cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
CP Violation in a Multi-Higgs Doublet Model
Creators: name: Deshpande, N. G.
name: He, Xiao-Gang
Publisher: name: arXiv
Year: 1994
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We study CP violation in a multi-Higgs doublet model based on a $S_3 \times Z_3$ horizontal symmetry. We consider two mechanisms for CP violation in this model: a) CP violation due to complex Yukawa couplings; and b) CP violation due to scalar-pseudoscalar mixings. We find that the predictions for $ε'/ε$, CP violation in B decays and the electric dipole moments of neutron and electron are different between these two mechanisms. These predictions are also dramatically different from the minimal Standard Model predictions.
description: 17 pages + one figure, Revtex. Talk presented by Deshpande at the Conference WHEPP-3, December 1993
N-body simulations of dark matter with frequent self-interactions
Creators: name: Fischer, Moritz S.
name: Brüggen, Marcus
name: Schmidt-Hoberg, Kai
name: Dolag, Klaus
name: Kahlhoefer, Felix
name: Ragagnin, Antonio
name: Robertson, Andrew
Publisher: name: Deutsches Elektronen-Synchrotron, DESY, Hamburg
Year: 2021
Subjects: subject: 520
subject: dark matter: halo
subject: scattering: small-angle
subject: galaxy: cluster
subject: many-body problem
subject: differential cross section
subject: drag force
subject: formation

description: 1-18 (2021). doi:10.1093/mnras/stab1198
description: Self-interacting dark matter (SIDM) models have the potential to solve the small-scale problems that arise in the cold dark matter paradigm. Simulations are a powerful tool for studying SIDM in the context of astrophysics, but it is numerically challenging to study differential cross-sections that favour small-angle scattering, as in light-mediator models. Here, we present a novel approach to model frequent scattering based on an effective drag force, which we have implemented into the N-body code gadget-3. In a range of test problems, we demonstrate that our implementation accurately models frequent scattering. Our implementation can be used to study differences between SIDM models that predict rare and frequent scattering. We simulate core formation in isolated dark matter haloes, as well as major mergers of galaxy clusters and find that SIDM models with rare and frequent interactions make different predictions. In particular, frequent interactions are able to produce larger offsets between the distribution of galaxies and dark matter in equal-mass mergers.
Additional file 1 of Comparative genome analysis of multidrug-resistant Pseudomonas aeruginosa JNQH-PA57, a clinically isolated mucoid strain with comprehensive carbapenem resistance mechanisms
Creators: name: Hao, Mingju
name: Ma, Wanshan
name: Dong, Xiutao
name: Li, Xiaofeng
name: Cheng, Fang
name: Wang, Yujiao
Publisher: name: figshare
Year: 2021
Subjects: subject: Genetics
subject: FOS: Biological sciences

description: Additional file 1: Table S1. List of the genomic features of mucoid strain P. aeruginosa JNQH-PA57 revealed from the complete genome (this study) and those representative P. aeruginosa clinical isolates listed in the Pseudomonas Genome Database (PGDB).
Axisymmetric magnetic modes of neutron stars having mixed poloidal and toroidal magnetic fields
Creators: name: Lee, Umin
Publisher: name: arXiv
Year: 2018
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: We calculate axisymmetric magnetic modes of a neutron star possessing a mixed poloidal and toroidal magnetic field, where the toroidal field is assumed to be proportional to a dimensionless parameter $ζ_0$. Here, we assume an isentropic structure for the neutron star and consider no effects of rotation. Ignoring the equilibrium deformation due to the magnetic field, we employ a polytrope of the index $n=1$ as the background model for our modal analyses. For the mixed poloidal and toroidal magnetic field with $ζ_0\not=0$, axisymmetric spheroidal and toroidal modes are coupled. We compute axisymmetric spheroidal and toroidal magnetic modes as a function of the parameter $ζ_0$ from $0$ to $\sim 1$ for the surface field strengths $B_S=10^{14}$G and $10^{15}$G. We find that the frequency $ω$ of the magnetic modes decreases with increasing $ζ_0$. We also find that the frequency of the spheroidal magnetic modes is almost exactly proportional to $B_S$ for $ζ_0\lesssim 1$ but that this proportionality holds only when $ζ_0\ll 1$ for the toroidal magnetic modes. The wave patterns of the spheroidal magnetic modes and toroidal magnetic modes are not strongly affected by the coupling so long as $ζ_0\lesssim 1$. We find no unstable modes having $ω^2<0$.
description: 17 pages, 10 figures, submitted to MNRAS
Entrevista com Denise Carreira: Diversidade e Educação
Creators: name: Carreira, Denise
Publisher: name: Zenodo
Year: 2020
Subjects: Políticas educacionais
Diversidade e inclusão
Gênero e sexualidade
Austeridade econômica
Resistência e mobilização social

description: A entrevista com Denise Carreira na Revista Diversidade e Educação aborda a relação entre políticas educacionais e diversidade, com foco em gênero, raça e sexualidade. A autora discute a emergência do conceito de diversidade nas políticas públicas brasileiras, suas possibilidades e armadilhas, além do impacto das políticas de austeridade na educação. Carreira analisa os desafios enfrentados por movimentos sociais e acadêmicos diante da crescente influência de setores ultraconservadores. A entrevista também destaca estratégias de resistência e promoção da equidade no campo educacional.

