cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Update on the X-ray variability plane for active galactic nuclei: The role of the obscuration
Creators: name: González-Martín, O.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: Scaling relations are the most powerful astrophysical tools to set constraints to the physical mechanisms of astro- nomical sources and to infer properties that cannot be accessed directly. We re-investigate here one of these scaling relations in active galactic nuclei (AGN); the so-called X-ray variability plane (or mass-luminosity-timescale relation, McHardy et al. 2006). This relation links the power-spectral density (PSD) break frequency with the super-massive black hole (SMBH) mass and the bolometric luminosity. We used available XMM -Newton observations of a sample of 22 AGN to study the PSD and spectra in short segments within each observation. This allows us to report for the first time that the PSD break frequency varies for each object, showing variations in 19 out of the 22 AGN analyzed. Our analysis of the variability plane confirms the relation between the break frequency and the SMBH mass and finds that the obscuration along the line of sight NH (or the variations on the obscuration using its standard deviation, $\rmΔ$(NH)) is also a required parameter, at least for the range of frequencies analyzed here (3x10E-5-5x10E-2Hz). We constrain a new variability plane of the form: log($ν_{Break}$) = (-0.589$\rm{\pm}$0.005) log(MBH ) + (0.10$\rm{\pm}$0.01) log(NH ) - (1.5$\rm{\pm}$0.3) (or log($ν_{Break}$)=(-0.549$\rm{\pm}$0.009)log(MBH)+(0.56$\rm{\pm}$0.06)$\rmΔ$(NH)+(0.19$\rm{\pm}$0.08)). The X-ray variability plane found by McHardy et al. (2006) is roughly recovered when we use unobscured segments. We speculate that this behavior is well explained if most of the reported frequencies are related to inner clouds (within 1pc), following Kepler orbits under the gravitational field of the SMBH.
description: 15 pages, 5 figures, 3 tables, accepted for publication in ApJ
IINSON SHAXSINING SHAKLLANISHIDA OILANING ROLI
Creators: name: Yo'ldashova, Marjona
Publisher: name: Zenodo
Year: 2025

description: Ushbu maqolada inson shaxsining shakllanishi murakkab va ko‘p bosqichli psixologik jarayon bo‘lib, bu jarayonning asosiy negizini oila muhiti belgilaydi. Oila — bu nafaqat biogenetik birlik, balki shaxsning qadriyatlari, emotsional barqarorligi, ijtimoiy me’yorlarni o‘rganishi va moslashuvchanlik ko‘nikmalari shakllanadigan birlamchi ijtimoiy institutdir. Maqolada oila tizimining psixologik ta’sir mexanizmlari, ota-ona va farzand o‘rtasidagi emotsional munosabatlarning shaxs tarbiyasidagi o‘rni, oilaning shaxsiy fazilatlarni rivojlantirishdagi psixopedagogik ahamiyati ilmiy asosda yoritilgan. Shuningdek, zamonaviy oilaviy tarbiyaning shaxs shakllanishiga ta’siri va sotsiokulturning o‘zgarishi natijasida yuzaga kelayotgan yangi tarbiyaviy muammolar keng tahlil qilinadi.
From cluster structures to nuclear molecules: the role of nodal structure of the single-particle wave functions
Creators: name: Afanasjev, A. V.
name: Abusara, H.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Nuclear Theory (nucl-th)
subject: FOS: Physical sciences

description: The nodal structure of the density distributions of the single-particle states occupied in rod-shaped, hyper- and megadeformed structures of non-rotating and rotating $N\sim Z$ nuclei has been investigated in detail. The single-particle states with the Nilsson quantum numbers of the $[NN0]1/2$ (with $N$ from 0 to 5) and $[N,N-1,1]Ω$ (with $N$ from 1 to 3 and $Ω=1/2$, 3/2) types are considered. These states are building blocks of extremely deformed shapes in the nuclei with mass numbers $A \leq 50$. Because of (near)axial symmetry and large elongation of such structures, the wave functions of the single-particle states occupied are dominated by a single basis state in cylindrical basis. This basis state defines the nodal structure of the single-particle density distribution. The nodal structure of the single-particle density distributions allows to understand in a relatively simple way the necessary conditions for $α$-clusterization and the suppression of the $α$-clusterization with the increase of mass number. It also explains in a natural way the coexistence of ellipsoidal mean-field type structures and nuclear molecules at similar excitation energies and the features of particle-hole excitations connecting these two types of the structures. Our analysis of the nodal structure of the single-particle density distributions does not support the existence of quantum liquid phase for the deformations and nuclei under study.
Updating the census of star clusters in the Small Magellanic Cloud
Creators: name: Bica, E.
name: Dutra, C. M.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Surveys using CCD detectors are retrieving bright and faint cataloged clusters and revealing new ones in the Magellanic Clouds. This paper discusses the contribution of the OGLE Survey to the overall census of star clusters in the SMC. A detailed cross-identification indicates that the new objects in the SMC OGLE catalog are 46. The increase in the number of cataloged clusters is ~ 7%, the total sample being ~ 700. This updated census includes embedded clusters in HII regions and a density range attaining loose systems.
description: manuscript in LATEX with 13 pages, 2 figures and one eletronic table. Also available: http://www.if.ufrgs.br/~dutra/catpage.html Accepted to: The Astronomical Journal
Additional file 8: of Functional annotation and distribution overview of RNA families in 27Â Streptococcus agalactiae genomes
Creators: name: Wolf, Ivan
name: Paschoal, Alexandre
name: Quiroga, Cecilia
name: Domingues, Douglas
name: RogĂŠrio De Souza
name: Pretto-Giordano, Lucienne
name: Laurival Vilas-Boas
Publisher: name: figshare
Year: 2018
Subjects: subject: Biochemistry
subject: Space Science
subject: Medicine
subject: Microbiology
subject: FOS: Biological sciences
subject: Genetics
subject: Molecular Biology
subject: Sociology
subject: FOS: Sociology
subject: 69999 Biological Sciences not elsewhere classified
subject: Developmental Biology
subject: 110309 Infectious Diseases
subject: FOS: Health sciences
subject: 60506 Virology
subject: Computational Biology

