cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Wind-Driven Gas Networks and Star Formation in Galaxies: Reaction-Advection Hydrodynamic Simulations
Creators: name: Chappell, David
name: Scalo, John
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: The effects of wind-driven star formation feedback on the spatio-temporal organization of stars and gas in galaxies is studied using two-dimensional intermediate-representational quasi-hydrodynamical simulations. The model retains only a reduced subset of the physics, including mass and momentum conservation, fully nonlinear fluid advection, inelastic macroscopic interactions, threshold star formation, and momentum forcing by winds from young star clusters on the surrounding gas. Expanding shells of swept-up gas evolve through the action of fluid advection to form a ``turbulent'' network of interacting shell fragments whose overall appearance is a web of filaments (in two dimensions). A new star cluster is formed whenever the column density through a filament exceeds a critical threshold based on the gravitational instability criterion for an expanding shell, which then generates a new expanding shell after some time delay. A filament- finding algorithm is developed to locate the potential sites of new star formation. The major result is the dominance of multiple interactions between advectively-distorted shells in controlling the gas and star morphology, gas velocity distribution and mass spectrum of high mass density peaks, and the global star formation history. The gas morphology observations of gas in the LMC and in local molecular clouds. The frequency distribution of present-to-past average global star formation rate, the distribution of gas velocities in filaments (found to be exponential), and the cloud mass spectra (estimated using a structure tree method), are discussed in detail.
description: 40 pp, 15 eps figs, mnras style, accepted for publication in MNRAS, abstract abridged, revisions in response to referee's comments
3D numerical modeling of liquid metal turbulent flow in an annular linear induction pump
Creators: name: Abdullina, K. I.
name: Bogovalov, S. V.
name: Zaikov, Yu. P.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Applied Physics (physics.app-ph)
subject: FOS: Physical sciences

description: 3D numerical simulation of the liquid metal flow affected by electromagnetic field in the Annular Linear Induction Pump (ALIP) is performed using modified ANSYS package. ANSYS/EMAG has been modified to take into account arbitrary velocity field at the calculation of the electromagnetic field and has been unified with CFX to provide integration of all the system of magnetohydrodynamic (MHD) equations defining dynamics of the conductive media in the variable electromagnetic field. The non-stationary problem is solved taking into account the influence of the metal flow on the electromagnetic field. The pump performance curve and the dependence of the pump efficiency on a flow rate are obtained.
On Multilateral Hierarchical Dynamic Decisions
Creators: name: Szajowski, Krzysztof
Publisher: name: arXiv
Year: 2018
Subjects: subject: Optimization and Control (math.OC)
subject: FOS: Mathematics
subject: 90D15, 93C30

description: Many decision problems in economics, information technology, and industry can be transformed to an optimal stopping of adapted random vectors with some utility function over the set of Markov times with respect to filtration build by the decision maker's knowledge. The optimal stopping problem formulation is to find a stopping time which maximizes the expected value of the accepted (stopped) random vector's utility. There are natural extensions of optimal stopping problem to stopping the games-the problem of stopping random vectors by two or more decision makers. Various approaches dependent on the information scheme and the aims of the agents in a considered model. This report unifies a group of non-cooperative stopping game models with forced cooperation by the role of the agents, their aims and aspirations (v. Assaf & Samuel-Cahn(1998), Szajowski & Yasuda(1995)) or extensions of the strategy sets (v. Ramsey & Szajowski(2008)).
Hosiea Hemsl. & E. H. Wilson
Creators: name: Rio, Cédric Del
name: Stull, Gregory W.
name: Franceschi, Dario De
Publisher: name: Zenodo
Year: 2020
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Magnoliopsida
Icacinales
Icacinaceae
Hosiea

description: Genus Hosiea Hemsl. & E.H.Wilson
Figs 9.19–9.25, 10.1–10.9
Description
FRUIT. Elliptical, slightly asymmetrical at the apex, laterally highly compressed, red-brown when mature. Epicarp glabrous. Calyx persistent.
ENDOCARP. Cream, elliptical in lateral view, lenticular in transverse section. Small keel surrounding the endocarp in the plane of symmetry. Apex slightly asymmetrical in lateral view; base rounded and symmetrical.Outer surface of the endocarp ridged, with thin rounded to sharp ridges delimiting a reticulate pattern enclosing areoles; most areoles with freely ending ridgelets. Vasculature of the endocarp free or resting on the ridges; endocarp primary vascular bundle positioned outside the endocarp wall. Endocarp wall thin, divided into distinctive layers, at least one layer with anticlinally oriented cells (outer part) and another with periclinally oriented cells (inner part). Locule surface with regularly spaced and large papillae, irregular in shape. Locule surface lacunate.
Fig. 9. (see full caption on page 22)
Key to the genus Hosiea
1. Endocarp ridges acute ......................................................................................... H. japonica Makino
– Endocarp ridges rounded .................................................. H. sinensis (Oliv.) Hemsl. & E.H.Wilson
description: Published as part of Rio, Cédric Del, Stull, Gregory W. & Franceschi, Dario De, 2020, Survey of the fruits and endocarps of Icacinaceae (Lamiids, Icacinales), pp. 1-130 in European Journal of Taxonomy 645 on pages 22-24, DOI: 10.5852/ejt.2020.645, http://zenodo.org/record/3829651
Musca plebeja Linnaeus, 1758, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1758
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Diptera
Anthomyiidae
Musca
Musca plebeja

