cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Self-Affirmation Improves Problem-Solving under Stress
Creators: name: J. David Creswell
name: Dutcher, Janine M.
name: Klein, William M.P.
name: Harris, Peter R.
name: Levine, John M.
Publisher: name: Carnegie Mellon University
Year: 2013
Subjects: subject: 170199 Psychology not elsewhere classified
subject: FOS: Psychology

description: High levels of acute and chronic stress are known to impair problem-solving and creativity on a broad range of tasks. Despite this evidence, we know little about protective factors for mitigating the deleterious effects of stress on problem-solving. Building on previous research showing that self-affirmation can buffer stress, we tested whether an experimental manipulation of self-affirmation improves problem-solving performance in chronically stressed participants. Eighty undergraduates indicated their perceived chronic stress over the previous month and were randomly assigned to either a self-affirmation or control condition. They then completed 30 difficult remote associate problem-solving items under time pressure in front of an evaluator. Results showed that self-affirmation improved problem-solving performance in underperforming chronically stressed individuals. This research suggests a novel means for boosting problem-solving under stress and may have important implications for understanding how self-affirmation boosts academic achievement in school settings.
Additional file 6 of METAMVGL: a multi-view graph-based metagenomic contig binning algorithm by integrating assembly and paired-end graphs
Creators: name: Zhang, Zhenmiao
name: Zhang, Lu
Publisher: name: figshare
Year: 2021
Subjects: subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: 69999 Biological Sciences not elsewhere classified
subject: 80699 Information Systems not elsewhere classified
subject: FOS: Computer and information sciences
subject: Cancer
subject: Plant Biology

description: Additional file 6. The performance of SolidBin, GraphBin and METAMVGLon the BMock12, SYNTH64 and Sharon datasets: (a) and (d) forBMock12 dataset; (b) and (e) for SYNTH64 dataset; (c) and (f) forSharon dataset. MEGAHIT and metaSPAdes are used to generate theassembly graphs. The initial binning tool is SolidBin.
The extinction curves of star-forming regions from z=0.1 to 6.7 using GRB afterglow spectroscopy
Creators: name: Zafar, Tayyaba
name: Watson, Darach
name: Fynbo, Johan P. U.
name: Malesani, Daniele
name: Jakobsson, Pall
name: Postigo, Antonio de Ugarte
Publisher: name: arXiv
Year: 2011
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: GRB afterglows are well suited to extinction studies due to their brightness, simple power-law spectra and the occurrence of GRBs in distant star forming galaxies. In this paper we present results from the SED analysis of a sample of 41 GRB afterglows, from X-ray to NIR wavelengths. This is the largest sample of extinction curves outside the Local Group and, to date, the only extragalactic sample of absolute extinction curves based on spectroscopy. Visual extinction correlation with HI column density as well as total and gas-phase metal column density are examined. Approximately half the sample require a cooling break between the optical and X-ray regimes. The broken power-law SEDs show an average change in the spectral index of delta_beta=0.51 with a standard deviation of 0.02. This is consistent with the expectation from a simple synchrotron model. Of the sample, 63% are well described by the SMC-type extinction curve and have moderate or low extinction, with AV<0.65. Almost a quarter of our sample is consistent with no significant extinction (typically AV<0.1). The 2175AA extinction bump is detected unequivocally in 7% of our sample (3 GRBs), which all have A_V>1.0. We find an anti-correlation between gas-to-dust ratio and metallicity consistent with the Local Group relation. Our metals-to-dust ratios derived from the soft X-ray absorption are always larger (3-30 times) than the Local Group value, which may mean that GRB hosts may be less efficient at turning their metals into dust. However, we find that gas, dust, and metal column densities are all likely to be influenced by photo-ionization and dust destruction effects from the GRB. [abridged]
description: 31 pages, 12 figures, 6 tables, Published in A&A
The topological biquandle of a link
Creators: name: Horvat, Eva
Publisher: name: arXiv
Year: 2018
Subjects: subject: Geometric Topology (math.GT)
subject: FOS: Mathematics

description: To every oriented link $L$, we associate a topologically defined biquandle $\widehat{\mathcal{B}}_{L}$, which we call the topological biquandle of $L$. The construction of $\widehat{\mathcal{B}}_{L}$ is similar to the topological description of the fundamental quandle given by Matveev. We find a presentation of the topological biquandle and explain how it is related to the fundamental biquandle of the link.
description: 14 pages, 12 figures
Global Food Price Increases and Repercussions on Africa: Which Public Policy Interventions are really appropriate?
Creators: name: Wohlmuth, Karl
Publisher: name: Universität Bremen
Year: 2012
Subjects: subject: -
subject: 330

description: In this contribution the impacts of the global food price increases of 2010/2011 on Africa are assessed. The impacts are severe, but there are differences with regard of country groupings, social groups and sub-regions. The various impacts have to be studied carefully as these do not affect only the macro-economy and the poor people, but also the development options and the long-term development perspectives of Af- rica. However, definitions and classifications have to be clarified first to understand the transmission effects and the poverty impacts of the global food price increases. It has to be made clear which food items, which African countries and which country groupings are affected by the price increases on the world market. Fragile and conflict countries, food insecure countries and oil exporting countries are affected most by the global price increases of food products and especially of staple crops. But also the poor in net food exporting countries may suffer.
Additional file 1 of Organizational attributes of interprofessional primary care for adults with intellectual and developmental disabilities in ontario, Canada: a multiple case study
Creators: name: Bobbette, Nicole
name: Lysaght, Rosemary
name: Ouellette-Kuntz, Hélène
name: Tranmer, Joan
name: Donnelly, Catherine
Publisher: name: figshare
Year: 2021
Subjects: subject: Medicine
subject: Biotechnology
subject: 59999 Environmental Sciences not elsewhere classified
subject: FOS: Earth and related environmental sciences
subject: Ecology
subject: FOS: Biological sciences
subject: Sociology
subject: FOS: Sociology
subject: 69999 Biological Sciences not elsewhere classified
subject: Science Policy

