5,101 research outputs found

    The Implications of Galaxy Formation Models for the TeV Observations of Current Detectors

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    This paper represents a step toward constraining galaxy formation models via TeV gamm a ray observations. We use semi-analytic models of galaxy formation to predict a spectral distribution for the intergalactic infrared photon field, which in turn yields information about the absorption of TeV gamma rays from extra-galactic sources. By making predictions for integral flux observations at >200 GeV for several known EGRE T sources, we directly compare our models with current observational upper limits obtained by Whipple. In addition, our predictions may offer a guide to the observing programs for the current population of TeV gamma ray observatories.Comment: 6 pages, 11 figures, to appear in the proceedings of the 6th TeV Workshop at Snowbird, U

    Comparing electronic monitoring regimes: Length, breadth, depth and weight equals tightness

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    This paper compares the use of electronic monitoring in three European jurisdictions – Belgium, England and Wales and the Netherlands. It suggests that rates of use, the accepted method of comparison in relation to imprisonment and a proxy measure of ‘punitiveness’ provide a misleading picture when applied to electronic monitoring. This paper transforms Crewe's concept of ‘tightness’ from a dimension of weight to encompass the overlapping elements of length, breadth, depth and weight to provide a framework for analysing how electronic monitoring regimes are designed to disrupt the lives of monitored individuals. Electronic monitoring regimes are diverse and ‘tightness’ varied as much, if not more, within as between jurisdictions. Comparisons of ‘tightness’ also inverted the scale of ‘punitiveness’ produced using rates of use

    A Study of the SP Geophysical Technique in a Campus Setting

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    The self potential (SP) method is a simple and inexpensive geophysical surveying technique, which involves measuring electrical potentials on the surface due to charge separations in the subsurface. These charge separations can arise from a number of different physical and electrochemical processes, and hence interpretations tend to be qualitative. Small anomalies are typically neglected as transient, inexplicable, or uninteresting. In contrast, large negative anomalies associated with ore bodies are noted for their constancy. In this study, an area on the campus of Memorial University was repeatedly surveyed in order to determine which natural and anthropogenic features generated SP anomalies, and whether these anomalies were constant or transient. We found anomalies associated with a building, a buried metallic pipe, trees, and subtler ground variations. The locations of anomalies, both large and small, were notably unvarying over a period of days and weeks. The building always generated a significant negative anomaly, but the sign of other anomalies (including that associated with the pipe) and the magnitude of all anomalies varied with time. In a second area dominated by a shallow sewer pipe, SP data allowed modeling of the burial depth and charge distribution of the pipe. Our results show that SP can be a useful and reliable method for shallow ground surveys, but that the time-varying nature of both sign and magnitude of small to moderate anomalies should be taken into account in data collection and interpretation. Résumé La mĂ©thode des potentiels spontanĂ©s est une technique d’exĂ©cution de levĂ©s gĂ©ophysiques simple et peu dispendieuse consistant Ă  mesurer les potentiels Ă©lectriques Ă  la surface liĂ©s aux sĂ©parations des charges dans le sous-sol. Ces sĂ©parations des charges peuvent dĂ©couler d’un certain nombre de processus physiques et Ă©lectrochimiques diffĂ©rents, de sorte que les interprĂ©tations donnĂ©es ont tendance Ă  ĂȘtre qualitatives. On nĂ©glige gĂ©nĂ©ralement les petites anomalies, les considĂ©rant comme des anomalies transitoires, inexplicables ou peu intĂ©ressantes. En revanche, on note les anomalies nĂ©gatives poussĂ©es qui sont associĂ©es aux corps minĂ©ralisĂ©s en raison de leur constance. Dans le cadre de cette Ă©tude, on a rĂ©alisĂ© des levĂ©s rĂ©pĂ©tĂ©s dans un secteur du campus de l’UniversitĂ© Memorial pour dĂ©terminer quelles particularitĂ©s naturelles et artificielles produisaient des anomalies des PS et si ces anomalies Ă©taient constantes ou transitoires. Nous avons dĂ©couvert des anomalies associĂ©es Ă  un bĂątiment, Ă  un tuyau en mĂ©tal enfoui, Ă  des arbres et Ă  des irrĂ©gularitĂ©s du terrain plus subtiles. Fait remarquable, les emplacements des anomalies, tant prononcĂ©es que minimes, n’ont pas changĂ© au cours d’une pĂ©riode de plusieurs jours et semaines. Le bĂątiment a toujours produit une anomalie nĂ©gative marquĂ©e, mais le signal d’autres anomalies (notamment celle associĂ©e au tuyau) et la magnitude de toutes les anomalies ont variĂ© au fil du temps. Dans un second secteur oĂč Ă©tait surtout prĂ©sent un tuyau d’égout peu profond, les donnĂ©es des PS ont permis la modĂ©lisation de la profondeur d’enfouissement et de la distribution des charges du tuyau. Nos rĂ©sultats rĂ©vĂšlent que la polarisation spontanĂ©e peut s’avĂ©rer une mĂ©thode utile et fiable pour les levĂ©s terrestres peu profonds, mais qu’il faudrait tenir compte de la nature variable des signaux et de la magnitude des anomalies minimes Ă  moyennes lors de la collecte et de l’interprĂ©tation des donnĂ©es. [Traduit par la redaction

