cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Shell-model calculations of stellar weak interaction rates: II. Weak rates for nuclei in the mass range A=45-65 in supernovae environment
Creators: name: Langanke, K.
name: Martinez-Pinedo, G.
Publisher: name: arXiv
Year: 2000
Subjects: subject: Nuclear Theory (nucl-th)
subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Based on large-scale shell model calculations we have determined the electron capture, positron capture and beta-decay rates on more than 100 nuclei in the mass range A=45-65. The rates are given for densities ρY_e =10^7-10^{10} mol/cm^3 and temperatures T=10^9-10^{10} K and hence are relevant for both types of supernovae (Type Ia and Type II). The shell model electron capture rates are significantly smaller than currently assumed. For proton-to-baryon ratios Y_e=0.42-0.46 mol/g, the beta-decay rates are faster than the electron capture rates during the core collapse of a massive star.
description: 16 pages, 10 figures
DataNord: Empowering Bremen's Research Community in Data Literacy. An Interdisciplinary Data Competence Center for Bremen.
Creators: name: Steinmann, Lena
name: Hörner, Tanja
Publisher: name: Zenodo
Year: 2024

description: The poster "DataNord: Empowering Bremen’s Research Community in Data Literacy" outlines the mission and structure of DataNord, an interdisciplinary data competence center in Bremen. It has been presented during the second Bremen Research Data Day in 2024 by Dr. Lena Steinmann and Dr. Tanja Hörner.

DataNord's mission: Enhance data skills among researchers at all career levels through interdisciplinary collaboration.

Scientific Profile Areas: Marine and Environmental Sciences, Material Sciences and Engineering, Health Sciences, Social Sciences, and Humanities.

Services Offered:

Learning Opportunities: In-depth training programs, Data Train, Lunch & Learn sessions, Data Hacks, and Summer Schools.

Expert Advice: Help Desk for data management and science support throughout the research lifecycle.

Consultation and Networking: Data Community Club, Hacky Hours & Data Stories, Citizen Science initiatives, and events connecting various sectors.

DataNord is supported by the Federal Ministry of Education and Research and funded by the European Union - NextGenerationEU.
title: PAC-Australia (2023): Recording with MV, word list n°2
title: 2019 - post PSS2
titleType: AlternativeTitle
Creators: name: Mas, Erwanne
Publisher: name: COCOON - https://cocoon.huma-num.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2023
Subjects: subject: Australian English
subject: eng

description: PAC word list n°2
description: Conforms to: Praat textgrid
description: Conforms to: doi:10.34847/cocoon.49aefa90-8c1f-3ba8-a099-0ebefc6a2aa7
title: ADCO, Cartulaire général de Cîteaux, dit de Jean de Cirey, (XVe siècle), tome VIII, Cart. 192 (11 H 77), 295 folios, f. 0231v
Creators: name: de la Côte d'Or, Archives départementales
name: Archives Départementales De La Côte-D'Or
name: Petot, Frédérique
name: Petot, Frédéric
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 VIII, Archives départementales de la Côte-d'Or, Cart. 192 (11 H 77), 295 folios, f. 0231v, 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 VIII, Archives départementales de la Côte-d'Or, Cart. 192 (11 H 77), 295 folios, f. 0231v, 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
ОБУСЛОВЛЕННОСТЬ ОБРАТНЫХ ЗАДАЧ И ИТЕРАЦИОННЫЕ МЕТОДЫ ИХ РЕШЕНИЯ
Creators: name: Сергей Борисович Сорокин
Publisher: name: Труды Международной конференции «АПВПМ»
Year: 2019
Subjects: задача Коши
эллиптические уравнения
неявный двухслойный итерационный метод
разделение переменных.

description: В работе строятся и исследуются неявные градиентные двухслойные итерационные методы численного решения задачи Коши для эллиптических уравнений. Приводятся результаты вычислительных экспериментов.
Additional file 1 of Effects of transport stress on pathological injury and expression of main heat shock proteins in the caprine stomach
Creators: name: Hu, Wei
name: Ye, Tian
name: Yang, Yanzhen
name: Liu, Ben
name: Zheng, Wenya
Publisher: name: figshare
Year: 2020
Subjects: subject: Biophysics
subject: Biochemistry
subject: Microbiology
subject: FOS: Biological sciences
subject: Genetics
subject: Molecular Biology
subject: Biotechnology
subject: Biological Sciences not elsewhere classified
subject: Developmental Biology
subject: Mental Health

description: Additional file 1. Western blot instructions and original images.
ЧИСЛЕННОЕ МОДЕЛИРОВАНИЕ ВОЛНОВЫХ ПРОЦЕССОВ В ГЕОЛОГИЧЕСКИХ СРЕДАХ С ГАЗОВЫМИ КАРМАНАМИ В ЗОНЕ АРКТИЧЕСКОГО ШЕЛЬФА С ПОМОЩЬЮ СЕТОЧНО-ХАРАКТЕРИСТИЧЕСКОГО МЕТОДА
Creators: name: Стогний Полина Владимировна
name: Хохлов Николай Игоревич
name: Петров Игорь Борисович
Publisher: name: Труды Международной конференции «АПВПМ»
Year: 2019
Subjects: Арктика
сеточно-характеристический метод
газовые карманы

