cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Performance of the EDELWEISS-III experiment for direct dark matter searches
Creators: name: Armengaud, E.
name: Arnaud, Q.
name: Augier, C.
name: Benoît, A.
name: Bergé, L.
name: Bergmann, T.
name: Billard, J.
name: de Boissière, T.
name: Bres, G.
name: Broniatowski, A.
name: Brudanin, V.
name: Camus, P.
name: Cazes, A.
name: Chapellier, M.
name: Charlieux, F.
name: De Jésus, M.
name: Dumoulin, L.
name: Eitel, K.
name: Filosofov, D.
name: Foerster, N.
name: Fourches, N.
name: Garde, G.
name: Gascon, J.
name: Giuliani, A.
name: Grollier, M.
name: Gros, M.
name: Hehn, L.
name: Hervé, S.
name: Heuermann, G.
name: Humbert, V.
name: Jin, Y.
name: Juillard, A.
name: Kéfélian, C.
name: Kleifges, M.
name: Kozlov, V.
name: Kraus, H.
name: Kudryavtsev, V. A.
name: Le-Sueur, H.
name: Lin, J.
name: Maisonobe, R.
name: Mancuso, M.
name: Marnieros, S.
name: Menshikov, A.
name: Navick, X. -F.
name: Nones, C.
name: Olivieri, E.
name: Pari, P.
name: Paul, B.
name: Poda, D.
name: Queguiner, E.
name: Robinson, M.
name: Rodenas, H.
name: Rozov, S.
name: Sanglard, V.
name: Schmidt, B.
name: Scorza, S.
name: Siebenborn, B.
name: Tcherniakhovski, D.
name: Vagneron, L.
name: Weber, M.
name: Yakushev, E.
name: Zhang, X.
name: Zolotarova, A.
Publisher: name: arXiv
Year: 2017
Subjects: subject: Instrumentation and Detectors (physics.ins-det)
subject: Instrumentation and Methods for Astrophysics (astro-ph.IM)
subject: FOS: Physical sciences

description: We present the results of measurements demonstrating the efficiency of the EDELWEISS-III array of cryogenic germanium detectors for direct dark matter searches. The experimental setup and the FID (Fully Inter-Digitized) detector array is described, as well as the efficiency of the double measurement of heat and ionization signals in background rejection. For the whole set of 24 FID detectors used for coincidence studies, the baseline resolutions for the fiducial ionization energy are mainly below 0.7 keV$_{ee}$ (FHWM) whereas the baseline resolutions for heat energies are mainly below 1.5 keV$_{ee}$ (FWHM). The response to nuclear recoils as well as the very good discrimination capability of the FID design has been measured with an AmBe source. The surface $β$- and $α$-decay rejection power of $R_{\rm surf} < 4 \times 10^{-5}$ per $α$ at 90% C.L. has been determined with a $^{210}$Pb source, the rejection of bulk $γ$-ray events has been demonstrated using $γ$-calibrations with $^{133}$Ba sources leading to a value of $R_{γ{\rm -mis-fid}} < 2.5 \times 10^{-6}$ at 90% C.L.. The current levels of natural radioactivity measured in the detector array are shown as the rate of single $γ$ background. The fiducial volume fraction of the FID detectors has been measured to a weighted average value of $(74.6 \pm 0.4)\%$ using the cosmogenic activation of the $^{65}$Zn and $^{68,71}$Ge isotopes. The stability and uniformity of the detector response is also discussed. The achieved resolutions, thresholds and background levels of the upgraded EDELWEISS-III detectors in their setup are thus well suited to the direct search of WIMP dark matter over a large mass range.
title: ADCO, Cartulaire général de Cîteaux, dit de Jean de Cirey, (XVe siècle), tome I, Cart. 185 (11 H 70), f. 0184v
Creators: name: de la Côte d'Or, Archives départementales
name: Archives Départementales De La Côte-D'Or
name: Petot, Frédérique
name: Projet CBMA
name: CG21/F.PETOT/2012
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2020
Subjects: subject: Corpus Burgundiae Medii Aevi
subject: Chartes de la Bourgogne du Moyen Âge
subject: cartulaire
subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris

description: Cartulaire général de Cîteaux, dit de Jean de Cirey, (XVe siècle), tome I, Archives départementales de la Côte-d'Or, Cart. 185 (11 H 70), f. 0184v, 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 I, Archives départementales de la Côte-d'Or, Cart. 185 (11 H 70), f. 0184v, 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
title: 1961-1962_TEISSIER Jacques_Un institut médico-pédagogique
Creators: name: Teissier, Jacques
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2023
Subjects: subject: Diplôme d'architecte

description: Prix du meilleur diplôme décerné par la SADG.
title: 02_1017
Creators: name: Wesley Baldwin, John
name: Baldwin, John W.
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2018
Subjects: subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris

description: L'ensemble de ces notes ont été crée par John Baldwin lors d'une de ses premières périodes de résidence à Paris. Ces documents comprennent tous les magistri qu’il avait pu rencontrer dans ses sources. Aux XIIème et XIIIème siècles, les universités n'existant pas encore, le titre de magister s'il évoque certainement une compétence n'est pas rattaché de façon systématique au passage par les écoles. De surcroît, les magistris sont le plus souvent désignés par leur seul prénom. La lecture de ces données est donc difficile et suppose un long travail pour tenter d'identifier un individu auquel on pourrait rattacher plusieurs mentions. John Baldwin avait donc renoncé à utiliser ces données pour donner un prolongement à sa magnifique étude sur les gradués d'université et leur emploi par les Capétiens et les Plantagenêts. Néanmoins, il a conservé ces données et elles sont potentiellement très utile dans le cadre de Studium, comme le sont toutes les mentions dans les volumes des Fasti Ecclesiae Gallicanae de chanoines portant ce titre de magister sans autres précisions. L'ampleur des dépouillements rend ces données très utiles et nous devons une grande reconnaissance à John Baldwin pour avoir pris la peine de faire photocopier ses fiches et de nous les avoir transmises amicalement.
Les données ainsi que les images des fiches sont accessibles sur le site Internet à l'adresse suivante : http://studium-baldwin.lamop.fr/.
Les transcriptions des fiches ont été effectuées par des étudiants de Paris 1 Panthéon - Sorbonne mais elles n'ont pas été corrigées par la suite.
description: Relation: https://lamop.hypotheses.org/
Formation of a Nematic Fluid at High Fields in Sr3Ru2O7
Creators: name: Borzi, R. A.
name: Grigera, S. A.
name: Farrell, J.
name: Perry, R. S.
name: Lister, S. J. S.
name: Lee, S. L.
name: Tennant, D. A.
name: Maeno, Y.
name: Mackenzie, A. P.
Publisher: name: arXiv
Year: 2006
Subjects: subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: FOS: Physical sciences

description: In principle, a complex assembly of strongly interacting electrons can self-organise into a wide variety of collective states, but relatively few such states have been identified in practice. We report that, in the close vicinity of a metamagnetic quantum critical point, high purity Sr3Ru2O7 possesses a large magnetoresistive anisotropy, consistent with the existence of an electronic nematic fluid. We discuss a striking phenomenological similarity between our observations and those made in high purity two-dimensional electron fluids in GaAs devices.
description: 14 pages, 3 figures, 11 extra pages of supplementary information
From the Termite Mound to the Stars: Meditations on Discussions With Ilya Prigogine
Creators: name: Werbos, Paul J.
Publisher: name: arXiv
Year: 2003
Subjects: subject: Populations and Evolution (q-bio.PE)
subject: Other Quantitative Biology (q-bio.OT)
subject: FOS: Biological sciences

description: This paper summarizes and re-evaluates Prigogine's evolution of thought, from a more classical view of thermodynamics with negative implications for the evolution and persistence of life, through to a far more general and open formulation of thermodynamics, which does not require assumption of a Big Bang. The paper also proposes an encoding scheme for the statistics of Lorentzian systems into mixed Fermi-Bose density matrices, to complete the program given in quant-ph/0309087, which forcibly points towards symmetry in time at the microscopic level. The paper suggests future directions to reconcile microscopic time symmetry and macroscopic asymmetry and evolution, and concludes that the space-time continuum may be larger and more interesting than we are able yet to pin down.
description: 5p. Invited paper for special issue in honor of Prigogine, published in Russian and in English
title: بطاقة وثائقية مبوّبة تتضمّن مذكّرات عن ميشيل عفلق وحزب البعث السوري بعد انقلاب 8 آذار 1963
title: Fiche de documentation préclassifiée portant des notes sur Michel Aflaq et le parti Baath syrien après le coup d'Etat du 8 mars 1963
title: Pre-classified documentation sheet including notes about Michel Aflaq and the Ba'th Party after the 1963 Coup d'etat
Creators: name: Seurat, Michel
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2019

description: Notes in French about the Syrian Baath Party for the writing of a chapter in a book or a thesis (Chapter 2).
description: مذكّرات في اللغة الفرنسية عن حزب البعث السوري من أجل كتابة الفصل الثاني لكتاب أو لرسالة دكتوراه
description: Notes en français liées au thème du parti Baath syrien pour la rédaction d'un chapitre d'ouvrage ou de thèse (chapitre 2)
Strongest Goldbach conjecture
Creators: name: Vega, Frank
Publisher: name: figshare
Year: 2018
Subjects: subject: Theoretical Computer Science
subject: 10101 Algebra and Number Theory
subject: FOS: Mathematics

description: The Goldbach's conjecture has been described as the most difficult problem in the history of Mathematics. This conjecture states that every even integer greater than 2 can be written as the sum of two primes. On the other hand, P versus NP is considered as one of the most important open problems in computer science. This consists in knowing the answer of the following question: Is P equal to NP? We will define as the strongest Goldbach conjecture when every even integer greater than 6 can be written as the sum of two different primes. We prove if P = NP, then the strongest Goldbach conjecture is false.
Supplementary document for Characterization of Cell-Induced Astigmatism in High-Resolution Imaging - 5598281.pdf
Creators: name: de Mercado, Rick Rodrigues
name: van Hoorn, Hedde
name: de Valois, Martin
name: Backendorf, Claude
name: Eckert, Julia
name: Schmidt, Thomas
Publisher: name: Optica Publishing Group
Year: 2021
Subjects: Biophysics

