cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Phalaena quadra Linnaeus, 1758, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1758
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Lepidoptera
Noctuidae
Phalaena
Phalaena quadra

description: Phalaena quadra [spec. nov.]
P. Noctua seticornis laevis, alis depressis luteis: superioribus punctis duobus atris.
Roes. ins. 1. phal. 2. t. 17.
Wilk. pap. 24. t. 3. a. 17.
Habitat in Pinu, Quercu.
Larva pilosa dorso punctis rubris maculaque nigra; lateribus lineis nigris. Phalaena in multis accedit phalangi Tinearum.
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 511, DOI: 10.5962/bhl.title.542, http://zenodo.org/record/3922206
Discovery of large-scale diffuse radio emission in low-mass galaxy cluster Abell 1931
Creators: name: Brüggen, M.
name: Rafferty, D.
name: Bonafede, A.
name: van Weeren, R. J.
name: Shimwell, T.
name: Intema, H.
name: Röttgering, H.
name: Brunetti, G.
name: Di Gennaro, G.
name: Savini, F.
name: Wilber, A.
name: O'Sullivan, S.
name: Ensslin, T. A.
name: De Gasperin, F.
name: Hoeft, M.
Publisher: name: arXiv
Year: 2018
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: Extended, steep-spectrum radio synchrotron sources are pre-dominantly found in massive galaxy clusters as opposed to groups. LOFAR Two-Metre Sky Survey images have revealed a diffuse, ultra-steep spectrum radio source in the low-mass cluster Abell 1931. The source has a fairly irregular morphology with a largest linear size of about 550 kpc. The source is only seen in LOFAR observations at 143 MHz and GMRT observations at 325 MHz. The spectral index of the total source between 143 MHz and 325 MHz is $α_{143}^{325} = -2.86 \pm 0.36$. The source remains invisible in Very Large Array (1-2 GHz) observations as expected given the spectral index. Chandra X-ray observations of the cluster revealed a bolometric luminosity of $L_X = (1.65 \pm 0.39) \times 10^{43}$ erg s$^{-1}$ and a temperature of $2.92_{-0.87}^{+1.89}$ keV which implies a mass of around $\sim 10^{14} M_{\odot}$. We conclude that the source is a remnant radio galaxy that has shut off around 200 Myr ago. The brightest cluster galaxy, a radio-loud elliptical galaxy, could be the source for this extinct source. Unlike remnant sources studied in the literature, our source has a steep spectrum at low radio frequencies. Studying such remnant radio galaxies at low radio frequencies is important for understanding the scarcity of such sources and their role in feedback processes.
description: MNRAS, in press
Disorder Induced Phase Transition in a Random Quantum Antiferromagnet
Creators: name: Sandvik, Anders W.
name: Vekic, Marco
Publisher: name: arXiv
Year: 1994
Subjects: subject: Condensed Matter (cond-mat)
subject: FOS: Physical sciences

description: A two-dimensional Heisenberg model with random antiferromagnetic nearest-neighbor exchange is studied using quantum Monte Carlo techniques. As the strength of the randomness is increased, the system undergoes a transition from an antiferromagnetically ordered ground state to a gapless disordered state. The finite-size scaling of the staggered structure factor and susceptibility is consistent with a dynamic exponent $z = 2$.
description: Revtex 3.0, 10 pages + 5 postscript figures available upon request, UCSBTH-94-16
Optimizing CNN Model Inference on CPUs
Creators: name: Liu, Yizhi
name: Wang, Yao
name: Yu, Ruofei
name: Li, Mu
name: Sharma, Vin
name: Wang, Yida
Publisher: name: arXiv
Year: 2018
Subjects: subject: Distributed, Parallel, and Cluster Computing (cs.DC)
subject: FOS: Computer and information sciences

description: The popularity of Convolutional Neural Network (CNN) models and the ubiquity of CPUs imply that better performance of CNN model inference on CPUs can deliver significant gain to a large number of users. To improve the performance of CNN inference on CPUs, current approaches like MXNet and Intel OpenVINO usually treat the model as a graph and use the high-performance libraries such as Intel MKL-DNN to implement the operations of the graph. While achieving reasonable performance on individual operations from the off-the-shelf libraries, this solution makes it inflexible to conduct optimizations at the graph level, as the local operation-level optimizations are predefined. Therefore, it is restrictive and misses the opportunity to optimize the end-to-end inference pipeline as a whole. This paper presents \emph{NeoCPU}, a comprehensive approach of CNN model inference on CPUs that employs a full-stack and systematic scheme of optimizations. \emph{NeoCPU} optimizes the operations as templates without relying on third-parties libraries, which enables further improvement of the performance via operation- and graph-level joint optimization. Experiments show that \emph{NeoCPU} achieves up to 3.45$\times$ lower latency for CNN model inference than the current state-of-the-art implementations on various kinds of popular CPUs.
description: 15 pages, 4 figures, published at USENIX ATC '19
Supplementary text from Detection of HIV transmission clusters from phylogenetic trees using a multi-state birth–death model
Creators: name: Barido-Sottani, Joëlle
name: Vaughan, Timothy G.
name: Stadler, Tanja
Publisher: name: The Royal Society
Year: 2018
Subjects: subject: 60102 Bioinformatics
subject: FOS: Computer and information sciences
subject: Computational Biology

