cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
SN 2003du: Signatures of the Circumstellar Environment in a Normal Type Ia Supernova?
Creators: name: Gerardy, C. L.
name: Hoeflich, P.
name: Fesen, R. A.
name: Marion, G. H.
name: Nomoto, K.
name: Quimby, R.
name: Schaefer, B. E.
name: Wang, L.
name: Wheeler, J. C.
Publisher: name: arXiv
Year: 2003
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present observations of the Type Ia supernova 2003du and report the detectionof an unusual, high-velocity component in the Ca II infrared triplet, similar tofeatures previously observed in SN 2000cx and SN 2001el. This feature exhibits a large expansion velocity (~18,000 km/s) which is nearly constant between -7 and +2 days relative to maximum light, and disappears shortly thereafter. Otherthan this feature, the spectral evolution and light curve resemble those of a normal SN Ia. We find that the Ca II feature can plausibly be caused by a dense shell formed when circumstellar material of solar abundance is overrun by the rapidly expanding outermost layers of the SN ejecta. Model calculations show that the optical and infrared spectra are remarkably unaffected by the circumstellar interaction. In particular, no hydrogen lines are detectable in either absorption or emission. The only qualitatively different features are the strong, high-velocity feature in the Ca II IR-triplet, and a somewhat weaker O I feature near 7,300 AA. The morphology and time evolution of these features provide an estimate for the amount of accumulated matter and an indication of the mixing in the dense shell. We apply these diagnostic tools to SN 2003du and infer that about 2 x 10^{-2} M_sun of solar abundance material may have accumulated in a circumstellar shell prior to the observations. Furthermore, the early light curve data imply that the circumstellar material was originally very close to the progenitor system, perhaps from an accretion disk, Roche lobe or common envelope.
description: 35 Pages, 11 Figures, to appear in ApJ. Resubmission includes expanded discussion & new figures to match with accepted journal version
Additional file 1 of Lists of potential diagnoses that final-year medical students need to consider: a modified Delphi study
Creators: name: Urushibara-Miyachi, Yuka
name: Kikukawa, Makoto
name: Masatomi Ikusaka
name: Otaki, Junji
name: Nishigori, Hiroshi
Publisher: name: figshare
Year: 2021
Subjects: subject: Medicine
subject: Genetics
subject: FOS: Biological sciences
subject: Biotechnology
subject: Sociology
subject: FOS: Sociology
subject: 69999 Biological Sciences not elsewhere classified
subject: Science Policy
subject: 111714 Mental Health
subject: FOS: Health sciences
subject: 110309 Infectious Diseases

description: Additional file 1. The final lists consisted of basic diagnostic considerations and the lists of essential other than basic diseases as the potential diagnoses for 37 common signs, symptoms, and pathophysiology that Japanese medical students should master before graduation.
Anisakidae
Creators: name: Arai, Hisao P.
name: Smith, John W.
Publisher: name: Zenodo
Year: 2016
Subjects: Biodiversity
Taxonomy
Animalia
Nematoda
Secernentea
Ascaridida
Anisakidae

description: * Anisakidae gen. sp.
Sites: body cavity, intestinal lumen, mesenteries, peritoneum
Hosts: Gadus morhua (1); Hippoglossus hippoglossus (5); Pollachius virens (3); Prosopium williamsoni (2); Pseudopleuronectes americanus (6, 7); Reinhardtius hippoglossoides (5); Salmo salar (8); Sebastes fasciatus (4)
Distribution: Atlantic, British Columbia
Records: 1. Appy & Burt 1982 (AT); 2. Anon. 1984 (BC); 3. Scott 1985 (AT); 4. Scott 1988 (AT); 5. Scott & Bray 1989 (AT); 6. Khan et al. 1992 (AT); 7. Barker et al. 1994 (AT); 8. Marty 2008 (BC)
description: Published as part of Arai, Hisao P. & Smith, John W., 2016, Guide to the Parasites of Fishes of Canada Part V: Nematoda, pp. 1-274 in Zootaxa 4185 (1) on page 128, DOI: 10.11646/zootaxa.4185.1.1, http://zenodo.org/record/165530
Three cooperative mechanisms required for recovery after brain damage
Creators: name: Berger, Damian
name: Varriale, Emanuele
name: van Kessenich, Laurens Michiels
name: Herrmann, Hans J.
name: de Arcangelis, Lucilla
Publisher: name: arXiv
Year: 2019
Subjects: subject: Neurons and Cognition (q-bio.NC)
subject: FOS: Biological sciences

description: Stroke is one of the main causes of human disabilities. Experimental observations indicate that several mechanisms are activated during the recovery of functional activity after a stroke. Here we unveil how the brain recovers by explaining the role played by three mechanisms: Plastic adaptation, hyperexcitability and synaptogenesis. We consider two different damages in a neural network: A diffuse damage that simply causes the reduction of the effective system size and a localized damage, a stroke, that strongly alters the spontaneous activity of the system. Recovery mechanisms observed experimentally are implemented both separately and in a combined way. Interestingly, each mechanism contributes to the recovery to a limited extent. Only the combined application of all three together is able to recover the spontaneous activity of the undamaged system. This explains why the brain triggers independent mechanisms, whose cooperation is the fundamental ingredient for the system recovery.
Scars on quantum networks ignore the Lyapunov exponent
Creators: name: Schanz, Holger
name: Kottos, Tsampikos
Publisher: name: arXiv
Year: 2003
Subjects: subject: Chaotic Dynamics (nlin.CD)
subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: FOS: Physical sciences

description: We show that enhanced wavefunction localization due to the presence of short unstable orbits and strong scarring can rely on completely different mechanisms. Specifically we find that in quantum networks the shortest and most stable orbits do not support visible scars, although they are responsible for enhanced localization in the majority of the eigenstates. Scarring orbits are selected by a criterion which does not involve the classical Lyapunov exponent. We obtain predictions for the energies of visible scars and the distributions of scarring strengths and inverse participation ratios.
description: 5 pages, 2 figures
Kinetic measurement systems in Individuals Following Anterior Cruciate Ligaments Reconstruction: A Scoping Review Protocol
Creators: Labban, Wasim.
Stadnyk, Meredith. Sommerfeldt, Mark. Nathanail, Stephanie. Dennett, Liz. Westover, Lindsey. Manaseer, Thaer. Beaupre, Lauren
Publisher: name: University of Alberta Libraries
Year: 2020

