cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Additional file 1: of Chest radiography versus lung ultrasound for identification of acute respiratory distress syndrome: a retrospective observational study
Creators: name: See, Kay
name: Ong, Venetia
name: Tan, Yi
name: Sahagun, Juliet
name: Juvel Taculod
Publisher: name: figshare
Year: 2018
Subjects: subject: Space Science
subject: Medicine
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: Developmental Biology

description: Table S1. Lung ultrasound reporting template. (DOCX 18 kb)
Spiral shocks in the accretion disc of IP Peg during outburst maximum
Creators: name: Harlaftis, E. T.
name: Steeghs, D.
name: Horne, K.
name: Martin, E.
name: Magazzu, A.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: In response to our recent discovery of spiral arms in the accretion disc of IP Peg during rise to outburst, we have obtained time-resolved spectrophotometry of IP Peg during outburst maximum. In particular, indirect imaging of HeII 4686, using Doppler tomography, shows a two-arm spiral pattern on the disc image, which confirms repeatability over different outbursts. The jump in HeII intensity (a factor of more than two) and in velocity (~200--300 km/s) clarifies the shock nature of the spiral structure. The HeII shocks show an azimuthal extent of ~90 degrees, a shallow power-law emissivity ~V^{-1}, an upper limit of 30 degrees in opening angle, and a flux contribution of 15 per cent of the total disc emission. We discuss the results in view of recent simulations of accretion discs which show that spiral shocks can be raised in the accretion disc by the secondary star.
description: 5 pages, 4 figures, MNRAS journal paper. in press
Larkin-Ovchinnikov-Fulde-Ferrell state in quasi-one-dimensional superconductors
Creators: name: Dupuis, N.
Publisher: name: arXiv
Year: 1994
Subjects: subject: Condensed Matter (cond-mat)
subject: FOS: Physical sciences

description: The properties of a quasi-one-dimensional (quasi-1D) superconductor with {\it an open Fermi surface} are expected to be unusual in a magnetic field. On the one hand, the quasi-1D structure of the Fermi surface strongly favors the formation of a non-uniform state (Larkin-Ovchinnikov-Fulde-Ferrell (LOFF) state) in the presence of a magnetic field acting on the electron spins. On the other hand, a magnetic field acting on an open Fermi surface induces a dimensional crossover by confining the electronic wave-functions wave-functions along the chains of highest conductivity, which results in a divergence of the orbital critical field and in a stabilization at low temperature of a cascade of superconducting phases separated by first order transistions. In this paper, we study the phase diagram as a function of the anisotropy. We discuss in details the experimental situation in the quasi-1D organic conductors of the Bechgaard salts family and argue that they appear as good candidates for the observation of the LOFF state, provided that their anisotropy is large enough. Recent experiments on the organic quasi-1D superconductor (TMTSF)$_2$ClO$_4$ are in agreement with the results obtained in this paper and could be interpreted as a signature of a high-field superconducting phase. We also point out the possibility to observe a LOFF state in some quasi-2D organic superconductors.
description: 24 pages+17 figures (upon request), RevTex, ORSAY-LPS-241094
Are you sure that the anisotropies in the microwave background radiation are really cosmological rather than purely Galactic in origin?
Creators: name: Lopez-Corredoira, M.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: New calculations of the Galactic contamination over microwave background radiation anisotropies are carried out. On one hand, when a frequency-dependent contrast of molecular clouds with respect to the Galactic background of the diffuse interstellar medium is taken into account, the anisotropic amplitude produced by Galactic dust is increased with respect to previous calculations and this is of the same order as that of the data from the observations. On the other hand, if we take into account rotational dust emission, for instance, a frequency independence of anisotropies in the microwave range may be obtained. This leads to the possibility that under some particular, but not impossible, conditions all the microwave background radiation anisotropies may be due to Galactic foregrounds rather than cosmological in origin. Moreover, a suspected coincidence between the typical angular sizes of the microwave background radiation anisotropies and those of nearby molecular clouds makes more plausible the hypothesis of a purely Galactic origin for these anisotropies. It is also argued that the correlation among structures at different frequencies, the comparison of the power spectrum at different frequencies and the galactic latitude dependence of the anisotropies are not yet proofs in favour of either a cosmological or Galactic origin.
description: 15 pages, 18 figures, to be published in A&A with a different title (to undergo censorship): "A conspicuous increase of Galactic contamination over CMBR anisotropies at large angular scales"
Additional file 1: of Objectively measured physical activity in population-representative parent-child pairs: parental modelling matters and is context-specific
Creators: name: Bringolf-Isler, Bettina
name: Schindler, Christian
name: Kayser, Bengt
name: L. Suzanne Suggs
name: Probst-Hensch, Nicole
Publisher: name: figshare
Year: 2018
Subjects: subject: Evolutionary Biology
subject: FOS: Biological sciences
subject: 69999 Biological Sciences not elsewhere classified
subject: Inorganic Chemistry
subject: FOS: Chemical sciences
subject: Science Policy

description: Table S1. Relation between children’s MVPA and parental MVPA in bouts of ≥10 min (linear regression models). (DOCX 21 kb)
Topological complexity of a map
Creators: name: Pavešić, Petar
Publisher: name: arXiv
Year: 2018
Subjects: subject: Algebraic Topology (math.AT)
subject: FOS: Mathematics