description: Supplementary methods, results and figures.
Additional file 3 of Elevated methylation of the vault RNA2-1 promoter in maternal blood is associated with preterm birth
Creators: name: You, Young-Ah
name: Kwon, Eun Jin
name: Hwang, Han-Sung
name: Choi, Suk-Joo
name: Choi, Sae Kyung
name: Kim, Young Ju
Publisher: name: figshare
Year: 2021
Subjects: subject: Genetics
subject: FOS: Biological sciences

description: Additional file 3: Table S3. Primer set for pyrosequencing designed by the PSQ Assay Design software.
title: ADCO, Neuvième cartulaire de Saint-Étienne de Dijon (1661 - 1684), Cart. 32 (G 136), 745 folios, f. 0055
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. 0055, 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. 0055, 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
Star Formation Histories from HST Color-Magnitude Diagrams of Six Fields of the LMC
Creators: name: Olsen, Knut A. G.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present results on the analysis of background field stars found in HST WFPC2 observations of six of the old globular clusters of the Large Magellanic Cloud. Treated as contaminants by the globular cluster analysts, we produce V-I,V color-magnitude diagrams of the field stars and use them to explore the LMC's star formation history. The photometry approaches V~26, well below the turnoff of an ancient ~14 Gyr LMC population of stars. We use a maximum-likelihood technique to fit model CMDs drawn from Bertelli et al. (1994) isochrones to the observed CMDs. We constrain the models by the age-metallicity relation derived from LMC clusters, test four IMF slopes, and fit for the reddening, distance modulus, and star formation rate. We find that we can just resolve structure in SFR(t) with time steps of ~0.15 in log age, implying a resolution of ~4x10^8 years at an age of 1 Gyr. For a Salpeter IMF, our derived star formation history for the NGC 1754 field is characterized by an enhanced star formation rate over the past 4 Gyr, qualitatively resembling that derived by others for a variety of LMC fields. The remaining four fields, however, appear to have had high levels of star formation activity as long as 5-8 Gyr ago; these fields lie in the LMC Bar while the NGC 1754 field lies in the disk, suggesting that the inner regions of the LMC contain significantly more older stars than the outer regions. Examining the residuals of the models and observations, we find that the old red giant branches of the models provide a poor fit to the observations, which suggests an error in the model isochrones. The effect of the disagreement appears to be to underestimate the contribution of the old population.
description: 48 pages, 19 Postscript figures, LaTeX, accepted by the Astronomical Journal
Supertrace formulae for nonlinearly realized supersymmetry
Creators: name: Murli, Divyanshu
name: Yamada, Yusuke
Publisher: name: arXiv
Year: 2018
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We derive the general supertrace formula for a system with $N$ chiral superfields and one nilpotent chiral superfield in global and local supersymmetry. The nilpotent multiplet is realized by taking the scalar-decoupling limit of a chiral superfield breaking supersymmetry spontaneously. As we show, however, the modified formula is not simply related to the scalar-decoupling limit of the supertrace in linearly-realized supersymmetry. We also show that the supertrace formula reduces to that of a linearly realized supersymmetric theory with a decoupled sGoldstino if the Goldstino is the fermion in the nilpotent multiplet.
description: 14 pages
Chemically-dissected rotation curves of the Galactic Bulge from Main Sequence proper motions
Creators: name: Clarkson, William I.
name: Calamida, Annalisa
name: Sahu, Kailash C.
name: Brown, Thomas M.
name: Gennaro, Mario
name: Avlia, Roberto
name: Valenti, Jeff A.
name: Debattista, Victor P.
name: Rich, R. Michael
name: Minniti, Dante
name: Zoccali, Manuela
name: Aufdemberge, Emily R.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: Instrumentation and Methods for Astrophysics (astro-ph.IM)
subject: FOS: Physical sciences

description: We report results from an exploratory study implementing a new probe of Galactic evolution using archival Hubble Space Telescope imaging observations. Precise proper motions are combined with photometric relative metallicity and temperature indices, to produce the proper motion rotation curves of the Galactic bulge separately for metal-poor and metal-rich Main Sequence samples. This provides a "pencil-beam" complement to large-scale wide-field surveys, which to-date have focused on the more traditional bright Giant Branch tracers. We find strong evidence that the Galactic bulge rotation curves drawn from "Metal-rich" and "Metal-poor" samples are indeed discrepant. The "Metal-rich" sample shows greater rotation amplitude and a steeper gradient against line of sight distance, as possibly a stronger central concentration along the line of sight. This may represent a new detection of differing orbital anisotropy between metal-rich and metal-poor bulge objects. We also investigate selection effects that would be implied for the longitudinal proper motion cut often used to isolate a "pure-bulge" sample. Extensive investigation of synthetic stellar populations suggest that instrumental and observational artifacts are unlikely to account for the observed rotation curve differences. Thus, proper motion-based rotation curves can be used to probe chemo-dynamical correlations for Main Sequence tracer stars, which are orders of magnitude more numerous in the Galactic Bulge than the bright Giant Branch tracers. We discuss briefly the prospect of using this new tool to constrain detailed models of Galactic formation and evolution.
description: 67 pages, 41 figures, 23 tables, ApJ accepted
Van Hove Exciton-Cageons and High-T$_c$ Superconductivity, XA: Role of Spin-Orbit Coupling in Generating a Diabolical Point
Creators: name: Markiewicz, R. S.
Publisher: name: arXiv
Year: 1994
Subjects: subject: Condensed Matter (cond-mat)
subject: FOS: Physical sciences