description: Supplemental Material
Simulations of Deep Pencil-Beam Redshift Surveys
Creators: name: Yoshida, N.
name: Colberg, J.
name: White, S. D. M.
name: Evrard, A. E.
name: MacFarland, T. J.
name: Couchman, H. M. P.
name: Jenkins, A.
name: Frenk, C. S.
name: Pearce, F. R.
name: Efstathiou, G.
name: Peacock, J. A.
name: Thomas, P. A.
Publisher: name: arXiv
Year: 2000
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We create mock pencil-beam redshift surveys from very large cosmological $N$-body simulations of two Cold Dark Matter cosmogonies, an Einstein-de Sitter model ($τ$CDM) and a flat model with $Ω_0 =0.3$ and a cosmological constant ($Λ$CDM). We use these to assess the significance of the apparent periodicity discovered by Broadhurst et al. (1990). Simulation particles are tagged as `galaxies' so as to reproduce observed present-day correlations. They are then identified along the past light-cones of hypothetical observers to create mock catalogues with the geometry and the distance distribution of the Broadhurst et al. data. We produce 1936 (2625) quasi-independent catalogues from our $τ$CDM ($Λ$CDM) simulation. A couple of large clumps in a catalogue can produce a high peak at low wavenumbers in the corresponding one-dimensional power spectrum, without any apparent large-scale periodicity in the original redshift histogram. Although the simulated redshift histograms frequently display regularly spaced clumps, the spacing of these clumps varies between catalogues and there is no `preferred' period over our many realisations. We find only a 0.72 (0.49) per cent chance that the highest peak in the power spectrum of a $τ$CDM ($Λ$CDM) catalogue has a peak-to-noise ratio higher than that in the Broadhurst et al. data. None of the simulated catalogues with such high peaks shows coherently spaced clumps with a significance as high as that of the real data. We conclude that in CDM universes, the kind of regularity observed by Broadhurst et al. has a priori probability well below $10^{-3}$.
description: 8 pages, 9 figures, submitted to MNRAS
Inverse dispersion method for calculation of complex photonic band diagram and $\cal{PT}$-symmetry
Creators: name: Rybin, Mikhail V.
name: Limonov, Mikhail F.
Publisher: name: arXiv
Year: 2017
Subjects: subject: Optics (physics.optics)
subject: Other Condensed Matter (cond-mat.other)
subject: FOS: Physical sciences

description: We suggest an inverse dispersion method for calculating photonic band diagram for materials with arbitrary frequency-dependent dielectric functions. The method is able to calculate the complex wave vector for a given frequency by solving the eigenvalue problem with a non-Hermitian operator. The analogy with $\cal{PT}$-symmetric Hamiltonians reveals that the operator corresponds to the momentum as a physical quantity and the singularities at the band edges are related to the branch points and responses for the features on the band edges. The method is realized using plane wave expansion technique for two-dimensional periodical structure in the case of TE- and TM-polarization. We illustrate the applicability of the method by calculation of the photonic band diagrams of an infinite two-dimension square lattice composed of dielectric cylinders using the measured frequency dependent dielectric functions of different materials (amorphous hydrogenated carbon, silicon, and chalcogenide glass). We show that the method allows to distinguish unambiguously between Bragg and Mie gaps in the spectra.
description: 8 pages, 5 figures
The Goldbach's Conjecture when P = NP
Creators: name: Vega, Frank
Publisher: name: figshare
Year: 2018
Subjects: subject: Theoretical Computer Science
subject: 10101 Algebra and Number Theory
subject: FOS: Mathematics

description: The Goldbach's conjecture has been described as the most difficult problem in the history of Mathematics. This conjecture states that every even integer greater than 2 can be written as the sum of two primes. On the other hand, P versus NP is considered as one of the most important open problems in computer science. This consists in knowing the answer of the following question: Is P equal to NP? We will define as the strongest Goldbach conjecture when every even integer greater than 6 can be written as the sum of two different primes. We prove if P = NP, then the strongest Goldbach conjecture is false.
Tetrahedral and Cubic Monopoles
Creators: name: Houghton, Conor
name: Sutcliffe, Paul
Publisher: name: arXiv
Year: 1996
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: Using a numerical implementation of the ADHMN construction, we compute the fields and energy densities of a charge three monopole with tetrahedral symmetry and a charge four monopole with octahedral symmetry. We then construct a one parameter family of spectral curves and Nahm data which represent charge four monopoles with tetrahedral symmetry, which includes the monopole with octahedral symmetry as a special case. In the moduli space approximation, this family describes a novel kind of four monopole scattering and we use our numerical scheme to construct the energy density at various times during the motion.
description: uuencoded latex, 22 pages, 3 figures To appear in Communications in Mathematical Physics
Host galaxy properties of mergers of stellar binary black holes and their implications for advanced LIGO gravitational wave sources
Creators: name: Cao, Liang
name: Lu, Youjun
name: Zhao, Yuetong
Publisher: name: arXiv
Year: 2017
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: Understanding the host galaxy properties of stellar binary black hole (SBBH) mergers is important for revealing the origin of the SBBH gravitational-wave sources detected by advanced LIGO and helpful for identifying their electromagnetic counterparts. Here we present a comprehensive analysis of the host galaxy properties of SBBHs by implementing semi-analytical recipes for SBBH formation and merger into cosmological galaxy formation model. If the time delay between SBBH formation and merger ranges from $\la$\,Gyr to the Hubble time, SBBH mergers at redshift $z\la0.3$ occur preferentially in big galaxies with stellar mass $M_*\ga2\times10^{10}\msun$ and metallicities $Z$ peaking at $\sim0.6Z_\odot$. However, the host galaxy stellar mass distribution of heavy SBBH mergers ($M_{\bullet\bullet}\ga50\msun$) is bimodal with one peak at $\sim10^9\msun$ and the other peak at $\sim2\times10^{10}\msun$. The contribution fraction from host galaxies with $Z\la0.2Z_\odot$ to heavy mergers is much larger than that to less heavy mergers. If SBBHs were formed in the early universe (e.g., $z>6$), their mergers detected at $z\la0.3$ occur preferentially in even more massive galaxies with $M_*>3\times10^{10}\msun$ and in galaxies with metallicities mostly $\ga0.2Z_\odot$ and peaking at $Z\sim0.6Z_\odot$, due to later cosmic assembly and enrichment of their host galaxies. SBBH mergers at $z\la0.3$ mainly occur in spiral galaxies, but the fraction of SBBH mergers occur in elliptical galaxies can be significant if those SBBHs were formed in the early universe; and about two thirds of those mergers occur in the central galaxies of dark matter halos. We also present results on the host galaxy properties of SBBH mergers at higher redshift.
description: 12 pages, 9 figures, MNRAS accepted
title: Villancicos que se han de cantar... Texte imprimé
Creators: name: Anonyme
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2020

