cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Evidence for Halo Kinematics among Cool Carbon-Rich Dwarfs
Creators: name: Farihi, J.
name: Arendt, A. R.
name: Machado, H. S.
name: Whitehouse, L. J.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: This paper reports preliminary yet compelling kinematical inferences for N ~ 600 carbon-rich dwarf stars that demonstrate around 30% to 60% are members of the Galactic halo. The study uses a spectroscopically and non-kinematically selected sample of stars from the SDSS, and cross-correlates these data with three proper motion catalogs based on Gaia DR1 astrometry to generate estimates of their 3-D space velocities. The fraction of stars with halo-like kinematics is roughly 30% for distances based on a limited number of parallax measurements, with the remainder dominated by the thick disk, but close to 60% of the sample lie below an old, metal-poor disk isochrone in reduced proper motion. An ancient population is consistent with an extrinsic origin for C/O >1 in cool dwarfs, where a fixed mass of carbon pollution more readily surmounts lower oxygen abundances, and with a lack of detectable ultraviolet-blue flux from younger white dwarf companions. For an initial stellar mass function that favors low-mass stars as in the Galactic disk, the dC stars are likely to be the dominant source of carbon-enhanced, metal-poor stars in the Galaxy.
description: 7 pages, 1 table, and 3 figures. Accepted to MNRAS
A Model for Solid $^3$He: II
Creators: name: Dubois, J.
name: Kumar, P.
Publisher: name: arXiv
Year: 1994
Subjects: subject: Condensed Matter (cond-mat)
subject: FOS: Physical sciences

description: We propose a simple Ginzburg-Landau free energy to describe the magnetic phase transition in solid $^3$He. The free energy is analyzed with due consideration of the hard first order transitions at low magnetic fields. The resulting phase diagram contains all of the important features of the experimentally observed ph ase diagram. The free energy also yields a critical field at which the transition from the disordered state to the high field state changes from a first order to a second order one.
description: This paper has been accepted for publication in Journal of Low Temperature Physics. Use regular Tex, with the D. Eardley version of Macros called jnl.tex. 10 pages, 4 figs available from dubois@phys.ufl.edu
Supplementary data for "The diagnostic odyssey in children and adolescents with X-linked hypophosphataemia: population-based, case-control study"
Creators: name: Boardman-Pretty, Freya
name: Clift, Ashley Kieran
name: Mahon, Hadley
name: Sawoky, Nadine
name: Mughal, M. Zulf
Publisher: name: figshare
Year: 2024
Subjects: classificationCode: 429999
subject: Other health sciences not elsewhere classified

description: This study explored the recording of clinical features and the diagnostic odyssey of children and adolescents with X-linked hypophosphataemia in primary care electronic healthcare records in the United Kingdom.
The Space Missions WAXS/WFXT and SWIFT: New Targets for the VLT
Creators: name: Chincarini, Guido
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: At OAB we were, during the year 1998, deeply involved in planning two important space missions for which very large ground based telescopes, VLT in particular, would play a very large and important role in the optical followup. The study of the first mission, Wide Angle X-ray Survey using a Wide Field X-ray Telescope, was coordinated by the Observatory of Brera, involved mainly Italian industries and resulted in a proposal to the Italian Space Agency under the Small Satellite Program. The second mission, SWIFT, has been coordinated and directed by the Goddard Space Flight Center and resulted in the submission of a proposal to NASA under the MIDEX program. The science goal of this mission is the detection and study of the Gamma-ray bursts.
description: 6 pages, including 1 figure, LaTex2e. To be published in the Proceedings of the ``VLT Opening Symposium'', Antofagasta (Chile), 1-4 March 1999
Effects of Next-Nearest-Neighbor Hopping on the Hole Motion in an Antiferromagnetic Background
Creators: name: Schiller, Avraham
name: Kumar, Pradeep
name: Strack, Rainer
name: Vollhardt, Dieter
Publisher: name: arXiv
Year: 1994
Subjects: subject: Condensed Matter (cond-mat)
subject: FOS: Physical sciences

description: In this paper we study the effect of next-nearest-neighbor hopping on the dynamics of a single hole in an antiferromagnetic (Néel) background. In the framework of large dimensions the Green function of a hole can be obtained exactly. The exact density of states of a hole is thus calculated in large dimensions and on a Bethe lattice with large coordination number. We suggest a physically motivated generalization to finite dimensions (e.g., 2 and 3). In $d=2$ we present also the momentum dependent spectral function. With varying degree, depending on the underlying lattice involved, the discrete spectrum for holes is replaced by a continuum background and a few resonances at the low energy end. The latter are the remanents of the bound states of the $t-J$ model. Their behavior is still largely governed by the parameters $t$ and $J$. The continuum excitations are more sensitive to the energy scales $t$ and $t_1$.
description: To appear in Phys. Rev. B, Revtex, 23 pages, 10 figures available on request from avraham@phys.ufl.edu
Additional file 3: of Evolutionarily conserved partial gene duplication in the Triticeae tribe of grasses confers pathogen resistance
Creators: name: Jeyaraman Rajaraman
name: Douchkov, Dimitar
name: Lück, Stefanie
name: Hensel, Götz
name: Nowara, Daniela
name: Pogoda, Maria
name: Rutten, Twan
name: Meitzel, Tobias
name: Brassac, Jonathan
name: Höfle, Caroline
name: Hückelhoven, Ralph
name: Klinkenberg, Jörn
name: Trujillo, Marco
name: Bauer, Eva
name: Schmutzer, Thomas
name: Himmelbach, Axel
name: Mascher, Martin
name: Lazzari, Barbara
name: Stein, Nils
name: Kumlehn, Jochen
name: Schweizer, Patrick
Publisher: name: figshare
Year: 2018
Subjects: subject: Biochemistry
subject: Space Science
subject: Microbiology
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Evolutionary Biology
subject: Ecology
subject: 69999 Biological Sciences not elsewhere classified
subject: 19999 Mathematical Sciences not elsewhere classified
subject: FOS: Mathematics
subject: Developmental Biology
subject: 110309 Infectious Diseases
subject: FOS: Health sciences

