cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
DELIGHT: Deep Learning Identification of Galaxy Hosts of Transients using Multi-resolution Images
Creators: name: Förster, Francisco
name: Arancibia, Alejandra M. Muñoz
name: Reyes, Ignacio
name: Gagliano, Alexander
name: Britt, Dylan
name: Cuellar-Carrillo, Sara
name: Figueroa-Tapia, Felipe
name: Polzin, Ava
name: Yousef, Yara
name: Arredondo, Javier
name: Rodríguez-Mancini, Diego
name: Correa-Orellana, Javier
name: Bayo, Amelia
name: Bauer, Franz E.
name: Catelan, Márcio
name: Cabrera-Vives, Guillermo
name: Dastidar, Raya
name: Estévez, Pablo A.
name: Pignata, Giuliano
name: Hernandez-Garcia, Lorena
name: Huijse, Pablo
name: Reyes, Esteban
name: Sánchez-Sáez, Paula
name: Ramirez, Mauricio
name: Grandón, Daniela
name: Pineda-García, Jonathan
name: Chabour-Barra, Francisca
name: Silva-Farfán, Javier
Publisher: name: arXiv
Year: 2022
Subjects: subject: Instrumentation and Methods for Astrophysics (astro-ph.IM)
subject: FOS: Physical sciences

description: We present DELIGHT, or Deep Learning Identification of Galaxy Hosts of Transients, a new algorithm designed to automatically and in real-time identify the host galaxies of extragalactic transients. The proposed algorithm receives as input compact, multi-resolution images centered at the position of a transient candidate and outputs two-dimensional offset vectors that connect the transient with the center of its predicted host. The multi-resolution input consists of a set of images with the same number of pixels, but with progressively larger pixel sizes and fields of view. A sample of \nSample galaxies visually identified by the ALeRCE broker team was used to train a convolutional neural network regression model. We show that this method is able to correctly identify both relatively large ($10\arcsec < r < 60\arcsec$) and small ($r \le 10\arcsec$) apparent size host galaxies using much less information (32 kB) than with a large, single-resolution image (920 kB). The proposed method has fewer catastrophic errors in recovering the position and is more complete and has less contamination ($< 0.86\%$) recovering the cross-matched redshift than other state-of-the-art methods. The more efficient representation provided by multi-resolution input images could allow for the identification of transient host galaxies in real-time, if adopted in alert streams from new generation of large etendue telescopes such as the Vera C. Rubin Observatory.
description: Submitted to The Astronomical Journal on Aug 5th, 2022. Comments and suggestions are welcome
Additional file 1 of Unmet needs in ankylosing spondylitis patients receiving tumour necrosis factor inhibitor therapy; results from a large multinational real-world study
Creators: name: A. Deodhar
name: V. Strand
name: P. Conaghan
name: E. Sullivan
name: S. Blackburn
name: H. Tian
name: K. Gandhi
name: S. Jugl
name: R. Alten
Publisher: name: figshare
Year: 2020
Subjects: subject: Medicine
subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences
subject: Sociology
subject: FOS: Sociology
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences

description: Additional file 1: Table S1. Patient characteristics, Description of data: Detailed patient characteristics, including disease severity and disease scores, are provided.
A facility for mass production of ultra-pure NaI powder for the COSINE-200 experiment
Creators: name: Shin, Keonah
name: Choe, Junseok
name: Gileva, Olga
name: Iltis, Alain
name: Kim, Yeongduk
name: Lee, Cheolho
name: Lee, Hyun Su
name: Lee, Moo Hyun
name: Park, Hyang Kyu
Publisher: name: arXiv
Year: 2020
Subjects: subject: Instrumentation and Detectors (physics.ins-det)
subject: Instrumentation and Methods for Astrophysics (astro-ph.IM)
subject: High Energy Physics - Experiment (hep-ex)
subject: Nuclear Experiment (nucl-ex)
subject: FOS: Physical sciences

description: COSINE-200 is the next phase of the ongoing COSINE-100 experiment. The main purpose of the experiment is the performance of an unambiguous verification of the annual modulation signals observed by the DAMA experiment. The success of the experiment critically depends on the production of a 200 kg array of ultra-pure NaI(Tl) crystal detectors that have lower backgrounds than the DAMA crystals. The purification of raw powder is the initial but important step toward the production of ultra-pure NaI(Tl) detectors. We have already demonstrated that fractional recrystallization from water solutions is an effective method for the removal of the problematic K and Pb elements. For the mass production of purified powder, a clean facility for the fractional recrystallization had been constructed at the Institute for Basic Science (IBS), Korea. Here, we report the design of the purification process, material recovery, and performance of the NaI powder purification facility.
description: Proceeding for INSTR20, accepted in JINST
Analysis of Quantum Light Memory in Atomic Systems
Creators: name: Kaatuzian, H.
name: Rostami, A.
name: Oskouei, A. A.
Publisher: name: arXiv
Year: 2004
Subjects: subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: We extend the theory to describe the quantum light memory in type atoms with considering (lower levels coherency decay rate) and detuning for the probe and the control fields. We obtain that with considering these parameters, group velocity of the probe pulse does not tend to zero by turning off the control field. We show that there are considerable decay for the probe pulse and the stored information. Also, it is inferred that the light field does not tend to zero when the control field is turned off. In addition, we obtain that in the off-resonance case there is considerable distortion of the output light pulse (with fast oscillations) that destroys the stored information. Then we present the limitations on detuning (bandwidths) of the probe and the control fields to achieve negligible distortion. We finally present the numerical calculations and compare them with obtained analytical results.
Additional file 7 of Adaptation of the Patient Benefit Assessment Scale for Hospitalised Older Patients: development, reliability and validity of the P-BAS picture version
Creators: name: van der Kluit, Maria Johanna
name: Dijkstra, Geke J.
name: de Rooij, Sophia E.
Publisher: name: figshare
Year: 2022
Subjects: subject: Space Science
subject: Medicine
subject: Biotechnology
subject: 59999 Environmental Sciences not elsewhere classified
subject: FOS: Earth and related environmental sciences
subject: Sociology
subject: FOS: Sociology
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: Science Policy

