cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
title: ADCO, Cartulaire de Cîteaux pour les possessions de Saulon-la-Chapelle et Saulon-la-Rue, Fénay, Noiron et la rivière Cent-fonds (XVe siècle), Cart. 179 (11 H 1075), 70 folios, f. 0099
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/2015
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 de Cîteaux pour les possessions de Saulon-la-Chapelle et Saulon-la-Rue, Fénay, Noiron et la rivière Cent-fonds (XVe siècle), Archives départementales de la Côte-d'Or, Cart. 179 (11 H 1075), 70 folios, f. 0099, Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Cartulaire de Cîteaux pour les possessions de Saulon-la-Chapelle et Saulon-la-Rue, Fénay, Noiron et la rivière Cent-fonds (XVe siècle), Archives départementales de la Côte-d'Or, Cart. 179 (11 H 1075), 70 folios, f. 0099, 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
Additional file 1 of Mild pulmonary hemodynamic alterations in patients with systemic sclerosis: relevance of the new 2022 ESC/ERS definition of pulmonary hypertension and impact on mortality
Creators: name: Puigrenier, Sébastien
name: Giovannelli, Jonathan
name: Lamblin, Nicolas
name: De Groote, Pascal
name: Fertin, Marie
name: Bervar, Jean-François
name: Lamer, Antoine
name: Edmé, Jean-Louis
name: Balquet, Marie-Hélène
name: Sobanski, Vincent
name: Launay, David
name: Hachulla, Éric
name: Sanges, Sébastien
Publisher: name: figshare
Year: 2022
Subjects: subject: Medicine
subject: Biotechnology
subject: Ecology
subject: FOS: Biological sciences
subject: Science Policy

description: Additional file 1: Multivariate analysis after adjusting for age, sex, SSc type, disease duration, presence of ILD, NYHA functional class and treatment.
PKS 1004+13: A High-Inclination, Highly-Absorbed Radio-Loud QSO -- The First Radio-Loud BAL QSO at Low Redshift?
Creators: name: Wills, Beverley J.
name: Brandt, W. N.
name: Laor, A.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: The existence of BAL outflows in only radio-quiet QSOs was thought to be an important clue to mass ejection and the radio-loud - radio-quiet dichotomy. Recently a few radio-loud BAL QSOs have been discovered at high redshift. We present evidence that PKS 1004+13 is a radio-loud BAL QSO. It would be the first known at low-redshift (z = 0.24), and one of the most radio luminous. For PKS 1004+13, there appear to be broad absorption troughs of O VI, N V, Si IV, and C IV, indicating high-ionization outflows up to about 10,000 km/s. There are also two strong, broad (~500 km/s), high-ionization, associated absorption systems that show partial covering of the continuum source. The strong UV absorption we have detected suggests that the extreme soft-X-ray weakness of PKS 1004+13 is primarily the result of absorption. The large radio-lobe dominance indicates BAL and associated gas at high inclinations to the central engine axis, perhaps in a line-of-sight that passes through an accretion disk wind.
description: To appear in Ap.J. Letters, 1999 (June or July); 4 pages, 5 figures
Library, librarian and library services in web 2.0 environment
Creators: name: KHAN, IMRAN
Publisher: name: figshare
Year: 2022
Subjects: subject: Library and Information Studies
subject: FOS: Media and communications
subject: 80799 Library and Information Studies not elsewhere classified
subject: 80706 Librarianship

description: Khan, Imran. (2013). Library, librarian and library services in web 2.0 environment. International Journal of Digital Library Services 3(4): pp. 14-36 [ISSN: 2349-302X (P), 2250-1142 (E)].
A Solution to the Polonyi Problem in the Minimum SUSY-GUT
Creators: name: Moroi, T.
name: Yanagida, T.
Publisher: name: arXiv
Year: 1994
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We show that the Polonyi problem is solved in the minimum SUSY-GUT model in which a self-coupling strength for a heavy Higgs $Σ$, $λΣ^{3}$, is very small $λ\sim 10^{-6}$. It is stressed that with this small $λ$ the mass of the physical $Σ$ becomes $m_Σ \sim 10^{12}\GEV$ and the unification scale is raised up to the gravitational one, $M\simeq 2\times 10^{18}\GEV$. A potential problem, however, is also pointed out in this GUT model.
QCD corrections to the t-->H+b decay within the minimal supersymmetric standard model
Creators: name: König, Heinz
Publisher: name: arXiv
Year: 1994
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: I present the contribution of gluinos and scalar quarks to the decay rate of the top quark into a charged Higgs boson and a bottom quark within the minimal supersymmetric standard model, including the mixing of the scalar partners of the left- and right-handed top quark. I show that for certain values of the supersymmetric parameters the standard QCD loop corrections to this decay mode are diminished or enhanced by several 10 per cent. I show that not only a small value of 3 GeV for the gluino mass (small mass window) but also much larger values of several hundreds of GeV's have a non-neglible effect on this decay rate, against general belief. Last but not least, if the ratio of the vacuum expectation values of the Higgs bosons are taken in the limit of $v_1\ll v_2$ I obtain a drastic enhancement due to a $\tanβ$\ dependence in the couplings.
description: UQAM-PHE-94/01, 6 pages, plain tex, 4 figures not included, available under request via mail or fax
Additional file 1: of Characterization of the hot pepper (Capsicum frutescens) fruit ripening regulated by ethylene and ABA
Creators: name: Bing-Zhu Hou
name: Li, Chun-Li
name: Han, Ying-Yan
name: Yuan-Yue Shen
Publisher: name: figshare
Year: 2018
Subjects: subject: Biochemistry
subject: Medicine
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Biotechnology
subject: Evolutionary Biology
subject: 69999 Biological Sciences not elsewhere classified
subject: Developmental Biology
subject: Marine Biology
subject: 110309 Infectious Diseases
subject: FOS: Health sciences
subject: Plant Biology