description: Methods S1. Detailed description of materials and methods used in this study. (PDF 183 kb)
Additional file 1: of Clinical signs and symptoms in a joint model of four disease activity parameters in juvenile dermatomyositis: a prospective, longitudinal, multicenter cohort study
Creators: name: E. Van Dijkhuizen
name: Iorio, Maria De
name: Wedderburn, Lucy
name: Deakin, Claire
Publisher: name: figshare
Year: 2018
Subjects: subject: Medicine
subject: Genetics
subject: FOS: Biological sciences
subject: Biotechnology
subject: 69999 Biological Sciences not elsewhere classified
subject: 80699 Information Systems not elsewhere classified
subject: FOS: Computer and information sciences
subject: 19999 Mathematical Sciences not elsewhere classified
subject: FOS: Mathematics
subject: Developmental Biology
subject: Cancer
subject: 110309 Infectious Diseases
subject: FOS: Health sciences
subject: Computational Biology

description: List of available covariates. (DOCX 14 kb)
title: ADCO, Huitième cartulaire de Saint-Étienne de Dijon (1661-1667), Cart. 31 (G 135), 549 folios, f. 0175
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: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris
subject: Corpus Burgundiae Medii Aevi
subject: Chartes de la Bourgogne du Moyen Âge
subject: cartulaire

description: Huitième cartulaire de Saint-Étienne de Dijon (1661-1667), Archives départementales de la Côte-d'Or, Cart. 31 (G 135), 549 folios, f. 0175, Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Huitième cartulaire de Saint-Étienne de Dijon (1661-1667), Archives départementales de la Côte-d'Or, Cart. 31 (G 135), 549 folios, f. 0175, in Projet CBMA - Corpus Burgundiae Medii Aevi [Ressource en ligne], https://manuscrits.cbma-project.eu/
description: Provenance: abbaye Saint-Étienne de Dijon
description: Provenance: http://www.wikidata.org/entity/Q15945019
A 1.4 GHz radio continuum and polarization survey at medium Galactic latitudes: II. First section
Creators: name: Uyaniker, B.
name: Fuerst, E.
name: Reich, W.
name: Reich, P.
name: Wielebinski, R.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present the first section of a radio continuum and polarization survey at medium Galactic latitudes carried out with the Effelsberg 100-m telescope at 1.4 GHz. Four large fields have been observed, which all together cover an area of about 1100 square degree. The rms-sensitivity is about 15 mK TB (about 7 mJy/beam area) in total intensity and is limited by confusion. A sensitivity of 8 mK TB is obtained in linear polarization. The angular resolution of the observations is 9.35 arcminute. The maps in total intensity and linear polarization have been absolutely calibrated by low resolution data where available. Significant linear polarization is seen in all the maps. In general, the intensity fluctuations measured in linear polarization are not correlated with total intensity structures. Areas of high polarization of some degrees extent are seen, again with no apparent corresponding total intensity feature. Modulation of polarized background emission by spatially varying Faraday rotation seems the most likely explanation. Quite unexpected is the detection of filamentary and ring-like depolarization structures in the direction of the anticentre region, whose extents are up to about 3 degree.
description: Latex2 document, 17 pages, 14 figures. Accepted for publication in Astronomy and Astrophysics Supp. Ser
title: 02_1530
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/
Hyper- and hybrid nonlocality
Creators: name: Li, Yanna
name: Gessner, Manuel
name: Li, Weidong
name: Smerzi, Augusto
Publisher: name: arXiv
Year: 2018
Subjects: subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: The controlled generation and identification of quantum correlations, usually encoded in either qubits or continuous degrees of freedom, builds the foundation of quantum information science. Recently, more sophisticated approaches, involving a combination of two distinct degrees of freedom have been proposed to improve on the traditional strategies. Hyperentanglement describes simultaneous entanglement in more than one distinct degree of freedom, whereas hybrid entanglement refers to entanglement shared between a discrete and a continuous degree of freedom. In this work we propose a scheme that allows to combine the two approaches, and to extend them to the strongest form of quantum correlations. Specifically, we show how two identical, initially separated particles can be manipulated to produce Bell nonlocality among their spins, among their momenta, as well as across their spins and momenta. We discuss possible experimental realizations with atomic and photonic systems.
description: 6 pages, 3 figures
Albertosaurus lancensis
Creators: name: Russell, Dale A.
Publisher: name: National Museum of Natural Sciences, Publications in Palaeontology, No. 1
Year: 1970
Subjects: Biodiversity
Taxonomy
Animalia
Chordata
Reptilia
Dinosauria
Tyrannosauridae
Albertosaurus
Albertosaurus lancensis