description: В работе представлены результаты численного моделирования распространения сейсмических волн в моделях с газонасыщенными средами в течение четырехлетнего периода. Моделирование проводилось с помощью сеточно-характеристического метода на основе схемы Русанова для трехмерного случая. Представлены волновые картины сейсмических откликов от различных геологических слоев с течением времени
On the Integrability of the Geodesic Flow on a Friedmann-Robertson-Walker Spacetime
Creators: name: Astorga, Francisco
name: Salazar, J. Felix
name: Zannias, Thomas
Publisher: name: arXiv
Year: 2017
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: Classical Physics (physics.class-ph)
subject: FOS: Physical sciences
subject: 83 Relativity and Gravitation

description: We study the geodesic flow on the cotangent bundle of a Friedman-Robertson-Walker spacetime (M, g). On this bundle, the HamiltonJacobi equation is completely separable and this separability leads us to construct four linearly independent integrals in involution i.e. Poisson commuting amongst themselves and pointwise linearly independent. These integrals involve the six linearly independent Killing fields of the background metric g. As a consequence, the geodesic flow on an FRW background is completely integrable in the Liouville-Arnold sense. For the case of a spatially closed universe we construct families of invariant by the flow sub manifolds.
description: 34 pages, no figures
A Search for Resonant Structures in the Zodiacal Cloud with COBE DIRBE: The Mars Wake and Jupiter's Trojan Clouds
Creators: name: Kuchner, Marc J.
name: Reach, William T.
name: Brown, Michael E.
Publisher: name: arXiv
Year: 2000
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We searched the COBE DIRBE Sky and Zodi Atlas for a wake of dust trailing Mars and for Trojan dust near Jupiter's L5 Lagrange point. We compare the DIRBE images to a model Mars wake based on the empirical model of the Earth's wake as seen by the DIRBE and place a 3-sigma upper limit on the fractional overdensity of particles in the Mars wake of 18% of the fractional overdensity trailing the Earth. We place a 3-sigma upper limit on the effective emitting area of large (10-100 micron diameter) particles trapped at Jupiter's L5 Lagrange point of 6 x 10^17 cm^2, assuming that these large dust grains are distributed in space like the Trojan asteroids. We would have detected the Mars wake if the surface area of dust in the wake scaled simply as the mass of the planet times the Poynting-Robertson time scale.
description: Sixteen pages, and figures 1, 2, 3a, 3b, 4, 5, 6, and 7. Accepted for publication in Icarus
PAC-Australia (2023): Recording with MV, "A Christmas interview"
Creators: name: Mas, Erwanne
Publisher: name: COCOON - https://cocoon.huma-num.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2023
Subjects: subject: Australian English
subject: eng

description: PAC-LVTI Reading Task
description: Conforms to: Praat textgrid
description: Conforms to: doi:10.34847/cocoon.49aefa90-8c1f-3ba8-a099-0ebefc6a2aa7
SBS 0909+532: A New Double Gravitational Lens or Binary Quasar?
Creators: name: Kochanek, C. S.
name: Falco, E. E.
name: Schild, R.
name: Dobrzycki, A.
name: Engels, D.
name: Hagen, H. -J.
Publisher: name: arXiv
Year: 1996
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: The z=1.377, B=17.0 mag quasar SBS 0909+532 A, B is a double with two images separated by 1.107 +/- 0.006 arcsec. Because the faint image has an emission line at the same wavelength as the MgII 2798 A emission line of the quasar, and lacks the broad MgIb absoption feature expected for a star with the same colors (a K star), we conclude that image B is a quasar with similar redshift to image A. The relative probabilities that the double is the smallest separation (4.8/h kpc for Ω_0=1) correlated quasar pair or a gravitational lens are \sim 1:10^6. If the object is a lens, the mean lens redshift is $=0.5$ with 90% confidence bounds of 0.18 < z_l < 0.83 for Ω_0=1. If the lens is an elliptical galaxy, we expect it to be brighter than I < 19.5 mag. The broad band flux ratio varies with wavelength, with ΔI=0.31, ΔR=0.58, and ΔB=1.29 magnitudes, which is difficult to reconcile with the lensing hypothesis.
description: 19 pages, 6 figures, ApJ in press
Carnet nº 25, commencé à Saïgon (p. 40)
Creators: name: Péraire, Lucien
name: CNRS
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2023

description: created: 21-1-1932
ТРЁХМЕРНОЕ МОДЕЛИРОВАНИЕ СИГНАЛОВ ЭЛЕКТРОМАГНИТНОГО ЗОНДА С ТОРОИДАЛЬНЫМИ КАТУШКАМИ
Creators: name: Суродина Ирина Владимировна
Publisher: name: Труды Международной конференции «АПВПМ»
Year: 2019
Subjects: электромагнитный каротаж
математическое моделирование
зонд с тороидальными катушками
конечные разности
система линейных алгебраических уравнений
итерационные методы
прямые методы

description: В работе рассматривается математическое моделирование электромагнитных откликов нового каротажного прибора в несимметричных изотропных средах, выполненное с помощью конечно-разностного метода. Описывается постановка задачи, методы решения. Приводятся численные эксперименты, показывающие необходимость центратора прибора для его использования на практике. Обсуждаются результаты моделирования
title: PAC-Australia (2023): Recording with MV, word list n°1
title: 2019 - post PSS2
titleType: AlternativeTitle
Creators: name: Mas, Erwanne
Publisher: name: COCOON - https://cocoon.huma-num.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2023
Subjects: subject: Australian English
subject: eng