description: We study certain topological problems that are inspired by applications to autonomous robot manipulation. Consider a continuous map $f\colon X\to Y$, where $f$ can be a kinematic map from the configuration space $X$ to the working space $Y$ of a robot arm or a similar mechanism. Then one can associate to $f$ a number $\mathrm{TC}(f)$, which is, roughly speaking, the minimal number of continuous rules that are necessary to construct a complete manipulation algorithm for the device. Examples show that $\mathrm{TC}(f)$ is very sensitive to small perturbations of $f$ and that its value depends heavily on the singularities of $f$. This fact considerably complicates the computations, so we focus here on estimates of $\mathrm{TC}(f)$ that can be expressed in terms of homotopy invariants of spaces $X$ and $Y$, or that are valid if $f$ satisfy some additional assumptions like, for example, being a fibration. Some of the main results are the derivation of a general upper bound for $\mathrm{TC}(f)$, invariance of $\mathrm{TC}(f)$ with respect to deformations of the domain and codomain, proof that $\mathrm{TC}(f)$ is a FHE-invariant, and the description of a cohomological lower bound for $\mathrm{TC}(f)$. Furthermore, if $f$ is a fibration we derive more precise estimates for $\mathrm{TC}(f)$ in terms of the Lusternik-Schnirelmann category and the topological complexity of $X$ and $Y$. We also obtain some results for the important special case of covering projections.
description: Corrected cohomology estimate of topological complexity in Theorem 3.21, which in full generality needs Cech cohomology
Additional file 6 of Qin Huang formula enhances the effect of Adriamycin in B-cell lymphoma via increasing tumor infiltrating lymphocytes by targeting toll-like receptor signaling pathway
Creators: name: Li, Weili
name: Lv, Lingling
name: Ruan, Ming
name: Xu, Jiayue
name: Zhu, Wenhua
name: Li, Qiong
name: Jiang, Xufeng
name: Zheng, Lan
name: Zhu, Weirong
Publisher: name: figshare
Year: 2022
Subjects: subject: Biochemistry
subject: Medicine
subject: Molecular Biology
subject: Pharmacology
subject: Biotechnology
subject: Immunology
subject: FOS: Clinical medicine
subject: Biological Sciences not elsewhere classified
subject: Information Systems not elsewhere classified
subject: Cancer
subject: Hematology
subject: Infectious Diseases
subject: FOS: Health sciences
subject: Virology
subject: Computational Biology

description: Additional file 6: Figure S4. Image J results of the WB bands. A. Bar plot of the expression of TLR2. Compared with the Control group (n=3) and the ADM group (n=3), the ADM+QHF group (n=3) significantly increased the expressions of TLR2 (v.s. Control group, ***p<0.001; v.s. ADM group, ****p<0.0001). B. Bar plot of the expression of p38.Compared with the Control group (n=3), the level of p38 MAPK was remarkably increased in ADM group (n=3, ***p<0.001) and ADM+QHF group (n=3, ***p<0.001)
title: ADCO, Cartulaire général de Cîteaux, dit de Jean de Cirey, (XVe siècle), tome VI, Cart. 190 (11 H 75), 316 folios, f. 0184r
Creators: name: de la Côte d'Or, Archives départementales
name: Archives Départementales De La Côte-D'Or
name: Petot, Frédérique
name: Projet CBMA
name: CG21/F.PETOT/2012
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2020
Subjects: subject: Corpus Burgundiae Medii Aevi
subject: Chartes de la Bourgogne du Moyen Âge
subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris
subject: cartulaire

description: Cartulaire général de Cîteaux, dit de Jean de Cirey, (XVe siècle), tome VI, Archives départementales de la Côte-d'Or, Cart. 190 (11 H 75), 316 folios, f. 0184r, Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Cartulaire général de Cîteaux, dit de Jean de Cirey, (XVe siècle), tome VI, Archives départementales de la Côte-d'Or, Cart. 190 (11 H 75), 316 folios, f. 0184r, in Projet CBMA - Corpus Burgundiae Medii Aevi [Ressource en ligne], https:// manuscrits.cbma-project.eu/
description: Provenance: abbaye de Cîteaux
description: Provenance: http://www.wikidata.org/entity/Q843261
description: Provenance: https://www.geonames.org/3024876
description: Provenance: http://www.idref.fr/030974844/id
description: Provenance: https://catalogue.bnf.fr/ark:/12148/cb12228351v
Magnetization in 2+1 dimensional QED at Finite Temperature and Density
Creators: name: Andersen, Jens O.
name: Haugset, Tor
Publisher: name: arXiv
Year: 1994
Subjects: subject: Condensed Matter (cond-mat)
subject: FOS: Physical sciences

description: We consider Dirac fermions moving in a plane with a static homogeneous magnetic field orthogonal to the plane. We calculate the effective action at finite temperature and density. The magnetization is derived and it is shown that the fermion gas exhibits de Haas-van Alphen oscillations at small temperatures and weak magnetic fields. We also comment upon earlier work.
description: 14 pages, plain LaTeX
Vespa arvensis Linnaeus, 1758, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1758
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hymenoptera
Vespidae
Vespa
Vespa arvensis

description: Vespa arvensis [spec. nov.]
V. abdominis fasciis quatuor flavis: tertia interrupta.
Fn. svec. 992.
Habitat in Europa.
description: Published as part of Linnaeus, Carolus, 1758, Systema Naturae per regna tria naturae: secundum classes, ordines, genera, species, cum characteribus, differentiis, synonymis, locis, Stockholm :Laurentius Salvius on page 573, DOI: 10.5962/bhl.title.542, http://zenodo.org/record/3922206
Approaching Carnot efficiency at maximum power in linear response regime
Creators: name: Bonança, Marcus V. S.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Statistical Mechanics (cond-mat.stat-mech)
subject: FOS: Physical sciences

