cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Ultraviolet Imaging Polarimetry of the Large Magellanic Cloud. II. Models
Creators: name: Cole, Andrew A.
name: Wood, Kenneth
name: Nordsieck, Kenneth H.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Motivated by new sounding-rocket wide-field polarimetric images of the Large Magellanic Cloud, we have used a three-dimensional Monte Carlo radiation transfer code to investigate the escape of near-ultraviolet photons from young stellar associations embedded within a disk of dusty material (i.e. a galaxy). As photons propagate through the disk, they may be scattered or absorbed by dust. Scattered photons are polarized and tracked until they escape to be observed; absorbed photons heat the dust, which radiates isotropically in the far-infrared, where the galaxy is optically thin. The code produces four output images: near- UV and far-IR flux, and near-UV images in the linear Stokes parameters Q and U. From these images we construct simulated UV polarization maps of the LMC. We use these maps to place constraints on the star + dust geometry of the LMC and the optical properties of its dust grains. By tuning the model input parameters to produce maps that match the observed polarization maps, we derive information about the inclination of the LMC disk to the plane of the sky, and about the scattering phase function g. We compute a grid of models with i = 28 deg., 36 deg., and 45 deg., and g = 0.64, 0.70, 0.77, 0.83, and 0.90. The model which best reproduces the observed polarization maps has i = 36 +2/-5 degrees and g ~0.7. Because of the low signal-to-noise in the data, we cannot place firm constraints on the value of g. The highly inclined models do not match the observed centro-symmetric polarization patterns around bright OB associations, or the distribution of polarization values. Our models approximately reproduce the observed ultraviolet photopolarimetry of the western side of the LMC; however, the output images depend on many input parameters and are nonunique.
description: Accepted to AJ. 20 pages, 7 figures
Innovation Management Plan
Creators: name: Bernabe, Rosemarie
Publisher: name: Zenodo
Year: 2021

description: ROSiE is a project supported by Horizon 2020. Its purpose includes creating innovative, useful tools in collaboration with all relevant parties in order to promote ethical open science (OS) and citizen science. Keeping with this vision, one of the goals of the ROSiE project is to make sure the project is managed effectively. Realizing the innovation management plan for the ROSiE project is Work Package 9 deliverable 9.5. To fulfill this deliverable, we have created a strategic plan on how to foster the novel product created in the ROSiE project.Our perspective is to share our resources to reach the target audience in order to maximize the impact of ROSiE. We want to extend our innovative products beyond academia. ROSiE will produce sustainable digital learning resources i.e. online training tools and the knowledge Hub to benefit stakeholders and potential users.
Evolution of the electric fields induced in high intensity laser-matter interactions
Creators: name: Bisesto, F. G.
name: Anania, M. P.
name: Botton, M.
name: Chiadroni, E.
name: Cianchi, A.
name: Curcio, A.
name: Ferrario, M.
name: Galletti, M.
name: Henis, Z.
name: Pompili, R.
name: Schleifer, E.
name: Zigler, A.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Plasma Physics (physics.plasm-ph)
subject: FOS: Physical sciences

description: Multi MeV protons \cite{snavely2000intense} and heavier ions are emitted by thin foils irradiated by high-intensity lasers, due to the huge accelerating fields, up to several teraelectronvolt per meter, at sub-picosecond timescale \cite{dubois2014target}. The evolution of these huge fields is not well understood till today. Here we report, for the first time, direct and temporally resolved measurements of the electric fields produced by the interaction of a short-pulse high-intensity laser with solid targets. The results, obtained with a sub-$100$ fs temporal diagnostics, show that such fields build-up in few hundreds of femtoseconds and lasts after several picoseconds.
title: Bidonvilles et extension de la ville européenne. Fédala planche V (1945-1948)
title: Bidonvilles et extension de la ville européenne. Fédala planche V (1945-1948)
Creators: name: :Unkn
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2023
Subjects: subject: Habitat
subject: Urbain
subject: Bidonville
subject: Ville nouvelle

