Pacemaker lead erosion simulating "Loch Ness Monster": conservative management.

Science.gov (United States)

Garg, Naveen; Moorthy, Nagaraja

2012-12-01

The majority of pacemaker pocket or lead erosions are due to either mechanical erosion by the bulky pulse generator or secondary to pacemaker pocket infection. We describe an unusual case of delayed pacemaker lead erosion causing extrusion of a portion of the pacing lead, with separate entry and exit points, with the gap filled with new skin formation, simulating the "Loch Ness Monster", which was successfully managed conservatively by surgical reinsertion.

Sources and fluxes of inorganic carbon in a deep, oligotrophic lake (Loch Ness, Scotland)

Science.gov (United States)

Jones, R. I.; Grey, J.; Quarmby, Christopher; Sleep, Darren

2001-12-01

The main river inflows to Loch Ness and several depths in the water column within the loch were sampled over an annual cycle. The carbon isotope composition of total dissolved inorganic carbon (DIC) from the samples was determined as well as that of phytoplankton from the loch. Values of δ13C for DIC in the rivers indicated that this DIC was derived from soil respiration in the catchment and achieved only partial equilibrium with the atmosphere during river transport. Riverine loading accounted for most of the DIC in Loch Ness, and the great depth of the loch relative to its surface area allows only limited exchange with the atmosphere. Despite the low productivity in Loch Ness, DIC concentrations in the low alkalinity water are appreciably influenced by plankton metabolism, and seasonal fluctuations in δ13C of DIC and phytoplankton revealed the particular impact of photosynthetic carbon fixation on DIC. However, the photosynthetic depletion of DIC during summer does not offset the riverine loading sufficiently to prevent the loch waters being supersaturated with CO2 throughout the year. Annual efflux of CO2 from Loch Ness is estimated to be 253 × 106 mol yr-1, of which around one quarter may be due to net heterotrophic mineralization within the loch of organic carbon of terrestrial origin. The remainder is attributable to inorganic carbon input to the lake via river inflow and derived from prior mineralization of soil organic matter within the drainage area. This annual efflux of CO2 can represent around 6% of net ecosystem production in the catchment.

NESS038C6, a novel selective CB1 antagonist agent with anti-obesity activity and improved molecular profile.

Science.gov (United States)

Mastinu, Andrea; Pira, Marilena; Pani, Luca; Pinna, Gérard Aimè; Lazzari, Paolo

2012-10-01

The present work aims to study the effects induced by a chronic treatment with a novel CB1 antagonist (NESS038C6) in C57BL/6N diet-induced obesity (DIO) mice. Mice treated with NESS038C6 and fed with a fat diet (NESS038C6 FD) were compared with the following three reference experimental groups: DIO mice fed with the same fat diet used for NESS038C6 and treated with vehicle or the reference CB1 antagonist/inverse agonist rimonabant, "VH FD" and "SR141716 FD", respectively; DIO mice treated with vehicle and switched to a normal diet (VH ND). NESS038C6 chronic treatment (30 mg/kg/day for 31 days) determined a significant reduction in DIO mice weight relative to that of VH FD. The entity of the effect was comparable to that detected in both SR141716 FD and VH ND groups. Moreover, if compared to VH FD, NESS038C6 FD evidenced: (i) improvement of cardiovascular risk factors; (ii) significant decrease in adipose tissue leptin expression; (iii) increase in mRNA expression of hypothalamic orexigenic peptides and a decrease of anorexigenic peptides; (iv) expression increase of metabolic enzymes and peroxisome proliferator-activated receptor-α in the liver; (v) normalization of monoaminergic transporters and neurotrophic expression in mesolimbic area. However, in contrast to the case of rimonabant, the novel CB1 antagonist improved the disrupted expression profile of genes linked to the hunger-satiety circuit, without altering monoaminergic transmission. In conclusion, the novel CB1 antagonist compound NESS038C6 may represent a useful candidate agent for the treatment of obesity and its metabolic complications, without or with reduced side effects relative to those instead observed with rimonabant. Copyright © 2012 Elsevier B.V. All rights reserved.

Coding "We-ness" in couple's relationship stories: A method for assessing mutuality in couple therapy.

Science.gov (United States)

Gildersleeve, Sara; Singer, Jefferson A; Skerrett, Karen; Wein, Shelter

2017-05-01

"We-ness," a couple's mutual investment in their relationship and in each other, has been found to be a potent dimension of couple resilience. This study examined the development of a method to capture We-ness in psychotherapy through the coding of relationship narratives co-constructed by couples ("We-Stories"). It used a coding system to identify the core thematic elements that make up these narratives. Couples that self-identified as "happy" (N = 53) generated We-Stories and completed measures of relationship satisfaction and mutuality. These stories were then coded using the We-Stories coding manual. Findings indicated that security, an element that involves aspects of safety, support, and commitment, was most common, appearing in 58.5% of all narratives. This element was followed by the elements of pleasure (49.1%) and shared meaning/vision (37.7%). The number of "We-ness" elements was also correlated with and predictive of discrepancy scores on measures of relationship mutuality, indicating the validity of the We-Stories coding manual. Limitations and future directions are discussed.

Media Language, Clear or Obscure

DEFF Research Database (Denmark)

Jakobsen, Bjarne le Fevre; Ejstrup, Michael

2015-01-01

Abstract— Be clear, not obscure. One of the four maxims for optimal communication is that it is essential to develop proficiency in being concise and clear. The question is whether this is really a good idea in all contexts. There is some evidence to the contrary. Undoubtedly, we have many contexts...

CT enteroclysis in the diagnosis of obscure gastrointestinal bleeding: initial results

International Nuclear Information System (INIS)

Jain, T.P.; Gulati, M.S.; Makharia, G.K.; Bandhu, S.; Garg, P.K.

2007-01-01

Aim: To evaluate the usefulness of computed tomography (CT) enteroclysis in patients with obscure gastrointestinal (GI) bleeding. Materials and methods: In a prospective study, CT enteroclysis was performed in 21 patients (median age 50 years; range 13-71 years) with obscure GI bleeding in which the source of the bleeding could not be detected despite the patient having undergone both upper GI endoscopic and colonoscopic examinations. The entire abdomen and pelvis was examined in the arterial and venous phases using multisection CT after distending the small intestine with 2 l of 0.5% methylcellulose as a neutral enteral contrast medium and the administration of 150 ml intravenous contrast medium. Results: Adequate distension of the small intestine was achieved in 20 of the 21 (95.2%) patients. Potential causes of GI bleeding were identified in 10 of the 21 (47.6%) patients using CT enteroclysis. The cause of the bleeding could be detected nine of 14 (64.3%) patients with overt, obscure GI bleeding. However, for patients with occult, obscure GI bleeding, the cause of the bleeding was identified in only one of the seven (14.3%) patients. The lesions identified by CT enteroclysis included small bowel tumours (n = 2), small bowel intussusceptions (n = 2), intestinal tuberculosis (n = 2), and vascular lesions (n = 3). All vascular lesions were seen equally well in both the arterial and venous phases. Conclusions: The success rate in detection of the cause of bleeding using CT enteroclysis was 47.6% in patients with obscure GI bleeding. The diagnostic yield was higher in patients with overt, obscure GI bleeding than in those with occult obscure GI bleeding

CT enteroclysis in the diagnosis of obscure gastrointestinal bleeding: initial results

Energy Technology Data Exchange (ETDEWEB)

Jain, T.P. [Department ofRadiodiagnosis, All India Institute of Medical Sciences, New Delhi (India); Gulati, M.S. [Department of Imaging, Queen Elizabeth Hospital NHS Trust, London (United Kingdom); Makharia, G.K. [Department of Gastroenterology and Human Nutrition, All India Institute of Medical Sciences, New Delhi (India)]. E-mail: govindmakharia@aiims.ac.in; Bandhu, S. [Department ofRadiodiagnosis, All India Institute of Medical Sciences, New Delhi (India); Garg, P.K. [Department of Gastroenterology and Human Nutrition, All India Institute of Medical Sciences, New Delhi (India)

2007-07-15

Aim: To evaluate the usefulness of computed tomography (CT) enteroclysis in patients with obscure gastrointestinal (GI) bleeding. Materials and methods: In a prospective study, CT enteroclysis was performed in 21 patients (median age 50 years; range 13-71 years) with obscure GI bleeding in which the source of the bleeding could not be detected despite the patient having undergone both upper GI endoscopic and colonoscopic examinations. The entire abdomen and pelvis was examined in the arterial and venous phases using multisection CT after distending the small intestine with 2 l of 0.5% methylcellulose as a neutral enteral contrast medium and the administration of 150 ml intravenous contrast medium. Results: Adequate distension of the small intestine was achieved in 20 of the 21 (95.2%) patients. Potential causes of GI bleeding were identified in 10 of the 21 (47.6%) patients using CT enteroclysis. The cause of the bleeding could be detected nine of 14 (64.3%) patients with overt, obscure GI bleeding. However, for patients with occult, obscure GI bleeding, the cause of the bleeding was identified in only one of the seven (14.3%) patients. The lesions identified by CT enteroclysis included small bowel tumours (n = 2), small bowel intussusceptions (n = 2), intestinal tuberculosis (n = 2), and vascular lesions (n = 3). All vascular lesions were seen equally well in both the arterial and venous phases. Conclusions: The success rate in detection of the cause of bleeding using CT enteroclysis was 47.6% in patients with obscure GI bleeding. The diagnostic yield was higher in patients with overt, obscure GI bleeding than in those with occult obscure GI bleeding.

Therapeutically induced changes in couple identity: the role of we-ness and interpersonal processing in relationship satisfaction.

Science.gov (United States)

Reid, David W; Dalton, E Jane; Laderoute, Kristine; Doell, Faye K; Nguyen, Thao

2006-08-01

Changes in partners' sense of self-in-relationship, which a systemic-constructivist couple therapy (SCCT) induced, led to robust improvement in satisfaction in 2 studies and a follow-up study. In each study, 13 referred couples completed measures of satisfaction, mutuality, similarities, and other-in-self construal pre-post 12 hours of SCCT. The authors reliably coded transcripts of 1st and final sessions for each partner's we-ness, the identity that each partner establishes in relationship to the other. Having met the criteria for the rigorous study of change in single group process-outcome design, changes in we-ness accompanied large posttherapy dyadic increments on all variables in each study. Therapeutic gains appeared at follow-up and correlated with increased we-ness obtained at end of therapy 2 years earlier. The authors raise theoretical implications for all types of couple therapies and explain clinical techniques.

Readability of self-illuminated signs obscured by black fuel-fire smoke.

Science.gov (United States)

1980-07-01

This study, using black fuel-fire generated smoke, is a partial replication of an earlier study using an inert white smoke as the obscuring agent in the study of the readability of smoke-obscured, self-illuminated emergency exit signs. : The results ...

Mixed Methods Research: The "Thing-ness" Problem.

Science.gov (United States)

Hesse-Biber, Sharlene

2015-06-01

Contemporary mixed methods research (MMR) veers away from a "loosely bounded" to a "bounded" concept that has important negative implications for how qualitatively driven mixed methods approaches are positioned in the field of mixed methods and overall innovation in the praxis of MMR. I deploy the concept of reification defined as taking an object/abstraction and treating it as if it were real such that it takes on the quality of "thing-ness," having a concrete independent existence. I argue that the contemporary reification of mixed methods as a "thing" is fueled by three interrelated factors: (a) the growing formalization of mixed methods as design, (b) the unexamined belief in the "synergy" of mixed methods and, (c) the deployment of a "practical pragmatism" as the "philosophical partner" for mixed methods inquiry. © The Author(s) 2015.

Focal intestinal lymphangiectasia: An unusual cause of acute overt obscure gastrointestinal bleeding

Directory of Open Access Journals (Sweden)

Ashish Kumar Jha

2014-01-01

Full Text Available Detection of bleeding lesion in a patient of acute overt obscure gastrointestinal bleeding is a real challenge. Recently, authors have showed superiority of urgent capsule endoscopy (CE over angiography in patients with acute overt obscure gastrointestinal bleeding. Focal type of intestinal lymphangiectasia is a rare cause of acute gastrointestinal bleeding. Here, we describe a case of focal lymphangiectasia who presented to us with acute overt obscure gastrointestinal bleeding and diagnosed by urgent CE.

"Cet obscur objet du Désir"

Directory of Open Access Journals (Sweden)

Reto Melchior

1996-09-01

Full Text Available Luis Bunuel’s last film is based on Pierre Louÿs’ La Femme et le Pantin. This now forgotten bestseller, published in 1898, is drawn from Goya s painting El Pelele, in which four women are playing with a male puppet. In Pierre Louÿs’ novel this scene is inverted so that one woman with two faces plays with four men. In Cet Obscur Objet du Désir this “femme fatale” is interpreted by two actresses. The concentric structure of the film puts focus on a scene of being excluded from knowing. The technique of continually interrupting the flash-back sequences frustrates the audience because of its exclusion from the “real” course of events and gives rise to doubts whether the male protagonist tells the truth about his love-affair or whether he satisfies the curiosity of the audience by telling them Pierre Louÿs’ novel as his own story. This ambiguous art of narration mirrors Bunuel’s claim that the main topic of Cet Obscur Objet du Désir is frustration.

The most luminous heavily obscured quasars have a high merger fraction: morphological study of wise -selected hot dust-obscured galaxies

Energy Technology Data Exchange (ETDEWEB)

Fan, Lulu; Gao, Ying; Zhang, Dandan; Jiang, Xiaoming; Wu, Qiaoqian; Yang, Jun; Li, Zhao [Shandong Provincial Key Lab of Optical Astronomy and Solar-Terrestrial Environment, Institute of Space Science, Shandong University, Weihai 264209 (China); Han, Yunkun [Yunnan Observatories, Chinese Academy of Sciences, Kunming 650011 (China); Fang, Guanwen, E-mail: llfan@sdu.edu.cn, E-mail: hanyk@ynao.ac.cn [Institute for Astronomy and History of Science and Technology, Dali University, Dali 671003 (China)

2016-05-10

Previous studies have shown that Wide-field Infrared Survey Explorer -selected hyperluminous, hot dust-obscured galaxies (Hot DOGs) are powered by highly dust-obscured, possibly Compton-thick active galactic nuclei (AGNs). High obscuration provides us a good chance to study the host morphology of the most luminous AGNs directly. We analyze the host morphology of 18 Hot DOGs at z ∼ 3 using Hubble Space Telescope /WFC3 imaging. We find that Hot DOGs have a high merger fraction (62 ± 14%). By fitting the surface brightness profiles, we find that the distribution of Sérsic indices in our Hot DOG sample peaks around 2, which suggests that most Hot DOGs have transforming morphologies. We also derive the AGN bolometric luminosity (∼10{sup 14} L {sub ⊙}) of our Hot DOG sample by using IR spectral energy distributions decomposition. The derived merger fraction and AGN bolometric luminosity relation is well consistent with the variability-based model prediction. Both the high merger fraction in an IR-luminous AGN sample and relatively low merger fraction in a UV/optical-selected, unobscured AGN sample can be expected in the merger-driven evolutionary model. Finally, we conclude that Hot DOGs are merger-driven and may represent a transit phase during the evolution of massive galaxies, transforming from the dusty starburst-dominated phase to the unobscured QSO phase.

Characterizing the evolution of WISE-selected obscured and unobscured quasars using HOD models.

Science.gov (United States)

Myers, Adam D.; DiPompeo, Michael A.; Mitra, Kaustav; Hickox, Ryan C.; Chatterjee, Suchetana; Whalen, Kelly

2018-06-01

Large-area imaging surveys in the infrared are now beginning to unlock the links between the activity of supermassive black holes and the cosmic evolution of dark matter halos during the significant times when black hole growth is enshrouded in dust. With data from the Wide-Field Infrared Survey Explorer (WISE) and complementary optical photometry, we construct samples of nearly half-a-million obscured and unobscured quasars around redshift 1. We study the dark matter halos of these populations using both angular autocorrelation functions and CMB lensing cross-correlations, carefully characterizing the redshift distribution of the obscured quasar sample using cross-correlations. Independent of our measurement technique, we find that obscured quasars occupy dark matter halos a few times more massive than their unobscured counterparts, despite being matched in luminosity at 12 and 22 microns. Modeling the two-point correlation function using a four-parameter Halo Occupation Distribution (HOD) formalism, we determine that purely optically selected quasars reside in dark matter halos that are about half the mass of WISE-selected obscured quasars, and that satellite fractions are somewhat larger for obscured quasars. We investigate scenarios such as merger-driven fueling and Eddington-dependent obscuration to explore what combinations of physical effects can reproduce our observed halo mass measurements. This work was, in part, supported by NASA ADAP award NNX16AN48G.

What is the best diagnostic approach for obscure gastrointestinal bleeding?

International Nuclear Information System (INIS)

Juliao Banos, Fabian

2010-01-01

For the gastroenterologist, the study of patients with obscure gastrointestinal bleeding is a diagnostic challenge. Using recent definitions as starting point for locating and defining the type of obscure bleeding allows better study and classification of these individuals. Since 25% of the causes of obscure gastrointestinal bleeding are within the reach of upper endoscopy and total colonoscopy, we are compelled to make good clinical evaluations and establish quality parameters for performance of these procedures. With the emergence of new techniques such as capsule endoscopy and balloon enteroscopy, the study of the small intestine with higher performance than previously available through imaging studies is now possible in our environment. Rational sequential use of these diagnostic tools, exhaustive reviews of capsule endoscopy images plus and adequate training in performing balloon enteroscopy including the two-way approach when necessary, will help us to establish and treat the cause in most patients with this condition.

Le monstre du Loch Ness : entre science et folklore

OpenAIRE

Fairise, Nicolas

2002-01-01

Depuis sa première véritable observation alléguée en 1933 jusqu'à nos jours, le monstre du loch Ness n'a cessé de défrayer la chronique. Cette fameuse créature est ainsi devenue l'un des rares mythes zoologiques modernes. Dans un premier temps, la présente étude s'intéresse au lac lui-même, notamment sur les plans géophysique et biologique, afin de donner des éléments de description concernant le cadre souvent méconnu d'une des énigmes les plus médiatisées du siècle dernier. Tantôt anecdotiqu...

The Halo Occupation Distribution of obscured quasars: revisiting the unification model

Science.gov (United States)

Mitra, Kaustav; Chatterjee, Suchetana; DiPompeo, Michael A.; Myers, Adam D.; Zheng, Zheng

2018-06-01

We model the projected angular two-point correlation function (2PCF) of obscured and unobscured quasars selected using the Wide-field Infrared Survey Explorer (WISE), at a median redshift of z ˜ 1 using a five parameter Halo Occupation Distribution (HOD) parametrization, derived from a cosmological hydrodynamic simulation by Chatterjee et al. The HOD parametrization was previously used to model the 2PCF of optically selected quasars and X-ray bright active galactic nuclei (AGNs) at z ˜ 1. The current work shows that a single HOD parametrization can be used to model the population of different kinds of AGN in dark matter haloes suggesting the universality of the relationship between AGN and their host dark matter haloes. Our results show that the median halo mass of central quasar hosts increases from optically selected (4.1^{+0.3}_{-0.4} × 10^{12} h^{-1} M_{⊙}) and infra-red (IR) bright unobscured populations (6.3^{+6.2}_{-2.3} × 10^{12} h^{-1} M_{⊙}) to obscured quasars (10.0^{+2.6}_{-3.7} × 10^{12} h^{-1} M_{⊙}), signifying an increase in the degree of clustering. The projected satellite fractions also increase from optically bright to obscured quasars and tend to disfavour a simple `orientation only' theory of active galactic nuclei unification. Our results also show that future measurements of the small-scale clustering of obscured quasars can constrain current theories of galaxy evolution where quasars evolve from an IR-bright obscured phase to the optically bright unobscured phase.

RR Tel: Determination of Dust Properties During Minimum Obscuration

Directory of Open Access Journals (Sweden)

Jurkić T.

2012-06-01

Full Text Available the ISO infrared spectra and the SAAO long-term JHKL photometry of RR Tel in the epochs during minimum obscuration are studied in order to construct a circumstellar dust model. the spectral energy distribution in the near- and the mid-IR spectral range (1–15 μm was obtained for an epoch without the pronounced dust obscuration. the DUSTY code was used to solve the radiative transfer through the dust and to determine the circumstellar dust properties of the inner dust regions around the Mira component. Dust temperature, maximum grain size, dust density distribution, mass-loss rate, terminal wind velocity and optical depth are determined. the spectral energy distribution and the long-term JHKL photometry during an epoch of minimum obscuration show almost unattenuated stellar source and strong dust emission which cannot be explained by a single dust shell model. We propose a two-component model consisting of an optically thin circmustellar dust shell and optically thick dust outside the line of sight in some kind of a flattened geometry, which is responsible for most of the observed dust thermal emission.

Notes on the tribe Mimagathidini Enderlein, with the description of a new genus (Hymenoptera: Braconidae: Orgilinae)

NARCIS (Netherlands)

Braet, Y.; Achterberg, van C.; Chen, X.

2000-01-01

Eleonoria gen. nov. (type species: E. mesembria spec. nov. from Malaysia; five additional species from Japan, China (including Taiwan), Philippines, and Indonesia (Halmahera) are included), Orgilonia pasohensis spec. nov. from Malaysia, Orgilus reclinatus spec. nov. from Congo, O. alboannulatus

Of Monsters, Myths and Marketing: The Case of the Loch Ness Monster

OpenAIRE

Moir, James

2015-01-01

This paper examines the status of the Loch Ness Monster within a diverse body of literature relating to Scotland. Within cryptozoology this creature is considered as a source of investigation, something to be taken seriously as a scientific or quasi-scientific object to be studied and known, particularly in light of its elusive nature. In terms of mythology the creature is bound up with Scottish cultural identifications through references to a rugged wilderness landscape and to...

X-Ray Spectral Properties of Seven Heavily Obscured Seyfert 2 Galaxies

Energy Technology Data Exchange (ETDEWEB)

Marchesi, S.; Ajello, M. [Department of Physics and Astronomy, Clemson University, Clemson, SC 29634 (United States); Comastri, A. [INAF—Osservatorio Astronomico di Bologna, via Ranzani 1, I-40127 Bologna (Italy); Cusumano, G.; Parola, V. La; Segreto, A., E-mail: smarche@clemson.edu [INAF—Istituto di Astrofisica Spaziale e Fisica Cosmica, Via U. La Malfa 153, I-90146 Palermo (Italy)

2017-02-10

We present the combined Chandra and Swift -BAT spectral analysis of seven Seyfert 2 galaxies selected from the Swift -BAT 100 month catalog. We selected nearby ( z ≤ 0.03) sources lacking a ROSAT counterpart that never previously been observed with Chandra in the 0.3–10 keV energy range, and targeted these objects with 10 ks Chandra ACIS-S observations. The X-ray spectral fitting over the 0.3–150 keV energy range allows us to determine that all the objects are significantly obscured, with N{sub H} ≥ 10{sup 23} cm{sup −2} at a >99% confidence level. Moreover, one to three sources are candidate Compton-thick Active Galactic Nuclei (CT-AGNs; i.e., N{sub H}≥10{sup 24} cm{sup −2}). We also test the recent spectral curvature method developed by Koss et al. to find candidate CT-AGNs, finding a good agreement between our results and their predictions. Because the selection criteria we adopted were effective in detecting highly obscured AGNs, further observations of these and other Seyfert 2 galaxies selected from the Swift -BAT 100 month catalog will allow us to create a statistically significant sample of highly obscured AGNs, therefore providing a better understanding of the physics of the obscuration processes.

The Constant Average Relationship Between Dust-obscured Star Formation and Stellar Mass from z=0 to z=2.5

Science.gov (United States)

Whitaker, Katherine E.; Pope, Alexandra; Cybulski, Ryan; Casey, Caitlin M.; Popping, Gergo; Yun, Min; 3D-HST Collaboration

2018-01-01

The total star formation budget of galaxies consists of the sum of the unobscured star formation, as observed in the rest-frame ultraviolet (UV), together with the obscured component that is absorbed and re-radiated by dust grains in the infrared. We explore how the fraction of obscured star formation depends (SFR) and stellar mass for mass-complete samples of galaxies at 0 MIPS 24μm photometry in the well-studied 5 extragalactic CANDELS fields. We find a strong dependence of the fraction of obscured star formation (f_obscured=SFR_IR/SFR_UV+IR) on stellar mass, with remarkably little evolution in this fraction with redshift out to z=2.5. 50% of star formation is obscured for galaxies with log(M/M⊙)=9.4 although unobscured star formation dominates the budget at lower masses, there exists a tail of low mass extremely obscured star-forming galaxies at z > 1. For log(M/M⊙)>10.5, >90% of star formation is obscured at all redshifts. We also show that at fixed total SFR, f_obscured is lower at higher redshift. At fixed mass, high-redshift galaxies are observed to have more compact sizes and much higher star formation rates, gas fractions and hence surface densities (implying higher dust obscuration), yet we observe no redshift evolution in f_obscured with stellar mass. This poses a challenge to theoretical models to reproduce, where the observed compact sizes at high redshift seem in tension with lower dust obscuration.

Speech masking and cancelling and voice obscuration

Science.gov (United States)

Holzrichter, John F.

2013-09-10

A non-acoustic sensor is used to measure a user's speech and then broadcasts an obscuring acoustic signal diminishing the user's vocal acoustic output intensity and/or distorting the voice sounds making them unintelligible to persons nearby. The non-acoustic sensor is positioned proximate or contacting a user's neck or head skin tissue for sensing speech production information.

The value of multidetector-row computed tomography for localization of obscure acute gastrointestinal bleeding

Energy Technology Data Exchange (ETDEWEB)

Chang, Wei-Chou [Department of Radiology, Tri-Service General Hospital, National Defense Medical Center, Taiwan (China); Tsai, Shih-Hung [Department of Emergency Medicine, Tri-Service General Hospital, National Defense Medical Center, Taiwan (China); Chang, Wei-Kuo [Division of Gasteroenterology, Department of Internal Medicine, Tri-Service General Hospital, National Defense Medical Center, Taiwan (China); Liu, Chang-Hsien [Department of Radiology, Tri-Service General Hospital, National Defense Medical Center, Taiwan (China); Tung, Ho-Jui [Department of Healthcare Administration, Asia University, Taichung, Taiwan (China); Hsieh, Chung-Bao [Department of Surgery, Tri-Service General Hospital, National Defense Medical Center, Taiwan (China); Huang, Guo-Shu; Hsu, Hsian-He [Department of Radiology, Tri-Service General Hospital, National Defense Medical Center, Taiwan (China); Yu, Chih-Yung, E-mail: chougo2002@yahoo.com.tw [Department of Radiology, Tri-Service General Hospital, National Defense Medical Center, Taiwan (China)

2011-11-15

Purpose: There are no simple guidelines on when to perform multidetector-row computed tomography (MDCT) for diagnosis of obscure acute gastrointestinal bleeding (AGIB). We used a risk scoring system to evaluate the diagnostic power of MDCT for patients with obscure AGIB. Materials and methods: Ninety-two patients with obscure AGIB who were referred for an MDCT scan after unsuccessful endoscopic treatment at presentation were studied. We recorded clinical data and calculated Blatchford score for each patient. Patients who required transfusion more than 500 mL of blood to maintain the vital signs were classified as high-risk patients. Two radiologists independently reviewed and categorized MDCT signs of obscure AGIB. Discordant findings were resolved by consensus. One-way ANOVA was used to compare clinical data between two groups; kappa statistics were used to estimate agreement on MDCT findings between radiologists. Results: Of the 92 patients, 62 (67.4%) were classified as high-risk patients. Blatchford scores of high-risk patients were significantly greater than those of low-risk patients. Sensitivity for MDCT diagnosing obscure AGIB was 81% in high-risk patients, as compared with 50% in the low-risk. When used in conjunction with selection of the cut-off value of 13 in Blatchford scoring system, the sensitivity and specificity of MDCT were 70.9% and 73.7%, respectively. Contrast extravasation was the most specific sign of AGIB (k = .87), recognition of which would have improved diagnostic accuracy. Conclusions: With the aid of Blatchford scoring system for evaluating the disease severity, MDCT can localize the bleeders of obscure AGIB more efficiently.

The value of multidetector-row computed tomography for localization of obscure acute gastrointestinal bleeding

International Nuclear Information System (INIS)

Chang, Wei-Chou; Tsai, Shih-Hung; Chang, Wei-Kuo; Liu, Chang-Hsien; Tung, Ho-Jui; Hsieh, Chung-Bao; Huang, Guo-Shu; Hsu, Hsian-He; Yu, Chih-Yung

2011-01-01

Purpose: There are no simple guidelines on when to perform multidetector-row computed tomography (MDCT) for diagnosis of obscure acute gastrointestinal bleeding (AGIB). We used a risk scoring system to evaluate the diagnostic power of MDCT for patients with obscure AGIB. Materials and methods: Ninety-two patients with obscure AGIB who were referred for an MDCT scan after unsuccessful endoscopic treatment at presentation were studied. We recorded clinical data and calculated Blatchford score for each patient. Patients who required transfusion more than 500 mL of blood to maintain the vital signs were classified as high-risk patients. Two radiologists independently reviewed and categorized MDCT signs of obscure AGIB. Discordant findings were resolved by consensus. One-way ANOVA was used to compare clinical data between two groups; kappa statistics were used to estimate agreement on MDCT findings between radiologists. Results: Of the 92 patients, 62 (67.4%) were classified as high-risk patients. Blatchford scores of high-risk patients were significantly greater than those of low-risk patients. Sensitivity for MDCT diagnosing obscure AGIB was 81% in high-risk patients, as compared with 50% in the low-risk. When used in conjunction with selection of the cut-off value of 13 in Blatchford scoring system, the sensitivity and specificity of MDCT were 70.9% and 73.7%, respectively. Contrast extravasation was the most specific sign of AGIB (k = .87), recognition of which would have improved diagnostic accuracy. Conclusions: With the aid of Blatchford scoring system for evaluating the disease severity, MDCT can localize the bleeders of obscure AGIB more efficiently.

Infrared Selection of Obscured Active Galactic Nuclei in the COSMOS Field

Science.gov (United States)

Chang, Yu-Yen; Le Floc'h, Emeric; Juneau, Stéphanie; da Cunha, Elisabete; Salvato, Mara; Civano, Francesca; Marchesi, Stefano; Ilbert, Olivier; Toba, Yoshiki; Lim, Chen-Fatt; Tang, Ji-Jia; Wang, Wei-Hao; Ferraro, Nicholas; Urry, Megan C.; Griffiths, Richard E.; Kartaltepe, Jeyhan S.

2017-12-01

We present a study of the connection among black hole accretion, star formation, and galaxy morphology at z≤slant 2.5. We focus on active galactic nuclei (AGNs) selected by their mid-IR power-law emission. By fitting optical to far-IR photometry with state-of-the-art spectral energy distribution (SED) techniques, we derive stellar masses, star formation rates, dust properties, and AGN contributions in galaxies over the whole COSMOS field. We find that obscured AGNs lie within or slightly above the star-forming sequence. We confirm our previous finding about compact host galaxies of obscured AGNs at z˜ 1, and find that galaxies with 20%-50% AGN contributions tend to have smaller sizes, by ˜25%-50%, compared to galaxies without AGNs. Furthermore, we find that a high merger fraction of up to 0.5 is appropriate for the most luminous ({log}({L}{IR}/{L}⊙ )˜ 12.5) AGN hosts and non-AGN galaxies, but not for the whole obscured AGN sample. Moreover, the merger fraction depends on the total and star-forming IR luminosity, rather than on the decomposed AGN infrared luminosity. Our results suggest that major mergers are not the main driver of AGN activity, and therefore obscured AGNs might be triggered by internal mechanisms, such as secular processes, disk instabilities, and compaction in a particular evolutionary stage. We make the SED modeling results publicly available.

Consolidation of the Victorian Marriage Tradition in Hardy’s Jude the Obscure

Directory of Open Access Journals (Sweden)

Parvin Ghasemi

2012-10-01

Full Text Available Jude the Obscure by Thomas Hardy has always been considered a novel in which the concept of the traditional Victorian marriage is severely criticized through various tones. New Historicism and Cultural Materialism are methodological approaches that provide us with a different interpretation of this novel. Therefore , on the basis of these "reading practices," as Greenblatt calls them, the researchers attempt to offer another reading of this novel. The present research concludes that Jude the Obscure at first presents an explicit, reproachful treatment of the conventional Victorian marriage but at the end it reinforces this type of marriage by repressing the characters whose views are at odds with the dominant views of the society. In other words, through marginalizing its own major characters as "the others", Jude the Obscure consolidates the dominant discourse of the Victorian society about "marriage".

Smokes and obscurants: A health and environmental effects data base assessment: A first-order, environmental screening and ranking of Army smokes and obscurants: Phase 1 report

Energy Technology Data Exchange (ETDEWEB)

Shinn, J.H.; Martins, S.A.; Cederwall, P.L.; Gratt, L.B.

1985-03-01

An initial environmental screening and ranking is provided for each Army smoke and obscurant (S and O) depending on smoke type and smoke-generating device. This was done according to the magnitude of the impact area, the characteristic environmental concentration, the relative inhalation toxicity, the relative toxicity when ingested by animals, the aquatic toxicity, the environmental mobility when freshly deposited, and the ultimate mobility and fate in the environment. The major smoke types considered were various forms of white phosphorus (WP), red phosphorus (RP), hexachloroethane-derived smokes (HC), fog oil (SGF-2), diesel fuel smokes (DF), and some infrared obscuring agents (IR).

Imprecise methods may both obscure and aggravate a relation between fat and breast cancer

DEFF Research Database (Denmark)

Heitmann, B L; Frederiksen, Peder

2007-01-01

Bias in diet reporting may be both random and non-random, and may be found with simpler as well as more advanced dietary instruments. A random bias will contribute to obscure relations between diet and disease. A systematic bias may obscure or aggravate such associations. Underreporting of non-pr...

Analysis of radiative heat transfer in the presence of obscurations

International Nuclear Information System (INIS)

Finkelstein, L.; Weissman, Y.

1981-05-01

Numerical simulation of radiative heat transfer problems in general axisymmetric geometry in the presence of an active gas is considered. Such simulation requires subdivision of the radiating surfaces into discrete elements, which are in the present case radiating rings. While the effect of a participating medium is easily taken into account by integration along the lines of vision between the surface elements, the calculation of the different obscurations poses the main difficulty. We have written a closed expression which formulates the problem exactly, and then developed a systematic and compact computational approach to the obscuration problem in complex configurations. The present procedure is particularly suited to computer calculations associated with engineering applications in the aircraft and furnace industries. (author)

Variable circumstellar obscuration of the carbon star R Fornacis

International Nuclear Information System (INIS)

Feast, M.W.; Whitelock, P.A.; Catchpole, R.M.; Roberts, G.; Overbeek, M.D.

1984-01-01

In 1983 the carbon Mira-type variable R For became unusually faint in the visible and infrared. This is interpreted as a change in circumstellar obscuration. For absorption by graphite spheres the required particle radius is 0.15 μm. (author)

AN INVESTIGATION OF INSECT OVIPOSITING REPELLENT ACTIVITY OF ANDROGRAPHIS PANICULATA NESS, ACACIA AURICULIFORMIS AND PIPER BETLE LINN LEAVES EXTRACTS TO BATROCERA CARAMBOLAE

Directory of Open Access Journals (Sweden)

Nurcahyo Iman Prakoso

2017-12-01

Full Text Available Batrocera carambolae was one of the main pests in some types of fruits. This pest attack resulted in quantitative damage in the form of fall of young fruit and qualitatively in the form of fruit to rot and contains maggots. This research was conducted to determine selected extract from Andrographis Paniculata Ness, Piper betle Linn and Acacia auriculiformis leaves which have repellent activity for Batrocera carambolae. Nine extracts from the maceration process of the three leaves were evaluated by placing the extracts and flies together in the cage. The ethanol, ethyl acetate, and n-hexane extracts from Andrographis Paniculata Ness, Piper betle Linn and Acacia auriculiformis leaves were applied to the test pieces and fed into a cage containing 10 male and female flies. From observation, N-hexane extracts from Andrographis Paniculata Ness and Piper betle Linn leaves and ethyl acetate extracts from Acacia auriculiformis leaf having good activity as repellent and potentially to be used as a insect ovipositing repellent of Batrocera carambolae.

Use of heparin in the investigation of obscure gastrointestinal bleeding

International Nuclear Information System (INIS)

Mernagh, J.R.; O'Donovan, N.; Somers, S.; Gill, G.; Sridhar, S.

2001-01-01

To determine if the administration of heparin improves the predictive value of angiography in the investigation of obscure gastrointestinal (GI) bleeding. 18 patients with a history of chronic GI bleeding were investigated with angiography. For 6 patients, the cause of GI bleeding was established with angiography; the 12 patients who had negative results were given heparin for 24 h and were reassessed with angiography. After heparin administration, the source of GI bleeding was determined with angiography for 6 of the remaining 12 patients. Thus, heparinization increased diagnostic yield from 33% (6 of 18) to 67% (12 of 18). No significant complications, such as uncontrolled GI bleeding, occurred. Heparinization improves the diagnostic yield of angiography when obscure GI bleeding is being investigated. (author)

Dessication tolerance of Cinnamomum zeylanicum Ness SeedsTolerância à dessecação de sementes de Cinnamomum zeylanicum Ness

Directory of Open Access Journals (Sweden)

Leandra Matos Barroso

2012-05-01

Full Text Available In order to evaluate the physiological quality of seeds of Cinnamomum zeylanicum Ness, submitted to different levels of drying, the fruits of dark brown and fully mature were collected and washed by hand, then the seeds were exposed to drying, on paper towel, under laboratory conditions. Treatments consisted of sampling for the determination of water content, germination and vigor tests at the beginning of the experiment and after 12, 24, 36, 48, 60, 72, 84 and 96 hours. The experimental design was completely randomized with four replications of 25 seeds each. The data were subjected to analysis of variance and polynomial regression. Cinnamon seeds are dispersed with high water content (39.43% and viability is compromised when dehydrated, the germination capacity as well as its speed decreases with dehydration, characterizing the recalcitrant behavior of seeds, with water content 34.82% less than both the percentage and the speed of germination are reduced. The seeds of C. zeylanicum tolerate desiccation to 12 hours without significant loss of vigor. Com o objetivo de avaliar a qualidade fisiológica das sementes de canela (Cinnamomum zeylanicum Ness submetidas a diferentes níveis de secagem, os frutos de coloração marrom escura e completamente maduros foram coletados e despolpados manualmente, em seguida, as sementes foram expostas para a secagem, sobre papel toalha, em condições de laboratório. Os tratamentos consistiram na amostragem para a determinação do teor de água, testes de germinação e vigor no início do experimento e após 12, 24, 36, 48, 60, 72, 84 e 96 horas. O delineamento experimental utilizado foi o inteiramente ao acaso, em quatro repetições de 25 sementes cada. Os dados obtidos foram submetidos à análise de variância e de regressão polinomial. As sementes de canela são dispersas com alto teor de água (39,43% e tem a viabilidade comprometida quando desidratadas; a capacidade de germinação bem como a sua

Bone scintigraphy in children with obscure skeletal pain

International Nuclear Information System (INIS)

Majd, Massoud

1979-01-01

In a group of 82 children with focal or generalized skeletal pain of obscure etiology, the radionuclide skeletal scintigraphy was the only, or the most informative, clue to the diagnosis of a variety of benign and malignant conditions. It is strongly recommended that any unexplained bone or joint pain in children be evaluated by this non-invasive technique [fr

Carbon Fiber Obscurant: Enhancing Warfighter Effectiveness While Meeting Environmental Regulations

National Research Council Canada - National Science Library

Phillips, Carlton T; Checkai, Ronald T; Kuperman, Roman G; Simini, Michael; Chester, Nancy A

2006-01-01

...) material obscuring in the 9-96 GMz range of the electromagnetic spectrum has become critical for the modern Warfighter in order to minimize radar detection by hostile forces, thus saving lives and equipment...

The [O III] Profiles of Infrared-selected Active Galactic Nuclei: More Powerful Outflows in the Obscured Population

Science.gov (United States)

DiPompeo, M. A.; Hickox, R. C.; Carroll, C. M.; Runnoe, J. C.; Mullaney, J. R.; Fischer, T. C.

2018-03-01

We explore the kinematics of ionized gas via the [O III] λ5007 emission lines in active galactic nuclei (AGNs) selected on the basis of their mid-infrared (IR) emission, and split into obscured and unobscured populations based on their optical‑IR colors. After correcting for differences in redshift distributions, we provide composite spectra of spectroscopically and photometrically defined obscured/Type 2 and unobscured/Type 1 AGNs from 3500 to 7000 Å. The IR-selected obscured sources contain a mixture of narrow-lined Type 2 AGNs and intermediate sources that have broad Hα emission and significantly narrower Hβ. Using both [O III] luminosities and AGN luminosities derived from optical‑IR spectral energy distribution fitting, we find evidence for enhanced large-scale obscuration in the obscured sources. In matched bins of luminosity we find that the obscured population typically has broader, more blueshifted [O III] emission than in the unobscured sample, suggestive of more powerful AGN-driven outflows. This trend is not seen in spectroscopically classified samples, and is unlikely to be entirely explained by orientation effects. In addition, outflow velocities increase from small to moderate AGN E(B ‑ V) values, before flattening out (as traced by FWHM) and even decreasing (as traced by blueshift). While difficult to fully interpret in a single physical model, due to both the averaging over populations and the spatially averaged spectra, these results agree with previous findings that simple geometric unification models are insufficient for the IR-selected AGN population, and may fit into an evolutionary model for obscured and unobscured AGNs.

Clinical approach to obscure GI bleeding - Diagnostic testing and management

Directory of Open Access Journals (Sweden)

Prashanth Prabakaran

2013-01-01

Full Text Available Obscure gastrointestinal bleeding (OGIB can present as a diagnostic dilemma and management can be challenging. The search for causes of OGIB is usually centered on visualizing the small bowel, and in the past decade, the technology to visualize the entire small bowel has significantly advanced. Moreover, small bowel endoscopic imaging has replaced, in many instances, prior radiographic evaluation for obscure GI bleeding. These new modalities, such as small bowel capsule endoscopy (CE, balloon-assisted deep enteroscopy [double balloon enteroscopy (DBE and single balloon enteroscopy (SBE], and overtube-assisted deep enteroscopy (spiral enteroscopy, are paving the way toward more accurately identifying and treating patients with OGIB. We will review the diagnostic modalities available in evaluating a patient with OGIB and also propose the management based on clinical and endoscopic findings.

Large Scale Obscuration and Related Climate Effects Workshop: Proceedings

Energy Technology Data Exchange (ETDEWEB)

Zak, B.D.; Russell, N.A.; Church, H.W.; Einfeld, W.; Yoon, D.; Behl, Y.K. [eds.

1994-05-01

A Workshop on Large Scale Obsurcation and Related Climate Effects was held 29--31 January, 1992, in Albuquerque, New Mexico. The objectives of the workshop were: to determine through the use of expert judgement the current state of understanding of regional and global obscuration and related climate effects associated with nuclear weapons detonations; to estimate how large the uncertainties are in the parameters associated with these phenomena (given specific scenarios); to evaluate the impact of these uncertainties on obscuration predictions; and to develop an approach for the prioritization of further work on newly-available data sets to reduce the uncertainties. The workshop consisted of formal presentations by the 35 participants, and subsequent topical working sessions on: the source term; aerosol optical properties; atmospheric processes; and electro-optical systems performance and climatic impacts. Summaries of the conclusions reached in the working sessions are presented in the body of the report. Copies of the transparencies shown as part of each formal presentation are contained in the appendices (microfiche).

Readability of self-illuminated signs in a smoke-obscured environment.

Science.gov (United States)

1979-11-01

This study investigates the ability of people with normal distant visual acuity to identify self-illuminated emergency signs in a smoke-obscured environment. The results indicate that signs whose background luminance meets or exceeds the requirements...

An Investigation of Insect Ovipositing Repellent Activity of Andrographis paniculata Ness, Acacia auriculiformis and Piper betle Linn Leaves Extracts to Batrocera carambolae

Directory of Open Access Journals (Sweden)

Nurcahyo Iman Prakoso

2018-03-01

Full Text Available Batrocera carambolae was one of the main pests in some types of fruits. This pest attack resulted in quantitative damage in the form of fall of young fruit and qualitatively in the form of fruit to rot and contains maggots. This research was conducted to determine selected extract from Andrographis Paniculata Ness, Piper betle Linn and Acacia auriculiformis leaves which have repellent activity for Batrocera carambolae. Nine extracts from the maceration process of the three leaves were evaluated by placing the extracts and flies together in the cage. The ethanol, ethyl acetate, and n-hexane extracts from Andrographis Paniculata Ness, Piper betle Linn and Acacia auriculiformis leaves were applied to the test pieces and fed into a cage containing 10 male and female flies. From observation, N-hexane extracts from Andrographis Paniculata Ness and Piper betle Linn leaves and ethyl acetate extracts from Acacia auriculiformis leaf  having good activity as repellent and potentially to be used as a insect ovipositing repellent of Batrocera carambolae.

Announcment: Conference on Obscured AGN Across Cosmic Time

Science.gov (United States)

2006-12-01

Current deep surveys, notably in X-rays and the mid-IR, are making it possible to carry out a census of essentially all the luminous AGN in the Universe. By pene-trating the obscuration that, in Type 2 sources, hides the nuclear regions in the UV to the near-IR spectrum, these new surveys are finding the radio quiet coun-terparts of the powerful radio galaxies.

Isolasi dan Identifikasi Andrografolida dari Herba Andrographis paniculata Ness

Directory of Open Access Journals (Sweden)

Suharmiati Suharmiati

2012-09-01

Full Text Available Andrographolide is the main constituent of Andrographis paniculata Ness (AP which was poorly soluble in water and bitter taste. As diterpenoid lactone andrographolide has many biological activities, some of them are immunostimulant, anti malaria, hepatoproccctor and anti mutagenic. The objective of this study were isolation and identification andrographolide from AP. In this study AP metanol extracted by percolation. Filtrate was collected and congealed ad viscous and was snaked by ethylacetate - water (1:1. Ethylacetate fraction was congealed until crystal formed. Recrystallization with hot metanol repeatedly until pure andrographolide isolate. Identification of andrographolide isolate by thin layer chromatography (TLC, UV spectrophotometer, Nuclear Magnetic Resonance (NMR and Fourier Transform Infra Red. Result of this study showed that from one kilogram AP herbs dried is produced 0,43% andrographolide isolate as identic as andrographolide standard (Sigma. The continued research to develop phytopharmaca product that consist andrographolide or AP herbs is needed to minimize taste bitter or to increase solubility is water so that its useful in health services.

Putting new economic geography to the test : Free-ness of trade and agglomeration in the EU regions

NARCIS (Netherlands)

Brakman, Steven; Garretsen, Harry; Schrannn, Marc; Schramm, M.

For the NUTS II EU regions we estimate the wage equation that is central to the new economic geography literature. Our first main finding is that a spatial wage structure exists for the EU regions. Next, we analyze what our estimations imply for the link between the free-ness of trade and

Obscured asymptotic giant branch stars in the Magellanic Clouds .2. Near-infrared and mid-infrared counterparts

NARCIS (Netherlands)

Zijlstra, AA; Loup, C; Waters, LBFM; Whitelock, PA; vanLoon, JT; Guglielmo, F

1996-01-01

We have carried out an infrared search for obscured asymptotic giant branch (AGB) stars in the Magellanic Clouds. Fields were observed in the vicinity of IRAS sources with colours and flux densities consistent with such a classification. The survey uncovered a number of obscured AGE stars as well as

Heavy X-ray obscuration in the most luminous galaxies discovered by WISE

Science.gov (United States)

Vito, F.; Brandt, W. N.; Stern, D.; Assef, R. J.; Chen, C.-T. J.; Brightman, M.; Comastri, A.; Eisenhardt, P.; Garmire, G. P.; Hickox, R.; Lansbury, G.; Tsai, C.-W.; Walton, D. J.; Wu, J. W.

2018-03-01

Hot dust-obscured galaxies (DOGs) are hyperluminous (L8-1000 μm > 1013 L⊙) infrared galaxies with extremely high (up to hundreds of K) dust temperatures. The sources powering both their extremely high luminosities and dust temperatures are thought to be deeply buried and rapidly accreting supermassive black holes (SMBHs). Hot DOGs could therefore represent a key evolutionary phase in which the SMBH growth peaks. X-ray observations can be used to study their obscuration levels and luminosities. In this work, we present the X-ray properties of the 20 most luminous (Lbol ≳ 1014 L⊙) known hot DOGs at z = 2-4.6. Five of them are covered by long-exposure (10-70 ks) Chandra and XMM-Newton observations, with three being X-ray detected, and we study their individual properties. One of these sources (W0116-0505) is a Compton-thick candidate, with column density NH = (1.0-1.5) × 1024 cm-2 derived from X-ray spectral fitting. The remaining 15 hot DOGs have been targeted by a Chandra snapshot (3.1 ks) survey. None of these 15 are individually detected; therefore, we applied a stacking analysis to investigate their average emission. From hardness ratio analysis, we constrained the average obscuring column density and intrinsic luminosity to be log NH (cm-2) > 23.5 and LX ≳ 1044 erg s-1, which are consistent with results for individually detected sources. We also investigated the LX-L6 μm and LX-Lbol relations, finding hints that hot DOGs are typically X-ray weaker than expected, although larger samples of luminous obscured quasi-stellar objects are needed to derive solid conclusions.

Nuclear Engine System Simulation (NESS). Volume 1: Program user's guide. Final Report

International Nuclear Information System (INIS)

Pelaccio, D.G.; Scheil, C.M.; Petrosky, L.J.

1993-03-01

A Nuclear Thermal Propulsion (NTP) engine system design analysis tool is required to support current and future Space Exploration Initiative (SEI) propulsion and vehicle design studies. Currently available NTP engine design models are those developed during the NERVA program in the 1960's and early 1970's and are highly unique to that design or are modifications of current liquid propulsion system design models. To date, NTP engine-based liquid design models lack integrated design of key NTP engine design features in the areas of reactor, shielding, multi-propellant capability, and multi-redundant pump feed fuel systems. Additionally, since the SEI effort is in the initial development stage, a robust, verified NTP analysis design tool could be of great use to the community. This effort developed an NTP engine system design analysis program (tool), known as the Nuclear Engine System Simulation (NESS) program, to support ongoing and future engine system and stage design study efforts. In this effort, Science Applications International Corporation's (SAIC) NTP version of the Expanded Liquid Engine Simulation (ELES) program was modified extensively to include Westinghouse Electric Corporation's near-term solid-core reactor design model. The ELES program has extensive capability to conduct preliminary system design analysis of liquid rocket systems and vehicles. The program is modular in nature and is versatile in terms of modeling state-of-the-art component and system options as discussed. The Westinghouse reactor design model, which was integrated in the NESS program, is based on the near-term solid-core ENABLER NTP reactor design concept. This program is now capable of accurately modeling (characterizing) a complete near-term solid-core NTP engine system in great detail, for a number of design options, in an efficient manner

AGN Obscuration Through Dusty Infrared Dominated Flows. 1; Radiation-Hydrodynamics Solution for the Wind

Science.gov (United States)

Dorodnitsyn, A.; Bisnovatyi-Kogan. G. S.; Kallman, T.

2011-01-01

We construct a radiation-hydrodynamics model for the obscuring toroidal structure in active galactic nuclei. In this model the obscuration is produced at parsec scale by a dense, dusty wind which is supported by infrared radiation pressure on dust grains. To find the distribution of radiation pressure, we numerically solve the 2D radiation transfer problem in a flux limited diffusion approximation. We iteratively couple the solution with calculations of stationary 1D models for the wind, and obtain the z-component of the velocity. Our results demonstrate that for AGN luminosities greater than 0.1 L(sub edd) external illumination can support a geometrically thick obscuration via outflows driven by infrared radiation pressure. The terminal velocity of marginally Compton-thin models (0.2 infrared-driven winds is a viable option for the AGN torus problem and AGN unification models. Such winds can also provide an important channel for AGN feedback.

New radiative transfer models for obscuring tori in active galaxies

NARCIS (Netherlands)

van Bemmel, IM; Dullemond, CP

Two-dimensional radiative transfer is employed to obtain the broad-band infrared spectrum of active galaxies. In the models we vary the geometry and size of the obscuring medium, the surface density, the opacity and the grain size distribution. Resulting spectral energy distributions are constructed

The effects of host obscuration on searches for tidal disruption events

Science.gov (United States)

Roth, Nathaniel; Mushotzky, Richard; Gezari, Suvi; van Velzen, Sjoert

2018-01-01

Tidal disruptions of stars by super-massive black holes (TDEs) offer opportunities to learn about black hole demographics and stellar dynamics. However, matching the observed TDE rate to that predicted by theory has remained a challenge, as most surveys to-date have found fewer flares than expected. Some of this discrepancy may relate to nuclear obscuration in host galaxies. This includes the effects of dust at optical and ultraviolet wavelengths, and the effects of neutral gas at x-ray wavelengths. I will discuss procedures to correct the observed TDE rate within existing and upcoming surveys to the intrinsic per-galaxy rate by accounting for host obscuration. I will also discuss how reddening might affect TDE selection criteria, and I will make predictions for the population of infrared TDE light echoes.

RUNX1 and RUNX3 protect against YAP-mediated EMT, stem-ness and shorter survival outcomes in breast cancer

Science.gov (United States)

Kulkarni, Madhura; Tan, Tuan Zea; Syed Sulaiman, Nurfarhanah Bte; Lamar, John M.; Bansal, Prashali; Cui, Jianzhou; Qiao, Yiting; Ito, Yoshiaki

2018-01-01

Hippo pathway target, YAP has emerged as an important player in solid tumor progression. Here, we identify RUNX1 and RUNX3 as novel negative regulators of oncogenic function of YAP in the context of breast cancer. RUNX proteins are one of the first transcription factors identified to interact with YAP. RUNX1 or RUNX3 expression abrogates YAP-mediated pro-tumorigenic properties of mammary epithelial cell lines in an interaction dependent manner. RUNX1 and RUNX3 inhibit YAP-mediated migration and stem-ness properties of mammary epithelial cell lines by co-regulating YAP-mediated gene expression. Analysis of whole genome expression profiles of breast cancer samples revealed significant co-relation between YAP–RUNX1/RUNX3 expression levels and survival outcomes of breast cancer patients. High RUNX1/RUNX3 expression proved protective towards YAP-dependent patient survival outcomes. High YAP in breast cancer patients’ expression profiles co-related with EMT and stem-ness gene signature enrichment. High RUNX1/RUNX3 expression along with high YAP reflected lower enrichment of EMT and stem-ness signatures. This antagonistic activity of RUNX1 and RUNX3 towards oncogenic function of YAP identified in mammary epithelial cells as well as in breast cancer expression profiles gives a novel mechanistic insight into oncogene–tumor suppressor interplay in the context of breast cancer progression. The novel interplay between YAP, RUNX1 and RUNX3 and its significance in breast cancer progression can serve as a prognostic tool to predict cancer recurrence. PMID:29581836

The angular clustering of WISE-selected active galactic nuclei: Different halos for obscured and unobscured active galactic nuclei

Energy Technology Data Exchange (ETDEWEB)

Donoso, E. [Instituto de Ciencias Astronómicas, de la Tierra, y del Espacio (ICATE), 5400 San Juan (Argentina); Yan, Lin [Infrared Processing and Analysis Center, Department of Astronomy, California Institute of Technology, Pasadena, CA 91125 (United States); Stern, D.; Assef, R. J. [Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA 91109 (United States)

2014-07-01

We calculate the angular correlation function for a sample of ∼170,000 active galactic nuclei (AGNs) extracted from the Wide-field Infrared Survey Explorer (WISE) catalog, selected to have red mid-IR colors (W1 – W2 > 0.8) and 4.6 μm flux densities brighter than 0.14 mJy). The sample is expected to be >90% reliable at identifying AGNs and to have a mean redshift of (z) = 1.1. In total, the angular clustering of WISE AGNs is roughly similar to that of optical AGNs. We cross-match these objects with the photometric Sloan Digital Sky Survey catalog and distinguish obscured sources with r – W2 > 6 from bluer, unobscured AGNs. Obscured sources present a higher clustering signal than unobscured sources. Since the host galaxy morphologies of obscured AGNs are not typical red sequence elliptical galaxies and show disks in many cases, it is unlikely that the increased clustering strength of the obscured population is driven by a host galaxy segregation bias. By using relatively complete redshift distributions from the COSMOS survey, we find that obscured sources at (z) ∼ 0.9 have a bias of b = 2.9 ± 0.6 and are hosted in dark matter halos with a typical mass of log (M/M {sub ☉} h {sup –1}) ∼ 13.5. In contrast, unobscured AGNs at (z) ∼ 1.1 have a bias of b = 1.6 ± 0.6 and inhabit halos of log (M/M {sub ☉} h {sup –1}) ∼ 12.4. These findings suggest that obscured AGNs inhabit denser environments than unobscured AGNs, and they are difficult to reconcile with the simplest AGN unification models, where obscuration is driven solely by orientation.

Jude the Obscure de Thomas Hardy et l’autorité de la lettre Jude the Obscure by Thomas Hardy and the Power of the Letter

Directory of Open Access Journals (Sweden)

Stéphanie Bernard

2009-10-01

Full Text Available Thomas Hardy is usually considered a Victorian writer. Nonetheless, his last novel Jude the Obscure, announced the era of modernity which started with the twentieth century, just before he abandoned fiction to concentrate on poetry. With modernity looming in the background, Jude the Obscure allowed for the rewriting of tragedy. Urban settings have replaced the countryside and all signs of transcendence have vanished from society. This defeat of the divine is nevertheless accompanied by a great number of biblical references. Thomas Hardy quotes and uses the Divine Letter as if to rewrite it rather than to appear faithful to the Word. The text keeps offering itself to the spell of voice: it does so when Job utters words of revolt and then worship, when Jude lets his imagination flow from his lips so that he seems to live on in the text after he is dead, or when the voice of the novelist becomes the voice of a poet.

AGN Obscuration Through Dusty Infrared Dominated Flows. II. Multidimensional, Radiation-Hydrodynamics Modeling

Science.gov (United States)

Dorodnitsyn, Anton; Kallman, Tim; Bisno\\vatyiI-Kogan, Gennadyi

2011-01-01

We explore a detailed model in which the active galactic nucleus (AGN) obscuration results from the extinction of AGN radiation in a global ow driven by the pressure of infrared radiation on dust grains. We assume that external illumination by UV and soft X-rays of the dusty gas located at approximately 1pc away from the supermassive black hole is followed by a conversion of such radiation into IR. Using 2.5D, time-dependent radiation hydrodynamics simulations in a ux-limited di usion approximation we nd that the external illumination can support a geometrically thick obscuration via out ows driven by infrared radiation pressure in AGN with luminosities greater than 0:05 L(sub edd) and Compton optical depth, Tau(sub T) approx > & 1.

Poder germinativo de sementes de capim-annoni-2 (Eragrostis plana Ness recuperadas em fezes de bovinos Germination of capim-annoni-2 (Eragrostis plana Ness seeds recovered in bovine feces

Directory of Open Access Journals (Sweden)

Celso Augusto Vargas Lisboa

2009-03-01

Full Text Available Objetivou-se com este trabalho avaliar o efeito do processo de digestão de bovinos sobre o poder germinativo de sementes de capim-annoni-2 (Eragrostisplana Ness recuperadas nas fezes. As sementes (6 g, 27.273 sementes foram colocadas no saco ventral do rúmem de oito novilhos fistulados, mantidos em gaiolas para ensaios metabólicos. Quarenta e três por cento das sementes fornecidas aos animais foram recuperadas nas fezes: aquelas recuperadas nos três primeiros dias corresponderam a 97,2% da quantidade de sementes fornecidas. Somente 7,2% das sementes recuperadas, equivalente a 3,1% da quantidade de sementes fornecidas, apresentaram viabilidade. O tempo de permanência no trato digestivo foi a principal causa do desaparecimento das sementes consumidas e da perda de seu poder germinativo. A ausência de sementes de capim-annoni-2 nas fezes ocorre a partir do oitavo dia após a ingestão, assim, bovinos devem permanecer em quarentena por sete dias em área livre de capim-annoni-2 para limpeza do trato digestivo.This work was carried out with the objective of evaluating the effect of the bovine digestion process on the germination capacity of the capim-annoni-2 (Eragrostisplana Ness seeds recovered in feces. The seeds (6 g, 27,273 seeds were placed in a ruminal ventral sack of eight fistulated steers kept in pen trial. Forthy-three percent of the offered seeds were recovered in the feces. Seeds recovered in the first three days corresponded to 97.2% of the offered seeds. Only 7.2% of the recovered seeds germinated and represented 3.1% of the offered seeds. The permanence time in the digestive trait was the main cause for the disappearance of consumed seeds and for the loss in their germination capacity. The absence of capim-annoni-2 seeds in the feces occurs in the eighth day after ingestion, then, bovines should be kept in quarantine for seven days in an area free of capim-annoni-2 seeds to clean their digestive trait.

Obscure bleeding colonic duplication responds to proton pump inhibitor therapy.

Science.gov (United States)

Jacques, Jérémie; Projetti, Fabrice; Legros, Romain; Valgueblasse, Virginie; Sarabi, Matthieu; Carrier, Paul; Fredon, Fabien; Bouvier, Stéphane; Loustaud-Ratti, Véronique; Sautereau, Denis

2013-09-21

We report the case of a 17-year-old male admitted to our academic hospital with massive rectal bleeding. Since childhood he had reported recurrent gastrointestinal bleeding and had two exploratory laparotomies 5 and 2 years previously. An emergency abdominal computed tomography scan, gastroscopy and colonoscopy, performed after hemodynamic stabilization, were considered normal. High-dose intravenous proton pump inhibitor (PPI) therapy was initiated and bleeding stopped spontaneously. Two other massive rectal bleeds occurred 8 h after each cessation of PPI which led to a hemostatic laparotomy after negative gastroscopy and small bowel capsule endoscopy. This showed long tubular duplication of the right colon, with fresh blood in the duplicated colon. Obscure lower gastrointestinal bleeding is a difficult medical situation and potentially life-threatening. The presence of ulcerated ectopic gastric mucosa in the colonic duplication explains the partial efficacy of PPI therapy. Obscure gastrointestinal bleeding responding to empiric anti-acid therapy should probably evoke the diagnosis of bleeding ectopic gastric mucosa such as Meckel's diverticulum or gastrointestinal duplication, and gastroenterologists should be aware of this potential medical situation.

Obscure gastrointestinal bleeding: difficulties in comparing CT enterography and video capsule endoscopy

International Nuclear Information System (INIS)

Soyer, Philippe

2012-01-01

A paper reports the results of a retrospective study that was designed to evaluate the potential role of video capsule endoscopy (VCE) in elucidating the cause of bleeding in patients with obscure gastrointestinal bleeding (OGIB) for whom CT enterography was negative. The authors highlight the limitations of dual-phase CT enterography for the detection of flat lesions of the small bowel such as ulcers, angiodysplasias or arteriovenous malformations, and confirm the superiority of VCE for the detection of this category of lesions. This commentary discusses some of the issues raised. Key Points circle Video capsule endoscopy surpasses CT enterography in detecting flat small bowel lesions. circle Retrospective VCE and CT enterography findings in obscure bleeding need further evaluation. circle A fair and unbiased comparison of the two investigations is still needed. (orig.)

The Near-Earth Space Surveillance (NESS) Mission: Discovery, Tracking, and Characterization of Asteroids, Comets, and Artificial Satellites with a Microsatellite

Science.gov (United States)

Hildebrand, A. R.; Carroll, K. A.; Balam, D. D.; Cardinal, R. D.; Matthews, J. M.; Kuschnig, R.; Walker, G. A. H.; Brown, P. G.; Tedesco, E. F.; Worden, S. P.

2001-01-01

The Near-Earth Space Surveillance (NESS) Mission, a microsatellite dedicated to observing near-Earth (NEO) and interior-to-the-Earth (IEO)asteroids and comets plus artificial satellites, is currently being studied under contract to the Canadian Space Agency. Additional information is contained in the original extended abstract.