description: PAC word list n°1
description: Conforms to: Praat textgrid
description: Conforms to: doi:10.34847/cocoon.49aefa90-8c1f-3ba8-a099-0ebefc6a2aa7
Four and Three Loop Calculations in QCD: Theory and Applications
Creators: name: Chetyrkin, K. G.
Publisher: name: arXiv
Year: 1996
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: The talk briefly reviews the current state of the art in doing multiloop QCD calculations in a completely analytic way. In particular, we discuss recent analytical calculation of 4-loop O(alpha_s**3) gluino contribution to R(s) and its implications to the Z boson and tau-lepton decay rates.
description: 14 pages, LaTeX, 3 figures; epsfig.sty and subfig.sty are used. Invited talk at the Cracow International Symposium on Radiative Corrections 1-5 August 1996, Cracow, Poland
Keck Speckle Imaging of the White Dwarf G29-38: No Brown Dwarf Companion Detected
Creators: name: Kuchner, Marc J.
name: Koresko, Christopher D.
name: Brown, Michael E.
Publisher: name: arXiv
Year: 2000
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: The white dwarf Giclas 29-38 has attracted much attention due to its large infrared excess and the suggestion that excess might be due to a companion brown dwarf. We observed this object using speckle interferometry at the Keck telescope, obtaining diffraction-limited resolution (55 milliarcseconds) at K band, and found it unresolved. Assuming the entire K band excess is due to a single point-like companion, we place an upper limit on the binary separation of 30 milliarcseconds, or 0.42 AU at the star's distance of 14.1 pc. This result, combined with astroseismological data and other images of G29-38, supports the hypothesis that the source of the near-infrared excess is not a cool companion but a dust cloud.
description: 7 pages, 2 figures
Two-point boundary correlation functions of dense loop models
Creators: name: Morin-Duchesne, Alexi
name: Jacobsen, Jesper Lykke
Publisher: name: arXiv
Year: 2017
Subjects: subject: Statistical Mechanics (cond-mat.stat-mech)
subject: High Energy Physics - Theory (hep-th)
subject: Mathematical Physics (math-ph)
subject: FOS: Physical sciences

description: We investigate six types of two-point boundary correlation functions in the dense loop model. These are defined as ratios $Z/Z^0$ of partition functions on the $m\times n$ square lattice, with the boundary condition for $Z$ depending on two points $x$ and $y$. We consider: the insertion of an isolated defect (a) and a pair of defects (b) in a Dirichlet boundary condition, the transition (c) between Dirichlet and Neumann boundary conditions, and the connectivity of clusters (d), loops (e) and boundary segments (f) in a Neumann boundary condition. For the model of critical dense polymers, corresponding to a vanishing loop weight ($β= 0$), we find determinant and pfaffian expressions for these correlators. We extract the conformal weights of the underlying conformal fields and find $Δ= -\frac18$, $0$, $-\frac3{32}$, $\frac38$, $1$, $\tfrac θπ(1+ \tfrac{2θ}π)$, where $θ$ encodes the weight of one class of loops for the correlator of type f. These results are obtained by analysing the asymptotics of the exact expressions, and by using the Cardy-Peschel formula in the case where $x$ and $y$ are set to the corners. For type b, we find a $\ln|x-y|$ dependence from the asymptotics, and a $\ln (\ln n)$ term in the corner free energy. This is consistent with the interpretation of the boundary condition of type b as the insertion of a logarithmic field belonging to a rank two Jordan cell. For the other values of $β= 2 \cos λ$, we use the hypothesis of conformal invariance to predict the conformal weights and find $Δ= Δ_{1,2}$, $Δ_{1,3}$, $Δ_{0,\frac12}$, $Δ_{1,0}$, $Δ_{1,-1}$ and $Δ_{\frac{2θ}λ+1,\frac{2θ}λ+1}$, extending the results of critical dense polymers. With the results for type f, we reproduce a Coulomb gas prediction for the valence bond entanglement entropy of Jacobsen and Saleur.
description: 49 pages. v2: minor changes
M-Subdwarfs: Spectroscopic Classification and the Metallicity Scale
Creators: name: Gizis, John E.
Publisher: name: arXiv
Year: 1996
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present a spectroscopic classification system for M-dwarfs and M-subdwarfs based on quantitative measures of TiO and CaH features in the region 6200 - 7400 Angstroms. Our sample of cool stars covers the range from solar metallicity stars to the most extreme subdwarfs known. Using synthetic spectra computed by Allard and Hauschildt (1995), we derive metallicities for the stars. Stars are classified as dwarfs (M V), subdwarfs (sdM), or extreme subdwarfs (esdM). These classifications correspond to [m/H] ~ 0.0, -1.2, and -2.0 respectively. Our metallicity scale agrees with theoretical HR diagrams and HST globular cluster measurements. We discuss some nearby subdwarfs of particular interest in light of our metallicity scale.
description: AASTeX, 43 pages, 11 figures, A.J. accepted
“БУДУЩЕЕ ЗЕМЛИ”: ГЛОБАЛЬНЫЕ ПРОБЛЕМЫ И РАДИАЦИОННОЕ ПОЛЕ, РАДИАЦИОННЫЙ ФОРСИНГ И ДИСТАНЦИОННОЕ ЗОНДИРОВАНИЕ ЗЕМЛИ
Creators: name: Сушкевич Тамара Алексеевна
name: Стрелков Сергей Александрович
name: Максакова Светлана Викторовна
Publisher: name: Труды Международной конференции «АПВПМ»
Year: 2019
Subjects: Будущее Земли
радиационное поле
световые технологии