    Seed predation and dispersal by small mammals in a landscape of fear: effects of personality, predation risk and land-use change

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    Scatter-hoarding small mammals act as both seed predators and seed dispersers in forest ecosystems. Their choices regarding consuming or caching seeds must balance the risk of predation with the energy rewards gained from immediate or delayed consumption of seeds. Several factors influence their interaction with seeds, including the individual's personality. Little is known about how personality affects foraging decisions in response to predation risk. This missing information is critical because if foraging decisions differ among individuals in response to perceived risk, then varying combinations of personality types in a population (and varying risks of predation across forest types) may have diverse effects on forest regeneration. Further, land-use change may influence the interplay of personality, risk perception and foraging decisions by altering the distribution of personality types in the landscape and the risk perceived by individuals. To contribute to filling these knowledge gaps, we designed a large-scale field experiment to evaluate how personality, perceived predation risk and land-use change affect the interaction of deer mice Peromyscus maniculatus and seeds. Using infrared cameras, we recorded the choices of individuals of known personality at paired experimental sites with high versus low perceived predation risk (n = 2389 observations from 74 individuals). We found that personality influenced multiple foraging decisions, and perceived risk affected how individuals with different personalities responded to those decisions. Specifically, exploration/activity influenced seed choice, boldness affected the number of seeds selected and docility influenced both foraging site selection and whether mice immediately consumed or removed seeds. Since personality only affected foraging microsite selection in unmanaged forests, our results show that land-use change decreased the importance of personality in affecting risk perception. We demonstrate the importance of considering personality on foraging decisions under varying levels of risk, and more generally, underscore the importance of considering individual variation in affecting ecological processes

    Balloon-borne radiometer measurement of Northern Hemisphere mid-latitude stratospheric HNO3 profiles spanning 12 years

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    Low-resolution atmospheric thermal emission spectra collected by balloon-borne radiometers over the time span of 1990–2002 are used to retrieve vertical profiles of HNO3, CFC-11 and CFC-12 volume mixing ratios between approximately 10 and 35 km altitude. All of the data analyzed have been collected from launches from a Northern Hemisphere mid-latitude site, during late summer, when stratospheric dynamic variability is at a minimum. The retrieval technique incorporates detailed forward modeling of the instrument and the radiative properties of the atmosphere, and obtains a best fit between modeled and measured spectra through a combination of onion-peeling and global optimization steps. The retrieved HNO3 profiles are consistent over the 12-year period, and are consistent with recent measurements by the Atmospheric Chemistry Experiment-Fourier transform spectrometer satellite instrument. This suggests that, to within the errors of the 1990 measurements, there has been no significant change in the HNO3 summer mid-latitude profile

    The role of psychological flexibility in the relationship between self-concealment and disordered eating symptoms

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    The present cross-sectional study investigated whether psychological flexibility mediates the association between self-concealment and disordered eating (DE) symptoms among non-clinical college students. Data of 209 male and female participants (nfemale = 165), aged 18-22 years old, were used for analyses. Self-concealment was found to be positively associated with DE symptoms (i.e., general eating disorder symptoms and eating disorder-related cognitions) and negatively associated with psychological flexibility. Psychological flexibility was inversely associated with DE symptoms. Finally, psychological flexibility was found to mediate the association between self-concealment and DE symptoms after accounting for gender, ethnic background, and body mass index (BMI)

    A preliminary longitudinal study of white matter alteration in cocaine use disorder subjects

