cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
The INES System II: Ripple Correction and Absolute Calibration for IUE High Resolution Spectra
Creators: name: Cassatella, A.
name: Altamore, A.
name: Gonzalez-Riestra, R.
name: Ponz, J. D.
name: Barbero, J.
name: Talavera, A.
name: Wamsteker, W.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: In this paper we document the results of the study which led to the ripple correction and absolute calibration algorithms applied to the high resolution spectra processed with the NEWSIPS software for the Final Archive of the IUE Project. In this analysis, based on a very large number of spectra, we find that both K and the alpha parameters (not only the former as previously believed) vary with order number. This fact, together with the finding that the central peaks of the blaze function vary also as a function of the THDA temperature (for the SWP camera) and of the date of observations (for the LWP and LWR cameras), makes the ripple correction algorithm more complex than previously considered but, at the same time, considerably more reliable. As for the high resolution absolute calibration, the method followed is similar to the one implemented in IUESIPS. The internal accuracy of the high resolution calibration is about 4%. We note that the ripple correction and absolute calibration algorithms here described apply also to IUE data processed and distributed with the INES system.
description: 11 pages, 16 figures, accepted for publication in A&A Supplement Series
title: ADCO, Sixième cartulaire de Saint-Étienne de Dijon (1662), Cart. 30 (G 133), 441 folios, f. 048
Creators: name: de la Côte d'Or, Archives départementales
name: CG21/F.PETOT/2012
name: Petot, Frédéric
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: Corpus Burgundiae Medii Aevi
subject: Chartes de la Bourgogne du Moyen Âge
subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris
subject: cartulaire

description: Sixième cartulaire de Saint-Étienne de Dijon (1662), Archives départementales de la Côte-d'Or, Cart. 30 (G 133), 441 folios, f. 048, 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. 048, 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
More on the Burkhardt-Cottingham Sum Rule in QCD
Creators: name: Kodaira, Jiro
name: Matsuda, Satoshi
name: Uematsu, Tsuneo
name: Sasaki, Ken
Publisher: name: arXiv
Year: 1994
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: The QCD higher order effects to the polarized structure function $g_2(x, Q^2 )$ are reanalyzed for massive quarks in the context of the operator product expansion. We confirm that the lowest moment of $g_2 (x, Q^2 )$ which corresponds to the Burkhardt-Cottingham sum rule does {\sl not} suffer from radiative corrections in perturbative QCD.
description: LaTeX, 9 pages, 1 figure appended after \end{document} as an uu-encoded and compressed .ps file, KUCP-70;HUPD-9410;YNU-HEPTh-94-105
HST - WFPC2 photometry of the globular cluster ngc 288: binary systems, blue stragglers and very blue stars
Creators: name: Bellazzini, M.
name: Messineo, M.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We report on new WFPC2 observations of the globular cluster NGC 288, focusing our attention on peculiar stars. A very pronounced binary sequence, paralleling the ordinary Main Sequence (MS) is clearly observed in the Color Magnitude Diagram (CMD) and a huge relative fraction of Blue Straggler Stars is measured. The dataset offers the opportunity of studying the evolution of a large population of binaries (and binary evolution by-products) in a low density environment, where the evolution of such systems is not dominated by collisions and encounters. Three (very) Extreme Horizontal Branch Stars have been found, all lying outside of the cluster core.
description: 6 pages, 3 figures, in press in the chemical evolution of the Milky Way: stars versus clusters, F. Matteucci and F. Giovannelli eds, Kluwer
Spin Structure Function $g_2$ and Twist-3 Operators in QCD
Creators: name: KODAIRA, Jiro
name: UEMATSU, Tsuneo
name: Yasui, Yoshiaki
Publisher: name: arXiv
Year: 1994
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We investigate the spin structure function $g_2 (x, Q^2 )$ in the framework of the operator product expansion and the renormalization group. The twist-3 operators appearing in QCD are examined and their relations are studied. It is noted that operators proportional to equation of motion appear in the operator mixing through renormalization, which can be studied from the relevant Green's functions. We also note that the coefficient functions can be properly fixed after the choice of independent operators.
description: LaTeX, 11 pages, KUCP-71; HUPD-9411
The angular momentum-mass relation: a fundamental law from dwarf irregulars to massive spirals
Creators: name: Posti, Lorenzo
name: Fraternali, Filippo
name: di Teodoro, Enrico
name: Pezzulli, Gabriele
Publisher: name: arXiv
Year: 2018
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: In a $Λ$CDM Universe, the specific stellar angular momentum ($j_\ast$) and stellar mass ($M_\ast$) of a galaxy are correlated as a consequence of the scaling existing for dark matter haloes ($j_{\rm h}\propto M_{\rm h}^{2/3}$). The shape of this law is crucial to test galaxy formation models, which are currently discrepant especially at the lowest masses, allowing to constrain fundamental parameters, e.g. the retained fraction of angular momentum. In this study, we accurately determine the empirical $j_\ast-M_\ast$ relation (Fall relation) for 92 nearby spiral galaxies (from S0 to Irr) selected from the Spitzer Photometry and Accurate Rotation Curves (SPARC) sample in the unprecedented mass range $7 \lesssim \log M_\ast/M_\odot \lesssim 11.5$. We significantly improve all previous estimates of the Fall relation by determining $j_\ast$ profiles homogeneously for all galaxies, using extended HI rotation curves, and selecting only galaxies for which a robust $j_\ast$ could be measured (converged $j_\ast(
description: A&A Letters, accepted
How activist should scientists be?
Creators: name: Vega, Jorge
name: Krueger, Tobias
name: König, Bettina
name: Garcia, Alicea
name: Sachet, Erwan
name: Molla, Nusrat
name: Chignell, Stephen
name: Tank, Lukas
name: Rege, Anushka
name: Intriago Zambrano, Juan Carlo
name: Edwards, Glory
name: Unverzagt, Krystin
name: Gürdan, Burag
name: Gasmi, Hela
name: Awuku-Sowah, Emma
name: Aysal, Lara
name: Tamang, Sangay
Publisher: name: Humboldt-Universität zu Berlin
Year: 2021
Subjects: subject: 333.7 Landflächen, Naturräume für Freizeit und Erholung, Naturreservate, Energie