The obscure factor analysis on the vibration reliability of the internals of nuclear power plant reactor and anti-vibration measures

International Nuclear Information System (INIS)

Fu Geyan; Zhu Qirong

1998-11-01

It is pointed out that the main reason making nuclear power plants reactors leak is the vibration of internals of reactors. The factors which lead the vibration all have randomness and obscureness. The obscure reliability theory is introduced to the vibration system of internals of nuclear power reactor. Based on a quantity of designing and moving data, the obscure factors effecting the vibration reliability of the internals of nuclear power plant reactor are analyzed and the anti-vibration reliability criteria and the evaluating model are given. And the anti-vibration reliability measures are advanced from different quarters of the machine design and building, the thermohydraulics design, the control of reactivity, etc.. They may benefit the theory and practice for building and perfecting the vibration obscure reliability model of the reactor internals

Advanced Boron Carbide-Based Visual Obscurants for Military Smoke Grenades

Science.gov (United States)

2014-07-13

components on grenade burning time must be accounted for. Also, how these factors affect smoke cloud thickness and perceived visible obscuration...of Boron Carbide-Based Smoke Compositions. Propellants, Explos., Pyrotech. 2013, 38, 622-628. (30) Commission Internationale de l’Éclairage ( CIE ...volume, gives equation 2. Since αm is only a characteristic of the aerosol, it does not account for

Geometrically Thick Obscuration by Radiation-driven Outflow from Magnetized Tori of Active Galactic Nuclei

Energy Technology Data Exchange (ETDEWEB)

Chan, Chi-Ho [Racah Institute of Physics, Hebrew University of Jerusalem, Jerusalem 91904 (Israel); Krolik, Julian H. [Department of Physics and Astronomy, Johns Hopkins University, Baltimore, MD 21218 (United States)

2017-07-01

Near-Eddington radiation from active galactic nuclei (AGNs) has significant dynamical influence on the surrounding dusty gas, plausibly furnishing AGNs with geometrically thick obscuration. We investigate this paradigm with radiative magnetohydrodynamics simulations. The simulations solve the magnetohydrodynamics equations simultaneously with the infrared (IR) and ultraviolet (UV) radiative transfer (RT) equations; no approximate closure is used for RT. We find that our torus, when given a suitable sub-Keplerian angular momentum profile, spontaneously evolves toward a state in which its opening angle, density distribution, and flow pattern change only slowly. This “steady” state lasts for as long as there is gas resupply toward the inner edge. The torus is best described as a midplane inflow and a high-latitude outflow. The outflow is launched from the torus inner edge by UV radiation and expands in solid angle as it ascends; IR radiation continues to drive the wide-angle outflow outside the central hole. The dusty outflow obscures the central source in soft X-rays, the IR, and the UV over three-quarters of solid angle, and each decade in column density covers roughly equal solid angle around the central source; these obscuration properties are similar to what observations imply.

Assessing Toxicity of Obscurant Grade Pan-Based Carbon Fiber Aquatic Species Chronic Tests

National Research Council Canada - National Science Library

Chester, N. A; Haley, M. V; Kumas, C. W; Checkai, R. T

2004-01-01

...). Use of polyacrylonitrile (PAN)-based carbon fiber in the module will provide user-capability for delivering large area obscurant screens in the millimeter wave-range of the electromagnetic spectrum while maintaining...

Wide-Spectrum Microscope with a Long Working Distance Aspherical Objective Based on Obscuration Constraint

Directory of Open Access Journals (Sweden)

Weibo Wang

2016-11-01

Full Text Available We present an approach for an initial configuration design based on obscuration constraint and on-axis Taylor series expansion to realize the design of long working distance microscope (numerical aperture (NA = 0.13 and working distance (WD = 525 mm with a low obscuration aspherical Schwarzschild objective in wide-spectrum imaging (λ = 400–900 nm. Experiments of the testing on the resolution target and inspection on United States Air Force (USAF resolution chart and a line charge-coupled device (CCD (pixel size of 14 μm × 56 μm with different wavelength light sources (λ = 480 nm, 550 nm, 660 nm, 850 nm were implemented to verify the validity of the proposed method.

NuSTAR observations of heavily obscured quasars at z ~ 0.5

DEFF Research Database (Denmark)

Lansbury, G. B.; Alexander, D. M.; Del Moro, A.

2014-01-01

We present NuSTAR hard X-ray observations of three Type 2 quasars at z ≈ 0.4-0.5, optically selected from the Sloan Digital Sky Survey. Although the quasars show evidence for being heavily obscured, Compton-thick systems on the basis of the 2-10 keV to [O III] luminosity ratio and multiwavelength...

New radiative transfer models for obscuring tori in active galaxies

OpenAIRE

van Bemmel, I. M.; Dullemond, C. P.

2003-01-01

Two-dimensional radiative transfer is employed to obtain the broad-band infrared spectrum of active galaxies. In the models we vary the geometry and size of the obscuring medium, the surface density, the opacity and the grain size distribution. Resulting spectral energy distributions are constructed for different orientations of the toroid. Colour-colour comparisons with observational data are consistent with previous observations that the emission longward of 60 micron is produced by star-fo...

A SUBMILLIMETER CONTINUUM SURVEY OF LOCAL DUST-OBSCURED GALAXIES

International Nuclear Information System (INIS)

Lee, Jong Chul; Hwang, Ho Seong; Lee, Gwang-Ho

2016-01-01

We conduct a 350 μ m dust continuum emission survey of 17 dust-obscured galaxies (DOGs) at z = 0.05–0.08 with the Caltech Submillimeter Observatory (CSO). We detect 14 DOGs with S 350μm = 114–650 mJy and signal-to-noise > 3. By including two additional DOGs with submillimeter data in the literature, we are able to study dust content for a sample of 16 local DOGs, which consist of 12 bump and four power-law types. We determine their physical parameters with a two-component modified blackbody function model. The derived dust temperatures are in the range 57–122 K and 22–35 K for the warm and cold dust components, respectively. The total dust mass and the mass fraction of the warm dust component are 3–34 × 10 7 M ⊙ and 0.03%–2.52%, respectively. We compare these results with those of other submillimeter-detected infrared luminous galaxies. The bump DOGs, the majority of the DOG sample, show similar distributions of dust temperatures and total dust mass to the comparison sample. The power-law DOGs show a hint of smaller dust masses than other samples, but need to be tested with a larger sample. These findings support that the reason DOGs show heavy dust obscuration is not an overall amount of dust content, but probably the spatial distribution of dust therein.

A SUBMILLIMETER CONTINUUM SURVEY OF LOCAL DUST-OBSCURED GALAXIES

Energy Technology Data Exchange (ETDEWEB)

Lee, Jong Chul [Korea Astronomy and Space Science Institute, 776 Daedeokdae-ro, Yuseong-gu, Daejeon 34055 (Korea, Republic of); Hwang, Ho Seong [School of Physics, Korea Institute for Advanced Study, 85 Hoegiro, Dongdaemun-gu, Seoul 02455 (Korea, Republic of); Lee, Gwang-Ho, E-mail: jclee@kasi.re.kr [Department of Physics and Astronomy, Seoul National University, 1 Gwanak-ro, Gwanak-gu, Seoul 151-742 (Korea, Republic of)

2016-12-20

We conduct a 350 μ m dust continuum emission survey of 17 dust-obscured galaxies (DOGs) at z = 0.05–0.08 with the Caltech Submillimeter Observatory (CSO). We detect 14 DOGs with S{sub 350μm} = 114–650 mJy and signal-to-noise > 3. By including two additional DOGs with submillimeter data in the literature, we are able to study dust content for a sample of 16 local DOGs, which consist of 12 bump and four power-law types. We determine their physical parameters with a two-component modified blackbody function model. The derived dust temperatures are in the range 57–122 K and 22–35 K for the warm and cold dust components, respectively. The total dust mass and the mass fraction of the warm dust component are 3–34 × 10{sup 7} M {sub ⊙} and 0.03%–2.52%, respectively. We compare these results with those of other submillimeter-detected infrared luminous galaxies. The bump DOGs, the majority of the DOG sample, show similar distributions of dust temperatures and total dust mass to the comparison sample. The power-law DOGs show a hint of smaller dust masses than other samples, but need to be tested with a larger sample. These findings support that the reason DOGs show heavy dust obscuration is not an overall amount of dust content, but probably the spatial distribution of dust therein.

Obscure gastrointestinal bleeding: preliminary comparison of 64-section CT enteroclysis with video capsule endoscopy

International Nuclear Information System (INIS)

Khalife, Samer; Vahedi, Kouroche; Dray, Xavier; Marteau, Philippe; Soyer, Philippe; Hamzi, Lounis; Place, Vinciane; Boudiaf, Mourad; Alatawi, Abdullah

2011-01-01

To retrospectively compare the diagnostic capabilities of 64-section CT enteroclysis with those of video capsule endoscopy (VCE) to elucidate the cause of obscure gastrointestinal bleeding. Thirty-two patients who had 64-section CT enteroclysis and VCE because of obscure gastrointestinal bleeding were included. Imaging findings were compared with those obtained at double balloon endoscopy, surgery and histopathological analysis, which were used as a standard of reference. Concordant findings were found in 22 patients (22/32; 69%), including normal findings (n = 13), tumours (n = 7), lymphangiectasia (n = 1) and inflammation (n = 1), and discrepancies in 10 patients (10/32; 31%), including ulcers (n = 3), angioectasias (n = 2), tumours (n = 2) and normal findings (n = 3). No statistical difference in the proportions of abnormal findings between 64-section CT enteroclysis (11/32; 34%) and VCE (17/32, 53%) (P = 0.207) was found. However, 64-section CT enteroclysis helped identify tumours not detected at VCE (n = 2) and definitely excluded suspected tumours (n = 3) because of bulges at VCE. Conversely, VCE showed ulcers (n = 3) and angioectasias (n = 2) which were not visible at 64-section CT enteroclysis. Our results suggest that 64-section CT enteroclysis and VCE have similar overall diagnostic yields in patients with obscure gastrointestinal bleeding. However, the two techniques are complementary in this specific population. (orig.)

NuSTAR and XMM-Newton observations of luminous, heavily obscured, WISE-selected quasars at z ∼ 2

Energy Technology Data Exchange (ETDEWEB)

Stern, D.; Eisenhardt, P. R. M. [Jet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Drive, Mail Stop 169-221, Pasadena, CA 91109 (United States); Lansbury, G. B.; Alexander, D. M.; Del Moro, A.; Gandhi, P. [Department of Physics, University of Durham, South Road, Durham DH1 3LE (United Kingdom); Assef, R. J. [Núcleo de Astronomía de la Facultad de Ingeniería, Universidad Diego Portales, Av. Ejército Libertador 441, Santiago (Chile); Brandt, W. N.; Griffith, R. L. [Department of Astronomy and Astrophysics, The Pennsylvania State University, 525 Davey Lab, University Park, PA 16802 (United States); Ballantyne, D. R. [Center for Relativistic Astrophysics, School of Physics, Georgia Institute of Technology, Atlanta, GA 30332 (United States); Baloković, M.; Bridge, C. [Cahill Center for Astronomy and Astrophysics, California Institute of Technology, Pasadena, CA 91125 (United States); Bauer, F. E. [Instituto de Astrofísica, Facultad de Física, Pontificia Universidad Católica de Chile, 306, Santiago 22 (Chile); Benford, D. [NASA Goddard Space Flight Center, Greenbelt, MD 20771 (United States); Blain, A. [Physics and Astronomy, University of Leicester, 1 University Road, Leicester, LE1 7RH (United Kingdom); Boggs, S. E.; Craig, W. W. [Space Sciences Laboratory, University of California, Berkeley, 7 Gauss Way, Berkeley, CA 94720-7450 (United States); Brightman, M. [Max-Planck-Institut für extraterrestrische Physik, Giessenbachstrasse 1, D-85748, Garching bei München (Germany); Christensen, F. E. [Danish Technical University, DK-2800 Lyngby (Denmark); Comastri, A., E-mail: daniel.k.stern@jpl.nasa.gov [INAF Osservatorio Astronomico di Bologna, via Ranzani 1, I-40127, Bologna (Italy); and others

2014-10-20

We report on a NuSTAR and XMM-Newton program that has observed a sample of three extremely luminous, heavily obscured WISE-selected active galactic nuclei (AGNs) at z ∼ 2 across a broad X-ray band (0.1 – 79 keV). The parent sample, selected to be faint or undetected in the WISE 3.4 μm (W1) and 4.6 μm (W2) bands but bright at 12 μm (W3) and 22 μm (W4), are extremely rare, with only ∼1000 so-called 'W1W2-dropouts' across the extragalactic sky. Optical spectroscopy reveals typical redshifts of z ∼ 2 for this population, implying rest-frame mid-IR luminosities of νL {sub ν}(6 μm) ∼ 6 × 10{sup 46} erg s{sup –1} and bolometric luminosities that can exceed L {sub bol} ∼ 10{sup 14} L {sub ☉}. The corresponding intrinsic, unobscured hard X-ray luminosities are L(2-10 keV) ∼ 4 × 10{sup 45} erg s{sup –1} for typical quasar templates. These are among the most AGNs known, though the optical spectra rarely show evidence of a broad-line region and the selection criteria imply heavy obscuration even at rest-frame 1.5 μm. We designed our X-ray observations to obtain robust detections for gas column densities N {sub H} ≤ 10{sup 24} cm{sup –2}. In fact, the sources prove to be fainter than these predictions. Two of the sources were observed by both NuSTAR and XMM-Newton, with neither being detected by NuSTAR (f {sub 3-24} {sub keV} ≲ 10{sup –13} erg cm{sup –2} s{sup –1}), and one being faintly detected by XMM-Newton (f {sub 0.5-10} {sub keV} ∼ 5 × 10{sup –15} erg cm{sup –2} s{sup –1}). A third source was observed only with XMM-Newton, yielding a faint detection (f {sub 0.5-10} {sub keV} ∼ 7 × 10{sup –15} erg cm{sup –2} s{sup –1}). The X-ray data imply these sources are either X-ray weak, or are heavily obscured by column densities N {sub H} ≳ 10{sup 24} cm{sup –2}. The combined X-ray and mid-IR analysis seems to favor this second possibility, implying the sources are extremely obscured, consistent with Compton

NuSTAR and XMM-Newton observations of luminous, heavily obscured, WISE-selected quasars at z ∼ 2

International Nuclear Information System (INIS)

Stern, D.; Eisenhardt, P. R. M.; Lansbury, G. B.; Alexander, D. M.; Del Moro, A.; Gandhi, P.; Assef, R. J.; Brandt, W. N.; Griffith, R. L.; Ballantyne, D. R.; Baloković, M.; Bridge, C.; Bauer, F. E.; Benford, D.; Blain, A.; Boggs, S. E.; Craig, W. W.; Brightman, M.; Christensen, F. E.; Comastri, A.

2014-01-01

We report on a NuSTAR and XMM-Newton program that has observed a sample of three extremely luminous, heavily obscured WISE-selected active galactic nuclei (AGNs) at z ∼ 2 across a broad X-ray band (0.1 – 79 keV). The parent sample, selected to be faint or undetected in the WISE 3.4 μm (W1) and 4.6 μm (W2) bands but bright at 12 μm (W3) and 22 μm (W4), are extremely rare, with only ∼1000 so-called 'W1W2-dropouts' across the extragalactic sky. Optical spectroscopy reveals typical redshifts of z ∼ 2 for this population, implying rest-frame mid-IR luminosities of νL ν (6 μm) ∼ 6 × 10 46 erg s –1 and bolometric luminosities that can exceed L bol ∼ 10 14 L ☉ . The corresponding intrinsic, unobscured hard X-ray luminosities are L(2-10 keV) ∼ 4 × 10 45 erg s –1 for typical quasar templates. These are among the most AGNs known, though the optical spectra rarely show evidence of a broad-line region and the selection criteria imply heavy obscuration even at rest-frame 1.5 μm. We designed our X-ray observations to obtain robust detections for gas column densities N H ≤ 10 24 cm –2 . In fact, the sources prove to be fainter than these predictions. Two of the sources were observed by both NuSTAR and XMM-Newton, with neither being detected by NuSTAR (f 3-24 keV ≲ 10 –13 erg cm –2 s –1 ), and one being faintly detected by XMM-Newton (f 0.5-10 keV ∼ 5 × 10 –15 erg cm –2 s –1 ). A third source was observed only with XMM-Newton, yielding a faint detection (f 0.5-10 keV ∼ 7 × 10 –15 erg cm –2 s –1 ). The X-ray data imply these sources are either X-ray weak, or are heavily obscured by column densities N H ≳ 10 24 cm –2 . The combined X-ray and mid-IR analysis seems to favor this second possibility, implying the sources are extremely obscured, consistent with Compton-thick, luminous quasars. The discovery of a significant population of heavily obscured, extremely luminous AGNs would not conform to the standard

DUST PROPERTIES OF LOCAL DUST-OBSCURED GALAXIES WITH THE SUBMILLIMETER ARRAY

International Nuclear Information System (INIS)

Hwang, Ho Seong; Andrews, Sean M.; Geller, Margaret J.

2013-01-01

We report Submillimeter Array observations of the 880 μm dust continuum emission for four dust-obscured galaxies (DOGs) in the local universe. Two DOGs are clearly detected with S ν (880 μm) =10-13 mJy and S/N > 5, but the other two are not detected with 3σ upper limits of S ν (880 μm) =5-9 mJy. Including an additional two local DOGs with submillimeter data from the literature, we determine the dust masses and temperatures for six local DOGs. The infrared luminosities and dust masses for these DOGs are in the ranges of 1.2-4.9 × 10 11 (L ☉ ) and 4-14 × 10 7 (M ☉ ), respectively. The dust temperatures derived from a two-component modified blackbody function are 23-26 K and 60-124 K for the cold and warm dust components, respectively. Comparison of local DOGs with other infrared luminous galaxies with submillimeter detections shows that the dust temperatures and masses do not differ significantly among these objects. Thus, as argued previously, local DOGs are not a distinctive population among dusty galaxies, but simply represent the high-end tail of the dust obscuration distribution

Technical Feasibility Study of an Effective Low-Toxicity Obscurant Material

Science.gov (United States)

2012-08-01

chloride based obscurant composition 11EM0745 p. 20 Figure 4.15 The variable electric current source and the resistance wire (Nickel- Chrome , 0.2...type of magnesium powder under the name AZ91D was obtained from Metal Powder Technology Ltd, from the UK and is free from hexavalent chromium. 6...The test samples (F), are ignited by a resistance wire (Nickel- Chrome , 0.2 mm diameter from British Driver Harris, UK). This wire is heated by

Recurrent Obscure Gastrointestinal Bleeding: Dilemmas and Success with Pharmacological Therapies. Case Series and Review

Directory of Open Access Journals (Sweden)

Majid Almadi

2009-01-01

Full Text Available The present article describes three difficult cases of recurrent bleeding from obscure causes, followed by a review of the pitfalls and pharmacological management of obscure gastrointestinal bleeding. All three patients underwent multiple investigations. An intervening complicating diagnosis or antiplatelet drugs may have compounded long-term bleeding in two of the cases. A bleeding angiodysplasia was confirmed in one case but was aggravated by the need for anticoagulation. After multiple transfusions and several attempts at endoscopic management in some cases, long-acting octreotide was associated with decreased transfusion requirements and increased hemoglobin levels in all three cases, although other factors may have contributed in some. In the third case, however, the addition of low-dose thalidomide stopped bleeding for a period of at least 23 months.

Security without obscurity a guide to confidentiality, authentication, and integrity

CERN Document Server

Stapleton, JJ

2014-01-01

The traditional view of information security includes the three cornerstones: confidentiality, integrity, and availability; however the author asserts authentication is the third keystone. As the field continues to grow in complexity, novices and professionals need a reliable reference that clearly outlines the essentials. Security without Obscurity: A Guide to Confidentiality, Authentication, and Integrity fills this need. Rather than focusing on compliance or policies and procedures, this book takes a top-down approach. It shares the author's knowledge, insights, and observations about infor

DUST PROPERTIES OF LOCAL DUST-OBSCURED GALAXIES WITH THE SUBMILLIMETER ARRAY

Energy Technology Data Exchange (ETDEWEB)

Hwang, Ho Seong; Andrews, Sean M.; Geller, Margaret J., E-mail: hhwang@cfa.harvard.edu, E-mail: sandrews@cfa.harvard.edu, E-mail: mgeller@cfa.harvard.edu [Smithsonian Astrophysical Observatory, 60 Garden Street, Cambridge, MA 02138 (United States)

2013-11-01

We report Submillimeter Array observations of the 880 μm dust continuum emission for four dust-obscured galaxies (DOGs) in the local universe. Two DOGs are clearly detected with S{sub ν}(880 μm) =10-13 mJy and S/N > 5, but the other two are not detected with 3σ upper limits of S{sub ν}(880 μm) =5-9 mJy. Including an additional two local DOGs with submillimeter data from the literature, we determine the dust masses and temperatures for six local DOGs. The infrared luminosities and dust masses for these DOGs are in the ranges of 1.2-4.9 × 10{sup 11}(L{sub ☉}) and 4-14 × 10{sup 7}(M{sub ☉}), respectively. The dust temperatures derived from a two-component modified blackbody function are 23-26 K and 60-124 K for the cold and warm dust components, respectively. Comparison of local DOGs with other infrared luminous galaxies with submillimeter detections shows that the dust temperatures and masses do not differ significantly among these objects. Thus, as argued previously, local DOGs are not a distinctive population among dusty galaxies, but simply represent the high-end tail of the dust obscuration distribution.

Large scale obscuration and related climate effects open literature bibliography

Energy Technology Data Exchange (ETDEWEB)

Russell, N.A.; Geitgey, J.; Behl, Y.K.; Zak, B.D.

1994-05-01

Large scale obscuration and related climate effects of nuclear detonations first became a matter of concern in connection with the so-called ``Nuclear Winter Controversy`` in the early 1980`s. Since then, the world has changed. Nevertheless, concern remains about the atmospheric effects of nuclear detonations, but the source of concern has shifted. Now it focuses less on global, and more on regional effects and their resulting impacts on the performance of electro-optical and other defense-related systems. This bibliography reflects the modified interest.

Large scale obscuration and related climate effects open literature bibliography

International Nuclear Information System (INIS)

Russell, N.A.; Geitgey, J.; Behl, Y.K.; Zak, B.D.

1994-05-01

Large scale obscuration and related climate effects of nuclear detonations first became a matter of concern in connection with the so-called ''Nuclear Winter Controversy'' in the early 1980's. Since then, the world has changed. Nevertheless, concern remains about the atmospheric effects of nuclear detonations, but the source of concern has shifted. Now it focuses less on global, and more on regional effects and their resulting impacts on the performance of electro-optical and other defense-related systems. This bibliography reflects the modified interest

The NuSTAR Serendipitous Survey: Hunting for the Most Extreme Obscured AGN at >10 keV

Science.gov (United States)

Lansbury, G. B.; Alexander, D. M.; Aird, J.; Gandhi, P.; Stern, D.; Koss, M.; Lamperti, I.; Ajello, M.; Annuar, A.; Assef, R. J.; Ballantyne, D. R.; Baloković, M.; Bauer, F. E.; Brandt, W. N.; Brightman, M.; Chen, C.-T. J.; Civano, F.; Comastri, A.; Del Moro, A.; Fuentes, C.; Harrison, F. A.; Marchesi, S.; Masini, A.; Mullaney, J. R.; Ricci, C.; Saez, C.; Tomsick, J. A.; Treister, E.; Walton, D. J.; Zappacosta, L.

2017-09-01

We identify sources with extremely hard X-ray spectra (I.e., with photon indices of {{Γ }}≲ 0.6) in the 13 deg2 NuSTAR serendipitous survey, to search for the most highly obscured active galactic nuclei (AGNs) detected at > 10 {keV}. Eight extreme NuSTAR sources are identified, and we use the NuSTAR data in combination with lower-energy X-ray observations (from Chandra, Swift XRT, and XMM-Newton) to characterize the broadband (0.5-24 keV) X-ray spectra. We find that all of the extreme sources are highly obscured AGNs, including three robust Compton-thick (CT; {N}{{H}}> 1.5× {10}24 cm-2) AGNs at low redshift (z< 0.1) and a likely CT AGN at higher redshift (z = 0.16). Most of the extreme sources would not have been identified as highly obscured based on the low-energy (< 10 keV) X-ray coverage alone. The multiwavelength properties (e.g., optical spectra and X-ray-mid-IR luminosity ratios) provide further support for the eight sources being significantly obscured. Correcting for absorption, the intrinsic rest-frame 10-40 keV luminosities of the extreme sources cover a broad range, from ≈ 5× {10}42 to 1045 erg s-1. The estimated number counts of CT AGNs in the NuSTAR serendipitous survey are in broad agreement with model expectations based on previous X-ray surveys, except for the lowest redshifts (z< 0.07), where we measure a high CT fraction of {f}{CT}{obs}={30}-12+16 % . For the small sample of CT AGNs, we find a high fraction of galaxy major mergers (50% ± 33%) compared to control samples of “normal” AGNs.

EVIDENCE FOR A WIDE RANGE OF ULTRAVIOLET OBSCURATION IN z {approx} 2 DUSTY GALAXIES FROM THE GOODS-HERSCHEL SURVEY

Energy Technology Data Exchange (ETDEWEB)

Penner, Kyle [Department of Astronomy, University of Arizona, Tucson, AZ 85721 (United States); Dickinson, Mark; Dey, Arjun; Kartaltepe, Jeyhan [National Optical Astronomy Observatory, Tucson, AZ 85719 (United States); Pope, Alexandra [Department of Astronomy, University of Massachusetts, Amherst, MA 01003 (United States); Magnelli, Benjamin [Max Planck Institut fuer Extraterrestrische Physik, Postfach 1312, D-85741 Garching (Germany); Pannella, Maurilio; Aussel, Herve; Daddi, Emanuele; Elbaz, David [Laboratoire AIM Paris-Saclay, CEA/DSM/Irfu-CNRS-Universite Paris Diderot, CEA-Saclay, pt courrier 131, F-91191 Gif-sur-Yvette (France); Altieri, Bruno; Coia, Daniela [Herschel Science Center, European Space Astronomy Center, Villanueva de la Canada, E-28691 Madrid (Spain); Buat, Veronique [Laboratoire d' Astrophysique de Marseille, OAMP, Universite Aix-marseille, CNRS, 38 rue Frederic Joliot-Curie, F-13388 Marseille Cedex 13 (France); Bussmann, Shane; Hwang, Ho Seong [Harvard-Smithsonian Center for Astrophysics, Cambridge, MA 02138 (United States); Charmandaris, Vassilis [Department of Physics and Institute of Theoretical and Computational Physics, University of Crete, GR-71003 Heraklion (Greece); Dannerbauer, Helmut [Institut fuer Astronomie, Universitaet Wien, Tuerkenschanzstrasse 17, A-1180 Vienna (Austria); Lin Lihwai [Institute of Astronomy and Astrophysics, Academia Sinica, Taipei 106, Taiwan (China); Magdis, Georgios [Department of Physics, University of Oxford, Keble Road, Oxford OX1 3RH (United Kingdom); Morrison, Glenn, E-mail: kpenner@as.arizona.edu [Institute for Astronomy, University of Hawaii, Honolulu, HI 96822 (United States); and others

2012-11-01

Dusty galaxies at z {approx} 2 span a wide range of relative brightness between rest-frame mid-infrared (8 {mu}m) and ultraviolet wavelengths. We attempt to determine the physical mechanism responsible for this diversity. Dust-obscured galaxies (DOGs), which have rest-frame mid-IR to UV flux density ratios {approx}> 1000, might be abnormally bright in the mid-IR, perhaps due to prominent emission from active galactic nuclei and/or polycyclic aromatic hydrocarbons, or abnormally faint in the UV. We use far-infrared data from the GOODS-Herschel survey to show that most DOGs with 10{sup 12} L {sub Sun} {approx}< L {sub IR} {approx}< 10{sup 13} L {sub Sun} are not abnormally bright in the mid-IR when compared to other dusty galaxies with similar IR (8-1000 {mu}m) luminosities. We observe a relation between the median IR to UV luminosity ratios and the median UV continuum power-law indices for these galaxies, and we find that only 24% have specific star formation rates that indicate the dominance of compact star-forming regions. This circumstantial evidence supports the idea that the UV- and IR-emitting regions in these galaxies are spatially coincident, which implies a connection between the abnormal UV faintness of DOGs and dust obscuration. We conclude that the range in rest-frame mid-IR to UV flux density ratios spanned by dusty galaxies at z {approx} 2 is due to differing amounts of UV obscuration. Of galaxies with these IR luminosities, DOGs are the most obscured. We attribute differences in UV obscuration to either (1) differences in the degree of alignment between the spatial distributions of dust and massive stars or (2) differences in the total dust content.

MILLIMETER OBSERVATIONS OF A SAMPLE OF HIGH-REDSHIFT OBSCURED QUASARS

International Nuclear Information System (INIS)

Martinez-Sansigre, Alejo; Karim, Alexander; Schinnerer, Eva

2009-01-01

We present observations at 1.2 mm with Max-Planck Millimetre Bolometer Array (MAMBO-II) of a sample of z ∼> 2 radio-intermediate obscured quasars, as well as CO observations of two sources with the Plateau de Bure Interferometer. The typical rms noise achieved by the MAMBO observations is 0.55 mJy beam -1 and five out of 21 sources (24%) are detected at a significance of ≥3σ. Stacking all sources leads to a statistical detection of (S 1.2mm ) = 0.96 ± 0.11 mJy and stacking only the non-detections also yields a statistical detection, with (S 1.2mm ) = 0.51 ± 0.13 mJy. At the typical redshift of the sample, z = 2, 1 mJy corresponds to a far-infrared luminosity L FIR ∼4 x 10 12 L sun . If the far-infrared luminosity is powered entirely by star formation, and not by active galactic nucleus heated dust, then the characteristic inferred star formation rate is ∼700 M sun yr -1 . This far-infrared luminosity implies a dust mass of M d ∼3 x 10 8 M sun , which is expected to be distributed on ∼kpc scales. We estimate that such large dust masses on kpc scales can plausibly cause the obscuration of the quasars. Combining our observations at 1.2 mm with mid- and far-infrared data, and additional observations for two objects at 350 μm using SHARC-II, we present dust spectral energy distributions (SEDs) for our sample and derive a mean SED for our sample. This mean SED is not well fitted by clumpy torus models, unless additional extinction and far-infrared re-emission due to cool dust are included. This additional extinction can be consistently achieved by the mass of cool dust responsible for the far-infrared emission, provided the bulk of the dust is within a radius ∼2-3 kpc. Comparison of our sample to other samples of z ∼ 2 quasars suggests that obscured quasars have, on average, higher far-infrared luminosities than unobscured quasars. There is a hint that the host galaxies of obscured quasars must have higher cool-dust masses and are therefore often

GNSS Wave Glider: First results from Loch Ness and demonstration of its suitability for determining the marine geoid

Science.gov (United States)

Penna, N. T.; Morales Maqueda, M.; Williams, S. D.; Foden, P.; Martin, I.; Pugh, J.

2013-12-01

We report on a first deployment of a GNSS Wave Glider designed for precise, unmanned, autonomous, mobile self-propelled sea level and sea state measurement in the open ocean. The Wave Glider, equipped with a dual frequency GPS+GLONASS receiver, was deployed in Loch Ness, Scotland, autonomously travelling 32 km in a north-easterly direction along the length of the loch in 26 hours, propelled by energy generated from waves of typical amplitude only 100-150 mm and frequency on the order 0.5-1 Hz. The Wave Glider GNSS data were analysed using a post-processed kinematic GPS+GLONASS precise point positioning (PPP) approach, which were quality controlled using double difference GPS kinematic processing with respect to onshore reference stations at either end of the loch. The PPP heights of the loch's surface revealed a clear geoid gradient of about 30 mm/km (i.e. just under 1 m over the whole length of the loch), very similar to both the EGM2008 and OSGM02 geoid models, demonstrating the potential use of a GNSS Wave Glider for marine geoid determination. After applying a low pass filter, the GNSS heights showed local deviations from both EGM2008 and OSGM02, potentially caused by omission errors or a lack of gravity data over Loch Ness. In addition to dual frequency GNSS data, the Wave Glider also recorded inclinometer data, bathymetry, and surface currents, which, in combination with tide gauge and wind data, were used to further control and interpret the GNSS time series.

The Geometry of the Infrared and X-Ray Obscurer in a Dusty Hyperluminous Quasar

DEFF Research Database (Denmark)

Farrah, Duncan; Baloković, Mislav; Stern, Daniel

2016-01-01

We study the geometry of the active galactic nucleus (AGN) obscurer in IRAS 09104+4109, an IR-luminous, radio-intermediate FR-I source at z = 0.442, using infrared data from Spitzer and Herschel, X-ray data from NuSTAR, Swift, Suzaku, and Chandra, and an optical spectrum from Palomar. The infrare...

Variable dust obscuration in the symbiotic Mira and very slow Nova, HM Sge

International Nuclear Information System (INIS)

Munari, U.; Whitelock, P.A.

1989-01-01

New infrared photometry is presented for the symbiotic Mira, HM Sge. Using this and published data a pulsation period of 527 day is derived. In addition to the normal pulsational modulation, the light curve for HM Sge has shown a distinct fading and reddening, starting in 1985. This is interpreted as a dust-obscuration event, and its possible association with the binary orbit is discussed. (author)

One Health-ness Evaluation of Cysticercosis Surveillance Design in Portugal

Directory of Open Access Journals (Sweden)

Ana Gloria Fonseca

2018-03-01

Full Text Available The increasing occurrence of human cysticercosis, a zoonotic neglected disease, is challenging the traditional prevention and control paradigm and calling for One Health (OH solutions in industrialized countries. OH solutions for health interventions are increasingly being used to capture expected and unexpected outcomes across people, animals, and the environment. The Network for Evaluation of One Health (NEOH proposes an evidence-based framework, relying on systems and mixed methods approaches to evaluate the One Health-ness. In this case study, this tool is used to evaluate the design of the Observatory of Taeniasis and Cysticercosis, as an example of intersectorial collaboration for surveillance in Portugal. The OH Initiative (drivers and expected outcomes and its system (boundaries, aim, dimensions, actors, and stakeholders were described. The different aspects of this Initiative were scored with values from 0 (=no OH approach to 1 (=perfect OH approach. The OH index was 0.31. Its OH ratio is 1.98. Overall scores were as follows: OH thinking 0.75; OH planning 0.60; OH working 0.60; OH sharing 0.35; OH learning 0.50; and systemic organization 0.50. Operational levels of the Initiative are the main strengths, indicating a comprehensive multidimensional innovative approach and transdisciplinarity. Critical issues in the supporting infrastructure were observed, related to communication, learning and organizational gaps in the project, with the evaluation being conducted as the project is being designed and implemented. The strengths and weaknesses detected may be used to refine the Initiative. This case study therefore exemplifies and supports OH assessment also for ongoing projects, at design and early implementation stages for guiding and guaranteeing an OH-oriented perspective.

An assessment, using stable isotopes, of the importance of allochthonous organic carbon sources to the pelagic food web in Loch Ness

Science.gov (United States)

Jones, R. I.; Grey, J.; Sleep, D.; Quarmby, C.

1998-01-01

The natural abundance of stable isotopes (δ13C and δ1315N) was determined for components of the pelagic food web in Loch Ness, a deep oligotrophic lake in northern Scotland, and compared with values from the inflow rivers and the catchment vegetation. Phytoplankton δ13C was low compared to values reported from other lakes, possibly reflecting a high use of 13C-depleted carbon dioxide from respired organic matter before further isotopic fractionation during photosynthesis. Phytoplankton δ13C was appreciably lower than that of dissolved and particulate organic matter (DOM and POM) in the loch. The DOM and POM were evidently overwhelmingly of allochthonous origin and ultimately derived from terrestrial plant detritus. The distinctive δ13C values for phytoplankton and detritus in the loch allowed the use of food sources by grazing crustacean zooplankton to be assessed, and the contributions of phytoplankton carbon and detrital carbon to zooplankton total body carbon appeared to be about equal. Comparison of δ13C and δ15N values for zooplankton and fish allowed assessment of trophic structure in the loch. The very high dependence of the pelagic food web in Loch Ness on allochthonous organic matter inputs from the catchment may be exceptional in a large lake, but has important implications for our understanding of lake ecosystem processes as well as for lake management.

Study on the morphology and agroecology of creat (Andrographis panculata ness. in various habitat

Directory of Open Access Journals (Sweden)

BAMBANG PUJIASMANTO

2007-10-01

Full Text Available Raw material supply which still depends on nature has caused genetic erotion of medicinal plants. The objectives of the research were to study creat (Andrographis paniculata Ness. morphology; and agroecology in many habitat for cultivated be medical substance. The research were conducted at three different locations, ie. at lowland ( 700 m asl.. The result showed that creat growth on 180 m – 861 m above sea level with environmental conditions : temperature 20.320C – 26.930C, relative humidity 78% - 87%, perticipation 2053.2 mm/ year – 3555.6 mm/ year. The creat can growth on soil mineral that contains N medium, P low, K medium, Mg low, Ca verylow until low ,C organic low until medium, and pH less acid until acid. The heihgt plant of creat in middleland is the highest of in lowland and upland, that also leaf of creat. The flower, fruit, and root of creat as good as in the habitat various. The highest andrographolid contain in middleland (2.27%, whereas in lowland (1.37% and upland (0.89%.

The Body and its Able-ness: Articulating In/Eligibility through Rhetorics of Motherhood, Unjust Language, and Questionable Medical Authority

Directory of Open Access Journals (Sweden)

Rachel D. Davidson

2016-03-01

Full Text Available This essay analyzes a controversy involving Amelia (Mia Rivera, a three-year old girl who was denied a life-saving kidney transplant in January 2012. As reported by Mia's mother, Chrissy, on her blog post, Mia was denied the kidney transplant because of her mental disability. Throughout the public discussion that took place over a few short weeks, we argue Mia's ineligibility was rearticulated through rhetorics of motherhood, unjust body language, and questions about medical authority. we suggest this indicates that descriptions of the body and its able-ness carry more weight in the public's understanding of health issues than does medical authority.

THE GEOMETRY OF THE INFRARED AND X-RAY OBSCURER IN A DUSTY HYPERLUMINOUS QUASAR

Energy Technology Data Exchange (ETDEWEB)

Farrah, Duncan; Harris, Kathryn [Department of Physics, Virginia Tech, Blacksburg, VA 24061 (United States); Baloković, Mislav; Brightman, Murray [Cahill Center for Astronomy and Astrophysics, California Institute of Technology, Pasadena, CA 91125 (United States); Stern, Daniel; Walton, Dominic J. [Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA 91109 (United States); Kunimoto, Michelle; Clements, David L. [Astrophysics Group, Imperial College London, Blackett Laboratory, Prince Consort Road, London SW7 2AZ (United Kingdom); Alexander, David M. [Department of Physics, Durham University, Durham DH1 3LE (United Kingdom); Arévalo, Patricia [Instituto de Física y Astronomía, Facultad de Ciencias, Universidad de Valparaíso, Gran Bretana N 1111, Playa Ancha, Valparaíso (Chile); Ballantyne, David R. [Center for Relativistic Astrophysics, School of Physics, Georgia Institute of Technology, 837 State Street, Atlanta, GA 30332-0430 (United States); Bauer, Franz E. [Instituto de Astrofísica, Facultad de Física, Pontificia Universidad Católica de Chile, Casilla 306, Santiago 22 (Chile); Boggs, Steven [Space Science Laboratory, University of California, Berkeley, CA 94720 (United States); Brandt, William N. [Department of Astronomy and Astrophysics, 525 Davey Lab, The Pennsylvania State University, University Park, PA 16802 (United States); Christensen, Finn [DTU Space, National Space Institute, Technical University of Denmark, Elektrovej 327, DK-2800 Lyngby (Denmark); Craig, William [EMBIGGEN Anillo, Concepción (Chile); Fabian, Andrew, E-mail: farrah@vt.edu [Institute of Astronomy, Madingley Road, Cambridge, CB3 0HA (United Kingdom); and others

2016-11-01

We study the geometry of the active galactic nucleus (AGN) obscurer in IRAS 09104+4109, an IR-luminous, radio-intermediate FR-I source at z = 0.442, using infrared data from Spitzer and Herschel , X-ray data from NuSTAR , Swift , Suzaku , and Chandra , and an optical spectrum from Palomar. The infrared data imply a total rest-frame 1–1000 μ m luminosity of 5.5 × 10{sup 46} erg s{sup −1} and require both an AGN torus and a starburst model. The AGN torus has an anisotropy-corrected IR luminosity of 4.9 × 10{sup 46} erg s{sup −1} and a viewing angle and half-opening angle both of approximately 36° from pole-on. The starburst has a star formation rate of (110 ± 34) M {sub ⊙} yr{sup −1} and an age of <50 Myr. These results are consistent with two epochs of luminous activity in IRAS 09104+4109: one approximately 150 Myr ago, and one ongoing. The X-ray data suggest a photon index of Γ ≃ 1.8 and a line-of-sight column density of N {sub H} ≃ 5 × 10{sup 23} cm{sup −2}. This argues against a reflection-dominated hard X-ray spectrum, which would have implied a much higher N {sub H} and luminosity. The X-ray and infrared data are consistent with a bolometric AGN luminosity of L {sub bol} ∼ (0.5–2.5) × 10{sup 47} erg s{sup −1}. The X-ray and infrared data are further consistent with coaligned AGN obscurers in which the line of sight “skims” the torus. This is also consistent with the optical spectra, which show both coronal iron lines and broad lines in polarized but not direct light. Combining constraints from the X-ray, optical, and infrared data suggest that the AGN obscurer is within a vertical height of 20 pc, and a radius of 125 pc, of the nucleus.

The Geometry of the Infrared and X-Ray Obscurer in a Dusty Hyperluminous Quasar

Science.gov (United States)

Farrah, Duncan; Balokovic, Mislav; Stern, Daniel; Harris, Kathryn; Kunimoto, Michelle; Walton, Dominc J.; Alexander, David M.; Arevalo, Patricia; Ballantyne, David R.; Bauer, Franz E.;

The X-ray to [Ne V]3426 flux ratio: discovering heavily obscured AGN in the distant Universe

Science.gov (United States)

Gilli, R.; Vignali, C.; Mignoli, M.; Iwasawa, K.; Comastri, A.; Zamorani, G.

2010-09-01

We investigate the possibility of using the ratio between the 2-10 keV flux and the [Ne V]3426 emission line flux (X/NeV) as a diagnostic diagram to discover heavily obscured, possibly Compton-thick active galactic nuclei (AGN) in the distant Universe. While it is on average about one order of magnitude fainter than the more commonly used [O III]5007 emission line, the [Ne V]3426 line can be observed with optical spectroscopy up to z~1.5, whereas the [O III]5007 line is redshifted out of the optical bands already at z~0.8. First, we calibrated a relation between X/NeV and the cold absorbing column density NH using a sample of 74 bright, nearby Seyferts with both X-ray and [Ne V] data available in the literature and for which the column density is determined unambiguously. Similar to what is found for the X-ray to [O III]5007 flux ratio (X/OIII), we found that the X/NeV ratio decreases towards high column densities, as expected if [Ne V]3426 emission is a good tracer of the AGN intrinsic power. Essentially all local Seyferts with X/NeV values below 15 are found to be Compton-thick objects. At X/NeV values below 100, the percentage of Compton-thick nuclei decreases to ~50%, but ~80% of the considered sample is still absorbed with NH > 1023 cm-2. Second, we applied this diagnostic diagram to different samples of distant obscured and unobscured QSOs in the Sloan Digital Sky Survey (SDSS). SDSS blue, unobscured, type-1 QSOs in the redshift range z = [0.1-1.5] indeed show X/NeV values typical of unobscured Seyfert 1s in the local Universe. Conversely, SDSS type-2 QSOs at z~0.5 classified either as Compton-thick or Compton-thin on the basis of their X/OIII ratio, would have mostly been classified in the same way based on the X/NeV ratio. We applied the X/NeV diagnostic diagram to 9 SDSS obscured QSOs in the redshift range z = [0.85-1.31], selected by means of their prominent [Ne V]3426 line (rest EW > 4 Å) and observed with Chandra ACIS-S for 10ks each (8 of them as part

"Observation Obscurer" - Time Series Viewer, Editor and Processor

Science.gov (United States)

Andronov, I. L.

The program is described, which contains a set of subroutines suitable for East viewing and interactive filtering and processing of regularly and irregularly spaced time series. Being a 32-bit DOS application, it may be used as a default fast viewer/editor of time series in any compute shell ("commander") or in Windows. It allows to view the data in the "time" or "phase" mode, to remove ("obscure") or filter outstanding bad points; to make scale transformations and smoothing using few methods (e.g. mean with phase binning, determination of the statistically opti- mal number of phase bins; "running parabola" (Andronov, 1997, As. Ap. Suppl, 125, 207) fit and to make time series analysis using some methods, e.g. correlation, autocorrelation and histogram analysis: determination of extrema etc. Some features have been developed specially for variable star observers, e.g. the barycentric correction, the creation and fast analysis of "OC" diagrams etc. The manual for "hot keys" is presented. The computer code was compiled with a 32-bit Free Pascal (www.freepascal.org).

HOT DUST OBSCURED GALAXIES WITH EXCESS BLUE LIGHT: DUAL AGN OR SINGLE AGN UNDER EXTREME CONDITIONS?

Energy Technology Data Exchange (ETDEWEB)

Assef, R. J.; Diaz-Santos, T. [Núcleo de Astronomía de la Facultad de Ingeniería, Universidad Diego Portales, Av. Ejército Libertador 441, Santiago (Chile); Walton, D. J.; Brightman, M. [Space Radiation Laboratory, California Institute of Technology, Pasadena, CA 91125 (United States); Stern, D.; Eisenhardt, P. R. M.; Tsai, C.-W. [Jet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Drive, Mail Stop 169-236, Pasadena, CA 91109 (United States); Alexander, D. [Department of Physics, Durham University, Durham DH1 3LE (United Kingdom); Bauer, F. [Departamento de Astronomía y Astrofísica, Pontificia Universidad Católica de Chile, Casilla 306, Santiago 22 (Chile); Blain, A. W. [Physics and Astronomy, University of Leicester, 1 University Road, Leicester LE1 7RH (United Kingdom); Finkelstein, S. L. [The University of Texas at Austin, 2515 Speedway, Stop C1400, Austin, TX 78712 (United States); Hickox, R. C. [Department of Physics and Astronomy, Dartmouth College, 6127 Wilder Laboratory, Hanover, NH 03755 (United States); Wu, J. W., E-mail: roberto.assef@mail.udp.cl [UCLA Astronomy, P.O. Box 951547, Los Angeles, CA 90095-1547 (United States)

2016-03-10

Hot dust-obscured galaxies (Hot DOGs) are a population of hyper-luminous infrared galaxies identified by the Wide-field Infrared Survey Explorer (WISE) mission from their very red mid-IR colors, and characterized by hot dust temperatures (T > 60 K). Several studies have shown clear evidence that the IR emission in these objects is powered by a highly dust-obscured active galactic nucleus (AGN) that shows close to Compton-thick absorption at X-ray wavelengths. Thanks to the high AGN obscuration, the host galaxy is easily observable, and has UV/optical colors usually consistent with those of a normal galaxy. Here we discuss a sub-population of eight Hot DOGs that show enhanced rest-frame UV/optical emission. We discuss three scenarios that might explain the excess UV emission: (i) unobscured light leaked from the AGN by reflection over the dust or by partial coverage of the accretion disk; (ii) a second unobscured AGN in the system; or (iii) a luminous young starburst. X-ray observations can help discriminate between these scenarios. We study in detail the blue excess Hot DOG WISE J020446.13–050640.8, which was serendipitously observed by Chandra/ACIS-I for 174.5 ks. The X-ray spectrum is consistent with a single, hyper-luminous, highly absorbed AGN, and is strongly inconsistent with the presence of a secondary unobscured AGN. Based on this, we argue that the excess blue emission in this object is most likely either due to reflection or a co-eval starburst. We favor the reflection scenario as the unobscured star formation rate needed to power the UV/optical emission would be ≳1000 M{sub ⊙} yr{sup −1}. Deep polarimetry observations could confirm the reflection hypothesis.

HOT DUST OBSCURED GALAXIES WITH EXCESS BLUE LIGHT: DUAL AGN OR SINGLE AGN UNDER EXTREME CONDITIONS?

International Nuclear Information System (INIS)

Assef, R. J.; Diaz-Santos, T.; Walton, D. J.; Brightman, M.; Stern, D.; Eisenhardt, P. R. M.; Tsai, C.-W.; Alexander, D.; Bauer, F.; Blain, A. W.; Finkelstein, S. L.; Hickox, R. C.; Wu, J. W.

2016-01-01

Hot dust-obscured galaxies (Hot DOGs) are a population of hyper-luminous infrared galaxies identified by the Wide-field Infrared Survey Explorer (WISE) mission from their very red mid-IR colors, and characterized by hot dust temperatures (T > 60 K). Several studies have shown clear evidence that the IR emission in these objects is powered by a highly dust-obscured active galactic nucleus (AGN) that shows close to Compton-thick absorption at X-ray wavelengths. Thanks to the high AGN obscuration, the host galaxy is easily observable, and has UV/optical colors usually consistent with those of a normal galaxy. Here we discuss a sub-population of eight Hot DOGs that show enhanced rest-frame UV/optical emission. We discuss three scenarios that might explain the excess UV emission: (i) unobscured light leaked from the AGN by reflection over the dust or by partial coverage of the accretion disk; (ii) a second unobscured AGN in the system; or (iii) a luminous young starburst. X-ray observations can help discriminate between these scenarios. We study in detail the blue excess Hot DOG WISE J020446.13–050640.8, which was serendipitously observed by Chandra/ACIS-I for 174.5 ks. The X-ray spectrum is consistent with a single, hyper-luminous, highly absorbed AGN, and is strongly inconsistent with the presence of a secondary unobscured AGN. Based on this, we argue that the excess blue emission in this object is most likely either due to reflection or a co-eval starburst. We favor the reflection scenario as the unobscured star formation rate needed to power the UV/optical emission would be ≳1000 M ⊙ yr −1 . Deep polarimetry observations could confirm the reflection hypothesis

The nature of the torus in the heavily obscured AGN Markarian 3: an X-ray study

DEFF Research Database (Denmark)

Guainazzi, M.; Risaliti, G.; Awaki, H.

2016-01-01

In this paper, we report the results of an X-ray monitoring campaign on the heavily obscured Seyfert galaxy, Markarian 3, carried out between the fall of 2014 and the spring of 2015 with NuSTAR, Suzaku and XMM–Newton. The hard X-ray spectrum of Markarian 3 is variable on all the time-scales probe...

Selective CT mesentericography in the diagnostics of obscure overt intestinal bleeding: preliminary results

International Nuclear Information System (INIS)

Schuermann, K.; Buecker, A.; Tacke, J.; Schmitz-Rode, T.; Guenther, R.W.; Jansen, M.

2002-01-01

Aim: To evaluate intra-arterial CT mesentericography (CTM) in the diagnostics of severe obscure overt intestinal bleeding in comparison with conventional mesentericography (MG) and surgery. Methods: In 8 patients (23 - 82 years, mean 59 years), CTM was performed via the catheter left in the superior mesenteric artery after MG to detect the source of bleeding. Early and late-phase spiral CT scans were acquired after administration of contrast medium. Active bleeding was considered to be present if extravasation of contrast medium into the bowel was found. The results of MG and CTM were compared with the results of surgery. Results: With MG active bleeding was found in one patient, with CTM in five patients. In three patients, both MG and CTM were negative. Six patients underwent surgery. Five cases of bleeding detected with CTM were confirmed by surgery. In one case, bleeding found with CTM was not confirmed by surgery. One patient underwent surgery although all imaging procedures were negative. The source of bleeding remained unknown. Surgically, the site of bleeding was located in the jejunum in 3 patients (jejunitis, jejunal ulcers, carcinoid), one patient had a diverticulum in the ascending colon. The colonic bleeding site was correctly localized with CTM, whereas the small bowel bleeding could only roughly be assigned to the proximal or distal jejunum or jejunoileal transition area. Conclusion: Preliminary results indicate that selective CTM is superior to MG in the evaluation of severe obscure overt intestinal bleeding. (orig.) [de

Learning From Nature: Biomimetic Polarimetry for Imaging in Obscuring Environments

Energy Technology Data Exchange (ETDEWEB)

VanderLaan, John [Sandia National Lab. (SNL-NM), Albuquerque, NM (United States); Scrymgeour, David [Sandia National Lab. (SNL-NM), Albuquerque, NM (United States); Kemme, Shanalyn A. [Sandia National Lab. (SNL-NM), Albuquerque, NM (United States)

2014-09-01

We find for infrared wavelengths there are broad ranges of particle sizes and refractive indices that represent fog and rain where the use of circular polarization can persist to longer ranges than linear polarization. Using polarization tracking Monte Carlo simulations for varying particle size, wavelength, and refractive index systematically, we show that for specific scene parameters circular polarization outperforms linear polarization in maintaining the intended polarization state for large optical depths. This enhancement in circular polarization can be exploited to improve range and target detection in obscurant environments that are important in many critical sensing applications. Specifically, circular polarization persists better than linear for radiation fog in the short-wave infrared, for advection fog in the short-wave infrared and the long-wave infrared, and large particle sizes of Sahara dust around the 4 micron wavelength.

Obscured AGN at z ~ 1 from the zCOSMOS-Bright Survey. I. Selection and optical properties of a [Ne v]-selected sample

Science.gov (United States)

Mignoli, M.; Vignali, C.; Gilli, R.; Comastri, A.; Zamorani, G.; Bolzonella, M.; Bongiorno, A.; Lamareille, F.; Nair, P.; Pozzetti, L.; Lilly, S. J.; Carollo, C. M.; Contini, T.; Kneib, J.-P.; Le Fèvre, O.; Mainieri, V.; Renzini, A.; Scodeggio, M.; Bardelli, S.; Caputi, K.; Cucciati, O.; de la Torre, S.; de Ravel, L.; Franzetti, P.; Garilli, B.; Iovino, A.; Kampczyk, P.; Knobel, C.; Kovač, K.; Le Borgne, J.-F.; Le Brun, V.; Maier, C.; Pellò, R.; Peng, Y.; Perez Montero, E.; Presotto, V.; Silverman, J. D.; Tanaka, M.; Tasca, L.; Tresse, L.; Vergani, D.; Zucca, E.; Bordoloi, R.; Cappi, A.; Cimatti, A.; Koekemoer, A. M.; McCracken, H. J.; Moresco, M.; Welikala, N.

2013-08-01

Aims: The application of multi-wavelength selection techniques is essential for obtaining a complete and unbiased census of active galactic nuclei (AGN). We present here a method for selecting z ~ 1 obscured AGN from optical spectroscopic surveys. Methods: A sample of 94 narrow-line AGN with 0.65 advantage of the large amount of data available in the COSMOS field, the properties of the [Ne v]-selected type 2 AGN were investigated, focusing on their host galaxies, X-ray emission, and optical line-flux ratios. Finally, a previously developed diagnostic, based on the X-ray-to-[Ne v] luminosity ratio, was exploited to search for the more heavily obscured AGN. Results: We found that [Ne v]-selected narrow-line AGN have Seyfert 2-like optical spectra, although their emission line ratios are diluted by a star-forming component. The ACS morphologies and stellar component in the optical spectra indicate a preference for our type 2 AGN to be hosted in early-type spirals with stellar masses greater than 109.5 - 10 M⊙, on average higher than those of the galaxy parent sample. The fraction of galaxies hosting [Ne v]-selected obscured AGN increases with the stellar mass, reaching a maximum of about 3% at ≈2 × 1011 M⊙. A comparison with other selection techniques at z ~ 1, namely the line-ratio diagnostics and X-ray detections, shows that the detection of the [Ne v] λ3426 line is an effective method for selecting AGN in the optical band, in particular the most heavily obscured ones, but cannot provide a complete census of type 2 AGN by itself. Finally, the high fraction of [Ne v]-selected type 2 AGN not detected in medium-deep (≈100-200 ks) Chandra observations (67%) is suggestive of the inclusion of Compton-thick (i.e., with NH > 1024 cm-2) sources in our sample. The presence of a population of heavily obscured AGN is corroborated by the X-ray-to-[Ne v] ratio; we estimated, by means of an X-ray stacking technique and simulations, that the Compton-thick fraction in our

SPITZER ANALYSIS OF H II REGION COMPLEXES IN THE MAGELLANIC CLOUDS: DETERMINING A SUITABLE MONOCHROMATIC OBSCURED STAR FORMATION INDICATOR

International Nuclear Information System (INIS)

Lawton, B.; Gordon, K. D.; Meixner, M.; Sewilo, M.; Shiao, B.; Babler, B.; Bracker, S.; Meade, M.; Block, M.; Engelbracht, C. W.; Misselt, K.; Bolatto, A. D.; Carlson, L. R.; Hora, J. L.; Robitaille, T.; Indebetouw, R.; Madden, S. C.; Oey, M. S.; Oliveira, J. M.; Vijh, U. P.

2010-01-01

H II regions are the birth places of stars, and as such they provide the best measure of current star formation rates (SFRs) in galaxies. The close proximity of the Magellanic Clouds allows us to probe the nature of these star forming regions at small spatial scales. To study the H II regions, we compute the bolometric infrared flux, or total infrared (TIR), by integrating the flux from 8 to 500 μm. The TIR provides a measure of the obscured star formation because the UV photons from hot young stars are absorbed by dust and re-emitted across the mid-to-far-infrared (IR) spectrum. We aim to determine the monochromatic IR band that most accurately traces the TIR and produces an accurate obscured SFR over large spatial scales. We present the spatial analysis, via aperture/annulus photometry, of 16 Large Magellanic Cloud (LMC) and 16 Small Magellanic Cloud (SMC) H II region complexes using the Spitzer Space Telescope's IRAC (3.6, 4.5, 8 μm) and MIPS (24, 70, 160 μm) bands. Ultraviolet rocket data (1500 and 1900 A) and SHASSA Hα data are also included. All data are convolved to the MIPS 160 μm resolution (40 arcsec full width at half-maximum), and apertures have a minimum radius of 35''. The IRAC, MIPS, UV, and Hα spatial analysis are compared with the spatial analysis of the TIR. We find that nearly all of the LMC and SMC H II region spectral energy distributions (SEDs) peak around 70 μm at all radii, from ∼10 to ∼400 pc from the central ionizing sources. As a result, we find the following: the sizes of H II regions as probed by 70 μm are approximately equal to the sizes as probed by TIR (∼70 pc in radius); the radial profile of the 70 μm flux, normalized by TIR, is constant at all radii (70 μm ∼ 0.45TIR); the 1σ standard deviation of the 70 μm fluxes, normalized by TIR, is a lower fraction of the mean (0.05-0.12 out to ∼220 pc) than the normalized 8, 24, and 160 μm normalized fluxes (0.12-0.52); and these results are the same for the LMC and the

Identification of creat (Andrographis paniculata Ness as basic for concervation and make use of germ plasm

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BAMBANG PUJIASMANTO

2007-07-01

Full Text Available This research is to learn the creat potention for cultivated as medical material producer plant. So that, the limited creat as medical material not occur. The method of research which used is survey. The survai include identification and creat distribution pattern. There was used vegetative analysis with quadrat method. The research result showed that 1 in creat habitat find out 11 species of tree, 20 species herba (include creat, and 16 species grasses, 2 The highest of importance value indeks Tectona grandis L. (tree group, Andrographis paniculata Ness (herb group, and Portulaca oleraceae L. (grasses group, 3 Distribution pattern of creat is clumped, and the herb others is uniform, 4 The creat growth on the common under shading Tectona grandis L. tree. The results of this research are domestication concept and theories which to basic the cultivated technology packet of creat wild plant which the statue increased be medical material produce crop. In the next ,expected can used for get conclusion policy of medical crop and planning, especially on creat propertion of creat medical material.

The Ideological Questions of Marriage in Thomas Hardy’s Jude the Obscure

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Salman Saleh, N.

2015-01-01

Full Text Available As one of the prominent ideologies of the nineteenth-century— in a complex interrelation with other contemporary ideological discourses particularly femininity and marriage—religion adopts a critical stance in Hardy’s presentation of characters. Breaching the religio-conventional image of femininity as “Angel in the House” and “Cow Woman,” Hardy’s Jude the Obscure (1895 is indeed deemed to be his milestone in presenting his anti-Christian attitudes towards the contemporary religion. This study aims to present Hardy’s outright hostility towards the nineteenth-century Christianity through his creation of non-conformist characters, necessitating a parallel study with other contemporary discourses regarding marriage and femininity, and conflict with the religion of the time. Hardy’s magnum opus, the work on which he was to stake his final reputation as a novelist, was clearly Jude the Obscure which as a noticeable socio-religious experimentation of the late nineteenth-century, reveals Hardy’s perception of new ideas about femininity and marriage by presenting the hot contemporary issues of “New Woman” and “Free Union” through the development and presentation of Sue Bridehead and her free union with Jude, respectively. Hardy’s presentation of Sue Bridehead as a “New Woman,” and employing the “Free Union” in marked contrast with the nineteenth-century convention of marriage as a “Bonded Pair” is Hardy’s closing upshot of his final novelistic attempt. The non-conformist Jude and Sue are presented as figures touching the Victorian Christian standards of morality, while, the final tragic destiny of Jude and Sue’s helplessness attest to the writer’s substantial contribution as a Victorian male novelist to the ideologies circulating at the time.

Tracking the Obscured Star Formation Along the Complete Evolutionary Merger Sequence of LIRGs

Science.gov (United States)

Diaz-Santos, Tanio

2014-10-01

We propose to obtain WFC3 narrow-band Pa-beta imaging of a sample of 24 nearby luminous infrared (IR) galaxies (LIRGs) from the Great Observatories All-sky LIRG survey (GOALS) selected to be in advanced stages of interaction. LIRGs account for half of the obscured star formation of the Universe at z ~ 1-2, and they represent a key population in galaxy formation and evolution. We will use the Pa-beta images to trace the ionized gas in LIRGs and study its spatial distribution from scales of ~ 100 pc to up to several kpc, probing the youngest, massive stars formed in the most buried environments of LIRGs due to the interaction process. This will allow us to measure how the gas in the center of mergers is converted into stars, which eventually leads to the build-up of a nuclear stellar cusp and the "inside-out" growth of bulges. We will also create spatially-resolved Pa-beta equivalent width maps to search for age gradients across the galaxies and correlate the distribution of Pa-beta emission with that of un-obscured star clusters detected in the UV and optical with HST on the same spatial scales. Finally, we will combine our data with previous studies mainly focused on isolated and early-stage interacting LIRG systems to analyze the size and compactness of the starburst along the complete merger sequence of LIRGs. The requested data represent a critical missing piece of information that will allow us to understand both the physics of merger-induced star formation and the applicability of local LIRGs as templates for high-z interacting starburst galaxies.

Active Galactic Nucleus Obscuration from Winds: From Dusty Infrared-Driven to Warm and X-Ray Photoionized

Science.gov (United States)

Dorodnitsyn, Anton V.; Kallman, Timothy R.

2012-01-01

We present calculations of active galactic nucleus winds at approx.parsec scales along with the associated obscuration. We take into account the pressure of infrared radiation on dust grains and the interaction of X-rays from a central black hole with hot and cold plasma. Infrared radiation (IR) is incorporated in radiation-hydrodynamic simulations adopting the flux-limited diffusion approximation. We find that in the range of X-ray luminosities L = 0.05-0.6 L(sub Edd), the Compton-thick part of the flow (aka torus) has an opening angle of approximately 72deg - 75deg regardless of the luminosity. At L > or approx. 0.1, the outflowing dusty wind provides the obscuration with IR pressure playing a major role. The global flow consists of two phases: the cold flow at inclinations (theta) > or approx.70deg and a hot, ionized wind of lower density at lower inclinations. The dynamical pressure of the hot wind is important in shaping the denser IR-supported flow. At luminosities < or = 0.1 L(sub Edd) episodes of outflow are followed by extended periods when the wind switches to slow accretion. Key words: acceleration of particles . galaxies: active . hydrodynamics . methods: numerical Online-only material: color figures

The Far-Infrared Luminosity Function and Star Formation Rate Density for Dust Obscured Galaxies in the Bootes Field

Science.gov (United States)

Calanog, Jae Alyson; Wardlow, J. L.; Fu, H.; Cooray, A. R.; HerMES

2013-01-01

We present the far-Infrared (FIR) luminosity function (LF) and the star-formation rate density (SFRD) for dust-obscured galaxies (DOGs) in the Bootes field at redshift 2. These galaxies are selected by having a large rest frame mid-IR to UV flux density ratio ( > 1000) and are expected to be some of the most luminous and heavily obscured galaxies in the Universe at this epoch. Photometric redshifts for DOGs are estimated from optical and mid-IR data using empirically derived low resolution spectral templates for AGN and galaxies. We use HerMES Herschel-SPIRE data to fit a modified blackbody to calculate the FIR luminosity (LFIR) and dust temperature (Td) for all DOGs individually detected in SPIRE maps. A stacking analyses was implemented to measure a median sub-mm flux of undetected DOGs. We find that DOGs have LIR and Td that are similar with the sub-millimeter galaxy (SMG) population, suggesting these two populations are related. The DOG LF and SFRD at 2 are calculated and compared to SMGs.

Star formation at high redshift and the importance of dust obscuration

DEFF Research Database (Denmark)

Michalowski, Michal

One of the aspects of the understanding of the Universe evolution is its star formation history. In order to gain a complete picture of the Universe evolution it is important to know when the stars we see today were formed. One of the method to study this problem is to use far-infrared and radio...... emission of galaxies. In this way it is possible to investigate the sites of star formation that are totally obscured by dust and therefore invisible at the optical wavelengths. It is because the energy absorbed by dust in the optical is re-emitted in the infrared, whereas radio emission is unaffected...... and/or radio, namely their enhanced submillimeter / radio emission combined with optical faintness and blue colors. I find that these four galaxies are young, highly star-forming, low-mass and dusty....