description: Additional file 7. Crosstabulations validity hypotheses baseline importance of goals.
MAGAZ3NE: High Stellar Velocity Dispersions for Ultra-Massive Quiescent Galaxies at $z\gtrsim3$
Creators: name: Forrest, Ben
name: Wilson, Gillian
name: Muzzin, Adam
name: MArchesini, Danilo
name: Cooper, M. C.
name: Marsan, Z. Cemile
name: Annunziatella, Marianna
name: McConachie, Ian
name: Zaidi, Kumail
name: Gomez, Percy
name: Stawinski, Stephanie M. Urbano
name: Chang, Wenjun
name: de Lucia, Gabriella
name: La Barbera, Francesco
name: Lubin, Lori
name: Nantais, Julie
name: Peña, Theodore
name: Saracco, Paolo
name: Surace, Jason
name: Stefanon, Mauro
Publisher: name: arXiv
Year: 2022
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: In this work we publish stellar velocity dispersions, sizes, and dynamical masses for 8 ultra-massive galaxies (UMGs; log($M$/M$_\odot>11$, $z\gtrsim3$) from the Massive Ancient Galaxies At $z>3$ NEar-infrared (MAGAZ3NE) Survey, more than doubling the number of such galaxies with velocity dispersion measurements at this epoch. Using the deep Keck/MOSFIRE and Keck/NIRES spectroscopy of these objects in the $H$- and $K$-bandpasses, we obtain large velocity dispersions of $\sim400$ km s$^{-1}$ for most of the objects, which are some of the highest stellar velocity dispersions measured, and $\sim40$\% larger than those measured for galaxies of similar mass at $z\sim1.7$. The sizes of these objects are also smaller by a factor of 1.5-3 compared to this same $z\sim1.7$ sample. We combine these large velocity dispersions and small sizes to obtain dynamical masses. The dynamical masses are similar to the stellar masses of these galaxies, consistent with a Chabrier initial mass function (IMF). Considered alongside previous studies of massive quiescent galaxies across $0.2
description: 17 pages and 8 figures in the main text, plus references and Appendices for a total of 25 pages and 14 figures. Accepted for publication in The Astrophysical Journal
How might student gender influence book choices a teacher makes : a study of reading motivation in middle school children
Creators: name: Fast, Sarah J.
Publisher: name: The University of British Columbia
Year: 2014

description: The purpose of this study was to explore the ways that gender might impact reading choices of a mixed gender group of grade 7 students and how such choices might inform language arts instruction. A survey of reading preferences was given to all grade 7 students enrolled. This survey consisted of Likert scale and open response questions that helped to determine which novels students would like to read, which novels they have already read, and their general feelings towards reading. The data was examined for trends within book choices and between genders. It was concluded, based on the responses on the surveys, that students are motivated by story elements and genre and a student's gender and a character's gender has less impact on a student's reading choice.
Additional file 2 of Effectiveness of alternative measures to reduce antimicrobial usage in pig production in four European countries
Creators: name: Raasch, Svenja
name: Collineau, Lucie
name: Postma, Merel
name: Backhans, Annette
name: Sjölund, Marie
name: Belloc, Catherine
name: Emanuelson, Ulf
name: Beilage, Elisabeth
name: Stärk, Katharina
name: Dewulf, Jeroen
Publisher: name: figshare
Year: 2020
Subjects: subject: Medicine
subject: 59999 Environmental Sciences not elsewhere classified
subject: FOS: Earth and related environmental sciences
subject: Ecology
subject: FOS: Biological sciences
subject: Sociology
subject: FOS: Sociology
subject: 69999 Biological Sciences not elsewhere classified
subject: Science Policy
subject: 110309 Infectious Diseases
subject: FOS: Health sciences
subject: Computational Biology

description: Additional file 2. Distribution of treatment incidences of farrow-to finish pig herds before and after the intervention study.
MAP Rwanda: Gira Ingoma Music Album
Creators: name: Primaire Ngoma, Ecole
name: Primaire Nyanza, Ecole
name: Primaire Saint Antoine, Ecole
name: Scolaire Cyarwa, Groupe
name: Scolaire Kabuga, Groupe
name: Scolaire Kinteko, Groupe
name: Scolaire Matyazo, Groupe
name: Scolaire Mpungwe, Groupe
name: Scolaire Musange, Groupe
name: Scolaire Rukira, Groupe
name: Scolaire Sovu, Groupe
Publisher: name: University of Lincoln
Year: 2025
Subjects: W352 - Community music
W353 - Music & gender
L320 - Gender studies

description: The school girls who participated in the Gira Ingoma – One Girl per Drum project in Rwanda created and performed poems and songs in which they express their self-confidence and tell the stories of great women (including themselves) to build a new artistic repertoire in which women are present and valued. In their creations, they use attributes and values considered masculine and feminine without distinction, blurring the lines of gender roles and expectations. The poems are inspired of the tradition of ibyivugo (self-praise poems performed by the Intore warriors) and the songs both pay tribute to the legacy of Ingoma Nshya and paint the promise of a proud and bright future for the girls.https://doi.org/10.24385/lincoln.28408442
Additional file 8 of Adaptation of the Patient Benefit Assessment Scale for Hospitalised Older Patients: development, reliability and validity of the P-BAS picture version
Creators: name: van der Kluit, Maria Johanna
name: Dijkstra, Geke J.
name: de Rooij, Sophia E.
Publisher: name: figshare
Year: 2022
Subjects: subject: Space Science
subject: Medicine
subject: Biotechnology
subject: 59999 Environmental Sciences not elsewhere classified
subject: FOS: Earth and related environmental sciences
subject: Sociology
subject: FOS: Sociology
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: Science Policy