description: On a Friday evening in late September 2019, 21 PhD students from every continent but Antarctica gathered in a dimly lit room on the second floor of Sophienstraße 22a in Berlin. This was the climax of a week-long summer school on ‘Transformative Human-Environment Research & Participatory Methods’ organised by the IRI THESys at Humboldt University. The preceding week’s lectures, discussions, and practicums on the democratization of knowledge production were fresh in everyone’s minds. Should scientists strive to be objective? Is it possible (not) to align our values with our scientific practice? What counts as ‘science’? The summer school students and faculty, as well as a handful of members of the public, took their seats among a few rows of chairs. At the front of the room were five chairs arranged in a semicircle facing the audience. The moderator, Krystin Unverzagt, welcomed the audience and explained how the event would proceed. Unlike a typical panel, this would be a ‘fishbowl’ discussion; the moderator would take the central chair, and each time an audience member wanted to add to the discussion, they would walk to the front, take a seat, and make their point. They were then free to stay for a few responses or return to the audience. Regardless of the direction of the conversation, one seat in the front would remain open, so there was always the opportunity for someone new to join. The following is a reconstruction of the ensuing conversation, collaboratively assembled by the participants the following day. The editors—themselves participants of the event—have added headings and made slight changes to wording for stylistic consistency
A Keck Survey of Gravitational Lens Systems: I. Spectroscopy of SBS 0909+532, HST 1411+5211, and CLASS B2319+051
Creators: name: Lubin, L. M.
name: Fassnacht, C. D.
name: Readhead, A. C. S.
name: Blandford, R. D.
name: Kundic, T.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present new results from a continuing Keck program to study gravitational lens systems. We have obtained redshifts for three lens systems, SBS 0909+532, HST 1411+5211, and CLASS B2319+051. For all of these systems, either the source or lens redshift (or both) has been previously unidentified. We find (z_l, z_s) = (0.830, 1.377) for SBS 0909+532; (z_l, z_s) = (0.465, 2.811) for HST 1411+5211, although the source redshift is still tentative; and (z_l1, z_l2) = (0.624, 0.588) for the two lensing galaxies in CLASS B2319+051. The background radio source in B2319+051 has not been detected optically; its redshift is, therefore, still unknown. We find that the spectral features of the central lensing galaxy in all three systems are typical of an early-type galaxy. The observed image splittings in SBS 0909+532 and HST 1411+5211 imply that the masses within the Einstein ring radii of the lensing galaxies are 1.4 x 10^{11} and 2.0 x 10^{11} h^{-1} M_sun, respectively. The resulting B band mass-to-light ratio for HST 1411+5211 is 41.3 +/- 1.2 h (M/L)_sun, a factor of 5 times higher than the average early-type lensing galaxy. This large mass-to-light is almost certainly the result of the additional mass contribution from the cluster CL 3C295 at z = 0.46. For the lensing galaxy in SBS 0909+532, we measure (M/L)_B = 4^{+11}_{-3} h (M/L)_sun where the large errors are the result of significant uncertainty in the galaxy luminosity. While we cannot measure directly the mass-to-light ratio of the lensing galaxy in B2319+051, we estimate that (M/L)_B is between 3-7 h (M/L)_sun.
description: Accepted for publication in Astronomical Journal. 21 pages, including 7 figures
Model Oriented Scheduling Algorithm for The Hardware-In-The-Loop Simulation
Creators: name: Al-Oraiqat, Anas M.
name: Ivanov, Yuriy O.
name: Amro, Aladdein M.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Distributed, Parallel, and Cluster Computing (cs.DC)
subject: FOS: Computer and information sciences

