cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Gravitational Waves from an Axi-symmetric Source in the Nonsymmetric Gravitational Theory
Creators: name: Cornish, N. J.
name: Moffat, J. W.
name: Tatarski, D. C.
Publisher: name: arXiv
Year: 1993
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: We examine gravitational waves in an isolated axi--symmetric reflexion symmetric NGT system. The structure of the vacuum field equations is analyzed and the exact solutions for the field variables in the metric tensor are found in the form of expansions in powers of a radial coordinate. We find that in the NGT axially symmetric case the mass of the system remains constant only if the system is static (as it necessarily is in the case of spherical symmetry). If the system radiates, then the mass decreases monotonically and the energy flux associated with waves is positive.
description: 15 pages, UTPT-92-17
title: ADCO, Cartulaire général de Cîteaux, dit de Jean de Cirey, (XVe siècle), tome VIII, Cart. 192 (11 H 77), 295 folios, f. 0112r
Creators: name: de la Côte d'Or, Archives départementales
name: Archives Départementales De La Côte-D'Or
name: Petot, Frédérique
name: Projet CBMA
name: CG21/F.PETOT/2012
name: Petot, Frédéric
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2020
Subjects: subject: Corpus Burgundiae Medii Aevi
subject: Chartes de la Bourgogne du Moyen Âge
subject: cartulaire
subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris

description: Cartulaire général de Cîteaux, dit de Jean de Cirey, (XVe siècle), tome VIII, Archives départementales de la Côte-d'Or, Cart. 192 (11 H 77), 295 folios, f. 0112r, Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Cartulaire général de Cîteaux, dit de Jean de Cirey, (XVe siècle), tome VIII, Archives départementales de la Côte-d'Or, Cart. 192 (11 H 77), 295 folios, f. 0112r, 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
Angular Power Spectrum of the Microwave Background Anisotropy seen by the COBE Differential Microwave Radiometer
Creators: name: Wright, E. L.
name: Smoot, G. F.
name: Bennett, C. L.
name: Lubin, P. M.
Publisher: name: arXiv
Year: 1994
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: The angular power spectrum estimator developed by Peebles (1973) and Hauser & Peebles (1973) has been modified and applied to the 2 year maps produced by the COBE DMR. The power spectrum of the real sky has been compared to the power spectra of a large number of simulated random skies produced with noise equal to the observed noise and primordial density fluctuation power spectra of power law form, with $P(k) \propto k^n$. Within the limited range of spatial scales covered by the COBE DMR, corresponding to spherical harmonic indices $3 \leq \ell \lsim 30$, the best fitting value of the spectral index is $n = 1.25^{+0.4}_{-0.45}$ with the Harrison-Zeldovich value $n = 1$ approximately 0.5$σ$ below the best fit. For $3 \leq \ell \lsim 19$, the best fit is $n = 1.46^{+0.39}_{-0.44}$. Comparing the COBE DMR $ΔT/T$ at small $\ell$ to the $ΔT/T$ at $\ell \approx 50$ from degree scale anisotropy experiments gives a smaller range of acceptable spectral indices which includes $n = 1$.
description: 22 pages of LaTex using aaspp.sty and epsf.sty with appended Postscript figures, COBE Preprint 94-02
SensApp_Deliverbale_D4.1_ Integrated system for calibration and testing_Brochure
Creators: name: Uusitalo, Sanna
name: Aikio Sanna
name: Pennala Riku
name: Anetjärvi Markus
Publisher: name: Zenodo
Year: 2021
Subjects: Integrated system, calibration, testing

description: Integrated system for calibration and testing_Brochure
Additional file 2 of Geometric morphology and population genomics provide insights into the adaptive evolution of Apis cerana in Changbai Mountain
Creators: name: Nannan, Liu
name: Huamiao, Liu
name: Yan, Ju
name: Xingan, Li
name: Yang, Li
name: Tianjiao, Wang
name: Jinming, He
name: Qingsheng, Niu
name: Xiumei, Xing
Publisher: name: figshare
Year: 2022
Subjects: subject: Genetics
subject: FOS: Biological sciences
subject: Evolutionary Biology

description: Additional file 2.
The role of DNA methylation in colorectal carcinogenesis and prognosis
Creators: name: Tsang, Julian S.
Publisher: name: Royal College of Surgeons in Ireland
Year: 2019
Subjects: Uncategorized