Como citar (ABNT): 

CARREIRA, Denise. Entrevista. Revista Diversidade e Educação, v. 8, n. 2, p. 7-20, jul./dez. 2020. Disponível em: https://doi.org/10.5281/zenodo.14783578. Acesso em: [data de acesso].
Polarimetry with POLAR
Creators: name: Kole, Merlin
Publisher: name: arXiv
Year: 2018
Subjects: subject: Instrumentation and Methods for Astrophysics (astro-ph.IM)
subject: FOS: Physical sciences

description: In the first half year of operation the satellite borne POLAR instrument detected a total of 55 Gamma-Ray Bursts about 10 of which were bright enough to allow for detailed polarization studies, thereby forming the start of the first Gamma-Ray Burst polarization catalog. In this paper a brief overview of the previous GRB polarization studies will be presented followed by an overview of the POLAR detector along with the first result of the in-flight performance. The detected Gamma-Ray bursts will be presented and finally prospects for polarization measurements of these events will be discussed.
description: Refereed review paper accepted for publication in the proceedings of the XII Multifrequency Behaviour of High Energy Cosmic Sources Workshop, held 17 June, 2017 in Palermo, Italy
Total intensity and polarized emission of the parsec-scale jet in 3C345
Creators: name: Ros, E.
name: Zensus, J. A.
name: Lobanov, A. P.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We have studied the parsec-scale structure of the quasar 3C345 at λλ1.3, 2, 3.6, and 6 cm, using total intensity and linear polarization images from 3 epochs of VLBA observations made in 1995.84, 1996.41, and 1996.81. The images show an unresolved "core" and a radio jet extending over distances up to 25 milliarcseconds. At 1.3 and 2 cm, images of the linearly polarized emission reveal an alignment of the electric vector with the extremely curved inner section of the jet. At 6 cm, the jet shows strong fractional polarization (m~15%), with the electric vector being oriented perpendicular to the jet. This is consistent with the existence of a transition from the shock-dominated to the plasma interaction-dominated emission regimes in the jet, occurring at a distance of ~1.5 milliarcseconds from the "core".
description: 13 pages, 13 figures, Accepted for publication in Astronomy & Astrophysics, main Journal
Supplementary Information from A new Palaeocene crocodylian from southern Argentina sheds light on the early history of caimanines
Creators: name: Bona, Paula
name: Ezcurra, Martín D.
name: Barrios, Francisco
name: Blanco, María V. Fernandez
Publisher: name: The Royal Society
Year: 2018
Subjects: subject: 40308 Palaeontology (incl. Palynology)
subject: FOS: Earth and related environmental sciences
subject: 60301 Animal Systematics and Taxonomy
subject: FOS: Biological sciences
subject: 60310 Plant Systematics and Taxonomy

description: Contents: i) – Stratigraphic and geographic provenance of Protocaiman peligrensis ii) – Additional anatomical information for Protocaiman peligrensis iii) – Phylogenetic relationships of Protocaiman peligrensis and other early caimanines iv) – Biogeographic analysis of early alligatorids v) – References
Additional file 9 of Comparative genome analysis of multidrug-resistant Pseudomonas aeruginosa JNQH-PA57, a clinically isolated mucoid strain with comprehensive carbapenem resistance mechanisms
Creators: name: Hao, Mingju
name: Ma, Wanshan
name: Dong, Xiutao
name: Li, Xiaofeng
name: Cheng, Fang
name: Wang, Yujiao
Publisher: name: figshare
Year: 2021
Subjects: subject: Genetics
subject: FOS: Biological sciences

description: Additional file 9: Table S9. Primers used for qRT-PCR (f, forward, sense, and r, reverse, antisense)
Pathway towards programmable wave anisotropy in cellular metamaterials
Creators: name: Celli, Paolo
name: Zhang, Weiting
name: Gonella, Stefano
Publisher: name: arXiv
Year: 2018
Subjects: subject: Applied Physics (physics.app-ph)
subject: Materials Science (cond-mat.mtrl-sci)
subject: FOS: Physical sciences

description: In this work, we provide a proof-of-concept experimental demonstration of the wave control capabilities of cellular metamaterials endowed with populations of tunable electromechanical resonators. Each independently tunable resonator comprises a piezoelectric patch and a resistor-inductor shunt, and its resonant frequency can be seamlessly re-programmed without interfering with the cellular structure's default properties. We show that, by strategically placing the resonators in the lattice domain and by deliberately activating only selected subsets of them, chosen to conform to the directional features of the beamed wave response, it is possible to override the inherent wave anisotropy of the cellular medium. The outcome is the establishment of tunable spatial patterns of energy distillation resulting in a non-symmetric correction of the wavefields.
title: ADCO, Cartulaire de l'abbaye de Cîteaux dit Cartulare Antiquum t.3 (2e moitié XIIIe siècle), Cart. 168 (11 H 66), f. 0104r
Creators: name: de la Côte d'Or, Archives départementales
name: Petot, Frédéric
name: Archives Départementales De La Côte-D'Or
name: Petot, Frédérique
name: Projet CBMA
name: CG21/F.PETOT/2010
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: cartulaire
subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris

