cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Three-dimensional structure of clumpy outflow from supercritical accretion flow onto black holes
Creators: name: Kobayashi, Hiroshi
name: Ohsuga, Ken
name: Takahashi, Hiroyuki R.
name: Kawashima, Tomohisa
name: Asahina, Yuta
name: Takeuchi, Shun
name: Mineshige, Shin
Publisher: name: arXiv
Year: 2018
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: We perform global three-dimensional (3D) radiation-hydrodynamic (RHD) simulations of out- flow from supercritical accretion flow around a 10 Msun black hole. We only solve the outflow part, starting from the axisymmetric 2D simulation data in a nearly steady state but with small perturbations in a sinusoidal form being added in the azimuthal direction. The mass accretion rate onto the black hole is ~10^2 L_E/c^2 in the underlying 2D simulation data and the outflow rate is ~10 L_E/c^2 (with LE and c being the Eddington luminosity and speed of light, respectively). We first confirm the emergence of clumpy outflow, which was discovered by the 2D RHD simulations, above the photosphere located at a few hundreds of Schwarzschild radii (r_S) from the central black hole. As prominent 3D features we find that the clumps have the shape of a torn sheet, rather than a cut string, and that they are rotating around the central black hole with a sub-Keplerian velocity at a distance of ~10^3 r_S from the center. The typical clump size is ~30 r_S or less in the radial direction, and is more elongated in the angular directions, ~hundreds of r_S at most. The sheet separation ranges from 50 to 150 r_S. We expect stochastic time variations when clumps pass across the line of the sight of a distant observer. Variation timescales are estimated to be several seconds for a black hole with mass of ten to several tens of Msun, in rough agreement with the observations of some ultra-luminous X-ray sources.
description: 12 pages, 8 figures, accepted for publication in PASJ
Additional file 1 of Omouma: a prospective mother and child cohort aiming to identify early biomarkers of pregnancy complications in women living in Qatar
Creators: name: Kumar, Manoj
name: Saadaoui, Marwa
name: Elhag, Duaa Ahmed
name: Murugesan, Selvasankar
name: Al Abduljabbar, Shaikha
name: Fagier, Yassin
name: Ortashi, Osman
name: Abdullahi, Hala
name: Ibrahim, Ibrahim
name: Alberry, Medhat
name: Abbas, Anthony
name: Ahmed, Sawssan R.
name: Hendaus, Mohamed A.
name: Kalache, Karim
name: Terranegra, Annalisa
name: Al Khodor, Souhaila
Publisher: name: figshare
Year: 2021
Subjects: subject: Medicine
subject: Cell Biology
subject: Genetics
subject: FOS: Biological sciences
subject: Biotechnology
subject: Sociology
subject: FOS: Sociology
subject: Immunology
subject: FOS: Clinical medicine
subject: Biological Sciences not elsewhere classified
subject: Mathematical Sciences not elsewhere classified
subject: Developmental Biology
subject: Cancer
subject: Infectious Diseases
subject: FOS: Health sciences
subject: Virology
subject: Computational Biology

description: Additional file 1.
Hidden chaotic attractors and chaos suppression in an impulsive discrete economical supply and demand dynamical system
Creators: name: Danca, M. -F.
name: Feckan, M.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Chaotic Dynamics (nlin.CD)
subject: FOS: Physical sciences

description: Impulsive control is used to suppress the chaotic behavior in an one-dimensional discrete supply and demand dynamical system. By perturbing periodically the state variable with constant impulses, the chaos can be suppressed. It is proved analytically that the obtained orbits are bounded and periodic. Moreover, it is shown for the first time that the difference equations with impulses, used to control the chaos, can generate hidden chaotic attractors. To the best of the authors knowledge, this interesting feature has not yet been discussed. The impulsive algorithm can be used to stabilize chaos in other classes of discrete dynamical systems.
Optical absorption spectra in fullerenes C60 and C70: Effects of Coulomb interactions, lattice fluctuations, and anisotropy
Creators: name: Harigaya, Kikuo
name: Abe, Shuji
Publisher: name: arXiv
Year: 1994
Subjects: subject: Condensed Matter (cond-mat)
subject: FOS: Physical sciences

description: Effects of Coulomb interactions and lattice fluctuations in the optical absorption spectra of C60 and C70 are theoretically investigated by using a tight binding model with long-range Coulomb interaction and bond disorder. Anisotropy effects in C70 are also considered. Optical spectra are calculated by using the Hartree-Fock approximation followed by the configuration interaction method. The main conclusions are as follows: (1) The broad peaks at excitation energies, 3.7eV, 4.7eV, and 5.7eV, observed in experiments of C60 molecules in a solution are reasonably described by the present theory. Peak positions and relative oscillator strengths are in overall agreement with the experiments. The broadening of peaks by lattice fluctuations is well simulated by the bond disorder model. (2) The optical gap of C70 is larger when the electric field of light is parallel to the long axis of the molecule. The shape of the frequency dispersion also depends on the orientation of the molecule. These properties are common in the free electron model and the model with Coulomb interactions. (3) The spectrum of C70 averaged over bond disorder and random orientations is compared with experiments in a solution. There is an overall agreement about the spectral shape. Differences in the spectra of C60 and C70 are discussed in connection with the symmetry reduction from a soccerball to a rugbyball.
description: PACS numbers: 78.66.Qn, 78.20.Dj, 71.35.+z, 31.20.Tz; LaTeX, 15 pages, 5 figures (Physical Review B); Note: Please request figures to Authors. They will be sent via snail mail
The dynamical-decoupling-based spatiotemporal noise spectroscopy
Creators: name: Krzywda, Jan
name: Szańkowski, Piotr
name: Cywiński, Łukasz
Publisher: name: arXiv
Year: 2018
Subjects: subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: Here we demonstrate how the standard, temporal-only, dynamical-decoupling-based noise spectroscopy method can be extended to also encompass the spatial degree of freedom. This spatiotemporal spectroscopy utilizes a system of multiple qubits arranged in a line that are undergoing pure dephasing due to environmental noise. When the qubits are driven by appropriately coordinated sequences of $π$ pulses the multi-qubit register becomes decoupled from all components of the noise, except for those characterized by frequencies and wavelengths specified by the pulse sequences. This allows for employment of the procedure for reconstruction of the two-dimensional spectral density that quantifies the power distribution among spatial and temporal harmonic components of the noise.
description: 17 pages, 6 figues
Whither Arab Free Trade Area.pdf
Creators: name: Malkawi, Bashar H.
Publisher: name: figshare
Year: 2018
Subjects: subject: 180105 Commercial and Contract Law
subject: FOS: Law