description: Фундаментальные основы для реализации Всемирной научной ПРОГРАММЫ "Будущее Земли" (World Global Research Projects "Future Earth" ) и исследования Климатической системы Земли под влиянием радиационного форсинга заложены в XX-м веке благодаря изобретению компьютера и выхода человека в космос и, конечно, достижений в математике. Сложнейшие задачи эволюции, климата, экологии, глобального мониторинга и дистанционного зондирования Земли (ДЗЗ) с гиперспектральными подходами и нанодиагностикой природной среды и объектов предлагается рассматривать как сопряженные. Электромагнитное излучение — единое физическое поле, объединяющее радиационное поле Земли с радиационно–активными компонентами. Гиперспектральное дистанционное зондирование Земли — важнейшая технология оценки воздействия естественно-природных и антропогенных факторов на планету Земля.
title: PAC-Australia (2023): Recording with NR2, word list n°2
title: 2019 - post PSS2
titleType: AlternativeTitle
Creators: name: Mas, Erwanne
Publisher: name: COCOON - https://cocoon.huma-num.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2023
Subjects: subject: Australian English
subject: eng

description: PAC word list n°2
description: Conforms to: Praat textgrid
description: Conforms to: doi:10.34847/cocoon.49aefa90-8c1f-3ba8-a099-0ebefc6a2aa7
Description of quadrupole collectivity in N ~ 20 nuclei with techniques beyond the mean field
Creators: name: Rodriguez-Guzman, R. R.
name: Egido, J. L.
name: Robledo, L. M.
Publisher: name: arXiv
Year: 2000
Subjects: subject: Nuclear Theory (nucl-th)
subject: FOS: Physical sciences

description: Properties of the ground and several collective excited states of the light nuclei ^{30,32,34}Mg are described in the framework of the angular momentum projected Generator Coordinate Method using the quadrupole moment as collective coordinate and the Gogny force as the effective interaction. The calculated excitation energies and B(E2) transition probabilities agree reasonably well with experiment. The results clearly indicate that both the restoration of the rotational symmetry and the quadrupole dynamics are key ingredients for the description of the properties of the above mentioned nuclei.
description: 15 pages, 4 figures, extended version
PAC-Australia (2023): Recording with NR2, "A Christmas interview"
Creators: name: Mas, Erwanne
Publisher: name: COCOON - https://cocoon.huma-num.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2023
Subjects: subject: Australian English
subject: eng

description: PAC-LVTI Reading Task
description: Conforms to: Praat textgrid
description: Conforms to: doi:10.34847/cocoon.49aefa90-8c1f-3ba8-a099-0ebefc6a2aa7
О РЕШЕНИИ ОБРАТНОЙ ГРАНИЧНОЙ ЗАДАЧИ ТЕПЛОПРОВОДНОСТИ ДЛЯ ШАРА, СОСТОЯЩЕГО ИЗ КОМПОЗИТНЫХ МАТЕРИАЛОВ
Creators: name: Танана Виталий Павлович
name: Марков Борис Анатольевич
Publisher: name: Труды Международной конференции «АПВПМ»
Year: 2019
Subjects: обратные задачи
композитные материалы
погрешность приближённого решения

description: В работе предлагается постановка обратной граничной задачи теплопроводности композитных материалов для шара. Впервые обратная граничная задача для уравнения теплопроводности была рассмотрена в [1]. Сложность решения задачи состоит в том, что не удаётся использовать классическое решение, так как, в силу композитности материала, производная решения терпит разрыв на границе раздела сред. Для обратной задачи приведена оценка погрешности [4, 8] приближённого решения.
Quenched Chiral Perturbation Theory for Vector Mesons
Creators: name: Booth, Michael
name: Chiladze, George
name: Falk, Adam F.
Publisher: name: arXiv
Year: 1996
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: High Energy Physics - Lattice (hep-lat)
subject: FOS: Physical sciences

description: We develop quenched chiral perturbation theory for vector mesons made of light quarks, in the limit where the vector meson masses are much larger than the pion mass. We use this theory to extract the leading nonanalytic dependence of the vector meson masses on the masses of the light quarks. By comparing with analogous quantities computed in ordinary chiral perturbation theory, we estimate the size of quenching effects, observing that in general they can be quite large. This estimate is relevant to lattice simulations, where the $ρ$ mass is often used to set the lattice spacing.
description: 18 pages, 8 figures, uses REVTeX and epsf.sty
ВОССТАНОВЛЕНИЕ КОЭФФИЦИЕНТОВ ОТРАЖЕНИЯ ЗЕМНОЙ ПОВЕРХНОСТИ ПО ДАННЫМ ПРИБОРОВ MODIS, САНГУР, ГСА И МСУ-100
Creators: name: Тарасенков Михаил Викторович
name: Белов Владимир Васильевич
name: Энгель Марина Владимировна
name: Зимовая Анна Викторовна
name: Гриднев Юрий Владимирович
Publisher: name: Труды Международной конференции «АПВПМ»
Year: 2019
Subjects: атмосферная коррекция
коэффициент отражения земной поверхности
метод МонтеКарло
MODIS
САНГУР
ГСА
МСУ-100