description: Cartulaire de l'abbaye de Cîteaux dit Cartulare Antiquum t.3 (2e moitié XIIIe siècle), Archives départementales de la Côte-d'Or, Cart. 168 (11 H 66), f. 0104r, Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Cartulaire de l'abbaye de Cîteaux dit Cartulare Antiquum t.3 (2e moitié XIIIe siècle), Archives départementales de la Côte-d'Or, Cart. 168 (11 H 66), f. 0104r, 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
Tidal disruption of stars in a supermassive black hole binary system: the influence of orbital properties on fallback and accretion rates
Creators: name: Vigneron, Quentin
name: Lodato, Giuseppe
name: Guidarelli, Alessio
Publisher: name: arXiv
Year: 2018
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: The disruption of a star by a supermassive black hole generates a sudden bright flare. Previous studies have focused on the disruption by single black holes, for which the fallback rate decays as~$\propto t^{-5/3}$. In this paper, we generalise the study to the case of a supermassive black hole binary (SMBHB), using both analytical estimates and hydrodynamical simulations, looking for specific observable signatures. The range of binary separation for which it is possible to distinguish between the disruption created by a single or a binary black hole concerns typically separations of order a few milliparsecs for a primary of mass $\sim 10^6M_{\odot}$. When the fallback rate is affected by the secondary, it undergoes two types interruptions, depending on the initial inclination $θ$ of the orbit of the star relative to the plane of the SMBHB. For $θ\lesssim 70^\circ$, periodic sharp interruptions occur and the time of first interruption depends on the distance of the secondary black hole with the debris. If $θ\gtrsim 70^\circ$, a first smooth interruption occurs, but not always followed by a further recovery of the fallback rate. This implies that most of the TDEs around a SMBHB will undergo periodic sharp interruptions of their lightcurve.
description: 12 pages, 7 figures, accepted in MNRAS. DOI: 10.1093/mnras/sty585
Ecosystem service responses to rewilding: first-order estimates from 27 years of rewilding in the Scottish Highlands
Creators: name: Sophus O.S.E. Zu Ermgassen
name: McKenna, Tom
name: Gordon, Jamie
name: Willcock, Simon
Publisher: name: Taylor & Francis
Year: 2018
Subjects: subject: Evolutionary Biology
subject: FOS: Biological sciences
subject: Ecology
subject: Sociology
subject: FOS: Sociology
subject: Science Policy

description: Rewilding as a conservation strategy is gaining increasing scientific, political and public attention, yet empirical evaluations of its impacts remain scarce, especially with regards to ecosystem services. We provide evidence of the change in three ecosystem services (timber [provisioning], pollination [regulating], and aesthetics [cultural]) from up to 27 years of a moorland rewilding strategy in the Scottish Highlands using a chronosequence of rewilded plots and adjacent controls. These services were assessed in the field and using online surveys. We found that rewilding increased aboveground woody biomass and restored natural tree recruitment processes, although the latter only emerged after at least 15 years of rewilding. Rewilding caused a linear increase in perceived aesthetic quality over the first 27 years, but had no effect on pollination visitation rates. Thus, we conclude that rewilding can be used for ecosystem service recovery in moorland landscapes, but that results vary depending on the preferred service.EDITED BY John Haslett EDITED BY John Haslett
Discovery of molecular hydrogen in a high-velocity cloud of the Galactic halo
Creators: name: Richter, P.
name: de Boer, K. S.
name: Widmann, H.
name: Kappelmann, N.
name: Gringel, W.
name: Grewing, M.
name: Barnstedt, J.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We report the discovery of molecular hydrogen absorption in a Galactic high-velocity cloud (HVC) in the direction of the Large Magellanic Cloud. For the same HVC we derive an iron abundance which is half of the solar value. Thus, all evidence points to a Galactic origin for high-velocity cloud complex in front of the LMC.
description: Published in Nature, this week; 14 pages, 3 figures
Additional file 7 of Comparative genome analysis of multidrug-resistant Pseudomonas aeruginosa JNQH-PA57, a clinically isolated mucoid strain with comprehensive carbapenem resistance mechanisms
Creators: name: Hao, Mingju
name: Ma, Wanshan
name: Dong, Xiutao
name: Li, Xiaofeng
name: Cheng, Fang
name: Wang, Yujiao
Publisher: name: figshare
Year: 2021
Subjects: subject: Genetics
subject: FOS: Biological sciences

description: Additional file 7: Table S7. COGs uniquely identified in P. aeruginosa JNQH-PA057 but absent in PAO1, ATCC 27853 and PA14
Stable source reconstruction from a finite number of measurements in the Multi-frequency Inverse Source Problem
Creators: name: Karamehmedović, Mirza
name: Kirkeby, Adrian
name: Knudsen, Kim
Publisher: name: arXiv
Year: 2018
Subjects: subject: Numerical Analysis (math.NA)
subject: FOS: Mathematics
subject: G.1.8
subject: 65N21

description: We consider the multi-frequency inverse source problem for the scalar Helmholtz equation in the plane. The goal is to reconstruct the source term in the equation from measurements of the solution on a surface outside the support of the source. We study the problem in a certain finite dimensional setting: From measurements made at a finite set of frequencies we uniquely determine and reconstruct sources in a subspace spanned by finitely many Fourier-Bessel functions. Further, we obtain a constructive criterion for identifying a minimal set of measurement frequencies sufficient for reconstruction, and under an additional, mild assumption, the reconstruction method is shown to be stable. Our analysis is based on a singular value decomposition of the source-to-measurement forward operators and the distribution of positive zeros of the Bessel functions of the first kind. The reconstruction method is implemented numerically and our theoretical findings are supported by numerical experiments.
Les réfugiés espagnols et les anciens volontaires internés en France 1938-1939_1
Creators: name: Marty, André
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2015