description: Table S1. The primers for qPCR based on RNA-Seq data. Figure S1. Phenotype of the red, cluster, upright and hot pepper plant (Capsicum frutescens, cv. â Chaotianjiao 6â ). Figure S2. Fluridone-promotion of the fruit coloration is related to squalene synthase (SQS) expression at transcription levels. (DOC 4362 kb)
title: 02_1177
Creators: name: Wesley Baldwin, John
name: Baldwin, John W.
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2018
Subjects: subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris

description: L'ensemble de ces notes ont été crée par John Baldwin lors d'une de ses premières périodes de résidence à Paris. Ces documents comprennent tous les magistri qu’il avait pu rencontrer dans ses sources. Aux XIIème et XIIIème siècles, les universités n'existant pas encore, le titre de magister s'il évoque certainement une compétence n'est pas rattaché de façon systématique au passage par les écoles. De surcroît, les magistris sont le plus souvent désignés par leur seul prénom. La lecture de ces données est donc difficile et suppose un long travail pour tenter d'identifier un individu auquel on pourrait rattacher plusieurs mentions. John Baldwin avait donc renoncé à utiliser ces données pour donner un prolongement à sa magnifique étude sur les gradués d'université et leur emploi par les Capétiens et les Plantagenêts. Néanmoins, il a conservé ces données et elles sont potentiellement très utile dans le cadre de Studium, comme le sont toutes les mentions dans les volumes des Fasti Ecclesiae Gallicanae de chanoines portant ce titre de magister sans autres précisions. L'ampleur des dépouillements rend ces données très utiles et nous devons une grande reconnaissance à John Baldwin pour avoir pris la peine de faire photocopier ses fiches et de nous les avoir transmises amicalement.
Les données ainsi que les images des fiches sont accessibles sur le site Internet à l'adresse suivante : http://studium-baldwin.lamop.fr/.
Les transcriptions des fiches ont été effectuées par des étudiants de Paris 1 Panthéon - Sorbonne mais elles n'ont pas été corrigées par la suite.
description: Relation: https://lamop.hypotheses.org/
Stable, Spinning Embedded Vortices
Creators: name: Perivolaropoulos, Leandros
Publisher: name: arXiv
Year: 1994
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: The spinning vortex is a stationary generalization of the Nielsen-Olesen vortex involving a linear time dependence of the Goldstone boson. Here we show that this vortex can be embedded in models with $SU(2)_{global}\times U(1)_{local}$ symmetry. We also map the stability sector in parameter space and show that for sufficiently large spinning velocities the vortex is stable for {\it any} value of the Higgs self coupling parameter $β$. This is a significant improvement of stability compared to the semilocal vortex introduced by Vachaspati and Achucarro which is stable only for $β<1$. This result may have significant implications for electroweak vortices.
description: 11 pages plus 2 figures (available in a postscript file from the author), submitted to Phys. Rev. D. Use LaTeX. Preprint No. CfA-3824
Propositioning Investigative Historiography as a niche  subfield within Twenty-first Century Historiography:  Making a case for Investigative historiography in  Twenty-first Century Social Sciences
Creators: name: Rao Mandavilli, Sujay
Publisher: name: Zenodo
Year: 2024

description: This is our fifth paper on twenty-first century historiography. In the first paper, which was published by us in the year 2015, we had defined and set forth the core objectives of what we called twentyfirst century historiography. In the second paper published by us in 2016, we had postulated the core principles of twenty-first century historiography. In the third paper published by us in 2018, we had had introduced the concept of Anthropological Historiography wherein we had sought to integrate history with pre-history and proto-history much better. In the fourth paper on qualified historiography published by us in 2022, we had tried to explain how historiography could be dealt with in the case of the unreliability and uncertainty of narratives. In the present paper, we put forward a case for investigative historiography which can be developed as a niche area well within mainstream twenty-first century historiography. The objective of this niche sub-field would be to lay bare the tools, techniques and the scientific methods that could be employed and put to use in carrying out historical investigations. Some of these tools and techniques may already exist and may already be in use, but we put forward new approaches keeping in mind the overall philosophy of twenty-first century historiography. Of course, the outputs of investigative historiography would provide crucial inputs into mainstream twenty-first century historiography, and investigative historiography would be an essential cog in the wheel of historical and scientific research.
Additional file 1 of Diagnostic and prognostic value of ventilatory power in pulmonary hypertension
Creators: name: Li, Xin
name: Zhang, Yi
name: Jin, Qi
name: Zhao, Zhihui
name: Zhao, Qing
name: Yan, Lu
name: Duan, Anqi
name: Huang, Zhihua
name: Hu, Meixi
name: Xiong, Changming
name: Luo, Qin
name: Liu, Zhihong
Publisher: name: figshare
Year: 2022
Subjects: subject: Medicine
subject: Cell Biology
subject: Immunology
subject: FOS: Clinical medicine
subject: Mathematical Sciences not elsewhere classified
subject: Cancer