description: Background: Colorectal cancer is one of the commonest cancers world-wide. Surgery remains the mainstay of treatment however an increasing emphasis is now placed on adjuvant treatment with chemotherapy and radiotherapy incorporating a multi-disciplinary approach to cancer care. Clinical background and pathological staging systems remain the most important predictive and prognostic indicators. It is well-established that colorectal cancers develop via the adenoma-carcinoma sequence. This sequence is characterised by a step-wise accumulation of genetic mutational changes involving primarily the adenomatous polyposis coli (APC). K-Ras and p53 genes. In addition, the microsatellite instability pathway is responsible for almost all of the hereditary colorectal cancers. Despite ongoing research into these known genetic markers involved in colorectal carcinogenesis, clinical application in diagnosis and prognosis is still limited. Recently, a novel molecular pathway involving epigenetic mechanisms has been described. This is now recognised to be an additional and distinctive molecular pathway to most neoplasia including colorectal cancers. This pathway is characterised by gene-silencing, most commonly through the process of DNA methylation of promoter regions of genes involved in carcinogenesis. The aim of this thesis was to examine the role DNA methylation plays in colorectal carcinogenesis, in particular its potential as a prognostic marker in colorectal cancer as well as a predictor of response to neoadjuvaut chemoradiotherapy in rectal cancer. Materials and Methods: Patients with colorectal cancer were identified and samples retrieved from the pathology tissue bank. Immunohistochemical staining was performed using the conmercially available 5-Methylcytidine (Euuogentec®, Belgium) and Ki-67 (DakoCytomation®, Denmark) antibodies. Automated image analysis of staining was carried out using the Aperio® (Vista, CA) image analysis platform. Image analysis results were correlated with clinico-pathological data of individual patients including response to neoadjuvant treatment and survival. Ethical approval was obtained from the local hospitals' ethics committees (Appendix V). Statistical analysis was carried out using the Statistical Package for Social Sciences (SPSS®) version 17.
On the Constraint Algebra of Degenerate Relativity
Creators: name: Romano, Joseph D.
Publisher: name: arXiv
Year: 1993
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: As shown by Ashtekar in the mid 80's, general relativity can be extended to incorporate degenerate metrics. This extension is not unique, however, as one can change the form of the hamiltonian constraints and obtain an {\it alternative} degenerate extension of general relativity that disagrees with Ashtekar's original theory when the triads vectors are degenerate. In this paper, the constraint algebra of a particular alternative theory is explicitly evaluated and compared with that of Ashtekar's original degenerate extension. A generic classification of the difference between the two theories is given in terms of the degeneracy and surface-forming properties of the triad vectors. (This classification is valid when the degeneracy and surface-forming properties of the triad vectors is the same everywhere in an open set about a point in space.) If the triad vectors are degenerate and surface-forming, then all the secondary constraints of the alternative degenerate extension are satisfied as a consequence of the primary constraints, and the constraints of this theory are weaker than those of Ashtekar's. If the degenerate triad vectors are not surface-forming, then the first secondary constraint of the alternative theory already implies equivalence with Ashtekar's degenerate extension. What happens when the degeneracy and surface-forming properties of the triad vectors change from point to point is an open question.
description: 14 pages (Latex file), UMDGR-93-204
Environmental, Social, and Governance Performance and Downside and Upside Risks
Creators: name: Khan, Vina Javed
name: Ali, Searat
name: Chang, Millicent
Publisher: name: University of Wollongong
Year: 2025
Subjects: classificationCode: 3502
subject: Banking, finance and investment

description: The term “environmental, social, and governance (ESG)” was first mentioned during the United Nations Global Compact Leaders’ Summit to determine how ESG activities can be integrated into capital markets. Since then, these activities have become a key priority for firms, investors, and other stakeholders. Sustainable and responsible investment in the United States (US) has grown exponentially, from $639 billion in 1995 to $17.1 trillion in 2020 (US SIF 2020) (Figure 8.1). Firm commitment is growing and increasingly willing to incorporate these activities into business and investment strategies. In 2019, 222 CEOs of the largest US companies signed and issued the “Statement on the Purpose of Corporation” in a business roundtable and committed to lead their companies in the best interests of all stakeholders: employees, customers, suppliers, and shareholders. The statement disregarded shareholder supremacy and reinvigorated contrasting views about shareholder and stakeholder orientations of firms (Harrison, Phillips, and Freeman 2020). Firms holding the shareholder view try to maximize their profits (as the core firm objective), assuming shareholders to be the key stakeholders (Eccles, Ioannou, and Serafeim 2014). In contrast, other companies presume a stakeholder view to account for the externalities of their activities and how they influence other stakeholders (Deegan 2002, Friedman and Miles 2002). To maintain both approaches, effective stakeholder engagement through ESG activities requires not undermining investor interest while delivering value to other stakeholders (Dumitrescu and Zakriya 2021). This raises a question: Do ESG activities undermine investors’ interests in practice? One way to answer is to examine the effect of ESG activities on firm risk.
Additional file 4: of Antimicrobial potentiality of actinobacteria isolated from two microbiologically unexplored forest ecosystems of Northeast India
Creators: name: Ranjita Das
name: Wahengbam Romi
name: Rictika Das
name: Hridip Sharma
name: Debajit Thakur
Publisher: name: figshare
Year: 2018
Subjects: subject: Biochemistry
subject: Microbiology
subject: FOS: Biological sciences
subject: Cell Biology
subject: Genetics
subject: Molecular Biology
subject: Pharmacology
subject: Biotechnology
subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences
subject: Developmental Biology
subject: Cancer
subject: Hematology
subject: 60506 Virology