description: This paper presents an approach for designing software for dynamical systems simulation. An algorithm is proposed to obtain a schedule for calculating each phase variable of a stiff system of differential equations. The problem is classified as a fixed-priority pre-emptive scheduling of periodic tasks. The Branch-and-Bound algorithm is modified to minimize the defined utilization function and to optimize the scheduling process for a numerical solver. A program for the experimental schedule is implemented solving a job-shop problem that proved the effectiveness of the proposed algorithm.
description: 10 pages, 5 figures
Silk Damping in Scalar-Induced Gravitational Waves: A Novel Probe for New Physics
Creators: name: Yu, Yan-Heng
name: Wang, Sai
Publisher: name: arXiv
Year: 2024
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: General Relativity and Quantum Cosmology (gr-qc)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: Silk damping is well known in the study of cosmic microwave background (CMB) and accounts for suppression of the angular power spectrum of CMB on large angular multipoles. In this Letter, we study the effect of Silk damping on the scalar-induced gravitational waves (SIGWs). Resulting from the dissipation of cosmic fluid, the Silk damping notably suppresses the energy-density spectrum of SIGWs on scales comparable to a diffusion scale at the decoupling time of feebly-interacting particles. The effect offers a novel observable for probing the underlying particle interaction, especially for those mediated by heavy gauge bosons beyond the standard model of particles. We anticipate that pulsar timing arrays are sensitive to gauge bosons with mass $\sim10^{3}-10^{4}\,\mathrm{GeV}$, while space- and ground-based interferometers to those with mass $\sim10^7-10^{12}\,\mathrm{GeV}$, leading to essential complements to on-going and future experiments of high-energy physics.
description: 7 pages, 2 figures, additional references added
ENHANCING THE EFFECTIVENESS OF CIVIL-LEGAL REMEDIES FOR PROTECTING AN INDIVIDUAL'S HONOR, DIGNITY, AND BUSINESS REPUTATION ON SOCIAL NETWORKS
Creators: name: Sarsenbaeva, Ellada
Publisher: name: Zenodo
Year: 2025

description: Nowadays, the use of social networks in Uzbekistan is rapidly increasing, becoming an integral part of both public and personal life. This process is bringing about new challenges related to the spread of false and offensive information that harms an individual’s honor, dignity, and business reputation [1]. The unique characteristics of social networks—such as the rapid dissemination of information, broad coverage, the possibility of anonymity, and the difficulty of deleting content—set new tasks for legal protection mechanisms, unlike traditional mass media. The Constitution of the Republic of Uzbekistan guarantees the inviolability of a person’s honor and dignity [2], yet ensuring the effective protection of these guarantees in the digital space remains a pressing issue.
Modeling UV Radiation Feedback from Massive Stars: II. Dispersal of Star-Forming Giant Molecular Clouds by Photoionization and Radiation Pressure
Creators: name: Kim, Jeong-Gyu
name: Kim, Woong-Tae
name: Ostriker, Eve C.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: UV radiation feedback from young massive stars plays a key role in the evolution of giant molecular clouds (GMCs) by photoevaporating and ejecting the surrounding gas. We conduct a suite of radiation hydrodynamic simulations of star cluster formation in marginally-bound, turbulent GMCs, focusing on the effects of photoionization and radiation pressure on regulating the net star formation efficiency (SFE) and cloud lifetime. We find that the net SFE depends primarily on the initial gas surface density, $Σ_0$, such that the SFE increases from 4% to 51% as $Σ_0$ increases from $13\,M_{\odot}\,{\rm pc}^{-2}$ to $1300\,M_{\odot}\,{\rm pc}^{-2}$. Cloud destruction occurs within $2$-$10\,{\rm Myr}$ after the onset of radiation feedback, or within $0.6$-$4.1$ freefall times (increasing with $Σ_0$). Photoevaporation dominates the mass loss in massive, low surface-density clouds, but because most photons are absorbed in an ionization-bounded Strömgren volume the photoevaporated gas fraction is proportional to the square root of the SFE. The measured momentum injection due to thermal and radiation pressure forces is proportional to $Σ_0^{-0.74}$, and the ejection of neutrals substantially contributes to the disruption of low-mass and/or high-surface density clouds. We present semi-analytic models for cloud dispersal mediated by photoevaporation and by dynamical mass ejection, and show that the predicted net SFE and mass loss efficiencies are consistent with the results of our numerical simulations.
description: Accepted to ApJ. 26 pages, 18 figures, 2 tables. For a simulation movie, see http://www.youtube.com/watch?v=_YC-ueHvEWw
A counterexample to a nonlinear version of the Krein-Rutman theorem by R. Mahadevan
Creators: name: Arapostathis, Ari
Publisher: name: arXiv
Year: 2018
Subjects: subject: Functional Analysis (math.FA)
subject: FOS: Mathematics
subject: Primary 47H07, 47H10, 47J10, secondary 47B65

description: In this short note we present a simple counterexample to a nonlinear version of the Krein-Rutman theorem reported in [Nonlinear Anal. 11 (2007), 3084-3090]. Correct versions of this theorem, and related results for superadditive maps are also presented.
description: To appear in Nonlinear Analysis, 6 pages
Additional file 1: of Rapid detection of respiratory organisms with the FilmArray respiratory panel in a large childrenâ s hospital in China
Creators: name: Li, Jin
name: Tao, Yue
name: Tang, Mingyu
name: Du, Bailu
name: Xia, Yijun
name: Mo, Xi
name: Cao, Qing
Publisher: name: figshare
Year: 2018
Subjects: subject: Space Science
subject: Medicine
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Biological Sciences not elsewhere classified
subject: Developmental Biology
subject: Infectious Diseases
subject: FOS: Health sciences

description: Table S1. Combinations of multiple organisms detected with FilmArray RP. (DOC 99 kb)
Additional file 3: of The effect of human resource management on performance in hospitals in Sub-Saharan Africa: a systematic literature review
Creators: name: Philipos Gile
name: Buljac-Samardzic, Martina
name: Klundert, Joris
Publisher: name: figshare
Year: 2018
Subjects: subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: Science Policy