description: Additional file 8. Comparison achievement of goals stated in open question and P-BAS-P scores.
Alexander's prescription for colloidal charge renormalization
Creators: name: Trizac, E.
name: Bocquet, L.
name: Aubouy, M.
name: von Grunberg, H. H.
Publisher: name: arXiv
Year: 2003
Subjects: subject: Soft Condensed Matter (cond-mat.soft)
subject: FOS: Physical sciences

description: The interactions between charged colloidal particles in an electrolyte may be described by usual Debye-Hückel theory provided the source of the electric field is suitably renormalized. For spherical colloids, we reconsider and simplify the treatment of the popular proposal put forward by Alexander {\it et al.} [J. Chem. Phys. {\bf 80}, 5776 (1984)], which has proven efficient in predicting renormalized quantities (charge and salt content). We give explicit formulae for the effective charge and describe the most efficient way to apply Alexander's et al. renormalization prescription in practice. Particular attention is paid to the definition of the relevant screening length, an issue that appears confused in the literature.
The information capacity of entanglement-assisted continuous variable measurement
Creators: name: Holevo, A. S.
name: Kuznetsova, A. A.
Publisher: name: arXiv
Year: 2020
Subjects: subject: Quantum Physics (quant-ph)
subject: Mathematical Physics (math-ph)
subject: FOS: Physical sciences

description: The present paper is devoted to investigation of the entropy reduction and entanglement-assisted classical capacity (information gain) of continuous variable quantum measurements. These quantities are computed explicitly for multimode Gaussian measurement channels. For this we establish a fundamental property of the entropy reduction of a measurement: under a restriction on the second moments of the input state it is maximized by a Gaussian state (providing an analytical expression for the maximum). In the case of one mode, the gain of entanglement assistance is investigated in detail.
description: 22 pages, 2 figures, eq. (43) corrected
Anomalous superconducting properties at magic doping levels in under-doped La2-xSrxCuO4 single crystals
Creators: name: Zhou, F.
name: Hor, P. H.
name: Dong, X. L.
name: Ti, W. X.
name: Xiong, J. W.
name: Zhao, Z. X.
Publisher: name: arXiv
Year: 2003
Subjects: subject: Superconductivity (cond-mat.supr-con)
subject: FOS: Physical sciences

description: A series of high-quality under-doped La2-xSrxCuO4 superconductor crystals with x = 0.063 - 0.125 were prepared by traveling-solvent floating-zone (TSFZ) technique. We found by dc magnetic measurements that, in this series of crystals, the superconducting transition was quite sharp in the vicinity of the hole densities of x = 1/16 and x = 1/9 while it was much broader away from these two "magic numbers", and the Meissner fraction showed a remarkable minimum near x = 1/9. We concluded that these phenomena are reflections of intrinsic properties of this cuprate system. Our observations are discussed in light of recently proposed composite charge model together with charge inhomogeneity and electronic phase separations.
description: 4 pages, 4 figures; Presented at the 7th Intl. Conf. M2S.(Rio de Janeiro, May 2003)
Styloleptus zorrillai
Creators: name: Monné, Miguel A.
Publisher: name: Zenodo
Year: 2005
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Coleoptera
Cerambycidae
Styloleptus
Styloleptus zorrillai

description: 21. Styloleptus zorrillai (Zayas, 1975)
Type locality — Cuba, Pinar del Rio: Cajálbana. (Zayas). Distribution — Cuba.
 Urgleptes zorrillai Zayas, 1975: 259; Chemsak et al., 1992: 149 (cat.).
 Styloleptus zorrillai; Monné & Giesbert, 1992: 253; Monné, 2001b: 31 (cat. hosts).
  Sympagus Bates, 1881
 Sympagus Bates, 1881a: 173.
 Type­species — Lepturges laetabilis Bates, 1872 (monotypy and original designation).
description: Published as part of Monné, Miguel A., 2005, Catalogue of the Cerambycidae (Coleoptera) of the Neotropical Region. Part II. Subfamily Lamiinae, pp. 1-760 in Zootaxa 1023 (1) on pages 1-760, DOI: 10.11646/zootaxa.946.1.1, http://zenodo.org/record/5049553
Marketing Operations of Dairy Cooperatives, 2002
Creators: name: Ling, K. Charles
name: Ling, K. Charles
Publisher: name: Unknown
Year: 2004
Subjects: subject: Livestock Production/Industries
subject: Marketing
subject: FOS: Economics and business
subject: Cooperatives
subject: dairy products
subject: marketing
subject: milk
subject: structure