description: Albertosaurus lancensis (Gilmore)
Gilmore (1946) has described the skull of a small carnivorous dinosaur from the Lance Formation of eastern Montana. The skull is quite different from that of Tyrannosaurus and Gilmore founded a new species on it, correctly referring it to
Gorgosaurus (= Albertosaurus).
Although the skull is only half as long as that of a fully grown A. libratus, the sutures between the bones of the skull roof are tightly interlocking, and some have been obscured through intergrowth; the supraoccipital alae of the parietals are well developed, and a clearly formed tuberosity is present on the ventral border of the jugal (Gilmore 1946). The opposite conditions prevail in the skull of AMNH 5664, a specimen of A. libratus of comparable size. The skull of A. lancensis is therefore probably from a fully grown individual, and its small size may be characteristic of the species.
Albertosaurus lancensis further differs from A. libratus and A. sarcophagus (AMNH 5222) in that the frontals meet on the midline throughout their entire length, while in the latter two species these elements are separated anteriorly by a small wedge of bone from the nasals. The frontals are not so deeply cleft above the orbits as is the case in A. libratus and A. sarcophagus. Gilmore (1946: 6) suggested that the prefrontal may be rather well exposed on the skull roof, unlike in the more ancient species of the genus. Otherwise the skulls of the three forms are quite similar.
description: Published as part of Russell, Dale A., 1970, Tyrannosaurs from the Late Cretaceous of western Canada, Ottawa :National Museum of Natural Sciences, Publications in Palaeontology, No. 1 on page 20, DOI: 10.5281/zenodo.1040973
Giant Outbursts of Luminous Blue Variables and the Formation of the Homunculus Nebula Around eta Carinae
Creators: name: Langer, Norbert
name: Garcia-Segura, Guillermo
name: Mac Low, Mordecai-Mark
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: The observed giant outbursts of Luminous Blue Variables (LBVs) may occur when these massive stars approach their Eddington limits. When this happens, they must reach a point where the centrifugal force and the radiative acceleration cancel out gravity at the equator. We call this the Omega-limit. When stars are close to the Omega-limit, strong non-spherical mass loss should occur. This suggests a scenario where a slow and very dense wind, strongly confined to the equatorial plane, is followed by a fast and almost spherical wind. We compute two-dimensional hydrodynamic models of the evolution of the nebula formed from such interacting winds, using parameters consistent with the outburst of eta Carinae in the last century. This outburst gave birth to the Homunculus, the hourglass-shaped inner part of a highly structured circumstellar nebula. Assuming the star was very close to the Omega-limit during outburst, our models produce gas distributions that strongly resemble the Homunculus on large and small scale. This supports the general conjecture that giant outbursts in LBVs occur when they approach the Eddington limit. Our models constrains the average mass loss rate since the outburst to values smaller than the present-day mass loss rate and suggest that eta Car is approaching another outburst. Our models imply that the occurrence of giant LBV outbursts depends on the initial stellar rotation rate, and that the initial angular momentum is as important to the evolution of very massive stars as their initial mass or metallicity.
description: Accepted to ApJ Letters, 11 pages, three GIF figures, original color postscript figures at http://www.mpia-hd.mpg.de/theory/maclow/papers/eta/
Cancer nucleus Linnaeus, 1758, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1758
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Malacostraca
Decapoda
Cancridae
Cancer
Cancer nucleus

description: Cancer nucleus [spec. nov.]
C. brachyurus, thorace laevi globoso: antice utrinque unidentato, postice rostroque bidentato.
Habitat in M. Mediterraneo ad littora Barbariae. E. Brander.
Statura C. craniolaris, magnitudo glandis, color flavus. Thorax pone rostrum utrinque dente unico, & ad postica thoracis margo obsolete bidentatus, at supra pedes posticos dens validior conicus. Cauda glaberrima. Femora antica punctis eminentibus adspersa. Ungues acuti.
description: Published as part of Linnaeus, Carolus, 1758, Systema Naturae per regna tria naturae: secundum classes, ordines, genera, species, cum characteribus, differentiis, synonymis, locis, Stockholm :Laurentius Salvius on page 627, DOI: 10.5962/bhl.title.542, http://zenodo.org/record/3922206
Power Density Spectra of Gamma-Ray Bursts in the Internal Shock Model
Creators: name: Panaitescu, A.
name: Spada, M.
name: Meszaros, P.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We simulate Gamma-Ray Bursts arising from internal shocks in relativistic winds, calculate their power density spectrum (PDS), and identify the factors to which the PDS is most sensitive: the wind ejection features, which determine the wind dynamics and its optical thickness, and the energy release parameters, which give the pulse 50-300 keV radiative efficiency. For certain combinations of ejection features and wind parameters the resulting PDS exhibits the features observed in real bursts. We found that the upper limit on the efficiency of conversion of wind kinetic energy into 50-300 keV photons is $\sim$ 1%. Winds with a modulated Lorentz factor distribution of the ejecta yield PDSs in accord with current observations and have efficiencies closer to $10^{-3}$, while winds with a random, uniform Lorentz factor ejection must be optically thick to the short duration pulses to produce correct PDSs, and have an overall efficiency around $10^{-4}$.
description: 6 pages, 4 figures, Latex, submitted to The Astrophysical Journal (05/04/99)
Additional file 1: of European Reference Network For Rare Vascular Diseases (VASCERN) Outcome Measures For Hereditary Haemorrhagic Telangiectasia (HHT)
Creators: name: Shovlin, Claire
name: Buscarini, Elisabetta
name: Kjeldsen, Anette
name: Mager, Hans
name: Sabba, Carlo
name: Droege, Freya
name: Geisthoff, Urban
name: Ugolini, Sara
name: Dupuis-Girod, Sophie
Publisher: name: figshare
Year: 2018
Subjects: subject: Biochemistry
subject: Medicine
subject: Physiology
subject: FOS: Biological sciences
subject: Pharmacology
subject: Sociology
subject: FOS: Sociology
subject: 19999 Mathematical Sciences not elsewhere classified
subject: FOS: Mathematics
subject: 110309 Infectious Diseases
subject: FOS: Health sciences
subject: Computational Biology

