social Work and Science

    Science.gov (United States)

    Gehlert, Sarah

    2016-01-01

    Interest has grown in the past few years about the place of social work in science. Questions remain, such as whether social work should be considered a science, and if so, where it fits into the constellation of sciences. This article attempts to shed light on these questions. After briefly considering past and present constructions of science…

  6. Social Work and Science

    Science.gov (United States)

    Gehlert, Sarah

    2016-01-01

    Interest has grown in the past few years about the place of social work in science. Questions remain, such as whether social work should be considered a science, and if so, where it fits into the constellation of sciences. This article attempts to shed light on these questions. After briefly considering past and present constructions of science…

  7. Two NIRCam channels are Better than One: How JWST Can Do More Science with NIRCam's Short-Wavelength Dispersed Hartmann Sensor

    CERN Document Server

    Schlawin, Everett; Leisenring, Jarron; Greene, Tom; Walker, Lisa May; Fraine, Jonathan; Kelly, Doug; Misselt, Karl; Line, Michael; Stansberry, John; Lewis, Nikole

    2016-01-01

    The James Webb Space Telescope (JWST) offers unprecedented sensitivity, stability, and wavelength coverage for transiting exoplanet studies, opening up new avenues for measuring atmospheric abundances, structure, and temperature profiles. Taking full advantage of JWST spectroscopy of planets from 0.6um to 28um, however, will require many observations with a combination of the NIRISS, NIRCam, NIRSpec, and MIRI instruments. In this white paper, we discuss a new NIRCam mode (not yet approved or implemented) that can reduce the number of necessary observations to cover the 1.0um to 5.0um wavelength range. Even though NIRCam was designed primarily as an imager, it also includes several grisms for phasing and aligning JWST's 18 hexagonal mirror segments. NIRCam's long-wavelength channel includes grisms that cover 2.4um to 5.0um with a resolving power of R = 1200 - 1550 using two separate configurations. The long-wavelength grisms have already been approved for science operations, including wide field and single obj...

  8. Making Science Teams Work

    Science.gov (United States)

    Miller, Roxanne Greitz

    2004-01-01

    Science teachers, likely have more experience with students working together than teachers in any other subject area due to teaming students for hands-on activities. While the importance of teamwork is emphasized in the National Science Education Standards, getting teams to actually work-meaning getting students to share equally in the academic…

  9. Ray-tracing for coordinate knowledge in the JWST Integrated Science Instrument Module

    CERN Document Server

    Sabatke, Derek; Rohrbach, Scott; Kubalak, David

    2014-01-01

    Optical alignment and testing of the Integrated Science Instrument Module of the James Webb Space Telescope is underway. We describe the Optical Telescope Element Simulator used to feed the science instruments with point images of precisely known location and chief ray pointing, at appropriate wavelengths and flux levels, in vacuum and at operating temperature. The simulator's capabilities include a number of devices for in situ monitoring of source flux, wavefront error, pupil illumination, image position and chief ray angle. Taken together, these functions become a fascinating example of how the first order properties and constructs of an optical design (coordinate systems, image surface and pupil location) acquire measurable meaning in a real system. We illustrate these functions with experimental data, and describe the ray tracing system used to provide both pointing control during operation and analysis support subsequently. Prescription management takes the form of optimization and fitting. Our core too...

  10. The ``One Archive'' for JWST

    Science.gov (United States)

    Greene, G.; Kyprianou, M.; Levay, K.; Sienkewicz, M.; Donaldson, T.; Dower, T.; Swam, M.; Bushouse, H.; Greenfield, P.; Kidwell, R.; Wolfe, D.; Gardner, L.; Nieto-Santisteban, M.; Swade, D.; McLean, B.; Abney, F.; Alexov, A.; Binegar, S.; Aloisi, A.; Slowinski, S.; Gousoulin, J.

    2015-09-01

    The next generation for the Space Telescope Science Institute data management system is gearing up to provide a suite of archive system services supporting the operation of the James Webb Space Telescope. We are now completing the initial stage of integration and testing for the preliminary ground system builds of the JWST Science Operations Center which includes multiple components of the Data Management Subsystem (DMS). The vision for astronomical science and research with the JWST archive introduces both solutions to formal mission requirements and innovation derived from our existing mission systems along with the collective shared experience of our global user community. We are building upon the success of the Hubble Space Telescope archive systems, standards developed by the International Virtual Observatory Alliance, and collaborations with our archive data center partners. In proceeding forward, the “one archive” architectural model presented here is designed to balance the objectives for this new and exciting mission. The STScI JWST archive will deliver high quality calibrated science data products, support multi-mission data discovery and analysis, and provide an infrastructure which supports bridges to highly valued community tools and services.

  11. Preparing the Public for JWST

    Science.gov (United States)

    Green, Joel D.; Smith, Denise A.; Lawton, Brandon L.; Jirdeh, Hussein; Meinke, Bonnie K.

    2016-01-01

    The James Webb Space Telescope is the successor to the Hubble Space Telescope. STScI and the Office of Public Outreach are committed to bringing awareness of the technology, the excitement, and the future science potential of this great observatory to the public, to educators and students, and to the scientific community, prior to its 2018 launch. The challenges in ensuring the high profile of JWST (understanding the infrared, the vast distance to the telescope's final position, and the unfamiliar science territory) requires us to lay the proper background. We currently engage the full range of the public and scientific communities using a variety of high impact, memorable initiatives, in combination with modern technologies to extend reach, linking the science goals of Webb to the ongoing discoveries being made by Hubble. We have injected Webb-specific content into ongoing E/PO programs: for example, simulated scientifically inspired but aesthetic JWST scenes, illustrating the differences between JWST and previous missions; partnering with high impact science communicators such as MinutePhysics to produce timely and concise content; educational materials in vast networks of schools through products like the Star Witness News.

  12. Lenses for JWST

    Science.gov (United States)

    Ebeling, Harald; Richard, Johan; Kneib, Jean-Paul; Repp, Andrew; Atek, Hakim; Egami, Eiichi; Windhorst, Rogier; Edge, Alastair

    2016-08-01

    JWST will dramatically advance our knowledge and understanding of the first generations of galaxies at z>10, their role in the re-ionization of the Universe, and the evolutionary processes that gave rise to the complexity and diversity of galaxies at the current epoch. As demonstrated by HST legacy projects like CLASH and the Hubble Frontier Fields, gravitational amplification by massive galaxy clusters can significantly extend the depth of the required observations. However, for JWST, reducing any diffuse background light will be just as crucial. We here propose Spitzer/IRAC observations of six massive cluster lenses, specifically selected as candidates for observation with JWST. By (a) quantifying the amount of intra-cluster light and (b) enabling us to improve our current lens models, the data resulting from the requested observations will be instrumental for the final selection of cluster targets that maximize the scientific returns of deep JWST observations.

  13. The science works

    OpenAIRE

    Sabrovsky Jauneau, Eduardo

    2008-01-01

    This paper has the purpose of showing the identity between science and technology from within scientific language. The traditional philosophical argument in favour of this identity is briefly examined, through the work of Heidegger. Then, following Henri Atlan (“Ordres et Significations”, 1979. Le crystal et la fumée. Essai sur l’organisation du vivant. Paris: Éd. Du Seuil) the scientific definitions of order and disorder are reviewed; then Boltzmann’s statistical formulation of the Second La...

  14. Transiting Exoplanets with JWST

    CERN Document Server

    Seager, S; Valenti, J A

    2008-01-01

    The era of exoplanet characterization is upon us. For a subset of exoplanets -- the transiting planets -- physical properties can be measured, including mass, radius, and atmosphere characteristics. Indeed, measuring the atmospheres of a further subset of transiting planets, the hot Jupiters, is now routine with the Spitzer Space Telescope. The James Webb Space Telescope (JWST) will continue Spitzer's legacy with its large mirror size and precise thermal stability. JWST is poised for the significant achievement of identifying habitable planets around bright M through G stars--rocky planets lacking extensive gas envelopes, with water vapor and signs of chemical disequilibrium in their atmospheres. Favorable transiting planet systems, are, however, anticipated to be rare and their atmosphere observations will require tens to hundreds of hours of JWST time per planet. We review what is known about the physical characteristics of transiting planets, summarize lessons learned from Spitzer high-contrast exoplanet m...

  15. NOSS science working group

    Science.gov (United States)

    The members of the NOSS Science Working Group are John Apel, Pacific Marine Environmental Laboratories/NOAA; Tim Barnett, Scripps Institution of Oceanography; Francis Bretherton (chairman), National Center for Atmospheric Research; Otis Brown, University of Miami; Joost Businger, University of Washington; Garrett Campbell, NCAR; Mark Cane, Massachusetts Institute of Technology; Robert Edwards, National Marine Fisheries Service/NOAA; James Mueller, Naval Postgraduate School; Peter Niiler, Oregon State University; James J. O'Brien, Florida State University; Norman Phillips, National Meteorological Center/NOAA; Owen Phillips, The Johns Hopkins University; Stephen Piacsek, NSTL Station, NORDA; Trevor Platt, Bedford Institute of Oceanography; Stephen Pond, University of British Columbia; Stanley Ruttenberg (executive secretary), NCAR; William Schmitz, Woods Hole Oceanographic Institution; Jerry Schubel, State University of New York; Robert Stewart, Scripps; Norbert Untersteiner, NOAA; and Alan Weinstein, Naval Environmental Prediction Research Facility.

  16. Key Exoplanets in the Era of JWST

    Science.gov (United States)

    Batalha, Natasha; Mandell, Avi; Lewis, Nikole K.; Pontoppidan, Klaus

    2017-01-01

    In 2018, exoplanet science will enter a new era with the launch of the James Webb Space Telescope (JWST). With JWST's observing power, several studies have sought to characterize how the instruments will perform and what atmospheric spectral features could theoretically be detected using transmission spectroscopy. With just two years left until launch, it is imperative that the exoplanet community begins to digest and integrate these studies into their observing plans and strategies. In order to encourage this and to allow all members of the community access to JWST simulations, we present here an open source tool for creating observation simulations of all observatory-supported time-series spectroscopy modes. We describe our tool, PandExo and use it to calculate the expected signal-to-noise ratio (SNR) for every confirmed planetary system with Jhours are needed to attain a SNR of 5 on key molecular absorption bands of H2O, CH4, and CO. We end by determining the number of planets (hot Jupiters, warm Neptunes, super-Earths, etc.) that are currently attainable with JWST.

  17. JWST Pathfinder Telescope Integration

    Science.gov (United States)

    Matthews, Gary W.; Kennard, Scott H.; Broccolo, Ronald T.; Ellis, James M.; Daly, Elizabeth A.; Hahn, Walter G.; Amon, John N.; Mt. Pleasant, Stephen M.; Texter, Scott; Atkinson, Charles B.; McKay, Andrew; Levi, Joshua; Keski-Kuha, Ritva; Feinberg, Lee

    2015-01-01

    The James Webb Space Telescope (JWST) is a 6.5m, segmented, IR telescope that will explore the first light of the universe after the big bang. In 2014, a major risk reduction effort related to the Alignment, Integration, and Test (AI&T) of the segmented telescope was completed. The Pathfinder telescope includes two Primary Mirror Segment Assemblies (PMSA's) and the Secondary Mirror Assembly (SMA) onto a flight-like composite telescope backplane. This pathfinder allowed the JWST team to assess the alignment process and to better understand the various error sources that need to be accommodated in the flight build. The successful completion of the Pathfinder Telescope provides a final integration roadmap for the flight operations that will start in August 2015.

  18. Origin of the Universe: From the First Stars to Planets with JWST

    Science.gov (United States)

    Clampin, Mark

    2008-01-01

    The James Webb Space Telescope (JWST) is a large aperture (6.5 meter), cryogenic space telescope with a suite of near and mid-infrared instruments. JWST's primary science goal is to detect and characterize the first galaxies. It will also study the assembly of galaxies, star formation, protoplanetary systems, and the formation of evolution of planetary systems. We will review the motivations for JWST's science goals in the context of recent Hubble Space Telescope, and Spitzer Space Telescope observations and review the status of the JWST Observatory.

  19. A Retrieval Architecture for JWST Observations of Directly Imaged Exoplanets

    Science.gov (United States)

    Howe, Alex

    2017-06-01

    I present a new modeling and retrieval code for atmospheres of directly imaged exoplanets designed for use on JWST observations, extending my previous work on transiting planets. I perform example retrievals of temperature-pressure profiles, common molecular abundances, and basic cloud properties on existing lower-resolution spectra and on simulated JWST data using forward model emission spectra for planned NIRISS and NIRCam targets. From these results, I estimate the expected return on prospective JWST observations in information-theoretic terms using the mutual information metric.

  20. Fermilab science at work

    CERN Document Server

    Six days. Three frontiers. One amazing lab. From 2010 to 2012, a film crew followed a group of scientists at the Department of Energy's Fermilab and filmed them at work and at home. This 40-minute documentary shows the diversity of the people, research and work at Fermilab. Viewers catch a true behind-the-scenes look of the United States' premier particle physics laboratory while scientists explain why their research is important to them and the world. Scientists included: Brendan Casey, Herman White, Craig Hogan, Denton Morris, Mary Convery, Bonnie Fleming, Deborah Harris, Dave Schmitz, Brenna Flaugher and Aron Soha.

  1. Preparing for JWST wavefront sensing and control operations

    Science.gov (United States)

    Perrin, Marshall D.; Acton, D. Scott; Lajoie, Charles-Philippe; Knight, J. Scott; Lallo, Matthew D.; Allen, Marsha; Baggett, Wayne; Barker, Elizabeth; Comeau, Thomas; Coppock, Eric; Dean, Bruce H.; Hartig, George; Hayden, William L.; Jordan, Margaret; Jurling, Alden; Kulp, Trey; Long, Joseph; McElwain, Michael W.; Meza, Luis; Nelan, Edmund P.; Soummer, Remi; Stansberry, John; Stark, Christopher; Telfer, Randal; Welsh, Andria L.; Zielinski, Thomas P.; Zimmerman, Neil T.

    2016-07-01

    The James Webb Space Telescopes segmented primary and deployable secondary mirrors will be actively con- trolled to achieve optical alignment through a complex series of steps that will extend across several months during the observatory's commissioning. This process will require an intricate interplay between individual wavefront sensing and control tasks, instrument-level checkout and commissioning, and observatory-level calibrations, which involves many subsystems across both the observatory and the ground system. Furthermore, commissioning will often exercise observatory capabilities under atypical circumstances, such as fine guiding with unstacked or defocused images, or planning targeted observations in the presence of substantial time-variable offsets to the telescope line of sight. Coordination for this process across the JWST partnership has been conducted through the Wavefront Sensing and Control Operations Working Group. We describe at a high level the activities of this group and the resulting detailed commissioning operations plans, supporting software tools development, and ongoing preparations activities at the Science and Operations Center. For each major step in JWST's wavefront sensing and control, we also explain the changes and additions that were needed to turn an initial operations concept into a flight-ready plan with proven tools. These efforts are leading to a robust and well-tested process and preparing the team for an efficient and successful commissioning of JWSTs active telescope.

  2. Group Work in Science Classrooms

    Science.gov (United States)

    McGregor, Debbie; Tolmie, Andrew

    2009-01-01

    This article considers how students might work together in small groups, from two to eight, in either a primary or secondary science classroom. The nature of group work can vary widely and could include, for example, a pair carrying out an illustrative experiment, a trio or quad debating climate change, or six or seven rehearsing how they will…

  3. Exoplanets and debris disk imaging with JWST

    Science.gov (United States)

    Pueyo, Laurent; Soummer, Remi; Perrin, Marshall D.

    2017-06-01

    Dramatic progress in exoplanetary systems imaging has occurred since the first generation of space coronagraphs on HST (NICMOS, STIS, ACS). While HST remains at forefront of both exoplanetary and circumstellar disk science, ground-based instruments have improved by three orders of magnitudes over the past decade. JWST will extend the current state of the art with a larger set of superior coronagraphs and greater sensitivity across more than a factor of 10 in wavelength, making it extraordinarily capable for detailed imaging characterization of planets and disks. We will address specific questions about nearby exoplanetary systems, while also optimizing observing strategies across the breadth of JWST’s high-contrast imaging modes, as follows: (a) Deep, multi-wavelength observations of selected nearby stars hosting known debris disks & planets. We will use the NIRCam and MIRI coronagraphs across the full range of JWST wavelengths, and perhaps MIRI MRS spatially resolved spectroscopy. Each comprehensive dataset will support a variety of investigations addressing both disk characterization and exoplanet detection & characterization. (b) Characterization of Planetary Systems around Cool M Stars. We will observe young and dusty M dwarfs, to complement observations of the closer but older M dwarf samples under consideration by other GTO groups. JWST observations will dramatically exceed HST images in their ability to address questions about the properties of dust rings, while the more favorable contrast ratios of planets relative to M dwarf hosts will enable sensitivity to relatively low mass planetary companions.

  4. Observer's Interface for JWST Observation Specifications

    Science.gov (United States)

    Link, Miranda; Douglas, Robert; Moriarty, Christopher; Roman, Anthony

    2016-01-01

    In support of the launch of the James Webb Space Telescope, various teams at STScI (the Space Telescope Science Institute) have collaborated on how to re-structure the view of a an observing program within the Astronomer's Proposal Tool (APT) to accommodate for the differences between HST and JWST. For HST APT programs, the structure is visit-dominant, and there is one generic form for entering observing information that spans all instruments with their required fields and options. This can result in sometimes showing irrelevant fields to the user for a given observing goal. Also, the generation of mosaicked observations in HST requires the user to manually calculate the position of each tile within the mosaic, accounting for positional offsets and the roll of the telescope, which is a time consuming process. Now, for JWST programs in APT, the description of the observations has been segregated by instrument and mode into discrete observing templates. Each template's form allows instrument specific choices and displays of relevant information. APT will manually manage the number of visits needed to perform the observation. This is particularly useful for mosaics and dithering with JWST. For example, users will select how they would like a mosaic to be tiled at the observation level, and the visits are automatically created. In this, visits have been re-structured to be purely informational; all editing is done at the observation level. These options and concepts are illustrated to future users via the corresponding poster.

  5. Preservation of Thermal Control Specular Gold Baffle Surface on the James Webb Space Telescope (JWST) Integrated Science Instrument Module (ISIM) Electronics Compartment (IEC)

    Science.gov (United States)

    MonteedeGarcia, Kristina; Patel, Jignasha; Perry, Radford, III

    2010-01-01

    Extremely tight thermal control property degradation allowances on the vapor-deposited, gold-coated IEC baffle surface, made necessary by the cryogenic JWST Observatory operations, dictate tight contamination requirements on adjacent surfaces. Theoretical degradation in emittance with contaminant thickness was calculated. Maximum allowable source outgassing rates were calculated using worst case view factors from source to baffle surface. Tight requirements pushed the team to change the design of the adjacent surfaces to minimize the outgassing sources

  6. Focus Groups for Solar System Investigations with the JWST

    Science.gov (United States)

    Hines, Dean C.; Milam, Stefanie N.; Stansberry, John; Hammel, Heidi B.; Sonneborn, George; Lunine, Jonathan; Rivkin, Andrew; Woodward, Charles; Norwood, Jim; Villanueva, Geronimo; Thomas, Cristina; Santos-Sanz, Pablo; Tiscareno, Matthew; Kestay, Laszlo; Nixon, Conor; Parker, Alex

    2014-11-01

    The unprecedented sensitivity and angular resolution of the James Webb Space Telescope (JWST) will make it NASA’s premier space-based facility for infrared astronomy. This 6.5-meter telescope, which is optimized for observations in the near and mid infrared, will be equipped with four state-of-the-art instruments that include imaging, spectroscopy, and coronagraphy. These instruments, along with the telescope’s moving target capabilities, will enable the infrared study of solar system objects with unprecedented detail. A new white paper (Norwood et al., 2014) provides a general overview of JWST observatory and instrument capabilities for Solar System science, and updates and expands upon an earlier study by Lunine et al. (2010). In order to fully realize the potential of JWST for Solar System observations, we have recently organized 10 focus groups to explore various science use cases in more detail on topics including: Asteroids, Comets, Giant Planets, Mars, Near Earth Objects, Occultations, Rings, Satellites, Titan, and Trans-Neptunian Objects. The findings from these groups will help guide the project as it develops and implements planning tools, observing templates, the data pipeline and archives so that they enable a broad range of Solar System Science investigations. The purpose of this presentation is to raise awareness of the JWST Solar System planning, and to invite participation of DPS members with our Focus Groups and other pre-launch activities.References:Lunine, J., Hammel, H., Schaller, E., Sonneborn, G., Orton, G., Rieke, G., and Rieke, M. 2010, JWST Planetary Observations within the Solar System, http://www.stsci.edu/jwst/doc-archive/white-papers.Norwood, J., Hammel, H., Milam, S.,Stansberry, J., Lunine, J., Chanover, N., Hines, D., Sonneborn, G., Tiscareno, M., Brown, M. and Ferruit, P., 2014, ArXiv e-prints, 1403.6845.

  7. The Impact of JWST Broadband Filter Choice on Photometric Redshift Estimation

    DEFF Research Database (Denmark)

    Bisigello, L.; Caputi, K. I.; Colina, L.;

    2016-01-01

    The determination of galaxy redshifts in the James Webb Space Telescope's (JWST) blank-field surveys will mostly rely on photometric estimates, based on the data provided by JWST's Near-Infrared Camera (NIRCam) at 0.6–5.0 μm and Mid Infrared Instrument (MIRI) at λ 5.0 μm. In this work we analyze ...

  8. NEOs in the mid-infrared: from Spitzer to JWST

    Science.gov (United States)

    Mueller, Michael; Thomas, Cristina A.

    2016-10-01

    Near-Earth Objects (NEOs) account for a surprisingly large fraction of the Spitzer observing time devoted to Solar System science. As a community, we should think of ways to repeat that success with JWST. JWST is planning an open Early Release Science Program, with the expected deadline for letters of intent in early 2017. We can't wait for next year's DPS to develop ideas. The time is now!In order to stir up the discussion, we will present ideas for NEO observing programs that are well adapted to JWST's capabilities and limitations, based on our recent PASP paper (Thomas et al., 2016). Obvious measurement objectives would include* size and albedo from thermal continuum (MIRI photometry)* thermal inertia for objects with well-known shape and spin state (MIRI)* taxonomy through reflection spectroscopy and emission spectroscopy in the NIR and MIR; NIR colors for faint objects.In all cases, JWST's sensitivity will allow us to go deeper than currently possible by at least an order of magnitude. Meter-sized NEOs similar to 2009 BD or 2011 MD are easy targets for MIRI spectrophotometry!The following limitations must be kept in mind, however: JWST's large size makes it slow to move. Most problematic for NEOs is probably the resulting 'speed limit': non-sidereal tracking is supported up to a rate of 30 mas/s, NEOs can easily move faster than that (ways to relax this constraint are under discussion). The average slew to a new target is budgeted to take 30 min, effectively ruling out programs many-target programs like ExploreNEOs or NEOSurvey (see D. Trilling's paper). Additionally, JWST will only observe close to quadrature, translating to large solar phase angles for NEO observations; this is familiar from other space-based IR facilities.

  9. Observing Dark Stars with JWST

    CERN Document Server

    Ilie, Cosmin; Valluri, Monica; Iliev, Ilian T; Shapiro, Paul

    2011-01-01

    We study the capability of the James Webb Space Telescope (JWST) to detect Supermassive Dark Stars (SMDS). If the first stars are powered by dark matter heating in triaxial dark matter haloes, they may grow to be very large and very bright, visible in deep imaging with JWST and even Hubble Space Telescope (HST). We use HST surveys to place bounds on the numbers of SMDSs that may be detected in future JWST imaging surveys. We showed that SMDS in the mass range $10^6-10^7 M_\\odot$ are bright enough to be detected in all the wavelength bands of the NIRCam on JWST . If SMDSs exist at z ~10, 12, and 14, they will be detectable as J-band, H-band, or K-band dropouts, respectively. With a total survey area of 150 arcmin^2 (assuming a multi-year deep parallel survey with JWST), we find that typically the number of $10^6 M_\\odot$ SMDSs found as H or K-band dropouts is ~10^5\\fsmds, where the fraction of early DM haloes hosting DS is likely to be small, \\fsmds10 from SMDSs would be possible with spectroscopy: the SMDS (w...

  10. Work flows in life science

    NARCIS (Netherlands)

    Wassink, Ingo

    2010-01-01

    The introduction of computer science technology in the life science domain has resulted in a new life science discipline called bioinformatics. Bioinformaticians are biologists who know how to apply computer science technology to perform computer based experiments, also known as in-silico or dry lab

  11. Work flows in life science

    NARCIS (Netherlands)

    Wassink, I.

    2010-01-01

    The introduction of computer science technology in the life science domain has resulted in a new life science discipline called bioinformatics. Bioinformaticians are biologists who know how to apply computer science technology to perform computer based experiments, also known as in-silico or dry lab

  12. James Webb Space Telescope (JWST) Integrated Science Instruments Module (ISIM) Electronics Compartment (IEC) Conformal Shields Composite Bond Structure Qualification Test Method

    Science.gov (United States)

    Yew, Calinda; Stephens, Matt

    2015-01-01

    The JWST IEC conformal shields are mounted onto a composite frame structure that must undergo qualification testing to satisfy mission assurance requirements. The composite frame segments are bonded together at the joints using epoxy, EA 9394. The development of a test method to verify the integrity of the bonded structure at its operating environment introduces challenges in terms of requirements definition and the attainment of success criteria. Even though protoflight thermal requirements were not achieved, the first attempt in exposing the structure to cryogenic operating conditions in a thermal vacuum environment resulted in approximately 1 bonded joints failure during mechanical pull tests performed at 1.25 times the flight loads. Failure analysis concluded that the failure mode was due to adhesive cracks that formed and propagated along stress concentrated fillets as a result of poor bond squeeze-out control during fabrication. Bond repairs were made and the structures successfully re-tested with an improved LN2 immersion test method to achieve protoflight thermal requirements.

  13. Synergy with HST and JWST Data Management Systems

    Science.gov (United States)

    Greene, Gretchen; Space Telescope Data Management Team

    2014-01-01

    The data processing and archive systems for the JWST will contain a petabyte of science data and the best news is that users will have fast access to the latest calibrations through a variety of new services. With a synergistic approach currently underway with the STScI science operations between the Hubble Space Telescope and James Webb Space Telescope data management subsystems (DMS), operational verification is right around the corner. Next year the HST archive will provide scientists on-demand fully calibrated data products via the Mikulski Archive for Space Telescopes (MAST), which takes advantage of an upgraded DMS. This enhanced system, developed jointly with the JWST DMS is based on a new CONDOR distributed processing system capable of reprocessing data using a prioritization queue which runs in the background. A Calibration Reference Data System manages the latest optimal configuration for each scientific instrument pipeline. Science users will be able to search and discover the growing MAST archive calibrated datasets from these missions along with the other multiple mission holdings both local to MAST and available through the Virtual Observatory. JWST data systems will build upon the successes and lessons learned from the HST legacy and move us forward into the next generation of multi-wavelength archive research.

  14. Design and Lessons Learned on the Development of a Cryogenic Pupil Select Mechanism Used in the Testing and Calibration of the Integrated Science Instrument Module (ISIM) on the James Webb Space Telescope (JWST)

    Science.gov (United States)

    Mitchell, Alissa; Capon, Thomas; Guzek, Jeffrey; Hakun, Claef; Haney, Paul; Koca, Corina

    2014-01-01

    Calibration and testing of the instruments on the Integrated Science Instrument Module (ISIM) of the James Webb Space Telescope (JWST) is being performed by the use of a cryogenic, full-field, optical simulator that was constructed for this purpose. The Pupil Select Mechanism (PSM) assembly is one of several mechanisms and optical elements that compose the Optical Telescope Element SIMulator, or OSIM. The PSM allows for several optical elements to be inserted into the optical plane of OSIM, introducing a variety of aberrations, distortions, obscurations, and other calibration states into the pupil plane. The following discussion focuses on the details of the design evolution, analysis, build, and test of this mechanism along with the challenges associated with creating a sub arc-minute positioning mechanism operating in an extreme cryogenic environment. In addition, difficult challenges in the control system design will be discussed including the incorporation of closed-loop feedback control into a system that was designed to operate in an open-loop fashion.

  15. AGN studies with JWST/MIRI

    NARCIS (Netherlands)

    Caputi, K.

    2015-01-01

    The forthcoming James Webb Space Telescope (JWST) will revolutionize galaxy evolution studies from the epoch of reionisation to the present day. In particular, a new era will be open for mid-IR astronomy, as the JWST Mid-Infrared Instrument (MIRI) will improve by an order of magnitude the sensitivit

  16. Improving JWST Coronagraphic Performance with Accurate Image Registration

    Science.gov (United States)

    Van Gorkom, Kyle; Pueyo, Laurent; Lajoie, Charles-Philippe; JWST Coronagraphs Working Group

    2016-06-01

    The coronagraphs on the James Webb Space Telescope (JWST) will enable high-contrast observations of faint objects at small separations from bright hosts, such as circumstellar disks, exoplanets, and quasar disks. Despite attenuation by the coronagraphic mask, bright speckles in the host’s point spread function (PSF) remain, effectively washing out the signal from the faint companion. Suppression of these bright speckles is typically accomplished by repeating the observation with a star that lacks a faint companion, creating a reference PSF that can be subtracted from the science image to reveal any faint objects. Before this reference PSF can be subtracted, however, the science and reference images must be aligned precisely, typically to 1/20 of a pixel. Here, we present several such algorithms for performing image registration on JWST coronagraphic images. Using both simulated and pre-flight test data (taken in cryovacuum), we assess (1) the accuracy of each algorithm at recovering misaligned scenes and (2) the impact of image registration on achievable contrast. Proper image registration, combined with post-processing techniques such as KLIP or LOCI, will greatly improve the performance of the JWST coronagraphs.

  17. JWST Near-Infrared Detector Degradation: Finding the Problem, Fixing the Problem, and Moving Forward

    Science.gov (United States)

    Rauscher, Bernard J.; Stahle, Carl; Hill, Bob; Greenhouse, Matt; Beletic, James; Babu, Sachidananda; Blake, Peter; Cleveland, Keith; Cofie, Emmanuel; Eegholm, Bente; Engelbracht, Chad; Hall, Don; Hoffman, Alan; Jeffers, Basil; Jhabvala, Christine; Kimble, Randy; Kopp, Robert; Lee, Don; Leidecker, Henning; Lindler, Don; McMurray, Bob; Mott, D. Brent; Ohl, Ray; Polis, Don; Pontius, Jim

    2012-01-01

    The James Webb Space Telescope (JWST) is the successor to the Hubble Space Telescope. JWST will be an infrared optimized telescope, with an approximately 6.5 m diameter primary mirror, that is located at the Sun-Earth L2 Lagrange point. Three of JWST's four science instruments use Teledyne HgCdTe HAWAII-2RG (H2RG) near infrared detector arrays. During 2010, the JWST Project noticed that a few of its 5 micron cutoff H2RG detectors were degrading during room temperature storage, and NASA chartered a "Detector Degradation Failure Review Board" (DD-FRB) to investigate. The DD-FRB determined that the root cause was a design flaw that allowed indium to interdiffuse with the gold contacts and migrate into the HgCdTe detector layer. Fortunately, Teledyne already had an improved design that eliminated this degradation mechanism. During early 2012, the improved H2RG design was qualified for flight and JWST began making additional H2RGs. In this article we present the two public DD-FRB "Executiye Summaries" that: (1) determined the root cause of the detector degradation and (2) defined tests to determine whether the existing detectors are qualified for flight. We supplement these with a brief introduction to H2RG detector arrays, and a discussion of how the JWST Project is using cryogenic storage to retard the degradation rate of the existing flight spare H2RGs.

  18. Social Work Science and Knowledge Utilization

    Science.gov (United States)

    Marsh, Jeanne C.; Reed, Martena

    2016-01-01

    Objective: This article advances understanding of social work science by examining the content and methods of highly utilized or cited journal articles in social work. Methods: A data base of the 100 most frequently cited articles from 79 social work journals was coded and categorized into three primary domains: content, research versus…

  19. Social Work Science and Knowledge Utilization

    Science.gov (United States)

    Marsh, Jeanne C.; Reed, Martena

    2016-01-01

    Objective: This article advances understanding of social work science by examining the content and methods of highly utilized or cited journal articles in social work. Methods: A data base of the 100 most frequently cited articles from 79 social work journals was coded and categorized into three primary domains: content, research versus…

  20. Exploring JWST's Capability to Constrain Habitability on Simulated Terrestrial TESS Planets

    Science.gov (United States)

    Tremblay, Luke; Britt, Amber; Batalha, Natasha; Schwieterman, Edward; Arney, Giada; Domagal-Goldman, Shawn; Mandell, Avi; Planetary Systems Laboratory; Virtual Planetary Laboratory

    2017-01-01

    In the following, we have worked to develop a flexible "observability" scale of biologically relevant molecules in the atmospheres of newly discovered exoplanets for the instruments aboard NASA's next flagship mission, the James Webb Space Telescope (JWST). We sought to create such a scale in order to provide the community with a tool with which to optimize target selection for JWST observations based on detections of the upcoming Transiting Exoplanet Satellite Survey (TESS). Current literature has laid the groundwork for defining both biologically relevant molecules as well as what characteristics would make a new world "habitable", but it has so far lacked a cohesive analysis of JWST's capabilities to observe these molecules in exoplanet atmospheres and thereby constrain habitability. In developing our Observability Scale, we utilized a range of hypothetical planets (over planetary radii and stellar insolation) and generated three self-consistent atmospheric models (of dierent molecular compositions) for each of our simulated planets. With these planets and their corresponding atmospheres, we utilized the most accurate JWST instrument simulator, created specically to process transiting exoplanet spectra. Through careful analysis of these simulated outputs, we were able to determine the relevant parameters that effected JWST's ability to constrain each individual molecular bands with statistical accuracy and therefore generate a scale based on those key parameters. As a preliminary test of our Observability Scale, we have also applied it to the list of TESS candidate stars in order to determine JWST's observational capabilities for any soon-to-be-detected planet in those solar systems.

  1. Teaching Political Science through Memory Work

    Science.gov (United States)

    Jansson, Maria; Wendt, Maria; Ase, Cecilia

    2009-01-01

    In this article, we present the results of a research project where we have tried to elaborate more socially inclusive ways of teaching and learning political science by making use of a specific feminist method of analyzing social relations--memory work. As a method, memory work involves writing and interpreting stories of personal experience,…

  2. Teaching Political Science through Memory Work

    Science.gov (United States)

    Jansson, Maria; Wendt, Maria; Ase, Cecilia

    2009-01-01

    In this article, we present the results of a research project where we have tried to elaborate more socially inclusive ways of teaching and learning political science by making use of a specific feminist method of analyzing social relations--memory work. As a method, memory work involves writing and interpreting stories of personal experience,…

  3. Using Exoplanet Models to Explore NGSS and the Nature of Science and as a Tool for Understanding the Scientific Results from NIRCam/JWST

    Science.gov (United States)

    Lebofsky, Larry A.; McCarthy, Donald W.; Higgins, Michelle L.; Lebofsky, Nancy R.

    2014-11-01

    Our Solar System is no longer unique. To date, about 1,800 planets are known to orbit over 1,100 other stars and nearly 50% are in multiple-planet systems. Planetary systems seem [to be] fairly common and astronomers are now finding Earth-sized planets in the Goldilocks Zone, suggesting there may be other habitable planets. To this end, characterizing the atmospheric chemistries of such planets is a major science goal of the NIRCam instrument on the James Webb Space Telescope.For NIRCam's E/PO program with the Girl Scouts of the USA, we have produced scale models and associated activities to compare the size, scale, and dynamics of the Solar System with several exoplanet systems. Our models illustrate the techniques used to investigate these systems: radial velocity, transits, direct observations, and gravitational microlensing. By comparing and contrasting these models, we place our Solar System in a more cosmic context and enable discussion of current questions within the scientific community: How do planetary systems form and evolve? Is our present definition of a planet a good definition in the context of other planetary systems? Are there other planets/moons that might harbor life as we know it?These models are appropriate for use in classrooms and conform to the Next Generation Science Standards (NGSS) through the Disciplinary Core Idea: Earth's Place in the Universe and Crosscutting Concepts—Patterns Scale, Portion, and Quantity; and Systems and System Models. NGSS also states that the Nature of Science (NOS) should be an “essential part” of science education. NOS topics include, for example, understanding that scientific investigations use a variety of methods, that scientific knowledge is based on empirical evidence, that scientific explanations are open to revision in light of new evidence, and an understanding the nature of scientific models.

  4. Calibration results using highly aberrated images for aligning the JWST instruments to the telescope

    Science.gov (United States)

    Smith, Koby Z.; Acton, D. Scott; Gallagher, Ben B.; Knight, J. Scott; Dean, Bruce H.; Jurling, Alden S.; Zielinski, Thomas P.

    2016-07-01

    The James Webb Space Telescope (JWST) project is an international collaboration led by NASA's Goddard Space Flight Center (GSFC) in Greenbelt, MD. JWST is NASA's flagship observatory that will operate nearly a million miles away from Earth at the L2 Lagrange point. JWST's optical design is a three-mirror anastigmat with four main optical components; 1) the eighteen Primary Mirror Segment Assemblies (PMSA), 2) a single Secondary Mirror Assembly (SMA), 3) an Aft-Optics Subsystem (AOS) consisting of a Tertiary Mirror and Fine Steering Mirror, and 4) an Integrated Science Instrument Module consisting of the various instruments for JWST. JWST's optical system has been designed to accommodate a significant amount of alignment capability and risk with the PMSAs and SMA having rigid body motion available on-orbit just for alignment purposes. However, the Aft-Optics Subsystem (AOS) and Integrated Science Instrument Module (ISIM) are essentially fixed optical subsystems within JWST, and therefore the cryogenic alignment of the AOS to the ISIM is critical to the optical performance and mission success of JWST. In support of this cryogenic alignment of the AOS to ISIM, an array of fiber optic sources, known as the AOS Source Plate Assembly (ASPA), are placed near the intermediate image location of JWST (between the secondary and tertiary mirrors) during thermal vacuum ground-test operations. The AOS produces images of the ASPA fiber optic sources at the JWST focal surface location, where they are captured by the various science instruments. In this manner, the AOS provides an optical yardstick by which the instruments within ISIM can evaluate their relative positions to and the alignment of the AOS to ISIM can be quantified. However, since the ASPA is located at the intermediate image location of the JWST three-mirror anastigmat design, the images of these fiber optic sources produced by the AOS are highly aberrated with approximately 2-3μm RMS wavefront error consisting

  5. Entanglement of science teacher's lives and work

    DEFF Research Database (Denmark)

    Daugbjerg, Peer

    of educational restructuring. The teachers’ work and lives in the contemporary school settings are based on the continuity of their experiences and the relations that have formed them. The interaction between critical influences and tensions shapes the personal and professional experiences, and further produces......This thesis focuses on science teachers’ lived experience, their social position and their teaching. The guiding question for the documented research has been: How is science teachers’ work related to their lives? The aim was to situate the voice and body of science teachers in the contemporary era...... negative or positive outcomes in terms of teachers’ sense of commitment, resilience, well-being and capacity to teach. Personal and professional events constitute and shape a teacher’s past and present experiences. They may not be conspicuous at first glance, but they somehow affect the way the teacher...

  6. Observations of Transiting Exoplanets with the James Webb Space Telescope (JWST), Publications of the Astronomical Society of the Pacific (PASP), December 2014

    CERN Document Server

    Beichman, Charles; Knutson, Heather; Smith, Roger; Dressing, Courtney; Latham, David; Deming, Drake; Lunine, Jonathan; Lagage, Pierre-Olivier; Sozzetti, Alessandro; Beichman, Charles; Sing, David; Kempton, Eliza; Ricker, George; Bean, Jacob; Kreidberg, Laura; Bouwman, Jeroen; Crossfield, Ian; Christiansen, Jessie; Ciardi, David; Fortney, Jonathan; Albert, Loïc; Doyon, René; Rieke, Marcia; Rieke, George; Clampin, Mark; Greenhouse, Matt; Goudfrooij, Paul; Hines, Dean; Keyes, Tony; Lee, Janice; McCullough, Peter; Robberto, Massimo; Stansberry, John; Valenti, Jeff; Deroo, Pieter D; Mandell, Avi; Ressler, Michael E; Shporer, Avi; Swain, Mark; Vasisht, Gautam; Carey, Sean; Krick, Jessica; Birkmann, Stephan; Ferruit, Pierre; Giardino, Giovanna; Greene, Tom; Howell, Steve

    2014-01-01

    This article summarizes a workshop held on March, 2014, on the potential of the James Webb Space Telescope (JWST) to revolutionize our knowledge of the physical properties of exoplanets through transit observations. JWST's unique combination of high sensitivity and broad wavelength coverage will enable the accurate measurement of transits with high signal-to-noise. Most importantly, JWST spectroscopy will investigate planetary atmospheres to determine atomic and molecular compositions, to probe vertical and horizontal structure, and to follow dynamical evolution, i.e. exoplanet weather. JWST will sample a diverse population of planets of varying masses and densities in a wide variety of environments characterized by a range of host star masses and metallicities, orbital semi-major axes and eccentricities. A broad program of exoplanet science could use a substantial fraction of the overall JWST mission.

  7. Advanced cryogenic thermal switches for JWST

    Science.gov (United States)

    Bugby, David; Beres, Matthew; Stouffer, Charles; Rodriguez, Jose

    2005-08-01

    This paper describes two cryogenic thermal switches (CTSWs) under development for instruments on the James Webb Space Telescope (JWST). The first thermal switch was designed to extend the life of the solid H2 dewar for the 6 K Mid Infrared Instrument (MIRI) while the second thermal switch is needed for contamination and over-temperature control of three 35 K instruments on the Integrated Science Instrument Module (ISIM). In both cases, differential thermal expansion (DTE) between two materials having differing CTE values is the process that underpins the thermal switching. The patented DTE-CTSW design utilizes two metallic end-pieces, one cup-shaped and the other disc-shaped (both MIRI end-pieces are Al while ISIM uses an Al/Invar cup and an Al disc), joined by an axially centered Ultem rod, which creates a narrow, flat gap between the cup (rim) and disc. A heater is bonded to the rod center. Upon cooling one or both end-pieces, the rod contracts relative to the end-pieces and the gap closes, turning the CTSW ON. When the rod heater is turned on, the rod expands relative to the end-pieces and the gap opens, turning the CTSW OFF. During testing from 6-35 K, ON conductances of 0.3-12 W/K and OFF resistances greater than 2500 K/W were measured. Of particular importance at 6 K was the Al oxide layer, which was found to significantly decrease DTE-CTSW ON conductance when the mating surfaces were bare Al. When the mating surfaces were gold-plated, the adverse impact of the oxide layer was mitigated. This paper will describe both efforts from design through model correlation.

  8. Commentary: JWST near-infrared detector degradation— finding the problem, fixing the problem, and moving forward

    Directory of Open Access Journals (Sweden)

    Bernard J. Rauscher

    2012-06-01

    Full Text Available The James Webb Space Telescope (JWST is the successor to the Hubble Space Telescope. JWST will be an infrared-optimized telescope, with an approximately 6.5 m diameter primary mirror, that is located at the Sun-Earth L2 Lagrange point. Three of JWST’s four science instruments use Teledyne HgCdTe HAWAII-2RG (H2RG near infrared detector arrays. During 2010, the JWST Project noticed that a few of its 5 μm cutoff H2RG detectors were degrading during room temperature storage, and NASA chartered a “Detector Degradation Failure Review Board” (DD-FRB to investigate. The DD-FRB determined that the root cause was a design flaw that allowed indium to interdiffuse with the gold contacts and migrate into the HgCdTe detector layer. Fortunately, Teledyne already had an improved design that eliminated this degradation mechanism. During early 2012, the improved H2RG design was qualified for flight and JWST began making additional H2RGs. In this article, we present the two public DD-FRB “Executive Summaries” that: (1 determined the root cause of the detector degradation and (2 defined tests to determine whether the existing detectors are qualified for flight. We supplement these with a brief introduction to H2RG detector arrays, some recent measurements showing that the performance of the improved design meets JWST requirements, and a discussion of how the JWST Project is using cryogenic storage to retard the degradation rate of the existing flight spare H2RGs.

  9. The JWST North Ecliptic Pole Survey Field for Time-domain Studies

    Science.gov (United States)

    Jansen, Rolf A.; Alpaslan, Mehmet; Ashby, Matthew; Ashcraft, Teresa; Cohen, Seth H.; Condon, James J.; Conselice, Christopher; Ferrara, Andrea; Frye, Brenda L.; Grogin, Norman A.; Hammel, Heidi B.; Hathi, Nimish P.; Joshi, Bhavin; Kim, Duho; Koekemoer, Anton M.; Mechtley, Matt; Milam, Stefanie N.; Rodney, Steven A.; Rutkowski, Michael J.; Strolger, Louis-Gregory; Trujillo, Chadwick A.; Willmer, Christopher; Windhorst, Rogier A.; Yan, Haojing

    2017-01-01

    The JWST North Ecliptic Pole (NEP) Survey field is located within JWST's northern Continuous Viewing Zone, will span ˜14‧ in diameter (˜10‧ with NIRISS coverage) and will be roughly circular in shape (initially sampled during Cycle 1 at 4 distinct orientations with JWST/NIRCam's 4.4‧×2.2‧ FoV —the JWST “windmill”) and will have NIRISS slitless grism spectroscopy taken in parallel, overlapping an alternate NIRCam orientation. This is the only region in the sky where JWST can observe a clean extragalactic deep survey field (free of bright foreground stars and with low Galactic foreground extinction AV) at arbitrary cadence or at arbitrary orientation. This will crucially enable a wide range of new and exciting time-domain science, including high redshift transient searches and monitoring (e.g., SNe), variability studies from Active Galactic Nuclei to brown dwarf atmospheres, as well as proper motions of extreme scattered Kuiper Belt and Oort Cloud Objects, and of nearby Galactic brown dwarfs, low-mass stars, and ultracool white dwarfs. We therefore welcome and encourage follow-up through GO programs of the initial GTO observations to realize its potential as a JWST time-domain community field. The JWST NEP Survey field was selected from an analysis of WISE 3.4+4.6 micron, 2MASS JHKs, and SDSS ugriz source counts and of Galactic foreground extinction, and is one of very few such ˜10‧ fields that are devoid of sources brighter than mAB = 16 mag. We have secured deep (mAB ˜ 26 mag) wide-field (˜23‧×25‧) Ugrz images of this field and its surroundings with LBT/LBC. We also expect that deep MMT/MMIRS YJHK images, deep 8-12 GHz VLA radio observations (pending), and possibly HST ACS/WFC and WFC3/UVIS ultraviolet-visible images will be available before JWST launches in Oct 2018.

  10. Emulating JWST Exoplanet Transit Observations in a Testbed laboratory experiment

    Science.gov (United States)

    Touli, D.; Beichman, C. A.; Vasisht, G.; Smith, R.; Krist, J. E.

    2014-12-01

    The transit technique is used for the detection and characterization of exoplanets. The combination of transit and radial velocity (RV) measurements gives information about a planet's radius and mass, respectively, leading to an estimate of the planet's density (Borucki et al. 2011) and therefore to its composition and evolutionary history. Transit spectroscopy can provide information on atmospheric composition and structure (Fortney et al. 2013). Spectroscopic observations of individual planets have revealed atomic and molecular species such as H2O, CO2 and CH4 in atmospheres of planets orbiting bright stars, e.g. Deming et al. (2013). The transit observations require extremely precise photometry. For instance, Jupiter transit results to a 1% brightness decrease of a solar type star while the Earth causes only a 0.0084% decrease (84 ppm). Spectroscopic measurements require still greater precision ppm. The Precision Projector Laboratory (PPL) is a collaboration between the Jet Propulsion Laboratory (JPL) and California Institute of Technology (Caltech) to characterize and validate detectors through emulation of science images. At PPL we have developed a testbed to project simulated spectra and other images onto a HgCdTe array in order to assess precision photometry for transits, weak lensing etc. for Explorer concepts like JWST, WFIRST, EUCLID. In our controlled laboratory experiment, the goal is to demonstrate ability to extract weak transit spectra as expected for NIRCam, NIRIS and NIRSpec. Two lamps of variable intensity, along with spectral line and photometric simulation masks emulate the signals from a star-only, from a planet-only and finally, from a combination of a planet + star. Three masks have been used to simulate spectra in monochromatic light. These masks, which are fabricated at JPL, have a length of 1000 pixels and widths of 2 pixels, 10 pixels and 1 pixel to correspond respectively to the noted above JWST instruments. From many-hour long observing

  11. Unique Spectroscopy and Imaging of Mars with JWST

    CERN Document Server

    Villanueva, Geronimo L; Clancy, Todd R; Encrenaz, Therese; Fouchet, Thierry; Hartogh, Paul; Lellouch, Emmanuel; Lopez-Valverde, Miguel A; Mumma, Michael J; Novak, Robert E; Smith, Michael D; Vandaele, Ann-Carine; Wolff, Michael J; Ferruit, Pierre; Milam, Stefanie N

    2015-01-01

    In this document, we summarize the main capabilities of the James Webb Space Telescope (JWST) for performing observations of Mars. The distinctive vantage point of JWST at the Sun-Earth Lagrange point (L2) will allow sampling the full observable disk, permitting the study of short-term phenomena, diurnal processes (across the East-West axis) and latitudinal processes between the hemispheres (including seasonal effects) with excellent spatial resolutions (0.07 arcsec at 2 {\\mu}m). Spectroscopic observations will be achievable in the 0.7-5 {\\mu}m spectral region with NIRSpec at a maximum resolving power of 2700, and with 8000 in the 1-1.25 {\\mu}m range. Imaging will be attainable with NIRCam at 4.3 {\\mu}m and with two narrow filters near 2 {\\mu}m, while the nightside will be accessible with several filters in the 0.5 to 2 {\\mu}m. Such a powerful suite of instruments will be a major asset for the exploration and characterization of Mars. Some science cases include the mapping of the water D/H ratio, investigatio...

  12. High Contrast Imaging with the JWST NIRCAM Coronagraph

    Science.gov (United States)

    Green, Joseph J.; Beichman, Charles; Basinger, Scott A.; Horner, Scott; Meyer, Michael; Redding, David C.; Rieke, Marcia; Trauger, John T.

    2005-01-01

    Relative to ground-based telescopes, the James Webb Space Telescope (JWST) will have a substantial sensitivity advantage in the 2.2-5pm wavelength range where brown dwarfs and hot Jupiters are thought to have significant brightness enhancements. To facilitate high contrast imaging within this band, the Near-Infrared Camera (NIRCAM) will employ a Lyot coronagraph with an array of band-limited image-plane occulting spots. In this paper, we provide the science motivation for high contrast imaging with NIRCAM, comparing its expected performance to that of the Keck, Gemini and 30 m (TMT) telescopes equipped with Adaptive Optics systems of different capabilities. We then describe our design for the NIRCAM coronagraph that enables imaging over the entire sensitivity range of the instrument while providing significant operational flexibility. We describe the various design tradeoffs that were made in consideration of alignment and aberration sensitivities and present contrast performance in the presence of JWST's expected optical aberrations. Finally we show an example of a that can provide 10-5 companion sensitivity at sub-arcsecond separations.

  13. Large Space Optics: From Hubble to JWST and Beyond

    Science.gov (United States)

    Stahl, H. Philip

    2008-01-01

    If necessity truly is the mother of invention, then advances in lightweight space mirror technology have been driven by launch vehicle mass and volume constraints. In the late 1970 s, at the start of Hubble development, the state of the art in ground based telescopes was 3 to 4 meter monolithic primary mirrors with masses of 6000 to 10,000 kg - clearly too massive for the planned space shuttle 25,000 kg capability to LEO. Necessity led Hubble to a different solution. Launch vehicle mass constraints (and cost) resulted in the development of a 2.4 meter lightweight eggcrate mirror. At 810 kg (180 kg/m2), this mirror was approximately 7.4% of HST s total 11,110 kg mass. And, the total observatory structure at 4.3 m x 13.2 m fit snuggly inside the space shuttle 4.6 m x 18.3 m payload bay. In the early 1990 s, at the start of JWST development, the state of the art in ground based telescopes was 8 meter class monolithic primary mirrors (16,000 to 23,000 kg) and 10 meter segmented mirrors (14,400 kg). Unfortunately, launch vehicles were still constrained to 4.5 meter payloads and 25,000 kg to LEO or 6,600 kg to L2. Furthermore, science now demanded a space telescope with 6 to 8 meter aperture operating at L2. Mirror technology was identified as a critical capability necessary to enable the next generation of large aperture space telescopes. Specific telescope architectures were explored via three independent design concept studies conducted during the summer of 1996 (1). These studies identified two significant architectural constraints: segmentation and areal density. Because the launch vehicle fairing payload dynamic envelop diameter is approximately 4.5 meters, the only way to launch an 8 meter class mirror is to segment it, fold it and deploy it on orbit - resulting in actuation and control requirements. And, because of launch vehicle mass limits, the primary mirror allocation was only 1000 kg - resulting in a maximum areal density of 20 kg/m2. At the inception of

  14. Lessons from Coronagraphic Imaging with HST that may apply to JWST

    Science.gov (United States)

    Grady, C. A.; Hines, Dean C.; Schneider, Glenn; McElwain, Michael W.

    2017-06-01

    One of the major capabilities offered by JWST is coronagraphic imaging from space, covering the near through mid-IR and optimized for study of planet formation and the evolution of planetary systems. Planning for JWST has resulted in expectations for instrument performance, observation strategies and data reduction approaches. HST with 20 years of coronagraphic imaging offers some experience which may be useful to those planning for JWST. 1) Real astronomical sources do not necessarily conform to expectations. Debris disks may be accompanied by more distant material, and some systems may be conspicuous in scattered light when offering only modest IR excesses. Proto-planetary disks are not constantly illuminated, and thus a single epoch observation of the source may not be sufficient to reveal everything about it. 2) The early expectation with NICMOS was that shallow, 2-roll observations would reveal a wealth of debris disks imaged in scattered light, and that only a limited set of PSF observations would be required. Instead, building up a library of spatially resolved disks in scattered light has proven to require alternate observing strategies, is still on-going, and has taken far longer than expected. 3) A wealth of coronagraphic options with an instrument may not be scientifically informative, unless there is a similar time investment in acquisition of calibration data in support of the science observations. 4) Finally, no one anticipated what can be gleaned from coronagraphic imaging. We should expect similar, unexpected, and ultimately revolutionary discoveries with JWST.

  15. Successful Science Learning from Practical Work

    Science.gov (United States)

    Moeed, Azra

    2011-01-01

    Science education research can be categorised into three broad dimensions: knowing science, doing of science and learning about the nature of science. The concerns, doubts and relative importance of each of these aspects in relation to students' learning are debated in the literature. The findings of the empirical research carried out in New…

  16. Women Working in Engineering and Science

    Science.gov (United States)

    Luna, Bernadette; Kliss, Mark (Technical Monitor)

    1998-01-01

    The presentation will focus on topics of interest to young women pursuing an engineering or scientific career, such as intrinsic personality traits of most engineers, average salaries for the various types of engineers, appropriate preparation classes at the high school and undergraduate levels, gaining experience through internships, summer jobs and graduate school, skills necessary but not always included in engineering curricula (i.e., multimedia, computer skills, communication skills), the work environment, balancing family and career, and sexual harassment. Specific examples from the speaker's own experience in NASA's Space Life Sciences Program will be used to illustrate the above topics. In particular, projects from Extravehicular Activity and Protective Systems research and Regenerative Life Support research will be used as examples of real world problem-solving to enable human exploration of the solar system.

  17. Emerging Technologies and Outreach with JWST

    Science.gov (United States)

    Green, Joel D.; Smith, Denise A.; Meinke, Bonnie K.; Lawton, Brandon L.; Kenney, Jessica; Jirdeh, Hussein

    2017-06-01

    The James Webb Space Telescope (JWST), NASA’s next great observatory launching in October 2018, required a dozen new technologies to develop. How will we maintain the prestige and cultural impact of Hubble as the torch passes to Webb? Emerging technologies such as augmented and virtual reality bring the viewer into the data and the concept in previously unimaginable immersive detail. Adoption of mobile devices has expanded access to information for wide swaths of the public. Software like Worldwide Telescope to hardware like the Occulus Rift are providing new avenues for learning. If we develop materials properly tailored to this medium, we can reach more diverse audiences than ever before. STScI is pioneering some tools related to JWST for showcasing at AAS, and in local events, which I highlight here.