Abstract
A New Empirical Model for the Structural Analysis of Early-type Galaxies and a Critical Review of the Nuker Model
Creators: name: Graham, Alister W.
name: Erwin, Peter
name: Trujillo, Ignacio
name: Ramos, Andres Asensio
Publisher: name: arXiv
Year: 2003
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: The Nuker law was designed to match the inner few (~3-10) arcseconds of predominantly nearby (< 30 Mpc) early-type galaxy light-profiles; it was never intended to describe an entire profile. The Sersic model, on the other hand, was developed to fit the entire profile; however, due to the presence of partially depleted galaxy cores, the Sersic model cannot always describe the very inner region. We have therefore developed a new empirical model consisting of an inner power-law, a transition region, and an outer Sersic model to connect the inner and outer structure of elliptical galaxies. Moreover, the stability of the Nuker model parameters are investigated. Surprisingly, none are found to be stable quantities; all are shown to vary systematically with a profile's fitted radial extent, and often by more than 100%. Considering elliptical galaxies spanning a range of 7.5 magnitudes, the central stellar density of the underlying host galaxy is observed to increase with galaxy luminosity until the onset of core formation, detected only in the brightest elliptical galaxies. We suggest that the so-called ``power-law'' galaxies may actually be described by the Sersic model over their entire radial range.
The Instanton Molecule Liquid and "Sticky Molasses" Above T_c
Creators: name: Brown, G. E.
name: Lee, C. -H.
name: Rho, M.
name: Shuryak, E.
Publisher: name: arXiv
Year: 2004
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: The main objective of this work is to explore the evolution in the structure of the quark-antiquark bound states in going down in the chirally restored phase from the so-called "zero binding points" T_zb to the QCD critical temperature T_c at which the Nambu-Goldstone and Wigner-Weyl modes meet. In doing this, we adopt the idea recently introduced by Shuryak and Zahed for charmed $\bar c c$, light-quark $\bar q q$ mesons $π, σ, ρ, A_1$ and gluons that at T_zb, the quark-antiquark scattering length goes through infinity at which conformal invariance is restored, thereby transforming the matter into a near perfect fluid behaving hydrodynamically, as found at RHIC. We show that the binding of these states is accomplished by the combination of (i) the color Coulomb interaction, (ii) the relativistic effects, and (iii) the interaction induced by the instanton-anti-instanton molecules. The spin-spin forces turned out to be small. While near T_zb all mesons are large-size nonrelativistic objects bound by Coulomb attraction, near T_c they get much more tightly bound, with many-body collective interactions becoming important and making the $σ$ and $π$ masses approach zero (in the chiral limit). The wave function at the origin grows strongly with binding, and the near-local four-Fermi interactions induced by the instanton molecules play an increasingly more important role as the temperature moves downward toward T_c.
description: Contribution to QM2004 proceedings, 4 pages
Nonlinear spherical gravitational downfall of gas onto a solid ball: analytic and numerical results
Creators: name: Gaite, Jose
name: Zorzano, Maria Paz
Publisher: name: arXiv
Year: 2003
Subjects: subject: Exactly Solvable and Integrable Systems (nlin.SI)
subject: Astrophysics (astro-ph)
subject: Fluid Dynamics (physics.flu-dyn)
subject: FOS: Physical sciences

description: The process of downfall of initially homogeneous gas onto a solid ball due to the ball's gravity (relevant in astrophysical situations) is studied with a combination of analytic and numerical methods. The initial explicit solution soon becomes discontinuous and gives rise to a shock wave. Afterwards, there is a crossover between two intermediate asymptotic similarity regimes, where the shock wave propagates outwards according to two self-similar laws, initially accelerating and eventually decelerating and vanishing, leading to a static state. The numerical study allows one to investigate in detail this dynamical problem and its time evolution, verifying and complementing the analytic results on the initial solution, intermediate self-similar laws and static long-term solution.
description: 19 pages, 10 PS figures (some large)
Deep learning predictions of galaxy merger stage and the importance of observational realism
Creators: name: Bottrell, Connor
name: Hani, Maan H.
name: Teimoorinia, Hossen
name: Ellison, Sara L.
name: Moreno, Jorge
name: Torrey, Paul
name: Hayward, Christopher C.
name: Thorp, Mallory
name: Simard, Luc
name: Hernquist, Lars
Publisher: name: arXiv
Year: 2019
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: Machine learning is becoming a popular tool to quantify galaxy morphologies and identify mergers. However, this technique relies on using an appropriate set of training data to be successful. By combining hydrodynamical simulations, synthetic observations and convolutional neural networks (CNNs), we quantitatively assess how realistic simulated galaxy images must be in order to reliably classify mergers. Specifically, we compare the performance of CNNs trained with two types of galaxy images, stellar maps and dust-inclusive radiatively transferred images, each with three levels of observational realism: (1) no observational effects (idealized images), (2) realistic sky and point spread function (semi-realistic images), (3) insertion into a real sky image (fully realistic images). We find that networks trained on either idealized or semi-real images have poor performance when applied to survey-realistic images. In contrast, networks trained on fully realistic images achieve 87.1% classification performance. Importantly, the level of realism in the training images is much more important than whether the images included radiative transfer, or simply used the stellar maps (87.1% compared to 79.6% accuracy, respectively). Therefore, one can avoid the large computational and storage cost of running radiative transfer with a relatively modest compromise in classification performance. Making photometry-based networks insensitive to colour incurs a very mild penalty to performance with survey-realistic data (86.0% with r-only compared to 87.1% with gri). This result demonstrates that while colour can be exploited by colour-sensitive networks, it is not necessary to achieve high accuracy and so can be avoided if desired. We provide the public release of our statistical observational realism suite, RealSim, as a companion to this paper.
description: MNRAS accepted. 25 pages, 15 figures, 4 tables. RealSim: https://github.com/cbottrell/RealSim
Quantum Doubles from a Class of Noncocommutative Weak Hopf Algebras
Creators: name: Li, Fang
name: Zhang, Yao-Zhong
Publisher: name: arXiv
Year: 2004
Subjects: subject: Quantum Algebra (math.QA)
subject: Mathematical Physics (math-ph)
subject: Rings and Algebras (math.RA)
subject: FOS: Mathematics
subject: FOS: Physical sciences