description: Effectifs du camp de Gurs, correspondance et notes à propos de l’internement de volontaires, rapport sur la situation des républicains
137,0359990900848. Quantitative ontology of the Number.
Creators: name: Ivanov, Viacheslav
Publisher: name: Zenodo
Year: 2025
Subjects: subject: Physical cosmology
subject: Fundamental physics
subject: Theory of everything
subject: Philosophy
subject: FOS: Philosophy, ethics and religion

description: Theoretical calculation of the constant and explanation of its origin in connection with the establishment of the mass of the electron.
On the interpretation of the multicolour disc model for black hole candidates
Creators: name: Merloni, A.
name: Fabian, A. C.
name: Ross, R. R.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present a critical analysis of the usual interpretation of the multicolour disc model parameters for black hole candidates in terms of the inner radius and temperature of the accretion disc. Using a self-consistent model for the radiative transfer and the vertical temperature structure in a Shakura-Sunyaev disc, we simulate the observed disc spectra, taking into account doppler blurring and gravitational redshift, and fit them with multicolour models. We show not only that such a model systematically underestimates the value of the inner disc radius, but that when the accretion rate and/or the energy dissipated in the corona are allowed to change the inner edge of the disc, as inferred from the multicolour model, appears to move even when it is in fact fixed at the innermost stable orbit.
description: 4 pages including 2 figures, accepted for publication in MNRAS
Additional Soft Jets in ${\rm t\bar{t}}$ Production at the Tevatron $\pp$ Collider
Creators: name: Orr, Lynne H.
name: Stirling, W. J.
Publisher: name: arXiv
Year: 1994
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: A large fraction of top quark events in $\pp$ collisions at $1.8\ \TeV$ will contain additional soft hadronic jets from gluon bremsstrahlung off the quarks and gluons in the hard processes $\qq, gg \to \tt \to \bb \ww$. These extra jets can cause complications when attempting to reconstruct $m_t$ from the invariant mass of combinations of final-state quarks and leptons. We show how such soft radiation cannot be unambiguously associated with either initial-state radiation or or with final-state radiation off the $b$ quarks. The top quarks can radiate too, and in fact the pattern of radiation has a very rich structure, which depends on the orientation of the final-state particles with respect to each other and with respect to the beam. We calculate the full radiation pattern of soft jets in the soft gluon approximation and compare with several approximate forms which are characteristic of parton shower Monte Carlos. The implications for top mass measurements are discussed.
description: plain LaTeX, 13 pages plus 9 figures included as a separate uuencoded file (or avail. from authors); DTP/94/60, UR-1365
title: 01_1982
Creators: name: Wesley Baldwin, John
name: Baldwin, John W.
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2018
Subjects: subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris

description: L'ensemble de ces notes ont été crée par John Baldwin lors d'une de ses premières périodes de résidence à Paris. Ces documents comprennent tous les magistri qu’il avait pu rencontrer dans ses sources. Aux XIIème et XIIIème siècles, les universités n'existant pas encore, le titre de magister s'il évoque certainement une compétence n'est pas rattaché de façon systématique au passage par les écoles. De surcroît, les magistris sont le plus souvent désignés par leur seul prénom. La lecture de ces données est donc difficile et suppose un long travail pour tenter d'identifier un individu auquel on pourrait rattacher plusieurs mentions. John Baldwin avait donc renoncé à utiliser ces données pour donner un prolongement à sa magnifique étude sur les gradués d'université et leur emploi par les Capétiens et les Plantagenêts. Néanmoins, il a conservé ces données et elles sont potentiellement très utile dans le cadre de Studium, comme le sont toutes les mentions dans les volumes des Fasti Ecclesiae Gallicanae de chanoines portant ce titre de magister sans autres précisions. L'ampleur des dépouillements rend ces données très utiles et nous devons une grande reconnaissance à John Baldwin pour avoir pris la peine de faire photocopier ses fiches et de nous les avoir transmises amicalement.
Les données ainsi que les images des fiches sont accessibles sur le site Internet à l'adresse suivante : http://studium-baldwin.lamop.fr/.
Les transcriptions des fiches ont été effectuées par des étudiants de Paris 1 Panthéon - Sorbonne mais elles n'ont pas été corrigées par la suite.
description: Relation: https://lamop.hypotheses.org/
Gauge invariance of excitonic linear and nonlinear optical response
Creators: name: Taghizadeh, Alireza
name: Pedersen, T. G.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Materials Science (cond-mat.mtrl-sci)
subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: FOS: Physical sciences