  18. The Home Stretch Almost! Science with the Hubble and James Webb Space Telescope V

    Science.gov (United States)

    Ochs, Bill

    2017-01-01

    JWST has Made tremendous progress in the last few years. JWST Is fully immersed in integration and test, but testing JWST is a formable challenge. JWST's size, complexity, and cryogenic characteristics require a multifaceted test plan to verify mission readiness. Each of these tests are opportunities to uncover issues which must be corrected to be able to move forward. All observatory control, science planning, and science data processing operational systems are on schedule.?

  19. WebbPSF for JWST and WFIRST

    Science.gov (United States)

    Long, Joseph D.; Perrin, Marshall D.; Zimmerman, Neil T.; Brooks, Keira

    2017-01-01

    Modeling a telescope's point spread function accurately is key to predicting its performance and extracting information from observations. WebbPSF is a flexible Python-based PSF simulation tool for JWST and WFIRST, developed at STScI. The WebbPSF-WFIRST module implements a model for the proposed Wide Field Instrument, as well as a proof-of-concept model for the Coronagraph Instrument. Since its announcement and public release at the Winter 2016 AAS, WebbPSF-WFIRST has been enhanced with the Cycle 6 design updates to the wide field instrument model. Additionally, the JupyterHub-based WFIRST Tools Server effort at STScI has provided access to these tools for dozens of users without the overhead of installing the software locally. For JWST, the optical models have been updated based on the latest test data and metrology for the instruments and the telescope flight hardware, including as-built mirror surface figures, variation between different field points, and updated optical budgets for in flight performance. WebbPSF has been checked against instrument test data from previous campaigns, and analysis of the PSF images taken during the JWST CV3 cryo-vac test campaign is currently underway.

  20. The Science of Social Work and Its Relationship to Social Work Practice

    Science.gov (United States)

    Anastas, Jeane W.

    2014-01-01

    As John Brekke has observed, social work does not use the word "science" to define itself, suggesting a need to articulate a science of social work. This article discusses the science of social work and its relationship to social work practice in the United States, arguing that a "rapprochement" between practice and science…

  1. An Update on Simulating Imaging, Spectroscopic, and Coronagraphic PSFs for JWST (and WFIRST too!)

    Science.gov (United States)

    Perrin, Marshall D.; Long, Joseph D.; Zimmerman, Neil T.; Van Gorkom, Kyle

    2016-06-01

    Simulated point spread functions (PSFs) are an essential tool in preparing for future space telescopes, supporting pre-launch science simulations, observation planning, and analysis software development. The open-source Python package WebbPSF provides simulated PSFs for all of JWST's instruments and observing modes. We present the latest updates to WebbPSF based on both updated models ofthe assembled telescope optics and recent cryo-test data for the science instruments. Outputs from this latest version of WebbPSF will support the JWST Exposure Time Calculator and the first calls for proposals in the year ahead, among many other uses by the community. Furthermore, the same toolkit also now provides support for simulating PSFs for both the WFI and CGI instruments planned for WFIRST.

  2. Simulated JWST/NIRISS Spectroscopy of Anticipated TESS Planets and Selected Super-Earths Discovered from K2 and Ground-Based Surveys

    Science.gov (United States)

    Louie, Dana; Albert, Loic; Deming, Drake

    2017-01-01

    The 2018 launch of James Webb Space Telescope (JWST), coupled with the 2017 launch of the Transiting Exoplanet Survey Satellite (TESS), heralds a new era in Exoplanet Science, with TESS projected to detect over one thousand transiting sub-Neptune-sized planets (Ricker et al, 2014), and JWST offering unprecedented spectroscopic capabilities. Sullivan et al (2015) used Monte Carlo simulations to predict the properties of the planets that TESS is likely to detect, and published a catalog of 962 simulated TESS planets. Prior to TESS launch, the re-scoped Kepler K2 mission and ground-based surveys such as MEarth continue to seek nearby Earth-like exoplanets orbiting M-dwarf host stars. The exoplanet community will undoubtedly employ JWST for atmospheric characterization follow-up studies of promising exoplanets, but the targeted planets for these studies must be chosen wisely to maximize JWST science return. The goal of this project is to estimate the capabilities of JWST’s Near InfraRed Imager and Slitless Spectrograph (NIRISS)—operating with the GR700XD grism in Single Object Slitless Spectrography (SOSS) mode—during observations of exoplanets transiting their host stars. We compare results obtained for the simulated TESS planets, confirmed K2-discovered super-Earths, and exoplanets discovered using ground-based surveys. By determining the target planet characteristics that result in the most favorable JWST observing conditions, we can optimize the choice of target planets in future JWST follow-on atmospheric characterization studies.

  3. Teaching "How Science Works" by Making and Sharing Videos

    Science.gov (United States)

    Ingram, Neil

    2010-01-01

    "Science.tv" is a website where teachers and pupils can find quality video clips on a variety of scientific topics. It enables pupils to share research ideas and adds a dynamic new dimension to practical work. It has the potential to become an innovative way of incorporating "How science works" into secondary science curricula by encouraging…

  4. The Planning Process for Multi-Object Spectroscopy with the JWST Near-Infrared Spectrograph

    Science.gov (United States)

    Beck, Tracy L.; Karakla, D. M.; Shyrokov, A.; Pontoppidan, K.; Soderblom, D. R.; Valenti, J. A.; Kassin, S. A.; Gilbert, K.; Blair, W. P.; Muzerolle, J.; Tumlinson, J.; Keyes, C. D.; Pavlovsky, C. M.; LeBlanc, T.

    2014-01-01

    The Near-Infrared Spectrograph (NIRSpec) for the James Webb Space Telescope (JWST) will have a powerful multi-object spectroscopy mode using four configurable Micro-Shutter Arrays (MSAs). The contiguous MSA shutters can be opened to form slits on astronomical targets, for simultaneous spectroscopy of up to 100 sources per exposure. The NIRSpec MSA shutters are in a fixed grid pattern, and careful analysis in the observation planning process will be crucial for optimal definition of science exposures. Our goal is to maximize the number of astronomical science sources observed in the fewest number of MSA slit configurations. We are developing algorithms in the NIRSpec MSA Planning Tool (MPT) to improve the quality of planned observations using several common science observing strategies as test use cases. For example, the needs for planning extremely deep exposures on a small number of JWST discovered z > 10 galaxy candidates will differ significantly from the requirements for planning spectral observations on a representative sample of stars from a galactic star cluster catalog. In this poster, we present a high level overview of our plans to develop and optimize the MPT for the JWST NIRSpec multi-object spectroscopy mode.

  5. NIRCam: Development and Testing of the JWST Near-Infrared Camera

    Science.gov (United States)

    Greene, Thomas; Beichman, Charles; Gully-Santiago, Michael; Jaffe, Daniel; Kelly, Douglas; Krist, John; Rieke, Marcia; Smith, Eric H.

    2011-01-01

    The Near Infrared Camera (NIRCam) is one of the four science instruments of the James Webb Space Telescope (JWST). Its high sensitivity, high spatial resolution images over the 0.6 - 5 microns wavelength region will be essential for making significant findings in many science areas as well as for aligning the JWST primary mirror segments and telescope. The NIRCam engineering test unit was recently assembled and has undergone successful cryogenic testing. The NIRCam collimator and camera optics and their mountings are also progressing, with a brass-board system demonstrating relatively low wavefront error across a wide field of view. The flight model?s long-wavelength Si grisms have been fabricated, and its coronagraph masks are now being made. Both the short (0.6 - 2.3 microns) and long (2.4 - 5.0 microns) wavelength flight detectors show good performance and are undergoing final assembly and testing. The flight model subsystems should all be completed later this year through early 2011, and NIRCam will be cryogenically tested in the first half of 2011 before delivery to the JWST integrated science instrument module (ISIM).

  6. Operationalizing Social Work Science through Research-Practice Partnerships: Lessons from Implementation Science

    Science.gov (United States)

    Palinkas, Lawrence A.; He, Amy S.; Choy-Brown, Mimi; Hertel, Amy Locklear

    2017-01-01

    Recent efforts to identify and promote a distinct science for the discipline of social work have led to an ongoing debate regarding the nature and function of such a science. Central to this debate is a lack of consensus as to how to operationalize a social work science. Drawing from the field of implementation science and its application in…

  7. Operationalizing Social Work Science through Research-Practice Partnerships: Lessons from Implementation Science

    Science.gov (United States)

    Palinkas, Lawrence A.; He, Amy S.; Choy-Brown, Mimi; Hertel, Amy Locklear

    2017-01-01

    Recent efforts to identify and promote a distinct science for the discipline of social work have led to an ongoing debate regarding the nature and function of such a science. Central to this debate is a lack of consensus as to how to operationalize a social work science. Drawing from the field of implementation science and its application in…

  8. Making Mathematics and Science Work for Hispanics.

    Science.gov (United States)

    Rendon, Laura I.; Triana, Estrella M.

    This document discusses barriers that impede the progress and participation of Hispanic American students in mathematics and science education, and recommends extensive educational reforms. Following an introduction, the first of two main sections reviews the current Hispanic American underrepresentation in mathematics and science and describes…

  9. Science, Innovation, and Social Work: Purpose: Clash or Convergence?

    Science.gov (United States)

    Flynn, Marilyn L.

    2017-01-01

    Social work as a human services profession has been distinctive for its inclusion of research as a required element of practice and instrument in instigating reform. At the present time, the relationship of social work to science and a redefinition of social work as a science have reentered our national dialogue with new force. This expansion of…

  10. Science, Innovation, and Social Work: Purpose: Clash or Convergence?

    Science.gov (United States)

    Flynn, Marilyn L.

    2017-01-01

    Social work as a human services profession has been distinctive for its inclusion of research as a required element of practice and instrument in instigating reform. At the present time, the relationship of social work to science and a redefinition of social work as a science have reentered our national dialogue with new force. This expansion of…

  11. Extrasolar Planets Observed with JWST and the ELTs

    Science.gov (United States)

    Deming, L. Drake

    2010-01-01

    The advent of cryogenic space-borne infrared observatories such as the Spitzer Space Telescope has lead to a revolution in the study of planets and planetary systems orbiting sun-like stars. Already Spitzer has characterized the emergent infrared spectra of close-in giant exoplanets using transit and eclipse techniques. The James Webb Space Telescope (JWST) will be able to extend these studies to superEarth exoplanets orbiting in the habitable zones of M-dwarf stars in the near solar neighborhood. The forthcoming ground-based Extremely Large Telescopes (ELTs) will playa key role in these studies, being especially valuable for spectroscopy at higher spectral resolving powers where large photon fluxes are needed. The culmination of this work within the next two decades will be the detection and spectral characterization of the major molecular constituents in the atmosphere of a habitable superEarth orbiting a nearby lower main sequence star.

  12. Comparing and Contrasting Detectors: JWST NIR vs HST WFC3

    Science.gov (United States)

    Rauscher, Bernard J.

    2015-01-01

    In many ways, WFC3s IR channel is a good indicator for what to expect with JWST. There are some differences, most of which should be beneficial in JWST- JWSTs lower operating temperature will freeze out charge traps that would affect WFC3. Benefits should include lower dark current, lower persistence, and better reciprocity- JWSTs more recent HgCdTe process has lower defect density. The benefits are as described above- JWST uses better indium barriers. The benefits should include fewer RC type pixels. One area where more study might be beneficial is stability. The detector electronics play a significant role in determining how stable a detector system is(v.s. bias drifts and photometry). JWSTs SIDECARs are completely WFC3s Ball electronics- Studies comparing the bias and photometric stability of WFC3 and JWST might be useful to informing data acquisition and calibration strategies for JWST.

  13. CHARACTERIZING TRANSITING EXOPLANET ATMOSPHERES WITH JWST

    Energy Technology Data Exchange (ETDEWEB)

    Greene, Thomas P. [NASA Ames Research Center, Space Science and Astrobiology Division, M.S. 245-6, Moffett Field, CA 94035 (United States); Line, Michael R.; Montero, Cezar; Fortney, Jonathan J. [Department of Astronomy and Astrophysics, University of California, Santa Cruz, CA 95064 (United States); Lustig-Yaeger, Jacob [Department of Astronomy, Box 351580, University of Washington, Seattle, WA 98195 (United States); Luther, Kyle, E-mail: tom.greene@nasa.gov [Department of Physics, University of California, 366 LeConte Hall MC 7300, Berkeley, CA 94720 (United States)

    2016-01-20

    We explore how well spectra from the James Webb Space Telescope (JWST) will likely constrain bulk atmospheric properties of transiting exoplanets. We start by modeling the atmospheres of archetypal hot Jupiter, warm Neptune, warm sub-Neptune, and cool super-Earth planets with atmospheres that are clear, cloudy, or of high mean molecular weight (HMMW). Next we simulate the λ = 1–11 μm transmission and emission spectra of these systems for several JWST instrument modes for single-transit or single-eclipse events. We then perform retrievals to determine how well temperatures and molecular mixing ratios (CH{sub 4}, CO, CO{sub 2}, H{sub 2}O, NH{sub 3}) can be constrained. We find that λ = 1–2.5 μm transmission spectra will often constrain the major molecular constituents of clear solar-composition atmospheres well. Cloudy or HMMW atmospheres will often require full 1–11 μm spectra for good constraints, and emission data may be more useful in cases of sufficiently high F{sub p} and high F{sub p}/F{sub *}. Strong temperature inversions in the solar-composition hot-Jupiter atmosphere should be detectable with 1–2.5+ μm emission spectra, and 1–5+ μm emission spectra will constrain the temperature–pressure profiles of warm planets. Transmission spectra over 1–5+ μm will constrain [Fe/H] values to better than 0.5 dex for the clear atmospheres of the hot and warm planets studied. Carbon-to-oxygen ratios can be constrained to better than a factor of 2 in some systems. We expect that these results will provide useful predictions of the scientific value of single-event JWST spectra until its on-orbit performance is known.

  14. Response: Epistemological Issues of Social Work Science as a Translational Action Science

    Science.gov (United States)

    Goppner, Hans-Jurgen

    2012-01-01

    A science-based practice should be caring, there is no dissent about this. But why a social work science? Until now "things are fine," and practice seems to be getting on very well without it!? It is claimed that there is no alternative in its own interest. Social work needs social work science because of the epistemological issues linked to the…

  15. Status of the JWST sunshield and spacecraft

    Science.gov (United States)

    Arenberg, J.; Flynn, J.; Cohen, A.; Lynch, R.; Cooper, J.

    2016-07-01

    This paper reports on the development, manufacture and integration of the James Webb Space Telescope's sunshield and spacecraft. Both of these JWST elements have completed design and development testing. This paper will review basic architecture and roles of these systems. Also to be presented is the current state of manufacture, assembly integration and test. This paper will conclude with a look at the road ahead for each subsystem prior to integration with the integrated telescope and instrument elements at Northrop Grumman's Space Park facility in late 2017.

  16. Analyzing the Scientific Evolution of Social Work Using Science Mapping

    Science.gov (United States)

    Martínez, Ma Angeles; Cobo, Manuel Jesús; Herrera, Manuel; Herrera-Viedma, Enrique

    2015-01-01

    Objectives: This article reports the first science mapping analysis of the social work field, which shows its conceptual structure and scientific evolution. Methods: Science Mapping Analysis Software Tool, a bibliometric science mapping tool based on co-word analysis and h-index, is applied using a sample of 18,794 research articles published from…

  17. Characterizing transiting exoplanet atmospheres with JWST

    CERN Document Server

    Greene, Thomas P; Montero, Cezar; Fortney, Jonathan J; Lustig-Yeager, Jacob; Luther, Kyle

    2015-01-01

    We explore how well James Webb Space Telescope (JWST) spectra will likely constrain bulk atmospheric properties of transiting exoplanets. We start by modeling the atmospheres of archetypal hot Jupiter, warm Neptune, warm sub-Neptune, and cool super-Earth planets with clear, cloudy, or high mean molecular weight atmospheres. Next we simulate the $\\lambda = 1 - 11$ $\\mu$m transmission and emission spectra of these systems for several JWST instrument modes for single transit and eclipse events. We then perform retrievals to determine how well temperatures and molecular mixing ratios (CH$_4$, CO, CO$_2$, H$_2$O, NH$_3$) can be constrained. We find that $\\lambda = 1 - 2.5$ $\\mu$m transmission spectra will often constrain the major molecular constituents of clear solar composition atmospheres well. Cloudy or high mean molecular weight atmospheres will often require full $1 - 11$ $\\mu$m spectra for good constraints, and emission data may be more useful in cases of sufficiently high $F_p$ and high $F_p/F_*$. Strong t...

  18. Science Education and the Work of Art

    Science.gov (United States)

    Toscano, Maurizio

    2012-01-01

    Martin Heidegger's seminal essay, "The Origin of the Work of Art", captures much of what is original and enduring in his philosophical offering. Although his essay takes as its subject the relationship between art, the work of art and the artist; Heidegger's inquiry covers conceptual ground that is particularly pertinent to…

  19. Dry Laboratories in Science Education : Computer-based Practical Work

    NARCIS (Netherlands)

    Kirschner, P.A.; Huisman, W.

    1998-01-01

    Practical (laboratory) work in science education has traditionally been used to allow students to rediscover already known concepts and ideas, to demonstrate concepts taught in the classroom or, in the case of inquirybased science curricula, to teach concepts. Often, these laboratory practicals do n

  20. Dry Laboratories in Science Education : Computer-based Practical Work

    NARCIS (Netherlands)

    Kirschner, P.A.; Huisman, W.

    1998-01-01

    Practical (laboratory) work in science education has traditionally been used to allow students to rediscover already known concepts and ideas, to demonstrate concepts taught in the classroom or, in the case of inquirybased science curricula, to teach concepts. Often, these laboratory practicals do n

  1. A Perspective on Primary School Science. Learning in Science Project (Primary). Working Paper No. 104.

    Science.gov (United States)

    Symington, David; And Others

    The Learning in Science Project (Primary--LISP(P)--designed to investigate the teaching and learning of science in New Zealand primary schools, arises from the work of the original Learning in Science Project (LISP). This paper is an attempt to clarify the direction of LISP(P) as it moves toward the central phase of the research. The ideas…

  2. Working Alongside Scientists. Impacts on Primary Teacher Beliefs and Knowledge About Science and Science Education

    Science.gov (United States)

    Anderson, Dayle; Moeed, Azra

    2017-05-01

    Current curriculum demands require primary teachers to teach about the Nature of Science; yet, few primary teachers have had opportunity to learn about science as a discipline. Prior schooling and vicarious experiences of science may shape their beliefs about science and, as a result, their science teaching. This qualitative study describes the impact on teacher beliefs about science and science education of a programme where 26 New Zealand primary (elementary) teachers worked fulltime for 6 months alongside scientists, experiencing the nature of work in scientific research institutes. During the 6 months, teachers were supported, through a series of targeted professional development days, to make connections between their experiences working with scientists, the curriculum and the classroom. Data for the study consisted of mid- and end-of-programme written teacher reports and open-ended questionnaires collected at three points, prior to and following 6 months with the science host and after 6 to 12 months back in school. A shift in many teachers' beliefs was observed after the 6 months of working with scientists in combination with curriculum development days; for many, these changes were sustained 6 to 12 months after returning to school. Beliefs about the aims of science education became more closely aligned with the New Zealand curriculum and its goal of developing science for citizenship. Responses show greater appreciation of the value of scientific ways of thinking, deeper understanding about the nature of scientists' work and the ways in which science and society influence each other.

  3. Bayesian Approach for Reliability Assessment of Sunshield Deployment on JWST

    Science.gov (United States)

    Kaminskiy, Mark P.; Evans, John W.; Gallo, Luis D.

    2013-01-01

    Deployable subsystems are essential to mission success of most spacecraft. These subsystems enable critical functions including power, communications and thermal control. The loss of any of these functions will generally result in loss of the mission. These subsystems and their components often consist of unique designs and applications, for which various standardized data sources are not applicable for estimating reliability and for assessing risks. In this study, a Bayesian approach for reliability estimation of spacecraft deployment was developed for this purpose. This approach was then applied to the James Webb Space Telescope (JWST) Sunshield subsystem, a unique design intended for thermal control of the observatory's telescope and science instruments. In order to collect the prior information on deployable systems, detailed studies of "heritage information", were conducted extending over 45 years of spacecraft launches. The NASA Goddard Space Flight Center (GSFC) Spacecraft Operational Anomaly and Reporting System (SOARS) data were then used to estimate the parameters of the conjugative beta prior distribution for anomaly and failure occurrence, as the most consistent set of available data and that could be matched to launch histories. This allows for an emperical Bayesian prediction for the risk of an anomaly occurrence of the complex Sunshield deployment, with credibility limits, using prior deployment data and test information.

  4. Practical work in secondary science a minds-on approach

    CERN Document Server

    Abrahams, Ian

    2011-01-01

    Practical work is an essential feature of secondary science education. However, questions have been raised by some science educators about its effectiveness as a teaching and learning strategy. Whilst such an approach is generally effective in getting pupils to do things with objects and materials, it is seen as relatively ineffective in developing their conceptual understanding of the associated scientific ideas and concepts. Ian Abrahams argues that this is because it is practiced as a 'hands-on' rather than 'minds-on' activity. Abrahams draws together theory and practice on effective teaching and learning in practical work in science - covering biology, chemistry and physics. He provides clear guidance to ensure that students are encouraged and supported to be 'minds-on' as well as a 'hands-on' so that they can make the most of this learning experience. An invaluable text for inspiringaspiring andexperienced secondary science professionals, especially for those on M-level secondary science PGCE programmes.

  5. Non-redundant Aperture Masking Interferometry (AMI) and segment phasing with JWST-NIRISS

    Science.gov (United States)

    Sivaramakrishnan, Anand; Lafrenière, David; Ford, K. E. Saavik; McKernan, Barry; Cheetham, Anthony; Greenbaum, Alexandra Z.; Tuthill, Peter G.; Lloyd, James P.; Ireland, Michael J.; Doyon, René; Beaulieu, Mathilde; Martel, André; Koekemoer, Anton; Martinache, Frantz; Teuben, Peter

    2012-09-01

    The Aperture Masked Interferometry (AMI) mode on JWST-NIRISS is implemented as a 7-hole, 15% throughput, non-redundant mask (NRM) that operates with 5-8% bandwidth filters at 3.8, 4.3, and 4.8 microns. We present refined estimates of AMI's expected point-source contrast, using realizations of noise matched to JWST pointing requirements, NIRISS detector noise, and Rev-V JWST wavefront error models for the telescope and instrument. We describe our point-source binary data reduction algorithm, which we use as a standardized method to compare different observational strategies. For a 7.5 magnitude star we report a 10-a detection at between 8.7 and 9.2 magnitudes of contrast between 100 mas to 400 mas respectively, using closure phases and squared visibilities in the absence of bad pixels, but with various other noise sources. With 3% of the pixels unusable, the expected contrast drops by about 0.5 magnitudes. AMI should be able to reach targets as bright as M=5. There will be significant overlap between Gemini-GPI and ESO-SPHERE targets and AMI's search space, and a complementarity with NIRCam's coronagraph. We also illustrate synthesis imaging with AMI, demonstrating an imaging dynamic range of 25 at 100 mas scales. We tailor existing radio interferometric methods to retrieve a faint bar across a bright nucleus, and explain the similarities to synthesis imaging at radio wavelengths. Modest contrast observations of dusty accretion flows around AGNs will be feasible for NIRISS AMI. We show our early results of image-plane deconvolution as well. Finally, we report progress on an NRM-inspired approach to mitigate mission-level risk associated with JWST's specialized wavefront sensing hardware. By combining narrow band and medium band Nyquist-sampled images taken with a science camera we can sense JWST primary mirror segment tip-tilt to lOmas, and piston to a few nm. We can sense inter-segment piston errors of up to 5 coherence lengths of the broadest bandpass filter used

  6. Phase and Pupil Amplitude Recovery for JWST Space-Optics Control

    Science.gov (United States)

    Dean, B. H.; Zielinski, T. P.; Smith, J. S.; Bolcar, M. R.; Aronstein, D. L.; Fienup, J. R.

    2010-01-01

    This slide presentation reviews the phase and pupil amplitude recovery for the James Webb Space Telescope (JWST) Near Infrared Camera (NIRCam). It includes views of the Integrated Science Instrument Module (ISIM), the NIRCam, examples of Phase Retrieval Data, Ghost Irradiance, Pupil Amplitude Estimation, Amplitude Retrieval, Initial Plate Scale Estimation using the Modulation Transfer Function (MTF), Pupil Amplitude Estimation vs lambda, Pupil Amplitude Estimation vs. number of Images, Pupil Amplitude Estimation vs Rotation (clocking), and Typical Phase Retrieval Results Also included is information about the phase retrieval approach, Non-Linear Optimization (NLO) Optimized Diversity Functions, and Least Square Error vs. Starting Pupil Amplitude.

  7. Shaping Social Work Science: What Should Quantitative Researchers Do?

    Science.gov (United States)

    Guo, Shenyang

    2015-01-01

    Based on a review of economists' debates on mathematical economics, this article discusses a key issue for shaping the science of social work--research methodology. The article describes three important tasks quantitative researchers need to fulfill in order to enhance the scientific rigor of social work research. First, to test theories using…

  8. Shaping Social Work Science: What Should Quantitative Researchers Do?

    Science.gov (United States)

    Guo, Shenyang

    2015-01-01

    Based on a review of economists' debates on mathematical economics, this article discusses a key issue for shaping the science of social work--research methodology. The article describes three important tasks quantitative researchers need to fulfill in order to enhance the scientific rigor of social work research. First, to test theories using…

  9. Phase-Retrieval Uncertainty Estimation and Algorithm Comparison for the JWST-ISIM Test Campaign

    Science.gov (United States)

    Aronstein, David L.; Smith, J. Scott

    2016-01-01

    Phase retrieval, the process of determining the exitpupil wavefront of an optical instrument from image-plane intensity measurements, is the baseline methodology for characterizing the wavefront for the suite of science instruments (SIs) in the Integrated Science Instrument Module (ISIM) for the James Webb Space Telescope (JWST). JWST is a large, infrared space telescope with a 6.5-meter diameter primary mirror. JWST is currently NASA's flagship mission and will be the premier space observatory of the next decade. ISIM contains four optical benches with nine unique instruments, including redundancies. ISIM was characterized at the Goddard Space Flight Center (GSFC) in Greenbelt, MD in a series of cryogenic vacuum tests using a telescope simulator. During these tests, phase-retrieval algorithms were used to characterize the instruments. The objective of this paper is to describe the Monte-Carlo simulations that were used to establish uncertainties (i.e., error bars) for the wavefronts of the various instruments in ISIM. Multiple retrieval algorithms were used in the analysis of ISIM phase-retrieval focus-sweep data, including an iterativetransform algorithm and a nonlinear optimization algorithm. These algorithms emphasize the recovery of numerous optical parameters, including low-order wavefront composition described by Zernike polynomial terms and high-order wavefront described by a point-by-point map, location of instrument best focus, focal ratio, exit-pupil amplitude, the morphology of any extended object, and optical jitter. The secondary objective of this paper is to report on the relative accuracies of these algorithms for the ISIM instrument tests, and a comparison of their computational complexity and their performance on central and graphical processing unit clusters. From a phase-retrieval perspective, the ISIM test campaign includes a variety of source illumination bandwidths, various image-plane sampling criteria above and below the Nyquist- Shannon

  10. Mathematics education a spectrum of work in mathematical sciences departments

    CERN Document Server

    Hsu, Pao-sheng; Pollatsek, Harriet

    2016-01-01

    Many in the mathematics community in the U.S. are involved in mathematics education in various capacities. This book highlights the breadth of the work in K-16 mathematics education done by members of US departments of mathematical sciences. It contains contributions by mathematicians and mathematics educators who do work in areas such as teacher education, quantitative literacy, informal education, writing and communication, social justice, outreach and mentoring, tactile learning, art and mathematics, ethnomathematics, scholarship of teaching and learning, and mathematics education research. Contributors describe their work, its impact, and how it is perceived and valued. In addition, there is a chapter, co-authored by two mathematicians who have become administrators, on the challenges of supporting, evaluating, and rewarding work in mathematics education in departments of mathematical sciences. This book is intended to inform the readership of the breadth of the work and to encourage discussion of its val...

  11. Behavioural science at work for Canada: National Research Council laboratories.

    Science.gov (United States)

    Veitch, Jennifer A

    2007-03-01

    The National Research Council is Canada's principal research and development agency. Its 20 institutes are structured to address interdisciplinary problems for industrial sectors, and to provide the necessary scientific infrastructure, such as the national science library. Behavioural scientists are active in five institutes: Biological Sciences, Biodiagnostics, Aerospace, Information Technology, and Construction. Research topics include basic cellular neuroscience, brain function, human factors in the cockpit, human-computer interaction, emergency evacuation, and indoor environment effects on occupants. Working in collaboration with NRC colleagues and with researchers from universities and industry, NRC behavioural scientists develop knowledge, designs, and applications that put technology to work for people, designed with people in mind.

  12. Preparing Science Teachers: Strong Emphasis on Science Content Course Work in a Master's Program in Education

    Science.gov (United States)

    Ajhar, Edward A.; Blackwell, E.; Quesada, D.

    2010-05-01

    In South Florida, science teacher preparation is often weak as a shortage of science teachers often prompts administrators to assign teachers to science classes just to cover the classroom needs. This results is poor preparation of students for college science course work, which, in turn, causes the next generation of science teachers to be even weaker than the first. This cycle must be broken in order to prepare better students in the sciences. At St. Thomas University in Miami Gardens, Florida, our School of Science has teamed with our Institute for Education to create a program to alleviate this problem: A Master of Science in Education with a Concentration in Earth/Space Science. The Master's program consists of 36 total credits. Half the curriculum consists of traditional educational foundation and instructional leadership courses while the other half is focused on Earth and Space Science content courses. The content area of 18 credits also provides a separate certificate program. Although traditional high school science education places a heavy emphasis on Earth Science, this program expands that emphasis to include the broader context of astronomy, astrophysics, astrobiology, planetary science, and the practice and philosophy of science. From this contextual basis the teacher is better prepared to educate and motivate middle and high school students in all areas of the physical sciences. Because hands-on experience is especially valuable to educators, our program uses materials and equipment including small optical telescopes (Galileoscopes), several 8-in and 14-in Celestron and Meade reflectors, and a Small Radio Telescope installed on site. (Partial funding provided by the US Department of Education through Minority Science and Engineering Improvement Program grant P120A050062.)

  13. Confronting the Problems of Primary School Science. Learning in Science Project (Primary). Working Paper No. 110.

    Science.gov (United States)

    Osborne, Roger; And Others

    The Learning in Science Project (Primary)--LISP(P)--was designed to investigate the teaching and learning of science in the primary school. This paper summarizes the work undertaken and the findings obtained during the first 9 months of the project. During the first 6 months, an exploratory phase, similar to the original Learning in Science…

  14. The James Webb STEM Innovation Project: Bringing JWST to the Education Community

    Science.gov (United States)

    Eisenhamer, Bonnie; Harris, J.; Ryer, H.; Taylor, J.; Bishop, M.

    2012-01-01

    Building awareness of a NASA mission prior to launch and connecting that mission to the education community can be challenging. In order to address this challenge, the Space Telescope Science Institute's Office of Public Outreach has developed the James Webb STEM innovation Project (SIP) - an interdisciplinary project that focuses on the engineering aspects and potential scientific discoveries of JWST, while incorporating elements of project-based learning. Students in participating schools will use skills from multiple subject areas to research an aspect of the JWST's design or potential science and create models, illustrated essays, or technology-based projects to demonstrate their learning. Student projects will be showcased during special events at select venues in the project states - thus allowing parents and community members to also be benefactors of the project. Currently, the SIP is being piloted in New York, California, and Maryland. In addition, we will be implementing the SIP in partnership with NASA Explorer Schools in the states of New Mexico, Michigan, Texas, Tennessee, and Iowa.

  15. Improving Group Work Practices in Teaching Life Sciences: Trialogical Learning

    Science.gov (United States)

    Tammeorg, Priit; Mykkänen, Anna; Rantamäki, Tomi; Lakkala, Minna; Muukkonen, Hanni

    2017-08-01

    Trialogical learning, a collaborative and iterative knowledge creation process using real-life artefacts or problems, familiarizes students with working life environments and aims to teach skills required in the professional world. We target one of the major limitation factors for optimal trialogical learning in university settings, inefficient group work. We propose a course design combining effective group working practices with trialogical learning principles in life sciences. We assess the usability of our design in (a) a case study on crop science education and (b) a questionnaire for university teachers in life science fields. Our approach was considered useful and supportive of the learning process by all the participants in the case study: the students, the stakeholders and the facilitator. Correspondingly, a group of university teachers expressed that the trialogical approach and the involvement of stakeholders could promote efficient learning. In our case in life sciences, we identified the key issues in facilitating effective group work to be the design of meaningful tasks and the allowance of sufficient time to take action based on formative feedback. Even though trialogical courses can be time consuming, the experience of applying knowledge in real-life cases justifies using the approach, particularly for students just about to enter their professional careers.

  16. A Science of Social Work? Response to John Brekke

    Science.gov (United States)

    Shaw, Ian

    2014-01-01

    I take the opportunity provided by John Brekke's (2012) article to respond to the general assumptions and approaches that may be brought when considering the question of a science of social work. I consider first, what should be our frames of reference, our communities of interest, or our boundaries of inclusion, for such a discussion?…

  17. Optical Coating Performance for Heat Reflectors of the JWST-ISIM Electronic Component

    Science.gov (United States)

    Rashford, Robert A.; Perrygo, Charles M.; Garrison, Matthew B.; White, Bryant K.; Threat, Felix T.; Quijada, Manuel A.; Jeans, James W.; Huber, Frank K.; Bousquet, Robert R.; Shaw, Dave

    2011-01-01

    A document discusses a thermal radiator design consisting of lightweight composite materials and low-emittance metal coatings for use on the James Webb Space Telescope (JWST) structure. The structure will have a Thermal Subsystem unit to provide passive cooling to the Integrated Science Instrument Module (ISIM) control electronics. The ISIM, in the JWST observatory, is the platform that provides the mounting surfaces for the instrument control electronics. Dissipating the control electronic generated-heat away from JWST is of paramount importance so that the spacecraft s own heat does not interfere with the infrared-light gathering of distant cosmic sources. The need to have lateral control in the emission direction of the IEC (ISIM Electronics Compartment) radiators led to the development of a directional baffle design that uses multiple curved mirrorlike surfaces. This concept started out from the so-called Winston non-imaging optical concentrators that use opposing parabolic reflector surfaces, where each parabola has its focus at the opposite edge of the exit aperture. For this reason they are often known as compound parabolic concentrators or CPCs. This radiator system with the circular section was chosen for the IEC reflectors because it offers two advantages over other designs. The first is that the area of the reflector strips for a given radiator area is less, which results in a lower mass baffle assembly. Secondly, the fraction of energy emitted by the radiator strips and subsequently reflected by the baffle is less. These fewer reflections reduced the amount of energy that is absorbed and eventually re-emitted, typically in a direction outside the design emission range angle. A baffle frame holds the mirrors in position above a radiator panel on the IEC. Together, these will direct the majority of the heat from the IEC above the sunshield away towards empty space.

  18. Scientists and Science Education: Working at the Interface

    Science.gov (United States)

    DeVore, E. K.

    2004-05-01

    "Are we alone?" "Where did we come from?" "What is our future?" These questions lie at the juncture of astronomy and biology: astrobiology. It is intrinsically interdisciplinary in its study of the origin, evolution and future of life on Earth and beyond. The fundamental concepts of origin and evolution--of both living and non-living systems--are central to astrobiology, and provide powerful themes for unifying science teaching, learning, and appreciation in classrooms and laboratories, museums and science centers, and homes. Research scientists play a key role in communicating the nature of science and joy of scientific discovery with the public. Communicating the scientific discoveries with the public brings together diverse professionals: research scientists, graduate and undergraduate faculty, educators, journalists, media producers, web designers, publishers and others. Working with these science communicators, research scientists share their discoveries through teaching, popular articles, lectures, broadcast and print media, electronic publication, and developing materials for formal and informal education such as textbooks, museum exhibits and documentary television. There's lots of activity in science communication. Yet, the NSF and NASA have both identified science education as needing improvement. The quality of schools and the preparation of teachers receive national attention via "No Child Left Behind" requirements. The number of students headed toward careers in science, technology, engineering and mathematics (STEM) is not sufficient to meet national needs. How can the research community make a difference? What role can research scientists fulfill in improving STEM education? This talk will discuss the interface between research scientists and science educators to explore effective roles for scientists in science education partnerships. Astronomy and astrobiology education and outreach projects, materials, and programs will provide the context for

  19. Spitzer/JWST Cross Calibration: IRAC Observations of Potential Calibrators for JWST

    Science.gov (United States)

    Carey, Sean J.; Gordon, Karl D.; Lowrance, Patrick; Ingalls, James G.; Glaccum, William J.; Grillmair, Carl J.; E Krick, Jessica; Laine, Seppo J.; Fazio, Giovanni G.; Hora, Joseph L.; Bohlin, Ralph

    2017-06-01

    We present observations at 3.6 and 4.5 microns using IRAC on the Spitzer Space Telescope of a set of main sequence A stars and white dwarfs that are potential calibrators across the JWST instrument suite. The stars range from brightnesses of 4.4 to 15 mag in K band. The calibration observations use a similar redundancy to the observing strategy for the IRAC primary calibrators (Reach et al. 2005) and the photometry is obtained using identical methods and instrumental photometric corrections as those applied to the IRAC primary calibrators (Carey et al. 2009). The resulting photometry is then compared to the predictions based on spectra from the CALSPEC Calibration Database (http://www.stsci.edu/hst/observatory/crds/calspec.html) and the IRAC bandpasses. These observations are part of an ongoing collaboration between IPAC and STScI investigating absolute calibration in the infrared.

  20. Revising laboratory work: sociological perspectives on the science classroom

    Science.gov (United States)

    Jobér, Anna

    2017-09-01

    This study uses sociological perspectives to analyse one of the core practices in science education: schoolchildren's and students' laboratory work. Applying an ethnographic approach to the laboratory work done by pupils at a Swedish compulsory school, data were generated through observations, field notes, interviews, and a questionnaire. The pupils, ages 14 and 15, were observed as they took a 5-week physics unit (specifically, mechanics). The analysis shows that the episodes of laboratory work could be filled with curiosity and exciting challenges; however, another picture emerged when sociological concepts and notions were applied to what is a very common way of working in the classroom. Laboratory work is characterised as a social activity that is expected to be organised as a group activity. This entails groups becoming, to some extent, `safe havens' for the pupils. On the other hand, this way of working in groups required pupils to subject to the groups and the peer effect, sometimes undermining their chances to learn and perform better. In addition, the practice of working in groups when doing laboratory work left some pupils and the teacher blaming themselves, even though the outcome of the learning situation was a result of a complex interplay of social processes. This article suggests a stronger emphasis on the contradictions and consequences of the science subjects, which are strongly influenced by their socio-historical legacy.

  1. Revising laboratory work: sociological perspectives on the science classroom

    Science.gov (United States)

    Jobér, Anna

    2016-08-01

    This study uses sociological perspectives to analyse one of the core practices in science education: schoolchildren's and students' laboratory work. Applying an ethnographic approach to the laboratory work done by pupils at a Swedish compulsory school, data were generated through observations, field notes, interviews, and a questionnaire. The pupils, ages 14 and 15, were observed as they took a 5-week physics unit (specifically, mechanics). The analysis shows that the episodes of laboratory work could be filled with curiosity and exciting challenges; however, another picture emerged when sociological concepts and notions were applied to what is a very common way of working in the classroom. Laboratory work is characterised as a social activity that is expected to be organised as a group activity. This entails groups becoming, to some extent, `safe havens' for the pupils. On the other hand, this way of working in groups required pupils to subject to the groups and the peer effect, sometimes undermining their chances to learn and perform better. In addition, the practice of working in groups when doing laboratory work left some pupils and the teacher blaming themselves, even though the outcome of the learning situation was a result of a complex interplay of social processes. This article suggests a stronger emphasis on the contradictions and consequences of the science subjects, which are strongly influenced by their socio-historical legacy.

  2. Epistemic foundations of the independent work in the natural sciences

    Directory of Open Access Journals (Sweden)

    Raúl De Miranda Rangel

    2015-09-01

    Full Text Available The article presents one of the partial results of the project "Deepening of the epistemological foundations of environmental education". The article has as purpose it specifies the main related epistemic elements with the independent work of the degree in the natural sciences. The theoretical systematization is highlighted, carrying out an analysis of the independent work from the approached perspective for different authors, that together with the employment of other methods of the empiric investigation, permitted approach the term work independent, by reaching to a more contemporary sight of your definition.

  3. Working with "rookies": A case study of science teachers mentors

    Science.gov (United States)

    Meagher, Thomas Francis

    To gain insight into the world of mentoring new science teachers it is imperative to examine how a veteran science teacher is influenced through his or her work mentoring a new teacher. The impacts of mentoring new teachers have been extensively researched within the literature, documenting many of the factors that may enhance the teaching abilities of new teachers (Hobson, Ashby, Malderez & Tomlinson, 2008; Ingersoll & Kralik, 2004; Wang & Odell, 2002). A thorough search of the literature reveals an unbalanced representation of research focusing on the many influences mentoring may bring to a new teacher while ignoring the impact on the mentor. It is when the activity of mentoring a new teacher is examined within the theoretical frame work of social cognitive learning, it is apparent that not only are two individuals participating in working together, but also that research needs to investigate both sides of the relationship. Also, since the mentoring relationship is situated within a community of practice, it becomes important to utilize a situated learning theoretical framework in tandem with social cognitive learning to provide the clearest picture of this dynamic social relationship. This case study seeks to share the impacts experienced by mentors through their work with new teachers and provide balance to the other side of research into the social partnership of mentoring. Five science teachers mentoring new teachers online, through the University of Minnesota's Science Engineering, Math Mentoring Program (STEMMP) and Science Teacher Induction Network (TIN), participated in this study that explores their experiences through a phenomenographic lens and follows an interpretive research approach. Four main themes emerged that identified how science teacher mentors were impacted from mentoring which included: (1) impacts to their teaching practice, (2) perceptions influenced from feedback, (3) enhanced reflection, and (4) enhancement of self-efficacy. The

  4. JWST observations of stellar occultations by solar system bodies and rings

    CERN Document Server

    Santos-Sanz, P; Pinilla-Alonso, N; Stansberry, J; Lin, Z-Y; Zhang, Z-W; Vilenius, E; Müller, Th; Ortiz, J L; Braga-Ribas, F; Bosh, A; Duffard, R; Lellouch, E; Tancredi, G; Young, L

    2015-01-01

    In this paper we investigate the opportunities provided by the James Webb Space Telescope (JWST) for significant scientific advances in the study of solar system bodies and rings using stellar occultations. The strengths and weaknesses of the stellar occultation technique are evaluated in light of JWST's unique capabilities. We identify several possible JWST occultation events by minor bodies and rings, and evaluate their potential scientific value. These predictions depend critically on accurate a priori knowledge of the orbit of JWST near the Sun-Earth Lagrange-point 2 (L2). We also explore the possibility of serendipitous stellar occultations by very small minor bodies as a by-product of other JWST observing programs. Finally, to optimize the potential scientific return of stellar occultation observations, we identify several characteristics of JWST's orbit and instrumentation that should be taken into account during JWST's development.

  5. Communicating Ocean Sciences College Courses: Science Faculty and Educators Working and Learning Together

    Science.gov (United States)

    Halversen, C.; Simms, E.; McDonnell, J. D.; Strang, C.

    2011-12-01

    scientists with experience using exemplary, research-based instructional materials that incorporate current learning theories and teaching strategies; 5) promote mutually beneficial collaborations between scientists and educators co-teaching the course; and 6) provide underrepresented K-12 students and visitors to informal science institutions with ocean sciences instruction and the opportunity to interact with the next generation of scientists. Evaluation findings over five years show that the course can be an effective mechanism to introduce scientists to education research and improve post-secondary science instruction. Students improved in their understanding of how people learn and how to effectively communicate. Science faculty reported that the course provided them with a heightened awareness and practical knowledge of learning theory and education research, and as a result, they felt they became more effective educators and communicators. This has implications for their work with future and fellow scientists, and the general public.

  6. Teaching science problem solving: An overview of experimental work

    Science.gov (United States)

    Taconis, R.; Ferguson-Hessler, M. G. M.; Broekkamp, H.

    2001-04-01

    The traditional approach to teaching science problem solving is having the students work individually on a large number of problems. This approach has long been overtaken by research suggesting and testing other methods, which are expected to be more effective. To get an overview of the characteristics of good and innovative problem-solving teaching strategies, we performed an analysis of a number of articles published between 1985 and 1995 in high-standard international journals, describing experimental research into the effectiveness of a wide variety of teaching strategies for science problem solving. To characterize the teaching strategies found, we used a model of the capacities needed for effective science problem solving, composed of a knowledge base and a skills base. The relations between the cognitive capacities required by the experimental or control treatments and those of the model were specified and used as independent variables. Other independent variables were learning conditions such as feedback and group work. As a dependent variable we used standardized learning effects. We identified 22 articles describing 40 experiments that met the standards we deemed necessary for a meta-analysis. These experiments were analyzed both with quantitative (correlational) methods and with a systematic qualitative method. A few of the independent variables were found to characterize effective strategies for teaching science problem solving. Effective treatments all gave attention to the structure and function (the schemata) of the knowledge base, whereas attention to knowledge of strategy and the practice of problem solving turned out to have little effect. As for learning conditions, both providing the learners with guidelines and criteria they can use in judging their own problem-solving process and products, and providing immediate feedback to them were found to be important prerequisites for the acquisition of problem-solving skills. Group work did not lead to

  7. Working with soils: soil science continuing professional development

    Science.gov (United States)

    Hannam, Jacqueline; Thompson, Dick

    2017-04-01

    The British Society of Soil Science launched the Working with Soils professional competency programme in 2011. This was in response to concerns from practitioners and professionals of a significant skills gap in various sectors that require soil science skills. The programme includes one and two day courses that cover the qualifications, knowledge and skills required of a professional scientist or engineer conducting a range of contract work. All courses qualify for continuing professional development points with various professional practice schemes. Three courses cover the foundations of soil science namely; describing a soil profile, soil classification and understanding soil variability in the field and landscape. Other tailored courses relate to specific skills required from consultants particularly in the planning process where land is assessed for agricultural quality (agricultural land classification). New courses this year include soil handling and restoration that provides practitioners with knowledge of the appropriate management of large volumes of soil that are disturbed during development projects. The courses have so far successfully trained over 100 delegates ranging from PhD students, environmental consultants and government policy advisors.

  8. Probing the dusty inhabitants of the Local Group Galaxies: JWST/MIRI colors of infrared stellar populations

    Science.gov (United States)

    Jones, Olivia; Meixner, Margaret

    2016-01-01

    The assembly of galaxies involves the life cycle of mass, metal enrichment and dust that JWST will probe. Detailed studies of nearby galaxies provides guidance for interpreting the more distant forming galaxies. JWST/MIRI will enable stellar population studies akin to work done with HST on the Local Group galaxies but over a new wavelength range. MIRI's imaging capability over nine photometric bands from 5 to 28 microns is particularly suited to survey stars with an infrared excess and to detangle the extinction or thermal emission from various species of dust. These dusty stellar populations include young stellar objects, evolved stars and supernovae that are bright in the infrared. Using the rich Spitzer-IRS spectroscopic dataset and spectral classifications from the Surveying the Agents of Galaxy Evolution (SAGE)-Spectroscopic survey of over a thousand objects in the Magellanic Clouds, we calculate the expected flux -densities and colors in the MIRI broadband filters for these prominent infrared sources. We uses these fluxes to illustrate what JWST will see in stellar population studies for other Local Group galaxies. JWST/MIRI observations of infrared sources in Local Group Galaxies will constrain the life cycle of galaxies through their dust emission. For example, how much of the interstellar dust is supplied by dying stars? Do the number of young stellar objects agree with star formation diagnostic for the galaxy? We discuss the locations of the post- and pre-main-sequence populations in MIRI color-color and color-magnitude space and examine which filters are best for identifying populations of sources. We connect these results to existing galaxies with HST data for instance Andromeda and M33.

  9. The impact of JWST broad-band filter choice on photometric redshift estimation

    CERN Document Server

    Bisigello, L; Colina, L; Fèvre, O Le; Nørgaard-Nielsen, H U; Pérez-González, P G; Pye, J; van der Werf, P; Ilbert, O; Grogin, N; Koekemoer, A

    2016-01-01

    The determination of galaxy redshifts in James Webb Space Telescope (JWST)'s blank-field surveys will mostly rely on photometric estimates, based on the data provided by JWST's Near-Infrared Camera (NIRCam) at 0.6-5.0 {\\mu}m and Mid Infrared Instrument (MIRI) at {\\lambda}>5.0 {\\mu}m. In this work we analyse the impact of choosing different combinations of NIRCam and MIRI broad-band filters (F070W to F770W), as well as having ancillary data at {\\lambda}=10, but the zphot quality significantly degrades at S/N<=5. Adding MIRI photometry with one magnitude brighter depth than the NIRCam depth allows for a redshift recovery of 83-99%, depending on SED type, and its effect is particularly noteworthy for galaxies with nebular emission. The vast majority of NIRCam galaxies with [F150W]=29 AB mag at z=7-10 will be detected with MIRI at [F560W, F770W]<28 mag if these sources are at least mildly evolved or have spectra with emission lines boosting the mid-infrared fluxes.

  10. Mercury Orbiter: Report of the Science Working Team

    Science.gov (United States)

    Belcher, John W.; Slavin, James A.; Armstrong, Thomas P.; Farquhar, Robert W.; Akasofu, Syun I.; Baker, Daniel N.; Cattell, Cynthia A.; Cheng, Andrew F.; Chupp, Edward L.; Clark, Pamela E.

    1991-01-01

    The results are presented of the Mercury Orbiter Science Working Team which held three workshops in 1988 to 1989 under the auspices of the Space Physics and Planetary Exploration Divisions of NASA Headquarters. Spacecraft engineering and mission design studies at the Jet Propulsion Lab were conducted in parallel with this effort and are detailed elsewhere. The findings of the engineering study, summarized herein, indicate that spin stabilized spacecraft carrying comprehensive particles and fields experiments and key planetology instruments in high elliptical orbits can survive and function in Mercury orbit without costly sun shields and active cooling systems.

  11. Training of Social Science Students to Work With Disabled Population

    Directory of Open Access Journals (Sweden)

    Carmen Eugenia Carvajal Palacios

    2014-07-01

    Full Text Available The research project was conducted at the University of Nariño in Pasto with undergraduate students of basic education with emphasis in Social Sciences, to care for people suffering from disabilities, this project enrolled within the qualitative paradigm with critical- social approach; it was participatory research-action, which favored the observation, interviews and workshops. 15 students of social science program and 4 teachers linked to PROFESA School, which was established as teaching and research center practice. The data analysis was performed from the categorial system resulting in the conceptualization of disability, feelings towards disability, work with parents and teacher training to look after people with disabilities. It was evident that at the University of Nariño specifically Welfare services does activities, programs and events to support the educational and social inclusion, however the forming of teachers with academic units still pending task of training on disability, inclusion and diversity. It was found that in the undergraduate program of basic education with emphasis on social sciences there is no problem oriented core, seminar or explicit activity in the curriculum regarding disability as indicated by Decree 2082/1996, which in turn, was established in the legal and indicative benchmark of this research.

  12. Response: From Fish and Bicycles to a Science of Social Work

    Science.gov (United States)

    Marsh, Jeanne Cay

    2012-01-01

    John Brekke challenges the field and profession of social work to define and develop the "science of social work". This response to Brekke's paper identifies the premises undergirding a discussion of the science of social work related to (1) a definition of "science";; (2 ) an organizing principle for social work; (3) a recognition that the task…

  13. Response: From Fish and Bicycles to a Science of Social Work

    Science.gov (United States)

    Marsh, Jeanne Cay

    2012-01-01

    John Brekke challenges the field and profession of social work to define and develop the "science of social work". This response to Brekke's paper identifies the premises undergirding a discussion of the science of social work related to (1) a definition of "science";; (2 ) an organizing principle for social work; (3) a…

  14. Working With Greenlandic Fishermen: A New Approach to Citizen Science

    Science.gov (United States)

    Turrin, M.; Porter, D. F.; Greve, S.

    2014-12-01

    'Leveraging Local Knowledge to Measure Greenland Fjords' is a science project designed with local knowledge sharing and data collection at its core. Citizen Science can take many different forms but in each instance it incorporates active participation of the general public in science research through integrating outreach, instruction, information gathering and data exchange. The strongest projects focus on two-way information exchange with both the citizen scientist and the professional scientist learning when they share their knowledge. Working in cooperation with both teachers and fishermen in a small local community in northwest Greenland, we collected novel oceanographic measurements from a small 5 m fishing boat in the local fjord. We established connections with the local school for developing education initiatives, sharing maps and other resources, and worked through the teachers to connect with the village residents. We hosted a community meeting to provide a forum for a two-way information exchange with the science team providing background on the research project and the local residents providing both narrative information on local environmental change over the last one to three decades, and more quantitative and immediately useful information on fjord depths, iceberg flow directions and timing of seasonal ice break up and move out. The local fishermen were intimately familiar with the local environment, having intrinsically collected data on fjord depth from their regular lowering of fishing line to catch Greenlandic halibut, a benthic fish. For our first trip they worked with us locating the deep and shallow parts of the fjord from many seasons of watching icebergs ground on the shallow shoals, and showed us how to navigate into the ice packed glacial front through the dense ice mélange. The local community interest in the project and in learning how to use the equipment we had brought encouraged us to discuss a long-term data gathering relationship

  15. Production of a Science Documentary and Its Usefulness in Teaching the Nature of Science: Indirect Experience of How Science Works

    Science.gov (United States)

    Kim, Sun Young; Yi, Sang Wook; Cho, Eun Hee

    2014-01-01

    In this study, we produced a documentary which portrays scientists at work and critically evaluated the use of this film as a teaching tool to help students develop an understanding of the nature of science. The documentary, "Life as a Scientist: People in Love with 'Caenorhabditis elegans,' a Soil Nematode" encompasses the…

  16. Production of a Science Documentary and Its Usefulness in Teaching the Nature of Science: Indirect Experience of How Science Works

    Science.gov (United States)

    Kim, Sun Young; Yi, Sang Wook; Cho, Eun Hee

    2014-01-01

    In this study, we produced a documentary which portrays scientists at work and critically evaluated the use of this film as a teaching tool to help students develop an understanding of the nature of science. The documentary, "Life as a Scientist: People in Love with 'Caenorhabditis elegans,' a Soil Nematode" encompasses the…

  17. Astrophysics in the Next Decade: JWST and Concurrent Facilities

    CERN Document Server

    Thronson, Harley A; Tielens, Alexander; The James Webb Space Telescope and Concurrent Facilities

    2009-01-01

    NASA’s James Webb Space Telescope (JWST), planned for operation in about five years, will have the capability to investigate – and answer – some of the most challenging questions in astronomy. Although motivated and designed to study the very early Universe, the performance of the observatory’s instruments over a very wide wavelength range will allow the world’s scientific community unequaled ability to study cosmic phenomena as diverse as small bodies in the Solar System and the formation of galaxies. As part of preparation to use JWST, a conference was held in Tucson, Arizona in 2007 that brought together astronomers from around the world to discuss the mission, other major facilities that will operate in the coming decade, and major scientific goals for them. This book is a compilation of those presentations by some of the leading researchers from all branches of astronomy. This book also includes a "pre-history" of JWST, describing the lengthy process and some of the key individuals that initiat...

  18. Simulating Exoplanet Transit and Eclipse Observations with JWST

    Science.gov (United States)

    Greene, Tom

    2011-01-01

    The James Webb Space Telescope (JWST) will be a nearly ideal machine for acquiring the transmission and emission spectra of transiting exoplanets over its large wavelength range 0.7 - 28 microns. The NIRSpec, NIRCam, nTFI, and MIRI instruments will have spectroscopic capabilities that span spectral resolutions from 20 - 3000 and can cover up to 2 - 3 octaves in wavelength simultaneously. This will allow observing multiple molecular features at once, facilitating the separation of atmospheric temperature and abundance effects on spectra. Many transiting planets will also be able to be observed with both transmission and eclipse spectroscopy, providing further insights and constraints on planetary thermal structures and energy transport. Simulated JWST spectra of planets ranging from mini-Neptunes to gas giants will be presented. These simulations include planets ranging from mini-Neptunes to gas giants will be presented. These simulations include current best estimates of actual instrument throughput, resolution, spectral range, systematic noise, and random noise terms. They show that JWST will be able to determine the atmospheric parameters of a wide variety of planets, often when observing only one or a few transit or eclipse event sequences. The thermal emissions of rocky super-Earths will also be quickly detectable via mid-IR eclipse observations if such planets are found around nearby M star hosts beforehand.