description: Methodological notes. (DOCX 28 kb)
Hard-core Final State Interaction Effects in Deep Inelastic Scattering
Creators: name: Besprosvany, Jaime
name: Gurvitz, S. A.
Publisher: name: arXiv
Year: 1994
Subjects: subject: Condensed Matter (cond-mat)
subject: Nuclear Theory (nucl-th)
subject: FOS: Physical sciences

description: Hard-core final state interaction effects in the response function are investigated in the asymptotic limit of momentum transfer q->Infinity. A new treatment of the response is presented, which displays the relevant scattering contribution. A modification of the otherwise expected free response is obtained for Fermi and Bose systems and smearing of the condensate peak is shown in this limit. A comparison with other treatments of final state interactions is made.
description: 13 pages, in RevTex. To be published in Physics Letters A. Figures can be obtained from ftbespro@weizmann.weizmann.ac.il
title: ADCO, Boursier de Cîteaux : comptes (1489-1493) (11 H 1166), f. 00513
Creators: name: de la Côte-d'Or, Archives départementales
name: Petot, Frédéric
name: Archives Départementales De La Côte-D'Or
name: Petot, Frédérique
name: Projet CBMA
name: CBMA/CG21/F.PETOT/2019
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2020
Subjects: subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris
subject: comptes
subject: Corpus Burgundiae Medii Aevi
subject: Chartes de la Bourgogne du Moyen Âge

description: Boursier de Cîteaux : comptes (1489-1493), Archives départementales de la Côte-d'Or, (11 H 1166). Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Boursier de Cîteaux : comptes (1489-1493), Archives départementales de la Côte-d'Or, (11 H 1166), f. 00513, in Projet CBMA - Corpus Burgundiae Medii Aevi \[Ressource en ligne\], https:// manuscrits.cbma-project.eu/
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
description: Provenance: abbaye de Cîteaux
Near-Infrared Spectroscopy of Molecular Hydrogen Emission in Four Reflection Nebulae: NGC 1333, NGC 2023, NGC 2068, and NGC 7023
Creators: name: Martini, Paul
name: Sellgren, K.
name: DePoy, D. L.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present near-infrared spectroscopy of fluorescent molecular hydrogen (H_2) emission from NGC 1333, NGC 2023, NGC 2068, and NGC 7023 and derive the physical properties of the molecular material in these reflection nebulae. Our observations of NGC 2023 and NGC 7023 and the physical parameters we derive for these nebulae are in good agreement with previous studies. Both NGC 1333 and NGC 2068 have no previously-published analysis of near-infrared spectra. Our study reveals that the rotational-vibrational states of molecular hydrogen in NGC 1333 are populated quite differently from NGC 2023 and NGC 7023. We determine that the relatively weak UV field illuminating NGC 1333 is the primary cause of the difference. Further, we find that the density of the emitting material in NGC 1333 is of much lower density, with n ~ 10^2 - 10^4 cm^-3. NGC 2068 has molecular hydrogen line ratios more similar to those of NGC 7023 and NGC 2023. Our model fits to this nebula show that the bright, H_2-emitting material may have a density as high as n ~ 10^5 cm^-3, similar to what we find for NGC 2023 and NGC 7023. Our spectra of NGC 2023 and NGC 7023 show significant changes in both the near-infrared continuum and H_2 intensity along the slit and offsets between the peaks of the H_2 and continuum emission. We find that these brightness changes may correspond to real changes in the density and temperatures of the emitting region, although uncertainties in the total column of emitting material along a given line of sight complicates the interpretation. The spatial difference in the peak of the H_2 and near-infrared continuum peaks in NGC 2023 and NGC 7023 shows that the near-infrared continuum is due to a material which can survive closer to the star than H_2 can.
description: Submitted for publication in ApJ. 34 pages including 12 embedded postscript figures. Also available at http://www.astronomy.ohio-state.edu/~martini/pubs
Imaginary potential in strongly coupled $\mathcal{N}=4$ SYM plasma in a magnetic field
Creators: name: Zhang, Zi-qiang
name: Hou, De-fu
Publisher: name: arXiv
Year: 2018
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We study the effect of a constant magnetic field on the imaginary part of a quarkonia potential in a strongly-coupled $\mathcal{N}=4$ SYM plasma. We consider the pair axis to be aligned perpendicularly and parallel to the magnetic field, respectively. For both cases, we find that the presence of the magnetic field tends to enhance the imaginary potential thus decreasing the the thermal width. In addition, the magnetic field has a stronger effect on the imaginary potential when the pair axis is perpendicular to the magnetic field rather than parallel.
description: 10 pages, 5 figures
Additional file 6 of Characterising sex differences of autosomal DNA methylation in whole blood using the Illumina EPIC array
Creators: name: Grant, Olivia A.
name: Wang, Yucheng
name: Kumari, Meena
name: Zabet, Nicolae Radu
name: Schalkwyk, Leonard
Publisher: name: figshare
Year: 2022
Subjects: subject: Genetics
subject: FOS: Biological sciences