description: The concept of biperfect (noncocommutative) weak Hopf algebras is introduced and their properties are discussed. A new type of quasi-bicrossed products are constructed by means of weak Hopf skew-pairs of the weak Hopf algebras which are generalizations of the Hopf pairs introduced by Takeuchi. As a special case, the quantum double of a finite dimensional biperfect (noncocommutative) weak Hopf algebra is built. Examples of quantum doubles from a Clifford monoid as well as a noncommutative and noncocommutative weak Hopf algebra are given, generalizing quantum doubles from a group and a noncommutative and noncocommutative Hopf algebra, respectively. Moreover, some characterisations of quantum doubles of finite dimensional biperfect weak Hopf algebras are obtained.
description: LaTex 18 pages, to appear in J. Math. Phys. (To compile, need pb-diagram.sty, pb-lams.sty, pb-xy.sty and lamsarrow.sty)
Development and standardization of the University of Cincinnati Auditory Processing Inventory (UCAPI)†
Creators: name: Keith, Robert W.
name: Tektas, Melisa
name: Ramsay, Kendall
name: Delaney, Sarah
Publisher: name: Taylor & Francis
Year: 2020
Subjects: subject: Medicine
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: Science Policy

description: Objective: A literature review found that questionnaires for persons with problems of listening seeking assessment of auditory processing skills are not applicable for adolescents and adults. We developed a questionnaire designed for adolescents and adults seeking evaluation of problems with listening or following diagnosis to determine the subject’s status.Design: Following a model described by Del Zoppo, Sanchez, and Lind, a 34-item questionnaire was developed that investigates auditory processing abilities in six common areas of complaint in Auditory processing disorders (APD) (Keith, et al. 2017).Sample:The questionnaire was administered to 278 typically-achieving young adults and normative values of performance were developed. Validation data were acquired from 3 studies of subjects with language-learning or auditory processing disorders.Results:The total UCAPI score found by combining the totals from the six listening conditions provides an overall value to categorise listening abilities. The listening conditions provide an auditory profile for the person being evaluated. Finally, UCAPI scores obtained from subjects with a previous diagnosis of APD were substantially poorer than typical subjects, data that provide evidence of the validity of questionnaire validity.Conclusions: Results from the UCAPI can be useful to professionals in helping to make recommendations when diagnosing problems of learning through listening, as well as aid in developing management strategies.
Anisakinae
Creators: name: Arai, Hisao P.
name: Smith, John W.
Publisher: name: Zenodo
Year: 2016
Subjects: Biodiversity
Taxonomy
Animalia
Nematoda
Secernentea
Ascaridida
Anisakidae

description: * Anisakinae gen. sp.
Sites: mesenteries, musculature, stomach, viscera
Hosts: Clupea harengus (1, 2); Glyptocephalus cynoglossus (4); Hippoglossoides platessoides (4); Hippoglossus hippoglossus (4); Limanda ferrugineus (4); Pleuronectes putnami (4); Pseudopleuronectes americanus (4); Scophthalmus aquosus (4); Sebastes fasciatus (5); Sebastes mentella (5); Sebastes norvegicus (3)
Distribution: Atlantic
Records: 1. Sindermann 1957; 2. Sindermann 1961a; 3. Sindermann 1961b; 4. Ronald 1963; 5. Moran et al. 1996
Tribe CONTRACAECINEA: genera Contracaecum and Phocascaris
The species of these two genera are defined by characteristics of the adults. It is difficult therefore to assign larvae
to any one species, and impossible to design a key for their reliable identification (Moravec 2013). Feeding
experiments to rear larvae to adults and/or the application of molecular markers to aid identification of species may
help solve these problems. Brattey (1995) used discriminant function analysis to reveal differences in shape among
larvae of Contracaecum and Phocascaris. He reported that larvae of Phocascaris sp. and C. osculatum B can
generally be distinguished by the use of three measurements (body length, and widths at mid-length and at the base
of the intestinal caecum) although larvae of C. osculatum A could not be reliably distinguished from the other two
species. The following taxa are included as their names have appeared in the relevant Canadian literature.
description: Published as part of Arai, Hisao P. & Smith, John W., 2016, Guide to the Parasites of Fishes of Canada Part V: Nematoda, pp. 1-274 in Zootaxa 4185 (1) on page 128, DOI: 10.11646/zootaxa.4185.1.1, http://zenodo.org/record/165530
Optical Flash of GRB 990123: constraints on the physical parameter of the reverse shock
Creators: name: Fan, Y. Z.
name: Dai, Z. G.
name: Huang, Y. F.
name: Lu, T.
Publisher: name: arXiv
Year: 2003
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: The optical flash accompanying GRB 990123 is believed to be powered by the reverse shock of a thin shell. With the best fitted physical parameters for GRB 990123 (Panaitescu & Kumar 2001) and the assumption that the parameters in the optical flash are the same as those in the afterglow, we show that: 1) the shell is thick but not thin, and we have provided the light curve for the thick shell case which coincides with the observation; 2) the theoretical peak flux of the optical flash accounts for only 3\times10^{-4} of the observed. In order to compensate this divergency, the physical parameters the electron energy ration and the magnetic ratio $ε_e$, $ε_B$ should be 0.61, 0.39 respectively, which are much different from those in the late afterglow.
description: 7 pages, no figure
Thermodynamically-Efficient Local Computation and the Inefficiency of Quantum Memory Compression
Creators: name: Loomis, Samuel P.
name: Crutchfield, James P.
Publisher: name: arXiv
Year: 2020
Subjects: subject: Quantum Physics (quant-ph)
subject: Statistical Mechanics (cond-mat.stat-mech)
subject: Information Theory (cs.IT)
subject: Chaotic Dynamics (nlin.CD)
subject: FOS: Physical sciences
subject: FOS: Computer and information sciences