  19. James Webb Space Telescope (JWST) and Star Formation

    Science.gov (United States)

    Greene, Thomas P.

    2010-01-01

    The 6.5-m aperture James Webb Space Telescope (JWST) will be a powerful tool for studying and advancing numerous areas of astrophysics. Its Fine Guidance Sensor, Near-Infrared Camera, Near-Infrared Spectrograph, and Mid-Infrared Instrument will be capable of making very sensitive, high angular resolution imaging and spectroscopic observations spanning 0.7 - 28 ?m wavelength. These capabilities are very well suited for probing the conditions of star formation in the distant and local Universe. Indeed, JWST has been designed to detect first light objects as well as to study the fine details of jets, disks, chemistry, envelopes, and the central cores of nearby protostars. We will be able to use its cameras, coronagraphs, and spectrographs (including multi-object and integral field capabilities) to study many aspects of star forming regions throughout the galaxy, the Local Group, and more distant regions. I will describe the basic JWST scientific capabilities and illustrate a few ways how they can be applied to star formation issues and conditions with a focus on Galactic regions.

  20. Characterizing Transiting Planets with JWST Spectra: Simulations and Retrievals

    Science.gov (United States)

    Greene, Tom; Line, Michael; Fortney, Jonathan

    2015-01-01

    There are now well over a thousand confirmed exoplanets, ranging from hot to cold and large to small worlds. JWST spectra will provide much more detailed information on the molecular constituents, chemical compositions, and thermal properties of the atmospheres of transiting planets than is now known. We explore this by modeling clear, cloudy,and high mean molecular weight atmospheres of typical hot Jupiter, warm Neptune, warm sub-Neptune, and cool super-Earth planets and then simulating their JWST transmission and emission spectra. These simulations were performed for several JWST instrument modes over 1 - 11 microns and incorporate realistic signal and noise components. We then performed state-of the art retrievals to determine how well temperatures and abundances (CO, CO2, H2O, NH3) will be constrained and over what pressures for these different planet types. Using these results, we appraise what instrument modes will be most useful for determining what properties of the different planets, and we assess how well we can constrain their compositions, CO ratios, and temperature profiles.

  1. The Science of Intelligence for Big, Complex Work

    Directory of Open Access Journals (Sweden)

    Pamela Noel Gray

    2009-05-01

    Full Text Available An epistemological 5GL shell, eGanges, offers systemic intelligence for big, complex work. It is designed for construction of e-learning aids in the workplaces of the finite domains of law, management and education; there may be other suitable uses as well. Law is concerned with large, complex social organisation, and business is concerned with large, complex commercial organisations; work skills for each organisation are taught in tertiary education. This paper illustrates how eGanges aids may be learned in these higher education vocational courses and then, applied seamlessly in the workplace. eGanges applications in the Australian Anti-Money Laundering and Counter-Terrorism Financing Act 2006, and the tasks of a corporate CEO are used to illustrate the nature of the e-Learning and Workplace aids. A major feature of these aids is that they can effect quality control because they permit precise, pre-planned micro-management with electronic memory and speed; they are super-agile aids that can be ubiquitous and foster common, comprehensive understanding of large, complex work matters. They show how a science of intelligence supports a leap in the coherence and co-ordination required for big societies and large work forces.

  2. Educators Who Work in Science: The Narratives of Women Negotiating Careers in Academic Science

    Science.gov (United States)

    Tullos, Kimberly C.

    2011-12-01

    The purpose of this life story narrative study was to explore how women scientists develop views of self that enable them to negotiate careers within academic science. I framed the study using feminist standpoint theory as my theoretical foundation, and used possible selves theory as my conceptual framework. Eight women scientists working in academe described their journey regarding their views of self and career-related experiences. The study produced two key findings. First, seven themes emerged from my data analysis; these themes suggest that these women shared significant experiences in their quest to become scientists. Second, my feminist analysis of the participants' narratives indicates that distinct, but submerged gender-related tensions shaped their views of themselves as scientists and their science career decisions. These tensions include career choice and advancement constrained by family obligations, work environments that do not recognize or undervalue their skills and contributions to the profession, and perceived pressure to de-feminize their behavior to blend in to their work environment. Not unlike other women negotiating careers in academic science, they generally accepted their status as women to be an inherent part of their career pursuits and viewed workplace challenges as an opportunity to prove their competency. Seven of the eight women did not attribute their challenges to gender differences. However, the combined narratives revealed underlying conflicts between their views of self as women and as scientists resulting from their experiences in, and perceptions of, academic science environments. The study's principal theoretical contribution, from the feminist standpoint perspective, highlights the pervasive and unseen influence of gender dynamics. In this study, the participants developed views of themselves, not as scientists, but as "educators who work in science." This critical distinction enabled these participants, perhaps unknowingly

  3. Boundary-Work in Science Education: A Case Study of GM Food

    Science.gov (United States)

    Lin, Yin-Ling

    2016-01-01

    The term "boundary-work" is used to refer to the constant effort to draw and re-draw the boundary of science; it has long been portrayed as constructed by the stakeholders of science to demarcate science from non-science to establish the authority of science. Twenty-nine semi-structured interviews were carried out with students from one…

  4. Boundary-Work in Science Education: A Case Study of GM Food

    Science.gov (United States)

    Lin, Yin-Ling

    2016-01-01

    The term "boundary-work" is used to refer to the constant effort to draw and re-draw the boundary of science; it has long been portrayed as constructed by the stakeholders of science to demarcate science from non-science to establish the authority of science. Twenty-nine semi-structured interviews were carried out with students from one…

  5. Epistemology, Practical Work and Academic Skills in Science Education

    NARCIS (Netherlands)

    Kirschner, P.A.

    1992-01-01

    This article discusses the inherent flaws in considering and using the epistemology of the natural sciences as equivalent to a pedagogic basis for teaching and learning in the natural sciences. It begins with a discussion of the difference between practising science and learning to practice science.

  6. In-focus phase retrieval using JWST-NIRISS's non-redundant mask

    Science.gov (United States)

    Greenbaum, Alexandra Z.; Gamper, Noah; Sivaramakrishnan, Anand

    2016-07-01

    The James Webb Space Telescope's Near InfraRed Imager and Slitless Spectrograph (NIRISS) contains a 7-hole non-redundant mask (NRM) in its pupil. NIRISS's Aperture Masking Interferometry (AMI) mode is useful both for science as well as wavefront sensing. In-focus science detector NRM and full pupil images of unresolved stars can be used to measure the wavefront without any dedicated wavefront sensing hardware or any moving mirrors. Using routine science operational sequences, these images can be taken before or after any science visit. NRM fringe phases constrain Gerchberg-Saxton phase retrieval to disambiguate the algorithm's two-fold degeneracy. We summarize how consecutive masked and unmasked exposures provide enough information to reconstruct a wavefront with up to ˜1-2 rms radians of error. We present our latest progress on using this approach on laboratory experiments, and discuss those results in the context of contingency for JWST segment phasing. We discuss extending our method to ground-based AO systems and future space telescopes.

  7. Can JWST Follow Up on Gravitational-Wave Detections?

    Science.gov (United States)

    Kohler, Susanna

    2016-02-01

    Bitten by the gravitational-wave bug? While we await Thursdays press conference, heres some food for thought: if LIGO were able to detect gravitational waves from compact-object mergers, how could we follow up on the detections? A new study investigates whether the upcoming James Webb Space Telescope (JWST) will be able to observe electromagnetic signatures of some compact-object mergers.Hunting for MergersStudying compact-object mergers (mergers of black holes and neutron stars) can help us understand a wealth of subjects, like high-energy physics, how matter behaves at nuclear densities, how stars evolve, and how heavy elements in the universe were created.The Laser Interferometer Gravitational-Wave Observatory (LIGO) is searching for the signature ripples in spacetime identifying these mergers, but gravitational waves are squirrelly: LIGO will only be able to localize wave sources to tens of square degrees. If we want to find out more about any mergers LIGO discovers in gravitational waves, well need a follow-up search for electromagnetic counterparts with other observatories.The Kilonova KeyOne possible electromagnetic counterpart is kilonovae, explosions that can be produced during a merger of a binary neutron star or a neutron starblack hole system. If the neutron star is disrupted during the merger, some of the hot mass is flung outward and shines brightly by radioactive decay.Kilonovae are especially promising as electromagnetic counterparts to gravitational waves for three reasons:They emit isotropically, so the number of observable mergers isnt limited by relativistic beaming.They shine for a week, giving follow-up observatories time to search for them.The source location can beeasily recovered.The only problem? We dont currently have any sensitive survey instruments in the near-infrared band (where kilonova emission peaks) that can provide coverage over tens of square degrees. Luckily, we will soon have just the thing: JWST, launching in 2018!JWSTs

  8. Model predictions and observed performance of JWST's cryogenic position metrology system

    Science.gov (United States)

    Lunt, Sharon R.; Rhodes, David; DiAntonio, Andrew; Boland, John; Wells, Conrad; Gigliotti, Trevis; Johanning, Gary

    2016-07-01

    The James Webb Space Telescope (JWST) cryogenic testing requires measurement systems that both obtain a very high degree of accuracy and can function in that environment. Close-range photogrammetry was identified as meeting those criteria. Testing the capability of a close-range photogrammetric system prior to its existence is a challenging problem. Computer simulation was chosen over building a scaled mock-up to allow for increased flexibility in testing various configurations. Extensive validation work was done to ensure that the actual as-built system meets accuracy and repeatability requirements. The simulated image data predicted the uncertainty in measurement to be within specification and this prediction was borne out experimentally. Uncertainty at all levels was verified experimentally to be <0.1 mm.

  9. Deciphering the Hot Giant Atmospheres Orbiting Nearby Extrasolar Systems with JWST

    Science.gov (United States)

    Afrin Badhan, Mahmuda; Batalha, Natasha; Deming, Drake; Domagal-Goldman, Shawn; HEBRARD, Eric; Kopparapu, Ravi Kumar; Irwin, Patrick Gerard Joseph

    2016-10-01

    Unique and exotic planets give us an opportunity to understand how planetary systems form and evolve over their lifetime, by placing our own planetary system in the context of the vastly different extrasolar systems that are being continually discovered by present space missions. With orbital separations that are less than one-tenth of the Mercury-Sun distance, these close-in planets provide us with valuable insights about the host stellar atmosphere and planetary atmospheres subjected to their enormous stellar insolation. Observed spectroscopic signatures reveal all spectrally active species in a planet, along with information about its thermal structure and dynamics, allowing us to characterize the planet's atmosphere. NASA's upcoming missions will give us the high-resolution spectra necessary to constrain the atmospheric properties with unprecedented accuracy. However, to interpret the observed signals from exoplanetary transit events with any certainty, we need reliable atmospheric retrieval tools that can model the expected observables adequately. In my work thus far, I have built a Markov Chain Monte Carlo (MCMC) convergence scheme, with an analytical radiative equilibrium formulation for the thermal structures, within the NEMESIS atmospheric modeling tool, to allow sufficient (and efficient) exploration of the parameter space. I also augmented the opacity tables to improve the speed and reliability of retrieval models. I then utilized this upgraded version to infer the pressure-temperature (P-T) structures and volume-mixing ratios (VMRs) of major gas species in hot Jupiter dayside atmospheres, from their emission spectra. I have employed a parameterized thermal structure to retrieve plausible P-T profiles, along with altitude-invariant VMRs. Here I show my retrieval results on published datasets of HD189733b, and compare them with both medium and high spectral resolution JWST/NIRSPEC simulations. In preparation for the upcoming JWST mission, my current work

  10. Teaching planetary sciences to elementary school teachers: Programs that work

    Science.gov (United States)

    Lebofsky, Larry A.; Lebofsky, Nancy R.

    1993-01-01

    Planetary sciences can be used to introduce students to the natural world which is a part of their lives. Even children in an urban environment are aware of such phenomena as day and night, shadows, and the seasons. It is a science that transcends cultures, has been prominent in the news in recent years, and can generate excitement in young minds as no other science can. Planetary sciences also provides a useful tool for understanding other sciences and mathematics, and for developing problem solving skills which are important in our technological world. However, only 15 percent of elementary school teachers feel very well qualified to teach earth/space science, while better than 80 percent feel well qualified to teach reading; many teachers avoid teaching science; very little time is actually spent teaching science in the elementary school: 19 minutes per day in K-3 and 38 minutes per day in 4-6. While very little science is taught in elementary and middle school, earth/space science is taught at the elementary level in less than half of the states. It was pointed out that science is not generally given high priority by either teachers or school districts, and is certainly not considered on a par with language arts and mathematics. Therefore, in order to teach science to our youth, we must empower our teachers, making them familiar and comfortable with existing materials. In our earlier workshops, several of our teachers taught in classrooms where the majority of the students were Hispanic (over 90 percent). However, few space sciences materials existed in Spanish. Therefore, most of our materials could not be used effectively in the classroom. To address this issue, NASA materials were translated into Spanish and a series of workshops for bilingual classroom teachers from Tucson and surrounding cities was conducted. Our space sciences workshops and our bilingual classroom workshops and how they address the needs of elementary school teachers in Arizona are

  11. Keep It Positive: Using Student Goals and Appraisals to Inform Small Group Work in Science

    Science.gov (United States)

    Woods-McConney, Amanda; Wosnitza, Marold; Donetta, Kevin

    2011-01-01

    In teaching science, small group work is often recommended and frequently used. In this study, we asked 130 students about their personal goals and views (appraisals) of small group work in science. We found significant relationships between students' personal goals and their views of doing science in small groups. We discuss the practical…

  12. Terrestrial Planet Finder Interferometer Science Working Group Report

    Science.gov (United States)

    Lawson, Peter R. (Editor); Lay, Oliver P. (Editor); Johnston, Kenneth J. (Editor); Beichman, Charles A. (Editor)

    2007-01-01

    Over the past two years, the focus of the project for the interferometric version of the Terrestrial Planet Finder(TPF-I) has been on the development of the scientific rational for the mission, the assessment of TPF-I architectures, the laboratory demonstration of key technologies, and the development of a detailed technology roadmap. The Science Working Group (SWG), in conjunction with European colleagues working on the European Space Agency's (ESA's) Darwin project, has reaffirmed the goals of TPF-I as part of a broad vision for the detection and characterization of Earth-like planets orbiting nearby stars and for the search for life on those planets. The SWG also helped to assess the performance of different interferometric configurations for TPF-I/Darwin. Building on earlier SWG reports, this document restates the scientific case for TPF-I, assesses suitable target stars and relevant wavelengths for observation, discusses dramatic new capabilities for general astrophysical observations, and summarizes how Spitzer has improved our knowledge of the incidence of zodiacal emission on the search for planets. This document discusses in some detail on laboratory advances in interferometric nulling and formation flying. Laboratory experiments have now achieved stable narrow- and broad-band nulling the levels of 10-6 and 2.0x10-5, respectively. A testbed has demonstrated formation flying using two realistic spacecraft mockups. With a suitably funded program of technology development, as summarized herein and described in more detail in the Technology Plan for the Terrestrial Planet Finder Interferometer (2005), the National Aeronautics and Space Administration (NASA) and ESA would be able to start within the coming decade a full-scale TPF-I/Darwin mission capable of finding Earths orbiting more than 150 nearby stars, or a scaled back interferometer capable of studying more than 30 stars. Finding evidence for life on just one of those planets would revolutionize our

  13. A Working Framework for Enabling International Science Data System Interoperability

    Science.gov (United States)

    Hughes, J. Steven; Hardman, Sean; Crichton, Daniel J.; Martinez, Santa; Law, Emily; Gordon, Mitchell K.

    2016-07-01

    For diverse scientific disciplines to interoperate they must be able to exchange information based on a shared understanding. To capture this shared understanding, we have developed a knowledge representation framework that leverages ISO level reference models for metadata registries and digital archives. This framework provides multi-level governance, evolves independent of the implementation technologies, and promotes agile development, namely adaptive planning, evolutionary development, early delivery, continuous improvement, and rapid and flexible response to change. The knowledge representation is captured in an ontology through a process of knowledge acquisition. Discipline experts in the role of stewards at the common, discipline, and project levels work to design and populate the ontology model. The result is a formal and consistent knowledge base that provides requirements for data representation, integrity, provenance, context, identification, and relationship. The contents of the knowledge base are translated and written to files in suitable formats to configure system software and services, provide user documentation, validate input, and support data analytics. This presentation will provide an overview of the framework, present a use case that has been adopted by an entire science discipline at the international level, and share some important lessons learned.

  14. Working Alongside Scientists: Impacts on Primary Teacher Beliefs and Knowledge about Science and Science Education

    Science.gov (United States)

    Anderson, Dayle; Moeed, Azra

    2017-01-01

    Current curriculum demands require primary teachers to teach about the Nature of Science; yet, few primary teachers have had opportunity to learn about science as a discipline. Prior schooling and vicarious experiences of science may shape their beliefs about science and, as a result, their science teaching. This qualitative study describes the…

  15. Exoplanets with JWST: degeneracy, systematics and how to avoid them

    Science.gov (United States)

    Barstow, Joanna K.; Irwin, Patrick G. J.; Kendrew, Sarah; Aigrain, Suzanne

    2016-07-01

    The high sensitivity and broad wavelength coverage of the James Webb Space Telescope will transform the field of exoplanet transit spectroscopy. Transit spectra are inferred from minute, wavelength-dependent variations in the depth of a transit or eclipse as the planet passes in front of or is obscured by its star, and the spectra contain information about the composition, structure and cloudiness of exoplanet atmospheres. Atmospheric retrieval is the preferred technique for extracting information from these spectra, but the process can be confused by astrophysical and instrumental systematic noise. We present results of retrieval tests based on synthetic, noisy JWST spectra, for clear and cloudy planets and active and inactive stars. We find that the ability to correct for stellar activity is likely to be a limiting factor for cloudy planets, as the effects of unocculted star spots may mimic the presence of a scattering slope due to clouds. We discuss the pros and cons of the available JWST instrument combinations for transit spectroscopy, and consider the effect of clouds and aerosols on the spectra. Aerosol high in a planet's atmosphere obscures molecular absorption features in transmission, reducing the information content of spectra in wavelength regions where the cloud is optically thick. We discuss the usefulness of particular wavelength regions for identifying the presence of cloud, and suggest strategies for solving the highly-degenerate retrieval problem for these objects.

  16. A 4K x 4K HgCdTe astronomical camera enabled by the JWST NIR detector development program

    Science.gov (United States)

    Hall, Donald N. B.; Luppino, Gerard; Hodapp, Klaus W.; Garnett, James D.; Loose, Markus; Zandian, Majid

    2004-09-01

    The ambitious science goals of the James Webb Space Telescope (JWST) have driven spectacular advances in λco ~ 5um detector technology over the past five years. This paper reviews both the UH/RSC team"s Phase A development and evaluation of 2Kx2K arrays exceeding the detector requirements for JWST"s near infrared instruments and also the hardware integration of these into a 4Kx4K (16Mpxl) close packed mosaic focal plane array housed in an Ultra Low Background test facility. Both individual first generation 2Kx2K SCA"s and 4Kx4K mosaic focal planes have been extensively characterized in the laboratory and, since September 2003, a NIR camera utilizing the 4Kx4K mosaic focal plane has been in use for nearly 100 nights at the UH 2.2 m telescope on Mauna Kea. Typical test results for the first generation 2Kx2K arrays and their integration into 4Kx4K mosaic focal planes are reported. Demonstration of the design concepts and both array and mosaic focal plane performance in actual hardware, as described here, has provided the foundation for design iterations leading to later generations of 2Kx2K arrays and 4Kx4K mosaic focal planes. Four major technology developments leading to first generation hardware demonstrations of both 2Kx2K SCA"s and a 4Kx4K mosaic FPA are reviewed. These are: 1) improvement in test equipment and procedures to characterize the detectors against JWST requirements and goals, primarily at 37K but with the capability to test from 30K to 100K; 2) optimization of λc ~ 5 um MBE HgCdTe material on a CZT substrate for low dark current (goal of 0.003 e-/sec at 37K) with high quantum efficiency, low cross-talk and greatly reduced image persistence; 3) development of the 2Kx2K HAWAII-2RG multiplexer designed specifically to take full advantage of these detector characteristics for a wide range of astronomical applications (and fully compatible with an ASIC controller developed under the JWST Instrument Technology Development initiative) and 4) development of

  17. Putting science to work in developing a climate policy.

    Science.gov (United States)

    Cicerone, Ralph J

    2009-01-01

    The National Academy of Sciences is an honorific society of distinguished scholars engaged in scientific and engineering research, dedicated to the furtherance of science and technology and to their use for the general welfare. This Viewpoint explores the interconnection between scientific research and policy making in developing a climate policy.

  18. College Students' Attitudes toward Science and Scientific Work

    Science.gov (United States)

    Sudas, L. G.; Iurasova, M. V.

    2006-01-01

    The reduction in the total numbers of scientists in Russia has been accompanied by negative changes in the age structure of science cadres. According to data of the Center for Research and Statistics of Science, in 1995, the ratio of specialists of the older age cohort (above the age of sixty) and the younger age cohort (up to the age of forty)…

  19. Soils. Science Education Research Unit. Working Paper 201.

    Science.gov (United States)

    Happs, John C.

    The Learning in Science Project has adopted the view that science teaching might be improved if teachers can be given some appreciation of students' views of the world and the beliefs, expectations, and language that learners bring to new learning situations. This investigation looks at the topic of soil, one of the basic resources of New Zealand…

  20. Social Work as an Action Science: A Perspective from Europe

    Science.gov (United States)

    Sommerfeld, Peter

    2014-01-01

    It is a surprising fact that social work is not conceived as a scientific discipline in many countries and especially in the United States. It is surprising because the extent of academic social work programs and the scientific output of people working at schools of social work are significant. And it is surprising anyway if social work is…

  1. Social Work as an Action Science: A Perspective from Europe

    Science.gov (United States)

    Sommerfeld, Peter

    2014-01-01

    It is a surprising fact that social work is not conceived as a scientific discipline in many countries and especially in the United States. It is surprising because the extent of academic social work programs and the scientific output of people working at schools of social work are significant. And it is surprising anyway if social work is…

  2. Solar System Science with the James Webb Space Telescope

    Science.gov (United States)

    Hammel, Heidi B.; Norwood, J.; Chanover, N.; Hines, D. C.; Stansberry, J.; Lunine, J. I.; Tiscareno, M. S.; Milam, S. N.; Sonneborn, G.; Brown, M.

    2013-10-01

    The James Webb Space Telescope (JWST) will succeed the Hubble Space Telescope as NASA’s premier space-based platform for observational astronomy. This 6.5-meter telescope, which is optimized for observations in the near and mid infrared, will be equipped with four state-of-the-art imaging, spectroscopic, and coronagraphic instruments. These instruments, along with the telescope’s moving target capabilities, will enable the infrared study of solar system objects with unprecedented detail (see companion presentation by Sonneborn et al.). This poster features highlights for planetary science applications, extracted from a white paper in preparation. We present a number of hypothetical solar system observations as a means of demonstrating potential planetary science observing scenarios; the list of applications discussed here is far from comprehensive. The goal of this poster and the subsequent white paper is to stimulate discussion and encourage participation in JWST planning among members of the planetary science community, and to encourage feedback to the JWST Project on any desired observing capabilities, data products, and analysis procedures that would enhance the use of JWST for solar system studies. The upcoming white paper updates and supersedes the solar system white paper published by the JWST Project in 2010 (Lunine et al., 2010), and is based in part on JWST events held at the 2012 DPS, the 2013 LPSC meeting, and this DPS (JWST Town Hall, Thursday, 10 October 2013, 12-1 pm).

  3. Connectivity Theory at Work: The Referrals between Science and Mathematics in a Science Unit

    Science.gov (United States)

    Mehmetlioglu, Deniz; Ozdem, Yasemin

    2014-01-01

    Researches carried out all around the world showed that students learn more effectively if they are able to make connections between subjects. This case reports based on an investigation of how mathematics concepts were connected to science concepts by a science teacher in an elementary science classroom, and on the science teacher's views…

  4. Primary Science: A View of the Classroom. Learning in Science Project (Primary). Working Paper No. 103.

    Science.gov (United States)

    Biddulph, Fred

    The first (exploratory) phase of the Learning in Science Project (Primary)--LISP(P)--focused on science teaching/learning in New Zealand primary schools. Previous information about science teaching/learning was obtained from interviews with children, teachers, principals, science advisers, teachers' college lecturers, and inspectors. To gain…

  5. The spectral calibration of JWST/NIRSpec: results from the recent cryo-vacuum campaign (ISIM-CV3)

    Science.gov (United States)

    Giardino, Giovanna; Luetzgendorf, Nora; Ferruit, Pierre; Dorner, Bernhard; Alves de Oliveira, Catarina; Birkmann, Stephan M.; Boeker, Torsten; Rawle, Tim; Sirianni, Marco

    2016-07-01

    The NIRSpec instrument of JWST can be operated in multi-object (MOS), long-slit, and integral field mode with spectral resolutions from 100 to 2700. Its MOS mode uses about a quarter of a million individually addressable mini-slits for object selection, covering a field of view of 9 square-arcminute. We have developed a procedure to optimize a parametric model of the instrument that provides the basis for the extraction of wavelength calibrated spectra from NIRSpec data, from any of the apertures and for all the modes. Here, we summarize the steps undertaken to optimize the instrument model parameters using the data acquired during the latest cryo-vacuum campaign of the JWST Integrated Science Instrument Module, recently carried out at NASA Goddard Space Flight Center. The calibrated parametric model is able to reproduce the spatial and spectral position of the input spectra with an intrinsic accuracy (1-sigma, RMS) ~ 1/10 of a pixel in spatial and spectral direction for all the modes. The overall wavelength calibration accuracy (RMS) of the model as measured on the extracted spectra is better than 1/20 of a resolution element for all of the grating-based spectral modes and at the level of 1/14 of a resolution element for the prism. These results are well within the allocations for the model in the overall spatial and spectral calibration budget of NIRSpec.

  6. Measuring segmented primary mirror WFE in the presence of vibration and thermal drift on the light-weighted JWST

    Science.gov (United States)

    Whitman, Tony L.; Dziak, Kenneth J.; Wells, Conrad; Olczak, Gene

    2012-09-01

    The light-weighted design of the Optical Telescope Element (OTE) of the James Webb Telescope (JWST) leads to additional sensitivity to vibration from the ground - an important consideration to the measurement uncertainty of the wavefront error (WFE) in the primary mirror. Furthermore, segmentation of the primary mirror leads to rigid-body movements of segment areas in the WFE. The ground vibrations are minimized with modifications to the test facility, and by the architecture of the equipment supporting the load. Additional special test equipment (including strategically placed isolators, tunable mass dampers, and cryogenic magnetic dampers) mitigates the vibration and the response sensitivity before reaching the telescope. A multi-wavelength interferometer is designed and operated to accommodate the predicted residual vibration. Thermal drift also adds to the measurement variation. Test results of test equipment components, measurement theory, and finite element analysis combine to predict the test uncertainty in the future measurement of the primary mirror. The vibration input to the finite element model comes from accelerometer measurements of the facility with the environmental control pumps operating. One of the isolators have been built and tested to validate the dynamic performance. A preliminary model of the load support equipment and the OTE with the Integrated Science Instrument Module (ISIM) is complete. The performance of the add-on dampers have been established in previous applications. And operation of the multi-wavelength interferometer was demonstrated on a scaled hardware version of the JWST in an environment with vibration and thermal drift.

  7. A new HST/Herschel deep field at the North Ecliptic Pole: preparing the way for JWST, SPICA and Euclid

    CERN Document Server

    Serjeant, Stephen; Burgarella, Denis; Clements, Dave; De Zotti, Gianfranco; Goto, Tomo; Hatsukade, Bunyo; Hopwood, Rosalind; Hwang, Narae; Inami, Hanae; Jeong, Woong-Seob; Kim, Seong Jin; Krumpe, Mirko; Lee, Myung Gyoon; Malkan, Matt; Matsuhara, Hideo; Miyaji, Takamitsu; Oyabu, Shinki; Pearson, Chris; Takeuchi, Tsutomu; Vaccari, Mattia; Valtchanov, Ivan; van der Werf, Paul; Wada, Takehiko; White, Glenn

    2012-01-01

    We propose a co-ordinated multi-observatory survey at the North Ecliptic Pole. This field is the natural extragalactic deep field location for most space observatories (e.g. containing the deepest Planck, WISE and eROSITA data), is in the continuous viewing zones for e.g. Herschel, HST, JWST, and is a natural high-visibility field for the L2 halo orbit of SPICA with deep and wide-field legacy surveys already planned. The field is also a likely deep survey location for the forthcoming Euclid mission. It is already a multi-wavelength legacy field in its own right (e.g. AKARI, LOFAR, SCUBA-2): the outstanding and unparalleled continuous mid-IR photometric coverage in this field and nowhere else enables a wide range of galaxy evolution diagnostics unachievable in any other survey field, by spanning the wavelengths of redshifted PAH and silicate features and the peak energy output of AGN hot dust. We argue from the science needs of Euclid and JWST, and from the comparative multiwavelength depths, that the logical ...

  8. Studying the spectral properties of Active Galactic Nuclei in the JWST era

    CERN Document Server

    Nakos, Th; Alonso-Herrero, A; Labiano, A

    2009-01-01

    The James Webb Space Telescope (JWST), due to launch in 2014, shall provide an unprecedented wealth of information in the near and mid-infrared wavelengths, thanks to its high-sensitivity instruments and its 6.5 m primary mirror, the largest ever launched into space. NIRSpec and MIRI, the two spectrographs onboard JWST, will play a key role in the study of the spectral features of Active Galactic Nuclei in the 0.6-28 micron wavelength range. This talk aims at presenting an overview of the possibilities provided by these two instruments, in order to prepare the astronomical community for the JWST era.

  9. Assessing Intrinsic Values of a Lecture-Free High School Science Education for Collegiate Science Work: A Case Study

    Science.gov (United States)

    Dorais, Christopher James

    2012-01-01

    This case study examined the efficacy of the individualized instruction teaching methodology as it was applied within high school science classes. Also examined was how individualized instruction at the high school level prepared students to do collegiate science level work. [The dissertation citations contained here are published with the…

  10. Response: Social Work, Science, Social Impact--Crafting an Integrative Conversation

    Science.gov (United States)

    Nurius, Paula S.; Kemp, Susan P.

    2012-01-01

    Shifts in the ways that science is being undertaken and marshaled toward social change argue for a new kind of professional competence. Taking the view that the science of social work is centrally about the relationship of research to social impact, the authors extend Fong's focus on transdisciplinary and translational approaches to science,…

  11. Recovering Knowledge for Science Education Research: Exploring the "Icarus Effect" in Student Work

    Science.gov (United States)

    Georgiou, Helen; Maton, Karl; Sharma, Manjula

    2014-01-01

    Science education research has built a strong body of work on students' understandings but largely overlooked the nature of science knowledge itself. Legitimation Code Theory (LCT), a rapidly growing approach to education, offers a way of analyzing the organizing principles of knowledge practices and their effects on science education. This…

  12. Toward a Framework. Learning in Science Project (Primary). Working Paper No. 101.

    Science.gov (United States)

    Osborne, Roger

    This paper proposes some possible areas of research and tentative theoretical guidelines for the Learning in Science Project (Primary)-- LISP(P). This new project, designed to investigate the teaching and learning of science in the primary school, arises from the work of the original Learning in Science Project (LISP). LISP(P) has two…

  13. How nature works the science of self-organized criticality

    CERN Document Server

    Bak, Per

    1996-01-01

    This is an acclaimed book intended for the general reader who is interested in science. The author is a physicist who is well-known for his development of the property called "self-organized criticality", a property or phenomenon that lies at the heart of large dynamical systems. It can be used to analyse systems that are complicated, and which are part of the new science of complexity. It is a unifying concept that can be used to study phenomena in fields as diverse as economics, astronomy, the earth sciences, and physics. The author discusses his discovery of self-organized criticality; its relation to the world of classical physics; computer simulations and experiments which aid scientists' understanding of the property; and the relation of the subject to popular areas such as fractal geometry and power laws; cellular automata, and a wide range of practical applications.

  14. Evolution of science II: Insights into working of Nature

    CERN Document Server

    Vahia, M N

    2016-01-01

    We attempt to provide a comprehensive model of evolution of science across millennia taking into account the contributions of other intellectual traditions, cultural value system and increasing in sophistication of humans in their study of nature. We also briefly discuss the role of technology and its interplay in the evolution of science. We identify five primary approaches to the study of nature, namely ad hoc formulations, religious approach, pragmatic approach, axiomatic approach and the logic based approach. Each of these approaches have had their prime periods and have contributed significantly to human understanding of nature and have also overlapped within a society. Each approach has had a central role over human evolution at some stage. We surmise that the currently dominant axiomatic method will reach its limits due to complexity of the system and may never be fully formalised. We suggest that the future progress of science will more be a logic based approach where experimentation and simulations r...

  15. JWST tunable filter imager: etalon prototype test results

    Science.gov (United States)

    Touahri, D.; Cameron, P.; Evans, C.; Greenberg, E.; Rowlands, N.; Scott, A.; Doyon, R.; Beaulieu, M.; Djazovski, O.

    2008-07-01

    We present the prototyping results and laboratory characterization of a narrow band Fabry-Perot etalon flight model which is one of the wavelength selecting elements of the Tunable Filter Imager. The latter is a part of the Fine Guidance Sensor which represents the Canadian contribution to NASA's James Webb Space Telescope. The unique design of this etalon provides the JWST observatory with the ability to image at 30 Kelvin, a 2.2'x2.2' portion of its field of view in a narrow spectral bandwidth of R~100 at any wavelength ranging between 1.6 and 4.9 μm (with a gap in coverage between 2.5 and 3.2 μm). Extensive testing has resulted in better understanding of the thermal properties of the piezoelectric transducers used as an actuation system for the etalon gap tuning. Good throughput, spectral resolution and contrast have been demonstrated for the full wavelength range.

  16. Science and technology awareness for preschool children: a working model

    CSIR Research Space (South Africa)

    Van Deventer, A

    2009-05-01

    Full Text Available these positive experiences as references to support their developing interests and attitudes towards Science and Technology. The Process TekkiTots started in 2006 when Morning Star Montessori preschool in the Pretoria area expressed the need for Science... to preschool children. I put together twenty-five lessons and presented it to a group of six children at a Montessori preschool once a week. It took on average an hour to complete a lesson. I observed the interest the children showed and eagerness to take...

  17. THE ROLE OF SCHOOL TECHNICIANS IN PROMOTING SCIENCE THROUGH PRACTICAL WORK

    Directory of Open Access Journals (Sweden)

    Anne T. Helliar

    2011-11-01

    Full Text Available This is a review of the role of practical work in UK’s secondary school science lessons, the impact that practical work has in the promotion of science, the challenges created through use of non-specialist science teachers and a possible additional role for science technicians. The paper considers how improved deployment of suitably experienced school science technicians and their recognition, by schools’ management, for their involvement in the delivery of training in the use of practical work, for less experienced teachers, could benefit schools and their students. This together with its companion paper endeavours to show how the more effective use of practical work and technicians can encourage more students to select science at higher, non-compulsory levels.

  18. As Science Evolves, How Can Science Policy? NBER Working Paper No. 16002

    Science.gov (United States)

    Jones, Benjamin

    2010-01-01

    Getting science policy right is a core objective of government that bears on scientific advance, economic growth, health, and longevity. Yet the process of science is changing. As science advances and knowledge accumulates, ensuing generations of innovators spend longer in training and become more narrowly expert, shifting key innovations (i)…

  19. As Science Evolves, How Can Science Policy? NBER Working Paper No. 16002

    Science.gov (United States)

    Jones, Benjamin

    2010-01-01

    Getting science policy right is a core objective of government that bears on scientific advance, economic growth, health, and longevity. Yet the process of science is changing. As science advances and knowledge accumulates, ensuing generations of innovators spend longer in training and become more narrowly expert, shifting key innovations (i)…

  20. Who Does Extra-Credit Work in Introductory Science Courses?

    Science.gov (United States)

    Moore, Randy

    2005-01-01

    On the first day of classes, 81% of students in an introductory biology course claimed that they would submit extra-credit work if given the opportunity. When given two chances for extra-credit work, fewer than one-fourth of students submitted one or both assignments. Students who submitted extra-credit work were more likely to attend class,…

  1. Science in the Sixth Form, Working Paper No. 4.

    Science.gov (United States)

    Schools Council, London (England).

    These proceedings of a 1965 conference on the teaching of science in the sixth form of English schools contain summaries of each speaker's introduction to his paper, the full text of his circulated paper, and a summary of the discussion that followed. The papers were titled the sixth form; "Structure and Properties of Matter" as a sixth…

  2. Environmental engineers receive top science paper award for investigative work

    OpenAIRE

    Nystrom, Lynn A.

    2010-01-01

    Marc Edwards and Simoni Triantafyllidou of Virginia Tech's College of Engineering, along with colleague Dr. Dana Best of Children's National Medical Center, published a 2009 article in "Environmental Science and Technology" (ES&T) that demonstrated a major increase in childhood lead poisoning of Washington, D.C., children during the 2001-04 lead-in-water crisis.

  3. Implementation Science: Why It Matters for the Future of Social Work

    Science.gov (United States)

    Cabassa, Leopoldo J.

    2016-01-01

    Bridging the gap between research and practice is a critical frontier for the future of social work. Integrating implementation science into social work can advance our profession's effort to bring research and practice closer together. Implementation science examines the factors, processes, and strategies that influence the uptake, use, and…

  4. Social Science and/or Social Work: Do We (Should We) Teach Them Both?

    Science.gov (United States)

    Frysztacki, Krzysztof

    2008-01-01

    Addresses teaching in social work on the basis of two different theories related to social work and social science, noting crucial aspects of each. Notes deep differences between theoretical and applied sciences and discusses ways in which a dynamic complementarity can be achieved in teaching the theoretical and the professional. Applies the major…

  5. ESIP Earth Sciences Data Analytics (ESDA) Cluster - Work in Progress

    Science.gov (United States)

    Kempler, Steven

    2015-01-01

    The purpose of this poster is to promote a common understanding of the usefulness of, and activities that pertain to, Data Analytics and more broadly, the Data Scientist; Facilitate collaborations to better understand the cross usage of heterogeneous datasets and to provide accommodating data analytics expertise, now and as the needs evolve into the future; Identify gaps that, once filled, will further collaborative activities. Objectives Provide a forum for Academic discussions that provides ESIP members a better understanding of the various aspects of Earth Science Data Analytics Bring in guest speakers to describe external efforts, and further teach us about the broader use of Data Analytics. Perform activities that:- Compile use cases generated from specific community needs to cross analyze heterogeneous data- Compile sources of analytics tools, in particular, to satisfy the needs of the above data users- Examine gaps between needs and sources- Examine gaps between needs and community expertise- Document specific data analytics expertise needed to perform Earth science data analytics Seek graduate data analytics Data Science student internship opportunities.

  6. Framing Education for a Science of Social Work: Missions, Curriculum, and Doctoral Training

    Science.gov (United States)

    Fong, Rowena

    2012-01-01

    Social work education has historically been grounded in professional practice but recent discussions have urged a reconsideration of social work as a science. Social work is progressively doing more intervention work, service systems research, implementation research, and translational research which are elevating research standards to new levels…

  7. A WIDER ROLE FOR TECHNICIANS IN SCIENCE PRACTICAL WORK WITH SCHOOL STUDENTS?

    Directory of Open Access Journals (Sweden)

    Timothy G. Harrison

    2011-12-01

    Full Text Available This paper reports the results of a study made on the impact of improved deployment of science technicians in the classroom could directly benefit students in practical science investigations. Science technicians are skilled individuals whose understanding of practical work is a valuable resource not being used of in support of students understanding of science. Aspects of practical work and technician support were scrutinised, through information attained from a post-16 student survey to improve understanding about this teaching tool, to establish if it was being used to its full potential within science lessons. Analysis was also made of students’ perceptions of school science. The main outcomes were that the majority of students enjoyed science practical work and felt that science could not be taught without it. Students studying science at pre-university level attained a greater understanding, through participating in relevant practical work, than students who had studied it at earlier, compulsory levels. Students reported that science technicians provide impact on student learning when contact time was the greatest.

  8. Working with DNA & Bacteria in Precollege Science Classrooms.

    Science.gov (United States)

    Horn, Toby Mogollon; Frame, Kathy, Ed.

    This document describes ways to work with DNA and host organisms in precollege classrooms. The guidelines are intended to assist the teacher who already has training in working with microbes, DNA, and associated chemicals. The contents of the guidelines include: (1) Permitted DNA molecules, vectors, and recommended host organisms for constructing…

  9. Optical Coating Performance and Thermal Structure Design for Heat Reflectors of JWST Electronic Control Unit

    Science.gov (United States)

    Quijada, Manuel A.; Threat, Felix; Garrison, Matt; Perrygo, Chuck; Bousquet, Robert; Rashford, Robert

    2008-01-01

    The James Webb Space Telescope (JWST) consists of an infrared-optimized Optical Telescope Element (OTE) that is cooled down to 40 degrees Kelvin. A second adjacent component to the OTE is the Integrated Science Instrument Module, or ISIM. This module includes the electronic compartment, which provides the mounting surfaces and ambient thermally controlled environment for the instrument control electronics. Dissipating the 200 watts generated from the ISIM structure away from the OTE is of paramount importance so that the spacecraft's own heat does not interfere with the infrared light detected from distant cosmic sources. This technical challenge is overcome by a thermal subsystem unit that provides passive cooling to the ISIM control electronics. The proposed design of this thermal radiator consists of a lightweight structure made out of composite materials and low-emittance metal coatings. In this paper, we will present characterizations of the coating emittance, bidirectional reflectance, and mechanical structure design that will affect the performance of this passive cooling system.

  10. Status of the JWST/MIRI Focal Plane System and Cooler

    Science.gov (United States)

    Ressler, Michael E.; Goodson, G. B.; Khorrami, M. A.; Larson, M. E.; Mahoney, J. C.; Sukhatme, K. G.

    2009-01-01

    The Mid-Infrared Instrument (MIRI) is a multipurpose imager, coronagraph, and spectrometer for the James Webb Space Telescope. It provides wavelength coverage from 5 through 28 microns and is an integral contributor to all four of JWST's primary science themes. MIRI is being developed as a partnership between NASA and ESA, with JPL providing the Focal Plane System (FPS, consisting of the detectors, control electronics, and flight software) and the cooler, and a consortium of European astronomical institutes providing the optical bench and structure. The flight FPS is being prepared for delivery to the European Consortium for its integration into the optical bench, while the cooler is nearing its Critical Design Review. We describe the capabilities of the FPS and cooler, present test results and the predicted sensitivity performance of the FPS, and update the current status of each these systems. The research described in this poster was carried out at the Jet Propulsion Laboratory, California Institute of Technology, under a contract with the National Aeronautics and Space Administration.

  11. Collaborative Reflection through Dilemma Cases of Science Practical Work during Practicum

    Science.gov (United States)

    Yoon, Hye-Gyoung; Kim, Mijung

    2010-02-01

    In the goal of science teacher education, the role of reflection to cultivate the teacher as a transformative practitioner has been largely recognised. Reflective thinking is crucial for teachers to be mindfully and knowledgeably situated in teaching and transforming their actions. This study looks into the dilemmas of teaching practical work in elementary science classes and the roles of reflective thinking. Five preservice teachers, one inservice teacher, and one science teacher educator participated in the process of collaborative reflection (reflective writing on dilemma cases, sharing, and discussing) of teaching practical work during the preservice teachers' practicum. All participants wrote and shared two cases of his/her own dilemmas after teaching or observing lessons with science experiments. Preservice teachers also participated in a survey questionnaire and interviews to share their perspectives of practical work and the process of reflection. Looking into their reflection and discussion on the dilemmas of teaching through science practical work, the study attempts to explore how to make collaborative learning opportunities through reflective thinking. The findings of this study showed that the dilemmas of science practical work emerged in various dimensions of teachers' expectation and classroom interactions. Discussions on dilemma cases could facilitate reflecting and learning from different perspectives among participants. Based on these findings, we further discuss the implication of interactive reflection and discussion on dilemmas of practical work to enhance science teaching and develop collaborative communities in science teacher education.

  12. The Philosophical Works of Ludwik Fleck and Their Potential Meaning for Teaching and Learning Science

    Science.gov (United States)

    Stuckey, Marc; Heering, Peter; Mamlok-Naaman, Rachel; Hofstein, Avi; Eilks, Ingo

    2015-04-01

    This paper discusses essential elements of the philosophical works of Ludwik Fleck (1896-1961) and their potential interpretation for the teaching and learning of science. In the early twentieth century, Fleck made substantial contributions to understanding the sociological character of the nature of science and explaining the embedding of science in society. His works have several parallels to the later and very popular work, The Structure of Scientific Revolutions, by Thomas S. Kuhn, although Kuhn only indirectly referred to the influence of Fleck on his own theories. Starting from a short review of the life of Ludwik Fleck, his philosophical work and its connections to Kuhn, this paper elaborates upon and illustrates how his theories can be considered for science education in order to provide learners with a better understanding of the nature of scientific endeavor and the bi-directional science-to-society links.

  13. A Science of Social Work, and Social Work as an Integrative Scientific Discipline: Have We Gone Too Far, or Not Far Enough?

    Science.gov (United States)

    Brekke, John S.

    2014-01-01

    There are two purposes to this article. The first is to update the science of social work framework. The second is to use recent discussions on the nature of realist science and on social work science to propose a definition of social work as an integrative scientific discipline that complements its definition as a profession.

  14. A Science of Social Work, and Social Work as an Integrative Scientific Discipline: Have We Gone Too Far, or Not Far Enough?

    Science.gov (United States)

    Brekke, John S.

    2014-01-01

    There are two purposes to this article. The first is to update the science of social work framework. The second is to use recent discussions on the nature of realist science and on social work science to propose a definition of social work as an integrative scientific discipline that complements its definition as a profession.

  15. Importance of empathy for social work practice: integrating new science.

    Science.gov (United States)

    Gerdes, Karen E; Segal, Elizabeth

    2011-04-01

    Empathy is more important than ever to a national population worried about difficult political and socioeconomic situations. During the last 10 years, an enormous amount of research has been carried out to elucidate the nature, mechanism, and function of empathy. New research from social-cognitive neuroscience and related fields indicates that, like language or eye-hand coordination, empathy is an innate human capability that can be greatly enhanced by purposeful and informed guidance. Empathy is particularly important to social work practice. Clients experiencing empathy through treatment have improved outcomes. Empathic social work practitioners are more effective and can balance their roles better. Social work practitioners can and should learn about emerging research on empathy and use that information to better serve their client populations. This article, emphasizing research of the past decade, focuses on empathy and its benefits as an asset to social work practitioners.

  16. Toward a Teaching Model for Primary Science. Learning in Science Project (Primary). Working Paper No. 114.

    Science.gov (United States)

    Harlen, Wynne; Osborne, Roger

    The Learning in Science Project (Primary)--LISP(P)--was designed to examine problems and difficulties in primary science and to explore ways of overcoming these problems. Early research led to a proposal that children's questions and explanations could form the basis of an alternative teaching approach. However, several issues were raised which…

  17. Science 101: How Does an Electron Microscope Work?

    Science.gov (United States)

    Robertson, Bill

    2013-01-01

    Contrary to popular opinion, electron microscopes are not used to look at electrons. They are used to look for structure in things that are too small to observe with an optical microscope, or to obtain images that are magnified much more than is obtainable with an optical microscope. To understand how electron microscopes work, it will help to go…

  18. Science 101: How Does an Electron Microscope Work?

    Science.gov (United States)

    Robertson, Bill

    2013-01-01

    Contrary to popular opinion, electron microscopes are not used to look at electrons. They are used to look for structure in things that are too small to observe with an optical microscope, or to obtain images that are magnified much more than is obtainable with an optical microscope. To understand how electron microscopes work, it will help to go…

  19. Doing science: how to get credit for your scientific work.

    Science.gov (United States)

    Caudri, Daan; Bjerg, Anders; Saad, Neil; Jacinto, Tiago; Chalmers, James; Hardavella, Georgia

    2015-06-01

    Everyone deserves to be acknowledged for their efforts and contributions to a shared goal, and getting credit for your scientific work should be part of a natural process and should be fair and straightforward. However, credit cannot be objectively measured despite it having a big influence and, unfortunately, getting appropriate credit can occasionally be both complicated and challenging.

  20. The impact of the `Getting Practical: Improving Practical Work in Science' continuing professional development programme on teachers' ideas and practice in science practical work

    Science.gov (United States)

    Abrahams, Ian; Reiss, Michael J.; Sharpe, Rachael

    2014-09-01

    Background:Despite the widespread use of practical work in school it has been recognised that more needs to be done to improve its effectiveness in developing conceptual understanding. The 'Getting Practical' CPD (Continuing Professional Development) programme was designed to contribute towards an improvement in the effectiveness of practical work through initiating changes in teachers' predominantly 'hands-on' approach to practical work to one which manifests a more equitable balance between 'hands-on' and 'minds-on'. Purpose:To evaluate the impact of the Getting Practical: Improving Practical Work in Science CPD programme on teachers' ideas and practice in science practical work in primary and secondary schools in England. Programme description:The CPD programme was designed to improve the effectiveness of science practical work in developing conceptual understanding in primary and secondary schools in England. Sample:Ten teachers of primary science and 20 secondary science teachers. Design and methods:The study employed a condensed fieldwork strategy with data collected using interviews, observational field notes and pre- and post-CPD training observations in practical lessons within 30 schools. Results:Whilst the CPD programme was effective in getting teachers to reflect on the ideas associated with the Getting Practical programme, it was much less effective in bringing about changes in actual teaching practice. Conclusion:The findings suggest that if change, rather than only an enhanced awareness of the issues, is to be brought about in established teaching practice then there is a need for ongoing support over an extended period of time. Furthermore, the impact of such CPD is more likely to be effective if it is undertaken by a senior member of a department or school with the full support of the SMT.

  1. Deep IRAC Imaging Lensing Galaxy Clusters for JWST 'First Light' Search

    Science.gov (United States)

    Yan, Haojing; Conselice, Christopher; Windhorst, Rogier; Cohen, Seth; Alpaslan, Mehmet; Zitrin, Adi; Broadhurst, Tom; Frye, Brenda; Driver, Simon; Robotham, Aaron; Hopkins, Andrew; Wyithe, Staurt; Jansen, Rolf; Hathi, Nimish; Mechtley, Matthew; Ryan, Russell; Rutkowski, Michael; Finkelstein, Steven; Koekemoer, Anton

    2016-08-01

    JWST has a key goal to search for First Light objects beyond z>10. Our 110-hr JWST GTO program, 'Webb Medium-Deep Fields' (WMDF), will target both blank and lensed fields to probe both the bright and the faint ends of the galaxy luminosity function at z > 10. While a number of well studied lensing clusters exist, not all of them are optimal for the JWST search of First Light objects, either because of their low Ecliptic latitudes (and hence high Zodiacal background) or because of their strong intra-cluster light (ICL) at the critical curve regions corresponding to the redshifts of interest. For this reason, our WMDF candidate lensing targets will include some recently discovered, high-mass (log[M/Msun] ~ 15) galaxy clusters, which we choose either because of their high Ecliptic latitude (beta > 40 deg) or because of their extreme compactness that minimizes the impact of the ICL. As part of our effort to collect ancillary data for these new systems to finalize the target list, we propose IRAC observations for 13 of them that are lacking sufficient data. These 3.6/4.5um data will be critical for our guaranteed JWST program: (1) they will greatly facilitate the modeling of the straylight that JWST will suffer in 1--5 um (the key range to search for z>10--20 objects), a problem that has recently been identified. If left untreated, such straylight components would severely hamper the detection of faint sources in a lensing field. The JWST observations alone would be difficult to separate the ICL from the straylight at the level needed. (2) the new 3.6/4.5um data will best match our deep optical imaging and spectroscopy at HST, Gemini, LBT and MMT. We will derive accurate photometric redshifts for any lensed background galaxies (at znote that these data will be highly valuable for the study of these clusters themselves before the JWST mission.

  2. "Solidarity and Support": Feminist Memory Work Focus Groups with Working-Class Women Studying Social Science Degrees in Australia

    Science.gov (United States)

    Michell, Dee; Beddoe, Liz; Fraser, Heather; Jarldorn, Michele

    2017-01-01

    This paper reports on our use of a two-phased, feminist memory work in a project conducted with 11 women, social science students at an Australian university. We begin by describing government-led attempts to widen participation in Australian universities because 10 of the 11 women who participated in our project were from…

  3. "Solidarity and Support": Feminist Memory Work Focus Groups with Working-Class Women Studying Social Science Degrees in Australia

    Science.gov (United States)

    Michell, Dee; Beddoe, Liz; Fraser, Heather; Jarldorn, Michele

    2017-01-01

    This paper reports on our use of a two-phased, feminist memory work in a project conducted with 11 women, social science students at an Australian university. We begin by describing government-led attempts to widen participation in Australian universities because 10 of the 11 women who participated in our project were from…

  4. Working-Class Women Study Social Science Degrees: Remembering Enablers and Detractors

    Science.gov (United States)

    Fraser, Heather; Michell, Dee; Beddoe, Liz; Jarldorn, Michele

    2016-01-01

    In this article, we report on a feminist memory work project conducted with 11 working-class women in Australia. Participants responded to the question: "what helps and hinders working-class women study social science degrees?" The women confirmed that to succeed at university, they needed opportunities, resources, support and…

  5. Boundary Work and Power in the Controversy over Therapeutic Touch in Finnish Nursing Science

    Science.gov (United States)

    Vuolanto, Pia

    2015-01-01

    The boundary work approach has been established as one of the main ways to study controversies in science. However, it has been proposed that it does not meet the power dynamics of the scientific field sufficiently. This article concentrates on the intertwining of boundary work and power. It combines the boundary work approach developed by Thomas…

  6. Working-Class Women Study Social Science Degrees: Remembering Enablers and Detractors

    Science.gov (United States)

    Fraser, Heather; Michell, Dee; Beddoe, Liz; Jarldorn, Michele

    2016-01-01

    In this article, we report on a feminist memory work project conducted with 11 working-class women in Australia. Participants responded to the question: "what helps and hinders working-class women study social science degrees?" The women confirmed that to succeed at university, they needed opportunities, resources, support and…

  7. Why Games Work and the Science of Learning

    Science.gov (United States)

    Murphy, Curtiss

    2012-01-01

    In 2010, the Navy formally added the Damage Control Trainer (DCT) to the recruit training program at Great Lakes, Illinois. Despite the incredibly dense training schedule at the Navy's boot camp, the instructors were willing to set aside two hours of time for recruits to play a game. Why? Because it worked. Even with just one hour of play, research showed that recruits gained a 50-80% improvement in performance that transferred to Battle Stations 21 (B821), the Navy's capstone training event. This paper explores why games makes these kinds of results possible. It argues that the things that are known to improve learning are almost exactly the same reasons why games work: the time-honored laws of learning. It concludes that the traditional gulf between instructional design and game design is really an issue of perspective, rather than fundamentals.

  8. The Coming Crisis in Social Work: Some Thoughts on Social Work and Science

    Science.gov (United States)

    Longhofer, Jeffrey; Floersch, Jerry

    2012-01-01

    In this essay, the authors consider the challenge made by two keynote speakers at recent social work research conferences, one in the United States and the other in Europe. Both spoke of a knowledge crisis in social work. Both John Brekke (Society for Social Work and Research) and Peter Sommerfeld (First Annual European Conference for Social Work…

  9. The Work of Popper and Kuhn on the Nature of Science.

    Science.gov (United States)

    Donnelly, James

    1979-01-01

    Discusses the work of T. S. Kuhn and Sir Karl Popper. Current views on the nature of science and some current ideology of scientific education are also analyzed with regard to the views of science due to Kuhn and Popper. (HM)

  10. Minutes of TOPEX/POSEIDON Science Working Team Meeting and Ocean Tides Workshop

    Science.gov (United States)

    Fu, Lee-Lueng (Editor)

    1995-01-01

    This third TOPEX/POSEIDON Science Working Team meeting was held on December 4, 1994 to review progress in defining ocean tide models, precision Earth orbits, and various science algorithms. A related workshop on ocean tides convened to select the best models to be used by scientists in the Geophysical Data Records.