description: We construct an example of heat engine whose efficiency at maximum power breaks down the previously derived bounds in the linear response regime. Such example takes a classical harmonic oscillator as the working substance undergoing a finite-time Otto cycle. Using a specific kind of shortcut to adiabaticity, valid only in the linear response regime, quasistatic work is performed at arbitrarily short times. The cycle duration is then reduced to the sum of relaxation times during the thermalization strokes exclusively. Thus, power is maximum since the work is maximum (quasistatic work) and the cycle duration is minimum. Efficiency at maximum power can be made arbitrarily close to Carnot efficiency with an appropriate choice of the ratio between the temperatures of the two heat baths.
description: 6 pages, 2 figures
APRESENTAÇÃO E TUTORIAL (2018) ENIC - UNINOVE[ENIC] Apresentação_Tutorial (2018) UNINOVE.pdfAPRESENTAÇÃO E TUTORIAL (2018) ENIC - UNINOVE
Creators: name: Cavalcante, Vinicius Holanda
Publisher: name: figshare
Year: 2018
Subjects: subject: 130305 Educational Counselling
subject: FOS: Educational sciences

description: Apresentação e tutorial, para os pesquisadores e alunos de Iniciação Científica interessados em participar do; Encontro de Iniciação Científica e Seminário Nacional de Pesquisa da Universidade Nove de Julho - UNINOVE
The emission-line pulse pattern in the intermediate polar RX J0558
Creators: name: Harlaftis, E. T.
name: Horne, K.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We observed the intermediate polar RX J0558+53 with the 4.2m WHT and find in the pulsed emission lines, a ``corkscrew'' pattern, which indicates a two-pole white dwarf accretion. The ``corkscrew'' pattern consists of two emission-line pulses, separated by half the white dwarf spin period, and moving from red to blue velocities. The detected emission-line pulsations have an amplitude of 1.1--2.7 per cent in the He II and Balmer emission lines on the 545-s spin period of the white dwarf which compare to 3.5-4.8 per cent for the continuum double-peak pulsations. We image the emission-line pulse pattern and is shown to lag the continuum pulse by 0.12 spin cycles. We interpret the pattern by invoking an accretion curtain from the disrupted, inner disc to the two poles of the magnetic white dwarf. The semi-amplitude of the He II pulse of 408+-35 km/s can be used to constrain the size of the magnetosphere, R ~ 4.1 x 10^4 km, and the magnetic moment of the white dwarf (~2.4 10^32 G cm^3). Power spectra show dominant frequencies at 2 ωand 2 (ω-Ω) which suggest reprocessing of the white dwarf's illuminating beams in the accretion disc. Finally, the steady He II emission line shows a strong sinusoidal component moving from red to blue on the orbital period, with a width similar to that expected from irradiation of the secondary star. Imaging of the emission lines indicate illuminated locations at the inner side of the red star and the back side of the accretion disc.
description: 12 pages, 11 figures, MNRAS journal paper. in press
Anomalous Spin Dynamics in Doped Quantum Antiferromagnets
Creators: name: Jaklic, J.
name: Prelovsek, P.
Publisher: name: arXiv
Year: 1994
Subjects: subject: Condensed Matter (cond-mat)
subject: FOS: Physical sciences

description: Finite-temperature spin dynamics in planar t-J model is studied using the method based on the Lanczos diagonalization of small systems. Dynamical spin structure factor at moderate dopings shows the coexistence of free-fermion-like and spin-fluctuation timescales. At T
description: 10 pages + 4 figures, Postscript in uuencoded compressed tar file, IJS-TP-94/24
Exact Markovian and non-Markovian time dynamics in waveguide QED: collective interactions, bound states in continuum, superradiance and subradiance
Creators: name: Dinc, Fatih
name: Ercan, İlke
name: Brańczyk, Agata M.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: We develop a formalism for modelling exact time dynamics in waveguide quantum electrodynamics (QED) using the real-space approach. The formalism does not assume any specific configuration of emitters and allows the study of Markovian dynamics fully analytically and non-Markovian dynamics semi-analytically with a simple numerical integration step. We use the formalism to study subradiance, superradiance and bound states in continuum. We discuss new phenomena such as subdivision of collective decay rates into symmetric and anti-symmetric subsets and non-Markovian superradiance effects that can lead to collective decay stronger than Dicke superradiance. We also discuss possible applications such as pulse-shaping and coherent absorption. We thus broaden the range of applicability of real-space approaches beyond steady-state photon transport.
description: The final version has been accepted for publication in Quantum on 03 Dec 2019
title: Koronavirus infektsionli bemorlarda kasallikning klinik ko’rinishlari
Creators: name: Begmatov, B.K.
name: Oganiezov, B.B.
Publisher: name: TASHKENT STATE DENTAL INSTITUTE
Year: 2021
Subjects: subject: FOS: Medical and health sciences
valueUri: http://www.oecd.org/science/inno/38235147.pdf