description: The Nation's 196 dairy cooperatives marketed 139.2 billion pounds of milk delivered by its 61,390 member-producers, or 83 percent of all milk sold to plants and dealers, in 2002. (Including non-member milk, the volume marketed by dairy cooperatives was 144.3 billion pounds, or 86 percent of the U.S. total.) Forty-six cooperatives operated 174 dairy processing and manufacturing plants, 19 handled milk through receiving stations only and 131 had no milk-handling facilities. In addition, cooperatives had investment in but did not directly operate 75 dairy plants. Cooperatives marketed 71 percent of the Nation's butter, 86 percent of the nonfat dry milk, 40 percent of the natural cheese, 7 percent of the packaged fluid milk products, 9 percent of the cottage cheese, 3 percent of the ice cream, 6 percent of the ice cream mix, 2 percent of the yogurt, 53 percent of the bulk condensed milk products, 52 percent of the dry whey products, 13 percent of the sour cream, and 34 percent of the condensed buttermilk.
Status of particle physics solutions to the UHECR puzzle
Creators: name: Kachelriess, M.
Publisher: name: arXiv
Year: 2004
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: The status of solutions to the ultra-high energy cosmic ray puzzle that involve particle physics beyond the standard model is reviewed. Signatures and experimental constraints are discussed for most proposals like the Z burst model and topological defects (both allowed only as subdominant contribution), supermassive dark matter (no positive evidence from its key signatures galactic anisotropy and photon dominance), strongly interacting neutrinos or new primaries (no viable models known), and violation of Lorentz invariance (possible).
description: 15 pages, 8 eps figures, contribution to the special issue "Ultimate energy particles in the Universe" of Comptes Rendues (eds. M. Boratav, G. Sigl)
iPTF14hls as a variable hyper-wind from a very massive star
Creators: name: Moriya, Takashi J.
name: Mazzali, Paolo A.
name: Pian, Elena
Publisher: name: arXiv
Year: 2019
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: The origin of iPTF14hls, which had Type IIP supernova-like spectra but kept bright for almost two years with little spectral evolution, is still unclear. We here propose that iPTF14hls was not a sudden outburst like supernovae but rather a long-term outflow similar to stellar winds. The properties of iPTF14hls, which are at odds with a supernova scenario, become natural when interpreted as a stellar wind with variable mass-loss rate. Based on the wind hypothesis, we estimate the mass-loss rates of iPTF14hls in the bright phase. We find that the instantaneous mass-loss rate of iPTF14hls during the 2-year bright phase was more than a few Msun/yr ("hyper-wind") and it reached as much as 10 Msun/yr. The total mass lost over two years was about 10 Msun. Interestingly, we find that the light curve of iPTF14hls has a very similar shape to that of eta Carinae during the Great Eruption, which also experienced a similar but less extreme brightening accompanied by extraordinary mass loss, shedding more than 10 Msun in 10 years. The progenitor of iPTF14hls is less than 150 Msun if it still exists, which is similar to eta Carinae. The two phenomena may be related to a continuum-driven extreme wind from very massive stars.
description: 8 pages, 7 figures, accepted by Monthly Notices of the Royal Astronomical Society
The Implicit Price of Aquatic Grasses
Creators: name: Guignet, Dennis
name: Griffiths, Charles
name: Klemick, Heather
name: Walsh, Patrick
name: Guignet, Dennis
name: Griffiths, Charles
name: Klemick, Heather
name: Walsh, Patrick
Publisher: name: Unknown
Year: 2014
Subjects: subject: Environmental Economics and Policy
subject: Resource /Energy Economics and Policy
subject: aquatic grasses
subject: Chesapeake Bay
subject: ecological input
subject: ecosystem services
subject: hedonics
subject: submerged aquatic vegetation
subject: SAV
subject: water quality

description: Almost 30% of aquatic grasses worldwide are either lost or degraded (Barbier et al, 2011). The Chesapeake Bay is no exception, with levels of submerged aquatic vegetation (SAV) remaining below half of the historic levels. This decline is largely attributed to excessive nutrient and sediment loads degrading Bay water quality. SAV provide many important functions to natural ecosystems, many of which are directly beneficial to local residents. To understand the implicit value residents place on SAV and the localized ecosystem services it provides, we undertake a hedonic property value study using residential transaction data from 1996 to 2008 in eleven Maryland counties adjacent to the Chesapeake Bay. These data are matched to high resolution maps of Baywide SAV coverage. We pose a quasi-experimental comparison and examine how the price of homes near and on the waterfront vary with the presence of SAV. On average, waterfront and near-waterfront homes within 200 meters of the shore sell at a 5% to 6% premium when SAV are present. Applying these estimates to the 185,000 acre SAV attainment goal yields total property value gains on the order of $300 to 400 million.
Climate Change and Space Heating Energy Demand: A Review of the Literature
Creators: name: Ranson, Matthew
name: Morris, Lauren
name: Kats-Rubin, Alex
name: Ranson, Matthew
name: Morris, Lauren
name: Kats-Rubin, Alex
Publisher: name: Unknown
Year: 2014
Subjects: subject: Environmental Economics and Policy
subject: Resource /Energy Economics and Policy
subject: Climate change
subject: space heating
subject: space cooling
subject: energy use
subject: integrated assessment models

description: This paper reviews recent evidence on the potential impacts of climate change on energy demand for space heating in residential and commercial buildings. We cover two main topics. First, we review empirical studies of the historical relationship between temperature and energy use for heating and cooling. These studies show consistent evidence of a U-shaped relationship between temperature and energy demand, in which energy use for heating is greatest at very low temperatures, and energy use for cooling is greatest at very high temperatures. The temperature at which energy use is minimized varies across geography and time periods, but in most studies is between 53°F and 72°F (12°C and 22°C). Second, we review studies that estimate how climate change will affect future energy use for space heating and cooling. Most studies predict that climate change will result in reductions in demand for heating and increases in demand for cooling. Although the sign of the net global effect depends on the time frame and climate change scenario, a very robust conclusion is that there is considerable variation across geographies, with the largest magnitude effects predicted for countries that currently have either very low or very high average temperatures. Overall, the results summarized in this paper will be useful for understanding the potential magnitude of the benefits of climate-related reductions in space heating, and for improving the damage functions used in integrated assessment models of climate change.
Monte Carlo simulations of the screening potential of the Yukawa one-component plasma
Creators: name: Caillol, J. -M.
name: Gilles, D.
Publisher: name: arXiv
Year: 2003
Subjects: subject: Statistical Mechanics (cond-mat.stat-mech)
subject: FOS: Physical sciences