description: Figure S2. â 96 well plate showing minimum inhibitory concentration (MIC) of EA-PWS52 extract against MRSA test microbial strain.â In this figure, wells present in rows B, C, D (column 1) are negative control and contain only MRSA cells. Rows B, C, D (column 2) are also negative control having MRSA cells and 10% DMSO, which also showed presence of viable cells (change of resazurin reagent colour from blue to pink). Column 3 to 10 (rows B, C, D) contain different concentrations of EA-PWS52 extract among which column 5 (purple in colour) shows decrease in cell viability. As column 6 has no change in colour (blue) of resazurin reagent, the corresponding concentration was taken as the MIC of EA-PWS52 extract against MRSA. Rows F, G, H (column 1) are positive controls, contain MRSA cells and ampicillin, and show no viable cells as the reagent colour (blue) has not changed. (DOCX 4199 kb)
Photon production through $A_1$ resonance in high energy heavy ion collisions
Creators: name: Xiong, L.
name: Shuryak, E.
name: Brown, G. E.
Publisher: name: arXiv
Year: 1992
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: Electromagnetic radiation from excited hadronic matter is one of the best ways to study the properties of the matter. Considering various processes in the hadronic gas, Kapusta et al \cite{Kapusta_photons} have found a $πρ\rightarrow πγ$ reaction with intermediate virtual pion or rho to be the main source of photons with energy greater than 0.7 GeV. However, at temperatures considered T=100-200 MeV, a $πρ$ pair can easily form an $A_1$(1260) resonance, and we show that this mechanism leads to the photon production rates exceeding those suggested previously. The paper is in LATEX, figures available from authors.
Radiative Rare B Decays into Higher K-Resonances
Creators: name: Ali, Ahmed
name: Mannel, Thomas
name: Ohl, Thorsten
Publisher: name: arXiv
Year: 1992
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We estimate the contributions of higher K-resonances to the radiative rare decays b -> s gamma. We use the spin symmetry for heavy quarks to reduce the number of independent form factors to four Isgur-Wise functions, which are estimated from the wave function model of Isgur, Scora, Grinstein, and Wise. Our results suggest a substantially larger branching fraction for the decay B -> K*2(1430) gamma than previous investigations.
description: 13 pages (one encapsulated PostScript figure appended), DESY 92-113, IKDA 92/23
Attenuation of the systemic inflammatory response syndrome following cardiac surgery using a pre-operative infusion of omega-3 fatty acids
Creators: name: Keenan, Niamh Mary
Publisher: name: Royal College of Surgeons in Ireland
Year: 2019
Subjects: Uncategorized

description: Advances in paediatric cardiac surgical techniques over the past two decades have resulted in increasingly successful complex corrective procedures, which are frequently performed on younger, more vulnerable infants. A degree of cardiac, pulmonary, renal and cerebral dysfunction is frequently seen post-operatively; this ranges in severity, but can in some progress to multiple organ failure. The exact mechanisms, pattern and timing of the post operative organ dysfunction following paediatric cardiac surgery has not been fully elucidated, however it is now appreciated that the systemic inflammatory response syndrome, induced by a number of factors present in cardiac surgery, has a central role. To date, much research has been undertaken in developing strategies to attenuate the SIRS; however, results are conflicting and none have consistently shown a benefit in clinical practice. Omega-3 fatty acids have been shown to have anti-inflammatory, anti-infarct and antiarrhythrnic properties. Multiple pathways for these effects have been recognized: a reduction in pro-inflammatory cytokines and an increase in anti-inflammatory cytokines; an increase in the omega-3/omega-6 fatty acid ratio in cell membranes; an attenuation of the period of post-operative immunosuppression; and the production of resolvins and protectins, important in the resolution of inflammation. The aim of this research therefore was two-fold: to determine the mechanisms involved in the injury induced by cardiac surgery, and to determine if omega-3 fatty acids, given in a clinically approved formulation, could attenuate the SIRS and produce beneficial clinical effects in a juvenile piglet model of cardiopulmonary bypass and circulatory arrest. The results obtained demonstrated a pattern of cardiac and pulmonary injury attributable to the SIRS. Renal injury occurred earlier and was not associated with SIRS. Omega-3 pre-treatment resulted in an attenuation of the systemic inflammatory response, as measured by cytokines and eicosanoids, and did demonstrate trends towards improved cardiopulmonary function. This research provides a basis for further study into the mechanisms of post cardiac surgical organ injury, and also the attenuation of the SIRS with omega-3 pretreatment in the clinical arena.
Additional file 4: of Echocardiographic parameters and renal outcomes in patients with preserved renal function, and mild- moderate CKD
Creators: name: Mavrakanas, Thomas
name: Khattak, Aisha
name: Karandeep Singh
name: Charytan, David
Publisher: name: figshare
Year: 2018
Subjects: subject: Space Science
subject: 29999 Physical Sciences not elsewhere classified
subject: FOS: Physical sciences
subject: Medicine
subject: Pharmacology
subject: Sociology
subject: FOS: Sociology
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: Developmental Biology
subject: Marine Biology
subject: Computational Biology

description: Table S4. Echocardiographic characteristics of patients with CHF at baseline (DOCX 17 kb).
Image-based deep learning for classification of noise transients in gravitational wave detectors
Creators: name: Razzano, Massimiliano
name: Cuoco, Elena
Publisher: name: arXiv
Year: 2018
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: Instrumentation and Methods for Astrophysics (astro-ph.IM)
subject: Computer Vision and Pattern Recognition (cs.CV)
subject: FOS: Physical sciences
subject: FOS: Computer and information sciences