description: Coverage plots for surrounding region of new detected RNA families in strain NEM316. (PDF 1039 kb)
Additional file 2 of HyperChIP: identification of hypervariable signals across ChIP-seq or ATAC-seq samples
Creators: name: Chen, Haojie
name: Tu, Shiqi
name: Yuan, Chongze
name: Tian, Feng
name: Zhang, Yijing
name: Sun, Yihua
name: Shao, Zhen
Publisher: name: figshare
Year: 2022
Subjects: subject: Genetics
subject: FOS: Biological sciences

description: Additional file 2: Note S1. Statistical simulation. Note S2. Applying HyperChIP without separating proximal and distal regions. S2.1. Evaluating separately the rankings of proximal and distal regions. S2.2. Evaluating the overall rankings of all peak regions. Note S3. Quality control. Note S4. Defining proximal and distal regions.
Charm Production in Hadronic and Heavy-Ion Collisions at RHIC and LHC Energies to $O(α_s^3)$
Creators: name: Sarcevic, Ina
name: Valerio, Peter
Publisher: name: arXiv
Year: 1994
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: Nuclear Theory (nucl-th)
subject: FOS: Physical sciences

description: We present results on rapidity and transverse momentum distributions of inclusive charm quark production in hadronic and heavy-ion collisions at RHIC and LHC energies, including the next-to-leading order, $O(α_s^3)$, radiative corrections and the nuclear shadowing effect. We determine the hadronic and the {\it effective} (in-medium) K-factor for the differential and total inclusive charm cross sections. We find the fraction of central and inelastic events that contain at least one charm quark pair at LHC energies and obtain the effective $A$-dependence of the inclusive charm production in proton-nucleus and nucleus-nucleus collisions at RHIC and in nucleus-nucleus collisions at the LHC. We discuss theoretical uncertainties inherent in our calculation. In particular, we show how different extrapolations of gluon density in a nucleon {\em and} in a nucleus to the low-$x$ region introduce large theoretical uncertainty in the calculation of charm production at LHC energies.
description: LaTex, 18 pages, 11 figs (available on request)
Eta Carinae: Binarity Confirmed
Creators: name: Damineli, Augusto
name: Kaufer, Andreas
name: Wolf, Bernhard
name: Stahl, Otmar
name: Lopes, Dalton F.
name: de Araujo, Francisco X.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We report the recovery of a spectroscopic event in eta Carinae in 1997/98 after a prediction by Damineli (1996). A true periodicity with P = 2020+-5 days (0.2% uncertainty) is obtained. The line intensities and the radial-velocity curve display a phase-locked behavior implying that the energy and dynamics of the event repeat from cycle to cycle. This rules out S Doradus oscillation or multiple shell ejection by an unstable star as the explanation of the spectroscopic events. A colliding-wind binary scenario is supported by our spectroscopic data and by X-ray observations. Although deviations from a simple case exist around periastron, intensive monitoring during the next event (mid 2003) will be crucial to the understanding of the system.
description: 13 pages, accepted by ApJ Letters (January 2000)
Driving factors behind multiple populations
Creators: name: Huang, Ruoyun
name: Tang, Baitian
name: Li, Chengyuan
name: Geisler, Doug
name: Mateo, Mario
name: Song, Ying-Yi
name: Baumgardt, Holger
name: Carballo-Bello, Julio A.
name: Wang, Yue
name: Nie, Jundan
name: Dias, Bruno
name: Fernández-Trincado, José G.
Publisher: name: arXiv
Year: 2024
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: Star clusters were historically considered simple stellar populations, with all stars sharing the same age and initial chemical composition. However, the presence of chemical anomalies in globular clusters (GCs), called multiple stellar populations (MPs), has challenged star formation theories in dense environments. Literature studies show that mass, metallicity, and age are likely controlling parameters for the manifestation of MPs. Identifying the limit between clusters with/without MPs in physical parameter space is crucial to reveal the driving mechanism behind their presence. In this study, we look for MP signals in Whiting 1, traditionally considered a young GC. Using the Magellan telescope, we obtained low-resolution spectra within $\rm λλ= 3850-5500 Å$ for eight giants of Whiting 1. We measured the C and N abundances from the CN and CH spectral indices. C and N abundances have variations comparable with their measurement errors ($\sim0.1$ dex), suggesting that MPs are absent from Whiting 1. Combining these findings with literature studies, we propose a limit in the metallicity vs. cluster compactness index parameter space, which relatively clearly separates star clusters with/without MPs (GCs/open clusters). This limit is physically motivated. On a larger scale, the galactic environment determines cluster compactness and metallicity, leading to metal-rich, diffuse, old clusters formed ex situ. Our proposed limit also impacts our understanding of the formation of the Sagittarius dwarf galaxy: star clusters formed after the first starburst (age$\lesssim 8-10$ Gyr). These clusters are simple stellar populations because the enriched galactic environment is no longer suitable for MP formation.
description: 11 pages, 4 figures, SCPMA accepted
Additional file 2 of LCAT deficiency: a systematic review with the clinical and genetic description of Mexican kindred
Creators: name: Mehta, Roopa
name: Elías-López, Daniel
name: Martagón, Alexandro J.
name: Pérez-Méndez, Oscar A
name: Sánchez, Maria Luisa Ordóñez
name: Segura, Yayoi
name: Tusié, Maria Teresa
name: Aguilar-Salinas, Carlos A.
Publisher: name: figshare
Year: 2021
Subjects: subject: Medicine
subject: Genetics
subject: FOS: Biological sciences
subject: Biotechnology
subject: Science Policy