description: Musca plebeja [spec. nov.]
M. antennis filatis subulatis, corpore cinereo hirto, abdominis incisuris margine albidis.
Habitat in Europa.
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 589, DOI: 10.5962/bhl.title.542, http://zenodo.org/record/3922206
Crossover and scaling in a nearly antiferromagnetic Fermi liquid in two dimensions
Creators: name: Sachdev, Subir
name: Chubukov, Andrey V.
name: Sokol, Alexander
Publisher: name: arXiv
Year: 1994
Subjects: subject: Condensed Matter (cond-mat)
subject: FOS: Physical sciences

description: We consider two-dimensional Fermi liquids in the vicinity of a quantum transition to a phase with commensurate, antiferromagnetic long-range order. Depending upon the Fermi surface topology, mean-field spin-density-wave theory predicts two different types of such transitions, with mean-field dynamic critical exponents $z=1$ (when the Fermi surface does not cross the magnetic zone boundary, type $A$) and $z=2$ (when the Fermi surface crosses the magnetic zone boundary, type $B$). The type $A$ system only displays $z=1$ behavior at all energies and its scaling properties are similar (though not identical) to those of an insulating Heisenberg antiferromagnet. Under suitable conditions precisely stated in this paper, the type $B$ system displays a crossover from relaxational behavior at low energies to type $A$ behavior at high energies. A scaling hypothesis is proposed to describe this crossover: we postulate a universal scaling function which determines the entire, temperature-, wavevector-, and frequency-dependent, dynamic, staggered spin susceptibility in terms of 4 measurable, $T=0$, parameters (determining the distance, energy, and order parameter scales, plus one crossover parameter). The scaling function contains the full scaling behavior in all regimes for both type $A$ and $B$ systems. The crossover behavior of the uniform susceptibility and the specific heat is somewhat more complicated and is also discussed. Explicit computation of the crossover functions is carried out in a large $N$ expansion on a mean-field model. Some new results for the critical properties on the ordered side of the transition are also obtained in a spin-density wave formalism. The possible relevance of our results to the doped cuprate compounds is briefly discussed.
description: 20 pages, REVTeX, 6 figures (uuencoded compressed PostScript file for figures is appended)
The Dynamics of Tightly-packed Planetary Systems in the Presence of an Outer Planet: case studies using Kepler-11 and Kepler-90
Creators: name: Contreras, A. P. Granados
name: Boley, A. C.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: FOS: Physical sciences

description: We explore the effects of an undetected outer giant planet on the dynamics, observability, and stability of Systems with Tightly-packed Inner Planets (STIPs). We use direct numerical simulations along with secular theory and synthetic secular frequency spectra to analyze how analogues of Kepler-11 and Kepler-90 behave in the presence of a nearly co-planar, Jupiter-like outer perturber with semi-major axes between 1 and 5.2 au. Most locations of the outer perturber do not affect the evolution of the inner planetary systems, apart from altering precession frequencies. However, there are locations at which an outer planet causes system instability due to, in part, secular eccentricity resonances. In Kepler-90, there is a range of orbital distances for which the outer perturber drives planets b and c, through secular interactions, onto orbits with inclinations that are $\sim16^\circ$ away from the rest of the planets. Kepler-90 is stable in this configuration. Such secular resonances can thus affect the observed multiplicity of transiting systems. We also compare the synthetic apsidal and nodal precession frequencies with the secular theory and find some misalignment between principal frequencies, indicative of strong interactions between the planets (consistent with the system showing TTVs). First-order libration angles are calculated to identify MMRs in the systems, for which two near-MMRs are shown in Kepler-90, with a 5:4 between b and c, as well as a 3:2 between g and h.
description: 17 pages, accepted for publication in AJ
Just a Little Bit? Historicizing Born-Digital Objects
Creators: name: Feichtinger, Moritz
Publisher: name: Zenodo
Year: 2025
Subjects: Digital History

description: Präsentation zum Vortrag von Moritz Feichtinger "Just a Little Bit? Historicizing Born-Digital Objects", gehalten am 8. Januar 2025 im 'Offenen Forschungskolloquium Digital History' an der Humboldt-Universität zu Berlin.

Link zum Abstract: https://dhistory.hypotheses.org/9346 Link zur Vortragsaufzeichnung (YouTube): https://www.youtube.com/watch?v=aXF7Q-3SQGM 

---

Slides for the talk by Moritz Feichtinger titled "Just a Little Bit? Historicizing Born-Digital Objects", held on January 8, 2025, at the 'Open Research Colloquium Digital History' at Humboldt-Universität zu Berlin.