description: SSA countries represented in selected studies. (DOCX 14 kb)
Connected Green function approach to ground state symmetry breaking in $Φ^4_{1+1}$-theory
Creators: name: Haeuser, J. M.
name: Cassing, W.
name: Peter, A.
name: Thoma, M. H.
Publisher: name: arXiv
Year: 1994
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: Using the cluster expansions for n-point Green functions we derive a closed set of dynamical equations of motion for connected equal-time Green functions by neglecting all connected functions higher than $4^{th}$ order for the $λΦ^4$-theory in $1+1$ dimensions. We apply the equations to the investigation of spontaneous ground state symmetry breaking, i.e. to the evaluation of the effective potential at temperature $T=0$. Within our momentum space discretization we obtain a second order phase transition (in agreement with the Simon-Griffith theorem) and a critical coupling of $λ_{crit}/4m^2=2.446$ as compared to a first order phase transition and $λ_{crit}/4m^2=2.568$ from the Gaussian effective potential approach.
description: 25 Revtex pages, 5 figures available via fpt from the directory ugi-94-11 of ftp@theorie.physik.uni-giessen.de as one postscript file (there was a bug in our calculations, all numerical results and figures have changed significantly), ugi-94-11
IMPACT OF GAME-SPECIFIC TRAINING ON SKILL PERFORMANCE VARIABLES OF FIELD HOCKEY PLAYERS
Creators: name: D. Prakash* & Dr. V. Saminathan**
Publisher: name: Zenodo
Year: 2025

description: This research examined the impact of a six-week training program tailored to game-specific training on specific skill performance variables of field hockey players. Thirty male participants, aged 18 to 23, were selected and randomly divided into two groups: an experimental group (n=15) and a control group (n=15). The experimental group engaged in game-specific training sessions three times weekly, while the control group adhered to their standard training regimen. Skills such as dribbling and pushing were evaluated both before and after the intervention. A dependent t-test was employed to compare the pre- and post-test results of both groups, with a significance threshold of 0.05 and 14 degrees of freedom. The analysis indicated statistically significant differences between the groups, with the experimental group showing marked progress in the targeted skill performance.
MOESM1 of Transforming Growth Factor-Î˛1 Downregulates Vascular Endothelial Growth Factor-D Expression in Human Lung Fibroblasts via the Jun NH2-Terminal Kinase Signaling Pathway
Creators: name: Cui, Ye
name: Osorio, Juan
name: Risquez, Cristobal
name: Wang, Hao
name: Shi, Ying
name: Gochuico, Bernadette
name: Morse, Danielle
name: Rosas, Ivan
name: El-Chemaly, Souheil
Publisher: name: figshare
Year: 2014
Subjects: subject: Biochemistry
subject: Space Science
subject: Medicine
subject: Microbiology
subject: FOS: Biological sciences
subject: Genetics
subject: Chemical Sciences not elsewhere classified
subject: Ecology
subject: Immunology
subject: FOS: Clinical medicine
subject: Developmental Biology
subject: Infectious Diseases
subject: FOS: Health sciences
subject: Virology
subject: Computational Biology

description: Supplementary material, approximately 700 KB.
A Design Space Exploration Methodology for Parameter Optimization in Multicore Processors
Creators: name: Kansakar, Prasanna
name: Munir, Arslan
Publisher: name: arXiv
Year: 2018
Subjects: subject: Distributed, Parallel, and Cluster Computing (cs.DC)
subject: Hardware Architecture (cs.AR)
subject: FOS: Computer and information sciences

description: The need for application-specific design of multicore/manycore processing platforms is evident with computing systems finding use in diverse application domains. In order to tailor multicore/manycore processors for application specific requirements, a multitude of processor design parameters have to be tuned accordingly which involves rigorous and extensive design space exploration over large search spaces. In this paper, we propose an efficient methodology for design space exploration. We evaluate our methodology over two search spaces - small and large, using a cycle-accurate simulator (ESESC) and a standard set of PARSEC and SPLASH-2 benchmarks. For the smaller design space, we compare results obtained from our design space exploration methodology with results obtained from fully exhaustive search. The results show that solution quality obtained from our methodology are within 1.35% - 3.69% of the results obtained from fully exhaustive search while only exploring 2.74% - 3% of the design space. For larger design space, we compare solution quality of different results obtained by varying the number of tunable processor design parameters included in the exhaustive search phase of our methodology. The results show that including more number of tunable parameters in the exhaustive search phase of our methodology greatly improves solution quality.
description: Published in IEEE Transactions on Parallel and Distributed Systems. arXiv admin note: text overlap with arXiv:1802.05123
Spatiotemporal Implicit Neural Representation as a Generalized Traffic Data Learner
Creators: name: Nie, Tong
name: Qin, Guoyang
name: Ma, Wei
name: Sun, Jian
Publisher: name: arXiv
Year: 2024
Subjects: subject: Machine Learning (cs.LG)
subject: FOS: Computer and information sciences