description: Additional file 2:
The Current Ability to Test Theories of Gravity with Black Hole Shadows
Creators: name: Mizuno, Yosuke
name: Younsi, Ziri
name: Fromm, Christian M.
name: Porth, Oliver
name: De Laurentis, Mariafelicia
name: Olivares, Hector
name: Falcke, Heino
name: Kramer, Michael
name: Rezzolla, Luciano
Publisher: name: arXiv
Year: 2018
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: Our Galactic Center, Sagittarius A* (Sgr A*), is believed to harbour a supermassive black hole (BH), as suggested by observations tracking individual orbiting stars. Upcoming sub-millimetre very-long-baseline-interferometry (VLBI) images of Sgr A* carried out by the Event-Horizon-Telescope Collaboration (EHTC) are expected to provide critical evidence for the existence of this supermassive BH. We assess our present ability to use EHTC images to determine if they correspond to a Kerr BH as predicted by Einstein's theory of general relativity (GR) or to a BH in alternative theories of gravity. To this end, we perform general-relativistic magnetohydrodynamical (GRMHD) simulations and use general-relativistic radiative transfer (GRRT) calculations to generate synthetic shadow images of a magnetised accretion flow onto a Kerr BH. In addition, and for the first time, we perform GRMHD simulations and GRRT calculations for a dilaton BH, which we take as a representative solution of an alternative theory of gravity. Adopting the VLBI configuration from the 2017 EHTC campaign, we find that it could be extremely difficult to distinguish between BHs from different theories of gravity, thus highlighting that great caution is needed when interpreting BH images as tests of GR.
description: Published in Nature Astronomy on 16.04.18 (including supplementary information); simulations at https://blackholecam.org/telling_bhs_apart/
Background and Scattered Light Subtraction in the High-Resolution Echelle Modes of the Space Telescope Imaging Spectrograph
Creators: name: Howk, J. Christopher
name: Sembach, Kenneth R.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present a simple, effective approach for estimating the on-order backgrounds of spectra taken with the highest-resolution modes of the Space Telescope Imaging Spectrograph (STIS) on-board the Hubble Space Telescope. Our scheme for determining the on-order background spectrum uses polynomial fits to the inter-order scattered light visible in the two-dimensional STIS MAMA images. We present a suite of high-resolution STIS spectra to demonstrate that our background subtraction routine produces the correct overall zero point, as judged by the small residual flux levels in the centers of strongly-saturated interstellar absorption lines. Although there are multiple sources of background light in STIS echelle mode data, this simple approach works very well for wavelengths longward of Lyman-alpha. At shorter wavelengths, the smaller order separation and generally lower signal-to-noise ratios of the data can reduce the effectiveness of our background estimation procedure. Slight artifacts in the background-subtracted spectrum can be seen in some cases, particularly at wavelengths <1300 Ang. Most of these are caused by echelle scattering of strong spectral features into the inter-order light. We discuss the limitations of high-resolution STIS data in light of the uncertainties associated with our background subtraction procedure. We compare our background-subtracted STIS spectra with GHRS Ech-A observations of the DA white dwarf G191-B2B and GHRS first-order G160M observations of the early-type star HD 218915. We find no significant differences between the GHRS data and the STIS data reduced with our method in either case.
description: To appear in The Astronomical Journal; 37 pages, including 2 embedded tables and 18 embedded figures. Version with high-resolution figures can be found at http://fuse.pha.jhu.edu/~howk/Papers/ . Software described in this paper is available to the general community; contact the authors for information
Additional file 1 of Distinct nitrogen isotopic compositions of healthy and cancerous tissue in mice brain and head&neck micro-biopsies
Creators: name: Straub, M.
name: Sigman, D. M.
name: Auderset, A.
name: Ollivier, J.
name: Petit, B.
name: Hinnenberg, B.
name: Rubach, F.
name: Oleynik, S.
name: Vozenin, M.-C.
name: Martínez-García, A.
Publisher: name: figshare
Year: 2021
Subjects: subject: Biochemistry
subject: Space Science
subject: Medicine
subject: Cell Biology
subject: Genetics
subject: FOS: Biological sciences
subject: Physiology
subject: Pharmacology
subject: Biotechnology
subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences
subject: Immunology
subject: FOS: Clinical medicine
subject: Cancer