description: The detection of gravitational waves has inaugurated the era of gravitational astronomy and opened new avenues for the multimessenger study of cosmic sources. Thanks to their sensitivity, the Advanced LIGO and Advanced Virgo interferometers will probe a much larger volume of space and expand the capability of discovering new gravitational wave emitters. The characterization of these detectors is a primary task in order to recognize the main sources of noise and optimize the sensitivity of interferometers. Glitches are transient noise events that can impact the data quality of the interferometers and their classification is an important task for detector characterization. Deep learning techniques are a promising tool for the recognition and classification of glitches. We present a classification pipeline that exploits convolutional neural networks to classify glitches starting from their time-frequency evolution represented as images. We evaluated the classification accuracy on simulated glitches, showing that the proposed algorithm can automatically classify glitches on very fast timescales and with high accuracy, thus providing a promising tool for online detector characterization.
description: 25 pages, 8 figures, accepted for publication in Classical and Quantum Gravity
Thouless time for mass-deformed SYK
Creators: name: Nosaka, Tomoki
name: Rosa, Dario
name: Yoon, Junggi
Publisher: name: arXiv
Year: 2018
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: Chaotic Dynamics (nlin.CD)
subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: We study the onset of RMT dynamics in the mass-deformed SYK model (i.e. an SYK model deformed by a quadratic random interaction) in terms of the strength of the quadratic deformation. We use as chaos probes both the connected unfolded Spectral Form Factor (SFF) as well as the Gaussian-filtered SFF, which has been recently introduced in the literature. We show that they detect the chaotic/integrable transition of the mass-deformed SYK model at different values of the mass deformation: the Gaussian-filtered SFF sees the transition for large values of the mass deformation; the connected unfolded SFF sees the transition at small values. The latter is in qualitative agreement with the transition as seen by the OTOCs. We argue that the chaotic/integrable deformation affect the energy levels inhomogeneously: for small values of the mass deformation only the low-lying states are modified while for large values of the mass deformation also the states in the bulk of the spectrum move to the integrable behavior.
description: 44 pages, many figures
Origin of Quasar Progenitors from the Collapse of Low-Spin Cosmological Perturbations
Creators: name: Eisenstein, Daniel J.
name: Loeb, Abraham
Publisher: name: arXiv
Year: 1994
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We show that seeds for quasar black holes could have originated from the initial cosmological collapse of overdense regions with unusually small rotation. The gas in these rare regions collapses into a compact disk that shrinks on a short viscous time scale. Using an analytical model, we calculate the low-spin tail of the probability distribution of angular momenta for objects that collapse out of a Gaussian random field of initial density perturbations. The population of low-spin systems is significant for any viable power spectrum of primordial density perturbations. Most objects form just above the cosmological Jeans mass (\sim 10^5 M_sun) at high redshifts z>10. In the standard cold dark matter cosmology, the comoving density of 10^{6-7} M_sun objects with viscous evolution times shorter than 10^{6-7} years is about 10^{-3} (h/0.5)^3 Mpc^{-3}, comparable to the local density of bright galaxies. The seed black holes tend to reside within larger mass systems that collapse later and supply the gas needed for the bright quasar activity.
description: 18 pages and one file of 3 figures, uuencoded compressed tarred Postscript. Final extended version, accepted to the Astrophysical Journal (4/10/95 issue)
From the Big Bang Theory to the Theory of a Stationary Universe
Creators: name: Linde, Andrei
name: Linde, Dmitri
name: Mezhlumian, Arthur
Publisher: name: arXiv
Year: 1993
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: Astrophysics (astro-ph)
subject: High Energy Physics - Lattice (hep-lat)
subject: FOS: Physical sciences

description: We consider chaotic inflation in the theories with the effective potentials phi^n and e^{αϕ}. In such theories inflationary domains containing sufficiently large and homogeneous scalar field ϕpermanently produce new inflationary domains of a similar type. We show that under certain conditions this process of the self-reproduction of the Universe can be described by a stationary distribution of probability, which means that the fraction of the physical volume of the Universe in a state with given properties (with given values of fields, with a given density of matter, etc.) does not depend on time, both at the stage of inflation and after it. This represents a strong deviation of inflationary cosmology from the standard Big Bang paradigm. We compare our approach with other approaches to quantum cosmology, and illustrate some of the general conclusions mentioned above with the results of a computer simulation of stochastic processes in the inflationary Universe.
description: No changes to the file, but original figures are included. They substantially help to understand this paper, as well as eternal inflation in general, and what is now called the "multiverse" and the "string theory landscape." High quality figures can be found at http://www.stanford.edu/~alinde/LLMbigfigs/
(2-Cyclohexyl-1-methylpropyl) cyclohexane isolated from garlic extract exhibits antidepressant-like activity: extraction, docking, drug-like properties, molecular dynamics simulations and MM/GBSA studies
Creators: name: Kumari, Priyanka
name: Sharma, Bechan
name: Som, Anup
Publisher: name: Taylor & Francis
Year: 2023
Subjects: Biochemistry
Pharmacology
Biotechnology
Chemical Sciences not elsewhere classified
Biological Sciences not elsewhere classified
Mental Health