description: Additional file 1: Supplementary figures.
title: Densités de populations [Haute Moulouya]
title: Densités de populations [Haute Moulouya]
Creators: name: :Unkn
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2023
Subjects: subject: Démographie
subject: Densité démographique

description: Cartographie
description: BESM-carto_1960-86-87-p298_86-87-07
description: 87
description: 86
description: Bulletin économique et social du Maroc
description: Source: Maison méditerranéenne des sciences de l'homme, Cité numérique de la Méditerranée (Cinumed), Bibliothèque nationale du Royaume du Maroc (BNRM)
description: Source: Bulletin économique et social du Maroc
description: Source: Bulletin économique et social du Maroc (BESM) > BESM (Cartographie)
description: Relation: https://cinumed.mmsh.univ-aix.fr/idurl/1/81853
description: Coverage: Moulouya
description: Coverage: Maroc
description: Coverage: XXe siècle
description: Temporal: XXe siècle
description: Bibliographic citation: « Densités de populations [Haute Moulouya] », In Bulletin économique et social du Maroc (BESM), n° 86, 1960
description: Provenance: Maison méditerranéenne des sciences de l'homme, Cité numérique de la Méditerranée (Cinumed), Bibliothèque nationale du Royaume du Maroc (BNRM)
description: Provenance: https://cinumed.mmsh.univ-aix.fr/
GRB 970228 Revisited: Evidence for a Supernova in the Light Curve and La te Spectral Energy Distribution of the Afterglow
Creators: name: Reichart, Daniel E.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: At the time of its discovery, the optical and X-ray afterglow of GRB 970228 appeared to be a ringing endorsement of the previously untried relativistic fireball model of gamma-ray burst (GRB) afterglows, but now that nearly a dozen optical afterglows to GRBs have been observed, the wavering light curve and reddening spectrum of this afterglow make it perhaps the most difficult of the observed afterglows to reconcile with the fireball model. In this Letter, we argue that this afterglow's unusual temporal and spectral properties can be attributed to a supernova that overtook the light curve nearly two weeks after the GRB. This is the strongest case yet for a GRB/supernova connection. It strengthens the case that a supernova also dominated the late afterglow of GRB 980326, and the case that GRB 980425 is related to SN 1998bw.
description: Accepted to The Astrophysical Journal (Letters), 14 pages, LaTeX
Approximating Stellar Orbits: Improving on Epicycle Theory
Creators: name: Dehnen, Walter
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Already slightly eccentric orbits, such as those occupied by many old stars in the Galactic disk, are not well approximated by Lindblad's epicycle theory. Here, alternative approximations for flat orbits in axisymmetric stellar systems are derived and compared to results from numeric integrations. All of these approximations are more accurate than Lindblad's classical theory. I also present approximate, but canonical, maps from ordinary phase-space coordinates to a set of action-angle variables. Unfortunately, the most accurate orbit approximation leads to non-analytical R(t). However, from this approximation simple and yet very accurate estimates can be derived for the peri- and apo-centers, frequencies, and actions integrals of galactic orbits, even for high eccentricities. Moreover, further approximating this approximation allows for an analytical R(t) and still an accurate approximation to galactic orbits, even with high eccentricities.
description: accepted for publication in AJ; 12 pages LaTeX, 9 figures (coloured only here, not in AJ) uses aas2pp4.sty
Notes on Oscillator-Like Interactions of Various Spin Relativistic Particles
Creators: name: Dvoeglazov, Valeri V.
name: Mesa, Antonio del Sol
Publisher: name: arXiv
Year: 1994
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: The equations for various spin particles with oscillator-like interactions are discussed in this talk. Contents: 1. Comment on "The Klein-Gordon Oscillator"; 2. The Dirac oscillator in quaternion form; 3. The Dirac-Dowker oscillator; 4. The Weinberg oscillator; 5. Note on the two-body Dirac oscillator.
description: LaTeX file, 12 pp. Talk given at the Second Workshop "Osciladores Arm\'onicos". Cocoyoc, M\'exico, March 23-25, 1994. To be published in NASA Conference Proceedings. Preprint IFUNAM FT-94-44, EFUAZ-94-01
Simple Distribution Functions for Stellar Disks
Creators: name: Dehnen, Walter
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Distribution functions (DFs) for dynamically warm thin stellar disks residing in arbitrary axisymmetric potentials are presented which approximately reproduce pre-described surface-density and velocity-dispersion profiles. The functional form of the DFs is obtained by `warming-up' a model made entirely of circular orbits. This can be done in various ways giving different functional forms for the DF. In the best case, the DF reproduces the pre-described profiles to within a few per cent for a typical case reminiscent to the old stellar disk in the Milky Way. This match may be improved to about one per cent or better by a simple iterative method. An algorithm is given to draw phase-space points randomly from the DFs for the purpose of, e.g., N-body simulations. All the relevant computer programs are available from the author.
description: accepted for publication in AJ, 10 pages, 5 figures (coloured only here, not in AJ), uses aas2pp4.sty
title: ADCO, Neuvième cartulaire de Saint-Étienne de Dijon (1661 - 1684), Cart. 32 (G 136), 745 folios, f. 0663
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: Laboratoire de Médiévistique Occidentale de Paris
subject: Corpus Burgundiae Medii Aevi
subject: Chartes de la Bourgogne du Moyen Âge
subject: cartulaire
subject: LaMOP