Link to the abstract: https://dhistory.hypotheses.org/9346 Link to the recording (YouTube): https://www.youtube.com/watch?v=aXF7Q-3SQGM
Cepheid Calibration of the Peak Brightness of SNe Ia -- IX. SN 1989B in NGC 3627
Creators: name: Saha, A.
name: Sandage, A.
name: Tammann, G. A.
name: Labhardt, L.
name: Macchetto, F. D.
name: Panagia, N.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: (Abridged) Repeated imaging observations have been made of NGC 3627 with the HST in 1997/98, over an interval of 58 days. Images were obtained on 12 epochs in the F555W band and on five epochs in the F814W band. The galaxy hosted the prototypical, `Branch normal', type Ia supernova SN 1989B. A total of 83 variables have been found, of which 68 are definite Cepheid variables with periods ranging from 75 days to 3.85 days. The de-reddened distance modulus is determined to be (m-M)_0= 30.22+/-0.12 (internal uncertainty) using a subset of the Cepheid data whose reddening and error parameters are secure. The photometric data of Wells et al. (1994), combined with the Cepheid data for NGC 3627 give M_B(max)= -19.36+/-0.18 and M_V(max)= -19.34+/-0.16 for SN 1989B. Combined with the previous six calibrations in this program, plus two additional calibrations determined by others gives the mean absolute magnitudes at maximum of = -19.48+/-0.07 and = -19.48 +/-0.07 for `Branch normal' SNe Ia at this interim stage in the calibration program. The second parameter correlations of M(max) of blue SNe Ia with decay rate, color at maximum, and Hubble type are re-investigated. The dependence of on decay rate is non-linear, showing a minimum for decay rates between 1.0< Delta m_15 <1.6. Magnitudes corrected for decay rate show no dependence on Hubble type, but a dependence on color remains. Correcting both the fiducial sample of 34 SNe Ia with decay-rate data and the current 8 calibrating SNe Ia for the correlation with decay rate as well as color gives H_0= 60+/-2 (internal) km/s/Mpc, in both B and V. The same value to within 4% is obtained if only the SNe Ia in spirals (without second parameter corrections) are considered.
description: 32 pages (with 7 tables and 14 figures) LaTeX, uses emulateapj.sty; a full-resolution version with complete figs. 4 and 5 is available at http://www.astro.unibas.ch/cosmology/papers.html ; accepted for publication in ApJ
title: ADCO, Sixième cartulaire de Saint-Étienne de Dijon (1662), Cart. 30 (G 133), 441 folios, f. 723
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: cartulaire
subject: Corpus Burgundiae Medii Aevi
subject: Chartes de la Bourgogne du Moyen Âge
subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris

description: Sixième cartulaire de Saint-Étienne de Dijon (1662), Archives départementales de la Côte-d'Or, Cart. 30 (G 133), 441 folios, f. 723, Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Sixième cartulaire de Saint-Étienne de Dijon (1662), Archives départementales de la Côte-d'Or, Cart. 30 (G 133), 441 folios, f. 723, 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
Mr-Moose: An advanced SED-fitting tool for heterogeneous multi-wavelength datasets
Creators: name: Drouart, Guillaume
name: Falkendal, Theresa
Publisher: name: arXiv
Year: 2018
Subjects: subject: Instrumentation and Methods for Astrophysics (astro-ph.IM)
subject: FOS: Physical sciences

description: We present the public release of MrMoose, a fitting procedure that is able to perform multi-wavelength and multi-object spectral energy distribution (SED) fitting in a Bayesian framework. This procedure is able to handle a large variety of cases, from an isolated source to blended multi-component sources from an heterogeneous dataset (i.e. a range of observation sensitivities and spectral/spatial resolutions). Furthermore, MrMoose handles upper-limits during the fitting process in a continuous way allowing models to be gradually less probable as upper limits are approached. The aim is to propose a simple-to-use, yet highly-versatile fitting tool fro handling increasing source complexity when combining multi-wavelength datasets with fully customisable filter/model databases. The complete control of the user is one advantage, which avoids the traditional problems related to the "black box" effect, where parameter or model tunings are impossible and can lead to overfitting and/or over-interpretation of the results. Also, while a basic knowledge of Python and statistics is required, the code aims to be sufficiently user-friendly for non-experts. We demonstrate the procedure on three cases: two artificially-generated datasets and a previous result from the literature. In particular, the most complex case (inspired by a real source, combining Herschel, ALMA and VLA data) in the context of extragalactic SED fitting, makes MrMoose a particularly-attractive SED fitting tool when dealing with partially blended sources, without the need for data deconvolution.
Hydrodynamic electron flow in high-mobility wires
Creators: name: de Jong, M. J. M.
name: Molenkamp, L. W.
Publisher: name: arXiv
Year: 1994
Subjects: subject: Condensed Matter (cond-mat)
subject: FOS: Physical sciences

description: Hydrodynamic electron flow is experimentally observed in the differential resistance of electrostatically defined wires in the two-dimensional electron gas in (Al,Ga)As heterostructures. In these experiments current heating is used to induce a controlled increase in the number of electron-electron collisions in the wire. The interplay between the partly diffusive wire-boundary scattering and the electron-electron scattering leads first to an increase and then to a decrease of the resistance of the wire with increasing current. These effects are the electronic analog of Knudsen and Poiseuille flow in gas transport, respectively. The electron flow is studied theoretically through a Boltzmann transport equation, which includes impurity, electron-electron, and boundary scattering. A solution is obtained for arbitrary scattering parameters. By calculation of flow profiles inside the wire it is demonstrated how normal flow evolves into Poiseuille flow. The boundary-scattering parameters for the gate-defined wires can be deduced from the magnitude of the Knudsen effect. Good agreement between experiment and theory is obtained.
description: 25 pages, RevTeX, 9 figures
Permutation Invariant Gaussian Matrix Models
Creators: name: Ramgoolam, Sanjaye
Publisher: name: arXiv
Year: 2018
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: Computation and Language (cs.CL)
subject: Mathematical Physics (math-ph)
subject: Representation Theory (math.RT)
subject: FOS: Physical sciences
subject: FOS: Computer and information sciences
subject: FOS: Mathematics