description: My inquiry will assess why, many decades after first attempts of economic integration, Arab countries have not been more successful in emulating the success of the European Union, a paradigm of successful economic integration. Specifically, I will explore obstacles to Arab economic integration and address the political and economic factors that play a role to achieve this goal
Fundamental classes in motivic homotopy theory
Creators: name: Déglise, Frédéric
name: Jin, Fangzhou
name: Khan, Adeel A.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Algebraic Geometry (math.AG)
subject: K-Theory and Homology (math.KT)
subject: FOS: Mathematics

description: We develop the theory of fundamental classes in the setting of motivic homotopy theory. Using this we construct, for any motivic spectrum, an associated bivariant theory in the sense of Fulton-MacPherson. We import the tools of Fulton's intersection theory into this setting: (refined) Gysin maps, specialization maps, and formulas for excess intersections, self-intersections, and blow-ups. We also develop a theory of Euler classes of vector bundles in this setting. For the Milnor-Witt spectrum recently constructed by Déglise-Fasel, we get a bivariant theory extending the Chow-Witt groups of Barge-Morel, in the same way the higher Chow groups extend the classical Chow groups. As another application we prove a motivic Gauss-Bonnet formula, computing Euler characteristics in the motivic homotopy category.
description: 45 pages, final version; to appear in JEMS
SPIRITS 16tn in NGC 3556: A heavily obscured and low-luminosity supernova at 8.8 Mpc
Creators: name: Jencson, Jacob E.
name: Kasliwal, Mansi M.
name: Adams, Scott M.
name: Bond, Howard E.
name: Lau, Ryan M.
name: Johansson, Joel
name: Horesh, Assaf
name: Mooley, Kunal P.
name: Fender, Robert
name: De, Kishalay
name: O'Sullivan, Dónal
name: Masci, Frank J.
name: Cody, Ann Marie
name: Blagorodnova, Nadia
name: Fox, Ori D.
name: Gehrz, Robert D.
name: Milne, Peter A.
name: Perley, Daniel A.
name: Smith, Nathan
name: Van Dyk, Schuyler D.
Publisher: name: arXiv
Year: 2018
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: We present the discovery by the SPitzer InfraRed Intensive Transients Survey (SPIRITS) of a likely supernova (SN) in NGC 3556 at only 8.8 Mpc, which, despite its proximity, was not detected by optical searches. A luminous infrared (IR) transient at $M_{[4.5]} = -16.7$ mag (Vega), SPIRITS 16tn is coincident with a dust lane in the inclined, star-forming disk of the host. Using IR, optical, and radio observations, we attempt to determine the nature of this event. We estimate $A_V \approx$ 8 - 9 mag of extinction, placing it among the three most highly obscured IR-discovered SNe to date. The [4.5] light curve declined at a rate of 0.013 mag day$^{-1}$, and the $[3.6] - [4.5]$ color grew redder from 0.7 to $\gtrsim$ 1.0 mag by 184.7 days post discovery. Optical/IR spectroscopy shows a red continuum, but no clearly discernible features, preventing a definitive spectroscopic classification. Deep radio observations constrain the radio luminosity of SPIRITS 16tn to $L_ν \lesssim 10^{24}$ erg s$^{-1}$ Hz$^{-1}$ between 3 - 15 GHz, excluding many varieties of radio core-collapse SNe. A type Ia SN is ruled out by the observed red IR color, and lack of features normally attributed to Fe-peak elements in the optical and IR spectra. SPIRITS 16tn was fainter at [4.5] than typical stripped-envelope SNe by $\approx$ 1 mag. Comparison of the spectral energy distribution to SNe II suggests SPIRITS 16tn was both highly obscured, and intrinsically dim, possibly akin to the low-luminosity SN 2005cs. We infer the presence of an IR dust echo powered by a peak luminosity of the transient of $5 \times 10^{40}$ erg s$^{-1} < L_{\mathrm{peak}} < 4\times10^{43}$ erg s$^{-1}$, consistent with the observed range for SNe II. This discovery illustrates the power of IR surveys to overcome the compounding effects of visible extinction and optically sub-luminous events in completing the inventory of nearby SNe.
description: 25 pages, 10 figures, submitted to ApJ
Kinetics of Macrostep Under Diffusion and Thermal Interactions in Stagnant Media
Creators: name: Potapenko, Serge Yu.
Publisher: name: arXiv
Year: 1994
Subjects: subject: Condensed Matter (cond-mat)
subject: FOS: Physical sciences