description: Additional file 1: Figure SI-1. Illustration of a tumor mass formed by H454 tumors (T) in the striatum of the neural and adjacent tissue (TB = tumor bed). The healthy, normal neural tissue (NT) was sampled in the contralateral region, which is tumor-free. Figure SI-2. The left panel shows an illustration of the tumor mass formed by MEERL95 tumors (T = tumor) in the submandibular region. It infiltrates the adjacent healthy subcutaneous and muscular tissues (S=skin, SG = salivary gland, M = muscle). The right panel shows a 20-fold higher magnification of the margin (m). Infiltration of tumor cells (purple) into the stromal tissue (pink) forms an irregular margin (m). Intravascular tumor cell aggregates and smaller clusters of tumor cells are also found further away from the primary tumor in the subcutaneous zone (*). For our study, margin and tumor were sampled. Table SI-1. Isotopic measurements performed on the cell samples. At the bottom of the table, average values for reference standards and procedural oxidation blank are shown. Table SI-2. Isotopic measurements performed in April 2019. The data includes the Head&Neck data from mice 1, 2 and 3 and the brain tumor data from mice 1, 2 and 3. At the bottom of the table, values for reference standards and procedural oxidation blank are shown. Table SI-3. Isotopic measurements performed in September 2019. The data include the Head&Neck data from mice 4 and 5. At the bottom of the table values for reference standards and procedural oxidation blank are shown. Table SI-4. Isotopic measurements performed in November 2019. The data includes the brain tumor data from mice 4, 5, 6 and 7. At the bottom of the table, values for reference standards and procedural oxidation blank are shown. Table SI-5. Results of USGS65 measurements across the range of N contents of our tissue samples. Our results show no statistically significant difference in δ15N, indicating full conversion of the organic N during the oxidation step.
title: Édition TEI de la pièce Ploutos d’Aristophane (Ve siècle avant J.-C.), traduite par Charles Zévort (1816-1887), 1889
title: Edition in TEI format of the play Ploutos by Aristophanes (5th century BC), translated by Charles Zévort (1816-1887), 1889
Creators: name: Bastin-Hammou, Malika
name: Mandhouj, Nassim
name: Aristophane (C. 446 – C. 386 BC)
name: Charles Zévort (Traducteur)
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2024
Subjects: subject: TEI
subject: Traduction
subject: Aristophane
subject: français (langue)
subject: XIXe siècle
subject: TEI
subject: translation
subject: Aristophanes
subject: 19th century
subject: french
subject: Theater–Greece
subject: 19th century
subject: French language

description: La présente édition s’inscrit dans le cadre du projet Translatoscope de l'Université Grenoble Alpes, dédié à l'étude de l’histoire des traductions d’Aristophane. L’encodage du texte a été réalisé en suivant les recommandations de la Text Encoding Initiative (http://www.tei-c.org/Guidelines/P5/).
description: This edition is part of the Translatoscope project at Grenoble Alpes University, dedicated to the study of the history of translations of Aristophanes. The text has been encoded in accordance with the recommendations of the Text Encoding Initiative (http://www.tei-c.org/Guidelines/P5/).
Tests for Tau's Charged-Current Structure
Creators: name: Nelson, Charles A.
Publisher: name: arXiv
Year: 1994
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: The Lorentz structure of the tau lepton's charged-current can almost be completely determined by use of stage-two spin-correlation functions for the $\{ρ^{-},ρ^{+}\}$ and $\{a_1^{-},a_1^{+}\}$ decay modes It is possible to test for a ``(V-A) + something'' structure in the ${J^{Charged}}_{Lepton}$ current, so as to bound the scales $Λ$ for ``new physics" such as arising from tau weak magnetism, weak electricity, and/or second-class currents.
description: 17 pages, latex, no figures
Odd-degree rational characters and the order of rational elements in finite groups
Creators: name: Grittini, N.
Publisher: name: arXiv
Year: 2023
Subjects: subject: Group Theory (math.GR)
subject: FOS: Mathematics
subject: 20C15

description: We prove that, in a finite group, if every rational irreducible character has odd degree, then all rational elements are 2-elements, as it was originally conjectured by Tiep and Tong-Viet.
Additional file 3: of Assessing imprecision in Cochrane systematic reviews: a comparison of GRADE and Trial Sequential Analysis
Creators: name: Castellini, Greta
name: Bruschettini, Matteo
name: Gianola, Silvia
name: Gluud, Christian
name: Moja, Lorenzo
Publisher: name: figshare
Year: 2018
Subjects: subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: Science Policy

description: Logistic regressions results. (DOCX 273 kb)
RankME: Reliable Human Ratings for Natural Language Generation
Creators: name: Novikova, Jekaterina
name: Dušek, Ondřej
name: Rieser, Verena
Publisher: name: arXiv
Year: 2018
Subjects: subject: Computation and Language (cs.CL)
subject: FOS: Computer and information sciences