description: Additional file 6. Figure S1: (A) QQ plot and lambda values (discovery data) distribution of the adjusted p values against the null distribution for EWAS of sex in the understanding society cohort. Genomic inflation lambda score is indicated in the QQ plot to indicate statistical inflation of p values. (B) Boxplots of estimated whole blood cell type proportions for males (orange) and females (blue) in the discovery data set, estimated using the estimateCellCounts function from bigmelon. We performed a Mann-Whitney U test (p value: n.s. 0.05, *p value < 0.05, **< 0.01 and ***< 0.001). (C) QQ plot and lambda values (validation data) distribution of the adjusted p values against the null distribution for EWAS of sex in the understanding society cohort. Genomic inflation lambda score is indicated in the QQ plot to indicate statistical inflation of p values. (D) Boxplots of estimated whole blood cell type proportions for males (orange) and females (blue) in the validation data set, estimated using the estimateCellCounts function from bigmelon. We performed a Mann–Whitney U test (p value: n.s. 0.05, *p value < 0.05, **< 0.01 and ***< 0.001). (E) Venn diagram showing overlap of differentially methylated positions identified in our validation and discovery data set before and after filtering of the list of saDMPs.
Analytical Approximations for Calculating the Escape and Absorption of Radiation in Clumpy Dusty Environments
Creators: name: Varosi, Frank
name: Dwek, Eli
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present analytical approximations for calculating the scattering, absorption and escape of nonionizing photons from a spherically symmetric two-phase clumpy medium, with either a central point source of isotropic radiation, a uniform distribution of isotropic emitters, or uniformly illuminated by external sources. The analytical approximations are based on the mega-grains model of two-phase clumpy media, as proposed by Hobson & Padman, combined with escape and absorption probability formulae for homogeneous media. The accuracy of the approximations is examined by comparison with 3D Monte Carlo simulations of radiative transfer, including multiple scattering. Our studies show that the combined mega-grains and escape/absorption probability formulae provide a good approximation of the escaping and absorbed radiation fractions for a wide range of parameters characterizing the medium. A realistic test is performed by modeling the absorption of a starlike source of radiation by interstellar dust in a clumpy medium, and by calculating the resulting equilibrium dust temperatures and infrared emission spectrum of both the clumps and the interclump medium. In particular, we find that the temperature of dust in clumps is lower than in the interclump medium if clumps are optically thick. Comparison with Monte Carlo simulations of radiative transfer in the same environment shows that the analytic model yields a good approximation of dust temperatures and the emerging UV to FIR spectrum of radiation for all three types of source distributions mentioned above. Our analytical model provides a numerically expedient way to estimate radiative transfer in a variety of interstellar conditions and can be applied to a wide range of astrophysical environments, from star forming regions to starburst galaxies.
description: 55 pages, 27 figures. ApJ 523 (1999), in press. Corrected equations and text so as to be same as ApJ version
title: ADCO, Grènetier de Cîteaux : comptes (1499-1503) (11 H 1173), f. 00756
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
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2020
Subjects: subject: comptes
subject: Corpus Burgundiae Medii Aevi
subject: Chartes de la Bourgogne du Moyen Âge
subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris

description: Grènetier de Cîteaux : comptes (1499-1503), Archives départementales de la Côte-d'Or, (11 H 1173). Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Grènetier de Cîteaux : comptes (1499-1503), Archives départementales de la Côte-d'Or, (11 H 1173), f. 00756, 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
Excitation mechanism of OI lines in Herbig Ae/Be stars
Creators: name: Mathew, Blesson
name: Manoj, P.
name: Narang, Mayank
name: Banerjee, D. P. K.
name: Nayak, Pratheeksha
name: Muneer, S.
name: Vig, S.
name: S., Pramod Kumar
name: T., Paul K.
name: Maheswar, G.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: We have investigated the role of a few prominent excitation mechanisms viz. collisional excitation, recombination, continuum fluorescence and Lyman beta fluorescence on the OI line spectra in Herbig Ae/Be stars. The aim is to understand which of them is the central mechanism that explains the observed OI line strengths. The study is based on an analysis of the observed optical spectra of 62 Herbig Ae/Be stars and near-infrared spectra of 17 Herbig Ae/Be stars. The strong correlation observed between the line fluxes of OI $λ$8446 and OI $λ$11287, as well as a high positive correlation between the line strengths of OI $λ$8446 and H$α$ suggest that Lyman beta fluorescence is the dominant excitation mechanism for the formation of OI emission lines in Herbig Ae/Be stars. Further, from an analysis of the emission line fluxes of OI $λλ$7774, 8446, and comparing the line ratios with those predicted by theoretical models, we assessed the contribution of collisional excitation in the formation of OI emission lines.
description: 13 pages, 2 tables, 6 figures, accepted for publication in ApJ
Charge Dynamics in the Planar t-J Model
Creators: name: Jaklic, J.
name: Prelovsek, P.
Publisher: name: arXiv
Year: 1994
Subjects: subject: Condensed Matter (cond-mat)
subject: FOS: Physical sciences