description: in-4
description: Source: Bibliothèque patrimoniale Villon (Rouen), fonds Liber, Mtm-8667
Octahedral and Dodecahedral Monopoles
Creators: name: Houghton, Conor
name: Sutcliffe, Paul
Publisher: name: arXiv
Year: 1996
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: It is shown that there exists a charge five monopole with octahedral symmetry and a charge seven monopole with icosahedral symmetry. A numerical implementation of the ADHMN construction is used to calculate the energy density of these monopoles and surfaces of constant energy density are displayed. The charge five and charge seven monopoles look like an octahedron and a dodecahedron respectively. A scattering geodesic for each of these monopoles is presented and discussed using rational maps. This is done with the aid of a new formula for the cluster decomposition of monopoles when the poles of the rational map are close together.
description: uuencoded latex, 20 pages, 2 figures To appear in Nonlinearity
Simulated metal and HI absorption lines at the conclusion of Reionization
Creators: name: Garcia, L. A.
name: Tescari, E.
name: Ryan-Weber, E. V.
name: Wyithe, J. S. B.
Publisher: name: arXiv
Year: 2017
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We present a theoretical study of intergalactic metal absorption lines imprinted in the spectra of distant quasars during and after the Epoch of Reionization (EoR). We use high resolution hydrodynamical simulations at high redshift ($4 6$, consistent with the current picture of the tail of the EoR. The simulated CII exhibits a bimodal distribution with large absorptions in and around galaxies, and some traces in the lower density IGM. We find some discrepancies between the observed and simulated column density relationships among different ionic species at $z=6$, probably due to uncertainties in the assumed UV background. Finally, our simulations are in good agreement with observations of the HI column density distribution function at $z = 4$ and the HI cosmological mass density $Ω_{HI}$ at $4 < z < 6$.
description: 17 pages, 11 figures. Published: 03 June 2017
Additional file 2 of Correlation between lung infection severity and clinical laboratory indicators in patients with COVID-19: a cross-sectional study based on machine learning
Creators: name: Wang, Xingrui
name: Che, Qinglin
name: Ji, Xiaoxiao
name: Meng, Xinyi
name: Zhang, Lang
name: Jia, Rongrong
name: Lyu, Hairong
name: Bai, Weixian
name: Tan, Lingjie
name: Gao, Yanjun
Publisher: name: figshare
Year: 2021
Subjects: subject: Medicine
subject: Microbiology
subject: FOS: Biological sciences
subject: Cell Biology
subject: Immunology
subject: FOS: Clinical medicine
subject: Mathematical Sciences not elsewhere classified
subject: Cancer
subject: Science Policy
subject: Infectious Diseases
subject: FOS: Health sciences
subject: Virology

description: Additional file 2. Clinical laboratory examination results of 31 patients with COVID-19 corresponding to pulmonary VOI and POI at the same stage of the disease.
Mid-Infrared observations of GRS 1915+105 and SS433
Creators: name: Fuchs, Y.
name: Mirabel, I. F.
name: Ogley, R. N.
Publisher: name: arXiv
Year: 2000
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We have observed in the mid-infrared (4-18 micron) the counterpart of the compact object GRS 1915+105, and the western jet of SS433. The images were carried out with the ISOCAM infrared camera on board of the Infrared Space Observatory (ISO). The mid-infrared photometry of GRS 1915+105 shows the presence of an additional contribution besides the synchrotron emission. The 15 micron images of the large-scale western lobe of the SS433/W50 nebula are compared to the radio and X-ray ones. They show infrared synchrotron emission on the western edge of SS433/W50 lobe.
description: 2 pages, 2 color figures, to be published in `Proceedings of the Third Microquasar Workshop: Granada Workshop on galactic relativistic jet sources', Eds A. J.Castro-Tirado, J. Greiner and J. M. Paredes, Astrophysics and Space Science special issue, in press
Universality Constraints on Three-Body Recombination for Cold Atoms: from 4He to 133Cs
Creators: name: Braaten, Eric
name: Kang, Daekyoung
name: Platter, Lucas
Publisher: name: arXiv
Year: 2006
Subjects: subject: Other Condensed Matter (cond-mat.other)
subject: Nuclear Theory (nucl-th)
subject: FOS: Physical sciences