description: Koronavirusli infeksiya tashxisi tasdiqlangan bemorda kasallanishning og’irlik darajalarini uchrash chastotasi va kasallik kechishining og’irlik darajasiga ta’sir qiluvchi omillar o’rganish.
The Power Spectrum, Bias Evolution, and the Spatial Three-Point Correlation Function
Creators: name: Buchalter, Ari
name: Kamionkowski, Marc
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We calculate perturbatively the normalized spatial skewness, $S_3$, and full three-point correlation function (3PCF), $ζ$, induced by gravitational instability of Gaussian primordial fluctuations for a biased tracer-mass distribution in flat and open cold-dark-matter (CDM) models. We take into account the dependence on the shape and evolution of the CDM power spectrum, and allow the bias to be nonlinear and/or evolving in time, using an extension of Fry's (1996) bias-evolution model. We derive a scale-dependent, leading-order correction to the standard perturbative expression for $S_3$ in the case of nonlinear biasing, as defined for the unsmoothed galaxy and dark-matter fields, and find that this correction becomes large when probing positive effective power-spectrum indices. This term implies that the inferred nonlinear-bias parameter, as usually defined in terms of the smoothed density fields, might depend on the chosen smoothing scale. In general, we find that the dependence of $S_3$ on the biasing scheme can substantially outweigh that on the adopted cosmology. We demonstrate that the normalized 3PCF, $Q$, is an ill-behaved quantity, and instead investigate $Q_V$, the variance-normalized 3PCF. The configuration dependence of $Q_V$ shows similarly strong sensitivities to the bias scheme as $S_3$, but also exhibits significant dependence on the form of the CDM power spectrum. Though the degeneracy of $S_3$ with respect to the cosmological parameters and constant linear- and nonlinear-bias parameters can be broken by the full configuration dependence of $Q_V$, neither statistic can distinguish well between evolving and non-evolving bias scenarios. We show that this can be resolved, in principle, by considering the redshift dependence of $ζ$.
description: 41 pages, including 12 Figures. To appear in The Astrophysical Journal, Vol. 521, #1
[ENIC] Apresentação_Tutorial (2018) UNINOVE.pdf
Creators: name: Cavalcante, Vinicius Holanda
Publisher: name: figshare
Year: 2018
Subjects: subject: 130305 Educational Counselling
subject: FOS: Educational sciences

description: Apresentação e tutorial, para os pesquisadores e alunos de Iniciação Científica interessados em participar do; Encontro de Iniciação Científica e Seminário Nacional de Pesquisa da Universidade Nove de Julho - UNINOVE
Climate Coffees Presentation: The role of sea ice initialisation on Arctic decadal prediction skill with EC-Earth3
Creators: name: Tian, Tian
Publisher: name: Zenodo
Year: 2021

description: A presentation on 27th May 2021 by Tian Tian (Danish Meteorological Institute, DK), on "The role of sea ice initialisation on the Arctic decadal prediction skill with EC-Earth3." Climate Coffees are organised by Blue-Action and the European Climate Research Alliance, and are a series of peer sharing events run by climate scientists to exchange knowledge and discussions.
Participation-Ratio Entropy and Critical Fluctuations in the Thermodynamics of Pancake Vortices
Creators: name: Hu, Jun
name: MacDonald, A. H.
Publisher: name: arXiv
Year: 1994
Subjects: subject: Condensed Matter (cond-mat)
subject: FOS: Physical sciences

description: We report on a study of the thermodynamics of the Ginzburg-Landau model for two-dimensional type-II superconductors near the transition from the normal state to the Abrikosov-lattice state. We couch our analysis in terms of the participation-ratio entropy, $s(P)$, which expresses the volume in order-parameter-space with a given participation-ratio for the local superfluid density. $s(P)$ completely determines the thermodynamics of the system. We report on results for $s(P)$ obtained analytically using perturbation expansion methods and numerically using Monte Carlo simulation methods and discuss the weak first-order phase transition which occurs in this system in terms of the properties of $s(P)$.
description: 12 pages (RevTeX 3.0) and 2 figures, available upon request, IUCM94-016
The Origin of Primordial Dwarf Stars and Baryonic Dark Matter
Creators: name: Hansen, Brad M. S.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: I present a scenario for the production of low mass, degenerate dwarfs of mass $>0.1 M_{\odot}$ via the mechanism of Lenzuni, Chernoff & Salpeter (1992). Such objects meet the mass limit requirements for halo dark matter from microlensing surveys while circumventing the chemical evolution constraints on normal white dwarf stars. I describe methods to observationally constrain this scenario and suggest that such objects may originate in small clusters formed from the thermal instability of shocked, heated gas in dark matter haloes, such as suggested by Fall & Rees (1985) for globular clusters.
description: TeX, 4 pages plus 2 postscript figures. To appear in Astrophysical Journal Letters
The KMOS Cluster Survey (KCS) II - The Effect of Environment on the Structural Properties of Massive Cluster Galaxies at Redshift $1.39 < z <1.61$
Creators: name: Chan, Jeffrey C. C.
name: Beifiori, Alessandra
name: Saglia, Roberto P.
name: Mendel, J. Trevor
name: Stott, John P.
name: Bender, Ralf
name: Galametz, Audrey
name: Wilman, David J.
name: Cappellari, Michele
name: Davies, Roger L.
name: Houghton, Ryan C. W.
name: Prichard, Laura J.
name: Lewis, Ian J.
name: Sharples, Ray
name: Wegner, Michael
Publisher: name: arXiv
Year: 2018
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We present results on the structural properties of massive passive galaxies in three clusters at $1.39
description: Accepted for publication in ApJ. 37 pages, 5 figures
Additional file 4 of Qin Huang formula enhances the effect of Adriamycin in B-cell lymphoma via increasing tumor infiltrating lymphocytes by targeting toll-like receptor signaling pathway
Creators: name: Li, Weili
name: Lv, Lingling
name: Ruan, Ming
name: Xu, Jiayue
name: Zhu, Wenhua
name: Li, Qiong
name: Jiang, Xufeng
name: Zheng, Lan
name: Zhu, Weirong
Publisher: name: figshare
Year: 2022
Subjects: subject: Biochemistry
subject: Medicine
subject: Molecular Biology
subject: Pharmacology
subject: Biotechnology
subject: Immunology
subject: FOS: Clinical medicine
subject: Biological Sciences not elsewhere classified
subject: Information Systems not elsewhere classified
subject: Cancer
subject: Hematology
subject: Infectious Diseases
subject: FOS: Health sciences
subject: Virology
subject: Computational Biology