description: Neuvième cartulaire de Saint-Étienne de Dijon (1661 - 1684), Archives départementales de la Côte-d'Or, Cart. 32 (G 136), 745 folios, f. 0663, Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Neuvième cartulaire de Saint-Étienne de Dijon (1661 - 1684), Archives départementales de la Côte-d'Or, Cart. 32 (G 136), 745 folios, f. 0663, 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
Correlated emission and spin-down variability in radio pulsars
Creators: name: Shaw, Benjamin
name: Stappers, Benjamin W.
name: Brook, Paul R.
name: Karastergiou, Aris
name: Lyne, Andrew G.
name: Weltevrede, Patrick
Publisher: name: arXiv
Year: 2018
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: The recent revelation that there are correlated period derivative and pulse shape changes in pulsars has dramatically changed our understanding of timing noise as well as the relationship between the radio emission and the properties of the magnetosphere as a whole. Using Gaussian processes we are able to model timing and emission variability using a regression technique that imposes no functional form on the data. We revisit the pulsars first studied by Lyne et al. (2010). We not only confirm the emission and rotational transitions revealed therein, but reveal further transitions and periodicities in 8 years of extended monitoring. We also show that in many of these objects the pulse profile transitions between two well-defined shapes, coincident with changes to the period derivative. With a view to the SKA and other telescopes capable of higher cadence we also study the detection limitations of period derivative changes.
description: 4 pages, 2 Figures, Proceedings of IAU Symposium 337 "Pulsar Astrophysics - The Next 50 Years" held at Jodrell Bank Observatory, UK Sept. 4-8 2017
Additional file 3: of Citrulline malate supplementation does not improve German Volume Training performance or reduce muscle soreness in moderately trained males and females
Creators: name: Chappell, Andrew
name: Allwood, Daniel
name: Johns, Rebecca
name: Brown, Samantha
name: Sultana, Kiran
name: Anand, Annie
name: Simper, Trevor
Publisher: name: figshare
Year: 2018
Subjects: subject: Physiology
subject: FOS: Biological sciences
subject: 59999 Environmental Sciences not elsewhere classified
subject: FOS: Earth and related environmental sciences
subject: Sociology
subject: FOS: Sociology
subject: Developmental Biology

description: Mean Number of Repetitions Performed Per Set, with and without Citrulline Malate Supplementation. (PDF 11 kb)
Interaction between the Intergalactic Medium and Galactic Outflows from Dwarf Galaxies
Creators: name: Murakami, I.
name: Babul, A.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We have carried out 2D hydrodynamical simulations in order to study the interaction between supernova-powered gas outflows from low-mass galaxies and the local intergalactic medium (IGM). We are specifically interested in investigating whether a high pressure IGM, such as that in clusters of galaxies, can prevent the gas from escaping from the galaxy. The interface between the outflow and ambient IGM is demarcated by a dense expanding shell formed by the gas swept-up by the outflow. A sufficiently high IGM pressure can bring the shell to a halt well before it escapes the galaxy. Galaxies in such high pressure environments are, however, to be ploughing through the IGM at relatively high velocities. Hence, they will also be subject to ram pressure, which acts to strip the gas from the galaxy. We have carried out simulations that take into account the combined impact of ram pressure and thermal pressure. We find that ram pressure deforms the shell into a tail-like structure, fragments it into dense clouds and eventually drags the clouds away from the galaxy. The clouds are potential sites of star formation and if viewed during this transient phase, the galaxy will appear to have a low-surface brightness tail much like the galaxies with diffuse comet-like tail seen in z=1.15 cluster 3C324. In contrast, the relatively unhindered outflows in low density, low temperature environments can drive the shells of swept-up gas out to large distances from the galaxy. Such shells, if they intersect a quasar line-of-sight, would give rise to Ly $α$ absorption lines of the kind seen in quasar spectra.
description: 32 pages, 6 encapsulated Postscript figures, 7 gif figures. Accepted for publication in MNRAS
Certifying reality of projections
Creators: name: Hauenstein, Jonathan
name: Kulkarni, Avinash
name: Sertöz, Emre Can
name: Sherman, Samantha
Publisher: name: arXiv
Year: 2018
Subjects: subject: Algebraic Geometry (math.AG)
subject: Numerical Analysis (math.NA)
subject: FOS: Mathematics
subject: 14Q99, 14P05, 14Q05