description: A Monte Carlo scheme to sample the screening potential H(r) of Yukawa plasmas notably at short distances is presented. This scheme is based on an importance sampling technique. Comparisons with former results for the Coulombic one-component plasma are given. Our Monte Carlo simulations yield an accurate estimate of H(r) as well for short range and long range interparticle distances.
description: to be published in Journal of Physics A: Mathematical and General
Integrals containing confluent hypergeometric functions with applications to perturbed singular potentials
Creators: name: Saad, Nasser
name: Hall, Richard L.
Publisher: name: arXiv
Year: 2003
Subjects: subject: Mathematical Physics (math-ph)
subject: FOS: Physical sciences
subject: 81Q05; 81Q20

description: We show that many integrals containing products of confluent hypergeometric functions follow directly from one single integral that has a very simple formula in terms of Appell's double series F_2. We present some techniques for computing such series. Applications requiring the matrix elements of singular potentials and the perturbed Kratzer potential are presented.
description: 20 pages
Atomic microwave-to-optical signal transduction via magnetic-field coupling in a resonant microwave cavity
Creators: name: Tretiakov, A.
name: Potts, C. A.
name: Lee, T. S.
name: Thiessen, M. J.
name: Davis, J. P.
name: LeBlanc, L. J.
Publisher: name: arXiv
Year: 2020
Subjects: subject: Quantum Physics (quant-ph)
subject: Applied Physics (physics.app-ph)
subject: Atomic Physics (physics.atom-ph)
subject: FOS: Physical sciences

description: Atomic vapors offer many opportunities for manipulating electromagnetic signals across a broad range of the electromagnetic spectrum. Here, a microwave signal with an audio-frequency modulation encodes information in an optical signal by exploiting an atomic microwave-to-optical double resonance, and magnetic-field coupling that is amplified by a resonant high-Q microwave cavity. Using this approach, audio signals are encoded as amplitude or frequency modulations in a GHz carrier, transmitted through a cable or over free space, demodulated through cavity-enhanced atom-microwave interactions, and finally, optically detected to extract the original information. This atom-cavity signal transduction technique provides a powerful means by which to transfer information between microwave and optical fields, all using a relatively simple experimental setup without active electronics.
Evolution of a neutrino-cooled disc in Gamma-Ray Bursts
Creators: name: Janiuk, Agnieszka
name: Perna, Rosalba
name: Di Matteo, Tiziana
name: Czerny, Bozena
Publisher: name: arXiv
Year: 2004
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Rapid, hyper-Eddington accretion is likely to power the central engines of gamma-ray bursts (GRBs). In the extreme conditions of densities and temperatures the accreting torus is cooled by neutrino emission rather than by radiation. Another important cooling mechanism is the advection of energy into the central black hole. We compute the time evolution of a neutrino-dominated disc that proceeds during the burst and investigate the changes in its density and temperature. The discrimination between short and long bursts is made on the basis of the different rates of material inflow to the outer parts of the disc, thus favoring the binary merger scenario for the short GRBs and the collapsar scenario for the long ones. Within the context of the collapsar model, we also study the evolution of the photon luminosity of the remnant disc up to times of the order of 1 day, and discuss its implications for the production of emission lines in GRB spectra.
description: v2: 10 pages, 8 figures. Outer boundary condition recalculated, minor changes in the results and text. Accepted for publication in MNRAS
Pulsar Emission Beam Geometry of Radio Broadband Arecibo Sources
Creators: name: Olszanski, Timothy
name: Rankin, Joanna
name: Venkataraman, Arun
name: Wahl, Haley
Publisher: name: arXiv
Year: 2022
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: We present radio pulsar emission beam analyses and models with the primary intent of examining pulsar beam geometry and physics over the broadest band of radio frequencies reasonably obtainable. We consider a set of well-studied pulsars that lie within the Arecibo sky. These pulsars stand out for the broad frequency range over which emission is detectable, and have been extensively observed at frequencies up to 4.5 GHz and down to below 100 MHz. We utilize published profiles to quantify a more complete picture of the frequency evolution of these pulsars using the core/double-cone emission beam model as our classification framework. For the low-frequency observations, we take into account measured scattering time-scales to infer intrinsic vs scatter broadening of the pulse profile. Lastly, we discuss the populational trends of the core/conal class profiles with respect to intrinsic parameters. We demonstrate that for this sub-population of pulsars, core and conal dominated profiles cluster together into two roughly segregated $P$-$\dot{P}$ populations, lending credence to the proposal that an evolution in the pair-formation geometries is responsible for core/conal emission and other emission effects such as nulling and mode-changing.
description: 22 pages, 24 figures; MNRAS, in press
Additional file 1 of Effectiveness of alternative measures to reduce antimicrobial usage in pig production in four European countries
Creators: name: Raasch, Svenja
name: Collineau, Lucie
name: Postma, Merel
name: Backhans, Annette
name: Sjölund, Marie
name: Belloc, Catherine
name: Emanuelson, Ulf
name: Beilage, Elisabeth
name: Stärk, Katharina
name: Dewulf, Jeroen
Publisher: name: figshare
Year: 2020
Subjects: subject: Medicine
subject: Molecular Biology
subject: Ecology
subject: FOS: Biological sciences
subject: Sociology
subject: FOS: Sociology
subject: 69999 Biological Sciences not elsewhere classified
subject: 80699 Information Systems not elsewhere classified
subject: FOS: Computer and information sciences
subject: Marine Biology
subject: Science Policy

description: Additional file 1. Details on recruitment of farms.
Additional file 1 of Acceptability and feasibility of a vestibular nerve stimulation headset protocol in children with cerebral palsy
Creators: name: McConnell, Karen
name: Topley, Daniel
name: McKeown, Jason
name: Kerr, Claire
Publisher: name: figshare
Year: 2022
Subjects: subject: Space Science
subject: Medicine
subject: Sociology
subject: FOS: Sociology
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: Science Policy