description: The finite-temperature optical conductivity $σ(ω)$ in the planar $t-J$ model is analysed using recently introduced numerical method based on the Lanczos diagonalization of small systems (up to 20 sites), as well as by analytical approaches, including the method of frequency moments and the retraceable-path approximation. Results for a dynamical mobility of a single hole at elevated temperatures $T>t$ reveal a Gaussian-like $μ(ω)$ spectra, however with a nonanalytical behavior at low $ω$. In the single hole response a difference between the ferromagnetic (J=0) and the antiferromagnetic ($J>0$) polaron shows up at $TT^*\ge 0.1~t$. $σ(ω)$ spectra show a non-Drude falloff at large frequencies. In particular for `optimum' doping $n_h \sim 0.2$ we obtain in the low-$ω,T$ regime the relaxation rate $τ^{-1} \sim 0.6 (ω+ξT)$ with $ξ\sim 3$, being consistent with the marginal Fermi liquid concept and experiments. Within the same regime we reproduce the nearly linear variation of dc resistivity $ρ$ with $T$. This behavior is weakly dependent on $J$, provided that $J
description: 21 pages of text plus 17 figures, postscript
Halometry from Astrometry
Creators: name: Van Tilburg, Ken
name: Taki, Anna-Maria
name: Weiner, Neal
Publisher: name: arXiv
Year: 2018
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: Astrophysics of Galaxies (astro-ph.GA)
subject: Instrumentation and Methods for Astrophysics (astro-ph.IM)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: Halometry---mapping out the spectrum, location, and kinematics of nonluminous structures inside the Galactic halo---can be realized via variable weak gravitational lensing of the apparent motions of stars and other luminous background sources. Modern astrometric surveys provide unprecedented positional precision along with a leap in the number of cataloged objects. Astrometry thus offers a new and sensitive probe of collapsed dark matter structures over a wide mass range, from one millionth to several million solar masses. It opens up a window into the spectrum of primordial curvature fluctuations with comoving wavenumbers between $5~\text{Mpc}^{-1}$ and $10^5~\text{Mpc}^{-1}$, scales hitherto poorly constrained. We outline detection strategies based on three classes of observables---multi-blips, templates, and correlations---that take advantage of correlated effects in the motion of many background light sources that are produced through time-domain gravitational lensing. While existing techniques based on single-source observables such as outliers and mono-blips are best suited for point-like lens targets, our methods offer parametric improvements for extended lens targets such as dark matter subhalos. Multi-blip lensing events may also unveil the existence, location, and mass of planets in the outer reaches of the Solar System, where they would likely have escaped detection by direct imaging.
description: 44 pages, 10 figures
Cancer lactatus Linnaeus, 1758, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1758
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Malacostraca
Decapoda
Cancridae
Cancer
Cancer lactatus

description: Cancer lactatus [spec. nov.]
C. brachyurus, thorace laevi utrinque serrato-quadri- lobo, manibus ovatis laevibus. M. L. U.
Habitat in Indiis.
description: Published as part of Linnaeus, Carolus, 1758, Systema Naturae per regna tria naturae: secundum classes, ordines, genera, species, cum characteribus, differentiis, synonymis, locis, Stockholm :Laurentius Salvius on page 627, DOI: 10.5962/bhl.title.542, http://zenodo.org/record/3922206
Tarbosaurus bataar Maleev 1955
Creators: name: Russell, Dale A.
Publisher: name: National Museum of Natural Sciences, Publications in Palaeontology, No. 1
Year: 1970
Subjects: Biodiversity
Taxonomy
Animalia
Chordata
Reptilia
Dinosauria
Tyrannosauridae
Tarbosaurus
Tarbosaurus bataar