description: For atoms with large scattering length, the dependence of the 3-body recombination rate on the collision energy is determined by the scattering length and the Efimov 3-body parameters and can be expressed in terms of universal functions of a single scaling variable. We use published results on the 3-body recombination rate for 4He atoms to constrain the universal functions. We then use those universal functions to calculate the 3-body recombination rate for other atoms with large scattering length at nonzero temperature. The constraints from the 4He results are strong if the scattering length is near the minimum of the 3-body recombination rate at threshold. We apply our results to 133Cs atoms with a large positive scattering length, and compare them with experimental results from the Innsbruck group.
description: 17 pages, 6 eps figures
Cultural models of child disability: perspectives of parents in Malaysia
Creators: name: Marshall, Jennifer
name: Doone, Elizabeth
name: Price, Mindy
Publisher: name: Taylor & Francis
Year: 2018
Subjects: subject: Medicine
subject: Biotechnology
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: Cancer
subject: Science Policy
subject: 111714 Mental Health
subject: FOS: Health sciences

description: Background: This study examined parents’ developmental concerns for their children within the context of systems of care in Malaysia. Methods: Focus groups and interviews were conducted in peninsular Malaysia and Borneo. Results: Parents’ perceptions of developmental delay stemmed from three sources: the cultural, resource, and the social environments. Conclusion: There is a need to develop a medical support system in Malaysia that considers a life-course perspective, including prenatal care, screening/diagnosis, and services. This system should embrace a family-centered approach to diagnosis, referral, intervention, and support with sensitivity to cultural beliefs, family preferences, and barriers to care.Implications for RehabilitationParental perceptions of disability affect the strategies they use to cope.This research found that cultural conceptions of disability, available resources, and social support affect parental perceptions of disability.The resource environment in Malaysia significantly restricts parents’ ability to cope with their child's disability.This research recommended that the medical system of Malaysia develops a life-course perspective to disability to provide a range of care for children with disabilities including prenatal care, screening and rehabilitation or coping services. Parental perceptions of disability affect the strategies they use to cope. This research found that cultural conceptions of disability, available resources, and social support affect parental perceptions of disability. The resource environment in Malaysia significantly restricts parents’ ability to cope with their child's disability. This research recommended that the medical system of Malaysia develops a life-course perspective to disability to provide a range of care for children with disabilities including prenatal care, screening and rehabilitation or coping services.
Additional file 1 of Correlation between lung infection severity and clinical laboratory indicators in patients with COVID-19: a cross-sectional study based on machine learning
Creators: name: Wang, Xingrui
name: Che, Qinglin
name: Ji, Xiaoxiao
name: Meng, Xinyi
name: Zhang, Lang
name: Jia, Rongrong
name: Lyu, Hairong
name: Bai, Weixian
name: Tan, Lingjie
name: Gao, Yanjun
Publisher: name: figshare
Year: 2021
Subjects: subject: Medicine
subject: Microbiology
subject: FOS: Biological sciences
subject: Cell Biology
subject: Immunology
subject: FOS: Clinical medicine
subject: Mathematical Sciences not elsewhere classified
subject: Cancer
subject: Science Policy
subject: Infectious Diseases
subject: FOS: Health sciences
subject: Virology

description: Additional file 1. Overal pulmonary infection results in 31 patients with COVID-19 calculated by AI system.
Tropical Geometry of Statistical Models
Creators: name: Pachter, Lior
name: Sturmfels, Bernd
Publisher: name: arXiv
Year: 2003
Subjects: subject: Quantitative Methods (q-bio.QM)
subject: Algebraic Geometry (math.AG)
subject: Genomics (q-bio.GN)
subject: FOS: Biological sciences
subject: FOS: Mathematics