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    Background Previous diffusion tensor imaging (DTI) studies have consistently shown that subjects with cocaine use disorder (CocUD) had altered white matter microstructure in the corpus callosum. It is believed that these alterations are due to preexisting factors, chronic cocaine use, or both. However, there is no published longitudinal DTI study on human cocaine users yet which could shed light on the relationship between cocaine use and DTI findings. Methods This study used a longitudinal design and DTI to test if the white matter microstructure shows quicker alteration in CocUD subjects than controls. DTI data were acquired from eleven CocUD subjects who participated a treatment study and eleven non-drug-using controls at baseline (Scan 1) and after ten weeks (Scan 2). The baseline fractional anisotropy (FA), a general measure of white matter microstucture, and the change in FA (ΔFA, equals Scan 1 FA minus Scan 2 FA) were both compared between groups. Results The two groups did not show a difference in FA at baseline. The CocUD subjects had significantly greater ΔFA than the controls in the left splenium of the corpus callosum. In CocUD subjects, greater ΔFA in this region was associated with shorter lifetime cocaine use and greater number of positive cocaine urine samples collected during the treatment. Conclusion The finding in the left splenium is consistent with previous animal studies and provide indirect evidence about the effects of chronic cocaine use on white matter alterations. The subject sample size is small, therefore the results should be treated as preliminary

    Nonlinear tree growth dynamics predict resilience to disturbance

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    Following a disturbance, why does one tree survive while another dies? Physiological mechanisms may explain varying responses to disturbance between different tree species, but fewer studies have investigated conspecific variation in resilience to forest disturbance. We propose that a dynamic signal found in trees may provide clues to their post-disturbance fate. Specifically, linear versus nonlinear growth dynamics of a tree may be an indicator of its likelihood to survive a disturbance. Here, we investigate stands of red oak (Quercus rubra L.) that experienced disturbances in the form of drought and insect attack. Earlier work indicated that oaks dying during these disturbances had faster growth rates in their first years of life, but there was no obvious difference in canopy status, size, age, or microsite habitat between trees that survived and those that died. To investigate potential differences in growth dynamics between these trees, we quantified radial growth of individual trees and used two forecasting models to classify tree growth dynamics as linear or nonlinear. Trees were classified as healthy, declining, or dying based on crown cover, and dynamic patterns of growth were related to these health classifications. Contrary to expectations, we found healthy Q. rubra were significantly more likely to exhibit nonlinear growth dynamics relative to declining and dying trees. The drivers of this effect remain unclear, but nonlinear growth dynamics in healthy trees may represent an enhanced ability to benefit from resource pulses, in turn promoting greater resilience. Our work suggests that forecasting models offer a means of predicting tree survival during forest disturbances and thus represent an increasingly valuable tool as forest disturbances increase in frequency and severity

    EROs found behind lensing clusters: II.Empirical properties, classification, and SED modelling based on multi-wavelength observations

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    We study the properties and nature of extremely red galaxies (ERO, R-K>5.6) found behind two lensing clusters and compare them with other known galaxy populations. New HST/ACS observations, Spitzer IRAC and MIPS, and Chandra/ACIS observations of the two lensing clusters Abell 1835 and AC114 contemplate our earlier optical and near-IR observations and have been used to study extremely red objects (EROs) in these deep fields. We have found 6 and 9 EROs in Abell 1835 and AC114. Several (7) of these objects are undetected up to the I and/or z band, and are hence ``optical'' drop-out sources. The photometric redshifts of most of our sources (80%) are z~0.7-1.5. According to simple colour-colour diagrams the majority of our objects would be classified as hosting old stellar populations. However, there are clear signs of dusty starbursts for several among them. These objects correspond to the most extreme ones in R-K colour. We estimate a surface density of (0.97+-0.31) arcmin-2 for EROs with (R-K>5.6) at K<20.5. Among our 15 EROs 6 (40 %) also classify as distant red galaxies (DRGs). 11 of 13 EROs with available IRAC photometry also fulfil the selection criteria for IRAC selected EROs (IEROs) of Yan et al. (2004). SED modelling shows that ~ 36 % of the IEROs in our sample are luminous or ultra-luminous infrared galaxies ((U)LIRG). Some very red DRGs are found to be very dusty starbursts, even (U)LIRGs, as also supported by their mid-IR photometry. No indication for AGNs is found, although faint activity cannot be excluded for all objects. From mid-IR and X-ray data 5 objects are clearly classified as starbursts. The derived properties are quite similar to those of DRGs and IEROs, except for 5 extreme objects in terms of colours, for which a very high extinction (Av>3) is found.Comment: 20 pages, 10 figures, accepted for publication in A&
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