description: Additional file 1.
The neutrino-neutrino interaction effects in supernovae: the point of view from the 'matter' basis
Creators: name: Galais, S.
name: Kneller, J.
name: Volpe, C.
Publisher: name: arXiv
Year: 2011
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We consider the Hamiltonian for neutrino oscillations in matter in the case of arbitrary potentials including off-diagonal complex terms. We derive the 'matter basis' Hamiltonian in terms of quantities one can derive from the flavor basis Hamiltonian and its derivative, for an arbitrary number of neutrino flavors. We make our expressions explicit for the two-neutrino flavor case and apply our results to the situation where the Hamiltonian includes both coupling to matter and to neutrinos, which describes neutrino propagation in core-collapse supernovae. We show that the neutrino flavour evolution depends on the mixing matrix derivatives involving not only the derivative of the matter mixing angles but also of the phases. In particular, we point out the important role of the phase derivatives, that appear due to the neutrino-neutrino interaction, and show how it can cause an oscillating degeneracy between the diagonal elements of the matter basis Hamiltonian. Our results also reveal, that the end of the synchronization regime is due to a rapid increase of the phase derivative, and identify the condition to be fulfilled for the onset of bipolar oscillations involving both the off-diagonal neutrino-neutrino interaction contributions and the vacuum terms.
description: 11 pages, 5 figures, text and manuscript structure improved
Creating the Slovak music register for coordinating private and public data infrastructure
Creators: name: Antal, Daniel
Publisher: name: Zenodo
Year: 2024
Subjects: subject: Work on automating curation processes
subject: Intellectual Property Rights, legal and policy issues around AI training data collection and use
subject: Trust and transparency between universal standards and expectations and that of context and discipline specific adaptations
subject: Building trust and transparency into research and curation techniques, costs, and workflows
subject: Music
subject: Statistics
subject: FOS: Mathematics
subject: Data coordination
subject: Registers

description: The planned data coordination will enable the Digital Music Observatory prototype to provide a comprehensive and unbiased view of creators, music works or recordings, or their financial, environmental, and social impact data with the connection of global privately-held and public data infrastructure. We are prototyping it in Slovakia.
Systematic Analysis of the Effects of Mode Conversion on Thermal Radiation from Neutron Stars
Creators: name: Yatabe, Akihiro
name: Yamada, Shoichi
Publisher: name: arXiv
Year: 2017
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: In this paper, we systematically calculate the polarization in soft X-rays emitted from magnetized neutron stars, which are expected to be observed by the next-generation X-ray satellites. Magnetars are one of the targets for these observations. This is because thermal radiation is normally observed in the soft X-ray band, and it is thought to be linearly polarized because of different opacities for two polarization modes of photons in the magnetized atmosphere of neutron stars and the dielectric properties of the vacuum in strong magnetic fields. In their previous study, Taverna et al. illustrated how strong magnetic fields influence the behavior of the polarization observables for radiation propagating in vacuo without addressing a precise, physical emission model. In this paper, we pay attention to the conversion of photon polarization modes that can occur in the presence of an atmospheric layer above the neutron star surface, computing the polarization angle and fraction and systematically changing the magnetic field strength, radii of the emission region, temperature, mass, and radii of the neutron stars. We confirmed that if plasma is present, the effects of mode conversion cannot be neglected when the magnetic field is relatively weak, $B \sim 10^{13} \mathrm{G}$. Our results indicate that strongly magnetized ($B \gtrsim 10^{14} \mathrm{G}$) neutron stars are suitable to detect polarizations, but not-so-strongly magnetized ($B \sim 10^{13} \mathrm{G}$) neutron stars will be the ones to confirm the mode conversion.
description: 34 pages, 29 figures, published in The Astrophysical Journal
Seeing It Differently: Visual Processing in Autism
Creators: name: Behrmann, Marlene
name: Cibu  Thomas
name: Humphreys, Kate
Publisher: name: Carnegie Mellon University
Year: 2006
Subjects: subject: 170199 Psychology not elsewhere classified
subject: FOS: Psychology

description: Several recent behavioral and neuroimaging studies have documented an impairment in face processing in individuals with Autism Spectrum Disorder (ASD). It remains unknown, however, what underlying mechanism gives rise to this face processing difficulty. One theory suggests that the difficulty derives from a pervasive problem in social interaction and/or motivation. An alternative view proposes that the faceprocessing problem is not entirely social in nature and that a visual perceptual impairment might also contribute. The focus of this review is on this latter, perceptual perspective, documenting the psychological and neural alterations that might account for the face processing impairment. The available evidence suggests that perceptual alterations are present in ASD, independent of social function.
Laminations of a graph on a pair of pants
Creators: name: Ramassamy, Sanjay
Publisher: name: arXiv
Year: 2018
Subjects: subject: Combinatorics (math.CO)
subject: Geometric Topology (math.GT)
subject: FOS: Mathematics