description: Spin-orbit coupling plays a large role in stabilizing the low-temperature orthorhombic phase of La$_{2-x}$Sr$_x$CuO$_4$. It splits the degeneracy of the van Hove singularities (thereby stabilizing the distorted phase) and completely changes the shape of the Fermi surfaces, potentially introducing diabolical points into the band structure. The present paper gives a detailed account of the resulting electronic structure. A slave boson calculation shows how these results are modified in the presence of strong correlation effects. A scaling regime, found very close to the metal-insulator transition, allows an analytical determination of the crossover, in the limit of zero oxygen-oxygen hopping, $t_{OO}\rightarrow 0$. Extreme care must exercised in chosing the parameters of the three-band model. In particular, $t_{OO}$ is renormalized from its LDA value. Furthermore, it is suggested that the slave boson model be spin-corrected, in which case the system is close to a metal-insulator transition at half filling.
description: 52 pages RevTeX, 18 figures available upon request
Rates of tidal disruption of stars by massive central black holes
Creators: name: Magorrian, John
name: Tremaine, Scott
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: There is strong evidence for some kind of massive dark object in the centres of many galaxy bulges. The detection of flares from tidally disrupted stars could confirm that these objects are black holes (BHs). Here we present calculations of the stellar disruption rates in detailed dynamical models of real galaxies, taking into account the refilling of the loss cone of stars on disruptable orbits by two-body relaxation and tidal forces in non-spherical galaxies. The highest disruption rates (one star per 10^4 yr) occur in faint (L>10^10 L_sun) galaxies, which have steep central density cusps. More luminous galaxies are less dense and have much longer relaxation times and more massive BHs. Dwarf stars in such galaxies are swallowed whole by the BH and hence do not emit flares; giant stars could produce flares as often as every 10^5 yr, although the rate depends sensitively on the shape of the stellar distribution function. We discuss the possibility of detecting disruption flares in current supernova searches. The total mass of stars consumed over the lifetime of the galaxy is of order 10^6 M_sun, independent of galaxy luminosity; thus disrupted stars may contribute significantly to the present BH mass in galaxies fainter than about 10^9 L_sun.
description: 14 pages, 5 figures, 1 landscape table. Submitted to MNRAS
MOESM1 of Treatment of migraines with Tianshu capsule: a multi-center, double-blind, randomized, placebo-controlled clinical trial
Creators: name: Yu, Shengyuan
name: Ran, Ye
name: Xiao, Wei
name: Tang, Wenjing
name: Zhao, Jianjun
name: Chen, Wei
name: Zhuang, Huikui
name: Ouyang, Cun
name: Lin, Hai
name: Liu, Dequan
name: Chen, Tongjun
name: Huang, Hui
name: Wang, Baoshen
name: Hao, Yanlei
name: Yan, Zhongrui
name: Zhao, Shike
name: Wang, Yanling
name: Ni, Jinjun
name: Wang, Chaodong
name: Ding, Wentao
name: Li, Guoqian
name: Cao, Jianhua
name: Tian, Shujuan
Publisher: name: figshare
Year: 2019
Subjects: Medicine
Neuroscience
Pharmacology
Developmental Biology
Cancer

description: Additional file 1. Flow chart of experiment course.
Subregion Action and Complexity
Creators: name: Alishahiha, Mohsen
name: Velni, Komeil Babaei
name: Mozaffar, M. Reza Mohammadi
Publisher: name: arXiv
Year: 2018
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: General Relativity and Quantum Cosmology (gr-qc)
subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: We evaluate finite part of the on-shell action for black brane solutions of Einstein gravity on different subregions of spacetime enclosed by null boundaries. These subregions include the intersection of WDW patch with past/future interior and left/right exterior for a two sided black brane. Identifying the on-shell action on the exterior regions with subregion complexity one finds that it obeys subadditivity condition. This gives an insight to define a new quantity named mutual complexity. We will also consider certain subregion that is a part of spacetime which could be causally connected to an operator localized behind/outside the horizon. Taking into account all terms needed to have a diffeomorphism invariant action with a well-defined variational principle, one observes that the main contribution that results to a nontrivial behavior of the on-shell action comes from joint points where two lightlike boundaries (including horizon) intersect. A spacelike boundary gives rise to a linear time growth, while we have a classical contribution due to a timelike boundary that is given by the free energy.
description: 26 pages, 5 figures, v2: typos corrected, references added, v3: matches published version
Additional file 5 of Elevated methylation of the vault RNA2-1 promoter in maternal blood is associated with preterm birth
Creators: name: You, Young-Ah
name: Kwon, Eun Jin
name: Hwang, Han-Sung
name: Choi, Suk-Joo
name: Choi, Sae Kyung
name: Kim, Young Ju
Publisher: name: figshare
Year: 2021
Subjects: subject: Genetics
subject: FOS: Biological sciences