description: Modularity dissipation identifies how locally-implemented computation entails costs beyond those required by Landauer's bound on thermodynamic computing. We establish a general theorem for efficient local computation, giving the necessary and sufficient conditions for a local operation to have zero modularity cost. Applied to thermodynamically-generating stochastic processes it confirms a conjecture that classical generators are efficient if and only if they satisfy retrodiction, which places minimal memory requirements on the generator. This extends immediately to quantum computation: Any quantum simulator that employs quantum memory compression cannot be thermodynamically efficient.
description: 12 pages, 4 figures; supplementary material 18 pages, 1 figure; http://csc.ucdavis.edu/~cmg/compmech/pubs/telc.htm
Parsec-Scale Radio Structure of the Double Active Nucleus of NGC 6240
Creators: name: Gallimore, Jack F.
name: Beswick, Robert
Publisher: name: arXiv
Year: 2003
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: NGC 6240 is a luminous infrared galaxy that, based on recent MERLIN and CHANDRA observations, appears to host a pair of active galactic nuclei. We present new, multiepoch and multifrequency radio observations of NGC 6240 obtained using the Very Long Baseline Array (VLBA). These observations resolve out all of the diffuse radio continuum emission related to starburst activity to reveal three compact sources, two associated with the infrared and X-ray nuclei: components N1, the northern nucleus, and S, the southern nucleus; and component S1, a weak point source lying northeast of component S. The radio continuum properties of N1 and S both resemble those of compact radio sources in Seyfert nuclei, including an inverted spectrum at low frequencies and high brightness temperatures. Component N1 further resolves into a 9 pc linear source, again resembling compact jets in some well-studied Seyfert nuclei. The inverted radio spectrum is most likely caused by free-free absorption through foreground plasma with emission measures of order 1E7 cm^(-6) pc, consistent with the X-ray spectroscopy which infers the presence of a foreground, Compton thick absorber. Synchrotron self-absorption may also contribute to the flat spectrum of component S. Component S1 better resembles a luminous radio supernova such as those detected in Arp 220, although we cannot specifically rule out the possibility that S1 may be ejected material from the southern active nucleus. We demonstrate that the light curve of S1 is at least consistent with current radio supernova models, and, given the high star-formation rate in the nuclear region and the (possible) proclivity of infrared merger galaxies to produce luminous RSNe, it is not surprising that one such supernova is detected serendipitously in the VLBA observations.
description: Accepted for publication in the Astronomical Journal. 38 pages PDF generated by MS Word and Adobe Acrobat. Larger PDF with better quality figures available at http://www.eg.bucknell.edu/physics/gallimore/research.htm
Additional file 1 of Validation of 18F-FDG PET/MRI and diffusion-weighted MRI for estimating the extent of peritoneal carcinomatosis in ovarian and endometrial cancer -a pilot study
Creators: name: Jónsdóttir, Björg
name: Ripoll, Montserrat Alemany
name: Bergman, Antonina
name: Silins, Ilvars
name: Poromaa, Inger Sundström
name: Ahlström, Håkan
name: Stålberg, Karin
Publisher: name: figshare
Year: 2021
Subjects: subject: Medicine
subject: Cell Biology
subject: Neuroscience
subject: Physiology
subject: FOS: Biological sciences
subject: Cancer
subject: 111714 Mental Health
subject: FOS: Health sciences

description: Additional file 1.
Additional file 1 of Vaspin in atherosclerotic disease and cardiovascular risk in axial spondyloarthritis: a genetic and serological study
Creators: name: Rueda-Gotor, Javier
name: López-Mejías, Raquel
name: Remuzgo-Martínez, Sara
name: Pulito-Cueto, Verónica
name: Corrales, Alfonso
name: Lera-Gómez, Leticia
name: Portilla, Virginia
name: González-Mazón, Íñigo
name: Blanco, Ricardo
name: Expósito, Rosa
name: Mata, Cristina
name: Llorca, Javier
name: Hernández-Hernández, Vanesa
name: Rodríguez-Lozano, Carlos
name: Barbarroja, Nuria
name: Castro, Rafaela Ortega
name: Vicente, Esther
name: Fernández-Carballido, Cristina
name: Martínez-Vidal, María Paz
name: Castro-Corredor, David
name: Anino-Fernández, Joaquín
name: Peiteado, Diana
name: Chamaida Plasencia-Rodríguez
name: Galíndez-Agirregoikoa, Eva
name: García-Vivar, María Luz
name: Gualillo, Oreste
name: Quevedo-Abeledo, Juan Carlos
name: Castañeda, Santos
name: Ferraz-Amaro, Iván
name: González-Gay, Miguel Á.
name: Genre, Fernanda
Publisher: name: figshare
Year: 2021
Subjects: subject: Biochemistry
subject: Medicine
subject: Genetics
subject: FOS: Biological sciences
subject: 59999 Environmental Sciences not elsewhere classified
subject: FOS: Earth and related environmental sciences
subject: Immunology
subject: FOS: Clinical medicine
subject: 69999 Biological Sciences not elsewhere classified
subject: Cancer
subject: Science Policy