description: Permutation invariant Gaussian matrix models were recently developed for applications in computational linguistics. A 5-parameter family of models was solved. In this paper, we use a representation theoretic approach to solve the general 13-parameter Gaussian model, which can be viewed as a zero-dimensional quantum field theory. We express the two linear and eleven quadratic terms in the action in terms of representation theoretic parameters. These parameters are coefficients of simple quadratic expressions in terms of appropriate linear combinations of the matrix variables transforming in specific irreducible representations of the symmetric group $S_D$ where $D$ is the size of the matrices. They allow the identification of constraints which ensure a convergent Gaussian measure and well-defined expectation values for polynomial functions of the random matrix at all orders. A graph-theoretic interpretation is known to allow the enumeration of permutation invariants of matrices at linear, quadratic and higher orders. We express the expectation values of all the quadratic graph-basis invariants and a selection of cubic and quartic invariants in terms of the representation theoretic parameters of the model.
description: 47 pages. Revision-small changes in presentation to align with NPB published version, typos corrected
Musca illucens Linnaeus, 1758, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1758
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Diptera
Anthomyiidae
Musca
Musca illucens

description: Musca illucens [spec. nov.]
M. antennis filatis clavatis, alis caeruleis, corpore nigro, abdominis segmento secundo lateribus pellucido.
Habitat in America australi. Mus. De Geer.
Antennae longae nigrae. Abdominis segmentum secundum glaucum, lateribus pellucidum.
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 589, DOI: 10.5962/bhl.title.542, http://zenodo.org/record/3922206
Lag of Low-Energy Photons in an X-ray Burst Oscillation: Doppler Delays
Creators: name: Ford, Eric C.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Numerous X-ray bursts show strong oscillations in their flux at several hundred Hz as revealed by RXTE. Analyzing one such oscillation from the X-ray binary Aql X-1, I find that low energy photons (3.5-5.7 keV) lag high energy photons (>5.7 keV) by approximately 1 radian. The oscillations are thought to be produced by hot spots on the spinning neutron star. The lags can then be explained by a Doppler shifting of emission from the hot spots; higher energy photons being emitted earlier in the spin phase as the spot approaches the observer. A quantitative test of this simple model shows a remarkable agreement with the data. Similar low energy lags have been measured in kilohertz quasi-periodic oscillations and in the accreting millisecond pulsar SAX J1808.4-3658. A Doppler delay mechanism may be at work there as well.
description: accepted ApJ Letters
Supplementary document for Strong Enhanced Efficiency of Natural Alginate for Polymer Solar Cells through Modifying ZnO Cathode Buffer Layer - 4832150.pdf
Creators: name: Zhang, Xiaolin
name: Shen, Wenfei
name: Bu, Fanchen
name: Wang, Yao
name: Yu, Xiaoshuang
name: Zhang, Wenna
name: Wang, Jiuxing
name: Belfiore, Laurence
name: tang, jianguo
Publisher: name: Optica Publishing Group
Year: 2020
Subjects: Uncategorized

description: supplement 1
Additional file 1: of A novel double-stranded RNA mycovirus isolated from Trichoderma harzianum
Creators: name: Liu, Chenchen
name: Li, Mei
name: Redda, Estifanos
name: Mei, Jie
name: Zhang, Jiantai
name: Wu, Beilei
name: Jiang, Xiliang
Publisher: name: figshare
Year: 2019
Subjects: subject: Space Science
subject: Medicine
subject: Biotechnology
subject: Evolutionary Biology
subject: FOS: Biological sciences
subject: Chemical Sciences not elsewhere classified
subject: Sociology
subject: FOS: Sociology
subject: Biological Sciences not elsewhere classified
subject: Plant Biology

description: Table S1. Information on Trichoderma strains collected from Xinjiang, Inner Mongolia, Jilin and Heilongjiang Provinces of China. Table S2. High identities between contig 36 and other mycoviruses as determined by next-generation sequencing (HGS). Table S3. The primers used for 5’ RACE and 3’ RACE of the mycovirus genome sequence. Table S4. RdRP data of mycoviruses used in the phylogenetic analysis, including the identities of RdRP between ThMV1 and the compared mycoviruses. Table S5. CP data of mycoviruses used in the phylogentic analysis, including the CP identities between ThMV1 and the compared mycoviruses. Table S6. RdRP+CP data of mycoviruses used in the phylogenetic analysis, including the identities of RdRP+ CP between ThMV1 and the compared mycoviruses. Table S7. Statistical analysis of hyphae from T525 and T525-F after 5 days on PDA medium by the Mann-Whitney U test. Table S8. Average growth rate, standard deviation, and statistical analysis of hyphae from T525 and T525-F after 8 days on CZA medium by the Mann-Whitney U test. Table S9. Biomass comparison, standard deviation, and statistical analysis of biomass between T525 and T525-F by the Mann-Whitney U test. Table S10. Statistical analysis for the comparison of biomass between T525 and T525-F by using SPSS. Figure S1. Electrophoresis images of 5’ RACE and 3’ RACE results for the genome sequence of the T525 mycovirus. Figure S2. The secondary RNA structures of the 5’UTR and 3’UTR. Figure S3. The antagonistic characteristics of T525 and T525-F against F. oxysporum f.sp. cucumebrium Owen, B. cinerea and F. oxysporum f. sp. vasinfectum . Figure S4. Experimental flow chart for evaluating the biocontrol capabilities of F. oxysporum f. sp. cucumebrium Owen in cucumber. (DOCX 293 kb)
Simulations of Supernova Remnants in Diffuse Media. II. Three Remnants and Their X-Ray Emission
Creators: name: Shelton, R. L.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: This paper describes the X-ray emission from supernova remnants evolving in warm, low density, nonthermal pressure dominated regions. Non-equilibrium ionization hydrocode simulations are used to predict the high resolution spectra, ROSAT PSPC countrates, spatial appearance, color temperatures, and the O VII and O VIII emission line fluxes as a function of time. For comparisons with observations, this paper also applies the standard observational analyses for determining the color temperature, electron density, and thermal pressure to ROSAT ``observations'' of one of the simulated remnants, thus providing a map between observational results and physical conditions. The simulated remnants' C IV, N V, and O VI column densities are also reported. The simulations are applied to studies of the Galactic halo and Local Bubble and additionally may be of interest to studies of external galaxies and Galactic interarm regions.
description: scheduled for the August 10, 1999 issue of ApJ, 29 pages and 26 figures
The interplay between electron-electron interactions and impurities in one-dimensional rings
Creators: name: Mori, Hiroyuki
Publisher: name: arXiv
Year: 1994
Subjects: subject: Condensed Matter (cond-mat)
subject: FOS: Physical sciences