description: Cartographie
description: BESM-carto_1950-48-p033_48-04
description: 33
description: 48
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/1/81646
description: Coverage: Maroc
description: Coverage: Mohammadia
description: Coverage: XXe siècle
description: Temporal: XXe siècle
description: Bibliographic citation: « Bidonvilles et extension de la ville européenne. Fédala planche V (1945-1948) », In Bulletin économique et social du Maroc (BESM), n° 48, 1950
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/
Novel CuI-based Metal Organic Frameworks for sensing applications
Creators: name: Khaled, Hassanein
name: Chiara, Cappuccino
name: Lucia, Maini
name: Barbara, Ventura
Publisher: name: Zenodo
Year: 2019

description: Poster presented at the "Symposium on Metal-Organic Frameworks and Porous Organic Materials (UK-MOF-2018)", 9-10 April 2018, Southampton, UK.
A New Approach for Higher Order Difference Equations and Eigenvalue problems via Physical Potentials
Creators: name: Bas, Erdal
name: Ozarslan, Ramazan
Publisher: name: arXiv
Year: 2018
Subjects: subject: Classical Analysis and ODEs (math.CA)
subject: FOS: Mathematics
subject: 39A06, 39A12, 39A70, 35A25

description: In this study, we give the variation of parameters method from a different viewpoint for the Nth order inhomogeneous linear ordinary difference equations with constant coefficient by means of delta exponential function . Advantage of this new approachment is to enable us to investigate the solution of difference equations in the closed form. Also, the method is supported with three difference eigenvalue problems, the second-order Sturm-Liouville problem, which is called also one dimensional Schrödinger equation, having Coulomb potential, hydrogen atom equation, and the fourth-order relaxation difference equations. We find sum representation of solution for the second order discrete Sturm-Liouville problem having Coulomb potential, hydrogen atom equation, and analytical solution of the fourth order discrete relaxation problem by the variation of parameters method via delta exponential and delta trigonometric functions .
description: 13 pages, 8 figures
IN03040 Riṭigala Āṇḍiyā-kanda Cave Inscription 7
Creators: name: Wickremasinghe, Don Martino de Zilva
Publisher: name: Zenodo
Year: 2019
Subjects: IN03040
Epigraphia Zeylanica
Riṭigala
Āṇḍiyā-kanda

description: IN03040 Riṭigala Āṇḍiyā-kanda Cave Inscription 7 - Transcript and Translation Source: Wickremasinghe, Don Martino de Zilva. (1904-12). ‘No. 10. Riṭigala Inscriptions,’ Epigraphia Zeylanica 1, pp. 135-153.
Connecting Majorana phases to the Geometric Parameters of Majorana Unitarity Triangle in a model of Neutrino Mass Matrix
Creators: name: Verma, Surender
name: Bharadwaj, Shankita
Publisher: name: arXiv
Year: 2018
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We have investigated a possible connection between the Majorana phases and geometric parameters of leptonic unitarity triangle(LUT) in two-texture zero neutrino mass matrix. Such analytical relations can, also, be obtained for other theoretical models viz. hybrid textures, neutrino mass matrix with vanishing minors and have profound implications for geometric description of $CP$ violation. As an example, we have considered two-texture zero neutrino mass model to obtain relation between Majorana phases and LUT parameters. In particular, we find that Majorana phases depend on only one of the three interior angles of LUT in each class of two-texture zero neutrino mass matrix. We have, also, constructed LUT for class $A$, $B$ and $C$ neutrino mass matrices. Non-vanishing areas and nontrivial orientations of these Majorana unitarity triangles indicate non-zero $CP$ violation as a generic feature of this class of mass models.
description: 11 pages, 4 figures
New probes of anomalous $WWγ$ couplings at future $e^+e^-$ linacs
Creators: name: Abraham, K. J.
name: Kalinowski, J.
name: Sciepko, P.
Publisher: name: arXiv
Year: 1994
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We investigate the sensitivity of single photon plus missing energy cross-sections at future $e^{+}e^{-}$ linacs to non-standard $WWγ$ couplings. We show that even with conservative estimates of systematic errors there is still considerable sensitivity to anomalous couplings. Analytic expressions for helicity amplitudes are presented.
description: 7 pages in LaTeX style, figures not included, can be obtained from the authors, IFT-94/14, presented at Kazimierz Conference, May 23-27, 1994
Thermographic measurements of spin-current-induced temperature modulation in metallic bilayers
Creators: name: Iguchi, R.
name: Yagmur, A.
name: Lau, Y. -C.
name: Daimon, S.
name: Saitoh, E.
name: Hayashi, M.
name: Uchida, K.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Materials Science (cond-mat.mtrl-sci)
subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: FOS: Physical sciences