description: This paper presents a unified mathematical framework for inference in graphical models, building on the observation that graphical models are algebraic varieties. From this geometric viewpoint, observations generated from a model are coordinates of a point in the variety, and the sum-product algorithm is an efficient tool for evaluating specific coordinates. The question addressed here is how the solutions to various inference problems depend on the model parameters. The proposed answer is expressed in terms of tropical algebraic geometry. A key role is played by the Newton polytope of a statistical model. Our results are applied to the hidden Markov model and to the general Markov model on a binary tree.
description: 14 pages, 3 figures. Major revision. Applications now in companion paper, "Parametric Inference for Biological Sequence Analysis"
Suppression of Bekenstein-Hawking radiation in $f(T)$-gravity
Creators: name: Addazi, Andrea
Publisher: name: arXiv
Year: 2017
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We discuss semiclassical Nariai black holes in the framework of $f(T)$-gravity. For a diagonal choice of tetrades, stable Nariai metrics can be found, emitting Bekenstein-Hawking radiation in semiclassical limit. However, for a non-diagonal choice of tetrades, evaporation and antievaporation instabilities are turned on. In turn, this causes a back-reaction effect suppressing the Bekenstein-Hawking radiation. In particular, evaporation instabilities produce a new radiation -- different by Bekenstein-Hawking emission -- non-violating unitarity in particle physics sector.
Stereo Imaging of the VHE Gamma-Rays with HEGRA and H.E.S.S
Creators: name: Konopelko, Alexander K
Publisher: name: arXiv
Year: 2000
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: At present, the ground-based astronomy of very high energy (VHE) (E>100 GeV) gamma-rays experiences the challenging transition phase caused by the substantial upgrading of its observational instrumentation. Recently the HEGRA collaboration has evidently demonstrated the power of arrays of imaging atmospheric Cherenkov telescopes and initiated a number of complementary projects, such as H.E.S.S., CANGAROO IV, VERITAS. The common philosophy of those projects is based on the stereoscopic observations of air showers with a number of imaging telescopes simultaneously. Such observations allow to reduce substantially the effective energy threshold of detected gamma-ray showers; to improve the angular and energy resolution for individual gamma-rays; to gain in suppression of the cosmic ray background. In my talk I have summarized the general advantages and achieved sensitivity of the stereoscopic observations using the HEGRA data taken with an array of 5 imaging telescopes having the energy threshold of 500 GeV. These results completed with the relevant simulations may be extrapolated on a firm ground towards the future H.E.S.S. (phase I) array of four 12 m imaging telescopes with the estimated energy threshold below 100 GeV. Here I discuss in short the anticipated performance of such an array.
description: 5 pages, 2 figures, to appear in proc. of ``Heidelberg International Symposium on High Energy Gamma-Ray Astronomy'' edited by F. Aharonian and H. Voelk, AIP Conf. Proc
On-line ethics education for occupational therapy clinician–educators: a single-group pre-/post-test study
Creators: name: VanderKaay, Sandra
name: Letts, Lori
name: Jung, Bonny
name: Moll, Sandra E.
Publisher: name: Taylor & Francis
Year: 2018
Subjects: subject: Medicine
subject: Biotechnology
subject: Sociology
subject: FOS: Sociology
subject: Cancer
subject: Science Policy
subject: 111714 Mental Health
subject: FOS: Health sciences

description: Purpose: Ethics education is a critical component of training rehabilitation practitioners. There is a need for capacity-building among ethics educators regarding facilitating ethical decision-making among students. The purpose of this study was to evaluate the utility of an on-line ethics education module for occupational therapy clinician-educators (problem-based learning tutors/clinical placement preceptors/evidence-based practice facilitators). Method: The Knowledge-to-Action Process informed development and evaluation of the module. Clinician–educators (n = 33) viewed the module and reported on its impact on knowledge and facilitation practices via pre, post, and follow-up questionnaires. Results: Pre- and post-test data indicated improvement in self-reported ethics knowledge (t = 8.275, p t = −1.483, p = 0.075). There was improvement in self-reported intent to change practice (t = 4.93, p t = −1.499, p = 0.072). Conclusion: This study provides preliminary data regarding an on-line ethics education module for clinician–educators. Future recommendations include broader consideration of context, adding supplemental knowledge translation components, and further research exploring outcomes with larger samples, longer follow-up and randomized trial methodology.Implications for RehabilitationThe on-line ethics module has potential to improve rehabilitation practice by addressing the noted gap in knowledge among clinician-educators.Viewing an on-line module regarding approaches to ethics education may not be sufficient to change clinician-educators’ teaching practices.More time and opportunities to discuss ethics with student occupational therapists may be required to effect practice change among clinician-educators.Developing ethics education tools for clinician-educators requires ongoing and iterative input from knowledge users to optimize translation of ideas to practice. The on-line ethics module has potential to improve rehabilitation practice by addressing the noted gap in knowledge among clinician-educators. Viewing an on-line module regarding approaches to ethics education may not be sufficient to change clinician-educators’ teaching practices. More time and opportunities to discuss ethics with student occupational therapists may be required to effect practice change among clinician-educators. Developing ethics education tools for clinician-educators requires ongoing and iterative input from knowledge users to optimize translation of ideas to practice.
title: ADCO, Cartulaire de Cîteaux pour les possessions de Chaugey et Maison-Dieu (Fin XVe siècle), Cart. 181 (11 H 754), 165 folios, f. 0071
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/2017
name: Petot, Frédéric
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2020
Subjects: subject: cartulaire
subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris
subject: Corpus Burgundiae Medii Aevi
subject: Chartes de la Bourgogne du Moyen Âge

description: Cartulaire de Cîteaux pour les possessions de Chaugey et Maison-Dieu (Fin XVe siècle), Archives départementales de la Côte-d'Or, Cart. 181 (11 H 754), 165 folios, f. 0071, Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Cartulaire de Cîteaux pour les possessions de Chaugey et Maison-Dieu (Fin XVe siècle), Archives départementales de la Côte-d'Or, Cart. 181 (11 H 754), 165 folios, f. 0071, 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
Rehabilitation for disabling hearing loss: evaluating the need relative to provision of hearing aids in the public health care system
Creators: name: Vera-Genevey Hlayisi
name: Lebogang Ramma
Publisher: name: Taylor & Francis
Year: 2019
Subjects: subject: Medicine
subject: Neuroscience
subject: Physiology
subject: FOS: Biological sciences
subject: Biotechnology
subject: 69999 Biological Sciences not elsewhere classified
subject: Science Policy
subject: 111714 Mental Health
subject: FOS: Health sciences
subject: Hematology