description: Additional file 1. Semi-structured interview schedules for children and parents/guardians
Toronaeus sumptuosus Lane 1973
Creators: name: Monné, Miguel A.
Publisher: name: Zenodo
Year: 2005
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Coleoptera
Cerambycidae
Toronaeus
Toronaeus sumptuosus

description: 8. Toronaeus sumptuosus Lane, 1973
Type locality — Brazil, Amazonas: Tefé. (MNRJ). Distribution — French Guiana, Brazil (Amazonas).
 Toronaeus sumptuosus Lane, 1973a: 403; Monné, 1974: 594, fig. 5; Tavakilian et al., 1997: 324, 325 (hosts); Julio et al., 2000: 51 (holotype); Monné, 2001b: 32 (cat. hosts).
description: Published as part of Monné, Miguel A., 2005, Catalogue of the Cerambycidae (Coleoptera) of the Neotropical Region. Part II. Subfamily Lamiinae, pp. 1-760 in Zootaxa 1023 (1) on pages 1-760, DOI: 10.11646/zootaxa.946.1.1, http://zenodo.org/record/5049553
Flavored anisotropic black holes
Creators: name: Garbayo, Ana
name: Hoyos, Carlos
name: Jokela, Niko
name: Penín, José Manuel
name: Ramallo, Alfonso V.
Publisher: name: arXiv
Year: 2022
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: General Relativity and Quantum Cosmology (gr-qc)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We construct a black hole geometry dual to a (2+1)-dimensional defect in an ambient (3+1)-dimensional gauge theory at non-zero temperature and quark density. The geometry is a solution to the equations of motion of type IIB supergravity with brane sources, a low energy limit of an intersection of stacks of color D3-branes and flavor D5-branes. We consider the case in which the number of D5-branes is large and they can be homogeneously distributed along the directions orthogonal to the defect, creating in this way a multilayer structure. The quark density is generated by exciting a gauge field in the worldvolume of the dynamic brane sources. We study the thermodynamics of the anisotropic black hole and compute the energy density of the dual theory, as well as the pressures and speeds of sound along the directions parallel and orthogonal to the defect. We also calculate transport coefficients in the shear channel, quark-antiquark potentials, and the entanglement entropies for slab subregions. These analyses give us a good overview on how the degrees of freedom are spread, entangled, and behave in this unquenched system in the deconfining phase at strong coupling.
description: 34 pages + appendices
Individuelle Verläufe von Asthma, Adipositas und ADHS beim Übergang von Kindheit und Jugend ins junge Erwachsenenalter
Creators: name: Krause, Laura
name: Vogelgesang, Felicitas
name: Thamm, Roma
name: Schienkiewitz, Anja
name: Damerow, Stefan
name: Scklack, Robert
name: Junker, Stephan
name: Mauz, Elvira
Publisher: name: Robert Koch-Institut
Year: 2021
Subjects: subject: Asthma
subject: Adipositas
subject: ADHS
subject: Lebensverlauf
subject: Junges Erwachsenenalter
subject: KIGGS
subject: 610 Medizin und Gesundheit

description: Die Studie zur Gesundheit von Kindern und Jugendlichen in Deutschland (KiGGS) liefert umfassende und belastbare Daten zur gesundheitlichen Lage der heranwachsenden Generation. In der KiGGS-Kohorte werden die Teilnehmenden der KiGGS-Basiserhebung (2003 – 2006) bis ins Erwachsenenalter begleitet. Bisher wurden mit KiGGS Welle 1 (2009 – 2012) und KiGGS Welle 2 (2014 – 2017) zwei Folgeerhebungen der Kohorte realisiert. In KiGGS Welle 2 wurde die Kohorte um die Vertiefungsstudie „Familiäre und versorgungsspezifische Einflussfaktoren auf die Entstehung, den Verlauf und die Auswirkungen von psychischen Störungen (insbesondere ADHS), Adipositas und allergischen Erkrankungen (insbesondere Asthma)“ ergänzt. Ein Ziel war, Verlaufsmuster dieser Gesundheitsstörungen zu identifizieren. Dafür wurden Wahrscheinlichkeiten für typische Übergänge von der KiGGS-Basiserhebung zu KiGGS Welle 2 berechnet. Ein wichtiges Ergebnis ist, dass relativ viele Teilnehmende der KiGGS-Basiserhebung mit Asthma, Adipositas oder ADHS auch gut zehn Jahre später noch von der Erkrankung betroffen sind – nämlich etwas mehr als ein Drittel von Asthma (35 %) und ADHS (37 %) sowie fast die Hälfte von Adipositas (47 %). Dieses Ergebnis verweist unter anderem auf die Notwendigkeit für früh einsetzende Präventionsmaßnahmen, um der Entstehung dieser potenziell chronisch verlaufenden Krankheiten im Kindes- und Jugendalter vorzubeugen.
How did air quality standards affect employment at U.S. power plants? The importance of stringency, geography, and timing
Creators: name: Sheriff, Glenn
name: Ferris, Ann E.
name: Shadbegian, Ron
name: Sheriff, Glenn
name: Ferris, Ann E.
name: Shadbegian, Ron
Publisher: name: Unknown
Year: 2015
Subjects: subject: Environmental Economics and Policy
subject: air pollution
subject: electricity
subject: employment
subject: regulation