description: Spatiotemporal Traffic Data (STTD) measures the complex dynamical behaviors of the multiscale transportation system. Existing methods aim to reconstruct STTD using low-dimensional models. However, they are limited to data-specific dimensions or source-dependent patterns, restricting them from unifying representations. Here, we present a novel paradigm to address the STTD learning problem by parameterizing STTD as an implicit neural representation. To discern the underlying dynamics in low-dimensional regimes, coordinate-based neural networks that can encode high-frequency structures are employed to directly map coordinates to traffic variables. To unravel the entangled spatial-temporal interactions, the variability is decomposed into separate processes. We further enable modeling in irregular spaces such as sensor graphs using spectral embedding. Through continuous representations, our approach enables the modeling of a variety of STTD with a unified input, thereby serving as a generalized learner of the underlying traffic dynamics. It is also shown that it can learn implicit low-rank priors and smoothness regularization from the data, making it versatile for learning different dominating data patterns. We validate its effectiveness through extensive experiments in real-world scenarios, showcasing applications from corridor to network scales. Empirical results not only indicate that our model has significant superiority over conventional low-rank models, but also highlight that the versatility of the approach extends to different data domains, output resolutions, and network topologies. Comprehensive model analyses provide further insight into the inductive bias of STTD. We anticipate that this pioneering modeling perspective could lay the foundation for universal representation of STTD in various real-world tasks. Code is available at https://github.com/tongnie/traffic_dynamics.
description: Accepted at TR-Part C
Cosmic Strings and Cosmic Variance
Creators: name: Gangui, Alejandro
name: Perivolaropoulos, Leandros
Publisher: name: arXiv
Year: 1994
Subjects: subject: Astrophysics (astro-ph)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: By using a simple analytical model based on counting random multiple impulses inflicted on photons by a network of cosmic strings we show how to construct the general q-point temperature correlation function of the Cosmic Microwave Background radiation. Our analysis is sensible specially for large angular scales where the Kaiser-Stebbins effect is dominant. Then we concentrate our study on the four-point function and in particular on its zero-lag limit, namely, the excess kurtosis parameter, for which we obtain a predicted value of $\sim 10^{-2}$. In addition, we estimate the cosmic variance for the kurtosis due to a Gaussian fluctuation field, showing its dependence on the primordial spectral index of density fluctuations $n$ and finding agreement with previous published results for the particular case of a flat Harrison-Zel'dovich spectrum. Our value for the kurtosis compares well with previous analyses but falls below the threshold imposed by the cosmic variance when commonly accepted parameters from string simulations are considered. In particular the non-Gaussian signal is found to be inversely proportional to the scaling number of defects, as could be expected by the central limit theorem.
description: 13 pages including 1 figure. Postscipt file appended (first line %!). To print the file with the figure, save the appended postscript file as kurtox.ps in the same directory as the tex file and then latex and print the tex file as usual. Submitted to the Astrophysical Journal
C IV BAL disappearance in a large SDSS QSO sample
Creators: name: De Cicco, D.
name: Brandt, W. N.
name: Grier, C. J.
name: Paolillo, M.
name: Ak, N. Filiz
name: Schneider, D. P.
name: Trump, J. R.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: Broad absorption lines (BALs) in the spectra of quasi-stellar objects (QSOs) originate from outflowing winds along our line of sight; winds are thought to originate from the inner regions of the QSO accretion disk, close to the central supermassive black hole (SMBH). Winds likely play a role in galaxy evolution and aid the accretion mechanism onto the SMBH. BAL equivalent widths can change on typical timescales from months to years; such variability is generally attributed to changes in the covering factor and/or in the ionization level of the gas. We investigate BAL variability, focusing on BAL disappearance. We analyze multi-epoch spectra of more than 1500 QSOs -the largest sample ever used for such a study- observed by different programs from the Sloan Digital Sky Survey-I/II/III (SDSS), and search for disappearing C IV BALs. The spectra rest-frame time baseline ranges from 0.28 to 4.9 yr; the source redshifts range from 1.68 to 4.27. We detect 73 disappearing BALs in the spectra of 67 sources. This corresponds to 3.9% of disappearing BALs, and 5.1% of our BAL QSOs exhibit at least one disappearing BAL. We estimate the average lifetime of a BAL along our line of sight (~ 80-100 yr), which appears consistent with the accretion disk orbital time at distances where winds are thought to originate. We inspect properties of the disappearing BALs and compare them to the properties of our main sample. We also investigate the existence of a correlation in the variability of multiple troughs in the same spectrum, and find it persistent at large velocity offsets between BAL pairs, suggesting that a mechanism extending on a global scale is necessary to explain the phenomenon. We select a more reliable sample of disappearing BALs following Filiz Ak et al. (2012), where a subset of our sample was analyzed, and compare the findings from the two works, obtaining generally consistent results.
description: 22 pages, 9 figures. Accepted for publication in A&A
Additional file 1: of Evidence-based practice educational intervention studies: a systematic review of what is taught and how it is measured
Creators: name: Loai Albarqouni
name: Hoffmann, Tammy
name: Glasziou, Paul
Publisher: name: figshare
Year: 2018
Subjects: subject: Medicine
subject: 59999 Environmental Sciences not elsewhere classified
subject: FOS: Earth and related environmental sciences
subject: Sociology
subject: FOS: Sociology
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: Science Policy