description: Human evaluation for natural language generation (NLG) often suffers from inconsistent user ratings. While previous research tends to attribute this problem to individual user preferences, we show that the quality of human judgements can also be improved by experimental design. We present a novel rank-based magnitude estimation method (RankME), which combines the use of continuous scales and relative assessments. We show that RankME significantly improves the reliability and consistency of human ratings compared to traditional evaluation methods. In addition, we show that it is possible to evaluate NLG systems according to multiple, distinct criteria, which is important for error analysis. Finally, we demonstrate that RankME, in combination with Bayesian estimation of system quality, is a cost-effective alternative for ranking multiple NLG systems.
description: Accepted to NAACL 2018 (The 2018 Conference of the North American Chapter of the Association for Computational Linguistics)
The Solar Wind Environment in Time
Creators: name: Pognan, Quentin
name: Garraffo, Cecilia
name: Cohen, Ofer
name: Drake, Jeremy J.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: We use magnetograms of 8 solar analogues of ages 30~Myr to 3.6~Gyr obtained from Zeeman Doppler Imaging (ZDI) and taken from the literature, together with two solar magnetograms, to drive magnetohydrodynamical (MHD) wind simulations and construct an evolutionary scenario of the solar wind environment and its angular momentum loss rate. With observed magnetograms of the radial field strength as the only variant in the wind model, we find that power law model fitted to the derived angular momentum loss rate against time, $t$, results in a spin down relation $Ω\propto t^{-0.51}$, for angular speed $Ω$, which is remarkably consistent with the well-established Skumanich law $Ω\propto t^{-0.5}$. We use the model wind conditions to estimate the magnetospheric standoff distances for an Earth-like test planet situated at 1~AU for each of the stellar cases, and to obtain trends of minimum and maximum wind ram pressure and average ram pressure in the solar system through time. The wind ram pressure declines with time as $\overline{P_{ram}}\propto t^{2/3}$, amounting to a factor of 50 or so over the present lifetime of the solar system.
description: 21 pages, 11 figures, accepted for publication in ApJ, 8th February 2018
Additional file 2: of Assessing imprecision in Cochrane systematic reviews: a comparison of GRADE and Trial Sequential Analysis
Creators: name: Castellini, Greta
name: Bruschettini, Matteo
name: Gianola, Silvia
name: Gluud, Christian
name: Moja, Lorenzo
Publisher: name: figshare
Year: 2018
Subjects: subject: Medicine
subject: Biotechnology
subject: Developmental Biology
subject: Science Policy
subject: 110309 Infectious Diseases
subject: FOS: Health sciences

description: Cochrane systematic reviews with general characteristics. (DOCX 24 kb)
title: ADCO, Comptes du Petit-Cîteaux (1477-1491) (11 H 1179), f. 00317
Creators: name: de la Côte d'Or, Archives départementales
name: Archives Départementales De La Côte D'Or
name: Petot, Frédérique
name: Projet CBMA
name: CBMA/CG21/F.PETOT/2019
name: Petot, Frédéric
name: Archives Départementales De La Côte-D'Or
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: comptes
subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris

description: Comptes du Petit-Cîteaux (1477-1491), Archives départementales de la Côte-d'Or, (11 H 1179). Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Comptes du Petit-Cîteaux (1477-1491), Archives départementales de la Côte-d'Or, (11 H 1179), f. 00317, 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
Discovery of a red and blue shifted iron disk line in the galactic jet source GRO J1655-40
Creators: name: Balucinska-Church, M.
name: Church, M. J.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We report the discovery of emission features in the X-ray spectrum of GRO J1655-40 obtained with RXTE during the observation of 1997, Feb 26. We have fitted the features firstly by two Gaussian lines which in four spectra analysed have average energies of 5.85 +/- 0.08 keV and 7.32 +/- 0.13 keV, strongly suggestive that these are the red and blue shifted wings of an iron disk line. These energies imply a velocity of ~0.33 c. The blue wing is less bright than in the calculated profiles of disk lines near a black hole subject to Doppler boosting, however known Fe absorption lines in GRO J1655-40 at energies between ~7 and 8 keV can reduce the apparent brightness of the blue wing. Secondly, we have fitted the spectra using the disk line model of Laor based on a full relativistic treatment plus an absorption line, and show that good fits are obtained. This gives a restframe energy of the disk line between 6.4 and 6.8 keV indicating that the line is iron K_alpha emission probably of significantly ionized material. The Laor model shows that the line originates in a region of the accretion disk extending from ~10 Schwarzschild radii from the black hole outwards. The line is direct evidence for the black hole nature of the compact object and is the first discovery of a highly red and blue shifted iron disk line in a Galactic source.
description: 5 pages, 5 ps figures, latex. MNRAS accepted (submitted 23rd August, 1999)
Additional file 5: of A facility-based study of womenâ satisfaction and perceived quality of reproductive and maternal health services in the Kenya output-based approach voucher program
Creators: name: Oyugi, Boniface
name: Urbanus Kioko
name: Kaboro, Stephen
name: Okumu, Clarice
name: Ogola-Munene, Sarah
name: Shaminder Kalsi
name: Thiani, Simon
name: Shadrack Gikonyo
name: Korir, Julius
name: Baltazar, Billy
name: Ranji, Moses
Publisher: name: figshare
Year: 2018
Subjects: subject: Biotechnology
subject: 59999 Environmental Sciences not elsewhere classified
subject: FOS: Earth and related environmental sciences
subject: Sociology
subject: FOS: Sociology
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: 80699 Information Systems not elsewhere classified
subject: FOS: Computer and information sciences
subject: 19999 Mathematical Sciences not elsewhere classified
subject: FOS: Mathematics