description: The step motions considered are those in which crystallization is controlled by a single diffusion process, either the substance diffusion for growth from solution or the flow of latent heat from the step for growth from melt. Quasi-static diffusion nearby two parallel steps and nearby a train of parallel steps is considered. Terraces and step risers are assumed flat with arbitrary angles between them. Flux of the crystallizing substance to the crystal or the heat sources on the crystal surface are nonvanishing on the step risers only. Kinematics of the steps under the diffusion interaction is investigated, when velocities of the steps are controlled by the supersaturation at the feet of the steps. For the solution growth it is shown that an equidistant train of steps is unstable against to doubling of period, i.e. neighbouring steps are attracted, when the angle of the riser is more than $π/3$. The diffusion interaction stabilizes the train of gently sloping steps. For the melt growth at equal thermal conductivities of the crystal and of the melt, the thermal interaction stabilizes the train of steps without overhanging when the riser angle is less than $π/2$. If the heat transfers through the crystals, then the equidistant train is stable at all riser angles.
description: 15 pages, latex, 3 figures not included
title: Цветочно-декоративные растения и дендрология
title: Учебное пособие для СПО
titleType: Subtitle
Creators: name: Исяньюлова Р.Р.
name:  Половникова М.В.
Publisher: name: Профобразование, Ай Пи Ар Медиа
Year: 2019

description: В учебном пособии рассмотрены основные вопросы, изучаемые в рамках дисциплины «Цветочно-декоративные растения и дендрология». Представлены классификации цветочно-декоративных растений, а также древесных и кустарниковых пород. Подробно рассматриваются морфологические и биологические особенности цветочно-декоративных растений открытого и закрытого грунта, размножение древесно-кустарниковых и цветочно-декоративных растений. Особое внимание уделено типам посадок. Кроме того, учебное пособие содержит информацию о методах защиты растений от вредителей и болезней. Подготовлено с учетом требований Федерального государственного образовательного стандарта среднего профессионального образования по специальности 35.02.12 «Садово-парковое и ландшафтное строительство».
Quantum Monte Carlo study of the H- impurity in small helium clusters
Creators: name: Casalegno, M.
name: Mella, M.
name: Morosi, G.
name: Bressanini, D.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Atomic and Molecular Clusters (physics.atm-clus)
subject: FOS: Physical sciences

description: We report ground state energies and structural properties for small helium clusters (4He) containing an H- impurity computed by means of variational and diffusion Monte Carlo methods. Except for 4He_2H- that has a noticeable contribution from collinear geometries where the H- impurity lies between the two 4He atoms, our results show that our 4He_NH- clusters have a compact 4He_N subsystem that binds the H- impurity on its surface. The results for $N\geq 3$ can be interpreted invoking the different features of the minima of the He-He and He-H- interaction potentials.
description: 12 pages, 7 Ps figures
title: ADCO, Septième cartulaire de Saint-Étienne de Dijon (1661-1665), Cart. 29 (G 134), 996 folios, f. 0585
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
name: Petot, Frédéric
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2020
Subjects: subject: Corpus Burgundiae Medii Aevi
subject: Chartes de la Bourgogne du Moyen Âge
subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris
subject: cartulaire

description: Septième cartulaire de Saint-Étienne de Dijon (1661-1665), Archives départementales de la Côte-d'Or, Cart. 29 (G 134), 996 folios, f. 0585, Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Septième cartulaire de Saint-Étienne de Dijon (1661-1665), Archives départementales de la Côte-d'Or, Cart. 29 (G 134), 996 folios, f. 0585, 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
Additional file 2 of Omouma: a prospective mother and child cohort aiming to identify early biomarkers of pregnancy complications in women living in Qatar
Creators: name: Kumar, Manoj
name: Saadaoui, Marwa
name: Elhag, Duaa Ahmed
name: Murugesan, Selvasankar
name: Al Abduljabbar, Shaikha
name: Fagier, Yassin
name: Ortashi, Osman
name: Abdullahi, Hala
name: Ibrahim, Ibrahim
name: Alberry, Medhat
name: Abbas, Anthony
name: Ahmed, Sawssan R.
name: Hendaus, Mohamed A.
name: Kalache, Karim
name: Terranegra, Annalisa
name: Al Khodor, Souhaila
Publisher: name: figshare
Year: 2021
Subjects: subject: Medicine
subject: Cell Biology
subject: Genetics
subject: FOS: Biological sciences
subject: Biotechnology
subject: Sociology
subject: FOS: Sociology
subject: Immunology
subject: FOS: Clinical medicine
subject: Biological Sciences not elsewhere classified
subject: Mathematical Sciences not elsewhere classified
subject: Developmental Biology
subject: Cancer
subject: Infectious Diseases
subject: FOS: Health sciences
subject: Virology
subject: Computational Biology

description: Additional file 2.
Chermes fraxini Linnaeus, 1758, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1758
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hemiptera
Aphididae
Chermes
Chermes fraxini

description: Chermes fraxini [spec. nov.]
C. Fraxini excelsioris. Fn. svec. 703.
Habitat in Fraxino excelsiore.
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 454, DOI: 10.5962/bhl.title.542, http://zenodo.org/record/3922206
Quality control of GEM detectors using scintillation techniques
Creators: name: Fraga, F. A. F.
name: Fetal, S. T. G.
name: Marques, R. Ferreira
name: Policarpo, A. J. P. L.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Instrumentation and Detectors (physics.ins-det)
subject: FOS: Physical sciences