  11. Secondary School Students' Perceptions of Working Life Skills in Science-Related Careers

    Science.gov (United States)

    Salonen, Anssi; Hartikainen-Ahia, Anu; Hense, Jonathan; Scheersoi, Annette; Keinonen, Tuula

    2017-01-01

    School students demonstrate a lack of interest in choosing science studies and science-related careers. To better understand the underlying reasons, this study aims to examine secondary school students' perceptions of working life skills and how these perceptions relate to the skills of the twenty-first century. The participants in this study were…

  12. Life Works: Explore Health and Medical Science Careers | NIH MedlinePlus the Magazine

    Science.gov (United States)

    ... My favorite subjects in school were always science, sociology, and math. My interest in science was so well known that in high school, I was voted most likely to become a scientist. “What I like best about my work is that almost every day is different and ...

  13. Beyond Contradiction: Exploring the Work of Secondary Science Teachers as They Embed Environmental Education in Curricula

    Science.gov (United States)

    Steele, Astrid

    2011-01-01

    Traditional secondary science education draws on markedly different pedagogies than those made use of in contemporary environmental education, therefore, embedding environmental education within secondary science curriculum presents both epistemological and practical difficulties for teachers. This ethnographic study examines the work of six…

  14. The Framework Revisited. Learning in Science Project (Primary). Working Paper No. 111.

    Science.gov (United States)

    Biddulph, Fred; And Others

    The first working paper of the Learning in Science Project (Primary)--LISP(P)--"Toward a Framework," outlined what was then seen (1982) as the major aim of the project and proposed a research plan that seemed capable of enabling the project to establish difficulties that teachers have teaching science, to identify difficulties children…

  15. Virginia Bioinformatics Institute offers fellowships for graduate work in transdisciplinary science

    OpenAIRE

    Bland, Susan

    2008-01-01

    The Virginia Bioinformatics Institute at Virginia Tech, in collaboration with Virginia Tech's Ph.D. program in genetics, bioinformatics, and computational biology, is providing substantial fellowships in support of graduate work in transdisciplinary team science.

  16. Predicting the High Redshift Galaxy Population for JWST

    Science.gov (United States)

    Flynn, Zoey; Benson, Andrew

    2017-01-01

    The James Webb Space Telescope will be launched in Oct 2018 with the goal of observing galaxies in the redshift range of z = 10 - 15. As redshift increases, the age of the Universe decreases, allowing us to study objects formed only a few hundred million years after the Big Bang. This will provide a valuable opportunity to test and improve current galaxy formation theory by comparing predictions for mass, luminosity, and number density to the observed data. We have made testable predictions with the semi-analytical galaxy formation model Galacticus. The code uses Markov Chain Monte Carlo methods to determine viable sets of model parameters that match current astronomical data. The resulting constrained model was then set to match the specifications of the JWST Ultra Deep Field Imaging Survey. Predictions utilizing up to 100 viable parameter sets were calculated, allowing us to assess the uncertainty in current theoretical expectations. We predict that the planned UDF will be able to observe a significant number of objects past redshift z > 9 but nothing at redshift z > 11. In order to detect these faint objects at redshifts z = 11-15 we need to increase exposure time by at least a factor of 1.66.

  17. What is Social Sciences and Humanities Research "Worth,"? Neoliberalism and the Framing of Social Sciences and Humanities Work in Canada

    Science.gov (United States)

    Davidson-Harden, Adam

    2013-01-01

    This article offers a critique of the discursive politics represented in attempts to frame social sciences and humanities work in the mould of neoliberal knowledge capitalism. The critique offered is inspired by Foucault's critical thought on neoliberalism and an interpretation of "neoliberal governmentality" that flows from his…

  18. What is Social Sciences and Humanities Research "Worth,"? Neoliberalism and the Framing of Social Sciences and Humanities Work in Canada

    Science.gov (United States)

    Davidson-Harden, Adam

    2013-01-01

    This article offers a critique of the discursive politics represented in attempts to frame social sciences and humanities work in the mould of neoliberal knowledge capitalism. The critique offered is inspired by Foucault's critical thought on neoliberalism and an interpretation of "neoliberal governmentality" that flows from his College…

  19. Evaluating the Development of Science Research Skills in Work-Integrated Learning through the Use of Workplace Science Tools

    Science.gov (United States)

    McCurdy, Susan M.; Zegwaard, Karsten E.; Dalgety, Jacinta

    2013-01-01

    Concept understanding, the development of analytical skills and a research mind set are explored through the use of academic tools common in a tertiary science education and relevant work-integrated learning (WIL) experiences. The use and development of the tools; laboratory book, technical report, and literature review are examined by way of…

  20. Exploring an Alternative Science Teaching Approach. Learning in Science Project (Primary). Working Paper No. 109.

    Science.gov (United States)

    Biddulph, Fred; Roger, Juliet

    An alternative teaching model has been proposed by the Learning in Science Project (Primary)--LISP(P). The model uses a six-step approach (outlined in an appendix) which fosters an environment in which children can ask questions about a situation, offer explanations, carry out investigations, and report their findings. This paper reports on the…

  1. Learning in Science Education Across School and Science Museums – Design and Development Work in a Multi-Professional Group

    Directory of Open Access Journals (Sweden)

    Cecilie Jahreie

    2011-06-01

    Full Text Available The MIRACLE project aims to design and develop learning activities in science that will be used across schools and museum settings. A combination of digital technologies plays a vital role in bridging these institutional contexts. Cultural Historical Activity Theory will be used to analyse how the multi-professional project group orients to designing for science learning. In the analysis, we identify three contradicting orientations: experience, emotional involvement, and conceptual understanding. We discuss the implication this has for the further design work.

  2. From the Big Bang to the Nobel Prize and the JWST

    Science.gov (United States)

    Mather, John C.

    2007-01-01

    I will describe the history of the universe, from the Big Bang to 2013, when the JWST is to be launched to look back towards our beginnings. I will discuss how the COBE results led to the Nobel Prize, how the COBE results have been confirmed and extended, and their implications for future observations. The James Webb Space Telescope will be used to examine every part of our history from the first stars and galaxies to the formation of individual stars and planets and the delivery of life-supporting materials to the Earth. I will describe the plans for the JWST and how observers may use it. With luck, the JWST may produce a Nobel Prize for some discovery we can only guess today.

  3. Design and implementation of an integrated computer working environment for doing mathematics and science

    NARCIS (Netherlands)

    Heck, A.; Kedzierska, E.; Ellermeijer, T.

    2009-01-01

    In this paper we report on the sustained research and development work at the AMSTEL Institute of the University of Amsterdam to improve mathematics and science education at primary and secondary school level, which has lead amongst other things to the development of the integrated computer working

  4. Students' Views About Secondary School Science Lessons: The Role of Practical Work

    Science.gov (United States)

    Toplis, Rob

    2012-06-01

    This paper reports an interpretive study that sought students' views about the role that practical work plays in their school science lessons. Twenty-nine students aged between 13 and 16 years were selected from three secondary schools in England. Data were collected from initial lesson observations and in-depth interviews in order to explore students' views about practical work. The findings suggest that students have three main reasons why practical work is important in their school science lessons: for interest and activity, including social and personal features such as participation and autonomy; as an alternative to other forms of science teaching involving a pedagogy of transmission, and as a way of learning, including memorizing and recall. The findings are discussed in the context of a critical view of previous work on the role of practical work, work on attitudes to science and on the student voice. The paper concludes that practical work is seen to provide opportunities for students to engage with and influence their own learning but that learning with practical work remains a complex issue that needs further research and evaluation about its use, effectiveness and of the role of scientific inquiry as a component of practical activity.

  5. Science, Social Work, and Intervention Research: The Case of "Critical Time Intervention"

    Science.gov (United States)

    Jenson, Jeffrey M.

    2014-01-01

    Intervention research is an important, yet often neglected, focus of social work scholars and investigators. The purpose of this article is to review significant milestones and recent advances in intervention research. Methodological and analytical developments in intervention research are discussed in the context of science and social work.…

  6. Design and implementation of an integrated computer working environment for doing mathematics and science

    NARCIS (Netherlands)

    Heck, A.; Kedzierska, E.; Ellermeijer, T.

    2009-01-01

    In this paper we report on the sustained research and development work at the AMSTEL Institute of the University of Amsterdam to improve mathematics and science education at primary and secondary school level, which has lead amongst other things to the development of the integrated computer working

  7. An Exploration of Teachers' Efforts to Understand Identity Work and its Relevance to Science Instruction

    Science.gov (United States)

    Smith, M. Cecil; Darfler, Anne

    2012-06-01

    US educators express concern that students are turning away from the study of science and have little interest in pursuing science careers. Nationally, science achievement scores for 8th graders are unchanged since 1996, but 12th graders' scores have significantly decreased. A shortcoming of education reform efforts is lack of attention to students' developmental needs. Science study should enable students to learn about themselves—to develop and refine their skills, define their values, explore personal interests, and understand the importance of science to themselves and others. Effective secondary science instruction requires attention to students' identity development—the key developmental task of adolescence. Secondary science teachers participated in an 8-week course focused on understanding adolescent identity development and methods for addressing identity. Transcripts of the teachers' online discussions of salient issues were analyzed to determine their perceptions regarding classroom identity work. Teachers identified several assets and obstacles to identity work that were organized into two broad categories: teacher knowledge, training opportunities, and administrative support, or lack of these; and, presence of inflexible curricula, standardized testing regimes, and increased teacher accountability. Implications for student growth and science teacher professional development are discussed.

  8. JWST NIRCam WFSS Ice Feature Spectroscopy in Nearby Molecular Cores

    Science.gov (United States)

    Chu, Laurie; Hodapp, Klaus W.; Rieke, Marcia J.; Meyer, Michael; Greene, Thomas P.; JWST NIRCam Science Team

    2017-06-01

    In molecular clouds above a few magnitudes of total visual extinction, some components of the molecular gas freeze out on the surfaces of dust grains. These ice mantles around dust grains are the site of complex surface chemistry that leads to the formation of simple organic molecules in these mantles. The icy surfaces also facilitate the coaggulation of the dust particles, setting the stage for grain growth and ultimately the formation of planetary bodies.As part of the JWST NIRCam GTO program, we plan to observe a selection of small molecular cores using the wide field grism spectroscopy mode of NIRCam.This poster presents the results of a preliminary study of several candidate molecular cores using UKIRT, Spitzer IRAC, IRTF SpeX, Keck MOSFIRE and Subaru MOIRCS data.After the prelimary studies we have selected three molecular cores in different evolutionary stages for the GTO program: B68, a quiescent molecular core, LDN 694-2, a collapsing pre-stellar core, and B335, a protostellar core. All these cores are seen against a dense background of stars in the inner Galaxy and offer the opportunity for spatially well resolved mapping of the ice feature distribution. We will obtain slitless grism spectroscopy in six filters covering the features of H2O, CO2, CO, CH3OH, and the XCN feature. Simulations using aXeSIM have shown that spectrum overlap will occur in a fraction of the spectra, but will not be a prohibitive problem.Our poster will discuss the details of observations planned out in the APT system.

  9. Astrochemistry with the Mid-InfraRed Instrument on JWST

    Science.gov (United States)

    van Dishoeck, E. F.; Merín, B.; Brandl, B.; Böker, T.; Greene, T.; Meixner, M.; Ressler, M.; Rieke, G.; Waelkens, C.; Wright, G.; Miri Team

    JWST-MIRI will have imaging and medium resolution (λ/Δλ ≍ 2000-3000) integral field spectroscopy with orders of magnitude improvements in sensitivity and/or spatial resolution compared with existing facilities. It will be a prime facility for astrochemical studies of gases and solids in a wide variety of objects in the next decade. 1. Introduction Mid-infrared spectroscopy is becoming a powerful tool in astrochemistry, with studies of molecules and sources that are highly complementary to those at millimeter wavelengths. Molecules without permanent dipole moments such CH4, C2H2 and CO2 can only be observed through their vibration-rotation transitions. Space-based missions open up the possibility to study molecules which are abundant in ouw own atmosphere, in particular H2O. Polycyclic Aromatic Hydrocarbons have their most prominent features at mid-infrared wavelengths, and the pure rotational transitions of the dominant molecule in the universe, H2, also occur in this band. Solid-state material is uniquely probed in the mid-infrared, including characteric bands of ices, silicates, oxides, carbides, carbonates and sulfides. The wealth of mid-infrared spectroscopy has been demonstrated by results from the ISO satellite (see van Dishoeck & Tielens 2001, van Dishoeck 2004 for reviews), by pioneering ground-based studies (Lacy et al. 1989, Evans et al. 1990) and most recently by the Spitzer Space Telescope. Targets include molecular clouds, PDRs, shocks, deeply embedded young stellar objects, UC HII regions, protoplanetary disks, planetary atmospheres, comets, evolved stars and even entire galaxies. In addition to an inventory of gaseous and solid-state material, the lines and line ratios provide powerful diagnostics of temperatures, densities, UV field, elemental abundances, etc. Systematic variations in features from region to region allow the physical and chemical processes to be traced. The MidInfraRed Instrument (MIRI) on board the 6m James Webb Space

  10. Prospects for Habitable World Detections Using James Webb Space Telescope (JWST)

    Science.gov (United States)

    Deming, Drake

    2010-01-01

    Doppler and transit surveys are finding extrasolar planets of ever smaller mass and radius, and are now sampling the domain of superEarths. Recent results from the Doppler surveys suggest that discovery of a transiting superEarth in the habitable zone of a lower main sequence star may be possible. We evaluate the prospects for an all-sky transit survey targeted to the brightest stars I that would find the most favorable cases for photometric and spectroscopic characterization using the James Webb Space Telescope. We use the proposed Transiting Exoplanet Survey Satellite (TESS) as representative of an all-sky survey. We couple the simulated TESS yield to a sensitivity model for the MIRI and NIRSpec instruments on JWST. Our sensitivity model includes all currently known and anticipated sources of random and systematic error for these instruments. We focus on the TESS planets with radii between Earth and Neptune. Our simulations consider secondary eclipse filter photometry using JWST/MIRI, comparing the 11- and 15- micron bands to measure carbon dioxide absorption in superEarths, as well as JWST!NIRSpec spectroscopy of water absorption from 1.7-3.0 microns, and carbon dioxide absorption at 4.3 microns. We find that JWST will be capable of characterizing dozens of TESS superEarths with temperatures above the habitable range, using both MIRI and NIRspec. We project that TESS will discover about eight nearby habitable transiting superEarths, all orbiting lower main sequence stars. The principal sources of uncertainty in the prospects for JWST characterization of habitable superEarths are superEarth frequency and the nature of superEarth atmospheres. Based on our estimates of these uncertainties, we project that JWST will be able to measure the temperature, and identify molecular absorptions (water, carbon dioxide) in one to four nearby habitable TESS superEarths orbiting lower main sequence stars.

  11. The James Webb Space Telescope Integrated Science Instrument Module

    Science.gov (United States)

    Greenhouse, M. A.; Boyce, L. A.; Glazer, S. D.; Johnson, E. L.; McCloskey, J. C.; Sullivan, P. C.; Voyton, M. F.

    2005-12-01

    In this poster, we describe the major design features of the James Webb Space Telescope (JWST) Integrated Science Instrument Module (ISIM). The JWST mission is under development by NASA in partnership with the European and Canadian Space Agencies for launch during 2013. The JWST is designed to enable a five year science mission that is focused on four themes: [1] observation of the first luminous objects after the Big Bang, [2] the assembly of these objects into galaxies, [3] the birth of stars and planetary systems, and [4] the formation of planets and the origins of life. The above science themes require high sensitivity and HST-like angular resolution over the near- to mid-infrared spectrum. A 40 K cryogenic radiatively cooled telescope with a 25 m2 collecting area was selected to meet these requirments. A mission architecture involving a Lissajous orbit about the Earth-Sun L2 point was chosen to meet optical stability and data downlink requirments. A modular flight segment architecture was selected to enable incremental integration and test of the cryogenic payload. The ISIM is one key feature of this modular architecture that enables a feasible cryogenic test program. The ISIM element is the science instrument payload of the observatory. It contains 70 million infrared detector pixels allocated among four science instrument systems and a fine guidance sensor system. Brief instrument descriptions are available at: www.stsci.edu/jwst/docs/flyers. The ISIM also contains a passive 40 K thermal control system, a 6 K cryo-cooler system, a command and data handling system, a flight software system, and an optical metering structure system. The ISIM element is responsible for acquisition of the JWST science data, fine guidance data for telescope pointing control, and wavefront sensing data for in-flight adjustment of the telescope optics. Further information about the JWST mission is available at: www.jwst.nasa.gov.

  12. Habitable worlds with JWST: transit spectroscopy of the TRAPPIST-1 system?

    Science.gov (United States)

    Barstow, J. K.; Irwin, P. G. J.

    2016-09-01

    The recent discovery of three Earth-sized, potentially habitable planets around a nearby cool star, TRAPPIST-1, has provided three key targets for the upcoming James Webb Space Telescope (JWST). Depending on their atmospheric characteristics and precise orbit configurations, it is possible that any of the three planets may be in the liquid water habitable zone, meaning that they may be capable of supporting life. We find that present-day Earth levels of ozone, if present, would be detectable if JWST observes 60 transits for innermost planet 1b and 30 transits for 1c and 1d.

  13. Habitable worlds with JWST: transit spectroscopy of the TRAPPIST-1 system?

    CERN Document Server

    Barstow, Joanna K

    2016-01-01

    The recent discovery of three Earth-sized, potentially habitable planets around a nearby cool star, TRAPPIST-1, has provided three key targets for the upcoming James Webb Space Telescope (JWST). Depending on their atmospheric characteristics and precise orbit configurations, it is possible that any of the three planets may be in the liquid water habitable zone, meaning that they may be capable of supporting life. We find that present-day Earth levels of ozone, if present, would be detectable if JWST observes 60 transits for innermost planet 1b and 30 transits for 1c and 1d.

  14. Applying gene flow science to environmental policy needs: a boundary work perspective.

    Science.gov (United States)

    Ridley, Caroline E; Alexander, Laurie C

    2016-08-01

    One application of gene flow science is the policy arena. In this article, we describe two examples in which the topic of gene flow has entered into the U.S. national environmental policymaking process: regulation of genetically engineered crops and clarification of the jurisdictional scope of the Clean Water Act. We summarize both current scientific understanding and the legal context within which gene flow science has relevance. We also discuss the process by which scientific knowledge has been synthesized and communicated to decision-makers in these two contexts utilizing the concept of 'boundary work'. Boundary organizations, the work they engage in to bridge the worlds of science, policy, and practice, and the boundary objects they produce to translate scientific knowledge existed in both examples. However, the specific activities and attributes of the objects produced varied based on the needs of the decision-makers. We close with suggestions for how scientists can contribute to or engage in boundary work with policymakers.

  15. Fighting for life: Religion and science in the work of fish and wildlife biologists

    Science.gov (United States)

    Geffen, Joel Phillip

    Philosophers, historians, and sociologists of science have argued that it is impossible to separate fact from value. Even so, Americans generally demand that scientists be "objective." No bias is permitted in their work. Religious motivations in particular are widely considered anathema within the halls of science. My dissertation addresses both theoretical and practical aspects concerning objectivity in science through an examination of fish and wildlife biologists. I hypothesized that they use the language of objective science as a tool to convince others to protect habitats and species. Further, I claimed that this "rhetoric of science" is employed either consciously or unconsciously on behalf of personal values, and that religious and/or spiritual values figure significantly among these. Regarding the issue's practical applications, I argued in support of Susan Longino's assertion that while subjective influences exist in science, they do not necessarily indicate that objectivity has been sacrificed. My primary methodology is ethnographic. Thirty-five biologists working in the Pacific Northwest were interviewed during the course of summer 2001. Participant ages ranged from 23 to 78. Both genders were represented, as were various ethnic and cultural backgrounds, including Native American. I used a questionnaire to guide respondents through a consistent set of open-ended queries. I organized their answers under four categories: the true, the good, the beautiful, and the holy. The first three were borrowed from the theoretical writings of philosopher Immanuel Kant. The last came from Rudolf Otto's theological work. These categories provided an excellent analytical framework. I found that the great majority of fish and wildlife biologists strive for objectivity. However, they are also informed by powerful contextual values. These are derived from environmental ethics, aesthetic preferences pertaining to ecosystem appearance and function, and visceral experiences of

  16. Undergraduate honors students' images of science: Nature of scientific work and scientific knowledge

    Science.gov (United States)

    Wallace, Michael L.

    This exploratory study assessed the influence of an implicit, inquiry-oriented nature of science (NOS) instructional approach undertaken in an interdisciplinary college science course on undergraduate honor students' (UHS) understanding of the aspects of NOS for scientific work and scientific knowledge. In this study, the nature of scientific work concentrated upon the delineation of science from pseudoscience and the value scientists place on reproducibility. The nature of scientific knowledge concentrated upon how UHS view scientific theories and how they believe scientists utilize scientific theories in their research. The 39 UHS who participated in the study were non-science majors enrolled in a Honors College sponsored interdisciplinary science course where the instructors took an implicit NOS instructional approach. An open-ended assessment instrument, the UFO Scenario, was designed for the course and used to assess UHS' images of science at the beginning and end of the semester. The mixed-design study employed both qualitative and quantitative techniques to analyze the open-ended responses. The qualitative techniques of open and axial coding were utilized to find recurring themes within UHS' responses. McNemar's chi-square test for two dependent samples was used to identify whether any statistically significant changes occurred within responses from the beginning to the end of the semester. At the start of the study, the majority of UHS held mixed NOS views, but were able to accurately define what a scientific theory is and explicate how scientists utilize theories within scientific research. Postinstruction assessment indicated that UHS did not make significant gains in their understanding of the nature of scientific work or scientific knowledge and their overall images of science remained static. The results of the present study found implicit NOS instruction even with an extensive inquiry-oriented component was an ineffective approach for modifying UHS

  17. The Molecular Universe as seen by JWST-MIRI

    Science.gov (United States)

    Lahuis, F.; van Dishoeck, E. F.; Wright, G.; Rieke, G.

    2011-05-01

    The Mid-InfraRed Instrument (MIRI, Wright et al. 2003) on board the James Webb Space Telescope (JWST) will be the next major mid-infrared facility in space. It combines a high sensitivity with medium resolution spectroscopy and subarcsec imaging. This makes it one of the prime facilities for astrochemical studies in the next decade. Mid-infrared spectroscopy is a very powerful astrochemical tool. Molecules without permanent dipoles such as CH_4, C_2H_2 and CO_2 can only be observed through their vibration-rotation transitions while atmospheric species, in particular H_2O, require space-based facilities. PAH and solid-state material have prominent features in the mid-infrared, and the pure rotational transitions of the dominant molecule in the universe, H_2, also occur in this band. The wealth of mid-infrared spectroscopy has been demonstrated by results from the ISO satellite (see van Dishoeck 2004 for a review), pioneering ground-based studies and most recently by the Spitzer Space Telescope. The targeted sources are extremely diverse and include objects in the local and distant universe. Variations in features allow both qualitative and quantitative studies of physical and chemical processes. MIRI consists of an imager (including low resolution (R=λ/Δλ≈100) spectroscopy and coronography) and a medium resolution spectrometer (R=2000-3000) operating in the 5-28μm wavelength range using 1024x1024 pixel Si:As arrays. The spectrometer uses four IFUs with fields ranging from 3.5 to 7 arcsec. MIRIs sensitivity, orders of magnitude higher compared to Spitzer and 8-m class ground-based telescopes, spatial and spectral resolution make it particularly well suited for studying gases and solids in disks around young stars and in the nuclei of (starburst) galaxies. The sensitive low resolution spectrometer will be ideal to characterize exoplanet atmospheres. MIRI is built in partnership by a European Consortium and the US. The MIRI flight model (FM) is now fully

  18. Recovering the Properties of High-redshift Galaxies with Different JWST Broadband Filters

    DEFF Research Database (Denmark)

    Bisigello, L.; Caputi, K. I.; Colina, L.

    2017-01-01

    Imaging with the James Webb Space Telescope (JWST) will allow observations of the bulk of distant galaxies at the epoch of reionization. The recovery of their properties, such as age, color excess , specific star formation rate (sSFR), and stellar mass, will mostly rely on spectral energy distrib...

  19. Social and natural sciences differ in their research strategies, adapted to work for different knowledge landscapes.

    Science.gov (United States)

    Jaffe, Klaus

    2014-01-01

    Do different fields of knowledge require different research strategies? A numerical model exploring different virtual knowledge landscapes, revealed two diverging optimal search strategies. Trend following is maximized when the popularity of new discoveries determine the number of individuals researching it. This strategy works best when many researchers explore few large areas of knowledge. In contrast, individuals or small groups of researchers are better in discovering small bits of information in dispersed knowledge landscapes. Bibliometric data of scientific publications showed a continuous bipolar distribution of these strategies, ranging from natural sciences, with highly cited publications in journals containing a large number of articles, to the social sciences, with rarely cited publications in many journals containing a small number of articles. The natural sciences seem to adapt their research strategies to landscapes with large concentrated knowledge clusters, whereas social sciences seem to have adapted to search in landscapes with many small isolated knowledge clusters. Similar bipolar distributions were obtained when comparing levels of insularity estimated by indicators of international collaboration and levels of country-self citations: researchers in academic areas with many journals such as social sciences, arts and humanities, were the most isolated, and that was true in different regions of the world. The work shows that quantitative measures estimating differences between academic disciplines improve our understanding of different research strategies, eventually helping interdisciplinary research and may be also help improve science policies worldwide.

  20. The Impact of JWST Broadband Filter Choice on Photometric Redshift Estimation

    Science.gov (United States)

    Bisigello, L.; Caputi, K. I.; Colina, L.; Le Fèvre, O.; Nørgaard-Nielsen, H. U.; Pérez-González, P. G.; Pye, J.; van der Werf, P.; Ilbert, O.; Grogin, N.; Koekemoer, A.

    2016-12-01

    The determination of galaxy redshifts in the James Webb Space Telescope’s (JWST) blank-field surveys will mostly rely on photometric estimates, based on the data provided by JWST’s Near-Infrared Camera (NIRCam) at 0.6-5.0 μm and Mid Infrared Instrument (MIRI) at λ \\gt 5.0 μ {{m}}. In this work we analyze the impact of choosing different combinations of NIRCam and MIRI broadband filters (F070W to F770W), as well as having ancillary data at λ \\lt 0.6 μ {{m}}, on the derived photometric redshifts (z phot) of a total of 5921 real and simulated galaxies, with known input redshifts z = 0-10. We found that observations at λ \\lt 0.6 μ {{m}} are necessary to control the contamination of high-z samples by low-z interlopers. Adding MIRI (F560W and F770W) photometry to the NIRCam data mitigates the absence of ancillary observations at λ \\lt 0.6 μ {{m}} and improves the redshift estimation. At z = 7-10, accurate z phot can be obtained with the NIRCam broadbands alone when {{S}}/{{N}}≥slant 10, but the z phot quality significantly degrades at {{S}}/{{N}}≤slant 5. Adding MIRI photometry with 1 mag brighter depth than the NIRCam depth allows for a redshift recovery of 83%-99%, depending on spectral energy distribution type, and its effect is particularly noteworthy for galaxies with nebular emission. The vast majority of NIRCam galaxies with [F150W] = 29 AB mag at z = 7-10 will be detected with MIRI at [F560W, F770W] \\lt 28 mag if these sources are at least mildly evolved or have spectra with emission lines boosting the mid-infrared fluxes.

  1. The Impact of APU Science Work at LEA and School Levels.

    Science.gov (United States)

    Harlen, Wynne

    1984-01-01

    Questionnaires were sent to local education authorities in England to determine what the advisory/inspectorial staff and the working groups of teachers and schools know about the national assessments of science education conducted by the APU and how they were being used. (RM)

  2. Particle Physics as a way to bring different cultures to work together in Science

    CERN Document Server

    Mikenberg, G

    2016-01-01

    Science has traditionally played an important role in sharing knowledge among people. Particle Physics, with its large experiments, has shown that one not only can share the knowledge among different cultures, but that one can also work together to achieve this knowledge. The present article gives a few examples where this has been possible among people that are sometimes in conflict situations.

  3. 77 FR 31592 - Notice of Proposed Information Collection Requests; Institute of Education Sciences; What Works...

    Science.gov (United States)

    2012-05-29

    ... Notice of Proposed Information Collection Requests; Institute of Education Sciences; What Works..., Washington, DC 20202-4537. Copies of the proposed information collection request may be accessed from http.... When you access the information collection, click on ``Download Attachments'' to view. Written...

  4. Rómulo De Carvalho's Work on the Popularization of Science during Salazarism

    Science.gov (United States)

    Galamba, Arthur

    2013-01-01

    This article provides an account of Rómulo de Carvalho's most prominent works on the popularization of science during the Salazarist regime in Portugal. Carvalho has been praised for his "unique" writing style, for his uncommon ability to communicate scientific knowledge with clarity to a wide audience: he wrote to teachers, to secondary…

  5. Innovations in Community-Based and Interdisciplinary Research: A Network Perspective on Innovation in Social Work Science

    Science.gov (United States)

    Rice, Eric; Petering, Robin; Stringfellow, Erin; Craddock, Jaih B.

    2017-01-01

    We present a preliminary theory of innovation in social work science. The focus of the piece is two case studies from our work that illustrate the social nature of innovations in the science of social work. This inductive theory focuses on a concept we refer to as transformative innovation, wherein two sets of individuals who possess different…

  6. 77 FR 6796 - Notification of Three Public Teleconferences of a Work Group of the Chartered Science Advisory Board

    Science.gov (United States)

    2012-02-09

    ... AGENCY Notification of Three Public Teleconferences of a Work Group of the Chartered Science Advisory... Board (SAB) Staff Office announces three public teleconferences of a work group of the Chartered Science... EPA policy, notice is hereby given that a work group of the chartered SAB will hold three...

  7. Innovations in Community-Based and Interdisciplinary Research: A Network Perspective on Innovation in Social Work Science

    Science.gov (United States)

    Rice, Eric; Petering, Robin; Stringfellow, Erin; Craddock, Jaih B.

    2017-01-01

    We present a preliminary theory of innovation in social work science. The focus of the piece is two case studies from our work that illustrate the social nature of innovations in the science of social work. This inductive theory focuses on a concept we refer to as transformative innovation, wherein two sets of individuals who possess different…

  8. Alignment of the James Webb Space Telescope Integrated Science Instrument Module Element

    Science.gov (United States)

    Hadjimichael, Theo; Ohl, Raymond G.; Antonille, Scott; Aronstein, David L.; Bartoszyk, Andrew; Berrier, Josh; Cofie, Emmanuel; Coulter, Phil; Gracey, Renee; Hayden, Joseph; Howard, Joseph; Hylan, Jason; Kubalak, David; McLean, Kyle; Miskey, Cherie; Redman, Kevin; Rohrbach, Scott; Sabatke, Derek; Telfer, Randal; Wenzel, Greg; Zielinski, Thomas; Sullivan, Joseph; Hartig, George; Eichhorn, William

    2016-10-01

    NASA's James Webb Space Telescope (JWST) is a 6.6m diameter, segmented, deployable telescope for cryogenic IR space astronomy. The JWST Observatory architecture includes the Optical Telescope Element (OTE) and the Integrated Science Instrument Module (ISIM) element which contains four science instruments (SI), including a guider. The SIs and guider are mounted to a composite metering structure with outer envelope approximate measurements of 2.2x2.2x1.7m. These SI units are integrated to the ISIM structure and optically tested at NASA Goddard Space Flight Center as an instrument suite using an Optical telescope element SIMulator (OSIM). OSIM is a high-fidelity, cryogenic JWST simulator that features a 1.5m diameter powered mirror. The SIs are aligned to the flight structure's coordinate system under ambient, clean room conditions using opto-mechanical metrology and customized interfaces. OSIM is aligned to the ISIM mechanical coordinate system at the cryogenic operating temperature via internal mechanisms and feedback from alignment sensors and metrology in six degrees of freedom. SI performance, including focus, pupil shear, pupil roll, boresight, wavefront error, and image quality, is evaluated at the operating temperature using OSIM. This work reports on the as-run ambient assembly and ambient alignment steps for the flight ISIM, including SI interface fixtures and customization and kinematic mount adjustment. The ISIM alignment plan consists of multiple steps to meet the "absolute" alignment requirements of the SIs and OSIM to the flight coordinate system. In this paper, we focus on key aspects of absolute, optical-mechanical alignment. We discuss various metrology and alignment techniques. In addition, we summarize our approach for dealing with and the results of ground-test factors, such as gravity.

  9. Influences on Interdisciplinary Collaboration among Social Work and Health Sciences Students

    Directory of Open Access Journals (Sweden)

    Sang Jung Lee

    2014-10-01

    Full Text Available Interdisciplinary collaboration is an effective and satisfying way to provide health care services and learning across professions. This study aimed to explore interdisciplinary collaboration experiences amongst social work and allied health sciences graduate students and examined factors that contributed to their interdisciplinary collaboration. An interdisciplinary survey was conducted in a Mid-Atlantic public university. Analysis was conducted using hierarchical regressions from 112 health sciences and social work students. Students with positive attitudes toward interdisciplinary health care teams and part-time students compared to full-time students presented higher flexibility of interdisciplinary collaboration. Students with positive experiences of interdisciplinary collaboration demonstrated higher levels of interdependence, compared to those with no and negative experiences of interdisciplinary collaboration. Students in medicine were less likely to show interdependence, compared to those in social work. Professional disciplines and educators should put efforts in offering opportunities for interdisciplinary collaboration practice and building curricula to promote positive attitudes toward interdisciplinary teamwork.

  10. The Complex Tasks Using for Practical Work in the Study of Computer Science in High School

    Directory of Open Access Journals (Sweden)

    Nelya V. Degtyareva

    2014-06-01

    Full Text Available In this article discusses methods for diagnosing of training results of high school students in the study of computer science. The author highlights the positive aspects of some methods of diagnosing anddiscusses the need for combining tasks in the practical work: testing, integrative tasks and tasks of competency-based. The author argues that testing helps to master the theoretical foundations of computer science, practical exercise promotes the development of skills of used information technology, the creative task stimulates intellectual activity and an unconventional approach to solving. The author gives an example of the practical work for the study of spreadsheets. In practical work demonstrates the testing and use of various types of tests in more detail. This article describes the results of a survey of teachers and students about objective method of diagnostics of knowledge. There is a study of the formation of IT-competencies and core competencies while performing tasks such.

  11. Optical Modeling Activities for NASA's James Webb Space Telescope (JWST). 4; Overview and Introduction of Matlab Based Toolkits used to Interface with Optical Design Software

    Science.gov (United States)

    Howard, Joseph

    2007-01-01

    This is part four of a series on the ongoing optical modeling activities for James Webb Space Telescope (JWST). The first two discussed modeling JWST on-orbit performance using wavefront sensitivities to predict line of sight motion induced blur, and stability during thermal transients. The third investigates the aberrations resulting from alignment and figure compensation of the controllable degrees of freedom (primary and secondary mirrors), which may be encountered during ground alignment and on-orbit commissioning of the observatory. The work here introduces some of the math software tools used to perform the work of the previous three papers of this series. NASA has recently approved these in-house tools for public release as open source, so this presentation also serves as a quick tutorial on their use. The tools are collections of functions written in Matlab, which interface with optical design software (CodeV, OSLO, and Zemax) using either COM or DDE communication protocol. The functions are discussed, and examples are given.

  12. Next Generation Very Large Array Memo No. 6, Science Working Group 1: The Cradle of Life

    CERN Document Server

    Isella, Andrea; Moullet, Arielle; Galván-Madrid, Roberto; Johnstone, Doug; Ricci, Luca; Tobin, John; Testi, Leonardo; Beltran, Maite; Lazio, Joseph; Siemion, Andrew; Liu, Hauyu Baobab; Du, Fujun; Öberg, Karin I; Bergin, Ted; Caselli, Paola; Bourke, Tyler; Carilli, Chris; Perez, Laura; Butler, Bryan; de Pater, Imke; Qi, Chunhua; Hofstadter, Mark; Moreno, Raphael; Alexander, David; Williams, Jonathan; Goldsmith, Paul; Wyatt, Mark; Loinard, Laurent; Di Francesco, James; Wilner, David; Schilke, Peter; Ginsburg, Adam; Sánchez-Monge, Álvaro; Zhang, Qizhou; Beuther, Henrik

    2015-01-01

    This paper discusses compelling science cases for a future long-baseline interferometer operating at millimeter and centimeter wavelengths, like the proposed Next Generation Vary Large Array (ngVLA). We report on the activities of the Cradle of Life science working group, which focused on the formation of low- and high-mass stars, the formation of planets and evolution of protoplanetary disks, the physical and compositional study of Solar System bodies, and the possible detection of radio signals from extraterrestrial civilizations. We propose 19 scientific projects based on the current specification of the ngVLA. Five of them are highlighted as possible Key Science Projects: (1) Resolving the density structure and dynamics of the youngest HII regions and high-mass protostellar jets, (2) Unveiling binary/multiple protostars at higher resolution, (3) Mapping planet formation regions in nearby disks on scales down to 1 AU, (4) Studying the formation of complex molecules, and (5) Deep atmospheric mapping of gian...

  13. What Does It Take for Social Work to Evolve to Science Status? Discussing Definition, Structure, and Contextual Challenges and Opportunities

    Science.gov (United States)

    Guerrero, Erick G.

    2014-01-01

    The emerging discourse on science in social work (SW) has generated much-needed analysis of the profession's status as a scientific enterprise. Brekke raised critical issues that must be addressed for SW to become a science. This response examines the contextual factors that led to the call for SW science. It also relies on a comparative…

  14. The fate of a progressive science: the Harvard Fatigue Laboratory, athletes, the science of work and the politics of reform.

    Science.gov (United States)

    Scheffler, Robin Wolfe

    2011-06-01

    In the early twentieth century, fatigue research marked a site of conflicting scientific, industrial, and cultural understandings of working bodies. Many fatigue researchers understood fatigue to be a physiological fact and allied themselves with Progressive-era reformers in urging industrial regulation. Reformers clashed with advocates of Taylorism, who held that productivity could be perpetually increased through managerial efficiency. Histories of this conflict typically cease with the end of the First World War. I examine the work of the Harvard Fatigue Laboratory in the 1920s and 1930s to explore the impact that the introduction of biochemical methods had on the relationship between science and reform. The Laboratory developed sophisticated techniques to study the blood of exercising individuals. In particular, it found that exercising individuals could attain a biochemically "steady state," or equilibrium, and extrapolated from this to assert that fatigue was psychological, not physiological, in nature. In contrast to Progressive-era research, the Laboratory reached this conclusion through laboratory examination, not of workers, but of Laboratory staff members and champion marathon runners. I present the Laboratory's institutional history, scientific work, and finally how common cultural understandings of athletes and work lent plausibility to its efforts to make authoritative statements about industrial conditions.

  15. Rómulo de Carvalho's Work on the Popularization of Science During Salazarism

    Science.gov (United States)

    Galamba, Arthur

    2013-10-01

    This article provides an account of Rómulo de Carvalho's most prominent works on the popularization of science during the Salazarist regime in Portugal. Carvalho has been praised for his `unique' writing style, for his uncommon ability to communicate scientific knowledge with clarity to a wide audience: he wrote to teachers, to secondary students, to the layman and even to the rural peasantry. Most of his books and articles on popularization explored the History and Philosophy of Science, and it has been claimed that he influenced many youngsters to pursue scientific careers. Given the repressive political context imposed by Salazarism, it is argued that Carvalho's work on the popularization of science had a humanist and libertarian connotation. However, intriguingly, different from some of his contemporaries who also promoted humanistic education for all, Carvalho was never targeted by the Dictatorship. The article seeks to shed light on this matter. It points out the educational reach of Carvalho's writings and suggests that popularization of science in repressive regimes is not necessarily a problematic issue as long as it does not threat the status quo.

  16. [The CSI effect and its impact on the perceptions of forensic science experts' work].

    Science.gov (United States)

    Stojer, Joanna

    2011-01-01

    The issue that has been analyzed in this work is the potential effect of crime films and TV series on people's perceptions of forensic medicine and science, and especially on the forming of expectations towards forensic science experts. This syndrome is being called the "CSI effect" after the popular franchise Crime Scene Investigation (CSI). Questionnaire surveys that have been conducted included "experts": 50 experts in various specialities, 77 prosecutors, 119 judges, 64 lay judges, 161 police staff and 80 members of general public. In-depth interviews have been conducted with 20 police staff, and also a focus group has been carried out with 15 law students. In the opinion of the respondents, people's perceptions and expectations of forensic science--as it can be observed during criminal trials--are largely inflated by the entertainment media. Among the surveyed persons, the category that declares watching crime series most rarely, is forensic science experts. Around half of the surveyed experts pointed out to excessive expectations towards they work instigated by TV crime series. The most common expectations towards forensic medicine experts are: immediate conclusiveness of post mortem examinations (going as far as indicating the cause of death at the crime scene), precision of death time estimation and a routine use of sophisticated methods known from TV.

  17. Education of natural science in the work of the Municipal Center for Extracurricular Activities

    Science.gov (United States)

    Jokin, I.

    2012-04-01

    In the description of my work I presented my own experience in the organizing and carrying out of extracurricular activities with the students, the used modes and methods of work, the obtained results and some good practices in the field of natural sciences. Organizing and carrying out of scientific festivals, participation in joint projects together with scientific organizations. Key words: European dimension, interactive methods, key competences, natural sciences, extracurricular activities. We are witnesses of a fundamental change in the pedagogical culture and practice in our schools to establish the parameters of the quality of training. The good scientific culture is an important part of the students' education. Unfortunately, at the present time the scientific and technological culture is on a low level. One of the contemporary problems and realities of the education in natural science school subjects, as a whole and in particular in the secondary education, is the decreased interest for the training in them and in particular in physics, as well as synchronization of the interrelations: school environment - society. In many countries there is a drop in the orientation of the students towards the science and technology - the problem of Science and Technology (S&T). The training of the young people often creates some problems. The teachers meet with the problem of insufficient motivation of the learners for study and difficulties that they encounter in the process of training. The students find it difficult to apply the mastered knowledge to an applied context. The knowledge is rather academic and rather remote from the context, in which the children live and communicate, which makes it nonfunctional. At present there are not enough extracurricular activities that should meet these necessities of the Bulgarian school. The reasons are various, but they mainly consist in the lack of a material base, an exchange of experience and good practices and motivation

  18. A Response to Anastas and Coffey: The Science of Social Work and Its Relationship to Social Work Education and Professional Organizations

    Science.gov (United States)

    Voisin, Dexter R.; Wong, Marleen; Samuels, Gina Miranda

    2014-01-01

    Relationships are central to the profession of social work; relationships with allied disciplines, among professional social work organizations, and between classroom and field education. However, embedded within these relationships are historical tensions, and contemporary opportunities that can advance both the science of social work and the…

  19. The James Webb Space Telescope and its Potential for Exoplanet Science

    Science.gov (United States)

    Clampin, Mark

    2008-01-01

    The James Webb Space Telescope (JWST) is a large aperture (6.5 meter), cryogenic space telescope with a suite of near and mid-infrared instruments covering the wavelength range of 0.6 microns to 28 microns. JWST s primary science goal is to detect and characterize the first galaxies. It will also study the assembly of galaxies, star formation, and the formation of evolution of planetary systems. Recent progress in hardware development for the observatory will be presented, including a discussion of the status of JWST s optical system and Beryllium mirror fabrication, progress with sunshield prototypes, and recent changes in the integration and test configuration. We also review the expected scientific performance of the observatory for observations of exosolar planets by means of transit imaging and spectroscopy and direct imaging. We also review the recent discovery of Fomalhaut B and implications for debris disk imaging nd exoplanet detection with JWST.

  20. Taking hermeneutics to science: Prospects and tactics suggested by the work of B. F. Skinner

    OpenAIRE

    Miller, Harold L.

    1994-01-01

    Skinner's contributions to the understanding of behavior are typically viewed as being in sufficiently tight alignment with traditional science to prevent their amenability to alternative discourses such as hermeneutics. However, it is possible to identify several concepts at work in radical behaviorism that might constitute its common ground with hermeneutics. The coextensiveness of individual and environment, the emphasis on contingency, and the interminableness of conversation promised by ...

  1. Anania Shirakatsi's Cosmographical Works and the Methodology of his Natural Science

    Science.gov (United States)

    Harutyunian, H. A.; Mickaelian, A. M.

    2014-10-01

    A review of Anania Shirakatsi's cosmographical works and the methodology of his natural science is given. It is based mainly on Shirakatsi's "Cosmography", which is based on the achievements of Greek astronomy, its further transformations and Shirakatsi's own observations. Individual parts of the book, such as "About the sky", "About the Earth", "About the heavenly bodies", "About the Milky Way", "About the Moon", and "About the Sun" are discussed.

  2. Observing transiting planets with JWST -- Prime targets and their synthetic spectral observations

    CERN Document Server

    Mollière, Paul; Bouwman, Jeroen; Henning, Thomas; Lagage, Pierre-Olivier; Min, Michiel

    2016-01-01

    The James Webb Space Telescope will enable astronomers to obtain exoplanet spectra of unprecedented precision. Especially the MIRI instrument may shed light on the nature of the cloud particles obscuring planetary transmission spectra in the optical and near-infrared. We provide self-consistent atmospheric models and synthetic JWST observations for prime exoplanet targets in order to identify spectral regions of interest and estimate the number of transits needed to distinguish between model setups. We select targets which span a wide range in planetary temperature and surface gravity, ranging from super-Earths to giant planets, and have a high expected SNR. For all targets we vary the enrichment, C/O ratio, presence of optical absorbers (TiO/VO) and cloud treatment. We calculate atmospheric structures and emission and transmission spectra for all targets and use a radiometric model to obtain simulated observations. We analyze JWST's ability to distinguish between various scenarios. We find that in very cloud...

  3. Exploring Biases of Atmospheric Retrievals in Simulated JWST Transmission Spectra of Hot Jupiters

    CERN Document Server

    Rocchetto, M; Venot, O; Lagage, P -O; Tinetti, G

    2016-01-01

    With a scheduled launch in October 2018, the James Webb Space Telescope (JWST) is expected to revolutionise the field of atmospheric characterization of exoplanets. The broad wavelength coverage and high sensitivity of its instruments will allow us to extract far more information from exoplanet spectra than what has been possible with current observations. In this paper, we investigate whether current retrieval methods will still be valid in the era of JWST, exploring common approximations used when retrieving transmission spectra of hot Jupiters. To assess biases, we use 1D photochemical models to simulate typical hot Jupiter cloud-free atmospheres and generate synthetic observations for a range of carbon-to-oxygen ratios. Then, we retrieve these spectra using TauREx, a Bayesian retrieval tool, using two methodologies: one assuming an isothermal atmosphere, and one assuming a parametrized temperature profile. Both methods assume constant-with-altitude abundances. We found that the isothermal approximation bi...

  4. Observing Resolved Stellar Populations with the JWST Near-Infrared Spectrograph

    Science.gov (United States)

    Gilbert, K. M.; Beck, T. L.; Karakla, D. M.

    2016-10-01

    The James Webb Space Telescope's (JWST) Near Infrared Spectrograph (NIRSpec) will provide a multi-object spectroscopy (MOS) mode through the Micro-Shutter Array (MSA). Each MSA quadrant is a grid of contiguous shutters that can be configured to form slits on more than 100 astronomical targets simultaneously. The combination of JWST's sensitivity and superb resolution in the infrared and NIRSpec's full wavelength coverage over 0.6 to 5 μm will open new parameter space for studies of galaxies and resolved stellar populations alike. We describe a NIRSpec MSA observing scenario of spectroscopy of individual stars in an external galaxy, and investigate the technical challenges posed by this scenario. This use case and others, including a deep galaxy survey and observations of Galactic HII regions, are guiding development of the NIRSpec user interfaces including proposal planning and pipeline calibrations.

  5. How to Teach High-School Students "How Science Really Works?"

    Science.gov (United States)

    Losiak, Anna; Students, High-School; Winiarska, Anna; Parys-Wasylkiewicz, Magdalena

    2016-04-01

    One of the largest problems in Poland (as well as in the large part of the developed world) is that people do not understand how science works. Based on what they learned at school, they think that science is an aggregation of facts that you need to learn by heart. Based on media coverage of the science topics, they think it is a collection of curiosities about the two-headed-snakes. Based on the way in which science is shown in movies and TV series, they envision science as a magic performed in a white coat with usage of colorful fluids and magic spells such as "transformative hermeneutics of quantum gravity". As a result, our societies include a large number of people who "do not believe" in evolution, think that vaccinations are causing autism and that anthropogenic global warming is a myth. This is not very surprising, given that most people never had a chance to perform a real scientific experiment. Most of people, if they are lucky, are able to see some science demonstrations in the classrooms. They are of course very useful, but it is quite clear for everyone that (if everything goes well) the demonstration can end up in one, pre-defined way. The "real" scientific experiment, as a part of the scientific process, is when the outcome is unknown until the end of the entire process. In order to teach high-school students "How Science Really Works" we have developed a project lasting one year (grant from Foundation for Polish Science 26/UD/SKILLS/2015): 1) At first students learned about scientific method, science history and performed a simple scientific experiment. 2) Later, students developed an experiment that was answering a real, unanswered scientific problem (the problem was given by the Leading Scientist). The aim of the project was to determine influence of albedo and emissivity of rock particles laying on a surface of a glacier on the rate of cryoconite holes formation. The results of this experiment can be used to better determine the rate of melting

  6. Organizational Climate and Work Addiction in Shahid Sadoughi University of Medical Sciences, 2014: a Case Study.

    Science.gov (United States)

    Rafiee, Noora; Bahrami, Mohammad Amin; Zare, Vahid; Mohammadi, Mahan

    2015-12-01

    The occupational nature of employees in headquarters units of the University requires them to deal with support issues. Thus, there is some pressure on these employees to complete their assignments on time so that employees in the line units can accurately and expeditiously perform their duties. As a result, work addiction behaviors are sometimes observed among the headquarters personnel. Considering the importance of work addiction and recognizing the factors that intensify it, this study investigated the relationship between organizational climate and the work addiction of headquarters personnel at the Shahid Sadoughi University of Medical Sciences. This descriptive-analytic study was conducted using stratified random sampling of 151 University employees in 2014. The data collection tool was an organizational climate questionnaire, which was supplemented by the Work Addiction Risk Test (WART). The data were analyzed using the Pearson test, Spearman test, independent t-test, Mann-Whitney test, one-way analysis of variance (ANOVA), and the Kruskal-Wallis test using IBM-SPSS version 20. The findings of this study showed that the organizational climate was at a moderate level, and employees were in the danger level in terms of work addiction. In addition, among the dimensions of organizational climate, the risk dimension had a significant relationship with work addiction (porganizational climate score was low and the work addiction score was at the high-risk level, this issue demands more attention of senior managers and human resource officers of organizations to improve the organizational climate and increase employees' awareness of work addiction.

  7. Science with KRAKENS

    CERN Document Server

    Mazin, Benjamin A; France, Kevin; Fraser, Wesley; Howell, D Andrew; Jones, Tucker; Meeker, Seth; O'Brien, Kieran; Prochaska, Jason X; Siana, Brian; Strader, Matthew; Szypryt, Paul; Tendulkar, Shriharsh P; Treu, Tommaso; Vasisht, Gautam

    2015-01-01

    The Keck science community is entering an era of unprecedented change. Powerful new instrument like ZTF, JWST, LSST, and the ELTs will catalyze this change, and we must be ready to take full advantage to maintain our position of scientific leadership. The best way to do this is to continue the UC and Caltech tradition of technical excellence in instrumentation. In this whitepaper we describe a new instrument called KRAKENS to help meet these challenges. KRAKENS uses a unique detector technology (MKIDs) to enable groundbreaking science across a wide range of astrophysical research topics. This document will lay out the detailed expected science return of KRAKENS.

  8. Follow-up and characterization of the TESS exoplanets with SOPHIE, SPIRou, and JWST

    Science.gov (United States)

    Crouzet, N.; Bonfils, X.; Delfosse, X.; Boisse, I.; Hébrard, G.; Forveille, T.; Donati, J.-F.; Bouchy, F.; Moutou, C.; Doyon, R.; Artigau, E.; Albert, L.; Malo, L.; Lecavelier des Etangs, A.; Santerne, A.; Author2, J.-P.; Author3, C. E.

    2016-12-01

    The NASA TESS mission will deliver hundreds of transiting exoplanet candidates orbiting bright stars. The spectrometers SOPHIE at OHP and SPIRou at CFHT will be ideal to obtain radial velocities of these candidates, confirm their nature, and derive the planets' masses. These measurements will be crucial to deliver the best targets for atmospheric characterization with JWST. Here, we calculate the required observing time with SOPHIE, SPIRou, and JWST for each of the TESS targets in order to prepare follow-up observations. To infer their potential for JWST, we restrict the calculations to the case of transmission spectroscopy with NIRISS. The radial velocity follow-up of the giant planets (R_p > 4 R_E) could be achieved with SOPHIE, with a median observing time of 3.47 hours per target, and a total observing time of 305 hours that includes the 80% most favorable cases. Several small planets (R_p R_E) could also be confirmed, but most of them would require an unrealistic time investment. On the other hand, SPIRou is ideally suited to the follow-up of the small planets, with a median observing time of 2.65 hours per target, and a median observing time of 4.70 hours for the terrestrial planets in the habitable zone (R_p R_E, S programs with SOPHIE and SPIRou before the first planet candidates are delivered by TESS.

  9. Electronic speckle pattern interferometric testing of JWST primary mirror segment assembly

    Science.gov (United States)

    Smith, Koby Z.; Chaney, David M.; Saif, Babak N.

    2011-09-01

    The James Webb Space Telescope (JWST) Primary Mirror Segment Assembly (PMSA) was required to meet NASA Technology Readiness Level (TRL) 06 requirements in the summer of 2006. These TRL06 requirements included verifying all mirror technology systems level readiness in simulated end-to-end operating conditions. In order to support the aggressive development and technology readiness schedule for the JWST Primary Mirror Segment Assembly (PMSA), a novel approach was implemented to verify the nanometer surface figure distortion effects on an in-process non-polished beryllium mirror surface. At the time that the TRL06 requirements needed to be met, a polished mirror segment had not yet been produced that could have utilized the baselined interferometric optical test station. The only JWST mirror segment available was a finished machined segment with an acid-etched optical surface. Therefore an Electronic Speckle Pattern Interferometer (ESPI) was used in coordination with additional metrology techniques to perform interferometric level optical testing on a non-optical surface. An accelerated, rigorous certification program was quickly developed for the ESPI to be used with the unfinished optical surface of the primary mirror segment. The ESPI was quickly implemented into the PMSA test program and optical testing was very successful in quantifying the nanometer level surface figure deformation changes in the PMSA due to assembly, thermal cycling, vibration, and acoustic testing. As a result of the successful testing, the PMSA passed all NASA TRL06 readiness requirements.

  10. Student Work Products as a Teaching Tool for Nature of Science Pedagogical Knowledge: A Professional Development Project with In-Service Secondary Science Teachers

    Science.gov (United States)

    Burton, Erin Peters

    2013-01-01

    The purpose was to examine NOS knowledge and pedagogical content knowledge about NOS of in-service secondary science teachers. Data sources included Views of Science and Education scale, lesson plans with rationales for choices, examples of student work products, videotapes of lesson peer reviews, and interviews conducted after the experience.…

  11. Individual to collaborative: guided group work and the role of teachers in junior secondary science classrooms

    Science.gov (United States)

    Fung, Dennis; Lui, Wai-mei

    2016-05-01

    This paper, through discussion of a teaching intervention at two secondary schools in Hong Kong, demonstrates the learning advancement brought about by group work and dissects the facilitating role of teachers in collaborative discussions. One-hundred and fifty-two Secondary Two (Grade 8) students were divided into three pedagogical groups, namely 'whole-class teaching', 'self-directed group work' and 'teacher-supported group work' groups, and engaged in peer-review, team debate, group presentation and reflection tasks related to a junior secondary science topic (i.e. current electricity). Pre- and post-tests were performed to evaluate students' scientific conceptions, alongside collected written responses and audio-recorded discussions. The results indicate that students achieved greater cognitive growth when they engaged in cooperative learning activities, the interactive and multi-sided argumentative nature of which is considered to apply particularly well to science education and Vygotsky's zone of proximal development framework. Group work learning is also found to be most effective when teachers play a role in navigating students during the joint construction of conceptual knowledge.