description: Characteristics and detailed descriptions of included studies. (DOC 55 kb)
Additional file 2 of Ferrostatin-1 alleviates lipopolysaccharide-induced acute lung injury via inhibiting ferroptosis
Creators: name: Liu, Pengfei
name: Feng, Yetong
name: Li, Hanwei
name: Chen, Xin
name: Wang, Guangsuo
name: Xu, Shiyuan
name: Li, Yalan
name: Zhao, Lei
Publisher: name: figshare
Year: 2020
Subjects: subject: Biochemistry
subject: Space Science
subject: Medicine
subject: Cell Biology
subject: Molecular Biology
subject: Physiology
subject: FOS: Biological sciences
subject: Sociology
subject: FOS: Sociology
subject: Biological Sciences not elsewhere classified
subject: Information Systems not elsewhere classified
subject: Developmental Biology

description: Additional file 2: Supplementary Fig.Â 2. Raw images of HE staining in Fig. 4a.
The Star Formation Histories of Two Northern LMC Fields
Creators: name: Dolphin, A. E.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Ground-based UBV photometry of two fields in the northern disk of the LMC are presented. A distance modulus of (m-M)_0 = 18.41 +/- 0.04 and an extinction of A_V = 0.30 +/- 0.05 has been calculated for these fields. The measurable star formation history of the LMC began no more than 12 Gyr ago with a strong star forming episode with [Fe/H] = -1.63 +/- 0.10 that accounted for approximately half (by mass) of the LMC's total star formation in the first 3 Gyr. The data does not give accurate star formation rates during intermediate ages, but there appears to have been a recent increase in the star formation rate in these fields, beginning approximately 2.5 Gyr ago, with the current metallicity in the region being [Fe/H] = -0.38 +/- 0.10. The two fields have had very similar star formation rates until 200 Myr ago, at which point one shows a large increase.
description: 8 pages, 11 figures Accepted for publication in MNRAS
A New Pulsar/SNR Pair: AX J1845-0258 in G29.6+0.1
Creators: name: Gotthelf, E. V.
name: Vasisht, G.
name: Torii, K.
name: Gaensler, B. M.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present a follow-up X-ray and radio study of the field containing the 7-s X-ray pulsar AX J1845-0258, the serendipitous ASCA source whose characteristics are found to be similar to those of the anomalous X-ray pulsars (AXPs). Newly acquired ASCA data confirms a dramatic reduction in flux from the pulsar and reveals instead a faint X-ray point source, AX J184453.3-025642, within the pulsar's error circle. This X-ray source is surrounded by a partial shell of emission coincident with a newly discovered young shell-type radio supernova remnant, G29.6+0.1. The central X-ray source is too faint to provide a detection of the expected pulsations which might confirm AX J184453.3-025642 as the pulsar. We argue that this system is similar to that of RCW 103, another AXP-like object whose central source displays low/high flux states (but no pulsations). The alternative interpretation of a binary system, perhaps associated with a supernova remnant, is still possible. In either case, this result may have profound implication on the evolution of young neutron stars.
description: 4 pages, to appear in the proceedings of the Bologna Conference on "X-ray Astronomy 1999: Stellar Endpoints, AGNs and the Diffuse X-ray Background" (Astroph. Lett. and Comm.)
Stress solution of static linear elasticity with mixed boundary conditions via adjoint linear operators
Creators: name: Gudoshnikov, Ivan
name: Křížek, Michal
Publisher: name: arXiv
Year: 2024
Subjects: subject: Analysis of PDEs (math.AP)
subject: Mathematical Physics (math-ph)
subject: Functional Analysis (math.FA)
subject: FOS: Mathematics
subject: FOS: Physical sciences
subject: 74B05, 47B02, 47B93, 35J56

description: We revisit stress problems in linear elasticity to provide a perspective from the geometrical and functionalanalytic points of view. For the static stress problem of linear elasticity with mixed boundary conditions we write the associated pair of unbounded adjoint operators. The stress solution is found as an intersection of affine translations of the fundamental subspaces of the adjoint operators. In particular, we treat the equilibrium equation in the operator form, involving spaces of traces on a part of the boundary, known as Lions-Magenes spaces. Our analysis of the pair of adjoint operators for the problem with mixed boundary conditions relies on the properties of the analogous pair of operators for the problem with the displacement boundary conditions, which we also include in the paper.
Additional file 1 of Porcine circovirus type 2 exploits JNK-mediated disruption of tight junctions to facilitate Streptococcus suis translocation across the tracheal epithelium
Creators: name: Wang, Qing
name: Zhou, Hong
name: Lin, Huixing
name: Ma, Zhe
name: Fan, Hongjie
Publisher: name: figshare
Year: 2020
Subjects: subject: Space Science
subject: Medicine
subject: Cell Biology
subject: Molecular Biology
subject: Physiology
subject: FOS: Biological sciences
subject: Sociology
subject: FOS: Sociology
subject: Biological Sciences not elsewhere classified
subject: Developmental Biology

