cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
MOESM1 of Linking genotype and phenotype in an economically viable propionic acid biosynthesis process
Creators: name: Luna-Flores, Carlos
name: Stowers, Chris
name: Cox, Brad
name: Nielsen, Lars
name: Marcellin, Esteban
Publisher: name: figshare
Year: 2018
Subjects: subject: Biochemistry
subject: Medicine
subject: Genetics
subject: FOS: Biological sciences
subject: 59999 Environmental Sciences not elsewhere classified
subject: FOS: Earth and related environmental sciences
subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences
subject: 69999 Biological Sciences not elsewhere classified
subject: 19999 Mathematical Sciences not elsewhere classified
subject: FOS: Mathematics
subject: Cancer
subject: Computational Biology

description: Additional file 1: Table S1. Parameters of the fermentations in serum bottles for some strains used in this study.
Multi-View Bayesian Correlated Component Analysis
Creators: name: Kamronn, Simon
name: Poulsen, Andreas Trier
name: Hansen, Lars Kai
Publisher: name: arXiv
Year: 2018
Subjects: subject: Machine Learning (stat.ML)
subject: FOS: Computer and information sciences

description: Correlated component analysis as proposed by Dmochowski et al. (2012) is a tool for investigating brain process similarity in the responses to multiple views of a given stimulus. Correlated components are identified under the assumption that the involved spatial networks are identical. Here we propose a hierarchical probabilistic model that can infer the level of universality in such multi-view data, from completely unrelated representations, corresponding to canonical correlation analysis, to identical representations as in correlated component analysis. This new model, which we denote Bayesian correlated component analysis, evaluates favourably against three relevant algorithms in simulated data. A well-established benchmark EEG dataset is used to further validate the new model and infer the variability of spatial representations across multiple subjects.
ชื่อหมู่บ้านในจังหวัดอุบลราชธานี
Creators: name: กรรณิการ์ สุพิชญ์
Publisher: name: คณะมนุษยศาสตร์และสังคมศาสตร์ มหาวิทยาลัยราชภัฏบ้านสมเด็จเจ้าพระยา
Year: 2021
Subjects: ผู้สูงอายุ
กิจกรรมทางกาย
สมรรถภาพทางกาย
Older Adult
Physical Activity
Physical Fitness

description: วารสารมนุษยศาสตร์และสังคมศาสตร์ มหาวิทยาลัยราชภัฏบ้านสมเด็จเจ้าพระยา, 15, 1, 47-67
MOESM1 of Streak and hierarchical structures of the Tohoku–Hokkaido subduction zone plate boundary
Creators: name: Okuda, Takashi
name: Ide, Satoshi
Publisher: name: figshare
Year: 2018
Subjects: subject: Biochemistry
subject: Space Science
subject: Medicine
subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences
subject: Sociology
subject: FOS: Sociology
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: Developmental Biology
subject: Cancer

description: Additional file 1. Tables S1–S5 and Figures S1–S18.
Atomic Carbon Is a Temperature Probe in Dark Clouds
Creators: name: Tatematsu, K.
name: Jaffe, D. T.
name: Plume, R.
name: Evans, N. J.
name: Keene, J.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We have mapped the C I 3P1-3P0 line at 492 GHzin three molecular clouds immersed in weak ultraviolet radiation fields, TMC-1, L134N, and IC 5146. In all three clouds, the CI peak TA* ~ 1 K, with very small dispersion. The spatial C I distribution is extended and rather smooth. The J = 2-1 transitions of CO isotopomers were observed at the same angular resolution as C I. The C I peak TA* is typically a third of the peak TA* of 13CO J = 2-1, and the C I emission is usually more extended than emission in 13CO or C18O J=2-1. The C I linewidth is close to the 13CO J = 2-1 linewidth, larger than the C18O J = 2-1 line width, and smaller than the 12CO J = 2-1 linewidth. The uniformity of the C I peak TA* is remarkable for a line in the Wien portion of the Planck function and indicates a very uniform excitation temperature. This uniformity is best explained if the line if opaque and thermalized. If so, the CI line probes kinetic temperature in clouds exposed to low ultraviolet fluxes. This conclusion has significant implications for the thermal balance in such clouds. At Av ~ 2, these clouds have a remarkably constant temperature from place to place and from cloud to cloud (7.9+/-0.8 K). Photodissociation region models of clouds immersed in the mean interstellar radiation field tend to predict stronger lines than we see, but this may be an artifact of assumptions about the temperature.
description: 2 pages, 16 PS figures, uses aaspp4.sty; Astrophys. J., in press
title: ADCO, Privilèges de l'Ordre de Cîteaux en matière de succession (Fin XVe siècle), Cart. 176 (11 H 8), f. 0150
Creators: name: de la Côte d'Or, Archives départementales
name: Archives Départementales De La Côte-D'Or
name: Petot, Frédérique
name: Projet CBMA
name: CG21/F.PETOT/2017
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2020
Subjects: subject: cartulaire
subject: Corpus Burgundiae Medii Aevi
subject: Chartes de la Bourgogne du Moyen Âge
subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris

description: Privilèges de l'Ordre de Cîteaux en matière de succession (Fin XVe siècle), Archives départementales de la Côte-d'Or, Cart. 176 (11 H 8), f. 0150, Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Privilèges de l'Ordre de Cîteaux en matière de succession (Fin XVe siècle), Archives départementales de la Côte-d'Or, Cart. 176 (11 H 8), f. 0150, in Projet CBMA - Corpus Burgundiae Medii Aevi [Ressource en ligne], https:// manuscrits.cbma-project.eu/
description: Provenance: https://www.geonames.org/3024876
description: Provenance: http://www.idref.fr/030974844/id
description: Provenance: https://catalogue.bnf.fr/ark:/12148/cb12228351v
description: Provenance: abbaye de Cîteaux
description: Provenance: http://www.wikidata.org/entity/Q843261
Mean fields and fluctuations in compressible magnetohydrodynamic flows
Creators: name: Hollins, J. F.
name: Sarson, G. R.
name: Evirgen, C. C.
name: Shukurov, A.
name: Fletcher, A.
name: Gent, F. A.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We apply Gaussian smoothing to obtain mean magnetic field, density, velocity, and magnetic and kinetic energy densities from our numerical model of the interstellar medium, based on three-dimensional magnetohydrodynamic equations in a shearing box $1 \times 1 \times 2 \, {\rm kpc}$ in size. The interstellar medium is highly compressible, as the turbulence is transonic or supersonic; it is thus an excellent context in which to explore the use of smoothing to represent physical variables in a compressible medium in terms of their mean and fluctuating parts. Unlike alternative averaging procedures, such as horizontal averaging, Gaussian smoothing retains the three-dimensional structure of the mean fields. Although Gaussian smoothing does not obey the Reynolds rules of averaging, physically meaningful and mathematically sound central statistical moments are defined as suggested by Germano (1992). We discuss methods to identify an optimal smoothing scale $\ell$ and the effects of this choice on the results. From spectral analysis of the magnetic, density and velocity fields, we find a suitable smoothing length for all three fields, of $\ell \approx 75 \, {\rm pc}$. Such a smoothing scale is likely to be sensitive to the choice of simulation parameters; this may be considered in future work, but here we just explore the methodology. We discuss the properties of third-order statistical moments in fluctuations of kinetic energy density in compressible flows, and suggest their physical interpretation. The mean magnetic field, amplified by a mean-field dynamo, significantly alters the distribution of kinetic energy in space and between scales, reducing the magnitude of kinetic energy at intermediate scales. This intermediate-scale kinetic energy is a useful diagnostic of the importance of SN-driven outflows.
description: 23 pages, 10 figures. Revised, submitted to Geophysical and Astrophysical Fluid Dynamics
Discovery of a Non-Thermal Galactic Center Filament (G358.85+0.47) Parallel to the Galactic Plane
Creators: name: Lang, Cornelia C.
name: Anantharamaiah, K. R.
name: Kassim, N. E.
name: Lazio, T. J. W.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We report the discovery of a new non-thermal filament, G358.85+0.47, the ``Pelican'', located ~225 pc in projection from SgrA, and oriented parallel to the Galactic plane. VLA continuum observations at 20 cm reveal that this 7' (17.5 pc) structure bends at its northern extension and is comprised of parallel strands, most apparent at its ends. Observations at 6 and 3.6 cm reveal that the Pelican is a synchrotron-emitting source and is strongly linearly polarized over much of its extent. The spectral index of the filament changes from alpha(20/6)=-0.8 to alpha(6/3.6)=-1.5. The rotation measures exhibit a smooth gradient, with values ranging from -1000 rad/m2 to +500 rad/m2. The intrinsic magnetic field is well-aligned along the length of the filament. Based on these properties, we classify the Pelican as one of the non-thermal filaments unique to the Galactic center. Since these filaments (most of which are oriented perpendicular to the Galactic plane) are believed to trace the overall magnetic field in the inner Galaxy, the Pelican is the first detection of a component of this field parallel to the plane. The Pelican may thus mark a transition region of the magnetic field orientation in the inner kiloparsec of the Galaxy.
description: 6 pages, 4 figures, to appear in ApJ Letters; Figs. 2 & 3 are color .ps files and best viewed in color
Supplementary document for Physics-based deep learning for modelling nonlinear pulse propagation in optical fibers - 5942449.pdf
Creators: name: Sui, Hao
name: Zhu, Hongna
name: Luo, Bin
name: Taccheo, Stefano
name: Zou, Xihua
name: Yan, Lianshan
Publisher: name: Optica Publishing Group
Year: 2022
Subjects: Uncategorized