description: Depressive disorders are among most common psychiatric diseases and second most common form of psychiatric illness globally. Commonly available chemical drugs used for treatment of nervous system disorders exert undesirable effects. Therefore, there is a growing need towards exploring novel antidepressants of herbal origin. Earlier, the antidepressant effect of methanolic extract of garlic has been shown. In this study, the ethanolic extract of garlic was prepared and chemically analysed using Gas Chromatography – Mass Spectrometry (GC-MS) screening. A total of 35 compounds were found to be present, which might act as antidepressant. Using computational analyses, these compounds were screened as potential inhibitors (selective serotonin reuptake inhibitor (SSRI)) against serotonin transporter (SERT)/leucine receptor (LEUT). In silico docking studies and other physicochemical, bioactivity and ADMET studies resulted in the selection of compound 1 ((2-Cyclohexyl-1-methylpropyl) cyclohexane) as potential SSRI (binding energy −8.1 kcal/mol) compared to known reference SSRI fluoxetine (binding energy −8.0 kcal/mol). Analysis of conformational stability, residue flexibility, compactness, binding interactions, solvent accessible surface area (SASA), dynamic correlation, and binding free energy predicted from molecular mechanics (MD) with generalised Born and surface area solvation (MM/GBSA) studies revealed formation of a more stable SSRI like complex with compound 1 having strong inhibitory interaction compared to known SSRI fluoxetine/reference complex. Thus, compound 1 may act as an active SSRI leading to discovery of potential antidepressant drug. Communicated by Ramaswamy H. Sarma
Modelling the Power Spectrum of Density Fluctuations: A Phenomenological Approach
Creators: name: Branchini, Enzo
name: Guzzo, Luigi
name: Valdarnini, Riccardo
Publisher: name: arXiv
Year: 1994
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We show how, based on considerations on the observed form of the galaxy 2-point spatial correlation function xi(r), a very simplified -- yet surprisingly effective -- model for the linear density fluctuations power spectrum can be constructed. We first relate the observed large-scale shape of xi(r) to a power-law form for the power spectrum, P(k)\propto k^{-2.2}. For a plausible value of the bias parameter b = 1/sigma_8 ~ 1.8, one has (delta_rho / rho)_{rms} ~ 1 r ~ 3.5/h Mpc, suggesting that the change of slope observed in xi(r) around this scale marks the transition between the linear and nonlinear gravitational regimes. Under this working hypothesis, we use a simple analytical form to fit the large-scale correlations constraints together with the COBE CMB anisotropy measurement, thus constructing a simple phenomenological model for the linear power spectrum. Despite its simplicity, the model fits remarkably well directly estimated power spectra from different optical galaxy samples, and when evolved through an N-body simulation it provides a good match to the observed galaxy correlations. One of the most interesting features of the model is the small-scale one-dimensional velocity dispersion produced: sigma_{1d} = 450 Km s^{-1} at 0.5/h Mpc and sigma_{1d} = 350 Km s^{-1} for separations larger than ~ 2/h Mpc.
description: ApJL in press, 10 pages in plain TeX, 3 figures available from guzzo@astmim.mi.astro.it, SISSA 110/93/A
Can Polarised Drell-Yan Shed More Light On The Proton Spin?
Creators: name: Mathews, Prakash
name: Ravindran, V.
Publisher: name: arXiv
Year: 1992
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We analyse polarised Drell-Yan process using the factorisation method and derive operator definitions for polarised parton distribution functions. We demonstrate that a factorisation analogous to that in the unpolarised Drell-Yan case holds in this process. We study the leading order gluonic contribution to the first moment of polarised Drell-Yan function and show that it is consistent with results obtained from polarised deep inelastic scattering.
description: 12 pages
Variability of Red Supergiants in M31 from the Palomar Transient Factory
Creators: name: Soraisam, Monika D.
name: Bildsten, Lars
name: Drout, Maria R.
name: Bauer, Evan B.
name: Gilfanov, Marat
name: Kupfer, Thomas
name: Laher, Russ R.
name: Masci, Frank
name: Prince, Thomas A.
name: Kulkarni, Shrinivas R.
name: Matheson, Thomas
name: Saha, Abhijit
Publisher: name: arXiv
Year: 2018
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: Most massive stars end their lives as Red Supergiants (RSGs), a short-lived evolution phase when they are known to pulsate with varying amplitudes. The RSG period-luminosity (PL) relation has been measured in the Milky Way, the Magellanic Clouds and M33 for about 120 stars in total. Using over 1500 epochs of R-band monitoring from the Palomar Transient Factory (PTF) survey over a five-year period, we study the variability of 255 spectroscopically cataloged RSGs in M31. We find that all RGSs brighter than M_K~ -10 mag (log(L/L_sun)>4.8) are variable at dm_R>0.05 mag. Our period analysis finds 63 with significant pulsation periods. Using the periods found and the known values of M_K for these stars, we derive the RSG PL relation in M31 and show that it is consistent with those derived earlier in other galaxies of different metallicities. We also detect, for the first time, a sequence of likely first-overtone pulsations. Comparison to stellar evolution models from MESA confirms the first overtone hypothesis and indicates that the variable stars in this sample have 12 M_sun
description: 17 pages, 10 figures
MOESM2 of Mapping visuospatial attention: the greyscales task in combination with repetitive navigated transcranial magnetic stimulation
Creators: name: Giglhuber, Katrin
name: Maurer, Stefanie
name: Zimmer, Claus
name: Meyer, Bernhard
name: Krieg, Sandro
Publisher: name: figshare
Year: 2018
Subjects: subject: Medicine
subject: Neuroscience
subject: Physiology
subject: FOS: Biological sciences
subject: Sociology
subject: FOS: Sociology
subject: 111714 Mental Health
subject: FOS: Health sciences