description: Computational tools in numerical algebraic geometry can be used to numerically approximate solutions to a system of polynomial equations. If the system is well-constrained (i.e., square), Newton's method is locally quadratically convergent near each nonsingular solution. In such cases, Smale's alpha theory can be used to certify that a given point is in the quadratic convergence basin of some solution. This was extended to certifiably determine the reality of the corresponding solution when the polynomial system is real. Using the theory of Newton-invariant sets, we certifiably decide the reality of projections of solutions. We apply this method to certifiably count the number of real and totally real tritangent planes for instances of curves of genus 4.
description: 9 pages
Approaching a homogeneous galaxy distribution: results from the Stromlo-APM redshift survey
Creators: name: Hatton, S. J.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Recent results from a number of redshift surveys suggest that the Universe is well described by an inhomogeneous, fractal distribution on the largest scales probed. This distribution has been found to have fractal dimension, D, approximately equal to 2.1, in contrast to a homogeneous distribution in which the dimension should approach the value 3 as the scale is increased. In this paper we demonstrate that estimates of D, based on the conditional density of galaxies, are prone to bias from several sources. These biases generally result in a smaller measured fractal dimension than the true dimension of the sample. We illustrate this behaviour in application to the Stromlo-APM redshift survey, showing that this dataset in fact provides evidence for fractal dimension increasing with survey depth. On the largest scale probed, r approximately 60 h^{-1}Mpc, we find evidence for a distribution with dimension D = 2.76 +/- 0.10. A comparison between this sample and mock Stromlo-APM catalogues taken from Nbody simulations (which assume a CDM cosmology) reveals a striking similarity in the behaviour of the fractal dimension. Thus we find no evidence for inhomogeneity in excess of that expected from conventional cosmological theory. We consider biases affecting future large surveys and demonstrate, using mock SDSS catalogues, that this survey will be able to measure the fractal dimension on scales at which we expect to see full turn-over to homogeneity, in an accurate and unbiased way.
description: 9 pages, changes made to agree with published version, accepted by MNRAS
Imitate or innovate: competition of strategy updating attitudes in spatial social dilemma games
Creators: name: Danku, Zsuzsa
name: Wang, Zhen
name: Szolnoki, Attila
Publisher: name: arXiv
Year: 2018
Subjects: subject: Physics and Society (physics.soc-ph)
subject: Adaptation and Self-Organizing Systems (nlin.AO)
subject: Populations and Evolution (q-bio.PE)
subject: FOS: Physical sciences
subject: FOS: Biological sciences

description: Evolution is based on the assumption that competing players update their strategies to increase their individual payoffs. However, while the applied updating method can be different, most of previous works proposed uniform models where players use identical way to revise their strategies. In this work we explore how imitation-based or learning attitude and innovation-based or myopic best response attitude compete for space in a complex model where both attitudes are available. In the absence of additional cost the best response trait practically dominates the whole snow-drift game parameter space which is in agreement with the average payoff difference of basic models. When additional cost is involved then the imitation attitude can gradually invade the whole parameter space but this transition happens in a highly nontrivial way. However, the role of competing attitudes is reversed in the stag-hunt parameter space where imitation is more successful in general. Interestingly, a four-state solution can be observed for the latter game which is a consequence of an emerging cyclic dominance between possible states. These phenomena can be understood by analyzing the microscopic invasion processes, which reveals the unequal propagation velocities of strategies and attitudes.
description: 7 two-column pages, 6 figures, accepted for publication in EPL
Signals of Disoriented Chiral Condensate
Creators: name: Huang, Zheng
name: Suzuki, Mahiko
name: Wang, Xin-Nian
Publisher: name: arXiv
Year: 1994
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: Nuclear Theory (nucl-th)
subject: FOS: Physical sciences

description: If a disoriented chiral condensate is created over an extended space-time region following a rapid cooling in hadronic or nuclear collisions, the misalignment of the condensate with the electroweak symmetry breaking can generate observable effects in the processes which involve both strong and electromagnetic interactions. We point out the relevance of the dilepton decay of light vector mesons as a signal for formation of the disoriented condensate. We predict that the decay ρ^0 to dileptons will be suppressed and/or the ρresonance peak widens, while the decay ωto dileptons will not be affected by the condensate.
description: 13 pages in LaTeX, UCB-PTH-94/05, LBL-35337
A relação entre as práticas de GRH e a inovação numa empresa tecnológica
Creators: name: Pinto, Eulália Cristina
name: Rodrigues, Ana C.
name: Lousã, Eva Petiz
Publisher: name: Conferência - Investigação e Intervenção em Recursos Humanos
Year: 2019

description: Recentemente, a literatura tem estudado como as empresas alcançam os seus objetivos com o recurso às práticas de Gestão de Recursos Humanos e como estas influenciam a inovação. Alguns autores defendem que a inovação e as práticas de Gestão de Recursos Humanos estão conectadas, mas a natureza dessa relação ainda não está completamente compreendida, sendo que, a inovação pode ser conceptualizada como o resultado da relação da Gestão de Recursos Humanos, quando várias práticas da Gestão de Recursos Humanos são aplicadas, isoladas ou em categorias, e exercem influência na inovação, através de várias condições. Nesse sentido, este artigo pretende analisar em profundidade as práticas de Gestão de Recursos Humanos e a sua relação com a inovação numa empresa tecnológica.
description: Conferência - Investigação e Intervenção em Recursos Humanos, n. 9 (2019): IX Conferência Internacional de Investigação e Intervenção em RH
title: Начало гиперреальности: неомиф и трансвиртуальность
Creators: name: Мурыгин, Георгий
name: Лир, Л.
Publisher: name: Новгородский государственный университет имени Ярослава Мудрого (НовГУ)
Year: 2021