description: Additional file 1. Immunofluorescence staining of ZO-1 and occludin in the lungs.
The Nature of Radio Emission from Distant Galaxies
Creators: name: Richards, E. A.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: I describe an observational program aimed at understanding the radio emission from distant, rapidly evolving galaxy populations. These observations were carried out at 1.4 and 8.5 GHz with the VLA centered on the Hubble Deep Field. Further MERLIN observations of the HDF region at 1.4 GHz provided an angular resolution of 0.2" and when combined with the VLA data produced an image with an unprecedented rms noise of 4 $μ$Jy. All radio sources detected in the VLA complete sample are resolved with a median angular size of 1-2". The differential count of the radio sources is marginally sub-Euclidean ($γ$ = -2.4 $\pm$ 0.1) and fluctuation analysis suggests nearly 60 sources per arcmin$^2$ are present at the 1 $μ$Jy level. A correlation analysis indicates spatial clustering among the 371 radio sources on angular scales of 1- 40 arcmin. Optical identifications are made primarily with bright (I = 22) disk systems composed of irregulars, peculiars, interacting/merging galaxies, and a few isolated field spirals. Available redshifts span the range 0.2 - 3. These clues coupled with the steep spectral index of the 1.4 GHz selected sample are indicative of diffuse synchrotron radiation in distant galactic disks. Thus the evolution in the microjansky radio population is driven principally by star-formation. I have isolated a number of optically faint radio sources (about 25% of the overall sample) which remain unidentified to I = 26-28 in the HDF and flanking optical fields. Several of these objects have extremely red counterparts and constitute a new class of radio sources which are candidate high-z dusty protogalaxies.
description: dissertation summary to be published in PASP, sucessfully defended on May 19, 1999 at the University of Virginia, committee composed of R. W. O'Connell (UVa), K. I. Kellermann (NRAO), E. B Fomalont (NRAO), T. X. Thuan (UVa), P. Humphreys (UVa), and J. Wall (Oxford)
Additional file 4 of Characterization of novel LncRNA P14AS as a protector of ANRIL through AUF1 binding in human cells
Creators: name: Ma, Wanru
name: Qiao, Juanli
name: Zhou, Jing
name: Gu, Liankun
name: Deng, Dajun
Publisher: name: figshare
Year: 2020
Subjects: subject: Biochemistry
subject: Cell Biology
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Developmental Biology
subject: Cancer
subject: Infectious Diseases
subject: FOS: Health sciences
subject: Computational Biology

description: Additional file 4 Figure S2.P14AS affects the expression level of the neighboring genes at 9p21.3. qRT-PCR data are normalized to GAPDH mRNA levels and shown as the means Â± SD. (a) The expression levels of P14, P16, and P15 genes in the P14AS vector stably transfected colon cancer cells (HCT116 and SW480), and gastric cancer cells (MGC803) were analyzed by qRT-PCR. (b) Detection of P16/P15/P14 proteins in MGC803 cells in Western blot analyses. (c) A fragment deletion in P14AS exon 1 was detected by PCR (top chart) in HEK293T or HCT116 P14AS-KO clones (KO). The expression changes of P14, P16, and P15 genes in HCT116 and HEK293T cells whose ARE-containing elements in P14AS exon-1 were homogenously deleted in the qRT-PCR analysis (bottom chart). Pooled P14AS ARE-KO-negative subclones were used as a wild-type (WT) control. (d) Detection of the P16, P15, and P14 proteins in HEK293T cells in Western blot analyses.
X-ray absorption towards high-redshift sources: probing the intergalactic medium with blazars
Creators: name: Arcodia, R.
name: Campana, S.
name: Salvaterra, R.
name: Ghisellini, G.
Publisher: name: arXiv
Year: 2018
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: The role played by the intergalactic medium (IGM) in the X-ray absorption towards high-redshift sources has recently drawn more attention in spectral analysis studies. Here, we study the X-ray absorption towards 15 flat-spectrum radio quasars at $z>2$, relying on high counting statistic ($\gtrsim10\,000$ photons) provided by XMM-Newton, with additional NuSTAR (and simultaneous Swift-XRT) observations when available. Blazars can be confidently considered to have negligible X-ray absorption along the line of sight within the host galaxy, likely swept by the kpc-scale relativistic jet. This makes our sources ideal for testing the absorption component along the IGM. Our new approach is to revisit the origin of the soft X-ray spectral hardening observed in high-z blazars in terms of X-ray absorption occurring along the IGM, with the help of a low-z sample used as comparison. We verify that the presence of absorption in excess of the Galactic value is the preferred explanation to explain the observed hardening, while intrinsic energy breaks, predicted by blazars' emission models, can easily occur out of the observing energy band in most sources. First, we perform an indirect analysis comparing the inferred amount of absorption in excess of the Galactic value with a simulated IGM absorption contribution, that increases with redshift and includes both a minimum component from diffuse IGM metals, and the additional contribution of discrete denser intervening regions. Then, we directly investigate the warm-hot IGM with a spectral model on the best candidates of our sample, obtaining an average IGM density of $n_0=1.01^{+0.53}_{-0.72}\times10^{-7}$ cm$^{-3}$ and temperature of $\log(T/\text{K})=6.45^{+0.51}_{-2.12}$. A more dedicated study is currently beyond reach, but our results can be used as a stepping stone for future more accurate analysis, involving Athena.
description: 32 pages, 7 figures. Accepted, to be published in A&A
Chiral Dynamics, Deconfinement and Thermal Dileptons
Creators: name: Kharzeev, D.
name: Satz, H.
Publisher: name: arXiv
Year: 1994
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We show that in a hot hadron gas, chiral symmetry restoration and deconfinement lead to a strong suppression of dilepton production by pion annihilation in the continuum above the $ρ-ω-ϕ$ peak. The suppression due to deconfinement persists also for annihilation reactions involving heavier mesons.
description: plain TeX, 7 pages, CERN-TH.7399/94, BI-TP 94/39 (the needed macro is added to this revised file)
Additional file 5 of Characterization of novel LncRNA P14AS as a protector of ANRIL through AUF1 binding in human cells
Creators: name: Ma, Wanru
name: Qiao, Juanli
name: Zhou, Jing
name: Gu, Liankun
name: Deng, Dajun
Publisher: name: figshare
Year: 2020
Subjects: subject: Biophysics
subject: Biochemistry
subject: Cell Biology
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Physiology
subject: Pharmacology
subject: Biological Sciences not elsewhere classified
subject: Developmental Biology
subject: Cancer
subject: Infectious Diseases
subject: FOS: Health sciences
subject: Computational Biology