description: Geographical dierences in U.S. Clean Air Act requirements are often used to identify environmental regulatory impacts. The standard approach abstracts from aspects of the law aecting which areas are regulated, how strictly they are regulated, and when regulatory changes occur. We nd that omitting these factors can bias results by contaminating the control group, leading to under- estimation of historical employment impacts and overestimation of projected impacts from tightening regulations. Results indicate that 1990 changes to ozone nonattainment provisions reduced power plant employment without signicantly aecting generation, suggesting that installation of pollution controls contributed to labor-saving technical change at aected sources.
Determining the dust environment of an unknown comet for a spacecraft fly-by: The case of ESA's Comet Interceptor mission
Creators: name: Marschall, Raphael
name: Zakharov, Vladimir
name: Tubiana, Cecilia
name: Kelley, Michael S. P.
name: van Damme, Carlos Corral
name: Snodgrass, Colin
name: Jones, Geraint H.
name: Ivanovski, Stavro L.
name: Postberg, Frank
name: Della Corte, Vincenzo
name: Vincent, Jean-Baptiste
name: Muñoz, Olga
name: La Forgia, Fiorangela
name: Levasseur-Regourd, Anny-Chantal
name: Team, the Comet Interceptor
Publisher: name: arXiv
Year: 2022
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: Instrumentation and Methods for Astrophysics (astro-ph.IM)
subject: FOS: Physical sciences

description: We present a statistical approach to assess the dust environment for a yet unknown comet (or when its parameters are known only with large uncertainty). This is of particular importance for missions such as ESA's Comet Interceptor mission to a dynamically new comet. We find that the lack of knowledge of any particular comet results in very large uncertainties (~3 orders of magnitude) for the dust densities within the coma. The most sensitive parameters affecting the dust densities are the dust size distribution, the dust production rate and coma brightness, often quantified by Af$ρ$. Further, the conversion of a coma's brightness (Af$ρ$) to a dust production rate is poorly constrained. The dust production rate can only be estimated down to an uncertainty of ~0.5 orders of magnitude if the dust size distribution is known in addition to the Af$ρ$. To accurately predict the dust environment of a poorly known comet, a statistical approach as we propose here needs to be taken to properly reflect the uncertainties. This can be done by calculating an ensemble of comae covering all possible combinations within parameter space as shown in this work.
description: 27 pages, 15 figures, data available under https://www.doi.org/10.5281/zenodo.6906815
Additional file 2 of Acceptability and feasibility of a vestibular nerve stimulation headset protocol in children with cerebral palsy
Creators: name: McConnell, Karen
name: Topley, Daniel
name: McKeown, Jason
name: Kerr, Claire
Publisher: name: figshare
Year: 2022
Subjects: subject: Space Science
subject: Medicine
subject: Sociology
subject: FOS: Sociology
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: Science Policy

description: Additional file 2. Semi-structured interview schedule for healthcare professionals
T-Dependent Dyson- Schwinger Equation In IR Regime Of QCD: The Critical Point
Creators: name: Mitra, A. N.
name: Hwang, W-Y. P.
Publisher: name: arXiv
Year: 2004
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: The quark mass function $Σ(p)$ in QCD is revisited, using a gluon propagator in the form $1/(k^2 + m_g^2)$ plus $2μ^2/ (k^2 + m_g^2)^2$, where the second (IR) term gives linear confinement for $m_g = 0$ in the instantaneous limit, $μ$ being another scale. To find $Σ(p)$ we propose a new (differential) form of the Dyson-Schwinger Equation (DSE) for $Σ(p)$, based on an infinitesimal $subtractive$ Renormalization via a differential operator which $lowers$ the degree of divergence in integration on the RHS, by $TWO$ units. This warrants $Σ(p-k)\approx Σ(p)$ in the integrand since its $k$-dependence is no longer sensitive to the principal term $(p-k)^2$ in the quark propagator. The simplified DSE (which incorporates WT identity in the Landau gauge) is satisfied for large $p^2$ by $Σ(p)$ = $Σ(0)/(1 + βp^2)$, except for Log factors. The limit $p^2 =0$ determines $Σ_0$.A third limit $p^2 = -m_0^2$ defines the $dynamical$ mass $m_0$ via $Σ(im_0) = + m_0$. After two checks ($f_π= 93\pm 1 MeV $ and $ $= $(280 \pm 5 MeV)^3$), for $1.5$ at $T_c$. PACS: 24.85.+p; 12.38.Lg; 12.38.Aw.
description: 25pp on dvi, LaTex File
Additional file 1 of Association of SMAD7 genetic markers and haplotypes with colorectal cancer risk
Creators: name: Alidoust, Maryam
name: Hamzehzadeh, Leila
name: Khorshid Shamshiri, Asma
name: Afzaljavan, Fahimeh
name: Kerachian, Mohammad Amin
name: Fanipakdel, Azar
name: Aledavood, Seyed Amir
name: Allahyari, Abolghasem
name: Bari, Alireza
name: Moosanen Mozaffari, Hooman
name: Goshayeshi, Ladan
name: Pasdar, Alireza
Publisher: name: figshare
Year: 2022
Subjects: subject: Genetics
subject: FOS: Biological sciences

description: Additional file 1. Table S1. Distribution of SMAD7 Haplotypes among Colorectal Cancer Patients and Controls.
Trichonyssodrys aureopilosus Monne 1990
Creators: name: Monné, Miguel A.
Publisher: name: Zenodo
Year: 2005
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Coleoptera
Cerambycidae
Trichonyssodrys
Trichonyssodrys aureopilosus