description: Additional file 1: Supplementary Table 1. Demographic, clinical, laboratory, and cardiovascular disease-related characteristics in patients with axial spondyloarthritis carrying or not the A allele of vaspin rs7159023.
An on-average Maeda-type conjecture in the level aspect
Creators: name: Martin, Kimball
Publisher: name: arXiv
Year: 2019
Subjects: subject: Number Theory (math.NT)
subject: FOS: Mathematics

description: We present a conjecture on the average number of Galois orbits of newforms when fixing the weight and varying the level. This conjecture implies, for instance, that the central L-values (resp. L-derivatives) are nonzero for 100% of even weight prime level newforms with root number +1 (resp. -1).
description: 12 pages
Time-course transcriptomic alterations reflect the pathophysiology of polyhexamethylene guanidine phosphate-induced lung injury in rats
Creators: name: Song, Mi-Kyung
name: Kim, Dong Im
name: Kyuhong Lee
Publisher: name: Taylor & Francis
Year: 2020
Subjects: subject: Medicine
subject: Cell Biology
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: 59999 Environmental Sciences not elsewhere classified
subject: FOS: Earth and related environmental sciences
subject: Immunology
subject: FOS: Clinical medicine
subject: 69999 Biological Sciences not elsewhere classified
subject: Cancer

description: Objective: Humidifier-disinfectant-induced lung injury is a new syndrome associated with a high mortality rate and characterized by severe hypersensitivity pneumonitis, acute interstitial pneumonia, or acute respiratory distress syndrome. Polyhexamethylene guanidine phosphate (PHMG-P), a guanidine-based antimicrobial agent, is a major component associated with severe lung injury. In-depth studies are needed to determine how PHMG-P affects pathogenesis at the molecular level. Therefore, in this study, we analyzed short-term (4 weeks) and long-term (10 weeks) PHMG-P-exposure-specific gene-expression patterns in rats to improve our understanding of time-dependent changes in fibrosis. Materials and methods: Gene-expression profiles were analyzed in rat lung tissues using DNA microarrays and bioinformatics tools. Results: Clustering analysis of gene-expression data showed different gene-alteration patterns in the short- and long-term exposure groups and higher sensitivity to gene-expression changes in the long-term exposure group than in the short-term exposure group. Supervised analysis revealed 34 short-term and 335 long-term exposure-specific genes, and functional analysis revealed that short-term exposure-specific genes were involved in PHMG-P-induced initial inflammatory responses, whereas long-term exposure-specific genes were involved in PHMG-P-related induction of chronic lung fibrosis. Conclusion: The results of transcriptomic analysis were consistent with lung histopathology results. These findings indicated that exposure-time-specific changes in gene expression closely reflected time-dependent pathological changes in PHMG-P-induced lung injury.
A Deep Chandra Observation of the Distant Galaxy Cluster MS1137.5+6625
Creators: name: Grego, Laura
name: Vrtilek, Jan
name: Van Speybroeck, Leon
name: David, Laurence P.
name: Forman, William
name: Carlstrom, John E.
name: Reese, Erik D.
name: Joy, Marshall K.
Publisher: name: arXiv
Year: 2004
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present results from a deep Chandra observation of MS1137.5+66, a distant (z=0.783) and massive cluster of galaxies. Only a few similarly massive clusters are currently known at such high redshifts; accordingly, this observation provides much-needed information on the dynamical state of these rare systems. The cluster appears both regular and symmetric in the X-ray image. However, our analysis of the spectral and spatial X-ray data in conjunction with interferometric Sunyaev-Zel'dovich effect data and published deep optical imaging suggests the cluster has a fairly complex structure. The angular diameter distance we calculate from the Chandra and Sunyaev-Zel'dovich effect data assuming an isothermal, spherically symmetric cluster implies a low value for the Hubble constant for which we explore possible explanations.
description: 16 pages, 6 figures, submitted to ApJ
Nine New Repeating Fast Radio Burst Sources from CHIME/FRB
Creators: name: Fonseca, E.
name: Andersen, B. C.
name: Bhardwaj, M.
name: Chawla, P.
name: Good, D. C.
name: Josephy, A.
name: Kaspi, V. M.
name: Masui, K. W.
name: Mckinven, R.
name: Michilli, D.
name: Pleunis, Z.
name: Shin, K.
name: Tendulkar, S. P.
name: Bandura, K. M.
name: Boyle, P. J.
name: Brar, C.
name: Cassanelli, T.
name: Cubranic, D.
name: Dobbs, M.
name: Dong, F. Q.
name: Gaensler, B. M.
name: Hinshaw, G.
name: Landecker, T. L.
name: Leung, C.
name: Li, D. Z.
name: Lin, H. -H.
name: Mena-Parra, J.
name: Merryfield, M.
name: Naidu, A.
name: Ng, C.
name: Patel, C.
name: Pen, U.
name: Rafiei-Ravandi, M.
name: Rahman, M.
name: Ransom, S. M.
name: Scholz, P.
name: Smith, K. M.
name: Stairs, I. H.
name: Vanderlinde, K.
name: Yadav, P.
name: Zwaniga, A. V.
Publisher: name: arXiv
Year: 2020
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: We report on the discovery and analysis of bursts from nine new repeating fast radio burst (FRB) sources found using the Canadian Hydrogen Intensity Mapping Experiment (CHIME) telescope. These sources span a dispersion measure (DM) range of 195 to 1380 pc cm$^{-3}$. We detect two bursts from three of the new sources, three bursts from four of the new sources, four bursts from one new source, and five bursts from one new source. We determine sky coordinates of all sources with uncertainties of $\sim$10$^\prime$. We detect Faraday rotation measures for two sources, with values $-20(1)$ and $-499.8(7)$ rad m$^{-2}$, that are substantially lower than the RM derived from bursts emitted by FRB 121102. We find that the DM distribution of our events, combined with the nine other repeaters discovered by CHIME/FRB, is indistinguishable from that of thus far non-repeating CHIME/FRB events. However, as previously reported, the burst widths appear statistically significantly larger than the thus far non-repeating CHIME/FRB events, further supporting the notion of inherently different emission mechanisms and/or local environments. These results are consistent with previous work, though are now derived from 18 repeating sources discovered by CHIME/FRB during its first year of operation. We identify candidate galaxies that may contain FRB 190303.J1353+48 (DM = 222.4 pc cm$^{-3}$).
description: Accepted for publication in ApJL
Additional file 1 of How to disseminate national recommendations for physical activity: a qualitative analysis of critical change agents in Germany
Creators: name: Wolbring, Laura
name: Reimers, Anne Kerstin
name: Niessner, Claudia
name: Demetriou, Yolanda
name: Schmidt, Steffen Christian Ekkehard
name: Woll, Alexander
name: Wäsche, Hagen
Publisher: name: figshare
Year: 2021
Subjects: subject: Medicine
subject: Biotechnology
subject: 59999 Environmental Sciences not elsewhere classified
subject: FOS: Earth and related environmental sciences
subject: Science Policy
subject: Cancer