description: Tarbosaurus bataar (Maleyev)
This species is known from the remains of at least seven individuals collected by the Palaeontological Institute of the Academy of Sciences of the U. S. S.R. (Maleyev 1955 b, 1955c) and six more collected by the Polish-Mongolian Palaeontological Expedition (Kielan-Jaworowska 1967), all from the Nemegt basin in strata that may be approximately Edmontonian {see L. S. Russell 1963) in age. The form has not yet been thoroughly described, although it has been the subject of several brief reports {see Introduction) and a cast of the skull of one specimen (NMC 10422) was available for study through an exchange with the Palaeontological Institute. Tarbosaurus seems to be most closely allied to Tyrannosaurus. It differs from this genus in that the nasals are not quite so constricted between the lacrimals, the frontals do have some dorsal expression (but not so much as in Albertosaurus or Daspletosaurus), the surangular foramen is small, and adult animals are smaller than adult specimens of Tyrannosaurus. (I am indebted to Dr. A. K. Rozhdestvensky for the above information on the morphology of Tarbosaurus.)
description: Published as part of Russell, Dale A., 1970, Tyrannosaurs from the Late Cretaceous of western Canada, Ottawa :National Museum of Natural Sciences, Publications in Palaeontology, No. 1 on page 20, DOI: 10.5281/zenodo.1040973
Additional file 7 of Characterising sex differences of autosomal DNA methylation in whole blood using the Illumina EPIC array
Creators: name: Grant, Olivia A.
name: Wang, Yucheng
name: Kumari, Meena
name: Zabet, Nicolae Radu
name: Schalkwyk, Leonard
Publisher: name: figshare
Year: 2022
Subjects: subject: Genetics
subject: FOS: Biological sciences

description: Additional file 7. Figure S2: (A) Integrated genomics viewer track of chromatin loop on chromosome 6 showing two male-biased CpGs contacting H1/H4/H3/H2V/H2A. (B) Integrated genomics viewer track of chromatin loop on chromosome 1 showing a female-biased CpG contacting the ODF2L gene. Blue lines represent the chromatin loops, with black lines showing the loop anchors. Orange vertical lines represent the male-biased CpGs and blue vertical lines represent the female-biased CpGs. Purple annotations represent genes. (C-D) Subnetworks of the top 30 genes annotated to male-biased CpGs (C) and females (D). Node colour represents the degree of connectivity. The scale from red to yellow represents the top 30 enriched genes rank from 1-30, with red indicating highest degree and yellow indicating lowest degree.
Additional file 15: of Impact of non-LTR retrotransposons in the differentiation and evolution of anatomically modern humans
Creators: name: Guichard, Etienne
name: Peona, Valentina
name: Guidantonio Malagoli Tagliazucchi
name: Abitante, Lucia
name: Jagoda, Evelyn
name: Musella, Margherita
name: Ricci, Marco
name: Rubio-RoldĂĄn, Alejandro
name: Sarno, Stefania
name: Luiselli, Donata
name: Pettener, Davide
name: Taccioli, Cristian
name: Pagani, Luca
name: Garcia-Perez, Jose
name: Boattini, Alessio
Publisher: name: figshare
Year: 2018
Subjects: subject: Medicine
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Evolutionary Biology
subject: 69999 Biological Sciences not elsewhere classified
subject: Developmental Biology
subject: Marine Biology
subject: 110309 Infectious Diseases
subject: FOS: Health sciences
subject: 60506 Virology
subject: Computational Biology

description: Distribution and clustering of genes preferentially expressed in specific tissues based on their length. A) Boxplot depicting the length of all human genes grouped by preferential expression. The letters under each box represent statistical similarity of the series (p-values
Wake of super-hydrophobic falling spheres: influence of the air layer deformation
Creators: name: Castagna, Marco
name: Mazellier, Nicolas
name: Kourta, Azeddine
Publisher: name: arXiv
Year: 2018
Subjects: subject: Fluid Dynamics (physics.flu-dyn)
subject: FOS: Physical sciences

description: We report an experimental investigation of the wake of free falling super-hydrophobic spheres. The mutual interaction between the air layer (plastron) encapsulating the super-hydrophobic spheres and the flow is emphasised by studying the hydrodynamic performances. It is found that the air plastron adapts its shape to the flow-induced stresses which compete with the surface tension. This competition is characterised by introducing the Weber number $\mathcal{W}e$, whilst the plastron deformation is estimated via the aspect ratio $χ$. While noticeable distortions are locally observed, the plastron becomes more and more spherical in average (i.e. $χ\rightarrow 1$) as far as $\mathcal{W}e$ increases. In comparison to the reference spheres, high deformation of the air plastron plastron (oblate shape) leads to lift and drag increase, whereas low deformation (spherical shape) yields lift and drag mitigation. Accordingly, taking into account the plastron deformation provides an attractive way to explain the somehow discordant results reported in other studies at comparable Reynolds numbers. If confirmed by additional studies, our findings would imply that plastron compliance and its feedback on the flow, which are currently neglected in most theoretical works and numerical simulations, must be accounted for to design super-hydrophobic surfaces and/or predict their performances.
Additional file 1: of Evolutionarily conserved partial gene duplication in the Triticeae tribe of grasses confers pathogen resistance
Creators: name: Jeyaraman Rajaraman
name: Douchkov, Dimitar
name: Lück, Stefanie
name: Hensel, Götz
name: Nowara, Daniela
name: Pogoda, Maria
name: Rutten, Twan
name: Meitzel, Tobias
name: Brassac, Jonathan
name: Höfle, Caroline
name: Hückelhoven, Ralph
name: Klinkenberg, Jörn
name: Trujillo, Marco
name: Bauer, Eva
name: Schmutzer, Thomas
name: Himmelbach, Axel
name: Mascher, Martin
name: Lazzari, Barbara
name: Stein, Nils
name: Kumlehn, Jochen
name: Schweizer, Patrick
Publisher: name: figshare
Year: 2018
Subjects: subject: Biochemistry
subject: Medicine
subject: Microbiology
subject: FOS: Biological sciences
subject: Genetics
subject: Molecular Biology
subject: Evolutionary Biology
subject: 69999 Biological Sciences not elsewhere classified
subject: Developmental Biology
subject: Hematology
subject: 110309 Infectious Diseases
subject: FOS: Health sciences
subject: Plant Biology
subject: 60506 Virology