description: Non destructive quality control of microstructures at the manufacturing stage is an important issue in the foreseen use of huge numbers of such gaseous detectors in the future high luminosity colliders. In this work we report on the use of the scintillation light emitted by the avalanches in GEM channels for checking defects in the foils. The test system is described and data on the relative efficiency of several gaseous mixtures are presented. The foil images obtained with a low-noise CCD system are analysed and compared with the optical images obtained with an industrial inspection system of high magnification. The validity of this test method is established and possible extensions of its use are discussed.
description: 11 pages, 9 figures
Hot subdwarfs formed from the merger of two He white dwarfs
Creators: name: Schwab, Josiah
Publisher: name: arXiv
Year: 2018
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: We perform stellar evolution calculations of the remnant of the merger of two He white dwarfs (WDs). Our initial conditions are taken from hydrodynamic simulations of double WD mergers and the viscous disc phase that follows. We evolve these objects from shortly after the merger into their core He-burning phase, when they appear as hot subdwarf stars. We use our models to quantify the amount of H that survives the merger, finding that it is difficult for $\gtrsim 10^{-4}\;{\rm M}_\odot$ of H to survive, with even less being concentrated in the surface layers of the object. We also study the rotational evolution of these merger remnants. We find that mass loss over the $\sim 10^4\;\rm yr$ following the merger can significantly reduce the angular momentum of these objects. As hot subdwarfs, our models have moderate surface rotation velocities of $30-100\; {\rm km\,s^{-1}}$. The properties of our models are not representative of many apparently-isolated hot subdwarfs, suggesting that those objects may form via other channels or that our modelling is incomplete. However, a sub-population of hot subdwarfs are moderate-to-rapid rotators and/or have He-rich atmospheres. Our models help to connect the observed properties of these objects to their progenitor systems.
description: 10 pages, 11 figures; Accepted to MNRAS
Relation between the Correlation Dimensions of Multifractal Wavefunctions and Spectral Measures in Integer Quantum Hall Systems
Creators: name: Huckestein, B.
name: Schweitzer, L.
Publisher: name: arXiv
Year: 1994
Subjects: subject: Condensed Matter (cond-mat)
subject: FOS: Physical sciences

description: We study the time evolution of wavepackets of non-interacting electrons in a two-dimensional disordered system in strong magnetic field. For wavepackets built from states near the metal-insulator transition in the center of the lowest Landau band we find that the return probability to the origin $p(t)$ decays algebraically, $p(t) \sim t^{-D_2/2}$, with a non-conventional exponent $D_2/2$. $D_2$ is the generalized dimension describing the scaling of the second moment of the wavefunction. We show that the corresponding spectral measure is multifractal and that the exponent $D_2/2$ equals the generalized dimension $\widetilde{D}_2$ of the spectral measure.
description: 8 pages, RevTeX 3.0, 4 PostScript figures in uuencoded compressed tar file included
How To Make Your Medieval Research More Visible With Open Scholarship Methods and Tools (Open Science Workshop at Carmen Annual Meeting 2018, Tampere University)
Creators: name: Wuttke, Ulrike
Publisher: name: figshare
Year: 2018
Subjects: subject: Digital Humanities
subject: History
subject: 220401 Christian Studies (incl. Biblical Studies and Church History)
subject: FOS: Philosophy, ethics and religion
subject: Art
subject: 210399 Historical Studies not elsewhere classified
subject: FOS: History and archaeology
subject: 220209 History of Ideas
subject: Literature
subject: 229999 Philosophy and Religious Studies not elsewhere classified

description: Open Science Workshop at Carmen Annual Meeting 2018
 How To Make Your Medieval Research More Visible With Open Scholarship Methods and Tools
 Dr. Ulrike Wuttke Academic publishing, scholarly communication, and requirements for good academic practices are changing. Open Access to scientific publications and research data is supported by a growing number of institutions and becomes increasingly a requirement of research funders. The communication of scientific results happens more and more in social networks and blogs. While these changing patterns of scholarly communication can positively impact their research dissemination, enhance the number of citations, not at least to prove the relevance of medieval studies against the backdrop of dwindling research budgets, humanities researchers are comparatively reluctant to embrace open scholarly practices. This workshop is targeted to all medievalists who wish to increase the visibility of their research and find out more about the opportunities of Open Science and Open Scholarship methods and tools. There will be an overview of practical solutions already existing, as well as space to discuss doubts and needs (e.g. more open access for books, more subject specific open access journals or repositories), how to overcome them and to connect with like-minded researchers to form new initiatives. The summarized (anonymous) results of this workshop will be reported back to relevant infrastructures and made public for funders e.g. in a blogpost, project deliverable etc.
The Fractal Universe: From the Planck to the Hubble Scale
Creators: name: Sidharth, B. G.
Publisher: name: arXiv
Year: 1999
Subjects: subject: General Physics (physics.gen-ph)
subject: FOS: Physical sciences

description: We examine the fractal structure of the physical universe from the large scale to the smallest scale, including the phenomenon of fractal scaling. This is explained in terms of a stochastic underpinning for the laws of physics. A picture in pleasing agreement with experiment and observation at all scales emerges, very much in the spirit of Wheeler's "Law Without Law". It is argued that our depiction of the universe is akin to a broad brush delineation of a jagged coastline, the Compton wavelength being comparable to the thickness of the brush strokes.
description: 10 pages, TeX
Additional file 2 of Identification of novel molecular markers of mastitis caused by Staphylococcus aureus using gene expression profiling in two consecutive generations of Chinese Holstein dairy cattle
Creators: name: Wang, Di
name: Liu, Lei
name: Augustino, Serafino M. A.
name: Duan, Tao
name: Hall, Thomas J.
name: MacHugh, David E.
name: Dou, Jinhuan
name: Zhang, Yi
name: Wang, Yachun
name: Yu, Ying
Publisher: name: figshare
Year: 2020
Subjects: subject: Medicine
subject: Microbiology
subject: FOS: Biological sciences
subject: Cell Biology
subject: Genetics
subject: Immunology
subject: FOS: Clinical medicine
subject: Biological Sciences not elsewhere classified
subject: Mathematical Sciences not elsewhere classified
subject: Cancer
subject: Infectious Diseases
subject: FOS: Health sciences
subject: Virology