description: Рассматриваются результаты восстановления коэффициентов отражения земной поверхности по спутниковым измерениям приборов MODIS, Сангур, ГСА и МСУ-100. Результаты получены с помощью разработанного программного обеспечения. Решение задачи состоит в формировании, исходя из спутниковых или наземных измерений, моделей атмосферы; моделировании методом Монте-Карло потоков, формирующих принимаемое излучение; и решении обратной задачи восстановления коэффициентов отражения земной поверхности по измерениям интенсивности принимаемого излучения.
An 11.6 Micron Keck Search For Exozodiacal Dust
Creators: name: Kuchner, Marc J.
name: Brown, Michael E.
name: Koresko, Christopher D.
Publisher: name: arXiv
Year: 2000
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We have begun an observational program to search nearby stars for dust disks that are analogous to the disk of zodiacal dust that fills the interior of our solar system. We imaged six nearby main-sequence stars with the Keck telescope at 11.6 microns, correcting for atmosphere-induced wavefront aberrations and deconvolving the point spread function via classical speckle analysis. We compare our data to a simple model of the zodiacal dust in our own system based on COBE/DIRBE observations and place upper limits on the density of exozodiacal dust in these systems.
description: 10 pages, figure1, figure2, figure3, and figures 4a-e
The Complex Broadband X-ray Spectrum of the Starburst Galaxy M82
Creators: name: Moran, Edward C.
name: Lehnert, Matthew D.
Publisher: name: arXiv
Year: 1996
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: The broadband X-ray spectrum of the prototypical starburst galaxy M82 is very complex. At least three spectral components are required to fit the combined ROSAT and ASCA spectrum in the 0.1--10 keV range. The observed X-ray flux in this band is dominated by a hard Gamma = 1.7, heavily absorbed power law component which originates in the nucleus and near-nuclear disk of the galaxy. Among the candidates for the origin of this hard X-ray emission, the most plausible appears to be inverse-Compton scattered emission from the interaction of M82's copious infrared photon flux with supernova-generated relativistic electrons. The measured intrinsic luminosity of the power law component agrees closely with calculations of the expected inverse-Compton luminosity. Moreover, the radio and X-ray emission in the nucleus of M82 have the same spectral slope, which should be the case if both types of emission are non- thermal and are associated with a common population of electrons. The other two spectral components, thermal plasmas with characteristic temperatures kT = 0.6 and 0.3 keV, are associated with the star formation and starburst-driven wind in M82. The warmer thermal component is heavily absorbed as well and must also originate in the central region of the galaxy. The softer thermal component, however, is not absorbed, and is likely to represent the X-ray emission which extends along M82's minor axis. The amount of absorption required in the three-component model suggests that the intrinsic luminosity of M82 in the 0.1--10 keV band is about four times greater than its observed luminosity of 4 x 10(40) ergs/s.
description: 23 pages, TeX, seven postscript figures, three tables Accepted for the March 20, 1997 issue of ApJ
ВАРИАЦИОННЫЕ МЕТОДЫ ПОСТРОЕНИЯ РАЗНОСТНЫХ УРАВНЕНИИ И ИТЕРАЦИОННЫХ АЛГОРИТМОВ ДЛЯ ПРИБЛИЖЕННОГО РЕШЕНИЯ ЗАДАЧИ ДИРИХЛЕ
Creators: name: Темирбеков Нурлан Муханович
name: Жаксылыкова Жадра Рахметовна
Publisher: name: Труды Международной конференции «АПВПМ»
Year: 2019
Subjects: эллиптическое уравнение второго порядка
задача Дирихле
разностная схема
метод Ритца
метод сопряженных градиентов

description: Рассматривается задача Дирихле для уравнения Пуассона, описываемое начально-краевой задачей для эллиптического типа второго порядка. Для ее приближенного решения используются вариационные методы построения разностных уравнений и вариационные методы построения итерационных алгоритмов. Приведены результаты расчетов для модельной задачи
title: PAC-Australia (2023): Recording with NR2, word list n°1
title: 2019 - post PSS2
titleType: AlternativeTitle
Creators: name: Mas, Erwanne
Publisher: name: COCOON - https://cocoon.huma-num.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2023
Subjects: subject: Australian English
subject: eng

description: PAC word list n°1
description: Conforms to: Praat textgrid
description: Conforms to: doi:10.34847/cocoon.49aefa90-8c1f-3ba8-a099-0ebefc6a2aa7
ДВУХСЕТОЧНЫЙ МЕТОД ДЛЯ НЕЛИНЕЙНОГО СИНГУЛЯРНО ВОЗМУЩЕННОГО УРАВНЕНИЯ ВТОРОГО ПОРЯДКА С ДВУМЯ ПАРАМЕТРАМИ
Creators: name: Тиховская Светлана Валерьевна
Publisher: name: Труды Международной конференции «АПВПМ»
Year: 2019
Subjects: сингулярно возмущенная задача
два малых параметра
сетка Шишкина
двухсеточный метод.

description: Рассмотрена краевая задача для нелинейного сингулярно возмущенного обыкновенного дифференциального уравнения второго порядка с двумя малыми параметрами. Для линеаризации используются итерации Ньютона и Пикара. Для решения задачи на каждой итерации применяется разностная схема второго порядка на сетке Шишкина, которая сходится равномерно по обоим малым параметрам. Для уменьшения требуемого количества арифметических операций для решения разностной схемы предлагается каскадный двухсеточный метод. Для повышения точности разностной схемы, применяется экстраполяция Ричардсона. Получена оценка первой производной решения дифференциальной задачи в случае различных малых параметров. Обсуждаются результаты некоторых численных экспериментов.
Cosmic Ray Rejection by Linear Filtering of Single Images
Creators: name: Rhoads, James E.
Publisher: name: arXiv
Year: 2000
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present a convolution-based algorithm for finding cosmic rays in single well-sampled astronomical images. The spatial filter used is the point spread function (approximated by a Gaussian) minus a scaled delta function, and cosmic rays are identified by thresholding the filtered image. This filter searches for features with significant power at spatial frequencies too high for legitimate objects. Noise properties of the filtered image are readily calculated, which allows us to compute the probability of rejecting a pixel not contaminated by a cosmic ray (the false alarm probability). We demonstrate that the false alarm probability for a pixel containing object flux will never exceed the corresponding probability for a blank sky pixel, provided we choose the convolution kernel appropriately. This allows confident rejection of cosmic rays superposed on real objects. Identification of multiple-pixel cosmic ray hits can be enhanced by running the algorithm iteratively, replacing flagged pixels with the background level at each iteration.
description: Accepted for publication in PASP (May 2000 issue). An iraf script implementing the algorithm is available from the author, or from http://sol.stsci.edu/~rhoads/ . 16 pages including 3 figures. Uses AASTeX aaspp4 style
LLM agent data for "Predicting energy social survey results with Large Language Model agents"
Creators: name: Fell, Michael J.
Publisher: name: OSF Registries
Year: 2024
Subjects: subject: Mechanical Engineering
subject: FOS: Mechanical engineering
subject: Power and Energy
subject: Energy Systems
subject: Public Affairs, Public Policy and Public Administration
subject: Energy Policy
subject: Electrical and Computer Engineering
subject: Social and Behavioral Sciences
subject: Engineering