description: Additional file 5: Table S5. Frequency of hypomethylation of the VTRNA2-1 promoter in Indian populations (n = 136).
MOESM1 of The plant defensin gene AtPDF2.1 mediates ammonium metabolism by regulating glutamine synthetase activity in Arabidopsis thaliana
Creators: name: Yao, Junyue
name: Luo, Jin-Song
name: Xiao, Yan
name: Zhang, Zhenhua
Publisher: name: figshare
Year: 2019
Subjects: subject: Biochemistry
subject: Medicine
subject: Cell Biology
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Biotechnology
subject: Biological Sciences not elsewhere classified
subject: Developmental Biology
subject: Infectious Diseases
subject: FOS: Health sciences
subject: Plant Biology
subject: Virology
subject: Computational Biology

description: Additional file 1: Figure S1. Nitrate concentration in A. thaliana, Figure S2. Relative expression level of AtGLT1 in the shoots of of Col-0, pdf2.1–1, and pdf2.1–2 A. thaliana plants grown in 1/4 plant nutrient solution for 21 d, Table S1. Primers used in the present study
Kinematical signatures of hidden stellar discs
Creators: name: Magorrian, John
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: The deprojection of the surface brightness distribution of an axisymmetric galaxy does not have a unique solution unless the galaxy is viewed precisely edge-on. I present an algorithm that finds the full range of smooth axisymmetric density distributions consistent with a given surface brightness distribution and inclination angle, and use it to investigate the effects of this non-uniqueness on the line-of-sight velocity profiles (VPs) of two-integral models of both real and toy disky galaxies viewed at a range of inclination angles. Photometrically invisible face-on disks leave very clear signatures in the minor-axis VPs of the models (Gauss--Hermite coefficients h_4>0.1), provided the disk-to-bulge ratio is greater than about 3%. I discuss the implications of these hitherto neglected disks for dynamical modelling.
description: 7 pages, 7 figures, uses mn.tex
Quantum Beat Photoelectron Imaging Spectroscopy of Xe in the VUV
Creators: name: Forbes, Ruaridh
name: Makhija, Varun
name: Underwood, Jonathan
name: Stolow, Albert
name: Wilkinson, Iain
name: Hockett, Paul
name: Lausten, Rune
Publisher: name: arXiv
Year: 2018
Subjects: subject: Atomic Physics (physics.atom-ph)
subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: Time-resolved pump-probe measurements of Xe, pumped at 133~nm and probed at 266~nm, are presented. The pump pulse prepared a long-lived hyperfine wavepacket, in the Xe $5p^5(^2P^{\circ}_{1/2})6s~^2[1/2]^{\circ}_1$ manifold ($E=$77185 cm$^{-1}=$9.57 eV). The wavepacket was monitored via single-photon ionization, and photoelectron images measured. The images provide angle- and time-resolved data which, when obtained over a large time-window (900~ps), constitute a precision quantum beat spectroscopy measurement of the hyperfine state splittings. Additionally, analysis of the full photoelectron image stack provides a quantum beat imaging modality, in which the Fourier components of the photoelectron images correlated with specific beat components can be obtained. This may also permit the extraction of isotope-resolved photoelectron images in the frequency domain, in cases where nuclear spins (hence beat components) can be uniquely assigned to specific isotopes (as herein), and also provides phase information. The information content of both raw, and inverted, image stacks is investigated, suggesting the utility of the Fourier analysis methodology in cases where images cannot be inverted.
Phalaena complana Linnaeus, 1758, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1758
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Lepidoptera
Noctuidae
Phalaena
Phalaena complana

description: Phalaena complana [spec. nov.]
P. Noctua seticornis laevis, alis depressis: superioribus canescentibus: exteriori margine inferioribusque totis flavis. Fn. svec. 918.
Alb. ins. t. 70. f. G. II.
Habitat in Quercu.
* * * Noctuae spirilingues dorso cristato.
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 512, DOI: 10.5962/bhl.title.542, http://zenodo.org/record/3922206
Electronic Raman scattering of Tl-2223 and the symmetry of the supercon- ducting gap
Creators: name: Hoffmann, A.
name: Lemmens, P.
name: Guentherodt, G.
name: Thomas, V.
name: Winzer, K.
Publisher: name: arXiv
Year: 1994
Subjects: subject: Condensed Matter (cond-mat)
subject: FOS: Physical sciences

description: Single crystalline Tl2Ba2Ca2Cu3O10 was studied using electronic Raman scattering. The renormalization of the scattering continuum was investigated as a function of the scattering geometry to determine the superconducting energy gap 2Delta(k). The A1g- and B2g-symmetry component show a linear frequency behaviour of the scattering intensity with a peak related to the energy gap, while the B1g-symmetry component shows a characteristic behaviour at higher frequencies. The observed frequency dependencies are consistent with a dx^2-y^2-wave symmetry of the gap and yield a ratio of 2Delta/k_BT_c=7.4. With the polarization of the scattered and incident light either parallel or perpendicular to the CuO2-planes a strong anisotropy due to the layered structure was detected, which indicates an almost 2 dimensional behaviour of this system.
description: 2 pages, Postscript-file including 2 figures. Accepted for publication in the Proceedings of the M^2SHTSC IV Conference, Grenoble (France), 5-9 July 1994. Proceedings to be published in Physica C. Contact address: ahoff@phys2.rwth-aachen.de
Research on Economics Development and Growth with Global Perspective
Creators: name: Iqbal Shaukat
Publisher: name: Zenodo
Year: 2025