Doing business:an obscure notion of the ethics of public associations in ordinary Chinese

Institute of Scientific and Technical Information of China (English)

Liao Shenbai

2006-01-01

Along with the notion of being a person(zuo ren 做人), the notion of doing business(zuo shi 做事)in ordinary Chinese is basically an over-all notion of the norms in the practical and associative activities,carrying typically obscure meanings on practice and association affairs in some external world.Ordinary Chinese not only distinguishes these two notions but also defines a dictionary order of them，with the affairs of the internal world prior to those of the external.The fact that the notion of doing business refers to business(shi 事)rather than person(ren 人)makes this order clear at a deeper level.It shows that this notion regards the practical affairs of the external world less important to the person itself than those of the internal.Except for these qualities,the notion of doing business holds some normative meanings,although contains no definite rules.These meanings indirectly relate to the notion of person that people form in their private associations and emerge as some mixture with a tactical attitude out of the need of earning a life.The notion of person gives birth to some obscure requirements,for instance, the requirement of 'doing business in accordance with your conscience' and that of 'doing business seriously'.The core world of family is marginalized in the pubfic transition of associations.There are reasons to anticipate that in this process the notion of doing business will undergo more radical changes than that of being a person.

Health tourism: definition focused on the Swiss market and conceptualisation of health(i)ness.

Science.gov (United States)

Hofer, Susanne; Honegger, Franziska; Hubeli, Jonas

2012-01-01

This paper's purpose is to give an overview of current research regarding the concept of "health tourism" with a focus on Switzerland, and to determine whether a consensus on this concept and its embedding in existing/future markets can be found. The paper is an explorative study combining literature review, questionnaires and qualitative interviews. Grounded theory was employed. A service from the field of health care must have been provided prior to health tourism, allowing it to be classified under the health care system. Thus, health tourism is classified under the market for the sick and not under tourism which targets the healthy. Furthermore a new market for the healthy is emerging, which needs to be defined. As an example health(i)ness could help to clarify the terminology, to be seen as a gatekeeper of health and as a cultural paradigm change from cure to prevention. Further research is needed, regarding the positioning and development of health tourism and its synergies, as the cost pressures in health care increase and will continue to have a sustainable impact on health tourism. The paper provides better knowledge of the term health tourism, its general classification, and particular reference to Switzerland, and information about upcoming changes in health care. The findings add to the knowledge of how health tourism is embedded into health care and tourism, and show potential within the market for the healthy. It provides information to members of the tourism and health care market.

Characterization of odor-active compounds in cooked meat of farmed obscure puffer (Takifugu obscurus using gas chromatography–mass spectrometry–olfactometry

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Ning-Ping Tao

2014-12-01

Full Text Available The volatile and odor-active compounds in cooked meat of farmed obscure puffer (Takifugu obscurus were analyzed by gas chromatography–mass spectrometry–olfactometry (GC–MS–O. The volatile compounds were extracted by the simultaneous distillation–extraction (SDE method, then separated and identified by GC–MS. Odor-active compounds in the SDE extract were characterized by GC–MS–O. A total of 68 volatile compounds were found, including 23 aldehydes, 10 alcohols, nine ketones, 17 N- or S-containing compounds and aromatics, three acids, three alkanes, and three esters. Of these, 31 odor-active compounds were detected and identified. Trimethylamine (fishy, octanal (grassy, leafy, green, (E-2-octenal (roast, fatty, 1-octen-3-ol (fishy, fatty, mushroom, grassy, 2-ethyl-1-hexanethiol (cooked fish, (E,E-2,4-octadienal (cooked meat, sweet, 2-acetylthiazole (meaty, roast, nutty, sulfur, 2-acetylpyrrole (nutty, walnut, bread were identified as the key odorants in the cooked meat of farmed obscure puffer based on posterior intensity and time-intensity methods.

Parsec-scale Obscuring Accretion Disk with Large-scale Magnetic Field in AGNs

Energy Technology Data Exchange (ETDEWEB)

Dorodnitsyn, A.; Kallman, T. [Laboratory for High Energy Astrophysics, NASA Goddard Space Flight Center, Code 662, Greenbelt, MD, 20771 (United States)

2017-06-10

A magnetic field dragged from the galactic disk, along with inflowing gas, can provide vertical support to the geometrically and optically thick pc-scale torus in AGNs. Using the Soloviev solution initially developed for Tokamaks, we derive an analytical model for a rotating torus that is supported and confined by a magnetic field. We further perform three-dimensional magneto-hydrodynamic simulations of X-ray irradiated, pc-scale, magnetized tori. We follow the time evolution and compare models that adopt initial conditions derived from our analytic model with simulations in which the initial magnetic flux is entirely contained within the gas torus. Numerical simulations demonstrate that the initial conditions based on the analytic solution produce a longer-lived torus that produces obscuration that is generally consistent with observed constraints.

Small bowel enteroscopy and intraoperative enteroscopy for obscure gastrointestinal bleeding.

Science.gov (United States)

Lewis, B S; Wenger, J S; Waye, J D

1991-02-01

Intraoperative endoscopy (IOE) is accepted as the ultimate diagnostic procedure for completely evaluating the small bowel in patients with obscure gastrointestinal (GI) bleeding. Small bowel enteroscopy (SBE) has been reported useful in the nonsurgical evaluation of the small intestine in these patients, but findings may be limited because of incomplete small bowel intubation and a lack of tip deflection. Twenty-three patients underwent 25 SBE exams and subsequently had 25 IOE exams during surgical exploration for continued bleeding. Patients' bleeding histories averaged 2 yr, with an average transfusion requirement of 27 units. Findings on IOE were the same as with SBE in 17/22 (77%) of examinations. We conclude that SBE and IOE are comparable in depth of insertion and ability to detect small vascular ectasias. Both procedures missed pathology due to limited visibility and the evanescent nature of ectasias. Long-term success in abolishing bleeding with these combined techniques can be expected in 55% of these patients. SBE should precede surgery, since the finding of diffuse ectasias precludes any benefit from operative intervention.

Diagnostic role of capsule endoscopy in patients of obscure gastrointestinal bleeding after negative CT enterography

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Jaswinder Singh Sodhi

2013-01-01

Full Text Available Background and Objectives: Computed tomographic enterography (CT-EG has emerged a useful tool for the evaluation of small bowel in patients of obscure gastrointestinal bleeding (OGIB. However, CT-EG may be negative in about 50-60% of patients. We aimed to see the efficacy of capsule endoscopy (CE in patients of OGIB, who had initial negative CT-EG. Materials and Methods: All consecutive patients of OGIB after initial hemodynamic stabilization were subjected to CT-EG. Those having negative CT-EG were further evaluated with CE. Results: Fifty-five patients of OGIB with mean standard deviation age, 52.7 (19.0, range 18-75 years, women 31/55 (56.4% were subjected to CT-EG. Nine (17.6% patients had positive findings on CT-EG, which included mass lesions in six, thickened wall of distal ileal loops, narrowing, and wall enhancement in two and jejunal wall thickening with wall hyperenhancement in one patient. Forty-two patients had negative CT-EG of which 25 underwent CE for further evaluation. CE detected positive findings in 11 of 25 (48% patients which included vascular malformations in three, ulcers in seven, and fresh blood without identifiable source in one. The diagnostic yield of CE in overt OGIB was more compared to occult OGIB ((7/14, 50% vs (4/11, 36.4% P = 0.2 and was higher if performed within 2 weeks of active gastrointestinal (GI bleed (P = 0.08. Conclusions: In conclusion, CE is an additional tool in the evaluation of obscure GI bleed, especially mucosal lesions which can be missed by CT-EG.

Manifest and Subtle Cyclic Behavior in Nonequilibrium Steady States

International Nuclear Information System (INIS)

Zia, R K P; Weiss, Jeffrey B; Mandal, Dibyendu; Fox-Kemper, Baylor

2016-01-01

Many interesting phenomena in nature are described by stochastic processes with irreversible dynamics. To model these phenomena, we focus on a master equation or a Fokker-Planck equation with rates which violate detailed balance. When the system settles in a stationary state, it will be a nonequilibrium steady state (NESS), with time independent probability distribution as well as persistent probability current loops. The observable consequences of the latter are explored. In particular, cyclic behavior of some form must be present: some are prominent and manifest, while others are more obscure and subtle. We present a theoretical framework to analyze such properties, introducing the notion of “probability angular momentum” and its distribution. Using several examples, we illustrate the manifest and subtle categories and how best to distinguish between them. These techniques can be applied to reveal the NESS nature of a wide range of systems in a large variety of areas. We illustrate with one application: variability of ocean heat content in our climate system. (paper)

Network 'small-world-ness': a quantitative method for determining canonical network equivalence.

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Mark D Humphries

Full Text Available BACKGROUND: Many technological, biological, social, and information networks fall into the broad class of 'small-world' networks: they have tightly interconnected clusters of nodes, and a shortest mean path length that is similar to a matched random graph (same number of nodes and edges. This semi-quantitative definition leads to a categorical distinction ('small/not-small' rather than a quantitative, continuous grading of networks, and can lead to uncertainty about a network's small-world status. Moreover, systems described by small-world networks are often studied using an equivalent canonical network model--the Watts-Strogatz (WS model. However, the process of establishing an equivalent WS model is imprecise and there is a pressing need to discover ways in which this equivalence may be quantified. METHODOLOGY/PRINCIPAL FINDINGS: We defined a precise measure of 'small-world-ness' S based on the trade off between high local clustering and short path length. A network is now deemed a 'small-world' if S>1--an assertion which may be tested statistically. We then examined the behavior of S on a large data-set of real-world systems. We found that all these systems were linked by a linear relationship between their S values and the network size n. Moreover, we show a method for assigning a unique Watts-Strogatz (WS model to any real-world network, and show analytically that the WS models associated with our sample of networks also show linearity between S and n. Linearity between S and n is not, however, inevitable, and neither is S maximal for an arbitrary network of given size. Linearity may, however, be explained by a common limiting growth process. CONCLUSIONS/SIGNIFICANCE: We have shown how the notion of a small-world network may be quantified. Several key properties of the metric are described and the use of WS canonical models is placed on a more secure footing.

The nature of the torus in the heavily obscured AGN Markarian 3: an X-ray study

OpenAIRE

Guainazzi, M.; Risaliti, G.; Awaki, H.; Arevalo, P.; Bauer, F. E.; Bianchi, S.; Boggs, S. E.; Brandt, W. N.; Brightman, M.; Christensen, Finn Erland; Craig, W. W.; Forster, K.; Hailey, C. J.; Harrison, F.; Koss, M.

2016-01-01

In this paper, we report the results of an X-ray monitoring campaign on the heavily obscured Seyfert galaxy, Markarian 3, carried out between the fall of 2014 and the spring of 2015 with NuSTAR, Suzaku and XMM–Newton. The hard X-ray spectrum of Markarian 3 is variable on all the time-scales probed by our campaign, down to a few days. The observed continuum variability is due to an intrinsically variable primary continuum seen in transmission through a large, but still Compton-thin column dens...

The COSPIX Mission: Focusing on the Energetic and Obscured Universe

Science.gov (United States)

Ferrando, P.; Goldwurm, A.; Laurent, P.; Limousin, O.; Beckmann, V; Arnaud, M.; Barcons, X.; Bomans, D.; Caballero, I.; Carrera, F.;

A 5ª subseção da ordem dos advogados do Brasil e a garantia da cidadania e democracia nesses 200 anos de fundação de Araraquara

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Tiago Romano

2017-11-01

Full Text Available É inconcebível garantir um estado democrático de direito e uma sociedade civil justa e fraterna sem órgãos que defendam as leis e normas vigentes. A Ordem dos Advogados do Brasil, sendo um ente federal contribui para o pleno exercício da cidadania e democracia no Brasil, compreendendo os Estados, Distrito Federal e Municípios. A 5ª Subseção nesse ano completa 85 anos de fundação e contribui para o crescimento e desenvolvimento da cidade de Araraquara que nesse mesmo ano completa 200 anos de fundação, exercendo sua função social na sociedade araraquarense. A OAB não é apenas uma instituição de classe e sim uma instituição que tem uma responsabilidade social muito grande, prevista pela própria Constituição Federal. A 5ª Subseção da Ordem dos Advogados do Brasil sediada em Araraquara conta com uma estrutura completa que visa atender aos advogados, advogadas, estagiários e estagiárias, bem como a população, os órgãos públicos, entidades etc.

Evaluate and characterize mechanisms controlling transport, fate and effects of army smokes in an aerosol wind tunnel: Transport, transformations, fate and terrestrial ecological effects of fog oil obscurant smokes: Final report

Energy Technology Data Exchange (ETDEWEB)

Cataldo, D.A.; Van Voris, P.; Ligotke, M.W.; Fellows, R.J.; McVeety, B.D.; Li, Shu-mei W.; Bolton, H. Jr.; Fredrickson, J.K.

1989-01-01

The terrestrial transport, chemical fate, and ecological effects of fog oil (FO) smoke obscurants were evaluated under controlled wind tunnel conditions. The primary objectives of this research program are to characterize and assess the impacts of smoke and obscurants on: (1) natural vegetation characteristic of US Army training sites in the United States; (2) physical and chemical properties of soils representative of these training sites; and (3) soil microbiological and invertebrate communities. Impacts and dose/responses were evaluated based on an exposure scenario, including exposure duration, exposure rate, and sequential cumulative dosing. Key to understanding the environmental impacts of fog oil smoke/obscurants is establishing the importance of environmental parameters, such as relative humidity and wind speed on airborne aerosol characteristics and deposition to receptor surfaces. Direct and indirect biotic effects were evaluated using five plant species and three soil types. 29 refs., 35 figs., 32 tabs.

Optical colours of AGN in the Extended Chandra Deep Field South: Obscured black holes in early type galaxies

OpenAIRE

Rovilos, E.; Georgantopoulos, I.

2007-01-01

We investigate the optical colours of X-ray sources from the Extended Chandra Deep Field South (ECDFS) using photometry from the COMBO-17 survey, aiming to explore AGN - galaxy feedback models. The X-ray sources populate both the ``blue'' and the ``red sequence'' on the colour-magnitude diagram. However, sources in the ``red sequence'' appear systematically more obscured. HST imaging from the GEMS survey demonstrates that the nucleus does not affect significantly the observed colours, and the...

NuSTAR J033202-2746.8: direct constraints on the Compton reflection in a heavily obscured quasar at z ≈ 2

DEFF Research Database (Denmark)

Del Moro, A.; Mullaney, J. R.; Alexander, D. M.

2014-01-01

We report Nuclear Spectroscopic Telescope Array (NuSTAR) observations of NuSTAR J033202-2746.8, a heavily obscured, radio-loud quasar detected in the Extended Chandra Deep Field-South, the deepest layer of the NuSTAR extragalactic survey (∼400 ks, at its deepest). NuSTAR J033202-2746.8 is reliably......-2746.8, indicating that this source is a heavily obscured quasar (NH = 5.6+−0.80.9 × 1023 cm−2) with luminosity L10-40 keV ≈ 6.4 × 1044 erg s−1. Although existing optical and near-infrared (near-IR) data, as well as follow-up spectroscopy with the Keck and VLT telescopes, failed to provide a secure redshift......-Newton data alone. The measured reflection fraction is higher than the R∼0 typically observed in bright radio-loud quasars such as NuSTAR J033202-2746.8, which has L1.4 GHz≈1027 W Hz−1. Constraining the spectral shape of active galactic nuclei (AGNs), including bright quasars, is very important...

Obscure phenomena in statistical analysis of quantitative structure-activity relationships. Part 1: Multicollinearity of physicochemical descriptors.

Science.gov (United States)

Mager, P P; Rothe, H

1990-10-01

Multicollinearity of physicochemical descriptors leads to serious consequences in quantitative structure-activity relationship (QSAR) analysis, such as incorrect estimators and test statistics of regression coefficients of the ordinary least-squares (OLS) model applied usually to QSARs. Beside the diagnosis of the known simple collinearity, principal component regression analysis (PCRA) also allows the diagnosis of various types of multicollinearity. Only if the absolute values of PCRA estimators are order statistics that decrease monotonically, the effects of multicollinearity can be circumvented. Otherwise, obscure phenomena may be observed, such as good data recognition but low predictive model power of a QSAR model.

Calcium Chloride and Calcium Gluconate in Neonatal Parenteral Nutrition Solutions without Cysteine: Compatibility Studies Using Laser Light Obscuration Methodology

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Robert K. Huston

2018-02-01

Full Text Available There are no compatibility studies for neonatal parenteral nutrition solutions without cysteine containing calcium chloride or calcium gluconate using light obscuration as recommended by the United States Pharmacopeia (USP. The purpose of this study was to do compatibility testing for solutions containing calcium chloride and calcium gluconate without cysteine. Solutions of TrophAmine and Premasol (2.5% amino acids, containing calcium chloride or calcium gluconate were compounded without cysteine. Solutions were analyzed for particle counts using light obscuration. Maximum concentrations tested were 15 mmol/L of calcium and 12.5 mmol/L of phosphate. If the average particle count of three replicates exceeded USP guidelines, the solution was determined to be incompatible. This study found that 12.5 and 10 mmol/L of calcium and phosphate, respectively, are compatible in neonatal parenteral nutrition solutions compounded with 2.5% amino acids of either TrophAmine or Premasol. There did not appear to be significant differences in compatibility for solutions containing TrophAmine or Premasol when solutions were compounded with either CaCl2 or CaGlu-Pl. This study presents data in order to evaluate options for adding calcium and phosphate to neonatal parenteral nutrition solutions during shortages of calcium and cysteine.

THE STAR FORMATION HISTORIES OF z ∼ 2 DUST-OBSCURED GALAXIES AND SUBMILLIMETER-SELECTED GALAXIES

International Nuclear Information System (INIS)

Bussmann, R. S.; Dey, Arjun; Jannuzi, B. T.; Armus, L.; Desai, V.; Soifer, B. T.; Brown, M. J. I.; Gonzalez, A. H.; Melbourne, J.

2012-01-01

The Spitzer Space Telescope has identified a population of ultraluminous infrared galaxies (ULIRGs) at z ∼ 2 that may play an important role in the evolution of massive galaxies. We measure the stellar masses (M * ) of two populations of Spitzer-selected ULIRGs that have extremely red R – [24] colors (dust-obscured galaxies, or DOGs) and compare our results with submillimeter-selected galaxies (SMGs). One set of 39 DOGs has a local maximum in their mid-infrared (mid-IR) spectral energy distribution (SED) at rest frame 1.6 μm associated with stellar emission ( b ump DOGs ) , while the other set of 51 DOGs have power-law mid-IR SEDs that are typical of obscured active galactic nuclei ( p ower-law DOGs ) . We measure M * by applying Charlot and Bruzual stellar population synthesis models to broadband photometry in the rest-frame ultraviolet, optical, and near-infrared of each of these populations. Assuming a simple stellar population and a Chabrier initial mass function, we find that power-law DOGs and bump DOGs are on average a factor of 2 and 1.5 more massive than SMGs, respectively (median and inter-quartile M * values for SMGs, bump DOGs, and power-law DOGs are log(M * /M ☉ ) = 10.42 +0.42 –0.36 , 10.62 +0.36 –0.32 , and 10.71 +0.40 –0.34 , respectively). More realistic star formation histories drawn from two competing theories for the nature of ULIRGs at z ∼ 2 (major merger versus smooth accretion) can increase these mass estimates by up to 0.5 dex. A comparison of our stellar masses with the instantaneous star formation rate (SFR) in these z ∼ 2 ULIRGs provides a preliminary indication supporting high SFRs for a given M * , a situation that arises more naturally in major mergers than in smooth accretion-powered systems.

Effect of Transitioning from Standard Reference Material 2806a to Standard Reference Material 2806b for Light Obscuration Particle Countering

Science.gov (United States)

2016-04-01

gravimetric mass limits. The light obscuration particle counters utilized to perform this testing are calibrated to ISO 11171, Hydraulic fluid power...Calibration of automatic particle counters for liquids (2) and operated according to the following test methods : • IP 564: Determination of the...level of cleanliness of aviation turbine fuel - Laboratory automatic particle counter method (3) • IP 565: Determination of the level of cleanliness of

"Lansania Journal of Arachnology and Zoology" - a rare and obscure Japanese natural history journal.

Science.gov (United States)

Tennent, W John; Yasuda, Masatoshi; Morimoto, Katsura

2008-01-01

Publication data relating to a rare and obscure Japanese journal "Lansania Journal of Arachnology and Zoology" (1929-1941) are examined. Available facts, together with a substantial body of circumstantial and anecdotal evidence suggest that many planned issues, including several cited by independent sources as having been published, were not published. Some biographical data relating to the editor, Kyukichi Kishida (1888-1968), are provided. Titles of all papers known to have been published in "Lansania," with page numbers and claimed publication dates are presented, together with a list of 113 new zoological names proposed in the journal. Known library holdings of the journal worldwide are indicated. Details are provided of unpublished manuscripts in proof obtained from Kishida in the 1960s. The strong probability that some printed publication dates are inaccurate is discussed in detail.

Rapid dating of recent sediments in Loch Ness. Inductively coupled plasma mass spectrometric measurements of global fallout plutonium

International Nuclear Information System (INIS)

Ketterer, Michael E.; Hafer, Kevin M.; Jones, Vivienne J.; Appleby, Peter G.

2004-01-01

The 239+240 Pu activity profile is determined for a sediment core collected from 170-m depth at Loch Ness, Scotland. These measurements use magnetic sector inductively coupled plasma mass spectrometry for rapid determination of Pu activities and 240 Pu/ 239 Pu atom ratios. A 239+240 Pu detection limit of 0.1 Bq/kg is obtained for 2 g of acid-leached sediment; 242 Pu is used as a spike isotope. The Pu activity profile exhibits a maximum of 42.7±0.3 Bq/kg 239+240 Pu in the 9-10-cm depth interval. The position of this maximum coincides with peaks in the 241 Am and 137 Cs activity profiles. These peak activities are ascribed to the 1963/1964 peak fallout from atmospheric testing of nuclear weapons. The 240 Pu/ 239 Pu atom ratios are in the range 0.15-0.20, in agreement with the expected range of 0.166-0.194 for Northern Hemisphere fallout, and do not suggest the presence of other contributing sources. This study demonstrates that ICPMS has considerable potential for rapid determination of the chronology of post-1950 sediments, and also for validating 210 Pb dates where chronologies over longer time-scales are needed

Rapid dating of recent sediments in Loch Ness. Inductively coupled plasma mass spectrometric measurements of global fallout plutonium

Energy Technology Data Exchange (ETDEWEB)

Ketterer, Michael E.; Hafer, Kevin M. [Department of Chemistry, Northern Arizona University, Flagstaff, AZ 86011-5698 (United States); Jones, Vivienne J. [Environmental Change Research Centre, University College London, 26 Bedford Way, London WC1H 0AP (United Kingdom); Appleby, Peter G. [Department of Mathematical Sciences, University of Liverpool, P.O. Box 147, Liverpool L69 3BX (United Kingdom)

2004-04-25

The {sup 239+240}Pu activity profile is determined for a sediment core collected from 170-m depth at Loch Ness, Scotland. These measurements use magnetic sector inductively coupled plasma mass spectrometry for rapid determination of Pu activities and {sup 240}Pu/{sup 239}Pu atom ratios. A {sup 239+240}Pu detection limit of 0.1 Bq/kg is obtained for 2 g of acid-leached sediment; {sup 242}Pu is used as a spike isotope. The Pu activity profile exhibits a maximum of 42.7{+-}0.3 Bq/kg {sup 239+240}Pu in the 9-10-cm depth interval. The position of this maximum coincides with peaks in the {sup 241}Am and {sup 137}Cs activity profiles. These peak activities are ascribed to the 1963/1964 peak fallout from atmospheric testing of nuclear weapons. The {sup 240}Pu/{sup 239}Pu atom ratios are in the range 0.15-0.20, in agreement with the expected range of 0.166-0.194 for Northern Hemisphere fallout, and do not suggest the presence of other contributing sources. This study demonstrates that ICPMS has considerable potential for rapid determination of the chronology of post-1950 sediments, and also for validating {sup 210}Pb dates where chronologies over longer time-scales are needed.

Suzaku  Observations of Heavily Obscured (Compton-thick) Active Galactic Nuclei Selected by the Swift/BAT Hard X-Ray Survey

Science.gov (United States)

Tanimoto, Atsushi; Ueda, Yoshihiro; Kawamuro, Taiki; Ricci, Claudio; Awaki, Hisamitsu; Terashima, Yuichi

2018-02-01

We present a uniform broadband X-ray (0.5–100.0 keV) spectral analysis of 12 Swift/Burst Alert Telescope selected Compton-thick ({log}{N}{{H}}/{{cm}}-2≥slant 24) active galactic nuclei (CTAGNs) observed with Suzaku. The Suzaku data of three objects are published here for the first time. We fit the Suzaku and Swift spectra with models utilizing an analytic reflection code and those utilizing the Monte-Carlo-based model from an AGN torus by Ikeda et al. The main results are as follows: (1) The estimated intrinsic luminosity of a CTAGN strongly depends on the model; applying Compton scattering to the transmitted component in an analytic model may largely overestimate the intrinsic luminosity at large column densities. (2) Unabsorbed reflection components are commonly observed, suggesting that the tori are clumpy. (3) Most of CTAGNs show small scattering fractions (<0.5%), implying a buried AGN nature. (4) Comparison with the results obtained for Compton-thin AGNs suggests that the properties of these CTAGNs can be understood as a smooth extension from Compton-thin AGNs with heavier obscuration; we find no evidence that the bulk of the population of hard-X-ray-selected CTAGNs are different from less obscured objects.

Application of wavelet analysis in optical coherence tomography for obscured pattern recognition

Science.gov (United States)

Buranachai, C.; Thavarungkul, P.; Kanatharanaa, P.; Meglinski, I. V.

2009-12-01

Nowadays the optical coherent tomography (OCT) is one of the most perspective optical diagnostic modalities widely used for non-invasive imaging of the internal structure of various complex turbid media from a range of composite materials to biological tissues. OCT has been attracting a great amount of attention due to its effective capability rejecting multiple scattering. However, for highly scattered composite structures the multiple scattering still remains a factor limiting OCT to the quasi-ballistic regime. In order to enhance the OCT imaging capabilities and reduce the statistical noise associated with the multiple scattering the wavelet analysis has been applied. The wavelet analysis has been used to decompose the OCT images of printed stripes covered by a highly scattered and not transparent layer of white correction tape. The obtained results demonstrate a significant reduction of speckle noise background and enhancement of OCT images of the obscured patterns. This likely to be enabled extending the applicability of the combined OCT-wavelet decomposition analysis to investigate sensitive documents, historical artworks and valuable security papers.

Application of wavelet analysis in optical coherence tomography for obscured pattern recognition

International Nuclear Information System (INIS)

Buranachai, C; Thavarungkul, P; Kanatharanaa, P; Meglinski, I V

2009-01-01

Nowadays the optical coherent tomography (OCT) is one of the most perspective optical diagnostic modalities widely used for non-invasive imaging of the internal structure of various complex turbid media from a range of composite materials to biological tissues. OCT has been attracting a great amount of attention due to its effective capability rejecting multiple scattering. However, for highly scattered composite structures the multiple scattering still remains a factor limiting OCT to the quasi-ballistic regime. In order to enhance the OCT imaging capabilities and reduce the statistical noise associated with the multiple scattering the wavelet analysis has been applied. The wavelet analysis has been used to decompose the OCT images of printed stripes covered by a highly scattered and not transparent layer of white correction tape. The obtained results demonstrate a significant reduction of speckle noise background and enhancement of OCT images of the obscured patterns. This likely to be enabled extending the applicability of the combined OCT-wavelet decomposition analysis to investigate sensitive documents, historical artworks and valuable security papers

Infrared spectroscopy of a Cygnus A - Implications for the obscured active nucleus

Science.gov (United States)

Ward, Martin J.; Blanco, Philip R.; Wilson, Andrew S.; Nishida, Minoru

1991-01-01

Near-infrared spectroscopic observations of the central regions of the luminous radio galaxy Cygnus A are presented and interpreted in terms of an obscured quasar nucleus. Strong emission is detected in the molecular hydrogen lines 1-0 S(1) and 1-0 S(3), the strengths of which are accounted for through heating by the nuclear hard X-ray source. The large equivalent widths of these molecular hydrogen lines and the near-infrared narrow hydrogen recombination lines suggest that the observed nuclear continuum is strongly attenuated at 2 microns. The observed upper limit to the flux of broad Pa-alpha implies an extinction to the putative broad line region AV(BL) of at least 24 mag, and the observed continuum intensity of the nuclear point source at 2.2 microns gives an extinction of 43 +/-9 mag toward the optical-infrared continuum. These estimates are consistent with the gas column density inferred from the low-energy X-ray cutoff. Strong forbidden Si VI 1.962-micron line emission from Cygnus A is also reported.

Obscured AGN at z similar to 1 from the zCOSMOS-Bright Survey : I. Selection and optical properties of a [Ne v]-selected sample

NARCIS (Netherlands)

Mignoli, M.; Vignali, C.; Gilli, R.; Comastri, A.; Zamorani, G.; Bolzonella, M.; Bongiorno, A.; Lamareille, F.; Nair, P.; Pozzetti, L.; Lilly, S. J.; Carollo, C. M.; Contini, T.; Kneib, J. -P.; Le Fevre, O.; Mainieri, V.; Renzini, A.; Scodeggio, M.; Bardelli, S.; Caputi, K.; Cucciati, O.; de la Torre, S.; de Ravel, L.; Franzetti, P.; Garilli, B.; Iovino, A.; Kampczyk, P.; Knobel, C.; Kovac, K.; Le Borgne, J. -F.; Le Brun, V.; Maier, C.; Pello, R.; Peng, Y.; Montero, E. Perez; Presotto, V.; Silverman, J. D.; Tanaka, M.; Tasca, L.; Tresse, L.; Vergani, D.; Zucca, E.; Bordoloi, R.; Cappi, A.; Cimatti, A.; Koekemoer, A. M.; McCracken, H. J.; Moresco, M.; Welikala, N.

Aims. The application of multi-wavelength selection techniques is essential for obtaining a complete and unbiased census of active galactic nuclei (AGN). We present here a method for selecting z similar to 1 obscured AGN from optical spectroscopic surveys. Methods. A sample of 94 narrow-line AGN

The Nature of the Torus in the Heavily Obscured AGN Markarian 3: an X-Ray Study

Science.gov (United States)

Guainazzi, M.; Risaliti, G.; Awaki, H.; Arevalo, P.; Bauer, F. E.; Bianchi, S.; Boggs, S.E; Brandt, W. N.; Brightman, M.; Christensen, F. E.;

X-ray View of Four High-Luminosity Swift-BAT AGN: Unveiling Obscuration and Reflection with Suzaku

Science.gov (United States)

Fiorettil, V.; Angelini, L.; Mushotzky, R. F.; Koss, M.; Malaguti, G.

2013-01-01

Aims. A complete census of obscured Active Galactic Nuclei (AGN) is necessary to reveal the history of the super massive black hole (SMBH) growth and galaxy evolution in the Universe given the complex feedback processes and the fact that much of this growth occurs in an obscured phase. In this context, hard X-ray surveys and dedicated follow-up observations represent a unique tool for selecting highly absorbed AGN and for characterizing the obscuring matter surrounding the SMBH. Here we focus on the absorption and reflection occurring in highly luminous, quasar-like AGN, to study the relation between the geometry of the absorbing matter and the AGN nature (e.g. X-ray, optical, and radio properties), and to help to determine the column density dependency on the AGN luminosity. Methods. The Swift/BAT nine-month survey observed 153 AGN, all with ultra-hard X-ray BAT fluxes in excess of 10(exp -11) erg per square centimeter and an average redshift of 0.03. Among them, four of the most luminous BAT AGN (44.73 less than LogLBAT less than 45.31) were selected as targets of Suzaku follow-up observations: J2246.0+3941 (3C 452), J0407.4+0339 (3C 105), J0318.7+6828, and J0918.5+0425. The column density, scattered/reflected emission, the properties of the Fe K line, and a possible variability are fully analyzed. For the latter, the spectral properties from Chandra, XMM-Newton and Swift/XRT public observations were compared with the present Suzaku analysis, adding an original spectral analysis when non was available from the literature. Results. Of our sample, 3C 452 is the only certain Compton-thick AGN candidate because of i) the high absorption (N(sub H) approximately 4 × 10(exp 23) per square centimeter) and strong Compton reflection; ii) the lack of variability; iii) the "buried" nature, i.e. the low scattering fraction (less than 0.5%) and the extremely low relative [OIII] luminosity. In contrast 3C 105 is not reflection-dominated, despite the comparable column density

Loch ness, special operations executive and the first surgeon in paradise: Robert Kenneth Wilson (26.1.1899-6.6.1969).

Science.gov (United States)

Watters, David A K

2007-12-01

Lieutenant Colonel Robert Kenneth Wilson (1899-1969) was a surgeon who fought in both world wars and joined the Special Operations Executive parachuting behind enemy lines into Holland, France and Borneo, the last mission being with Australian forces (Semut II). He was an expert on firearms and gave opinion on ballistics at the Old Bailey during the 1930s. He also wrote a definitive text on automatic pistols with editions published in 1943 and 1975. He was an Edinburgh Fellow (1926), who had a practice in general surgery and gynaecology in Queen Anne Street during the 1930s. He took the famous 1934 'surgeon's photo' of the Loch Ness monster that was not admitted to be a hoax until 1994. After World War II, he became the first surgical specialist to work in the public service of the then Territory of Papua and New Guinea (1950-1956), where he wrote several papers on surgical topics. He married Gwen (1924), the daughter of Henrietta Gulliver, an Australian painter. They had two sons, Richard and Phillip. After practice he retired to Melbourne where he died of carcinoma oesophagus.

CONSTRAINTS ON OBSCURED STAR FORMATION IN HOST GALAXIES OF GAMMA-RAY BURSTS

International Nuclear Information System (INIS)

Hatsukade, Bunyo; Ohta, Kouji; Hashimoto, Tetsuya; Nakanishi, Kouichiro; Tamura, Yoichi; Kohno, Kotaro

2012-01-01

We present the results of the 16 cm wave band continuum observations of four host galaxies of gamma-ray bursts (GRBs) 990705, 021211, 041006, and 051022 using the Australia Telescope Compact Array. Radio emission was not detected in any of the host galaxies. The 2σ upper limits on star formation rates derived from the radio observations of the host galaxies are 23, 45, 27, and 26 M ☉ yr –1 , respectively, which are less than about 10 times those derived from UV/optical observations, suggesting that they have no significant dust-obscured star formation. GRBs 021211 and 051022 are known as the so-called dark GRBs and our results imply that dark GRBs do not always occur in galaxies enshrouded by dust. Because large dust extinction was not observed in the afterglow of GRB 021211, our result suggests the possibility that the cause of the dark GRB is the intrinsic faintness of the optical afterglow. On the other hand, by considering the high column density observed in the afterglow of GRB 051022, the likely cause of the dark GRB is the dust extinction in the line of sight of the GRB.

High-z X-ray Obscured Quasars in Galaxies with Extreme Mid-IR/Optical Colors

Science.gov (United States)

Piconcelli, E.; Lanzuisi, G.; Fiore, F.; Feruglio, C.; Vignali, C.; Salvato, M.; Grappioni, C.

2009-05-01

Extreme Optical/Mid-IR color cuts have been used to uncover a population of dust-enshrouded, mid-IR luminous galaxies at high redshifts. Several lines of evidence point towards the presence of an heavily absorbed, possibly Compton-thick quasar at the heart of these systems. Nonetheless, the X-ray spectral properties of these intriguing sources still remain largely unexplored. Here we present an X-ray spectroscopic study of a large sample of 44 extreme dust-obscured galaxies (EDOGs) with F24 μm/FR>2000 and F24 μm>1.3 mJy selected from a 6 deg2 region in the SWIRE fields. The application of our selection criteria to a wide area survey has been capable of unveiling a population of X-ray luminous, absorbed z>1 quasars which is mostly missed in the traditional optical/X-ray surveys performed so far. Advances in the understanding of the X-ray properties of these recently-discovered sources by Simbol-X observations will be also discussed.

The shape of the cosmic X-ray background: nuclear starburst discs and the redshift evolution of AGN obscuration

Science.gov (United States)

Gohil, R.; Ballantyne, D. R.

2018-04-01

A significant number of active galactic nuclei (AGNs) are observed to be hidden behind dust and gas. The distribution of material around AGNs plays an important role in modelling the cosmic X-ray background (CXB), especially the fraction of type 2 AGNs (f2). One of the possible explanations for obscuration in Seyfert galaxies at intermediate redshifts is dusty starburst discs. We compute the two-dimensional (2D) hydrostatic structure of 768 nuclear starburst discs (NSDs) under various physical conditions and also the distribution of column density along the line of sight (NH) associated with these discs. Then the NH distribution is evolved with redshift by using the redshift-dependent distribution function of input parameters. Parameter f2 shows a strong positive evolution up to z = 2, but only a weak level of enhancement at higher z. The Compton-thin and Compton-thick AGN fractions associated with these starburst regions increase ∝ (1 + z)δ, where δ is estimated to be 1.12 and 1.45, respectively. The reflection parameter Rf associated with column density NH ≥ 1023.5 cm-2 extends from 0.13 at z = 0 to 0.58 at z = 4. A CXB model employing this evolving NH distribution indicates that more compact (Rout < 120 pc) NSDs provide a better fit to the CXB. In addition to `Seyfert-like' AGNs obscured by nuclear starbursts, we predict that 40-60 per cent of quasars must be Compton-thick to produce a peak of the CXB spectrum within the observational uncertainty. The predicted total number counts of AGNs in 8-24 keV bands are in fair agreement with observations from the Nuclear Spectroscopic Telescope Array (NuSTAR).

Knowledge-based-ness and synthesis of indigenous knowledge with climate in traditional architecture: Evidence from Naeen city

Directory of Open Access Journals (Sweden)

Ali Zangi Abadi

2014-01-01

Full Text Available Application of indigenous knowledge is an example of knowledge-based-ness considered as the main agenda in most current urban and climate planning as well as geographical studies. It is one of the interesting topics in research on the role of climate on human dwelling and immediate environment. Indeed, building ecology emphasizes the ability to combine climate and environmental factors and rendering them to spatial qualities and structural comfort. This paper investigates the application of indigenous knowledge and the correspondence between traditional texture of Naeen city and its climate. In this regard, the climatic conditions in Naeen were studied in terms of temperature, humidity, wind and tourist comfort index (TCI of climatourism. The data was collected from Isfahan Meteorology Website over the period 1985-2005. Subsequently, the traditional texture of Naeen, construction materials and building styles were studied through considering the special architectural conditions and compatible materials. Eventually, the correspondence between architectural styles and climatic conditions was studied. The results show that traditional architecture based on indigenous knowledge was consistent with climatic conditions. In this regard, using such materials as mud bricks and thatch with suitable heat capacity as well as using wind catchers, high walls around houses, dome construction, southward direction of houses were consistent with east-west wind direction. In addition, concentration of the traditional texture of the city, wall thickness, corridors, long hallways, courtyard ponds and roofed alleys are evidence of the effect of climatic conditions on urban texture in order to provide comfort in different seasons.

Those Obscure Objects: Projections and Puppets of Desire Between Literature and Cinema

Directory of Open Access Journals (Sweden)

Claudio Panella

2013-08-01

Full Text Available The paper deals with one of the most popular female projections or phantoms of male desire, that is the charmer who never cedes, by comparing some literary and cinematic texts. This “allumeuse” which turns men into puppets in a dynamic of impossible seduction is the protagonist of La Femme et le Pantin (1898 by Pierre Louÿs (1870-1925, whose unforgettable Conchita from Sevilla was inspired by the young Charpillon who maddened the expert seducer Casanova. Conchita’s fame was deepened by the numerous adaptations of the text for the screen, especially von Sternberg’s The Devil is a Woman (1935 starring Marlene Dietrich, Duvivier’s La Femme et le Pantin (1959 with Brigitte Bardot, and Buñuel’s free and outstanding reinterpretation in Cet obscur objet du désir (1977. In the end, the adaptation of the novel Singularidades de uma Rapariga Loura (1874 by Portuguese Eça de Queirós (1845-1900 which Manoel de Oliveira directed in 2009 will be evoked  to argue that the unattainable female character could represent a projection of the male protagonists’ desire and romantic idealizations as well as of their fears and bourgeois conventions.

Duodenal plexiform fibromyxoma as a cause of obscure upper gastrointestinal bleeding: A case report.

Science.gov (United States)

Moris, Demetrios; Spanou, Evangelia; Sougioultzis, Stavros; Dimitrokallis, Nikolaos; Kalisperati, Polyxeni; Delladetsima, Ioanna; Felekouras, Evangelos

2017-01-01

We are reporting the first-to our knowledge-case of duodenal Plexiform Fibromyxoma causing obscure upper gastrointestinal bleeding. Plexiform fibromyxoma triggered recurrent upper gastrointestinal bleeding episodes in a 63-year-old man who remained undiagnosed, despite multiple hospitalizations, extensive diagnostic workups and surgical interventions (including gastrectomies), for almost 17 years. During hospitalization for the last bleeding episode, an upper gastrointestinal endoscopy revealed an intestinal hemorrhagic nodule. The lesion was deemed unresectable by endoscopic means. An abdominal computerized tomography disclosed no further lesions and surgery was decided. The lesion at operation was found near the edge of the duodenal stump and treated with pancreas-preserving duodenectomy (1st and 2nd portion). Postoperative recovery was mainly uneventful and a 20-month follow-up finds the patient in good health with no need for blood transfusions.Plexiform fibromyxomas stand for a rare and widely unknown mesenchymal entity. Despite the fact that they closely resemble other gastrointestinal tumors, they distinctly vary in clinical management as well as the histopathology. Clinical awareness and further research are compulsory to elucidate its clinical course and prognosis.

THE SPITZER MID-INFRARED ACTIVE GALACTIC NUCLEUS SURVEY. I. OPTICAL AND NEAR-INFRARED SPECTROSCOPY OF OBSCURED CANDIDATES AND NORMAL ACTIVE GALACTIC NUCLEI SELECTED IN THE MID-INFRARED

Energy Technology Data Exchange (ETDEWEB)

Lacy, M. [National Radio Astronomy Observatory, 520 Edgemont Road, Charlottesville, VA 22903 (United States); Ridgway, S. E. [National Optical Astronomy Observatory, 950 North Cherry Avenue, Tucson, AZ 85719 (United States); Gates, E. L. [UCO/Lick Observatory, P.O. Box 85, Mount Hamilton, CA 95140 (United States); Nielsen, D. M. [Department of Astronomy, University of Wisconsin, 475 N. Charter Street, Madison, WI 53706 (United States); Petric, A. O. [Department of Astronomy, California Institute of Technology, Pasadena, CA 91125 (United States); Sajina, A. [Department of Physics and Astronomy, Tuffs University, 212 College Avenue, Medford, MA 02155 (United States); Urrutia, T. [Leibniz-Institut für Astrophysik Potsdam, An der Sternwarte 16, D-14482 Potsdam (Germany); Cox Drews, S. [946 Mangrove Avenue 102, Sunnyvale, CA 94086 (United States); Harrison, C. [Department of Astronomy, University of Michigan, Ann Arbor, MI 48109 (United States); Seymour, N. [CSIRO, P.O. Box 76, Epping, NSW 1710 (Australia); Storrie-Lombardi, L. J. [Spitzer Science Center, California Institute of Technology, Pasadena, CA 91125 (United States)

2013-10-01

We present the results of a program of optical and near-infrared spectroscopic follow-up of candidate active galactic nuclei (AGNs) selected in the mid-infrared. This survey selects both normal and obscured AGNs closely matched in luminosity across a wide range, from Seyfert galaxies with bolometric luminosities L {sub bol} ∼ 10{sup 10} L {sub ☉} to highly luminous quasars (L {sub bol} ∼ 10{sup 14} L {sub ☉}), all with redshifts ranging from 0 to 4.3. Samples of candidate AGNs were selected with mid-infrared color cuts at several different 24 μm flux density limits to ensure a range of luminosities at a given redshift. The survey consists of 786 candidate AGNs and quasars, of which 672 have spectroscopic redshifts and classifications. Of these, 137 (20%) are type 1 AGNs with blue continua, 294 (44%) are type 2 objects with extinctions A{sub V} ∼> 5 toward their AGNs, 96 (14%) are AGNs with lower extinctions (A{sub V} ∼ 1), and 145 (22%) have redshifts, but no clear signs of AGN activity in their spectra. Of the survey objects 50% have L {sub bol} > 10{sup 12} L {sub ☉}, in the quasar regime. We present composite spectra for type 2 quasars and objects with no signs of AGN activity in their spectra. We also discuss the mid-infrared—emission-line luminosity correlation and present the results of cross correlations with serendipitous X-ray and radio sources. The results show that: (1) obscured objects dominate the overall AGN population, (2) mid-infrared selected AGN candidates exist which lack AGN signatures in their optical spectra but have AGN-like X-ray or radio counterparts, and (3) X-ray and optical classifications of obscured and unobscured AGNs often differ.

Partial dust obscuration in active galactic nuclei as a cause of broad-line profile and lag variability, and apparent accretion disc inhomogeneities

Science.gov (United States)

Gaskell, C. Martin; Harrington, Peter Z.

2018-04-01

The profiles of the broad emission lines of active galactic nuclei (AGNs) and the time delays in their response to changes in the ionizing continuum ("lags") give information about the structure and kinematics of the inner regions of AGNs. Line profiles are also our main way of estimating the masses of the supermassive black holes (SMBHs). However, the profiles often show ill-understood, asymmetric structure and velocity-dependent lags vary with time. Here we show that partial obscuration of the broad-line region (BLR) by outflowing, compact, dusty clumps produces asymmetries and velocity-dependent lags similar to those observed. Our model explains previously inexplicable changes in the ratios of the hydrogen lines with time and velocity, the lack of correlation of changes in line profiles with variability of the central engine, the velocity dependence of lags, and the change of lags with time. We propose that changes on timescales longer than the light-crossing time do not come from dynamical changes in the BLR, but are a natural result of the effect of outflowing dusty clumps driven by radiation pressure acting on the dust. The motion of these clumps offers an explanation of long-term changes in polarization. The effects of the dust complicate the study of the structure and kinematics of the BLR and the search for sub-parsec SMBH binaries. Partial obscuration of the accretion disc can also provide the local fluctuations in luminosity that can explain sizes deduced from microlensing.

Obscure Gastrointestinal Bleeding from an Ampullary Tumour in a Patient with a Remote History of Renal Cell Carcinoma: A Diagnostic Conundrum

Directory of Open Access Journals (Sweden)

Rhonda M Janzen

1998-01-01

Full Text Available Metastasis of renal cell carcinoma to the ampulla of Vater is a rare occurrence. The outlined case, which presented as an upper gastrointestinal bleed, is only the eighth such reported case in the English-language literature. This case is the longest reported time interval between surgical nephrectomy to presentation with ampullary metastasis at 17.5 years. The ampullary source of bleeding in this case was initially obscure and missed by conventional gastroscopy. Diagnosis was made with a side-viewing endoscope, emphasizing the usefulness of this instrument in the investigation of active bleeding from a small bowel source.

NuSTAR Observations of WISE J1036+0449, A Galaxy at zeta approx 1 Obscured by Hot Dust

Science.gov (United States)

Ricci, C.; Assef, R. J.; Stern, Daniel K.; Nikutta, R.; Alexander, D. M.; Asmus, D.; Ballantyne, D. R.; Bauer, F. E.; Blain, A.W.; Zhang, William W.;

NuSTAR Observations of WISE J1036+0449, A Galaxy at Z Approx. 1 Obscured by Hot Dust

Science.gov (United States)

Ricci, C.; Assef, R. J.; Stern, D.; Nikutta, R.; Alexander, D. M.; Asmus, D.; Ballantyne, D. R.; Bauer, F. E.; Blain, A. W.; Boggs, S.;

Arteriojejunal Fistula Presenting with Recurrent Obscure GI Hemorrhage in a Patient with a Failed Pancreas Allograft

Directory of Open Access Journals (Sweden)

Nirmit Desai

2013-01-01

Full Text Available We present a case of a patient with a failed pancreaticoduodenal allograft with exocrine enteric-drainage who developed catastrophic gastrointestinal (GI hemorrhage. Over the course of a week, she presented with recurrent GI bleeds of obscure etiology. Multiple esophago-gastro-duodenoscopic (EGD and colonoscopic evaluations failed to reveal the source of the hemorrhage. A capsule endoscopy and a technetium-labeled red blood cells (RBC imaging study were similarly unrevealing for source of bleeding. She subsequently developed hemorrhagic shock requiring emergent superior mesenteric arteriography. Run off images revealed an external iliac artery aneurysm with fistulization into the jejunum. Coiled embolization was attempted but abandoned because of hemodynamic instability. Deployment of a covered endovascular stent into the right external iliac artery over the fistula site resulted in immediate hemodynamic stabilization. A high index of suspicion for arterioenteric fistulae is needed for diagnosis of this uncommon but eminently treatable form of GI hemorrhage in this patient population.

Simultaneous Chandra and NuSTAR Observations of the Highly Obscured AGN Candidate in NGC660.

Science.gov (United States)

Annuar, Ady

2014-09-01

We are using NuSTAR to undertake a detailed investigation of the obscured AGN population at D<15Mpc. Our latest target is NGC660 where the presence of an AGN has been ambiguous. However, recently it was observed to undergo a radio outburst which reveals a bright continuum source (Argo et al. 2015), coincident with Chandra 2-8 keV emission from one of the three point sources near the nucleus (<5"). This confirms and pinpoints the X-ray position of the AGN. Comparisons of the Chandra flux with the radio emission and other multiwavelength luminosity indicators indicate that the X-ray flux is suppressed, suggesting that it is absorbed by a high column of gas. A NuSTAR observation for this object has been scheduled as part of our program. The requested Chandra observation is essential to unambiguously constrain the AGN and isolate it from other sources at <8 keV. When combined with NuSTAR, we will then be able to accurately characterise the 0.5-30 keV spectrum of the AGN for the first time.

Storm in a Teacup: X-Ray View of an Obscured Quasar and Superbubble

Science.gov (United States)

Lansbury, George B.; Jarvis, Miranda E.; Harrison, Chris M.; Alexander, David M.; Del Moro, Agnese; Edge, Alastair C.; Mullaney, James R.; Thomson, Alasdair P.

2018-03-01

We present the X-ray properties of the “Teacup AGN” (SDSS J1430+1339), a z = 0.085 type 2 quasar that is interacting dramatically with its host galaxy. Spectral modeling of the central quasar reveals a powerful, highly obscured active galactic nucleus (AGN) with a column density of N H = (4.2–6.5) × 1023 cm‑2 and an intrinsic luminosity of L 2–10 keV = (0.8–1.4) × 1044 erg s‑1. The current high bolometric luminosity inferred (L bol ≈1045–1046 erg s‑1) has ramifications for previous interpretations of the Teacup as a fading/dying quasar. High-resolution Chandra imaging data reveal a ≈10 kpc loop of X-ray emission, cospatial with the “eastern bubble” previously identified in luminous radio and ionized gas (e.g., [O III] line) emission. The X-ray emission from this structure is in good agreement with a shocked thermal gas, with T = (4–8) × 106 K, and there is evidence for an additional hot component with T ≳ 3 × 107 K. Although the Teacup is a radiatively dominated AGN, the estimated ratio between the bubble power and the X-ray luminosity is in remarkable agreement with observations of ellipticals, groups, and clusters of galaxies undergoing AGN feedback.

HerMES: THE FAR-INFRARED EMISSION FROM DUST-OBSCURED GALAXIES

International Nuclear Information System (INIS)

Calanog, J. A.; Wardlow, J.; Fu, Hai; Cooray, A.; Assef, R. J.; Bock, J.; Riechers, D.; Schulz, B.; Casey, C. M.; Conley, A.; Farrah, D.; Oliver, S. J.; Roseboom, I. G.; Ibar, E.; Kartaltepe, J.; Magdis, G.; Rigopoulou, D.; Marchetti, L.; Pérez-Fournon, I.; Scott, Douglas

2013-01-01

Dust-obscured galaxies (DOGs) are an ultraviolet-faint, infrared-bright galaxy population that reside at z ∼ 2 and are believed to be in a phase of dusty star-forming and active galactic nucleus (AGN) activity. We present far-infrared (far-IR) observations of a complete sample of DOGs in the 2 deg 2 of the Cosmic Evolution Survey. The 3077 DOGs have (z) = 1.9 ± 0.3 and are selected from 24 μm and r + observations using a color cut of r + – [24] ≥ 7.5 (AB mag) and S 24 ≥ 100 μJy. Based on the near-IR spectral energy distributions, 47% are bump DOGs (star formation dominated) and 10% are power-law DOGs (AGN-dominated). We use SPIRE far-IR photometry from the Herschel Multi-tiered Extragalactic Survey to calculate the IR luminosity and characteristic dust temperature for the 1572 (51%) DOGs that are detected at 250 μm (≥3σ). For the remaining 1505 (49%) that are undetected, we perform a median stacking analysis to probe fainter luminosities. Herschel-detected and undetected DOGs have average luminosities of (2.8 ± 0.4) × 10 12 L ☉ and (0.77 ± 0.08) × 10 12 L ☉ , and dust temperatures of (33 ± 7) K and (37 ± 5) K, respectively. The IR luminosity function for DOGs with S 24 ≥ 100 μJy is calculated, using far-IR observations and stacking. DOGs contribute 10%-30% to the total star formation rate (SFR) density of the universe at z = 1.5-2.5, dominated by 250 μm detected and bump DOGs. For comparison, DOGs contribute 30% to the SFR density for all z = 1.5-2.5 galaxies with S 24 ≥ 100 μJy. DOGs have a large scatter about the star formation main sequence and their specific SFRs show that the observed phase of star formation could be responsible for their total observed stellar mass at z ∼ 2

HerMES: THE FAR-INFRARED EMISSION FROM DUST-OBSCURED GALAXIES

Energy Technology Data Exchange (ETDEWEB)

Calanog, J. A.; Wardlow, J.; Fu, Hai; Cooray, A. [Department of Physics and Astronomy, University of California, Irvine, CA 92697 (United States); Assef, R. J. [Jet Propulsion Laboratory, 4800 Oak Grove Drive, Pasadena, CA 91109 (United States); Bock, J.; Riechers, D.; Schulz, B. [California Institute of Technology, 1200 E. California Boulevard, Pasadena, CA 91125 (United States); Casey, C. M. [Institute for Astronomy, University of Hawaii, 2680 Woodlawn Drive, Honolulu, HI 96822 (United States); Conley, A. [Center for Astrophysics and Space Astronomy 389-UCB, University of Colorado, Boulder, CO 80309 (United States); Farrah, D.; Oliver, S. J.; Roseboom, I. G. [Astronomy Centre, Department of Physics and Astronomy, University of Sussex, Brighton BN1 9QH (United Kingdom); Ibar, E. [Instituto de Astrofísica, Facultad de Física, Pontificia Universidad Católica de Chile, Casilla 306, Santiago 22 (Chile); Kartaltepe, J. [National Optical Astronomy Observatory, 950 North Cherry Avenue, Tucson, AZ 85719 (United States); Magdis, G.; Rigopoulou, D. [Department of Astrophysics, Denys Wilkinson Building, University of Oxford, Keble Road, Oxford OX1 3RH (United Kingdom); Marchetti, L. [Department of Physical Sciences, The Open University, Milton Keynes MK7 6AA (United Kingdom); Pérez-Fournon, I. [Instituto de Astrofísica de Canarias (IAC), E-38200 La Laguna, Tenerife (Spain); Scott, Douglas [Department of Physics and Astronomy, University of British Columbia, 6224 Agricultural Road, Vancouver, BC V6T 1Z1 (Canada); and others

2013-09-20

Dust-obscured galaxies (DOGs) are an ultraviolet-faint, infrared-bright galaxy population that reside at z ∼ 2 and are believed to be in a phase of dusty star-forming and active galactic nucleus (AGN) activity. We present far-infrared (far-IR) observations of a complete sample of DOGs in the 2 deg{sup 2} of the Cosmic Evolution Survey. The 3077 DOGs have (z) = 1.9 ± 0.3 and are selected from 24 μm and r {sup +} observations using a color cut of r {sup +} – [24] ≥ 7.5 (AB mag) and S{sub 24} ≥ 100 μJy. Based on the near-IR spectral energy distributions, 47% are bump DOGs (star formation dominated) and 10% are power-law DOGs (AGN-dominated). We use SPIRE far-IR photometry from the Herschel Multi-tiered Extragalactic Survey to calculate the IR luminosity and characteristic dust temperature for the 1572 (51%) DOGs that are detected at 250 μm (≥3σ). For the remaining 1505 (49%) that are undetected, we perform a median stacking analysis to probe fainter luminosities. Herschel-detected and undetected DOGs have average luminosities of (2.8 ± 0.4) × 10{sup 12} L{sub ☉} and (0.77 ± 0.08) × 10{sup 12} L{sub ☉}, and dust temperatures of (33 ± 7) K and (37 ± 5) K, respectively. The IR luminosity function for DOGs with S{sub 24} ≥ 100 μJy is calculated, using far-IR observations and stacking. DOGs contribute 10%-30% to the total star formation rate (SFR) density of the universe at z = 1.5-2.5, dominated by 250 μm detected and bump DOGs. For comparison, DOGs contribute 30% to the SFR density for all z = 1.5-2.5 galaxies with S{sub 24} ≥ 100 μJy. DOGs have a large scatter about the star formation main sequence and their specific SFRs show that the observed phase of star formation could be responsible for their total observed stellar mass at z ∼ 2.

NuSTAR observations of heavily obscured quasars at z ∼ 0.5

Energy Technology Data Exchange (ETDEWEB)

Lansbury, G. B.; Alexander, D. M.; Moro, A. Del; Gandhi, P.; Aird, J. [Department of Physics, University of Durham, South Road, Durham DH1 3LE (United Kingdom); Assef, R. J. [Núcleo de Astronomía de la Facultad de Ingeniería, Universidad Diego Portales, Av. Ejército Libertador 441, Santiago (Chile); Stern, D. [Jet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Drive, Mail Stop 169-221, Pasadena, CA 91109 (United States); Ballantyne, D. R. [Center for Relativistic Astrophysics, School of Physics, Georgia Institute of Technology, Atlanta, GA 30332 (United States); Baloković, M.; Grefenstette, B. W.; Harrison, F. A. [Cahill Center for Astrophysics, 1216 East California Boulevard, California Institute of Technology, Pasadena, CA 91125 (United States); Bauer, F. E. [Instituto de Astrofísica, Facultad de Física, Pontificia Universidad Catlica de Chile, Casilla 306, Santiago 22 (Chile); Boggs, S. E. [Space Sciences Laboratory, University of California, Berkeley, CA 94720 (United States); Brandt, W. N. [Department of Astronomy and Astrophysics, 525 Davey Lab, The Pennsylvania State University, University Park, PA 16802 (United States); Christensen, F. E.; Craig, W. W. [DTU Space-National Space Institute, Technical University of Denmark, Elektrovej 327, DK-2800 Lyngby (Denmark); Elvis, M. [Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138 (United States); Hailey, C. J. [Columbia Astrophysics Laboratory, 550 W 120th Street, Columbia University, NY 10027 (United States); Hickox, R. C. [Department of Physics and Astronomy, Dartmouth College, 6127 Wilder Laboratory, Hanover, NH 03755 (United States); Koss, M., E-mail: g.b.lansbury@durham.ac.uk [Institute for Astronomy, Department of Physics, ETH Zurich, Wolfgang-Pauli-Strasse 27, CH-8093 Zurich (Switzerland); and others

2014-04-10

We present NuSTAR hard X-ray observations of three Type 2 quasars at z ≈ 0.4-0.5, optically selected from the Sloan Digital Sky Survey. Although the quasars show evidence for being heavily obscured, Compton-thick systems on the basis of the 2-10 keV to [O III] luminosity ratio and multiwavelength diagnostics, their X-ray absorbing column densities (N {sub H}) are poorly known. In this analysis, (1) we study X-ray emission at >10 keV, where X-rays from the central black hole are relatively unabsorbed, in order to better constrain N {sub H}. (2) We further characterize the physical properties of the sources through broad-band near-UV to mid-IR spectral energy distribution analyses. One of the quasars is detected with NuSTAR at >8 keV with a no-source probability of <0.1%, and its X-ray band ratio suggests near Compton-thick absorption with N {sub H} ≳ 5 × 10{sup 23} cm{sup –2}. The other two quasars are undetected, and have low X-ray to mid-IR luminosity ratios in both the low-energy (2-10 keV) and high-energy (10-40 keV) X-ray regimes that are consistent with extreme, Compton-thick absorption (N {sub H} ≳ 10{sup 24} cm{sup –2}). We find that for quasars at z ∼ 0.5, NuSTAR provides a significant improvement compared to lower energy (<10 keV) Chandra and XMM-Newton observations alone, as higher column densities can now be directly constrained.

CT enterography in obscure gastrointestinal bleeding: a systematic review and meta-analysis

International Nuclear Information System (INIS)

Wang, Zhen; Chen, Jun-qiang; Liu, Jin-lu; Qin, Xin-gan; Huang, Yuan

2013-01-01

The objective of this article is to provide a comprehensive and update overview of clinical application of CT enterography (CTE) in the evaluation of obscure gastrointestinal bleeding (OGIB). We performed a systematic review of relevant literatures in PubMed, EMBASE and The Cochrane Library and pooled the yield of CTE and the incremental yield (IY) of CTE over an alternate modality. A total of 18 studies (n=660) reported the yield of CTE in evaluating OGIB and the pooled yield was 40% (95% confidence interval (CI): 33–49%). Seven studies (n=279) compared the yield of CTE with capsule endoscopy (CE). The yield for CTE and CE for all findings was 34% and 53%, respectively (IY=−19%, 95% CI=−34% to −4%). When considering the types of identified lesions, the yield was significantly different for vascular and inflammatory lesions but not significantly different for neoplastic or other lesions. Two studies (n=63) compared the yield of CTE with double-balloon enteroscopy (DBE). The yield for CTE and DBE was 38% and 78%, respectively (IY=−40%, 95% CI=−55% to −25%). Three studies (n=49) compared the yield of CTE with digital subtraction angiography. The yield for CTE and digital subtraction angiography was 64% and 60%, respectively (IY=4%, 95% CI=−40% to 47%). CTE is an excellent diagnostic tool in patients with OGIB. It may play a complementary role to CE and can be used as a triage tool prior to DBE in evaluating OGIB.

X-ray effects on karyotype of Drosophila pseudo obscure. Pilot experience

International Nuclear Information System (INIS)

Salceda, V. M.

2009-10-01

Four groups of 100 males of Drosophila pseudo obscure carriers of genetic sequence Tree Line were treated with X-rays, through the use of a X-ray equipment Phillips MCN321; with absorbed individual doses of 28.2 Gy, 37.6 Gy, 47.6 Gy and 56.4 Gy, once irradiated these were crossed individually with two or three virgin females of the same constitution and the descendant emergency was took a larva of each crossing in order to detect the radiation effect on karyotype Tree Line of these organisms, chromosomal aberrations fundamentally, as well as on masculine sterility. Our observations gave as result for smaller dose, in a total of 61 analyzed larva, the obtaining of seven translocations equivalent to 11.5% as well as an inversion of 1.6%; with the following dose (58 analyzed larva) were obtained four translocations equal to 6.9%, two corresponding inversions to 3.4%, a mosaic and a deletion equivalent to 1.7%; with the dose of 47.6 Gy four translocations were induced 6.8% and deletion corresponding to 1.1%, again two respective inversions to 3.4% and a mosaic 1.7% in 59 analyzed larvas, meantime with the dose of 56.4 Gy appeared two translocations only equal to 3.7% in a sample of 54 individuals. The effect about masculine sterility was equal that the witness of 12% and for two following doses and finally of 41 and 46% respectively for the remaining doses. Comparisons with another authors gave similar values in the total cases. In accordance with our main objective, it is suggested to increase the sample size and to repeat the experiments using different genetic sequences as well as the possibility to use different radiation sources like gamma radiation and this way to utilize this system like a biological dosemeter. (Author)

Imaging through obscurations for sluicing operations in the waste storage tanks

International Nuclear Information System (INIS)

Peters, T.J.; McMakin, D.L.; Sheen, D.M.; Chieda, M.A.

1994-08-01

Waste remediators have identified that surveillance of waste remediation operations and periodic inspections of stored waste are required under very demanding and difficult viewing environments. In many cases, obscurants such as dust or water vapor are generated as part of the remediation activity. Methods are required for viewing or imaging beyond the normal visual spectrum. Work space images guide the movement of remediation equipment, creating a need for rapidly updated, near real-time imaging capability. In addition, there is a need for three-dimensional topographical data to determine the contours of the wastes, to plan retrieval campaigns, and to provide a three-dimensional map of a robot's work space as basis for collision avoidance. Three basic imaging techniques were evaluated: optical, acoustic and radar. The optical imaging methods that were examined used cameras which operated in the visible region and near-infrared region and infrared cameras which operated in the 3--5 micron and 8--12 micron wavelength regions. Various passive and active lighting schemes were tested, as well as the use of filters to eliminate reflection in the visible region. Image enhancement software was used to extend the range where visual techniques could be used. In addition, the operation of a laser range finder, which operated at 0.835 microns, was tested when fog/water droplets were suspended in the air. The acoustic technique involved using commercial acoustic sensors, operating at approximately 50 kHz and 215 kHz, to determine the attenuation of the acoustic beam in a high-humidity environment. The radar imaging methods involved performing millimeter wave (94 GHz) attenuation measurement sin the various simulated sluicing environments and performing preliminary experimental imaging studies using a W-Band (75--110 GHz) linearly scanned transceiver in a laboratory environment. The results of the tests are discussed

Environmental and health effects review for obscurant graphite flakes. Final report, 1991 July--1993 May

Energy Technology Data Exchange (ETDEWEB)

Driver, C.J.; Ligotke, M.W.; Landis, W.G.; Downs, J.L.; Tiller, B.L.; Moore, E.B. Jr.; Cataldo, D.A.