description: We study the equivalence of four different approaches to calculate the excitonic linear and nonlinear optical response of multiband semiconductors. These four methods derive from two choices of gauge, i.e. length and velocity gauges, and two ways of computing the current density, i.e. direct evaluation and evaluation via the time-derivative of the polarization density. The linear and quadratic response functions are obtained for all methods by employing a perturbative density matrix approach within the mean-field approximation. The equivalence of all four methods is shown rigorously, when a correct interaction Hamiltonian is employed for the velocity gauge approaches. The correct interaction is written as a series of commutators containing the unperturbed Hamiltonian and position operators, which becomes equivalent to the conventional velocity gauge interaction in the limit of infinite Coulomb screening and infinitely many bands. As a case study, the theory is applied to hexagonal boron nitride monolayers, and the linear and nonlinear optical response found in different approaches are compared.
description: 11 pages, 3 figures
Is Nova Sco 1994 (GRO 1655-40) a Relic of a GRB ?
Creators: name: Brown, G. E.
name: Lee, C. -H.
name: Lee, H. K.
name: Bethe, H. A.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We suggest Nova Sco 1994 (GRO 1655-40) as a possible relic of a Gamma Ray Burster (GRB) and Type Ib supernova (SN) explosion, showing that there is evidence both that the black hole was spun up by accretion and that there was a supernova explosion. We use the disc energy delivered from the rotational energy of the black hole to power the SN, and give arguments that roughly equal energy goes into the GRB and into the accretion disc to power the supernova.
description: 5 pages, Proceedings of the 5th Huntsville Gamma Ray Burst Symposium, Oct. 18-22, 1999
ФОРМИРОВАНИЕ ЧИТАТЕЛЬСКОЙ И ИНФОРМАЦИОННОЙ КУЛЬТУРЫ МЛАДШИХ ШКОЛЬНИКОВ С ПОМОЩЬЮ РАЗНЫХ ВИДОВ ЧТЕНИЯ (ИЗУЧАЮЩЕГО, ПОИСКОВОГО, ОЗНАКОМИТЕЛЬНОГО, ВЫБОРОЧНОГО И ДР.)
Creators: name: Умарова, Маржана
Publisher: name: Zenodo
Year: 2025

description: В статье рассматривается проблема формирования читательской и информационной культуры у младших школьников как ключевая педагогическая задача современного образования. На основе анализа научных трудов отечественных исследователей (Т.Г. Галактионовой, В.Н. Зборовской, Ю.П. Мелентьевой, Н.В. Пономаревой, С.А. Трубникова) раскрывается сущность читательской культуры как комплексного феномена, включающего культуру отбора, восприятия и осмысления текстов. Особое внимание уделяется трехуровневой модели культуры чтения (предкоммуникативная, коммуникативная, посткоммуникативная фазы) и ее трансформации в условиях цифровизации. Автор анализирует различные способы чтения (изучающее, поисковое, ознакомительное, выборочное) и их роль в развитии информационной грамотности учащихся. Подчеркивается необходимость формирования у детей осознанных читательских практик, критического мышления и навыков работы с мультимодальными текстами. Статья адресована педагогам, библиотекарям и исследователям в области педагогики и библиотековедения.
The Dust Content and Opacity of Actively Star-Forming Galaxies
Creators: name: Calzetti, D.
name: Armus, L.
name: Bohlin, R. C.
name: Kinney, A. L.
name: Koornneef, J.
name: Storchi-Bergmann, T.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: (Abridged) We present far-infrared (FIR) photometry at 150 micron and 205 micron of eight low-redshift starburst galaxies obtained with the ISO Photometer. Five of the eight galaxies are detected in both wavebands and these data are used, in conjunction with IRAS archival photometry, to model the dust emission at lambda>40 micron. The FIR spectral energy distributions (SEDs) are best fitted by a combination of two modified Planck functions, with T~40-55 K (warm dust) and T~20-23 K (cool dust), and with a dust emissivity index epsilon=2. The cool dust can be a major contributor to the FIR emission of starburst galaxies, representing up to 60% of the total flux. This component is heated not only by the general interstellar radiation field, but also by the starburst itself. The cool dust mass is up to ~150 times larger than the warm dust mass, bringing the gas-to-dust ratios of the starbursts in our sample close to Milky Way values, once rescaled for the appropriate metallicity. The ratio between the total dust FIR emission in the range 1-1000 micron and the IRAS FIR emission in the range 40-120 micron is ~1.75, with small variations from galaxy to galaxy. The FIR emission predicted by the dust reddening of the UV-to-nearIR stellar emission is within a factor ~2 of the observed value in individual galaxies and within 20% when averaged over a large sample. If our sample of local starbursts is representative of high-redshift (z>1), UV-bright, star-forming galaxies, these galaxies' FIR emission will be generally undetected in sub-mm surveys, unless (1) their bolometric luminosity is comparable to or larger than that of ultraluminous FIR galaxies and (2) their FIR SED contains a cool dust component.
description: 27 pages, Latex, uses AAS Latex macro, includes 3 embedded postscript Figures, and 9 external postscript tables. Accepted for publication in the Astrophysical Journal
Ecosystem service responses to rewilding: first-order estimates from 27 years of rewilding in the Scottish Highlands
Creators: name: Sophus O. S. E. Zu Ermgassen
name: McKenna, Tom
name: Gordon, Jamie
name: Willcock, Simon
Publisher: name: Taylor & Francis
Year: 2018
Subjects: subject: Evolutionary Biology
subject: FOS: Biological sciences
subject: Ecology
subject: Sociology
subject: FOS: Sociology
subject: Science Policy

description: Rewilding as a conservation strategy is gaining increasing scientific, political and public attention, yet empirical evaluations of its impacts remain scarce, especially with regards to ecosystem services. We provide evidence of the change in three ecosystem services (timber [provisioning], pollination [regulating], and aesthetics [cultural]) from up to 27 years of a moorland rewilding strategy in the Scottish Highlands using a chronosequence of rewilded plots and adjacent controls. These services were assessed in the field and using online surveys. We found that rewilding increased aboveground woody biomass and restored natural tree recruitment processes, although the latter only emerged after at least 15 years of rewilding. Rewilding caused a linear increase in perceived aesthetic quality over the first 27 years, but had no effect on pollination visitation rates. Thus, we conclude that rewilding can be used for ecosystem service recovery in moorland landscapes, but that results vary depending on the preferred service.EDITED BY John Haslett EDITED BY John Haslett
R code and data for "Weighted Software Metrics Aggregation and its Application to Defect Prediction"
Creators: name: Ulan, Maria
name: Löwe, Welf
name: Ericsson, Morgan
name: Wingkvist, Anna
Publisher: name: Zenodo
Year: 2021