description: The persistent current and charge stiffness of a one-dimensional Luttinger liquid on a ring threaded by a magnetic flux are calculated by Monte Carlo simulation. By changing the random impurity potential strength and the electron-electron interaction, we see a crossover behavior between weak and strong impurity limits. For weak impurity potentials, interactions enhance impurity effects, that is, interactions decrease the current and the stiffness. On the other hand, interactions tend to screen impurities when the impurity potential is strong. Temperature dependence of the persistent current and the charge stiffness shows a peak at a characteristic temperature, consistent with a recent single impurity study.
description: 4 pages (ReVTeX3.0) + 3 figures (in uuencoded postscript format) appended in the end of the file
The Zoo of X-ray sources in the Galactic Center Region: Observations with BeppoSAX
Creators: name: Sidoli, L.
name: Mereghetti, S.
name: Israel, G. L.
name: Chiappetti, L.
name: Treves, A.
name: Orlandini, M.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We report the results of a survey of the Galactic Center region (|l| < 2deg, |b| < 0.5deg) performed with the BeppoSAX satellite. The flux from the center of our Galaxy corresponds to a luminosity of ~3 10^{35} erg/s in the 2-10 keV range. Due to the limited angular resolution ($\gsim 1'$) only part of it is supposed to come from Sagittarius A*, the non-thermal radio source which is believed to mark the dynamical center of the Galaxy. In addition to the diffuse emission, several bright (L$_X\gsim10^{36} ergs/s) point sources have been observed, both persistent (A 1742-294, SLX 1744-299, SLX 1744-300, 1E 1743.1-2843, 1E 1740.7-2942) and transient (XTE J1748-288, SAX J1747.0-2853 and KS 1741-293). The Low Mass X-ray Binary AX J1745.6-2901, discovered with ASCA at only $1.3'$ from SgrA* was detected in a low luminosity state in August 1997. Two fainter sources are very likely associated with young neutron stars: the (possibly diffuse) X-ray source at the center of the composite supernova remnant G0.9+0.1, and the "head" of the axially symmetric radio source G359.23-0.92. The latter has been detected above 6 keV, supporting a non-thermal emission mechanism.
description: 34 pages, 11 figures and 3 tables included, accepted for publication in ApJ
The Maveric Survey: a Red Straggler Binary with an Invisible Companion in the Galactic Globular Cluster M10
Creators: name: Shishkovsky, Laura
name: Strader, Jay
name: Chomiuk, Laura
name: Bahramian, Arash
name: Tremou, Evangelia
name: Li, Kwan-Lok
name: Salinas, Ricardo
name: Tudor, Vlad
name: Miller-Jones, James C. A.
name: Maccarone, Thomas J.
name: Heinke, Craig O.
name: Sivakoff, Gregory R.
Publisher: name: arXiv
Year: 2018
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: We present the discovery and characterization of a radio-bright binary in the Galactic globular cluster M10. First identified in deep radio continuum data from the Karl G. Jansky Very Large Array, M10-VLA1 has a flux density of $27\pm4$ $μ$Jy at 7.4 GHz and a flat to inverted radio spectrum. Chandra imaging shows an X-ray source with $L_X \approx 10^{31}$ erg s$^{-1}$ matching the location of the radio source. This places M10-VLA1 within the scatter of the radio--X-ray luminosity correlation for quiescent stellar-mass black holes, and a black hole X-ray binary is a viable explanation for this system. The radio and X-ray properties of the source disfavor, though do not rule out, identification as an accreting neutron star or white dwarf system. Optical imaging from the Hubble Space Telescope and spectroscopy from the SOAR telescope show the system has an orbital period of 3.339 d and an unusual "red straggler" component: an evolved star found redward of M10's red giant branch. These data also show UV/optical variability and double-peaked H$α$ emission characteristic of an accretion disk. However, SOAR spectroscopic monitoring reveals that the velocity semi-amplitude of the red straggler is low. We conclude that M10-VLA1 is most likely either a quiescent black hole X-ray binary with a rather face-on ($ i < $ 4$^{\circ}$) orientation or an unusual flaring RS CVn-type active binary, and discuss future observations that could distinguish between these possibilities.
description: ApJ accepted, 13 pages, 8 figures
Additional file 1: of circPTN sponges miR-145-5p/miR-330-5p to promote proliferation and stemness in glioma
Creators: name: Chen, Jiansheng
name: Chen, Taoliang
name: Zhu, Yubo
name: Li, Yan
name: Zhang, Yuxuan
name: Wang, Yun
name: Li, Xiao
name: Xie, Xiaomi
name: Wang, Jihui
name: Huang, Min
name: Sun, Xinlin
name: Ke, Yiquan
Publisher: name: figshare
Year: 2019
Subjects: subject: Biochemistry
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Evolutionary Biology
subject: Environmental Sciences not elsewhere classified
subject: Ecology
subject: Biological Sciences not elsewhere classified
subject: Developmental Biology
subject: Marine Biology
subject: Cancer