description: Purpose: To determine the demand relative to supply of hearing rehabilitation through hearing aids for those with disabling hearing loss in a public health care setting in South Africa. Methods: Retrospective cross-sectional survey of medical records of all patients were seen at a public hospital (Polokwane Provincial Academic) during 2012–2014, was conducted. Audiological data from 3894 medical folders were accessed and reviewed; thereafter, results were analyzed using descriptive statistics. Results: Of the 3894 medical folders reviewed, two-third (62%, n = 2402) were diagnosed with hearing loss, mostly bilaterally (81%). More than 30% of all patients diagnosed with hearing loss were ≤10 years old. Sensorineural (permanent) hearing loss was diagnosed most often (38%, n = 913) and 74% (n = 1778) of hearing losses diagnosed were of moderate or worse severity (i.e., disabling loss). Hearing aids were fitted to only 15% (n = 272) of those diagnosed with disabling hearing loss and most hearing aid fittings were to low-income adult patients (≥25 years old) with more severe-profound hearing losses. Conclusions: This study showed that the need for hearing aids to provide hearing rehabilitation far exceeds the supply. Therefore, a multi-pronged approach that includes increased budget allocation and exploring low-cost interventions for developing countries to meet the demand for hearing aids. Furthermore, study highlighted a high prevalence of hearing loss in those younger than 10 years of age, and thus highlights the need for early intervention as well as intensifying efforts to reduce preventable causes of hearing loss. Implications for RehabilitationAudiologists need to advocate for an increase in budget allocation for hearing rehabilitation devices.Study indicates need to explore low-cost hearing devices/rehabilitation interventions for developing countries.Health professionals should consider preventative measures to reduce prevalence of preventable hearing loss. Audiologists need to advocate for an increase in budget allocation for hearing rehabilitation devices. Study indicates need to explore low-cost hearing devices/rehabilitation interventions for developing countries. Health professionals should consider preventative measures to reduce prevalence of preventable hearing loss.
Magnetic Connections in Curved Spacetime
Creators: name: Asenjo, Felipe A.
name: Comisso, Luca
Publisher: name: arXiv
Year: 2017
Subjects: subject: Plasma Physics (physics.plasm-ph)
subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: The ideal MHD theorem on the conservation of the magnetic connections between plasma elements is generalized to relativistic plasmas in curved spacetime. The connections between plasma elements, which are established by a covariant connection equation, display a particularly complex structure in curved spacetime. Nevertheless, it is shown that these connections can be interpreted in terms of magnetic field lines alone by adopting a $3+1$ foliation of spacetime.
Monopole Scattering with a Twist
Creators: name: Houghton, Conor
name: Sutcliffe, Paul
Publisher: name: arXiv
Year: 1996
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: By imposing certain combined inversion and rotation symmetries on the rational maps for SU(2) BPS monopoles we construct geodesics in the monopole moduli space. In the moduli space approximation these geodesics describe a novel kind of monopole scattering. During these scattering processes axial symmetry is instantaneously attained and, in some, monopoles with the symmetries of the regular solids are formed. The simplest example corresponds to a charge three monopole invariant under a combined inversion and 90 degree rotation symmetry. In this example three well-separated collinear unit charge monopoles coalesce to form first a tetrahedron, then a torus, then the dual tetrahedron and finally separate again along the same axis of motion. We explicitly construct the spectral curves in this case and use a numerical ADHMN construction to compute the energy density at various times during the motion. We find that the dynamics of the zeros of the Higgs field is extremely rich and we discover a new phenomenon; there exist charge k SU(2) BPS monopoles with more than k zeros of the Higgs field.
description: uuencoded latex, 32 pages, 4 figures To appear in Nuclear Physics B
Spectral properties of 441 radio pulsars
Creators: name: Jankowski, F.
name: van Straten, W.
name: Keane, E. F.
name: Bailes, M.
name: Barr, E.
name: Johnston, S.
name: Kerr, M.
Publisher: name: arXiv
Year: 2017
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: We present a study of the spectral properties of 441 pulsars observed with the Parkes radio telescope near the centre frequencies of 728, 1382 and 3100 MHz. The observations at 728 and 3100 MHz were conducted simultaneously using the dual-band 10-50cm receiver. These high-sensitivity, multi-frequency observations provide a systematic and uniform sample of pulsar flux densities. We combine our measurements with spectral data from the literature in order to derive the spectral properties of these pulsars. Using techniques from robust regression and information theory we classify the observed spectra in an objective, robust and unbiased way into five morphological classes: simple or broken power law, power law with either low or high-frequency cut-off and log-parabolic spectrum. While about $79 \%$ of the pulsars that could be classified have simple power law spectra, we find significant deviations in 73 pulsars, 35 of which have curved spectra, 25 with a spectral break and 10 with a low-frequency turn-over. We identify 11 gigahertz-peaked spectrum (GPS) pulsars, with 3 newly identified in this work and 8 confirmations of known GPS pulsars; 3 others show tentative evidence of GPS, but require further low-frequency measurements to support this classification. The weighted mean spectral index of all pulsars with simple power law spectra is $-1.60 \pm 0.03$. The observed spectral indices are well described by a shifted log-normal distribution. The strongest correlations of spectral index are with spin-down luminosity, magnetic field at the light-cylinder and spin-down rate. We also investigate the physical origin of the observed spectral features and determine emission altitudes for three pulsars.
description: 33 pages, 11 figures, 13 tables, accepted in MNRAS
ОСОБЕННОСТИ ПРОДВИЖЕНИЯ ЭТНОКУЛЬТУРНЫХ БРЕНДОВ В КОНТЕКСТЕ ФОРМИРОВАНИЯ И РЕАЛИЗАЦИИ ПОТЕНЦИАЛА ТЕРРИТОРИАЛЬНЫХ МУЗЕЕВ
Creators: name: Горлова Ирина Ивановна
name: Бычкова Ольга Ивановна
name: Костина Наталья Анатольевна
Publisher: name: Культурное наследие России
Year: 2019
Subjects: Региональная культурная политика
брендинг
этнокультурный бренд
потенциал
продвижение
территориальные музеи