  12. Using science and psychology to improve the dissemination and evaluation of scientific work.

    Science.gov (United States)

    Buttliere, Brett T

    2014-01-01

    Here I outline some of what science can tell us about the problems in psychological publishing and how to best address those problems. First, the motivation behind questionable research practices is examined (the desire to get ahead or, at least, not fall behind). Next, behavior modification strategies are discussed, pointing out that reward works better than punishment. Humans are utility seekers and the implementation of current change initiatives is hindered by high initial buy-in costs and insufficient expected utility. Open science tools interested in improving science should team up, to increase utility while lowering the cost and risk associated with engagement. The best way to realign individual and group motives will probably be to create one, centralized, easy to use, platform, with a profile, a feed of targeted science stories based upon previous system interaction, a sophisticated (public) discussion section, and impact metrics which use the associated data. These measures encourage high quality review and other prosocial activities while inhibiting self-serving behavior. Some advantages of centrally digitizing communications are outlined, including ways the data could be used to improve the peer review process. Most generally, it seems that decisions about change design and implementation should be theory and data driven.

  13. A Review of Filovirus Work and Facilities at The Defence Science and Technology Laboratory Porton Down

    Directory of Open Access Journals (Sweden)

    Mark S. Lever

    2012-08-01

    Full Text Available Porton Down houses two separate sites capable of conducting high containment research on ACDP (Advisory Committee on Dangerous Pathogens Hazard Group 4 agents: the Defence Science and Technology Laboratory (Dstl and the Health Protection Agency (HPA, and filovirus research has been performed at Porton Down since the first Marburg virus disease outbreak in 1967. All work is conducted within primary containment either within cabinet lines (for in vitro work or large rigid half-suit isolators (for in vivo work. There are extensive aerobiological facilities at high containment and the use of these facilities will be reported. Research at Dstl is primarily focused on assessing and quantifying the hazard, and testing the efficacy of medical countermeasures against filoviruses. Fundamental research directed to the study and understanding of the infectious and pathogenic nature of the filoviruses, particularly in aerosols, will be reported.

  14. The James Webb Space Telescope: Capabilities for Exoplanet Science

    Science.gov (United States)

    Clampin, Mark

    2011-01-01

    The James Webb Space Telescope (JWST) is a large aperture (6.5 meter), cryogenic space telescope with a suite of near and mid-infrared instruments covering the wavelength range of 0.6 micron to 28 micron. JWST's primary science goal is to detect and characterize the first galaxies. It will also study the assembly of galaxies, stellar and planetary system formation, and the formation and evolution of planetary systems. We will review the design of JWST, and discuss the current status of the project, with emphasis on recent progress in the construction of the observatory. We also review the capabilities of the observatory for observations of exosolar planets and debris disks by means of coronagraphic imaging, and high contrast imaging and spectroscopy. This discussion will focus on the optical and thermal performance of the observatory, and will include the current predictions for the performance of the observatory, with special reference to the demands of exoplanet science observations.

  15. Status report on the land processes aircraft science management operations working group

    Science.gov (United States)

    Lawless, James G.; Mann, Lisa J.

    1991-01-01

    Since its inception three years ago, the Land Processes Aircraft Science Management Operations Working Group (MOWG) provided recommendations on the optimal use of the Agency's aircraft in support of the Land Processes Science Program. Recommendations covered topics such as aircraft and sensor usage, development of long-range plans, Multisensor Airborne Campaigns (MAC), program balance, aircraft sensor databases, new technology and sensor development, and increased University scientist participation in the program. Impacts of these recommendations improved the efficiency of various procedures including the flight request process, tracking of flight hours, and aircraft usage. The group also created a bibliography focused on publications produced by Land Processes scientists from the use of the aircraft program, surveyed NASA funded PI's on their participation in the aircraft program, and developed a planning template for multi-sensor airborne campaigns. Benefits from these activities are summarized.

  16. General experiences + race + racism = Work lives of Black faculty in postsecondary science education

    Science.gov (United States)

    Parsons, Eileen R. C.; Bulls, Domonique L.; Freeman, Tonjua B.; Butler, Malcolm B.; Atwater, Mary M.

    2016-12-01

    Existent research indicates that postsecondary Black faculty members, who are sorely underrepresented in the academy especially in STEM fields, assume essential roles; chief among these roles is diversifying higher education. Their recruitment and retention become more challenging in light of research findings on work life for postsecondary faculty. Research has shown that postsecondary faculty members in general have become increasingly stressed and job satisfaction has declined with dissatisfaction with endeavors and work overload cited as major stressors. In addition to the stresses managed by higher education faculty at large, Black faculty must navigate diversity-related challenges. Illuminating and understanding their experiences can be instrumental in lessening stress and job dissatisfaction, outcomes that facilitate recruitment and retention. This study featured the experiences and perceptions of Black faculty in science education. This study, framed by critical race theory, examines two questions: What characterizes the work life of some Black faculty members who teach, research, and serve in science education? How are race and racism present in the experiences of these postsecondary Black faculty members? A phenomenological approach to the study situates the experiences of the Black participants as valid phenomena worthy of investigation, illuminates their experiences, and seeks to retain the authenticity of their voices.

  17. Great Explorations in Math and Science[R] (GEMS[R]) Space Science. What Works Clearinghouse Intervention Report

    Science.gov (United States)

    What Works Clearinghouse, 2012

    2012-01-01

    "Great Explorations in Math and Science[R] (GEMS[R]) Space Science" is an instructional sequence for grades 3-5 that covers fundamental concepts, including planetary sizes and distance, the Earth's shape and movement, gravity, and moon phases and eclipses. Part of the "GEMS"[R] core curriculum, "GEMS[R] Space Science"…

  18. Primary Science: The Views of Teachers and Pupils. Learning in Science Project (Primary). Working Paper No. 102.

    Science.gov (United States)

    Biddulph, Fred

    The first (exploratory) phase of the Learning in Science Project (Primary)--LISP(P)--focused on science teaching/learning in New Zealand primary schools. Project goals included the identification of major problems of classroom teaching and learning and the study of factors which promote or limit individual children's learning of science. This…

  19. The advent of canine performance science: offering a sustainable future for working dogs.

    Science.gov (United States)

    Cobb, Mia; Branson, Nick; McGreevy, Paul; Lill, Alan; Bennett, Pauleen

    2015-01-01

    Working and sporting dogs provide an essential contribution to many industries worldwide. The common development, maintenance and disposal of working and sporting dogs can be considered in the same way as other animal production systems. The process of 'production' involves genetic selection, puppy rearing, recruitment and assessment, training, housing and handling, handler education, health and working life end-point management. At present, inefficiencies throughout the production process result in a high failure rate of dogs attaining operational status. This level of wastage would be condemned in other animal production industries for economic reasons and has significant implications for dog welfare, as well as public perceptions of dog-based industries. Standards of acceptable animal use are changing and some historically common uses of animals are no longer publicly acceptable, especially where harm is caused for purposes deemed trivial, or where alternatives exist. Public scrutiny of animal use appears likely to increase and extend to all roles of animals, including working and sporting dogs. Production system processes therefore need to be transparent, traceable and ethically acceptable for animal use to be sustainable into the future. Evidence-based approaches already inform best practice in fields as diverse as agriculture and human athletic performance. This article introduces the nascent discipline of canine performance science, which aims to facilitate optimal product quality and production efficiency, while also assuring evidence-based increments in dog welfare through a process of research and development. Our thesis is that the model of canine performance science offers an objective, transparent and traceable opportunity for industry development in line with community expectations and underpins a sustainable future for working dogs. This article is part of a Special Issue entitled: Canine Behavior.

  20. Exploring new ways of working using virtual research environments in library and information science

    DEFF Research Database (Denmark)

    Sonnenwald, Diane H.; Lassi, Monica; Olson, Nasrine

    2009-01-01

    Purpose: The purpose of this paper is to present current and ongoing research investigating new ways of working across geographic distances and time within library and information science (LIS). Design/methodology/approach: A total of four studies were conducted focusing on: the design of a virtual...... research environment (VRE) to facilitate the sharing of data collection instruments among students, researchers and professionals; new ways professionals and researchers can collaborate; collaborative decision making in the context of purchasing a library management system; and collaboration among LIS...

  1. Exploring new ways of working using virtual research environments in library and information science

    DEFF Research Database (Denmark)

    Sonnenwald, Diane H.; Lassi, Monica; Olson, Nasrine

    2009-01-01

    Purpose: The purpose of this paper is to present current and ongoing research investigating new ways of working across geographic distances and time within library and information science (LIS). Design/methodology/approach: A total of four studies were conducted focusing on: the design of a virtual...... research environment (VRE) to facilitate the sharing of data collection instruments among students, researchers and professionals; new ways professionals and researchers can collaborate; collaborative decision making in the context of purchasing a library management system; and collaboration among LIS...

  2. Organizational Climate and Work Addiction in Shahid Sadoughi University of Medical Sciences, 2014: a Case Study

    Science.gov (United States)

    Rafiee, Noora; Bahrami, Mohammad Amin; Zare, Vahid; Mohammadi, Mahan

    2015-01-01

    Introduction The occupational nature of employees in headquarters units of the University requires them to deal with support issues. Thus, there is some pressure on these employees to complete their assignments on time so that employees in the line units can accurately and expeditiously perform their duties. As a result, work addiction behaviors are sometimes observed among the headquarters personnel. Considering the importance of work addiction and recognizing the factors that intensify it, this study investigated the relationship between organizational climate and the work addiction of headquarters personnel at the Shahid Sadoughi University of Medical Sciences. Methods This descriptive-analytic study was conducted using stratified random sampling of 151 University employees in 2014. The data collection tool was an organizational climate questionnaire, which was supplemented by the Work Addiction Risk Test (WART). The data were analyzed using the Pearson test, Spearman test, independent t-test, Mann-Whitney test, one-way analysis of variance (ANOVA), and the Kruskal-Wallis test using IBM-SPSS version 20. Results The findings of this study showed that the organizational climate was at a moderate level, and employees were in the danger level in terms of work addiction. In addition, among the dimensions of organizational climate, the risk dimension had a significant relationship with work addiction (porganizational climate score was low and the work addiction score was at the high-risk level, this issue demands more attention of senior managers and human resource officers of organizations to improve the organizational climate and increase employees’ awareness of work addiction. PMID:26816586

  3. Getting Data Should be Easy! Working with NASA to Improve Earth Science Data Accessibility with Metadata

    Science.gov (United States)

    le Roux, J.

    2016-12-01

    One of the key components of Earth Science data stewardship is high quality metadata. Ideally, all Earth Science/ Earth Observation datasets should be accompanied by a comprehensive metadata record including information such as: where to download data, the data format, the data temporal and spatial resolution, instruments used, and the purpose of the data collection (to name a few). While there are metadata formats and standards in place for NASA Earth Science data, many records either fail to provide critical information, or the information provided may be inaccurate, inconsistent, or outdated. The ARC Team at Marshall Space Flight Center has been working to improve the quality of records in the Common Metadata Repository (CMR), which serves as the authoritative management system for all NASA EOSDIS metadata. This process requires direct collaboration with personnel at NASA Distributed Active Archive Centers (DAACs) to ensure that their metadata holdings in CMR are optimal for search and discovery. The first DAAC to undergo a metadata review was the Global Hydrology Resource Center (GHRC). In this presentation, we will describe challenges and lessons learned from the metadata review process undertaken with GHRC. These lessons pave the way for a more efficient metadata review process with other DAACs in the future, which will ultimately result in improved data search capabilities for CMR users. A quantitative overview of improvements made to GHRC metadata since the start of its review process will also be provided.

  4. Using science to improve the dissemination and evaluation of scientific work.

    Directory of Open Access Journals (Sweden)

    Brett Thomas Buttliere

    2014-08-01

    Full Text Available Here we examine what science can tell us about the problems in psychological publishing and how to best address those problems. First, the motivation behind questionable research practices is examined (the desire to get ahead or, at least, not fall behind. Next, behavior modification strategies are discussed, pointing out that the carrot works better than the stick. Finally, we suggest that the best way to achieve real change is to make a tool so useful that academics make time to learn and utilize it on their own. Implementation of current change initiatives is hindered by a lack of norms, high initial buy-in costs, and uncertain payoffs. With this in mind, we pull together current open science tools to increase the utility while lowering effort and risk. One, centralized, easy to use, platform, with a profile, a feed of targeted science stories based on previous system interaction, a sophisticated (public comment and rating section, and impact metrics which use the available data can be used to realign individual and group motives. Some advantages of centrally digitizing communications are outlined, including ways the data could be used to improve the peer review process.

  5. Conceptual Demand of Practical Work in Science Curricula. A Methodological Approach

    Science.gov (United States)

    Ferreira, Sílvia; Morais, Ana M.

    2014-02-01

    This article addresses the issue of the level of complexity of practical work in science curricula and is focused on the discipline of Biology and Geology at high school. The level of complexity is seen in terms of the emphasis on and types of practical work and, most importantly, in terms of its level of conceptual demand as given by the complexity of scientific knowledge, the degree of inter-relation between knowledges, and the complexity of cognitive skills. The study also analyzes recontextualizing processes that may occur within the official recontextualizing field. The study is psychologically and sociologically grounded, particularly on Bernstein's theory of pedagogic discourse. It uses a mixed methodology. The results show that practical work is poorly represented in the curriculum, particularly in the case of laboratory work. The level of conceptual demand of practical work varies according to the text under analysis, between the two subjects Biology and Geology, and, within each of them, between general and specific guidelines. Aspects studied are not clearly explicated to curriculum receivers (teachers and textbooks authors). The meaning of these findings is discussed in the article. In methodological terms, the study explores assumptions used in the analysis of the level of conceptual demand and presents innovative instruments constructed for developing this analysis.

  6. FOREWORD: Some thoughts about Jürgen Hafner's work in computational materials science Some thoughts about Jürgen Hafner's work in computational materials science

    Science.gov (United States)

    Heine, Volker

    2011-10-01

    Jürgen Hafner started in the early 1970s with pseudopotential calculations on the structures and properties of sp-bonded metals, improving on work done elsewhere [1]. This expanded in four directions: transition metals, molten metals, magnetism and alloys, and combinations of these. As well as electronic structure calculations, he helped to advance the statistical mechanical classical theory of liquids for the molten metals [2]. In magnetism he was one of the pioneers of calculations with non-collinear spins [3, 4]. As well as simple (solid and molten) alloys, he also treated materials with strong chemical interaction such as sulphides and liquids such as arsenic and tellurium [5, 6]. All this fed into two directions which dominated much of his work for many years, namely the theory of glassy metals [7] and that of quasicrystals [8]. One notable result in the latter was to show that it was possible to construct hypothetical materials for which the quasicrystalline state is indeed the lowest energy structure. This displaced the established wisdom of the time that quasicrystals were necessarily metastable forms. In more recent years he has turned to calculations in surface science [9, 10], including catalysis of chemical reactions on surfaces [11, 12]. What really brought Jürgen first to my attention was that he had managed to do a better job than we had of calculations with the new approach of pseudopotentials, particularly regarding the screening part of the calculation. This is very important in alloys where there is a large difference in the electron density in the two types of atom due to their different volumes or valences such as in the phase diagram and structure of LiK or KPb [5, 13]. We have been in contact over many years including one close collaboration and I always learned something new in talking with Jürgen. In the late 1970s in Cambridge we performed phonon calculations on models of amorphous silicon [14], to see if these could distinguish between

  7. Interagency Working Group on Ocean Social Science: Incorporating ecosystem services approaches into ocean and coastal decision-making and governance

    Science.gov (United States)

    The application of social science has been recognized as a priority for effective ocean and coastal management, driving much discussion and fostering emerging efforts in several areas. The Interagency Working Group on Ocean Social Science (IWG-OSS) is tasked with assisting the Su...

  8. Working with the Nature of Science in Physics Class: Turning "Ordinary" Classroom Situations into Nature of Science Learning Situations

    Science.gov (United States)

    Hansson, Lena; Leden, Lotta

    2016-01-01

    In the science education research field there is a large body of literature on the "nature of science" (NOS). NOS captures issues about what characterizes the research process as well as the scientific knowledge. Here we, in line with a broad body of literature, use a wide definition of NOS including also e.g. socio-cultural aspects. It…

  9. Working with the Nature of Science in Physics Class: Turning "Ordinary" Classroom Situations into Nature of Science Learning Situations

    Science.gov (United States)

    Hansson, Lena; Leden, Lotta

    2016-01-01

    In the science education research field there is a large body of literature on the "nature of science" (NOS). NOS captures issues about what characterizes the research process as well as the scientific knowledge. Here we, in line with a broad body of literature, use a wide definition of NOS including also e.g. socio-cultural aspects. It…

  10. AN IMAGE-PLANE ALGORITHM FOR JWST'S NON-REDUNDANT APERTURE MASK DATA

    Energy Technology Data Exchange (ETDEWEB)

    Greenbaum, Alexandra Z. [Johns Hopkins University Department of Physics and Astronomy 3400 North Charles, Baltimore, MD 21218 (United States); Pueyo, Laurent; Sivaramakrishnan, Anand [Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218 (United States); Lacour, Sylvestre [LESIA, CNRS/UMR-8109, Observatoire de Paris, UPMC, Université Paris Diderot 5 place Jules Janssen, 92195 Meudon (France)

    2015-01-10

    The high angular resolution technique of non-redundant masking (NRM) or aperture masking interferometry (AMI) has yielded images of faint protoplanetary companions of nearby stars from the ground. AMI on James Webb Space Telescope (JWST)'s Near Infrared Imager and Slitless Spectrograph (NIRISS) has a lower thermal background than ground-based facilities and does not suffer from atmospheric instability. NIRISS AMI images are likely to have 90%-95% Strehl ratio between 2.77 and 4.8 μm. In this paper we quantify factors that limit the raw point source contrast of JWST NRM. We develop an analytic model of the NRM point spread function which includes different optical path delays (pistons) between mask holes and fit the model parameters with image plane data. It enables a straightforward way to exclude bad pixels, is suited to limited fields of view, and can incorporate effects such as intra-pixel sensitivity variations. We simulate various sources of noise to estimate their effect on the standard deviation of closure phase, σ{sub CP} (a proxy for binary point source contrast). If σ{sub CP} < 10{sup –4} radians—a contrast ratio of 10 mag—young accreting gas giant planets (e.g., in the nearby Taurus star-forming region) could be imaged with JWST NIRISS. We show the feasibility of using NIRISS' NRM with the sub-Nyquist sampled F277W, which would enable some exoplanet chemistry characterization. In the presence of small piston errors, the dominant sources of closure phase error (depending on pixel sampling, and filter bandwidth) are flat field errors and unmodeled variations in intra-pixel sensitivity. The in-flight stability of NIRISS will determine how well these errors can be calibrated by observing a point source. Our results help develop efficient observing strategies for space-based NRM.

  11. Unveiling the First Black Holes With JWST:Multi-wavelength Spectral Predictions

    Science.gov (United States)

    Natarajan, Priyamvada; Pacucci, Fabio; Ferrara, Andrea; Agarwal, Bhaskar; Ricarte, Angelo; Zackrisson, Erik; Cappelluti, Nico

    2017-04-01

    Growing supermassive black holes (∼ {10}9 {M}ȯ ) that power luminous z> 6 quasars from light seeds—the remnants of the first stars—within a Gyr of the Big Bang poses a timing challenge. The formation of massive black hole seeds via direct collapse with initial masses ∼ {10}4{--}{10}5 {M}ȯ alleviates this problem. Viable direct-collapse black hole formation sites, the satellite halos of star-forming galaxies, merge and acquire stars to produce a new, transient class of high-redshift objects, obese black hole galaxies (OBGs). The accretion luminosity outshines that of the stars in OBGs. We predict the multi-wavelength energy output of OBGs and growing Pop III remnants at z = 9 for standard and slim disk accretion, as well as high and low metallicities of the associated stellar population. We derive robust selection criteria for OBGs—a pre-selection to eliminate blue sources, followed by color–color cuts ([{F}090W-{F}220W]> 0;-0.3< [{F}200W-{F}444W]< 0.3) and the ratio of X-ray flux to rest-frame optical flux ({F}X/{F}444W\\gg 1). Our cuts sift out OBGs from other bright, high- and low-redshift contaminants in the infrared. OBGs with predicted {M}{AB}< 25 are unambiguously detectable by the Mid-Infrared Instrument (MIRI), on the upcoming James Webb Space Telescope (JWST). For parameters explored here, growing Pop III remnants with predicted {M}{AB}< 30 will likely be undetectable by JWST. We demonstrate that JWST has the power to discriminate between initial seeding mechanisms.

  12. High contrast imaging with the JWST-NIRSpec Integral Field Unit

    Science.gov (United States)

    Ygouf, Marie; Beichman, Charles A.; Hodapp, Klaus W.; Roellig, Thomas L.; NIRCam GTO

    2017-06-01

    With its integral field unit, the near-infrared spectrograph NIRSpec on JWST will allow to measure high-resolution spectra into the 3-5 μm range with an increased sensitivity over ground-based systems. This capability will considerably extend our knowledge of brown dwarfs and bright exoplanets at large separations from their host star. But because there is not any coronagraph on NIRSpec, the performance in term of contrast at close separation will be extremely limited. In this communication, we explore possibilities to further push this limitation by comparing different observing strategies and associated post-processing techniques.

  13. Capabilities of the James Webb Space Telescope for Exoplanet Science

    Science.gov (United States)

    Clampin, Mark

    2009-01-01

    The James Webb Space Telescope (JWST) is a large aperture (6.5 meter), cryogenic space telescope with a suite of near and mid-infrared instruments covering the wavelength range of 0.6 m to 28 m. JWST s primary science goal is to detect and characterize the first galaxies. It will also study the assembly of galaxies, star formation, and the formation of evolution of planetary systems. We also review the expected scientific performance of the observatory for observations of exosolar planets by means of transit photometry and spectroscopy, and direct coronagraphic imaging.

  14. Religion and Science in the Works of the Founder of the First Wave of Positivism

    Directory of Open Access Journals (Sweden)

    Arkadiy Korsakov

    2012-04-01

    Full Text Available This article attempts to deal with the last phase of the life and work of Auguste Conte, the founder of the philosophy of positivism. The appearance and development of this type of philosophy were conditioned by the new waves of thought which dominated European philosophy during the nineteenth century. It was believed that faith in a scientific method would guarantee the success of any kind of scientific endeavor. Conte developed his idea of a three level intellectual evolution from notions which had already been posited by Saint-Simon. According to this ideology, man begins to mature when he begins to abandon his childish and immature notions about the world, or in other words, his religious-mystical preoccupations. Eventually he becomes an adult and begins to discover a type of God in himself. But in this way, positivism itself begins to develop its own religious and mystical traits while at the same time conducting a fierce battle with a religious conception of the world. These ideas come especially to the fore in the later works of Conte. In these works, the philosopher stipulates that although sociology is at the absolute pinnacle of the sciences, there is yet another level, still higher than all these - and that is the domain of the so-called religion of mankind

  15. Science Divulgation: The Social Representations of Brazilian Researchers Working in the Field of Astronomy

    Science.gov (United States)

    Carneiro, Dalira Lúcia Cunha Maradei; Longhini, Marcos Daniel

    2015-12-01

    This article addresses the role of scientific divulgation in the interaction between science and society, debating the importance of Astronomy as a prime starter of the scientific divulgation. In the light of Moscovici’s Social Representations Theory, the social representations on scientific divulgation of Brazilian researchers that work in the field of Astronomy are studied. Individuals from different educational trajectories ansewered semi-structured interviews, which were analyzed according to Spink. The results indicate two representations: one for the society at large, moved by passion, based on values and beliefs, and on the satisfaction of seeing the results of their actions on people’s life; and another for their peers. In the first representation, gaps that obstruct the science divulgation emerge, such as the lack of training and the difficulty to use a plain language, the bureaucracy required for the projects’ execution and its negative representation in the media. Other inferences are that Astronomy is neither part of a systematic teaching nor a part of the media at large, and it often presents conceptual mistakes. Those representations find an echo in the theoretical framework, showing that, despite their advances, scientific divulgation and Astronomy Education are in a context of social fragility.

  16. [Story life CHENG Dan-an's, works and his achievements on acupuncture and moxibustion science].

    Science.gov (United States)

    Lu, Xiang; Cai, Yue

    2011-05-01

    Mr. CHENG Dan-an, who devoted himself to the renaissance of the course of modern Chinese acupuncture, the establishment of acupuncture education unit, correspondence education, acupuncture personnel fostering and publication of periodicals on acupuncture, has great contribution to the academic exchanges and popularization of acupuncture. Mr. CHENG has completed over 10 articles and more than 20 works and translations. According to him, mechanism on meridians, collaterals, acupoints and acupuncture techniques were explored with the promotion on application of "Shen" and "qi" in clinic. Pulse and tongue diagnosis as well as acupuncture treatment were supplemented into Shanghanlun (Treatise on Febrile Diseases). And great importance was attached on the scientific validity and practicability. His professional ethics and dedication are worth to be learned by all medical workers nowadays. His acupuncture theories and academic achievements still inspire us today, which are also taken as the origin for the innovation and development of modern acupuncture science.

  17. Work.

    Science.gov (United States)

    Haines, Annette M.

    2003-01-01

    Draws upon Maria Montessori's writings to examine work as a universal human tendency throughout life. Discusses the work of adaptation of the infant, work of "psycho-muscular organism" for the preschooler, work of the imagination for the elementary child, community work of the adolescent, and work of the adult. Asserts that…

  18. DEVELOPMENT OF PHYSICS STUDENT WORK SHEET (SWS TO BUILD SCIENCE PROCESS SKILL VALUED CONSERVATION

    Directory of Open Access Journals (Sweden)

    D. Yulianti

    2015-07-01

    Full Text Available Student Work Sheet (SWS which contains only a summary of the material and exercises does not train students to investigate and develop conservation values. The research objective is to also prepared worksheets guided inquiry that can enhance science process skills, understanding of the concept and develop conservation value. Elements of inquiry and conservation value generated through work instructions and investigation. The study was performed by using one group pretest-posttest design. Research procedures include observation and identification of weaknesses worksheets, planning, early product development and initial field trials. Feasibility and legibility using questionnaires and tests hiatus. The value of understanding the concept derived from the pretest-posttest. Data science process skills gained from the observation during the lesson. Conservation values obtained from the students' self-assessment questionnaire and assessment questionnaire between friends. The analysis showed guided inquiry SWS easy to understand and very fit for use as teaching materials. Test gain showed guided inquiry SWS can enhance science process skills and conceptual understanding, and can be used as a medium to develop conservation value.LKS yang hanya berisi ringkasan materi dan latihan soal tidak melatih siswa melakukan penyelidikan dan mengembangkan nilai konservasi. Tujuan penelitian R&D ini adalah menyususn LKS yang mampu meningkatkan keterampilan proses sains, pemahaman konsep dan nilai konservasi. Nilai konservasi dimunculkan melalui petunjuk kerja dan kegiatan penyelidikan.Ujicoba menggunakanOne Group Pretest-Posttest Design. Prosedur penelitian meliputi observasi dan identifikasi kelemahan LKS, perencanaan, pengembangan produk awal dan uji coba lapangan awal. Uji kelayakan dan keterbacaan menggunakan angket dan tes rumpang. Nilai pemahaman konsep  diperoleh dari pretest-posttest. Data keterampilan proses sains diperoleh dari hasil observasi

  19. Finding Citations to Social Work Literature: The Relative Benefits of Using "Web of Science," "Scopus," or "Google Scholar"

    Science.gov (United States)

    Bergman, Elaine M. Lasda

    2012-01-01

    Past studies of citation coverage of "Web of Science," "Scopus," and "Google Scholar" do not demonstrate a consistent pattern that can be applied to the interdisciplinary mix of resources used in social work research. To determine the utility of these tools to social work researchers, an analysis of citing references to well-known social work…

  20. Finding Citations to Social Work Literature: The Relative Benefits of Using "Web of Science," "Scopus," or "Google Scholar"

    Science.gov (United States)

    Bergman, Elaine M. Lasda

    2012-01-01

    Past studies of citation coverage of "Web of Science," "Scopus," and "Google Scholar" do not demonstrate a consistent pattern that can be applied to the interdisciplinary mix of resources used in social work research. To determine the utility of these tools to social work researchers, an analysis of citing references to well-known social work…

  1. THE FORMATION OF STUDENTS’ LEARNING-COGNITIVE COMPETENCES BASED ON LABORATORY WORKS IN COMPUTER SCIENCE AND ICT

    National Research Council Canada - National Science Library

    EVGENIY YUR’EVICH ANDRUSENKO

    2015-01-01

    .... Laboratory work in computer science and ICT is one of such means. Laboratory work is a link between theoreti-cal and practical learning and is an important component of theory and practice: it strengthens and improves knowledge and skills, which are used in the process of further studies.

  2. New and Better Near-Infrared Detectors for JWST Near Infrared Spectrograph

    Science.gov (United States)

    Rauscher, Bernard J.; Mott, D. Brent; Wen, Yiting; Linder, Don; Greenhouse, Matthew A.; Hill, Robert J.

    2014-01-01

    ESA and NASA recently selected two 5 m cutoff Teledyne H2RG sensor chip assemblies (SCA) for flight on the James Webb Space Telescope (JWST) Near Infrared Spectrograph (NIRSpec). These HgCdTe SCAs incorporate Teledynes improved barrier layer design that eliminates the degradation that affected earlier JWST H2RGs(Rauscher et al. 2012a). The better indium barrier, together with other design changes, has improved the performance and reliability of JWSTs SCAs. In this article, we describe the measured performance characteristics that most directly affect scientific observations including read noise, total noise, dark current, quantum efficiency (QE), and image persistence. As part of measuring QE, we measured the quantum yield as a function of photon energy,, and found that it exceeds unity for photon energies E (2.65.2) Eg, where Eg is the HgCdTe bandgap energy. This corresponds to. 2 m for NIRSpecs 5 m cutoff HgCdTe. Our measurements agree well with a previous measurement by McCullough et al. (2008) for. 1.3. For 1.3, we find a slower increase in with photon energy than McCullough et al. did. However, and as McCullough et al. note, their two state model of the yield process is not valid for large 1.

  3. Mechanical blind gap measurement tool for alignment of the JWST Optical Telescope Element

    Science.gov (United States)

    Liepmann, Till

    2016-09-01

    This paper describes a novel gap gauge tool that is used to provide an independent check of the James Webb Space Telescope (JWST) Optical Telescope Element (OTE) primary mirror alignment. Making accurate measurements of the mechanical gaps between the OTE mirror segments is needed to verify that the segments were properly aligned relative to each other throughout the integration and test of the 6.6 meter telescope. The gap between the Primary Mirror Segment Assemblies (PMSA) is a sensitive indicator of the relative clocking and decenter. Further, the gap measurements are completely independent of all the other measurements use in the alignment process (e.g. laser trackers and laser radar). The gap measurement is a challenge, however, that required a new approach. Commercial gap measurements tools were investigated; however no suitable solution is available. The challenge of this measurement is due to the required 0.1 mm accuracy, the close spacing of the mirrors segments (approximately 3-9mm), the acute angle between the segment sides (approximately 4 degrees), and the difficult access to the blind gap. Several techniques were considered and tested before selecting the gauge presented here. This paper presents the theory, construction and calibration of the JWST gap gauge that is being used to measure and verify alignment of the OTE primary mirror segments.

  4. An image-plane algorithm for JWST's non-redundant aperture mask data

    CERN Document Server

    Greenbaum, Alexandra Z; Sivaramakrishnan, Anand; Lacour, Sylvestre

    2014-01-01

    The high angular resolution technique of non-redundant masking (NRM) or aperture masking interferometry (AMI) has yielded images of faint protoplanetary companions of nearby stars from the ground. AMI on James Webb Space Telescope (JWST)'s Near Infrared Imager and Slitless Spectrograph (NIRISS) has a lower thermal background than ground-based facilites and does not suffer from atmospheric instability. NIRISS AMI images are likely to have 90 - 95% Strehl ratio between 2.77 and 4.8 micron. In this paper we quantify factors that limit the raw point source contrast of JWST NRM. We develop an analytic model of the NRM point spread function which includes different optical path delays (pistons) between mask holes and fit the model parameters with image plane data. It enables a straightforward way to exclude bad pixels, is suited to limited fields of view, and can incorporate effects such as intra-pixel sensitivity variations. We simulate various sources of noise to estimate their effect on the standard deviation of...

  5. Hearing and Speech Sciences in Educational Environment Mapping in Brazil: education, work and professional experience.

    Science.gov (United States)

    Celeste, Letícia Corrêa; Zanoni, Graziela; Queiroga, Bianca; Alves, Luciana Mendonça

    2017-03-09

    To map the profile of Brazilian Speech Therapists who report acting in Educational Speech Therapy, with regard to aspects related to training, performance and professional experience. Retrospective study, based on secondary database analysis of the Federal Council of Hearing and Speech Sciences on the questionnaires reporting acting with Educational Environment. 312 questionnaires were completed, of which 93.3% by women aged 30-39 years. Most Speech Therapists continued the studies, opting mostly for specialization. Almost 50% of respondents, have worked for less than six years with the speciality, most significantly in the public service (especially municipal) and private area. The profile of the Speech Therapists active in the Educational area in Brazil is a professional predominantly female, who values to continue their studies after graduation, looking mostly for specialization in the following areas: Audiology and Orofacial Motor. The time experience of the majority is up to 10 years of work whose nature is divided mainly in public (municipal) and private schools. The performance of Speech Therapists in the Educational area concentrates in Elementary and Primary school, with varied workload.

  6. Observing Planetary Nebulae with JWST and Extremely Large Telescopes

    Science.gov (United States)

    Sahai, Raghvendra

    2015-01-01

    Most stars in the Universe that leave the main sequence in a Hubble time will end their lives evolving through the Planetary Nebula (PN) evolutionary phase. The heavy mass loss which occurs during the preceding AGB phase is important across astrophysics, dramatically changing the course of stellar evolution, dominantly contributing to the dust content of the interstellar medium, and influencing its chemical composition. The evolution from the AGB phase to the PN phases remains poorly understood, especially the dramatic transformation that occurs in the morphology of the mass-ejecta as AGB stars and their round circumstellar envelopes evolve into mostly PNe, the majority of which deviate strongly from spherical symmetry. In addition, although the PN [OIII] luminosity function (PNLF) has been used as a standard candle (on par with distance indicators such as Cepheids), we do not understand why it works. It has been argued that the resolution of these issues may be linked to binarity and associated processes such as mass transfer and common envelope evolution.Thus, understanding the formation and evolution of PNe is of wide astrophysical importance. PNe have long been known to emit across a very large span of wavelengths, from the radio to X-rays. Extensive use of space-based observatories at X-ray (Chandra/ XMM-Newton), optical (HST) and far-infrared (Spitzer, Herschel) wavelengths in recent years has produced significant new advances in our knowledge of these objects. Given the expected advent of the James Webb Space Telescope in the near future, and ground-based Extremely Large Telescope(s) somewhat later, this talk will focus on future high-angular-resolution, high-sensitivity observations at near and mid-IR wavelengths with these facilities that can help in addressing the major unsolved problems in the study of PNe.

  7. Participating in Science at Home: Recognition Work and Learning in Biology

    Science.gov (United States)

    Zimmerman, Heather Toomey

    2012-01-01

    This article presents an analysis of the longitudinal consequences of out-of-school science learning with a conceptual framework that connects the intentions of youth to their participation in science. The focus is on one girl's science activities in her home and hobby pursuits from fourth to seventh grade to create an empirical account of how…

  8. Collaborations in a Community of Practice Working to Integrate Engineering Design in Elementary Science Education

    Science.gov (United States)

    Lehman, James D.; Kim, WooRi; Harris, Constance

    2014-01-01

    The new standards for K-12 science education in the United States call for science teachers to integrate engineering concepts and practices within their science teaching in order to improve student learning. To accomplish this, teachers need appropriate instructional materials as well as the knowledge and skills to effectively use them. This mixed…

  9. Crowdsourcing Scientific Work: A Comparative Study of Technologies, Processes, and Outcomes in Citizen Science

    Science.gov (United States)

    Wiggins, Andrea

    2012-01-01

    Citizen science projects involve the public with scientists in collaborative research. Information and communication technologies for citizen science can enable massive virtual collaborations based on voluntary contributions by diverse participants. As the popularity of citizen science increases, scientists need a more thorough understanding of…

  10. Titan Science with the James Webb Space Telescope

    Science.gov (United States)

    Nixon, Conor A.; Achterberg, Richard; Adamkovics, Mate; Bezard, Bruno; Bjoraker, Gordon; Cornet, Thomas; Hayes, Alexander; Lellouch, Emmanuel; Lemmon, Mark; Lopez Puertas, Manuel; Rodriguez, Sebastien; Sotin, Christophe; Teanby, Nicholas; Turtle, Elizabeth; West, Robert

    2015-11-01

    The James Webb Space Telescope (JWST), scheduled for launch in 2018, is an ambitious next-generation large-aperture (6.5 m) space observatory focused on pushing the boundaries of infrared astronomy (0.6-28.0 μm). This long-wavelength focus gives it very substantial potential for solar system science, since the thermal emissions from the surfaces and atmospheres of many planets, moons and small bodies peak in this part of the spectrum. Here we report the findings of a task team convened to examine the potential for Titan science using JWST. These can be divided into five broad areas: (i) the surface, especially the rotational lightcurve; (ii) clouds in the lower atmosphere from direct imaging and near-IR spectroscopy; (iii) composition of the lower atmosphere, especially methane relative humidity; (iv) composition of the middle atmosphere, including thermal and fluorescent emissions from gases; (v) hazes in the middle atmosphere, including seasonal changes in hemispheric contrast. The capability of the major JWST instruments in each area is considered, and limitations such as potential saturation is noted and mitigation strategies (such as sub-arraying) discussed. Overall we find that JWST can make significant contributions to Titan science in many areas, not least in temporal monitoring of seasonal change after the end of the Cassini mission in 2017, in partnership with other next-generation observing facilities (TMT, GMT, EELT, ALMA).

  11. Assessment of Predictable Productivity of Nurses Working in Kerman University of Medical Sciences' Teaching Hospitals via the Dimensions of Quality of Work Life.

    Science.gov (United States)

    Borhani, Fariba; Arbabisarjou, Azizollah; Kianian, Toktam; Saber, Saman

    2016-10-01

    Despite the existence of a large community of nurses, specific mechanisms have not been developed yet to consider their needs and the quality of their work life. Moreover, few studies have been conducted to analyze the nature of nursing, nursing places or nurses' quality of work life. In this regard, the present study aimed to assess predictable productivity of nurses working in Kerman University of Medical Sciences' teaching hospitals via the dimensions of Quality of Work Life. The present descriptive-correlational study was conducted to assess predictable productivity of nurses via the dimensions of Quality of Work Life. The study's population consisted of all nurses working in different wards of teaching hospitals associated with Kerman University of Medical Sciences. Out of the whole population, 266 nurses were selected based on the simple random sampling method. To collect data, the questionnaires of 'Quality of Nursing Work Life' and 'Productivity' were used after confirming their reliability (test-retest) and content validity. Finally, the collected data were analyzed through the SPSS software (version 16). Although the quality of work life for nurses was average and their productivity was low but the results showed that quality of life is directly related to nurses' productivity. Quality of life and its dimensions are predictive factors in the in the nurses' productivity. It can conclude that by recognizing the nurses' quality of work life situation, it can realize this group productivity and their values to the efficiency of the health system. For the quality of working life improvement and increasing nurses' productivity more efforts are needed by authorities. The findings can be applied by managers of hospitals and nursing services along with head nurses to enhance the quality of health services and nursing profession in general.

  12. Action research in gender issues in science education: Towards an understanding of group work with science teachers

    Science.gov (United States)

    Nyhof-Young, Joyce Marion

    Action research is emerging as a promising means of promoting individual and societal change in the context of university programmes in teacher education. However, significant gaps exist in the literature regarding the use of action research groups for the education of science teachers. Therefore, an action research group, dealing with gender issues in science education, was established within the context of a graduate course in action research at OISE. For reasons outlined in the thesis, action research was deemed an especially appropriate means for addressing issues of gender. The group met 14 times from September 1992 until May 1993 and consisted of myself and five other science teachers from the Toronto area. Two of us were in the primary panel, two in the intermediate panel, and two in the tertiary panel. Five teachers were female. One was male. The experiences of the group form the basis of this study. A methodology of participant observation supported by interviews, classroom visits, journals, group feedback and participant portfolios provides a means of examining experiences from the perspective of the participants in the group. The case study investigates the nature of the support and learning opportunities that the action research group provided for science teachers engaged in curiculum and professional development in the realm of gender issues in science education, and details the development of individuals, the whole group and myself (as group worker, researcher and participant) over the life of the project. The action research group became a resource for science teachers by providing most participants with: A place to personalize learning and research; a place for systematic reflection and research; a forum for discussion; a source of personal/professional support; a source of friendship; and a place to break down isolation and build self-confidence. This study clarifies important relational and political issues that impinge on action research in

  13. The Federation of Earth Science Information Partners (ESIP Federation): Facilitating Partnerships that Work to Bring Earth Science Data into Educational Settings

    Science.gov (United States)

    Freuder, R.; Ledley, T. S.; Dahlman, L.

    2004-12-01

    The Federation of Earth Science Information Partners (ESIP Federation, http://www.esipfed.org) formed seven years ago and now with 77 member organizations is working to "increase the quality and value of Earth science products and services .for the benefit of the ESIP Federation's stakeholder communities." Education (both formal and informal) is a huge audience that we serve. Partnerships formed by members within the ESIP Federation have created bridges that close the gap between Earth science data collection and research and the effective use of that Earth science data to explore concepts in Earth system science by the educational community. The Earth Exploration Toolbook is one of those successful collaborations. The Earth Exploration Toolbook (EET, http://serc.carleton.edu/eet) grew out of a need of the educational community (articulated by the Digital Library for Earth System Education (DLESE) community) to have better access to Earth science data and data analysis tools and help in effectively using them with students. It is a collection of web-accessible chapters, each featuring step-by-step instructions on how to use an Earth science dataset and data analysis tool to investigate an issue or concept in Earth system science. Each chapter also provides the teacher information on the outcome of the activity, grade level, standards addressed, learning goals, time required, and ideas for exploring further. The individual ESIP Federation partners alone could not create the EET. However, the ESIP Federation facilitated the partnering of members, drawing from data providers, researchers and education tool developers, to create the EET. Interest in the EET has grown since it went live with five chapters in July 2003. There are currently seven chapters with another six soon to be released. Monthly online seminars in which over a hundred educators have participated have given very positive feedback. Post workshop surveys from our telecon-online workshops indicate that

  14. Science and Society: The Life and Work of a Great Russian Physicist

    CERN Multimedia

    2002-01-01

    In 1934, the eminent Russian physicist and optics specialist Sergei Ivanovitch Vavilov (1891-1951) was the first, together with Pavel Cherenkov, to observe the famous radiation we now call Cherenkov radiation, a discovery commonly used in the Laboratory's detectors. His most well-known discoveries also include that of the non-linear optical effect in 1926. Vavilov founded the Lebedev Physics Institute in Moscow, which prospered under his directorship, and contributed to the rise of nuclear physics and cosmic radiation in the USSR. The highpoint of his career came in 1945, when he was appointed President of the Soviet Academy of Sciences. However, Sergei Vavilov worked under the Stalinist dictatorship, which was responsible for the death of his elder brother, the biologist Nikolai Vavilov. His own health compromised, he died two months before his 60th birthday. His remarkable life, which is interesting not only for his scientific discoveries but also in terms of its historical context, will be the subject of...

  15. The effect of a science work experience program for teachers on the classroom environment: A qualitative program evaluation

    Science.gov (United States)

    Frazier, Wendy Michelle

    Science Work Experience Programs for Teachers (SWEPTs) provide an opportunity for science and math teachers to work in research laboratories during the summer to experience science as it is practiced in the laboratory-setting. Through the use of interviews with teachers and students, classroom observations, and an analysis of printed student sheets and student work, the lived experience of a cohort of program participants in Columbia University's Summer Research Program for Secondary School Science Teachers was recorded in an effort to describe the effect of experience in a SWEPT on the classroom environment of teacher participants and student outcomes. Relying on Social Learning Theory and science education reform documentation as a theoretical framework the following dimensions of the classroom were examined: (1) emergent themes that include the participants' perceptions of the importance of technology in the classroom, (2) interpersonal relationships with the teachers at the participants' schools, fellow program participants, research scientists, and students, and (3) changes in epistemological structure, curriculum, instructional strategies, and classroom practices. Methodological and theoretical implications are addressed with respect to future studies, and suggestions for refinement of SWEPTs are provided.

  16. SOCIAL RESPONSIBILITY AND CITIZENSHIP AWARENESS IN "THIS IS MY WORK" SCIENCE PROJECTS IN TERMS OF CITIZENSHIP EDUCATION

    Directory of Open Access Journals (Sweden)

    Cemalettin AYAS

    2013-06-01

    Full Text Available Science is an individual and social activity with a long history, having unique characteristics, and is contributed to its development by many people from different cultures. This is closely related with the principle of economic and social benefits for the society as it is in the context of "This is My Work: Math and Science Projects Competition" carried out by the Ministry of National Education since 2006. Therefore, this study examined the notion of "Citizenship Awareness" in each of 455 Science and Technology projects which were among the top 100 projects in "This is My Work: Math Science Projects Competition" carried out across the country every year since 2006. For the methodology, Science projects entered the competition for the last seven years were subjected to content analysis in terms of content on "Citizenship and Social Responsibility." Conclusions were finally made with idea that student works in the projects competition were largely emerged from and implemented with an understanding of social responsibility; solving a problem in the society and environment; consciousness of environmental protection; cleanliness and the health; aesthetics; hazard prevention and safety of life; helping disabled people as one of the basic human values of the social life.

  17. Viewing past science from the point of view of present science, thereby illuminating both: Philosophy versus experiment in the work of Robert Boyle.

    Science.gov (United States)

    Chalmers, Alan

    2016-02-01

    The seventeenth century witnessed the replacement of an Aristotelian worldview by a mechanical one. It also witnessed the beginnings of significant experimental enquiry. Alerted by the fact that the methods involved in the latter, but not in the former, resemble those employed in later science, I argue the historical case that the emergence of the mechanical worldview and the emergence of science were not closely related and that it was the latter that was to develop into science as we have come to know it. The details are explored in the context of the philosophical and experimental work of Robert Boyle and the relationship between them. Copyright © 2015 Elsevier Ltd. All rights reserved.

  18. Developing an instrument simulator: experience feedback from the JWST/NIRSpec and VLT/MUSE simulators

    Science.gov (United States)

    Jarno, Aurélien; Piqueras, Laure; Bacon, Roland; Ferruit, Pierre; Legros, Emeline; Pécontal-Rousset, Arlette; Gnata, Xavier; Streicher, Ole; Weilbacher, Peter

    2012-09-01

    The Centre de Recherche Astrophysique de Lyon (CRAL) has recently developed two instrument simulators for spectrographic instruments. They are based on Fourier optics, and model the whole chain of acquisition, taking into account both optical aberrations and diffraction effects, by propagating a wavefront through the instrument, according to the Fourier optics concept. One simulates the NIRSpec instrument, a near-infrared multi-object spectrograph for the future James Webb Space Telescope (JWST). The other one models the Multi Unit Spectroscopic Explorer (MUSE) instrument, a second-generation integral-field spectrograph for the Very Large Telescope (VLT). The two simulators have been developed in different contexts (subcontracted versus developed internally), and for very different instruments (space-based versus ground-based), which strengthen the CRAL experience. This paper describes the lessons learned while developing these simulators: development methods, phasing with the project, points to focus on, getting data, interacting with scientists and users, etc.

  19. The infrared signatures of very small grains in the Universe seen by JWST

    CERN Document Server

    Pilleri, Paolo; Joblin, Christine

    2015-01-01

    The near- and mid-IR spectrum of many astronomical objects is dominated by emission bands due to UV-excited polycyclic aromatic hydrocarbons (PAH) and evaporating very small grains (eVSG). Previous studies with the ISO, Spitzer and AKARI space telescopes have shown that the spectral variations of these features are directly related to the local physical conditions that induce a photo-chemical evolution of the band carriers. Because of the limited sensitivity and spatial resolution, these studies have focused mainly on galactic star-forming regions. We discuss how the advent of JWST will allow to extend these studies to previously unresolved sources such as near-by galaxies, and how the analysis of the infrared signatures of PAHs and eVSGs can be used to determine their physical conditions and chemical composition.

  20. The Mid-Infrared Instrument for JWST, II: Design and Build

    CERN Document Server

    Wright, G S; Goodson, G B; Rieke, G H; Aitink-Kroes, Gabby; Amiaux, J; Aricha-Yanguas, Ana; Azzolini, Ruyman; Banks, Kimberly; Barrado-Navascues, D; Belenguer-Davila, T; Bloemmart, J A D L; Bouchet, Patrice; Brandl, B R; Colina, L; Detre, Ors; Diaz-Catala, Eva; Eccleston, Paul; Friedman, Scott D; Garcia-Marin, Macarena; Guedel, Manuel; Glasse, Alistair; Glauser, Adrian M; Greene, T P; Groezinger, Uli; Grundy, Tim; Hastings, Peter; Henning, Th; Hofferbert, Ralph; Hunter, Faye; Jessen, N C; Justtanont, K; Karnik, Avinash R; Khorrami, Mori A; Krause, Oliver; Labiano, Alvaro; Lagage, P -O; Langer, Ulrich; Lemke, Dietrich; Lim, Tanya; Lorenzo-Alvarez, Jose; Mazy, Emmanuel; McGowan, Norman; Meixner, M E; Morris, Nigel; Morrison, Jane E; Mueller, Friedrich; Norgaard-Nielson, H -U; Olofsson, Goeran; O'Sullivan, Brian; Pel, J -W; Penanen, Konstantin; Petach, M B; Pye, J P; Ray, T P; Renotte, Etienne; Renouf, Ian; Ressler, M E; Samara-Ratna, Piyal; Scheithauer, Silvia; Schneider, Analyn; Shaughnessy, Bryan; Stevenson, Tim; Sukhatme, Kalyani; Swinyard, Bruce; Sykes, Jon; Thatcher, John; Tikkanen, Tuomo; van Dishoeck, E F; Waelkens, C; Walker, Helen; Wells, Martyn; Zhender, Alex

    2015-01-01

    The Mid-InfraRed Instrument (MIRI) on the James Webb Space Telescope (JWST) provides measurements over the wavelength range 5 to 28.5 microns. MIRI has, within a single 'package', four key scientific functions: photometric imaging, coronagraphy, single-source low-spectral resolving power (R ~ 100) spectroscopy, and medium-resolving power (R ~ 1500 to 3500) integral field spectroscopy. An associated cooler system maintains MIRI at its operating temperature of < 6.7 K. This paper describes the driving principles behind the design of MIRI, the primary design parameters, and their realization in terms of the 'as-built' instrument. It also describes the test program that led to delivery of the tested and calibrated Flight Model to NASA in 2012, and the confirmation after delivery of the key interface requirements.

  1. Reconstructing Emission from Pre-Reionization Sources with Cosmic Infrared Background Fluctuation Measurements by the JWST

    Science.gov (United States)

    Kashlinsky, A.; Mather, J. C.; Helgason, K.; Arendt, R. G.; Bromm, V.; Moseley, S. H.

    2015-01-01

    We present new methodology to use cosmic infrared background (CIB) fluctuations to probe sources at 10 less than or approx. equal to z less than or approx. equal to 30 from a James Webb Space Telescope (JWST) NIRCam configuration that will isolate known galaxies to 28 AB mag at 0.55 m. At present significant mutually consistent source-subtracted CIB fluctuations have been identified in the Spitzer and AKARI data at 25 m, but we demonstrate internal inconsistencies at shorter wavelengths in the recent CIBER data. We evaluate CIB contributions from remaining galaxies and show that the bulk of the high-z sources will be in the confusion noise of the NIRCam beam, requiring CIB studies. The accurate measurement of the angular spectrum of the fluctuations and probing the dependence of its clustering component on the remaining shot noise power would discriminate between the various currently proposed models for their origin and probe the flux distribution of its sources. We show that the contribution to CIB fluctuations from remaining galaxies is large at visible wavelengths for the current instruments precluding probing the putative Lyman-break of the CIB fluctuations. We demonstrate that with the proposed JWST configuration such measurements will enable probing the Lyman-break. We develop a Lyman-break tomography method to use the NIRCam wavelength coverage to identify or constrain, via the adjacent two-band subtraction, the history of emissions over 10 less than or approx. equal to z less than or approx. equal to 30 as the universe comes out of the Dark Ages. We apply the proposed tomography to the current SpitzerIRAC measurements at 3.6 and 4.5 m, to find that it already leads to interestingly low upper limit on emissions at z greater than or approx. equal to 30.

  2. Reconstructing Emission from Pre-reionization Sources with Cosmic Infrared Background Fluctuation Measurements by the JWST

    Science.gov (United States)

    Kashlinsky, A.; Mather, J. C.; Helgason, K.; Arendt, R. G.; Bromm, V.; Moseley, S. H.

    2015-05-01

    We present new methodology to use cosmic infrared background (CIB) fluctuations to probe sources at 10≲ z≲ 30 from a James Webb Space Telescope (JWST)/NIRCam configuration that will isolate known galaxies to 28 AB mag at 0.5-5 μm. At present significant mutually consistent source-subtracted CIB fluctuations have been identified in the Spitzer and AKARI data at ˜2-5 μm, but we demonstrate internal inconsistencies at shorter wavelengths in the recent CIBER data. We evaluate CIB contributions from remaining galaxies and show that the bulk of the high-z sources will be in the confusion noise of the NIRCam beam, requiring CIB studies. The accurate measurement of the angular spectrum of the fluctuations and probing the dependence of its clustering component on the remaining shot noise power would discriminate between the various currently proposed models for their origin and probe the flux distribution of its sources. We show that the contribution to CIB fluctuations from remaining galaxies is large at visible wavelengths for the current instruments precluding probing the putative Lyman-break of the CIB fluctuations. We demonstrate that with the proposed JWST configuration such measurements will enable probing the Lyman-break. We develop a Lyman-break tomography method to use the NIRCam wavelength coverage to identify or constrain, via the adjacent two-band subtraction, the history of emissions over 10≲ z≲ 30 as the universe comes out of the “Dark Ages.” We apply the proposed tomography to the current Spitzer/IRAC measurements at 3.6 and 4.5 μm, to find that it already leads to interestingly low upper limit on emissions at z≳ 30.

  3. The Galactic Center Seen Through the Precise, Multiplexed Eye of JWST

    Science.gov (United States)

    Lu, Jessica R.

    2013-01-01

    The Galactic center harbors the closest supermassive black hole and contains warm, turbulent molecular clouds, dense stellar populations, and some of the most active star forming regions in the Milky Way. These unique conditions make the Galactic Center a compelling target for understanding how star formation varies with environment, how nuclear star clusters in galaxies evolve, and how supermassive black holes influence their surroundings. Detailed studies of the Galactic center have previously been conducted with ground-based telescopes equipped with adaptive optics in pencil-beam studies. However, Galactic center studies can be dramatically expanded with JWST's combination of large fields-of-view (FOV) and high spatial resolution in the infrared. Of particular relevance for the Galactic Center are NIRCam's suite of narrow-band imaging filters and NIRSpec's IFU spectrograph. The narrow-band imaging should provide precise astrometry, rough spectral types, and emission line maps for ~50,000 stars within a 2' x 2' FOV, while follow up IFU spectroscopy will give precise types and radial velocities for the most interesting subsets of stars. Potential results include: (1) counting the intermediate age red and yellow supergiants that will give information about the recent star formation history; (2) measuring the initial mass function below 1 Msun and studying young stellar objects in known and new young star clusters; (3) using 3D dynamics to model the kinematic evolution of the entire nuclear cluster, find hypervelocity stars, and trace the orbits of gas features and clusters in the region. Galactic Center observations with JWST will give us a more complete picture of the gas, stars, black hole, and their interactions in this dynamic region.

  4. Exploring Biases of Atmospheric Retrievals in Simulated JWST Transmission Spectra of Hot Jupiters

    Science.gov (United States)

    Rocchetto, M.; Waldmann, I. P.; Venot, O.; Lagage, P.-O.; Tinetti, G.