description: Replication pack that includes the data and the R scripts to reproduce the results in the paper. README.txt is a file with instructions.
Precision medicine for age-related macular degeneration: current developments and prospects
Creators: name: Biarnés, Marc
name: Vassilev, Vassil
name: Everson Nogoceke
name: Emri, Eszter
name: Rodríguez-Bocanegra, Eduardo
name: Ferraro, Lucia
name: Míriam Garcia
name: Fauser, Sascha
name: Monés, Jordi
name: Lengyel, Imre
name: Tunde Peto
Publisher: name: Taylor & Francis
Year: 2019
Subjects: subject: Medicine
subject: Genetics
subject: FOS: Biological sciences
subject: Neuroscience
subject: Pharmacology
subject: Biotechnology
subject: 59999 Environmental Sciences not elsewhere classified
subject: FOS: Earth and related environmental sciences
subject: Developmental Biology
subject: 111714 Mental Health
subject: FOS: Health sciences
subject: 110309 Infectious Diseases
subject: Computational Biology

description: Introduction: With the aging population, diseases such as age-related macular degeneration (AMD) will become more prevalent. This will increase the demand for provision of care on affected individuals, society, and the health-care system. To develop the best, individually tailored treatment for every patient, however, remains challenging. Areas covered: Recent identifications of interactions between environmental, lifestyle, genetic, and non-genetic factors opened the potential for developing personalized approaches for the prevention and treatment of AMD. In this review, we will discuss the implications of these interactions for early to late disease stage conversion, for neovascularization, and for cell atrophy. We will put the findings of recent studies within the context of the regulatory framework requirements surrounding the development of personalized medicine approach to AMD. Expert commentary: Precision medicine is now at a stage that it has its theoretical framework in place for the management of risk for patients with AMD requiring early diagnosis and timely treatment as several key components for such an approach are now clearly identified and are being applied to clinical developments successfully.
Hierarchical clustering and the baryon distribution in galaxy clusters
Creators: name: Tittley, Eric R.
name: Couchman, H. M. P.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: The baryon fraction of galaxy clusters in numerical simulations is found to be dependant on the cluster formation method. In all cases, the gas is anti-biased compared with the dark matter. However, clusters formed hierarchically are found to be more depleted in baryons than clusters formed non-hierarchically. There is a depletion of 10 to 15% for hierarchically formed clusters while the depletion is less than 10% for those clusters formed non-hierarchically. This difference is dependent on the mass of the clusters. The mean baryon enrichment profile for the hierarchically formed clusters shows an appreciable baryon enhancement around the virial radius not seen in the clusters formed without substructure. If this phenomenon applies to real clusters, it implies that determinations of the baryon fractions in clusters of galaxies require data extending beyond the virial radius of the clusters in order to achieve an unbiased value.
description: 13 pages including 2 tables and 2 figures. Submitted to MNRAS
$b \to s(d) γ$ with a Vector-like Quark as Fourth-generation
Creators: name: Handoko, L. T.
name: Pages, T. Morozumi
name: :
name: pages, 19
Publisher: name: arXiv
Year: 1994
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We study the implications of a vector-like quark, especially a down-type vector-like quark in $b \rightarrow s(d) γ$ including the neutral Higgs in the calculation. After analyzing some possible constraints for the mixing, the contribution may be significant for the $b \rightarrow d γ$, but not for the $b \rightarrow s γ$. We also find that the FCNC among ordinary quarks vanishes for a special form of down-type quark mass matrix.
description: 4 figures are included and 1 figure is excluded
Toward Understanding the B[e] Phenomenon. VII. AS 386, a single-lined binary with a candidate black hole component
Creators: name: Khokhlov, S. A.
name: Miroshnichenko, A. S.
name: Zharikov, S. V.
name: Manset, N.
name: Arkharov, A. A.
name: Efimova, N.
name: Klimanov, S.
name: Larionov, V M.
name: Kusakin, A. V.
name: Kokumbaeva, R. I.
name: Omarov, Ch. T.
name: Kuratov, K. S.
name: Kuratova, A. K.
name: Rudy, R. J.
name: Laag, E. A.
name: Crawford, K. B.
name: Swift, T. K.
name: Puetter, R. C.
name: Perry, R. B.
name: Chojnowski, S. D.
name: Agishev, A.
name: Caton, D. B.
name: Hawkins, R. L.
name: Smith, A. B.
name: Reichart, D. E.
name: Kouprianov, V. V.
name: Haislip, J. B.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: We report the results of spectroscopic and photometric observations of the emission-line object AS 386. For the first time, we found that it exhibits the B[e] phenomenon and fits the definition of an FS CMa type object. The optical spectrum shows the presence of a B-type star with the following properties: T_ eff = 11000+/-500 K, log L/L_sun = 3.7+/-0.3, a mass of 7+/-1 M_sun, and a distance D = 2.4+/-0.3 kpc from the Sun. We detected regular radial velocity variations of both absorption and emission lines with the following orbital parameters: P_orb = 131.27+/-0.09 days, semi-amplitude K_1 = 51.7+/-3.0 km/s, systemic radial velocity gamma = -31.8+/-2.6 km/s, and a mass function of f(m) = 1.9+/-0.3 M_sun. AS 386 exhibits irregular variations of the optical brightness (V=10.92+/-0.05 mag), while the near-IR brightness varies up to ~0.3 mag following the spectroscopic period. We explain this behavior by a variable illumination of the dusty disk inner rim by the B-type component. Doppler tomography based on the orbital variations of emission-line profiles shows that the material is distributed near the B-type component and in a circumbinary disk. We conclude that the system has undergone a strong mass transfer that created the circumstellar material and increased the B-type component mass. The absence of any traces of a secondary component, whose mass should be >= 7 M_sun, suggests that it is most likely a black hole.
description: 18 pages, 4 tables, 13 figures, Accepted for publication in ApJ
The short-run relationship between inequality and growth: evidence from OECD regions during the Great Recession
Creators: name: Royuela, Vicente
name: Veneri, Paolo
name: Ramos, Raul
Publisher: name: Taylor & Francis
Year: 2018
Subjects: subject: Medicine
subject: Sociology
subject: FOS: Sociology
subject: Developmental Biology
subject: Cancer
subject: Computational Biology