description: Additional file 4: Figure S2. IHC stainingsfor M1 and M2 macrophages. A. Representative images of IHC staining for M1 macrophages among the three groups (200×). B. Bar plot of the positive cell rate of M1 macrophages of the control group (n=3), ADM group (n=3), and QHF+ADM group (n=3). C. Representative images of IHC staining for M2 macrophages among the three groups (200×). D. Bar plot of the positive cell rate of M2 macrophages of the control group (n=3), ADM group (n=3), and QHF+ADM group (n=3).Ns: p>0.05
Thermal Conductivity Anisotropy in Superconducting $UPt_3$
Creators: name: Fledderjohann, A.
name: Hirschfeld, P. J.
Publisher: name: arXiv
Year: 1994
Subjects: subject: Condensed Matter (cond-mat)
subject: FOS: Physical sciences

description: Recent thermal conductivity measurements on $UPt_3$ single crystals by Lussier et al. indicate the existence of a strong b--c anisotropy in the superconducting state. We calculate the thermal conductivity in various unconventional candidate states appropriate for the $UPt_3$ ``B phase" and compare with experiment, specifically the $E_{2u}$ and $E_{1g}$ $(1,i)$ states predicted in some Ginzburg-Landau analyses of the phase diagram. For the simplest realizations of these states over spherical or ellipsoidal Fermi surfaces, the normalized $E_{2u}$ conductivity is found, surprisingly, to be completely isotropic. We discuss the effects of inelastic scattering and realistic Fermi surface anisotropy, and deduce constraints on the symmetry class of the $UPt_3$ ground state.
description: 4 postscript pages, UFL1025
MPEC 2025-H20 : 2024 WH3
Creators: name: Minor Planet Center Staff
Publisher: name: The Minor Planet Center
Year: 2025
Subjects: subject: Small Solar System bodies
valueUri: http://astrothesaurus.org/uat/1469

description: The Minor Planet Electronic Circulars contain information on unusual minor planets, routine data on comets and natural satellites, and occasional editorial announcements.  They are published on behalf of Division F of the International Astronomical Union by the Minor Planet Center, Smithsonian Astrophysical Observatory, Cambridge, MA 02138, U.S.A.
The BINGO telescope: a new instrument exploring the new 21-cm cosmology window
Creators: name: Wuensche, C. A.
name: Collaboration, the BINGO
Publisher: name: arXiv
Year: 2018
Subjects: subject: Instrumentation and Methods for Astrophysics (astro-ph.IM)
subject: FOS: Physical sciences

description: BINGO is a unique radio telescope designed to make the first detection of Baryon Acoustic Oscillations (BAO) at radio frequencies. This will be achieved by measuring the distribution of neutral hydrogen gas at cosmological distances using a technique called Intensity Mapping. Along with the Cosmic Microwave Background anisotropies, the scale of BAO is one of the most powerful probes of cosmological parameters, including dark energy. The telescope will be built in a very low RFI site in South America and will operate in the frequency range from 0.96 GHz to 1.26 GHz. The telescope design consists of two $\thicksim$ 40-m compact mirrors with no moving parts. Such a design will give the excellent polarization performance and very low sidelobe levels required for intensity mapping. With a feedhorn array of 50 receivers, it will map a $15^{\circ}$ declination strip as the sky drifts past the field-of-view of the telescope. The BINGO consortium is composed Universidade de São Paulo, Instituto Nacional de Pesquisas Espaciais (Brazil), University of Manchester and University College London (United Kingdom), ETH Zürich (Switzerland) and Universidad de La Republica (Uruguay). The telescope assembly and horn design and fabrication are under way in Brazil. The receiver was designed in UK and will be developed in Brazil, with most of the components for the receiver will also be supplied by Brazilian industry. The experience and science goals achieved by the BINGO team will be advantageous as a pathfinder mission for the Square Kilometre Array (SKA) project. This paper reports the current status of the BINGO mission, as well as preliminary results already obtained for the instrumentation development.
description: 11 pages, 10 figures, to be published in The Journal of Physics Conference Series - Proceedings of the 4th Algerian Conference in Astronomy and Astrophysics (2018)
title: Atlas des DOM. - La Réunion - Planche 25 : La pêche : notices, pages 2, 3, 4
Creators: name: Bertile, Wilfrid
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2017
Subjects: subject: pêche
subject: bateau de pêche
subject: produit de la pêche
subject: pêche artisanale
subject: pêcheur
subject: faune aquatique
subject: pêche côtière
subject: pêche industrielle
subject: pêche maritime
subject: crustacé
subject: espèce démersale