    2016-12-01

    With a scheduled launch in 2018 October, the James Webb Space Telescope (JWST) is expected to revolutionize the field of atmospheric characterization of exoplanets. The broad wavelength coverage and high sensitivity of its instruments will allow us to extract far more information from exoplanet spectra than what has been possible with current observations. In this paper, we investigate whether current retrieval methods will still be valid in the era of JWST, exploring common approximations used when retrieving transmission spectra of hot Jupiters. To assess biases, we use 1D photochemical models to simulate typical hot Jupiter cloud-free atmospheres and generate synthetic observations for a range of carbon-to-oxygen ratios. Then, we retrieve these spectra using TauREx, a Bayesian retrieval tool, using two methodologies: one assuming an isothermal atmosphere, and one assuming a parameterized temperature profile. Both methods assume constant-with-altitude abundances. We found that the isothermal approximation biases the retrieved parameters considerably, overestimating the abundances by about one order of magnitude. The retrieved abundances using the parameterized profile are usually within 1σ of the true state, and we found the retrieved uncertainties to be generally larger compared to the isothermal approximation. Interestingly, we found that by using the parameterized temperature profile we could place tight constraints on the temperature structure. This opens the possibility of characterizing the temperature profile of the terminator region of hot Jupiters. Lastly, we found that assuming a constant-with-altitude mixing ratio profile is a good approximation for most of the atmospheres under study.

  5. SCASim: A Flexible and Reusable Detector Simulator for the MIRI instrument of the JWST

    Science.gov (United States)

    Beard, S.; Morin, J.; Gastaud, R.; Azzollini, R.; Bouchet, P.; Chaintreuil, S.; Lahuis, F.; Littlejohns, O.; Nehme, C.; Pye, J.

    2012-09-01

    The JWST Mid Infrared Instrument (MIRI) operates in the 5-28μm wavelength range and can be configured for imaging, coronographic imaging, long-slit, low-resolution spectroscopy or medium resolution spectroscopy with an integral field unit. SCASim is one of a suite of simulators which operate together to simulate all the different modes of the instrument. These simulators are essential for the efficient operation of MIRI; allowing more accurate planning of MIRI observations on sky or during the pre-launch testing of the instrument. The data generated by the simulators are essential for testing the data pipeline software. The simulators not only need to reproduce the behaviour of the instrument faithfully, they also need to be adaptable so that information learned about the instrument during the pre-launch testing and in-orbit commissioning can be fed back into the simulation. SCASim simulates the behaviour of the MIRI detectors, taking into account cosmetic effects, quantum efficiency, shot noise, dark current, read noise, amplifier layout, cosmic ray hits, etc... The software has benefited from three major design choices. First, the development of a suite of MIRI simulators, rather than single simulator, has allowed MIRI simulators to be developed in parallel by different teams, with each simulator able to concentrate on one particular area. SCASim provides a facility common to all the other simulators and saves duplication of effort. Second, SCASim has a Python-based object-oriented design which makes it easier to adapt as new information about the instrument is learned during testing. Third, all simulator parameters are maintained in external files, rather than being hard coded in the software. These design choices have made SCASim highly reusable. In its present form it can be used to simulate any JWST detector, and it can be adapted for future instruments with similar, photon-counting detectors.

  6. Some Issues Relating to Children's Questions and Explanations. Learning in Science Project (Primary). Working Paper No. 106.

    Science.gov (United States)

    Biddulph, Fred; Osborne, Roger

    One area explored in the Learning in Science Project (Primary--LISP(P)--was children's questions about and explanations of phenomena. Data were obtained from work with classes of children, interviews with children, informal discussions with teachers, and observations of two teachers using an alternative teaching model (outlined in an appendix)…

  7. Working toward a Continuum of Professional Learning Experiences for Teachers of Science and Mathematics. Research Monograph.

    Science.gov (United States)

    Mundry, Susan; Spector, Barbara; Stiles, Katherine; Loucks-Horsley, Susan

    This monograph is the result of a one-year qualitative study conducted by the National Institute for Science Education (NISE) of reform-oriented interventions, structures, and relationships in preservice and inservice education of teachers of science and mathematics. The study investigated 61 initiatives of reform activity involving teachers of…

  8. Making Interdisciplinary Courses Work with Constructivism and Science, Technology and Society (STS)

    Science.gov (United States)

    Hollenbeck, James E.

    2006-01-01

    Educators expect students to question, explain, hypothesize, and devise tests to determine validity concerning science and its applications. The traditional approach of presenting individual courses concentrating on single disciplines and ignoring linkages to other disciplines is abysmal. If we expect students to understand how science is related…

  9. Students' Roles in Group-Work with Visual Data: A Site of Science Learning

    Science.gov (United States)

    Radinsky, Josh

    2008-01-01

    Learning science includes learning to argue with "inscriptions": images used to symbolize information persuasively. This study examined sixth-graders learning to invest inscriptions with representational status, in a geographic information system (GIS)-based science investigation. Learning to reason with inscriptions was studied in emergent…

  10. An Initial Framework. Learning in Science Project. Working Paper No. 1.

    Science.gov (United States)

    Osborne, Roger; And Others

    The aim of the Learning in Science Project is to: (1) investigate science teaching/learning at the Form 1 to 4 level (ages 10 to 14); (2) identify some of the key difficulties in this subject area; and (3) find ways of overcoming such difficulties. The project is seen both as an evaluative and a research project in that it is concerned with…

  11. Floating and Sinking: First Teacher Trials. Learning in Science Project (Primary). Working Paper No. 120.

    Science.gov (United States)

    Appleton, Ken; And Others

    Two booklets were developed by the Learning in Science Project (Primary)--LISP(P)--to help teachers adopt an approach to primary science teaching which would enhance children's understanding of floating and sinking. Both booklets were designed to enable teachers to reconceptualize their teaching task from activity-driven, didactic teaching to…

  12. Floating and Sinking: Second Teacher Trials. Learning in Science Project (Primary). Working Paper No. 121.

    Science.gov (United States)

    Biddulph, Fred; And Others

    Two booklets were developed by the Learning in Science Project (primary)--LISP(P)--to help teachers adopt an approach to science teaching which would enhance children's understanding of floating and sinking; the strategy enables teachers to reconceptualize their teaching task from activity-driven, didactic teaching to conceptual-change teaching.…

  13. The sociology of scientific work the fundamental relationship between science and society

    CERN Document Server

    Vinck, Dominique

    2010-01-01

    More than ever before, science and technology play a significant role in modern society as evidenced by the development of nanotechnologies and the controversies surrounding GMOs and climate change. This book comprehensively explores the flourishing field of science and technology studies and examines its creation, development and interaction with contemporary society. Dominique Vinck examines the various relationships between science and society including the emergence of sciences, the dynamics of innovation and technical democracy. He also investigates the principal social mechanisms of science and technology such as institutions, organizations, exchanges between researchers and the construction of scientific knowledge, expertise and innovation. The book provides a thorough overview of the field and reviews the major theoretical and methodological approaches as well as the current state of research on a range of topics. This original book will strongly appeal to students and researchers in the social scie...

  14. The relationship between quality of work life and job satisfaction of faculty members in Zahedan University of Medical Sciences.

    Science.gov (United States)

    Kermansaravi, Fatihe; Navidian, Ali; Navabi Rigi, Shahindokht; Yaghoubinia, Fariba

    2014-10-29

    Quality of work life is one of the most important factors for human motivating and improving of job satisfaction. The current study was carried out aimed to determine the relationship between quality of work life and job satisfaction in faculty members of Zahedan University of Medical Sciences. In this descriptive-analytic study, 202 faculty members of Zahedan University of Medical Sciences in 2012 were entered the study through census. The job satisfaction questionnaire of Smith and Kendall and Walton Quality of Work Life questionnaire were used for data collection. Validity and reliability of questionnaires were confirmed in previous studies. Data analysis was done using SPSS 18. The Pearson correlation coefficient and multiple regression tests were used for data analysis. The mean score of quality of work life was 121/30±37/08 and job satisfaction was 135/98 ±33/78. There was a significant and positive correlation between job satisfaction of faculty members and their quality of work life (P=0.003). In addition, two components of quality of work life "adequate and fair compensation" (β=0.3) and "Social Integration" (β=0.4) can predict job satisfaction of faculty members. According to correlation between job satisfaction and quality of work life in faculty members, job satisfaction can be improved through the changing and manipulating the components of quality of work life and in this way; the suitable environment for organization development should be provided.

  15. Working knowledges before and after circa 1800: practices and disciplines in the history of science, technology, and medicine.

    Science.gov (United States)

    Pickstone, John V

    2007-09-01

    Historians of science, inasmuch as they are concerned with knowledges and practices rather than institutions, have tended of late to focus on case studies of common processes such as experiment and publication. In so doing, they tend to treat science as a single category, with various local instantiations. Or, alternatively, they relate cases to their specific local contexts. In neither approach do the cases or their contexts build easily into broader histories, reconstructing changing knowledge practices across time and space. This essay argues that by systematically deconstructing the practices of science and technology and medicine (STM) into common, recurrent elements, we can gain usefully "configurational" views, not just of particular cases and contexts but of synchronic variety and diachronic changes, both short term and long. To this end, we can begin with the customary actors' disciplines of early modern knowledge (natural philosophy, natural history, mixed mathematics, and experimental philosophy), which can be understood as elemental "ways of knowing and working," variously combined and disputed. I argue that these same working knowledges, together with a later mode-synthetic experimentation and systematic invention-may also serve for the analysis of STM from the late eighteenth century to the present. The old divisions continued explicitly and importantly after circa 1800, but they were also "built into" an array of new sciences. This historiographic analysis can help clarify a number of common problems: about the multiplicity of the sciences, the importance of various styles in science, and the relations between science and technology and medicine. It suggests new readings of major changes in STM, including the first and second scientific revolutions and the transformations of biomedicine from the later twentieth century. It offers ways of recasting both microhistories and macrohistories, so reducing the apparent distance between them. And it may thus

  16. Review of Cold war social science: Knowledge production, liberal democracy, and human nature, and Working knowledge: Making the human sciences from Parsons to Kuhn.

    Science.gov (United States)

    Erickson, Paul

    2013-11-01

    Reviews the books, Cold War Social Science: Knowledge Production, Liberal Democracy, and Human Nature by Mark Solovey and Hamilton Cravens (2012) and Working Knowledge: Making the Human Sciences From Parsons to Kuhn by Joel Isaac (see record 2012-13212-000). Taken together, these two important books make intriguing statements about the way to write the histories of fields like psychology, sociology, anthropology, and economics in the Anglo American world during the 20th century. To date, histories of these fields have drawn on a number of fairly well-established punctuation marks to assist in periodization: the shift from interwar institutionalism in economics to postwar neoclassicism, with its physics-like emphasis on mathematical theory-building; the transition from the regnant prewar behaviorism through a postwar "cognitive revolution" in American psychology; and the move in fields like sociology and anthropology away from positivism and the pursuit of what has sometimes been called "grand theory" in the early postwar era toward a period defined by intellectual and political fragmentation, the reemergence of interpretive approaches and a reaction to the scientistic pretensions of the earlier period. These books, by contrast, provide perspectives orthogonal to such existing narrative frameworks by adopting cross-cutting lenses like the "Cold War" and the working practices of researchers in the social and behavioral sciences. As a result, they do much to indicate the value of casting a historiographical net beyond individual disciplines, or even beyond the "social sciences" or the "human sciences" sensu stricto, in the search for deeper patterns of historical development in these fields. (PsycINFO Database Record (c) 2013 APA, all rights reserved).

  17. Titan Science with the James Webb Space Telescope

    Science.gov (United States)

    Nixon, Conor A.; Achterberg, Richard K.; Ádámkovics, Máté; Bézard, Bruno; Bjoraker, Gordon L.; Cornet, Thomas; Hayes, Alexander G.; Lellouch, Emmanuel; Lemmon, Mark T.; López-Puertas, Manuel; Rodriguez, Sébastien; Sotin, Christophe; Teanby, Nicholas A.; Turtle, Elizabeth P.; West, Robert A.

    2016-01-01

    The James Webb Space Telescope (JWST), scheduled for launch in 2018, is the successor to the Hubble Space Telescope (HST) but with a significantly larger aperture (6.5 m) and advanced instrumentation focusing on infrared science (0.6-28.0 μm). In this paper, we examine the potential for scientific investigation of Titan using JWST, primarily with three of the four instruments: NIRSpec, NIRCam, and MIRI, noting that science with NIRISS will be complementary. Five core scientific themes are identified: (1) surface (2) tropospheric clouds (3) tropospheric gases (4) stratospheric composition, and (5) stratospheric hazes. We discuss each theme in depth, including the scientific purpose, capabilities, and limitations of the instrument suite and suggested observing schemes. We pay particular attention to saturation, which is a problem for all three instruments, but may be alleviated for NIRCam through use of selecting small sub-arrays of the detectors—sufficient to encompass Titan, but with significantly faster readout times. We find that JWST has very significant potential for advancing Titan science, with a spectral resolution exceeding the Cassini instrument suite at near-infrared wavelengths and a spatial resolution exceeding HST at the same wavelengths. In particular, JWST will be valuable for time-domain monitoring of Titan, given a five- to ten-year expected lifetime for the observatory, for example, monitoring the seasonal appearance of clouds. JWST observations in the post-Cassini period will complement those of other large facilities such as HST, ALMA, SOFIA, and next-generation ground-based telescopes (TMT, GMT, EELT).

  18. Municipal consultants’ participation in building networks to support science teachers’ work

    DEFF Research Database (Denmark)

    Sillasen, Martin Krabbe; Valero, Paola

    2013-01-01

    This paper focuses particularly on the role of municipal science consultants in developing and maintaining network activities and connections among primary school science teachers. The hypothesis is that consultants play a crucial role in supporting strategic planning, and sustaining contacts...... and activities within professional learning networks. The research is framed by a project that involved 80 primary science teachers in 20 schools. The aim of the project was to develop network activities that facilitate sustainable change of the participating schools’ collective culture and practice of science...... teaching. The authors were involved as researchers and evaluators in the project. Data consist of reports from the consultants about their participation in various network activities, school assessment reports and a longitudinal survey. Three distinct cases are analysed through the use of a framework...

  19. Possibilities, misunderstandings and limits in the work of the teacher/researcher in science education

    Directory of Open Access Journals (Sweden)

    Maria José P.M.de Almeida

    1996-08-01

    Full Text Available This paper presents fragments of the research “Individualized ‘Supletivo’: Possibilities, Misunderstandings, and Limits in Science Teaching”, which emphasized the student/teacher and student/instructional materials relationships, as well as the analysis of changes in the pedagogical practice, in the area of sciences, in an adult education course. The focus of this presentation is the trajectory of the teacher/researcher who proposed and conducted this research.

  20. Evidence-based creativity: Working between art and science in the field of fine dining.

    Science.gov (United States)

    Borkenhagen, Chad

    2017-08-01

    This article examines how scientific knowledge drives creativity in the small but influential culinary movement of 'modernist cuisine'. Originating in the mid-1990s, modernist cuisine began with a small group of avant-garde chefs using science to produce wildly innovative culinary creations. Since then, many of the movement's innovations, as well as its more general 'science-based' approach to cooking, have gained adoption among a diverse range of culinary professionals. But while science has enabled modernist chefs to produce a wide array of innovations and refinements, the group's embrace of scientific values poses a potential threat to the subjective, intuition-driven logic of culinary creativity. Using data gathered through interviews and participant observation, I describe how modernist chefs navigate the potential challenges of using science in a creative field. I find that advocates of modernist cuisine address these challenges by adopting two separate rhetorical repertoires - one emphasizing science-based cooking's advantages over traditional methods, and another that minimizes the differences between these approaches. Observing the strategic deployment of these repertoires illustrates the challenges to incorporating science into creative fields and reveals a complex and nuanced relationship between objectivity, evidence, and aesthetic judgement.

  1. Working with the nature of science in physics class: turning ‘ordinary’ classroom situations into nature of science learning situations

    Science.gov (United States)

    Hansson, Lena; Leden, Lotta

    2016-09-01

    In the science education research field there is a large body of literature on the ‘nature of science’ (NOS). NOS captures issues about what characterizes the research process as well as the scientific knowledge. Here we, in line with a broad body of literature, use a wide definition of NOS including also e.g. socio-cultural aspects. It is argued that NOS issues, for a number of reasons, should be included in the teaching of science/physics. Research shows that NOS should be taught explicitly. There are plenty of suggestions on specific and separate NOS activities, but the necessity of discussing NOS issues in connection to specific science/physics content and to laboratory work, is also highlighted. In this article we draw on this body of literature on NOS and science teaching, and discuss how classroom situations in secondary physics classes could be turned into NOS-learning situations. The discussed situations have been suggested by secondary teachers, during in-service teacher training, as situations from every-day physics teaching, from which NOS could be highlighted.

  2. Educating elementary-aged English learners in science: Scientists and teachers working together

    Science.gov (United States)

    Banuelos, Gloria Rodriguez

    California's K-12 schools contain 40% of the nation's English learners, the majority of them enrolled at the elementary level. Traditionally, English learners in California have difficulty performing at the same level as their native English speaking counterparts on national achievement tests, such as the National Assessment of Educational Progress. In 1998, California voters passed Proposition 227 mandating that English learners be taught "overwhelmingly" in English, thus making teachers, many without expertise, responsible for teaching multilevel English proficient students subject matter. I studied the use of scientist-teacher partnerships as a resource for teachers of English learners. University scientists (graduate students) partnered with local elementary school teachers designed and implemented integrated science and English lessons for classrooms with at least 30% English learners. The study explored two major foci. First, integrated science and language lessons implemented by six scientist-teacher partnerships were investigated. Second, the responsibilities taken on by the team members during the implementation of integrated science and language lessons were examined. Three data sources were analyzed: (1) six lesson sequences comprised of 28 lessons; (2) 18 lesson worksheet; and (3) 24 participant Retrospective interview transcripts (12 scientists and 12 teachers). Lessons across were examined according to four analytical categories which included the following: (1) nature of the science activities (e.g. hands-on); nature of language activities (e.g. speaking); (2) nature of instructional practices (e.g. student grouping); and (3) responsibilities of teachers and scientists (e.g. classroom). A micro level analysis illustrates how one scientist-teacher team innovatively used a children's story, Goldilocks and the Three Bears, to teach the measurement of length and temperature. A macro level analysis identified three characteristics of science activities

  3. Large Volume, Optical and Opto-Mechanical Metrology Techniques for ISIM on JWST

    Science.gov (United States)

    Hadjimichael, Theo

    2015-01-01

    The final, flight build of the Integrated Science Instrument Module (ISIM) element of the James Webb Space Telescope is the culmination of years of work across many disciplines and partners. This paper covers the large volume, ambient, optical and opto-mechanical metrology techniques used to verify the mechanical integration of the flight instruments in ISIM, including optical pupil alignment. We present an overview of ISIM's integration and test program, which is in progress, with an emphasis on alignment and optical performance verification. This work is performed at NASA Goddard Space Flight Center, in close collaboration with the European Space Agency, the Canadian Space Agency, and the Mid-Infrared Instrument European Consortium.

  4. Characterization of the JWST Pathfinder Mirror Dynamics Using the Center of Curvature Optical Assembly (CoCOA)

    Science.gov (United States)

    Wells, C.; Hadaway, J.; Olczak, G.; Cosentino, J.; Johnston, J.; Whitman, T.; Connolly, M.; Chaney, D.; Knight, J.; Telfer, R.

    2016-01-01

    The JWST (James Webb Space Telescope) Optical Telescope Element (OTE) consists of a 6.6 meter clear aperture, 18-segment primary mirror, all-reflective, three-mirror anastigmat operating at cryogenic temperatures. To verify performance of the primary mirror, a full aperture center of curvature optical null test is performed under cryogenic conditions in Chamber A at NASA Johnson Space Center using an instantaneous phase measuring interferometer. After phasing the mirrors during the JWST Pathfinder testing, the interferometer is utilized to characterize the mirror relative piston and tilt dynamics under different facility configurations. The correlation between the motions seen on detectors at the focal plane and the interferometer validates the use of the interferometer for dynamic investigations. The success of planned test hardware improvements will be characterized by the multi-wavelength interferometer (MWIF) at the Center of Curvature Optical Assembly (CoCOA).

  5. Characterization of the JWST Pathfinder mirror dynamics using the center of curvature optical assembly (CoCOA)

    Science.gov (United States)

    Wells, Conrad; Hadaway, James B.; Olczak, Gene; Cosentino, Joseph; Johnston, John D.; Whitman, Tony; Connolly, Mark; Chaney, David; Knight, J. Scott; Telfer, Randal

    2016-07-01

    The James Webb Space Telescope (JWST) Optical Telescope Element (OTE) consists of a 6.6 m clear aperture, 18 segment primary mirror, all-reflective, three-mirror anastigmat operating at cryogenic temperatures. To verify performance of the primary mirror, a full aperture center of curvature optical null test is performed under cryogenic conditions in Chamber A at the National Aeronautics and Space Administration (NASA) Johnson Space Center (JSC) using an instantaneous phase measuring interferometer. After phasing the mirrors during the JWST Pathfinder testing, the interferometer is utilized to characterize the mirror relative piston and tilt dynamics under different facility configurations. The correlation between the motions seen on detectors at the focal plane and the interferometer validates the use of the interferometer for dynamic investigations. The success of planned test hardware improvements will be characterized by the multi-wavelength interferometer (MWIF) at the Center of Curvature Optical Assembly (CoCOA).

  6. The Potential Improvement of Team-Working Skills in Biomedical and Natural Science Students Using a Problem-Based Learning Approach

    Science.gov (United States)

    Nowrouzian, Forough L.; Farewell, Anne

    2013-01-01

    Teamwork has become an integral part of most organisations today, and it is clearly important in Science and other disciplines. In Science, research teams increase in size while the number of single-authored papers and patents decline. Team-work in laboratory sciences permits projects that are too big or complex for one individual to be tackled.…

  7. Performance of the primary mirror center-of-curvature optical metrology system during cryogenic testing of the JWST Pathfinder telescope

    Science.gov (United States)

    Hadaway, James B.; Wells, Conrad; Olczak, Gene; Waldman, Mark; Whitman, Tony; Cosentino, Joseph; Connolly, Mark; Chaney, David; Telfer, Randal

    2016-07-01

    The James Webb Space Telescope (JWST) primary mirror (PM) is 6.6 m in diameter and consists of 18 hexagonal segments, each 1.5 m point-to-point. Each segment has a six degree-of-freedom hexapod actuation system and a radius of-curvature (RoC) actuation system. The full telescope will be tested at its cryogenic operating temperature at Johnson Space Center. This testing will include center-of-curvature measurements of the PM, using the Center-of-Curvature Optical Assembly (COCOA) and the Absolute Distance Meter Assembly (ADMA). The COCOA includes an interferometer, a reflective null, an interferometer-null calibration system, coarse and fine alignment systems, and two displacement measuring interferometer systems. A multiple-wavelength interferometer (MWIF) is used for alignment and phasing of the PM segments. The ADMA is used to measure, and set, the spacing between the PM and the focus of the COCOA null (i.e. the PM center-of-curvature) for determination of the ROC. The performance of these metrology systems was assessed during two cryogenic tests at JSC. This testing was performed using the JWST Pathfinder telescope, consisting mostly of engineering development and spare hardware. The Pathfinder PM consists of two spare segments. These tests provided the opportunity to assess how well the center-of-curvature optical metrology hardware, along with the software and procedures, performed using real JWST telescope hardware. This paper will describe the test setup, the testing performed, and the resulting metrology system performance. The knowledge gained and the lessons learned during this testing will be of great benefit to the accurate and efficient cryogenic testing of the JWST flight telescope.

  8. Municipal consultants’ participation in building networks to support science teachers’ work

    DEFF Research Database (Denmark)

    Sillasen, Martin Krabbe; Valero, Paola

    2013-01-01

    of professional learning networks to assess the consultants’ opportunities and constraints in terms of participating in network development. The results indicate that the consultants’ roles in successful network formation is characterized by personal stable contacts within the science teacher community......This paper focuses particularly on the role of municipal science consultants in developing and maintaining network activities and connections among primary school science teachers. The hypothesis is that consultants play a crucial role in supporting strategic planning, and sustaining contacts...... teaching. The authors were involved as researchers and evaluators in the project. Data consist of reports from the consultants about their participation in various network activities, school assessment reports and a longitudinal survey. Three distinct cases are analysed through the use of a framework...

  9. Secure Grid Services for Cooperative Work in Medicine and Life Science

    Science.gov (United States)

    Weisbecker, Anette; Falkner, Jürgen

    MediGRID provides a grid infrastructure to solve challenging problems in medical and life sciences by enhancing the productivity and by enabling locationindependent, interdisciplinary collaboration. The usage of grid technology has enabled the development of new application and services for research in medical and life sciences. In order to enlarge the range of services and to get a broader range of users sustainable business models are needed. In Services@MediGRID methods for monitoring, accounting, and billing which fulfilled the high security demands within medicine and life sciences will be developed. Also different requirements of academic and industrial grid customers are considered in order to establish the sustainable business models for grid computing.

  10. Bridging Social Innovation and Social Work: Balancing Science, Values, and Speed

    Science.gov (United States)

    Halvorsen, Cal J.

    2017-01-01

    This article highlights how the social work academy can support innovative research, dissemination, and implementation and is a response to and extension of arguments made by Dr. Marilyn L. Flynn on innovation in social work. It argues that social work researchers need to strike a balance between the often slow and methodical scientific research…

  11. Bridging Social Innovation and Social Work: Balancing Science, Values, and Speed

    Science.gov (United States)

    Halvorsen, Cal J.

    2017-01-01

    This article highlights how the social work academy can support innovative research, dissemination, and implementation and is a response to and extension of arguments made by Dr. Marilyn L. Flynn on innovation in social work. It argues that social work researchers need to strike a balance between the often slow and methodical scientific research…

  12. Relationship between work - family conflict and marital satisfaction among nurses and midwives in hospitals of Zabol university of medical sciences

    Directory of Open Access Journals (Sweden)

    A. Mansouri

    2016-08-01

    Full Text Available Background: Work-family conflicts described as incompatibility between work and family roles. There is mutual relationship between marital satisfaction and job so that the tension in one of two areas of career and family are affected. Objective: To examine the relationship between marital satisfaction and work-family conflict among nurses and midwives. Methods: All of 289 employees of married nursing and midwifery of Zabol University of Medical Sciences hospitals participated in the study in 2014. The data were collected with questionnaires of Enrich marital satisfaction and Carlson work-family conflict and were analyzed with statistical tests including Pearson correlation coefficient, t-test and linear regression analysis. Findings: Marital satisfaction score of the staff was 168.52 which indicates the relative satisfaction of spouses from each other. The mean score of work-family conflict among employees was 3.26; it can be said that employees in terms of work-family conflict, the conflict a moderate experience. There is a significant negative correlation among marital satisfaction and work-family conflict of employees. In fact, marital satisfaction decreases when the conflict between work and family is decreased. Nursing staffs have a higher marital satisfaction and in terms of work-family conflict they experience less conflict. Conclusion: According to the findings, the managers should create conditions that minimize the role conflicts and consequently increase the level of marital satisfaction.

  13. Exploring for Galaxies in the First Billion Years with Hubble and Spitzer - Pathfinding for JWST

    Science.gov (United States)

    Illingworth, Garth D.

    2017-01-01

    Hubble has revolutionized the field of distant galaxies through its deep imaging surveys, starting with the Hubble Deep Field (HDF) in 1995. That first deep survey revealed galaxies at redshift z~1-3 that provided insights into the development of the Hubble sequence. Each new HST instrument has explored new regimes, through the peak of star formation at z~2-3, just 2-3 billion years after the Big Bang, to our first datasets at a billion years at z~6, and then earlier to z~11. HST's survey capabilities were enhanced by 40X with ACS, and then similarly with the WFC3/IR, which opened up the first billion years to an unforeseen degree. I will discuss what we have learned from the remarkable HST and Spitzer imaging surveys (HUDF, GOODS, HUDF09/12 and CANDELS), as well as surveys of clusters like the Hubble Frontier Fields (HFF). Lensing clusters provide extraordinary opportunities for characterizing the faintest earliest galaxies, but also present extraordinary challenges. Together these surveys have resulted in the measurement of the volume density of galaxies in the first billion years down to astonishingly faint levels. The role of faint galaxies in reionizing the universe is still much-discussed, but there is no doubt that such galaxies contribute greatly to the UV ionizing flux, as shown by deep luminosity function studies. Together Hubble and Spitzer have also established the stellar-mass buildup over 97% of cosmic history. Yet some of the greatest surprises have come from the discovery of very luminous galaxies at z~8-11, around 400-650 million years after the Big Bang. Spectroscopic followup by Keck of some of these very rare, bright galaxies has confirmed redshifts from z~7 to z~9, and revealed, surprisingly, strong Lyα emission near the peak of reionization when the HI fraction in the IGM is high. The recent confirmation of a z=11.1 galaxy, just 400 million years after the Big Bang, by a combination of Hubble and Spitzer data, moved Hubble into JWST territory

  14. How should we prepare rehabilitation sciences students to work with low English-proficient Spanish-speaking patients?

    Science.gov (United States)

    Summers, Connie; Gonzalez, Eugenia; Pechak, Celia

    2015-01-01

    Misinterpretations or lack of compliance with national standards established to guide health professionals working with low-English-proficient (LEP) patients continue to negatively impact patient care. Most of the literature on training health professionals to work with interpreters focuses on physicians. We reviewed this current literature and propose an interprofessional educational module to extend the interpreter training to other health professions. Our module trains rehabilitation science students from different health disciplines (physical therapy, occupational therapy, and speech-language pathology) using strategies from the literature. The educational module is tailored to student's bilingual proficiency, suggests relevant outcomes measures, and highlights unanswered questions and areas for future research.

  15. Science-based prevention through communities that care: a model of social work practice for public health.

    Science.gov (United States)

    Haggerty, Kevin P; Shapiro, Valerie B

    2013-01-01

    This article describes a public health orientation to drug and alcohol abuse prevention; reviews the state of the science underlying a risk and protective factor approach to alcohol and drug abuse prevention; describes Communities That Care, a community practice model that makes use of this evidence; and considers how this model reflects four important principles of social work practice. The intent of this article is to provide guidance to social workers who support the National Association of Social Work's intention to make prevention practice central to the provision of alcohol and drug abuse services by social workers.

  16. From an Idea to a Working Robot Prototype: Distributing Knowledge of Robotics through Science Museum Workshops

    Science.gov (United States)

    Polishuk, Alexander; Verner, Igor; Mir, Ronen

    This paper presents our experience of teaching robotics to primary and middle school students at the Gelfand Center for Model Building, Robotics & Communication which is part of the Israel National Museum of Science, Technology and Space (MadaTech). The educational study examines the value and characteristics of students’ teamwork in the museum robotics workshops.

  17. Toward a Social Practice Perspective on the Work of Reading Inscriptions in Science Texts

    Science.gov (United States)

    Pozzer-Ardenghi, Lilian; Roth, Wolff-Michael

    2010-01-01

    In the social studies of science, visuals and graphical representations are theorized by means of the concept of inscription, a term that denotes all representations other than text inscribed in some medium including graphs, tables, photographs, and equations. Inscriptions constitute an intrinsic and integral part of scientific practice; their…

  18. Improving farm animal welfare : science and society working together: the welfare quality approach

    NARCIS (Netherlands)

    Blokhuis, H.J.; Miele, M.; Veissier, I.; Jones, B.

    2013-01-01

    How do you define the quality of life of a farmed animal? This book addresses the complex and often controversial issues surrounding the assessment and improvement of farm animal welfare. It discusses the relevance of science based welfare assessments and the importance of establishing a fruitful

  19. Working with Gifted Science Students in a Public High School Environment: One School's Approach

    Science.gov (United States)

    Ngoi, Mephie; Vondracek, Mark

    2002-01-01

    The Chemistry/Physics Program at Evanston Township High School was designed to provide an environment for the rigorous teaching of advanced science and mathematics to accelerated students. This type of student makes up the bulk of students in the Advanced Placement Chemistry and Physics classes. However, there is a small number of students who…

  20. Pupils' Ideas about Flowering Plants. Learning in Science Project (Primary). Working Paper No. 125.

    Science.gov (United States)

    Biddulph, Fred

    The Learning in Science Project (Primary)--LISP(P)--investigated the ideas and interests children have about flowering plants (in particular whether these plants have a life cycle). Data were obtained from: individual interviews with children, ages 7- to 14-year-old (10 students for each age level), using the "interview-about-instances"…

  1. How Science Really Works: The Student Experience of Research-Led Education

    Science.gov (United States)

    Smyth, Lillian; Davila, Federico; Sloan, Thomas; Rykers, Ellen; Backwell, Sam; Jones, Stephen B.

    2016-01-01

    There has been a shift in modern tertiary education theory that has moved away from a traditional, didactic model of education, towards a more student-led, constructivist approach. Nowhere is this more the case than in science and mathematical education, where the concept of research-led education is gaining more and more traction. The focus of…

  2. Pupils' Views about Spiders. Learning in Science Project (Primary). Working Paper No. 123.

    Science.gov (United States)

    Hawe, Eleanor

    The Learning in Science Project (Primary)--LISP(P)--investigated the ideas and interests about spiders held by 8- to 10-year-old children. Data included 303 questions--and answers to some of the questions--about spiders obtained from children in four classes and from responses obtained during individual interviews with 10 children from each age…

  3. Explaining how the mind works: on the relation between cognitive science and philosophy.

    Science.gov (United States)

    Trigg, Jonathan; Kalish, Michael

    2011-04-01

    In this paper, we argue that under certain prevalent interpretations of the nature and aims of cognitive science, theories of cognition generate a forced choice between a conception of cognition which depends on the possibility of a private language, and a conception of cognition which depends on mereological confusions. We argue, further, that this should not pose a fundamental problem for cognitive scientists since a plausible interpretation of the nature and aims of cognitive science is available that does not generate this forced choice. The crucial difference between these interpretations is that on the one hand the aim of theories of cognition is to tell us what thinking (etc.) is, and on the other it is to tell us what is causally necessary if an intelligent creature is to be able to think. Our argument draws heavily on a Wittgensteinian conception of philosophy in which no philosophical theory can explain what thinking, perceiving, remembering, etc. are, either. The positive, strictly therapeutic, purpose of a philosophy of cognitive science should be to show that, since the traditional problems which constitute the philosophy of mind are chimerical, there is nothing for philosophical theorizing in cognitive science to achieve.

  4. Video: Floating and Sinking. Learning in Science Project (Primary). Working Paper No. 115.

    Science.gov (United States)

    Osborne, Roger

    This paper, designed to be used in conjunction with a video-tape developed by the Learning in Science Project (Primary)--LISP(P)--shows excerpts from some of the interview schedules used to examine children's ideas about floating and sinking. These interviews involved the use of "interview-about-instances" (IAI) cards (included in an…

  5. Primary School Pupils' Ideas about Rocks. Learning in Science Project (Primary). Working Paper No. 107.

    Science.gov (United States)

    Symington, David; And Others

    The Learning in Science Project (Primary)--LISP(P)--investigated the questions and explanations primary children have about rocks. Data were collected during teaching sessions from New Zealand students (ages 8-11) and Australian students (ages 10-11). The teaching sessions required the teacher to create a situation in which children generated some…

  6. Pupils' Ideas about Flowering Plants. Learning in Science Project (Primary). Working Paper No. 125.

    Science.gov (United States)

    Biddulph, Fred

    The Learning in Science Project (Primary)--LISP(P)--investigated the ideas and interests children have about flowering plants (in particular whether these plants have a life cycle). Data were obtained from: individual interviews with children, ages 7- to 14-year-old (10 students for each age level), using the "interview-about-instances"…

  7. Children's Ideas about "Metals." Learning in Science Project (Primary). Working Paper No. 112.

    Science.gov (United States)

    Biddulph, Fred; Osborne, Roger

    The topic of metals is frequently taught in primary schools. However, when metals are suggested as one of a series of topics for study, students often initially show little enthusiasm for the topic. To determine the ideas that children have about metals the Learning in Science Project (Primary)--LISP(P)--interviewed thirty-eight 9- to 10-year-old…

  8. Primary School Childrens' Ideas about Spiders. Learning in Science Project (Primary). Working Paper No. 108.

    Science.gov (United States)

    Biddulph, Fred

    The Learning in Science Project (Primary)--LISP(P)--investigated the questions and explanations primary children have about spiders. The data comprise 112 questions and 104 explanations (included in appendices) offered by children after being shown a picture of a spider. Additional data were collected during individual interviews with 18 students.…

  9. Children's Ideas about Hot and Cold. Learning in Science Project (Primary). Working Paper No. 127.

    Science.gov (United States)

    Appleton, Ken

    The Learning in Science Project (Primary)--LISP(P)--investigated the ideas and interests children have about hot and cold. Data were obtained from 25 children (12 boys and 13 girls), ages 8 to 11, using the "interview-about-instances" (IAI) procedure. Areas investigated included: (1) the meanings of the words…

  10. The Effective Use of Management Science in University Administration. Working Paper No. 9.

    Science.gov (United States)

    Schroeder, Roger G.; Adams, Carl R.

    Most college administrators are anxious to make use of management science techniques to assist them in operating their organizations. Despite their positive attitude, however, these administrators seem to lack a systematic method of approaching their specific organizations to decide which areas of application and what techniques should be…

  11. Investigation of the Relationship Between Mental Health and Organizational Employees’ work Fatigue and Deputyships of Yasouj Medical Science University

    Directory of Open Access Journals (Sweden)

    A Mahmoodi

    2015-08-01

    Full Text Available Background & aim: Peoples’ mental health in improvement of society’s national and ideal aims have the main and most importance such as thriftiness in material and spiritual costs. Work fatigue is the result of severe decrease of person’s capabilities sources that counter with long –time stress, especially work stress. This study was designed with the aim of investigating the relationship between mental health and work fatigue at Yasuj University of Medical Sciences. Method of investigation: The present co-operation – descriptive study was conducted on 274 participants from 961 organization employees and deputyships of Yasuj University of Medical Sciences in 2013-2014 who were chosen randomly. In order to collect data, Maslach questionnaire of mental health condition and work fatigue was used. Data were analysed with statistical tests of the interconnection index Pearson and Friedman’s test. Findings: There was no significant relationship between mental health and work fatigue dimensions (p<0/05. A meaningful relationship was observed between studied models after usage. High attention and metamorphosis of personality had the least importance. Conclusion: When employees have full mental health and job satisfaction, the ability to achieve maximum efficiency in the organization is reachable.

  12. Using interactive family science shows to improve public knowledge on antibiotic resistance: does it work?

    Science.gov (United States)

    Lecky, Donna M; Hawking, Meredith K D; Verlander, Neville Q; McNulty, Cliodna A M

    2014-01-01

    The public plays an important role in controlling the emergence and spread of antibiotic resistance. A large British survey showed that there is still public misunderstanding about microbes and antibiotics. e-Bug, a European DG Sanco sponsored project, aims to disseminate a school antibiotic and hygiene educational pack and website across Europe. Interactive science shows based on the e-Bug educational packs were developed to take the key health and hygiene messages from the e-Bug school resources to families. The science show was evaluated to assess public knowledge and understanding of antibiotics and antibiotic resistance pre and post intervention. An interactive stall comprised of a 3×2 m backing stand with background information, an interactive activity and discussions with a trained demonstrator was on display at a family holiday resort. Pre-piloted knowledge questionnaires were completed by parents and children pre and post intervention. Adult (≥19 years) baseline knowledge regarding antibiotics and antibiotic resistance was high although significant knowledge improvement was observed where baseline knowledge was low. Children's (5-11 years) knowledge around antibiotics and antibiotic resistance was significantly improved for all questions. The science show can be viewed as a success in improving parents' and children's knowledge of antibiotic use thereby highlighting the importance of educating the public through interaction.

  13. Using interactive family science shows to improve public knowledge on antibiotic resistance: does it work?

    Directory of Open Access Journals (Sweden)

    Donna M Lecky

    Full Text Available The public plays an important role in controlling the emergence and spread of antibiotic resistance. A large British survey showed that there is still public misunderstanding about microbes and antibiotics. e-Bug, a European DG Sanco sponsored project, aims to disseminate a school antibiotic and hygiene educational pack and website across Europe. Interactive science shows based on the e-Bug educational packs were developed to take the key health and hygiene messages from the e-Bug school resources to families. The science show was evaluated to assess public knowledge and understanding of antibiotics and antibiotic resistance pre and post intervention. An interactive stall comprised of a 3×2 m backing stand with background information, an interactive activity and discussions with a trained demonstrator was on display at a family holiday resort. Pre-piloted knowledge questionnaires were completed by parents and children pre and post intervention. Adult (≥19 years baseline knowledge regarding antibiotics and antibiotic resistance was high although significant knowledge improvement was observed where baseline knowledge was low. Children's (5-11 years knowledge around antibiotics and antibiotic resistance was significantly improved for all questions. The science show can be viewed as a success in improving parents' and children's knowledge of antibiotic use thereby highlighting the importance of educating the public through interaction.

  14. Slitless spectroscopy with the James Webb Space Telescope Near-Infrared Camera (JWST NIRCam)

    CERN Document Server

    Greene, Thomas P; Egami, Eiichi; Hodapp, Klaus W; Kelly, Douglas M; Leisenring, Jarron; Rieke, Marcia; Robberto, Massimo; Schlawin, Everett; Stansberry, John

    2016-01-01

    The James Webb Space Telescope near-infrared camera (JWST NIRCam) has two 2.'2 $\\times$ 2.'2 fields of view that are capable of either imaging or spectroscopic observations. Either of two $R \\sim 1500$ grisms with orthogonal dispersion directions can be used for slitless spectroscopy over $\\lambda = 2.4 - 5.0$ $\\mu$m in each module, and shorter wavelength observations of the same fields can be obtained simultaneously. We present the latest predicted grism sensitivities, saturation limits, resolving power, and wavelength coverage values based on component measurements, instrument tests, and end-to-end modeling. Short wavelength (0.6 -- 2.3 $\\mu$m) imaging observations of the 2.4 -- 5.0 $\\mu$m spectroscopic field can be performed in one of several different filter bands, either in-focus or defocused via weak lenses internal to NIRCam. Alternatively, the possibility of 1.0 -- 2.0 $\\mu$m spectroscopy (simultaneously with 2.4 -- 5.0 $\\mu$m) using dispersed Hartmann sensors (DHSs) is being explored. The grisms, wea...

  15. A model-based approach to the spatial and spectral calibration of NIRSpec onboard JWST

    CERN Document Server

    Dorner, Bernhard; Ferruit, Pierre; de Oliveira, Catarina Alves; Birkmann, Stephan M; Böker, Torsten; De Marchi, Guido; Gnata, Xavier; Köhler, Jess; Sirianni, Marco; Jakobsen, Peter

    2016-01-01

    Context: The NIRSpec instrument for the James Webb Space Telescope (JWST) can be operated in multiobject (MOS), long-slit, and integral field (IFU) mode with spectral resolutions from 100 to 2700. Its MOS mode uses about a quarter of a million individually addressable minislits for object selection, covering a field of view of $\\sim$9 $\\mathrm{arcmin}^2$. Aims: The pipeline used to extract wavelength-calibrated spectra from NIRSpec detector images relies heavily on a model of NIRSpec optical geometry. We demonstrate how dedicated calibration data from a small subset of NIRSpec modes and apertures can be used to optimize this parametric model to the necessary levels of fidelity. Methods: Following an iterative procedure, the initial fiducial values of the model parameters are manually adjusted and then automatically optimized, so that the model predicted location of the images and spectral lines from the fixed slits, the IFU, and a small subset of the MOS apertures matches their measured location in the main o...

  16. Views of Sport Science Graduates Regarding Work Skills Developed at University

    Science.gov (United States)

    Sleap, Mike; Reed, Helen

    2006-01-01

    There has been recent interest in how higher education might improve the employability of students, although there is little feedback from graduates about the value of university experiences to their working life. The aim of the study therefore was to investigate the views of graduates regarding the extent to which work skills had been developed…

  17. Teacher Interventions in Small Group Work in Secondary Mathematics and Science Lessons

    Science.gov (United States)

    Hofmann, R.; Mercer, N.

    2016-01-01

    Collaborative problem solving, when students work in pairs or small groups on a curriculum-related task, has become an increasingly common feature of classroom education. This paper reports a study of a topic which has received relatively little attention: how teachers can most usefully intervene when students are working in a group, but have…

  18. Defining the public, defining sociology: hybrid science-public relations and boundary-work in early American sociology.

    Science.gov (United States)

    Evans, Michael S

    2009-01-01

    In this paper, I examine how scientific disciplines define their boundaries by defining the publics with whom they engage. The case study is an episode in the development of early American sociology. In response to the dual challenge of credibility set up by the conflict between religious Baconian science and secular positivist science, key actors engaged in specific strategies of boundary-work to create their desired "sociological public"--a hybrid form of science-public relations that appealed to hostile university scientists while excluding a supportive religious audience from participation in the production of scientific knowledge. Using this case, I offer two specific insights. First I illustrate how, in the pursuit of scientific credibility, actors engage in boundary-work to differentiate audiences, not just practitioners. Such defining of publics is constitutive of scientific disciplines in their formative stage. Second, I demonstrate how audience boundaries can be redefined through the capture of existing boundary objects. Specifically, the removal of informational content in key boundary objects creates durable boundaries that are difficult to overcome.

  19. Racing for What? Anticipation and Acceleration in the Work and Career Practices of Academic Life Science Postdocs

    Directory of Open Access Journals (Sweden)

    Ruth Müller

    2014-09-01

    Full Text Available In the wake of contemporary new public management, the temporalities of academic work have undergone significant transformations. One key feature of these changes is a perceived acceleration of working pace. While this phenomenon is widely acknowledged in scholarship about the transforming universities, to date there are only few studies investigating its empirical details. Building on qualitative interviews with 38 postdoctoral life scientists in Austria, this article investigates how these researchers experience the temporalities of their work and career practices. Postdocs are particularly susceptible to the changing demands of academic work life, as they mostly inhabit fragile institutional positions while they aspire to establish themselves in academia. The experience of being in a highly competitive race that requires a continuously accelerating working pace as well as a strong focus on individual achievement is central to their narratives about working for a career in academia. Drawing on recent scholarship on anticipation (ADAMS, MURPHY & CLARKE, 2009, acceleration (ROSA, 2003 and the entrepreneurial self (BRÖCKLING, 2007, I develop the concepts of anticipatory acceleration and latent individualization to analytically capture postdocs' experiences of temporalities in the context of their work and career practices. In conclusion I discuss the possible impacts of these particular temporal orientations for the contents and formats of academic knowledge production and ask in how far concepts and movements such as "slow science" help to address effects and problems of these specific forms of acceleration and anticipation. URN: http://nbn-resolving.de/urn:nbn:de:0114-fqs1403150

  20. Science in and out of the classroom: A look at Water Resource at Gammams Water Care Works, Namibia

    Science.gov (United States)

    Iileka-Shinavene, Leena

    2016-04-01

    Primary school pupils in Van Rhyn School in Namibia are taught Natural Sciences from grade 4 at the age of 9. The curriculum is mainly theory/classroom based and natural science is taught through theory and various practical activities. However occasionally teachers have opportunities to supplement the pupils' learning experience through outdoor activities such as excursions to museums, municipal works and science fairs. Apart from enhancing the learning experience and improving understanding, such activities make the Natural science subject more interesting subject to learners. Water, a scarce/limited resource in Namibia, is one of the topics we cover in Natural sciences. Sustainable management of water is one of the top priorities of the government, which through various initiatives including the National Development Plan supports innovative ideas and technologies to reclaim water from sewage, recycling of industry and mining water and use semi-purified water for public recreational places. Most of the water used in Windhoek is reclaimed by City of Windhoek. To better illustrate this to the pupils, a school trip with 40 pupils of seventh grade was taken to the City of Windhoek's Gammams Water Care works. The aim of the trip was to show how the sewage purification process works and how the water is reclaimed from sewage. A guided tour of the water works was given by the resident scientists and the pupils were provided with the worksheet to complete after the tour around the Centre. They were encouraged to ask questions in all stages of water purification process and write down short notes. Most learners completed their worksheet during the tour session as they are getting information from the tour guide. The rest had to retrieve information and do further research as they got back to class so they could complete their worksheets. After the tour to Gammams, learners were asked to share what they had learned with the lower grades, 5 and 6, in a classroom

  1. Simulations suggest that social and natural sciences differ in their research strategies adapted to work for different knowledge landscapes

    CERN Document Server

    Jaffe, Klaus

    2014-01-01

    Do different field of knowledge require different research strategies? A numerical model exploring different virtual knowledge landscapes, revealed different optimal search strategies. Trend following is maximized when the popularity of new discoveries determine the number of individuals researching it. This strategy works best when many researchers explore few large areas of knowledge. In contrast, individuals or small groups of researchers are better in discovering small bits of information in dispersed knowledge landscapes. The best technique for all situations simulated, is to adjust the number of researchers needed to explore a knowledge cluster according to the opportunities and the level of crowding in that cluster. Bibliometric data of scientific publications showed a continuous bipolar distribution of these strategies, ranging from natural sciences, with highly cited publications in journals containing a large number of articles, to the social sciences, with rarely cited publications in journals cont...

  2. Polar communications: Status and recommendations. Report of the Science Working Group

    Science.gov (United States)

    Rosenberg, T. J. (Editor); Jezek, K. C. (Editor)

    1987-01-01

    The capabilities of the existing communication links within the polar regions, as well as between the polar regions and the continental United States, are summarized. These capabilities are placed in the context of the principal scientific disciplines that are active in polar research, and in the context of how scientists both utilize and are limited by present technologies. Based on an assessment of the scientific objectives potentially achievable with improved communication capabilities, a list of requirements on and recommendations for communication capabilities necessary to support polar science over the next ten years is given.

  3. Heterogeneity at work: implications of the 2012 Clinical Translational Science Award evaluators survey.

    Science.gov (United States)

    Kane, Cathleen; Alexander, Angela; Hogle, Janice A; Parsons, Helen M; Phelps, Lauren

    2013-12-01

    The Clinical and Translational Science Award (CTSA) program is an ambitious multibillion dollar initiative sponsored by the National Institutes of Health (NIH) organized around the mission of facilitating the improved quality, efficiency, and effectiveness of translational health sciences research across the country. Although the NIH explicitly requires internal evaluation, funded CTSA institutions are given wide latitude to choose the structure and methods for evaluating their local CTSA program. The National Evaluators Survey was developed by a peer-led group of local CTSA evaluators as a voluntary effort to understand emerging differences and commonalities in evaluation teams and techniques across the 61 CTSA institutions funded nationwide. This article presents the results of the 2012 National Evaluators Survey, finding significant heterogeneity in evaluation staffing, organization, and methods across the 58 CTSAs institutions responding. The variety reflected in these findings represents both a liability and strength. A lack of standardization may impair the ability to make use of common metrics, but variation is also a successful evolutionary response to complexity. Additionally, the peer-led approach and simple design demonstrated by the questionnaire itself has value as an example of an evaluation technique with potential for replication in other areas across the CTSA institutions or any large-scale investment where multiple related teams across a wide geographic area are given the latitude to develop specialized approaches to fulfilling a common mission.

  4. [The work of Hernandez and its repercussions in the natural sciences].

    Science.gov (United States)

    Alvarez Peláez, R

    1995-01-01

    The most important source of knowledge and diffusion of the great American work from Hernández, was carried out starting from the selection and summary produced by the Napolitan physician Nardo Antonio Recchi. Starting from his manuscript they published the Rerum Medicarum Novai Hispaniae Thesaurus (Rome 1651), piece prepared by the Accademia dei Lincei, and the four Books of Nature (Mexico, 1615), carried out by Brother Francisco Ximénez with the intention--intention that also had Recchi--of having a practical handbook of medicine utilizing the American products. This paper treats, essentially, of those works.

  5. The Rudolf Mössbauer story his scientific work and its impact on science and history

    CERN Document Server

    Kienle, Paul

    2012-01-01

    The “Rudolf Mössbauer Story” recounts the history of the discovery of the “Mössbauer Effect” in 1958 by Rudolf Mössbauer as a graduate student of Heinz Maier-Leibnitz for which he received the Nobel Prize in 1961 when he was 32 years old. The development of numerous applications of the Mössbauer Effect in many fields of sciences , such as physics, chemistry, biology and medicine is reviewed by experts who contributed to this wide spread research. In 1978 Mössbauer focused his research interest on a new field “Neutrino Oscillations” and later on the study of the properties of the neutrinos emitted by the sun.

  6. Genomics, "Discovery Science," Systems Biology, and Causal Explanation: What Really Works?

    Science.gov (United States)

    Davidson, Eric H

    2015-01-01

    Diverse and non-coherent sets of epistemological principles currently inform research in the general area of functional genomics. Here, from the personal point of view of a scientist with over half a century of immersion in hypothesis driven scientific discovery, I compare and deconstruct the ideological bases of prominent recent alternatives, such as "discovery science," some productions of the ENCODE project, and aspects of large data set systems biology. The outputs of these types of scientific enterprise qualitatively reflect their radical definitions of scientific knowledge, and of its logical requirements. Their properties emerge in high relief when contrasted (as an example) to a recent, system-wide, predictive analysis of a developmental regulatory apparatus that was instead based directly on hypothesis-driven experimental tests of mechanism.

  7. Working on the robot society. : Visions and insights from science about the relation technology and employment.

    NARCIS (Netherlands)

    van Est, R.; Kool, L.

    2015-01-01

    The report Working on the robot society sets out current scientific findings for the relationship between technology and employment. It looks at the future and describes the policy options. In so doing, the report provides a joint fund of knowledge for societal and political debate on how the Nether

  8. Individual to Collaborative: Guided Group Work and the Role of Teachers in Junior Secondary Science Classrooms

    Science.gov (United States)

    Fung, Dennis; Lui, Wai-mei

    2016-01-01

    This paper, through discussion of a teaching intervention at two secondary schools in Hong Kong, demonstrates the learning advancement brought about by group work and dissects the facilitating role of teachers in collaborative discussions. One-hundred and fifty-two Secondary Two (Grade 8) students were divided into three pedagogical groups, namely…

  9. Values in a Science of Social Work: Values-Informed Research and Research-Informed Values

    Science.gov (United States)

    Longhofer, Jeffrey; Floersch, Jerry

    2014-01-01

    While social work must be evaluative in relation to its diverse areas of practice and research (i.e., values-informed research), the purpose of this article is to propose that values are within the scope of research and therefore research on practice should make values a legitimate object of investigation (i.e., research-informed values). In this…

  10. Fitness for work in health care workers from the prospective of ethics, science and good practices.

    Science.gov (United States)

    Alessio, L; Arici, Cecilia; Franco, G

    2012-01-01

    Fitness for work (FFW) is the final task of both risk assessment and health surveillance, aimed at protecting workers' health and working capacity. There are numerous specific concerns regarding health care workers. In particular: i) the frequent difficulty in determining at pre-employment/pre-placement examinations the specific task that the individual worker will perform; ii) the prevalence of female workers and the contemporary presence of numerous occupational risk factors that are a potential cause of harmful effects on women's reproductive health; iii) the progressive aging of the staff especially nurses; iv) the risk to third parties, with particular reference to the issues of biological risk and substance abuse, also in relation to shift work, fatigue and occupational stress; v) the increasing number of immigrant workers among support staff In such cases the occupational physician, respecting both ethical principles and regulations and with an appropriate balance between scientific evidence and the precautionary principle, should express a FFW judgment that allows both the adaptation of work to the worker and vice versa, as recommended by the World Health Organization (WHO) and the International Commission on Occupational Health (ICOH). Proper FFW judgment also permits the expected benefits to be achieved, not only for the workers but also for employers, companies and society.

  11. An Overview of the Use of Mechanical Turk in Behavioral Sciences: Implications for Social Work

    Science.gov (United States)

    Chan, Chitat; Holosko, Michael J.

    2016-01-01

    Crowdsourcing is a process in which a firm parcels out work to a "crowd" and offers payment for anyone within the crowd who completes the task determined by that firm. A growing number of behavioral scientists have begun using the Mechanical Turk (MTurk) to facilitate their research and practice, but there is apparently not one academic…

  12. Social Work Science and Identity Formation for Doctoral Scholars within Intellectual Communities

    Science.gov (United States)

    Mor Barak, Michàlle E.; Brekke, John S.