description: Additional file 5 Figure S3. P14AS expression decreased P16 mRNA-AUF1 binding. (a) AUF1 directly bound to ANRIL and P16 mRNA in HCT116 cells in the AUF1-RIP-PCR. (b) P14AS overexpression decreased ANRIL and P16 mRNA-AUF1 interaction in by the AUF1-RIP-qPCR. (c) An illustration of how the competitive AUF1-P14AS binding protects ANRIL and P16 mRNA from the decay. AUF1 complexes were drawn as dimers based on the reports that AUF1 isoforms (p37, p40, p42, and p45) could form functional dimers [25, 26].
Gamma-ray beams with large orbital angular momentum via nonlinear Compton scattering with radiation reaction
Creators: name: Chen, Yue-Yue
name: Li, Jian-Xing
name: Hatsagortsyan, and Karen Z.
name: Keitel, Christoph H.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Plasma Physics (physics.plasm-ph)
subject: FOS: Physical sciences

description: Gamma-ray beams with large angular momentum are a very valuable tool to study astrophysical phenomena in a laboratory. We investigate generation of well-collimated $γ$-ray beams with a very large orbital angular momentum using nonlinear Compton scattering of a strong laser pulse of twisted photons at ultra-relativistic electrons. Angular momentum conservation among absorbed laser photons, quantum radiation and electrons are numerically demonstrated in the quantum radiation dominated regime. We point out that the angular momentum of the absorbed laser photons is not solely transferred to the emitted $γ$-photons, but due to radiation reaction shared between the $γ$-photons and interacting electrons. The efficiency of the angular momentum transfer is optimized with respect to the laser and electron beam parameters. The accompanying process of electron-positron pair production is furthermore shown to enhance the orbital angular momentum gained by the $γ$-ray beam.
title: ADCO, Ordre cistercien et abbaye de Cîteaux : comptes pour l'ordre (1337-1347), comptes du boursier (1377-1402) (11 H 1160), f. 00397
Creators: name: de la Côte-d'Or, Archives départementales
name: Archives Départementales De La Côte-D'Or
name: Petot, Frédérique
name: Projet CBMA
name: CBMA/CG21/F.PETOT/2017
name: Petot, Frédéric
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2020
Subjects: subject: Corpus Burgundiae Medii Aevi
subject: Chartes de la Bourgogne du Moyen Âge
subject: comptes
subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris

description: Ordre cistercien et abbaye de Cîteaux : comptes pour l'ordre (1337-1347), comptes du boursier (1377-1402), Archives départementales de la Côte-d'Or, (11 H 1160). Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Ordre cistercien et abbaye de Cîteaux : comptes pour l'ordre (1337-1347), comptes du boursier (1377-1402), Archives départementales de la Côte-d'Or, (11 H 1160), f. 00397, in Projet CBMA - Corpus Burgundiae Medii Aevi \[Ressource en ligne\], https:// manuscrits.cbma-project.eu/
description: Provenance: https://www.geonames.org/3024876
description: Provenance: http://www.idref.fr/030974844/id
description: Provenance: https://catalogue.bnf.fr/ark:/12148/cb12228351v
description: Provenance: abbaye de Cîteaux
description: Provenance: http://www.wikidata.org/entity/Q843261
THEORETICAL ASPECTS OF LISTING REQUIREMENTS FOR JOINT-STOCK COMPANIES
Creators: name: Narimonov, Sayfullokhon
Publisher: name: Zenodo
Year: 2024

description: Resources are becoming more scarce due to the current drastic changes taking place in the global economy, and economic organizations are becoming more dependent on raw commodities. Since 2017, Uzbekistan's intricate integration procedures into the global market have become more robust, as evidenced by the stock market's explosive growth and the continued expansion of businesses' internationalization.
Supernovae Ia Constraints on a Time-Variable Cosmological "Constant"
Creators: name: Podariu, Silviu
name: Ratra, Bharat
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: The energy density of a scalar field $ϕ$ with potential $V(ϕ) \propto ϕ^{-α}$, $α> 0$, behaves like a time-variable cosmological constant that could contribute significantly to the present energy density. Predictions of this spatially-flat model are compared to recent Type Ia supernovae apparent magnitude versus redshift data. A large region of model parameter space is consistent with current observations. (These constraints are based on the exact scalar field model equations of motion, not on the widely used time-independent equation of state fluid approximation equations of motion.) We examine the consequences of also incorporating constraints from recent measurements of the Hubble parameter and the age of the universe in the constant and time-variable cosmological constant models. We also study the effect of using a non-informative prior for the density parameter.
description: Accepted for publication in ApJ