description: Figure S1. Asexual life cycle of Blumeria graminis and the assessment of fungal development on barley (Hordeum vulgare) and wheat (Triticum aestivum). Figure S2. Alignment of HvPUB15 and HvARM1 genomic sequences. Figure S3. Protein sequence alignment and dN/dS analysis of ARM1 and PUB15. Figure S4. Off-target prediction in transgenic barley carrying the RNAi hairpin construct pIPKb009 for silencing of HvARM1. Figure S5. Expression of HvARM1 endogenous transcripts in powdery mildew-attacked barley epidermis. Figure S6. Localization of YFP-tagged proteins in barley and N. benthamiana epidermal cells. Figure S7. In vitro ubiquitin ligase activity of HvPUB15. Figure S8: Additional controls for BiFC in N. benthamiana leaves. Figure S9. Quantification of BiFC signals in N. benthamiana leaves. Figure S10. Additional, array-based transcript regulation data of selected genes in the epidermis of powdery mildew-attacked barley leaves. Figure S11. Plasmid map of pIPKTA48 for the subcellular localization of N-terminal fusion proteins with YFP. Figure S12. Plasmid map of pIPKTA49 for the subcellular localization of C-terminal fusion proteins with YFP. Figure S13. Genome-wide analysis of expressed and conserved gene duplicates. Figure S14. Mutation of HvARM1 disrupts its resistance-enhancing function. Table S8. HvARM1-interacting candidates from yeast two-hybrid screening. Table S9. List of primers used in this study. Table S10. Sequences used for phylogenetic and dN/dS analyses. (PDF 2000 kb)
Infrared Photometry of Red Supergiants in Young Clusters in the Magellanic Clouds
Creators: name: Keller, Stefan C.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present broad-band infrared photometry for 52 late-type supergiants in the young Magellanic Clouds clusters NGC 330, NGC 1818, NGC 2004 and NGC 2100. Standard models are seen to differ in the temperature they predict for the red supergiant population on the order of 300K. It appears that these differences most probably due to the calibration of the mixing-length parameter, $α_{P}$, in the outermost layers of the stellar envelope. Due to the apparent model dependent nature of $α_{P}$ we do not quantitatively compare $α_{P}$ between models. Qualitatively, we find that $α_{P}$ decreases with increased stellar mass within standard models. We do not find evidence for a metallicity dependence of $α_{P}$.
description: 11 pages, 4 figures. AJ accepted
An introduction to Bayesian inference in gravitational-wave astronomy: parameter estimation, model selection, and hierarchical models
Creators: name: Thrane, Eric
name: Talbot, Colm
Publisher: name: arXiv
Year: 2018
Subjects: subject: Instrumentation and Methods for Astrophysics (astro-ph.IM)
subject: FOS: Physical sciences

description: This is an introduction to Bayesian inference with a focus on hierarchical models and hyper-parameters. We write primarily for an audience of Bayesian novices, but we hope to provide useful insights for seasoned veterans as well. Examples are drawn from gravitational-wave astronomy, though we endeavor for the presentation to be understandable to a broader audience. We begin with a review of the fundamentals: likelihoods, priors, and posteriors. Next, we discuss Bayesian evidence, Bayes factors, odds ratios, and model selection. From there, we describe how posteriors are estimated using samplers such as Markov Chain Monte Carlo algorithms and nested sampling. Finally, we generalize the formalism to discuss hyper-parameters and hierarchical models. We include extensive appendices discussing the creation of credible intervals, Gaussian noise, explicit marginalization, posterior predictive distributions, and selection effects.
description: 16 pages, 3 figures, v8 includes erratum
Gas Dynamics in the Luminous Merger NGC 6240
Creators: name: Tacconi, L. J.
name: Genzel, R.
name: Tecza, M.
name: Gallimore, J. F.
name: Downes, D.
name: Scoville, N. Z.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We report 0.5"x0.9" resolution, interferometric observations of the 1.3 mm CO J=2-1 line in the infrared luminous galactic merger NGC 6240. About half of the CO flux is concentrated in a rotating but highly turbulent, thick disk structure centered between the two radio and near-infrared nuclei. A number of gas features connect this ~500 pc diameter central disk to larger scales. Throughout this region the molecular gas has local velocity widths which exceed 300 km/s FWHM and even reach FWZP line widths of 1000 km/s in a number of directions. The mass of the central gas concentration constitutes a significant fraction of the dynamical mass, M_gas(R<470 pc) ~ 2-4x10^9 M_o ~ 0.3-0.7 M_dyn. We conclude that NGC 6240 is in an earlier merging stage than the prototypical ultraluminous galaxy, Arp 220. The interstellar gas in NGC 6240 is in the process of settling between the two progenitor stellar nuclei, is dissipating rapidly and will likely form a central thin disk. In the next merger stage, NGC 6240 may well experience a major starburst like that observed in Arp 220.
description: To be published in Ap.J.; 7 figures