description: Additional file 2: Supplementary Figur S2. Volcano plots of DEGs for (A) the S vs. H comparison, (B) the SM vs. HM comparison, and (C) the SMD vs. HMD comparison.
The Density Profile and Kinematics of the Milky Way with RR Lyrae Stars
Creators: name: Ablimit, Iminhaji
name: Zhao, Gang
Publisher: name: arXiv
Year: 2018
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: Most of known RR Lyraes are type ab RR Lyraes (RRLab), and they are the excellent tool to map the Milky Way and its substructures. We find that 1148 RRLab stars determined by Drake et al.(2013) have been observed by spectroscopic surveys of SDSS and LAMOST. We derived radial velocity dispersion, circular velocity and mass profile from 860 halo tracers in our paper I. Here, we present the stellar densities and radial velocity distributions of thick disk and halo of the Milky Way. The 288 RRLab stars located in the thick disk have the mean metallicity of [Fe/H]$=-1.02$. Three thick disk tracers have the radial velocity lower than 215 km $\rm s^{-1}$. With 860 halo tracers which have a mean metallicity of [Fe/H]$=-1.33$, we find a double power-law of $n(r) \propto r^{-2.8}$ and $n(r) \propto r^{-4.8}$ with a break distance of 21 kpc to express the halo stellar density profile. The radial velocity dispersion at 50 kpc is around 78 km $\rm s^{-1}$.
description: 12pages, 4 figures; accepted by ApJ
Additional file 1: of Organophosphorus pesticide chlorpyrifos intake promotes obesity and insulin resistance through impacting gut and gut microbiota
Creators: name: Liang, Yiran
name: Zhan, Jing
name: Liu, Donghui
name: Luo, Mai
name: Han, Jiajun
name: Liu, Xueke
name: Liu, Chang
name: Cheng, Zheng
name: Zhou, Zhiqiang
name: Wang, Peng
Publisher: name: figshare
Year: 2019
Subjects: subject: Biochemistry
subject: Microbiology
subject: FOS: Biological sciences
subject: Genetics
subject: Molecular Biology
subject: Biotechnology
subject: Chemical Sciences not elsewhere classified
subject: Ecology
subject: Plant Biology
subject: Computational Biology

description: Figure S1. Effects of chlorpyrifos administration on food intake (a and e), colon length (b and f), fecal bacteria amount (c and g), and fecal LPS levels (d and h) in C57Bl/6 (a–d) and CD-1 (ICR) mice (e–h). Data are expressed as the mean ± SEM. *P < 0.05 versus NFD group; # P < 0.05 versus HFD group. NFD, normal-fat diet; NCPF, normal-fat diet + chlorpyrifos; HFD, high-fat diet; HCPF, high-fat diet + chlorpyrifos. (DOCX 197 kb)
Asymptotically exact solution of the multi-channel resonant-level model
Creators: name: Zhang, G. M.
name: Su, Z. B.
name: Yu, L.
Publisher: name: arXiv
Year: 1994
Subjects: subject: Condensed Matter (cond-mat)
subject: FOS: Physical sciences

description: An asymptotically exact partition function of the multi-channel resonant-level model is obtained through Tomonaga-Luttinger bosonization. A Fermi-liquid vs non-Fermi-liquid transition, resulting from a competition between the Kondo and X-ray edge physics, is elucidated explicitly via the renormalization group theory. In the strong-coupling limit, the model is renormalized to the Toulouse limit.
description: 11 pages, one postscript (attached), to appear in Phys. Rev. B
Additional file 8 of Identification of novel molecular markers of mastitis caused by Staphylococcus aureus using gene expression profiling in two consecutive generations of Chinese Holstein dairy cattle
Creators: name: Wang, Di
name: Liu, Lei
name: Augustino, Serafino M. A.
name: Duan, Tao
name: Hall, Thomas J.
name: MacHugh, David E.
name: Dou, Jinhuan
name: Zhang, Yi
name: Wang, Yachun
name: Yu, Ying
Publisher: name: figshare
Year: 2020
Subjects: subject: Medicine
subject: Microbiology
subject: FOS: Biological sciences
subject: Cell Biology
subject: Genetics
subject: Immunology
subject: FOS: Clinical medicine
subject: Biological Sciences not elsewhere classified
subject: Mathematical Sciences not elsewhere classified
subject: Cancer
subject: Infectious Diseases
subject: FOS: Health sciences
subject: Virology

description: Additional file 8: Table S4. Six significantly enriched upregulated gene sets.
Optical conductivity of the Hubbard model at finite temperature
Creators: name: Riera, Jose A.
name: Dagotto, Elbio
Publisher: name: arXiv
Year: 1994
Subjects: subject: Condensed Matter (cond-mat)
subject: FOS: Physical sciences