description: Additional file 1. Recommendations for action.
Contracaecum osculatum (Rudolphi, 1802) Baylis 1920
Creators: name: Arai, Hisao P.
name: Smith, John W.
Publisher: name: Zenodo
Year: 2016
Subjects: Biodiversity
Taxonomy
Animalia
Nematoda
Secernentea
Ascaridida
Anisakidae
Contracaecum
Contracaecum osculatum

description: * Contracaecum osculatum (Rudolphi, 1802) Baylis, 1920 (sensu lato)
Includes: * C. osculatum A auct.; * C. osculatum B auct.; and * C. osculatum C auct.
Description (after J. W. Smith & Wootten 1984c, and Moravec 2013). NB: the following description applies also to
* Phocascaris sp. and/or * Contracaecum sp. (see below). Greenish brown in colour, sometimes tinged with red, L3
about 7 to 30 long, lying coiled in capsules of irregular shape (J. W. Smith & Wootten 1984c). Mouth, lips, boring
tooth, and excretory pore similar to those of Anisakis simplex L3 (see Fig. 73 A,B,C).
According to Moravec (2013), L3 are 3.81–22.00 long, maximum width 0.15–0.53. Oesophagus 0.55–1.71 long,
ventricular appendix 0.54–1.58, and intestinal caecum 0.20–0.89. Single excretory cell extends posteriorly to mid-
body region. Tail 0.09–0.21 long, narrows rapidly to a point lacking a mucron. Anterior and posterior ends of an L3
shown diagrammatically in Fig. 75 A,B.
Sites: intestinal lumen, mesenteries, musculature, viscera
Hosts: Boreogadus saida (13); Gadus macrocephalus (11); Gadus morhua (1, 4, 5, 7, 8, 9, 10, 14, 16); Glyptocephalus cynoglossus (1); Hippoglossoides platessoides (10); Hippoglossus hippoglossus (11); Mallotus villosus (10); Myoxocephalus scorpius (10); Oncorhynchus mykiss (6); Oncorhynchus tshawytscha (12); Pseudopleuronectes americanus (10); Theragra chalcogramma (11); Urophycis tenuis (5, 15); unspecified “fish” (2, 3)
Distribution: Atlantic, Nunavut, Pacific
Records: 1. McClelland et al. 1985 (AT); 2. Berland et al. 1989 (AT); 3. Burt et al. 1989a (AT); 4. Brattey et al.
1990 (AT); 5. McClelland et al. 1990 (AT); 6. J. W. Smith et al. 1990 (EX, AT); 7. Likely & Burt 1992 (AT); 8. Marcogliese & Boily 1994 (AT); 9. McClelland & Marcogliese 1994 (AT); 10. Brattey 1995 (AT); 11. Paggi et al. 1998 (PA); 12. Urawa et al. 1998 (PA); 13. Køie 2009 (NU); 14. Khan et al. 2011 (AT); 15. Melendy et al. 2005 (AT); 16. McClelland & Melendy 2011 (AT)
description: Published as part of Arai, Hisao P. & Smith, John W., 2016, Guide to the Parasites of Fishes of Canada Part V: Nematoda, pp. 1-274 in Zootaxa 4185 (1) on pages 128-129, DOI: 10.11646/zootaxa.4185.1.1, http://zenodo.org/record/165530
Is pi Men c's atmosphere hydrogen-dominated? Insights from a non-detecton of Hy Ly-alpha absorption
Creators: name: Muñoz, Antonio García
name: Youngblood, Allison
name: Fossati, Luca
name: Gandolfi, Davide
name: Cabrera, Juan
name: Rauer, Heike
Publisher: name: arXiv
Year: 2019
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: FOS: Physical sciences