description: Table S1. Sequences of si-circPTN, primers and probes for FISH. (DOCX 19 kb)
Constituent-quark model with pionic contributions: electromagnetic $N\rightarrowΔ$ transition
Creators: name: Jung, Ju-Hyun
name: Schweiger, Wolfgang
name: Biernat, Elmar P.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Nuclear Theory (nucl-th)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We report on ongoing work to determine the pion-cloud contribution to the electromagnetic $N\rightarrowΔ$ transition form factors. The starting point is an $SU(6)$ spin-flavor symmetric constituent-quark model with instantaneous confinement that is augmented by dynamical pions which couple directly to the quarks. This system is treated in a relativistically invariant way within the framework of point-form quantum mechanics using a multichannel formulation. The first step is to determine the electromagnetic form factors of the bare particles that consist only of three quarks. These form factors are basic ingredients for calculating the pion-cloud contributions. Already without the pion cloud, electromagnetic nucleon and $N\rightarrow Δ$ transition form factors compare reasonably well with the data. By inclusion of the pion-cloud contribution coming from the $π$-$N$ intermediate state the reproduction of the data is further improved.
Musca chamaeleon Linnaeus, 1758, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1758
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Diptera
Anthomyiidae
Musca
Musca chamaeleon

description: Musca chamaeleon [spec. nov.]
M. antennis filatis clavatis, scutello bidentato luteo, abdomine nigro: fasciis lateralibus luteis.
Swamm. metam. t. 4.
bibl. t. 42. f. 2.
Habitat Larva in Aquis dulcibus.
Musca supra aquam obambulare solet.
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 589, DOI: 10.5962/bhl.title.542, http://zenodo.org/record/3922206
Context-Aware Attention for Understanding Twitter Abuse
Creators: name: Chakrabarty, Tuhin
name: Gupta, Kilol
Publisher: name: arXiv
Year: 2018
Subjects: subject: Computation and Language (cs.CL)
subject: FOS: Computer and information sciences

description: The original goal of any social media platform is to facilitate users to indulge in healthy and meaningful conversations. But more often than not, it has been found that it becomes an avenue for wanton attacks. We want to alleviate this issue and hence we try to provide a detailed analysis of how abusive behavior can be monitored in Twitter. The complexity of the natural language constructs makes this task challenging. We show how applying contextual attention to Long Short Term Memory networks help us give near state of art results on multiple benchmarks abuse detection data sets from Twitter.
description: The full published version of this work is available at: \url{https://www.aclweb.org/anthology/W19-3508/}. Please use the version published in the ACL anthology for citation purposes
Statics and Dynamics of an Interface in a Temperature Gradient
Creators: name: Boyanovsky, D.
name: Jasnow, D.
name: Llambias, J.
name: Takakura, F.
Publisher: name: arXiv
Year: 1994
Subjects: subject: Condensed Matter (cond-mat)
subject: FOS: Physical sciences

description: The response and nonconserved dynamics of a two-phase interface in the presence of a temperature gradient oriented normally to the interface are considered. Two types of boundary conditions on the order parameter are considered, and the structure of the effective free energy and the Langevin equation for the collective coordinate specifying the interface position are analyzed.
description: 15 pages, Revtex 3.0, 5 figures available upon request
Additional file 10: of Incidence and death in 29 cancer groups in 2017 and trend analysis from 1990 to 2017 from the Global Burden of Disease Study
Creators: name: Lin, Longfei
name: Yan, Lei
name: Liu, Yuling
name: Yuan, Fang
name: Li, Hui
name: Ni, Jian
Publisher: name: figshare
Year: 2019
Subjects: Medicine
Biological Sciences not elsewhere classified
Marine Biology
Science Policy

description: The ASIR of 29 specified cancer groups in 2017 and 1990, and relative changes between 1990 and 2017 in 195 countries and territories. (PDF 1526 kb)
The Late Time Light Curve of SN 1998bw Associated with GRB980425
Creators: name: McKenzie, Eric H.
name: Schaefer, Bradley E.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We report 139 photometric observations through the B, V, and I filters of the supernova SN 1998bw, an object which is associated with the Gamma-Ray Burst GRB 980425. Detailed light curves of this unique supernova can be compared to theoretical models, so we report here our light curve for 123 days between 27 June 1998 and 28 October 1998. The light curve of SN 1988bw is consistent with those of the Type Ic class. We find that the magnitude-versus-time relation for this supernova is linear to within 0.05 mags in all colors over the entire duration of our study. Our measured uniform decline rates are $0.0141 \pm 0.0002$, $0.0184 \pm 0.0003$, and $0.0181 \pm 0.0003$ magnitudes per day in the B, V, and I bands. The linear decline and the rate of that decline suggest that late time light curve is powered by the radioactive decay of cobalt with some leakage of the gamma rays.
description: 15 pages, 1 figure, 1 table, Accepted for publication in PASP
High Sensitivity RF Spectroscopy of a Strongly-Interacting Fermi Gas
Creators: name: Shkedrov, Constantine
name: Florshaim, Yanay
name: Ness, Gal
name: Gandman, Andrey
name: Sagi, Yoav
Publisher: name: arXiv
Year: 2018
Subjects: subject: Quantum Gases (cond-mat.quant-gas)
subject: Atomic Physics (physics.atom-ph)
subject: FOS: Physical sciences