description: A lamination of a graph embedded on a surface is a collection of pairwise disjoint non-contractible simple closed curves drawn on the graph. In the case when the surface is a sphere with three punctures (a.k.a. a pair of pants), we first identify the lamination space of a graph embedded on that surface as a lattice polytope, then we characterize the polytopes that arise as the lamination space of some graph on a pair of pants. This characterizes the image of a purely topological version of the spectral map for the vector bundle Laplacian for a flat connection on a pair of pants. The proof uses a graph exploration technique akin to the peeling of planar maps.
description: 17 pages, 8 figures. Final version to appear in the Bulletin of the London Mathematical Society
title: Die Orte, an denen wir heilen. Für Schwarze Communities of Practice, Dialogue and Care
Creators: name: Adamou, Jamila
Publisher: name: Humboldt-Universität zu Berlin
Year: 2021
Subjects: subject: Brustkrebs
subject: Gesundheit
subject: Rassismus
subject: Schwarzer Feminismus
subject: ddc:300

description: Weltweit waren 2020 2,3 Millionen Frauen weltweit von Brustkrebs betroffen, 685.000 starben daran. Dies macht Brustkrebs zu einer der am weitesten verbreiteten Krebserkrankung. Laut US-Studien haben Schwarze Frauen – im Vergleich zu weißen Frauen – relativ höhere Inzidenzen von und Risiken für schwerere Verläufe und tödliche Formen von Brustkrebs. Dies ist alarmierend angesichts der Tatsache, dass die frühzeitige Erkennung und adäquate Behandlung von Brustkrebs enorm wichtig und lebensrettend sind. Die Gründe für die unterschiedlichen und erhöhten Inzidenzen und Risiken sind vielfältig. In Deutschland existieren spezifische Analysen der Auswirkungen von Rassismen und anderen Formen intersektionaler Diskriminierungen im medizinischen System einerseits und deren multiple Wirkweisen (Traumata, Erkrankungen, Ausgrenzung u.v.m.) andererseits nicht. Vor dem Hintergrund der Erfahrung mehrfacher Traumata, durch Diskriminierung, Ausgrenzung und möglichen Auswirkungen historischer Dimensionen auf den Körper, plädiert der Artikel einerseits dafür, Schwarze Communities und Individuen ernst zu nehmen und hier eine Gestaltung von Communities of Practice, Dialoge and Care für Schwarze Frauen und LGBTIQA+ zu gestalten. Anderseits zielt er auf grundlegende Transformationen des Medizinsystems, die die intersektionalen Realitäten Schwarzer Frauen und LGBTQIA+ reflektieren und integrieren und so eine diskriminierungs- und rassismusbewusste inklusive gendergerechte gleichberechtigte und chancengerechte Medizin für alle ermöglichen.
Global properties of tight Reeb flows with applications to Finsler geodesic flows on $S^2$
Creators: name: Hryniewicz, Umberto
name: Salomão, Pedro A. S.
Publisher: name: arXiv
Year: 2011
Subjects: subject: Symplectic Geometry (math.SG)
subject: Differential Geometry (math.DG)
subject: FOS: Mathematics
subject: 53D25, 32Q65

description: We show that if a Finsler metric on $S^2$ with reversibility $r$ has flag curvatures $K$ satisfying $(\frac{r}{r+1})^2
description: 27 pages
Additional file 2 of Organizational attributes of interprofessional primary care for adults with intellectual and developmental disabilities in ontario, Canada: a multiple case study
Creators: name: Bobbette, Nicole
name: Lysaght, Rosemary
name: Ouellette-Kuntz, Hélène
name: Tranmer, Joan
name: Donnelly, Catherine
Publisher: name: figshare
Year: 2021
Subjects: subject: Medicine
subject: Biotechnology
subject: 59999 Environmental Sciences not elsewhere classified
subject: FOS: Earth and related environmental sciences
subject: Ecology
subject: FOS: Biological sciences
subject: Sociology
subject: FOS: Sociology
subject: 69999 Biological Sciences not elsewhere classified
subject: Science Policy

description: Additional file 2.
Reconciling conflicting data curation actions: transparency through argumentation
Creators: name: Ludäscher, Bertram
name: Bowers, Shawn
name: Xia, Yilin
Publisher: name: Zenodo
Year: 2024
Subjects: Work on automating curation processes
Building trust and transparency into research and curation techniques, costs, and workflows
Transparency as a means of demonstrating research integrity
data curation
provenance
conflict resolution
formal argumentation

description: We propose to automatically reconcile conflicting data cleaning actions, which naturally arise in collaborative data curation settings. The key idea is to model conflicting updates as a formal argumentation framework that can be automatically analyzed, yielding a transparent solution in which conflicting updates are accepted, rejected, or flagged for human resolution, depending on which actions are "most justified".
title: Eine intersektional-feministische Perspektive für die Klimabewegung: Zur Anerkennung und Wertschätzung (marginalisierter) Stimmen von Black, Indigenous und Women of Color
Creators: name: Anderson, Sheena
Publisher: name: Humboldt-Universität zu Berlin
Year: 2021
Subjects: subject: Intersektionalität
subject: Klimagerechtigkeit
subject: Schwarzer Feminismus
subject: ddc:300