description: AbstractEconomic devlopment is a continuous process.it is not possible in one years,it takes the many years,the impact of economic devlopment is very long.Economic devlopment is the right example of revolution.Economic devlopment is the very integreal part of country human life.Some countries are symbol of Economic devlopment.All the nation should fellow the path way of devlopment..Many countries are the examples for other world.Deregulation,cottage industry,Micro finance, Motivation economic and management policies.Such economy got the destination of Economic development with steadily and smoothly.for example in china and India and Japan have the economic growth target of two percentage,through this way they achieved the economic growth and Devlopment. Economics education is very important for every nation.in the case of economic education we can get the good status in the socitey Economics is the back bone of every country and socitey.Economics system provide the way how to get the goal of devlopment.With the help of economics we can get the consumer price index.Economic data provide information regarding the national income and percapita income.The benefit of economic study we can prove more beneficial for the socitey.Economic education provide the way how the all sectors can be devloped.Economics data provide the information regarding the difficulties of nation

Key words: Economic, education Devlopment, growth, education
Axisymmetric Three-Integral Models for Galaxies
Creators: name: Cretton, Nicolas
name: de Zeeuw, P. Tim
name: van der Marel, Roeland P.
name: Rix, Hans-Walter
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We describe an improved, practical method for constructing galaxy models that match an arbitrary set of observational constraints, without prior assumptions about the phase-space distribution function (DF). Our method is an extension of Schwarzschild's orbit superposition technique. As in Schwarzschild's original implementation, we compute a representative library of orbits in a given potential. We then project each orbit onto the space of observables, consisting of position on the sky and line-of-sight velocity, while properly taking into account seeing convolution and pixel binning. We find the combination of orbits that produces a dynamical model that best fits the observed photometry and kinematics of the galaxy. A key new element of this work is the ability to predict and match to the data the full line-of-sight velocity profile shapes. A dark component (such as a black hole and/or a dark halo) can easily be included in the models. We have tested our method, by using it to reconstruct the properties of a two-integral model built with independent software. The test model is reproduced satisfactorily, either with the regular orbits, or with the two-integral components. This paper mainly deals with the technical aspects of the method, while applications to the galaxies M32 and NGC 4342 are described elsewhere (van der Marel et al., Cretton & van den Bosch). (abridged)
description: minor changes, accepted for publication in the Astrophysical Journal Supplements
title: ADCO, Premier cartulaire de Saint-Étienne de Dijon (XIIe siècle), Cart. 21 (G 125), 71 folios, f. 00134
Creators: name: de la Côte d'Or, Archives départementales
name: CG21/F.PETOT/2015
name: Archives Départementales De La Côte-D'Or
name: Petot, Frédérique
name: Projet CBMA
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2020
Subjects: subject: LaMOP
subject: Corpus Burgundiae Medii Aevi
subject: Laboratoire de Médiévistique Occidentale de Paris
subject: Chartes de la Bourgogne du Moyen Âge
subject: cartulaire

description: Premier cartulaire de Saint-Étienne de Dijon (XIIe siècle), Archives départementales de la Côte-d'Or, Cart. 21 (G 125), 71 folios, f. 00134, Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Premier cartulaire de Saint-Étienne de Dijon (XIIe siècle), Archives départementales de la Côte-d'Or, Cart. 21 (G 125), 71 folios, f. 00134, 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
Gyrokinetic theory of slab universal modes and the non-existence of the Gradient Drift Coupling (GDC) instability
Creators: name: Rogers, Barrett N.
name: Zhu, Ben
name: Francisquez, Manaure
Publisher: name: arXiv
Year: 2018
Subjects: subject: Plasma Physics (physics.plasm-ph)
subject: FOS: Physical sciences

description: A gyrokinetic linear stability analysis of a collisionless slab geometry in the local approximation is presented. We focus on $k_\parallel=0$ universal (or entropy) modes driven by plasma gradients at small and large plasma $β$. These are small scale non-MHD instabilities with growth rates that typically peak near $k_\perpρ_i\sim 1$ and vanish in the long wavelength $k_\perp\to 0$ limit. This work also discusses a mode known as the Gradient Drift Coupling (GDC) instability previously reported in the gyrokinetic literature, which has a finite growth rate $γ= \sqrt{β/[2(1+β)]} C_s/|L_p|$ with $C_s^2=p_0/ρ_0$ for $k_\perp\to 0$ and is universally unstable for $1/L_p\neq 0$. We show the GDC instability is a spurious, unphysical artifact that erroneously arises due to the failure to respect the total equilibrium pressure balance $p_0+B_0^2/(8π)=\text{constant}$, which renders the assumption $B_0'=0$ inconsistent if $p_0'\neq 0$.
Fluorescence quantum yield of CDOM in coastal zones of the Arctic seas
Creators: name: Drozdova, Anastasia N.
name: Kravchishina, Marina D.
name: Khundzhua, Daria A.
name: Freidkin, Mihail P.
name: Patsaeva, Svetlana V.
Publisher: name: Taylor & Francis
Year: 2018
Subjects: subject: Biotechnology
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: Ecology
subject: FOS: Biological sciences
subject: Inorganic Chemistry