description: Additional file 2. Subject-related deviation scores per cortical spot for the right hemisphere Results for stimulation of the right hemisphere. Deviation scores of subject 1–10. Number of subjects with negative deviation scores (“leftward”) and mean of their scores. Number of subjects with positive deviation scores (“rightward”) and mean of their scores. Outline per cortical spot (no. 1–52) plus mean, standard deviation (SD), minimum (MIN), and maximum (MAX).
Breakdown of Dimensional Regularization in the Sudakov Problem
Creators: name: Collins, J. C.
name: Tkachov, F. V.
Publisher: name: arXiv
Year: 1992
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: An explicit example is presented (a one-loop triangle graph) where dimensional regularization fails to regulate the infra-red singularities that emerge at intermediate steps of studying large-$Q^2$ Sudakov factorization. The mathematical nature of the phenomenon is explained within the framework of the theory of the $As$-operation.
description: 12 pages + 3 figures (not included), LaTeX
A Perfect Specialization Model for Gravity Equation in Bilateral Trade based on Production Structure
Creators: name: Einian, Majid
name: Ravasan, Farshad Ranjbar
Publisher: name: arXiv
Year: 2018
Subjects: subject: Econometrics (econ.EM)
subject: General Finance (q-fin.GN)
subject: FOS: Economics and business

description: Although initially originated as a totally empirical relationship to explain the volume of trade between two partners, gravity equation has been the focus of several theoretic models that try to explain it. Specialization models are of great importance in providing a solid theoretic ground for gravity equation in bilateral trade. Some research papers try to improve specialization models by adding imperfect specialization to model, but we believe it is unnecessary complication. We provide a perfect specialization model based on the phenomenon we call tradability, which overcomes the problems with simpler initial. We provide empirical evidence using estimates on panel data of bilateral trade of 40 countries over 10 years that support the theoretical model. The empirical results have implied that tradability is the only reason for deviations of data from basic perfect specialization models.
description: 8 pages, 2 figures, 3 tables
MOESM2 of A mathematical model relates intracellular TLR4 oscillations to sepsis progression
Creators: name: Razvan Stan
name: Soriano, Francisco
name: Maristela Camargo
Publisher: name: figshare
Year: 2018
Subjects: subject: Medicine
subject: Genetics
subject: FOS: Biological sciences
subject: Immunology
subject: FOS: Clinical medicine
subject: 69999 Biological Sciences not elsewhere classified
subject: 80699 Information Systems not elsewhere classified
subject: FOS: Computer and information sciences
subject: 19999 Mathematical Sciences not elsewhere classified
subject: FOS: Mathematics
subject: Inorganic Chemistry
subject: FOS: Chemical sciences
subject: Hematology

description: Additional file 2: Table S1. Modeling and clinical data of sepsis patients. Table S2. Clinical qPCR data.
Gauge Model of Generation Nonuniversality Reexamined
Creators: name: Li, Xiaoyuan
name: Ma, Ernest
Publisher: name: arXiv
Year: 1992
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: A gauge model of generation nonuniversality proposed in 1981 is reexamined in the light of present precision electroweak measurements. Two necessary features of this model are that the tau lifetime should be longer than predicted by the standard model and that the rho parameter measured at the Z peak should have an additional negative contribution. Both trends are noticeable in present data. A future decisive test of this model would be the discovery of new W and Z bosons with nearly degenerate masses of a few TeV.
description: 19 pages (5 figures, not included)
Empirical Constraints on Cosmological Gamma-Ray Bursts
Creators: name: Woods, Eric
name: Loeb, Abraham
Publisher: name: arXiv
Year: 1994
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We place empirical constraints on the physical properties of $γ-$ray burst events at cosmological distances. In particular we derive probability distributions for the radiation energy $E_γ$, the minimum Lorentz factor $γ_{\rm min}$, the maximum baryonic mass $M_{\rm max}$ and the upper bound on the surrounding gas density $n_{\rm max}$ in the events, based on 169 bursts from the first BATSE catalog. Using peak flux as a distance indicator we probe bursts where the constraints are stronger than average. The resulting variance and skewness of the cosmological probability distributions are calculated in addition to their mean values: $\langle E_γ\rangle=4\times 10^{51} h^{-2} {\rm erg}$, $\langle γ_{\rm min}\rangle= 5\times 10^2$, $\langle M_{\rm max}\rangle=10^{-5}ξ^{-1} M_\odot$, and $\langle (γ/γ_{\rm min})^{-5} n_{\rm max}\rangle\lsim 10^{2} ξ^{-1}{\rm cm^{-3}}$, where $ξ$ is the fraction of the total energy which is converted to $γ-$rays. The distribution of burst energies ends at about $10^{53} {\rm erg}$, close to the binding energy of a neutron star.
description: 13 pages, TEX, 2 figures can be obtained from woods@cfata3.harvard.edu
Additional file 2: of Genome-wide analysis and identification of the low potassium stress responsive gene SiMYB3 in foxtail millet (Setariaitalica L.)
Creators: name: Cao, Xinyou
name: Hu, Liqin
name: Chen, Xueyan
name: Zhang, Rongzhi
name: Cheng, Dungong
name: Li, Haosheng
name: Xu, Zhaoshi
name: Li, Liancheng
name: Zhou, Yongbin
name: Liu, Aifeng
name: Song, Jianming
name: Liu, Cheng
name: Liu, Jianjun
name: Zhao, Zhendong
name: Chen, Ming
name: Ma, Youzhi
Publisher: name: figshare
Year: 2019
Subjects: subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Evolutionary Biology
subject: Biological Sciences not elsewhere classified
subject: Developmental Biology