description: Figure S1. Pareto chart for the level of satisfaction of clients with the OBA services. (DOCX 17 kb)
A Nonperturbative, Schwinger-Dyson-Equation Analysis of Quark Masses and Mixings in a Model with QCD and Higgs Interactions
Creators: name: Smith, Lesley L.
name: Jain, Pankaj
name: McKay, Douglas W.
Publisher: name: arXiv
Year: 1994
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: The Landau gauge Schwinger-Dyson Equation for the quark self-energy is solved in the quenched ladder approximation for several cases of one- and two-quark-generations. The exchanges of Standard Model gluons and Higgs bosons are taken into account. It is found that Higgs boson exchange dominates the quark self-energy for sufficiently large input quark masses (>75 GeV), causing the running quark propagator mass to increase with energy-scale. The running of the quark mixing angles is also considered. No running of the quark mixing angles is found, to one part in a billion, for input quark masses up to and including 500 GeV.
description: 18 pages, LaTeX twice, 4 figures available upon request
Additional file 3 of HyperChIP: identification of hypervariable signals across ChIP-seq or ATAC-seq samples
Creators: name: Chen, Haojie
name: Tu, Shiqi
name: Yuan, Chongze
name: Tian, Feng
name: Zhang, Yijing
name: Sun, Yihua
name: Shao, Zhen
Publisher: name: figshare
Year: 2022
Subjects: subject: Genetics
subject: FOS: Biological sciences

description: Additional file 3: Table S1. Top 20 GO terms enriched from the genes linked with the significant proximal LVRs identified for the H3K27ac ChIP-seq data set. Table S2. Top 20 GO terms enriched from the genes linked with the significant proximal HVRs identified for the H3K27ac ChIP-seq data set. Table S3. Cancer types involved in the TCGA ATAC-seq data set. Note that in TCGA studies the abbreviation CESC refers to both cervical squamous cell carcinoma and endocervical adenocarcinoma, but all the 4 CESC patients in this data set belong in the former. Note also that the 18 ESCA patients in this data set consist of 12 ESSC (esophageal squamous cell carcinoma) and 6 ESAD (esophageal adenocarcinoma) cases, which belong in the SC and DIAD classes, respectively. SC, squamous cell carcinoma; DIAD, digestive adenocarcinoma.
Physics Prospects at the Hadron Colliders
Creators: name: Roy, D. P.
Publisher: name: arXiv
Year: 1994
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: I start with a brief introduction to the elementary particles and their interactions, Higgs mechanism and supersymmetry. The major physics objectives of the Tevatron and LHC colliders are identified. The status and prospects of the top quark, charged Higgs boson and superparticle searches are discussed in detail, while those of the neutral Higgs boson(s) are covered in a parallel talk by R.J.N. Phillips at this workshop.
description: 16 pages Latex + 15 figures (available on request)
DeepTSF: Codeless machine learning operations for time series forecasting
Creators: name: Pelekis, Sotiris
name: Karakolis, Evangelos
name: Pountridis, Theodosios
name: Kormpakis, George
name: Lampropoulos, George
name: Mouzakitis, Spiros
name: Askounis, Dimitris
Publisher: name: arXiv
Year: 2023
Subjects: subject: Machine Learning (cs.LG)
subject: Software Engineering (cs.SE)
subject: FOS: Computer and information sciences