description: Supplemental Document of 460489
The Baryonic and Dark Matter Distributions in Abell 401
Creators: name: Nevalainen, J.
name: Markevitch, M.
name: Forman, W. R.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We combine spatially resolved ASCA temperature data with ROSAT imaging data to constrain the total mass distribution in the cluster A401, assuming that the cluster is in hydrostatic equilibrium. We obtain a total mass within the X-ray core (290/h_50 kpc) of 1.2[+0.1,-0.5] 10^14 /h_50 Msun at the 90% confidence level, 1.3 times larger than the isothermal estimate. The total mass within r_500 (1.7/h_50 Mpc) is M_500 = 0.9[+0.3,-0.2] 10^15/ h_50 Msun at 90% confidence, in agreement with the optical virial mass estimate, and 1.2 times smaller than the isothermal estimate. Our M_500 value is 1.7 times smaller than that estimated using the mass-temperature scaling law predicted by simulations. The best fit dark matter density profile scales as r^{-3.1} at large radii, which is consistent with the Navarro, Frenk & White (NFW) ``universal profile'' as well as the King profile of the galaxy density in A401. From the imaging data, the gas density profile is shallower than the dark matter profile, scaling as r^{-2.1} at large radii, leading to a monotonically increasing gas mass fraction with radius. Within r_500 the gas mass fraction reaches a value of f_gas = 0.21[+0.06,-0.05] h_50^{-3/2} (90% confidence errors). Assuming that f_gas (plus an estimate of the stellar mass) is the universal value of the baryon fraction, we estimate the 90% confidence upper limit of the cosmological matter density to be Omega_m < 0.31.
description: 17 pages, 6 figures, accepted by ApJ
เพลงช้า: ความสำคัญต่อการฝึกหัดสู่การแสดงนาฏศิลป์ไทย (โขนพระ)
Creators: name: พิชญ์ภัทร  ฉายอรุณ
Publisher: name: คณะมนุษยศาสตร์และสังคมศาสตร์ มหาวิทยาลัยราชภัฏบ้านสมเด็จเจ้าพระยา
Year: 2021
Subjects: เพลงช้า
โขนพระ
การฝึกหัด
นาฏศิลป์ไทย
Pleng Cha
Male character in khon
Dance training
Thai classical dance

description: วารสารมนุษยศาสตร์และสังคมศาสตร์ มหาวิทยาลัยราชภัฏบ้านสมเด็จเจ้าพระยา, 15, 1, 68-111
Beta Function Quintessence Cosmological Parameters and Fundamental Constants I: Power and Inverse Power Law Dark Energy Potentials
Creators: name: Thompson, Rodger I.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: This investigation explores using the beta function formalism to calculate analytic solutions for the observable parameters in rolling scalar field cosmologies. The beta function in this case is the derivative of the scalar $ϕ$ with respect to the natural log of the scale factor $a$, $β(ϕ)=\frac{d ϕ}{d \ln(a)}$. Once the beta function is specified, modulo a boundary condition, the evolution of the scalar $ϕ$ as a function of the scale factor is completely determined. A rolling scalar field cosmology is defined by its action which can contain a range of physically motivated dark energy potentials. The beta function is chosen so that the associated "beta potential" is an accurate, but not exact, representation of the appropriate dark energy model potential. The basic concept is that the action with the beta potential is so similar to the action with the model potential that solutions using the beta action are accurate representations of solutions using the model action. The beta function provides an extra equation to calculate analytic functions of the cosmologies parameters as a function of the scale factor that are that are not calculable using only the model action. As an example this investigation uses a quintessence cosmology to demonstrate the method for power and inverse power law dark energy potentials. An interesting result of the investigation is that the Hubble parameter H is almost completely insensitive to the power of the potentials and that $Λ$CDM is part of the family of quintessence cosmology power law potentials with a power of zero.
description: Accepted for publication by the Monthly Notices of the Royal Astronomical Society
Poisson-Arago spot for gravitational waves
Creators: name: Hongsheng, Zhang
name: Xilong, Fan
Publisher: name: arXiv
Year: 2018
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: For the observer at infinity, a Schwarzschild black hole serves as an attractive opaque disk with a radius of 3$\sqrt{3} M$ that will produce the diffraction pattern of gravitational waves (GWs). In this study, we demonstrate that a bright spot, which is a diffraction effect analogous to the Poisson-Arago spot in optics, will appear when an ingoing (quasi-) plane GW is diffracted by a Schwarzschild black hole. Here, we propose the diffraction effect of the GWs described by the exact diffraction solution of the GWs using the Heun function. For the first time, the Fresnel half-wave zone method is proposed to calculate the angular part of the GW scattering stripes for the observer at infinity. The prospect of observing the diffraction bright spot is discussed with an eikonal approximation. For normal incidence (quasi)-plane waves with 100 Hz (0.1 Hz) frequency diffracted by the central black hole of the Milky Way, the time delay between the Earth bathed in a bright spot and the minimum of the first dark stripe is 3.86 (3860) days. We will witness the second bright fringe (40% amplitude of the central bright spot) after 6.2 (6200) days. This new diffraction pattern involving the early phase of inspirals and pulsars as continuous gravitational wave sources is a potential scientific target for future space-and ground-based gravitational wave detectors, respectively.
Three views of a saleroom. Valorization in and valuation of visual artworks by (mostly) Watteau, Altman and Banksy
Creators: name: Hutter, Michael
Publisher: name: Journal for Art Market Studies
Year: 2021