description: La page 2 explique comment interpréter les chiffres fournis. Présente la répartition spatiale, la production et la commercialisation de la pêche artisanale. Un tableau appuie ces propos : un tableau donne l'évolution de la production de 1965 à 1973. Page 3 : suite de la présentation du produit de la pêche artisanale et explication des problèmes liés aux développement de la pêche côtière. Présente les conditions de développement de la pêche industrielle. Trois tableaux, deux graphiques et un carton appuient ces propos : un tableau donne la production de la pêche en 1967 et 1968, un graphique circulaire montre la répartition des différents types de production de la pêche côtière en 1968, un tableau donne l'évolution de la pêche côtière en terme de nombre de barques, de pêcheurs inscrits et de production de 1936 à 1972, un graphique en courbes montre l'évolution de la production de la pêche côtière de 1965 à 1973, un tableau montre l'augmentation des prix du poisson à la barque et des charges de 1962 à 1972, un carton montre les différentes zones de pêche dans l'Océan Indien au départ de La Réunion. Page 4 : suite de la présentation des conditions de développement de la pêche industrielle. Puis présente un panorama de la production et de la commercialisation du produit de la pêche industrielle. Et termine sur un focus sur la Pointe des Galets qui est la base thonière de l'Océan Indien. Un graphique et un tableau appuient ces propos : un histogramme montre l'évolution de la production de la pêche industrielle de 1966 à 1972, un tableau donne l'évolution de la production de la pêche industrielle de 1965 à 1972. Une orientation bibliographique est fournie en fin de notice.
description: Relation: http://www.nakala.fr/data/11280/b994f11f
description: Coverage: La Réunion
description: Coverage: Pointe des Galets
description: Coverage: Océan Indien
description: Temporal: start=1965; end=1973;
Learning force fields from stochastic trajectories
Creators: name: Frishman, Anna
name: Ronceray, Pierre
Publisher: name: arXiv
Year: 2018
Subjects: subject: Soft Condensed Matter (cond-mat.soft)
subject: Statistical Mechanics (cond-mat.stat-mech)
subject: FOS: Physical sciences

description: When monitoring the dynamics of stochastic systems, such as interacting particles agitated by thermal noise, disentangling deterministic forces from Brownian motion is challenging. Indeed, we show that there is an information-theoretic bound, the capacity of the system when viewed as a communication channel, that limits the rate at which information about the force field can be extracted from a Brownian trajectory. This capacity provides an upper bound to the system's entropy production rate, and quantifies the rate at which the trajectory becomes distinguishable from pure Brownian motion. We propose a practical and principled method, Stochastic Force Inference, that uses this information to approximate force fields and spatially variable diffusion coefficients. It is data efficient, including in high dimensions, robust to experimental noise, and provides a self-consistent estimate of the inference error. In addition to forces, this technique readily permits the evaluation of out-of-equilibrium currents and the corresponding entropy production with a limited amount of data.
description: 10 pages text + 24 pages appendix
The Type Ia Supernova 1997br in ESO 576-G40
Creators: name: Li, W. D.
name: Qiu, Y. L.
name: Zhu, X. H.
name: Hu, J. Y.
name: Richmond, M. W.
name: Treffers, A. V. Filippenko R. R.
name: Peng, C. Y.
name: Leonard, D. C.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: The peculiar type Ia supernova SN 1997br in ESO 576-G40 was extensively observed at Beijing Astronomical Observatory and Lick Observatory. In this paper, we present and discuss the BVRI photometry and the spectra collected over 3 months, beginning 9 days before maximum brightness. The light curves of SN 1997br are similar to those of SN 1991T, with slow decline rates after the B maximum. Well-sampled data before the B maximum show unambiguously that SN 1997br rises more slowly and has a wider peak than normal type Ia supernovae. The optical color evolution of SN 1997br is also similar to that of SN 1991T. We estimate the extinction of SN 1997br to be E(B-V) = 0.35+/-0.10 mag by comparing its BVRI light curves with those of SN 1991T and by measureing the equivalent width of interstellar Na I D absorption lines. We have conducted a thorough comparison of the spectroscopic evolution of SN 1997br, SN 1991T, and SN 1994D. Although SN 1997br is generally very similar to SN 1991T, it shows some interesting differences at various epoches. Spectra of SN 1997br seem to indicate an earlier transition to the dominant phase of Fe-peak elements after the B maximum. Si II lines in SN 1997br show a very short duration after the B maximum. We discuss the implications of our observations of SN 1997br for models of type Ia supernovae. Specifically, we suggest that some SNe Ia may result from decelerated detonations of white dwarfs.
description: 25 pages, 17 figures, 4 tables, will be published the June,1999 issue of AJ
Optimal demand shaping for a dual-channel retailer under growing e-commerce adoption
Creators: name: Mutlu, Nevin
name: Bish, Ebru K.
Publisher: name: Taylor & Francis
Year: 2019
Subjects: subject: Medicine
subject: Biotechnology
subject: Sociology
subject: FOS: Sociology
subject: 80699 Information Systems not elsewhere classified
subject: FOS: Computer and information sciences
subject: Science Policy
subject: Computational Biology