description: В контексте социокультурного развития территорий этнокультурное брендирование выступает как мультипликатор развития региона и инструмент повышения конкурентоспособности локации. Коммуникационная составляющая этнокультурного брендирования представляется особенно важной для его регионального развития и продвижения. Деятельность по поддержке и продвижению разнообразных этнокультурных проектов напрямую влияет на реализацию регионального потенциала по этнокультурному брендированию. В такой ситуации процесс приближения этнокультурных брендов к трендам современности возможен на базе региональных музеев, где сосредоточены объекты культурного наследия, которые можно рассматривать как потенциальные объекты этнокультурного брендирования. В статье предложена методика определения территориальных рейтингов формирования и реализации потенциала территориальных музеев в этнокультурном брендинге региона. Установление итоговой рейтинговой оценки позволяет дифференцировать регионы в области этнокультурного брендирования в зависимости от социокультурных и экономических особенностей территории.
Analytic models for mechanotransduction: gating a mechanosensitive channel
Creators: name: Wiggins, Paul
name: Phillips, Rob
Publisher: name: arXiv
Year: 2003
Subjects: subject: Biomolecules (q-bio.BM)
subject: FOS: Biological sciences

description: Analytic estimates for the forces and free energy generated by bilayer deformation reveal a compelling and intuitive model for MscL channel gating analogous to the nucleation of a second phase. We argue that the competition between hydrophobic mismatch and tension results in a surprisingly rich story which can provide both a quantitative comparison to measurements of opening tension for MscL when reconstituted in bilayers of different thickness and qualitative insights into the function of the MscL channel and other transmembrane proteins.
New Results on the Helium Stars in the Galactic Center Using BEAR Spectro-Imagery
Creators: name: Paumard, T.
name: Maillard, J. P.
name: Morris, M.
name: Rigaut, F.
Publisher: name: arXiv
Year: 2000
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Integral field spectroscopy of the central parsec of the Galactic Center was obtained at 2.06 microns using BEAR, an imaging Fourier Transform Spectrometer, at a spectral resolution of 74 km/s. Sixteen stars were confirmed as helium stars by detecting the He I 2.058 microns line in emission, providing a homogeneous set of fully resolved line profiles. These observations allow us to discard some of the earlier detections of such stars in the central cluster and to add three new stars. The sources detected in the BEAR data were compared with adaptive optics images in the K band to determine whether the emission was due to single stars. Two sub-classes of almost equal number are clearly identified from the width of their line profiles, and from the brightness of their continuum. Most of the emission lines show a P Cygni profile. From these results, we propose that the latter group is formed of stars in or near the LBV phase, and the other one of stars at the WR stage. The division into two groups is also shown by their spatial distribution, with the narrow-line stars in a compact central cluster (IRS 16) and the other group distributed at the periphery of the central cluster of hot stars. In the same data cube, streamers of interstellar helium gas are also detected. The helium emission traces the densest parts of the SgrA West Mini-Spiral. Several helium stars have a radial velocity comparable to the velocity of the interstellar gas in which they are embedded. In the final discussion, all these findings are examined to present a possible scenario for the formation of very massive stars in the exceptional conditions of the vicinity of the central Black Hole.
description: 16 pages, 9 figures. To be published in Astronomy & Astrophysics
M2-brane Dynamics in the Classical Limit of the BMN Matrix Model
Creators: name: Axenides, Minos
name: Floratos, Emmanuel
name: Linardopoulos, Georgios
Publisher: name: arXiv
Year: 2017
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We investigate the large-N limit of the BMN matrix model by analyzing the dynamics of ellipsoidal M2-branes that spin in the 11-dimensional maximally supersymmetric SO(3)xSO(6) plane-wave background. We identify finite-energy solutions by specifying the local minima of the corresponding energy functional. These configurations are static in SO(3) due to the Myers effect and rotate in SO(6) with an angular momentum that is bounded from above. As a first step towards studying their chaotic properties, we evaluate the Lyapunov exponents of their radial fluctuations.
description: 7 pages, 8 figures