1993-07-01

The health and environmental effects of obscurant graphite flakes were reviewed and compared to predicted levels of graphite flake material in the field during typical testing and training scenarios. Graphite flake dispersion and deposition for simulated mechanical and pyrotechnic releases were determined using a modified Gaussian atmospheric plume-dispersion model. The potential for wind resuspension of graphite flakes is controlled by weathering processes and incorporation rates in soil. Chemically, graphite flakes pose little risk to aquatic or terrestrial systems. Mechanical damage to plants and invertebrate and vertebrate organisms from the flakes is also minimal. In humans, the pathological and physiological response to inhaled graphite flake is similar to that induced by nuisance dusts and cause only transient pulmonary changes. Repeated exposure to very high concentrations (such as those near the source generator) may overwhelm the clearance mechanisms of the lung and result in pulmonary damage from the retained particles in unprotected individuals. However, these lesions either resolve with time or are of limited severity. Health effects of mixed aerosols of mixed aerosols of graphite and fog oil are similar to those produced by graphite flakes alone. Environmental impacts of fog oil-coated graphite flakes are not well known.

VizieR Online Data Catalog: FIR data of IR-bright dust-obscured galaxies (DOGs) (Toba+, 2017)

Science.gov (United States)

Toba, Y.; Nagao, T.; Wang, W.-H.; Matsuhara, H.; Akiyama, M.; Goto, T.; Koyama, Y.; Ohyama, Y.; Yamamura, I.

2017-11-01

We investigate the star-forming activity of a sample of infrared (IR)-bright dust-obscured galaxies (DOGs) that show an extreme red color in the optical and IR regime, (i-[22])AB>7.0. Combining an IR-bright DOG sample with the flux at 22μm>3.8mJy discovered by Toba & Nagao (2016ApJ...820...46T) with the IRAS faint source catalog version 2 and AKARI far-IR (FIR) all-sky survey bright source catalog version 2, we selected 109 DOGs with FIR data. For a subsample of seven IR-bright DOGs with spectroscopic redshifts (0.07DOGs and (2) the contribution of the active galactic nucleus to IR luminosity increases with IR luminosity. By comparing the stellar mass and SFR relation for our DOG sample and the literature, we found that most of the IR-bright DOGs lie significantly above the main sequence of star-forming galaxies at similar redshift, indicating that the majority of IRAS- or AKARI-detected IR-bright DOGs are starburst galaxies. (1 data file).

Effects of dietary amylose/amylopectin ratio on growth performance, feed utilization, digestive enzymes, and postprandial metabolic responses in juvenile obscure puffer Takifugu obscurus.

Science.gov (United States)

Liu, Xiang-he; Ye, Chao-xia; Ye, Ji-dan; Shen, Bi-duan; Wang, Chun-yan; Wang, An-li

2014-10-01

The effect of dietary amylose/amylopectin (AM/AP) ratio on growth, feed utilization, digestive enzyme activities, plasma parameters, and postprandial blood glucose responses was evaluated in juvenile obscure puffer, Takifugu obscurus. Five isonitrogenous (430 g kg(-1) crude protein) and isolipidic (90 g kg(-1) crude lipid) diets containing an equal starch level (250 g kg(-1) starch) with different AM/AP ratio diets of 0/25, 3/22, 6/19, 9/16 and 12/13 were formulated. Each experimental diet was fed to triplicate groups (25 fish per tank), twice daily during a period of 60 days. After the growth trial, a postprandial blood response test was carried out. Fish fed diet 6/19 showed best growth, feed efficiency and protein efficiency ratio. Hepatosomatic index, plasma total cholesterol concentration, liver glycogen and lipid content, and gluconokinase, pyruvate kinase and fructose-1,6-bisphosphatase activities were lower in fish fed highest AM/AP diet (12/13) than in fish fed the low-amylose diets. Activities of liver and intestinal trypsin in fish fed diet 3/22 and diet 6/19 were higher than in fish fed diet 9/16 and diet 12/13. Activities of liver and intestinal amylase and intestinal lipase, and starch digestibility were negatively correlated with dietary AM/AP ratio. Fish fed diet 3/22 and diet 6/19 showed higher plasma total amino acid concentration than fish fed the other diets, while plasma urea nitrogen concentration and activities of alanine aminotransferase and aspartate aminotransferase showed the opposite trend. Equal values were found for viscerosomatic index and condition factor, whole body and muscle composition, plasma high-density and low-density lipoprotein cholesterol concentrations, and activities of lipase and hexokinase and glucose-6-phosphatase in liver. Postprandial plasma glucose and triglyceride peak value of fish fed diet 12/13 were lower than in fish fed the low-amylose diets, and the peak time of plasma glucose was later than in fish fed the

Contingency blindness: location-identity binding mismatches obscure awareness of spatial contingencies and produce profound interference in visual working memory.

Science.gov (United States)

Fiacconi, Chris M; Milliken, Bruce

2012-08-01

The purpose of the present study was to highlight the role of location-identity binding mismatches in obscuring explicit awareness of a strong contingency. In a spatial-priming procedure, we introduced a high likelihood of location-repeat trials. Experiments 1, 2a, and 2b demonstrated that participants' explicit awareness of this contingency was heavily influenced by the local match in location-identity bindings. In Experiment 3, we sought to determine why location-identity binding mismatches produce such low levels of contingency awareness. Our results suggest that binding mismatches can interfere substantially with visual-memory performance. We attribute the low levels of contingency awareness to participants' inability to remember the critical location-identity binding in the prime on a trial-to-trial basis. These results imply a close interplay between object files and visual working memory.

NuSTAR observations of WISE J1036+0449, a galaxy at z ∼ 1 obscured by hot dust

DEFF Research Database (Denmark)

Ricci, C.; Assef, R. J.; Stern, D.

2017-01-01

Hot dust-obscured galaxies (hot DOGs), selected from Wide-Field Infrared Survey Explorer’s all-sky infrared survey, host some of the most powerful active galactic nuclei known and may represent an important stage in the evolution of galaxies. Most known hot DOGs are located at z > 1.5, due in part...... to a strong bias against identifying them at lower redshift related to the selection criteria. We present a new selection method that identifies 153 hot DOG candidates at z ~ 1, where they are significantly brighter and easier to study. We validate this approach by measuring a redshift z = 1.009 and finding...... the mid-infrared/X-ray correlation. We also find that other hot DOGs observed by X-ray facilities show a similar deficiency of X-ray flux. We discuss the origin of the X-ray weakness and the absorption properties of hot DOGs. Hot DOGs at z ≲ 1 could be excellent laboratories to probe the characteristics...

THE KILOPARSEC-SCALE STAR FORMATION LAW AT REDSHIFT 4: WIDESPREAD, HIGHLY EFFICIENT STAR FORMATION IN THE DUST-OBSCURED STARBURST GALAXY GN20

Energy Technology Data Exchange (ETDEWEB)

Hodge, J. A. [National Radio Astronomy Observatory, 520 Edgemont Road, Charlottesville, VA 22903 (United States); Riechers, D. [Department of Astronomy, Cornell University, Ithaca, New York, NY 14853 (United States); Decarli, R.; Walter, F. [Max-Planck-Institut für Astronomie, Königstuhl 17, D-69117 Heidelberg (Germany); Carilli, C. L. [National Radio Astronomy Observatory, P.O. Box 0, Socorro, NM 87801-0387 (United States); Daddi, E. [CEA, Laboratoire AIM-CNRS-Université Paris Diderot, Irfu/SAp, Orme des Merisiers, F-91191 Gif-sur-Yvette (France); Dannerbauer, H., E-mail: jhodge@nrao.edu [Universität Wien, Institut für Astrophysik, Türkenschanzstraße 17, 1180 Wien (Austria)

2015-01-01

We present high-resolution observations of the 880 μm (rest-frame FIR) continuum emission in the z = 4.05 submillimeter galaxy GN20 from the IRAM Plateau de Bure Interferometer (PdBI). These data resolve the obscured star formation (SF) in this unlensed galaxy on scales of 0.''3 × 0.''2 (∼2.1 × 1.3 kpc). The observations reveal a bright (16 ± 1 mJy) dusty starburst centered on the cold molecular gas reservoir and showing a bar-like extension along the major axis. The striking anti-correlation with the Hubble Space Telescope/Wide Field Camera 3 imaging suggests that the copious dust surrounding the starburst heavily obscures the rest-frame UV/optical emission. A comparison with 1.2 mm PdBI continuum data reveals no evidence for variations in the dust properties across the source within the uncertainties, consistent with extended SF, and the peak star formation rate surface density (119 ± 8 M {sub ☉} yr{sup –1} kpc{sup –2}) implies that the SF in GN20 remains sub-Eddington on scales down to 3 kpc{sup 2}. We find that the SF efficiency (SFE) is highest in the central regions of GN20, leading to a resolved SF law with a power-law slope of Σ{sub SFR} ∼ Σ{sub H{sub 2}{sup 2.1±1.0}}, and that GN20 lies above the sequence of normal star-forming disks, implying that the dispersion in the SF law is not due solely to morphology or choice of conversion factor. These data extend previous evidence for a fixed SFE per free-fall time to include the star-forming medium on ∼kiloparsec scales in a galaxy 12 Gyr ago.

Black hole growth and starburst activity at z = 0.6-4 in the Chandra Deep Field South. Host galaxies properties of obscured AGN

Science.gov (United States)

Brusa, M.; Fiore, F.; Santini, P.; Grazian, A.; Comastri, A.; Zamorani, G.; Hasinger, G.; Merloni, A.; Civano, F.; Fontana, A.; Mainieri, V.

2009-12-01

Aims: The co-evolution of host galaxies and the active black holes which reside in their centre is one of the most important topics in modern observational cosmology. Here we present a study of the properties of obscured active galactic nuclei (AGN) detected in the CDFS 1 Ms observation and their host galaxies. Methods: We limited the analysis to the MUSIC area, for which deep K-band observations obtained with ISAAC@VLT are available, ensuring accurate identifications of the counterparts of the X-ray sources as well as reliable determination of photometric redshifts and galaxy parameters, such as stellar masses and star formation rates. In particular, we: 1) refined the X-ray/infrared/optical association of 179 sources in the MUSIC area detected in the Chandra observation; 2) studied the host galaxies observed and rest frame colors and properties. Results: We found that X-ray selected (LX ⪆ 1042 erg s-1) AGN show Spitzer colors consistent with both AGN and starburst dominated infrared continuum; the latter would not have been selected as AGN from infrared diagnostics. The host galaxies of X-ray selected obscured AGN are all massive (Mast > 1010 M_⊙) and, in 50% of the cases, are also actively forming stars (1/SSFR mass up to a value of 30% at z > 1 and Mast > 3 × 1011 M_⊙, a fraction significantly higher than in the local Universe for AGN of similar luminosities. Tables [see full textsee full textsee full text] and [see full textsee full textsee full text] are only available in electronic form at http://www.aanda.org

Computed tomography versus digital subtraction angiography for the diagnosis of obscure gastrointestinal bleeding

Energy Technology Data Exchange (ETDEWEB)

Wildgruber, Moritz, E-mail: moritzwildgruber@ukmuenster.de [Institut für Röntgendiagnostik, Universitätsklinikum Regensburg, D-93053 Regensburg (Germany); Institut für klinische Radiologie, Universitätsklinikum Münster, D-48149 Münster (Germany); Wrede, Christian E. [Notfallzentrum, Helios Klinikum Berlin-Buch, D-13125 Berlin (Germany); Zorger, Niels [Institut für Radiologie, Neuroradiologie und Nuklearmedizin, Krankenhaus Barmherzige Brüder, D-93049 Regensburg (Germany); Müller-Wille, René; Hamer, Okka W. [Institut für Röntgendiagnostik, Universitätsklinikum Regensburg, D-93053 Regensburg (Germany); Zeman, Florian [Zentrum für Klinische Studien, Universitätsklinikum Regensburg, D-93053 Regensburg (Germany); Stroszczynski, Christian; Heiss, Peter [Institut für Röntgendiagnostik, Universitätsklinikum Regensburg, D-93053 Regensburg (Germany)

2017-03-15

Purpose: The diagnostic yield of computed tomography angiography (CTA) compared to digital subtraction angiography (DSA) for major obscure gastrointestinal bleeding (OGIB) is not known. Aim of the study was to prospectively evaluate the diagnostic yield of CTA versus DSA for the diagnosis of major OGIB. Material and methods: The institutional review board approved the study and informed consent was obtained from each patient. Patients with major OGIB were prospectively enrolled to undergo both CTA and DSA. Two blinded radiologists each reviewed the CTA and DSA images retrospectively and independently. Contrast material extravasation into the gastrointestinal lumen was considered diagnostic for active bleeding. Primary end point of the study was the diagnostic yield, defined as the frequency a technique identified an active bleeding or a potential bleeding lesion. The diagnostic yield of CTA and DSA were compared by McNemar's test. Results: 24 consecutive patients (11 men; median age 64 years) were included. CTA and DSA identified an active bleeding or a potential bleeding lesion in 92% (22 of 24 patients; 95% CI 72%–99%) and 29% (7 of 24 patients; 95% CI 12%–49%) of patients, respectively (p < 0.001). CTA and DSA identified an active bleeding in 42% (10 of 24; 95% CI 22%–63%) and 21% (5 of 24; 95% CI 7%–42%) of patients, respectively (p = 0.06). Conclusion: Due to the lower invasiveness and higher diagnostic yield CTA should be favored over DSA for the diagnosis of major OGIB.

Computed tomography versus digital subtraction angiography for the diagnosis of obscure gastrointestinal bleeding

International Nuclear Information System (INIS)

Wildgruber, Moritz; Wrede, Christian E.; Zorger, Niels; Müller-Wille, René; Hamer, Okka W.; Zeman, Florian; Stroszczynski, Christian; Heiss, Peter

2017-01-01

Purpose: The diagnostic yield of computed tomography angiography (CTA) compared to digital subtraction angiography (DSA) for major obscure gastrointestinal bleeding (OGIB) is not known. Aim of the study was to prospectively evaluate the diagnostic yield of CTA versus DSA for the diagnosis of major OGIB. Material and methods: The institutional review board approved the study and informed consent was obtained from each patient. Patients with major OGIB were prospectively enrolled to undergo both CTA and DSA. Two blinded radiologists each reviewed the CTA and DSA images retrospectively and independently. Contrast material extravasation into the gastrointestinal lumen was considered diagnostic for active bleeding. Primary end point of the study was the diagnostic yield, defined as the frequency a technique identified an active bleeding or a potential bleeding lesion. The diagnostic yield of CTA and DSA were compared by McNemar's test. Results: 24 consecutive patients (11 men; median age 64 years) were included. CTA and DSA identified an active bleeding or a potential bleeding lesion in 92% (22 of 24 patients; 95% CI 72%–99%) and 29% (7 of 24 patients; 95% CI 12%–49%) of patients, respectively (p < 0.001). CTA and DSA identified an active bleeding in 42% (10 of 24; 95% CI 22%–63%) and 21% (5 of 24; 95% CI 7%–42%) of patients, respectively (p = 0.06). Conclusion: Due to the lower invasiveness and higher diagnostic yield CTA should be favored over DSA for the diagnosis of major OGIB.

Interferometric follow-up of WISE hyper-luminous hot, dust-obscured galaxies

Energy Technology Data Exchange (ETDEWEB)

Wu, Jingwen; Wright, Edward L. [Department of Physics and Astronomy, University of California, Los Angeles, CA 90095 (United States); Bussmann, R. Shane [Harvard-Smithsonian Center for Astrophysics, 60 Garden St., MS78, Cambridge, MA 02138 (United States); Tsai, Chao-Wei; Eisenhardt, Peter R. M.; Stern, Daniel; Moustakas, Leonidas [Jet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Dr., Pasadena, CA 91109 (United States); Petric, Andreea [Institute for Astronomy, 2680 Woodlawn Drive, Honolulu, HI 96822-1839 (United States); Blain, Andrew [Department of Physics and Astronomy, University of Leicester, Leicester, LE1 7RH (United Kingdom); Bridge, Carrie R. [Division of Physics, Math, and Astronomy, California Institute of Technology, Pasadena, CA 91125 (United States); Benford, Dominic J. [NASA Goddard Space Flight Center, Greenbelt, MD 20771 (United States); Assef, Roberto J. [Núcleo de Astronomía de la Facultad de Ingeniería, Universidad Diego Portales, Av., Santiago, Ejército Libertador 441 (Chile); Gelino, Christopher R., E-mail: jingwen@astro.ucla.edu [Infrared Processing and Analysis Center, California Institute of Technology, Pasadena, CA 91125 (United States)

2014-09-20

The Wide-field Infrared Survey Explorer (WISE) has discovered an extraordinary population of hyper-luminous dusty galaxies that are faint in the two bluer passbands (3.4 μm and 4.6 μm) but are bright in the two redder passbands of WISE (12 μm and 22 μm). We report on initial follow-up observations of three of these hot, dust-obscured galaxies, or Hot DOGs, using the Combined Array for Research in Millimeter-wave Astronomy and the Submillimeter Array interferometer arrays at submillimeter/millimeter wavelengths. We report continuum detections at ∼1.3 mm of two sources (WISE J014946.17+235014.5 and WISE J223810.20+265319.7, hereafter W0149+2350 and W2238+2653, respectively), and upper limits to CO line emission at 3 mm in the observed frame for two sources (W0149+2350 and WISE J181417.29+341224.8, hereafter W1814+3412). The 1.3 mm continuum images have a resolution of 1''-2'' and are consistent with single point sources. We estimate the masses of cold dust are 2.0 × 10{sup 8} M {sub ☉} for W0149+2350 and 3.9 × 10{sup 8} M {sub ☉} for W2238+2653, comparable to cold dust masses of luminous quasars. We obtain 2σ upper limits to the molecular gas masses traced by CO, which are 3.3 × 10{sup 10} M {sub ☉} and 2.3 × 10{sup 10} M {sub ☉} for W0149+2350 and W1814+3412, respectively. We also present high-resolution, near-IR imaging with the WFC3 on the Hubble Space Telescope for W0149+2653 and with NIRC2 on Keck for W2238+2653. The near-IR images show morphological structure dominated by a single, centrally condensed source with effective radius less than 4 kpc. No signs of gravitational lensing are evident.

Study on the Hymenoptera parasitoid associated with Lepidoptera larvae in reforestation and agrosilvopastoral systems at Fazenda Canchim (Embrapa Pecuária Sudeste) São Carlos, SP, Brazil.

Science.gov (United States)

Pereira, A G; Silva, R B; Dias, M M; Penteado-Dias, A M

2015-11-01

The aim of this study was to characterize the local fauna of Hymenoptera parasitoids associated with Lepidoptera larvae in areas of reforestation and agrosilvopastoral systems at Fazenda Canchim (Embrapa Pecuária Sudeste, São Carlos, SP, Brazil). Lepidoptera larvae collected with entomological umbrella were kept in the laboratory until emergence of adults or their parasitoids. From those collected in the agrosilvopastoral system, emerged 267 specimens of hymenopteran parasitoids belonging to 16 genera: Braconidae, Agathidinae (Alabagrus), Braconinae (Bracon), Microgastrinae (Cotesia, Diolcogaster, Glyptapanteles, Pholetesor and Protapanteles), Orgilinae (Orgilus); Ichneumonidae, Campopleginae (Casinaria, Charops and Microcharops); Chalcididae, Chalcidinae (Brachymeria and Conura); Eulophidae, Entedoninae (Horismenus), Eulophinae (Elachertus and Euplectrus). From the Lepidoptera larvae collected in the reforestation, emerged 68 specimens of hymenopteran parasitoids, belonging to 8 genera: Chalcididae, Chalcidinae (Conura); Ichneumonidae, Pimplinae (Neotheronia), Campopleginae (Charops and Microcharops) and Braconidae, Microgastrinae (Apanteles, Diolcogaster, Distatrix, Glyptapanteles and Protapanteles). The results of this study suggest the occurrence of a wide variety of Hymenoptera parasitoids in the studied environments.

Study on the Hymenoptera parasitoid associated with Lepidoptera larvae in reforestation and agrosilvopastoral systems at Fazenda Canchim (Embrapa Pecuária Sudeste São Carlos, SP, Brazil

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A. G. Pereira

Full Text Available Abstract The aim of this study was to characterize the local fauna of Hymenoptera parasitoids associated with Lepidoptera larvae in areas of reforestation and agrosilvopastoral systems at Fazenda Canchim (Embrapa Pecuária Sudeste, São Carlos, SP, Brazil. Lepidoptera larvae collected with entomological umbrella were kept in the laboratory until emergence of adults or their parasitoids. From those collected in the agrosilvopastoral system, emerged 267 specimens of hymenopteran parasitoids belonging to 16 genera: Braconidae, Agathidinae (Alabagrus, Braconinae (Bracon, Microgastrinae (Cotesia, Diolcogaster, Glyptapanteles, Pholetesor and Protapanteles, Orgilinae (Orgilus; Ichneumonidae, Campopleginae (Casinaria, Charops and Microcharops; Chalcididae, Chalcidinae (Brachymeria and Conura; Eulophidae, Entedoninae (Horismenus, Eulophinae (Elachertus and Euplectrus. From the Lepidoptera larvae collected in the reforestation, emerged 68 specimens of hymenopteran parasitoids, belonging to 8 genera: Chalcididae, Chalcidinae (Conura; Ichneumonidae, Pimplinae (Neotheronia, Campopleginae (Charops and Microcharops and Braconidae, Microgastrinae (Apanteles, Diolcogaster, Distatrix, Glyptapanteles and Protapanteles. The results of this study suggest the occurrence of a wide variety of Hymenoptera parasitoids in the studied environments.

Thomas: o primeiro blanchotiano = Thomas: the first Blanchotian

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Pimentel, Davi Andrade

2013-01-01

Full Text Available Este artigo analisa a narrativa Thomas l’obscur, de Maurice Blanchot, a partir da configuração da outra noite blanchotiana, noite que apresenta a falta e a ausência da palavra no que ela tem de mais agressiva, de mais excessiva e de mais absurdamente maravilhosa. Neste artigo, tenho como interlocutor teórico os escritos sobre literatura do próprio autor. O interesse nesse diálogo consiste em apresentar a fusão apaixonada de seus escritos ficcionais e teóricos. Em Maurice Blanchot, não há pontos de isolamento e nem de divergência entre seus dois pólos de escritura, mas sim uma complementação, uma convergência, entre o que denominamos de ficção e de teoria

Molecular Outflow and Feedback in an Obscured Quasar at z˜1.5 Revealed by ALMA

Science.gov (United States)

Brusa, Marcella

2017-11-01

We imaged with ALMA and ARGOS/LUCI the molecular gas and the dust and stellar continuum in XID2028, an obscured QSO at z=1.593, where the presence of a massive outflow in the ionized gas component traced by the [O III]5007 emission has been resolved up to 10 kpc. This target does represent a unique test case to study QSO 'feedback in action' at the peak epoch of AGN- galaxy coevolution. The QSO has been detected both in the CO(5-4) transition and in the 1.3mm continuum, with emissions confined in the central ( consumption conditions in XID2028, possibly due to feedback effects on the host galaxy. Finally, we observe an asymmetric profile of the CO(5-4) line, which suggests the presence of high velocity gas up to 700 km/s. An image of the blueshfited and redshifted CO wings provides the first detection of a spatially resolved, galaxy-scale molecular outflow at high-z, extended in opposite directions with the approaching component spatially coincident with the ionised gas outflow. The resolved, molecular outflow appear to be cospatial with the component observed int the ionised gas. XID2028 therefore represents the first example of molecular and ionised kpc scales outflows at high-z.

Probing highly obscured, self-absorbed galaxy nuclei with vibrationally excited HCN

Science.gov (United States)

Aalto, S.; Martín, S.; Costagliola, F.; González-Alfonso, E.; Muller, S.; Sakamoto, K.; Fuller, G. A.; García-Burillo, S.; van der Werf, P.; Neri, R.; Spaans, M.; Combes, F.; Viti, S.; Mühle, S.; Armus, L.; Evans, A.; Sturm, E.; Cernicharo, J.; Henkel, C.; Greve, T. R.

2015-12-01

We present high resolution (0.̋4) IRAM PdBI and ALMA mm and submm observations of the (ultra) luminous infrared galaxies ((U)LIRGs) IRAS 17208-0014, Arp220, IC 860 and Zw049.057 that reveal intense line emission from vibrationally excited (ν2 = 1) J = 3-2 and 4-3 HCN. The emission is emerging from buried, compact (r 5 × 1013 L⊙ kpc-2. These nuclei are likely powered by accreting supermassive black holes (SMBHs) and/or hot (>200 K) extreme starbursts. Vibrational, ν2 = 1, lines of HCN are excited by intense 14 μm mid-infrared emission and are excellent probes of the dynamics, masses, and physical conditions of (U)LIRG nuclei when H2 column densities exceed 1024 cm-2. It is clear that these lines open up a new interesting avenue to gain access to the most obscured AGNs and starbursts. Vibrationally excited HCN acts as a proxy for the absorbed mid-infrared emission from the embedded nuclei, which allows for reconstruction of the intrinsic, hotter dust SED. In contrast, we show strong evidence that the ground vibrational state (ν = 0), J = 3-2and 4-3 rotational lines of HCN and HCO+ fail to probe the highly enshrouded, compact nuclear regions owing to strong self- and continuum absorption. The HCN and HCO+ line profiles are double-peaked because of the absorption and show evidence of non-circular motions - possibly in the form of in- or outflows. Detections of vibrationally excited HCN in external galaxies are so far limited to ULIRGs and early-type spiral LIRGs, and we discuss possible causes for this. We tentatively suggest that the peak of vibrationally excited HCN emission is connected to a rapid stage of nuclear growth, before the phase of strong feedback. Based on observations carried out with the IRAM Plateau de Bure and ALMA Interferometers. IRAM is supported by INSU/CNRS (France), MPG (Germany), and IGN (Spain). ALMA is a partnership of ESO (representing its member states), NSF (USA), and NINS (Japan), together with NRC (Canada) and NSC and ASIAA

NuSTAR J033202-2746.8: Direct constraints on the Compton reflection in a heavily obscured quasar at z ≈ 2

Energy Technology Data Exchange (ETDEWEB)

Del Moro, A.; Mullaney, J. R.; Alexander, D. M.; Aird, J. A.; Gandhi, P. [Department of Physics, Durham University, South Road, Durham, DH1 3LE (United Kingdom); Comastri, A.; Vignali, C.; Gilli, R. [INAF-Osservatorio Astronomico di Bologna, Via Ranzani 1, I-40127 Bologna (Italy); Bauer, F. E. [Instituto de Astrofísica, Facultad de Física, Pontificia Universidad Católica de Chile, 306, Santiago 22 (Chile); Treister, E. [Departamento de Astronomía, Universidad de Concepción, Casilla 160-C, Concepción (Chile); Stern, D. [Jet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Drive, Mail Stop 169-221, Pasadena, CA 91109 (United States); Civano, F. [Department of Physics and Astronomy, Dartmouth College, 6127 Wilder Laboratory, Hanover, NH 03755 (United States); Ranalli, P. [National Observatory of Athens, Institute of Astronomy, Astrophysics, Space Applications and Remote Sensing, Metaxa and Pavlou St., 15236 Penteli (Greece); Ballantyne, D. R. [Center for Relativistic Astrophysics, School of Physics, Georgia Institute of Technology, Atlanta, GA 30332 (United States); Baloković, M. [Cahill Center for Astrophysics, 1216 East California Boulevard, California Institute of Technology, Pasadena, CA 91125 (United States); Boggs, S. E. [Space Sciences Laboratory, University of California, Berkeley, CA 94720 (United States); Brandt, W. N. [Department of Astronomy and Astrophysics, 525 Davey Lab, The Pennsylvania State University, University Park, PA 16802 (United States); Christensen, F. E. [DTU Space-National Space Institute, Technical University of Denmark, Elektrovej 327, DK-2800 Lyngby (Denmark); Craig, W. W. [Lawrence Livermore National Laboratory, Livermore, CA 94550 (United States); Hailey, C. J., E-mail: agnese.del-moro@durham.ac.uk [Columbia Astrophysics Laboratory, 550 W 120th Street, Columbia University, NY 10027 (United States); and others

2014-05-01

We report Nuclear Spectroscopic Telescope Array (NuSTAR) observations of NuSTAR J033202-2746.8, a heavily obscured, radio-loud quasar detected in the Extended Chandra Deep Field-South, the deepest layer of the NuSTAR extragalactic survey (∼400 ks, at its deepest). NuSTAR J033202-2746.8 is reliably detected by NuSTAR only at E > 8 keV and has a very flat spectral slope in the NuSTAR energy band (Γ=0.55{sub −0.64}{sup +0.62}; 3-30 keV). Combining the NuSTAR data with extremely deep observations by Chandra and XMM-Newton (4 Ms and 3 Ms, respectively), we constrain the broad-band X-ray spectrum of NuSTAR J033202-2746.8, indicating that this source is a heavily obscured quasar (N{sub H}=5.6{sub −0.8}{sup +0.9}×10{sup 23} cm{sup –2}) with luminosity L {sub 10-40} {sub keV} ≈ 6.4 × 10{sup 44} erg s{sup –1}. Although existing optical and near-infrared (near-IR) data, as well as follow-up spectroscopy with the Keck and VLT telescopes, failed to provide a secure redshift identification for NuSTAR J033202-2746.8, we reliably constrain the redshift z = 2.00 ± 0.04 from the X-ray spectral features (primarily from the iron K edge). The NuSTAR spectrum shows a significant reflection component (R=0.55{sub −0.37}{sup +0.44}), which was not constrained by previous analyses of Chandra and XMM-Newton data alone. The measured reflection fraction is higher than the R ∼ 0 typically observed in bright radio-loud quasars such as NuSTAR J033202-2746.8, which has L {sub 1.4} {sub GHz} ≈ 10{sup 27} W Hz{sup –1}. Constraining the spectral shape of active galactic nuclei (AGNs), including bright quasars, is very important for understanding the AGN population, and can have a strong impact on the modeling of the X-ray background. Our results show the importance of NuSTAR in investigating the broad-band spectral properties of quasars out to high redshift.

Performing "Chinese-ness" in Singkawang

NARCIS (Netherlands)

Ong, C.E.; Ormond, M.E.; Sulianti, Dian

2017-01-01

Through an examination of two festivals – Qing Ming and Cap Go Meh – in the town of Singkawang in Indonesian Borneo (Kalimantan), we show how Singkawang-bound Chinese Indonesian tourists and their Singkawang-based relatives produce a diasporic heritage network through ‘moorings’ generated by both

Evaluate and characterize mechanisms controlling transport, fate, and effects of army smokes in the aerosol wind tunnel: Transport, transformations, fate, and terrestrial ecological effects of hexachloroethane obscurant smokes

Energy Technology Data Exchange (ETDEWEB)

Cataldo, D.A.; Ligotke, M.W.; Bolton, H. Jr.; Fellows, R.J.; Van Voris, P.; McVeety, B.D.; Li, Shu-mei W.; McFadden, K.M.

1989-09-01

The terrestrial transport, chemical fate, and ecological effects of hexachloroethane (HC) smoke were evaluated under controlled wind tunnel conditions. The primary objectives of this research program are to characterize and assess the impacts of smoke and obscurants on: (1) natural vegetation characteristic of US Army training sites in the United States; (2) physical and chemical properties of soils representative of these training sites; and (3) soil microbiological and invertebrate communities. Impacts and dose/responses were evaluated based on exposure scenarios, including exposure duration, exposure rate, and sequential cumulative dosing. Key to understanding the environmental impacts of HC smoke/obscurants is establishing the importance of environmental parameters such as relative humidity and wind speed on airborne aerosol characteristics and deposition to receptor surfaces. Direct and indirect biotic effects were evaluated using five plant species and two soil types. HC aerosols were generated in a controlled atmosphere wind tunnel by combustion of hexachloroethane mixtures prepared to simulate normal pot burn rates and conditions. The aerosol was characterized and used to expose plant, soil, and other test systems. Particle sizes of airborne HC ranged from 1.3 to 2.1 {mu}m mass median aerodynamic diameter (MMAD), and particle size was affected by relative humidity over a range of 20% to 85%. Air concentrations employed ranged from 130 to 680 mg/m{sup 3}, depending on exposure scenario. Chlorocarbon concentrations within smokes, deposition rates for plant and soil surfaces, and persistence were determined. The fate of principal inorganic species (Zn, Al, and Cl) in a range of soils was assessed.

STAR FORMATION AND DUST OBSCURATION AT z ∼ 2: GALAXIES AT THE DAWN OF DOWNSIZING

International Nuclear Information System (INIS)

Pannella, M.; Carilli, C. L.; Owen, F. N.; Strazzullo, V.; Daddi, E.; Aussel, H.; McCracken, H. J.; Mellier, Y.; Renzini, A.; Civano, F.; Koekemoer, A. M.; Schinnerer, E.; Scoville, N.; Smolcic, V.; Salvato, M.; Taniguchi, Y.; Kneib, J. P.; Ilbert, O.; Thompson, D.; Willott, C. J.

2009-01-01

We present first results of a study aimed to constrain the star formation rate (SFR) and dust content of galaxies at z ∼ 2. We use a sample of BzK-selected star-forming galaxies, drawn from the Cosmic Evolution Survey, to perform a stacking analysis of their 1.4 GHz radio continuum as a function of different stellar population properties, after cleaning the sample from contamination by active galactic nuclei. Dust unbiased SFRs are derived from radio fluxes assuming the local radio-IR correlation. The main results of this work are: (1) specific star formation rate (SSFR)s are constant over about 1 dex in stellar mass and up to the highest stellar mass probed, (2) the dust attenuation is a strong function of galaxy stellar mass with more massive galaxies being more obscured than lower mass objects, (3) a single value of the UV extinction applied to all galaxies would lead to a gross underestimate of the SFR in massive galaxies, (4) correcting the observed UV luminosities for dust attenuation based on the Calzetti recipe provides results in very good agreement with the radio derived ones, (5) the mean SSFR of our sample steadily decreases by a factor of ∼4 with decreasing redshift from z = 2.3 to 1.4 and a factor of ∼40 down the local universe. These empirical SFRs would cause galaxies to dramatically overgrow in mass if maintained all the way to low redshifts; we suggest that this does not happen because star formation is progressively quenched, likely starting from the most massive galaxies.

Upper gastrointestinal findings detected by capsule endoscopy in obscure gastrointestinal bleeding Hallazgos digestivos altos de la cápsula endoscópica en la hemorragia digestiva de origen oscuro

Directory of Open Access Journals (Sweden)

B. Velayos

2009-01-01

Full Text Available Objective: we analyzed our experience with the use of capsule endoscopy in areas that can be explored with gastroscopy to justify obscure bleeding, as well as the outcome after a new recommended gastroscopy in order to determine if a second gastroscopy before the capsule study can provide any benefit in the management of this disease. Methods: we retrospectively studied 82 patients who were explored with capsule endoscopy for obscure gastrointestinal bleeding who had undergone previously only one gastroscopy. Findings in the zones which were accessible by gastroscopy were normal, mild/known and severe/unknown. In the latter cases we recommended a second gastroscopy, and their treatment and outcome were subjected to further study. Results: capsule endoscopy did not find any unknown esophageal findings. In 63% of cases, no gastric or duodenal lesions were shown; in 20%, lesions were mild or had been previously diagnosed, and in 17%, a new gastroscopy was recommended due to the discovery of an unknown condition which could be the cause of the obscure bleeding. This new information brought about a change in treatment for 78% of patients in this group, all of whom improved from their illness. Capsule endoscopy found significant intercurrent alterations in the small intestine in only 14% of cases. Conclusions: the performance of a second gastroscopy, previous to capsule endoscopy, in the study of obscure gastrointestinal bleeding can offer benefits in diagnostic terms and may introduce therapeutic changes. A detailed analysis of the upper tract frames in intestinal capsule endoscopy studies is mandatory since it may provide relevant information with clinical impact on the management of these patients.Objetivo: hemos analizado los hallazgos que la cápsula endoscópica aportó de las zonas accesibles a una gastroscopia que podrían justificar un sangrado digestivo oscuro, así como la evolución de estos enfermos tras la nueva gastroscopia recomendada

ALMA observations of the host galaxy of GRB 090423 at z = 8.23: deep limits on obscured star formation 630 million years after the big bang

Energy Technology Data Exchange (ETDEWEB)

Berger, E.; Zauderer, B. A.; Chary, R.-R.; Laskar, T.; Chornock, R.; Davies, J. E. [Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138 (United States); Tanvir, N. R. [Department of Physics and Astronomy, University of Leicester, University Road, Leicester LE1 7RH (United Kingdom); Stanway, E. R.; Levan, A. J. [Department of Physics, University of Warwick, Gibbet Hill Road, Coventry CV4 7AL (United Kingdom); Levesque, E. M. [CASA, University of Colorado UCB 389, Boulder, CO 80309 (United States)

2014-12-01

We present rest-frame far-infrared (FIR) and optical observations of the host galaxy of GRB 090423 at z = 8.23 from the Atacama Large Millimeter Array (ALMA) and the Spitzer Space Telescope, respectively. The host remains undetected to 3σ limits of F {sub ν}(222 GHz) ≲ 33 μJy and F {sub ν}(3.6 μm) ≲ 81 nJy. The FIR limit is about 20 times fainter than the luminosity of the local ULIRG Arp 220 and comparable to the local starburst M 82. Comparing this with model spectral energy distributions, we place a limit on the infrared (IR) luminosity of L {sub IR}(8-1000 μm) ≲ 3 × 10{sup 10} L {sub ☉}, corresponding to a limit on the obscured star formation rate of SFR{sub IR}≲5 M {sub ☉} yr{sup –1}. For comparison, the limit on the unobscured star formation rate from Hubble Space Telescope rest-frame ultraviolet (UV) observations is SFR{sub UV} ≲ 1 M {sub ☉} yr{sup –1}. We also place a limit on the host galaxy stellar mass of M {sub *} ≲ 5 × 10{sup 7} M {sub ☉} (for a stellar population age of 100 Myr and constant star formation rate). Finally, we compare our millimeter observations to those of field galaxies at z ≳ 4 (Lyman break galaxies, Lyα emitters, and submillimeter galaxies) and find that our limit on the FIR luminosity is the most constraining to date, although the field galaxies have much larger rest-frame UV/optical luminosities than the host of GRB 090423 by virtue of their selection techniques. We conclude that GRB host galaxies at z ≳ 4, especially those with measured interstellar medium metallicities from afterglow spectroscopy, are an attractive sample for future ALMA studies of high redshift obscured star formation.

HIGH-REDSHIFT DUST OBSCURED GALAXIES: A MORPHOLOGY-SPECTRAL ENERGY DISTRIBUTION CONNECTION REVEALED BY KECK ADAPTIVE OPTICS

International Nuclear Information System (INIS)

Melbourne, J.; Matthews, K.; Soifer, B. T.

2009-01-01

A simple optical to mid-IR color selection, R - [24]>14, i.e., f ν (24 μm)/f ν (R) ∼> 1000, identifies highly dust obscured galaxies (DOGs) with typical redshifts of z ∼ 2 ± 0.5. Extreme mid-IR luminosities (L IR > 10 12-14 ) suggest that DOGs are powered by a combination of active galactic nuclei (AGNs) and star formation, possibly driven by mergers. In an effort to compare their photometric properties with their rest-frame optical morphologies, we obtained high-spatial resolution (0.''05-0.''1) Keck Adaptive Optics K'-band images of 15 DOGs. The images reveal a wide range of morphologies, including small exponential disks (eight of 15), small ellipticals (four of 15), and unresolved sources (two of 15). One particularly diffuse source could not be classified because of low signal-to-noise ratio. We find a statistically significant correlation between galaxy concentration and mid-IR luminosity, with the most luminous DOGs exhibiting higher concentration and smaller physical size. DOGs with high concentration also tend to have spectral energy distributions (SEDs) suggestive of AGN activity. Thus, central AGN light may be biasing the morphologies of the more luminous DOGs to higher concentration. Conversely, more diffuse DOGs tend to show an SED shape suggestive of star formation. Two of 15 in the sample show multiple resolved components with separations of ∼1 kpc, circumstantial evidence for ongoing mergers.

WITNESSING THE KEY EARLY PHASE OF QUASAR EVOLUTION: AN OBSCURED ACTIVE GALACTIC NUCLEUS PAIR IN THE INTERACTING GALAXY IRAS 20210+1121

International Nuclear Information System (INIS)

Piconcelli, Enrico; Fiore, Fabrizio; Maiolino, Roberto; Nicastro, Fabrizio; Vignali, Cristian; Bianchi, Stefano; Mathur, Smita; Guainazzi, Matteo; Lanzuisi, Giorgio

2010-01-01

We report the discovery of an active galactic nucleus (AGN) pair in the interacting galaxy system IRAS 20210+1121 at z = 0.056. An XMM-Newton observation reveals the presence of an obscured (N H ∼ 5 x 10 23 cm -2 ), Seyfert-like (L 2-10keV = 4.7 x 10 42 erg s -1 ) nucleus in the northern galaxy, which lacks unambiguous optical AGN signatures. Our spectral analysis also provides strong evidence that the IR-luminous southern galaxy hosts a Type 2 quasar embedded in a bright starburst emission. In particular, the X-ray primary continuum from the nucleus appears totally depressed in the XMM-Newton band as expected in the case of a Compton-thick absorber, and only the emission produced by Compton scattering ('reflection') of the continuum from circumnuclear matter is seen. As such, IRAS 20210+1121 seems to provide an excellent opportunity to witness a key, early phase in the quasar evolution predicted by the theoretical models of quasar activation by galaxy collisions.

INFRARED LUMINOSITIES AND DUST PROPERTIES OF z ∼ 2 DUST-OBSCURED GALAXIES

International Nuclear Information System (INIS)

Bussmann, R. S.; Dey, Arjun; Jannuzi, B. T.; Borys, C.; Desai, V.; Sheth, K.; Soifer, B. T.; Le Floc'h, E.; Melbourne, J.

2009-01-01

We present SHARC-II 350 μm imaging of twelve 24 μm bright (F 24μm > 0.8 mJy) Dust-Obscured Galaxies (DOGs) and Combined Array for Research in Millimeter-wave Astronomy (CARMA) 1 mm imaging of a subset of two DOGs. These objects are selected from the Booetes field of the NOAO Deep Wide-Field Survey. Detections of four DOGs at 350 μm imply infrared (IR) luminosities which are consistent to within a factor of 2 of expectations based on a warm-dust spectral energy distribution (SED) scaled to the observed 24 μm flux density. The 350 μm upper limits for the 8 non-detected DOGs are consistent with both Mrk 231 and M82 (warm-dust SEDs), but exclude cold dust (Arp 220) SEDs. The two DOGs targeted at 1 mm were not detected in our CARMA observations, placing strong constraints on the dust temperature: T dust > 35-60 K. Assuming these dust properties apply to the entire sample, we find dust masses of ∼3 x 10 8 M sun . In comparison to other dusty z ∼ 2 galaxy populations such as submillimeter galaxies (SMGs) and other Spitzer-selected high-redshift sources, this sample of DOGs has higher IR luminosities (2 x 10 13 L sun versus 6 x 10 12 L sun for the other galaxy populations) that are driven by warmer dust temperatures (>35-60 K versus ∼30 K) and lower inferred dust masses (3 x 10 8 M sun versus 3 x 10 9 M sun ). Wide-field Herschel and Submillimeter Common-User Bolometer Array-2 surveys should be able to detect hundreds of these power-law-dominated DOGs. We use the existing Hubble Space Telescope and Spitzer/InfraRed Array Camera data to estimate stellar masses of these sources and find that the stellar to gas mass ratio may be higher in our 24 μm bright sample of DOGs than in SMGs and other Spitzer-selected sources. Although much larger sample sizes are needed to provide a definitive conclusion, the data are consistent with an evolutionary trend in which the formation of massive galaxies at z ∼ 2 involves a submillimeter bright, cold-dust, and star

Travels Through Heterotopia: The Textual Realms of Patrick Modiano's Rue des Boutiques Obscures and Mikhail Kuraev's Kapitan Dikshtein

Directory of Open Access Journals (Sweden)

Vitaly Chernetsky

1998-06-01

Full Text Available Within contemporary prose, one distinct mode or paradigm that can be discerned is constituted by the texts that daringly tackle the dark, suppressed, erased parts of our history and mentality; however, they approach this task not by way of self-righteous denunciatory investigations, but by provocatively problematizing the most established everyday facts, by depriving the reader of the possibility of even conceiving any firm ground of the stable construct of an origin or a self-identification—historically and culturally. Their irreverent and playful deconstruction of the all-pervasive national cultural mythologies has mounted a powerful challenge to ideological constructs big and small. This article considers two representative examples of texts of this kind, which the author proposes to call heterotopic: Patrick Modiano's Rue des Boutiques Obscures and Mikhail Kuraev's Kapitan Dikshtein . It offers an attempt at defining this paradigm through a reading of these two novels, drawing upon Michel Foucault's usage of the term "heterotopia" for the purpose of designating the "other" cultural spaces of our civilization, as well as on Deleuze and Guattari's concept of "minor literature" and the work of several other theorists. The texts of the kind exemplified by these two novels are considered as an instance of successful partaking in the project of cognitive mapping, which has been proposed by Fredric Jameson and others as the positive political edge of postmodern culture.

The Role of the Most Luminous Obscured AGNs in Galaxy Assembly at z ∼ 2

Energy Technology Data Exchange (ETDEWEB)

Farrah, Duncan [Department of Physics, Virginia Tech, Blacksburg, VA 24061 (United States); Petty, Sara [Green Science Policy Institute, Berkeley, CA 94709 (United States); Connolly, Brian [Cincinnati Children’s Hospital Medical Center, 3333 Burnet Avenue, Cincinnati, OH 45229 (United States); Blain, Andrew [Department of Physics and Astronomy, University of Leicester, Leicester LE1 7RH (United Kingdom); Efstathiou, Andreas [School of Sciences, European University Cyprus, Diogenes Street, Engomi, 1516 Nicosia (Cyprus); Lacy, Mark [National Radio Astronomy Observatory, 520 Edgemont Road, Charlottesville, VA 22903 (United States); Stern, Daniel; Bridge, Carrie; Eisenhardt, Peter; Moustakas, Leonidas [Jet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Drive, Pasadena, CA 91109 (United States); Lake, Sean; Tsai, Chao-Wei [Physics and Astronomy Department, University of California, Los Angeles, CA 90095 (United States); Jarrett, Tom [Department of Astronomy, University of Cape Town, 7700 Rondebosch, Capetown 7700 (South Africa); Benford, Dominic [Observational Cosmology Lab., Code 665, NASA at Goddard Space Flight Center, Greenbelt, MD 20771 (United States); Jones, Suzy [Department of Space, Earth, and Environment, Chalmers University of Technology, Onsala Space Observatory, SE-43992 Onsala (Sweden); Assef, Roberto [Núcleo de Astronomía de la Facultad de Ingeniería, Universidad Diego Portales, Av. Ejército Libertador 441, Santiago (Chile); Wu, Jingwen [National Astronomical Observatories, Chinese Academy of Sciences, 20A Datun Road, Chaoyang District, Beijing, 100012 (China)

2017-08-01

We present Hubble Space Telescope WFC3 F160W imaging and infrared spectral energy distributions for 12 extremely luminous, obscured active galactic nuclei (AGNs) at 1.8 < z < 2.7 selected via “hot, dust-obscured” mid-infrared colors. Their infrared luminosities span (2–15) × 10{sup 13} L {sub ⊙}, making them among the most luminous objects in the universe at z ∼ 2. In all cases, the infrared emission is consistent with arising at least for the most part from AGN activity. The AGN fractional luminosities are higher than those in either submillimeter galaxies or AGNs selected via other mid-infrared criteria. Adopting the G , M {sub 20}, and A morphological parameters, together with traditional classification boundaries, infers that three-quarters of the sample are mergers. Our sample does not, however, show any correlation between the considered morphological parameters and either infrared luminosity or AGN fractional luminosity. Moreover, the asymmetries and effective radii of our sample are distributed identically to those of massive galaxies at z ∼ 2. We conclude that our sample is not preferentially associated with mergers, though a significant merger fraction is still plausible. Instead, we propose that our sample includes examples of the massive galaxy population at z ∼ 2 that harbor a briefly luminous, “flickering” AGN and in which the G and M {sub 20} values have been perturbed due to either the AGN and/or the earliest formation stages of a bulge in an inside-out manner. Furthermore, we find that the mass assembly of the central black holes in our sample leads the mass assembly of any bulge component. Finally, we speculate that our sample represents a small fraction of the immediate antecedents of compact star-forming galaxies at z ∼ 2.

Capsule Endoscopy in the Assessment of Obscure Gastrointestinal Bleeding: An Evidence-Based Analysis

Science.gov (United States)

2015-01-01

Background Obscure gastrointestinal bleeding (OGIB) is defined as persistent or recurrent bleeding associated with negative findings on upper and lower gastrointestinal (GI) endoscopic evaluations. The diagnosis and management of patients with OGIB is particularly challenging because of the length and complex loops of the small intestine. Capsule endoscopy (CE) is 1 diagnostic modality that is used to determine the etiology of bleeding. Objectives The objective of this analysis was to review the diagnostic accuracy, safety, and impact on health outcomes of CE in patients with OGIB in comparison with other diagnostic modalities. Data Sources A literature search was performed using Ovid MEDLINE, Ovid MEDLINE In-Process and Other Non-Indexed Citations, Ovid Embase, the Wiley Cochrane Library, and the Centre for Reviews and Dissemination database, for studies published between 2007 and 2013. Review Methods Data on diagnostic accuracy, safety, and impact on health outcomes were abstracted from included studies. Quality of evidence was assessed using Grading of Recommendations Assessment, Development, and Evaluation (GRADE). Results The search yielded 1,189 citations, and 24 studies were included. Eight studies reported diagnostic accuracy comparing CE with other diagnostic modalities. Capsule endoscopy has a higher sensitivity and lower specificity than magnetic resonance enteroclysis, computed tomography, and push enteroscopy. Capsule endoscopy has a good safety profile with few adverse events, although comparative safety data with other diagnostic modalities are limited. Capsule endoscopy is associated with no difference in patient health-related outcomes such as rebleeding or follow-up treatment compared with push enteroscopy, small-bowel follow-through, and angiography. Limitations There was significant heterogeneity in estimates of diagnostic accuracy, which prohibited a statistical summary of findings. The analysis was also limited by the fact that there is no

NESSE - New Standards in Sample Environment

International Nuclear Information System (INIS)

Schober, H.; Lelievre-Berna, E.

2011-01-01

The actual sample environment equipments suite has been designed for instruments built a few decades ago. Since then, we have considerably improved the ILL instruments and the experiments are slowed down by the performance of the sample environment. We propose to establish a new standard that will permit to exploit the new-generation instruments and to develop the environments not presently available for investigating novel scientific challenges. Not only we need reliable equipments covering very large ranges of temperature, pressure, magnetic and electric fields, we must also be able to change the physical parameters much more rapidly as well as exchanging samples automatically. Further to these needs, there are many scientific challenges that cannot be investigated without specific equipment presently unavailable at ILL. For example, among many subjects, high-pressure gas-handling systems are required to improve the storage of hydrogen; specific pressure cells would contribute to the optimization of the food distribution and ultra-high temperature furnaces would allow us to investigate the preparation process of ceramics, cement and refracting materials

Jekyll & Hyde: quiescence and extreme obscuration in a pair of massive galaxies 1.5 Gyr after the Big Bang

Science.gov (United States)

Schreiber, C.; Labbé, I.; Glazebrook, K.; Bekiaris, G.; Papovich, C.; Costa, T.; Elbaz, D.; Kacprzak, G. G.; Nanayakkara, T.; Oesch, P.; Pannella, M.; Spitler, L.; Straatman, C.; Tran, K.-V.; Wang, T.

2018-03-01

We obtained ALMA spectroscopy and deep imaging to investigate the origin of the unexpected sub-millimeter emission toward the most distant quiescent galaxy known to date, ZF-COSMOS-20115 at z = 3.717. We show here that this sub-millimeter emission is produced by another massive (M* 1011 M⊙), compact (r1/2 = 0.67 ± 0.14 kpc) and extremely obscured galaxy (AV 3.5), located only 0.43'' (3.1 kpc) away from the quiescent galaxy. We dub the quiescent and dusty galaxies Jekyll and Hyde, respectively. No dust emission is detected at the location of the quiescent galaxy, implying SFR < 13 M⊙ yr-1 which is the most stringent upper limit ever obtained for a quiescent galaxy at these redshifts. The two sources are spectroscopically confirmed to lie at the same redshift thanks to the detection of [C II]158 in Hyde (z = 3.709), which provides one the few robust redshifts for a highly-obscured "H-dropout" galaxy (H - [4.5] = 5.1 ± 0.8). The [C II] line shows a clear rotating-disk velocity profile which is blueshifted compared to the Balmer lines of Jekyll by 549 ± 60 km s-1, demonstrating that it is produced by another galaxy. Careful de-blending of the Spitzer imaging confirms the existence of this new massive galaxy, and its non-detection in the Hubble images requires extremely red colors and strong attenuation by dust. Full modeling of the UV-to-far-IR emission of both galaxies shows that Jekyll has fully quenched at least 200Myr prior to observation and still presents a challenge for models, while Hyde only harbors moderate star-formation with SFR ≲ 120 M⊙ yr-1, and is located at least a factor 1.4 below the z 4 main sequence. Hyde could also have stopped forming stars less than 200 Myr before being observed; this interpretation is also suggested by its compactness comparable to that of z 4 quiescent galaxies and its low [C II]/FIR ratio, but significant on-going star-formation cannot be ruled out. Lastly, we find that despite its moderate SFR, Hyde hosts a dense

ALMA Observations of the Host Galaxy of GRB 090423 at z = 8.23: Deep Limits on Obscured Star Formation 630 Million Years after the Big Bang

Science.gov (United States)

Berger, E.; Zauderer, B. A.; Chary, R.-R.; Laskar, T.; Chornock, R.; Tanvir, N. R.; Stanway, E. R.; Levan, A. J.; Levesque, E. M.; Davies, J. E.

2014-12-01

We present rest-frame far-infrared (FIR) and optical observations of the host galaxy of GRB 090423 at z = 8.23 from the Atacama Large Millimeter Array (ALMA) and the Spitzer Space Telescope, respectively. The host remains undetected to 3σ limits of F ν(222 GHz) Space Telescope rest-frame ultraviolet (UV) observations is SFRUV ~ 4 (Lyman break galaxies, Lyα emitters, and submillimeter galaxies) and find that our limit on the FIR luminosity is the most constraining to date, although the field galaxies have much larger rest-frame UV/optical luminosities than the host of GRB 090423 by virtue of their selection techniques. We conclude that GRB host galaxies at z >~ 4, especially those with measured interstellar medium metallicities from afterglow spectroscopy, are an attractive sample for future ALMA studies of high redshift obscured star formation.

Seafood substitutions obscure patterns of mercury contamination in Patagonian toothfish (Dissostichus eleginoides or "Chilean sea bass".

Directory of Open Access Journals (Sweden)

Peter B Marko

Full Text Available Seafood mislabeling distorts the true abundance of fish in the sea, defrauds consumers, and can also cause unwanted exposure to harmful pollutants. By combining genetic data with analyses of total mercury content, we have investigated how species substitutions and fishery-stock substitutions obscure mercury contamination in Patagonian toothfish (Dissostichus eleginoides, also known as "Chilean sea bass". Patagonian toothfish show wide variation in mercury concentrations such that consumers may be exposed to either acceptable or unacceptable levels of mercury depending on the geographic origins of the fish and the allowable limits of different countries. Most notably, stocks of Patagonian toothfish in Chile accumulate significantly more mercury than stocks closer to the South Pole, including the South Georgia/Shag Rocks stock, a fishery certified by the Marine Stewardship Council (MSC as sustainably fished. Consistent with the documented geography of mercury contamination, our analysis showed that, on average, retail fish labeled as MSC-certified Patagonian toothfish had only half the mercury of uncertified fish. However, consideration of genetic data that were informative about seafood substitutions revealed a complex pattern of contamination hidden from consumers: species substitutions artificially inflated the expected difference in mercury levels between MSC-certified and uncertified fish whereas fishery stock substitutions artificially reduced the expected difference in mercury content between MSC-certified and uncertified fish that were actually D. eleginoides. Among MSC-certified fish that were actually D. eleginoides, several with exogenous mtDNA haplotypes (i.e., not known from the certified fishery had mercury concentrations on par with uncertified fish from Chile. Overall, our analysis of mercury was consistent with inferences from the genetic data about the geographic origins of the fish, demonstrated the potential negative impact of

In the workup of patients with obscure gastrointestinal bleed, does 64-slice MDCT have a role?

International Nuclear Information System (INIS)

Kulkarni, Chinmay; Moorthy, Srikanth; Sreekumar, KP; Rajeshkannan, R; Nazar, PK; Sandya, CJ; Sivasubramanian, S; Ramchandran, PV

2012-01-01

The purpose was to prospectively determine the sensitivity of 64-slice MDCT in detecting and diagnosing the cause of obscure gastrointestinal bleed (OGIB). Our study included 50 patients (male 30, female 20) in the age range of 3–82 years (average age: 58.52 years) who were referred to our radiology department as part of their workup for clinically evident gastrointestinal (GI) bleed or as part of workup for anemia (with and without positive fecal occult blood test). All patients underwent conventional upper endoscopy and colonoscopy before undergoing CT scan. Following a noncontrast scan, all patients underwent triple-phase contrast CT scan using a 64-slice CT scan system. The diagnostic performance of 64-slice MDCT was compared to the results of capsule endoscopy, 99m-technetium-labeled red blood cell scintigraphy (99mTc-RBC scintigraphy), digital subtraction angiography, and surgery whenever available. CT scan showed positive findings in 32 of 50 patients. The sensitivity, specificity, positive predictive value, and negative predictive values of MDCT for detection of bleed were 72.2%, 42.8%, 81.2%, and 44.4%, respectively. Capsule endoscopy was done in 15 patients and was positive in 10 patients; it had a sensitivity of 71.4%. Eleven patients had undergone 99mTc-RBC scintigraphy prior to CT scan, and the result was positive in seven patients (sensitivity 70%). Digital subtraction angiography was performed in only eight patients and among them all except one patient showed findings consistent with the lesions detected on MDCT. MDCT is a sensitive and noninvasive tool that allows rapid detection and localization of OGIB. It can be used as the first-line investigation in patients with negative endoscopy and colonoscopy studies. MDCT and capsule endoscopy have complementary roles in the evaluation of OGIB

Robust forecasts on fundamental physics from the foreground-obscured, gravitationally-lensed CMB polarization

Energy Technology Data Exchange (ETDEWEB)

Errard, Josquin [Sorbonne Universités, Institut Lagrange de Paris (ILP), 98 bis Boulevard Arago, 75014 Paris (France); Feeney, Stephen M.; Jaffe, Andrew H. [Department of Physics, Blackett Laboratory, Imperial College London, Prince Consort Road, London SW7 2AZ (United Kingdom); Peiris, Hiranya V., E-mail: josquin.errard@lpnhe.in2p3.fr, E-mail: s.feeney@imperial.ac.uk, E-mail: h.peiris@ucl.ac.uk, E-mail: a.jaffe@imperial.ac.uk [Department of Physics and Astronomy, University College London, Gower Street, London WC1E 6BT (United Kingdom)

2016-03-01

Recent results from the BICEP, Keck Array and Planck Collaborations demonstrate that Galactic foregrounds are an unavoidable obstacle in the search for evidence of inflationary gravitational waves in the cosmic microwave background (CMB) polarization. Beyond the foregrounds, the effect of lensing by intervening large-scale structure further obscures all but the strongest inflationary signals permitted by current data. With a plethora of ongoing and upcoming experiments aiming to measure these signatures, careful and self-consistent consideration of experiments' foreground- and lensing-removal capabilities is critical in obtaining credible forecasts of their performance. We investigate the capabilities of instruments such as Advanced ACTPol, BICEP3 and Keck Array, CLASS, EBEX10K, PIPER, Simons Array, SPT-3G and SPIDER, and projects as COrE+, LiteBIRD-ext, PIXIE and Stage IV, to clean contamination due to polarized synchrotron and dust from raw multi-frequency data, and remove lensing from the resulting co-added CMB maps (either using iterative CMB-only techniques or through cross-correlation with external data). Incorporating these effects, we present forecasts for the constraining power of these experiments in terms of inflationary physics, the neutrino sector, and dark energy parameters. Made publicly available through an online interface, this tool enables the next generation of CMB experiments to foreground-proof their designs, optimize their frequency coverage to maximize scientific output, and determine where cross-experimental collaboration would be most beneficial. We find that analyzing data from ground, balloon and space instruments in complementary combinations can significantly improve component separation performance, delensing, and cosmological constraints over individual datasets. In particular, we find that a combination of post-2020 ground- and space-based experiments could achieve constraints such as σ(r)∼1.3×10{sup −4}, σ(n{sub t})∼0

Historical collections reveal patterns of diffusion of sweet potato in Oceania obscured by modern plant movements and recombination.

Science.gov (United States)

Roullier, Caroline; Benoit, Laure; McKey, Doyle B; Lebot, Vincent

2013-02-05

The history of sweet potato in the Pacific has long been an enigma. Archaeological, linguistic, and ethnobotanical data suggest that prehistoric human-mediated dispersal events contributed to the distribution in Oceania of this American domesticate. According to the "tripartite hypothesis," sweet potato was introduced into Oceania from South America in pre-Columbian times and was then later newly introduced, and diffused widely across the Pacific, by Europeans via two historically documented routes from Mexico and the Caribbean. Although sweet potato is the most convincing example of putative pre-Columbian connections between human occupants of Polynesia and South America, the search for genetic evidence of pre-Columbian dispersal of sweet potato into Oceania has been inconclusive. Our study attempts to fill this gap. Using complementary sets of markers (chloroplast and nuclear microsatellites) and both modern and herbarium samples, we test the tripartite hypothesis. Our results provide strong support for prehistoric transfer(s) of sweet potato from South America (Peru-Ecuador region) into Polynesia. Our results also document a temporal shift in the pattern of distribution of genetic variation in sweet potato in Oceania. Later reintroductions, accompanied by recombination between distinct sweet potato gene pools, have reshuffled the crop's initial genetic base, obscuring primary patterns of diffusion and, at the same time, giving rise to an impressive number of local variants. Moreover, our study shows that phenotypes, names, and neutral genes do not necessarily share completely parallel evolutionary histories. Multidisciplinary approaches, thus, appear necessary for accurate reconstruction of the intertwined histories of plants and humans.

Remote Optical Imagery of Obscured Objects in Low-Visibility Environments Using Parametric Amplification

Energy Technology Data Exchange (ETDEWEB)

Asher, R.B.; Bliss, D.E.; Cameron, S.M.; Hamil, R.A.

1998-10-14

The development of unconventional active optical sensors to remotely detect and spatially resolve suspected threats obscured by low-visibility observation conditions (adverse weather, clouds, dust, smoke, precipitation, etc.) is fundamental to maintaining tactical supremacy in the battlespace. In this report, the authors describe an innovative frequency-agile image intensifier technology based on time-gated optical parametic amplification (OPA) for enhanced light-based remote sensing through pervasive scattering and/or turbulent environments. Improved dynamic range characteristics derived from the amplified passband of the OPA receiver combined with temporal discrimination in the image capture process will offset radiant power extinction losses, while defeating the deugradative effects & multipath dispersion and ,diffuse backscatter noise along the line-of-sight on resultant image contrast and range resolution. Our approach extends the operational utility of the detection channel in existing laser radar systems by increasing sensitivity to low-level target reffectivities, adding ballistic rejection of scatter and clutter in the range coordinate, and introducing multispectral and polarization discrimination capability in a wavelen~h-tunable, high gain nonlinear optical component with strong potential for source miniaturization. A key advantage of integrating amplification and tlequency up-conversion functions within a phasematched three-wave mixing parametric device is the ability to petiorm background-free imaging with eye-safe or longer inilared illumination wavelengths (idler) less susceptible to scatter without sacrificing quantum efficiency in the detection process at the corresponding signal wavelength. We report benchmark laboratory experiments in which the OPA gating process has been successfidly demonstrated in both transillumination and reflection test geometries with extended pathlengths representative of realistic coastal sea water and cumulus cloud

GEMINI/GeMS Observations Unveil the Structure of the Heavily Obscured Globular Cluster Liller 1.

Science.gov (United States)

Saracino, S.; Dalessandro, E.; Ferraro, F. R.; Lanzoni, B.; Geisler, D.; Mauro, F.; Villanova, S.; Moni Bidin, C.; Miocchi, P.; Massari, D.