description: The optical conductivity, $σ(ω)$, of the two dimensional one-band Hubbard model is calculated at finite temperature using exact diagonalization techniques on finite clusters. The in-plane d.c. resistivity, $ρ_{ab}$, is also evaluated. We find that at large U/t and temperature T, $ρ_{ab}$ is approximately linear with temperature, in reasonable agreement with experiments on high-T$_c$ superconductors. Moreover, we note that $σ(ω)$ displays charge excitations, a mid-infrared (MIR) band and a Drude peak, also as observed experimentally. The combination of the Drude peak and the MIR oscillator strengths leads to a conductivity that decays slower than $1/ω^2$ at energies smaller than the insulator gap near half-filling.
description: 12 pages, 3 figures appended, Revtex version 2.0, preprint
Singular Shape of a Fluid Drop in an Electric or Magnetic Field
Creators: name: Li, Hao
name: Halsey, Thomas C.
name: Lobkovsky, Alexander
Publisher: name: arXiv
Year: 1994
Subjects: subject: Condensed Matter (cond-mat)
subject: FOS: Physical sciences

description: Beyond a threshold, electric or magnetic fields cause a dielectric or ferromagnetic fluid drop respectively to develop conical tips. We analyze the appearance of the conical tips and the associated shape transition of the drop using a local force balance as well as a global energy argument. We find that a conical interface is possible only when the dielectric constant (or permeability) of the fluid exceeds a critical value $ε_c=17.59$. For a fluid with $ε>ε_c$, a conical interface is possible at two angles, one stable and one unstable. We calculate the critical field required to sustain a drop with stable conical tips. Such a drop is energetically favored at sufficiently high field. Our results also apply to the formation of conical dimples when a pool of fluid is placed in a normal field.
description: 10 pages, Plain TeX, 3 postscript figures available on request via email
Additional file 1 of Epigenetic loci for blood pressure are associated with hypertensive target organ damage in older African Americans from the genetic epidemiology network of Arteriopathy (GENOA) study
Creators: name: Kho, Minjung
name: Zhao, Wei
name: Ratliff, Scott M.
name: Ammous, Farah
name: Mosley, Thomas H.
name: Shang, Lulu
name: Kardia, Sharon L. R.
name: Zhou, Xiang
name: Smith, Jennifer A.
Publisher: name: figshare
Year: 2020
Subjects: subject: Biophysics
subject: Medicine
subject: Cell Biology
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Biotechnology
subject: Biological Sciences not elsewhere classified
subject: Marine Biology
subject: Cancer
subject: Mental Health
subject: Hematology

description: Additional file 1: Table S1. Interactions between CpG sites and target organ damage risk factors including BMI, current smoking, and diabetes on target organ damage phenotypes in GENOA African ancestry population. Table S2. Results of mediation analysis of CpG sites-systolic blood pressure-target organ damage phenotypes in GENOA African ancestry population. Table S3. Results of mediation analysis of CpG sites-systolic blood pressure-target organ damage phenotypes adjusted for BMI, current smoking, and diabetes in GENOA African ancestry population. Table S4. Mendelian randomization results showing the inverse-variance weighted effects of multiple cis-SNP used as instrumental variables in the association of DNA methylation and target organ damage measures in GENOA African ancestry population. Figure S1. Interaction plots between a CpG site and the traditional risk factors for arteriosclerosis (BMI and diabetes) on urine albumin-to-creatinine ratio (UACR). Figure S2. Mendelian randomization (MR) scatterplot of urine albumin-to-creatinine ratio vs. CpG with estimates from inverse-variance weighted (IVW) MR using cis-SNPs within ±1 Mb of corresponding CpG site in GENOA African Americans.
Dielectronic Recombination of Ground-State and Metastable Li+ Ions
Creators: name: Saghiri, A. A.
name: Linkemann, J.
name: Schmitt, M.
name: Schwalm, D.
name: Wolf, A.
name: Bartsch, T.
name: Hoffknecht, A.
name: Mueller, A.
name: Graham, W. G.
name: Price, A. D.
name: Badnell, N. R.
name: Gorczyca, T. W.
name: Tanis, J. A.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Atomic Physics (physics.atom-ph)
subject: Accelerator Physics (physics.acc-ph)
subject: FOS: Physical sciences

description: Dielectronic recombination has been investigated for Delta-n = 1 resonances of ground-state Li+(1s^2) and for Delta-n = 0 resonances of metastable Li+(1s2s ^3S). The ground-state spectrum shows three prominent transitions between 53 and 64 eV, while the metastable spectrum exhibits many transitions with energies < 3.2 eV. Reasonably good agreement of R-matrix, LS coupling calculations with the measured recombination rate coefficient is obtained. The time dependence of the recombination rate yields a radiative lifetime of 52.2 +- 5.0 s for the 2 ^3S level of Li+.
description: Submitted to Phys. Rev. A; REVTeX, 4 pages, 3 figures
Low Temperature Properties of Anisotropic Superconductors with Kondo Impurities
Creators: name: Borkowski, L. S.
name: Hirschfeld, P. J.
Publisher: name: arXiv
Year: 1994
Subjects: subject: Condensed Matter (cond-mat)
subject: FOS: Physical sciences

description: We present a self-consistent theory of superconductors in the presence of Kondo impurities, using large-$N$ slave-boson methods to treat the impurity dynamics. The technique is tested on the s-wave case and shown to give good results compared to other methods for $T_K > T_c$. We calculate low temperature thermodynamic and transport properties for various superconducting states, including isotropic s-wave and representative anisotropic model states with line and point nodes on the Fermi surface.
description: 21 pages, RevTeX 3.0, 12 figures available upon request, UF preprint
title: ADCO, Cartulaire général de Cîteaux, dit de Jean de Cirey, (XVe siècle), tome IV, Cart. 188 (11 H 73), f. 0111r
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: cartulaire
subject: Corpus Burgundiae Medii Aevi
subject: Chartes de la Bourgogne du Moyen Âge