description: The e-commerce adoption level within our society has been growing in the past decade, leading to dynamically evolving demand patterns across retailing channels. In this work, we study a dual-channel retailer’s optimal demand shaping strategy, through e-commerce marketing efforts and store service levels, in the presence of this dynamic evolution. Our stylized model integrates the growing adoption of e-commerce within society with individual consumers’ channel choice, and explicitly models the reference effects of the retailer’s prior decisions on consumer decision-making in a multi-period setting. This model allows us to characterize the settings in which e-commerce marketing is beneficial for the retailer, and to show that the retailer’s optimal demand shaping strategy depends on the product’s e-commerce adoption phase. Interestingly, we find that if the retailer provides the consumers with information on store availability levels, then the retailer’s optimal service levels stay constant over time, even if e-commerce adoption in the society grows.
Sequence-dependent Three Interaction Site (TIS) Model for Single and Double-stranded DNA
Creators: name: Chakraborty, Debayan
name: Hori, Naoto
name: Thirumalai, Dave
Publisher: name: arXiv
Year: 2018
Subjects: subject: Biomolecules (q-bio.BM)
subject: Soft Condensed Matter (cond-mat.soft)
subject: FOS: Biological sciences
subject: FOS: Physical sciences

description: We develop a robust coarse-grained model for single and double stranded DNA by representing each nucleotide by three interaction sites (TIS) located at the centers of mass of sugar, phosphate, and base. The resulting TIS model includes base-stacking, hydrogen bond, and electrostatic interactions as well as bond-stretching and bond angle potentials that account for the polymeric nature of DNA. The choices of force constants for stretching and the bending potentials were guided by a Boltzmann inversion procedure using a large representative set of DNA structures extracted from the Protein Data Bank. Some of the parameters in the stacking interactions were calculated using a learning procedure, which ensured that the experimentally measured melting temperatures of dimers are faithfully reproduced. Without any further adjustments, the calculations based on the TIS model reproduces the experimentally measured salt and sequence dependence of the size of single stranded DNA (ssDNA), as well as the persistence lengths of poly(dA) and poly(dT) chains. Interestingly, upon application of mechanical force the extension of poly(dA) exhibits a plateau, which we trace to the formation of stacked helical domains. In contrast, the force-extension curve (FEC) of poly(dT) is entropic in origin, and could be described by a standard polymer model. We also show that the persistence length of double stranded DNA is consistent with the prediction based on the worm-like chain. The persistence length, which decreases with increasing salt concentration, is in accord with the Odijk-Skolnick-Fixman theory intended for stiff polyelectrolyte chains near the rod limit. The range of applications, which did not require adjusting any parameter after the initial construction based solely on PDB structures and melting profiles of dimers, attests to the transferability and robustness of the TIS model for ssDNA and dsDNA.
$D$-dimensional Arrays of Josephson Junctions, Spin Glasses and $q$-deformed Harmonic Oscillators
Creators: name: Parisi, Giorgio
Publisher: name: arXiv
Year: 1994
Subjects: subject: Condensed Matter (cond-mat)
subject: High Energy Physics - Lattice (hep-lat)
subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We study the statistical mechanics of a $D$-dimensional array of Josephson junctions in presence of a magnetic field. In the high temperature region the thermodynamical properties can be computed in the limit $D \to \infty$, where the problem is simplified; this limit is taken in the framework of the mean field approximation. Close to the transition point the system behaves very similar to a particular form of spin glasses, i.e. to gauge glasses. We have noticed that in this limit the evaluation of the coefficients of the high temperature expansion may be mapped onto the computation of some matrix elements for the $q$-deformed harmonic oscillator.
Optimal Demand Shaping for a Dual-channel Retailer under Growing E-commerce Adoption
Creators: name: Mutlu, Nevin
name: Bish, Ebru K.
Publisher: name: Taylor & Francis
Year: 2018
Subjects: subject: Medicine
subject: Biotechnology
subject: Sociology
subject: FOS: Sociology
subject: 80699 Information Systems not elsewhere classified
subject: FOS: Computer and information sciences
subject: Science Policy
subject: Computational Biology

description: The e-commerce adoption level within the society has been growing in the past decade, leading to dynamically evolving demand patterns across retailing channels. In this work, we study a dual-channel retailer’s optimal demand shaping strategy, through e-commerce marketing efforts and store service levels, in the presence of this dynamic evolution. Our stylized model integrates the growing adoption of e-commerce within the society with individual consumers’ channel choice, and explicitly models the reference effects of the retailer’s prior decisions on consumer decision-making in a multi-period setting. This model allows us to characterize the settings in which e-commerce marketing is beneficial for the retailer, and to show that the retailer’s optimal demand shaping strategy depends on the product’s e-commerce adoption phase. Interestingly, we find that if the retailer provides the consumers with information on store availability levels, then the retailer’s optimal service levels stay constant over time, even if e-commerce adoption in the society grows.
High Energy Cosmic Neutrinos
Creators: name: Barwick, Steven W.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: While the general principles of high-energy neutrino detection have been understood for many years, the deep, remote geographical locations of suitable detector sites have challenged the ingenuity of experimentalists, who have confronted unusual deployment, calibration, and robustness issues. Two high energy neutrino programs are now operating (Baikal and AMANDA), with the expectation of ushering in an era of multi-messenger astronomy, and two Mediterranean programs have made impressive progress. The detectors are optimized to detect neutrinos with energies of the order of 1-10 TeV, although they are capable of detecting neutrinos with energies of tens of MeV to greater than PeV. This paper outlines the interdisciplinary scientific agenda, which span the fields of astronomy, particle physics, and cosmic ray physics, and describes ongoing worldwide experimental programs to realize these goals.
description: 15 pages, 9 figures, talk presented at the Nobel Symposium on Particle Physics and the Universe, Sweden, August 1998
Challenges and growth opportunities: the landscape of Chinese medical publication professionals in the global context: a questionnaire-based survey
Creators: name: Zhang, Jining
name: Ge, Yilin
name: Wang, Jiao
name: Wu, Zhihua
name: Wang, Ying
name: Bhat, Amit
name: Lin, Yutao
Publisher: name: Taylor & Francis
Year: 2021
Subjects: subject: Medicine
subject: Immunology
subject: FOS: Clinical medicine
subject: Biological Sciences not elsewhere classified
subject: Developmental Biology
subject: Science Policy