description: This paper presents DeepTSF, a comprehensive machine learning operations (MLOps) framework aiming to innovate time series forecasting through workflow automation and codeless modeling. DeepTSF automates key aspects of the ML lifecycle, making it an ideal tool for data scientists and MLops engineers engaged in machine learning (ML) and deep learning (DL)-based forecasting. DeepTSF empowers users with a robust and user-friendly solution, while it is designed to seamlessly integrate with existing data analysis workflows, providing enhanced productivity and compatibility. The framework offers a front-end user interface (UI) suitable for data scientists, as well as other higher-level stakeholders, enabling comprehensive understanding through insightful visualizations and evaluation metrics. DeepTSF also prioritizes security through identity management and access authorization mechanisms. The application of DeepTSF in real-life use cases of the I-NERGY project has already proven DeepTSF's efficacy in DL-based load forecasting, showcasing its significant added value in the electrical power and energy systems domain.
The Ionization Source in the Nucleus of M84
Creators: name: Bower, G. A.
name: Green, R. F.
name: Quillen, A. C.
name: Danks, A.
name: Gull, T.
name: Hutchings, J.
name: Joseph, C.
name: Kaiser, M. E.
name: Weistrop, D.
name: Woodgate, B.
name: Malumuth, E. M.
name: Nelson, C.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We have obtained new Hubble Space Telescope (HST) observations of M84, a nearby massive elliptical galaxy whose nucleus contains a 1.5 X 10^9 Msun dark compact object, which presumably is a supermassive black hole. Our Space Telescope Imaging Spectrograph (STIS) spectrum provides the first clear detection of emission lines in the blue (e.g., [O II] 3727, Hbeta, and [O III] 4959, 5007), which arise from a compact region 0.28" across centered on the nucleus. Our Near Infrared Camera and Multi-Object Spectrometer (NICMOS) images exhibit the best view through the prominent dust lanes evident at optical wavelengths and provide a more accurate correction for the internal extinction. The relative fluxes of the emission lines we have detected in the blue together with those detected in the wavelength range 6295 - 6867 AA by Bower et al. (1998, ApJ, 492, L111) indicate that the gas at the nucleus is photoionized by a nonstellar process, instead of hot stars. Stellar absorption features from cool stars at the nucleus are very weak. We update the spectral energy distribution of the nuclear point source and find that although it is roughly flat in most bands, the optical to UV continuum is very red, similar to the spectral energy distribution of BL Lac. Thus, the nuclear point source seen in high-resolution optical images (Bower et al. 1997, ApJ, 483, L33) is not a star cluster but is instead a nonstellar source. Assuming isotropic emission from this source, we estimate that the ratio of bolometric luminosity to Eddington luminosity is 5 X 10^(-7). However, this could be underestimated if this source is a misaligned BL Lac object, which is a possibility suggested by the spectral energy distribution and the evidence of optical variability we describe.
description: 24 pages, 7 figures, accepted for publication in The Astrophysical Journal
Absolute Distances to Nearby Type Ia Supernovae via Light Curve Fitting Methods
Creators: name: Vinkó, J.
name: Ordasi, A.
name: Szalai, T.
name: Sárneczky, K.
name: Bányai, E.
name: Bíró, I. B.
name: Borkovits, T.
name: Hegedüs, T.
name: Hodosán, G.
name: Kelemen, J.
name: Klagyivik, P.
name: Kriskovics, L.
name: Kun, E.
name: Marion, G. H.
name: Marschalkó, G.
name: Molnár, L.
name: Nagy, A. P.
name: Pál, A.
name: Silverman, J. M.
name: Szakáts, R.
name: Szegedi-Elek, E.
name: Székely, P.
name: Szing, A.
name: Vida, K.
name: Wheeler, J. C.
Publisher: name: arXiv
Year: 2018
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: We present a comparative study of absolute distances to a sample of very nearby, bright Type Ia supernovae (SNe) derived from high cadence, high signal-to-noise, multi-band photometric data. Our sample consists of four SNe: 2012cg, 2012ht, 2013dy and 2014J. We present new homogeneous, high-cadence photometric data in Johnson-Cousins BVRI and Sloan g'r'i'z' bands taken from two sites (Piszkesteto and Baja, Hungary), and the light curves are analyzed with publicly available light curve fitters (MLCS2k2, SNooPy2 and SALT2.4). When comparing the best-fit parameters provided by the different codes, it is found that the distance moduli of moderately-reddened SNe Ia agree within ~0.2 mag, and the agreement is even better (< 0.1 mag) for the highest signal-to-noise BVRI data. For the highly-reddened SN~2014J the dispersion of the inferred distance moduli is slightly higher. These SN-based distances are in good agreement with the Cepheid distances to their host galaxies. We conclude that the current state-of-the-art light curve fitters for Type Ia SNe can provide consistent absolute distance moduli having less than ~0.1 -- 0.2 mag uncertainty for nearby SNe. Still, there is room for future improvements to reach the desired ~0.05 mag accuracy in the absolute distance modulus.
description: accepted for publication in PASP
title: Atlas des DOM. - La Réunion - Planches 11 et 12 : Le Passé : notice, page 2 "II. La Réunion de 1780 à 1815 (suite)"
Creators: name: Defos du Rau, Jean
name: Wanquet, Claude
name: France, Compagnie Des Indes Orientales
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2017
Subjects: histoire
organisation administrative
région administrative
café
production agricole
géographie historique
histoire coloniale
peuplement
colonisation
culture vivrière
démographie
histoire économique et sociale
politique démographique
recensement
répartition de la population
activité économique
esclavage
organisation sociale

description: Suite de la présentation de l'évolution politique et administrative de l'île de 1780 à 1815. Trois cartons représentent le découpage administratif de l'île en districts, cantons et sections de commune pour les périodes de 1790 à 1793, de 1794 à 1797 et de 1798 à 1808. Présente ensuite, pour la période de 1780 à 1815, le peuplement des populations dites "blanches", celles tenues en esclavage et celles libres de naissances ou affranchies. Un histogramme en barres donne la répartition par localité, sexe et âge de la population d'esclaves en 1779 sur neuf localités et un tableau donne le nombre d'habitants pour onze localités d'après les recensements partiels des années 1805-1808. Puis la vie économique est abordée, sont présentées les conditions générales et les productions agricoles.
description: Relation: http://www.nakala.fr/data/11280/0861029d
description: Relation: http://www.nakala.fr/data/11280/5577d7fb
description: Relation: http://www.nakala.fr/data/11280/ff9819a6
description: Coverage: La Réunion
description: Coverage: Archipel des Mascareignes
description: Coverage: Saint-Paul
description: Coverage: Saint-Benoît
description: Coverage: Saint-André
description: Coverage: Sainte-Suzanne
description: Coverage: Sainte-Marie
description: Coverage: Saint-Denis
description: Coverage: Saint-Louis
description: Coverage: Mascareigne
description: Coverage: Mascarin
description: Coverage: Sainte-Apolline
description: Coverage: Île Bourbon
description: Coverage: Repos-Laleu
description: Coverage: Rivière d'Abord
description: Temporal: start=1780; end=1815;
EXIST: A High Sensitivity Hard X-ray Imaging Sky Survey Mission for ISS
Creators: name: Grindlay, J.
name: Bildsten, L.
name: Chakrabarty, D.
name: Elvis, M.
name: Fabian, A.
name: Fiore, F.
name: Gehrels, N.
name: Hailey, C.
name: Harrison, F.
name: Hartmann, D.
name: Prince, T.
name: Ramsey, B.
name: Rothschild, R.
name: Skinner, G.
name: Woosley, S.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: A deep all-sky imaging hard x-ray survey and wide-field monitor is needed to extend soft (ROSAT) and medium (ABRIXAS2) x-ray surveys into the 10-100 keV band (and beyond) at comparable sensitivity (~0.05 mCrab). This would enable discovery and study of >3000 obscured AGN, which probably dominate the hard x-ray background; detailed study of spectra and variability of accreting black holes and a census of BHs in the Galaxy; Gamma-ray bursts and associated massive star formation (PopIII) at very high redshift and Soft Gamma-ray Repeaters throughout the Local Group; and a full galactic survey for obscured supernova remnants. The Energetic X-ray Imaging Survey Telescope (EXIST) is a proposed array of 8 x 1m^2 coded aperture telescopes fixed on the International Space Station (ISS) with 160deg x 40deg field of view which images the full sky each 90 min orbit. EXIST has been included in the most recent NASA Strategic Plan as a candidate mission for the next decade. An overview of the science goals and mission concept is presented.
description: 5 pages LaTeX. To appear in Proc. 5th Compton Symp. (M. McConnell, ed.; AIP Conf. Proc.)
A Simple Method for Computing the Non-Linear Mass Correlation Function with Implications for Stable Clustering
Creators: name: Caldwell, R. R.
name: Juszkiewicz, Roman
name: Steinhardt, Paul J.
name: Bouchet, Francois
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We propose a simple and accurate method for computing analytically the mass correlation function for cold dark matter and scale-free models that fits N-body simulations over a range that extends from the linear to the strongly non-linear regime. The method, based on the dynamical evolution of the pair conservation equation, relies on a universal relation between the pair-wise velocity and the smoothed correlation function valid for high and low density models, as derived empirically from N-body simulations. An intriguing alternative relation, based on the stable-clustering hypothesis, predicts a power-law behavior of the mass correlation function that disagrees with N-body simulations but conforms well to the observed galaxy correlation function if negligible bias is assumed. The method is a useful tool for rapidly exploring a wide span of models and, at the same time, raises new questions about large scale structure formation.
description: 10 pages, 3 figures
MPEC 2024-K92 : DAILY ORBIT UPDATE (2024 May 24)
Creators: name: Minor Planet Center Staff
Publisher: name: The Minor Planet Center
Year: 2024
Subjects: subject: Small Solar System bodies
valueUri: http://astrothesaurus.org/uat/1469