description: Rf spectroscopy is one of the most powerful probing techniques in the field of ultracold gases. We report on a novel rf spectroscopy scheme with which we can detect very weak signals of only a few atoms. Using this method, we extended the experimentally accessible photon-energies range by an order of magnitude compared to previous studies. We verify directly a universal property of fermions with short-range interactions which is a power-law scaling of the rf spectrum tail all the way up to the interaction scale. We also employ our technique to precisely measure the binding energy of Feshbach molecules in an extended range of magnetic fields. This data is used to extract a new calibration of the Feshbach resonance between the two lowest energy levels of 40K
description: 4 pages, 4 figures
Iodes cirrhosa Turcz.
Creators: name: Rio, Cédric Del
name: Stull, Gregory W.
name: Franceschi, Dario De
Publisher: name: Zenodo
Year: 2020
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Magnoliopsida
Icacinales
Icacinaceae
Iodes
Iodes cirrhosa

description: Iodes cirrhosa Turcz.
Fig. 12.14–12.23
Material examined
Specimen used for endocarp and fruit description
VIETNAM • “ Indo-chine, Ba Drang ”; 18 May 1921; B. Hayata 672; P[MNHN-P-P06672331].
Other material
VIETNAM • “ Indo-chine ”, Annam; 23 May 1923; E. Poilane 6622; P[MNHN-P-P06672332].
Description
FRUIT. Elliptical, cleft at the base, red when mature. Epicarp puberulent with yellow simple hairs with granular ornamentation, shriveled when dry, revealing the underlying endocarp ridges. Mesocarp 270– 320 µm thick when dry. Length 12–20 mm, width 10–15 mm, thickness 7–10 mm.
ENDOCARP. Cream, elliptical in lateral view, lenticular in transverse section, length ca 12.6 mm, width ca 9.5 mm, thickness ca 4.5 mm. Keel thick, surrounding the endocarp in the plane of symmetry, with the thicker margin containing the primary vascular bundle embedded within the endocarp wall. Apex asymmetrical with an acute protuberance on either side in lateral view; base flat and cleft on one side. Outer surface of the endocarp ridged and faintly rugose, with two thin rectangular to sharp ridges on each face, the median ridge running from the base up to ¾ of the endocarp length and the second ridge running up to the subapical part. Endocarp possessing a symmetrical pair of horn-like protrusions compressed on the keel, positioned eccentrically and subapically one on either endocarp face, each protrusion with a central pit. Endocarp wall 380–405 µm thick excluding ridges (813–1064 µm thick including ridges). Endocarp wall with three cell layers, sometimes homogeneous: outermost layer with 15–17 rows of isodiametric, occasionally anticlinally oriented cells, cells 22–49 µm in diameter, followed by a layer with 3–4 rows of small periclinally oriented cells, cells 7–10 µm in width; innermost layer with one row of periclinally oriented cells, cells ca 6.5 µm in width, covering the inner endocarp surface with regularly spaced, sessile rounded papillae, papillae 8.6–15.5 µm (av. 10.2 µm) in diameter, ca 460 papillae per 0.25 mm 2. Locule surface lacunate.
Fig. 12. (see full caption on page 32)
Remarks
The endocarp was considered “smooth inside” (Sleumer 1971). Here we demonstrate that the locule is densely covered by papillae. These papillae are difficult to observe without SEM.
description: Published as part of Rio, Cédric Del, Stull, Gregory W. & Franceschi, Dario De, 2020, Survey of the fruits and endocarps of Icacinaceae (Lamiids, Icacinales), pp. 1-130 in European Journal of Taxonomy 645 on pages 34-36, DOI: 10.5852/ejt.2020.645, http://zenodo.org/record/3829651
Andreev Spectroscopy of Josephson Coupling
Creators: name: Hekking, F. W. J.
name: Glazman, L. I.
name: Schoen, Gerd
Publisher: name: arXiv
Year: 1994
Subjects: subject: Condensed Matter (cond-mat)
subject: FOS: Physical sciences

description: It is shown that the low energy spectrum of mesoscopic superconductors coupled by Josephson interaction can be probed by two-electron tunneling from a normal electrode. The Andreev reflection in the NS junction of a normal-superconductor-superconductor double junction (NSS transistor) provides a unique spectroscopic tool to probe the coherent Cooper pair tunneling and the energy spectrum of the Josephson (SS) junction. The ground state properties are reflected in a resonant structure of the linear conductance; excited states with an energy as low as the Josephson coupling energy lead to a threshold in the nonlinear $I$-$V$ characteristic.
description: 9 pages REVTEX , 2 figures available upon request
In search for natural wormholes
Creators: name: Anchordoqui, Luis A.
name: Romero, G. E.
name: Torres, Diego F.
name: Andruchow, I.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We have investigated 631 time profiles of gamma ray bursts from the BATSE database searching for observable signatures produced by microlensing events related to natural wormholes. The results of this first search of topologically nontrivial objects in the Universe can be used to constrain their number and mass.
description: Mod. Phys. Lett. A. (in press) Latex (revtex style) with no figures
Additional file 1: of Incidence and death in 29 cancer groups in 2017 and trend analysis from 1990 to 2017 from the Global Burden of Disease Study
Creators: name: Lin, Longfei
name: Yan, Lei
name: Liu, Yuling
name: Yuan, Fang
name: Li, Hui
name: Ni, Jian
Publisher: name: figshare
Year: 2019
Subjects: subject: Medicine
subject: Genetics
subject: FOS: Biological sciences
subject: Biotechnology
subject: Immunology
subject: FOS: Clinical medicine
subject: Mathematical Sciences not elsewhere classified
subject: Cancer
subject: Science Policy
subject: Virology