description: In the European tradition, markets have usually been represented as the place where the actual, live exchanges take place. The article therefore focuses on saleroom representations. These affect their own artistic value in two ways, leading to two questions: in a first move, the saleroom is an artistic device. How does the artist, or those who collaborate in creating an artwork, use references to a saleroom in order to put value into the work, to enrich it and thus contribute to its valorization? In a second move, spectators attribute value to the work, and they assess its value in comparison with that of other, similar works, and they pay money to possess works. How do they react to the use of the saleroom, what part does it play in their valuation of a particular work? To explore these questions, three works were selected: Antoine Watteau’s Shopsign of the art dealer Gersaint is a fictitious version of the dealer’s showroom; Robert Altman’s film Vincent and Theo opens with the Christie’s auction sale of one of Van Gogh’s Vase with sunflowers paintings and goes on to recapitulate the relationship between Vincent and his brother Theo; Banksy’s 2006 canvas version of Girl with Balloon, half-shreddered during its Sotheby’s auction sale and renamed Love is in the Bin, was applauded as the first artwork to be created during an auction event. Salerooms, however, show only one part of art markets. The conditions of production as well as the drives that shape consumption remain unnoticed. They would require other forms of representation and conceptualization. Salerooms are also an unlikely conceptual device to show features of political domination. And yet, the three works contain quite explicit references to this sphere of value.
description: Journal for Art Market Studies, Vol. 5 No. 1 (2021): Representing the Art Market
MOESM1 of Signaling of High Mobility Group Box 1 (HMGB1) through Toll-like Receptor 4 in Macrophages Requires CD14
Creators: name: Kim, Sodam
name: Kim, Sun
name: Pribis, John
name: Lotze, Michael
name: Mollen, Kevin
name: Shapiro, Richard
name: Loughran, Patricia
name: Scott, Melanie
name: Billiar, Timothy
Publisher: name: figshare
Year: 2013
Subjects: subject: Cell Biology
subject: Neuroscience
subject: Immunology
subject: FOS: Clinical medicine
subject: Inorganic Chemistry
subject: FOS: Chemical sciences
subject: Science Policy
subject: Mental Health

description: Supplementary material, approximately 2.27 MB.
Stability of boron-doped graphene/copper interface: DFT, XPS and OSEE studies
Creators: name: Boukhvalov, D. W.
name: Zhidkov, I. S.
name: Kukharenko, A. I.
name: Slesarev, A. I.
name: Zatsepin, A. F.
name: Cholakh, S. O.
name: Kurmaev, E. Z.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Materials Science (cond-mat.mtrl-sci)
subject: Applied Physics (physics.app-ph)
subject: Chemical Physics (physics.chem-ph)
subject: FOS: Physical sciences

description: Two different types of boron-doped graphene/copper interfaces synthesized using two different flow rates of Ar through the bubbler containing the boron source were studied. X-ray photoelectron spectra (XPS) and optically stimulated electron emission (OSEE) measurements have demonstrated that boron-doped graphene coating provides a high corrosion resistivity of Cu-substrate with the light traces of the oxidation of carbon cover. The density functional theory calculations suggest that for the case of substitutional (graphitic) boron-defect only the oxidation near boron impurity is energetically favorable and creation of the vacancies that can induce the oxidation of copper substrate is energetically unfavorable. In the case of non-graphitic boron defects oxidation of the area, a nearby impurity is metastable that not only prevent oxidation but makes boron-doped graphene. Modeling of oxygen reduction reaction demonstrates high catalytic performance of these materials.
description: 15 pages, 8 figures, to appear in Appl. Surf. Sci
Additional file 1: of Connexin 30 deficiency attenuates A2 astrocyte responses and induces severe neurodegeneration in a 1-methyl-4-phenyl-1,2,3,6-tetrahydropyridine hydrochloride Parkinson’s disease animal model
Creators: name: Fujita, Atsushi
name: Yamaguchi, Hiroo
name: Yamasaki, Ryo
name: Yiwen Cui
name: Matsuoka, Yuta
name: Ken-Ichi Yamada
name: Jun-Ichi Kira
Publisher: name: figshare
Year: 2018
Subjects: subject: Biochemistry
subject: Medicine
subject: Cell Biology
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Neuroscience
subject: Immunology
subject: FOS: Clinical medicine
subject: 110309 Infectious Diseases
subject: FOS: Health sciences
subject: Computational Biology

description: Figure S1. Western blots of Cx30 on day 1. Figure S2. Western blots of Cx30 on day 7. Figure S3. Effects of MPTP on Cx30 expression in SNc. (a, b) Upper panels: triple immunostaining on days 1 (a) and 7 (b). Lower panels: enlarged images inwhite boxes. Scale bars: upper panels, 100 μm; lower panels, 50 μm. Figure S4. Cx30 (green) and GFAP(red)immunostaining in striatum and SN. Scale bars: 100 μm. Figure S5. Effects of MPTP on Cx43 expression in SNc. Left two columns: triple immunostainingon days 1 (a) and 7 (b). Right two columns show enlarged images inwhite boxes. Scale bars: left two columns, 100 μm; right two columns, 50 μm. Figure S6. Effects of MPTP on Cx43 expression. (a, b) Number of Cx43-immunoreactive dots. (c, d) RT-PCR analysis of Cx43 mRNA levels. (e, f) Western blot analysis of Cx43 protein levels. Blot images in Figure S2. Figure S7. Western blots of Cx43 on days 1 and 7. Figure S8. Western blots of Cx43 on day 7. Figure S9. MPP+ concentration. Figure S10. DAT immunostaining (a) and quantification of DAT-positive fibre density (b). Scale bar: 50 μm. Figure S11. Heatmap of A1, A2, and pan-reactive astrocyte gene expression. Figure S12. Western blotsof GFAP. Figure S13. Heatmap of M1, M2, and M1/M2 mixed microglia gene expression. Figure S14. KEGG pathway map of the axon guidance pathway. Figure S15. Microarray expression dataofaxon guidance pathway-related genes. (a) Scatter plots. (b) Heatmap. Table S1. Antibodies used for immunohistochemistry. Table S2. Primers used for ISH. Table S3. Gene names indicated by red dots in Fig. 6. Table S4. Gene names indicated by red dots in Fig. 11. Table S5. KEGG pathway analysis of microarray data. Table S6. Gene names indicated by red dots in Additional file 1: Figure S15a. (DOCX 100840 kb)
"Twice as valuable as that of Eumorphopulos and twice as famous..." (Vita Sackville-West, All Passion Spent, 1931) - The real and imaginary world of the Chinese art collector
Creators: name: Pearce, Nick
Publisher: name: Journal for Art Market Studies
Year: 2021