description: Die Klimakrise trifft nicht alle gleich, ganz im Gegenteil. Sie unterscheidet nach race, Gender, geografischem Standort, soziökonomischem Hintergrund, Alter, körperlicher Einschränkung und vielen anderen Kategorien. Am Beispiel von Black, Indigenous und Women of Color (BIWoC) zeigt dieser Beitrag auf, dass einerseits eine besondere Betroffenheit marginalisierter Gruppen in Bezug auf die Klimakrise besteht und andererseits es genau BIWoC sind die nicht nur führende Rollen in der Klimabewegung einnehmen, sondern von deren spezialisiertem Wissen, basierend auf ihrer intersektionalen Unterdrückung, ihrem (Überlebens-)Kampf und ihrer Art Wissen zu produzieren und weiterzugeben, die Klimabewegung auf ungeahnte Weise lernen kann. Anders als häufig angenommen, ist die Klimabewegung im weiten Sinne nicht „zu weiß“, sondern es sind tatsächlich Black, Indigenous und People of Color, die diese Bewegung seit Jahrzehnten prägen. Es wird Zeit, dass sie die Anerkennung und Wertschätzung erhalten, die ihnen gebührt. Auf eine kurze Analyse der Ursprünge intersektionalen Feminismus in Schwarzen Feminismen und den Kämpfen Schwarzer Frauen folgen in diesem Beitrag theorie-basierte und durch Interviews mit BIWoC Klimaaktivistinnen gewonnene intersektional-feministische Guidelines für die Klimabewegung. Sie sind ein Angebot, um der Klimabewegung zu einer Vision zu verhelfen, in ihrem Protest die Verwobenheit und gegenseitige Bedingung globaler Herausforderungen zu berücksichtigen; anzuerkennen, dass diese unterschiedlichen Auswirkungen für marginalisierte Menschen haben und den Schutz von Menschen sowie der Umwelt gleichermaßen in den Vordergrund zu rücken. Um der Klimakrise die Stirn zu bieten, bedarf es einer radikalen Systemveränderung, Klimagerechtigkeit bildet die anzuwendende Strategie und Intersektionaler Feminismus liefert die Perspektive zur Umsetzung.
title: Fonctionnement des petits bassins versants miniers. Volume II : rapports thématiques (annexes)
Creators: name: Allenbach, Michel
name: Andréoli, Rémi
name: Cavarero, Virgil
name: Caze, Nicolas
name: Cluzel, Dominique
name: Couturier, Arnaud
name: Boissieu, Florian de
name: Despinoy, Marc
name: Dumas, Pascal Sébastien
name: Flouvat, Frédéric
name: Gunkel-Grillon, Peggy
name: Hoibian, Thierry
name: Jeanpert, Julie
name: Join, Jean-Lambert
name: Kranitz, Thierry
name: Mangeas, Morgan
name: Mathys, Nicolle
name: Métayer, Cyrille
name: Meyer, Michael
name: Recking, Alain
name: Richard, Didier
name: Rouet, Isabelle
name: Selmaoui-Folcher, Nazha
name: Tehei, Temaui
name: Touraivane, T.
Publisher: name: CNRT Nickel et son environnement
Year: 2016
Subjects: subject: FOS: Earth and related environmental sciences
valueUri: http://www.oecd.org/science/inno/38235147.pdf

description: Programme FPBVM. (Tome Nickel et Environnement)
Growing up in a megalopolis: Environmental effects on galaxy evolution in a supercluster at z~0.65 in UKIDSS UDS
Creators: name: Galametz, Audrey
name: Pentericci, Laura
name: Castellano, Marco
name: Mendel, Trevor
name: Hartley, Will G.
name: Fossati, Matteo
name: Finoguenov, Alexis
name: Almaini, Omar
name: Beifiori, Alessandra
name: Fontana, Adriano
name: Grazian, Andrea
name: Scodeggio, Marco
name: Kocevski, Dale D.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We present a large-scale galaxy structure Cl J021734-0513 at z~0.65 discovered in the UKIDSS UDS field, made of ~20 galaxy groups and clusters, spreading over 10 Mpc. We report on a VLT/VIMOS spectroscopic follow-up program that, combined with past spectroscopy, allowed us to confirm four galaxy clusters (M200 ~ 10^14 Msol) and a dozen associated groups and star-forming galaxy overdensities. Two additional filamentary structures at z ~ 0.62 and z ~ 0.69 and foreground and background clusters at 0.6 < z < 0.7 were also confirmed along the line-of-sight. The structure subcomponents are at different formation stages. The clusters have a core dominated by passive galaxies and an established red sequence. The remaining structures are a mix of star-forming galaxy overdensities and forming groups. The presence of quiescent galaxies in the core of the latter shows that `preprocessing' has already happened before the groups fall into their more massive neighbours. Our spectroscopy allows us to derive spectral index measurements e.g. emission/absorption line equivalent widths, strength of the 4000A break, valuable to investigate the star formation history of structure members. Based on these line measurements, we select a population of `poststarburst' galaxies. These galaxies are preferentially found within the virial radius of clusters, supporting a scenario in which their recent quenching could be prompted by gas stripping by the dense intracluster medium. We derive stellar age estimates using MCMC-based spectral fitting for quiescent galaxies and find a correlation between ages and colours/stellar masses which favours a top-down formation scenario of the red sequence. A catalogue of ~650 redshifts in UDS will be released alongside the paper.
description: 23 pages, 19 figures, 4 tables, accepted for publication in MNRAS. A catalogue of ~650 VIMOS spectroscopic redshifts in UKIDSS UDS will be released alongside the paper. Feel free to contact the authors for early access to the catalogue
Additional file 3 of Organizational attributes of interprofessional primary care for adults with intellectual and developmental disabilities in ontario, Canada: a multiple case study
Creators: name: Bobbette, Nicole
name: Lysaght, Rosemary
name: Ouellette-Kuntz, Hélène
name: Tranmer, Joan
name: Donnelly, Catherine
Publisher: name: figshare
Year: 2021
Subjects: subject: Medicine
subject: Biotechnology
subject: 59999 Environmental Sciences not elsewhere classified
subject: FOS: Earth and related environmental sciences
subject: Ecology
subject: FOS: Biological sciences
subject: Sociology
subject: FOS: Sociology
subject: 69999 Biological Sciences not elsewhere classified
subject: Science Policy