2015-06-01

By exploiting the exceptional high-resolution capabilities of the near-IR camera GSAOI combined with the Gemini Multi-Conjugate Adaptive System at the GEMINI South Telescope, we investigated the structural and physical properties of the heavily obscured globular cluster Liller 1 in the Galactic bulge. We have obtained the deepest and most accurate color-magnitude diagram published so far for this cluster, reaching {{K}s}˜ 19 (below the main-sequence turnoff level). We used these data to redetermine the center of gravity of the system, finding that it is located about 2.″2 southeast from the literature value. We also built new star density and surface brightness profiles for the cluster and rederived its main structural and physical parameters (scale radii, concentration parameter, central mass density, total mass). We find that Liller 1 is significantly less concentrated (concentration parameter c=1.74) and less extended (tidal radius {{r}t}=298\\prime\\prime and core radius {{r}c}=5\\buildrel{\\prime\\prime}\\over{.} 39) than previously thought. By using these newly determined structural parameters, we estimated the mass of Liller 1 to be {{M}tot}=2.3+0.3-0.1× {{10}6} {{M}⊙ } ({{M}tot}=1.5+0.2-0.1× {{10}6} {{M}⊙ } for a Kroupa initial mass function), which is comparable to that of the most massive clusters in the Galaxy (ω Centari and Terzan 5). Also, Liller 1 has the second-highest collision rate (after Terzan 5) among all star clusters in the Galaxy, thus confirming that it is an ideal environment for the formation of collisional objects (such as millisecond pulsars). Based on observations obtained at the Gemini Observatory, which is operated by the Association of Universities for Research in Astronomy, Inc., under a cooperative agreement with the NSF on behalf of the Gemini partnership: the National Science Foundation (United States), the National Research Council (Canada), CONICYT (Chile), the Australian Research Council (Australia), Ministério da

New Evidence on the Impact of Antithrombotics in Patients Submitted to Small Bowel Capsule Endoscopy for the Evaluation of Obscure Gastrointestinal Bleeding

Directory of Open Access Journals (Sweden)

Pedro Boal Carvalho

2014-01-01

Full Text Available Objectives. Small bowel capsule endoscopy (SBCE plays a decisive role in the obscure gastrointestinal bleeding (OGIB diagnosis. Antithrombotics may increase bleeding risk in patients with preexistent lesions or through direct mucosal aggression. We aimed to correlate antithrombotics usage with lesions with bleeding potential found in SBCE. Methods. Retrospective single-center study including 274 consecutive SBCE performed over 7 years for OGIB. The lesions were classified as P0 (no bleeding potential, P1 (uncertain bleeding potential: erosions, and P2 (high bleeding potential: angioectasias, ulcers, and tumors. We assessed antiplatelet and anticoagulant drug use during the 60 days preceding SBCE. Results. One-third of the patients were under antithrombotic therapy. The diagnostic yield of SBCE for P2 lesions was 30.0%. Angioectasias (20.4% were the most frequently observed lesions. There was a significant correlation between anticoagulant drug use and a higher incidence of P2 lesions in the small bowel (43.2% versus 26.5%; OR = 2.11, P=0.026. We found no significant correlation between antiplatelets and lesions with bleeding potential in SBCE. Conclusions. Small bowel lesions with high bleeding potential were more frequently detected when the patient was on anticoagulant drugs, resulting in a twofold risk. Antiplatelet drugs were not associated with small bowel lesions.

Loch Ness, Yeti og læringsstile

DEFF Research Database (Denmark)

Johansen, Martin Blok; Oksbjerg, Marianne

2013-01-01

Analyse og diskussion af læringsstilsbegrebet, som det fremstilles af Dunn og Dunn. I artiklen argumenteres der for, at der ikke er noget videnskabeligt belæg for at bringe læringsstile ind i klasseværelset. Det er alene en tros- og følelsessag....

Hexachloroethane Obscurant Replacement

Science.gov (United States)

2012-01-01

were not totally dispersed in aerosol form; significant solid slag formation was observed. Thus, smoke density efficiency was only one quarter of that...determine smoke density and analyze for toxicity of combustion gases and particulates. Results: Compositions containing divalent zinc and...solid slag formation was observed. Thus, smoke density efficiency was only one quarter of that of the hexachloroethane containing baseline. The

SPIRITS 15c and SPIRITS 14buu: Two Obscured Supernovae in the Nearby Star-forming Galaxy IC 2163

Energy Technology Data Exchange (ETDEWEB)

Jencson, Jacob E.; Kasliwal, Mansi M.; Cao, Yi [Cahill Center for Astronomy and Astrophysics, California Institute of Technology, Pasadena, CA 91125 (United States); Johansson, Joel [Benoziyo Center for Astrophysics, Weizmann Institute of Science, 76100 Rehovot (Israel); Contreras, Carlos; Castellón, Sergio; Morrell, Nidia; Phillips, Mark [Las Campanas Observatory, Carnegie Observatories, Casilla 601, La Serena (Chile); Bond, Howard E.; Monson, Andrew J. [Dept. of Astronomy and Astrophysics, Pennsylvania State University, University Park, PA 16802 (United States); Masci, Frank J.; Helou, George [Infrared Processing and Analysis Center, California Institute of Technology, Pasadena, CA 91125 (United States); Cody, Ann Marie [NASA Ames Research Center, Moffett Field, CA 94035 (United States); Andrews, Jennifer E. [Steward Observatory, University of Arizona, 933 North Cherry Avenue, Tucson, AZ 85721 (United States); Bally, John; Green, Wayne [Center for Astrophysics and Space Astronomy, University of Colorado, 389 UCB, Boulder, CO 80309 (United States); Fox, Ori D. [Space Telescope Science Institute, 3700 San Martin Dr., Baltimore, MD 21218 (United States); Gburek, Timothy; Gehrz, Robert D. [Minnesota Institute for Astrophysics, School of Physics and Astronomy, 116 Church Street, S. E., University of Minnesota, Minneapolis, MN 55455 (United States); Hsiao, Eric, E-mail: jj@astro.caltech.edu [Department of Physics, Florida State University, 77 Chieftain Way, Tallahassee, FL, 32306 (United States); and others

2017-03-10

SPitzer InfraRed Intensive Transients Survey—SPIRITS—is an ongoing survey of nearby galaxies searching for infrared (IR) transients with Spitzer /IRAC. We present the discovery and follow-up observations of one of our most luminous ( M {sub [4.5]} = −17.1 ± 0.4 mag, Vega) and reddest ([3.6] − [4.5] = 3.0 ± 0.2 mag) transients, SPIRITS 15c. The transient was detected in a dusty spiral arm of IC 2163 ( D ≈ 35.5 Mpc). Pre-discovery ground-based imaging revealed an associated, shorter-duration transient in the optical and near-IR (NIR). NIR spectroscopy showed a broad (≈8400 km s{sup −1}), double-peaked emission line of He i at 1.083 μ m, indicating an explosive origin. The NIR spectrum of SPIRITS 15c is similar to that of the Type IIb SN 2011dh at a phase of ≈200 days. Assuming an A {sub V} = 2.2 mag of extinction in SPIRITS 15c provides a good match between their optical light curves. The NIR light curves, however, show some minor discrepancies when compared with SN 2011dh, and the extreme [3.6]–[4.5] color has not been previously observed for any SN IIb. Another luminous ( M {sub 4.5} = −16.1 ± 0.4 mag) event, SPIRITS 14buu, was serendipitously discovered in the same galaxy. The source displays an optical plateau lasting ≳80 days, and we suggest a scenario similar to the low-luminosity Type IIP SN 2005cs obscured by A{sub V} ≈ 1.5 mag. Other classes of IR-luminous transients can likely be ruled out in both cases. If both events are indeed SNe, this may suggest that ≳18% of nearby core-collapse SNe are missed by currently operating optical surveys.

SPIRITS 15c and SPIRITS 14buu: Two Obscured Supernovae in the Nearby Star-forming Galaxy IC 2163

International Nuclear Information System (INIS)

Jencson, Jacob E.; Kasliwal, Mansi M.; Cao, Yi; Johansson, Joel; Contreras, Carlos; Castellón, Sergio; Morrell, Nidia; Phillips, Mark; Bond, Howard E.; Monson, Andrew J.; Masci, Frank J.; Helou, George; Cody, Ann Marie; Andrews, Jennifer E.; Bally, John; Green, Wayne; Fox, Ori D.; Gburek, Timothy; Gehrz, Robert D.; Hsiao, Eric

2017-01-01

SPitzer InfraRed Intensive Transients Survey—SPIRITS—is an ongoing survey of nearby galaxies searching for infrared (IR) transients with Spitzer /IRAC. We present the discovery and follow-up observations of one of our most luminous ( M [4.5] = −17.1 ± 0.4 mag, Vega) and reddest ([3.6] − [4.5] = 3.0 ± 0.2 mag) transients, SPIRITS 15c. The transient was detected in a dusty spiral arm of IC 2163 ( D ≈ 35.5 Mpc). Pre-discovery ground-based imaging revealed an associated, shorter-duration transient in the optical and near-IR (NIR). NIR spectroscopy showed a broad (≈8400 km s −1 ), double-peaked emission line of He i at 1.083 μ m, indicating an explosive origin. The NIR spectrum of SPIRITS 15c is similar to that of the Type IIb SN 2011dh at a phase of ≈200 days. Assuming an A V = 2.2 mag of extinction in SPIRITS 15c provides a good match between their optical light curves. The NIR light curves, however, show some minor discrepancies when compared with SN 2011dh, and the extreme [3.6]–[4.5] color has not been previously observed for any SN IIb. Another luminous ( M 4.5 = −16.1 ± 0.4 mag) event, SPIRITS 14buu, was serendipitously discovered in the same galaxy. The source displays an optical plateau lasting ≳80 days, and we suggest a scenario similar to the low-luminosity Type IIP SN 2005cs obscured by A V ≈ 1.5 mag. Other classes of IR-luminous transients can likely be ruled out in both cases. If both events are indeed SNe, this may suggest that ≳18% of nearby core-collapse SNe are missed by currently operating optical surveys.

LIFTING THE VEIL ON OBSCURED ACCRETION: ACTIVE GALACTIC NUCLEI NUMBER COUNTS AND SURVEY STRATEGIES FOR IMAGING HARD X-RAY MISSIONS

International Nuclear Information System (INIS)

Ballantyne, D. R.; Draper, A. R.; Madsen, K. K.; Rigby, J. R.; Treister, E.

2011-01-01

Finding and characterizing the population of active galactic nuclei (AGNs) that produces the X-ray background (XRB) is necessary to connect the history of accretion to observations of galaxy evolution at longer wavelengths. The year 2012 will see the deployment of the first hard X-ray imaging telescope which, through deep extragalactic surveys, will be able to measure the AGN population at the energies where the XRB peaks (∼20-30 keV). Here, we present predictions of AGN number counts in three hard X-ray bandpasses: 6-10 keV, 10-30 keV, and 30-60 keV. Separate predictions are presented for the number counts of Compton thick AGNs, the most heavily obscured active galaxies. The number counts are calculated for five different models of the XRB that differ in the assumed hard X-ray luminosity function, the evolution of the Compton thick AGNs, and the underlying AGN spectral model. The majority of the hard X-ray number counts will be Compton thin AGNs, but there is a greater than tenfold increase in the Compton thick number counts from the 6-10 keV to the 10-30 keV band. The Compton thick population shows enough variation that a hard X-ray number counts measurement will constrain the models. The computed number counts are used to consider various survey strategies for the NuSTAR mission, assuming a total exposure time of 6.2 Ms. We find that multiple surveys will allow a measurement of Compton thick evolution. The predictions presented here should be useful for all future imaging hard X-ray missions.

Gemini long-slit observations of luminous obscured quasars: Further evidence for an upper limit on the size of the narrow-line region

International Nuclear Information System (INIS)

Hainline, Kevin N.; Hickox, Ryan C.; Greene, Jenny E.; Myers, Adam D.; Zakamska, Nadia L.; Liu, Guilin; Liu, Xin

2014-01-01

We examine the spatial extent of the narrow-line regions (NLRs) of a sample of 30 luminous obscured quasars at 0.4 < z < 0.7 observed with spatially resolved Gemini-N GMOS long-slit spectroscopy. Using the [O III] λ5007 emission feature, we estimate the size of the NLR using a cosmology-independent measurement: the radius where the surface brightness falls to 10 –15 erg s –1 cm –2 arcsec –2 . We then explore the effects of atmospheric seeing on NLR size measurements and conclude that direct measurements of the NLR size from observed profiles are too large by 0.1-0.2 dex on average, as compared to measurements made to best-fit Sérsic or Voigt profiles convolved with the seeing. These data, which span a full order of magnitude in IR luminosity (log (L 8 μm /erg s –1 ) = 44.4-45.4), also provide strong evidence that there is a flattening of the relationship between NLR size and active galactic nucleus luminosity at a seeing-corrected size of ∼7 kpc. The objects in this sample have high luminosities which place them in a previously under-explored portion of the size-luminosity relationship. These results support the existence of a maximal size of the NLR around luminous quasars; beyond this size, there is either not enough gas or the gas is over-ionized and does not produce enough [O III] λ5007 emission.

Stationary Distribution and Thermodynamic Relation in Nonequilibrium Steady States

KAUST Repository

Komatsu, Teruhisa S.; Nakagawa, Naoko; Sasa, Shin-ichi; Tasaki, Hal; Ito, Nobuyasu

2010-01-01

We describe our recent attempts toward statistical mechanics and thermodynamics for nonequilibrium steady states (NESS) realized, e.g., in a heat conducting system. Our first result is a simple expression of the probability distribution (of microscopic states) of a NESS. Our second result is a natural extension of the thermodynamic Clausius relation and a definition of an accompanying entropy in NESS. This entropy coincides with the normalization constant appearing in the above mentioned microscopic expression of NESS, and has an expression similar to the Shannon entropy (with a further symmetrization). The NESS entropy proposed here is a clearly defined measurable quantity even in a system with a large degrees of freedom. We numerically measure the NESS entropy in hardsphere fluid systems with a heat current, by observing energy exchange between the system and the heat baths when the temperatures of the baths are changed according to specified protocols.

Probabilistic object and viewpoint models for active object recognition

CSIR Research Space (South Africa)

Govender, N

2013-09-01

Full Text Available ,θ′(f occ). V. EXPERIMENTS A. Dataset For our experiments, we use the active recognition dataset introduced by [12]. The training data consists of everyday objects such as cereal boxes, ornaments, spice bottle, etc. Images were captured every 20 degrees... are to be verified TABLE I CONFUSION MATRIX FOR BINARY A MODEL Obscured Obscured Obscured Obscured Obscured Obscured Obscured Obscured Obscured Obscured Cereal Battery Curry box Elephant Handbag MrMin Salad Bottle Spice Bottle Spray Can Spray Can 1 Cereal 0.9800 0...

Tool – Material, Metaphor – Metonymy, Instrument(ness)

DEFF Research Database (Denmark)

Bertelsen, Olav Wedege; Breinbjerg, Morten; Pold, Søren

2008-01-01

creativity , supported by analysis of, and interviews with, musical composers. Instrumentness is explained through discussions of materiality and metonymy as central strategies for computer mediated creativity. The paper is contributing to an investigation of the aesthetics of use in relation to software...... are controlled and conceptualized through values such as virtuosity and palyability, which are important for computer-mediated creative work supporting development in use beyond what is initially designed for. The papet performs a conceptual investigation into qualities in software interfaces that support...

In vitro propagation of avocado (Persea drymifolia Ness.)

International Nuclear Information System (INIS)

Barrera-Guerra, J.L.; Ramirez-Malagon, R.; Martinez-Jaime, O.A.

2001-01-01

In the past 20 years, reports on micropropagation and rooting in vitro of avocado shoots, with diverse origins and treatments, have been published. However, none of them reached the level required for large scale propagation of the species. It is considered that, in the first place, the micropropagation of avocado requires an efficient system of rooting. Therefore, a system to induce the rooting in vitro of avocado shoots, based on indole-3-butyric acid (IBA) pulses and some treatments based on thidiazuron (TDZ) was tested, using 40 explants per treatment. The treatments with TDZ did not succeed in rooting shoots. Some treatments with pulses of IBA induced the following rooting results: without growth regulators, 16%; 4,000 mg L -1 of IBA for 5 seconds, 8.3% rooted; 100 mg L -1 for 72 hours, 20%; 50 mg L -1 for 72 hours, 15.4%; 150 mg L -1 for 24 hours, 5% rooted. It is considered possible to improve these results by adjusting the range of IBA concentrations as well as in the time range of pulse applications. Finally, it is easier to establish in vitro explants derived from mature seeds or embryos germinated in vitro. (author)

NES consensus redefined by structures of PKI-type and Rev-type nuclear export signals bound to CRM1.

Science.gov (United States)

Güttler, Thomas; Madl, Tobias; Neumann, Piotr; Deichsel, Danilo; Corsini, Lorenzo; Monecke, Thomas; Ficner, Ralf; Sattler, Michael; Görlich, Dirk

2010-11-01

Classic nuclear export signals (NESs) confer CRM1-dependent nuclear export. Here we present crystal structures of the RanGTP-CRM1 complex alone and bound to the prototypic PKI or HIV-1 Rev NESs. These NESs differ markedly in the spacing of their key hydrophobic (Φ) residues, yet CRM1 recognizes them with the same rigid set of five Φ pockets. The different Φ spacings are compensated for by different conformations of the bound NESs: in the case of PKI, an α-helical conformation, and in the case of Rev, an extended conformation with a critical proline docking into a Φ pocket. NMR analyses of CRM1-bound and CRM1-free PKI NES suggest that CRM1 selects NES conformers that pre-exist in solution. Our data lead to a new structure-based NES consensus, and explain why NESs differ in their affinities for CRM1 and why supraphysiological NESs bind the exportin so tightly.

Dark Matter remains obscure

CERN Multimedia

Fabio Capello

2011-01-01

It is one of the hidden secrets that literally surround the Universe. Experiments have shown no result so far because trying to capture particles that do not seem to interact with ordinary matter is no trivial exercise. The OSQAR experiment at CERN is dedicated to the search for axions, one of the candidates for Dark Matter. For its difficult challenge, OSQAR counts on one of the world’s most powerful magnets borrowed from the LHC. In a recent publication, the OSQAR collaboration was able to confirm that no axion signal appears out of the background. In other words: the quest is still on.   The OSQAR experiment installed in the SM18 hall. (Photo by F. Capello) The OSQAR “Light Shining Through a Wall” experiment was officially launched in 2007 with the aim of detecting axions, that is, particles that might be the main components of Dark Matter. OSQAR uses the powerful LHC dipole magnet to intensify the predicted photon-axion conversions in the presence of strong m...

Notch signaling is required for maintaining stem-cell features of neuroprogenitor cells derived from human embryonic stem cells

Directory of Open Access Journals (Sweden)

Chung Hyung-Min

2009-08-01

Full Text Available Abstract Background Studies have provided important findings about the roles of Notch signaling in neural development. Unfortunately, however, most of these studies have investigated the neural stem cells (NSCs of mice or other laboratory animals rather than humans, mainly owing to the difficulties associated with obtaining human brain samples. It prompted us to focus on neuroectodermal spheres (NESs which are derived from human embryonic stem cell (hESC and densely inhabited by NSCs. We here investigated the role of Notch signaling with the hESC-derived NESs. Results From hESCs, we derived NESs, the in-vitro version of brain-derived neurospheres. NES formation was confirmed by increased levels of various NSC marker genes and the emergence of rosette structures in which neuroprogenitors are known to reside. We found that Notch signaling, which maintains stem cell characteristics of in-vivo-derived neuroprogenitors, is active in these hESC-derived NESs, similar to their in-vivo counterpart. Expression levels of Notch signaling molecules such as NICD, DLLs, JAG1, HES1 and HES5 were increased in the NESs. Inhibition of the Notch signaling by a γ-secretase inhibitor reduced rosette structures, expression levels of NSC marker genes and proliferation potential in the NESs, and, if combined with withdrawal of growth factors, triggered differentiation toward neurons. Conclusion Our results indicate that the hESC-derived NESs, which share biochemical features with brain-derived neurospheres, maintain stem cell characteristics mainly through Notch signaling, which suggests that the hESC-derived NESs could be an in-vitro model for in-vivo neurogenesis.

Hemorragia de tronco cerebral após remoção cirúrgica de cisto aracnóide da fissura silviana: Relato de caso Brainstem hemorrhage after surgical removal of arachnoid cyst of the sylvian fissure: case report

Directory of Open Access Journals (Sweden)

Guilherme Borges

1995-12-01

Full Text Available Os autores relatam um caso de hemorragia de tronco cerebral após craniotomia para ressecção de grande cisto aracnóide de fissura silviana esquerda. A sintomatologia inicial pré-operatória incluía sinais de hipertensão intracraniana e a tomografia computadorizada mostrava desvio de linha média. Diversos fatores são discutidos para explicar o sangramento parenquimatoso pós-operatório: edema cerebral, diminuição do retorno venoso e de fluxo sanguíneo no lado comprimido. Entretanto a fisiopatologia da hemorragia parenquimatosa em casos como o relatado permanece obscura. Uma abordagem cirúrgica mais cautelosa é proposta nesses pacientes com de hipertensão intracraniana.The authors report a case of a hemorrhage of the brainstem after craniotomy for resection of a huge arachnoid cyst of the sylvian fissure on the left hemisphere. The previous simptomatology included clinical signs of increased intracranial pressure, and the computerized tomography showed midline shift. Some factors may contribute to brain hemorrhage post-operatively: cerebral edema, ipsilateral changes in the venous reflux and blood perfusion, although the physiopathology remains obscure. A more careful approach is suggested in such cases with intracranial hypertension.

A TALE OF TWO NARROW-LINE REGIONS: IONIZATION, KINEMATICS, AND SPECTRAL ENERGY DISTRIBUTIONS FOR A LOCAL PAIR OF MERGING OBSCURED ACTIVE GALAXIES

Energy Technology Data Exchange (ETDEWEB)

Hainline, Kevin N.; Hickox, Ryan C.; Chen, Chien-Ting; Carroll, Christopher M.; Jones, Mackenzie L.; Zervos, Alexandros S. [Department of Physics and Astronomy, Dartmouth College, Hanover, NH 03755 (United States); Goulding, Andrew D. [Department Astrophysical Sciences, Princeton University, Princeton, NJ 08544 (United States)

2016-05-20

We explore the gas ionization and kinematics, as well as the optical-IR spectral energy distributions for UGC 11185, a nearby pair of merging galaxies hosting obscured active galactic nuclei (AGNs), also known as SDSS J181611.72+423941.6 and J181609.37+423923.0 (J1816NE and J1816SW, z ≈ 0.04). Due to the wide separation between these interacting galaxies (∼23 kpc), observations of these objects provide a rare glimpse of the concurrent growth of supermassive black holes at an early merger stage. We use BPT line diagnostics to show that the full extent of the narrow-line emission in both galaxies is photoionized by an AGN, and confirm the existence of a 10 kpc-scale ionization cone in J1816NE, while in J1816SW the AGN narrow-line region is much more compact (1–2 kpc) and relatively undisturbed. Our observations also reveal the presence of ionized gas that nearly spans the entire distance between the galaxies, which is likely in a merger-induced tidal stream. In addition, we carry out a spectral analysis of the X-ray emission using data from XMM-Newton . These galaxies represent a useful pair to explore how the [O iii] luminosity of an AGN is dependent on the size of the region used to explore the extended emission. Given the growing evidence for AGN “flickering” over short timescales, we speculate that the appearances and impacts of these AGNs may change multiple times over the course of the galaxy merger, which is especially important given that these objects are likely the progenitors of the types of systems commonly classified as “dual AGNs.”.

A small mesolithic site at Fife Ness, Fife, Scotland

Directory of Open Access Journals (Sweden)

Caroline R. Wickham-Jones

1998-08-01

Full Text Available In the summer of 1996 work to build a new golf course on the coast at Crail in Fife, Scotland, uncovered a small patch of dark soil associated with microliths. Excavation revealed an arc of seven pits or post-holes, a hearth site and several other pit-like features. There was a small lithic assemblage, and also a quantity of carbonised hazelnut shell, samples of which were sent off for radiocarbon assay. The site was remarkable for several reasons: ◦Size ◦Its size (75m2 was unusual in that most mesolithic sites in Scotland (and elsewhere are often much larger. Small sites have played an important role in theoretical interpretations of the mesolithic way of life, but few have been excavated. ◦Lithic assemblage ◦The lithic assemblage was small, even for such a small site, and comprised solely of flint, which is very rare in Scotland. There was relatively little knapping debris, but several retouched tools, over half of which were narrow blade microliths. The microliths were very interesting because they were dominated by crescentic microliths, while more common types such as scalene triangles were absent. ◦Dates ◦A series of fourteen radiocarbon dates were obtained for the site and all centred round the same period: between 7400 and 7600 BC, calibrated. This was earlier than had been expected, and is an interesting addition to knowledge of the early settlement of eastern Scotland since most other early dates have been from west coast sites. The similarity of the dates adds weight to the argument that the site represents a single occupation which, in view of its size, is likely to have been of short duration. This, and the nature of the lithic assemblage, have lead us to the interpretation that the site was a specialised camp site, probably making use of coastal resources.

Aligning records management and risk management with busi- ness ...

African Journals Online (AJOL)

Ngulup

Moi University, School of Information Sciences, Eldoret, Kenya .... risk from the perspective of the impact upon organisational objectives. ... equipment failure); financial and systems risks (risks with financial controls and systems, such .... The World Bank (2000) states that poor record keeping affects the entire accounting.

Successes and failures in the construction of NESS-states

International Nuclear Information System (INIS)

Narnhofer, Heide

2010-01-01

We construct non-equilibrium states by coupling a large but finite system with quasifree evolution to two temperature baths of free fermions or bosons with different temperature. We are interested in the resulting behaviour of the temperature baths as well as in the consequences for the finite system, especially what happens in the limit when the finite system tends to infinity. As a special example we consider the Kronig-Penney model and the tight binding model. Here a heat current remains that changes the baths but does not allow a limiting behaviour when the finite system tends to infinity. For the random versions of these models, especially the Anderson model, the heat current disappears exponentially with the size of the system. We show that a limit state is attained that is independent of the time direction and does not show any kind of symmetry breaking.

Autophagic cell death: Loch Ness monster or endangered species?

Science.gov (United States)

Shen, Han-Ming; Codogno, Patrice

2011-05-01

The concept of autophagic cell death was first established based on observations of increased autophagic markers in dying cells. The major limitation of such a morphology-based definition of autophagic cell death is that it fails to establish the functional role of autophagy in the cell death process, and thus contributes to the confusion in the literature regarding the role of autophagy in cell death and cell survival. Here we propose to define autophagic cell death as a modality of non-apoptotic or necrotic programmed cell death in which autophagy serves as a cell death mechanism, upon meeting the following set of criteria: (i) cell death occurs without the involvement of apoptosis; (ii) there is an increase of autophagic flux, and not just an increase of the autophagic markers, in the dying cells; and (iii) suppression of autophagy via both pharmacological inhibitors and genetic approaches is able to rescue or prevent cell death. In light of this new definition, we will discuss some of the common problems and difficulties in the study of autophagic cell death and also revisit some well-reported cases of autophagic cell death, aiming to achieve a better understanding of whether autophagy is a real killer, an accomplice or just an innocent bystander in the course of cell death. At present, the physiological relevance of autophagic cell death is mainly observed in lower eukaryotes and invertebrates such as Dictyostelium discoideum and Drosophila melanogaster. We believe that such a clear definition of autophagic cell death will help us study and understand the physiological or pathological relevance of autophagic cell death in mammals.

Linking Drugs to Obscure Illnesses

DEFF Research Database (Denmark)

Bennett, Charles L; Starko, Karen M; Thomsen, Henrik S

2012-01-01

Identification of serious adverse drug reactions (sADRS) associated with commonly used drugs can elude detection for years. Reye's syndrome (RS), nephrogenic systemic fibrosis (NSF), and pure red cell aplasia (PRCA) among chronic kidney disease (CKD) patients were recognized in 1951, 2000, and 1998......-savings considerations, and a European regulatory requirement requiring removal of albumin as a stabilizer, led to toxicity. Overall, 81, 13, and 17 years elapsed between drug introduction into practice and identification of a causal relationship for aspirin, erythropoietin, and gadodiamide, respectively. A substantial...... decline in new cases of these sADRs occurred within two years of identification of the offending drug. Clinicians should be vigilant for sADRs, even for frequently-prescribed pharmaceuticals, particularly in settings where formulation or regulatory changes have occurred, or when over-the-counter, off...

Optimization under uncertainty of parallel nonlinear energy sinks

Science.gov (United States)

Boroson, Ethan; Missoum, Samy; Mattei, Pierre-Olivier; Vergez, Christophe

2017-04-01

Nonlinear Energy Sinks (NESs) are a promising technique for passively reducing the amplitude of vibrations. Through nonlinear stiffness properties, a NES is able to passively and irreversibly absorb energy. Unlike the traditional Tuned Mass Damper (TMD), NESs do not require a specific tuning and absorb energy over a wider range of frequencies. Nevertheless, they are still only efficient over a limited range of excitations. In order to mitigate this limitation and maximize the efficiency range, this work investigates the optimization of multiple NESs configured in parallel. It is well known that the efficiency of a NES is extremely sensitive to small perturbations in loading conditions or design parameters. In fact, the efficiency of a NES has been shown to be nearly discontinuous in the neighborhood of its activation threshold. For this reason, uncertainties must be taken into account in the design optimization of NESs. In addition, the discontinuities require a specific treatment during the optimization process. In this work, the objective of the optimization is to maximize the expected value of the efficiency of NESs in parallel. The optimization algorithm is able to tackle design variables with uncertainty (e.g., nonlinear stiffness coefficients) as well as aleatory variables such as the initial velocity of the main system. The optimal design of several parallel NES configurations for maximum mean efficiency is investigated. Specifically, NES nonlinear stiffness properties, considered random design variables, are optimized for cases with 1, 2, 3, 4, 5, and 10 NESs in parallel. The distributions of efficiency for the optimal parallel configurations are compared to distributions of efficiencies of non-optimized NESs. It is observed that the optimization enables a sharp increase in the mean value of efficiency while reducing the corresponding variance, thus leading to more robust NES designs.

X-ray effects on karyotype of Drosophila pseudo obscure. Pilot experience; Efecto de los rayos X en el cariotipo de Drosophila pseudoobscura. Experimento piloto

Energy Technology Data Exchange (ETDEWEB)

Salceda, V. M. [ININ, Departamento de Biologia, Carretera Mexico-Toluca s/n, 52750 Ocoyoacac, Estado de Mexico (Mexico)], e-mail: victor.salceda@inin.gob.mx

2009-10-15

Four groups of 100 males of Drosophila pseudo obscure carriers of genetic sequence Tree Line were treated with X-rays, through the use of a X-ray equipment Phillips MCN321; with absorbed individual doses of 28.2 Gy, 37.6 Gy, 47.6 Gy and 56.4 Gy, once irradiated these were crossed individually with two or three virgin females of the same constitution and the descendant emergency was took a larva of each crossing in order to detect the radiation effect on karyotype Tree Line of these organisms, chromosomal aberrations fundamentally, as well as on masculine sterility. Our observations gave as result for smaller dose, in a total of 61 analyzed larva, the obtaining of seven translocations equivalent to 11.5% as well as an inversion of 1.6%; with the following dose (58 analyzed larva) were obtained four translocations equal to 6.9%, two corresponding inversions to 3.4%, a mosaic and a deletion equivalent to 1.7%; with the dose of 47.6 Gy four translocations were induced 6.8% and deletion corresponding to 1.1%, again two respective inversions to 3.4% and a mosaic 1.7% in 59 analyzed larvas, meantime with the dose of 56.4 Gy appeared two translocations only equal to 3.7% in a sample of 54 individuals. The effect about masculine sterility was equal that the witness of 12% and for two following doses and finally of 41 and 46% respectively for the remaining doses. Comparisons with another authors gave similar values in the total cases. In accordance with our main objective, it is suggested to increase the sample size and to repeat the experiments using different genetic sequences as well as the possibility to use different radiation sources like gamma radiation and this way to utilize this system like a biological dosemeter. (Author)

Systemic aspects of conjugal resilience in couples with a child facing cancer and marrow transplantation.

Science.gov (United States)

Martin, Julie; Péloquin, Katherine; Vachon, Marie-France; Duval, Michel; Sultan, Serge

The negative impact of paediatric cancer on parents is well known and is even greater when intensive treatments are used. This study aimed to describe how couples whose child has received a transplant for the treatment of leukaemia view conjugal resilience and to evaluate the role of we-ness as a precursor of conjugal adjustment. Four parental couples were interviewed. Interviews were analysed in two ways: inductive thematic analysis and rating of verbal content with the We-ness Coding Scale . Participants report that conjugal resilience involves the identification of the couple as a team and cohesion in the couple. Being a team generates certain collaborative interactions that lead to conjugal resilience. A sense of we-ness in parents is associated with fluctuation in the frequency of themes. Participants' vision of conjugal resilience introduced novel themes. The sense of we-ness facilitates cohesion and the process of conjugal resilience.

THE SPECTRAL ENERGY DISTRIBUTIONS AND INFRARED LUMINOSITIES OF z ≈ 2 DUST-OBSCURED GALAXIES FROM Herschel AND Spitzer

International Nuclear Information System (INIS)

Melbourne, J.; Soifer, B. T.; Desai, Vandana; Armus, Lee; Pope, Alexandra; Alberts, Stacey; Dey, Arjun; Jannuzi, B. T.; Bussmann, R. S.

2012-01-01

Dust-obscured galaxies (DOGs) are a subset of high-redshift (z ≈ 2) optically-faint ultra-luminous infrared galaxies (ULIRGs, e.g., L IR > 10 12 L ☉ ). We present new far-infrared photometry, at 250, 350, and 500 μm (observed-frame), from the Herschel Space Telescope for a large sample of 113 DOGs with spectroscopically measured redshifts. Approximately 60% of the sample are detected in the far-IR. The Herschel photometry allows the first robust determinations of the total infrared luminosities of a large sample of DOGs, confirming their high IR luminosities, which range from 10 11.6 L ☉ IR (8-1000 μm) 13.6 L ☉ . 90% of the Herschel-detected DOGs in this sample are ULIRGs and 30% have L IR > 10 13 L ☉ . The rest-frame near-IR (1-3 μm) spectral energy distributions (SEDs) of the Herschel-detected DOGs are predictors of their SEDs at longer wavelengths. DOGs with 'power-law' SEDs in the rest-frame near-IR show observed-frame 250/24 μm flux density ratios similar to the QSO-like local ULIRG, Mrk 231. DOGs with a stellar 'bump' in their rest-frame near-IR show observed-frame 250/24 μm flux density ratios similar to local star-bursting ULIRGs like NGC 6240. None show 250/24 μm flux density ratios similar to extreme local ULIRG, Arp 220; though three show 350/24 μm flux density ratios similar to Arp 220. For the Herschel-detected DOGs, accurate estimates (within ∼25%) of total IR luminosity can be predicted from their rest-frame mid-IR data alone (e.g., from Spitzer observed-frame 24 μm luminosities). Herschel-detected DOGs tend to have a high ratio of infrared luminosity to rest-frame 8 μm luminosity (the IR8 = L IR (8-1000 μm)/νL ν (8 μm) parameter of Elbaz et al.). Instead of lying on the z = 1-2 'infrared main sequence' of star-forming galaxies (like typical LIRGs and ULIRGs at those epochs) the DOGs, especially large fractions of the bump sources, tend to lie in the starburst sequence. While, Herschel-detected DOGs are similar to scaled up

Ser(mos) com e sem cancro we-ness no casal

OpenAIRE

Santos, Inês Jorge

2016-01-01

Dissertação de Mestrado apresentada no ISPA – Instituto Universitário para obtenção do grau de Mestre em Psicologia especialidade de Psicologia Clínica. O objetivo desde estudo é compreender se o “We-ness” aumenta quando se verifica a presença da doença oncológica numa tónica de comparação de casais com cancro e casais sem cancro e verificar a perceção que os casais têm face ao “We-ness” e ao significado deste sentimento. A evidência de estudos ao nível do individuo, como memb...

Invisible-hand explanations: From blindness to lack of we-ness

OpenAIRE

Dayer-Tieffenbach, Emma

2013-01-01

The unintendedness of the phenomenon that is to be explained is a constraint visible in the various applications and clarifications of invisible hand explanations. The article casts doubt on such a requirement and proposes a revised account. To have a role in an invisible hand process it is argued agents may very well act with a view to contributing to the occurrence of the social outcome that is to be explained provided they see what they do as an aggregation of their individual actions rath...

We-ness and the Cultivation of Wisdom in Couple Therapy.

Science.gov (United States)

Skerrett, Karen

2016-03-01

Wisdom has played a key role in the attempt to understand the positive nature of human behavior since the time of Aristotle. In the past decade, psychology and related fields have experienced an expanding interest in the empirical and theoretical pursuit of wisdom. The relational dimension of wisdom has received less attention, although it may be viewed as embedded in the practice of all couple therapists. This article integrates previous work on resilience and positive functioning in committed partnerships and proposes relational wisdom to be a master virtue of relationship development, one that can be cultivated across the lifespan of the partnership. The aspects of relational wisdom such as self-reflection, attunement to self and other, balancing conflicting partner aims, the interpretation of rules and principles in light of the uniqueness of each situation and the capacity to learn from experience point to couples therapy as an ideal context for such skill building. Wisdom is built through dialog and the resulting individual and couple stories can serve as touchstones to what is most precious and vital in the relationship as well as guides for action through challenges and conflict. A clinical case is described to illustrate selected aspects of relational wisdom and implications for therapeutic practice. © 2015 Family Process Institute.

Stressing Knowledge: Organisational closed-ness and knowledge acquisition under pressure

NARCIS (Netherlands)

Koraeus, M.A.P.

2017-01-01

Organisations have been analytically conceptualised as being somewhat analogous to individuals for a long time. They have culture; they can learn; and they can behave in various odd ways. But how far can the simile be stretched? What other types of organisational cognition can we imagine? And what

Percutaneous stone removal | van der Ness | SA Journal of Radiology

African Journals Online (AJOL)

percutaneous nephrolithotomy (PCNL) at our academic hospital. The primary objective was to determine the percentage successful PCNL procedures performed. Methods. The study included 169 patients (116 males, 53 females; mean age 45 years, range 6 - 75 years) treated with PCNL in our Department of Radiology ...

Stranger-ness and Belonging in a Neighbourhood WhatsApp Group

Directory of Open Access Journals (Sweden)

Dixon Natalie

2018-01-01

Full Text Available The messaging application WhatsApp is often adopted in urban neighbourhoods to distribute and discuss information as part of neighbourhood watch programmes. In this context, certain notions of information sharing and the cherishing this implies, are often entangled with ideals of protection in the neighbourhood. Using the case study of an enclosed neighbourhood in Johannesburg, this essay draws on theories of affect and mobility to introduce the concept of affective mooring. That is, that a neighbourhood WhatsApp group constitutes an affective mooring-an established practice and point of fixity-that generates a sense of being held in a community through feelings of collective presence and safety. Notably, these feelings of presence and safety are hinged on acts of resistance and alienation towards strangers. In this way, WhatsApp as an affective mooring in the neighbourhood is also a site for negotiating ideals of belonging.

Inhalation Toxicity of Cogenerated Graphite Flake and Fog Oil Smoke in the Brown-Headed Cowbird and the Red-Winged Blackbird, Size-Specific Inhalation Surrogates for the Red-Cockaged Woodpecker

National Research Council Canada - National Science Library

Driver, Crystal; Fulton, Robert; Ollero, Jennifer; Clark, Mark; Dennis, Gary; Tiller, Brett; Balbach, Harold E

2005-01-01

.... Conducting maneuvers under obscurant cover is important for realistic training. Generators that combine fog oil for visual obscuration with graphite flakes for infrared obscuration are being deployed for training scenarios...

Pulmonary Effects of Pyrotechnically Disseminated Titanium Dioxide Smoke in Rats

National Research Council Canada - National Science Library

Anthony, J. S; Kristovich, Robert L; McCaskey, David A; Davis, Emily A; Matson, Kathy L; Burnett, David; Gaviola, Bernardita P; Crouse, Charles L; Horsmon, Michael S; Kimmel, Edgar C

2007-01-01

The Fast Obscurant Grenade (FOG) is a bursting type grenade that has been developed within the Family of Tactical Obscuration Devices to fulfill the small through medium area screening obscuration need...

Systemic aspects of conjugal resilience in couples with a child facing cancer and marrow transplantation

Directory of Open Access Journals (Sweden)

Julie Martin

2016-09-01

Full Text Available Introduction: The negative impact of paediatric cancer on parents is well known and is even greater when intensive treatments are used. This study aimed to describe how couples whose child has received a transplant for the treatment of leukaemia view conjugal resilience and to evaluate the role of we-ness as a precursor of conjugal adjustment. Methods: Four parental couples were interviewed. Interviews were analysed in two ways: inductive thematic analysis and rating of verbal content with the We-ness Coding Scale. Results: Participants report that conjugal resilience involves the identification of the couple as a team and cohesion in the couple. Being a team generates certain collaborative interactions that lead to conjugal resilience. A sense of we-ness in parents is associated with fluctuation in the frequency of themes. Discussion: Participants’ vision of conjugal resilience introduced novel themes. The sense of we-ness facilitates cohesion and the process of conjugal resilience.

UV CONTINUUM SLOPE AND DUST OBSCURATION FROM z ∼ 6 TO z ∼ 2: THE STAR FORMATION RATE DENSITY AT HIGH REDSHIFT

International Nuclear Information System (INIS)

Bouwens, R. J.; Illingworth, G. D.; Franx, M.; Chary, R.-R.; Meurer, G. R.; Ford, H.; Conselice, C. J.; Giavalisco, M.; Van Dokkum, P.

2009-01-01

We provide a systematic measurement of the rest-frame UV continuum slope β over a wide range in redshift (z ∼ 2-6) and rest-frame UV luminosity (0.1 L* z = 3 to 2 L* z= 3 ) to improve estimates of the star formation rate (SFR) density at high redshift. We utilize the deep optical and infrared data (Advanced Camera for Surveys/NICMOS) over the Chandra Deep Field-South and Hubble Deep Field-North Great Observatories Origins Deep Survey fields, as well as the UDF for our primary UBVi 'dropout' Lyman Break Galaxy sample. We also use strong lensing clusters to identify a population of very low luminosity, high-redshift dropout galaxies. We correct the observed distributions for both selection biases and photometric scatter. We find that the UV-continuum slope of the most luminous galaxies is substantially redder at z ∼ 2-4 than it is at z ∼ 5-6 (from ∼-2.4 at z ∼ 6 to ∼-1.5 at z ∼ 2). Lower luminosity galaxies are also found to be bluer than higher luminosity galaxies at z ∼ 2.5 and z ∼ 4. We do not find a large number of galaxies with β's as red as -1 in our dropout selections at z ∼ 4, and particularly at z ∼> 5, even though such sources could be readily selected from our data (and also from Balmer Break Galaxy searches at z ∼ 4). This suggests that star-forming galaxies at z ∼> 5 almost universally have very blue UV-continuum slopes, and that there are not likely to be a substantial number of dust-obscured galaxies at z ∼> 5 that are missed in 'dropout' searches. Using the same relation between UV-continuum slope and dust extinction as has been found to be appropriate at both z ∼ 0 and z ∼ 2, we estimate the average dust extinction of galaxies as a function of redshift and UV luminosity in a consistent way. As expected, we find that the estimated dust extinction increases substantially with cosmic time for the most UV luminous galaxies, but remains small (∼ 4.

Avances en el tratamiento farmacológico de la hemorragia digestiva de origen oscuro Update on medical therapy for obscure gastrointestinal hemorrhage

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J. Molina Infante

2007-08-01

Full Text Available El desarrollo de la cápsula endoscópica y la enteroscopia de doble balón ha aumentado las tasas de diagnóstico y tratamiento en la hemorragia digestiva de origen oscuro, en la que las angiodisplasias del intestino delgado son la causa más frecuente. Sin embargo, el 25-40% de los pacientes, no subsidiarios o no respondedores a la terapéutica endoscópica, angiográfica o quirúrgica, pueden tener alto riesgo de resangrado y carecen de tratamiento médico claramente eficaz. La utilidad de la terapia hormonal está cuestionada actualmente, sin olvidar los frecuentes y limitantes efectos secundarios. El octreótido suele ser eficaz en el control de la hemorragia pero no parece la terapia de mantenimiento más óptima. Los beta-bloqueantes no selectivos, de igual manera que en la profilaxis de la hemorragia por hipertensión portal, pueden ser útiles en combinación con otros fármacos. Recientemente, el octreotido LAR, una formulación de liberación retardada que se administra una vez al mes por vía intramuscular, y la talidomida oral, un potente inhibidor de la angiogénesis, han demostrado su eficacia y seguridad a largo plazo en casos graves aislados.The development of capsule endoscopy and double-balloon enteroscopy has increased diagnostic and therapeutic rates in obscure gastrointestinal hemorrhage, where angiodysplasia of the small bowel is the most frequent cause. Nevertheless, almost 25-40% of patients who are not candidates or do not respond to endoscopic, angiographic, or surgical management may be at high risk of rebleeding, and therefore lack a clearly effective medical therapy. The utility of hormonal therapy remains unclear and is burdened by adverse effects. Subcutaneous octreotide usually controls bleeding but does not seem adequate for mainteinance therapy. Non-selective beta-blockers alone or in combination with other treatments, as in the prophylaxis of portal hypertension variceal bleeding, may be helpful. Recently

A Battlefield Obscuration Model (Smoke & Dust)

Science.gov (United States)

1979-10-01

ia £ utace of clouds, izsclacioon (incoming radiation) during :he day ts dependent upon solar ali.::ude, which is a fuc nof time of: d&7 and time of...year. ’Irnn clouds exisc, chai~r cover and :b*ickness decrease incoming and ouzgoingS radiation. Z-a this syscea iasola:ion ts estimated b7 solar ...alzictude and =odi44ed -or existing condi:±ons of total cloud cover and cloud ceiling height. kc zig~ic, estimates of oucgoing radiacion are =ade by

Anders Breivik: On Copying the Obscure

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Vincent W.J. van Gerven Oei

2011-09-01

Full Text Available Co-author of Follow Us or Die (Atropos Press, 2009—a collection of journal entries, manifestoes and even a play from people that would go on to massacre their fellow classates and students at their local schools—van Gerven Oei presents a critical analysis of Anders Breivik, the Norwegian mass murderer.

Heavily Obscured AGN with SIMBOL-X

International Nuclear Information System (INIS)

Ceca, R. Della; Caccianiga, A.; Severgnini, P.

2009-01-01

By comparing an optically selected sample of narrow lines AGN with an X-ray selected sample of AGN we have recently derived an estimate of the intrinsic (i.e. before absorption) 2-10 keV luminosity function (XLF) of Compton Thick AGNs. We will use this XLF to derive the number of Compton Thick AGN that will be found in the SIMBOL-X survey(s).

Heavily Obscured AGN with SIMBOL-X

Science.gov (United States)

Della Ceca, R.; Caccianiga, A.; Severgnini, P.

2009-05-01

By comparing an optically selected sample of narrow lines AGN with an X-ray selected sample of AGN we have recently derived an estimate of the intrinsic (i.e. before absorption) 2-10 keV luminosity function (XLF) of Compton Thick AGNs. We will use this XLF to derive the number of Compton Thick AGN that will be found in the SIMBOL-X survey(s).

Developmentalism: An Obscure but Pervasive Restriction

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J. E. Stone

1996-04-01

Full Text Available Despite continuing criticism of public education, experimentally demonstrated and field tested teaching methods have been ignored, rejected, and abandoned. Instead of a stable consensus regarding best teaching practices, there seems only an unending succession of innovations. A longstanding educational doctrine appears to underlie this anomalous state of affairs. Termed developmentalism, it presumes "natural" ontogenesis to be optimal and it requires experimentally demonstrated teaching practices to overcome a presumption that they interfere with an optimal developmental trajectory. It also discourages teachers and parents from asserting themselves with children. Instead of effective interventions, it seeks the preservation of a postulated natural perfection. Developmentalism's rich history is expressed in a literature extending over 400 years. Its notable exponents include Jean Jacques Rousseau, John Dewey, and Jean Piaget; and its most recent expressions include "developmentally appropriate practice" and "constructivism." In the years during which it gained ascendance, developmentalism served as a basis for rejecting harsh and inhumane teaching methods. Today it impedes efforts to hold schools accountable for student academic achievement.

Textural and morphological studies on zinc–iron alloy electrodeposits

Indian Academy of Sciences (India)

ness of the coating was measured in Vicker's hard- ness number (VHN) by static indentation method, using. Leco microhardness tester (Model M 400) at a given load for 15 seconds time duration. X-ray diffraction pat- terns were taken by using JEOL PANalytical, X' per. PRO model. Samples were scanned between 20. ◦ and.

Hyper IgE in Childhood Eczema and Risk of Asthma in Chinese Children.

Science.gov (United States)

Ng, Chantel; Hon, Kam Lun; Kung, Jeng Sum Charmaine; Pong, Nga Hin; Leung, Ting-Fan; Wong, Chun Kwok

2016-06-10

Atopic eczema is a common childhood disease associated with high IgE and eosinophilia. We characterized the clinical features associated with hyper-IgE (defined as IgE > 2000 IU/L) in eczema. Nottingham Eczema Severity Score (NESS), family and personal history of atopy, skin prick test (SPT) for common food and aeroallergens, highest serum IgE ever and eosinophil counts were evaluated in 330 children eczema patients. Childhood-NESS (NESS performed at 10 years of age) were further analyzed. IgE correlated with NESS (spearman coefficient 0.35, p asthma (p childhood (p asthma (exp(B) = 5.12, p = 0.002) and eczema severity during childhood and adolescence (p 10years of age, food allergen sensitization was associated with hyper-IgE (p = 0.008). Hyper-IgE is independently associated with asthma, more severe atopy and more severe eczema during childhood and adolescence. IgE > 2000 IU/L may be a tool to aid prognostication of this chronic relapsing dermatologic disease and its progression to asthma.

Stochastic theory of nonequilibrium steady states and its applications. Part I

International Nuclear Information System (INIS)

Zhang Xuejuan; Qian Hong; Qian Min

2012-01-01

The concepts of equilibrium and nonequilibrium steady states are introduced in the present review as mathematical concepts associated with stationary Markov processes. For both discrete stochastic systems with master equations and continuous diffusion processes with Fokker–Planck equations, the nonequilibrium steady state (NESS) is characterized in terms of several key notions which are originated from nonequilibrium physics: time irreversibility, breakdown of detailed balance, free energy dissipation, and positive entropy production rate. After presenting this NESS theory in pedagogically accessible mathematical terms that require only a minimal amount of prerequisites in nonlinear differential equations and the theory of probability, it is applied, in Part I, to two widely studied problems: the stochastic resonance (also known as coherent resonance) and molecular motors (also known as Brownian ratchet). Although both areas have advanced rapidly on their own with a vast amount of literature, the theory of NESS provides them with a unifying mathematical foundation. Part II of this review contains applications of the NESS theory to processes from cellular biochemistry, ranging from enzyme catalyzed reactions, kinetic proofreading, to zeroth-order ultrasensitivity.

for presence of hookworms (Uncinaria spp. on San Miguel Island, California

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Lyons E. T.

2016-06-01

Full Text Available Necropsy and extensive parasitological examination of dead northern elephant seal (NES pups was done on San Miguel Island, California, in February, 2015. The main interest in the current study was to determine if hookworms were present in NESs on San Miguel Island where two hookworm species of the genus Uncinaria are known to be present - Uncinaria lyonsi in California sea lions and Uncinaria lucasi in northern fur seals. Hookworms were not detected in any of the NESs examined: stomachs or intestines of 16 pups, blubber of 13 pups and blubber of one bull. The results obtained in the present study of NESs on San Miguel Island plus similar finding on Año Nuevo State Reserve and The Marine Mammal Center provide strong indication that NES are not appropriate hosts for Uncinaria spp. Hookworm free-living third stage larvae, developed from eggs of California sea lions and northern fur seals, were recovered from sand. It seems that at this time, further search for hookworms in NESs would be nonproductive.

Bloqueio peridural caudal: técnica anestésica de uso exclusivo em crianças? É possível sua realização em adultos? Qual o papel do ultrassom nesse contexto?

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Ilana Esquenazi Najman

2011-02-01

Full Text Available JUSTIFICATIVA E OBJETIVOS: O bloqueio peridural caudal é a mais popular entre todas as técnicas de anestesia regional em crianças. Com o avanço da idade, apenas a relativa dificuldade em localizar o hiato sacral limita seu uso. Entretanto, em adultos a técnica vem sendo largamente utilizada para controle de dor crônica com o auxílio da fluoroscopia. Assim, a habilidade em localizar o hiato e definir as variações anatômicas é o principal fator determinante do sucesso e segurança na execução do bloqueio peridural pela via caudal. Nesse contexto, o ultrassom vem ganhando espaço como guia para a realização do bloqueio caudal. O objetivo desta revisão foi elucidar o papel do ultrassom na anestesia caudal, além de demonstrar que o bloqueio caudal, muito utilizado em crianças, também é útil e pode ser usado em adultos. CONTEÚDO: Uma revisão literária sobre a anatomia da região sacral e da técnica anestésica necessária para a realização adequada do bloqueio caudal foi promovida. Além disso, artigos recentes sobre estudos realizados com bloqueios peridurais caudais guiados por ultrassom tanto em crianças quanto em adultos também foram incluídos. CONCLUSÕES: O ultrassom, apesar de suas limitações, pode ser útil como ferramenta adjuvante no posicionamento da agulha no espaço caudal. Permite a fácil identificação da anatomia sacral, além de visualização da injeção, em tempo real. Sua natureza portátil, não invasiva e livre de exposição à radiação faz dele uma tecnologia atrativa na sala operatória, principalmente na emergência de casos difíceis. Entretanto, como seu uso em bloqueios centrais do neuroeixo ainda é muito primitivo, é necessário que mais pesquisas sejam feitas para se consagre como técnica de rotina na prática anestésica.

NESmapper: accurate prediction of leucine-rich nuclear export signals using activity-based profiles.

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Shunichi Kosugi

2014-09-01

Full Text Available The nuclear export of proteins is regulated largely through the exportin/CRM1 pathway, which involves the specific recognition of leucine-rich nuclear export signals (NESs in the cargo proteins, and modulates nuclear-cytoplasmic protein shuttling by antagonizing the nuclear import activity mediated by importins and the nuclear import signal (NLS. Although the prediction of NESs can help to define proteins that undergo regulated nuclear export, current methods of predicting NESs, including computational tools and consensus-sequence-based searches, have limited accuracy, especially in terms of their specificity. We found that each residue within an NES largely contributes independently and additively to the entire nuclear export activity. We created activity-based profiles of all classes of NESs with a comprehensive mutational analysis in mammalian cells. The profiles highlight a number of specific activity-affecting residues not only at the conserved hydrophobic positions but also in the linker and flanking regions. We then developed a computational tool, NESmapper, to predict NESs by using profiles that had been further optimized by training and combining the amino acid properties of the NES-flanking regions. This tool successfully reduced the considerable number of false positives, and the overall prediction accuracy was higher than that of other methods, including NESsential and Wregex. This profile-based prediction strategy is a reliable way to identify functional protein motifs. NESmapper is available at http://sourceforge.net/projects/nesmapper.

Missing Things and Methodological Swerves: Unsettling the It-Ness of VET

Science.gov (United States)

Shore, Sue; Butler, Elaine

2012-01-01

This paper argues for approaches to research methodologies that interrupt the machinic metaphors and relationships for living circulating in so much VET research. Using the schematic of "cyborg as a figuration" and Wilson's (2009) four epistemological interventions (witnessing, situating, diffracting, acquiring) the authors practice a form of…

Educational Status, Aware Ness and Sources of Information of Osteoporosis Patients

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Yeşim Gökçe Kutsal

2002-09-01

Full Text Available Osteoporosis is one of the major public health problems. Higher prevalence of most chronic diseases has been encountered in less educated subjects. Aim of this study was to assess educational status, knowledge and sources of information among subjects with osteoporosis. A multicentered trial involving 10 centers was carried out. Patients with bone mineral densities below –2.5 standard deviations either in femoral or lomber region were included in the study. Age, sex, height, weight, educational status, clothing style, drugs used for osteoporosis, age at menarche, age at menopause, type of menopause, oral contraception, presence of chronic disease, smoking status, physical activity level, calcium intake, knowledge about osteoporosis and sources of information was gathered using a questionnaire. 54 % of our patients had knowledge about osteoporosis. Doctors were the most commonly utilized source of information (56.8%. Patients were divided into 3 groups according to educational status: less than 5 years (392 patients, 68.9 %, 6 to 8 years (53 patients, 9.3 % and more than 9 years (124 patients, 21.8 %. Body mass index, presence of obesity, smoking status and physical activity levels were significantly different between the groups. Knowledge about osteoporosis was compared according to years of formal education. 43.7 % of patients with formal education less than five years, 62.3 % of patients with formal education 6-8 years and 83.7 % of patients with formal education more than 9 years had knowledge about osteoporosis. Knowledge about osteoporosis was significantly different between groups. Patients within different geographical regions were compared. Educational status, clothing style, smoking status, activity levels, calcium intake and knowledge about osteoporosis was found to be statistically significantly different between the groups. Education of both patients and doctors will lead to better understanding of concept of “bone health”.

Good parenthood and the constitution of we-ness in everyday life

DEFF Research Database (Denmark)

Westerling, Allan

2014-01-01

This paper analyzes the practice and meaning of good parenthood in contemporary family life. It focusing on the so-°©‐called reconstituted families, parenting post divorce. The paper explores practices and narratives of sharing parental responsibility in everyday life among parents who do not live...

The Australian-Ness of Curriculum Jigsaws: Where Does Environmental Education Fit?

Science.gov (United States)

Gough, Annette

2011-01-01

This paper reviews Australian Government actions related to environmental education, particularly in the past decade, and examines the actions forthcoming from two national action plans (Environment Australia, 2000 and DEWHA, 2009), the implementation strategy for the Decade of ESD (DEWHA, 2006) and developments related to the Australian…

High levels of absorption in orientation-unbiased, radio-selected 3CR Active Galaxies

Science.gov (United States)

Wilkes, Belinda J.; Haas, Martin; Barthel, Peter; Leipski, Christian; Kuraszkiewicz, Joanna; Worrall, Diana; Birkinshaw, Mark; Willner, Steven P.

2014-08-01

A critical problem in understanding active galaxies (AGN) is the separation of intrinsic physical differences from observed differences that are due to orientation. Obscuration of the active nucleus is anisotropic and strongly frequency dependent leading to complex selection effects for observations in most wavebands. These can only be quantified using a sample that is sufficiently unbiased to test orientation effects. Low-frequency radio emission is one way to select a close-to orientation-unbiased sample, albeit limited to the minority of AGN with strong radio emission.Recent Chandra, Spitzer and Herschel observations combined with multi-wavelength data for a complete sample of high-redshift (1half the sample is significantly obscured with ratios of unobscured: Compton thin (22 24.2) = 2.5:1.4:1 in these high-luminosity (log L(0.3-8keV) ~ 44-46) sources. These ratios are consistent with current expectations based on modelingthe Cosmic X-ray Background. A strong correlation with radio orientation constrains the geometry of the obscuring disk/torus to have a ~60 degree opening angle and ~12 degree Compton-thick cross-section. The deduced ~50% obscured fraction of the population contrasts with typical estimates of ~20% obscured in optically- and X-ray-selected high-luminosity samples. Once the primary nuclear emission is obscured, AGN X-ray spectra are frequently dominated by unobscured non-nuclear or scattered nuclear emission which cannot be distinguished from direct nuclear emission with a lower obscuration level unless high quality data is available. As a result, both the level of obscuration and the estimated instrinsic luminosities of highly-obscured AGN are likely to be significantly (*10-1000) underestimated for 25-50% of the population. This may explain the lower obscured fractions reported for optical and X-ray samples which have no independent measure of the AGN luminosity. Correcting AGN samples for these underestimated luminosities would result in

Ground based THz Spectroscopy of Obscured Starbursts in the Early Universe enabled by the 2nd generation Redshift (z) & Early Universe Spectrometer (ZEUS-2)

Science.gov (United States)

Vishwas, Amit; Stacey, Gordon; Nikola, Thomas; Ferkinhoff, Carl; Parshley, Stephen; Schoenwald, Justin; Lamarche, Cody James; Higdon, James; Higdon, Sarah; Brisbin, Drew; Güesten, Rolf; Weiss, Axel; Menten, Karl; Irwin, Kent; Cho, Hsiao-Mei; Niemack, Michael; Hilton, Gene; Hubmayr, Johannes; Amiri, Mandana; Halpern, Mark; Wiebe, Donald; Hasselfield, Matthew; Ade, Peter; Tucker, Carole

2018-01-01

Galaxies were surprisingly dusty in the early Universe, with more than half of the light emitted from stars being absorbed by dust within the system and re-radiated into far infrared (FIR, ~50-150μm) wavelengths. Dusty star forming galaxies (DSFGs) dominate the co-moving star formation rate density of the Universe that peaks around redshift, z~2, making it compelling to study them in rest frame FIR bands. From galaxies at z > 1, the FIR line emission from abundant ions like [O III], [C II] and [N II], are redshifted into the short sub-mm telluric windows. My thesis work is based on building and deploying the 2nd Generation Redshift (z) and Early Universe Spectrometer (ZEUS-2), a long-slit, echelle grating spectrometer optimized to study broad (Δv = 300km/s) spectral lines from galaxies in the 200-650µm telluric windows using TES bolometers. These far-IR lines being extinction free and major coolants of the gas heated by (young) massive stars, are powerful probes of the physical conditions of the gas and the stellar radiation field. I present results from our survey of the [O III] 88µm line in galaxies at redshift, z ~ 2.8 to 4.6, with ZEUS-2 at the Atacama Pathfinder Experiment (APEX) Telescope. To interpret our observations along with ancillary data from optical to radio facilities, we apply photoionization models for HII regions and Photo Dissociation Region (PDR) models and confirm that the galaxies host substantial ongoing obscured star formation. The presence of doubly ionized oxygen suggests hard radiation fields and hence, elevated ionization parameters that can only be accounted for by a large population of massive stars formed during the ongoing starburst, that contribute a large fraction of the infrared luminosity. This study highlights the use of FIR line emission to trace the assembly of current day massive galaxies, conditions of star formation and details of their stellar populations. The construction and operation of ZEUS-2 were funded by NSF ATI

The role of non-equilibrium fluxes in the relaxation processes of the linear chemical master equation.

Science.gov (United States)

de Oliveira, Luciana Renata; Bazzani, Armando; Giampieri, Enrico; Castellani, Gastone C

2014-08-14

We propose a non-equilibrium thermodynamical description in terms of the Chemical Master Equation (CME) to characterize the dynamics of a chemical cycle chain reaction among m different species. These systems can be closed or open for energy and molecules exchange with the environment, which determines how they relax to the stationary state. Closed systems reach an equilibrium state (characterized by the detailed balance condition (D.B.)), while open systems will reach a non-equilibrium steady state (NESS). The principal difference between D.B. and NESS is due to the presence of chemical fluxes. In the D.B. condition the fluxes are absent while for the NESS case, the chemical fluxes are necessary for the state maintaining. All the biological systems are characterized by their "far from equilibrium behavior," hence the NESS is a good candidate for a realistic description of the dynamical and thermodynamical properties of living organisms. In this work we consider a CME written in terms of a discrete Kolmogorov forward equation, which lead us to write explicitly the non-equilibrium chemical fluxes. For systems in NESS, we show that there is a non-conservative "external vector field" whose is linearly proportional to the chemical fluxes. We also demonstrate that the modulation of these external fields does not change their stationary distributions, which ensure us to study the same system and outline the differences in the system's behavior when it switches from the D.B. regime to NESS. We were interested to see how the non-equilibrium fluxes influence the relaxation process during the reaching of the stationary distribution. By performing analytical and numerical analysis, our central result is that the presence of the non-equilibrium chemical fluxes reduces the characteristic relaxation time with respect to the D.B. condition. Within a biochemical and biological perspective, this result can be related to the "plasticity property" of biological systems and to their

The role of non-equilibrium fluxes in the relaxation processes of the linear chemical master equation

International Nuclear Information System (INIS)

Oliveira, Luciana Renata de; Bazzani, Armando; Giampieri, Enrico; Castellani, Gastone C.