description: Cartulaire général de Cîteaux, dit de Jean de Cirey, (XVe siècle), tome IV, Archives départementales de la Côte-d'Or, Cart. 188 (11 H 73), f. 0111r, Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Cartulaire général de Cîteaux, dit de Jean de Cirey, (XVe siècle), tome IV, Archives départementales de la Côte-d'Or, Cart. 188 (11 H 73), f. 0111r, 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
Cluster mechanisms in the fully frustrated Ising model
Creators: name: Kerler, Werner
name: Rehberg, Peter
Publisher: name: arXiv
Year: 1994
Subjects: subject: Condensed Matter (cond-mat)
subject: High Energy Physics - Lattice (hep-lat)
subject: FOS: Physical sciences

description: The cluster algorithm in the fully frustrated Ising model on the square lattice is essentially different from the ones used in other systems. Thus its better understanding is particularly important for finding new lines of development. Therefore we investigate it in detail. In our simulations of high statistics more appropriate choices of the probability for freezing bonds and of that for flipping spins are seen to lead to better results. In an analysis of the topological properties we derive a set of rules for possible cluster configurations and give a classification by pairs of winding numbers.
description: 17 pages (latex), 14 figures (sorry, not included); to appear in Physical Review B
Study of the one-dimensional Schroedinger equation generated from the hypergeometric equation
Creators: name: Natanzon, G. A.
Publisher: name: arXiv
Year: 1999
Subjects: subject: History and Philosophy of Physics (physics.hist-ph)
subject: FOS: Physical sciences

description: Original English Summary. - A systematic method of constructing potentials, for which the one-variable Schroedinger equation can be solved in terms of the hypergeometric (HGM) function, is presented. All the potentials, obtained by energy-independent transformations of the HGM equation, are determined together with eigenvalues and eigenfunctions. A class of potentials derived from the confluent HGM equation is found by means of a limit process
description: 9 pages in LaTex, translated by H.C. Rosu, thanks are due to R. Milson for sending me a xerocopy of the paper
Strong-Correlations Versus U-Center Pairing and Fractional Aharonov-Bohm Effect
Creators: name: Kusmartsev, F. V.
name: Weisz, J. F.
name: Kishore, R.
name: Takahashi, Minoru
Publisher: name: arXiv
Year: 1994
Subjects: subject: Condensed Matter (cond-mat)
subject: FOS: Physical sciences

description: The influence of the interaction between electrons on the Aharonov-Bohm effect is investigated in the framework of the Hubbard model. The repulsion between electrons associated with strong correlation is compared with the case of attraction such as $U$-center pairing. The most interesting case, when two electrons are located on a ring, is investigated in detail using the Bethe ansatz method and by exact numerical diagonalization of the Hubbard hamiltonian. It is shown that the quasi half quantum flux periodicity occurs for any nonzero values of $U$. For large number of sites, or strong U, the quasi periodicity becomes an exact half quantum flux periodicity. However the character of the state created on the ring is different in both cases. In the case of $U$-center pairing the electrons are bound in pairs located on the same site. For strong correlations(large positive $ U$) the electrons tend to be far from each other as possible. We show by numerical solution of Bethe ansaz equations that for three electrons the flux periodicity of the ground state energy is equal to 1/3. The one third periodicity may occur even for small values of the ratio $U/t$, for the very dilute system. It is shown analytically using the Bethe ansaz equations for $N$ electrons, that for dilute systems with arbitrary value of the Hubbard repulsion $U$,
description: 30 pages (Latex), 10 figures upon request, submitted to Phys. Rev
A sufficient condition for finiteness of Frobenius test exponents
Creators: name: Maddox, Kyle
Publisher: name: arXiv
Year: 2018
Subjects: subject: Commutative Algebra (math.AC)
subject: FOS: Mathematics
subject: 13A35, 13D45

description: The Frobenius test exponent $\operatorname{Fte}(R)$ of a local ring $(R,\mathfrak{m})$ of prime characteristic $p > 0$ is the smallest $e_0 \in \mathbb{N}$ such that for every ideal $\mathfrak{q}$ generated by a (full) system of parameters, the Frobenius closure $\mathfrak{q}^F$ has $(\mathfrak{q}^F)^{[p^{e_0}]} = \mathfrak{q}^{[p^{e_0}]}$. We establish a suffcient condition for $\operatorname{Fte}(R)
description: 10 pages, comments welcome
Proximity Effect and Charging in Mesoscopic Normal Metal - Superconductor Junction Systems
Creators: name: Bruder, C.
name: Fazio, Rosario
name: Schön, Gerd
Publisher: name: arXiv
Year: 1994
Subjects: subject: Condensed Matter (cond-mat)
subject: FOS: Physical sciences