description: Основной темой является трансформация человеческого сознания под воздействием современных информационно-коммуникационных технологий и появление неомифического архетипа сознания, формирующие гиперреальность. Были описаны основные тенденции происходящей социальной революции и описана структура гиперреальности. Сформулирован признак трансвиртуального искусства и
метод конституирования культурных артефактов неомифа.
The broad band spectral properties of binary X-ray pulsars
Creators: name: Fiume, D. Dal
name: Orlandini, M.
name: Del Sordo, S.
name: Frontera, F.
name: Oosterbroek, T.
name: Palazzi, E.
name: Parmar, A. N.
name: Piraino, S.
name: Santangelo, A.
name: Segreto, A.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: The X-ray telescopes on board BeppoSAX are an optimal set of instruments to observe bright galactic binary pulsars. These sources emit very hard and quite complex X-ray spectra that can be accurately measured with BeppoSAX between 0.1 and 200 keV. A prototype of this complexity, the source Her X-1, shows at least seven different components in its spectrum. A broad band measure is therefore of paramount importance to have a thorough insight into the physics of the emitting region. Moreover the detection of cyclotron features, when present, allows a direct and highly significant measure of the magnetic field intensity in the emission region. In this paper we briefly report the results obtained with BeppoSAX on this class of sources, with emphasis on the detection and on the measured properties of the cyclotron lines.
description: 10 Latex pages, 4 figures, uses psfig.sty. Accepted for publication in Advances in Space Research, in Proceedings of 32nd Scientific Assembly of COSPAR - Symposium E1.1: "Broad-Band X-ray Spectroscopy of Cosmic Sources"
Winds as the origin of radio emission in $z=2.5$ radio-quiet extremely red quasars
Creators: name: Hwang, Hsiang-Chih
name: Zakamska, Nadia L.
name: Alexandroff, Rachael M.
name: Hamann, Fred
name: Greene, Jenny E.
name: Perrotta, Serena
name: Richards, Gordon T.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: Most active galactic nuclei (AGNs) are radio-quiet, and the origin of their radio emission is not well-understood. One hypothesis is that this radio emission is a by-product of quasar-driven winds. In this paper, we present the radio properties of 108 extremely red quasars (ERQs) at $z=2-4$. ERQs are among the most luminous quasars ($L_{bol} \sim 10^{47-48}$ erg/s) in the Universe, with signatures of extreme ($\gg 1000$ km/s) outflows in their [OIII]$λ$5007 Å emission, making them the best subjects to seek the connection between radio and outflow activity. All ERQs but one are unresolved in the radio on $\sim 10$ kpc scales, and the median radio luminosity of ERQs is $νL_ν[{\rm 6\,GHz}] = 10^{41.0}$ erg/s, in the radio-quiet regime, but one to two orders of magnitude higher than that of other quasar samples. The radio spectra are steep, with a mean spectral index $\langle α\rangle = -1.0$. In addition, ERQs neatly follow the extrapolation of the low-redshift correlation between radio luminosity and the velocity dispersion of [OIII]-emitting ionized gas. Uncollimated winds, with a power of one per cent of the bolometric luminosity, can account for all these observations. Such winds would interact with and shock the gas around the quasar and in the host galaxy, resulting in acceleration of relativistic particles and the consequent synchrotron emission observed in the radio. Our observations support the picture in which ERQs are signposts of extremely powerful episodes of quasar feedback, and quasar-driven winds as a contributor of the radio emission in the intermediate regime of radio luminosity $νL_ν= 10^{39}-10^{42}$ erg/s.
description: accepted by MNRAS
A case study of good practices at diversity and inclusion management
Creators: name: Ripado, Luis Miguel
name: Jorge, Fátima
name: Dionísio, Andreia
Publisher: name: Proceedings - Research and Intervention in Human Resources
Year: 2019

description: The scope of this research concerns the theme of diversity and inclusion and values and behaviors, and it purpose is to define and validate a theoretical model which allows the relationship of Diversity and Inclusion (D&I) with Values and Behaviors (V&B) and its repercussion in Organizational Performance. This case study is supported by variables from different european affiliates of Novartis Pharmaceuticals.
description: Proceedings - Research and Intervention in Human Resources, n. 9 (2019): IX Conferência Internacional de Investigação e Intervenção em RH
Resummations in Hot Scalar Electrodynamics
Creators: name: Kraemmer, U.
name: Rebhan, A. K.
name: Schulz, H.
Publisher: name: arXiv
Year: 1994
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: The gauge-boson sector of perturbative scalar electrodynamics is investigated in detail as a testing ground for resummation methods in hot gauge theories. It also serves as a simple non-trivial reference system for the non-Abelian gluon plasma. The complete next-to-leading order contributions to the polarization tensor are obtained within the resummation scheme of Braaten and Pisarski. The simpler scheme proposed recently by Arnold and Espinosa is shown to apply to static quantities only, whereas Braaten-Pisarski resummation turns out to need modification for collective phenomena close to the light-cone. Finally, a recently proposed resummation of quasi-particle damping contributions is assessed critically.
description: 53 p. LaTeX, 7 figs. (2 in LaTeX, 5 EPS appended as uu-encoded file), ITP-UH-01/94 & DESY 94-034
Decomposition and Completion of Sum-of-Squares Matrices
Creators: name: Zheng, Yang
name: Fantuzzi, Giovanni
name: Papachristodoulou, Antonis
Publisher: name: arXiv
Year: 2018
Subjects: subject: Optimization and Control (math.OC)
subject: Systems and Control (eess.SY)
subject: FOS: Mathematics
subject: FOS: Electrical engineering, electronic engineering, information engineering