2014-01-01

We propose a non-equilibrium thermodynamical description in terms of the Chemical Master Equation (CME) to characterize the dynamics of a chemical cycle chain reaction among m different species. These systems can be closed or open for energy and molecules exchange with the environment, which determines how they relax to the stationary state. Closed systems reach an equilibrium state (characterized by the detailed balance condition (D.B.)), while open systems will reach a non-equilibrium steady state (NESS). The principal difference between D.B. and NESS is due to the presence of chemical fluxes. In the D.B. condition the fluxes are absent while for the NESS case, the chemical fluxes are necessary for the state maintaining. All the biological systems are characterized by their “far from equilibrium behavior,” hence the NESS is a good candidate for a realistic description of the dynamical and thermodynamical properties of living organisms. In this work we consider a CME written in terms of a discrete Kolmogorov forward equation, which lead us to write explicitly the non-equilibrium chemical fluxes. For systems in NESS, we show that there is a non-conservative “external vector field” whose is linearly proportional to the chemical fluxes. We also demonstrate that the modulation of these external fields does not change their stationary distributions, which ensure us to study the same system and outline the differences in the system's behavior when it switches from the D.B. regime to NESS. We were interested to see how the non-equilibrium fluxes influence the relaxation process during the reaching of the stationary distribution. By performing analytical and numerical analysis, our central result is that the presence of the non-equilibrium chemical fluxes reduces the characteristic relaxation time with respect to the D.B. condition. Within a biochemical and biological perspective, this result can be related to the “plasticity property” of biological

Comportamento ingestivo diurno de vacas primíparas em pastagem nativa dominada por capim-annoni-2 com suplementação proteica e mineral em diversas estações climáticas Diurnal ingestive behaviour of pregnant heifers grazing on natural grasslands invaded by Eragrostis plana Ness as affected by protein and mineral supplements in the different climatic seasons

Directory of Open Access Journals (Sweden)

Silvane Barcelos Carlotto

2010-03-01

Full Text Available Avaliou-se a influência da suplementação proteica e mineral sobre o comportamento ingestivo de vacas primíparas em pastagem nativa dominada por capim-annoni-2 (Eragrostis plana Ness recebendo suplementação com sal comum; sal mineral; sal proteinado; ou sal para reprodução e sal proteinado (1:1. Testou-se a hipótese de que suplementos minerais e proteinados pudessem promover alterações no comportamento ingestivo dos animais em pastejo. O estudo foi desenvolvido em uma área de 37 ha de pastagem nativa invadida por capim-annoni-2, dividida em oito potreiros (unidades experimentais. Os animais foram avaliados no período diurno, por dois dias consecutivos, em cada uma das estações climáticas, de abril de 2006 a março de 2007. O delineamento experimental foi inteiramente casualizado com duas repetições. Os tempos de pastejo, de ruminação, de ócio e de outras atividades não diferiram entre suplementos, e os valores médios diários para essas atividades foram 505, 108, 70 e 11 minutos, respectivamente. Os tempos de pastejo, ruminação e ócio e a taxa de bocados diferiram significativamente entre as estações climáticas. A suplementação proteica e mineral não promove alterações significativas no comportamento ingestivo dos animais. O comportamento ingestivo, no entanto, é influenciado pelas estações climáticas.The influence was assessed of protein and mineral supplementation on the ingestive behavior of pregnant heifers on a native grassland dominated by capim-annoni-2 (Eragrostis plana Ness supplementation with common salt, mineral salt, protein salt and protein salt and reproduction salt (1:1. The hypothesis was tested that different mineral and protein salt supplements could promote alterations in the animal grazing ingestive behavior. The study was carried out in a 37 ha area of native pasture invaded by capim-annoni-2, divided into 8 paddocks (experimental units. The animals were evaluated during the daylight

UV Continuum Slope and Dust Obscuration from z ~ 6 to z ~ 2: The Star Formation Rate Density at High Redshift

Science.gov (United States)

Bouwens, R. J.; Illingworth, G. D.; Franx, M.; Chary, R.-R.; Meurer, G. R.; Conselice, C. J.; Ford, H.; Giavalisco, M.; van Dokkum, P.

2009-11-01

We provide a systematic measurement of the rest-frame UV continuum slope β over a wide range in redshift (z ~ 2-6) and rest-frame UV luminosity (0.1 L* z = 3 to 2 L* z = 3) to improve estimates of the star formation rate (SFR) density at high redshift. We utilize the deep optical and infrared data (Advanced Camera for Surveys/NICMOS) over the Chandra Deep Field-South and Hubble Deep Field-North Great Observatories Origins Deep Survey fields, as well as the UDF for our primary UBVi "dropout" Lyman Break Galaxy sample. We also use strong lensing clusters to identify a population of very low luminosity, high-redshift dropout galaxies. We correct the observed distributions for both selection biases and photometric scatter. We find that the UV-continuum slope of the most luminous galaxies is substantially redder at z ~ 2-4 than it is at z ~ 5-6 (from ~-2.4 at z ~ 6 to ~-1.5 at z ~ 2). Lower luminosity galaxies are also found to be bluer than higher luminosity galaxies at z ~ 2.5 and z ~ 4. We do not find a large number of galaxies with β's as red as -1 in our dropout selections at z ~ 4, and particularly at z gsim 5, even though such sources could be readily selected from our data (and also from Balmer Break Galaxy searches at z ~ 4). This suggests that star-forming galaxies at z gsim 5 almost universally have very blue UV-continuum slopes, and that there are not likely to be a substantial number of dust-obscured galaxies at z gsim 5 that are missed in "dropout" searches. Using the same relation between UV-continuum slope and dust extinction as has been found to be appropriate at both z ~ 0 and z ~ 2, we estimate the average dust extinction of galaxies as a function of redshift and UV luminosity in a consistent way. As expected, we find that the estimated dust extinction increases substantially with cosmic time for the most UV luminous galaxies, but remains small (lsim2 times) at all times for lower luminosity galaxies. Because these same lower luminosity galaxies

The Compton-thick Growth of Supermassive Black Holes constrained

Science.gov (United States)

Buchner, J.; Georgakakis, A.; Nandra, K.

2017-10-01

A heavily obscured growth phase of supermassive black holes (SMBH) is thought to be important in the co-evolution with galaxies. X-rays provide a clean and efficient selection of unobscured and obscured AGN. Recent work with deeper observations and improved analysis methodology allowed us to extend constraints to Compton-thick number densities. We present the first luminosity function of Compton-thick AGN at z=0.5-4 and constrain the overall mass density locked into black holes over cosmic time, a fundamental constraint for cosmological simulations. Recent studies including ours find that the obscuration is redshift and luminosity-dependent in a complex way, which rules out entire sets of obscurer models. A new paradigm, the radiation-lifted torus model, is proposed, in which the obscurer is Eddington-rate dependent and accretion creates and displaces torus clouds. We place observational limits on the behaviour of this mechanism.

A Relative Ranking Approach for Nano-Enabled Applications to Improve Risk-Based Decision Making: A Case Study of Army Materiel

Science.gov (United States)

2014-12-24

accidental expo- sures to carbon nanotubes and copper flakes incorporated into energy and obscurant materiel by Army workers rank highest relative to...that inhalation from accidental exposures to carbon nanotubes and copper flakes incorporated into energy and obscurant materiel by Army workers rank... copper (Cu), and titanium (Ti) flakes used in smokes and obscurants ranked the highest on the risk scale for sce- narios primarily involving accidental

Simultaneous Mean and Covariance Correction Filter for Orbit Estimation.

Science.gov (United States)

Wang, Xiaoxu; Pan, Quan; Ding, Zhengtao; Ma, Zhengya

2018-05-05

This paper proposes a novel filtering design, from a viewpoint of identification instead of the conventional nonlinear estimation schemes (NESs), to improve the performance of orbit state estimation for a space target. First, a nonlinear perturbation is viewed or modeled as an unknown input (UI) coupled with the orbit state, to avoid the intractable nonlinear perturbation integral (INPI) required by NESs. Then, a simultaneous mean and covariance correction filter (SMCCF), based on a two-stage expectation maximization (EM) framework, is proposed to simply and analytically fit or identify the first two moments (FTM) of the perturbation (viewed as UI), instead of directly computing such the INPI in NESs. Orbit estimation performance is greatly improved by utilizing the fit UI-FTM to simultaneously correct the state estimation and its covariance. Third, depending on whether enough information is mined, SMCCF should outperform existing NESs or the standard identification algorithms (which view the UI as a constant independent of the state and only utilize the identified UI-mean to correct the state estimation, regardless of its covariance), since it further incorporates the useful covariance information in addition to the mean of the UI. Finally, our simulations demonstrate the superior performance of SMCCF via an orbit estimation example.

MISALIGNED DISKS AS OBSCURERS IN ACTIVE GALAXIES

International Nuclear Information System (INIS)

Lawrence, Andy; Elvis, Martin

2010-01-01

We critically review the evidence concerning the fraction of active galactic nuclei (AGNs) that appear as Type 2 AGNs, carefully distinguishing strict Type 2 AGNs from both more lightly reddened Type 1 AGNs, and from low excitation narrow line AGNs, which may represent a different mode of activity. Low-excitation AGNs occur predominantly at low luminosities; after removing these, true Type 2 AGNs represent 58% ± 5% of all AGNs, and lightly reddened Type 1 AGNs a further ∼15%. Radio, IR, and volume-limited samples all agree in showing no change of Type 2 fraction with luminosity. X-ray samples do show a change with luminosity; we discuss possible reasons for this discrepancy. We test a very simple picture which produces this Type 2 fraction with minimal assumptions. In this picture, infall from large scales occurs in random directions, but must eventually align with the inner accretion flow, producing a severely warped disk on parsec scales. If the re-alignment is dominated by tilt, with minimal twist, a wide range of covering factors is predicted in individual objects, but with an expected mean fraction of Type 2 AGNs of exactly 50%. This 'tilted disk' picture predicts reasonable alignment of observed nuclear structures on average, but with distinct misalignments in individual cases. Initial case studies of the few well-resolved objects show that such misalignments are indeed present.

A case of jaundice of obscure origin.

Science.gov (United States)

Khan, Fahad M; Alcorn, Joseph; Hanson, Joshua

2014-05-01

Idiopathic painless jaundice with significant elevations in serum transaminases, occurring in a previously healthy patient, invokes a circumscribed set of possibilities including viral hepatitis, auto-immune hepatitis (AIH) and drug-induced liver injury (DILI). In this described case, common causes of cholestatic jaundice were considered including drug-induced liver injury, viral causes of hepatitis, and auto-immune antibodies. Biliary obstruction was excluded by appropriate imaging studies. Liver biopsy was obtained, though not definitive. After detailed investigation failed to reveal a cause of the jaundice, an empiric trial of steroids was initiated on the possibility that our patient had antibody-negative AIH and not DILI, with an associated grave prognosis. Empiric treatment with prednisone led to rapid resolution of jaundice and to the conclusion that the correct diagnosis was antibody-negative AIH.

Light Obscuration Particle Counter Fuel Contamination Limits

Science.gov (United States)

2015-10-08

two methods for measuring particulate contamination by gravimetric analysis: ASTM D2276 - Standard Test Method for Particulate Contaminant in Aviation...problems with the gravimetric methods is the poor repeatability and reproducibility of the methods , ASTM D2276 has a repeatability of 0.25 mg/L and...collected failing either the particle count or the gravimetric limit, 314 of which failed both methods . 245 false negatives were recorded where the

Evidence for circumstellar obscuration of OB stars

International Nuclear Information System (INIS)

Bohannan, B.

1975-01-01

Reddish found a strong increase of color excess with increasing stellar luminosity: here referred to as the Reddish Effect: in ten young galactic clusters and associations. New photometric and spectroscopic observations drawn from the literature are combined with data used by Reddish to reconsider the color excess versus intrinsic magnitude diagrams of the same ten stellar groups. The reality of the Effect is questioned in all but one of the systems; this was accomplished by identifying possible foreground stars and by recognizing some of the brightest stars as supergiants, then applying correct intrinsic color indices. After careful reanalysis, the one stellar group to retain an indication of the Reddish Effect is Cygnus OB2. No correlation of reddening with luminosity was found for five additional very young stellar groups in the southern hemisphere; these groups should exhibit the Effect if it is a natural consequence of stellar evolution. Reddish ascribed the correlation to massive circumstellar remnants of material from which the stars formed. However, a peculiar dispersion in color excess could also be attributed to patchy dust within the stellar group. In several stellar systems previously identified as displaying the Reddish Effect, a correlation of observed color excess with dust and gas concentrations is noted on Palomar Sky Survey prints. If present, circumstellar dust clouds should []anifest their existence in modes other than a correlation of color excess with luminosity. The following possibilities are considered and all show negative results: correlation of color excess with spectral type; correlation of reddening slope E/subU//sub -//subB//E/subB//sub -//subV/ with spectral type; observable infrared excess. The preceding astrophysical arguments strongly imply that circumstellar dust remnants from stellar formation do not remain around stars during their main-sequence lifetimes. (auth)

ROLE OF DIAGNOSTIC LAPAROSCOPY IN OBSCURE ASCITES ...

African Journals Online (AJOL)

Scientific Medical Journal. Journal Home · ABOUT THIS JOURNAL · Advanced Search · Current Issue · Archives · Journal Home > Vol 12, No 4 (2000) >. Log in or Register to get access to full text downloads.

Hyper IgE in Childhood Eczema and Risk of Asthma in Chinese Children

Directory of Open Access Journals (Sweden)

Chantel Ng

2016-06-01

Full Text Available Background: Atopic eczema is a common childhood disease associated with high IgE and eosinophilia. We characterized the clinical features associated with hyper-IgE (defined as IgE > 2000 IU/L in eczema. Methods: Nottingham Eczema Severity Score (NESS, family and personal history of atopy, skin prick test (SPT for common food and aeroallergens, highest serum IgE ever and eosinophil counts were evaluated in 330 children eczema patients. Childhood-NESS (NESS performed at <10 years of age and adolescent-NESS (NESS performed at >10 years of age were further analyzed. Results: IgE correlated with NESS (spearman coefficient 0.35, p < 0.001 and eosinophil percentage (spearman coefficient 0.56, p = 0.001. Compared with IgE ≤ 2000IU/L (n = 167, patients with hyper-IgE (n = 163 were associated with male gender (p = 0.002; paternal atopy (p = 0.026; personal history of atopic rhinitis (p = 0.016; asthma (p < 0.001; dietary avoidance (p < 0.001; use of wet wrap (p < 0.001; traditional Chinese medicine use (TCM, p < 0.001; immunomodulant use (azathioprine or cyclosporine, p < 0.001; skin prick sensitization by dust mites (p < 0.001, cats (p = 0.012, dogs (p = 0.018, food (p = 0.002; eosinophilia (p < 0.001; more severe disease during childhood (p < 0.0001 and during adolescence (p < 0.0001, but not onset age of eczema or maternal atopy. Logistic regression showed that hyper-IgE was associated with personal history of asthma (exp(B = 5.12, p = 0.002 and eczema severity during childhood and adolescence (p < 0.001. For patients <10 years of age, dust mite sensitization (p = 0.008 was associated with hyper-IgE. For patients >10years of age, food allergen sensitization was associated with hyper-IgE (p = 0.008. Conclusions: Hyper-IgE is independently associated with asthma, more severe atopy and more severe eczema during childhood and adolescence. IgE > 2000 IU/L may be a tool to aid prognostication of this chronic relapsing dermatologic disease and its

Dissipation, generalized free energy, and a self-consistent nonequilibrium thermodynamics of chemically driven open subsystems.

Science.gov (United States)

Ge, Hao; Qian, Hong

2013-06-01

Nonequilibrium thermodynamics of a system situated in a sustained environment with influx and efflux is usually treated as a subsystem in a larger, closed "universe." A question remains with regard to what the minimally required description for the surrounding of such an open driven system is so that its nonequilibrium thermodynamics can be established solely based on the internal stochastic kinetics. We provide a solution to this problem using insights from studies of molecular motors in a chemical nonequilibrium steady state (NESS) with sustained external drive through a regenerating system or in a quasisteady state (QSS) with an excess amount of adenosine triphosphate (ATP), adenosine diphosphate (ADP), and inorganic phosphate (Pi). We introduce the key notion of minimal work that is needed, W(min), for the external regenerating system to sustain a NESS (e.g., maintaining constant concentrations of ATP, ADP and Pi for a molecular motor). Using a Markov (master-equation) description of a motor protein, we illustrate that the NESS and QSS have identical kinetics as well as the second law in terms of the same positive entropy production rate. The heat dissipation of a NESS without mechanical output is exactly the W(min). This provides a justification for introducing an ideal external regenerating system and yields a free-energy balance equation between the net free-energy input F(in) and total dissipation F(dis) in an NESS: F(in) consists of chemical input minus mechanical output; F(dis) consists of dissipative heat, i.e. the amount of useful energy becoming heat, which also equals the NESS entropy production. Furthermore, we show that for nonstationary systems, the F(dis) and F(in) correspond to the entropy production rate and housekeeping heat in stochastic thermodynamics and identify a relative entropy H as a generalized free energy. We reach a new formulation of Markovian nonequilibrium thermodynamics based on only the internal kinetic equation without further

Desenvolvimento de líderes na educação básica: uma proposta para a formação de estudantes

OpenAIRE

Patrícia Roberta Pinheiro Pereira; Júlio Fernando da Silva

2016-01-01

O estudo da liderança está presente em inúmeros setores da sociedade, extrapolando o âmbito empresarial. Por esse motivo, um avanço nesse campo é a incorporação de uma proposta de desenvolvimento de líderes ao contexto educacional. Nesse sentido, o presente ensaio busca compreender como desenvolver líderes na educação básica através de metodologias educacionais voltadas para essa finalidade. Const...

A second perspective on the Amann–Schmiedl–Seifert criterion for non-equilibrium in a three-state system

International Nuclear Information System (INIS)

Jia, Chen; Chen, Yong

2015-01-01

In the work of Amann, Schmiedl and Seifert (2010 J. Chem. Phys. 132 041102), the authors derived a sufficient criterion to identify a non-equilibrium steady state (NESS) in a three-state Markov system based on the coarse-grained information of two-state trajectories. In this paper, we present a mathematical derivation and provide a probabilistic interpretation of the Amann–Schmiedl–Seifert (ASS) criterion. Moreover, the ASS criterion is compared with some other criterions for a NESS. (paper)

Auld Rock meets Nordic Noir: A Danish gaze on Shetlandic Scandinavian-ness

DEFF Research Database (Denmark)

Tange, Hanne; Agger, Gunhild

as a symbolic marker of Shetland’s link to Scandinavia. The Nordic connection has been used by artists to claim the existence of a distinctively Shetlandic tradition. In this paper we examine Shetland’s invented North through the lens by our indigenous knowledge of Danish language and heritage, asking to what...... is the motto of the Shetland Islands Council, Med logum skal land byggja, which Danes know as the prologue to the Jutland Law of 1241. Next we examine how space and language come together to create a sense of Nordic difference in Robert Alan Jamieson’s Da Happie Laand (2010). Finally, we look at Ann Cleaves...

Thought 2 Talk

DEFF Research Database (Denmark)

Hendricks, Vincent F.

Thought2Talk is a crash course on argument, reasoning and logical method honoring the Swedish poet and Bishop of Lund, Esaias Tegnér, who once said: The words and thoughts of men are born together: To speak obscurely is to think obscurely. In 100 humorous yet erudite pages, Thought2Talk takes the...... the reader through key concepts like statement, argument, validity, fallacy, modality and demonstration.......Thought2Talk is a crash course on argument, reasoning and logical method honoring the Swedish poet and Bishop of Lund, Esaias Tegnér, who once said: The words and thoughts of men are born together: To speak obscurely is to think obscurely. In 100 humorous yet erudite pages, Thought2Talk takes...

Measurement of Fog Oil Penetration into Model Underground Burrow and Hollow Tree Nest Cavities

National Research Council Canada - National Science Library

Guelta, Mark A; Balbach, Harold E

2007-01-01

.... On installations where troop readiness training is conducted, an important component of realistic troop readiness training is the generation of obscurant material and the conduct of maneuvers under obscurant cover. Fog oil (FO...

Sustained currents in coupled diffusive systems

International Nuclear Information System (INIS)

Larralde, Hernán; Sanders, David P

2014-01-01

Coupling two diffusive systems may give rise to a nonequilibrium stationary state (NESS) with a non-trivial persistent, circulating current. We study a simple example that is exactly soluble, consisting of random walkers with different biases towards a reflecting boundary, modelling, for example, Brownian particles with different charge states in an electric field. We obtain analytical expressions for the concentrations and currents in the NESS for this model, and exhibit the main features of the system by numerical simulation. (paper)

Prepositions in MSA and English

Directory of Open Access Journals (Sweden)

Saad Nasser Aldwayan

2013-01-01

Full Text Available Spatial scenes are identical in the world languages. However, cultures may diverge in profiling spatial scenes (Levinson 2003. This paper selects for study the prepositions in and on in English and their Modern Standard Arabic (MSA counterparts fi and 3ala, arguing that MSA and English seem to diverge in the spatial configurations and meanings of these prepositions. The sub-schemas of CONTAINMENT (in-ness in MSA are found to partially overlap with those of English, with the other sub-schemas being taken care of by SUPPORT (on-ness and PUNCTUALITY (point-ness. Such differences classify MSA more as a CONTAINMENT-based language than English, which seems to prefer SUPPORT and PUNCTUALITY. However, English and MSA seem to converge in their metaphoric conceptualizations of states owing to conceptual embodiment (Lakoff 1987. The article discusses the implications of such findings for spatial cognition and cultural cognition and EFL/ESL writing and translating.

Stochastic theory of nonequilibrium steady states. Part II: Applications in chemical biophysics

International Nuclear Information System (INIS)

Ge Hao; Qian Min; Qian Hong

2012-01-01

The mathematical theory of nonequilibrium steady state (NESS) has a natural application in open biochemical systems which have sustained source(s) and sink(s) in terms of a difference in their chemical potentials. After a brief introduction in Section , in Part II of this review, we present the widely studied biochemical enzyme kinetics, the workhorse of biochemical dynamic modeling, in terms of the theory of NESS (Section ). We then show that several phenomena in enzyme kinetics, including a newly discovered activation–inhibition switching (Section ) and the well-known non-Michaelis–Menten-cooperativity (Section ) and kinetic proofreading (Section ), are all consequences of the NESS of driven biochemical systems with associated cycle fluxes. Section is focused on nonlinear and nonequilibrium systems of biochemical reactions. We use the phosphorylation–dephosphorylation cycle (PdPC), one of the most important biochemical signaling networks, as an example (Section ). It starts with a brief introduction of the Delbrück–Gillespie process approach to mesoscopic biochemical kinetics (Sections ). We shall discuss the zeroth-order ultrasensitivity of PdPC in terms of a new concept — the temporal cooperativity (Sections ), as well as PdPC with feedback which leads to biochemical nonlinear bistability (Section ). Also, both are nonequilibrium phenomena. PdPC with a nonlinear feedback is kinetically isomorphic to a self-regulating gene expression network, hence the theory of NESS discussed here could have wide applications to many other biochemical systems.

Combustion Control System Design of Diesel Engine via ASPR based Output Feedback Control Strategy with a PFC

Science.gov (United States)

Mizumoto, Ikuro; Tsunematsu, Junpei; Fujii, Seiya

2016-09-01

In this paper, a design method of an output feedback control system with a simple feedforward input for a combustion model of diesel engine will be proposed based on the almost strictly positive real-ness (ASPR-ness) of the controlled system for a combustion control of diesel engines. A parallel feedforward compensator (PFC) design scheme which renders the resulting augmented controlled system ASPR will also be proposed in order to design a stable output feedback control system for the considered combustion model. The effectiveness of our proposed method will be confirmed through numerical simulations.

BIOPROSPECÇÃO DE ANTIBIÓTICOS PRODUZIDOS POR FUNGOS DA CAATINGA

OpenAIRE

Clementino, Leandro Costa; Barbosa, Camila Castro; Silva, Dayse Pereira Dias; Silva, Felipe Douglas; Queiroz, Jean César Farias

2015-01-01

O desenvolvimento de novos antibióticos está atrelado ao desafio de combater microrganismos super-resistentes, bem como possuir amplo espectro de ação. Para atingir essa meta, várias fontes de obtenção são pesquisadas nos mais diversos ambientes. Nesse sentido, este trabalho buscou a utilização de fungos filamentosos coletados no Bioma Caatinga na microrregião do Cariri paraibano para a produção de antibióticos, considerando-se a importância de pesquisas nesse sentido, utilizando fungos dessa...

Os velhos capoeiras ensinam pegando na mão

Directory of Open Access Journals (Sweden)

Pedro Rodolpho Jungers Abib

Full Text Available Esse artigo trata de analisar as formas tradicionais de transmissão dos saberes presentes no âmbito da cultura popular. A partir dessa abordagem, trazemos as experiências educacionais existentes no universo da capoeira angola uma importante manifestação da cultura afro-brasileira para uma reflexão sobre o papel dos mestres nesse processo. A memória, a ancestralidade, a ritualidade e a temporalidade são categorias fundamentais para compreendermos as relações de educação presentes nesse universo.

Analysis and prediction of leucine-rich nuclear export signals

DEFF Research Database (Denmark)

La Cour, T.; Kiemer, Lars; Mølgaard, Anne

2004-01-01

We present a thorough analysis of nuclear export signals and a prediction server, which we have made publicly available. The machine learning prediction method is a significant improvement over the generally used consensus patterns. Nuclear export signals (NESs) are extremely important regulators...... this analysis is that the most important properties of NESs are accessibility and flexibility allowing relevant proteins to interact with the signal. Furthermore, we show that not only the known hydrophobic residues are important in defining a nuclear export signals. We employ both neural networks and hidden...

EVOLUTION OF THE MOST LUMINOUS DUSTY GALAXIES

International Nuclear Information System (INIS)

Weedman, Daniel W.; Houck, James R.

2009-01-01

A summary of mid-infrared continuum luminosities arising from dust is given for very luminous galaxies, L IR > 10 12 L sun , with 0.005 0.7 in the 9.7 μm silicate absorption feature (i.e., half of the continuum is absorbed) and having equivalent width of the 6.2 μm polycyclic aromatic hydrocarbon feature ν (8 μm) for the most luminous obscured AGNs is found to scale as (1+z) 2.6 to z = 2.8. For unobscured AGNs, the scaling with redshift is similar, but luminosities νL ν (8 μm) are approximately three times greater for the most luminous sources. Using both obscured and unobscured AGNs having total infrared fluxes from the Infrared Astronomical Satellite, empirical relations are found between νL ν (8 μm) and L IR . Combining these relations with the redshift scaling of luminosity, we conclude that the total infrared luminosities for the most luminous obscured AGNs, L IR (AGN obscured ) in L sun , scale as log L IR (AGN obscured ) = 12.3 ± 0.25 + 2.6(±0.3)log(1+z), and for the most luminous unobscured AGNs, scale as log L IR (AGN1) = 12.6(±0.15) + 2.6(±0.3)log(1+z). We previously determined that the most luminous starbursts scale as log L IR (SB) = 11.8 ± 0.3 + 2.5(±0.3)log(1+z), indicating that the most luminous AGNs are about 10 times more luminous than the most luminous starbursts. Results are consistent with obscured and unobscured AGNs having the same total luminosities with differences arising only from orientation, such that the obscured AGNs are observed through very dusty clouds which extinct about 50% of the intrinsic luminosity at 8 μm. Extrapolations of observable f ν (24 μm) to z = 6 are made using evolution results for these luminous sources. Both obscured and unobscured AGNs should be detected to z ∼ 6 by Spitzer surveys with f ν (24 μm) > 0.3 mJy, even without luminosity evolution for z > 2.5. By contrast, the most luminous starbursts cannot be detected for z > 3, even if luminosity evolution continues beyond z = 2.5.

Extreme river flow dependence in Northern Scotland

Science.gov (United States)

Villoria, M. Franco; Scott, M.; Hoey, T.; Fischbacher-Smith, D.

2012-04-01

Various methods for the spatial analysis of hydrologic data have been developed recently. Here we present results using the conditional probability approach proposed by Keef et al. [Appl. Stat. (2009): 58,601-18] to investigate spatial interdependence in extreme river flows in Scotland. This approach does not require the specification of a correlation function, being mostly suitable for relatively small geographical areas. The work is motivated by the Flood Risk Management Act (Scotland (2009)) which requires maps of flood risk that take account of spatial dependence in extreme river flow. The method is based on two conditional measures of spatial flood risk: firstly the conditional probability PC(p) that a set of sites Y = (Y 1,...,Y d) within a region C of interest exceed a flow threshold Qp at time t (or any lag of t), given that in the specified conditioning site X > Qp; and, secondly the expected number of sites within C that will exceed a flow Qp on average (given that X > Qp). The conditional probabilities are estimated using the conditional distribution of Y |X = x (for large x), which can be modeled using a semi-parametric approach (Heffernan and Tawn [Roy. Statist. Soc. Ser. B (2004): 66,497-546]). Once the model is fitted, pseudo-samples can be generated to estimate functionals of the joint tails of the distribution of (Y,X). Conditional return level plots were directly compared to traditional return level plots thus improving our understanding of the dependence structure of extreme river flow events. Confidence intervals were calculated using block bootstrapping methods (100 replicates). We report results from applying this approach to a set of four rivers (Dulnain, Lossie, Ewe and Ness) in Northern Scotland. These sites were chosen based on data quality, spatial location and catchment characteristics. The river Ness, being the largest (catchment size 1839.1km2) was chosen as the conditioning river. Both the Ewe (441.1km2) and Ness catchments have

When Transparency Obscures: The Political Spectacle of Accountability

Science.gov (United States)

Koyama, Jill; Kania, Brian

2014-01-01

In the United States (US), an increase in standardization, quantification, competition, and large-scale comparison--cornerstones of neoliberal accountability--have been accompanied by devices of transparency, through which various forms of school data are made available to the public. Such public reporting, we are told by politicians and education…

Mining the Obscured OB Star Population in Carina

Science.gov (United States)

Smith, Michael

2016-04-01

Massive OB stars are very influential objects in the ecology of galaxies like our own. Current catalogues of Galactic OB stars are heavily biased towards bright (g selected OB stars across the entire Southern Galactic plane, both within clusters and in the field, down to ∼20th magnitude in g. For the first time, a complete accounting of the OB star runaway phenomenon becomes possible. Along with making the primary selection using VPHAS+ colours, I have performed Markov-Chain Monte Carlo fitting of the spectral energy distributions of the selected stars by combining VPHAS+ u, g, r, i with published J, H, K photometry. This gives rough constraints on effective temperature and distance, whilst delivering much more precise reddening parameters A0 and RV - allowing us to build a much richer picture of how extinction and extinction laws vary across the Galactic Plane. My thesis begins with a description of the method of photometric selection of OB star candidates and its validation across a 2 square degree field including the well-known young massive star cluster Westerlund 2 (Mohr-Smith et al., 2015). Following on from this I present spectroscopy with AAOmega of 283 candidates identified by our method, which confirms that ∼94% of the sample are the expected O and early B stars. I then develop this method further and apply it to a Galactic Plane strip of 42 square-degrees that runs from the Carina Arm tangent region to the much studied massive cluster in NGC 3603. A new aspect I attend to in this expansion of method is tightening up the uniform photometric calibration of the data, paying particular attention to the always-challenging u band. This leads to a new and reliable catalogue of 5915 OB stars. As well as increasing the numbers of identified massive stars in this large region of the sky by nearly an order of magnitude, a more complete picture of massive star formation in the Carina Arm has emerged. I have found a broad over-density of O stars around the highly luminous cluster NGC 3603 and have uncovered two new candidate OB clusters/associations. I have also paired up the ionization sources of a number of HII regions catalogued by the RMS survey. It is also shown that the OB star scale-height can serve as a roughly standard ruler, leading to the result that the OB star layer shows the onset of warping at RG ∼10kpc. My results confirm that this entire region requires a non-standard (3.5 < RV < 4.0) reddening law for distances greater than ∼2 kpc. The methods developed in this study are ready to roll out across the rest of the VPHAS+ footprint that has been observed to date. This extension will take in a strip ∼ ±2 degrees across the entire Southern Galactic mid-plane (a sky area of over 700 square degrees), within which we expect to find the majority of massive OB stars. This will result in the largest catalogue of Galactic OB stars to date.

Imaging the Obscuring Torus in Nearby Active Galaxies

Science.gov (United States)

Wilson, Andrew S.; Storchi Bergmann, Thaisa; Morris, Simon

2000-02-01

We propose to study a sample of Seyfert galaxies with the aim of resolving spatially the torus of dense molecular gas and dust which is believed to surround the nuclei of these objects. The galaxies, selected to have strong molecular hydrogen emission and jet-like radio continuum sources, will be imaged in various molecular hydrogen lines and in [Fe II] or Br (gamma). The goals are to a) confirm the existence of such tori, b) determine whether the extended molecular gas is excited thermally or through fluorescence, and c) compare with the distribution of ionized gas, which may show an ionization cone structure from polar escape of ionizing photons. The availability of IR imaging capabilities with tip-tilt and narrow-band filters, which allow imaging in the H_2(lambda) 2.122(micron) line up to a recession velocity of 6,000 km s^-1, makes the Blanco 4m telescope very well suited to this project.

KWIK Smoke Obscuration Model: User’s Guide.

Science.gov (United States)

1982-09-01

t ’ustr ( td I IK,j) 384: prt 3o :: pr t 6 k AC 1-4G" 36~b : pr t " ~ L 3b7: if j~i;prt &t(t1,] 3 8 8: it J=2;pr. "&str(Zjl,1,KI) 3 0 9: j~r t "I 39u...t.2~t71. * j3 3 2u: w r t 7uX ,"i(Lz~j i21iJ "c3wt70, )i: lnt 4 5X, "irI I U uIL - = 01 17.2;wrt 701,kq3 j~b: Lirt. 45x,"a..~c4 uAT - LiLY = g,t4.2

How mainstream economics serves the rich, obscures reality

African Journals Online (AJOL)

12Economics of the 1%: How mainstream economics serves the rich, ... revealing analysis of economic inequality contrasts with the silence of mainstream ... been the coordinating editor of the Journal of Australian Political Economy for the last ...

Obscured and unobscured growth of supermassive black holes

OpenAIRE

X. Barcons; J. Bussons; F. J. Carrera; M. T. Ceballos; A. Corral; J. Ebrero; S. Mateos; M. J. Page; F. Panessa; M. G. Watson

2007-01-01

La acreción es el mecanismo dominante en el crecimiento de los agujeros negros presentes en los centros galácticos. Los rastreos del cielo a longitudes de onda de rayos X trazan la historia de esta acreción en el Universo y muestran que la mayor parte de ella ocurre en objetos oscurecidos. En este artículo presentamos algunos resultados obtenidos con el XMM-Newton Medium Sensitivity survey (XMS), que investiga la población de fuentes que produce aproximadamente la mitad más brilla...

Pinus ponderosa: A checkered past obscured four species.

Science.gov (United States)

Willyard, Ann; Gernandt, David S; Potter, Kevin; Hipkins, Valerie; Marquardt, Paula; Mahalovich, Mary Frances; Langer, Stephen K; Telewski, Frank W; Cooper, Blake; Douglas, Connor; Finch, Kristen; Karemera, Hassani H; Lefler, Julia; Lea, Payton; Wofford, Austin

2017-01-01

Molecular genetic evidence can help delineate taxa in species complexes that lack diagnostic morphological characters. Pinus ponderosa (Pinaceae; subsection Ponderosae) is recognized as a problematic taxon: plastid phylogenies of exemplars were paraphyletic, and mitochondrial phylogeography suggested at least four subdivisions of P. ponderosa. These patterns have not been examined in the context of other Ponderosae species. We hypothesized that putative intraspecific subdivisions might each represent a separate taxon. We genotyped six highly variable plastid simple sequence repeats in 1903 individuals from 88 populations of P. ponderosa and related Ponderosae (P. arizonica, P. engelmannii, and P. jeffreyi). We used multilocus haplotype networks and discriminant analysis of principal components to test clustering of individuals into genetically and geographically meaningful taxonomic units. There are at least four distinct plastid clusters within P. ponderosa that roughly correspond to the geographic distribution of mitochondrial haplotypes. Some geographic regions have intermixed plastid lineages, and some mitochondrial and plastid boundaries do not coincide. Based on relative distances to other species of Ponderosae, these clusters diagnose four distinct taxa. Newly revealed geographic boundaries of four distinct taxa (P. benthamiana, P. brachyptera, P. scopulorum, and a narrowed concept of P. ponderosa) do not correspond completely with taxonomies. Further research is needed to understand their morphological and nuclear genetic makeup, but we suggest that resurrecting originally published species names would more appropriately reflect the taxonomy of this checkered classification than their current treatment as varieties of P. ponderosa. © 2017 Willyard et al. Published by the Botanical Society of America. This work is licensed under a Creative Commons public domain license (CC0 1.0).

A Monster CME Obscuring a Demon Star Flare

Science.gov (United States)

Moschou, Sofia-Paraskevi; Drake, Jeremy J.; Cohen, Ofer; Alvarado-Gomez, Julian D.; Garraffo, Cecilia

2017-12-01

We explore the scenario of a coronal mass ejection (CME) being the cause of the observed continuous X-ray absorption of the 1997 August 30 superflare on the eclipsing binary Algol (the Demon Star). The temporal decay of the absorption is consistent with absorption by a CME undergoing self-similar evolution with uniform expansion velocity. We investigate the kinematic and energetic properties of the CME using the ice cream cone model for its three-dimensional structure in combination with the observed profile of the hydrogen column density decline with time. Different physically justified length scales were used that allowed us to estimate lower and upper limits of the possible CME characteristics. Further consideration of the maximum available magnetic energy in starspots leads us to quantify its mass as likely lying in the range 2× {10}21 {--} 2× {10}22 g and kinetic energy in the range 7× {10}35 {--} 3× {10}38 erg. The results are in reasonable agreement with extrapolated relations between flare X-ray fluence and CME mass and kinetic energy derived for solar CMEs.

27 CFR 30.32 - Determination of proof obscuration.

Science.gov (United States)

2010-04-01

... added to the temperature corrected hydrometer reading will give the true proof. (c) Distillation method... use of a precision hydrometer and thermometer in accordance with the provisions of § 13.23 to the...

Obscure pulmonary masses: bronchial impaction revealed by CT

International Nuclear Information System (INIS)

Pugatch, R.D.; Gale, M.E.

1983-01-01

Dilated bronchi impacted with mucus or tumor are recognized on standard chest radiographs because they are surrounded by aerated pulmonary parenchyma. When imaged in different projections, these lesions produce a variety of appearances that are generally familiar. This report characterizes less familiar computed tomographic (CT) findings in eight patients with pathologic bronchial distension of congenital, neoplastic, or infectious etiologies and correlates them with chest films. In seven patients, CT readily revealed dilated bronchi and/or regional lung hypodensity. In four of these cases, CT led to the initial suspicion of dilated bronchi. CT should be used early in the evaluation of atypical pulmonary mass lesions or to confirm suspected bronchial impaction because of the high probability it will reveal diagnostic features

Dynamics and Formation of Obscuring Tori in AGNs

Energy Technology Data Exchange (ETDEWEB)

Bannikova, Elena Yu.; Sergeyev, Alexey V., E-mail: bannikova@astron.kharkov.ua [Institute of Radio Astronomy, National Academy of Science of Ukraine, Kharkiv (Ukraine); Institute of Astronomy, V. N. Karazin Kharkiv National University, Kharkiv (Ukraine)

2017-12-12

We considered the evolution of a self-gravitating clumpy torus in the gravitational field of the central mass of an active galactic nucleus (AGN) in the framework of the N-body problem. The initial conditions take into account winds with different opening angles. Results of our N-body simulations show that the clouds moving on orbits with a spread in inclinations and eccentricities form a toroidal region. The velocity of the clouds at the inner boundary of the torus is lower than in a disk model that can explain the observed rotation curves. We discuss the scenario of torus formation related with the beginning of the AGN stage.

Pinus ponderosa : A checkered past obscured four species

Science.gov (United States)

Ann Willyard; David S. Gernandt; Kevin Potter; Valerie Hipkins; Paula E. Marquardt; Mary Frances Mahalovich; Stephen K. Langer; Frank W. Telewski; Blake Cooper; Connor Douglas; Kristen Finch; Hassani H. Karemera; Julia Lefler; Payton Lea; Austin Wofford

2016-01-01

PREMISE OF THE STUDY: Molecular genetic evidence can help delineate taxa in species complexes that lack diagnostic morphological characters. Pinus ponderosa (Pinaceae; subsection Ponderosae ) is recognized as a problematic taxon: plastid phylogenies of exemplars were paraphyletic, and mitochondrial phylogeography suggested at...

How mainstream economics serves the rich, obscures reality

African Journals Online (AJOL)

Mainstream economics is in a sorry state. Books and articles criticising it have proliferated in recent years. Students are grumbling about its evident incapacity to illuminate the troubled world in which they live: they have recently formed an international organisation to coordinate and publicise their drive for reform. Leading.

Multiple Erythema Lesions Obscured As Fungal Skin Infection

OpenAIRE

Koçinaj, Allma; Gërçari, Antigona; Ferizi, Mybera; Lashi, Edlira; Gjunkshi, Lorela; Fida, Monika

2014-01-01

Erythema migrans is a ring like erythema, with a few centimeters in diameter. Usually it occur solitary, days to weeks after an infected tick bite. According to skin changes it can be manifested acutely such as erythema migrans in Lyme Borreliosis, borrelial lymphocytoma (subacute), or as a late Lyme disease with acrodermatitis chronica atrophicans. All stages of this disease can be treatable with antimicrobial agents. As a first case in our department with multiple lesions, we describe a 14-...

Multiple Erythema Lesions Obscured As Fungal Skin Infection

Directory of Open Access Journals (Sweden)

Allma Koçinaj

2014-09-01

Full Text Available Erythema migrans is a ring like erythema, with a few centimeters in diameter. Usually it occur solitary, days to weeks after an infected tick bite. According to skin changes it can be manifested acutely such as erythema migrans in Lyme Borreliosis, borrelial lymphocytoma (subacute, or as a late Lyme disease with acrodermatitis chronica atrophicans. All stages of this disease can be treatable with antimicrobial agents. As a first case in our department with multiple lesions, we describe a 14-year-old female and review the patient’s clinical and laboratory features, the causes of the disease, diagnosis as well as treatment.

The close environments of accreting massive black holes are shaped by radiative feedback.

Science.gov (United States)

Ricci, Claudio; Trakhtenbrot, Benny; Koss, Michael J; Ueda, Yoshihiro; Schawinski, Kevin; Oh, Kyuseok; Lamperti, Isabella; Mushotzky, Richard; Treister, Ezequiel; Ho, Luis C; Weigel, Anna; Bauer, Franz E; Paltani, Stephane; Fabian, Andrew C; Xie, Yanxia; Gehrels, Neil

2017-09-27

The majority of the accreting supermassive black holes in the Universe are obscured by large columns of gas and dust. The location and evolution of this obscuring material have been the subject of intense research in the past decades, and are still debated. A decrease in the covering factor of the circumnuclear material with increasing accretion rates has been found by studies across the electromagnetic spectrum. The origin of this trend may be driven by the increase in the inner radius of the obscuring material with incident luminosity, which arises from the sublimation of dust; by the gravitational potential of the black hole; by radiative feedback; or by the interplay between outflows and inflows. However, the lack of a large, unbiased and complete sample of accreting black holes, with reliable information on gas column density, luminosity and mass, has left the main physical mechanism that regulates obscuration unclear. Here we report a systematic multi-wavelength survey of hard-X-ray-selected black holes that reveals that radiative feedback on dusty gas is the main physical mechanism that regulates the distribution of the circumnuclear material. Our results imply that the bulk of the obscuring dust and gas is located within a few to tens of parsecs of the accreting supermassive black hole (within the sphere of influence of the black hole), and that it can be swept away even at low radiative output rates. The main physical driver of the differences between obscured and unobscured accreting black holes is therefore their mass-normalized accretion rate.

Wet-Bulb-Globe Temperature Data Report

Science.gov (United States)

2015-03-01

Hour Min Pressure Dry Nat Wet Globe Dry Nat Wet Globe Dry Nat Wet Globe Wind Cld amt Cld type Obscuration Quest RH Kestrel RH VPSc RH S1 WBGT Q WBGT...Wet Globe Dry Nat Wet Globe Dry Nat Wet Globe Wind Cld amt Cld type Obscuration Quest RH Kestrel RH VPSc RH S1 WBGT Q WBGT K2 WBGT GMT millibars deg F...Dry Nat Wet Globe Dry Nat Wet Globe Wind Cld amt Cld type Obscuration Quest RH Kestrel RH VPSc RH S1 WBGT Q WBGT K2 WBGT GMT millibars deg F deg F deg

Influence of cultivar and of conventional and organic agricultural practices on phenolic and sensory profile of blackberries (Rubus fruticosus).

Science.gov (United States)

Pinto, Teresa; Vilela, Alice; Pinto, Andreia; Nunes, Fernando M; Cosme, Fernanda; Anjos, Rosário

2018-03-06

Consumer demand for organic products is increasing because of their claimed health benefits. Blackberries are a rich source of polyphenols, with high antioxidant activity; nevertheless, the impact of organic versus conventional agricultural practices on its phytochemical composition is unknown. 'Loch Ness' and 'Chester Thornless' were selected as blackberry cultivars for this study because of their desired sensory and technological properties, which make them more suitable for export. 'Loch Ness' variety presented a higher amounts of polyphenols and higher antioxidant activity when compared to the 'Chester Thornless' variety. The impact of agricultural practices on the phytochemical composition of the two varieties was contradictory. Under organic agricultural practices, levels of polyphenols increased for 'Loch Ness' and decreased for 'Chester Thornless', whereas the soluble solids content increased in both varieties. These changes in composition were correlated with changes observed in the blackberries' sensory profile. The effect of agricultural practices on the blackberries' chemical and sensory profile was dependent on the variety and cannot be generalized. © 2018 Society of Chemical Industry. © 2018 Society of Chemical Industry.

Dismantling reified African culture through localised homosexualities in Uganda.

Science.gov (United States)

Nyanzi, Stella

2013-01-01

Uganda's Anti-Homosexuality Bill of 2009 aimed at protecting the cherished culture of the people against emergent threats to the traditional heterosexual family. The Bill's justification, however, lay in myopic imaginings of a homogenous African-ness and pedestrian oblivion to pluralities within African sexualities. This paper revisits the debate that homosexuality is 'un-African'. Rhetoric analysis of the Anti-Homosexuality Bill exposes how dominant discourses of law, medicine, religion, geography and culture reinforce the view that homosexuality is foreign to Africa. Based on ethnography in contemporary Uganda, I explore how self-identified same-sex-loving individuals simultaneously claim their African-ness and their homosexuality. Their strategies include ethnic belonging, membership to kinship structures, making connections with pre-colonial histories of homosexuality, civic participation in democratic processes, national identity, organising of lesbian, gay, bisexual, transgender, intersex and questioning support groups, language and nomenclature, visibility and voice in local communal activities, solidarity and adherence to cultural rituals. In present-day Uganda, same-sex-loving men, women and transgender people variously assert their African-ness.

We can work it out: age differences in relational pronouns, physiology, and behavior in marital conflict.

Science.gov (United States)

Seider, Benjamin H; Hirschberger, Gilad; Nelson, Kristin L; Levenson, Robert W

2009-09-01

This study examined the relationship that personal pronouns spoken during a marital conversation have with the emotional qualities of those interactions and with marital satisfaction. Middle-aged and older couples (N = 154) engaged in a 15-min conflict conversation during which physiology and emotional behavior were continuously monitored. Verbatim transcripts of the conversations were coded into 2 lexical categories: (a) we-ness (we-words), pronouns that focus on the couple; (b) separateness (me/you-words), pronouns that focus on the individual spouses. Analyses revealed that greater we-ness was associated with a number of desirable qualities of the interaction (lower cardiovascular arousal, more positive and less negative emotional behavior), whereas greater separateness was associated with a less desirable profile (more negative emotional behavior, lower marital satisfaction). In terms of age differences, older couples used more we-ness words than did middle-aged couples. Further, the associations between separateness and marital satisfaction were strongest for older wives. These findings indicate that the emotional aspects of marital quality are expressed in the natural language of couples engaged in conversation. (c) 2009 APA, all rights reserved.

Associations between Relational Pronoun Usage and the Quality of Early Family Interactions.

Science.gov (United States)

Galdiolo, Sarah; Roskam, Isabelle; Verhofstadt, Lesley L; De Mol, Jan; Dewinne, Laura; Vandaudenard, Sylvain

2016-01-01

Our study examined the relationships of relational pronouns used in parental conversation to the quality of early family interactions, as indexed by Family Alliance (FA). We hypothesized that more positive family interactions were associated with the use of more we-pronouns (e.g., we, us, our; we-ness ) and fewer I- and you-pronouns (e.g., I, me, you, your; separateness ) by both mothers and fathers. Our statistical model using a multilevel modeling framework and two levels of analysis (i.e., a couple level and an individual level) was tested on 47 non-referred families ( n = 31 primiparous families; child's age, M = 15.75 months, SD = 2.73) with we-ness and separateness as outcomes and FA functions as between-dyads variables. Analyses revealed that we-ness within the parental couple was only positively associated with family affect sharing while separateness was negatively associated with different FA functions (e.g., communication mistakes). Our main finding suggested that the kinds of personal pronouns used by parental couples when discussing children's education would be associated to the emotional quality of the family interactions.

Humanidades e ciência: uma leitura a partir da Bioética de Van Rensselaer (V. R. Potter

Directory of Open Access Journals (Sweden)

Diego Carlos Zanella

Full Text Available A Bioética surgiu em um momento em que a distância entre a ciência e as humanidades parecia intransponível. Em seu surgimento, a Bioética possuía um apelo para superar essa distância que se revelava fatal para o futuro desenvolvimento da humanidade e para a manutenção das condições de vida nesse planeta. É nesse contexto que V. R. Potter propôs seu conceito original de Bioética como uma integração entre a Biologia e os valores humanos - especialmente a filosofia moral - para orientar a sobrevivência humana. Nesse sentido, o presente texto procurará desenvolver o significado do conceito de Bioética para V. R. Potter e o problema das “duas culturas”, isto é, da necessidade de construção de um diálogo entre as humanidades e a ciência, buscando uma convergência da relação ética de todos os saberes em torno do cuidado da vida.

Understanding Constructions of Danish-ness using Heterogeneous Types of Sources across Historical Settings

DEFF Research Database (Denmark)

Øland, Trine; Ydesen, Christian

-state construct ‘disturbing/disquieting behavior’, delinquency, and misbehavior and how these constructions are made into a category that activates educational and other interventions. Using a comparative outlook between the two historical settings the purpose is to understand 1) the boundaries of legitimate...

Four-wavelength lidar evaluation of particle characteristics and aerosol densities

Science.gov (United States)

Uthe, E. E.; Livingston, J. M.; Delateur, S. A.; Nielsen, N. B.

1985-06-01

The SRI International four-wavelength (0.53, 1.06, 3.8, 10.6 micron) lidar systems was used during the SNOW-ONE-B and Smoke Week XI/SNOW-TWO field experiments to validate its capabilities in assessing obscurant optical and physical properties. The lidar viewed along a horizontal path terminated by a passive reflector. Data examples were analyzed in terms of time-dependent transmission, wavelength dependence of optical depth, and range-resolved extinction coefficients. Three methods were used to derive extinction data from the lidar signatures. These were target method, Klett method and experimental data method. The results of the field and analysis programs are reported in the journal and conference papers that are appended to this report, and include: comparison study of lidar extinction methods, submitted to applied optics, error analysis of lidar solution techniques for range-resolved extinction coefficients based on observational data, smoke/obscurants symposium 9, Four--Wavelength Lidar Measurements from smoke week 6/SNOW-TWO, smoke/obscurants symposium 8, SNOW-ONE-B multiple-wavelength lidar measurements. Snow symposium 3, and lidar applications for obscurant evaluations, smoke/obscurants Symposium 7. The report also provides a summary of background work leading to this project, and of project results.

Human walking estimation with radar

NARCIS (Netherlands)

Dorp, Ph. van; Groen, F.C.A.

2003-01-01

Radar can be used to observe humans that are obscured by objects such as walls. These humans cannot be visually observed. The radar measurements are used to animate an obscured human in virtual reality. This requires detailed information about the motion. The radar measurements give detailed

Laser-beam apodization with a graded random phase window

Energy Technology Data Exchange (ETDEWEB)

Haas, R.A.; Summers, M.A.; Linford, G.J.

1986-10-01

Experiments and analysis indicate that graded random phase modulation can be usesd to apodize a laser beam. In the case of an obscuration or a hard edge it can prevent the formation of Fresnel-diffraction ripples. For example, here the interaction of a 1-..mu..m-wavelength laser beam with a central obscuration of half-width a -- 100 ..mu..m is studied theoretically. It is found that if the exit surface of a window, placed immediately downstream of the obstacle, is randomly modulated with a Gaussian amplitude transverse correlation length l -- 50..mu..m and a mean-square amplitude that decreases exponentially from a peak height of --1..mu..m/sup 2/ away from the center of the obscuration with transverse scale length L -- 500 ..mu..m, then the Fresenel-diffraction ripples normally produced by the obscuration are elimated. The scaling of these results is also discussed. The calculations are in general agreement with experimental results.

Laser-beam apodization with a graded random phase window

International Nuclear Information System (INIS)

Haas, R.A.; Summers, M.A.; Linford, G.J.

1986-01-01

Experiments and analysis indicate that graded random phase modulation can be usesd to apodize a laser beam. In the case of an obscuration or a hard edge it can prevent the formation of Fresnel-diffraction ripples. For example, here the interaction of a 1-μm-wavelength laser beam with a central obscuration of half-width a -- 100 μm is studied theoretically. It is found that if the exit surface of a window, placed immediately downstream of the obstacle, is randomly modulated with a Gaussian amplitude transverse correlation length l -- 50μm and a mean-square amplitude that decreases exponentially from a peak height of --1μm 2 away from the center of the obscuration with transverse scale length L -- 500 μm, then the Fresenel-diffraction ripples normally produced by the obscuration are elimated. The scaling of these results is also discussed. The calculations are in general agreement with experimental results

Alterações do ciclo sono-vigília moduladas por Dopamina e suas consequências Mnemônicas

OpenAIRE

Franca, Arthur Sergio Cavalcanti de

2012-01-01

As descobertas da neurociência estão em franca ascensão. A sua grande interdisciplinaridade facilita uma abordagem mais complexa do cérebro, abrangendo com profundidade diversas áreas. No entanto, muitos fenômenos que fascinam a humanidade estão longe de ser completamente elucidados; nesse contexto se encontra a relação entre a consolidação das memórias e o sono. Nesse trabalho investigamos o papel de parte do sistema dopaminérgico no processo de consolidação de memórias e n...

Development of the Nordic Bioeconomy: NCM reporting: Test centers for green energy solutions - Biorefineries and business needs

DEFF Research Database (Denmark)

Lange, Lene; Björnsdóttir, Bryndís; Brandt, Asbjørn

In 2014 the Nordic Council of Ministers initiated a new bioeconomy project: “Test centers for green energy solutions – Biorefineries and Busi-ness needs”. The purpose was to strengthen green growth in the area of the bioeconomy by analyzing and mapping the current status of the bio-economy in the......In 2014 the Nordic Council of Ministers initiated a new bioeconomy project: “Test centers for green energy solutions – Biorefineries and Busi-ness needs”. The purpose was to strengthen green growth in the area of the bioeconomy by analyzing and mapping the current status of the bio...

A inserção do design e da gestão de design : estudo de caso em uma indústria calçadista gaúcha

OpenAIRE

Galina, Andréa Capra; Bernardes, Mauricio Moreira e Silva

2012-01-01

O calçado gaúcho está perdendo mercado exportador considerando-se o número de pares exportados, porém esse segmento pertence ao estado brasileiro com maior faturamento gerado da exportação. Nesse contexto, o design assume um importante papel na gestão, promovendo a integração entre todos os setores, agindo em nível estratégico. Diante disso, este artigo, ao propor um estudo de caso baseado no modelo praticado por uma empresa calçadista do Rio Grande do Sul, busca entender como ocorre nesse es...

El farol bar problem e jogo minoritário: uma introdução à econofísica

OpenAIRE

Bertulino, Diogo de Toledo

2014-01-01

Propõe-se nesse trabalho um estudo do El Farol Bar Problem e do Jogo Minoritário, a partir dos conceitos de racionalidade limitada e raciocínio indutivo na tomada de decisões em situações cotidianas, quando o número de agentes é grande. Nesses casos, verifica-se a impraticabilidade da Teoria dos Jogos. As novas linhas de pensamento, principalmente as propostas pelo Jogo Minoritário, revelam grande importância para o estudo da Econofísica porque servem de instrumento para a análise de situaçõe...

Deslocamento de empresas para os estados do Ceará e da Bahia: o caso da indústria calçadista

OpenAIRE

Santos, Angela Maria Medeiros Martins; Correa, Abidack Raposo; Alexim, Flavia Menna Barreto; Peixoto, Gabriel Barros Tavares

2002-01-01

Este artigo objetiva apresentar o deslocamento do setor calçadista brasileiro das regiões Sul e Sudeste para o Nordeste, especialmente para os Estados do Ceará e da Bahia. Nesse sentido, procura-se mostrar as políticas de atração de novos investimentos do setor nesses estados, assim como suas perspectivas e seus principais problemas. Serão apresentadas as características gerais do setor no Ceará e na Bahia, os fatores que determinaram a migração de empresas calçadistas, a logística de suprime...

Whitening filter and innovational representation of fractional Brownian motion

International Nuclear Information System (INIS)

Wang Xiaotian; Wu Min

2009-01-01

In this paper, by means of fractional differential-integral technique we give a new whitening filter formula for fractional Brownian motion defined by Mandelbrot and van Ness [Mandelbrot BB, van Ness JW. SIAM Rev 1968;10(4):422]. This new formula has potential use in time series analysis and in detecting signals as Barton and Vincent Poor [Barton RJ, Vincent Poor H. IEEE Trans Inform Theory 1988;34(5):943] have shown. Another potential application of it is behavioral finance, where the arbitrage opportunities that come from the reversal effect of stock returns, can be eliminated by such a formula.

Baryon-charge chemical potential in AdS/CFT

International Nuclear Information System (INIS)

Nakamura, Shin; Seo, Yunseok; Sin, Sang-Jin; Yogendran, K.P.

2008-01-01

We investigate the D3-D7 model at finite U(1) B -charge chemical potential. We point out that the D3-D7 model with only the black-hole embeddings does not have the low-temperature and low-chemical-potential region in the grand-canonical ensemble, hence it is incomplete. The incomplete-ness is also seen as the thermodynamic instability in the canonical ensemble. We propose to solve the incomplete-ness problem by introducing the Minkowski embeddings at the finite U(1) B -charge. A possible physical interpretation of our model is given. (author)

O Papel da Gestão da Farmácia Hospitalar na Alta Qualificada de Acordo com as Políticas de Humanização do SUS

OpenAIRE

Giacomini, Karina Paula; Liberal, Márcia Mello Costa de

2015-01-01

Embora a Política de Humanização do SUS não tenha contornos claramente definidos, sabe-se que o tratamento não ocorre apenas quando o paciente se encontra internado, nem termina quando este deixa a internação, mas se estende após a alta hospitalar. Nesse caso, deve ter seu tratamento continuado no ambiente extra-hospitalar, em ambiente domiciliar, sob a supervisão e acompanhamento de um responsável pela medicação, nesse caso, o próprio farmacêutico hospitalar, que lhe deve fornecer orientação...

Aplicação do QFD e do PCP a produtos digitais em uma empresa brasileira de telecomunicações móveis

OpenAIRE

Márcio Barbosa Guimarães Cota Júnior; Lin Chih Cheng

2009-01-01

O desenvolvimento tecnológico na área de informática e telecomunicações fez surgir novos conceitos de economia e produto, além de novos modelos de organização das empresas envolvidas nesse mercado. Este trabalho tem o objetivo de avaliar a aplicabilidade de métodos de Gestão de Desenvolvimento de Produtos (GDP) e Gestão da Produção (GP) a produtos digitais, e verificar algumas particularidades da aplicação nesse campo. São estudados, em especial, o Desdobramento da Função Qualidade (QFD) e o ...

UV, X-ray, and Optical Variability of the Young Star T Cha Produced by Inner Disk Obscuration: Results from a Coordinated HST, XMM-Newton, LCOGT, and SMARTS Observing Campaign

Science.gov (United States)

Brown, Alexander; France, Kevin; Walter, Frederick M.; Schneider, P. Christian; Brown, Timothy M.; Andrews, Sean M.; Wilner, David J.

2018-06-01

The young (7 Myr) 1.5 solar mass T Tauri star T Chamaeleontis shows dramatic variability. The optical extinction varies by at least 3 magnitudes on few hour time-scales with no obvious periodicity. The obscuration is produced by material at the inner edge of the circumstellar disk and therefore characterizing the absorbing material can reveal important clues regarding the transport of gas and dust within such disks. The inner disk of T Cha is particularly interesting, because T Cha has a transitional disk with a large gap at 0.2-15 AU in the dust disk and allows study of the gas and dust structure in the terrestrial planet formation zone during this important rapid phase of protoplanetary disk evolution. For this reason we have conducted a major multi-spectral-region observing campaign to study the UV/X-ray/optical variability of T Cha. During 2018 February/March we monitored the optical photometric and spectral variability using LCOGT (Chile/South Africa/Australia) and the SMARTS telescopes in Chile. These optical data provide a broad context within which to interpret our shorter UV and X-ray observations. We observed T Cha during 3 coordinated observations (each 5 HST orbits + 25 ksec XMM; on 2018 Feb 22, Feb 26, Mar 2) using the HST COS/STIS spectrographs to measure the FUV/NUV spectra and XMM-Newton to measure the corresponding X-ray energy distribution. The observed spectral changes are well correlated and demonstrate the influence of the same absorbing material in all the spectral regions observed. By examining which spectral features change and by how much we can determine the location of different emitting regions relative to the absorbers along the line-of-sight to the star. In this poster we provide an overview of the variability seen in the different spectral regions and quantify the dust and gas content of T Cha's inner disk edge.(This work is supported by grant HST-GO-15128 and time awarded by HST, XMM-Newton, LCOGT, and SMARTS. We acknowledge the

Quantum state engineering in hybrid open quantum systems

Science.gov (United States)

Joshi, Chaitanya; Larson, Jonas; Spiller, Timothy P.

2016-04-01

We investigate a possibility to generate nonclassical states in light-matter coupled noisy quantum systems, namely, the anisotropic Rabi and Dicke models. In these hybrid quantum systems, a competing influence of coherent internal dynamics and environment-induced dissipation drives the system into nonequilibrium steady states (NESSs). Explicitly, for the anisotropic Rabi model, the steady state is given by an incoherent mixture of two states of opposite parities, but as each parity state displays light-matter entanglement, we also find that the full state is entangled. Furthermore, as a natural extension of the anisotropic Rabi model to an infinite spin subsystem, we next explored the NESS of the anisotropic Dicke model. The NESS of this linearized Dicke model is also an inseparable state of light and matter. With an aim to enrich the dynamics beyond the sustainable entanglement found for the NESS of these hybrid quantum systems, we also propose to combine an all-optical feedback strategy for quantum state protection and for establishing quantum control in these systems. Our present work further elucidates the relevance of such hybrid open quantum systems for potential applications in quantum architectures.

Associations between relational pronoun usage and the quality of early family interactions

Directory of Open Access Journals (Sweden)

Sarah Galdiolo

2016-11-01

Full Text Available Our study examined the relationships of relational pronouns used in parental conversation to the quality of early family interactions, as indexed by Family Alliance (FA. We hypothesized that more positive family interactions were associated with the use of more we-pronouns (e.g., we, us, our; we-ness and fewer I- and you-pronouns (e.g., I, me, you, your; separateness by both mothers and fathers. Our statistical model using a multilevel modelling framework and two levels of analysis (i.e., a couple level and an individual level was tested on 47 non-referred families (n = 31 primiparous families; child’s age, M = 15.75 months, SD = 2.73 with we-ness and separateness as outcomes and FA functions as between-dyads variables. Analyses revealed that we-ness within the parental couple was only positively associated with family affect sharing while separateness was negatively associated with different FA functions (e.g., communication mistakes. Our main finding suggested that the kinds of personal pronouns used by parental couples when discussing children’s education would be associated to the emotional quality of the family interactions.

Evaluating the role of CRM1-mediated export for adenovirus gene expression

International Nuclear Information System (INIS)

Carter, Christoph C.; Izadpanah, Reza; Bridge, Eileen

2003-01-01

A complex of the Adenovirus (Ad) early region 1b 55-kDa (E1b-55kDa) and early region 4 ORF6 34-kDa (E4-34kDa) proteins promotes viral late gene expression. E1b-55kDa and E4-34kDa have leucine-rich nuclear export signals (NESs) similar to that of HIV Rev. It was proposed that E1b-55kDa and/or E4-34kDa might promote the export of Ad late mRNA via their Rev-like NESs, and the transport receptor CRM1. We treated infected cells with the cytotoxin leptomycin B to inhibit CRM1-mediated export; treatment initially delays the onset of late gene expression, but this activity completely recovers as the late phase progresses. We find that the E1b-55kDa NES is not required to promote late gene expression. Previous results showed that E4-34kDa-mediated late gene expression does not require an intact NES (J. Virol. 74 (2000), 6684-6688). Our results indicate that these Ad regulatory proteins promote late gene expression without intact NESs or active CRM1

Humanidades e ciência: uma leitura a partir da Bioética de Van Rensselaer (V. R.) Potter

OpenAIRE

Zanella, Diego Carlos

2018-01-01

A Bioética surgiu em um momento em que a distância entre a ciência e as humanidades parecia intransponível. Em seu surgimento, a Bioética possuía um apelo para superar essa distância que se revelava fatal para o futuro desenvolvimento da humanidade e para a manutenção das condições de vida nesse planeta. É nesse contexto que V. R. Potter propôs seu conceito original de Bioética como uma integração entre a Biologia e os valores humanos - especialmente a filosofia moral - para orientar a sobrev...