    2014-01-01

    Three themes are central to preparing doctoral students for the professoriate: identity formation, scientific integration, and intellectual communities. In this article, we argue that these three themes are not separate pillars but interlocking circles. Our main thesis is that (1) social work must develop into a distinct integrative scientific…

  13. Individual to Collaborative: Guided Group Work and the Role of Teachers in Junior Secondary Science Classrooms

    Science.gov (United States)

    Fung, Dennis; Lui, Wai-mei

    2016-01-01

    This paper, through discussion of a teaching intervention at two secondary schools in Hong Kong, demonstrates the learning advancement brought about by group work and dissects the facilitating role of teachers in collaborative discussions. One-hundred and fifty-two Secondary Two (Grade 8) students were divided into three pedagogical groups, namely…

  14. Integrated Contextual Learning and Food Science Students' Perception of Work Readiness

    Science.gov (United States)

    Coorey, Ranil; Firth, Ann

    2013-01-01

    The expectation that universities will produce graduates with high levels of work readiness is now a commonplace in government policies and statements from industry representatives. Meeting the demand requires that students gain industry related experience before graduation. Traditionally students have done so by undertaking extended work…

  15. 3rd Annual NASA Ames Space Science and Astrobiology Jamboree

    Science.gov (United States)

    Dotson, Jessie

    2015-01-01

    The Space Science and Astrobiology Division at NASA Ames Research Center consists of over 50 civil servants and more than 110 contractors, co-­-ops, post-­-docs and associates. Researchers in the division are pursuing investigations in a variety of fields including exoplanets, planetary science, astrobiology and astrophysics. In addition, division personnel support a wide variety of NASA missions including (but not limited to) Kepler, SOFIA, LADEE, JWST, and New Horizons. With such a wide variety of interesting research going on, distributed among three branches in at least 5 different buildings, it can be difficult to stay abreast of what one's fellow researchers are doing. Our goal in organizing this symposium is to facilitate communication and collaboration among the scientists within the division, and to give center management and other ARC researchers and engineers an opportunity to see what scientific research and science mission work is being done in the division. We are also continuing the tradition within the Space Science and Astrobiology Division to honor one senior and one early career scientist with the Pollack Lecture and the Early Career Lecture, respectively. With the Pollack Lecture, our intent is to select a senior researcher who has made significant contributions to any area of research within the space sciences, and we are pleased to honor Dr. William Borucki this year. With the Early Career Lecture, our intent is to select a young researcher within the division who, by their published scientific papers, shows great promise for the future in any area of space science research, and we are pleased to honor Dr. Melinda Kahre this year

  16. Teaching Planetary Sciences with the Master in Space Science and Technology at Universidad del País Vasco UPV/EHU: Theory and Practice works

    Science.gov (United States)

    Sanchez-Lavega, Agustin; Hueso, R.; Perez-Hoyos, S.

    2012-10-01

    The Master in Space Science and Technology is a postgraduate course at the Universidad del País Vasco in Spain (http://www.ehu.es/aula-espazio/master.html). It has two elective itineraries on space studies: scientific and technological. The scientific branch is intended for students aiming to access the PhD doctorate program in different areas of space science, among them the research of the solar system bodies. The theoretical foundations for the solar system studies are basically treated in four related matters: Astronomy and Astrophysics, Physics of the Solar System, Planetary Atmospheres, and Image Processing and Data Analysis. The practical part is developed on the one hand by analyzing planetary images obtained by different spacecrafts from public archives (e. g. PDS), and on the other hand from observations obtained by the students employing the 50 cm aperture telescope and other smaller telescopes from the Aula EspaZio Gela Observatory at the Engineering Faculty. We present the scheme of the practice works realized at the telescope to get images of the planets in different wavelengths pursuing to study the following aspects of Planetary Atmospheres: (1) Data acquisition; (2) Measurements of cloud motions to derive winds; (3) Measurement of the upper cloud reflectivity at the different wavelengths and position in the disk to retrieve the upper cloud properties and vertical structure. The theoretical foundations accompanying these practices are then introduced: atmospheric dynamics and thermodynamics, and the radiative transfer problem. Acknowledgments: This work was supported by Departamento de Promoción Económica of Diputación Foral Bizkaia through a grant to Aula EspaZio Gela at E.T.S. Ingeniería (Bilbao, Spain).

  17. A model-based approach to the spatial and spectral calibration of NIRSpec onboard JWST

    Science.gov (United States)

    Dorner, B.; Giardino, G.; Ferruit, P.; Alves de Oliveira, C.; Birkmann, S. M.; Böker, T.; De Marchi, G.; Gnata, X.; Köhler, J.; Sirianni, M.; Jakobsen, P.

    2016-08-01

    Context. The NIRSpec instrument for the James Webb Space Telescope (JWST) can be operated in multiobject spectroscopy (MOS), long-slit, and integral field unit (IFU) mode with spectral resolutions from 100 to 2700. Its MOS mode uses about a quarter of a million individually addressable minislits for object selection, covering a field of view of ~9 arcmin2. Aims: The pipeline used to extract wavelength-calibrated spectra from NIRSpec detector images relies heavily on a model of NIRSpec optical geometry. We demonstrate how dedicated calibration data from a small subset of NIRSpec modes and apertures can be used to optimize this parametric model to the necessary levels of fidelity. Methods: Following an iterative procedure, the initial fiducial values of the model parameters are manually adjusted and then automatically optimized, so that the model predicted location of the images and spectral lines from the fixed slits, the IFU, and a small subset of the MOS apertures matches their measured location in the main optical planes of the instrument. Results: The NIRSpec parametric model is able to reproduce the spatial and spectral position of the input spectra with high fidelity. The intrinsic accuracy (1-sigma, rms) of the model, as measured from the extracted calibration spectra, is better than 1/10 of a pixel along the spatial direction and better than 1/20 of a resolution element in the spectral direction for all of the grating-based spectral modes. This is fully consistent with the corresponding allocation in the spatial and spectral calibration budgets of NIRSpec.

  18. Information Content Analysis for Selection of Optimal JWST Observing Modes for Transiting Exoplanet Atmospheres

    Science.gov (United States)

    Batalha, Natasha E.; Line, M. R.

    2017-04-01

    The James Webb Space Telescope (JWST) is nearing its launch date of 2018, and is expected to revolutionize our knowledge of exoplanet atmospheres. In order to specifically identify which observing modes will be most useful for characterizing a diverse range of exoplanetary atmospheres, we use an information content (IC) based approach commonly used in the studies of solar system atmospheres. We develop a system based upon these IC methods to trace the instrumental and atmospheric model phase space in order to identify which observing modes are best suited for particular classes of planets, focusing on transmission spectra. Specifically, the atmospheric parameter space we cover is T = 600-1800 K, C/O = 0.55-1, [M/H] = 1-100 × Solar for an R = 1.39 R J , M = 0.59 M J planet orbiting a WASP-62-like star. We also explore the influence of a simplified opaque gray cloud on the IC. We find that obtaining broader wavelength coverage over multiple modes is preferred over higher precision in a single mode given the same amount of observing time. Regardless of the planet temperature and composition, the best modes for constraining terminator temperatures, C/O ratios, and metallicity are NIRISS SOSS+NIRSpec G395. If the target’s host star is dim enough such that the NIRSpec prism is applicable, then it can be used instead of NIRISS SOSS+NIRSpec G395. Lastly, observations that use more than two modes should be carefully analyzed because sometimes the addition of a third mode results in no gain of information. In these cases, higher precision in the original two modes is favorable.

  19. THE FORMATION OF STUDENTS’ LEARNING-COGNITIVE COMPETENCES BASED ON LABORATORY WORKS IN COMPUTER SCIENCE AND ICT

    Directory of Open Access Journals (Sweden)

    EVGENIY YUR’EVICH ANDRUSENKO

    2015-01-01

    Full Text Available Changes in Russian education must be made in an inte-grated way. Strategic goal of the state policy in the field of education is to enhance access to quality education, which must be relevant to the requirements of the inno-vative development of economy, current needs of society and all citizens. The list of tasks includes the competence approach as an important part of modernization of educa-tion. Among the key competences are distinguished learning-cognitive competences, for the formation of which are indicated teaching methods, forms and means. Laboratory work in computer science and ICT is one of such means. Laboratory work is a link between theoreti-cal and practical learning and is an important component of theory and practice: it strengthens and improves knowledge and skills, which are used in the process of further studies.

  20. Academic Work—Faster, Higher, Further? On the (Missing Proportion of Work to Spare Time in the (Cultural Sciences

    Directory of Open Access Journals (Sweden)

    Gert Dressel

    2008-01-01

    Full Text Available We make the practices of the academic production of knowledge a subject of critical discussion by focusing on the world of academic work and the academics themselves. Based on interviews with academics in the field of cultural sciences we conclude that with regard to their daily routines, their annual schedules, and their life-courses the so-called private life (family life, leisure time etc. becomes dominated by the social and cultural logics of the working sphere. Although it might appear exaggerated, we will refer to the humanities as a "total institution" which entails social, physical, and mental costs for its "inmates" as well as for those who never managed to become "inmates" (in spite of their efforts and those who don’t belong to the institution any more. URN: urn:nbn:de:0114-fqs0801385

  1. Ecological Theory Origin from Natural to Social Science of Vice Versa? A Brief Conceptual History for Social Work

    Directory of Open Access Journals (Sweden)

    Karen Smith Rotabi

    2007-05-01

    Full Text Available The origin of holistic social work and ecological theory was investigated. Emphasis was placed on Howard W. Odum, founding dean of the University of North Carolina School of Public Welfare, and subsequent scholarship by his sons, collaborators on the first American ecology text. Eugene and Howard Thomas Odum, internationally recognized ecological scholars, identified holism as a universal concept originating in social sciences, crediting their father’s earlier sociological work,which later bridged to ecosystems ecology. A historical review of the influential sociologists, social workers, and ecologists is presented to build the case for ecological theory transfer across the three disciplines, beginning with sociology. Critique of the current use of the ecological perspective is discussed, specifically social work’s tendency to target social systems and behavior while largely ignoring the natural environment.

  2. Cross-disciplinary working in the sciences and humanities: historical data rescue activities in Southeast Asia and beyond

    Science.gov (United States)

    Williamson, Fiona

    2016-12-01

    This paper argues that more work is needed to facilitate cross-disciplinary collaborations by scholars across the physical sciences and humanities to improve Data Rescue Activities (DARE). Debate over the scale and potential impact of anthropogenic global warming is one of the dominant narratives of the twenty-first century. Predicting future climates and determining how environment and society might be affected by climate change are global issues of social, economic and political importance. They require responses from different research communities and necessitate closer inter-disciplinary working relationships for an integrated approach. Improving the datasets required for long-term climate models is an important part of this process. Establishing a multi-disciplinary dialogue and approach to DARE activities is increasingly being recognised as the best way to achieve this. This paper focuses on the recovery of the long-term instrumental weather observations used for models and reconstructions of the climate over the past two-hundred years. Written from the perspective of an historian working in the field, it does not seek to explore the reconstructions themselves but the process of data gathering, advocating a closer working relationship between the arts, social sciences, and sciences to extend the geographic and temporal coverage of extant datasets. This is especially important for regions where data gaps exist currently. First, it will offer a justification for extending data recovery activities for Southeast Asia and the China Seas region. Second, it will offer a brief overview of the data recovery projects currently operating in that area and the typesof historic source material that are used. Third, it will explore the work currently being undertaken for Southeast Asia and China under the Atmospheric Circulation Reconstructions over the Earth initiative as an example of a successful cross-disciplinary program. Finally, it will argue the importance of

  3. James Webb Space Telescope - L2 Communications for Science Data Processing

    Science.gov (United States)

    Johns, Alan; Seaton, Bonita; Gal-Edd, Jonathan; Jones, Ronald; Fatig, Curtis; Wasiak, Francis

    2008-01-01

    JWST is the first NASA mission at the second Lagrange point (L2) to identify the need for data rates higher than 10 megabits per second (Mbps). JWST will produce approximately 235 Gigabits of science data every day that will be downlinked to the Deep Space Network (DSN). To get the data rates desired required moving away from X-band frequencies to Ka-band frequencies. To accomplish this transition, the DSN is upgrading its infrastructure. This new range of frequencies are becoming the new standard for high data rate science missions at L2. With the new frequency range, the issues of alternatives antenna deployment, off nominal scenarios, NASA implementation of the Ka-band 26 GHz, and navigation requirements will be discussed in this paper. JWST is also using Consultative Committee for Space Data Systems (CCSDS) standard process for reliable file transfer using CCSDS File Delivery Protocol (CFDP). For JWST the use of the CFDP protocol provides level zero processing at the DSN site. This paper will address NASA implementations of Ground Stations in support of Ka-band 26 GHz and lesson learned from implementing a file base (CFDP) protocol operational system.

  4. Climate Science in Social Media: What's Worked, and What Hasn't

    Science.gov (United States)

    Sinclair, P.

    2015-12-01

    A common conception of social media is that the definition of success is a huge number of viewers and followers. While these outcomes not undesirable, they are not the only signs of success. More important than the size of the audience, is how well that audience follows and in turn, propagates the desired message. Dark Snow project has been successful in driving a global conversation about the Greenland ice sheet, not by creating huge numbers of viewers and followers, but due to a significant, and highly motivated, following among media gatekeepers, academic messengers, and social media activists. It's very important that, from the start, the Dark Snow story - that changes in ice sheet albedo may be driving increased melt, was effectively encoded, or "branded", in the project's name - "Dark Snow" - a vivid and easily illustrated visual image. A simple concept that is easy to describe and understand, but profound in implication, has allowed for wide discussion among professionals in science and media, as well as the general public.

  5. When citizens and scientists work together : a french collaborative science network on earthworms communities distribution

    Science.gov (United States)

    Guernion, Muriel; Hoeffner, Kevin; Guillocheau, Sarah; Hotte, Hoël; Cylly, Daniel; Piron, Denis; Cluzeau, Daniel; Hervé, Morgane; Nicolai, Annegret; Pérès, Guénola

    2017-04-01

    Scientists have become more and more interested in earthworms because of their impact on soil functioning and their importance in provision of many ecosystem services. To improve the knowledge on soil biodiversity and integrate earthworms in soil quality diagnostics, it appeared necessary to gain a large amount of data on their distribution. The University of Rennes 1 developed since 2011 a collaborative science project called Observatoire Participatif des Vers de Terre (OPVT, participative earthworm observatory). It has several purposes : i) to offer a simple tool for soil biodiversity evaluation in natural and anthropic soils through earthworm assessment, ii) to offer trainings to farmers, territory managers, gardeners, pupils on soil ecology, iii) to build a database of reference values on earthworms in different habitats, iv) to propose a website (https://ecobiosoil.univ-rennes1.fr/OPVT_accueil.php) providing for example general scientific background (earthworm ecology and impacts of soil management), sampling protocols and online visualization of results (data processing and earthworms mapping). Up to now, more than 5000 plots have been prospected since the opening of the project in 2011., Initially available to anyone on a voluntary basis, this project is also used by the French Ministry of Agriculture to carry out a scientific survey throughout the French territory.

  6. Next Generation Very Large Array Memo No. 5: Science Working Groups -- Project Overview

    CERN Document Server

    Carilli, C L; Ott, J; Beasley, A; Isella, A; Murphy, E; Leroy, A; Casey, C; Moullet, A; Lacy, M; Hodge, J; Bower, G; Demorest, P; Hull, C; Hughes, M; di Francesco, J; Narayanan, D; Kent, B; Clark, B; Butler, B

    2015-01-01

    We summarize the design, capabilities, and some of the priority science goals of a next generation Very Large Array (ngVLA). The ngVLA is an interferometric array with 10x larger effective collecting area and 10x higher spatial resolution than the current VLA and the Atacama Large Millimeter Array (ALMA), optimized for operation in the wavelength range 0.3cm to 3cm. The ngVLA opens a new window on the Universe through ultra-sensitive imaging of thermal line and continuum emission down to milliarcecond resolution, as well as unprecedented broad band continuum polarimetric imaging of non-thermal processes. The continuum resolution will reach 9mas at 1cm, with a brightness temperature sensitivity of 6K in 1 hour. For spectral lines, the array at 1" resolution will reach 0.3K surface brightness sensitivity at 1cm and 10 km/s spectral resolution in 1 hour. These capabilities are the only means with which to answer a broad range of critical scientific questions in modern astronomy, including direct imaging of plane...

  7. From boundary‐work to boundary object: how biology left and re‐entered the social sciences

    Science.gov (United States)

    Meloni, Maurizio

    2016-01-01

    Abstract In an archaeological spirit this paper comes back to a founding event in the construction of the twentieth‐century episteme, the moment at which the life‐ and the social sciences parted ways and intense boundary‐work was carried out on the biology/society border, with significant benefits for both sides. Galton and Weismann for biology, and Alfred Kroeber for anthropology delimit this founding moment and I argue, expanding on an existing body of historical scholarship, for an implicit convergence of their views. After this excavation, I look at recent developments in the life sciences, which I have named the ‘social turn’ in biology (Meloni, 2014), and in particular at epigenetics with its promise to destabilize the social/biological border. I claim here that today a different account of ‘the biological’ to that established during the Galton–Kroeber period is emerging. Rather than being used to support a form of boundary‐work, biology has become a boundary object that crosses previously erected barriers, allowing different research communities to draw from it. PMID:27818538

  8. From boundary-work to boundary object: how biology left and re-entered the social sciences.

    Science.gov (United States)

    Meloni, Maurizio

    2016-03-01

    In an archaeological spirit this paper comes back to a founding event in the construction of the twentieth-century episteme, the moment at which the life- and the social sciences parted ways and intense boundary-work was carried out on the biology/society border, with significant benefits for both sides. Galton and Weismann for biology, and Alfred Kroeber for anthropology delimit this founding moment and I argue, expanding on an existing body of historical scholarship, for an implicit convergence of their views. After this excavation, I look at recent developments in the life sciences, which I have named the 'social turn' in biology (Meloni, 2014), and in particular at epigenetics with its promise to destabilize the social/biological border. I claim here that today a different account of 'the biological' to that established during the Galton-Kroeber period is emerging. Rather than being used to support a form of boundary-work, biology has become a boundary object that crosses previously erected barriers, allowing different research communities to draw from it.

  9. The role and working conditions of Movement Science students employed in sport and recreational facilities: An Italian multicenter study.

    Science.gov (United States)

    Gallè, Francesca; Di Onofrio, Valeria; Arpesella, Marisa; Bacci, Silvia; Bianco, Antonino; Brandi, Giorgio; Bruno, Stefania; Anastasi, Daniela; Carraro, Elisabetta; Flacco, Maria Elena; Giampaoli, Saverio; Izzotti, Alberto; Leoni, Erica; Bertoncello, Chiara; Minelli, Liliana; Napoli, Christian; Nobile, Carmelo; Pasquarella, Cesira; Liguori, Giorgio; Romano Spica, Vincenzo

    2015-01-01

    In Italy, students from Movement Science (MS) Degree Courses often work in sport and recreational facilities before graduation. The employment conditions of Movement Science students working in sport/recreational facilities were investigated, and the management and structural features of the facilities were evaluated, including safety policies. Regional differences were also considered. Questionnaires were administered to undergraduate and graduate students (N = 4,217) in 17 Universities. Students' perceptions of the quality of the facilities where they had been employed was evaluated using multivariate analysis. A latent class model with covariates was used to evaluate how variables relating to participants, employment facilities or regions influence their opinions. A high proportion of MS students were employed in sporting facilities (undergraduate level: 33% ; graduate level: 55%), in most cases without any formal employment contracts. Both the structural and hygienic features, as well as the professional knowledge of the staff, were considered good to excellent by the majority of participants (about 70%). Communication of the basic behavioral rules was considered adequate by 61-63% of undergraduate students and 71-75% of graduate students, while nearly half of the participants were dissatisfied with the staff safety training. Correlations between the perceived good structural/hygienic conditions, the presence of regulations and training programs for the staff were investigated. Differences regarding occupational level and safety training among different regions of Italy were also observed. Italian students in Movement Science were easily employed in sport/recreational facilities, but frequently without a formal contract. This is a consequence of the lack of specific regulations in the field of recreational/leisure employment and could have negative implications, especially in terms of safety.

  10. [Science and nation: romanticism and natural history in the works of E. J. da Silva Maia].

    Science.gov (United States)

    Kury, L

    1998-01-01

    The works of physician and naturalist Emílio Joaquim da Silva Maia (1808-59) can be viewed as a scientific project that discovers Brazil and its inhabitants. Maia's nationalism and his romantic view of nature formed the underpinnings of his scientific theories, especially his studies on zoological geography. He subordinated the issue of the biological specificity of different regions of the world to his era's debates on the construction of Brazil as an independent nation. In his interpretations of European natural history, Maia endeavored to understand Brazilian nature as a specific achievement of the Cosmos, in keeping with Alexander von Humboldt's approach.

  11. Combinatorial Algorithms to Enable Computational Science and Engineering: Work from the CSCAPES Institute

    Energy Technology Data Exchange (ETDEWEB)

    Boman, Erik G. [Sandia National Lab. (SNL-NM), Albuquerque, NM (United States). Scalable Algorithms Dept.; Catalyurek, Umit V. [The Ohio State Univ., Columbus, OH (United States). Biomedical Informatics. Electrical and Computer Engineering; Chevalier, Cedric [Alternative Energies and Atomic Energy Commission (CEA), Cadarache (France); Devine, Karen D. [Sandia National Lab. (SNL-NM), Albuquerque, NM (United States). Scalable Algorithms Dept.; Gebremedhin, Assefaw H. [Purdue Univ., West Lafayette, IN (United States). Computer Science; Hovland, Paul D. [Argonne National Lab. (ANL), Argonne, IL (United States). Mathematics and Computer Science Division; Pothen, Alex [Purdue Univ., West Lafayette, IN (United States). Computer Science; Rajamanickam, Sivasankaran [Sandia National Lab. (SNL-NM), Albuquerque, NM (United States). Scalable Algorithms Dept.; Safro, Ilya [Argonne National Lab. (ANL), Argonne, IL (United States). Mathematics and Computer Science Division; Wolf, Michael M. [Massachusetts Inst. of Technology (MIT), Lexington, MA (United States). Lincoln Lab.; Zhou, Min [Rensselaer Polytechnic Inst., Troy, NY (United States). Scientific Computation Research Center

    2015-01-16

    This final progress report summarizes the work accomplished at the Combinatorial Scientific Computing and Petascale Simulations Institute. We developed Zoltan, a parallel mesh partitioning library that made use of accurate hypergraph models to provide load balancing in mesh-based computations. We developed several graph coloring algorithms for computing Jacobian and Hessian matrices and organized them into a software package called ColPack. We developed parallel algorithms for graph coloring and graph matching problems, and also designed multi-scale graph algorithms. Three PhD students graduated, six more are continuing their PhD studies, and four postdoctoral scholars were advised. Six of these students and Fellows have joined DOE Labs (Sandia, Berkeley), as staff scientists or as postdoctoral scientists. We also organized the SIAM Workshop on Combinatorial Scientific Computing (CSC) in 2007, 2009, and 2011 to continue to foster the CSC community.

  12. Color Symbolism in the Folk Fairy-Tale and Science Fiction Works by R. Bradbury, C. Simak, A. and B. Strugatsky

    Directory of Open Access Journals (Sweden)

    Elena Kibalka

    2013-08-01

    Full Text Available The given article deals with the symbolism of color in the British and Russian fairy-tale tradition, which is reflected in the science fiction literature. The symbolic meaning of the color palette in the science fiction works by R. Bradbury, C. Simak, A. and B. Strugatsky is analyzed. It is proved that folkloric indication of colors serves as the peculiar way of constructing a science fiction space and plays an important role in the understanding of the concept of works.

  13. Exo-C: Mission and Science Payload Design

    Science.gov (United States)

    Dekens, Frank G.; Stapelfeldt, Karl R.; Warfield, Keith; Unwin, Stephen C.; Exo-C Science; Technology Definition Team, Exo-C JPL Study Design Team

    2015-01-01

    We present NASA's Exoplanet Coronagraph (Exo-C) mission design and science payload completed as part of a probe-class concept study under consideration for launch following JWST. The payload consists of an unobscured Cassegrain telescope with a 1.4-m clear aperture, a barrel assembly, and an internal coronagraph instrument. The mission has a 3 year lifetime and is in a highly stable Earth-trailing orbit. The coronagraph instrument is mounted laterally on the anti-Sun side of the telescope, obviating the need for high incidence reflections and better isolating it from spacecraft disturbances. The instrument has both an Imaging Camera and an Integral Field Spectrograph (IFS). The former obtains filter imaging with 1e-9 raw contrast from 2 - 20 λ/D in radius, while the IFS delivers the same contrast with spectral resolution of R = 70 from 450 to 1000 nm, but with a reduced outer working angle.The Exo-C science performance requirements are achieved with a specialized observatory design enabled by several new technologies. The telescope is designed for precision pointing and high stability to maintain a slowly evolving speckle pattern. Vibration isolation is achieved with two stages between the reaction wheels and the science payload. The solar arrays and high gain antenna are body-fixed, and a stiff barrel assembly is used as the telescope metering structure. Telescope pointing is updated at a high rate by monitoring the bright science target star with a low order wavefront sensor and driving a fine steering mirror for compensation. Active thermal control is used to minimize thermal drifts of the telescope, instrument, and barrel assemblies. Stability analyses via modeling of the structural, thermal, and optical performance of this configuration show that the proposed mission configuration would enable unprecedented exoplanet and circumstellar disk science with direct imaging.

  14. Augmented Method to Improve Thermal Data for the Figure Drift Thermal Distortion Predictions of the JWST OTIS Cryogenic Vacuum Test

    Science.gov (United States)

    Park, Sang C.; Carnahan, Timothy M.; Cohen, Lester M.; Congedo, Cherie B.; Eisenhower, Michael J.; Ousley, Wes; Weaver, Andrew; Yang, Kan

    2017-01-01

    The JWST Optical Telescope Element (OTE) assembly is the largest optically stable infrared-optimized telescope currently being manufactured and assembled, and is scheduled for launch in 2018. The JWST OTE, including the 18 segment primary mirror, secondary mirror, and the Aft Optics Subsystem (AOS) are designed to be passively cooled and operate near 45K. These optical elements are supported by a complex composite backplane structure. As a part of the structural distortion model validation efforts, a series of tests are planned during the cryogenic vacuum test of the fully integrated flight hardware at NASA JSC Chamber A. The successful ends to the thermal-distortion phases are heavily dependent on the accurate temperature knowledge of the OTE structural members. However, the current temperature sensor allocations during the cryo-vac test may not have sufficient fidelity to provide accurate knowledge of the temperature distributions within the composite structure. A method based on an inverse distance relationship among the sensors and thermal model nodes was developed to improve the thermal data provided for the nanometer scale WaveFront Error (WFE) predictions. The Linear Distance Weighted Interpolation (LDWI) method was developed to augment the thermal model predictions based on the sparse sensor information. This paper will encompass the development of the LDWI method using the test data from the earlier pathfinder cryo-vac tests, and the results of the notional and as tested WFE predictions from the structural finite element model cases to characterize the accuracies of this LDWI method.

  15. Science fair: Is it worth the work? A qualitative study on deaf students' perceptions and experiences regarding science fair in primary and secondary school

    Science.gov (United States)

    Smith, Vivian Lee

    Science fairs have a long history in American education. They play an important role for establishing inquiry-based experiences in a science classroom. Students may be more motivated to learn science content when they are allowed to choose their own science fair topics. The purpose of this study was to examine Deaf college students' perceptions and experiences regarding science fair participation during primary and/or secondary school and determine the influence of science fair involvement on the development of language skills, writing skills, and higher order thinking skills as well as its impact on choice of a STEM major. This study examined responses from Deaf students attending Gallaudet University and National Technical Institute for the Deaf (NTID) majoring in a Science, Technology, Engineering, or Math (STEM) field. An electronic questionnaire and a semi-structured interview were used to collect data. The electronic questionnaire was divided into two strands: demographics and science fair experience. Twenty-one respondents participated in the questionnaire and ten participants were interviewed. A cross-case analysis revealed communication was the key to a successful science fair experience. Findings showed the educational background of participants influenced their perspective regarding the experience of a science fair. When communicating through American Sign Language, the science fair experience was more positive. When communicating through an interpreter or having no interpreter at all, the science fair experience was viewed in a negative light. The use of science fairs to enhance language development, writing skills, and higher order thinking skills was supported. Teachers and parents were strong influences for Deaf students participating in a science fair. Participation in a science fair did influence students to choose a STEM major but there were other considerations as well.

  16. Effect of Shift Work on the Frequency of Depression in Nursing Staff of Yazd University of Medical Sciences

    Directory of Open Access Journals (Sweden)

    Gholam Hossein Halvani

    2012-12-01

    Full Text Available Introduction: Depression as a disorder is relatively common in all societies; several factors are involved in depression development, that shift work is one of these factors. This study compared the frequency of depression in different shifts of nurses in hospitals of Yazd University of medical sciences. Materials & Methods: This study is a descriptive analytical study. Based on statistical methods, 150 nurses participated in this study. The research tool was a questionnaire that included 15 personal questions and 21 questions related to Beck test. The results were analysed by SPSS software. Results: 13.3% of all subjects were males and 86.7% were females. Results showed that, there is no significant relationship between gender, education, type of job, employment status and satisfaction levels of income with depression. Marital status (P-Value = 0.009 and F = 6.93, shift work (day working and shift work (P-Value = 0.032 and F = 1.11, job satisfaction (P-Value = 0.000 and F = 7.641 and the satisfaction of the employer (P-Value = 0.001 and F = 5.414 were significantly associated with depression. 3.49% of the nurses were in normal status, 7.26% had mild depression, 3.9% required consultation with the psychiatrist,% 7.8% suffered from moderate depression, 75.4% from severe depression and 3.1% from very severe depression. Conclusion: It seems that shift work can not cause depression alone, but depression is the result of the interaction of several factors.

  17. Learning to Work with Databases in Astronomy: Quantitative Analysis of Science Educators' and Students' Pre-/Post-Tests

    Science.gov (United States)

    Schwortz, Andria C.; Burrows, Andrea C.; Myers, Adam D.

    2015-01-01

    Astronomy is increasingly moving towards working with large databases, from the state-of-the-art Sloan Digital Sky Survey Data Release 10, to the historical Digital Access to a Sky Century at Harvard. Non-astronomy fields as well tend to work with large datasets, be it in the form of warehouse inventory, health trends, or the stock market. However very few fields explicitly teach students the necessary skills to analyze such data. The authors studied a matched set of 37 participants working with 200-entry databases in astronomy using Google Spreadsheets, with limited information about a random set of quasars drawn from SDSS DR5. Here the authors present the quantitative results from an eight question pre-/post-test, with questions designed to span Bloom's taxonomy, on both the topics of the skills of using spreadsheets, and the content of quasars. Participants included both Astro 101 summer students and professionals including in-service K-12 teachers and science communicators. All groups showed statistically significant gains (as per Hake, 1998), with the greatest difference between women's gains of 0.196 and men's of 0.480.

  18. Workforce development and the organization of work: the science we need.

    Science.gov (United States)

    Schoenwald, Sonja K; Hoagwood, Kimberly Eaton; Atkins, Marc S; Evans, Mary E; Ringeisen, Heather

    2010-03-01

    The industrialization of health care, underway for several decades, offers instructive guidance and models for speeding access of children and families to clinically and cost effective preventive, treatment, and palliative interventions. This industrialization--i.e., the systematized production of goods or services in large-scale enterprises--has the potential to increase the value and effects of care for consumers, providers, and payers (Hayes and Gregg in Integrated behavioral healthcare: Positioning mental health practice with medical/surgical practice. Academic Press, San Diego, 2001), and to generate efficiencies in care delivery, in part because workforce responsibilities become more functional and differentiated such that individuals with diverse educational and professional backgrounds can effectively execute substantive clinical roles (Rees in Clin Exp Dermatol, 33, 39-393, 2008). To date, however, the models suggested by this industrialization have not been applied to children's mental health services. A combination of policy, regulatory, fiscal, systemic, and organizational changes will be needed to fully penetrate the mental health and substance abuse service sectors. In addition, problems with the availability, preparation, functioning, and status of the mental health workforce decried for over a decade will need to be addressed if consumers and payers are to gain access to effective interventions irrespective of geographic location, ethnic background, or financial status. This paper suggests that critical knowledge gaps exist regarding (a) the knowledge, skills, and competencies of a workforce prepared to deliver effective interventions; (b) the efficient and effective organization of work; and (c) the development and replication of effective workforce training and support strategies to sustain effective services. Three sets of questions are identified for which evidence-based answers are needed. Suggestions are provided to inform the development of a

  19. Science and Mathematics Teachers Working Toward Equity Through Teacher Research: Tracing Changes Across Their Research Process and Equity Views

    Science.gov (United States)

    Brenner, Mary E.; Bianchini, Julie A.; Dwyer, Hilary A.

    2016-12-01

    We investigated secondary science and mathematics teachers engaged in a two-and-a-half-year professional development effort focused on equity. We examined how teachers conducting research on their own instructional practices—a central learning strategy of the professional development project—informed and/or constrained their views related to three strands of equity: teachers and teaching, students and learning, and students' families and communities. Data collected included recordings of professional development seminars and school-site meetings, three sets of individual interviews with teacher researchers, and drafts and final products of the classroom research teachers conducted. From our qualitative analyses of data, we found that most teachers addressed at least two of the three equity strands in researching their own practice. We also found that most transformed their understandings of teachers and students as a result of their teacher research process. However, teachers' views of families and communities changed in less substantive ways. We close with recommendations for other researchers and professional developers intent on supporting science and mathematics teachers in using teacher research to work toward equity.

  20. The accretion/ejection paradigm in young stellar objects: from HST and Herschel to JWST

    Science.gov (United States)

    Podio, Linda

    2012-07-01

    Stellar jets and molecular outflows are observed in association with young accreting stars and are believed to play a key role in the star formation process. In this talk I will show how current and future space missions are of crucial importance to investigate the origin of stellar jets and their link to the accretion process. Thanks to its high angular (˜0.1") resolution, HST has been the first telescope allowing us to investigate the jet physics at optical/UV wavelengths down to the heart of the launching mechanism. We recently analysed a datacube of the jet emitted by the T Tauri star DG Tau obtaining spatio-kinematical maps of the hot atomic gas in the jet and of its physical conditions (Maurri et al., submitted). These data confirm the predictions of theoretical models including the fact that jets may extract the excess angular momentum from the system. In the last two years Herschel has further improved our comprehension of the ejection process observing the far infrared counterpart of fast and collimated atomic jets. PACS and HIFI observations, acquired within the GASPS (GAS in Protoplanetary Systems) Open Time Key Project (PI: B. Dent), show that T Tauri stars driving optical jets are also associated with a warm gas component emitting not only atomic ([OI], [CII]) but also molecular (high-J CO, H_2O, OH) lines. The comparison with Class 0 outflows highlights a clear evolutionary trend: the emission associated with evolved Class I/II sources is fainter and more compact and the estimated mass loss rates and lines cooling are one to two orders of magnitudes lower (Podio et al., to be submitted). The arrival of JWST will fill-in the gap between HST and Herschel opening a new window in the near and mid-infrared range at unprecedented angular resolution (down to 0.03"). This will allow resolving the emission in both atomic (e.g., [FeII]) and molecular (e.g., H_2) lines and understanding if the molecular gas is entrained by the atomic jet or launched with it

  1. Data sharing in stem cell translational science: policy statement by the International Stem Cell Forum Ethics Working Party.

    Science.gov (United States)

    Bredenoord, Annelien L; Mostert, Menno; Isasi, Rosario; Knoppers, Bartha M

    2015-01-01

    Data and sample sharing constitute a scientific and ethical imperative but need to be conducted in a responsible manner in order to protect individual interests as well as maintain public trust. In 2014, the Global Alliance for Genomics and Health (GA4GH) adopted a common Framework for Responsible Sharing of Genomic and Health-Related Data. The GA4GH Framework is applicable to data sharing in the stem cell field, however, interpretation is required so as to provide guidance for this specific context. In this paper, the International Stem Cell Forum Ethics Working Party discusses those principles that are specific to translational stem cell science, including engagement, data quality and safety, privacy, security and confidentiality, risk-benefit analysis and sustainability.

  2. Standards for the application of bibliometrics in the evaluation of individual researchers working in the natural sciences

    CERN Document Server

    Bornmann, Lutz

    2013-01-01

    Although bibliometrics has been a separate research field for many years, there is still no uniformity in the way bibliometric analyses are applied to individual researchers. Therefore, this study aims to set up standards for the use of bibliometrics in the evaluation of individual researchers working in the natural sciences. 2005 saw the introduction of the h index, which gives information about a researcher's productivity and the impact of his or her publications in a single number (h is the number of publications with at least h citations); however, it is not possible to cover the multidimensional complexity of research performance and to undertake inter-personal comparisons with this number. This study therefore includes recommendations for a set of indicators to be used for evaluating researchers. Our standards relate to the selection of data on which an evaluation is based, the analysis of the data and the presentation of the results.

  3. Deep Underground Science and Engineering Lab: S1 Dark Matter Working Group

    Energy Technology Data Exchange (ETDEWEB)

    Akerib, Daniel S.; Aprile, E.; /Case Western Reserve U. /Columbia U.; Baltz, E.A.; /KIPAC, Menlo Park; Dragowsky, M.R.; /Case Western Reserve U.; Gaitskell, R.J.; /Brown U.; Gondolo, P.; /Utah U.; Hime, A.; /Los Alamos; Martoff, C.J.; /Temple U.; Mei, D.-M.; /Los Alamos; Nelson, H.; /UC, Santa Barbara; Sadoulet, B.; /UC, Berkeley; Schnee, R.W.; /Case Western; Sonnenschein, A.H.; /Fermilab; Strigari, L.E.; /UC, Irvine

    2006-06-09

    In this report we have described the broad and compelling range of astrophysical and cosmological evidence that defines the dark matter problem, and the WIMP hypothesis, which offers a solution rooted in applying fundamental physics to the dynamics of the early universe. The WIMP hypothesis is being vigorously pursued, with a steady march of sensitivity improvements coming both from astrophysical searches and laboratory efforts. The connections between these approaches are profound and will reveal new information from physics at the smallest scales to the origin and workings of the entire universe. Direct searches for WIMP dark matter require sensitive detectors that have immunity to electromagnetic backgrounds, and are located in deep underground laboratories to reduce the flux from fast cosmic-ray-muon-induced neutrons which is a common background to all detection methods. With US leadership in dark matter searches and detector R&D, a new national laboratory will lay the foundation of technical support and facilities for the next generation of scientists and experiments in this field, and act as magnet for international cooperation and continued US leadership. The requirements of depth, space and technical support for the laboratory are fairly generic, regardless of the approach. Current experiments and upgraded versions that run within the next few years will probe cross sections on the 10{sup -45}-10{sup -44} cm{sup 2} scale, where depths of 3000-4000 m.w.e. are sufficient to suppress the neutron background. On the longer term, greater depths on the 5000-6000 level are desirable as cross sections down to 10{sup -46} cm{sup 2} are probed, and of course, if WIMPs are discovered then building up a statistical sample free of neutron backgrounds will be essential to extracting model parameters and providing a robust solution to the dark matter problem. While most of the detector technologies are of comparable physical scale, i.e., the various liquid and solid

  4. Deep Underground Science and Engineering Lab: S1 Dark Matter Working Group

    Energy Technology Data Exchange (ETDEWEB)

    Akerib, Daniel S.; Aprile, E.; /Case Western Reserve U. /Columbia U.; Baltz, E.A.; /KIPAC, Menlo Park; Dragowsky, M.R.; /Case Western Reserve U.; Gaitskell, R.J.; /Brown U.; Gondolo, P.; /Utah U.; Hime, A.; /Los Alamos; Martoff, C.J.; /Temple U.; Mei, D.-M.; /Los Alamos; Nelson, H.; /UC, Santa Barbara; Sadoulet, B.; /UC, Berkeley; Schnee, R.W.; /Case Western; Sonnenschein, A.H.; /Fermilab; Strigari, L.E.; /UC, Irvine

    2006-06-09

    In this report we have described the broad and compelling range of astrophysical and cosmological evidence that defines the dark matter problem, and the WIMP hypothesis, which offers a solution rooted in applying fundamental physics to the dynamics of the early universe. The WIMP hypothesis is being vigorously pursued, with a steady march of sensitivity improvements coming both from astrophysical searches and laboratory efforts. The connections between these approaches are profound and will reveal new information from physics at the smallest scales to the origin and workings of the entire universe. Direct searches for WIMP dark matter require sensitive detectors that have immunity to electromagnetic backgrounds, and are located in deep underground laboratories to reduce the flux from fast cosmic-ray-muon-induced neutrons which is a common background to all detection methods. With US leadership in dark matter searches and detector R&D, a new national laboratory will lay the foundation of technical support and facilities for the next generation of scientists and experiments in this field, and act as magnet for international cooperation and continued US leadership. The requirements of depth, space and technical support for the laboratory are fairly generic, regardless of the approach. Current experiments and upgraded versions that run within the next few years will probe cross sections on the 10{sup -45}-10{sup -44} cm{sup 2} scale, where depths of 3000-4000 m.w.e. are sufficient to suppress the neutron background. On the longer term, greater depths on the 5000-6000 level are desirable as cross sections down to 10{sup -46} cm{sup 2} are probed, and of course, if WIMPs are discovered then building up a statistical sample free of neutron backgrounds will be essential to extracting model parameters and providing a robust solution to the dark matter problem. While most of the detector technologies are of comparable physical scale, i.e., the various liquid and solid

  5. Progress Report on the ASCII for Science Data, Airborne and Geospatial Working Groups of the 2014 ESDSWG for MEaSUREs

    Science.gov (United States)

    Evans, K. D.; Krotkov, N. A.; Mattmann, C. A.; Boustani, M.; Law, E.; Conover, H.; Chen, G.; Olding, S. W.; Walter, J.

    2014-12-01

    The Earth Science Data Systems Working Groups (ESDSWG) were setup by NASA HQ 10 years ago. The role of the ESDSWG is to make recommendations relevant to NASA's Earth science data systems from users experiences. Each group works independently focussing on a unique topic. Participation in ESDSWG groups comes from a variety of NASA-funded science and technology projects, NASA information technology experts, affiliated contractor staff and other interested community members from academia and industry. Recommendations from the ESDSWG groups will enhance NASA's efforts to develop long term data products. The ASCII for Science Data Working Group (WG) will define a minimum set of information that should be included in ASCII file headers so that the users will be able to access the data using only the header information. After reviewing various use cases, such as field data and ASCII data exported from software tools, and reviewing ASCII data guidelines documentation, this WG will deliver guidelines for creating ASCII files that contain enough header information to allow the user to access the science data. The Airborne WG's goal is to improve airborne data access and use for NASA science. The first step is to evaluate the state of airborne data and make recommendations focusing on data delivery to the DAACs (data centers). The long term goal is to improve airborne data use for Earth Science research. Many data aircraft observations are reported in ASCII format. The ASCII and Airborne WGs seem like the same group, but the Airborne WG is concerned with maintaining and using airborne for science research, not just the data format. The Geospatial WG focus is on the interoperability issues of Geospatial Information System (GIS) and remotely sensed data, in particular, focusing on DAAC(s) data from NASA's Earth Science Enterprise. This WG will provide a set of tools (GIS libraries) to use with training and/or cookbooks through the use of Open Source technologies. A progress

  6. Engaging Students with the Nature of Science and the Nature of Technology by Modeling the Work of Scientists

    Science.gov (United States)

    Kruse, Jerrid W.; Wilcox, Jesse L.

    2013-01-01

    Just as science education is too often limited to the acquisition of facts, technology education is too often limited to proficient use of technology. Neither of these goals fully realize a robust definition of science and technology literacy. To achieve greater science and technology literacy, students must understand the natures of both science…

  7. High-precision cryogenic wheel mechanisms of the JWST/MIRI instrument: performance of the flight models

    Science.gov (United States)

    Krause, O.; Müller, F.; Birkmann, S.; Böhm, A.; Ebert, M.; Grözinger, U.; Henning, Th.; Hofferbert, R.; Huber, A.; Lemke, D.; Rohloff, R.-R.; Scheithauer, S.; Gross, T.; Fischer, T.; Luichtel, G.; Merkle, H.; Übele, M.; Wieland, H.-U.; Amiaux, J.; Jager, R.; Glauser, A.; Parr-Burman, P.; Sykes, J.

    2010-07-01

    The Mid Infrared Instrument (MIRI) aboard JWST is equipped with one filter wheel and two dichroic-grating wheel mechanisms to reconfigure the instrument between observing modes such as broad/narrow-band imaging, coronagraphy and low/medium resolution spectroscopy. Key requirements for the three mechanisms with up to 18 optical elements on the wheel include: (1) reliable operation at T = 7 K, (2) high positional accuracy of 4 arcsec, (3) low power dissipation, (4) high vibration capability, (5) functionality at 7 K ball bearing, a central torque motor for actuation, a ratchet system with monolithic CuBe flexural pivots for precise and powerless positioning and a magnetoresistive position sensor has been implemented. We report here the final performance and lessons-learnt from the successful acceptance test program of the MIRI wheel mechanism flight models. The mechanisms have been meanwhile integrated into the flight model of the MIRI instrument, ready for launch in 2014 by an Ariane 5 rocket.

  8. Research results reported by OEO summer (1981) student employees of LLNL working with Earth Sciences (K) Division personnel

    Energy Technology Data Exchange (ETDEWEB)

    Doyle, M. C.; Griffith, P. J.; Kreevoy, E. P.; Turner, III, H. J.; Tatman, D. A.

    1982-01-01

    Significant experimental results were achieved in a number of research programs that were carried out during the summer of 1981 by students sponsored by the Office of Equal Opportunity at the Lawrence Livermore National Laboratory. These students were working with Earth Sciences (K) Division personnel. Accomplishments include the following: (1) preparation of post-burn stratigraphic sections for the Hoe Creek III experiment, Underground Coal Gasification project; (2) preparation of miscellaneous stratigraphic sections in the Climax granite near the Spent Fuel Test, Nevada Test Site, for the Waste Isolation Project; (3) confirmation of the applicability of a new theory relating to subsidence (solid matrix movement); (4) experimental confirmation that organic groundwater contaminants produced during an underground coal gasification experiment can be removed by appropriate bacterial treatment; (5) development of data supporting the extension of the Greenville Fault Zone into the Northern Diablo Range (Alameda and Santa Clara Counties, California); (6) completion of a literature review on hazardous waste (current disposal technology, regulations, research needs); (7) preparation of a map showing levels of background seismic noise in the USSR; (8) demonstration of a correlation of explosion size with the P-wave magnitude of the seismic signal produced by the explosion; and (9) reduction of data showing the extent of ground motion resulting from subsidence in the vicinity of the Hoe Creek III experiment, Underground Coal Gasification Project.

  9. Identifying with Science: A case study of two 13-year-old `high achieving working class' British Asian girls

    Science.gov (United States)

    Wong, Billy

    2012-01-01

    This paper provides an in-depth, 'case study' style analysis of the experiences of two 13-year-old British Asian girls from a larger qualitative study investigating minority ethnic students' aspirations in science. Through the lens of identity as performativity and Bourdieu's notions of habitus and capital, the ways in which two girls engage with the field of science is examined. Samantha is British Indian and Fay is British Bangladeshi and they are both 'top set' students in science, but only one aspired to study triple science, while the other desired to be 'famous'. The experiences of the two girls are explicated in this paper, teasing out their experiences and constructions of science. It is argued that cultural discourses of family, peers and teacher expectations can shape students' perceptions of science and education.

  10. Teaching Galileo? Get to know Riccioli! -- What a forgotten Italian astronomer can teach students about how science works

    CERN Document Server

    Graney, Christopher M

    2011-01-01

    What can physics students learn about science from those scientists who got the answers wrong? Students encounter little science history, and what they have encountered typically portrays scientists as The People with the Right Answers. But those who got the wrong answers can teach students that in science answers are often elusive -- not found in the back of a book or discovered in a bold stroke of genius. Giovanni Battista Riccioli, a 17th-century astronomer who argued that science supported a geocentric universe, and whose arguments made sense given the knowledge of the time -- is an example of such a person.

  11. Communicating Ocean Sciences to Informal Audiences (COSIA): Universities, Oceanographic Institutions, Science Centers and Aquariums Working Together to Improve Ocean Education and Public Outreach

    Science.gov (United States)

    Glenn, S.; McDonnell, J.; Halversen, C.; Zimmerman, T.

    2006-12-01

    Ocean observatories have already demonstrated their ability to maintain long-term time series, capture episodic events, provide context for improved shipboard sampling, and improve accessibility to a broader range of participants. Communicating Ocean Sciences, an already existing college course (http://www.cacosee.net/collegecourse) from COSEE California has demonstrated its ability to teach future scientists essential communication skills. The NSF-funded Communicating Ocean Sciences to Informal Audiences (COSIA) project will leverage these experiences and others to demonstrate a long-term model for promoting effective science communication skills and techniques applicable to diverse audiences. The COSIA effort will be one of the pathfinders for ensuring that the new scientific results from the increasing U.S. investments in ocean observatories is effectively communicated to the nation, and will serve as a model for other fields. Our presentation will describe a long-term model for promoting effective science communication skills and techniques applicable to diverse audiences. COSIA established partnerships between informal science education institutions and universities nationwide to facilitate quality outreach by scientists and the delivery of rigorous, cutting edge science by informal educators while teaching future scientists (college students) essential communication skills. The COSIA model includes scientist-educator partnerships that develop and deliver a college course derived from COS that teaches communication skills through the understanding of learning theory specifically related to informal learning environments and the practice of these skills at aquariums and science centers. The goals of COSIA are to: provide a model for establishing substantive, long-term partnerships between scientists and informal science education institutions to meet their respective outreach needs; provide future scientists with experiences delivering outreach to informal

  12. Development of Environmental Knowledge, Team Working Skills and Desirable Behaviors on Environmental Conservation of Matthayomsuksa 6 Students Using Good Science Thinking Moves Method with Metacognition Techniques

    Science.gov (United States)

    Ladawan, Charinrat; Singseewo, Adisak; Suksringarm, Paitool

    2015-01-01

    The research aimed to investigate environmental knowledge, team working skills, and desirable behaviors of students learning through the good science thinking moves method with metacognition techniques. The sample group included Matthayomsuksa 6 students from Nadoon Prachasan School, Nadoon District, Maha Sarakham Province. The research tools were…

  13. [20th century Galileo? The significance of Freud's life and work, seen in terms of the history of science (lecture on May 6th, 2006)].

    Science.gov (United States)

    Hirschmiüller, Albrecht

    2006-01-01

    This paper gives a sketch of Freud's life and work, discusses the difficulties of reception he met, and, referring to the well-known statement that psychoanalysis represents the third blow to the narcissism of mankind, maintains that, in terms of the history of science, a more meaningful parallel can be drawn between Freud and Galileo than between Freud and Copernicus or Darwin.

  14. Impact of "Grassroots on Work" (GROW) Extension Program to the Bachelor of Arts in Political Science Students' Sense of Civic Responsibility

    Science.gov (United States)

    Paga, Mark Leo Huit

    2015-01-01

    Purpose: The purpose of this study was to determine the medium term effect of service-learning program or "Grassroots on Work" extension program to civic responsibility of AB Political Science students. Methodology: This study employed an impact evaluation research design and both qualitative and quantitative. The data on goals and…

  15. Unsustainable Growth, Hyper-Competition, and Worth in Life Science Research: Narrowing Evaluative Repertoires in Doctoral and Postdoctoral Scientists' Work and Lives

    Science.gov (United States)

    Fochler, Maximilian; Felt, Ulrike; Müller, Ruth

    2016-01-01

    There is a crisis of valuation practices in the current academic life sciences, triggered by unsustainable growth and "hyper-competition." Quantitative metrics in evaluating researchers are seen as replacing deeper considerations of the quality and novelty of work, as well as substantive care for the societal implications of research.…

  16. Professional development that works: Impacting elementary science teachers' learning and practice during the implementation of an inquiry-oriented science curriculum

    Science.gov (United States)

    Schlang, Jodi A.

    One of the most important factors for developing science literacy for all students is teacher knowledge of science content and pedagogy. This study was designed to evaluate the impact of professional development on teacher learning, changes in teacher behavior, and student learning. The goal was to develop a deeper understanding of how the Elementary Science Teaching and Learning (ESTL) program affected teacher learning and changed teacher behavior in the classroom. This study also provided insight into the effect of the ESTL program on student learning during the first year of the professional development. This mixed method case study was used to examine the link between participation in the ESTL program, teacher learning, changes in teacher classroom behavior, and student learning. Qualitative observations and videotaped sessions provided rich description of the professional development and implementation of inquiry-oriented strategies in participant's classrooms. Artifacts and interviews provided evidence of teacher learning and changes in teacher behaviors. Quantitative data included self-report survey data examining changes in teacher behavior and the measurement of student learning used both science district assessment scores and CSAP writing scores. Key findings include: (1) teacher learning was reported in the areas of questioning and scope and sequence of the curriculum occurred; (2) statistically significant changes teacher behavior were reported and were noted in teacher interviews; (3) participation in the ESTL program did not positively impact student learning; (4) unanticipated findings include the role of camaraderie in professional development and the role of additional training in teacher's confidence in both their own teaching and in helping others; and, (5) teacher's perceptions identified the role of inquiry-based science curriculum as providing the rich experiences necessary for improved student writing. Overall participation in the ESTL

  17. Lesson Adaptations and Accommodations: Working with Native Speakers and English Language Learners in the Same Science Classroom

    Science.gov (United States)

    Rice, Diana C.; Pappamihiel, N. Eleni; Lake, Vickie E.

    2004-01-01

    This article brings theory into practice and demonstrates clearly how to apply commonly accepted language acquisition theories to science lesson plans designed for native speakers of English. In the first section of the article, readers will learn not only how to apply theory to science lessons, but also, and more important, why to apply certain…

  18. Portraying Science as Humanism--A Historical Case Study of Cultural Boundary Work from the Dawn of the "Atomic Age"

    Science.gov (United States)

    Lynning, Kristine Hays

    2007-01-01

    In the late 1950s, when a new curriculum for the Danish upper secondary school was under construction, the reform debates on science were strongly concerned with the scarcity of technologically and scientifically educated labour, and thus relations between science, technology and welfare were stressed. Simultaneously however, the relationship…

  19. Becoming (Less) Scientific: A Longitudinal Study of Students' Identity Work from Elementary to Middle School Science

    Science.gov (United States)

    Carlone, Heidi B.; Scott, Catherine M.; Lowder, Cassi

    2014-01-01

    Students' declining science interest in middle school is often attributed to psychological factors like shifts of motivational values, decrease in self-efficacy, or doubts about the utility of schooling in general. This paper adds to accounts of the middle school science problem through an ethnographic, longitudinal case study of three…

  20. The Duty to Prevent Emotional Harm at Work: Arguments from Science and Law, Implications for Policy and Practice

    Science.gov (United States)

    Shain, Martin

    2004-01-01

    Although science and law employ different methods to gather and weigh evidence, their conclusions are remarkably convergent with regard to the effect that workplace stress has on the health of employees. Science, using the language of probability, affirms that certain stressors predict adverse health outcomes such as disabling anxiety and…

  1. Emotional and Motivational Outcomes of Lab Work in the Secondary Intermediate Track: The Contribution of a Science Center Outreach Lab

    Science.gov (United States)

    Itzek-Greulich, Heike; Vollmer, Christian

    2017-01-01

    Students' interest in science declines in secondary school. Therefore, motivating students to become competent and engaged in science topics that are relevant for their everyday lives is an important goal, so they can be better citizens and decision makers with socioscientific issues (e.g., climate change and waste disposal). The present study…

  2. Boundary-Work in the Health Research Field: Biomedical and Clinician Scientists' Perceptions of Social Science Research

    Science.gov (United States)

    Albert, Mathieu; Laberge, Suzanne; Hodges, Brian D.

    2009-01-01

    Funding agencies in Canada are attempting to break down the organizational boundaries between disciplines to promote interdisciplinary research and foster the integration of the social sciences into the health research field. This paper explores the extent to which biomedical and clinician scientists' perceptions of social science research operate…

  3. Portraying Science as Humanism--A Historical Case Study of Cultural Boundary Work from the Dawn of the "Atomic Age"

    Science.gov (United States)

    Lynning, Kristine Hays

    2007-01-01

    In the late 1950s, when a new curriculum for the Danish upper secondary school was under construction, the reform debates on science were strongly concerned with the scarcity of technologically and scientifically educated labour, and thus relations between science, technology and welfare were stressed. Simultaneously however, the relationship…

  4. Boundary-Work in the Health Research Field: Biomedical and Clinician Scientists' Perceptions of Social Science Research

    Science.gov (United States)

    Albert, Mathieu; Laberge, Suzanne; Hodges, Brian D.