description: The period between about 1900 and 1937 witnessed the opening up of an international market in Chinese artefacts at a time when China was vulnerable to encroachment and, after 1911 with the fall of the last imperial dynasty, was in political, social and economic turmoil. During the post-WW1 decades the visibility of the country and its cultural history also stimulated an academic and popular interest in Chinese material culture of all types and periods, but particularly burial objects being unearthed through railway construction (bronzes, jades and ceramics), which initiated both legal and illegal excavations and the market circulation of collections formerly owned by the Chinese élite. These opportunities to 'collect' ended only with the outbreak of the Sino-Japanese War in 1937, when access to China was severely curtailed. In this article, I will focus on the way in which the visibility of these collectors impacted upon popular culture of the inter-war period, particularly the novel. Referencing actual collectors against their fictional counterparts offers an intriguing insight into character, motivation and the market for Chinese works of art at the time. Indeed the eccentricity and flamboyance of a number of real collectors made them ideal material for the writers of fiction.
description: Journal for Art Market Studies, Vol. 5 No. 1 (2021): Representing the Art Market
On the anomalous X-ray afterglows of GRB 970508 and GRB 970828
Creators: name: Vietri, M.
name: Perola, C.
name: Piro, L.
name: Stella, L.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Recently, BeppoSAX and ASCA have reported an unusual resurgence of soft X-ray emission during the afterglows of GRB 970508 and GRB 970828, together with marginal evidence for the existence of Fe-lines in both objects. We consider the implications of the existence of a torus of iron-rich material surrounding the sites of gamma ray bursts as would be expected in the SupraNova model; in particular, we show that the fireball will quickly hit this torus, and bring it to a temperature ~3x10^7 K. Bremsstrahlung emission from the heated up torus will cause a resurgence of the soft X-ray emission with all expected characteristics (flux level, duration and spectral hardening with time) identical to those observed during the reburst. Also, thermal emission from the torus will account for the observed iron line flux. These events are also observable, for instance by new missions such as SWIFT, when beaming away from our line sight makes us miss the main burst, as Fast (soft) X-ray Transients, with durations ~10^3 s, and fluences ~10^-7-10^-4 erg cm^-2. This model provides evidence in favor of the SupraNova model for Gamma Ray Bursts.
description: To appear in MN Pink pages, MN-LateX, no figures
Inverting the Angular Correlation Function
Creators: name: Dodelson, Scott
name: Gaztanaga, Enrique
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: The two point angular correlation function is an excellent measure of structure in the universe. To extract from it the three dimensional power spectrum, one must invert Limber's Equation. Here we perform this inversion using a Bayesian prior constraining the smoothness of the power spectrum. Among other virtues, this technique allows for the possibility that the estimates of the angular correlation function are correlated from bin to bin. The output of this technique are estimators for the binned power spectrum and a full covariance matrix. Angular correlations mix small and large scales but after the inversion, small scale data can be trivially eliminated, thereby allowing for realistic constraints on theories of large scale structure. We analyze the APM catalogue as an example, comparing our results with previous results. As a byproduct of these tests, we find -- in rough agreement with previous work -- that APM places stringent constraints on Cold Dark Matter inspired models, with the shape parameter constrained to be $0.25\pm 0.04$ (using data with wavenumber $k \le 0.1 h{\rm Mpc}^{-1}$). This range of allowed values use the full power spectrum covariance matrix, but assumes negligible covariance in the off-diagonal angular correlation error matrix, which is estimated with a large angular resolution of 0.5degrees (in the range 0.5 and 20 degrees).
description: 7 pages, 11 figures, replace to match accepted version, MNRAS in press
CloudForest: An integrated and dynamic phylogenomic toolset for the modern age
Creators: name: Toups, Benjamin S
name: Wilgenbusch, James C.
name: McGowan, Thomas
name: Brown, Jeremy M.
name: Gallivan, Kyle A.
Publisher: name: F1000 Research Limited
Year: 2020