description: The Chinese healthcare industry has immense potential for innovation and requires competent publication professionals for global reach. Changes in regulatory landscape of China necessitates pharmaceutical industries to collaborate with medical professionals who are capable of keeping up with both changes in regulations and innovative medicine. We initiated an online questionnaire-based survey via WeChat from August 3 to August 14, 2019 which focused on experience level, challenges, career development, and training requirements of survey participants. A total of 53 medical publication professionals participated in this survey. Contrary to global trends, 77% of participants had <5 years of professional experience in publication, although only 36% of participants had <5 years of experience in healthcare industry. In all, 63% of respondents spent <50% of their time in publication-related activities, contributing to <10 manuscripts per year. Their expertise in manuscripts spanned clinical studies (68%), post-marketing studies (62%), and reviews (38%). Poor research design and data quality, limited medical writing skill, and inefficient communication with authors were major challenges for developing high-quality publications. Awareness of good publication practices guidelines was high (49%) and 15% of respondents were Certified Medical Publication Professionals. Strategic publication planning (72%), industry trends (66%), and best practices (55%) were some of training requirements identified to increase competencies among respondents. Although the Chinese medical publication professional industry is at a nascent stage, an attempt is being made to provide opportunities for its publication professionals to develop their competencies to match global standards.
The Fully Frustrated Hypercubic Model is Glassy and Aging at Large $D$
Creators: name: Marinari, Enzo
name: Parisi, Giorgio
name: Ritort, Felix
Publisher: name: arXiv
Year: 1994
Subjects: subject: Condensed Matter (cond-mat)
subject: High Energy Physics - Lattice (hep-lat)
subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We discuss the behavior of the fully frustrated hypercubic cell in the infinite dimensional mean-field limit. In the Ising case the system undergoes a glass transition, well described by the random orthogonal model. Under the glass temperature aging effects show clearly. In the $XY$ case there is no sign of a phase transition, and the system is always a paramagnet.
description: Figures added in uufiles format, and epsf included
The VMC Survey. XXIX. Turbulence-Controlled Hierarchical Star Formation in the Small Magellanic Cloud
Creators: name: Sun, Ning-Chen
name: de Grijs, Richard
name: Cioni, Maria-Rosa L.
name: Rubele, Stefano
name: Subramanian, Smitha
name: van Loon, Jacco Th.
name: Bekki, Kenji
name: Bell, Cameron P. M.
name: Ivanov, Valentin D.
name: Marconi, Marcella
name: Muraveva, Tatiana
name: Oliveira, Joana M.
name: Ripepi, Vincenzo
Publisher: name: arXiv
Year: 2018
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: In this paper we report a clustering analysis of upper main-sequence stars in the Small Magellanic Cloud, using data from the VMC survey (the VISTA near-infrared YJKs survey of the Magellanic system). Young stellar structures are identified as surface overdensities on a range of significance levels. They are found to be organized in a hierarchical pattern, such that larger structures at lower significance levels contain smaller ones at higher significance levels. They have very irregular morphologies, with a perimeter-area dimension of 1.44 +/- 0.02 for their projected boundaries. They have a power-law mass-size relation, power-law size/mass distributions, and a lognormal surface density distribution. We derive a projected fractal dimension of 1.48 +/- 0.03 from the mass-size relation, or of 1.4 +/- 0.1 from the size distribution, reflecting significant lumpiness of the young stellar structures. These properties are remarkably similar to those of a turbulent interstellar medium (ISM), supporting a scenario of hierarchical star formation regulated by supersonic turbulence.
description: 16 pages, 13 figures. Accepted for publication in ApJ
Quinolizidine alkaloids from the roots of Sophora flavescens
Creators: name: Li, Jian-Chun
name: Zhang, Zhi-Jun
name: Liu, Dan
name: Jiang, Ming-Yan
name: Li, Rong-Tao
name: Li, Hong-Mei
Publisher: name: Taylor & Francis
Year: 2020
Subjects: subject: Biochemistry
subject: Space Science
subject: Pharmacology
subject: Environmental Sciences not elsewhere classified
subject: Chemical Sciences not elsewhere classified
subject: Ecology
subject: FOS: Biological sciences
subject: Biological Sciences not elsewhere classified
subject: Plant Biology

description: Seventeen quinolizidine alkaloids, including a new matrine-type one, sophcence A (1), were isolated from the roots of Sophora flavescens Alt. The structure of compound 1 was elucidated by means of 1D and 2D NMR, as well as HR-ESI-MS spectroscopic data. The NMR data of (-)-Δ7-dehydrosophoramine (10) and oxy-N-methylcytisine (12) were reported for the first time. In addition, (+)-sophoranol (4) exhibited moderate inhibition on lipopolysaccharide (LPS)-induced nitric oxide (NO) production in RAW 264.7 macrophages with IC50 value of 22.14 μM, while lupanine (17) was found to inhibit the growth of human glioma stem cells GSC-3# at 20 μg/mL.