description: Along with traditional optical indices, calculated from absorption and fluorescence spectra to describe chromophoric dissolved organic matter (CDOM) naturally occurring in water, the fluorescence quantum yield (FQY) becomes significant. Knowledge of CDOM optical properties is important for satellite remote sensing as well as for lidar ground-true measurements. The FQY as a function of excitation wavelength within 240–500 nm range for a variety of the Arctic shelf waters was determined for the first time in order to identify the characteristic chromophores peculiar to different regions of the Arctic basin affected by freshwater runoff. The surface water samples were collected during several cruises in 2015–2017 in the following sites: the mouth areas of the Khatanga and Lena Rivers (the Laptev Sea), the delta area of the Northern Dvina River (the White Sea), desalinated waters of the Kara Sea (influenced by freshwater of the Ob and Yenisei Rivers) and the East Siberian Sea (influenced by freshwaters of the Indigirka and Kolyma Rivers), as well the shelf areas of those seas not affected by terrigenous runoff. To characterize DOM, conventional optical indices SR, HIX, and BIX were calculated. In most cases, important humic character of DOM was established, while the contribution of autochthonous organic matter varied from low to intermediate level. For the samples with terrestrial impact, the FQY decreased from excitation at 240 nm to 270–280 nm and then increased, demonstrating two peaks at 340 and 380 nm, with constant decrease towards longer excitation wavelengths; at λex = 380 nm FQY varied from 1.4% to 3.1%. In some cases, additional maximum at 270 nm of FQY-excitation dependency was observed as an indicator of autochthonous nature of biological material. Minimal FQY was measured for the White Sea surface waters, the maximal for the Laptev and East Siberian seas.
Additional file 6 of Elevated methylation of the vault RNA2-1 promoter in maternal blood is associated with preterm birth
Creators: name: You, Young-Ah
name: Kwon, Eun Jin
name: Hwang, Han-Sung
name: Choi, Suk-Joo
name: Choi, Sae Kyung
name: Kim, Young Ju
Publisher: name: figshare
Year: 2021
Subjects: subject: Genetics
subject: FOS: Biological sciences

description: Additional file 6: Figure S1. Comparison of seven differential CpG sites on VTRNA2-1 between women with term and preterm births in initial samples (n = 10).
3C 295, a cluster and its cooling flow at z=0.46
Creators: name: Neumann, D. M.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present ROSAT HRI data of the distant and X-ray luminous (L_x(bol)=2.6^ {+0.4}_{-0.2} 10^{45}erg/sec) cluster of galaxies 3C 295. We fit both a one-dimensional and a two-dimensional isothermal beta-model to the data, the latter one taking into account the effects of the point spread function (PSF). For the error analysis of the parameters of the two-dimensional model we introduce a Monte-Carlo technique. Applying a substructure analysis, by subtracting a cluster model from the data, we find no evidence for a merger, but we see a decrement in emission South-East of the center of the cluster, which might be due to absorption. We confirm previous results by Henry & Henriksen(1986) that 3C 295 hosts a cooling flow. The equations for the simple and idealized cooling flow analysis presented here are solely based on the isothermal beta-model, which fits the data very well, including the center of the cluster. We determine a cooling flow radius of 60-120kpc and mass accretion rates of dot{M}=400-900 Msun/y, depending on the applied model and temperature profile. We also investigate the effects of the ROSAT PSF on our estimate of dot{M}, which tends to lead to a small overestimate of this quantity if not taken into account. This increase of dot{M} (10-25%) can be explained by a shallower gravitational potential inferred by the broader overall profile caused by the PSF, which diminishes the efficiency of mass accretion. We also determine the total mass of the cluster using the hydrostatic approach. At a radius of 2.1 Mpc, we estimate the total mass of the cluster (M{tot}) to be (9.2 +/- 2.7) 10^{14}Msun. For the gas to total mass ratio we get M{gas}/M{tot} =0.17-0.31, in very good agreement with the results for other clusters of galaxies, giving strong evidence for a low density universe.
description: 26 pages, 7 figures, accepted for publication in ApJ
Positivity-preserving scheme for two-dimensional advection-diffusion equations including mixed derivatives
Creators: name: Toit, Erasmus J. du
name: O'Brien, Martin R.
name: Vann, Roddy G. L.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Computational Physics (physics.comp-ph)
subject: Plasma Physics (physics.plasm-ph)
subject: FOS: Physical sciences