description: Constraining the composition of super-Earth-to-sub-Neptune-size planets is a priority to understand the processes of planetary formation and evolution. pi Men c represents a unique target for the atmospheric and compositional characterization of such planets because it is strongly irradiated and its bulk density is consistent with abundant H2O. We searched for hydrogen from photodissociating H2/H2O in pi Men c's upper atmosphere through H i Ly-alpha transmission spectroscopy with the Hubble Space Telescope's STIS instrument, but did not detect it. We set 1 (3) upper limits for the effective planet-to-star size ratio RLy-alpha/Rearth=0.13 (0.24) and 0.12 (0.20) at velocities [-215,-91] km/s and [+57,+180] km/s, respectively. We reconstructed the stellar spectrum, and estimate that Men c receives about 1350 erg cm-2 s-1 of 5-912-Angstroms-energy, enough to cause rapid atmospheric escape. An interesting scenario to explain the non-detection is that Men c's atmosphere is dominated by H2O or other heavy molecules rather than H2/He. According to our models, abundant oxygen results in less extended atmospheres, which transition from neutral to ionized hydrogen closer to the planet. We compare our non-detection to other detection attempts, and tentatively identify two behaviors: planets with densities <2 g cm-3 (and likely hydrogen-dominated atmospheres) result in H i Ly-alpha absorption, whereas planets with densities >3 g cm-3 (and plausibly non-hydrogen-dominated atmospheres) do not result in measurable absorption. Investigating a sample of strongly-irradiated sub-Neptunes may provide some statistical confirmation if it is shown that they do not generally develop extended atmospheres.
description: Accepted for publication in the Astrophysical Journal Letters. 30 pages, 6+2 figures, 1+1 tables
Dynamical Friction of Galactic Center Star Clusters with an Intermediate-Mass Black Hole
Creators: name: Kim, Sungsoo S.
name: Figer, Donald F.
name: Morris, Mark
Publisher: name: arXiv
Year: 2004
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Numerical simulations of the dynamical friction suffered by a Galactic center star cluster harboring an intermediate-mass black hole (IMBH) have been performed. Gerhard has suggested that dynamical friction, which causes a cluster to lose orbital energy and spiral in toward the Galactic center, may explain the presence of a cluster of very young stars in the central parsec, where star formation might be prohibitively difficult because of strong tidal forces. However, numerical simulations by Kim & Morris showed that this is only possible if the cluster initially has an extremely dense core. Hansen & Milosavljevic recently suggested that the presence of an IMBH in the cluster core might stabilize the core against tidal disruption during the inspiral through dynamical friction, and thus might easily deliver young stars down to the central parsec. We find that the presence of an IMBH does lower the minimum initial core density required to transport young stars down to the central parsec, but this is possible only when the mass of the IMBH is at least ~10% of the total cluster mass. This fraction is significantly higher than that estimated by Portegies Zwart & McMillan with numerical simulations of IMBH formation by successive merging of stars in the cluster core, so it does not appear that a realistic IMBH can help transport young stars into the central parsec.
description: To appear in ApJ, 607, L123 (June 1, 2004)
title: Fiche – questionnaire pour l’investigateur
Creators: name: Leibowitch, Jacques (1942-2020)
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2020
Subjects: Lipodystrophies

description: En-tête : Essai CINQ A ZERO / CINQ A QUATRE Lipodystrophie
description: created: start=2000;end=2003
Representation stability for sequences of 0-Hecke modules
Creators: name: Laudone, Robert P.
Publisher: name: arXiv
Year: 2019
Subjects: subject: Representation Theory (math.RT)
subject: Commutative Algebra (math.AC)
subject: Combinatorics (math.CO)
subject: FOS: Mathematics
subject: 13A50, 13C05, 16P40, 05E05, 05E10

description: We define a new category analogous to ${\bf FI}$ for the $0$-Hecke algebra $H_n(0)$ called the $0$-Hecke category, $\mathcal{H}$, indexing sequences of representations of $H_n(0)$ as $n$ varies under suitable compatibility conditions. We establish a new type of representation stability in this setting and prove it is implied by being a finitely generated $\mathcal{H}$-module. We then provide examples of $\mathcal{H}$-modules and discuss further desirable properties these modules possess.
description: 51 pages
Bright Lyman Break Galaxy Candidates in the Sloan Digital Sky Survey First Data Release
Creators: name: Bentz, Misty C.
name: Osmer, Patrick S.
name: Weinberg, David H.
Publisher: name: arXiv
Year: 2003
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: {Abridged} We report the discovery of six compact, starburst galaxy candidates with redshifts 2.3 < z < 2.8 and r-band magnitudes 19.8-20.5 in the Quasar Catalog of the Sloan Digital Sky Survey First Data Release (SDSS DR1). The SDSS spectra of these objects resemble the composite spectrum of Lyman Break Galaxies (LBGs) at z ~ 3 (albeit with some differences and broader spectral lines), but the systems are 4-5 magnitudes brighter than an ``L*'' LBG and 2-3 magnitudes brighter than the most luminous objects in typical LBG spectroscopic surveys. These objects could be extremely luminous LBGs, normal LBGs amplified by gravitational lensing (like MS 1512-cB58), or a rare class of unusual BAL quasars. Under the first hypothesis, star formation rates inferred from the UV continuum luminosities are about 300-1000 M_sun yr^-1 with no correction for dust extinction. The SDSS images show no evidence of multiple imaging or foreground lensing structures, but lensing amplification cannot be ruled out with the present data. The spectra have fairly broad absorption features and prominent high-ionization absorption, but they do not have high ionization emission lines, nor do they resemble spectra of known BAL quasars. Assuming that lensing and AGN contributions are unimportant, we estimate the high end of the z ~ 2.5 galaxy luminosity function, making the crude but conservative assumption of unit detection efficiency over our observed redshift and magnitude range. The estimated comoving space density is above a Schechter function extrapolation of the LBG luminosity function from fainter magnitudes. Improved optical spectra and measurements at X-ray, IR, and sub-mm wavelengths could help determine the nature of these remarkable objects.
description: 12 pages, 2 tables, 2 figures, submitted to ApJ Letters; replaced figure 1 and revised text in response to comments on the original version; final refereed version
Duality for Finite Multiple Harmonic q-Series
Creators: name: Bradley, David M.
Publisher: name: arXiv
Year: 2004
Subjects: subject: Combinatorics (math.CO)
subject: Number Theory (math.NT)
subject: FOS: Mathematics
subject: 05A30; 33D15