    2009-01-01

    Funding agencies in Canada are attempting to break down the organizational boundaries between disciplines to promote interdisciplinary research and foster the integration of the social sciences into the health research field. This paper explores the extent to which biomedical and clinician scientists' perceptions of social science research operate…

  5. Experimenting with an Alternative Teaching Approach on "Metals." Learning in Science Project (Primary). Working Paper No. 113.

    Science.gov (United States)

    Biddulph, Fred; McMinn, Bill

    An alternative approach for teaching primary school science has been proposed by the Learning in Science Project (Primary--LISP(P). This study investigated the use of the approach during three series of lessons on the topic "metals." Each series followed the same general pattern: (1) an introductory session to stimulate children to ask…

  6. Science cases, wavelength ranges, and strategies for ELTs: some remarks and conclusions

    Science.gov (United States)

    Gustafsson, Bengt

    2008-04-01

    Discussions at the Symposium ELTs: Which wavelengths? in Lund in December 2007 are summarized and in particular comments are made on the relation between the optimization of the presently planned ELTs, and their corresponding background science cases. The division of labour between the ELTs and the JWST is commented on. The need for an ELT (and/or a future Space Telescope) for the optical wavelength region is stressed. Possible strategies for pursuing the ELT projects are commented on.

  7. Framing Doctoral Education for a Science of Social Work: Positioning Students for the Scientific Career, Promoting Scholars for the Academy, Propagating Scientists of the Profession, and Preparing Stewards of the Discipline

    Science.gov (United States)

    Fong, Rowena

    2014-01-01

    Social work education grounded in social work practice has been recently challenged to examine the role of science in its history, core constructs and domains, philosophical underpinnings, and graduate curriculum. Doctoral education has been added to the scrutiny at the recent Science in Social Work Roundtable in Doctoral Education. Based on Lev…

  8. Measurement of Nursing's Complex Health Care Work: Evolution of the Science For Determining the Required Staffing For Safe and Effective Patient Care.

    Science.gov (United States)

    Malloch, Kathy

    2015-01-01

    The availability of technology to monitor and manage data increases our ability to better understand the processes and outcomes needed for patient care. It is important to remember this work requires not only the science of data management, but also the art of integrating the multiple variables involved in the dynamic of safe staffing. Fasoli and Haddock (2010) provided an excellent summary of the literature. Nurse leaders must be open to new additions to this work and the possibility that the essential ingredient of the gold standard for patient classification systems (PCS) might still be missing. The goal of a new approach to determine time for nurse work was to advance the science of PCS from the perspective of the characteristics identified by Fasoli and Haddock.

  9. National works of soldiers and officers of the Great Patriotic War of 1941–1945 in documents of Russian Academy of Sciences Archive

    Directory of Open Access Journals (Sweden)

    Mikhail Yu. Kiselyov

    2016-09-01

    Full Text Available Information on work of Institute of ethnography of Academy of Sciences of the USSR on collecting in 1944–1945 of works of national works of the soldiers and officers of Red Army created by them in the period of the Great Patriotic War 1941–1945 gg. is provided in article or in the first post-war years. The texts of poems, chastushkas and the story of soldiers and officers postponed in archival fund of institute in Archive of the Russian Academy of Sciences are provided. Letters of soldiers and officers of Red Army can fill up source study base on stories of the Great Patriotic War of 1941–1945 and domestic culture, they can be used both in research, and in the educational purposes.

  10. Goddard's Astrophysics Science Divsion Annual Report 2014

    Science.gov (United States)

    Weaver, Kimberly (Editor); Reddy, Francis (Editor); Tyler, Pat (Editor)

    2015-01-01

    The Astrophysics Science Division (ASD, Code 660) is one of the world's largest and most diverse astronomical organizations. Space flight missions are conceived, built and launched to observe the entire range of the electromagnetic spectrum, from gamma rays to centimeter waves. In addition, experiments are flown to gather data on high-energy cosmic rays, and plans are being made to detect gravitational radiation from space-borne missions. To enable these missions, we have vigorous programs of instrument and detector development. Division scientists also carry out preparatory theoretical work and subsequent data analysis and modeling. In addition to space flight missions, we have a vibrant suborbital program with numerous sounding rocket and balloon payloads in development or operation. The ASD is organized into five labs: the Astroparticle Physics Lab, the X-ray Astrophysics Lab, the Gravitational Astrophysics Lab, the Observational Cosmology Lab, and the Exoplanets and Stellar Astrophysics Lab. The High Energy Astrophysics Science Archive Research Center (HEASARC) is an Office at the Division level. Approximately 400 scientists and engineers work in ASD. Of these, 80 are civil servant scientists, while the rest are resident university-based scientists, contractors, postdoctoral fellows, graduate students, and administrative staff. We currently operate the Swift Explorer mission and the Fermi Gamma-ray Space Telescope. In addition, we provide data archiving and operational support for the XMM mission (jointly with ESA) and the Suzaku mission (with JAXA). We are also a partner with Caltech on the NuSTAR mission. The Hubble Space Telescope Project is headquartered at Goddard, and ASD provides Project Scientists to oversee operations at the Space Telescope Science Institute. Projects in development include the Neutron Interior Composition Explorer (NICER) mission, an X-ray timing experiment for the International Space Station; the Transiting Exoplanet Sky Survey (TESS

  11. Science or Science Fiction?

    DEFF Research Database (Denmark)

    Lefsrud, Lianne M.; Meyer, Renate

    2012-01-01

    This paper examines the framings and identity work associated with professionals’ discursive construction of climate change science, their legitimation of themselves as experts on ‘the truth’, and their attitudes towards regulatory measures. Drawing from survey responses of 1077 professional......, legitimation strategies, and use of emotionality and metaphor. By linking notions of the science or science fiction of climate change to the assessment of the adequacy of global and local policies and of potential organizational responses, we contribute to the understanding of ‘defensive institutional work...

  12. Historical and Epistemological Reflections on the Culture of Machines around the Renaissance: How Science and Technique Work?

    Directory of Open Access Journals (Sweden)

    Raffaele Pisano

    2014-10-01

    Full Text Available This paper is divided into two parts, this being the first one. The second is entitled ‘Historical and Epistemological Reflections on the Culture of Machines around Renaissance: Machines, Machineries and Perpetual Motion’ and will be published in Acta Baltica Historiae et Philosophiae Scientiarum in 2015. Based on our recent studies, we provide here a historical and epistemological feature on the role played by machines and machineries. Ours is an epistemological thesis based on a series of historical examples to show that the relations between theoretical science and the construction of machines cannot be taken for granted, a priori. Our analysis is mainly based on the culture of machines around 15th and 17th centuries, namely the epoch of Late Renaissance and Early Modern Age. For this is the period of scientific revolution and this age offers abundant interesting material for researches into the relations of theoretical science/construction of machines as well. However, to prove our epistemological thesis, we will also exploit examples of machines built in other historical periods. Particularly, a discussion concerning the relationship between science theory and the development of science art crafts produced by non-recognized scientists in a certain historical time is presented. The main questions are: when and why did the tension between science (physics, mathematics and geometry give rise to a new scientific approach to applied discipline such as studies on machines and machineries? What kind of science was used (if at all for projecting machines and machineries? Was science at the time a necessary precondition to build a machine? In the first part we will focus on the difference between Aristotelian-Euclidean and Archimedean approaches and we will outline the heritage of these two different approaches in late medieval and Renaissance science. In the second part, we will apply our reconstructions to some historical and epistemological

  13. Poetry, Nature and Science: Romantic Nature Philosophy in the Works of Novalis and E. T. a. Hoffmann

    Science.gov (United States)

    Weisend, Ausma Skerbele

    The nature philosophy of the early Romantic period in Germany attempted to find a synthesis of science and philosophy in a new philosophy of nature. This philosophy was first formulated by F. W. J. Schelling and influenced by the galvanic experiments of J. W. Ritter. Novalis is a unique figure in romanticism since he combines scientific expertise with philosophical insight and poetic imagination. In Lehrlinge zu Sais he explores the significance of nature's language and presents different relationships between man and nature. Novalis thinks that a synthesis of all divergent elements in nature and society is necessary to transform the world. In Klingsohrs Marchen this transformation is accomplished by poetic activation of the physical sciences and by the power of love. After 1800 the romantic movement becomes interested in the problems of subconscious and abnormal psychological states, which are seen as contacts with a more spiritual level of existence. These ideas, expressed in a popular form by G. H. Schubert, provide a rich source of materials for E. T. A. Hoffmann, who elevates the realms of poetry and music in his fairy tales, but sees only negative qualities in science. Hoffmann's protagonists find that love, music, and poetry are the greatest forces in life. The figure of the scientist becomes an evil magician with no regard for human values. The romantic movement failed to unite the values of humanities with the insights of physical sciences. The problem of autonomy isolates both modern science and modern literature from the ethical values of society.

  14. Negotiating the relevance of laboratory work: Safety, procedures and accuracy brought to the fore in science education

    Directory of Open Access Journals (Sweden)

    Mattias Lundin

    2014-04-01

    Full Text Available This text addresses the problem of the discrepancy between teachers’ and students’ positions in negotiations about the authenticity and legitimacy of school science activities. The study focuses on the apparent conflicts concerning legitimacy and authenticity when teachers and students bring attention to safety, authenticity and accuracy during issues laboratory activities. The analysed data are excerpts made from video observations in two science classes. Analysis was made using epistemological moves describing how teachers and students make their activities relevant. The result indicates that in the classroom conversation about laboratory practice, teachers sometimes draw the attention to safety, procedures and accuracy to legitimize the activity and how they try to control it. Negotiations concerning the legitimacy and authenticity of activities seem inevitable. Unless understandable agreements are reached, the negotiations jeopardize a successful understanding of the Nature of Science (NOS. Misunderstanding of the authenticity of activities contributes to a reduction of their legitimacy, and undermining teaching of context independent knowledge.

  15. The "invention" of the working class as a discursive practice and the genesis of the empiric method of social sciences in France (1830-48

    Directory of Open Access Journals (Sweden)

    Federico Tomasello

    2016-12-01

    Full Text Available The essay explores some of the processes through which the ‘working class’ emerged both as a collective subjectivity and as a field of social science inquiry and public policies in 19th century France. Starting from the 1831 Canuts revolt, widely recognized as the stepping stone of the European workers’ movement, the first part retraces the process of the ‘making’ of a social and political subjectivity by stressing the relevance of its linguistic and discursive dimension. The second part examines the emergence of the empiric method of the modern social sciences through new strategies of inquiry on urban misery, which progressively focuses on the ‘working class’ and on labour conditions as a field of knowledge, rights, and governmental practices.

  16. Development and Acceptance Testing of the Dual Wheel Mechanism for the Tunable Filter Imager Cryogenic Instrument on the JWST

    Science.gov (United States)

    Leckie, Martin; Ahmad, Zakir

    2010-01-01

    The James Webb Space Telescope (JWST) will carry four scientific instruments, one of which is the Tunable Filter Imager (TFI), which is an instrument within the Fine Guidance Sensor. The Dual Wheel (DW) mechanism is being designed, built and tested by COM DEV Ltd. under contract from the Canadian Space Agency. The DW mechanism includes a pupil wheel (PW) holding seven coronagraphic masks and two calibration elements and a filter wheel (FW) holding nine blocking filters. The DW mechanism must operate at both room temperature and at 35K. Successful operation at 35K comprises positioning each optical element with the required repeatability, for several thousand occasions over the five year mission. The paper discusses the results of testing geared motors and bearings at the cryogenic temperature. In particular bearing retainer design and PGM-HT material, the effects of temperature gradients across bearings and the problems associated with cooling mechanisms down to cryogenic temperatures. The results of additional bearing tests are described that were employed to investigate an abnormally high initial torque experienced at cryogenic temperatures. The findings of these tests, was that the bearing retainer and the ball/race system could be adversely affected by the large temperature change from room temperature to cryogenic temperature and also the temperature gradient across the bearing. The DW mechanism is now performing successfully at both room temperature and at cryogenic temperature. The life testing of the mechanism is expected to be completed in the first quarter of 2010.

  17. Towards Precise Constraints on the Chemical Compositions and Thermal Structures of Giant Exoplanets with a JWST GTO Program

    Science.gov (United States)

    Bean, Jacob; Lunine, Jonathan I.

    2017-06-01

    The chemical compositions and thermal structures of close-in planets are two of the major questions raised over the last 15+ years of exoplanet atmospheric characterization. These are fundamental questions in their own right, and answering them also has the potential to improve our understanding of the planets in the Solar System. JWST offers the opportunity to make a major advance on these topics by revealing a more complete and accurate inventory of the chemical species in exoplanet atmospheres and by precisely measuring atmospheric temperatures over a broad range of pressures. I will describe how we plan to use an Interdisciplinary Scientist GTO program to determine the compositions and thermal structures of transiting, hot giant exoplanets using dayside thermal emission measurements obtained at secondary eclipse. Our composition measurements are focused on determining absolute molecular abundances as a tracer of atmospheric metallicity and the abundance ratio of carbon to oxygen. The targets in our program have a range of masses and irradiation, which will enable us to test theories of how atmospheric metallicity varies with planet mass and how thermal structures respond to different levels of stellar forcing.

  18. Workshop “Science with the VLT in the ELT Era”

    CERN Document Server

    Astrophysics and Space Science Proceedings

    2008-01-01

    The Workshop ‘Science with the VLT in the ELT era’ was organised by ESO as a forum for the astronomical community to debate its expected future use of ESO’s Very Large Telescope ( and its VLTI interferometric mode) when other facilities such as ALMA, JWST and, hopefully, at least one extremely large 30-40m class telescope will be operating. VLT/I science highlights were presented, future science priorities argued, synergies between the VLT and the future facilities confirmed and specific new VLT/I instruments proposed.

  19. Math and Science Education with English Language Learners: Contributions of the DR K-12 Program. Targeted Study Group Working Paper

    Science.gov (United States)

    Martinez, Alina; Rhodes, Hilary; Copson, Elizabeth; Tiano, Megan; DellaRocco, Nicole; Donoghue, Nathaniel; Marco, Lisa

    2011-01-01

    Although educational leaders, policy makers, and researchers have long emphasized the importance of science, technology, engineering, and mathematics (STEM) for the country's continued prosperity, increasing participation in STEM has remained a challenge for both the education and scientific communities (Pearson & Fechter, 1994; National…

  20. Analogies as Tools for Meaning Making in Elementary Science Education: How Do They Work in Classroom Settings?

    Science.gov (United States)

    Guerra-Ramos, Maria Teresa

    2011-01-01

    In this paper there is a critical overview of the role of analogies as tools for meaning making in science education, their advantages and disadvantages. Two empirical studies on the use of analogies in primary classrooms are discussed and analysed. In the first study, the "string circuit" analogy was used in the teaching of electric circuits with…

  1. Developing Low-Cost Solutions to Improve Public Policy: The Work of MDRC's Center for Applied Behavioral Science. Issue Focus

    Science.gov (United States)

    MDRC, 2016

    2016-01-01

    Many social policy and education programs start from the assumption that people act in their best interest. But behavioral science shows that people often weigh intuition over reason, make inconsistent choices, and put off big decisions. The individuals and families who need services and the staff who provide them are no exception. From city…

  2. Hot Spots and Mantle Plumes: A Window Into the Deep Earth and a Lesson on How Science Really Works

    Science.gov (United States)

    Caplan-Auerbach, J.

    2010-12-01

    Despite years of discussion, debate and controversy over the causes of ocean island volcanism, most students simply learn that such features form from fixed plumes of hot material rising from the core mantle boundary. Although we know that the Hawaiian plume exhibited substantial southward motion, most introductory geology textbooks still report that hot spots are fixed and that the Hawaiian-Emperor bend reflects a change in plate motion. That mantle plumes are the focus of significant controversy within the scientific community is rarely, if ever, discussed, and alternative models for the formation of intraplate volcanoes are ignored. Students may thus complete their studies without learning about the dynamic debate focused on the existence and formation of mantle plumes. This issue represents an opportunity for students to see how science really works, how new models are constructed, and what distinguishes a hypothesis from a theory. The culminating project in Western Washington University’s Introduction to Geophysics class, a course required for the BS degree in geology, focuses on the hot spot and mantle plume debate. For the first nine weeks of the quarter students learn about general topics in geophysics including plate tectonics, magnetism, seismology, gravity and heat flow. At the end of the course, students break into small research groups with the goal of investigating how geophysics may be used to address three questions: (1) Do ocean island volcanoes form from mantle plumes? (2) Are “hot spots” actually hot? (3) Are hot spots stationary? Each group examines how these questions may be addressed using a specific geophysical tool. In addition to the five topics described above, a sixth group investigates the question of “if not hot spots/mantle plumes, how do ocean island volcanoes form?” Students read the current literature on the topic and present their results to their classmates. Presentations focus on topics such as the use of seismic

  3. Empirical study on work value of science and engineering college students%理工科大学生职业价值观实证研究

    Institute of Scientific and Technical Information of China (English)

    沈克祥

    2012-01-01

    目的:探讨理工科大学生职业价值观特点,为职业生涯教育工作提供依据。方法:采用个人价值观问卷(PVS)对410名理工科大学生进行测试,并进行统计分析。结果:理工科大学生实用型价值观偏好明显;不同专业学生价值观类型偏好存在差异,理科生偏好实用一科学型,工科生偏好实用型,商科生偏好实用一政治型。结论:理工科大学生职业价值观总体有偏好,不同专业类型价值观存在差异。%Objective To investigate the characteristics of work value of the science and engineering col- lege students, and provide some reference materials for career education. Methods The 410 science and engineering college students were randomly collected to take the questionnaire of personal value state- ment(PVS),and the data were statistically analyzed. Results The college students of science and egi- neering prefered economic value obviously, and the difference existed among the different major, sci- ence students prefered economic--science value, engineering students prefered ecnomic value, bussiness students prefered economic--political value. Conclusion there were some tendency about the work value of science and engineering college students generally, the difference existed among the different major.

  4. Alignment test results of the JWST Pathfinder Telescope mirrors in the cryogenic environment

    Science.gov (United States)

    Whitman, Tony L.; Wells, Conrad; Hadaway, James B.; Knight, J. Scott; Lunt, Sharon

    2016-07-01

    After integration of the Optical Telescope Element (OTE) to the Integrated Science Instrument Module (ISIM) to become the OTIS, the James Webb Space Telescope OTIS is tested at NASA's Johnson Space Center (JSC) in the cryogenic vacuum Chamber A for alignment and optical performance. The alignment of the mirrors comprises a sequence of steps as follows: The mirrors are coarsely aligned using photogrammetry cameras with reflective targets attached to the sides of the mirrors. Then a multi-wavelength interferometer is aligned to the 18-segment primary mirror using cameras at the center of curvature to align reflected light from the segments and using fiducials at the edge of the primary mirror. Once the interferometer is aligned, the 18 primary mirror segments are then adjusted to optimize wavefront error of the aggregate mirror. This process phases the piston and tilt positions of all the mirror segments. An optical fiber placed at the Cassegrain focus of the telescope then emits light towards the secondary mirror to create a collimated beam emitting from the primary mirror. Portions of the collimated beam are retro-reflected from flat mirrors at the top of the chamber to pass through the telescope to the Science Instrument (SI) detector. The image on the detector is used for fine alignment of the secondary mirror and a check of the primary mirror alignment using many of the same analysis techniques used in the on-orbit alignment. The entire process was practiced and evaluated in 2015 at cryogenic temperature with the Pathfinder telescope.

  5. Impact of the Diamond Light Source on research in Earth and environmental sciences: current work and future perspectives

    OpenAIRE

    Burke, IT; Mosselmans, FW; S. Shaw; Peacock, CL; Benning, LG; Coker, VS

    2015-01-01

    Diamond Light Source Ltd celebrated its 10th anniversary as a company in December 2012 and has now accepted user experiments for over 5 years. This paper describes the current facilities available at Diamond and future developments that enhance its capacities with respect to the Earth and environmental sciences. A review of relevant research conducted at Diamond thus far is provided. This highlights how synchrotron-based studies have brought about important advances in our understanding of th...

  6. Harnessing the Power of Digital Data for Science and Society: Report of the Interagency Working Group on Digital Data to the Committee on Science of the National Science and Technology Council

    Data.gov (United States)

    Networking and Information Technology Research and Development, Executive Office of the President — This report provides a strategy to ensure that digital scientific data can be reliably preserved for maximum use in catalyzing progress in science and...

  7. Plurality and Fragmentation in Social Work: Analyzing the Implications of Flexner Using a Philosophy of Science Perspective

    Science.gov (United States)

    Brady, Shane R.; Moxley, David

    2016-01-01

    The authors examine how the profession's adaptation to Flexner's criteria influences the emergence of the neomedical model as the majoritarian paradigm within social work even in the face of a pluralism manifest by the existence of other competing paradigms. One endorses empowerment in social work, and the other embraces societal transformation in…

  8. Plurality and Fragmentation in Social Work: Analyzing the Implications of Flexner Using a Philosophy of Science Perspective

    Science.gov (United States)

    Brady, Shane R.; Moxley, David

    2016-01-01

    The authors examine how the profession's adaptation to Flexner's criteria influences the emergence of the neomedical model as the majoritarian paradigm within social work even in the face of a pluralism manifest by the existence of other competing paradigms. One endorses empowerment in social work, and the other embraces societal transformation in…

  9. The Learning of Science Basic Concept by Using Scientifiq Inquiry to Improve Student’s Thinking, Working, and Scientific Attitude Abilities

    Directory of Open Access Journals (Sweden)

    Wachidatul Linda Yuhanna

    2016-03-01

    Full Text Available This research was a classroom action research which was conducted intwo cycles, each cycle consists of planning, implementing, observing, and reflecting. The data used was quantitative data on student observation sheet instruments. The Results of the study which were obtained from the first cycle showed about the students’ thinking skills and scientific works. They were categorized as excellent 18.18%, good 22.73%, enough 52.27%, and sufficiently less 6.82%. As for the scientific attitude with a very active category of 11.36%, 43.18% and less active 45.45%. It has not reached indicators of success, so it was necessary to cycle II. Cycle II demonstrated the excellent category 38.63%, 36.36% good, good enough18.18% and less 6.81%. While the scientific attitude in the cycle II was an active attitude 29.54%, active 54.54%, inactive 15.91%. These results show an increase from the cycle I to cycle II. The conclusion of this study were: 1 learning the basic concepts of science with scientific inquiry in students can be conducible applied.2 Learning the basic concepts of science with scientific inquiry can improve thinking ability and scientific work and students’ scientific attitude. 3 Learning the basic concepts of science with scientific inquiry be able to explore and develop student creativity in designing simple experiments which can be applied in primary schools.

  10. RESEARCH ON THE PROBLEMS OF interaction BETWEEN SCIENCE AND RELIGION IN UNIVERSITY COURSE OF PHILOSOPHY (BASED ON WORKS BY RUSSIAN RELIGIOUS THINKERS

    Directory of Open Access Journals (Sweden)

    Aleksey I. Belkin

    2016-03-01

    Full Text Available Introduction: the article explores the interrelations between science and religion in the context of shaping integrated world outlook of future specialists in the framework of the competence-based approach. Axiological and ethical aspects of the interaction between the two major branches of human culture are considered using the example of works by Russian religious thinkers: Archbishop Luke (V. F. Voyno-Yasenetsky, V. S. Soloviev, N. A. Berdyaev. Materials and Methods: materials and methods: the study employed the method of original sources, i. e. works by N. A. Berdyaev, V. F. Voino-Yasenetsky, V. S. Solovyov, considering the problems of interaction between science and religion. The method of original sources was combined with methods of analysis, synthesis and generalisation. Results: attention is paid to different approaches to addressing this problem over the historical development of human thought. When analysing the works by V. S. Solovyov emphasis is made on the concept of integral knowledge, considering the true knowledge as a result of the interaction of rational, empirical and mystical aspects. Much attention is paid to the interpretation of Archbishop Luke’s thoughts (V. F. Voyno-Yasenetsky who advocated theoretically and practically the idea of the synthesis of the knowledge and belief in their inextricable link to the genuine scientific and philosophical works. When discussing N. A. Berdyaev’s ideas the focus is on the critical analysis of the three types of relationships between science and religion, established in human culture: 1 supremacy of knowledge and denial of faith, 2 supremacy of faith and denial of knowledge, and 3 the dualism of knowledge and faith. The article also gives a thorough account of the philosopher’s idea about the synthesis of knowledge, faith and intuition that contradicts traditional approach. The article presents the arguments of modern science about the importance of interaction between religious

  11. Wetlands Work

    Science.gov (United States)

    Messina, Linda; Blanchard, Pamela Borne

    2004-01-01

    This article describes how a biology teacher's search for a cross-curricular project in science, math, history, and environmental science, that would help her students connect what they were learning in the classroom to their everyday life, resulted in an ongoing stewardship project. Working together with the Louisiana Sea Grant College Program…

  12. Wetlands Work

    Science.gov (United States)

    Messina, Linda; Blanchard, Pamela Borne

    2004-01-01

    This article describes how a biology teacher's search for a cross-curricular project in science, math, history, and environmental science, that would help her students connect what they were learning in the classroom to their everyday life, resulted in an ongoing stewardship project. Working together with the Louisiana Sea Grant College Program…

  13. A Comparison between Science Fiction Works of Arthur C. Clarke and Douglas Adams's Parody of the Genre

    OpenAIRE

    Horák, Michal

    2017-01-01

    The first purpose of this paper is to define the term of science fiction genre, using literature specialized in the subject and later analyse the theoretical concept of parody in literature. The second part of the paper will consist of brief biographies of both authors (Arthur C. Clarke and Douglas Adams) and an analysis of Clarke's novel series Space Odyssey. The purpose of this paper is a comparison of Clarke's legendary series with Adams' parody of the genre The Hitchhiker's Guide to the G...

  14. Survey on distributing situation in nursing group working in Tehran Medical Science University Emam Khomeinee Hospital During2013-14

    Directory of Open Access Journals (Sweden)

    Azari S

    2017-01-01

    Full Text Available Introduction: Nowadays justice in health and injustice elimination in health section turns out to a most important concern of health systems in the world, especially for developing countries. So current research happened with purpose to survey manner of distribution and dedication ofTehran Medical Science University Emam Khomeinee (may rest in peace Hospital nursing staff. Analysis method: The studying society of this descriptive analytical research in Tehran Medical Science University Emam Khomeinee Hospital During 2013-14 includes entire units nursing group personnel (Nurse, Paramedic and Nurse Aid. Information has been gathered by self-made forms and data analyzing has done by EXCEL Software, Descriptive statistical indexes and suggested standard guidance from Ministry of Health. Findings: Results of done estimation in 27 units of studying hospital and comparing that to current situation shows that based on suggested pattern of Health Ministry just one unit (3.7% from manpower staff matches this pattern, 18 units (66.67% were lower and 8 units (29.62% were far upon this pattern. Conclusion: Generally in studying hospital lack of nursing staff was obvious that combination and distribution of nursing forces in their different units was uneven and they didn’t match the current situation. Hereupon, intended hospitals require correct management and planning in this field, so that will cause increase in hospital performance and presenting service quality to patients.

  15. Environmental health research recommendations from the Inter-Environmental Health Sciences Core Center Working Group on unconventional natural gas drilling operations.

    Science.gov (United States)

    Penning, Trevor M; Breysse, Patrick N; Gray, Kathleen; Howarth, Marilyn; Yan, Beizhan

    2014-11-01

    Unconventional natural gas drilling operations (UNGDO) (which include hydraulic fracturing and horizontal drilling) supply an energy source that is potentially cleaner than liquid or solid fossil fuels and may provide a route to energy independence. However, significant concerns have arisen due to the lack of research on the public health impact of UNGDO. Environmental Health Sciences Core Centers (EHSCCs), funded by the National Institute of Environmental Health Sciences (NIEHS), formed a working group to review the literature on the potential public health impact of UNGDO and to make recommendations for needed research. The Inter-EHSCC Working Group concluded that a potential for water and air pollution exists that might endanger public health, and that the social fabric of communities could be impacted by the rapid emergence of drilling operations. The working group recommends research to inform how potential risks could be mitigated. Research on exposure and health outcomes related to UNGDO is urgently needed, and community engagement is essential in the design of such studies.

  16. Alignment Test Results of the JWST Pathfinder Telescope Mirrors in the Cryogenic Environment

    Science.gov (United States)

    Whitman, Tony L.; Wells, Conrad; Hadaway, James; Knight, J. Scott; Lunt, Sharon

    2016-01-01

    After integration of the Optical Telescope Element (OTE) to the Integrated Science Instrument Module (ISIM) to become the OTIS, the James Webb Space Telescope OTIS is tested at NASAs Johnson Space Center (JSC) in the cryogenic vacuum Chamber A for alignment and optical performance. The alignment of the mirrors comprises a sequence of steps as follows: The mirrors are coarsely aligned using photogrammetry cameras with reflective targets attached to the sides of the mirrors. Then a multi-wavelength interferometer is aligned to the 18-segment primary mirror using cameras at the center of curvature to align reflected light from the segments and using fiducials at the edge of the primary mirror. Once the interferometer is aligned, the 18 primary mirror segments are then adjusted to optimize wavefront error of the aggregate mirror. This process phases the piston and tilt positions of all the mirror segments. An optical fiber placed at the Cassegrain focus of the telescope then emits light towards the secondary mirror to create a collimated beam emitting from the primary mirror. Portions of the collimated beam are retro-reflected from flat mirrors at the top of the chamber to pass through the telescope to the SI detector. The image on the detector is used for fine alignment of the secondary mirror and a check of the primary mirror alignment using many of the same analysis techniques used in the on-orbit alignment. The entire process was practiced and evaluated in 2015 at cryogenic temperature with the Pathfinder telescope.

  17. Educational experiences in Chemistry with Adult and Youth: incursions at science, work and ideology and its curriculums implications

    Directory of Open Access Journals (Sweden)

    Alceu Júnior Paz da Silva

    2015-11-01

    Full Text Available The contemporary setting of huge unemployment and precarization of work has brought to Adult and Youth Education courses an imaginary that secondary education is fundamental for professional qualification and achievement of (better jobs. The objective of this work is to problematize the Chemistry curriculum according to young and adults interests in order to qualify them to the world of work. For that purpose, we adopted some contributions of Gramsci’s Marxist social theory as methodological and theoretical tools to investigate hegemonic aspects in which the curriculum is immersed. By analyzing the curriculum as a space of struggle for social hegemony, we conclude that is promising to explore the historical approach of the chemical knowledge as a mediator element of counter-hegemonic educational practices.

  18. On A Project Work for International Students Paired with Japanese Partners in a Summer Intensive Japanese Program for Science and Technology

    Science.gov (United States)

    Fudano, Hiroko

    A project work in which learners of a foreign language engage in a task with the native speakers is one of the effective ways to bring in ample real communication opportunities to a classroom. This scheme also gives both parties meaningful experiences for intercultural understanding. This paper reports a “Pythagoras” machine production project in which international students were paired up with Japanese students as a part of a Japanese for science and technology course in a summer intensive program. Based on the participants‧ course evaluation data, the paper also discusses the effectiveness of the project for Japanese language learning and for promoting intercultural understanding.

  19. What works in planetary science outreach and what doesn't: an attempt to create a functional framing

    Science.gov (United States)

    Urban, Z.

    2014-04-01

    A thorough synthesis of experience from several decades (including 14 years on a full-time basis) of writing in the media and lecturing about the exploration of the Solar System and search for planets of other stars for the general public in Slovakia and in the Czech Republic is presented. The emphasis is given on detailed evaluation of specific feedbacks from readership and audience of various backgrounds and age groups communicated to the author. A list of 10 + 1 main pro arguments is compiled, consisting of reasonings (in addition to scientific or general knowledge/cultural value) like embodiment of our exploratory spirit, colonization, "emergency backup" world or worlds for mankind, comparative planetology as a tool for the explanation and full understanding of Earth's properties, transfer of environmentally unfriendly but irreplaceable (in mid term, at least) technologies to lifeless environments of other planetary bodies, etc. Similarly, a list of 5 main con arguments (like it is wasting of money badly needed to solve a number of urgent social problems, or it is in conflict with valued traditional beliefs) related to planetary exploration or manned and robotic space exploration in general is compiled. A short review of best practices how to counter them is presented alongside. It is demonstrated that one can construct a coherent, balanced framing of planetary science. It assertively supports the relevant efforts in both the general public and special groups involved (for example, enterpreneurs, politicians, members of the media, various activists) while treats the differing opinions and worldviews of critics with respect they deserve. The open conflict, if only in discussion, does not represent any way out. It is counterproductive in both the short-term and the long-term context. In fact, even sharply dissenting opinions often contain some points which can be used, with the help of empathy, psychology and - to be candid - a little, still tolerable dose of

  20. Impact of the Diamond Light Source on research in Earth and environmental sciences: current work and future perspectives

    Science.gov (United States)

    Burke, Ian T.; Mosselmans, J. Frederick W.; Shaw, Samuel; Peacock, Caroline L.; Benning, Liane G.; Coker, Victoria S.

    2015-01-01

    Diamond Light Source Ltd celebrated its 10th anniversary as a company in December 2012 and has now accepted user experiments for over 5 years. This paper describes the current facilities available at Diamond and future developments that enhance its capacities with respect to the Earth and environmental sciences. A review of relevant research conducted at Diamond thus far is provided. This highlights how synchrotron-based studies have brought about important advances in our understanding of the fundamental parameters controlling highly complex mineral–fluid–microbe interface reactions in the natural environment. This new knowledge not only enhances our understanding of global biogeochemical processes, but also provides the opportunity for interventions to be designed for environmental remediation and beneficial use. PMID:25624516

  1. Impact of the Diamond Light Source on research in Earth and environmental sciences: current work and future perspectives.

    Science.gov (United States)

    Burke, Ian T; Mosselmans, J Frederick W; Shaw, Samuel; Peacock, Caroline L; Benning, Liane G; Coker, Victoria S

    2015-03-06

    Diamond Light Source Ltd celebrated its 10th anniversary as a company in December 2012 and has now accepted user experiments for over 5 years. This paper describes the current facilities available at Diamond and future developments that enhance its capacities with respect to the Earth and environmental sciences. A review of relevant research conducted at Diamond thus far is provided. This highlights how synchrotron-based studies have brought about important advances in our understanding of the fundamental parameters controlling highly complex mineral-fluid-microbe interface reactions in the natural environment. This new knowledge not only enhances our understanding of global biogeochemical processes, but also provides the opportunity for interventions to be designed for environmental remediation and beneficial use.

  2. Shift Work and Related Health Problems among Medical and Diagnostic Staff of the General Teaching Hospitals Affiliated to Shiraz University of Medical Sciences, 2012

    Directory of Open Access Journals (Sweden)

    Zahra Sajjadnia

    2015-07-01

    Full Text Available Introduction:Today, shift work is considered as a necessity in many jobs and for some 24-hour services the use of shift-work is growing. However, shift work can lead to physiological and psycho-social problems for shift workers. This study aimed to determine the effects of shift work on the associated health problems, together with the demographic and job characteristics underlying the problems, among the medical and diagnostic staff of the general teaching hospitals affiliated to Shiraz University of Medical Sciences in 2012. Method:This study was an applied, cross-sectional and descriptive-analytical one. The study employed a sample of 205 employees from the medical and diagnostic staff using stratified sampling proportional to the size and simple random sampling methods. Data were collected using the Survey of Shift workers (SOS questionnaire, validity and reliability of which have already been confirmed. Finally, the collected data were analyzed using SPSS 16.0 software through ANOVA, Chi-square, Independent-Samples T-Test, as well as Pearson Correlation Coefficient. A P<0.05 was considered statistically significant. Results: The results showed that among the demographic and job characteristics studied, the individual, family and social problems had significant associations with work schedules, shift work and job satisfaction. In addition, there were significant associations between musculoskeletal disorders and the satisfaction of shift work; cardiovascular disorders and marital status and occupation; digestive disorders and the work schedules; sleep disorders and the satisfaction of shift work; musculoskeletal disorders, cardiovascular disorders and sleep disorders and age, job experience and shift work experience. And finally, there were significant associations among sleep disorders and age, job experience and the shift work experience. Conclusion: Based on the findings of this study, demographic characteristics such as age, marital

  3. Student Perceptions of the Value of Career Development Learning to a Work-Integrated Learning Course in Exercise Science

    Science.gov (United States)

    Reddan, Gregory; Rauchle, Maja

    2012-01-01

    Work-integrated learning has become a significant feature of Australian universities over the past decade. Earlier research indicates that some form of career development is essential to prepare undergraduate students for a competitive employment market. The 2008 National Association of Graduate Careers Advisory Services (NAGCAS) Symposium sought…

  4. Student Perceptions of the Value of Career Development Learning to a Work-Integrated Learning Course in Exercise Science

    Science.gov (United States)

    Reddan, Gregory; Rauchle, Maja

    2012-01-01

    Work-integrated learning has become a significant feature of Australian universities over the past decade. Earlier research indicates that some form of career development is essential to prepare undergraduate students for a competitive employment market. The 2008 National Association of Graduate Careers Advisory Services (NAGCAS) Symposium sought…

  5. The work of Otto Fischer and the historical development of his method of principal vectors for mechanism and machine science

    NARCIS (Netherlands)

    Wijk, van der Volkert; Herder, Just L.; Koetsier, T.; Ceccarelli, M.

    2012-01-01

    This article gives an overview of the distinctive work of Otto Fischer (1861-1916) on the motion of the human musculoskeletal system. In order to be able to derive the individual muscle forces for human in motion, he invented the method of principal vectors to describe the motion of the centers-of-m

  6. Model Predictions and Observed Performance of JWST's Cryogenic Position Metrology System

    Science.gov (United States)

    Lunt, Sharon R.; Rhodes, David; DiAntonio, Andrew; Boland, John; Wells, Conrad; Gigliotti, Trevis; Johanning, Gary

    2016-01-01

    The James Webb Space Telescope cryogenic testing requires measurement systems that both obtain a very high degree of accuracy and can function in that environment. Close-range photogrammetry was identified as meeting those criteria. Testing the capability of a close-range photogrammetric system prior to its existence is a challenging problem. Computer simulation was chosen over building a scaled mock-up to allow for increased flexibility in testing various configurations. Extensive validation work was done to ensure that the actual as-built system meet accuracy and repeatability requirements. The simulated image data predicted the uncertainty in measurement to be within specification and this prediction was borne out experimentally. Uncertainty at all levels was verified experimentally to be less than 0.1 millimeters.

  7. Cryogenic optical test planning using the Optical Telescope Element Simulator with the James Webb Space Telescope Integrated Science Instrument Module

    Science.gov (United States)

    Reichard, Timothy A.; Bond, Nicholas A.; Greeley, Bradford W.; Malumuth, Eliot M.; Melendez, Marcio; Shiri, Ron; Alves de Oliveira, Catarina; Antonille, Scott R.; Birkmann, Stephan; Davis, Clinton; Dixon, William V.; Martel, André R.; Miskey, Cherie L.; Ohl, Raymond G.; Sabatke, Derek; Sullivan, Joseph

    2016-09-01

    NASA's James Webb Space Telescope (JWST) is a 6.5 m diameter, segmented, deployable telescope for cryogenic infrared space astronomy ( 40 K). The JWST Observatory architecture includes the Optical Telescope Element (OTE) and the Integrated Science Instrument Module (ISIM) element that contains four science instruments (SIs), including a guider. The SI and guider units are integrated to the ISIM structure and optically tested at NASA Goddard Space Flight Center as an instrument suite using a telescope simulator (Optical Telescope Element SIMulator; OSIM). OSIM is a high-fidelity, cryogenic JWST telescope simulator that features a 1.5m diameter powered mirror. The SIs are aligned to the flight structure's coordinate system under ambient, clean room conditions using optomechanical metrology and customized interfaces. OSIM is aligned to the ISIM mechanical coordinate system at the cryogenic operating temperature via internal mechanisms and feedback from alignment sensors and metrology in six degrees of freedom. SI performance, including focus, pupil shear, pupil roll, boresight, wavefront error, and image quality, is evaluated at the operating temperature using OSIM. The comprehensive optical test plans include drafting OSIM source configurations for thousands of exposures ahead of the start of a cryogenic test campaign. We describe how we predicted the performance of OSIM light sources illuminating the ISIM detectors to aide in drafting these optical tests before a test campaign began. We also discuss the actual challenges and successes of those exposure predictions encountered during a test campaign to fulfill the demands of the ISIM optical performance verification.

  8. Recent Developments in the Alignment and Test Plans for the James Webb Space Telescope Integrated Science Instrument Module

    Science.gov (United States)

    Ohl, Raymond

    2008-01-01

    The James Webb Space Telescope (JWST) is a 6.6m diameter, segmented, deployable telescope for cryogenic IR space astronomy (approximately 40K). The JWST Observatory architecture includes the Optical Telescope Element (OTE) and the Integrated Science Instrument Module (ISIM) element that contains four science instruments (SI) including a Guider. The SIs and Guider are mounted to a composite metering structure with outer dimensions of 2.1 x 2.2 x 1.9m. The SI and Guider units are integrated to the ISIM structure and optically tested at NASA/Goddard Space Flight Center as an instrument suite using an OTE SIMulator (OSIM). OSIM is a high-fidelity, cryogenic JWST telescope simulator that features a approximately 1.5m diameter powered mirror. The SIs are aligned to the structure's coordinate system under ambient, clean room conditions using laser tracker and theodolite metrology. Temperature-induced mechanical SI alignment and structural changes are measured using a photogrammetric measurement system at ambient and cryogenic temperatures. OSIM is aligned to the ISIM mechanical coordinate system at the cryogenic operating temperature via internal mechanisms and feedback from alignment sensors in six degrees of freedom. SI performance, including focus, pupil shear and wavefront error, is evaluated at the operating temperature using OSIM. We present an updated plan for the assembly and ambient and cryogenic optical alignment, test and verification of the ISIM element.

  9. Scientific Integrity and Professional Ethics at AGU - Strategies and Actions to Impact Sexual Harassment in Science and other Work Climate Issues

    Science.gov (United States)

    McPhaden, Michael; Davidson, Eric; McEntee, Christine; Williams, Billy

    2017-04-01

    The American Geophysical Union (AGU), a scientific society of 62,000 members worldwide, has established a set of scientific integrity and professional ethics guidelines for the actions of its members, for the governance of the union in its internal activities, and for the operations and participation in its publications and scientific meetings. More recently AGU has undertaken strategies and actions to help address the issue of harassment in the sciences and other work climate issues. This presentation will provide an overview of the role of scientific societies in helping to address these important issues, as well as specific strategies and actions underway at AGU and other societies. Progress to date and remaining challenges of this effort will be discussed, including AGU's work to provide additional program strength in this area.

  10. Next Generation Very Large Array Memo No. 8 Science Working Group 3: Galaxy Assembly through Cosmic Time

    CERN Document Server

    Casey, Caitlin M; Lacy, Mark; Hales, Christopher A; Barger, Amy; Narayanan, Desika; Carilli, Chris; Alatalo, Katherine; da Cunha, Elisabete; Emonts, Bjorn; Ivison, Rob; Kimball, Amy; Kohno, Kotaro; Murphy, Eric; Riechers, Dominik; Sargent, Mark; Walter, Fabian

    2015-01-01

    The Next-Generation Very Large Array (ngVLA) will be critical for understanding how galaxies are built and evolve at the earliest epochs. The sensitivity and frequency coverage will allow for the detection of cold gas and dust in `normal' distant galaxies, including the low-J transitions of molecular gas tracers such as CO, HNC, and HCO+; synchrotron and free-free continuum emission; and even the exciting possibility of thermal dust emission at the highest (z~7) redshifts. In particular, by enabling the total molecular gas reservoirs to be traced to unprecedented sensitivities across a huge range of epochs simultaneously -- something no other radio or submillimeter facility will be capable of -- the detection of the crucial low-J transitions of CO in a diverse body of galaxies will be the cornerstone of ngVLA's contribution to high-redshift galaxy evolution science. The ultra-wide bandwidths will allow a complete sampling of radio SEDs, as well as the detection of emission lines necessary for spectroscopic co...

  11. What’s in a slogan? Translational science and the rhetorical work of cancer researchers in a UK university

    Directory of Open Access Journals (Sweden)

    Alex Rushforth

    2016-07-01

    Full Text Available Translational science is currently proving a highly influential term in framing how biomedical research is promoted and evaluated in a great number of countries. Although there has been a steady trickle of scholarly literature on the topic, the performative uses effects of the term in practices of academic researchers has been under-researched. Drawing on interviews with members of a cancer laboratory and research institute in a UK research university, the paper analyzes various uses and contexts in which the slogan is deployed. The findings demonstrate the multi-dimensional uses of the term across different levels of the organisation, acting at one level as a managerial function for formulating an ‘impact’ narrative, whilst also fulfilling researcher requirements to satisfy demands made of them in pursuing funding and positions. Analyzing how this specific slogan functions in this site evokes a wider set of considerations about the kinds of rhetoric invoked and increasingly expected of cancer scientists in academic settings.

  12. Teacher Education that Works: Preparing Secondary-Level Math and Science Teachers for Success with English Language Learners Through Content-Based Instruction

    Directory of Open Access Journals (Sweden)

    Margo Elisabeth DelliCarpini

    2014-11-01

    Full Text Available Little research exists on effective ways to prepare secondary mathematics and science teachers to work with English language learners (ELLs in mainstream mathematics and science (subsequently referred to as STEM classrooms. Given the achievement gap that exists between ELLs and their native-speaking counterparts in STEM subjects, as well as the growing numbers of ELLs in US schools, this becomes a critical issue, as academic success for these students depends on the effectiveness of instruction they receive not only in English as a second language classes (ESL, but in mainstream classrooms as well. This article reports on the effects of a program restructuring that implemented coursework specifically designed to prepare pre-service and in-service mathematics, science, and ESL teachers to work with ELLs in their content and ESL classrooms through collaboration between mainstream STEM and ESL teachers, as well as effective content and language integration. We present findings on teachers’ attitudes and current practices related to the inclusion of ELLs in the secondary-level content classroom and their current level of knowledge and skills in collaborative practice. We further describe the rationale behind the development of the course, provide a description of the course and its requirements as they changed throughout its implementation during two semesters, and present findings from the participants enrolled. Additionally, we discuss the lessons learned; researchers’ innovative approaches to implementation of content-based instruction (CBI and teacher collaboration, which we term two-way CBI (DelliCarpini & Alonso, 2013; and implications for teacher education programs.

  13. Art,Science and Technology——Computed Aided Design in Practice & How computer technology affect designer’s work

    Institute of Scientific and Technical Information of China (English)

    赵耀

    2010-01-01

    Introduction:Computing technology has developed significantly in the past few decades.It affects almost everyone in the modern society,creating new ways of communication which affects both our work and leisure activities.Particularly,in today’s world of design and technology,computer aided design is fast becoming a technologically and economically feasible reality.Most designers have accepted the fact that computer aided design plays an important role in the success of their practices,not due to it’s value as an efficient drafting and modeling tool,but also because of clients’perception that it makes sound financial sense to utilize CAD.On the other hand,many people argue that computers are not fully autonomous,they are merely unconscious digital slaves or tools of production.In addition,the abusive use of software technology would turn creative art design into a purely industrial activity.

  14. Power of Streams and Power of Management: How Community and Fluvial Science Work Together for Massachusetts Rivers

    Science.gov (United States)

    Hatch, C. E.; Mabee, S. B.; Slovin, N. B.; Vogel, E.; Gartner, J. D.; Gillett, N.; Warner, B. P.

    2015-12-01

    In the Northeastern U.S., the most costly damages from intense storm events were impacts to road-stream crossings. In steep post-glacial terrain, erosion by floodwater and entrained sediment is the largest destructive force during intense storms, and the most likely driver of major morphological changes to riverbanks and channels. Steam power analysis is a tool that can successfully quantify floodwater energy that caused damage afterward, however, prediction of which reaches or watersheds may experience future impacts remains uncertain. We must better determine how states with thousands of river miles may better prioritize flood mitigation studies, crossing replacements, or other infrastructure upgrades for future flood resilience within resource constraints. This challenged us to develop a statewide-scale scientific method for screening waterways and translating the results into effective policies for river corridor management. Here we present a method based on stream power analysis using widely-available 10-m DEMs and stream flow data to identify locations with extreme high or low stream power values (i.e., >300 W⁄m2 or power are prone to landslides, bank failures, and other pulse sediment inputs in flood events. These are also the focal points of wood input to rivers, which combined with increased sediment load, makes culverts in these reaches especially prone to failure. Integration of this information into state databases allows communities to prioritize and make land-use decisions that are informed by the fluvial geomorphic workings of the larger watershed, but that have powerful local implications. Outreach and educational programs focused on stream power and fluvial systems for river practitioners and politicians at all levels align communities' attitudes about their rivers and result in ecologically sound, more flood resilient policies and practices.

  15. The Power of Cooperation in International Paleoclimate Science: Examples from the PAGES 2k Network and the Ocean2k Working Group

    Science.gov (United States)

    Addison, J. A.

    2015-12-01

    The Past Global Changes (PAGES) project of IGBP and Future Earth supports research to understand the Earth's past environment to improve future climate predictions and inform strategies for sustainability. Within this framework, the PAGES 2k Network was established to provide a focus on the past 2000 years, a period that encompasses Medieval Climate Anomaly warming, Little Ice Age cooling, and recent anthropogenically-forced climate change. The results of these studies are used for testing earth system models, and for understanding decadal- to centennial-scale variability, which is needed for long-term planning. International coordination and cooperation among the nine regional Working Groups that make up the 2k Network has been critical to the success of PAGES 2k. The collaborative approach is moving toward scientific achievements across the regional groups, including: (i) the development of a community-driven open-access proxy climate database; (ii) integration of multi-resolution proxy records; (iii) development of multivariate climate reconstructions; and (iv) a leap forward in the spatial resolution of paleoclimate reconstructions. The last addition to the 2k Network, the Ocean2k Working Group has further innovated the collaborative approach by: (1) creating an open, receptive environment to discuss ideas exclusively in the virtual space; (2) employing an array of real-time collaborative software tools to enable communication, group document writing, and data analysis; (3) consolidating executive leadership teams to oversee project development and manage grassroots-style volunteer pools; and (4) embracing the value-added role that international and interdisciplinary science can play in advancing paleoclimate hypotheses critical to understanding future change. Ongoing efforts for the PAGES 2k Network are focused on developing new standards for data quality control and archiving. These tasks will provide the foundation for new and continuing "trans-regional" 2k

  16. Surveying the familiarity and usage of up-to-date database among nurses working in the hospitals affiliated with Ahvaz Jundishapur University of Medical Sciences.

    Science.gov (United States)

    Ghassemi, A H; AghazadeAsl, E; Bigdeli, Z; SakiMalehi, A

    2015-01-01

    Background and Objectives: The evidence-based databases provide the details of the latest scientific findings of research on an individual subject. Factual databases have gained a significant attention regarding the importance and application of evidence-based medical information. Therefore, the purpose of present study was to investigate the level of familiarity by using an Up-To-Date database among the nurses working at the hospitals affiliated with Ahvaz Jundishapur University of Medial Sciences, and by this, making ground for cost-efficiency and cost-effectiveness analyses. Materials and Methods: This was a descriptive-analytical research, conducted on a sample of 293 nurses selected from a population of 1246 nurses, working at the hospitals affiliated with Ahvaz Jundishapur University of Medical Sciences. For the data collection, a researcher built questionnaire was used, and its validity and reliability were confirmed, its Cronbach's alpha coefficient being calculated as 0.71. For the data analysis, descriptive statistics and Kruskal-Wallis test were run. Results: According to the findings, the majority of the nurses were female, having a Bachelor's degree. The nurses had a mid-familiarity with the Up-To-Date database, and most of them used this database in a very limited manner. When using the Up-To-Date database, their primary goal was to update their information and to answer to the clinical questions of the patients. Conclusions: According to the findings, it could be concluded that the access to the recent and up-to-date information in the domain of nursing required the training of the nurses with the necessary skills in information use, to be able to obtain updated information from evidence-based databases and other information resources.

  17. JWST and Exoplanets

    Science.gov (United States)

    Mather, John C.

    2009-01-01

    The James Webb Space Telescope is on track for a launch in 2013. The author reviews the status and progress on the key hardware. The first primary mirror segments are already at MSFC for cryogenic tests, the mid IR instrument (MIRI) has already had successful tests of the engineering model, and the detectors are showing excellent performance. The author also describes the scientific objectives of the mission, with emphasis on the predicted capabilities for observing planets by the transit technique and through direct imaging. Recent direct observations of planets by HST and by adaptive optics from the ground have shown that, under favorable circumstances, much can be learned.

  18. Philosophy of the social sciences

    OpenAIRE

    J. A. Kimelyev; N. L. Polyakova

    2014-01-01

    Philosophy of social science is a branch of philosophy where relations between philosophy and social sciences are traced and investigated. The main functions of philosophy of social science are: to work out social ontology, methodology and metatheory of social science.

  19. Work preferences, life values, and personal views of top math/science graduate students and the profoundly gifted: Developmental changes and gender differences during emerging adulthood and parenthood.

    Science.gov (United States)

    Ferriman, Kimberley; Lubinski, David; Benbow, Camilla P

    2009-09-01

    Work preferences, life values, and personal views of top math/science graduate students (275 men, 255 women) were assessed at ages 25 and 35 years. In Study 1, analyses of work preferences revealed developmental changes and gender differences in priorities: Some gender differences increased over time and increased more among parents than among childless participants, seemingly because the mothers' priorities changed. In Study 2, gender differences in the graduate students' life values and personal views at age 35 were compared with those of profoundly gifted participants (top 1 in 10,000, identified by age 13 and tracked for 20 years: 265 men, 84 women). Again, gender differences were larger among parents. Across both cohorts, men appeared to assume a more agentic, career-focused perspective than women did, placing more importance on creating high-impact products, receiving compensation, taking risks, and gaining recognition as the best in their fields. Women appeared to favor a more communal, holistic perspective, emphasizing community, family, friendships, and less time devoted to career. Gender differences in life priorities, which intensify during parenthood, anticipated differential male-female representation in high-level and time-intensive careers, even among talented men and women with similar profiles of abilities, vocational interests, and educational experiences.

  20. Detecting Proxima b’s Atmosphere with JWST Targeting CO2 at 15 μm Using a High-pass Spectral Filtering Technique

    Science.gov (United States)

    Snellen, I. A. G.; Désert, J.-M.; Waters, L. B. F. M.; Robinson, T.; Meadows, V.; van Dishoeck, E. F.; Brandl, B. R.; Henning, T.; Bouwman, J.; Lahuis, F.; Min, M.; Lovis, C.; Dominik, C.; Van Eylen, V.; Sing, D.; Anglada-Escudé, G.; Birkby, J. L.; Brogi, M.

    2017-08-01

    Exoplanet Proxima b will be an important laboratory for the search for extraterrestrial life for the decades ahead. Here, we discuss the prospects of detecting carbon dioxide at 15 μm using a spectral filtering technique with the Medium Resolution Spectrograph (MRS) mode of the Mid-Infrared Instrument (MIRI) on the James Webb Space Telescope (JWST). At superior conjunction, the planet is expected to show a contrast of up to 100 ppm with respect to the star. At a spectral resolving power of R = 1790-2640, about 100 spectral CO2 features are visible within the 13.2-15.8 μm (3B) band, which can be combined to boost the planet atmospheric signal by a factor of 3-4, depending on the atmospheric temperature structure and CO2 abundance. If atmospheric conditions are favorable (assuming an Earth-like atmosphere), with this new application to the cross-correlation technique, carbon dioxide can be detected within a few days of JWST observations. However, this can only be achieved if both the instrumental spectral response and the stellar spectrum can be determined to a relative precision of ≤1 × 10-4 between adjacent spectral channels. Absolute flux calibration is not required, and the method is insensitive to the strong broadband variability of the host star. Precise calibration of the spectral features of the host star may only be attainable by obtaining deep observations of the system during inferior conjunction that serve as a reference. The high-pass filter spectroscopic technique with the MIRI MRS can be tested on warm Jupiters, Neptunes, and super-Earths with significantly higher planet/star contrast ratios than the Proxima system.