description: In this work, we propose a positivity-preserving scheme for solving two-dimensional advection-diffusion equations including mixed derivative terms, in order to improve the accuracy of lower-order methods. The solution to these equations, in the absence of mixed derivatives, has been studied in detail, while positivity-preserving solutions to mixed derivative terms have received much less attention. A two-dimensional diffusion equation, for which the analytical solution is known, is solved numerically to show the applicability of the scheme. It is further applied to the Fokker-Planck collision operator in two-dimensional cylindrical coordinates under the assumption of local thermal equilibrium. For a thermal equilibration problem, it is shown that the scheme conserves particle number and energy, while the preservation of positivity is ensured and the steady-state solution is the Maxwellian distribution.
The ultraviolet study of B[e] stars: evidence for pulsations, LBV-type variations, and processes in envelope
Creators: name: Krtickova, I.
name: Krticka, J.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: Stars with B[e] phenomenon comprise a very diverse group of objects in a different evolutionary status. These objects show common spectral characteristics, including presence of Balmer lines in emission, forbidden lines, and strong infrared excess due to the dust. The observations of emission lines indicate the illumination by ultraviolet ionizing source, which is a key part to understand the elusive nature of these objects. We study the ultraviolet variability of many B[e] stars to specify the geometry of the circumstellar environment and its variability. We analyse massive hot B[e] stars from our Galaxy and from Magellanic Clouds. We study the ultraviolet broad-band variability derived from the flux-calibrated data. We determine variations of individual lines and its correlation with the total flux variability. We detected variability of the spectral energy distribution and of the line profiles. The variability has several sources of origin, including the light absorption by the disk, pulsations, LBV-type variations, and eclipses in the case of binaries. The stellar radiation of most of B[e] stars is heavily obscured by circumstellar material. This suggests that the circumstellar material is not present only in the disk but also above its plane. The flux and line variability is consistent with a two-component model of circumstellar environment composed of the dense disk and ionized envelope. The observations of B[e] supergiants show that many of these stars have nearly the same luminosity of about $1.9\times10^{5}\,L_\odot$ and similar effective temperature.
description: 20 pages, accepted for publication in MNRAS
Phalaena pacta Linnaeus, 1758, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1758
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Lepidoptera
Noctuidae
Phalaena
Phalaena pacta

description: Phalaena pacta [spec. nov.]
P. Noctua spiriliuguis cristata, alis deflexis cinerascentibus; inferioribus rubris fasciis duabus nigris.
Wilk. pap. 33. t. 1. a. 1.
Habitat in Salice, Quercu.
Larva fusca, subvillosa, subtus ferruginea.
Varietas major in Europa australiore vix nisi sextupla magnitudine differt, nec Larva dissentit.
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 512, DOI: 10.5962/bhl.title.542, http://zenodo.org/record/3922206
Additional file 7 of Elevated methylation of the vault RNA2-1 promoter in maternal blood is associated with preterm birth
Creators: name: You, Young-Ah
name: Kwon, Eun Jin
name: Hwang, Han-Sung
name: Choi, Suk-Joo
name: Choi, Sae Kyung
name: Kim, Young Ju
Publisher: name: figshare
Year: 2021
Subjects: subject: Genetics
subject: FOS: Biological sciences

description: Additional file 7: Figure S2. Schematic representation of the human VTRNA2-1 gene. (a) Identified CpG site of VTRNA2-1 (b) PCR products (c) Pyrogram.
MOESM2 of Development of a biomarker mortality risk model in acute respiratory distress syndrome
Creators: name: Bime, Christian
name: Casanova, Nancy
name: Oita, Radu
name: Ndukum, Juliet
name: Lynn, Heather
name: Camp, Sara
name: Lussier, Yves
name: Abraham, Ivo
name: Carter, Darrick
name: Miller, Edmund
name: Mekontso-Dessap, Armand
name: Downs, Charles
name: Garcia, Joe
Publisher: name: figshare
Year: 2019
Subjects: subject: Space Science
subject: Medicine
subject: Microbiology
subject: FOS: Biological sciences
subject: Pharmacology
subject: Sociology
subject: FOS: Sociology
subject: Biological Sciences not elsewhere classified
subject: Inorganic Chemistry
subject: FOS: Chemical sciences
subject: Virology

description: Additional file 2: Table S1. Ranking algorithm. Eight CART iterations, algorithm conditions imposed, and number of biomarkers used. Table S2. Logistic regression analysis of mortality prediction capacity of the eight ARDS biomarkers-Day Zero. Table S3. Logistic regression analysis of mortality prediction capacity of the eight ARDS biomarkers-Day Seven. Table S4. Logistic regression analysis to assess the mortality prediction for change in measurements for the eight biomarkers. Table S5. Number of individuals per latent class. Table S6. Ranking of ARDS biomarker importance in predicting mortality.
Additional file 1 of Depression among healthcare workers in the Eastern Mediterranean Region: a systematic review and meta-analysis
Creators: name: Abraham, Amit
name: Chaabna, Karima
name: Doraiswamy, Sathyanarayanan
name: Bhagat, Sapna
name: Sheikh, Javaid
name: Mamtani, Ravinder
name: Cheema, Sohaila
Publisher: name: figshare
Year: 2021
Subjects: subject: Medicine
subject: Biotechnology
subject: Cancer
subject: Science Policy
subject: 111714 Mental Health
subject: FOS: Health sciences