description: The Minor Planet Electronic Circulars contain information on unusual minor planets, routine data on comets and natural satellites, and occasional editorial announcements.  They are published on behalf of Division F of the International Astronomical Union by the Minor Planet Center, Smithsonian Astrophysical Observatory, Cambridge, MA 02138, U.S.A.
The Evolutionary Status of SS433
Creators: name: King, Andrew R.
name: Taam, Ronald E.
name: Begelman, Mitchell C.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We consider possible evolutionary models for SS 433. We assume that common-envelope evolution is avoided if radiation pressure is able to expel most of a super-Eddington accretion flow from a region smaller than the accretor's Roche lobe. This condition is satisfied, at least initially, for largely radiative donors with masses in the range 4-12 solar masses. For donors more massive than about 5 solar masses, moderate mass ratios q = M_2/M_1 > 1 are indicated, thus tending to favor black-hole accretors. For lower mass donors, evolutionary considerations do not distinguish between a neutron star or black hole accretor. In all cases the mass transfer (and mass loss) rates are much larger than the likely mass-loss rate in the precessing jets. Almost all of the transferred mass is expelled at radii considerably larger than the jet acceleration region, producing the "stationary" H-alpha line, the infrared luminosity, and accounting for the low X-ray luminosity.
description: 13 pages, Astrophysical Journal Letters, accepted
g-factor calculations from the generalized seniority approach
Creators: name: Maheshwari, Bhoomika
name: Jain, Ashok Kumar
Publisher: name: arXiv
Year: 2018
Subjects: subject: Nuclear Theory (nucl-th)
subject: FOS: Physical sciences

description: The generalized seniority approach proposed by us to understand the B(E1)/B(E2)/B(E3) properties of semi-magic nuclei has been widely successful in the explanation of the same and has led to an expansion in the scope of seniority isomers. In the present paper, we apply the generalized seniority scheme to understand the behavior of g-factors in semi-magic nuclei. We find that the magnetic moment and the gfactors do show a particle number independent behavior as expected and the understanding is consistent with the explanation of transition probabilities.
Additional file 6: of Functional annotation and distribution overview of RNA families in 27Â Streptococcus agalactiae genomes
Creators: name: Wolf, Ivan
name: Paschoal, Alexandre
name: Quiroga, Cecilia
name: Domingues, Douglas
name: RogĂŠrio De Souza
name: Pretto-Giordano, Lucienne
name: Laurival Vilas-Boas
Publisher: name: figshare
Year: 2018
Subjects: subject: Space Science
subject: Medicine
subject: Microbiology
subject: FOS: Biological sciences
subject: Genetics
subject: Molecular Biology
subject: 80699 Information Systems not elsewhere classified
subject: FOS: Computer and information sciences
subject: 110309 Infectious Diseases
subject: FOS: Health sciences
subject: 60506 Virology

description: Plots of Features vs Cluster Assignments obtained on Weka by EM algorithm. (PDF 16 kb)
El fin de la Guerra Civil española y el exilio republicano: visiones y prácticas de la sociedad argentina a través de la prensa. El caso de Mar del Plata, 1939
Creators: name: Bocanegra Barbecho, Lidia
Publisher: name: Universitat de Lleida
Year: 2012
Subjects: Argentina
Mar del Plata
Exilio republicano
Guerra Civil española
Prensa
Republican exile
Spanish Civil War

description: Analysis of the influence that caused the Spanish Civil War and the
republican exile into the Argentinean society. The main methodology has been the use of the interviews to exiles and the analysis of the Argentinean press from Buenos Aires and Mar del Plata
description: Fecha de defensa: 16-06-2006