description: This pre-registration is for data generated by LLM agents, as described in this previous pre-registration: https://osf.io/gx286
Primordial Star Forming Regions in a CDM Universe
Creators: name: Zhang, Yu
name: Norman, Michael L.
name: Anninos, Peter
name: Abel, Tom
Publisher: name: arXiv
Year: 1996
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We developed a three-dimensional 2-level hierarchical cosmological code with a realistic and robust treatment of multi-species non-equilibrium ionization and radiative cooling processes, and use it to investigate primordial star forming regions that originate from high-σperturbations in a standard CDM dominated cosmology. We find it is possible to produce gravitationally bound and cooled structures at very high redshift (z ~ 40) with baryonic masses as small as ~1000Ms. The molecular hydrogen formation in these small scale structures follows very well the analytical predictions of Abel (1995) and Tegmark et al. (1996). We also discuss the minimum mass that cosmological structures must have in order to be able to cool and collapse.
description: 4 pages, with one figure that prints in color. To appear in the proceedings of the 7th Annual Astrophysics Conference in Maryland, STAR FORMATION, NEAR AND FAR, eds. Stephen S. Holt and Lee G. Mundy. This paper and some of the referenced articles are also available at http://lca.ncsa.uiuc.edu/~tom/PGas/bib.html
Bound States and Power Counting in Effective Field Theories
Creators: name: Luke, Michael
name: Manohar, Aneesh V.
Publisher: name: arXiv
Year: 1996
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: Nuclear Theory (nucl-th)
subject: FOS: Physical sciences

description: The problem of bound states in effective field theories is studied. A rescaled version of nonrelativistic effective field theory is formulated which makes the velocity power counting of operators manifest. Results obtained using the rescaled theory are compared with known results from NRQCD. The same ideas are then applied to study Yukawa bound states in 1+1 and 3+1 dimensions, and to analyze when the Yukawa potential can be replaced by a delta-function potential. The implications of these results for the study of nucleon-nucleon scattering in chiral perturbation theory is discussed.
description: 23 pages, eps figures, uses revtex
Oxytocin augmented psychotherapy: A systematic review and meta-analysis protocol
Creators: name: Schneider, Ekaterina
Publisher: name: OSF Registries
Year: 2024
Subjects: subject: Clinical Psychology
subject: Health Psychology
subject: Biological Psychology
subject: Social and Behavioral Sciences
subject: Psychology
subject: FOS: Psychology

description: Oxytocin is known as a hormone that plays a significant role in attachment and social behavior. Consequently, it has been suggested as a potential treatment for conditions with social impairments, such as schizophrenia, depression, or anxiety disorders. While oxytocin is often evaluated as an individual treatment, several studies have also been conducted to investigate the effects of oxytocin when combined with psychotherapy in psychiatric patients. However, the results of these studies combining oxytocin with psychotherapy have been inconclusive. Therefore, here we describe a protocol for a planned systematic review and meta-analysis that aims to synthesize and evaluate studies that investigate the augmenting effects of oxytocin on psychotherapy in various psychiatric conditions.
Dressing the nucleon in a dispersion approach
Creators: name: Kondratyuk, S.
name: Scholten, O.
Publisher: name: arXiv
Year: 2000
Subjects: subject: Nuclear Theory (nucl-th)
subject: FOS: Physical sciences

description: We present a model for dressing the nucleon propagator and vertices. In the model the use of a K-matrix approach (unitarity) and dispersion relations (analyticity) are combined. The principal application of the model lies in pion-nucleon scattering where we discuss effects of the dressing on the phase shifts.
description: 17 pages, using REVTeX, 6 figures
Effect of spatial design on the normativity of sexual assault and helping behaviors in RER train stations
Creators: name: Blaison, Christophe
name: Baklouti, Dora
name: ADAMCZAK, Raphaël
Publisher: name: OSF Registries
Year: 2024
Subjects: subject: Social Psychology
subject: Social and Behavioral Sciences
subject: Psychology
subject: FOS: Psychology

description: This study aims to reduce the normativity of sexual assault in public transportation and increase the normativity of helping behaviors when witnessing such events through a modification of spatial design.
Work from home during COVID-19-disequilibrium of mental health and well-being among employees
Creators: name: Shankar, Nisha
Publisher: name: IfADo - Leibniz Research Centre for Working Environment and Human Factors, Dortmund
Year: 2021
Subjects: pandemic
employees
mental stress
well-being