description: This paper introduces a notion of decomposition and completion of sum-of-squares (SOS) matrices. We show that a subset of sparse SOS matrices with chordal sparsity patterns can be equivalently decomposed into a sum of multiple SOS matrices that are nonzero only on a principal submatrix. Also, the completion of an SOS matrix is equivalent to a set of SOS conditions on its principal submatrices and a consistency condition on the Gram representation of the principal submatrices. These results are partial extensions of chordal decomposition and completion of scalar matrices to matrices with polynomial entries. We apply the SOS decomposition result to exploit sparsity in matrix-valued SOS programs. Numerical results demonstrate the high potential of this approach for solving large-scale sparse matrix-valued SOS programs.
description: 6 pages
MOESM4 of Dehiscence method: a seed-saving, quick and simple viability assessment in rice
Creators: name: Xu, Ling-Xiang
name: Lin, Yi-Xin
name: Wang, Li-Hong
name: Zhou, Yuan-Chang
Publisher: name: figshare
Year: 2018
Subjects: subject: Biochemistry
subject: Cell Biology
subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: 80699 Information Systems not elsewhere classified
subject: FOS: Computer and information sciences
subject: Developmental Biology
subject: Science Policy

description: Additional file 4: Figure S2. Rice protrusion promoting machine. ( https://item.taobao.com/item.htm?spm=a230r.1.14.81.271c5f56M4eN7D&id=549178602323&ns=1&abbucket=10#detail , 20180606).
title: Lettre de Jacques Leibowitch à Madame Yvette Sultan (Hôpital Cochin, Centre des hémophiles)
Creators: name: Leibowitch, Jacques
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2020

description: Source: http://www.calames.abes.fr/pub/ms/Calames-20193111133930946
description: created: start=1991-06-05;end=1995-05-02
Stay or Leave? A relação entre as práticas de gestão de recursos humanos de alta performance e a intenção de turnover
Creators: name: Murcho, Ana Raquel
name: Duarte, Ana Patrícia
name: Neves, José
Publisher: name: Conferência - Investigação e Intervenção em Recursos Humanos
Year: 2019

description: O conhecimento tem vindo a ganhar particular relevância no mercado de trabalho, fenómeno que se deve a várias mudanças ao nível da sociedade, como a globalização ou os avanços tecnológicos (Holtom, Mitchell, Lee, & Eberly, 2008). Também devido às alterações nas organizações e nas suas formas de trabalhar, as empresas baseadas em conhecimento intensivo têm despertado bastante interesse desde as últimas décadas, uma vez que são notórios o crescimento e o aumento do número das mesmas (Alvesson, 1993). Adquirir vantagem competitiva e potenciar os resultados organizacionais são alguns dos principais objetivos das empresas atualmente. A gestão estratégica do capital humano, numa altura em que o conhecimento especializado é cada vez mais relevante, é uma necessidade das organizações e, por isso, esta abordagem tem vindo a ganhar particular importância no âmbito académico. Aliada a esta mudança de paradigma está a realidade das empresas de consultoria, cuja rotatividade voluntária dos recursos humanos é elevada. Tendo em conta estas tendências, o objetivo inicial deste trabalho é compreender a relação entre as práticas de gestão de recursos Humanos (GRH) de alta performance e a intenção de turnover e, posteriormente, averiguar se o compromisso organizacional afetivo e a satisfação no trabalho explicam esta relação. Por fim, pretende-se também analisar a influência do compromisso de carreira nestas relações.
description: Conferência - Investigação e Intervenção em Recursos Humanos, n. 9 (2019): IX Conferência Internacional de Investigação e Intervenção em RH
A Detection of the Environmental Dependence of the Sizes and Stellar Haloes of Massive Central Galaxies
Creators: name: Huang, Song
name: Leauthaud, Alexie
name: Greene, Jenny
name: Bundy, Kevin
name: Lin, Yen-Ting
name: Tanaka, Masayuki
name: Mandelbaum, Rachel
name: Miyazaki, Satoshi
name: Komiyama, Yutaka
Publisher: name: arXiv
Year: 2018
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We use ~100 square deg of deep (>28.5 mag arcsec$^{-2}$ in i-band), high-quality (median 0.6 arcsec seeing) imaging data from the Hyper Suprime-Cam (HSC) survey to reveal the halo mass dependence of the surface mass density profiles and outer stellar envelopes of massive galaxies. The i-band images from the HSC survey reach ~4 magnitudes deeper than Sloan Digital Sky Survey and enable us to directly trace stellar mass distributions to 100 kpc without requiring stacking. We conclusively show that, at fixed stellar mass, the stellar profiles of massive galaxies depend on the masses of their dark matter haloes. On average, massive central galaxies with $\log M_{\star, 100\ \mathrm{kpc}}>11.6$ in more massive haloes at 0.3 < z < 0.5 have shallower inner stellar mass density profiles (within ~10-20 kpc) and more prominent outer envelopes. These differences translate into a halo mass dependence of the mass-size relation. Central galaxies in haloes with $\log M_{\rm{Halo}}>14.0$ are ~20% larger in $R_{\mathrm{50}}$ at fixed stellar mass. Such dependence is also reflected in the relationship between the stellar mass within 10 and 100 kpc. Comparing to the mass--size relation, the $\log M_{\star, 100\ \rm{kpc}}$-$\log M_{\star, 10\ \rm{kpc}}$ relation avoids the ambiguity in the definition of size, and can be straightforwardly compared with simulations. Our results demonstrate that, with deep images from HSC, we can quantify the connection between halo mass and the outer stellar halo, which may provide new constraints on the formation and assembly of massive central galaxies.
description: Accepted for the publication in MNRAS, 19 Pages, 12 Figures, and 1 Table
Lepton Spectra and the B Polarization at LEP
Creators: name: Mele, Barbara
Publisher: name: arXiv
Year: 1994
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: I review the present state of knowledge on lepton energy spectra in the inclusive semileptonic decay of beauty hadrons, as a means to measure b polarization effects on the Z peak. Charged-lepton as well as neutrino spectra are considered.
description: 15 pages + 5 figs (available upon request), LaTex, preprint Rome University "La Sapienza" n.1009, March 1994
Additional file 1 of Binning long reads in metagenomics datasets using composition and coverage information
Creators: name: Wickramarachchi, Anuradha
name: Lin, Yu
Publisher: name: figshare
Year: 2022
Subjects: subject: Biochemistry
subject: Genetics
subject: FOS: Biological sciences
subject: Evolutionary Biology
subject: Ecology
subject: Sociology
subject: FOS: Sociology
subject: Biological Sciences not elsewhere classified
subject: Information Systems not elsewhere classified