description: We define two finite q-analogs of certain multiple harmonic series with an arbitrary number of free parameters, and prove identities for these q-analogs, expressing them in terms of multiply nested sums involving the Gaussian binomial coefficients. Special cases of these identities--for example, with all parameters equal to 1--have occurred in the literature. The special case with only one parameter reduces to an identity for the divisor generating function, which has received some attention in connection with problems in sorting theory. The general case can be viewed as a duality result, reminiscent of the duality relation for the ordinary multiple zeta function.
description: 12 pages AMSLaTeX. Submitted for publication October 26, 2003; revised September 14, 2004. New title reflects change in emphasis and new section devoted to connections with inverse pairs and Hoffman duality. References added and typos corrected
Constraining the nuclear equation of state via gravitational-wave radiation of short gamma-ray burst remnants
Creators: name: Lan, Lin
name: Lü, Hou-Jun
name: Rice, Jared
name: Liang, En-Wei
Publisher: name: arXiv
Year: 2020
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: The observed internal plateau of X-ray emission in some short GRBs suggests the formation of a remnant supra-massive magnetar following a double neutron star (NS) merger. In this paper, we assume that the rotational energy is lost mainly via gravitational wave (GW) radiation instead of magnetic dipole (MD) radiation, and present further constraints on the NS nuclear equation of state (EoS) via mass quadrupole deformation and r-mode fluid oscillations of the magnetar. We present two short GRBs with measured redshifts, 101219A and 160821B, whose X-ray light curves exhibit an internal plateau. This suggests that a supra-massive NS may survive as the central engine. By considering twelve NS EoSs, within the mass quadrupole deformation scenario we find that the GM1, DD2, and DDME2 models give an $M_{\rm p}$ band falling within the 2$σ$ region of the proto-magnetar mass distribution for $\varepsilon=0.01$. This is consistent with the constraints from the MD radiation dominated model of rotational energy loss. However, for an r-mode fluid oscillation model with $α=0.1$ the data suggest that the NS EOS is close to the Shen and APR models, which is obviously different from the MD radiation dominated and mass quadrupole deformation cases.
description: 7 pages, 1 table, and 4 figures. ApJ in press, matched the published version
Contracaecum rudolphii Hartwich 1964
Creators: name: Arai, Hisao P.
name: Smith, John W.
Publisher: name: Zenodo
Year: 2016
Subjects: Biodiversity
Taxonomy
Animalia
Nematoda
Secernentea
Ascaridida
Anisakidae
Contracaecum
Contracaecum rudolphii

description: * Contracaecum rudolphii Hartwich, 1964
Synonym: Contracaecum spiculigerum auct. nec Rudolphi, 1809
Description (after Bartlett 1996, and Moravec 2013). Ten 87-day-old L3 from experimentally infected guppies Poecilia reticulata were 0.8–2.9 long, and 0.030–0.090 maximum width. Five 152-day-old L3 were 3.1–3.9 (mean 3.5) long, and 0.110–0.120 (0.114) maximum width. Older larvae were 15.0–24.0 long, and 0.9–2.1 wide. Mouth, lips, boring tooth, and excretory pore similar to those of Anisakis simplex L3 (see Fig. 76 A,B,C). Nerve ring 0.150– 0.200 (0.167) from anterior end. Length of preventriculus 0.370–0.415 (0.391), ventriculus 0.025–0.030 (0.029), ventricular appendix 0.320–0.380 (0.359), intestinal caecum 0.170–0.225 (0.191) [Fig. 76 A], and tail 0.085–0.090 (0.088) [Fig. 76 B].
Sites: body cavity, intestinal lumen, musculature
Hosts: Fundulus heteroclitus; Poecilia reticulata (EX)
Distribution: Nova Scotia
Record: Bartlett 1996
description: Published as part of Arai, Hisao P. & Smith, John W., 2016, Guide to the Parasites of Fishes of Canada Part V: Nematoda, pp. 1-274 in Zootaxa 4185 (1) on pages 130-131, DOI: 10.11646/zootaxa.4185.1.1, http://zenodo.org/record/165530
Phase diagram of the large $N$ Gross-Neveu model in a finite periodic box
Creators: name: Narayanan, Rajamani
Publisher: name: arXiv
Year: 2020
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: High Energy Physics - Lattice (hep-lat)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We analyze the Gross-Neveu model in the limit of large number of flavors of massless fermions. We study the phase diagram in a two and three dimensional periodic box at a fixed thermal to spatial aspect ratio, $\fracβ{\ell}$, with a flavor independent chemical potential. We assume the bilinear condensate, when one exists, has a specific momentum in the spatial direction(s). The main known features of the phase diagram in the $\ell\to\infty$ limit of the two dimensional model are also seen on a finite $\ell\timesβ$ torus -- a phase with a homogeneous (zero momentum) condensate; a phase with an inhomogeneous (non-zero momentum) condensate and a phase with no condensate. We observe that the inhomogeneous phase contains several sub-phases characterized by a specific spatial momentum. Unlike the two dimensional model, we do not find evidence for a phase with a inhomogeneous condensate in the three dimensional model.
description: 26 pages, 13 figures, Added one figure and one reference
Additional file 1 of Knowledge of prostate cancer presentation, etiology, and screening practices among women: a mixed-methods systematic review
Creators: name: Wiafe, Ebenezer
name: Mensah, Kofi Boamah
name: Adwoa Bemah Boamah Mensah
name: Bangalee, Varsha
name: Frasia Oosthuizen
Publisher: name: figshare
Year: 2021
Subjects: Medicine
Cell Biology
Biotechnology
Cancer
Science Policy

description: Additional file 1:. Proposed search strategy using Medline via EBSCOhost