O efeito país de origem na comercialização da carne bovina brasileira na Europa: um estudo com estudantes e funcionários de universidades europeias, importador europeu e exportadores brasileiros

OpenAIRE

Fernanda de Tavares Canto Guina

2011-01-01

Estudos têm demonstrado que idéias pré-estabelecidas e estereotipadas dos indivíduos com relação a países podem afetar suas atitudes em relação a produtos oriundos dessas nações. Tal fato é conhecido como efeito país de origem. Nesse contexto, vale destacar que apesar de o Brasil ter assumido nesta década a posição de maior exportador de carne bovina do mundo, seu papel de liderança nesse campo é criticado por muitos europeus, que acreditam que a pecuária brasileira é responsável por grande p...

Relações raça e gênero em jogo: a questão reprodutiva de mulheres negras e brancas

OpenAIRE

Raquel Souzas

2004-01-01

Introdução: No âmbito das discussões de gênero e raça, as desigualdades que marcam a condição da mulher, nem sempre, são contempladas, ao contrário, há uma série de discursos que visam a naturalizar diferenças, forjadas historicamente. Nesse sentido, indagar sobre o significado dessas diferenças, no âmbito da saúde reprodutiva, apresenta-se como problema de investigação. Nesse campo, decisões e arranjos reprodutivos dos indivíduos partem ou resultam em processos de negociação, não só condici...

Relationships, Being-ness, and Voice: Exploring Multiple Dimensions of Humanizing Work with Black Girls

Science.gov (United States)

Edwards, Erica; McArthur, Sherell A.; Russell-Owens, LaToya

2016-01-01

This work argues for an approach to research and education practices that considers the historically deficit-based research practices and views on Black girls and develops humanizing research methods that consider the multiple oppressions that act as barriers for this group. Research must acknowledge the precarious position of Black girls in order…

Seeing is believing: are cancer stem cells the Loch Ness monster of tumor biology?

Science.gov (United States)

Lathia, Justin D; Venere, Monica; Rao, Mahendra S; Rich, Jeremy N

2011-06-01

Tumors are complex systems with a diversity of cell phenotypes essential to tumor initiation and maintenance. With the heterogeneity present within the neoplastic compartment as its foundation, the cancer stem cell hypothesis posits that a fraction of tumor cells has the capacity to recapitulate the parental tumor upon transplantation. Over the last decade, the cancer stem cell hypothesis has gained support and shown to be relevant in many highly lethal solid tumors. However, the cancer stem cell hypothesis is not without its controversies and critics question the validity of this hypothesis based upon comparisons to normal somatic stem cells. Cancer stem cells may have direct therapeutic relevance due to resistance to current treatment paradigms, suggesting novel multimodal therapies targeting the cancer stem cells may improve patient outcomes. In this review, we will use the most common primary brain tumor, glioblastoma multiforme, as an example to illustrate why studying cancer stem cells holds great promise for more effective therapies to highly lethal tumors. In addition, we will discuss why the abilities of self-renewal and tumor propagation are the critical defining properties of cancer stem cells. Furthermore, we will examine recent progress in defining appropriate cell surface selection markers and mouse models which explore the potential cell(s) or origin for GBMs. What remains clear is that a population of cells is present in many tumors which are resistant to conventional therapies and must be considered in the design of the next generation of cancer treatments.

Family characteristics oF NigeriaN womeN with severe meNtal illNess

African Journals Online (AJOL)

2011-06-06

Jun 6, 2011 ... East African Medical Journal Vol. 88 No. 6 June ... mental illnesses like schizophrenia impair ability or potential to ... from relatives, in which case institutional caregivers ... overload; physical and emotional burnouts may make.

Major galaxy mergers and the growth of supermassive black holes in quasars.

Science.gov (United States)

Treister, Ezequiel; Natarajan, Priyamvada; Sanders, David B; Urry, C Megan; Schawinski, Kevin; Kartaltepe, Jeyhan

2010-04-30

Despite observed strong correlations between central supermassive black holes (SMBHs) and star formation in galactic nuclei, uncertainties exist in our understanding of their coupling. We present observations of the ratio of heavily obscured to unobscured quasars as a function of cosmic epoch up to z congruent with 3 and show that a simple physical model describing mergers of massive, gas-rich galaxies matches these observations. In the context of this model, every obscured and unobscured quasar represents two distinct phases that result from a massive galaxy merger event. Much of the mass growth of the SMBH occurs during the heavily obscured phase. These observations provide additional evidence for a causal link between gas-rich galaxy mergers, accretion onto the nuclear SMBH, and coeval star formation.

Purchase of electric power: the obscure side of contracts

International Nuclear Information System (INIS)

Richard, Roger

2003-01-01

The progressive opening of the French power market prepares the spreading of eligibility to the overall professional consumers by July 1, 2004. Only the domestic market will have to wait until July 1, 2007 to be able to freely chose a power 'dealer'. However, this market opening leaves some doubts about the formalities to comply with to be able to change of power supplier. This article shows that, today, the rules are far to be fixed: an eligible client has to sign 5 types of different contracts (contract(s) of purchase, convention of connection to the grid, convention of exploitation (when the client is also producer), contract of access to the grid, contract with a balance responsible authority). Thus the commission of electricity regulation (CRE) has to elaborate a unique and simpler contract for the future consumers. (J.S.)

Does Lateral Transmission Obscure Inheritance in Hunter-Gatherer Languages?

Science.gov (United States)

Bowern, Claire; Epps, Patience; Gray, Russell; Hill, Jane; Hunley, Keith; McConvell, Patrick; Zentz, Jason

2011-01-01

In recent years, linguists have begun to increasingly rely on quantitative phylogenetic approaches to examine language evolution. Some linguists have questioned the suitability of phylogenetic approaches on the grounds that linguistic evolution is largely reticulate due to extensive lateral transmission, or borrowing, among languages. The problem may be particularly pronounced in hunter-gatherer languages, where the conventional wisdom among many linguists is that lexical borrowing rates are so high that tree building approaches cannot provide meaningful insights into evolutionary processes. However, this claim has never been systematically evaluated, in large part because suitable data were unavailable. In addition, little is known about the subsistence, demographic, ecological, and social factors that might mediate variation in rates of borrowing among languages. Here, we evaluate these claims with a large sample of hunter-gatherer languages from three regions around the world. In this study, a list of 204 basic vocabulary items was collected for 122 hunter-gatherer and small-scale cultivator languages from three ecologically diverse case study areas: northern Australia, northwest Amazonia, and California and the Great Basin. Words were rigorously coded for etymological (inheritance) status, and loan rates were calculated. Loan rate variability was examined with respect to language area, subsistence mode, and population size, density, and mobility; these results were then compared to the sample of 41 primarily agriculturalist languages in [1]. Though loan levels varied both within and among regions, they were generally low in all regions (mean 5.06%, median 2.49%, and SD 7.56), despite substantial demographic, ecological, and social variation. Amazonian levels were uniformly very low, with no language exhibiting more than 4%. Rates were low but more variable in the other two study regions, in part because of several outlier languages where rates of borrowing were especially high. High mobility, prestige asymmetries, and language shift may contribute to the high rates in these outliers. No support was found for claims that hunter-gatherer languages borrow more than agriculturalist languages. These results debunk the myth of high borrowing in hunter-gatherer languages and suggest that the evolution of these languages is governed by the same type of rules as those operating in large-scale agriculturalist speech communities. The results also show that local factors are likely to be more critical than general processes in determining high (or low) loan rates. PMID:21980394

Collarless metal ceramic restorations to obscure the umbrella effect

Directory of Open Access Journals (Sweden)

Afroz Shaista

2010-01-01

Full Text Available Esthetics with porcelain fused to metal restoration in the anterior region can be adversely affected due to the inadequate teeth preparations and design of the prosthesis. We presented here a case report where esthetics was compromised due to darkening of the interdental papilla and marginal gingival and overcontoured restorations in relation to porcelain fused to metal restorations. Good esthetic results were obtained by using basic principles of tooth preparation and using collarless metal ceramic restorations.

Environmental and Health Effects Review for Obscurant Fog Oil

Science.gov (United States)

1993-09-01

planktonic shrimp, Luciferfaxoni. Percy and Mullin (1977) reported that minute dispersions (25 pl of oil in 500 ml seawater) reduced locomotor activity of the...Munch, R. P. Streicher, H. P. Ringhand, and F. C. Kopfler. 1984. "The Identification and Measurement of Components in Gasoline , Kerosene, and No. 2

Painting blindness and obscuring vision: Rembrandt and the senses

OpenAIRE

Smith, Samantha Leanne

2014-01-01

This thesis takes three paintings by seventeenth- century Dutch artist Rembrandt van Rijn (1606- 1669) and analyses them in the light of the interrelated themes of blindness, sight and touch. The choice of theme originates from Rembrandt's frequent use of blindness as subject matter. The discussion takes its inspiration from Svetlana Alpers' discussion in a chapter from her book on Rembrandt, The Master's Touch' and French philosopher Jacques Derrida's book Memoirs...

Travails of travel. Subtle and obscure causes of illness.

Science.gov (United States)

Gordon, M E

1988-07-01

Knowledge of patients' travel history is an important facet of diagnosis. Malaria, Chagas' disease, toxoplasmosis, Lyme disease, arboviruses, and many other relatively unusual diseases can be contracted while the patient is traveling, and the symptoms, which may mimic another disease, may not become obvious until the patient returns. The Roman philosopher Marcus Aurelius Antoninus alerts us to easier resolutions of our daily diagnostic dilemmas: "Look within and let neither the peculiar quality of anything nor its value escape thee."

Distinctive genomic signature of neural and intestinal organoids from familial Parkinson's disease patient-derived induced pluripotent stem cells.

Science.gov (United States)

Son, M-Y; Sim, H; Son, Y S; Jung, K B; Lee, M-O; Oh, J-H; Chung, S-K; Jung, C-R; Kim, J

2017-12-01

The leucine-rich repeat kinase 2 (LRRK2) G2019S mutation is the most common genetic cause of Parkinson's disease (PD). There is compelling evidence that PD is not only a brain disease but also a gastrointestinal disorder; nonetheless, its pathogenesis remains unclear. We aimed to develop human neural and intestinal tissue models of PD patients harbouring an LRRK2 mutation to understand the link between LRRK2 and PD pathology by investigating the gene expression signature. We generated PD patient-specific induced pluripotent stem cells (iPSCs) carrying an LRRK2 G2019S mutation (LK2GS) and then differentiated into three-dimensional (3D) human neuroectodermal spheres (hNESs) and human intestinal organoids (hIOs). To unravel the gene and signalling networks associated with LK2GS, we analysed differentially expressed genes in the microarray data by functional clustering, gene ontology (GO) and pathway analyses. The expression profiles of LK2GS were distinct from those of wild-type controls in hNESs and hIOs. The most represented GO biological process in hNESs and hIOs was synaptic transmission, specifically synaptic vesicle trafficking, some defects of which are known to be related to PD. The results were further validated in four independent PD-specific hNESs and hIOs by microarray and qRT-PCR analysis. We provide the first evidence that LK2GS also causes significant changes in gene expression in the intestinal cells. These hNES and hIO models from the same genetic background of PD patients could be invaluable resources for understanding PD pathophysiology and for advancing the complexity of in vitro models with 3D expandable organoids. © 2017 British Neuropathological Society.

IC 3639—a New Bona Fide Compton-Thick AGN Unveiled by NuSTAR

Science.gov (United States)

Boorman, Peter G.; Gandhi, P.; Alexander, D. M.; Annuar, A.; Ballantyne, D. R.; Bauer, F.; Boggs, S. E.; Brandt, W. N.; Brightman, M.; Christensen, F. E.; Craig, W. W.; Farrah, D.; Hailey, C. J.; Harrison, F. A.; Hönig, S. F.; Koss, M.; LaMassa, S. M.; Masini, A.; Ricci, C.; Risaliti, G.; Stern, D.; Zhang, W. W.

2016-12-01

We analyze high-quality NuSTAR observations of the local (z = 0.011) Seyfert 2 active galactic nucleus (AGN) IC 3639, in conjunction with archival Suzaku and Chandra data. This provides the first broadband X-ray spectral analysis of the source, spanning nearly two decades in energy (0.5-30 keV). Previous X-ray observations of the source below 10 keV indicated strong reflection/obscuration on the basis of a pronounced iron fluorescence line at 6.4 keV. The hard X-ray energy coverage of NuSTAR, together with self-consistent toroidal reprocessing models, enables direct broadband constraints on the obscuring column density of the source. We find the source to be heavily Compton-thick (CTK) with an obscuring column in excess of 3.6× {10}24 cm-2, unconstrained at the upper end. We further find an intrinsic 2-10 keV luminosity of {{log}}10({L}2{--10{keV}} [{erg} {{{s}}}-1])={43.4}-1.1+0.6 to 90% confidence, almost 400 times the observed flux, and consistent with various multiwavelength diagnostics. Such a high ratio of intrinsic to observed flux, in addition to an Fe-Kα fluorescence line equivalent width exceeding 2 keV, is extreme among known bona fide CTK AGNs, which we suggest are both due to the high level of obscuration present around IC 3639. Our study demonstrates that broadband spectroscopic modeling with NuSTAR enables large corrections for obscuration to be carried out robustly and emphasizes the need for improved modeling of AGN tori showing intense iron fluorescence.

A POSSÍVEL FLEXIBILIZAÇÃO DOS DIREITOS SOCIAIS E POLÍTICAS PÚBLICAS: SOLUÇÃO PARA O MERCOSUL EM TEMPOS DE CRISE? / LA POSIBLE FLEXIBILIZACIÓN DE LOS DERECHOS SOCIALES Y POLÍTICAS PÚBLICAS: SOLUCIÓN PARA EL MERCOSUR EN TIEMPOS DE CRISIS?

Directory of Open Access Journals (Sweden)

Eduardo Biacchi Gomes

2015-08-01

Full Text Available Resumo: O presente artigo teve por objetivo examinar a temática da flexibilização dos direitos trabalhistas como possível solução para o aumento dos postos de trabalho em tempos de crise mundial. Nesse sentido, investigando-se se uma melhor interpretação das normas sociais, pode-se considerar a chamada flexibilização positiva? A resposta é afirmativa se o direito do trabalho passa a atuar no sentido de servir de instrumento de emprego e das condições mínimas de vida digna ao trabalhador. Nesse contexto, o artigo apresenta as principais possibilidades de flexibilização, assim como a necessidade de um novo delineamento nesse instituto, de forma a proporcionar um novo olhar e uma nova perspectiva, interpretando a norma do ponto de vista da proteção do empregado e dos propósitos de expansão e de promoção da dignidade da pessoa humana, sob a perspectiva dos direitos humanos dentro de um contexto regional, como é o caso do Mercosul. Palavras-chave: Flexibilização. Mercosul. Direitos Sociais. Direito do Trabalho. Flexibilização positiva.

Entanglement negativity and entropy in non-equilibrium conformal field theory

Directory of Open Access Journals (Sweden)

Marianne Hoogeveen

2015-09-01

Full Text Available We study the dynamics of the entanglement in one-dimensional critical quantum systems after a local quench in which two independently thermalized semi-infinite halves are joined to form a homogeneous infinite system and left to evolve unitarily. We show that under certain conditions a nonequilibrium steady state (NESS is reached instantaneously as soon as the entanglement interval is within the light cone emanating from the contact point. In this steady state, the exact expressions for the entanglement entropy and the logarithmic negativity are in agreement with the steady state density matrix being a boosted thermal state, as expected. We derive various general identities: relating the negativity after the quench with unequal left and right initial temperatures with that where the left and right temperatures are equal; and relating these with the negativity in equilibrium thermal states. In certain regimes the resulting expressions can be analytically evaluated. Immediately after the interval intersects the light cone, we find logarithmic growth. For a very long interval, we find that the negativity approaches a plateau after sufficiently long times, different from its NESS value. The NESS value is reached instantly as soon as the entire interval is contained in the light cone. This provides a theoretical framework explaining recently obtained numerical results.

Entanglement negativity and entropy in non-equilibrium conformal field theory

International Nuclear Information System (INIS)

Hoogeveen, Marianne; Doyon, Benjamin

2015-01-01

We study the dynamics of the entanglement in one-dimensional critical quantum systems after a local quench in which two independently thermalized semi-infinite halves are joined to form a homogeneous infinite system and left to evolve unitarily. We show that under certain conditions a nonequilibrium steady state (NESS) is reached instantaneously as soon as the entanglement interval is within the light cone emanating from the contact point. In this steady state, the exact expressions for the entanglement entropy and the logarithmic negativity are in agreement with the steady state density matrix being a boosted thermal state, as expected. We derive various general identities: relating the negativity after the quench with unequal left and right initial temperatures with that where the left and right temperatures are equal; and relating these with the negativity in equilibrium thermal states. In certain regimes the resulting expressions can be analytically evaluated. Immediately after the interval intersects the light cone, we find logarithmic growth. For a very long interval, we find that the negativity approaches a plateau after sufficiently long times, different from its NESS value. The NESS value is reached instantly as soon as the entire interval is contained in the light cone. This provides a theoretical framework explaining recently obtained numerical results

No safe place: parental alcoholism and adolescent suicide.

Science.gov (United States)

Meyer, D C; Phillips, W M

1990-10-01

A child growing up in an alcoholic home develops either little self-consolidation (I-ness) and efficacy (I can) or a distorted self (I am insignificant). This results in a desperate search for a soothing-object (We-ness). The sadomasochistic behaviors, which a youth witnesses and is subjected to, become internalized as survival skills, but ultimately fail. These factors set the stage for a destructive modus operandi. When there is peer group attachment pressure, this teen does not find security when questioning, "Who am I?" because there is no "I" and no "We". Instead, this adolescent experiences fear, anxiety, and range, and wonders, "What's going to happen to me?" This propels the youth into frantic behaviors that are meant to confirm a sense of "We-ness" and competence. The result, however, is greater frustration and a mirroring of the opposite. Also, since there is a diminutive capacity for trust and an exiguous chance to reach out or respond to significant others, external soothingness becomes unobtainable. When the adolescent is confronted with aloneness, helplessness, and hopelessness, desperation results and a search for a safe place ensues. Suicide holds such an illusion. It is the embodiment of sadomasochism and permits the cognition "I am capable." A case study illustrates the problems.

UM ESTUDO DA INFLUÊNCIA DA GESTÃO DE PESSOAS NO DESEMPENHO DO TRABALHADOR E NA MELHORIA DA QUALIDADE

Directory of Open Access Journals (Sweden)

Crislaine Carvalho

2017-01-01

Full Text Available A qualidade é uma das principais preocupações presentes dentro das organizações, e estas estão sempre à procura de ferramentas que possam auxiliar nesse processo. A influência da gestão de pessoas no desempenho do trabalhador pode ser um diferencial para as empresas no mercado competitivo. Este trabalho tem a finalidade de apresentar o relacionamento entre a gestão de pessoas e a gestão da qualidade e seus reflexos no processo de melhoria contínua. Nesse contexto, foi feita uma revisão bibliográfica da evolução histórica da qualidade e os reflexos da gestão de pessoas nesse processo. Foi estudado também uma evolução do termo Gestão de Pessoas e suas diversas nomenclaturas adotadas ao longo do tempo, e as influências dessas nomenclaturas no relacionamento com os funcionários. Essa pesquisa trouxe resultados positivos a respeito da influência da gestão de pessoas na melhoria da qualidade, mostrando que os interesses da empresa e dos funcionários podem sim caminhar juntos, desde que ambos os lados estejam satisfeitos, o que confirmou a hipótese inicial desse trabalho.

Phlebotomus Sandflies of the Paloich Area in the Sudan (Diptera, Psychodidae)

Science.gov (United States)

1964-10-01

Hamster, Cricetus auratus Toad, Bufo regularis (?) Gecko, H. turicus Skink, M. striata Puff adder Snake, CMNH HH-9111’ Snake, CMNH HH-9112’ Hedgehog ...Pharynx unarmed distally or only with few, smail spines ; pigment patch not dark enough to obscure teeth .................. 8 Pharynx heavily...armed distally with numerous, dark spines ; pigment patch very dark, 1964 Quate: Sudanese sandflies 237 often obscuring teeth unless specimen well

Peering through the dust: NuSTAR observations of two first-2MASS red quasars

DEFF Research Database (Denmark)

LaMassa, Stephanie M.; Ricarte, Angelo; Glikman, Eilat

2016-01-01

through this gas and dust, revealing the properties of circumnuclear obscuration. Here, we present NuSTAR and XMM-Newton/Chandra observations of FIRST-2MASS-selected red quasars F2M 0830+3759 and F2M 1227+3214. We find that though F2M 0830+3759 is moderately obscured (NH,Z = (2.1 ± 0.2) ×  1022 cm−2...

Stable lead isotopic characterisation of the historical record of environmental lead contamination in dated freshwater lake sediment cores from northern and central Scotland

Energy Technology Data Exchange (ETDEWEB)

Eades, L.J.; Farmer, J.G. [Environmental Chemistry Unit, Department of Chemistry, University of Edinburgh, West Mains Road, EH9 3JJ, Scotland Edinburgh (United Kingdom); MacKenzie, A.B. [Scottish Universities Research and Reactor Centre, East Kilbride, G75 0QF, Scotland Glasgow (United Kingdom); Kirika, A.; Bailey-Watts, A.E. [NERC Centre for Ecology and Hydrology, EH26 0QB, Scotland Penicuik (United Kingdom)

2002-06-20

Sediment cores from three Scottish freshwater lakes, Loch Ness in the remote north and Loch Lomond and the Lake of Menteith, much closer to the heavily populated and industrialised central belt, were analysed for 210Pb, 137Cs, Pb and stable Pb isotopic composition (206Pb/207Pb). The radionuclide data were used to establish chronologies for the Loch Ness and Loch Lomond cores, but a chronology could not be developed for the Lake of Menteith core, in which the surface sediment had been subject to intense mixing. Although Pb concentrations generally started increasing during the mid-17th Century, a small peak occurred for Loch Ness in the early 16th Century, perhaps attributable to the influence of medieval mining and smelting in mainland Europe. Temporal trends in the pattern of Pb accumulation were similar for Loch Ness and both sites in Loch Lomond, with 40-50% of the anthropogenic Pb deposited prior to the 20th Century. Fluxes of anthropogenic Pb to the lake sediments peaked during the 1950s at all locations where chronologies could be established. The 5-fold increase in anthropogenic Pb inventory for the southern basin of Loch Lomond relative to Loch Ness reflected geographical proximity to the main polluting sources. The 206Pb/207Pb data for anthropogenic Pb in the sediments from Loch Ness and Loch Lomond exhibited largely similar trends related to five different time periods. Pre-1820, the 206Pb/207Pb ratio was close to that for coal (1.181). From 1820 to 1900, a fairly constant 206Pb/207Pb ratio of 1.17 probably resulted from a combination of emissions from the smelting of indigenous Pb ore (1.170) and coal burning (1.181) in Scotland, and industrial activity to the south in England, where Australian Pb of characteristically low 206Pb/207Pb ratio (1.04) was already in use. From 1901 to 1930, the 206Pb/207Pb ratio declined by <0.01, due to the increasing influence of Australian Pb. From 1931 to 1975/1985, the 206Pb/207Pb ratio of anthropogenic Pb declined by a

Stable lead isotopic characterisation of the historical record of environmental lead contamination in dated freshwater lake sediment cores from northern and central Scotland.

Science.gov (United States)

Eades, L J; Farmer, J G; MacKenzie, A B; Kirika, A; Bailey-Watts, A E

2002-06-20

Sediment cores from three Scottish freshwater lakes, Loch Ness in the remote north and Loch Lomond and the Lake of Menteith, much closer to the heavily populated and industrialised central belt were analysed for 210Pb, 137Cs, Pb and stable Pb isotopic composition (206Pb/207Pb). The radionuclide data were used to establish chronologies for the Loch Ness and Loch Lomond cores, but a chronology could not be developed for the Lake of Menteith core, in which the surface sediment had been subject to intense mixing. Although Pb concentrations generally started increasing during the mid-17th Century, a small peak occurred for Loch Ness in the early 16th Century, perhaps attributable to the influence of medieval mining and smelting in mainland Europe. Temporal trends in the pattern of Pb accumulation were similar for Loch Ness and both sites in Loch Lomond, with 40-50% of the anthropogenic Pb deposited prior to the 20th Century. Fluxes of anthropogenic Pb to the lake sediments peaked during the 1950s at all locations where chronologies could be established. The 5-fold increase in anthropogenic Pb inventory for the southern basin of Loch Lomond relative to Loch Ness reflected geographical proximity to the main polluting sources. The 206Pb/207Pb data for anthropogenic Pb in the sediments from Loch Ness and Loch Lomond exhibited largely similar trends related to five different time periods. Pre-1820, the 206Pb/207Pb ratio was close to that for coal (1.181). From 1820 to 1900, a fairly constant 206Pb/207Pb ratio of approximately 1.17 probably resulted from a combination of emissions from the smelting of indigenous Pb ore (1.170) and coal burning (1.181) in Scotland, and industrial activity to the south in England, where Australian Pb of characteristically low 206Pb/207Pb ratio (1.04) was already in use. From 1901 to 1930, the 206Pb/207Pb ratio declined by <0.01, due to the increasing influence of Australian Pb. From 1931 to 1975/1985, the 206Pb/207Pb ratio of anthropogenic Pb

Laser Imaging Video Camera Sees Through Fire, Fog, Smoke

Science.gov (United States)

2015-01-01

Under a series of SBIR contracts with Langley Research Center, inventor Richard Billmers refined a prototype for a laser imaging camera capable of seeing through fire, fog, smoke, and other obscurants. Now, Canton, Ohio-based Laser Imaging through Obscurants (LITO) Technologies Inc. is demonstrating the technology as a perimeter security system at Glenn Research Center and planning its future use in aviation, shipping, emergency response, and other fields.

Nonequilibrium steady state and induced currents of a mesoscopically glassy system: interplay of resistor-network theory and Sinai physics.

Science.gov (United States)

Hurowitz, Daniel; Rahav, Saar; Cohen, Doron

2013-12-01

We introduce an explicit solution for the nonequilibrium steady state (NESS) of a ring that is coupled to a thermal bath, and is driven by an external hot source with log-wide distribution of couplings. Having time scales that stretch over several decades is similar to glassy systems. Consequently there is a wide range of driving intensities where the NESS is like that of a random walker in a biased Brownian landscape. We investigate the resulting statistics of the induced current I. For a single ring we discuss how sign of I fluctuates as the intensity of the driving is increased, while for an ensemble of rings we highlight the fingerprints of Sinai physics on the distribution of the absolute value of I.

A POLÍTICA DE JUVENTUDE E SEUS ATORES SOCIAIS

Directory of Open Access Journals (Sweden)

Lúbia Badaró

2013-12-01

Full Text Available O presente artigo promove uma apreciação sobre o processo de construção da Política Nacional de Juventude, discutindo como essa demanda chegou à agenda pública e quais os atores e eventos que contribuíram nesse processo de inclusão dessa temática na arena de debate. Chegou-se à conclusão que os movimentos sociais e organizações da sociedade civil tiveram um papel importante nesse processo, pois favoreceram as mobilizações, abriram o debate e aproximaram a temática da juventude da esfera do governo federal, que então direcionou parte da sua atenção também para esse segmento.

Sobre a importância da equipe para gestão de projetos sob a óptica da produtividade

Directory of Open Access Journals (Sweden)

Antonio Mendes Silva Filho

2015-03-01

Full Text Available Dispor de talentos numa equipe de projeto constitui um diferencial competitivo. Contudo, há outros elementos que podem influenciadores a gestão de um projeto. Nesse sentido, destacam-se (1 a volatilidade dos requisitos do produto, (3 as oportunidades de negócios, (3 a legislação existente e termos contratuais de projeto, (4 a certeza da incerteza nas estimativas e (5 a montagem da equipe. A escolha das pessoas e respectivas competências podem ser o fator principal que separa o sucesso do insucesso de um projeto. Nesse sentido, o artigo destaca as atividades para montar uma equipe de projeto e discute questões da montagem da equipe sob a óptica da produtividade.

IC 3639 - A New Bona Fide Compton-Thick AGN Unveiled By NuSTAR

Science.gov (United States)

Boorman, Peter G.; Gandhi, P.; Alexander, D. M.; Annuar, A.; Ballantyne, D. R.; Bauer, F.; Boggs, S. E.; Brandt, W. N.; Brightman, M.; Christensen, F. E.;

How Quasar Feedback May Shape the Co-evolutionary Paths

Energy Technology Data Exchange (ETDEWEB)

Ishibashi, Wako, E-mail: wako.ishibashi@physik.uzh.ch [Physik-Institut, University of Zurich, Zürich (Switzerland)

2017-10-17

Observations point toward some form of “co-evolutionary sequence,” from dust-enshrouded starbursts to luminous unobscured quasars. Active galactic nucleus (AGN) feedback is generally invoked to expel the obscuring dusty gas in a blow-out event, eventually revealing the hidden central quasar. However, the physical mechanism driving AGN feedback, either due to winds or radiation, remains uncertain and is still a source of much debate. We consider quasar feedback, based on radiation pressure on dust, which directly acts on the obscuring dusty gas. We show that AGN radiative feedback is capable of efficiently removing the obscuring cocoon, and driving powerful outflows on galactic scales, consistent with recent observations. I will discuss how such quasar feedback may provide a natural physical interpretation of the observed evolutionary path, and the physical implications in the broader context of black hole-host galaxy co-evolution.

Coeval Starburst and AGN Activity in the CDFS

Science.gov (United States)

Brusa, M.; Fiore, F.

2009-10-01

Here we present a study on the host galaxies properties of obscured Active Galactic Nuclei (AGN) detected in the CDFS 1Ms observation and for which deep K-band observations obtained with ISAAC@VLT are available. The aim of this study is to characterize the host galaxies properties of obscured AGN in terms of their stellar masses, star formation rates, and specific star formation rates. To this purpose we refined the X-ray/optical association of 179 1 Ms sources in the MUSIC area, using a three-bands (optical, K, and IRAC) catalog for the counterparts search and we derived the rest frame properties from SED fitting. We found that the host of obscured AGN at z>1 are associated with luminous, massive, red galaxies with significant star formation rates episodes still ongoing in about 50% of the sample.

S¯adhan¯a Vol. 30, 2005 Author Index

Indian Academy of Sciences (India)

Ion cyclotron resonance heating system on. Aditya. 21 ... Hemachandra N. Perishable inventory management and ... Narahari Y. Combinatorial auctions for electronic busi- ness. 179 ... binary text document images based on linear regression ...

Antropofagia, mestiçagem e estranhamento:tradução em (discurso

Directory of Open Access Journals (Sweden)

Alice Maria Araújo Ferreira

2013-02-01

Full Text Available http://dx.doi.org/10.5007/2175-7968.2013v1n31p35 O objetivo do artigo é discutir a antropofagia em suas relações paradigmáticas com a tradução, e historicamente, dar continuidade ao sentido da Semana de Arte Moderna de 1922 e ao Manifesto Antropófago de 1928. Nesse sentido, importa destacar a antropofagia como movimento crítico baseado nos termos de “devoração/digestão/transformação”, pois se a arte (enquanto objeto é, ao mesmo tempo,um processo crítico-teórico e artístico-criativo do fazer, logo a tradução pode ser definida nesses mesmos termos. Isso implica também resgatar uma dupla relação da tradução, situando-a entre o “fazer” tradução e o “pensar este fazer da tradução, num movimento de autorreflexividade que sustenta o paradigma construído nos Estudos da Tradução”. A consequência é colocar o tradutor em trêslugares de fala:tradutor, crítico e poiesiador. Nesse sentido, a tradução define-se como processo criativo (sujeito/tempo/espaço e como processo crítico-teórico

ENSINO DE FILOSOFIA E EJA: CONTEXTUALIZAÇÃO HISTÓRICA E DESAFIOS DA CONTEMPORANEIDADE

Directory of Open Access Journals (Sweden)

Luiz Roberto Santos

2011-09-01

Full Text Available O labor apresentado aqui pretende discutir o intercurso histórico e conceitual da Educação de Jovens e Adultos - EJA – e a disciplina de Filosofia nesse contexto de situação. Nesse sentido, o trabalho fez uma contextualização histórica destas duas realidades distintas e a apreciação de documentos originais que tratam da referida modalidade de oferta de ensino. Em seguida, realizou-se uma atividade empírica com 79 alunos da modalidade EJA do IFRN campus Macau, que responderam a um questionário sobre a percepção e expectativas do ensino de Filosofia. O IFRN tem gerado um quadro de qualificação, de natureza profissional e humanística, que certamente está contribuindo para o crescimento socioeconômico da microrregião salineira. Nesse contexto, os conteúdos inerentes à disciplina de Filosofia têm sido essenciais à concretização dos valores agenciados pela Educação. Tais valores se referem principalmente ao desenvolvimento de um sentimento de cidadania que ultrapasse a mera formalização legal. Ademais, foi feito um levantamento bibliográfico para consubstanciar teoricamente todas as intuições primeiras, à luz de Aranha e Martins (1998, 2009, Cortela (2006, Paiva (2003, Paiva (2005 e Pinsky (2005.

Study on GIF PR/PP evaluation methodology

Energy Technology Data Exchange (ETDEWEB)

Lee, B. H.; Kwon, E. H.; Kim, H. D. [KAERI, Daejeon (Korea, Republic of)

2012-10-15

Proliferation resistance (PR) and physical protection (PP) is one of the four technology goals of generation IV nuclear energy systems (NESs). The PR component of the goal focuses on providing strong assurance that generation IV NESs are the least desirable sources for the diversion or undeclared production of nuclear materials, whereas the PP portion of the goal ensures that generation IV NESs are robust against theft and sabotage. In 2002, the road map of the Generation IV International Forum (GIF) envisioned that the R and D program for PR and PP would have three areas: 1) safeguards and physical protection technology R and D for each GIF system; 2) formulation of PR and PP criteria and metrics; and 3) evaluation of the criteria and metrics. To cover these R and D items, the PR and PP Working Group (PRPPWG) was formed in late 2002 and has since developed a methodology for PR and PP evaluation. In a succession of revisions beginning in 2004, consensus was achieved amongst all participating GIF countries and related organizations (i.e., IAEA and EU), and Revision 6 of the methodology report was approved by GIF for open distribution in 2011. The paper describes in detail the methodology developed by the PRPPWG and discusses its applicability to the sodium-cooled fast reactor (SFR) fuel cycle with pyro processing currently under development in Korea.

Gestão de pessoas na indústria criativa: o caso dos estúdios de animação brasileiros

Directory of Open Access Journals (Sweden)

Marta Corrêa Machado

Full Text Available Resumo Esta pesquisa visa entender a gestão de pessoas na indústria criativa a partir do estudo de um de seus segmentos, os estúdios de animação. Partindo da conceituação de Chaston (2008 de indústria criativa como o encontro entre negócio e cultura, observou-se o dilema entre a realização artística e os objetivos comerciais presente também nesse segmento da indústria. No estudo, pudemos aprofundar o entendimento sobre como esse dilema se reflete na operação da gestão de pessoas nesses estúdios brasileiros. Para entender essa questão foi conduzida uma pesquisa qualitativa através de estudos de casos em quatro produtoras nacionais nos quais foram entrevistados um funcionário e um sócio de cada empresa. Os dados encontrados apontam que ainda é incipiente a gestão de pessoas nesses ambientes, embora esteja presente a noção de que esses são os recursos principais que movem essas empresas. Foi observado ainda que a retenção dos colaboradores ocorre muito mais pela sua identificação com a atividade em si do que por outras retribuições, como salário ou garantias trabalhihstas.

On Literature's Use(ful/less)ness: Reconceptualizing the Literature Curriculum in the Age of Globalization

Science.gov (United States)

Choo, Suzanne S.

2011-01-01

This paper begins by examining how debates about literature's usefulness or, more specifically, its uselessness, have been framed in terms of the binary between utilitarianism and pragmatism on the one hand, and between humanism and idealism on the other. Instead of conceiving the literature curriculum in terms of a position one privileges in a…

Two-year Facebook strategy to increase brand aware-ness and fan engagement. Case: Finlayson Oy

OpenAIRE

Rasinen, Beda

2016-01-01

During the last few years social media has not only become a channel in which we can connect and share with our family and friends, but it has grown to be one of the most cost efficient and effective marketing channels around. However, it is no longer enough for companies to just show up. To use the channels to their full potential, well designed strategies must be devised and applied. This study looks into one of the tools of perhaps the most current marketing methodology; inbound market...

The Loch Ness Monster approach to bilingual language lateralization: a response to Berquier and Ashton.

Science.gov (United States)

Paradis, M

1992-10-01

To continue to search for a difference in language lateralization between bilinguals and unilinguals is at best a futile task in the face of all the clinical evidence to the contrary and inconsistent experimental findings. No amount of refining of dichotic, tachistoscopic, or concurrent task procedures, or statistical sophistication, is likely to tap the differential reliance on pragmatic cues that might very well exist in some nonbalanced bilinguals.

Erratum: "Space Density of Optically Selected Type 2 Quasars" (2008, AJ, 136, 2373)

Science.gov (United States)

Reyes, Reinabelle; Zakamska, Nadia L.; Strauss, Michael A.; Green, Joshua; Krolik, Julian H.; Shen, Yue; Richards, Gordon T.; Anderson, Scott F.; Schneider, Donald P.

2010-03-01

Figure 12 of the paper "Space Density of Optically Selected Type 2 Quasars" compares the obscured quasar fractions derived in our work with those of other studies. Unfortunately, some of the points from these other studies were shown incorrectly. Specifically, the results from X-ray data—Hasinger (2004; open circles) and Ueda et al. (2003; open squares)—which we had taken from Figure 16 of Hopkins et al. (2006), were affected by a luminosity conversion error, in the sense that the displayed luminosities for these data were too high by ~1 dex. With this erratum, we correct this problem and update the figure. The new version (Figure 12) shows more recent results from Hasinger (2008), in lieu of the Hasinger (2004) data points. These are based on data in the redshift range z = 0.2-3.2 (open circles) in that work. The best linear fit to these data (black dashed line) is consistent with that derived for the redshift slice z = 0.4-0.8, which overlaps with the highest redshift bin in our study, and is higher than that derived for redshifts smaller than 0.4 (corresponding to a shift of ~0.7 dex in luminosity). Figure 12 also shows estimates of the obscured quasar fraction derived from the ratio of IR to bolometric luminosities of an AGN sample at redshift z ~ 1 (Treister et al. 2008; filled triangles). Because the obscured quasar fractions derived from our analysis (colored arrows) are strict lower limits, there was already a hint in the previous version of Figure 12 that at high quasar luminosities, we find higher obscured quasar fractions than X-ray surveys. The correction and updates of Figure 12 strengthen this conclusion. At face value, our derived obscured quasar fractions are consistent with those from IR data (Treister et al. 2008; filled triangles). However, we find that they are significantly higher than those derived from X-ray surveys at L_[O\\,\\mathsc {iii]}\\gtrsim 10^{9.5}\\;L_{\\odot }, especially those from the recent analysis by Hasinger (2008). This

Nonequilibrium steady state in open quantum systems: Influence action, stochastic equation and power balance

International Nuclear Information System (INIS)

Hsiang, J.-T.; Hu, B.L.

2015-01-01

The existence and uniqueness of a steady state for nonequilibrium systems (NESS) is a fundamental subject and a main theme of research in statistical mechanics for decades. For Gaussian systems, such as a chain of classical harmonic oscillators connected at each end to a heat bath, and for classical anharmonic oscillators under specified conditions, definitive answers exist in the form of proven theorems. Answering this question for quantum many-body systems poses a challenge for the present. In this work we address this issue by deriving the stochastic equations for the reduced system with self-consistent backaction from the two baths, calculating the energy flow from one bath to the chain to the other bath, and exhibiting a power balance relation in the total (chain + baths) system which testifies to the existence of a NESS in this system at late times. Its insensitivity to the initial conditions of the chain corroborates to its uniqueness. The functional method we adopt here entails the use of the influence functional, the coarse-grained and stochastic effective actions, from which one can derive the stochastic equations and calculate the average values of physical variables in open quantum systems. This involves both taking the expectation values of quantum operators of the system and the distributional averages of stochastic variables stemming from the coarse-grained environment. This method though formal in appearance is compact and complete. It can also easily accommodate perturbative techniques and diagrammatic methods from field theory. Taken all together it provides a solid platform for carrying out systematic investigations into the nonequilibrium dynamics of open quantum systems and quantum thermodynamics. -- Highlights: •Nonequilibrium steady state (NESS) for interacting quantum many-body systems. •Derivation of stochastic equations for quantum oscillator chain with two heat baths. •Explicit calculation of the energy flow from one bath to the

Preeclampsia and Eclampsia

Science.gov (United States)

... NICHD Research Information Find a Study More Information Bullying About NICHD Research Information Find a Study More ... Hubel, C. A., Markovic, N., Ness, R. B., & Powers, R. W. (2005). Uric acid is as important ...

Identification of two genes potentially associated in iron-heme ...

Indian Academy of Sciences (India)

2013-03-15

Mar 15, 2013 ... include the degree of vessel stenosis, ulceration, inflamma- tory cell infiltration and ... ness, ulceration, hemorrhage, necrosis, calcification, in- flammation ... treatment. Clinical .... An alternative would be to use only tissue from ...

The Belmont Valley integrated algae pond system in retrospect

African Journals Online (AJOL)

2013-03-26

Mar 26, 2013 ... ness amongst all stakeholders including the public at large, the three spheres of ...... (2011) Algae biofuel from wastewater treatment high rate algal ponds. .... and OELMÜLLER R (2002) Photosynthetic electron transport.

Family Planning, Abortion, and HIV in Ghanaian Print Media: A 15 ...

African Journals Online (AJOL)

Erah

15-Month Content Analysis of a National Ghanaian Newspaper ... ness, and influence policy—an initiative that ... expense of the principle of proportionality in media ... analysis can have actionable results. The .... General Elections in Ghana.

Seeking the epoch of maximum luminosity for dusty quasars

International Nuclear Information System (INIS)

Vardanyan, Valeri; Weedman, Daniel; Sargsyan, Lusine

2014-01-01

Infrared luminosities νL ν (7.8 μm) arising from dust reradiation are determined for Sloan Digital Sky Survey (SDSS) quasars with 1.4 10 46.6 erg s –1 for all 2 obscured' quasars as those having >5 mag of ultraviolet extinction. We present a new summary of obscured quasars discovered with the Spitzer Infrared Spectrograph and determine the infrared luminosity function of these obscured quasars at z ∼ 2.1. This is compared with infrared luminosity functions of optically discovered, unobscured quasars in the SDSS and in the AGN and Galaxy Evolution Survey. The comparison indicates comparable numbers of obscured and unobscured quasars at z ∼ 2.1 with a possible excess of obscured quasars at fainter luminosities.

JASA PRIVATE BANKING PADA LEMBAGA PERBANKAN SEBAGAI SASARAN DAN SARANA PENCUCIAN UANG

Directory of Open Access Journals (Sweden)

Ari Purwadi

2012-01-01

Full Text Available Bank can experience the risk used by criminal as purposes to do money laundry for their crime. The technique of money laundry is often used by bank industry. It is occurred because bank offer lots of services in flowing the money which can conceal the history of fund. One of them is private service of bank offered by bank in which it gives advantages for criminal to hide their crime. The role of private banker as advisors must be loyal to their customers, either for professionally or personally. It gives impact to customers that they do not response towards the criminality of the customers’ activities. The culture of secret ness has spread and inserted to banking private industry. With the tight bank secret ness, it provides potential for money laundry purposes.

Estimation of Anonymous Email Network Characteristics through Statistical Disclosure Attacks

Directory of Open Access Journals (Sweden)

Javier Portela

2016-11-01

Full Text Available Social network analysis aims to obtain relational data from social systems to identify leaders, roles, and communities in order to model profiles or predict a specific behavior in users’ network. Preserving anonymity in social networks is a subject of major concern. Anonymity can be compromised by disclosing senders’ or receivers’ identity, message content, or sender-receiver relationships. Under strongly incomplete information, a statistical disclosure attack is used to estimate the network and node characteristics such as centrality and clustering measures, degree distribution, and small-world-ness. A database of email networks in 29 university faculties is used to study the method. A research on the small-world-ness and Power law characteristics of these email networks is also developed, helping to understand the behavior of small email networks.

Estimation of Anonymous Email Network Characteristics through Statistical Disclosure Attacks

Science.gov (United States)

Portela, Javier; García Villalba, Luis Javier; Silva Trujillo, Alejandra Guadalupe; Sandoval Orozco, Ana Lucila; Kim, Tai-Hoon

2016-01-01

Social network analysis aims to obtain relational data from social systems to identify leaders, roles, and communities in order to model profiles or predict a specific behavior in users’ network. Preserving anonymity in social networks is a subject of major concern. Anonymity can be compromised by disclosing senders’ or receivers’ identity, message content, or sender-receiver relationships. Under strongly incomplete information, a statistical disclosure attack is used to estimate the network and node characteristics such as centrality and clustering measures, degree distribution, and small-world-ness. A database of email networks in 29 university faculties is used to study the method. A research on the small-world-ness and Power law characteristics of these email networks is also developed, helping to understand the behavior of small email networks. PMID:27809275

Fisiologia do transporte de fluidos e solutos atraves da membrana peritoneal

Directory of Open Access Journals (Sweden)

Anna Rita Aguirre

2014-03-01

Full Text Available Nesta revisão, são explicados os fenômenos envolvidos nas trocas de fluidos e solutos através da membrana peritoneal, tanto na situação fisiológica quanto no contexto da diálise peritoneal. Para tanto, são utilizados os modelos matemáticos desenvolvidos para estudo do transporte pela membrana, tais como o "Modelo de Poros" e o "Modelo Distributivo". Os ganhos científicos com as pesquisas nesse campo são contemplados e as áreas que merecem pesquisas adicionais também são citadas. Assim, o estado atual do conhecimento fisiológico a respeito dessa modalidade de terapia renal substitutiva, no que se refere aos eventos relacionados à membrana peritoneal, encontra-se sintetizado nesse manuscrito.

Landau superfluids as nonequilibrium stationary states

International Nuclear Information System (INIS)

Wreszinski, Walter F.

2015-01-01

We define a superfluid state to be a nonequilibrium stationary state (NESS), which, at zero temperature, satisfies certain metastability conditions, which physically express that there should be a sufficiently small energy-momentum transfer between the particles of the fluid and the surroundings (e.g., pipe). It is shown that two models, the Girardeau model and the Huang-Yang-Luttinger (HYL) model, describe superfluids in this sense and, moreover, that, in the case of the HYL model, the metastability condition is directly related to Nozières’ conjecture that, due to the repulsive interaction, the condensate does not suffer fragmentation into two (or more) parts, thereby assuring its quantum coherence. The models are rigorous examples of NESS in which the system is not finite, but rather a many-body system

An expression of excess work during the transition between nonequilibrium steady states

International Nuclear Information System (INIS)

Yuge, Tatsuro

2014-01-01

Excess work is a nondiverging part of the work during the transition between nonequilibrium steady states (NESSs). It is a central quantity in steady-state thermodynamics (SST), which is a candidate for nonequilibrium thermodynamics theory. We derive an expression of excess work during quasistatic transitions between NESSs by using the macroscopic linear response relation of the NESS. This expression is a line integral of a vector potential in the space of control parameters. We show a relationship between the vector potential and the response function of the NESS, and thus obtain a relationship between the SST and a macroscopic quantity. We also connect the macroscopic formulation to microscopic physics through a microscopic expression of the nonequilibrium response function, which gives a result that is consistent with previous studies. (paper)

Heidegger E A Técnica Moderna Como Perigo E Como Salvação

Directory of Open Access Journals (Sweden)

Robson Costa Cordeiro

2014-04-01

Full Text Available O mundo contemporâneo é marcado por uma compreensão de técnica que se ergue como tal a partir de um sentido próprio e autônomo. Este sentido pode ser caracterizado como um logos que se constitui a partir de sua própria natureza e se manifesta como tecnologia no decorrer da história. Compreender esse sentido e assumi-lo como condição de nossa existência no mundo é comprender a técnica como nossa herança e nosso envio. Nesse sentido, compreender a essência da técnica é fundamental para o mundo contemporâneo, assumindo que, nesse processo, consiste o perigo e a salvação da espécie.

Membranous glomerulopathy with spherules: an uncommon variant with obscure pathogenesis.

Science.gov (United States)

Kowalewska, Jolanta; Smith, Kelly D; Hudkins, Kelly L; Chang, Anthony; Fogo, Agnes B; Houghton, Donald; Leslie, Deena; Aitchison, John; Nicosia, Roberto F; Alpers, Charles E

2006-06-01

Occasional case reports of membranous glomerulopathy described unique subepithelial accumulations of an unusual type of immune deposit composed of spherular structures. The identity of such structures as nuclear pores has been suggested, but not established. We identified a cohort of patients (n = 14, including 1 patient with disease recurrence in an allograft) who presented with nephrotic syndrome and had renal biopsy specimens with light and immunofluorescence microscopic findings characteristic of membranous glomerulopathy. These patients were distinguished by ultrastructural studies that showed glomerular capillary wall accumulations of subepithelial immune deposits composed of uniform spherular structures, while lacking the typical granular electron-dense deposits seen in membranous glomerulopathy. The molecular identity of these spherular structures as nuclear pores was tested by using immunofluorescence microscopy and immunohistochemistry with mouse monoclonal antinuclear pore antibodies (Covance, Princeton, NJ) and anti-Nuclear Pore-O-Linked Glycoprotein (Affinity BioReagents Inc, Golden, CO) antibodies. Measurement of spherular structures by using high-magnification electron microscopy showed an average diameter of 84.5 nm, which correlated well with accepted diameters of nuclear pores (80 to 120 nm). Immunofluorescence microscopy and immunoperoxidase staining with both antibodies showed characteristic beaded staining of nuclear membranes of multiple cell types within normal control kidney, but no staining of immune-type deposits within glomerular basement membranes. These cases form a rare, but distinctive, morphological subclass of membranous glomerulopathy. The antigenic specificity of immune deposits in these cases remains elusive.

Europe as a nuclear power, this obscure object of desire

International Nuclear Information System (INIS)

Mallard, Gregoire

2009-01-01

This article proposes an historical and analytical overview of the creation and role of European bodies dedicated to the control of nuclear industry and materials, and of international relationships between Europe and the USA in this respect. The author adopts an approach of these issues within the framework of sociology of diplomatic action and of tactics of enunciation which give sense to European treaties. He discusses how the control of the German nuclear development has been addressed during the first stage of development of the European community. He evokes negotiations of 1955 about the common market treaty and the Euratom treaty. Then, he comments the opinion of a federalist action committee (the action committee for the United States of Europe), and outlines the role played by the US government in the negotiations between Euratom and the USA. The roles of these bodies are notably commented regarding European activities of uranium enrichment

Discovery of Highly Obscured Galaxies in the Zone of Avoidance

Science.gov (United States)

2008-08-01

the optical (e.g., Roman et al. 2000), near-infrared (DENIS, Schroder et al. 1999; Two Micron All Sky Survey ( 2MASS ), Jarrett et al. 2000), far... 2MASS (Skrutskie et al. 2006), downloaded directly from the NASA/IPAC Infrared Science Archive (IRSA).5 The boundaries of our search were set by the...Figure 3. 2MASS J (blue), H (green), and /is (red) color composite images of the same galaxies. The galaxies are displayed in the same order as shown

Versatile Boron Carbide-Based Visual Obscurant Compositions for Smoke Munitions

Science.gov (United States)

2015-04-17

volatilize and disperse reaction products and inert diluents. Unlike the refractory oxides of common pyrotechnic fuels such as magnesium and aluminum, boron...peaks marked. [1] Akagi, R.; Ohtori, N.; Umesaki, N. Raman spectra of K2O–B2O3 glasses and melts. Journal of Non-Crystalline Solids. 2001

Multidrug-resistant pattern of food borne illness associated bacteria ...

African Journals Online (AJOL)

This study aimed at determining anti-microbial resistance pattern of food borne illness ... bial drugs in the pharmaceutical pipeline.2 The effective- ness of ... Materials and methods ... selected based on local availability, clinical efficiency, liter-.

Zamyšlení nad publikací Ročenka konkurenceschopnosti České republiky 2005

Czech Academy of Sciences Publication Activity Database

Lízal, Lubomír

2006-01-01

Roč. 54, č. 4 (2006), s. 549-556 ISSN 0032-3233 Institutional research plan: CEZ:AV0Z70850503 Keywords : competitive ness * Czech Republic Subject RIV: AH - Economics Impact factor: 0.363, year: 2006

Innovation generation: how to produce creative and useful scientific ideas

National Research Council Canada - National Science Library

Ness, Roberta B

2012-01-01

... innovative. In Innovation Generation, internationally renowned physician and scientist Roberta Ness provides all the tools you need to cast aside your habitual ways of navigating the every-day world and to think "outside the box...

Mitochondrial Myopathies

Science.gov (United States)

... noting “soft signs” in unaffected relatives. These include deaf- ness, short stature, migraine headaches and PEO. Muscle ... mitochondrial defects and provide valuable information for family planning. Perhaps most important, knowing the genetic defects that ...

EVIDENCE FROM THE VERY LONG BASELINE ARRAY THAT J1502SE/SW ARE DOUBLE HOTSPOTS, NOT A SUPERMASSIVE BINARY BLACK HOLE

International Nuclear Information System (INIS)

Wrobel, J. M.; Walker, R. C.; Fu, H.

2014-01-01

SDSS J150243.09+111557.3 is a merging system at z = 0.39 that hosts two confirmed active galactic nuclei (AGNs), one unobscured and one dust-obscured, offset by several kiloparsecs. Deane et al. recently reported evidence from the European VLBI Network (EVN) that the dust-obscured AGN exhibits two flat-spectrum radio sources, J1502SE/SW, offset by 26 mas (140 pc), with each source being energized by its own supermassive black hole (BH). This intriguing interpretation of a close binary BH was reached after ruling out a double-hotspot scenario, wherein both hotspots are energized by a single, central BH, a configuration occurring in the well-studied compact symmetric objects. When observed with sufficient sensitivity and resolution, an object with double hotspots should have an edge-brightened structure. We report evidence from the Very Long Baseline Array (VLBA) for just such a structure in an image of the obscured AGN with higher sensitivity and resolution than the EVN images. We thus conclude that a double-hotspot scenario should be reconsidered as a viable interpretation for J1502SE/SW, and suggest further VLBA tests of that scenario. A double-hotspot scenario could have broad implications for feedback in obscured AGNs. We also report a VLBA detection of high-brightness-temperature emission from the unobscured AGN that is offset several kiloparsecs from J1502SE/SW

Best-Matched Internal Standard Normalization in Liquid Chromatography-Mass Spectrometry Metabolomics Applied to Environmental Samples.

Science.gov (United States)

Boysen, Angela K; Heal, Katherine R; Carlson, Laura T; Ingalls, Anitra E

2018-01-16

The goal of metabolomics is to measure the entire range of small organic molecules in biological samples. In liquid chromatography-mass spectrometry-based metabolomics, formidable analytical challenges remain in removing the nonbiological factors that affect chromatographic peak areas. These factors include sample matrix-induced ion suppression, chromatographic quality, and analytical drift. The combination of these factors is referred to as obscuring variation. Some metabolomics samples can exhibit intense obscuring variation due to matrix-induced ion suppression, rendering large amounts of data unreliable and difficult to interpret. Existing normalization techniques have limited applicability to these sample types. Here we present a data normalization method to minimize the effects of obscuring variation. We normalize peak areas using a batch-specific normalization process, which matches measured metabolites with isotope-labeled internal standards that behave similarly during the analysis. This method, called best-matched internal standard (B-MIS) normalization, can be applied to targeted or untargeted metabolomics data sets and yields relative concentrations. We evaluate and demonstrate the utility of B-MIS normalization using marine environmental samples and laboratory grown cultures of phytoplankton. In untargeted analyses, B-MIS normalization allowed for inclusion of mass features in downstream analyses that would have been considered unreliable without normalization due to obscuring variation. B-MIS normalization for targeted or untargeted metabolomics is freely available at https://github.com/IngallsLabUW/B-MIS-normalization .

Evaluation of groundwater resources potential in the Ejisu-Juaben ...

African Journals Online (AJOL)

EJIRO

African Journal of Environmental Science and Technology Vol. 3 (10), pp. ..... ness of the saturated zone, m; A = hydrogeological basin ∼ extent of the study ..... system southern voltain sedimentary basin of Ghana: An isotopic approach, J.

Peripartum Cardiomyopathy

Science.gov (United States)

... short- ness of breath, and palpitations. •  Electrocardiogram (heart tracing) to assess heart rate and rhythm, to look ... Accessed January 22, 2013. The Peripartum Cardiomyopathy Network Web site. http: / / www. peripartumcmnetwork. pitt. edu. Accessed January ...

Nominal Ocular Dazzle Distance (NODD)

Science.gov (United States)

2015-02-23

4P πd2MDE r : (21) Fig. 3. A schematic of a laser dazzle scenario with the observer on the left experiencing dazzle from the laser on the right. The...more moderate level of obscuration. During the day, only angles of a few degrees can be obscured for this case. 5. Sensitivity Analysis In order to...understand the most important input parameters to the model, a sensitivity analysis of the NODD calculation has been performed. In Table 10, a set of

A philosophical analysis of the evidence-based medicine debate

OpenAIRE

Sehon, Scott R; Stanley, Donald E

2003-01-01

Abstract Background The term "evidence-based medicine" (or EBM) was introduced about ten years ago, and there has been considerable debate about the value of EBM. However, this debate has sometimes been obscured by a lack of conceptual clarity concerning the nature and status of EBM. Discussion First, we note that EBM proponents have obscured the current debate by defining EBM in an overly broad, indeed almost vacuous, manner; we offer a clearer account of EBM and its relation to the alternat...

An Existential-Phenomenological Investigation of Women's ...

African Journals Online (AJOL)

addictions, BDD, as well as low self-esteem (Rieves. & Cash .... ness and Prevention (1999), body image includes how .... her family, peers, and romantic partnerships. ...... Behaviour Research and Therapy, 32(5), 497–502. doi: 10.1016/0005-.

Young Children's Mathematics References during Free Play in Family Childcare Settings

Science.gov (United States)

Hendershot, Shawnee M.; Berghout Austin, Ann M.; Blevins-Knabe, Belinda; Ota, Carrie

2016-01-01

Very little is known about children's discussion of mathematics topics during unstructured play. Ginsburg, Lin, Ness, and Seo [2003. Young American and Chinese children's everyday mathematical activity. Mathematical Thinking and Learning, 5(4), 235-258. Retrieved from…

THE TREATMENT OF OPEN- AND NARROW-ANGLE GLAUCOMA

African Journals Online (AJOL)

1971-04-10

Apr 10, 1971 ... glaucoma will be considered: narrow-angle glaucoma. (acute glaucoma) and ... emotional or a physical crisis. The pain is in the distribu- .... ness, not increased pressure, haunts people suffering from glaucoma'.' The saga of ...

As paisagens da transição energética: uma perspectiva política

Directory of Open Access Journals (Sweden)

Marie-José Fortin

2015-11-01

Full Text Available Além de grandes objetivos genéricos, a transição energética necessita ser traduzida em políticas e em projetos bastante concretos. A implementação destes últimos, frequentemente na forma de amplos sítios de produção de energia, provoca fortes reações nos territórios, entre outros, em nome da paisagem. Entretanto, ao invés de reconhecer nesse fato uma reação sistemática de oposição, sugere-se considerar a paisagem enquanto uma forma de testar o nível de territorialização das propostas realizadas em nome da transição energética: na qualidade de arcabouço cognitivo e político, a paisagem permitiria, deste modo, confrontar “projeto” e “território”, e compreender se o primeiro demonstra-se coerente e representativo em relação ao futuro do segundo. Nesse sentido, propõe-se um roteiro de análise estruturado em três níveis, referindo-se a abordagens teóricas complementares, quais sejam: a paisagem 1 como representação social, 2 como instrumento e objeto negociado e 3 como paradigma societal. O recente desenvolvimento da matriz eólica no Québec ilustra como a “paisagem” poderia ser mobilizada nesse sentido.

DESENVOLVIMENTO E VALIDAÇÃO DE UMA ESCALA DE AVALIAÇÃO DE ATRIBUTOS IMPORTANTES PARA A ESCOLHA DE CURSOS DE INGLÊS

Directory of Open Access Journals (Sweden)

Fernanda Elisa Jesus Silva

2007-12-01

Full Text Available O crescimento de instituições que oferecem cursos de idiomas no Brasil tem sido notório nas últimas décadas, fazendo com que a competição nesse setor se tornasse bastante acirrada (Silva, 2005. Para que tais instituições possam sobreviver e crescer nesse mercado, é fundamental desenvolver estratégias mercadológicas eficazes para atrair estudantes. Nesse sentido, é imprescindível identificar os atributos que afetam a sua decisão de compra. Assim sendo, esse trabalho teve por objetivo desenvolver e validar uma escala de avaliação dos atributos considerados importantes pelos clientes na escolha de cursos de inglês. Para tanto, realizou-se um survey, por meio de entrevistas pessoais com 216 clientes potenciais em Belo Horizonte, Minas Gerais. Verificou-se que os atributos considerados importantes na escolha de cursos de inglês podem ser avaliados com base nos seguintes fatores: Qualidade dos serviços, Marca e tradição, Intercâmbio internacional, Rapidez no aprendizado, Localização comodidade, Professores (Qualidade técnica, Metodologia (Atividades extras, Infra-estrutura, Preço, Metodologia (Enfoque prático, Professores (Responsabilidade, Flexibilidade de horários e Endosso social. Os indicadores validados para avaliar tais dimensões são apresentados ao final desse artigo, bem como as limitações do trabalho e sugestões para pesquisas futuras.

Current status and future directions of development of PR/PP evaluation methodology

International Nuclear Information System (INIS)

Kim, D. Y.; Kwon, E. H.; Kim, H. D.

2012-01-01

A mandatory design requirement for the introduction of generation IV nuclear energy systems (NESs) is defined as the characteristic of a nuclear energy system that impedes the diversion or undeclared production of nuclear material, or misuse of technology, by State in order to acquire nuclear weapons or other nuclear explosive devices. The same report also defines physical protection (PP) as the use of technical, administrative, and operational measures to prevent the theft of nuclear/radioactive material for the purpose of producing nuclear weapons, producing nuclear devices for nuclear terrorism, or using the facility or transportation system for radiological sabotage. Since the early 1970s right after the Indian nuclear test, the international community has recognized the limits of political and diplomatic means to prevent overt proliferation by states and looked for ways to incorporate technical features that are inherent in NESs. As a first step, active research has been conducted to develop a methodology to evaluate PR and PP components of NESs and has now been reduced to two main R and D streams: the Generation IV International Forum (GIF) and International Project on Innovative Nuclear Reactors and Fuel Cycles (INPRO). (Currently, GIF and INPRO are leading the debate as major projects for PR and PP evaluation methods.) This paper presents an overview of the R and D accomplishments during the development of PR and PP evaluation methodology. It also suggests some directions for future research

A Gestão e o Empreendedorismo nos cursos de formação Docente

Directory of Open Access Journals (Sweden)

Felipe Chibás Ortiz

2014-12-01

Full Text Available O presente artigo analisa o conceito de gestão no âmbito da educação e aborda os principais resultados obtidos a partir de uma primeira aproximação exploratória à situação das disciplinas com temas sobre gestão e empreendedorismo no contexto dos cursos de formação de professores. A pesquisa quanti-quali aqui apresentada realizou um levantamento estatístico analisando-se a grade curricular dos cursos de Pedagogia, Letras, Artes e Educação Física do Estado de São Paulo, assim como das questões da prova do ENADE referentes aos temas de gestão e empreendedorismo nesses cursos. Os resultados obtidos apontam a carência de disciplinas que lidam com o tema de Gestão e Empreendedorismo nesses cursos, tanto no que se refere à formação teórica como à falta de estimulação sistemática das competências necessárias para gerir projetos culturais ou educativos. Como consideração final, sugere-se a implementação nesses cursos de uma disciplina que reúna tais conhecimentos relativos ao termo Gestão e Empreendedorismo, e incrementar o número e complexidade das questões de Gestão e Empreendedorismo nas provas do ENADE correspondentes a estes cursos.

Current status and future directions of development of PR/PP evaluation methodology

Energy Technology Data Exchange (ETDEWEB)

Kim, D. Y.; Kwon, E. H.; Kim, H. D. [KAERI, Daejeon (Korea, Republic of)

2012-10-15

A mandatory design requirement for the introduction of generation IV nuclear energy systems (NESs) is defined as the characteristic of a nuclear energy system that impedes the diversion or undeclared production of nuclear material, or misuse of technology, by State in order to acquire nuclear weapons or other nuclear explosive devices. The same report also defines physical protection (PP) as the use of technical, administrative, and operational measures to prevent the theft of nuclear/radioactive material for the purpose of producing nuclear weapons, producing nuclear devices for nuclear terrorism, or using the facility or transportation system for radiological sabotage. Since the early 1970s right after the Indian nuclear test, the international community has recognized the limits of political and diplomatic means to prevent overt proliferation by states and looked for ways to incorporate technical features that are inherent in NESs. As a first step, active research has been conducted to develop a methodology to evaluate PR and PP components of NESs and has now been reduced to two main R and D streams: the Generation IV International Forum (GIF) and International Project on Innovative Nuclear Reactors and Fuel Cycles (INPRO). (Currently, GIF and INPRO are leading the debate as major projects for PR and PP evaluation methods.) This paper presents an overview of the R and D accomplishments during the development of PR and PP evaluation methodology. It also suggests some directions for future research.