description: Text S1. The sequence of SiMYB3. (DOCX 11 kb)
SensApp_Deliverbale_D4.1_ Integrated system for calibration and testing_Video
Creators: name: Uusitalo, Sanna
name: Pennala Riku
name: Anetjärvi Markus
name: Aikio Sanna
Publisher: name: Zenodo
Year: 2021
Subjects: Integrated system

description: Integrated system for calibration and testing
New disk discovered with VLT/SPHERE around the M star GSC 07396-00759
Creators: name: Sissa, E.
name: Olofsson, J.
name: Vigan, A.
name: Augereau, J. C.
name: D'Orazi, V.
name: Desidera, S.
name: Gratton, R.
name: Rigliaco, M. Langlois E.
name: Boccaletti, A.
name: Kral, Q.
name: Lazzoni, C.
name: Mesa, D.
name: Messina, S.
name: Sezestre, E.
name: Thébault, P.
name: Zurlo, A.
name: Bhowmik, T.
name: Bonnefoy, M.
name: Chauvin, G.
name: Feldt, M.
name: Hagelberg, J.
name: Lagrange, A. -M.
name: Janson, M.
name: Maire, A. -L.
name: Ménard, F.
name: Schlieder, J.
name: Schmidt, T.
name: Szulágyi, J.
name: Stadler, E.
name: Deboulbé, D. Maurel A.
name: Feautrier, P.
name: Ramos, J.
name: Rigal, R.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: FOS: Physical sciences

description: Debris disks are usually detected through the infrared excess over the photospheric level of their host star. The most favorable stars for disk detection are those with spectral types between A and K, while the statistics for debris disks detected around low-mass M-type stars is very low, either because they are rare or because they are more difficult to detect. Terrestrial planets, on the other hand, may be common around M-type stars. Here, we report on the discovery of an extended (likely) debris disk around the M-dwarf GSC 07396-00759. The star is a wide companion of the close accreting binary V4046 Sgr. The system probably is a member of the $β$ Pictoris Moving Group. We resolve the disk in scattered light, exploiting high-contrast, high-resolution imagery with the two near-infrared subsystems of the VLT/SPHERE instrument, operating in the YJ bands and the H2H3 doublet. The disk is clearly detected up to 1.5" ($\sim110$ au) from the star and appears as a ring, with an inclination $i\sim83$ degree, and a peak density position at $\sim 70$ au. The spatial extension of the disk suggests that the dust dynamics is affected by a strong stellar wind, showing similarities with the AU Mic system that has also been resolved with SPHERE. The images show faint asymmetric structures at the widest separation in the northwest side. We also set an upper limit for the presence of giant planets to $2 M_J$. Finally, we note that the 2 resolved disks around M-type stars of 30 such stars observed with SPHERE are viewed close to edge-on, suggesting that a significant population of debris disks around M dwarfs could remain undetected because of an unfavorable orientation.
description: 10 pages, 10 figures, in press by A&A
title: ADCO, Cinquième cartulaire de Saint-Étienne de Dijon (1664), Cart. 28 (G 132), 258 folios, f. 00168
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: Chartes de la Bourgogne du Moyen Âge
subject: cartulaire
subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris
subject: Corpus Burgundiae Medii Aevi