description: Additional file 3.
Gauguin's questions in particle physics: Where are we coming from? What are we? Where are we going?
Creators: name: Ellis, John
Publisher: name: arXiv
Year: 2007
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: Within particle physics itself, Gauguin's questions may be interpreted as: P1 - What is the status of the Standard Model? P2 - What physics may lie beyond the Standard Model? P3 - What is the `Theory of Everything'? Gauguin's questions may also asked within a cosmological context: C1 - What were the early stages of the Big Bang? C2 - What is the material content of the Universe today? C3 - What is the future of the Universe? In this talk I preview many of the topics to be discussed in the plenary sessions of this conference, highlighting how they bear on these fundamental questions.
description: 16 pages, 11 figures, plenary talk at the International Europhysics Conference on High-Energy Physics (EPS-HEP2007), Manchester, England, July 2007
Seeds aren't anchors
Creators: name: N R Brown
name: Siegler, Robert
Publisher: name: Carnegie Mellon University
Year: 2001
Subjects: subject: 170199 Psychology not elsewhere classified
subject: FOS: Psychology

description: Exposure to a few task-relevant numerical facts (seed facts) often improves subsequent numerical estimates. We performed two experiments to investigate the mechanism that produces these seeding effects. In Experiment 1, participants estimated national populations; in Experiment 2, they estimated between-city distances. In both, items were selected so that the actual value of the seed facts (S-1) was, on average, below participants' initial estimates for those items (S,) and above the initial estimates for the transfer items (T-1). Given this configuration, the anchoring position predicts that the postseeding transfer estimates should be greater than the preseeding transfer estimates (T-2 > T-1), whereas the feedback/ induction position predicts the opposite (T-2 < T-1). In both experiments, the latter pattern of results emerged, supporting the conclusion that seeds aren't anchors.
title: ADCO, Ordre cistercien et abbaye de Cîteaux : comptes pour l'ordre (1337-1347), comptes du boursier (1377-1402) (11 H 1160), f. 00025
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: CBMA/CG21/F.PETOT/2017
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: comptes

description: Ordre cistercien et abbaye de Cîteaux : comptes pour l'ordre (1337-1347), comptes du boursier (1377-1402), Archives départementales de la Côte-d'Or, (11 H 1160). Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Ordre cistercien et abbaye de Cîteaux : comptes pour l'ordre (1337-1347), comptes du boursier (1377-1402), Archives départementales de la Côte-d'Or, (11 H 1160), f. 00025, 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
Producing Distant Planets by Mutual Scattering of Planetary Embryos
Creators: name: Silsbee, Kedron
name: Tremaine, Scott
Publisher: name: arXiv
Year: 2017
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: FOS: Physical sciences

description: It is likely that multiple bodies with masses between those of Mars and Earth ("planetary embryos") formed in the outer planetesimal disk of the solar system. Some of these were likely scattered by the giant planets into orbits with semi-major axes of hundreds of AU. Mutual torques between these embryos may lift the perihelia of some of them beyond the orbit of Neptune, where they are no longer perturbed by the giant planets so their semi-major axes are frozen in place. We conduct N-body simulations of this process, and its effect on smaller planetesimals in the region of the giant planets and the Kuiper belt. We find that (i) there is a significant possibility that one sub-Earth mass embryo, or possibly more, is still present in the outer solar system; (ii) the orbit of the surviving embryo(s) typically has perihelion of 40--70 AU, semi-major axis less than 200 AU, and inclination less than 30 degrees; (iii) it is likely that any surviving embryos could be detected by current or planned optical surveys or have a significant effect on solar-system ephemerides; (iv) whether or not an embryo has survived to the present day, their dynamical influence earlier in the history of the solar system can explain the properties of the detached disk (defined in this paper as containing objects with perihelia > 38 AU and semi-major axes between 80 and 500 AU).
description: Accepted to A.J
On the claimed X-shaped structure in the Milky Way bulge
Creators: name: Han, Daniel
name: Lee, Young-Wook
Publisher: name: arXiv
Year: 2018
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: A number of recent studies have claimed that the double red clump (RC) observed in the Milky Way bulge is a consequence of a giant X-shaped structure. In particular, Ness & Lang (2016) reported a direct detection of a faint X-shaped structure from the residual map of the Wide-Field Infrared Survey Explorer (WISE) bulge image. Here we show, however, that their result is affected substantially by whether the conventional dust extinction correction is applied or not and partly by a bulge model subtracted from the original image. We find that the residuals obtained by subtracting either ellipsoidal or boxy bulge models from the dereddened images show no obvious X-shaped structure. We further show that, even if it is real, the stellar density in the claimed X-shaped structure is way too low to be observed as a strong double RC at l=0.
description: Submitted to AJ
A Hierarchical Latent Vector Model for Learning Long-Term Structure in Music
Creators: name: Roberts, Adam
name: Engel, Jesse
name: Raffel, Colin
name: Hawthorne, Curtis
name: Eck, Douglas
Publisher: name: arXiv
Year: 2018
Subjects: subject: Machine Learning (cs.LG)
subject: Sound (cs.SD)
subject: Audio and Speech Processing (eess.AS)
subject: Machine Learning (stat.ML)
subject: FOS: Computer and information sciences
subject: FOS: Electrical engineering, electronic engineering, information engineering