description: Variation across inferred gene trees is arguably the most consistent and striking observation from empirical phylogenomic studies, yet many unanswered questions remain about the causes of this variation. One important reason these questions persist is because the field lacks robust, efficient, and reproducible workflows for investigating this variation. To meet this need, we are developing a portable cyberinfrastructure framework called CloudForest. CloudForest will provide researchers with a set of streamlined and integrated tools to explore the structure of large phylogenetic tree sets, including those generated by phylogenomic studies. CloudForest will meet many of the outstanding needs of empirical phylogenomic studies, such as (1) visualizing variation across gene trees, (2) revealing structure in sets of trees (forests), (3) conducting hypothesis tests regarding the causes of gene-tree variation, and (4) detecting genes that may have outlying (and potentially aberrant) histories. By addressing these challenges in a consistent way across computing platforms that range from a desktop computer to university high-performance computing systems to commercial cloud computing, CloudForest will allow biologists to make efficient use of any computational resources at their disposal with workflows appropriate for addressing a variety of important, unresolved questions in both evolutionary biology and other applied fields.
Dynamics of a Disoriented Chiral Condensate
Creators: name: Blaizot, J. P.
name: Krzywicki, A.
Publisher: name: arXiv
Year: 1994
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We use the linear $σ$ model to analyse the dynamics of a disoriented chiral condensate. For idealized boundary conditions appropriate to high energy collisions, the problem can be reduced to a one dimensional one. The evolution of the chiral state is then that of a simple dynamical system and can be studied analytically.
description: 14 pages Latex, LPTHE Orsay 94/18 , SPhT T94/019
Interaction of Individual Skyrmions in Nanostructured Cubic Chiral Magnet
Creators: name: Du, H.
name: Zhao, X.
name: Rybakov, F. N.
name: Borisov, A. B.
name: Wang, S.
name: Tang, J.
name: Jin, C.
name: Wang, C.
name: Wei, W.
name: Kiselev, N. S.
name: Zhang, Y.
name: Che, R.
name: Blügel, S.
name: Tian, M.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: FOS: Physical sciences

description: We report the direct evidence of field-dependent character of the interaction between individual magnetic skyrmions as well as between skyrmions and edges in B20-type FeGe nanostripes observed by means of high resolution Lorentz transmission electron microscopy. It is shown that above certain critical values of external magnetic field the character of such long-range skyrmion interactions change from attraction to repulsion. Experimentally measured equilibrium inter-skyrmion and skrymion-edge distances as function of applied magnetic field shows quantitative agreement with the results of micromagnetic simulations. Important role of demagnetizing fields and internal symmetry of three-dimensional magnetic skyrmions are discussed in details.
description: accepted in PRL
(Con)Artistic Strategies for How to Succeed in the Art Market
Creators: name: Schon, Bernd Friedrich
Publisher: name: Journal for Art Market Studies
Year: 2021

description: In today’s fast-paced art market environment, uncertainty is rampant as to whether works of art are of lasting value, especially contemporary ones. In popular imagination, this gives rise to the fear that many an artist could be nothing more than an impostor who is primarily interested in enriching himself. Within cultural representation, so the artist’s "authenticity“ and "originality” become the most important resources for building trust. The examination of Orson Welles‘ F for Fake and Banksy’s Exit through the Gift Shop shows how artists articulate their own authenticity, originality credibility, and thus their trustworthiness – and how they distinguish themselves to counterfeiters, impostors, and fraudsters. Furthermore, it becomes obvious that both artists and impostors – at least as they’re represented – (have to) use similar strategies in order to be successful. Both films also reveal tectonic changes in the art market from the 1970s until today: whereas in the past market access used to be achieved exclusively via experts and specialists who had to be convinced or deceived by means of outstanding craftmanship, their influence on the contemporary art market now appears to have diminished. Instead, the purposeful generation of attention through spectacle, the intelligent utilization of social relationships to key figures and the skilful manipulation of the media have become indispensable. This results in the fact that art forgers now can sell their own “original” and “authentic” forgeries at notable prices.
description: Journal for Art Market Studies, Vol. 5 No. 1 (2021): Representing the Art Market
Closing the Universe by relaxing the cosmological constant
Creators: name: Lopez, J.
name: Nanopoulos, D.
Publisher: name: arXiv
Year: 1994
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: Astrophysics (astro-ph)
subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We propose a string-inspired model which correlates several aspects of particle physics and cosmology. Inspired by the flat directions and the absence of adjoint Higgs representations found in typical string models, we consider a no-scale $SU(5)\times U(1)$ supergravity model. This model entails well determined low-energy phenomenology, such as the value of the neutralino dark matter relic abundance and a negative contribution to the vacuum energy. A positive contribution to the vacuum energy is also typically present in string theory as a consequence of the running of the fundamental constants towards their fixed point values. If these two contributions cancel appropriately, one may end up with a vacuum energy which brings many cosmological observations into better agreement with theoretical expectations. The present abundance of neutralinos would then be fixed. We delineate the regions of parameter space allowed in this scenario, and study the ensuing predictions for the sparticle and Higgs-boson masses in this model.
description: 5 pages, 2 figures (included), Latex, CTP-TAMU-06/94
title: ADCO, Neuvième cartulaire de Saint-Étienne de Dijon (1661 - 1684), Cart. 32 (G 136), 745 folios, f. 1289
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: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris
subject: Corpus Burgundiae Medii Aevi
subject: Chartes de la Bourgogne du Moyen Âge
subject: cartulaire