description: Charging effects in mesoscopic junctions suppress the tunneling of electrons. In normal metal - superconductor systems they also suppress the proximity effect, thereby revealing the nature of the microscopic processes and of the ground state of the system. The effect can be made visible since the charging and proximity effect and hence the transport properties of the system can be modulated by gate voltages. If the superconducting electrode is isolated, electron number parity effect lead to an even-odd asymmetry in the proximity effect.
description: 7 Pages Revtex, 5 postscript figures appended (shell archive), tfp-1994-1
The allowed parameter space of a long-lived neutron star as the merger remnant of GW170817
Creators: name: Ai, Shunke
name: Gao, He
name: Dai, Zi-Gao
name: Wu, Xue-Feng
name: Li, Ang
name: Zhang, Bing
Publisher: name: arXiv
Year: 2018
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: Limited by the sensitivities of the current gravitational wave (GW) detectors, the central remnant of the binary neutron star (NS) merger associated with GW170817 remains an open question. Considering the relatively large total mass, it is generally proposed that the merger of GW170817 would lead to a shortly lived hypermassive NS or directly produce a black hole (BH). There is no clear evidence to support or rule out a long-lived NS as the merger remnant. Here we utilize the GW and electromagnetic (EM) signals to comprehensively investigate the parameter space that allows a long-lived NS to survive as the merger remnant of GW170817. We find that for some stiff equations of state, the merger of GW170817 could, in principle, lead to a massive NS, which has a millisecond spin period. The post-merger GW signal could hardly constrain the ellipticity of the NS. If the ellipticity reaches $10^{-3}$, in order to be compatible with the multi-band EM observations, the dipole magnetic field of the NS ($B_p$) is constrained to the magnetar level of $\sim10^{14}$ G. If the ellipticity is smaller than $10^{-4}$, $B_p$ is constrained to the level of $\sim10^{10}-10^{12}\,$G. These conclusions weakly depend on the adoption of equations of state.
description: 8 pages, 1 figures
Structural glaciology of Isunguata Sermia, West Greenland
Creators: name: Jones, Christine
name: Ryan, Jonathan
name: Holt, Tom
name: Hubbard, Alun
Publisher: name: Taylor & Francis
Year: 2018
Subjects: subject: Biochemistry
subject: Neuroscience
subject: Pharmacology
subject: 59999 Environmental Sciences not elsewhere classified
subject: FOS: Earth and related environmental sciences
subject: Ecology
subject: FOS: Biological sciences
subject: Computational Biology

description: We present a 1:42,000 scale map of Isunguata Sermia, a land-terminating outlet glacier draining the western-sector of the Greenland Ice Sheet. Structure-from-Motion software applied to ∼3,600 aerial images collected by a fixed-wing unmanned aerial vehicle in July 2015 allowed us to produce a high resolution (0.3 m ground sampling distance (GSD)) orthomosaic and digital elevation model (DEM; 1.5 m GSD).These products were used to map and describe the structural, geomorphological and hydrological features of the lower 16 km terminus of Isunguata Sermia and include many thousands of crevasses, crevasse traces and supraglacial channels. Additionally, several geomorphological features and pro-glacial hydrological features were identified, including debris-covered ice, lateral moraines and ice-marginal lakes. The map has potential for informing and reconstructing the long-term dynamic history of the glacier, including its response to variable environmental forcing.
Jet shapes of isolated photon-tagged jets in PbPb and pp collisions at $\sqrt{s_\mathrm{NN}} =$ 5.02 TeV
Creators: name: CMS Collaboration
Publisher: name: arXiv
Year: 2018
Subjects: subject: High Energy Physics - Experiment (hep-ex)
subject: Nuclear Experiment (nucl-ex)
subject: FOS: Physical sciences

description: The modification of jet shapes in PbPb collisions, relative to those in pp collisions, is studied for jets associated with an isolated photon. The data were collected with the CMS detector at the LHC at a nucleon-nucleon center-of-mass energy of 5.02 TeV. Jet shapes are constructed from charged particles with track transverse momenta ($p_\mathrm{T}$) above 1 GeV/c in annuli around the axes of jets with $p^\mathrm{jet}_\mathrm{T}$ $>$ 30 GeV/c associated with an isolated photon with $p^γ_\mathrm{T}$ $>$ 60 GeV/c. The jet shape distributions are consistent between peripheral PbPb and pp collisions, but are modified for more central PbPb collisions. In these central PbPb events, a larger fraction of the jet momentum is observed at larger distances from the jet axis compared to pp, reflecting the interaction between the partonic medium created in heavy ion collisions and the traversing partons.
description: Replaced with the published version. Added the journal reference and the DOI. All the figures and tables, including additional supplementary figures, can be found at http://cms-results.web.cern.ch/cms-results/public-results/publications/HIN-18-006 (CMS Public Pages)
Gas expulsion in highly substructured embedded star clusters
Creators: name: Farias, J. P.
name: Fellhauer, M.
name: Smith, R.
name: Dominguez, R.
name: Dabringhausen, J.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: We investigate the response of initially substructured, young, embedded star clusters to instantaneous gas expulsion of their natal gas. We introduce primordial substructure to the stars and the gas by simplistically modelling the star formation process so as to obtain a variety of substructure distributed within our modelled star forming regions. We show that, by measuring the virial ratio of the stars alone (disregarding the gas completely), we can estimate how much mass a star cluster will retain after gas expulsion to within 10% accuracy, no matter how complex the background structure of the gas is, and we present a simple analytical recipe describing this behaviour. We show that the evolution of the star cluster while still embedded in the natal gas, and the behavior of the gas before being expelled, are crucial processes that affect the timescale on which the cluster can evolve into a virialized spherical system. Embedded star clusters that have high levels of substructure are subvirial for longer times, enabling them to survive gas expulsion better than a virialized and spherical system. By using a more realistic treatment for the background gas than our previous studies, we find it very difficult to destroy the young clusters with instantaneous gas expulsion. We conclude that gas removal may not be the main culprit for the dissolution of young star clusters.
description: 19 pages, 8 figures, 2 tables. Accepted for publication in MNRAS