description: This paper provides evidence on the relationship between income inequality and economic growth in Organisation for Economic Co-operation and Development (OECD) regions during the decade 2003–13. It combines household survey data and macroeconomic databases, covering over 200 comparable regions in 15 OECD countries. The econometric results, based on two alternative sets of instruments, highlight a general negative association between inequalities and economic growth since the start of the economic crisis. This relationship is sensitive to the type of urban structure. Higher inequalities seem to be more detrimental for growth in regions characterized by medium to large-sized cities, while regions characterized by small cities and rural areas are less affected.
Additional file 1 of Identification and characterization of HAK/KUP/KT potassium transporter gene family in barley and their expression under abiotic stress
Creators: name: Cai, Kangfeng
name: Zeng, Fanrong
name: Wang, Junmei
name: Zhang, Guoping
Publisher: name: figshare
Year: 2021
Subjects: subject: Genetics
subject: FOS: Biological sciences

description: Additional file 1. Protein sequences of 27 HvHAKs.
Mapping the CMB Sky: The BOOMERANG experiment
Creators: name: de Bernardis, P.
name: Ade, P. A. R.
name: Artusa, R.
name: Bock, J. J.
name: Boscaleri, A.
name: Crill, B. P.
name: De Troia, G.
name: Farese, P. C.
name: Giacommetti, M.
name: Hristov, V. V.
name: Iacoangeli, A.
name: Lange, A. E.
name: Lee, A. T.
name: Masi, S.
name: Martinis, L.
name: Mason, P. V.
name: Mauskopf, P. D.
name: Melchiorri, F.
name: Miglio, L.
name: Montroy, T.
name: Netterfield, C. B.
name: Pascale, E.
name: Piacentini, F.
name: Richards, P. L.
name: Ruhl, J. E.
name: Scaramuzzi, F.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We describe the BOOMERanG experiment, a stratospheric balloon telescope intended to measure the Cosmic Microwave Background anisotropy at angular scales between a few degrees and ten arcminutes. The experiment has been optimized for a long duration (7 to 14 days) flight circumnavigating Antarctica at the end of 1998. A test flight was performed on Aug.30, 1997 in Texas. The level of performance achieved in the test flight was satisfactory and compatible with the requirements for the long duration flight.
description: 11 pages, 6 figures
Anti-screening of the Galileon force around a disk center hole
Creators: name: Ogawa, Hiromu
name: Hiramatsu, Takashi
name: Kobayashi, Tsutomu
Publisher: name: arXiv
Year: 2018
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: The Vainshtein mechanism is known as an efficient way of screening the fifth force around a matter source in modified gravity. This has been verified mainly in highly symmetric matter configurations. To study how the Vainshtein mechanism works in a less symmetric setup, we numerically solve the scalar field equation around a disk with a hole at its center in the cubic Galileon theory. We find, surprisingly, that the Galileon force is enhanced, rather than suppressed, in the vicinity of the hole. This anti-screening effect is larger for a thinner, less massive disk with a smaller hole. At this stage our setup is only of academic interest and its astrophysical consequences are unclear, but this result implies that the Vainshtein screening mechanism around less symmetric matter configurations is quite nontrivial.
description: 11 pages, 18 figures
Meson Supermultiplet Decay Constants
Creators: name: Jones, N.
name: Delbourgo, R.
Publisher: name: arXiv
Year: 1994
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We use a covariant supermultiplet theory to determine the primary coupling constant associated with several types of two-body meson decay. Despite the diverse range of decays considered the primary coupling constant is surprisingly uniform. We envisage the extension of the techniques to heavy quark cases, including as preliminary examples the calculation of the $D^{*+}$ and $D^{*0}$ total decay widths with results $57.7 \pm 1.5$ KeV and $42.5 \pm 2.6$ KeV respectively, as well as some predictions about $D^*$ and $B^*$ radiative decays. (3 uuencoded Postscript Files are appended at the end of the TexFile.)
description: 18 pages, UTAS-PHYS-94-26, Latex
A Stationary Core with a One-sided Jet in the Center of M81
Creators: name: Bietenholz, M. F.
name: Bartel, N.