description: Cinquième cartulaire de Saint-Étienne de Dijon (1664), Archives départementales de la Côte-d'Or, Cart. 28 (G 132), 258 folios, f. 00168, Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Cinquième cartulaire de Saint-Étienne de Dijon (1664), Archives départementales de la Côte-d'Or, Cart. 28 (G 132), 258 folios, f. 00168, 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
Soft dilepton production in relativistic heavy ion collisions
Creators: name: Haglin, K.
name: Gale, C.
name: Emel'yanov, V.
Publisher: name: arXiv
Year: 1992
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: Production of electron-positron pairs with invariant masses less than 300 MeV from thermalized hadronic matter in relativistic heavy ion collisions is calculated using a soft virtual photon approximation. The general theoretical framework is reviewed and extended to include arbitrarily massed and charged reaction partners, which we apply to pions and quarks. This result, exact within the soft photon approximation, is compared with a widely used approximate result which uses an electromagnetic amplitude limited in validity to momentum transfers less than $4m_{π(q)}^{2}$. A comparison is made between the rate of production of zero total momentum soft dileptons obtained using resummation techniques in QCD perturbation theory to that which we calculate using this soft photon approximation.
description: 29 pages typed in revtex, 13 figures (not included), hardcopy available by regular mail upon request, McGill/92-33
A Spectroscopic Method to Measure Macho Proper Motions
Creators: name: Maoz, Dan
name: Gould, Andrew
Publisher: name: arXiv
Year: 1994
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: A Massive Compact Halo Object (Macho) that lenses a background star will magnify different parts of the rotating stellar disk by varying amounts. The differential magnification will cause a shift in the centroid of the star's spectral lines during the lensing event. The shift is proportional to the ratio of the stellar radius to the projected separation of the Macho from the star. It therefore provides a direct measure of the Einstein ring radius, and so also a measure of the Macho's proper motion (angular speed). This measurement can remove some of the degeneracy between mass, distance to the lens, and transverse velocity that exists in the interpretation of results from ongoing microlensing experiments, and is an independent test of the lensing nature of the event. We show that using the high precision attainable by stellar radial velocity measurements, it is possible to measure proper motions for $\sim 10\%$ of Machos that lens A-stars in the Large Magellanic Cloud (LMC), i.e.\ $\sim 7\%$ of the type of relatively high-magnification events that have been reported to date. If this proper-motion measurement were combined with a parallax measurement of the ``reduced velocity'', then the Macho mass, distance, speed, and direction could each be separately determined. The shift can be measured for $\sim 20\%$ of the A-star events generated by Machos in the dark halo of the LMC. This in turn would provide a measurement of the fraction of LMC vs. Galactic Macho events.
description: 16 pages, LaTex, two PostScript figures, OSU-TA-1/94
The Stretched Horizon and Black Hole Complementarity
Creators: name: Susskind, L.
name: Thorlacius, L.
name: Uglum, J.
Publisher: name: arXiv
Year: 1993
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: Three postulates asserting the validity of conventional quantum theory, semi-classical general relativity and the statistical basis for thermodynamics are introduced as a foundation for the study of black hole evolution. We explain how these postulates may be implemented in a ``stretched horizon'' or membrane description of the black hole, appropriate to a distant observer. The technical analysis is illustrated in the simplified context of 1+1 dimensional dilaton gravity. Our postulates imply that the dissipative properties of the stretched horizon arise from a course graining of microphysical degrees of freedom that the horizon must possess. A principle of black hole complementarity is advocated. The overall viewpoint is similar to that pioneered by 't~Hooft but the detailed implementation is different.
description: (some misprints in equations have been fixed), 48 pages (including figures), SU-ITP-93-15
title: ADCO, Cartulaire de Cîteaux pour les possessions de Chaugey et Maison-Dieu (Fin XVe siècle), Cart. 180 (11 H 755), 83 folios, f. 0088
Creators: name: de la Côte d'Or, Archives départementales
name: Archives Départementales De La Côte-D'Or
name: Petot, Frédérique
name: Projet CBMA
name: CG21/F.PETOT/2017
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2020
Subjects: subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris
subject: Corpus Burgundiae Medii Aevi
subject: Chartes de la Bourgogne du Moyen Âge
subject: cartulaire

description: Cartulaire de Cîteaux pour les possessions de Chaugey et Maison-Dieu (Fin XVe siècle), Archives départementales de la Côte-d'Or, Cart. 180 (11 H 755), 83 folios, f. 0088, Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Cartulaire de Cîteaux pour les possessions de Chaugey et Maison-Dieu (Fin XVe siècle), Archives départementales de la Côte-d'Or, Cart. 180 (11 H 755), 83 folios, f. 0088, in Projet CBMA - Corpus Burgundiae Medii Aevi [Ressource en ligne], https:// manuscrits.cbma-project.eu/
description: Provenance: abbaye de Cîteaux
description: Provenance: http://www.wikidata.org/entity/Q843261
description: Provenance: https://www.geonames.org/3024876
description: Provenance: http://www.idref.fr/030974844/id
description: Provenance: https://catalogue.bnf.fr/ark:/12148/cb12228351v
Fragmentation of Transversely Polarized Quarks Probed in Transverse Momentum Distributions
Creators: name: Collins, John
Publisher: name: arXiv
Year: 1992
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: It is shown that the azimuthal dependence of the distribution of hadrons in a quark jet is a probe of the transverse spin of the quark initiating the jet. This results in a new spin-dependent fragmentation function that acts at the twist-2 level. One example of a process where it contributes is semi-inclusive deeply inelastic scattering with a transversely polarized nucleon target but with an {\em unpolarized} electron beam. This process is treated in detail. Another process is the cross section for singly polarized hadron-hadron scattering when two high $p_{\perp}$ hadrons are measured in the final state and are close to back-to-back in azimuth. The new fragmentation function is sensitive to the coupling of the fragmentation process to (spontaneous) chiral symmetry breaking.
description: 22 pages + 4 figures (included), LaTeX. V. 2 has misprints corrected and an appendix added, as in the published version
Large Scale Morphological Segregation in Optically Selected Galaxy Redshift Catalogs
Creators: name: Dominguez-Tenreiro, R.
name: Campos, A.
name: Gómez-Flechoso, M. A.
name: Yepes, G.
Publisher: name: arXiv
Year: 1994
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present the results of an exhaustive analysis of the morphological segregation of galaxies in the CfA and SSRS catalogs through the scaling formalism. Morphological segregation between ellipticals and spirals has been detected at scales up to 15-20 h$^{-1}$ Mpc in the CfA catalog, and up to 20-30 h$^{-1}$ Mpc in the SSRS catalog. Moreover, it is present not only in the densest areas of the galaxy distribution, but also in zones of moderate density.
description: 9 pages, (1 figure included), uuencode compressed Postscript, (accepted for publication in ApJ Letters), FTUAM-93-25