description: The Variational Autoencoder (VAE) has proven to be an effective model for producing semantically meaningful latent representations for natural data. However, it has thus far seen limited application to sequential data, and, as we demonstrate, existing recurrent VAE models have difficulty modeling sequences with long-term structure. To address this issue, we propose the use of a hierarchical decoder, which first outputs embeddings for subsequences of the input and then uses these embeddings to generate each subsequence independently. This structure encourages the model to utilize its latent code, thereby avoiding the "posterior collapse" problem, which remains an issue for recurrent VAEs. We apply this architecture to modeling sequences of musical notes and find that it exhibits dramatically better sampling, interpolation, and reconstruction performance than a "flat" baseline model. An implementation of our "MusicVAE" is available online at http://g.co/magenta/musicvae-code.
description: ICML Camera Ready Version (w/ fixed typos)
Joint Decoding of LDPC Codes and Finite-State Channels via Linear-Programming
Creators: name: Kim, Byung-Hak
name: Pfister, Henry D.
Publisher: name: arXiv
Year: 2011
Subjects: subject: Information Theory (cs.IT)
subject: FOS: Computer and information sciences

description: This paper considers the joint-decoding (JD) problem for finite-state channels (FSCs) and low-density parity-check (LDPC) codes. In the first part, the linear-programming (LP) decoder for binary linear codes is extended to JD of binary-input FSCs. In particular, we provide a rigorous definition of LP joint-decoding pseudo-codewords (JD-PCWs) that enables evaluation of the pairwise error probability between codewords and JD-PCWs in AWGN. This leads naturally to a provable upper bound on decoder failure probability. If the channel is a finite-state intersymbol interference channel, then the joint LP decoder also has the maximum-likelihood (ML) certificate property and all integer-valued solutions are codewords. In this case, the performance loss relative to ML decoding can be explained completely by fractional-valued JD-PCWs. After deriving these results, we discovered some elements were equivalent to earlier work by Flanagan on LP receivers. In the second part, we develop an efficient iterative solver for the joint LP decoder discussed in the first part. In particular, we extend the approach of iterative approximate LP decoding, proposed by Vontobel and Koetter and analyzed by Burshtein, to this problem. By taking advantage of the dual-domain structure of the JD-LP, we obtain a convergent iterative algorithm for joint LP decoding whose structure is similar to BCJR-based turbo equalization (TE). The result is a joint iterative decoder whose per-iteration complexity is similar to that of TE but whose performance is similar to that of joint LP decoding. The main advantage of this decoder is that it appears to provide the predictability of joint LP decoding and superior performance with the computational complexity of TE. One expected application is coding for magnetic storage where the required block-error rate is extremely low and system performance is difficult to verify by simulation.
description: Accepted to IEEE Journal of Selected Topics in Signal Processing (Special Issue on Soft Detection for Wireless Transmission)
Effects of the stellar wind on X-ray spectra of Cygnus X-3
Creators: name: Szostek, A.
name: Zdziarski, A. A.
Publisher: name: arXiv
Year: 2007
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We study X-ray spectra of Cyg X-3 from BeppoSAX, taking into account absorption and emission in the strong stellar wind of its companion. We find the intrinsic X-ray spectra are well modelled by disc blackbody emission, its upscattering by hot electrons with a hybrid distribution, and by Compton reflection. These spectra are strongly modified by absorption and reprocessing in the stellar wind, which we model using the photoionization code cloudy. The form of the observed spectra implies the wind is composed of two phases. A hot tenuous plasma containing most of the wind mass is required to account for the observed features of very strongly ionized Fe. Small dense cool clumps filling <0.01 of the volume are required to absorb the soft X-ray excess, which is emitted by the hot phase but not present in the data. The total mass-loss rate is found to be (0.6--1.6) x 10^-5 solar masses per year. We also discuss the feasibility of the continuum model dominated by Compton reflection, which we find to best describe our data. The intrinsic luminosities of our models suggest that the compact object is a black hole.
description: MNRAS, in press
Calibration of the island effect: Experimental validation of closed-loop focal plane wavefront control on Subaru/SCExAO
Creators: name: N'Diaye, Mamadou
name: Martinache, Frantz
name: Jovanovic, Nemanja
name: Lozi, Julien
name: Guyon, Olivier
name: Norris, Barnaby
name: Ceau, Alban
name: Mary, David
Publisher: name: arXiv
Year: 2017
Subjects: subject: Instrumentation and Methods for Astrophysics (astro-ph.IM)
subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: FOS: Physical sciences