description: Neuvième cartulaire de Saint-Étienne de Dijon (1661 - 1684), Archives départementales de la Côte-d'Or, Cart. 32 (G 136), 745 folios, f. 1289, Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Neuvième cartulaire de Saint-Étienne de Dijon (1661 - 1684), Archives départementales de la Côte-d'Or, Cart. 32 (G 136), 745 folios, f. 1289, 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
The 16\half-N_f Expansion and the Infrared Fixed Point in Perturbative QCD
Creators: name: Stevenson, P. M.
Publisher: name: arXiv
Year: 1994
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: In QCD with 16\half-epsilon massless quark flavours there is an infrared fixed point with alpha_s/pi = (8/321)epsilon in the limit epsilon -> 0+. I develop the idea of Banks and Zaks to expand about N_f=16\half. This expansion is certainly useful for N_f=16, 15, 14, ..., and arguably it can reach the phenomenologically interesting case N_f=2, where it suggests that alpha_s/pi "freezes" to a value of order of magnitude 0.4 in the infrared.
description: 10 pages, LaTeX. 3 figures (see top of file). Revised version; some extra discussion. (To appear in Phys. Lett. B.) DE-FG05-92ER40717-12
An improved sum-product bound for quaternions
Creators: name: Basit, Abdul
name: Lund, Ben
Publisher: name: arXiv
Year: 2018
Subjects: subject: Combinatorics (math.CO)
subject: FOS: Mathematics

description: We show that there exists an absolute constant $c > 0$, such that, for any finite set $A$ of quaternions, \[ \max\{|A+A, |AA| \} \gtrsim |A|^{4/3 + c}. \] This generalizes a sum-product bound for real numbers proved by Konyagin and Shkredov.
description: Appeared in SIAM J. Discrete Math. This version corrects some errors from the previous version, and clarifies the analysis
Spiral galaxy distance indicators based on near-infrared photometry
Creators: name: de Grijs, R.
name: Peletier, R. F.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We compare two methods of distance determination to spiral galaxies using optical/near-infrared (NIR) observations, the (I-K) versus M_K colour - absolute magnitude (CM) relation and the I and K-band Tully-Fisher relation (TFR). Dust-free colours and NIR absolute magnitudes greatly enhance the usefulness of the NIR CM relation as a distance indicator for moderately to highly inclined_spiral_ galaxies_in the field_ (inclinations between ~ 80 and 90 deg); by avoiding contamination by dust the scatter in the CM relation is significantly reduced, compared to similar galaxy samples published previously. The CM relation can be used to determine distances to field spiral galaxies with M_K > -25.5, to at least M_K ~ -20. Our results, supplemented with previously published observations for which we can - to some degree - control the effects of extinction, are consistent with a universal nature of the CM relation for field spiral galaxies. High-resolution observations done with the Hubble Space Telescope can provide a powerful tool to calibrate the relation and extend the useful distance range by more than a factor of 2 compared to ground-based observations. The intrinsic scatter in the NIR CM relation in the absolute K-band magnitudes is ~0.5 mag, yielding a lower limit to the accuracy of distance determinations on the order of 25%. Although we find an unusually low scatter in the TFR (probably a statistical accident), a typical scatter in the TFR would yield distances to our sample galaxies with uncertainties of only about 15%. However, one of the main advantages of the use of the NIR CM relation is that_we only need photometric data_ to obtain distance estimates; use of the TFR requires additional kinematic data, although it can be used to significantly greater distances.
description: 12 pages, incl. 5 postscript files, LaTeX, accepted for publication in MNRAS
MOESM9 of Loss of SETDB1 decompacts the inactive X chromosome in part through reactivation of an enhancer in the IL1RAPL1 gene
Creators: name: Sun, Zhuo
name: Chadwick, Brian
Publisher: name: figshare
Year: 2018
Subjects: subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Immunology
subject: FOS: Clinical medicine
subject: Developmental Biology
subject: Science Policy
subject: Hematology
subject: 110309 Infectious Diseases
subject: FOS: Health sciences

description: Additional file 9. IL1RAPL1 RNA FISH data for the BACs indicated in the cells listed. Xi expression is defined as a single associated with the XIST RNA cloud. Each column represents data from replicate experiments. Therefore, a clone with BAC data in two columns indicates that the experiment was done twice, whereas that in four columns indicates the experiment was done on four occasions
Meson Structure in Deep Inelastic Scattering
Creators: name: Shigetani, T.
name: Suzuki, K.
name: Toki, H.
Publisher: name: arXiv
Year: 1994
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We study the deep inelastic structure functions of mesons within the Nambu and Jona-Lasinio model. We calculate the valence quark distributions in $π$, $K $, and $ρ$ mesons at the low energy model scale, which are evoluted to the experimental momentum scale in terms of the Altarelli-Parisi equation. The resulting distribution functions show reasonable agreements with experiment. We also discuss the semi-inclusive lepton nucleon scattering process with a slow nucleon in coincidence in the final state, which reveals the off-shell structure of the pion.
description: 31 pages with 16 figures as uuencoded postscript files, TMU-NT-940101 (plain LaTeX)
CloudForest: An integrated and dynamic phylogenomic toolset for the modern age
Creators: name: Toups, Benjamin S
name: McGowan, Thomas
name: Brown, Jeremy M.
name: Gallivan, Kyle A.
name: Wilgenbusch, James C.
Publisher: name: F1000 Research Limited
Year: 2020