description: EXCLI Journal; 20:Doc1287; ISSN 1611-2156
Additional file 1 of CDK13 upregulation-induced formation of the positive feedback loop among circCDK13, miR-212-5p/miR-449a and E2F5 contributes to prostate carcinogenesis
Creators: name: Qi, Jin-Chun
name: Yang, Zhan
name: Lin, Tao
name: Ma, Long
name: Wang, Ya-Xuan
name: Zhang, Yong
name: Gao, Chun-Cheng
name: Liu, Kai-Long
name: Li, Wei
name: Zhao, An-Ning
name: Shi, Bei
name: Zhang, Hong
name: Wang, Dan-Dan
name: Wang, Xiao-Lu
name: Wen, Jin-Kun
name: Qu, Chang-Bao
Publisher: name: figshare
Year: 2021
Subjects: subject: Biophysics
subject: Biochemistry
subject: Cell Biology
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Physiology
subject: Developmental Biology
subject: Cancer
subject: Hematology
subject: Computational Biology

description: Additional file 1.
Entanglement Entropy of Compactified Branes and Phase Transition
Creators: name: Huang, Wung-Hong
Publisher: name: arXiv
Year: 2017
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We first calculate the holographic entanglement entropy of M5 branes on a circle and see that it has phase transition during decreasing the compactified radius. In particular, it is shown that the entanglement entropy scales as $N^3$. Next, we investigate the holographic entanglement entropy of D0+D4 system on a circle and see that it scales as $N^2$ at low energy, likes as a gauge theory with instantons. However, at high energy it transforms to a phase which scales as $N^3$, like as M5 branes system. We also present the general form of holographic entanglement entropy of Dp, ${\rm D_p+D_{p+4}}$ and M-branes on a circle and see some simple relations between them. Finally, we present an analytic method to prove that they all have phase transition from connected to disconnected surface during increasing the line segment of length $\ell$ which dividing the space.
description: Latex 14 pages. Add 2 figures, some derivations, discussions and references
title: PAC-Australia (2023): Recording with PR, word list n°2
title: 2019 - post PSS2
titleType: AlternativeTitle
Creators: name: Mas, Erwanne
Publisher: name: COCOON - https://cocoon.huma-num.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2023
Subjects: subject: Australian English
subject: eng

description: PAC word list n°2
description: Conforms to: Praat textgrid
description: Conforms to: doi:10.34847/cocoon.49aefa90-8c1f-3ba8-a099-0ebefc6a2aa7
title: ADCO, Cartulaire de l'abbaye de Cîteaux dit Cartulare Antiquum t.3 (2e moitié XIIIe siècle), Cart. 168 (11 H 66), f. 0155r
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/2010
name: Petot, Frédéric
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2020
Subjects: subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris
subject: cartulaire
subject: Corpus Burgundiae Medii Aevi
subject: Chartes de la Bourgogne du Moyen Âge

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. 0155r, 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. 0155r, in Projet CBMA - Corpus Burgundiae Medii Aevi [Ressource en ligne], https:// manuscrits.cbma-project.eu/
description: Provenance: https://www.geonames.org/3024876
description: Provenance: http://www.idref.fr/030974844/id
description: Provenance: https://catalogue.bnf.fr/ark:/12148/cb12228351v
description: Provenance: abbaye de Cîteaux
description: Provenance: http://www.wikidata.org/entity/Q843261
title: Hydrotalcite als neuartige Treibmittel für Polyethylenschäume
Creators: name: Werne, Lisa
Publisher: name: UNSPECIFIED
Year: 2019

description: Im Rahmen dieser Arbeit wurde ein Treibmittelsystem bestehend aus Calciumhydrotalcit und Polymaleinsäureanhydrid-co-styrol entwickelt, welches in LLDPE zu einer Dichtereduktion von 30% führt. Der hergestellte Schaum weist bei einer engen Zellgrößenverteilung Zellen kleiner als 50 µm auf. Dabei wirkt das Calciumhydrotalcit als kombiniertes Treib- und Nukleierungsmittel. Als Treibgas bei der Schaumextrusion wird Wasser verwendet.
Consistent hydrodynamic theory of chiral electrons in Weyl semimetals
Creators: name: Gorbar, E. V.
name: Miransky, V. A.
name: Shovkovy, I. A.
name: Sukhachov, P. O.
Publisher: name: arXiv
Year: 2017
Subjects: subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: Nuclear Theory (nucl-th)
subject: FOS: Physical sciences

description: The complete set of Maxwell's and hydrodynamic equations for the chiral electrons in Weyl semimetals is presented. The formulation of the Euler equation takes into account the explicit breaking of the Galilean invariance by the ion lattice. It is shown that the Chern-Simons (or Bardeen-Zumino) contributions should be added to the electric current and charge densities in Maxwell's equations that provide the information on the separation of Weyl nodes in energy and momentum. On the other hand, these topological contributions do not directly affect the Euler equation and the energy conservation relation for the electron fluid. By making use of the proposed consistent hydrodynamic framework, we show that the Chern-Simons contributions strongly modify the dispersion relations of collective modes in Weyl semimetals. This is reflected, in particular, in the existence of distinctive anomalous Hall waves, which are sustained by the local anomalous Hall currents.
description: 6+8 pages, 1 figure; published version; a few minor typos in the definitions of $d_z$ and $b_0$ are corrected
PAC-Australia (2023): Recording with PR, "A Christmas interview"
Creators: name: Mas, Erwanne
Publisher: name: COCOON - https://cocoon.huma-num.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2023
Subjects: subject: Australian English
subject: eng