description: Island effect (IE) aberrations are induced by differential pistons, tips, and tilts between neighboring pupil segments on ground-based telescopes, which severely limit the observations of circumstellar environments on the recently deployed exoplanet imagers (e.g., VLT/SPHERE, Gemini/GPI, Subaru/SCExAO) during the best observing conditions. Caused by air temperature gradients at the level of the telescope spiders, these aberrations were recently diagnosed with success on VLT/SPHERE, but so far no complete calibration has been performed to overcome this issue. We propose closed-loop focal plane wavefront control based on the asymmetric Fourier pupil wavefront sensor (APF-WFS) to calibrate these aberrations and improve the image quality of exoplanet high-contrast instruments in the presence of the IE. Assuming the archetypal four-quadrant aperture geometry in 8m class telescopes, we describe these aberrations as a sum of the independent modes of piston, tip, and tilt that are distributed in each quadrant of the telescope pupil. We calibrate these modes with the APF-WFS before introducing our wavefront control for closed-loop operation. We perform numerical simulations and then experimental tests on a real system using Subaru/SCExAO to validate our control loop in the laboratory and on-sky. Closed-loop operation with the APF-WFS enables the compensation for the IE in simulations and in the laboratory for the small aberration regime. Based on a calibration in the near infrared, we observe an improvement of the image quality in the visible range on the SCExAO/VAMPIRES module with a relative increase in the image Strehl ratio of 37%. Our first IE calibration paves the way for maximizing the science operations of the current exoplanet imagers. Such an approach and its results prove also very promising in light of the Extremely Large Telescopes (ELTs) and the presence of similar artifacts.
description: 9 pages, 11 figures, accepted for publication in A&A
Deep learning for sequential decision-making problems in wireless systems
Creators: name: Evmorfos, Spilios
Publisher: name: No Publisher Supplied
Year: 2025

description: The recent advancements in deep learning, coupled with its integration into sequential decision-making frameworks such as dynamic programming, have transformed the approach to solving complex optimization problems in dynamic environments. In wireless systems, spanning both communication and sensing/localization, the need for intelligent and adaptive paradigms has grown increasingly critical. These systems operate in highly dynamic settings characterized by mobility, fluctuating channels, and varying performance demands, which render traditional myopic approaches inadequate. Deep learning enables the modeling of intricate dependencies, and its fusion with sequential decision-making frameworks allows for the approximation of optimal decision policies directly from data and system interactions. This combination facilitates adaptive responses to evolving conditions, making it essential for addressing the challenges and meeting the performance requirements of next-generation wireless networks. This dissertation develops deep learning-based sequential decision-making approaches for various settings and challenges in wireless sensing and communications. Specifically, it addresses the general problem of antenna/sensor selection for thin array design in wireless systems, a recurring issue tackled in prior work through supervised learning, convex optimization, or greedy methods. Here, the problem is reframed as a sequential decision-making task modeled as a deterministic Markov Decision Process. The Generative Flow Networks paradigm is adapted to learn an action-sampling policy, ensuring the probability of reaching each terminal state aligns with its reward. This approach outperforms greedy methods, convex optimization, and supervised learning across standard benchmarks. The second focus is mobile relay motion control. A deep reinforcement learning approach is proposed to optimize relay movement over time under spatiotemporally correlated channels, maximizing the cumulative SINR at the destination. The channel variability introduces high-frequency components into the optimal value function, addressed by integrating Fourier features into the neural network for improved value function estimation. The third setting involves designing Intelligent Reflective Surface (IRS) phase shift values for MISO communication systems under correlated channels. A deep reinforcement learning actor-critic method is developed, leveraging sufficient conditions on the critic's Neural Tangent Kernel to facilitate convergence under deep Q updates.
Second Language Processing in Japanese Scrambled Sentences
Creators: name: Sanako  Mitsugi
name: Macwhinney, Brian
Publisher: name: Carnegie Mellon University
Year: 2010
Subjects: subject: 170199 Psychology not elsewhere classified
subject: FOS: Psychology