description: Additional file 1. Information about datasets. LR_Binner_BMC___Supp_ESM.pdf. Evaluation of LRBinner for varying composition k-mer sizes. Extended assembly quality evaluation.
title: In Vitro Enzymatic Assay of RNA Methylation
Creators: name: Pamela Jean Eubanks
Publisher: name: Old Dominion University
publisherIdentifier: https://ror.org/04zjtrb98
publisherIdentifierScheme: ROR
Year: 1981

description: An assay procedure for in vitro enzymatic methylation of mannnalian ribosomal RNA has been developed in this study. The assay procedure, utilized for the comparison of normal and neoplastic methylase activities (using mouse liver and Ehrlich ascites cells as sources of enzyme), is a modification of previously published methods (52,53). A 100,000 x g supernatant (SlOO) enzyme preparation was incubated with 28S-5.8S rRNA and tritium-labeled S-adenosyl-L-methionine. The RNA was extracted, applied to DEAE cellulose paper, washed, and the radioactivity counted. The neoplastic cell methylase preparation was more active in methylating both exogenous neoplastic and normal 28S-5.8S rRNA than the normal enzyme preparation. However, based on DEAESephadex chromatograms of ribonuclease T2 digests of tritium-labeled RNA from neoplastic cell methylase assays, the in vitro methylation is almost exclusively restricted to the purine and pyrimidine bases. Although this in vitro base methylation may not represent the cellular situation, which is almost exclusively 2'-O-ribose methylation, the higher neoplastic cell methylase activity correlates well with previously published studies and indicates that this assay procedure is a useful tool for further study of normal and neoplastic cell methylase activities.
The uncertainties in the synthetic indices for stellar populations
Creators: name: Maraston, Claudia
name: Greggio, Laura
name: Thomas, Daniel
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: The study of line strengths in the spectra of early-type galaxies has proven to be a powerful tool for investigating the age and the metallicity of these systems. When computing models for spectrophotometric narrow-band indices, index calibrations as functions of the relevant stellar parameters (e.g. temperature, gravity and metal content) are used. Thus synthetic indices depend upon these calibrations (called fitting functions), as well as on the stellar evolution ingredients adopted. All these inputs suffer from uncertainties, which impact on the derived value for the indices. In this paper we address this problem quantitatively. We compute synthetic Mg2, Fe5270, Fe5335 and Hbeta indices for Simple Stellar Populations (SSP) of various ages and metallicities, under different prescriptions for the fitting functions. This allows us to estimate the impact of the uncertainties in the fitting functions. By comparing our models to those of other authors computed with the same fitting functions, we estimate the uncertainty associated to the use of different stellar evolution prescriptions. It is found that the modelling of the Horizontal Branch impacts particularly on and Hbeta. In the range of parameters explored, the uncertainties introduced by the use of different fitting functions can be appreciably larger than the error affecting the observational data. This typically occurs at high Z for the metallic line strengths, at low Z for the Hbeta index.
description: 8 pages, 3 figures, to appear in "The Evolution of galaxies on Cosmological timescales", A&SS, in press
Additional file 2 of Gamma-secretase inhibitor does not induce cytotoxicity in adult T-cell leukemia cell lines despite NOTCH1 expression
Creators: name: Suzuki, Shinsuke
name: Hourai, Sawako
name: Uozumi, Kimiharu
name: Uchida, Yuichirou
name: Yoshimitsu, Makoto
name: Miho, Hachiman
name: Arima, Naomichi
name: Ueno, Shin-ichi
name: Ishitsuka, Kenji
Publisher: name: figshare
Year: 2022
Subjects: subject: Medicine
subject: Cell Biology
subject: Molecular Biology
subject: Pharmacology
subject: Cancer
subject: Hematology
subject: Infectious Diseases
subject: FOS: Health sciences
subject: Virology

description: Additional file 2.