description: Variation across inferred gene trees is arguably the most consistent and striking observation from empirical phylogenomic studies, yet many unanswered questions remain about the causes of this variation. One important reason these questions persist is because the field lacks robust, efficient, and reproducible workflows for investigating this variation. To meet this need, we are developing a portable cyberinfrastructure framework called CloudForest. CloudForest will provide researchers with a set of streamlined and integrated tools to explore the structure of large phylogenetic tree sets, including those generated by phylogenomic studies. CloudForest will meet many of the outstanding needs of empirical phylogenomic studies, such as (1) visualizing variation across gene trees, (2) revealing structure in sets of trees (forests), (3) conducting hypothesis tests regarding the causes of gene-tree variation, and (4) detecting genes that may have outlying (and potentially aberrant) histories. By addressing these challenges in a consistent way across computing platforms that range from a desktop computer to university high-performance computing systems to commercial cloud computing, CloudForest will allow biologists to make efficient use of any computational resources at their disposal with workflows appropriate for addressing a variety of important, unresolved questions in both evolutionary biology and other applied fields.
Abstraction Principles and the Classification of Second-Order Equivalence Relations
Creators: name: Ebels-Duggan, Sean C.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Logic (math.LO)
subject: FOS: Mathematics

description: This paper improves two existing theorems of interest to neo-logicist philosophers of mathematics. The first is a classification theorem due to Fine for equivalence relations between concepts definable in a well-behaved second-order logic. The improved theorem states that if an equivalence relation $E$ is defined without non-logical vocabulary, then the bicardinal slice of any equivalence class---those equinumerous elements of the equivalence class with equinumerous complements---can have one of only three profiles. The improvements to Fine's theorem allow for an analysis of the well-behaved models had by an abstraction principle, and this in turn leads to an improvement of Walsh and Ebels-Duggan's relative categoricity theorem.
Akn 564: an unusual component in the X-ray spectra of NLSy1 galaxies
Creators: name: Turner, T. J.
name: George, I. M.
name: Netzer, Hagai
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present an ASCA observation of the NLSy1 Ark 564. The X-ray light curve shows rapid variability, but no evidence for energy-dependence to these variations, within the 0.6 -- 10 keV bandpass. A strong (EW ~ 70 eV) spectral feature is observed close to 1 keV. A similar feature has been observed in TON S180 (another NLSy1) but has not been observed in broad-line Seyfert galaxies. The feature energy suggests a large contribution from Fe L-shell lines but its intensity is difficult to explain in terms of emission and/or absorption from photoionized gas. Models based on gas in thermal equilibrium with kT ~1 keV provide an alternative parameterization of the soft spectrum. The latter may be interpreted as the hot intercloud medium, undergoing rapid cooling and producing strong Fe L-shell recombination lines. In all cases the physical conditions are rather different from those observed in broad-line Seyferts. The hard X-ray spectrum shows a broad and asymmetric Fe Kalpha line of large equivalent width (~550 eV) which can be explained by a neutral disk viewed at ~ 60 degrees to the line-of-sight, contrary to the hypothesis that NLSy1s are viewed pole-on. The large EW of this line, the strong 1 keV emission and the strong optical Fe emission lines all suggest an extreme Fe abundance in this and perhaps other NLSy1s.
description: 15 pages, 5 figures. LaTeX with encapsulated postscript. Accepted for publication in the Astrophysical Journal
Violence, Globalization and the Trade in "ethnographic" Artefacts in nineteenth-century Sudan
Creators: name: Cormack, Zoe
Publisher: name: Journal for Art Market Studies
Year: 2020

description: This article explores the links between African artefacts in European museum collections and the slave and ivory trade in Sudan in the nineteenth century. It examines how ‘ethnographic’ collections were acquired from southern Sudan and how this process was entangled with the expansion of predatory commerce. Presenting evidence from contemporary travel accounts, museum archives and from the examination of objects themselves, I argue that the nineteenth-century trade in artefacts from South Sudan was inseparable from a history of enslavement and extraction. This evidence from Sudan illuminates the relationship between collecting artefacts in Africa and other markets. It shows how collecting interests intersected with Ottoman and European imperial networks in Sudan and helps to better understand the history of African collections in European museums.
description: Journal for Art Market Studies, Vol. 4 No. 1 (2020)
Kaiser Family Foundation Poll: Public Opinion and Knowledge on Reproductive Health Policy
Creators: name: Kaiser Family Foundation
Publisher: name: Roper Center for Public Opinion Research
Year: 2019

description: Knowledge about the Affordable Care Act (ACA) (6); importance of federal funding for reproductive health services (1); federal funding going to organizations that take part in various activities (6); Planned Parenthood funding (3); funding can/cannot be used to pay for abortions (1); funding for foreign groups that provide counseling/referrals for abortions (2); Roe vs. Wade (2); ban on abortions once fetal heartbeat is detected (2); abstinence-only education (1); teenagers receiving confidential health services without parental involvement (1); health insurance coverage (4); health status (1); ever visited Planned Parenthood clinic for health care (1); registered to vote (1); President Donald Trump job performance (1).
Additional file 1 of Histological criteria for selecting patients who need clonality test for non-gastric MALT lymphoma diagnosis
Creators: name: Park, Dajeong
name: Cho, Junhun
Publisher: name: figshare
Year: 2024
Subjects: subject: Space Science
subject: Medicine
subject: Genetics
subject: FOS: Biological sciences
subject: Biotechnology
subject: Environmental Sciences not elsewhere classified
subject: Biological Sciences not elsewhere classified
subject: Information Systems not elsewhere classified
subject: Cancer
subject: Inorganic Chemistry
subject: FOS: Chemical sciences
subject: Hematology
subject: Plant Biology

description: Supplementary Material 1