description: Additional file 1. Additional Information.
Fluctuations and Intrinsic Pinning in Layered Superconductors
Creators: name: Balents, Leon
name: Nelson, David R.
Publisher: name: arXiv
Year: 1994
Subjects: subject: Condensed Matter (cond-mat)
subject: FOS: Physical sciences

description: A flux liquid can condense into a smectic crystal in a pure layered superconductors with the magnetic field oriented nearly parallel to the layers. If the smectic order is commensurate with the layering, this crystal is {\sl stable} to point disorder. By tilting and adjusting the magnitude of the applied field, both incommensurate and tilted smectic and crystalline phases are found. We discuss transport near the second order smectic freezing transition, and show that permeation modes lead to a small non--zero resistivity and large but finite tilt modulus in the smectic crystal.
description: 4 pages + 1 style file + 1 figure (as uufile) appended, REVTEX 3.0
Additional file 1 of Deforestation and fragmentation trends of seasonal dry tropical forest in Ecuador: impact on conservation
Creators: name: Rivas, Carlos A.
name: Guerrero-Casado, José
name: Navarro-Cerillo, Rafael M.
Publisher: name: figshare
Year: 2021
Subjects: subject: Cell Biology
subject: 59999 Environmental Sciences not elsewhere classified
subject: FOS: Earth and related environmental sciences
subject: Ecology
subject: FOS: Biological sciences
subject: 69999 Biological Sciences not elsewhere classified
subject: Plant Biology

description: Additional file 1: Figure S1. Percentage of RFI per tile between the years 1990 and 2018 for the following values: disappeared, very high, high, medium, low and very high.
Effectiveness of mobile application for menstrual management of working women in Japan: randomized controlled trial and medical economic evaluation
Creators: name: Mihyon Song
name: Hidenobu Kanaoka
Publisher: name: Taylor & Francis
Year: 2018
Subjects: subject: Medicine
subject: Biotechnology
subject: Sociology
subject: FOS: Sociology
subject: Science Policy

description: Aims: Hormonal imbalances can affect a woman’s physical and mental condition, impacting her daily life and productivity. A mobile application, “Karada-no-kimochi”, predicts the menstrual cycle based on recorded data, and provides the information regarding menstruation. This study investigates the effectiveness of the application from health condition and labor productivity loss perspectives, and evaluates its cost-effectiveness for employed women in Japan. Materials and methods: A randomized controlled trial (RCT) was performed to compare the use of the application and non-intervention in female workers (20–45 years) based on an online survey. A discrete-event model based on the RCT data, published literature, and claims data was used for the cost-effectiveness analysis. Results: The intervention and non-intervention groups comprised 612 and 914 women, respectively. In the intervention group, the incidences of depression (0.16%) and dysmenorrhea (0.33%) were significantly lower than those of the non-intervention group (0.77% and 1.31%, respectively) in the third month. While labor productivity and absenteeism varied, presenteeism showed almost no change across groups. The quality-adjusted life year in the intervention group was 6.84 (0.07 higher than that in the non-intervention group). By analyzing medical expenses and making assumptions regarding productivity, we estimated that the aggregate of medical expenses, productivity loss, and application fee for the intervention group could be lower than that of the non-intervention group by over JPY 130,000 (USD 1,170, as of December 2017) per individual. Limitations: The subjects included were willing or relatively willing to use the application. Because all outcomes were based on online surveys, the results depended on the objectivity and preciseness of the reports provided by users, and those with severe symptoms might not provide reports. Conclusions: The results suggest that using the application is cost-effective and might reduce the incidence of dysmenorrhea and depression.
Phalaena pronuba Linnaeus, 1758, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1758
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Lepidoptera
Noctuidae
Phalaena
Phalaena pronuba

description: Phalaena pronuba [spec. nov.]
P. Noctua spirilinguis cristata, alis incumbentibus griseis; inferioribus luteis: fascia atra submarginali.
Wilk. pap. 1. t. 1. a. 1.
Habitat in Cheirantho, Thlaspi, Senecione, Primula.
Larva nuda, testacea, linea dorsali nigra interrupta.
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 512, DOI: 10.5962/bhl.title.542, http://zenodo.org/record/3922206
Dust Measurements in the Outer Solar System
Creators: name: Grün, Eberhard
name: Krüger, Harald
name: Landgraf, Markus
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Dust measurements in the outer solar system are reviewed. Only the plasma wave instrument on board Voyagers 1 and 2 recorded impacts in the Edgeworth-Kuiper belt (EKB). Pioneers 10 and 11 measured a constant dust flux of 10-micron-sized particles out to 20 AU. Dust detectors on board Ulysses and Galileo uniquely identified micron-sized interstellar grains passing through the planetary system. Impacts of interstellar dust grains onto big EKB objects generate at least about a ton per second of micron-sized secondaries that are dispersed by Poynting-Robertson effect and Lorentz force. We conclude that impacts of interstellar particles are also responsible for the loss of dust grains at the inner edge of the EKB. While new dust measurements in the EKB are in an early planning stage, several missions (Cassini and STARDUST) are en route to analyze interstellar dust in much more detail.
description: 10 pages, 5 figures, Proceedings of the ESO workshop on ``Minor bodies in the outer solar system''