Reproducing whiteness and enacting kin in the Nordic context of transnational egg donation: Matching donors with cross-border traveller recipients in Finland.

Science.gov (United States)

Homanen, Riikka

2018-04-01

The multimillion-euro fertility industry increasingly tailors its treatments to infertile people who are willing to travel across national borders for treatments inaccessible at home, especially reproductive tissue donor treatments. Finland is the Nordic destination for access to donor eggs, particularly for Swedes and Norwegians hoping for a donor match that will achieve a child of phenotypically plausible biological descent. Finns are seen as Nordic kin, and the inheritability of "Nordicness" is reinforced at clinics. Drawing on ethnographic material from three fertility clinics in Finland during 2015-2017, this article discusses how Nordic relatedness and whiteness are enacted in the practices of matching of donors with recipient parents. The analysis shows a selective and exclusionary rationale to matching built around whiteness: matches between donors with dark skin tone and recipients with fair skin tone are rejected, but a match of a donor with fair skin and recipients with dark skin may be made. Within the context of transnational egg donation, the whiteness or Nordicness of Finns is not questioned as it has been in other historical circumstances. Even the establishment of a state donor register offers a guarantee of kin-ness, especially non-Russian kin-ness. It is concluded that the logics of matching protect the "purity" of whiteness but not browness or blackness, enacting Nordic(kin)ness in ways that are part of broader intra-European histories of racism and post-socialist Othering. Copyright © 2018 Elsevier Ltd. All rights reserved.

Understanding the build-up of supermassive black holes and galaxies

Science.gov (United States)

Carrera, Francisco; Ueda, Yoshihiro; Georgakakis, Antonis

2016-07-01

One of the main open questions in modern Astrophysics is understanding the coupled growth of supermassive black holes by accretion and their host galaxies via star formation, from their peak at redshifts z~ 1-4 to the present time. The generic scenario proposed involves an early phase of intense black hole growth that takes place behind large obscuring columns of inflowing dust and gas clouds. It is postulated that this is followed by a blow-out stage during which some form of AGN feedback controls the fate of the interstellar medium and hence, the evolution of the galaxy. X-rays are essential for testing this scenario as they uniquely probe AGN at both the early heavily obscured stage and the later blow-out phase. X-ray spectral analysis can identify the smoking gun evidence of heavily obscured black hole growth (e.g. intense iron Kalpha line). It therefore provides the most robust method for compiling clean samples of deeply shrouded AGN with well-defined selection functions and unbiased determinations of their intrinsic properties (accretion luminosity, obscuring column). X-rays are also the best window for studying in detail AGN feedback. This process ultimately originates in the innermost regions close to the supermassive black hole and is dominated, in terms of energy and mass flux, by highly ionisedmaterial that remains invisible at other wavelengths. The most important epoch for investigating the relation between AGN and galaxies is the redshift range z~1-4, when most black holes and stars we see in the present-day Universe were put in place. Unfortunately, exhaustive efforts with current high-energy telescopes only scrape the tip of the iceberg of the most obscured AGN population. Moreover, Xray studies of the incidence, nature and energetics of AGN feedback are limited to the local Universe. The Athena observatory will provide the technological leap required for a breakthrough in our understanding of AGN and galaxy evolution at the heyday of the Universe

Understanding the build-up of SMBH and Galaxies

Science.gov (United States)

Carrera, Francisco; Georgakakis, Antonis; Ueda, Yoshihiro; Akylas, Thanassis; Lanzuisi, Giorgio; Castello, N.

2015-09-01

One of the main open questions in modern Astrophysics is understanding the coupled growth of supermassive black holes by accretion and their host galaxies via star formation, from their peak at redshifts z~ 1-4 to the present time. The generic scenario proposed involves an early phase of intense black hole growth that takes place behind large obscuring columns of inflowing dust and gas clouds. It is postulated that this is followed by a blow-out stage during which some form of AGN feedback controls the fate of the interstellar medium and hence, the evolution of the galaxy. X-rays are essential for testing this scenario as they uniquely probe AGN at both the early heavily obscured stage and the later blow-out phase. X-ray spectral analysis can identify the smoking gun evidence of heavily obscured black hole growth (e.g. intense iron Kalpha line). It therefore provides the most robust method for compiling clean samples of deeply shrouded AGN with well-defined selection functions and unbiased determinations of their intrinsic properties (accretion luminosity, obscuring column). X-rays are also the best window for studying in detail AGN feedback. This process ultimately originates in the innermost regions close to the supermassive black hole and is dominated, in terms of energy and mass flux, by highly ionised material that remains invisible at other wavelengths. The most important epoch for investigating the relation between AGN and galaxies is the redshift range z~1-4, when most black holes and stars we see in the present-day Universe were put in place. Unfortunately, exhaustive efforts with current high-energy telescopes only scrape the tip of the iceberg of the most obscured AGN population. Moreover, Xray studies of the incidence, nature and energetics of AGN feedback are limited to the local Universe. The Athena observatory will provide the technological leap required for a breakthrough in our understanding of AGN and galaxy evolution at the heyday of the Universe

Socio-clinical factors related to the perinatal outcome of teenage ...

African Journals Online (AJOL)

owner

2013-02-25

Feb 25, 2013 ... education, disruption of the family system and prema- ture assumption of the ... ness and knowledge of sexuality without commensurate good use of ... mortality among the products of teenage pregnancies.5-7. The survival of ...

Characterization of Ag/Ag2SO4 system as reference electrode for in ...

Indian Academy of Sciences (India)

of water.10 For example, tetrafluoroborates, the most popular salts ... forming aggressive hydrofluoric acid.10–12. 'Tradi- ..... in figure 6(b) (its characteristics are also presented in table 2). .... leaders (viz., Maxwell, NessCap) working with elec-.

Effect of weld heat input on toughness and structure of HAZ of a new ...

Indian Academy of Sciences (India)

Unknown

Key Laboratory of Liquid Structure and Heredity of Materials, Ministry of Education, School of Materials Science .... should be controlled (t8/5 = 10 ~ 20 s) to improve tough- ness in the .... nology, Harbin Institute of Technology, People's Repub-.

Infinite genus surfaces and irrational polygonal billiards

OpenAIRE

Valdez, Ferrán

2009-01-01

We prove that the natural invariant surface associated with the billiard game on an irrational polygonal table is homeomorphic to the Loch Ness monster, that is, the only orientable infinite genus topological real surface with exactly one end.

Consciousness: The flipside of anaesthesia

African Journals Online (AJOL)

Adele

This option includes “perfect” simulation of conscious- ness, without it actually ... in particular, the search for molecular mechanisms has been greatly hindered by our .... q-bits in a distributed array of cytoskeletal proteins through- out the cell.

Atividade antimicrobiana e antioxidante do óleo essencial de ho-sho (Cinnamomum camphora Ness e Eberm Var. Linaloolifera fujita Antimicrobial and antioxidant activities of ho-sho (Cinnamomum camphora Ness e Eberm Var. Linaloolifera fujita essential oil

Directory of Open Access Journals (Sweden)

Rogério Luis Cansian

2010-06-01

Full Text Available Este trabalho teve como objetivo determinar a atividade antimicrobiana e antioxidante do óleo essencial de Ho-Sho. O principal componente do óleo essencial obtido a partir de folhas da planta submetidas ao processo de hidrodestilação foi o linalol (80 a 95% m/m. O óleo essencial mostrou atividade antimicrobiana para todos os microrganismos testados, com exceção de Pseudomonas aeruginosa. A maior atividade antimicrobiana do óleo essencial sobre as bactérias testadas foi observada sobre Xanthomonas campestris (33,0 mm e a menor sobre Yersinia enterocolitica (10,5 mm. Para a concentração inibitória mínima (CIM, observou-se que todos os microrganismos apresentaram-se susceptíveis ao óleo essencial de Ho-Sho. A variação das CIM para as bactérias Gram-positivas foi de 1,00 mg.mL-1 (Streptococcus mutans a 1,75 mg.mL-1 (Staphylococcus epidermidis. Já a variação das CIM para as bactérias Gram-negativas foi de 0,625 mg.mL-1 (Citrobacter freundii a 2,50 mg.mL-1 (Shigella flexneri. Os resultados obtidos na determinação da atividade antioxidante do óleo essencial demonstram que o percentual antioxidante aumenta proporcionalmente à concentração de óleo essencial adicionado, atingindo o valor máximo de 97,49% de atividade antioxidante para a concentração de 50000 μg.mL-1.The main objective of this work was to evaluate the antimicrobial and antioxidant activities of the Ho-Sho essential oil. The major component of the essential oil obtained from the leaves submitted to hydro-distillation was linalool (80-95 wt%. The essential oil showed antimicrobial activity for all tested microorganisms, except for Pseudomonas aeruginosa. Higher antimicrobial activities over the tested bacterium were observed for Xanthomonas campestris (33.0 mm, and lower activities were obtained for Yersinia enterocolitica (10.5 mm. For the minimal inhibition concentration (MIC, it was observed that all microorganisms presented susceptibility to the Ho-Sho essential oil. For Gram-positive bacteria, the MIC varied from 1.00 mg.mL-1 (Streptococcus mutans to 1.75 mg.mL-1 (Staphylococcus epidermidis. In the case of Gram-negative bacteria, the MIC was 0.625 mg.mL-1 for Citrobacter freundii and 2.50 mg.mL-1 for Shigella flexneri. The results related to antioxidant activities demonstrated that the antioxidant percentage increases proportionally to the concentration of the essential oil added reaching the maximum value of 97.49% for the essential oil concentration of 50000 μg.mL-1.

AGN UNIFICATION AT z ∼ 1: u - R COLORS AND GRADIENTS IN X-RAY AGN HOSTS

International Nuclear Information System (INIS)

Mark Ammons, S.; Rosario, David J. V.; Koo, David C.

2011-01-01

We present uncontaminated rest-frame u - R colors of 78 X-ray-selected active galactic nucleus (AGN) hosts at 0.5 1.1 kpc. These three observations imply that AGN obscuration is uncorrelated with the star formation rate beyond ∼1 kpc. These observations favor a unification scenario for intermediate-luminosity AGNs in which obscuration is determined geometrically. Scenarios in which the majority of intermediate-luminosity AGNs at z ∼ 1 are undergoing rapid, galaxy-wide quenching due to AGN-driven feedback processes are disfavored.

Passado, presente e futuro dos princípios contábeis norte-americanos - US GAAP Lições para contabilidade brasileira

Directory of Open Access Journals (Sweden)

João Henrique Pederiva

2009-10-01

Full Text Available Como se estruturam as normas contábeis adotadas para registrar as atividades econômicas norte-americanas - United States Generally Accepted Accounting Principles - US GAAP (Princípios Contábeis Geralmente Aceitos Norte Americanos, quais os seus principais eixos de desenvolvimento doutrinário e que interesse há nesse conhecimento para a contabilidade brasileira? A relevância de obter respostas a esses questionamentos resulta da importância econômica dos Estados Unidos da America para as demais nações. Afinal, os recentes problemas nos mercados de capitais norte-americanos comprometeram, em dois anos e meio, US$ 7,7 trilhões da poupança destinada a aposentadoria dos trabalhadores daquele país. Atente-se que muitos países, inclusive o Brasil, buscam recursos nesses mercados de capitais.

PIBID – PRIMORDIAL PARA A FORMAÇÃO DE PROFESSORES

Directory of Open Access Journals (Sweden)

Rafael Dias Rios de Souza

2016-12-01

Full Text Available Resumo - Realizamos nesse artigo, reflexões necessárias para as compreensões e os significados relativos ao Programa de Bolsa de Iniciação à Docência (PIBID, cujo objetivo é o de contribuir de maneira significativa para a formação inicial de professores de História. Constatamos que esse programa é compreendido como um espaço que possibilita a integração entre universidade-escola, oportunizando aos futuros professores, o entendimento e a análise sobre a profissão docente e a realidade escolar. Isso ocorre por meio do desenvolvimento de temáticas que priorizam a inserção de diferentes materiais e abordagens didáticas no ensino de história, visando a renovação nesse campo do conhecimento.

Age-related changes of structures in cerebellar cortex of cat

Indian Academy of Sciences (India)

Madhu

ness of the cerebellar cortex as well as loss of neurons, and hypertrophy and ... Purkinje cells. (PCs) in old cats showed much fewer NF-IR dendrites than those in young adults. ... diminution in motor control and motor learning) underlying.

Levantamento dos métodos de análise de hemoglobina glicada utilizados em laboratórios da Serra Gaúcha = Survey on methods of analysis of glicated hemoglobin used by laboratories from Serra Gaúcha

Directory of Open Access Journals (Sweden)

Panarotto, Daniel

2005-01-01

Conclusões: A maioria dos laboratórios não utiliza métodos certificados pela NGSP. Nesses casos, os resultados não podem ser diretamente relacionados com os do estudo Diabetes Control and Complications Trial (DCCT

BAT AGN Spectroscopic Survey. VIII. Type 1 AGN with Massive Absorbing Columns

Science.gov (United States)

Shimizu, T. Taro; Davies, Richard I.; Koss, Michael; Ricci, Claudio; Lamperti, Isabella; Oh, Kyuseok; Schawinski, Kevin; Trakhtenbrot, Benny; Burtscher, Leonard; Genzel, Reinhard; Lin, Ming-yi; Lutz, Dieter; Rosario, David; Sturm, Eckhard; Tacconi, Linda

2018-04-01

We explore the relationship between X-ray absorption and optical obscuration within the BAT AGN Spectroscopic Survey (BASS), which has been collecting and analyzing the optical and X-ray spectra for 641 hard X-ray selected (E > 14 keV) active galactic nuclei (AGNs). We use the deviation from a linear broad Hα-to-X-ray relationship as an estimate of the maximum optical obscuration toward the broad line region (BLR) and compare the A V to the hydrogen column densities ({N}{{H}}) found through systematic modeling of their X-ray spectra. We find that the inferred columns implied by A V toward the BLR are often orders of magnitude less than the columns measured toward the X-ray emitting region, indicating a small-scale origin for the X-ray absorbing gas. After removing 30% of Sy 1.9s that potentially have been misclassified due to outflows, we find that 86% (164/190) of the Type 1 population (Sy 1–1.9) are X-ray unabsorbed as expected based on a single obscuring structure. However, 14% (26/190), of which 70% (18/26) are classified as Sy 1.9, are X-ray absorbed, suggesting that the BLR itself is providing extra obscuration toward the X-ray corona. The fraction of X-ray absorbed Type 1 AGNs remains relatively constant with AGN luminosity and Eddington ratio, indicating a stable BLR covering fraction.

Intentional intravenous mercury injection

African Journals Online (AJOL)

In this case report, intravenous complications, treatment strategies and possible ... Mercury toxicity is commonly associated with vapour inhalation or oral ingestion, for which there exist definite treatment options. Intravenous mercury ... personality, anxiousness, irritability, insomnia, depression and drowsi- ness.[1] However ...

Modelling traffic congestion using queuing networks

Indian Academy of Sciences (India)

Flow-density curves; uninterrupted traffic; Jackson networks. ... ness - also suffer from a big handicap vis-a-vis the Indian scenario: most of these models do .... more well-known queuing network models and onsite data, a more exact Road Cell ...

High energy asymptotics of the scattering amplitude for the ...

Indian Academy of Sciences (India)

R. Narasimhan (Krishtel eMaging) 1461 1996 Oct 15 13:05:22

Keywords. Scattering matrix; asymptotic expansion; high energy; diagonal singula- ..... (see subsection 2 of § 3) with functions of the generator of dilations. A = 1. 2 d ..... ness in quantum scattering theory, Ann. Inst. Henri Poincaré, Phys. Théor.

East African Medical Journal

African Journals Online (AJOL)

REpORTINg ON MENTAl HEAlTH IllNESS (MHI) IN KENyA: HOw wEll ARE. wE dOINg? ... fundamental for evidence-based decision-making and improved service ... Owiti, MBChB, MSc, Academic Model for Prevention and Treatment of HIV ...

The logic of logistics: theory, algorithms and applications for logistics management

Directory of Open Access Journals (Sweden)

Claudio Barbieri da Cunha

2010-04-01

Full Text Available

Nesse texto o autor apresenta uma resenha acerca do livro "The logic of logistics: theory, algorithms and applications for logistics management", de autoria de Julien Bramel e David Simchi-Levi, publicado pela Springer-Verlag, em 1997.

Numerical simulation model of multijunction solar cell

NARCIS (Netherlands)

Babar, M.; Al-Ammar, E.A.; Malik, N.H.

2012-01-01

Multi-junction solar cells play an important and significant role in the Concentrated Photovoltaic (CPV) Systems. Recent developments in Concentrated Photovoltaic concerning high power production and cost effective- ness along with better efficiency are due to the advancements in multi-junction

Surface morphology, structural and electrical properties of RF ...

Indian Academy of Sciences (India)

2018-05-19

May 19, 2018 ... ITO thin films; sputtering; structure; electrical properties; AFM; Hall effect. 1. Introduction ... ness range (61–768 nm) and to see if this system present properties that .... using the Bragg equation, and the relation linking the inter-.

Kronisk pancreatitis og øvre gastrointestinal blødning

DEFF Research Database (Denmark)

Larsen, H C; Bak, Martin

1995-01-01

A 46 year-old woman with a history of chronic pancreatitis, upper epigastric pain and upper gastrointestinal bleeding of obscure origin is presented. A haemoductal pancreatitis was the source of bleeding due to erosion of the splenic artery with bleeding into a pancreatic pseudocyst communicating...... with the pancreatic duct. This case was special, because there was no aneurysmal dilatation of the splenic artery. This rare entity must always be considered in the diagnosis of gastrointestinal haemorrhage of obscure origin. The appropriate investigation to confirm the diagnosis is visceral angiography, if necessary...

Fibroma cardíaco mimetizando cardiomiopatia hipertrófica Cardiac fibroma mimicking hypertrophic cardiomyopathy

Directory of Open Access Journals (Sweden)

Luís Alberto Dallan

1989-12-01

Full Text Available É relatado o caso de paciente com queixa de dor precordial, dispnéia e arritmia desde a adolescência, tratada clinicamente por mais de 10 anos. Nesse período, foi submetida a inúmeros exames ângio e ecocardiográficos, com suspeita inicial de endomiocardiofibrose e, posteriormente, de cardiomiopatia hipertrófica de ventrículo esquerdo. Como houve piora progressiva da sintomatologia e ausência de resposta à medicação, foi encaminhada ao nosso Serviço, onde se diagnosticou fibroma de ventrículo esquerdo. Foi submetida, com sucesso, à ressecção cirúrgica do tumor, sendo realizada reconstrução geométrica do ventrículo esquerdo. Apresenta boa evolução, decorridos dois anos, com remissão completa dos sintomas. Destacamos a dificuldade no diagnóstico diferencial desses tumores benignos e de crescimento lento, com as cardiomiopatias hipertróficas do ventrículo esquerdo.A 33 year-old woman was seen, for the first time, ten years ago, for evaluation of a recurrent chest pain, dyspnea and arrhythmia. She was submitted to echocardiographic studies and a cardiac catheterization. The diagnoses was endomyocardial fibrosis at first, and hypertrophic cardiomyopathy after. Despite treatment with propranolol and quinidine, the episodes of dyspnea and tachyarrhythmias became more frequent and severe, and the patient was guided to our Service. Cardiac re-catheterization, echocardiographic and computed tomography studies identified in traumural cardiac fibroma and the patient was referred for surgical treatment. The cardiac fibroma was successfully resected on extracorporeal bypass and with cardioplegic arrest of the heart. Repair of the heart was accomplished with a patch placed to close the left ventricular cavity. The postoperative course was uncomplicated, and she remains assymptomatic two years later. We have emphazied tha this tumor often produces clinically obscure disease, simulating particularly the left ventricle hypertrophic

When Whole(ness is more than the Sum of the Parts: somatics as contemporary epistemological field

Directory of Open Access Journals (Sweden)

Ciane

2014-12-01

Full Text Available In the text, it is discussed some aspects on somatics in contemporary times, from the starting point of its technical and conceptual basis, clarifying premises and applications, as well as misunderstandings and restrictions. Some aspects include: conceptual, historical, and technical origins; common premises and principles developed by diverse somatic techniques; the difference between somatic technique, method, and approach; transculturality, decolonization, and repatterning; Somatic Attunement and Wisdom; institutionalization in technical and/or academic courses; somatics as autonomous field of therapy, education, aesthetics, and research; somatics as practice as research; somatic-performative research.

Welcome to the Largest International Fair of the Balkans: The Borderli-ness of Kara Boaz Fair

Directory of Open Access Journals (Sweden)

S. Antova

2015-08-01

Full Text Available The location of this study is the border area of the North – West Bulgaria at Bulgarian – Serbian border, near the town of Belogradchik. As a result of several times redrawing of nation state borders between Serbia (Yugoslavia and Bulgaria during 20th century the borderland population, named Torlatsi had been separated. The Kada Boaz Fair creates a safe space and time for meeting of the separated families and friends, living at the both sides of the border. Very significant point is that the place of the Kada Boaz Fair is widely exploited of all local and governmental authorities from both sides since 2000 as a place to re-construct economic and social relations. The aim of the paper is to discuss which are the factors influencing the real openness and the making borders pervious. The paper explores the border crossing of Bulgarian and Serbian population, living at both sides of national borders on an everyday level, while trying to explain its notions in different periods of time (Socialist past, Yugo-embargo, EU accession of Bulgaria. The presentation answers the question how people use the political situations and politicians so that they could benefit from certain circumstances on their everyday level of life.

Proving the correctness of client/server software

Indian Academy of Sciences (India)

ness of an OSEKtime (OSE 2001) like distributed real time operating system and all ... kernel but concentrate on the security-sensitive services running on top of it. This multi- ...... in case of a call to a procedure other than MUL send denial. (16).

Journal of Special Operations Medicine, Volume 7, Edition 3

Science.gov (United States)

2007-01-01

to evidence- based practice in the hospital environment initiated more analysis of the cost-benefit relationship of the early uti - lization of these...for reasons of acute ill- ness, recent surgery, pregnancy , immunosuppressive therapy, human immunodeficiency virus (HIV) infection or another chronic

Naturalness and image quality: Chroma and hue variation in color images of natural scenes

NARCIS (Netherlands)

Ridder, de H.; Blommaert, F.J.J.; Fedorovskaya, E.A.; Eschbach, R.; Braun, K.

1997-01-01

The relation between perceptual image quality and natural ness was investigated by varying the colorfulness and hue of color images of natural scenes. These variations were created by digitizing the images, subsequently determining their color point distributions in the CIELUV color space and

Fulltext PDF

Indian Academy of Sciences (India)

Madhu

greater forward tilt needed to get going. Turning ... ness of mass to accelerate; the force of surface tension from .... lar field in which the ratio first found use–which force carried ...... energy to sustain the process comes from the steady loss of.

Walking through clouds and rains

Indian Academy of Sciences (India)

Lawrence

with particular reference to human psychology. He was the chief ... record, I pursued the studies for M.Sc. in Physics at the University of Pune. My father's ... ness in the area of Meteorology has grown tremendously in recent years. At present ...

Co-occurring Conditions Toolkit: Mild Traumatic Brain Injury and Psychological Health

Science.gov (United States)

2009-01-01

diarrhea, vomit- ing, abdominal pain, polyuria and polydipsia yy Normal fluid and salt intake must be maintained during therapy yy Half life...weak- ness, tremor, headache, hand tremor, nausea, diarrhea, vomit- ing, abdominal pain, polyuria and polydipsia yy Normal fluid and salt intake

A case study of the sensitivity of forecast skill to data and data analysis techniques

Science.gov (United States)

Baker, W. E.; Atlas, R.; Halem, M.; Susskind, J.

1983-01-01

A series of experiments have been conducted to examine the sensitivity of forecast skill to various data and data analysis techniques for the 0000 GMT case of January 21, 1979. These include the individual components of the FGGE observing system, the temperatures obtained with different satellite retrieval methods, and the method of vertical interpolation between the mandatory pressure analysis levels and the model sigma levels. It is found that NESS TIROS-N infrared retrievals seriously degrade a rawinsonde-only analysis over land, resulting in a poorer forecast over North America. Less degradation in the 72-hr forecast skill at sea level and some improvement at 500 mb is noted, relative to the control with TIROS-N retrievals produced with a physical inversion method which utilizes a 6-hr forecast first guess. NESS VTPR oceanic retrievals lead to an improved forecast over North America when added to the control.

REFLEXÕES E DESCOBERTAS NA PAISAGEM DE CEMITÉRIOS URBANOS: UM OLHAR ENTRE MUROS EM CEMITÉRIOS DE JOÃO PESSOA-PB

Directory of Open Access Journals (Sweden)

Kátia Maria Santos de Andrade Pizzol

2011-04-01

Full Text Available RESUMO A arte funerária reflete a necessidade do homem eternizar sua presença, registrar sua importância na sociedade. Assim, objetiva-se nesse estudo a compreensão da paisagem cemiterial, que reflete a sociedade, a história, a cultura e revela o simbolismo que envolve a representação arquitetônica dos túmulos. Dessa forma estudou-se a forma e a simbologia presentes em dois cemitérios da cidade de João Pessoa. E pode-se verificar que refletem muitos valores do cotidiano das pessoas na forma de encarar a morte. Nesse passeio intramuros encontram-se disputas, segregações, valores que refletem o urbano nessa paisagem silenciosa que muito nos fala, revela encontros, lembranças, atitudes e expressões desse universo intrigante da imortalidade. Palavras chaves: Paisagem, morfologia e representação.

Entre donos e guardiões: a natureza como propriedade particular

Directory of Open Access Journals (Sweden)

Luciana Braga Silveira

2010-01-01

Full Text Available Este paper trata das relações sociais estruturadas no âmbito das Reservas Particulares do Patrimônio Natural (RPPNs, áreas naturais protegidas pela legislação ambiental que podem ser institucionalizadas em domínios privados. Emerge, nesse contexto, uma nova identidade social, o "RPPNista", aquele que além de deter a propriedade privada do espaço natural ainda recebe e se autoatribui o direito e o dever de zelar por sua proteção. Através de articulações, acordos, dissensos, produzidos nesse campo de relações, constitui-se a "comunidade RPPNista". Pretende-se refletir aqui sobre o "campo de possibilidades" a partir do qual se estruturam os projetos dos RPPNistas e sobre como, ao instituir tal comunidade de sentidos, esses sujeitos reconfiguram a si mesmos, enquanto constroem simbolicamente a natureza apropriada como reserva particular.

Reapresentação

Directory of Open Access Journals (Sweden)

Ulpiano Toledo Bezerra de Meneses

1983-06-01

Full Text Available (primeiro parágrafo do texto Fruto da iniciativa, do entusiasmo e da permanente dedicação do Professor Eurípedes Simões de Paula, a Revista de História, iniciada em 1950, foi por ele dirigida até sua inesperada morte, em novembro de 1977. Tendo atingido, nesses vinte e sete anos, com uma espantosa freqüência bimestral, cento e doze números, tornou-se, sem dúvida, a mais notória publicação nesse campo, no Brasil.  Com a doação da Revista ao Departamento de História da Faculdade de Filosofia, Letras e Ciências Humanas da Universidade de São Paulo, pelos herdeiros e segundo as intenções de seu fundador, entra ela em nova fase, após quase cinco anos de interrupção.

Two methods to measure granular gas temperature

Science.gov (United States)

Chastaing, J.-Y.; Géminard, J.-C.; Naert, A.

2017-07-01

Grains are vibrated so as to achieve a granular gas, here regarded as an archetype of a dissipative non equilibrium steady state (NESS). We report on two distinct and concordant experimental measures of the system effective temperature. To do so, a blade fastened to the shaft of a small DC-motor, immersed in the grains, behaves as a driven 1D Brownian rotator, which is used as both actuator and sensor simultaneously. On the one hand, the Gallavotti-Cohen fluctuation theorem, which involves a measure of the asymmetry of the energy exchanges between the rotator and the NESS reservoir, provides a first effective temperature. On the other hand, the fluctuation-dissipation theorem, which involves the relation between the spontaneous fluctuations and the response to a weak perturbation, defines a second, independent, effective temperature. Both methods, even though they are based on drastically different ideas, give nicely concordant results.

Methodological aspects of measuring injuries from traffic accidents at the site of occurrence

Directory of Open Access Journals (Sweden)

Martha C. Híjar-Medina

Full Text Available Os acidentes de trânsito de veículos a motor representam problema de saúde pública, em nível mundial. No México, a pesquisa, nesse campo, é limitada e a metodologia para seu estudo é pouco desenvolvida. Na literatura científica internacional são escassos os artigos que discutem os aspectos metodológicos de pesquisa nesse campo. Assim, realizou-se estudo com o objetivo de apresentar alguns aspectos metodológicos úteis para os interessados em pesquisar lesões por acidentes de trânsito. Foram discutidos aspectos sobre como medir, no local de ocorrência, as variáveis básicas para o estudo dessas lesões, tais como: se o motorista sofreu ou não lesões, uso de cinto de segurança, velocidade e consumo de álcool.

Aspectos metodologicos de la medición en el sitio de ocurrencia de lesiones por accidentes de tráfico

Directory of Open Access Journals (Sweden)

Híjar-Medina Martha C.

1997-01-01

Full Text Available Os acidentes de trânsito de veículos a motor representam problema de saúde pública, em nível mundial. No México, a pesquisa, nesse campo, é limitada e a metodologia para seu estudo é pouco desenvolvida. Na literatura científica internacional são escassos os artigos que discutem os aspectos metodológicos de pesquisa nesse campo. Assim, realizou-se estudo com o objetivo de apresentar alguns aspectos metodológicos úteis para os interessados em pesquisar lesões por acidentes de trânsito. Foram discutidos aspectos sobre como medir, no local de ocorrência, as variáveis básicas para o estudo dessas lesões, tais como: se o motorista sofreu ou não lesões, uso de cinto de segurança, velocidade e consumo de álcool.

ISOTROPIC LUMINOSITY INDICATORS IN A COMPLETE AGN SAMPLE

International Nuclear Information System (INIS)

Diamond-Stanic, Aleksandar M.; Rieke, George H.; Rigby, Jane R.

2009-01-01

The [O IV] λ25.89 μm line has been shown to be an accurate indicator of active galactic nucleus (AGN) intrinsic luminosity in that it correlates well with hard (10-200 keV) X-ray emission. We present measurements of [O IV] for 89 Seyfert galaxies from the unbiased revised Shapley-Ames (RSA) sample. The [O IV] luminosity distributions of obscured and unobscured Seyferts are indistinguishable, indicating that their intrinsic AGN luminosities are quite similar and that the RSA sample is well suited for tests of the unified model. In addition, we analyze several commonly used proxies for AGN luminosity, including [O III] λ5007 A, 6 cm radio, and 2-10 keV X-ray emission. We find that the radio luminosity distributions of obscured and unobscured AGNs show no significant difference, indicating that radio luminosity is a useful isotropic luminosity indicator. However, the observed [O III] and 2-10 keV luminosities are systematically smaller for obscured Seyferts, indicating that they are not emitted isotropically.

An Archival Chandra and XMM-Newton Survey of Type 2 Quasars

Science.gov (United States)

Jia, Jianjun; Ptak, Andrew Francis; Heckman, Timothy; Zakamska, Nadia L.

2013-01-01

In order to investigate obscuration in high-luminosity type 2 active galactic nuclei (AGNs), we analyzed Chandra and XMM-Newton archival observations for 71 type 2 quasars detected at 0.05 100 eV in the rest frame) and we detect this line in the other sources through a joint fit (spectral stacking). The correlation between the Fe K alpha and [O III] fluxes and the inverse correlation of the equivalent width of the Fe Ka line with the ratio of hard X-ray and [O III] fluxes is consistent with previous results for lower luminosity Seyfert 2 galaxies. We conclude that obscuration is the cause of the weak hard X-ray emission rather than intrinsically low X-ray luminosities. We find that about half of the population of optically selected type 2 quasars are likely to be Compton thick. We also find no evidence that the amount of X-ray obscuration depends on the AGN luminosity (over a range of more than three orders of magnitude in luminosity).

Genetically engineered monogamy in voles lends credence to the ...

Indian Academy of Sciences (India)

Administrator

ness benefits to the worker bee who rears sisters related to her by 0.75 instead of ... ing to selectively destroy the koels' eggs without destroying her own? What are the ... montane vole males, and most attention has been focused on a class of ...

Conflito em Darfur: das motivações internas à reação internacional

Directory of Open Access Journals (Sweden)

Evandro Farid Zago

2010-10-01

Full Text Available Desde 2003 se estende na região sudanesa de Dafur um intenso conflito, tido como um dos mais sangrentos do continente africano. Nesse sentido este artigo busca explicar as questões internacionais e os constrangimentos locais que envolvem tal conflito.

Model Checking Process Algebra of Communicating Resources for Real-time Systems

DEFF Research Database (Denmark)

Boudjadar, Jalil; Kim, Jin Hyun; Larsen, Kim Guldstrand

2014-01-01

This paper presents a new process algebra, called PACOR, for real-time systems which deals with resource constrained timed behavior as an improved version of the ACSR algebra. We define PACOR as a Process Algebra of Communicating Resources which allows to express preemptiveness, urgent ness...

Conversational Flow Promotes Solidarity

NARCIS (Netherlands)

Koudenburg, Namkje; Postmes, Tom; Gordijn, Ernestine H.

2013-01-01

Social interaction is fundamental to the development of various aspects of "we-ness''. Previous research has focused on the role the content of interaction plays in establishing feelings of unity, belongingness and shared reality (a cluster of variables referred to as solidarity here). The present

Adaptation of eight American blackberry ( Rubus fructicosus L ...

African Journals Online (AJOL)

evaluate the performance of Arapaho, Black Satin, Cherokee, Chester Thornless, Dirksen Thornless, Jumbo, Navaho and Loch Ness cultivars of American origin for adaptation under Central Anatolian conditions at Ankara during 2002 - 06. The results showed that changes in the environmental conditions affected yield, ...

Travelling wave solutions to the K-P-P equation at supercritical wave speeds: a parallel to Simon Harris' probabilistic analysis

NARCIS (Netherlands)

Kyprianou, A.E.

2000-01-01

Recently Harris using probabilistic methods alone has given new proofs for the known existence asymptotics and unique ness of travelling wave solutions to the KPP equation Following in this vein we outline alternative probabilistic proofs for wave speeds exceeding the critical minimal wave speed

Soil seed banks in plant invasions: promoting species invasiveness and long-term impakt on plant community dynamics

Czech Academy of Sciences Publication Activity Database

Gioria, M.; Pyšek, Petr; Moravcová, Lenka

2012-01-01

Roč. 84, č. 2 (2012), s. 327-350 ISSN 0032-7786 R&D Projects: GA ČR GA206/09/0563 Institutional support: RVO:67985939 Keywords : soil seed bank * plant invasions * species invasive ness Subject RIV: EF - Botanics Impact factor: 2.833, year: 2012

Lytic phages obscure the cost of antibiotic resistance in Escherichia coli.

Science.gov (United States)

Tazzyman, Samuel J; Hall, Alex R

2015-03-17

The long-term persistence of antibiotic-resistant bacteria depends on their fitness relative to other genotypes in the absence of drugs. Outside the laboratory, viruses that parasitize bacteria (phages) are ubiquitous, but costs of antibiotic resistance are typically studied in phage-free experimental conditions. We used a mathematical model and experiments with Escherichia coli to show that lytic phages strongly affect the incidence of antibiotic resistance in drug-free conditions. Under phage parasitism, the likelihood that antibiotic-resistant genetic backgrounds spread depends on their initial frequency, mutation rate and intrinsic growth rate relative to drug-susceptible genotypes, because these parameters determine relative rates of phage-resistance evolution on different genetic backgrounds. Moreover, the average cost of antibiotic resistance in terms of intrinsic growth in the antibiotic-free experimental environment was small relative to the benefits of an increased mutation rate in the presence of phages. This is consistent with our theoretical work indicating that, under phage selection, typical costs of antibiotic resistance can be outweighed by realistic increases in mutability if drug resistance and hypermutability are genetically linked, as is frequently observed in clinical isolates. This suggests the long-term distribution of antibiotic resistance depends on the relative rates at which different lineages adapt to other types of selection, which in the case of phage parasitism is probably extremely common, as well as costs of resistance inferred by classical in vitro methods.

Pulmonary vasculitis may obscure large cell lung carcinoma. A case report

NARCIS (Netherlands)

Kreeftenberg, HG; Ligtenberg, JJM; van der Werf, TS; Timens, W; Tervaert, JWC

2001-01-01

Several vasculitic syndromes are recognized as paraneoplastic symdromes of an underlying malignant disease. Most frequently small vessel vasculitis of the skin has been reported. We describe the case of a 62-year-old man with a pulmonary mass due to pulmonary vasculitis. After resection of the

Nuclear warning: the dangerous obscure arguments. Is the History repeating again?

International Nuclear Information System (INIS)

Zylbersztajn, D.; Bernini, E.J.

1993-01-01

Some considerations about the continuity of Angra-2 Nuclear Power Plant building are presented, with a warning by the authors to the environment and human dangers involved. The real cost and investments for nuclear power in Brazil are also described. (C.G.C.)

Disclosing or obscuring? The politics of transparency in global climate governance

NARCIS (Netherlands)

Gupta, Aarti; Mason, Michael

2016-01-01

Transparency is increasingly evoked within public and private climate governance arrangements as a key means to enhance accountability and improve environmental outcomes. We review assumed links between transparency, accountability and environmental sustainability here, by identifying four

Diagenesis of lower Cretaceous pelagic carbonates, North Atlantic: Paleoceanographic signals obscured

Science.gov (United States)

Frank, T.D.; Arthur, M.A.; Dean, W.E.

1999-01-01

The stable isotope and minor element geochemistry of Neocomian (Lower Cretaceous) pelagic carbonates of the North Atlantic Basin (Deep Sea Drilling Project Sites 105, 367, 387, 391, and 603) was examined to develop a diagenetic model for pelagic limestones. In particular, we hoped to test the fidelity of whole-rock geochemical records as paleoceanographic indicators for pelagic deposits of pre-Aptian age, in which individual microfossils are not available for analysis. Data indicate that in addition to depth of burial, rhythmic variations in primary carbonate content have strongly controlled diagenetic patterns and associated geochemical signatures in these Neocomian sequences. Samples become increasingly depleted in Sr and 18O with increasing CaCO3 content. Within individual sedimentary sections, substantial decreases in Sr/Ca ratios and ??18O values are evident over a range of 4 to 98% CaCO3. However, even over a relatively narrow range of 50 to 98% CaCO3 a 2.5%c variation in ??18O values and a change of a factor of 1.7 in Sr/Ca ratios are observed. Carbon isotope compositions do not vary as extensively with CaCO3 content, but carbonate-rich intervals tend to be relatively depleted in 13C. Petrographic analysis reveals that these geochemical patterns are related to the transfer of CaCO3 from carbonate-poor intervals (calcareous shales and marlstones) to adjacent carbonate-rich intervals (limestones) during burial compaction and pressure solution. This process results in the addition of diagenetic cement to carbonate-rich intervals to produce a bulk composition that is relatively depleted in Sr and 18O and, at the same time, enables the retention of more-or-less primary carbonate that is relatively enriched in Sr and 18O in adjacent carbonate-poor intervals. Thus, although cyclic variations in CaCO3 content are primary in the Neocomian sequences examined, measured variations in Sr/Ca ratios and ??18O values are not and, as such, do not provide reliable proxies for past variations in climate, oceanographic conditions, or global ice volume.

Proceedings of the 1987 Scientific Conference on Obscuration and Aerosol Research

Science.gov (United States)

1988-10-01

can do this because of the orthogonality reliLionships, 2fr ffA (m, )(O,6)*’B(m,,)(O,O)ain(O)d~dO = 0 (2.23) 00 and A(.,.O)C(m,n) = 0 = B(mk).C(m,n... bPp ) ]( P )Z’l (r)A ( )+ a4P) 1.. (rZ &u:p(r))B (~~~~ 𔃻’(I (n + (-kA1P 18 +a’I • r nk #.Pn) Z’ (r)A )(9,€) + a (r ))B (O,9)S-- p ),= ) n.pn (m , O) C

Anesthetic concerns in a huge congenital sublingual swelling obscuring airway access

Directory of Open Access Journals (Sweden)

Nilesh Kumar

2015-01-01

Full Text Available Presence of intraoral pathology poses a great challenge during management of pediatric airway. We report management of big intraoral cystic swelling physically occupying the entire oral cavity restricting access to airway. Preintubation aspiration of swelling was done to decrease its size and make room for airway manipulation, followed by laryngoscopy and intubation in lateral position. Airway patency is at risk in postoperative period also, in this case, though the swelling decreased in size postoperatively but presence of significant edema required placement of tongue stitch and modified nasopharyngeal airway. Case report highlights simple maneuvers to manage a difficult case.

Extracting foreground-obscured μ-distortion anisotropies to constrain primordial non-Gaussianity

Science.gov (United States)

Remazeilles, M.; Chluba, J.

2018-04-01

Correlations between cosmic microwave background (CMB) temperature, polarization and spectral distortion anisotropies can be used as a probe of primordial non-Gaussianity. Here, we perform a reconstruction of μ-distortion anisotropies in the presence of Galactic and extragalactic foregrounds, applying the so-called Constrained ILC component separation method to simulations of proposed CMB space missions (PIXIE, LiteBIRD, CORE, PICO). Our sky simulations include Galactic dust, Galactic synchrotron, Galactic free-free, thermal Sunyaev-Zeldovich effect, as well as primary CMB temperature and μ-distortion anisotropies, the latter being added as correlated field. The Constrained ILC method allows us to null the CMB temperature anisotropies in the reconstructed μ-map (and vice versa), in addition to mitigating the contaminations from astrophysical foregrounds and instrumental noise. We compute the cross-power spectrum between the reconstructed (CMB-free) μ-distortion map and the (μ-free) CMB temperature map, after foreground removal and component separation. Since the cross-power spectrum is proportional to the primordial non-Gaussianity parameter, fNL, on scales k˜eq 740 Mpc^{-1}, this allows us to derive fNL-detection limits for the aforementioned future CMB experiments. Our analysis shows that foregrounds degrade the theoretical detection limits (based mostly on instrumental noise) by more than one order of magnitude, with PICO standing the best chance at placing upper limits on scale-dependent non-Gaussianity. We also discuss the dependence of the constraints on the channel sensitivities and chosen bands. Like for B-mode polarization measurements, extended coverage at frequencies ν ≲ 40 GHz and ν ≳ 400 GHz provides more leverage than increased channel sensitivity.

Proceedings of the 1998 Scientific Conference on Obscuration and Aerosol Research

National Research Council Canada - National Science Library

Coverstone, Amy

1999-01-01

...: Aerosol Particle Generation and Dynamics, Aerosol Characterization Methods-Aerosol Samplers and Collectors, Preparing, Aerosolizing and Characterizing Erwinia Herbicola, and Optical Properties of Aerosols...

Method for the detection of flaws in a tube proximate a contiguous member

International Nuclear Information System (INIS)

Holt, A.E.; Wehrmeister, A.E.; Whaley, H.L.

1979-01-01

A method for deriving the eddy current signature of a flaw in a tube proximate a contiguous member which is obscured in a composite signature of the flaw and contiguous member comprises subtracting from the composite signature a reference eddy current signature generated by scanning a reference or facsimile tube and contiguous member. The method is particularly applicable to detecting flaws in the tubes of heat exchangers of fossil fuel and nuclear power plants to enable the detection of flaws which would otherwise be obscured by contiguous members such as support plates supporting the tubes. (U.K.)

AGN Clustering in the BAT Sample

Science.gov (United States)

Powell, Meredith; Cappelluti, Nico; Urry, Meg; Koss, Michael; BASS Team

2018-01-01

We characterize the environments of local growing supermassive black holes by measuring the clustering of AGN in the Swift-BAT Spectroscopic Survey (BASS). With 548 AGN in the redshift range 0.012MASS galaxies, we constrain the halo occupation distribution (HOD) of the full sample with unprecedented sensitivity, as well as in bins of obscuration with matched luminosity distributions. In doing so, we find that AGN tend to reside in galaxy groups, agreeing with previous studies of AGN throughout a large range of luminosity and redshift. We also find evidence that obscured AGN tend to reside in denser environments than unobscured AGN.

AMANTADINE HYDROCHWRIDE IN THE TREATMENT OF ...

African Journals Online (AJOL)

1971-04-17

Apr 17, 1971 ... seemed beneficial. Side-effects occurred in 22% of patients and consisted of restlessness. insomnia, abdominal uneasiness, dizzi- ness, depression, confusion and, in a few cases, hallucinations. In most cases side-effects were controlled by reducing the dose of amantadine or of concomitant medication.

Assessing business proposals: genre conventions and audience response in document design

NARCIS (Netherlands)

Lagerwerf, L.; Bossers, Ellis

2002-01-01

We carried out two studies in which several genre conventions were tested on professional readers to verify the usefulness of applying genre conventions to business proposals. In the first study, 39 male business clients of the company IBM Netherlands compared an authentic busi ness proposal with a

Unigene BLAST: CBRC-HSAP-07-0070 [SEVENS

Lifescience Database Archive (English)

Full Text Available CBRC-HSAP-07-0070 gnl|UG|Hs#S1730883 Homo sapiens opsin 1 (cone pigments), short-wave-sensitive (color blind...ness, tritan) (OPN1SW), mRNA /cds=p(8,1054) /gb=NM_001708 /gi=4502386 /ug=Hs.656404 /len=1101 0.0 100% ...

The public choice of university organization.A stylized story of a constitutional reform

DEFF Research Database (Denmark)

Paldam, Martin

checks and balances. It was meant as a more business-like system to increasing effective-ness. However, the result has been precisely the reverse. Both the (relative) size and the salaries of the bureaucracy have increased, while its effectiveness has fallen. The bureaucracy has grown particularly fast...

The public choice of university organzation

DEFF Research Database (Denmark)

Paldam, Martin

2015-01-01

checks and balances. It was meant as a more business-like system to increasing effective-ness. However, the result has been precisely the reverse. Both the (relative) size and the salaries of the bureaucracy have increased, while its effectiveness has fallen. The bureaucracy has grown particularly fast...

Squeeze film between porous rough elliptical plates | Deheri ...

African Journals Online (AJOL)

The roughness of the bearing surface is described by a stochastic random variable with non zero mean, variance and skew ness. The associated Reynolds' equation is solved with appropriate boundary conditions. Results for bearing performance characteristics such as load carrying capacity and response time for different ...

Vodcasting space weather: The Space Weather FX vodcast series

Science.gov (United States)

Collins Petersen, C.; Erickson, P. J.

2008-06-01

The topic of space weather is the subject of a series of nine vodcasts (video podcasts) being created by MIT Haystack Observatory (Westford, Massachusetts, USA) and Loch Ness Productions (Groton, Massachusetts, USA). This paper describes the project, its science and outreach goals, and introduces the principal participants.

Human dignity and biomedical ethics from a Christian theological ...

African Journals Online (AJOL)

2011-07-11

Jul 11, 2011 ... Not only is there no Christian or humanistic idea of man. (because they do not .... ness which can be denied only at the cost of doing violence to the text. ... of an existential interpretation of the New Testament would not have to ...

Migraine Trainers as Models: the effectiveness of Lay trainerswith migraine for behavioural attack prevention

NARCIS (Netherlands)

S.Y.M. Mérelle (Saskia)

2008-01-01

textabstractMigraine is a chronic brain disorder, characterized by attacks of severe headache accompanied by nausea, vomiting and sensitivity to light, sound and smell. Attacks can be preceded by premonitory symptoms such as fatigue, muscular stiff ness or negative aff ect. It has been shown that

Materialidade e memória do Rio de Janeiro nas fotografias de Augusto Malta e do projeto Rio 365

Directory of Open Access Journals (Sweden)

Débora Gauziski

2013-12-01

Full Text Available Neste artigo investigamos a relação da fotografia com a produção e difusão de imagens da cidade do Rio de Janeiro em dois momentos distintos: durante a modernização de Pereira Passos (início do século XX e no Rio dos megaeventos (século XXI. Em ambos os períodos históricos, a cidade sofreu profundas transformações urbanísticas e a fotografia atua como importante agente nesse processo. Para analisar o papel que a fotografia tem nesse contexto, trabalhamos com as imagens clicadas pelo fotógrafo Augusto Malta e com aquelas produzidas por usuários do Instagram no contexto do projeto Rio 365. Ao longo do artigo, nossa base teórica concentra-se em autores que trabalham ou tangenciam as questões da memória e da materialidade.

A Consistência das Memórias da Infância

Directory of Open Access Journals (Sweden)

Maria Salomé Pinho

Full Text Available Resumo A coleta de relatos retrospetivos constitui um procedimento frequente em psicologia. Neste estudo, analisou-se, em uma amostra de adultos jovens não institucionalizados, a consistência desses relatos sobre diversas experiências da infância (vitimação, medos, dificuldades de aprendizagem, confrontando-os com os relatos atuais dos seus pais e/ou professores. Os resultados mostraram uma relação significativa entre os relatos retrospetivos dos próprios participantes e as informações atuais fornecidas pelas outras fontes, exceto para os medos na infância. A magnitude dessa relação variou entre pequena e média. Com base nesses resultados, sugere-se que, nos estudos que recorram a relatos retrospetivos e atuais, indiquem-se medidas de relação entre relatos, bem como a sua magnitude, de modo a melhor se avaliar a qualidade das inferências baseadas nesses relatos.

A polifonia de enunciadores nas cartas dos leitores: uma abordagem enunciativa = The polyphony enunciators in letters from readers: a stated approach

Directory of Open Access Journals (Sweden)

Silva, Telma Cristina Gomes da

2016-01-01

Full Text Available Este trabalho analisa o gênero discursivo carta do leitor à luz da Teoria da Argumentação na Língua desenvolvida por Anscombre, Ducrot (1977, 1987, 1988 e colaboradores para quem a língua e seus usos são fundamentalmente argumentativos. A análise incide sobre uma amostragem constituída por 03 cartas dos leitores recortadas de um corpus mais amplos coletado nas revistas Istoé e Veja entre janeiro e março de 2003. Nesse corpus, identificamos as marcas linguístico-discursivas ativadoras de pressuposto, considerando o dialogismo entre o locutor e os outros enunciadores (vozes sociais para a constituição da carta. Os resultados apontaram que a negação polêmica constitui um recurso linguístico produtor de sentido na carta do leitor, mostrando a polifonia de enunciadores como uma das principais estratégias argumentativas nesse gênero discursivo

Being me and being us in a family living close to death at home.

Science.gov (United States)

Carlander, Ida; Ternestedt, Britt-Marie; Sahlberg-Blom, Eva; Hellström, Ingrid; Sandberg, Jonas

2011-05-01

We used interpretive description to describe how everyday life close to death was experienced and dealt with in families with one member who had a life-threatening illness. We performed 28 individual, couple, and group interviews with five families. We found two patterns, namely, "being me in a family living close to death" and "being us in a family living close to death." "Being me" meant that every individual in the family had to deal with the impending death, regardless of whether or not he or she was the person with the life-threatening illness. This was linked to ways of promoting the individual's self-image, or "me-ness." This pattern was present at the same time as the pattern of "being us," or in other words, being a family, and dealing with impending death and a new "we-ness" as a group. "Striving for the optimal way of living close to death" was the core theme.

Identification of the nuclear export signals that regulate the intracellular localization of the mouse CMP-sialic acid synthetase

International Nuclear Information System (INIS)

Fujita, Akiko; Sato, Chihiro; Kitajima, Ken.

2007-01-01

The CMP-sialic acid synthetase (CSS) catalyzes the activation of sialic acid (Sia) to CMP-Sia which is a donor substrate of sialyltransferases. The vertebrate CSSs are usually localized in nucleus due to the nuclear localization signal (NLS) on the molecule. In this study, we first point out that a small, but significant population of the mouse CMP-sialic acid synthetase (mCSS) is also present in cytoplasm, though mostly in nucleus. As a mechanism for the localization in cytoplasm, we first identified two nuclear export signals (NESs) in mCSS, based on the localization studies of the potential NES-deleted mCSS mutants as well as the potential NES-tagged eGFP proteins. These two NESs are conserved among mammalian and fish CSSs, but not present in the bacterial or insect CSS. These results suggest that the intracellular localization of vertebrate CSSs is regulated by not only the NLS, but also the NES sequences

AS MÚLTIPLAS DIMENSÕES DO CURRÍCULO NO PROCESSO DE INCLUSÃO E EXCLUSÃO EM EDUCAÇÃO

Directory of Open Access Journals (Sweden)

Mônica Pereira dos Santos

2011-03-01

Full Text Available Pretendemos nesse ensaio estabelecer diálogos entre teorias curriculares e o processo de inclusão e exclusão em educação, sob a perspectiva dos estudos culturais. Usaremos uma estrutura explicativa que vem sendo elaborada desde o final dos anos 80 (BOOTH, 1981, referente à compreensão dos processos de inclusão/exclusão, que se manifestam por meio de três dimensões: a da criação de culturas, a do desenvolvimento de políticas e a da orquestração das práticas de inclusão/exclusão no interior das instituições e sistemas. Nesse trabalho procuraremos articular a relação entre currículo, cultura e poder com os processos de exclusão vinculados às barreiras à aprendizagem e à não-participação no processo de escolarização.

IMAGEM, MÍDIA E NOVAS TECNOLOGIAS – O DISCURSO DE VEJA EM AS CORES DA CRISE

Directory of Open Access Journals (Sweden)

Welisson Marques

2012-01-01

Full Text Available Esse artigo propõe discorrer sobre análise imagética nos discursos em geral, bem como no discurso midiático em especial, em face das novas tecnologias contemporâneas. A AD (isto é, Análise do Discurso a que nos referimos é aquela erigida por Michel Pêcheux. Nesse sentido, os conceitos de intericonicidade em Courtine e policromia em Souza são profícuas ferramentas teóricas para se analisar textos não-verbais. Tomamo-los como sustentáculo para a análise da matéria As Cores da Crise, publicada em Veja na época da suposta crise do mensalão. Nesse exercício, voltar-nos-emos para a constituição do sujeito ao se referir ao Partido dos Trabalhadores e como se dá essa relação, atentando-se para os elementos verbais e não-verbais materializados no corpus.

Relação família-escola: possibilidades e desafios para a construção de uma parceria DOI: http://dx.doi.org/10.15601/2237-0587/fd.v5n1p43-57

Directory of Open Access Journals (Sweden)

Camila Mendes Martins Tavares

2013-06-01

Full Text Available Esta pesquisa tem como objetivo principal analisar como família e escola podem construir uma parceria que possa beneficiar o aluno em seu processo de aprendizagem. Através de uma revisão bibliográfica, foram abordados temas como histórico dessa relação família e escola. Analisou-se, também, se ocorre inversão ou separação de funções educativas e propõe uma prática para que família e escola sejam parceiras nesse processo. Como contribuição na formação docente, pretendeu-se mostrar aos professores a grande diferença que podem fazer nesse processo. Com base na análise feita, é possível concluir que família e escola dependem uma da outra para obter êxito no processo educativo de cada aluno. 

A ponte mágica: como Luísa, aos 11 anos, cria sua primeira empresa para realizar o seu sonho, de Fernando Dolabela

Directory of Open Access Journals (Sweden)

Sérgio Lourenço Simões

2007-12-01

Full Text Available No atual cenário globalizado, as distanciasse estreitam e tornam os fatos onipresentes, numa sobreposição de ações que envolvem indivíduos em luta pela  sobrevivência e  na busca de  meios para diminuir desigualdades sociais. Nesse percurso, o homem questiona-se sobre as razões que distanciaram o ser humano de seu verdadeiro propósito: congregar  esforços  para  atender  às  necessidades do “outro”, ajudando-o a resgatar a identidade, a auto-estima e os valores de solidariedade por meio de ações  que  se  firmam  em pequenas causas  sonhadas. Nesse contexto está a menina Luísa que, desde  cedo,  demonstra  disposição  de  perseguir um sonho e de buscar meios para concretizá-lo.

Os pais da psicanálise com crianças

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Adela Stoppel de Gueller

Full Text Available Durante meio século, a história da psicanálise com crianças guiou-se pelas linhas mestras estabelecidas no Colóquio sobre análise infantil, que em 1927 entronou Melanie Klein e Anna Freud como suas genuínas mães. Um dos efeitos que se produziram foi a psicanálise com crianças se haver consagrado como um campo de mulheres. Contudo, anteriores a essas mulheres, estão os que podemos considerar os pais da psicanálise com crianças — mas que não foram reconhecidos como tais. Entre eles, Karl Abraham, Carl Jung e Max Graf. O que se esconde nesse apagamento? Que efeitos isso teve na prática psicanalítica com crianças? O artigo levanta a hipótese de que a fantasia do pai sedutor dissuadiu os homens de se aventurarem nesse campo.

Remoção de fármacos e desreguladores endócrinos em estações de tratamento de esgoto: revisão da literatura

Directory of Open Access Journals (Sweden)

Sérgio Francisco de Aquino

2013-09-01

Full Text Available O monitoramento ambiental dos chamados microcontaminantes ou micropoluentes vem ganhando grande interesse da comunidade científica desde os anos 1970. Nesse grupo de contaminantes estão incluídos fármacos de diversas classes, produtos de limpeza e higiene pessoal, substâncias aplicadas na produção de plásticos e resinas, pesticidas, hormônios naturais e seus subprodutos, entre outros compostos. A principal via de contaminação do meio ambiente com fármacos e desreguladores endócrinos (DE é o lançamento de esgotos in natura e tratado. Nesse contexto, este artigo compila dados de ocorrência de fármacos e DE no afluente e efluente de estações de tratamento de esgoto (ETE, discute os mecanismos envolvidos na sua remoção em ETE e faz uma análise comparativa da remoção de tais compostos em diferentes sistemas de tratamento

Factors impacting on organisational learning in three rural health ...

African Journals Online (AJOL)

a relatively new concept in the healthcare system.1. A learning ... challenges to those working in a rural setting because of the distance from academic ... ness to change entire routines and standard operating procedures embedded in ... priorities for an intervention to create learning organisations of district hospitals and ...

Unigene BLAST: CBRC-MMUS-14-0020 [SEVENS

Lifescience Database Archive (English)

Full Text Available CBRC-MMUS-14-0020 gnl|UG|Mm#S8040853 Mus musculus opsin 1 (cone pigments), short-wave-sensitive (color blind...ness, tritan) (Opn1sw), mRNA /cds=p(66,1106) /gb=NM_007538 /gi=31543369 /ug=Mm.56987 /len=2521 9e-37 29% ...

Unigene BLAST: CBRC-HSAP-23-0073 [SEVENS

Lifescience Database Archive (English)

Full Text Available CBRC-HSAP-23-0073 gnl|UG|Hs#S1730883 Homo sapiens opsin 1 (cone pigments), short-wave-sensitive (color blind...ness, tritan) (OPN1SW), mRNA /cds=p(8,1054) /gb=NM_001708 /gi=4502386 /ug=Hs.656404 /len=1101 1e-80 43% ...

Unigene BLAST: CBRC-MMUS-03-0073 [SEVENS

Lifescience Database Archive (English)

Full Text Available CBRC-MMUS-03-0073 gnl|UG|Mm#S8040853 Mus musculus opsin 1 (cone pigments), short-wave-sensitive (color blind...ness, tritan) (Opn1sw), mRNA /cds=p(66,1106) /gb=NM_007538 /gi=31543369 /ug=Mm.56987 /len=2521 2e-27 27% ...

GRAMMATICAL PREREQUISITES TO PHONOLOGICAL CHANGE?*

African Journals Online (AJOL)

1947), I do not wish to suggest that considerations of meaning and ... may at first use the new articulation at the expense of a linguistic distinction. .... Classical generative approaches to historical linguistics ex- .... ness, phonetic motivation) is accompanied by an increase first in ...... Units with basic, intrinsic (lexical) meanings.

Unigene BLAST: CBRC-MMUS-20-0033 [SEVENS

Lifescience Database Archive (English)

Full Text Available CBRC-MMUS-20-0033 gnl|UG|Mm#S8040853 Mus musculus opsin 1 (cone pigments), short-wave-sensitive (color blind...ness, tritan) (Opn1sw), mRNA /cds=p(66,1106) /gb=NM_007538 /gi=31543369 /ug=Mm.56987 /len=2521 5e-78 42% ...

Unigene BLAST: CBRC-HSAP-10-0031 [SEVENS

Lifescience Database Archive (English)

Full Text Available CBRC-HSAP-10-0031 gnl|UG|Hs#S1730883 Homo sapiens opsin 1 (cone pigments), short-wave-sensitive (color blind...ness, tritan) (OPN1SW), mRNA /cds=p(8,1054) /gb=NM_001708 /gi=4502386 /ug=Hs.656404 /len=1101 1e-32 28% ...

Unigene BLAST: CBRC-HSAP-23-0072 [SEVENS

Lifescience Database Archive (English)

Full Text Available CBRC-HSAP-23-0072 gnl|UG|Hs#S1730883 Homo sapiens opsin 1 (cone pigments), short-wave-sensitive (color blind...ness, tritan) (OPN1SW), mRNA /cds=p(8,1054) /gb=NM_001708 /gi=4502386 /ug=Hs.656404 /len=1101 1e-80 43% ...

Unigene BLAST: CBRC-MMUS-01-0101 [SEVENS

Lifescience Database Archive (English)

Full Text Available CBRC-MMUS-01-0101 gnl|UG|Mm#S8040853 Mus musculus opsin 1 (cone pigments), short-wave-sensitive (color blind...ness, tritan) (Opn1sw), mRNA /cds=p(66,1106) /gb=NM_007538 /gi=31543369 /ug=Mm.56987 /len=2521 3e-33 28% ...

Unigene BLAST: CBRC-MMUS-17-0171 [SEVENS

Lifescience Database Archive (English)

Full Text Available CBRC-MMUS-17-0171 gnl|UG|Mm#S8040853 Mus musculus opsin 1 (cone pigments), short-wave-sensitive (color blind...ness, tritan) (Opn1sw), mRNA /cds=p(66,1106) /gb=NM_007538 /gi=31543369 /ug=Mm.56987 /len=2521 2e-22 22% ...

Unigene BLAST: CBRC-HSAP-04-0044 [SEVENS

Lifescience Database Archive (English)

Full Text Available CBRC-HSAP-04-0044 gnl|UG|Hs#S1730883 Homo sapiens opsin 1 (cone pigments), short-wave-sensitive (color blind...ness, tritan) (OPN1SW), mRNA /cds=p(8,1054) /gb=NM_001708 /gi=4502386 /ug=Hs.656404 /len=1101 5e-23 25% ...

Checklist de Fanniidae (Insecta, Diptera do Estado de Mato Grosso do Sul

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Diana Grisales

Full Text Available RESUMO Nesse artigo é fornecida uma lista de espécies de Fanniidae do estado de Mato Grosso do Sul. Até o momento são registradas 11 espécies, o que representa 21% das espécies de Fanniidae conhecidas para o Brasil.

Manual for Courts-Martial United States. 2002 Edition

Science.gov (United States)

2002-01-01

bedridden conspirator may knowingly furnish the car to be used in a robbery. The joining of another conspirator after the conspiracy has been established...the extremely elderly , hostile wit- nesses, and witnesses identified with the adverse party. It is also appropriate with the military judge’s consent to

The Role of NGOs in Canada and the USA in the Transformation of ...

African Journals Online (AJOL)

sulaiman.adebowale

2008-01-29

Jan 29, 2008 ... popular culture, which present the African lifeworld as inferior and primitive, ... that they become development tourists who regularly visit Africa, bringing back ..... Simply put, hegemony is a 'style of state .... and decision making. ... ness and financial directors and make policy decisions that affect – in the.

Internet Investigations: Mixing Talent with Teachers and Telecommunications.

Science.gov (United States)

Brown, Mark E.; Riley, Tracy L.

1998-01-01

Describes how teams of grade 4-9 gifted students investigated unsolved mysteries like Bigfoot, aliens and UFOs, the Loch Ness Monster, and Stonehenge to develop Internet and research skills. Highlights student observations on difficulties encountered using the Internet for research, notes student evaluation of the workshop, and provides addresses…

Effects of soil characteristics, allelopathy and frugivory on establishment of the invasive plant Carpobrotus edulis and a cooccuring native, Malcolmia littorea

Czech Academy of Sciences Publication Activity Database

Novoa, A.; González, L.; Moravcová, Lenka; Pyšek, Petr

2012-01-01

Roč. 7, č. 12 (2012) E-ISSN 1932-6203 R&D Projects: GA ČR GA206/09/0563 Institutional support: RVO:67985939 Keywords : biological invasions * phenotypic plsticity * mediterranean islands * species invasive ness * coastal California * aizoaceae * germination Subject RIV: EF - Botanics Impact factor: 3.730, year: 2012