description: PAC-LVTI Reading Task
description: Conforms to: Praat textgrid
description: Conforms to: doi:10.34847/cocoon.49aefa90-8c1f-3ba8-a099-0ebefc6a2aa7
Automatic Data Driven Vegetation Modeling for Lidar Simulation
Creators: name: Jean-Emmanuel  Deschaud
name: Prasser, David
name: M. Freddie Dias
name: Browning, Brett
name: Rander, Peter
Publisher: name: Carnegie Mellon University
Year: 2012
Subjects: subject: 80101 Adaptive Agents and Intelligent Robotics
subject: FOS: Computer and information sciences

description: Traditional lidar simulations render surface models to generate simulated range data. For objects with welldefined surfaces, this approach works well, and traditional 3D scene reconstruction algorithms can be employed to automatically generate the surface models. This approach breaks down, though, for many trees, tall grasses, and other objects with fine-scale geometry: surface models do not easily represent the geometry, and automated reconstruction from real data is difficult. In this paper, we introduce a new stochastic volumetric model that better captures the complexities of real lidar data of vegetation and is far better suited for automatic modeling of scenes from field collected lidar data. We also introduce several methods for automatic modeling and for simulating lidar data utilizing the new model. To measure the performance of the stochastic simulation we use histogram comparison metrics to quantify the differences between data produced by the real and simulated lidar. We evaluate our approach on a range of real world datasets and show improved fidelity for simulating geo-specific outdoor, vegetation scenes.
Dynamical Projective Curvature in Gravitation
Creators: name: Brensinger, Samuel
name: Rodgers, Vincent G. J.
Publisher: name: arXiv
Year: 2017
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: General Relativity and Quantum Cosmology (gr-qc)
subject: Differential Geometry (math.DG)
subject: FOS: Physical sciences
subject: FOS: Mathematics

description: By using a projective connection over the space of two-dimensional affine connections, we are able to show that the metric interaction of Polyakov 2D gravity with a coadjoint element arises naturally through the projective Ricci tensor. Through the curvature invariants of Thomas-Whitehead, we are able to define an action that could describe dynamics to the projective connection. We discuss implications of the projective connection in higher dimensions as related to gravitation.
description: 30 pages. Made revisions in accordance with International Journal of Modern Physics A for acceptance
title: PAC-Australia (2023): Recording with PR, word list n°1
title: 2019 - post PSS2
titleType: AlternativeTitle
Creators: name: Mas, Erwanne
Publisher: name: COCOON - https://cocoon.huma-num.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2023
Subjects: subject: Australian English
subject: eng

description: PAC word list n°1
description: Conforms to: Praat textgrid
description: Conforms to: doi:10.34847/cocoon.49aefa90-8c1f-3ba8-a099-0ebefc6a2aa7
Additional file 2 of CDK13 upregulation-induced formation of the positive feedback loop among circCDK13, miR-212-5p/miR-449a and E2F5 contributes to prostate carcinogenesis
Creators: name: Qi, Jin-Chun
name: Yang, Zhan
name: Lin, Tao
name: Ma, Long
name: Wang, Ya-Xuan
name: Zhang, Yong
name: Gao, Chun-Cheng
name: Liu, Kai-Long
name: Li, Wei
name: Zhao, An-Ning
name: Shi, Bei
name: Zhang, Hong
name: Wang, Dan-Dan
name: Wang, Xiao-Lu
name: Wen, Jin-Kun
name: Qu, Chang-Bao
Publisher: name: figshare
Year: 2021
Subjects: subject: Biophysics
subject: Biochemistry
subject: Cell Biology
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Physiology
subject: Developmental Biology
subject: Cancer
subject: Hematology
subject: Computational Biology

description: Additional file 2.
The Variation of Gas Mass Distribution in Galaxy Clusters: Effects of Preheating and Shocks
Creators: name: Fujita, Yutaka
name: Takahara, Fumio
Publisher: name: arXiv
Year: 2000
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We investigate the origin of the variation of the gas mass fraction in the core of galaxy clusters, which was indicated by our work on the X-ray fundamental plane. The adopted model supposes that the gas distribution characterized by the slope parameter is related to the preheated temperature. Comparison with observations of relatively hot (~> 3 keV) and low redshift clusters suggests that the preheated temperature is about 0.5-2 keV, which is higher than expected from the conventional galactic wind model and possibly suggests the need for additional heating such as quasars or gravitational heating on the largest scales at high redshift. The dispersion of the preheated temperature may be attributed to the gravitational heating in subclusters. We calculate the central gas fraction of a cluster from the gas distribution, assuming that the global gas mass fraction is constant within a virial radius at the time of the cluster collapse. We find that the central gas density thus calculated is in good agreement with the observed one, which suggests that the variation of gas mass fraction in cluster cores appears to be explained by breaking the self-similarity in clusters due to preheated gas. We also find that this model does not change major conclusions on the fundamental plane and its cosmological implications obtained in previous papers, which strongly suggests that not only for the dark halo but also for the intracluster gas the core structure preserves information about the cluster formation.
description: 17 pages, to be published in ApJ
D-NOSES POPD - Requirement nº 2 (Deliverable 8.2)
Creators: name: Sanz, Francisco
name: Pelacho, Maite
name: Arias, Rosa
name: Agulló, Oriol
Publisher: name: Zenodo
Year: 2021
Subjects: Protection of Personal Data

description: Deliverable D8.2 corresponds to Requirement No. 2 on Protection of Personal Data (PODP). This requirement mainly implies that the contact details of the Data Protection Officer (DPO) are available to all data subjects involved in the research.