description: 1. Trichonyssodrys aureopilosus Monné, 1990
Type locality — Venezuela, Aragua: Rancho Grande (1100 m). (FAUV). Distribution — Venezuela.
 Trichonyssodrys aureopilosus Monné, 1990b: 681, fig. 3.
description: Published as part of Monné, Miguel A., 2005, Catalogue of the Cerambycidae (Coleoptera) of the Neotropical Region. Part II. Subfamily Lamiinae, pp. 1-760 in Zootaxa 1023 (1) on pages 1-760, DOI: 10.11646/zootaxa.946.1.1, http://zenodo.org/record/5049553
Skyrmions in antiferromagnets: thermal stability and the effect of external field and impurities
Creators: name: Potkina, Maria N.
name: Lobanov, Igor S.
name: Jónsson, Hannes
name: Uzdin, Valery M.
Publisher: name: arXiv
Year: 2020
Subjects: subject: Materials Science (cond-mat.mtrl-sci)
subject: FOS: Physical sciences

description: Calculations of skyrmions in antiferromagnets (AFMs) are presented, and their properties compared with skyrmions in corresponding ferromagnets (FMs). The rates of skyrmion collapse and escape through the boundary of a track, as well as the binding to and collapse at a non-magnetic impurity, are calculated as a function of applied magnetic field. The activation energy for skyrmion annihilation is the same in AFMs and corresponding FMs in the absence of an applied magnetic field. The pre-exponential factor in the Arrhenius rate law is, however, different because skyrmion dynamics is different in the two systems. An applied magnetic field has opposite effects on skyrmions in the two types of materials. In AFMs the rate of collapse of skyrmions as well as the rate of escape through the edge of a magnetic strip decreases slightly with increasing field, while these rates increase strongly for a skyrmion in the corresponding FMs when the field is directed antiparallel to the magnetization in the center of the skyrmion. A non-magnetic impurity is less likely to trap a skyrmion in AFMs especially in the presence of a magnetic field. This, together with the established fact that a spin polarized current moves skyrmions in AFMs in the direction of the current, while in FMs skyrmions move at an angle to the current, demonstrates that skyrmions in AFMs have several advantageous properties over skyrmions in FMs for memory and spintronic devices.
The differential structure of the Brieskorn lattice
Creators: name: Schulze, Mathias
Publisher: name: arXiv
Year: 2003
Subjects: subject: Complex Variables (math.CV)
subject: FOS: Mathematics
subject: 32S35; 16S32

description: We describe an algorithm to compute M. Saito's matrices A0 and A1 for an isolated hypersurface singularity. They determine the differential structure of the Brieskorn lattice, the spectral pairs and Hodge numbers, and the complex monodromy of the singularity.
description: 10 pages, 0 figures, http://www.mathematik.uni-kl.de/~mschulze
Perceptions et pratiques des intervenants en soutien à l’autodétermination des personnes présentant une déficience intellectuelle, Revue Internationale de Communication et de socialisation,1(1), 23-49
Creators: name: Caouette, Martin
name: Lachapelle, Yves
Publisher: name: figshare
Year: 2020
Subjects: Education

description: Depuis une trentaine d’années, l’autodétermination occupe un espace croissant dans les différentes recherches réalisées en déficience intellectuelle (DI). Ce concept qui concerne le fait de gouverner sa vie sans influence externe indue amène les différents intervenants œuvrant auprès des personnes présentant une DI à adopter de nouvelles pratiques professionnelles favorables à l’autodétermination. Il devient donc indispensable de connaître les perceptions et les pratiques des intervenants en regard de l’autodétermination des personnes présentant une DI. Cette recension d’écrits présente les principales études qui ont traité de cette question. Au total, 10 études sont identifiées et présentées en fonction des 4 principaux thèmes abordés. Les résultats de ces études sont discutés et des implications pour la pratique et la recherche sont dégagées en conclusion.
Towards a comprehensive view of accretion, inner disks, and extinction in classical T Tauri stars: an ODYSSEUS study of the Orion OB1b association
Creators: name: Pittman, Caeley V.
name: Espaillat, Catherine C.
name: Robinson, Connor E.
name: Thanathibodee, Thanawuth
name: Calvet, Nuria
name: Wendeborn, John
name: Hernández, Jesus
name: Manara, Carlo F.
name: Walter, Fred
name: Ábrahám, Péter
name: Alcalá, Juan M.
name: Alencar, Sílvia H. P.
name: Arulanantham, Nicole
name: Cabrit, Sylvie
name: Eislöffel, Jochen
name: Fiorellino, Eleonora
name: France, Kevin
name: Gangi, Manuele
name: Grankin, Konstantin
name: Herczeg, Gregory J.
name: Kóspál, Ágnes
name: Mendigutía, Ignacio
name: Serna, Javier
name: Venuti, Laura
Publisher: name: arXiv
Year: 2022
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: FOS: Physical sciences

description: The coevolution of T Tauri stars and their surrounding protoplanetary disks dictates the timescales of planet formation. In this paper, we present magnetospheric accretion and inner disk wall model fits to NUV-NIR spectra of nine classical T Tauri stars in Orion OB1b as part of the Outflows and Disks around Young Stars: Synergies for the Exploration of ULLYSES Spectra (ODYSSEUS) Survey. Using NUV-optical spectra from the Hubble UV Legacy Library of Young Stars as Essential Standards (ULLYSES) Director's Discretionary Program and optical-NIR spectra from the PENELLOPE VLT Large Programme, we find that the accretion rates of these targets are relatively high for the region's intermediate age of 5.0 Myr; rates range from $0.5-17.2 \times 10^{-8}$ M$_{\odot}$/yr, with a median value of $1.2\times 10^{-8}$ M$_{\odot}$/yr. The NIR excesses can be fit with 1200-1800 K inner disk walls located at 0.05-0.10 AU from the host stars. We discuss the significance of the choice in extinction law, as the measured accretion rate depends strongly on the adopted extinction value. This analysis will be extended to the complete sample of T Tauri stars being observed through ULLYSES to characterize accretion and inner disks in star-forming regions of different ages and stellar populations.
description: 22 pages, 3 figures, 8 tables. Accepted for publication in AJ