description: Table S1. The age standardized of global death and incidence of 29 specified cancer groups in 2017 by gender. Table S2. The cancer cases of global death and incidence of 29 specified cancer groups in 2017 by gender. Table S3. Age-Specific Global Contributions of Cancer Types to Total Cancer incidence in 2017. (DOCX 32 kb)
Bernstein operators and super-Schur functions: combinatorial aspects
Creators: name: Alarie-Vézina, L.
name: Blondeau-Fournier, O.
name: Lapointe, L.
name: Mathieu, P.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Mathematical Physics (math-ph)
subject: Combinatorics (math.CO)
subject: FOS: Physical sciences
subject: FOS: Mathematics

description: The Bernstein vertex operators, which can be used to build recursively the Schur functions, are extended to superspace. Four families of super vertex operators are defined, corresponding to the four natural families of Schur functions in superspace. Combinatorial proofs that the super Bernstein vertex operators indeed build the Schur functions in superspace recursively are provided. We briefly mention a possible realization, in terms of symmetric functions in superspace, of the super-KP hierarchy, where the tau-function naturally expands in one of the super-Schur bases.
Detection of nuclear recoils in prototype dark matter detectors, made from Al, Sn and Zn Superheated Superconducting Granules
Creators: name: Abplanalp, M.
name: Berger, C.
name: Czapek, G.
name: Diggelmann, U.
name: Furlan, M.
name: Gabutti, A.
name: Janos, S.
name: Moser, U.
name: Pozzi, R.
name: Pretzl, K.
name: Schmiemann, K.
name: Perret-Gallix, D.
name: Brandt, B. van den
name: Konter, J. A.
name: Mango, S.
Publisher: name: arXiv
Year: 1994
Subjects: subject: Condensed Matter (cond-mat)
subject: High Energy Physics - Experiment (hep-ex)
subject: FOS: Physical sciences

description: This work is part of an ongoing project to develop a Superheated Superconducting Granule (SSG) detector for cold dark matter and neutrinos. The response of SSG devices to nuclear recoils has been explored irradiating SSG detectors with a 70MeV neutron beam. The aim of the experiment was to test the sensitivity of Sn, Al and Zn SSG detectors to nuclear recoil energies down to a few keV. The detector consisted of a hollow teflon cylinder (0.1cm$^3$ inner volume) filled with tiny superconducting metastable granules embedded in a dielectric medium. The nuclear recoil energies deposited in the SSG were determined measuring the neutron scattering angles with a neutron hodoscope. Coincidences in time between the SSG and the hodoscope signals have been clearly established. In this paper the results of the neutron irradiation experiments at different SSG intrinsic thresholds are discussed and compared to Monte Carlo simulations. The results show that SSG are sensitive to recoil energies down to $\sim$1keV. The limited angular resolution of the neutron hodoscope prevented us from measuring the SSG sensitivity to even lower recoil energies.
description: 14 pages in pure LaTeX, 17 figures available on request from schmiemann@lhep.unibe.ch, submitted to Phys. Rev. D, August 1994
Musca microleon Linnaeus, 1758, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1758
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Diptera
Anthomyiidae
Musca
Musca microleon

description: Musca microleon [spec. nov.]
M. antennis filatis clavatis, scutello bidentato nigro, abdomine atro: strigis lateralibus albis.
Habitat in Europa.
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 589, DOI: 10.5962/bhl.title.542, http://zenodo.org/record/3922206
Additional file 3: of Genomic regions underlying uniformity of yearling weight in Nellore cattle evaluated under different response variables
Creators: name: Laiza Iung
name: Mulder, Herman
name: Haroldo Neves
name: Carvalheiro, Roberto
Publisher: name: figshare
Year: 2018
Subjects: subject: Medicine
subject: 59999 Environmental Sciences not elsewhere classified
subject: FOS: Earth and related environmental sciences
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: Computational Biology

description: Manhattan plot and linkage disequilibrium (LD) map in each 1-Mb window discussed in our study. (PDF 419 kb)
A splitting theorem for scalar curvature
Creators: name: Chodosh, Otis
name: Eichmair, Michael
name: Moraru, Vlad
Publisher: name: arXiv
Year: 2018
Subjects: subject: Differential Geometry (math.DG)
subject: FOS: Mathematics

description: We show that a Riemannian $3$-manifold with non-negative scalar curvature is flat if it contains an area-minimizing cylinder. This scalar-curvature analogue of the classical splitting theorem of J.~Cheeger and D.~Gromollhas been conjectured by D.~Fischer-Colbrie and R.~Schoen and by M.~Cai and G.~Galloway.
description: All comments welcome!