description: This study used self-paced reading to examine the processing of Japanese ditransitive scrambling by native speakers and second language (L2) learners of Japanese.Because Japanese places the verb at the end of the clause, the impact of verb-based expectations should be less than it is in English(Trueswell, Tanenhaus & Kello, 1993). Instead of using verb-driven processing,Japanese relies on case markers, and structure-building decisions are made locally(Miyamoto,2002).As a result, if learners are able to utilize the information encoded by case markers, there should not be any extra processing load involved in scrambled sentences.Fifteen native speakers,16 first language (L1) Korean intermediate-level learners, and 16 L1 English intermediate-level learners participated in the study. The conditions included canonical order, accusative scramble order, dative scramble order and dative-accusative scramble order. The results demonstrated that there are no significant differences in reading times among word-order types.These findings indicate that (1) Japanese native speakers make use of case-marked arguments as reliable cues for incremental processing, and (2) L2 learners can acquire this processing strategy at native-like levels, regardless of their L1 backgrounds
Average [O II] nebular emission associated with Mg II absorbers: Dependence on Fe II absorption
Creators: name: Joshi, Ravi
name: Srianand, Raghunathan
name: Petitjean, Patrick
name: Noterdaeme, Pasquier
Publisher: name: arXiv
Year: 2018
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We investigate the effect of Fe II equivalent width ($W_{2600}$) and fibre size on the average luminosity of [O II]$λλ$3727,3729 nebular emission associated with Mg II absorbers (at $0.55 \le z \le 1.3$) in the composite spectra of quasars obtained with 3 and 2 arcsec fibres in the Sloan Digital Sky Survey. We confirm the presence of strong correlations between [O II] luminosity (L$_{[\rm O~II]}$) and equivalent width ($W_{2796}$) and redshift of Mg II absorbers. However, we show L$_{[\rm O~II]}$ and average luminosity surface density suffers from fibre size effects. More importantly, for a given fibre size the average L$_{[\rm O~II]}$ strongly depends on the equivalent width of Fe II absorption lines and found to be higher for Mg II absorbers with $R \equiv$ $W_{\rm 2600}/W_{\rm 2796}$ $\ge 0.5$. In fact, we show the observed strong correlations of L$_{[\rm O~II]}$ with $W_{2796}$ and $z$ of Mg II absorbers are mainly driven by such systems. Direct [O II] detections also confirm the link between L$_{[\rm O~II]}$ and $R$. Therefore, one has to pay attention to the fibre losses and dependence of redshift evolution of Mg II absorbers on $W_{2600}$ before using them as a luminosity unbiased probe of global star formation rate density. We show that the [O II] nebular emission detected in the stacked spectrum is not dominated by few direct detections (i.e., detections $\ge 3 σ$ significant level). On an average the systems with $R$ $\ge 0.5$ and $W_{2796}$ $\ge 2$ Å are more reddened, showing colour excess E($B-V$) $\sim$ 0.02, with respect to the systems with $R$ $< 0.5$ and most likely traces the high H I column density systems.
description: 16 Pages, 5 Tables, 13 Figures (Accepted for the publication in MNRAS main Journal)
Quantum interference and entanglement of photons which do not overlap in time
Creators: name: Wiegner, R.
name: Thiel, C.
name: von Zanthier, J.
name: Agarwal, G. S.
Publisher: name: arXiv
Year: 2011
Subjects: subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: We discuss the possibility of quantum interferences and entanglement of photons which exist at different intervals of time, i.e., one photon being recorded before the other has been created. The corresponding two-photon correlation function is shown to violate Bell's inequalities.
description: 3 pages, 2 figures
Crawling technicolor
Creators: name: Catà, O.
name: Crewther, R. J.
name: Tunstall, Lewis C.
Publisher: name: arXiv
Year: 2018
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: High Energy Physics - Lattice (hep-lat)
subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We analyze the Callan-Symanzik equations when scale invariance at a nontrivial infrared (IR) fixed point $α^{}_{\mathrm{IR}}$ is realized in the Nambu-Goldstone (NG) mode. As a result, Green's functions at $α^{}_{\mathrm{IR}}$ do not scale in the same way as for the conventional Wigner-Weyl (WW) mode. This allows us to propose a new mechanism for dynamical electroweak symmetry breaking where the running coupling $α$ "crawls" towards (but does not pass) $α^{}_{\mathrm{IR}}$ in the exact IR limit. The NG mechanism at $α^{}_{\mathrm{IR}}$ implies the existence of a massless dilaton $σ$, which becomes massive for IR expansions in $ε\equiv α^{}_{\mathrm{IR}} - α$ and is identified with the Higgs boson. Unlike "dilatons" that are close to a WW-mode fixed point or associated with a Coleman-Weinberg potential, our NG-mode dilaton is genuine and hence naturally light. Its (mass)$^2$ is proportional to $εβ'(4+β')F_σ^{-2} \langle\hat{G}^2\rangle_{\text{vac}}$, where $β'$ is the (positive) slope of the beta function at $α^{}_{\mathrm{IR}}$, $F_σ$ is the dilaton decay constant and $\langle\hat{G}^2\rangle_{\text{vac}}$ is the technigluon condensate. Our effective field theory for this works because it respects Zumino's consistency condition for dilaton Lagrangians. We find a closed form of the Higgs potential with $β'$-dependent deviations from that of the Standard Model. Flavor-changing neutral currents are suppressed if the crawling region $α\lesssim α^{}_{\mathrm{IR}}$ includes a sufficiently large range of energies above the TeV scale. In Appendix A, we observe that, contrary to folklore, condensates protect fields from decoupling in the IR limit.
description: 42 pages, 4 figures, as in PRD except for the Table of Contents, with Zumino's consistency condition for dilaton Lagrangians highlighted in Sec. 4
title: Appel à candidatures résidence Fondation Camargo 2014
Creators: name: LabexMed
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2020

description: Appel à résidence initié par la Fondation Camargo, en partenariat avec le LabexMed.
Additional file 4 of Organizational attributes of interprofessional primary care for adults with intellectual and developmental disabilities in ontario, Canada: a multiple case study
Creators: name: Bobbette, Nicole
name: Lysaght, Rosemary
name: Ouellette-Kuntz, Hélène
name: Tranmer, Joan
name: Donnelly, Catherine
Publisher: name: figshare
Year: 2021
Subjects: subject: Medicine
subject: Biotechnology
subject: 59999 Environmental Sciences not elsewhere classified
subject: FOS: Earth and related environmental sciences
subject: Ecology
subject: FOS: Biological sciences
subject: Sociology
subject: FOS: Sociology
subject: 69999 Biological Sciences not elsewhere classified
subject: Science Policy

description: Additional file 4.