name: Rupen, M. P.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: The nucleus of M81 was observed at 8.3 GHz with VLBI at 20 epochs over 4.5yrs, with a linear resolution at the source of about 2000 AU or 0.01 pc. Phase-referenced mapping with respect to the geometric center of supernova 1993J enabled us to find, with a standard error of about 600 AU, a stationary point in the source. We identify this point as the location of the core and the putative black hole at the gravitational center of the galaxy. The upper bound on the core's average velocity on the sky is <730 km/s. A short, one-sided jet extends from the core. The orientation of the jet varies smoothly, with timescales of about 1yr and an rms of 6degrees about the mean of 50degrees. Occasionally the jet appears to bend to the east. The length of the jet is only about 1 mas (3,600 AU), and varies with an rms of about 20%. The inferred speeds are below 0.08c. The total flux density of the core-jet varies erratically, changing on occasion by a factor of two over a few weeks, without any significant changes in the source size and orientation. The inferred velocity of the plasma flow is >0.25c. The results are consistent with a model in which plasma condensations with short lifetimes are ejected relativistically from the core on a timescale of less than a few weeks, and then travel along a tube whose pattern and geometry are also variable but only on a timescale of about one year. The central engine of M81 has qualitative similarities to those of powerful the AGN of radio galaxies and quasars, and may also represent in power and size a scaled-up version of the largely hidden nucleus in our own Galaxy.
description: 31 pages (including Figures); Accepted for publication in the Astrophysical Journal
A morphology-independent data analysis method for detecting and characterizing gravitational wave echoes
Creators: name: Tsang, Ka Wa
name: Rollier, Michiel
name: Ghosh, Archisman
name: Samajdar, Anuradha
name: Agathos, Michalis
name: Chatziioannou, Katerina
name: Cardoso, Vitor
name: Khanna, Gaurav
name: Broeck, Chris Van Den
Publisher: name: arXiv
Year: 2018
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: The ability to directly detect gravitational waves has enabled us to empirically probe the nature of ultra-compact relativistic objects. Several alternatives to the black holes of classical general relativity have been proposed which do not have a horizon, in which case a newly formed object (e.g. as a result of binary merger) may emit echoes: bursts of gravitational radiation with varying amplitude and duration, but arriving at regular time intervals. Unlike in previous template-based approaches, we present a morphology-independent search method to find echoes in the data from gravitational wave detectors, based on a decomposition of the signal in terms of generalized wavelets consisting of multiple sine-Gaussians. The ability of the method to discriminate between echoes and instrumental noise is assessed by inserting into the noise two different signals: a train of sine-Gaussians, and an echoing signal from an extreme mass-ratio inspiral of a particle into a Schwarzschild vacuum spacetime, with reflective boundary conditions close to the horizon. We find that both types of signals are detectable for plausible signal-to-noise ratios in existing detectors and their near-future upgrades. Finally, we show how the algorithm can provide a characterization of the echoes in terms of the time between successive bursts, and damping and widening from one echo to the next.
description: 5 pages, 4 figures
title: ADCO, Abbaye de Cîteaux, 'Transcrits des titres de la layette marquée QQ, 1er cartable, liasses 1, 2 et 3' / Cartulaire d'Ouges (XVIIIe siècle, 2e moitié), Cart. 196 (11 H 938), f. 0063
Creators: name: de la Côte d'Or, Archives départementales
name: CG21/F.PETOT/2017
name: Petot, Frédéric
name: Archives Départementales De La Côte-D'Or
name: Petot, Frédérique
name: Projet CBMA
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2020
Subjects: subject: Laboratoire de Médiévistique Occidentale de Paris
subject: Corpus Burgundiae Medii Aevi
subject: Chartes de la Bourgogne du Moyen Âge
subject: cartulaire
subject: LaMOP

description: Abbaye de Cîteaux, 'Transcrits des titres de la layette marquée QQ, 1er cartable, liasses 1, 2 et 3' / Cartulaire d'Ouges (XVIIIe siècle, 2e moitié), Archives départementales de la Côte-d'Or, Cart. 196 (11 H 938), Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Abbaye de Cîteaux, 'Transcrits des titres de la layette marquée QQ, 1er cartable, liasses 1, 2 et 3' / Cartulaire d'Ouges (XVIIIe siècle, 2e moitié), Archives départementales de la Côte-d'Or, Cart. 196 (11 H 938), f. 0063, 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
Additional file 9 of m6A demethylase ALKBH5 inhibits tumor growth and metastasis by reducing YTHDFs-mediated YAP expression and inhibiting miR-107/LATS2â€“mediated YAP activity in NSCLC
Creators: name: Jin, Dan
name: Guo, Jiwei
name: Wu, Yan
name: Yang, Lijuan
name: Wang, Xiaohong
name: Du, Jing
name: Dai, Juanjuan
name: Chen, Weiwei
name: Gong, Kaikai
name: Miao, Shuang
name: Li, Xuelin
name: Sun, Hongliang
Publisher: name: figshare
Year: 2020
Subjects: Biochemistry
Molecular Biology
Pharmacology
Biological Sciences not elsewhere classified
Developmental Biology
Cancer

description: Additional file 9 Fig. S8. YTHDF1 promotes tumor growth and metastasis in NSCLC.