description: Spin-to-heat current conversion effects have been investigated in bilayer films consisting of a paramagnetic metal (PM; Pt, W, or Ta) and a ferromagnetic metal (FM; CoFeB or permalloy). When a charge current is applied to the PM/FM bilayer film, a spin current is generated across the PM/FM interface owing to the spin Hall effect in PM. The spin current was found to exhibit cooling and heating features depending on the sign of the spin Hall angle of PM, where the spin-current-induced contribution is estimated by subtracting the contribution of the anomalous Ettingshausen effect in FM monolayer films. We also found that the magnitude of the spin-current-induced temperature modulation in the Pt/CoFeB film is greater than but comparable to that in the Pt/permalloy film, although the spin dependence of the Peltier coefficient for CoFeB is expected to be greater than that for permalloy. We discuss the origin of the observed behaviors with the aid of model calculations; the signals in the PM/FM films may contain the contributions not only from the electron-driven spin-dependent Peltier effect but also from the magnon-driven spin Peltier effect.
description: 21 pages, 6 figures
Additional file 3: of Effects of hyperoxia on vascular tone in animal models: systematic review and meta-analysis
Creators: name: Smit, Bob
name: Smulders, Yvo
name: Eringa, Etto
name: Straaten, Heleen Oudemans-Van
name: Girbes, Armand
name: Wever, Kimberley
name: Hooijmans, Carlijn
name: Man, Angelique Spoelstra-De
Publisher: name: figshare
Year: 2018
Subjects: subject: Medicine
subject: Cell Biology
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: Developmental Biology
subject: Science Policy

description: Funnel plots. Results of the publication bias assessment in the form of funnel plots. (PDF 344 kb)
Monomorium (Syllophopsis) modestum Santschi
Creators: name: Santschi, F.
Publisher: name: Zenodo
Year: 1915
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hymenoptera
Formicidae
Monomorium
Monomorium modestum

description: Monomorium (Syllophopsis) modestum Santschi.
La description de cette espece doit etre modifiee comme suit: Le scape n'atteint pas tout a fait le bord posterieur de la tete. Le dernier article de l'antenne est aussi long que les 7 precedents reunis. Des lobes frontaux contigus, partent les deux faibles carenes de l'epistome qui se reunissent en avant. La face basale de l'epinotum est faiblement concave de droite a gauche, surtout en arriere, base du gastre un peu echancree devant.
description: Published as part of Santschi, F., 1915, Nouvelles fourmis d'Afrique., pp. 244-282 in Annales de la Société Entomologique de France 84 on page 260
Secondary stars in CVs - the observational picture
Creators: name: Beuermann, K.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Recent theoretical and observational progress has substantially improved the definition of the lower main sequence and established a new basis for a comparison of main sequence stars and the secondaries in CVs. The evolutionary sequences of Kolb & Baraffe [1999] imply that the secondaries in many CVs are expanded compared with main sequence stars of the same mass as a consequence of unusually high mass transfer rates and/or pre-CV nuclear evolution. We show that the location of the secondaries of all well-studied CVs in the spectral type period diagram implies that they are consistent with having near-solar metallicities. We show, furthermore, that the surface brightness of K/M stars depends on gravity and metallicity and present new Barnes-Evans relations valid for dwarfs of near-solar metallicity and the secondaries in CVs of the galactic disk population. Distances derived by the surface brightness method agree with recent measurements of the trigonometric parallaxes of a few selected systems.
description: 7 pages, 4 Figures, accepted for publication in New Astronomy Reviews
title: ADCO, Neuvième cartulaire de Saint-Étienne de Dijon (1661 - 1684), Cart. 32 (G 136), 745 folios, f. 1227
Creators: name: de la Côte d'Or, Archives départementales
name: Petot, Frédéric
name: Archives Départementales De La Côte-D'Or
name: Petot, Frédérique
name: Projet CBMA
name: CG21/F.PETOT/2012
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2020
Subjects: subject: cartulaire
subject: Corpus Burgundiae Medii Aevi
subject: Chartes de la Bourgogne du Moyen Âge
subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris

description: Neuvième cartulaire de Saint-Étienne de Dijon (1661 - 1684), Archives départementales de la Côte-d'Or, Cart. 32 (G 136), 745 folios, f. 1227, 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. 1227, 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
Connecting Planetary Composition with Formation
Creators: name: Pudritz, Ralph E.
name: Cridland, Alex J.
name: Alessi, Matthew
Publisher: name: arXiv
Year: 2018
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: FOS: Physical sciences

description: The rapid advances in observations of the different populations of exoplanets, the characterization of their host stars and the links to the properties of their planetary systems, the detailed studies of protoplanetary disks, and the experimental study of the interiors and composition of the massive planets in our solar system provide a firm basis for the next big question in planet formation theory. How do the elemental and chemical compositions of planets connect with their formation? The answer to this requires that the various pieces of planet formation theory be linked together in an end-to-end picture that is capable of addressing these large data sets. In this review, we discuss the critical elements of such a picture and how they affect the chemical and elemental make up of forming planets. Important issues here include the initial state of forming and evolving disks, chemical and dust processes within them, the migration of planets and the importance of planet traps, the nature of angular momentum transport processes involving turbulence and/or MHD disk winds, planet formation theory, and advanced treatments of disk astrochemistry. All of these issues affect, and are affected by the chemistry of disks which is driven by X-ray ionization of the host stars. We discuss how these processes lead to a coherent end-to-end model and how this may address the basic question.
description: Invited review, accepted for publication in the 'Handbook of Exoplanets', eds. H.J. Deeg and J.A. Belmonte, Springer (2018). 46 pages, 10 figures
The Extraordinary `Superthin' Spiral Galaxy UGC7321. I. Disk Color Gradients and Global Properties from Multiwavelength Observations
Creators: name: Matthews, L. D.
name: Gallagher, J. S.
name: van Driel, W.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present B- and R-band imaging and photometry, H-alpha narrow-band imaging, NIR H-band imaging, and HI 21-cm spectroscopy of the nearby Sd spiral galaxy UGC7321. UGC7321 exhibits a remarkably thin stellar disk with no bulge component. The galaxy has a very diffuse, low surface brightness disk, which appears to suffer little internal extinction in spite of its edge-on geometry. The UGC7321 disk shows significant B-R color gradients in both the radial and vertical directions. These color gradients cannot be explained solely by dust and are indicative of changes in the mix of stellar ages and/or metallicity as a function of both radius and height above the galaxy plane. The outer regions of the UGC7321 disk are too blue to be explained by low metallicity alone (B-R<0.6), and must be relatively young. However, the galaxy also contains stellar populations with B-R>1.1, indicating it is not a young or recently-formed galaxy. The disk of UGC7321 is not a simple exponential, but exhibits a light excess at small radii, as well as distinct surface brightness zones. Together the properties of UGC7321 imply that it is an under-evolved galaxy in both a dynamical and in a star-formation sense. (Abridged)
description: Accepted to the Astronomical Journal; 28 pages, 1 table and 21 figures (GIF and postscript)
MOESM3 of The jasmonate receptor COI1 is required for AtPep1-induced immune responses in Arabidopsis thaliana
Creators: name: Danalyn Holmes
name: Grubb, Lauren
name: Monaghan, Jacqueline
Publisher: name: figshare
Year: 2018
Subjects: subject: Biochemistry
subject: Cell Biology
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Physiology
subject: Ecology
subject: Immunology
subject: FOS: Clinical medicine
subject: 69999 Biological Sciences not elsewhere classified
subject: Plant Biology

description: Additional file 3: AtPep1-induced PEPR1 expression in coi1-16 mutants. Twelve 14-day-old Col gl1 and coi1-16 seedlings were treated with water (-) or 1 µM AtPep1 (+) for 120 minutes prior to RNA extraction. Quantitative real-time PCR was used to assess expression level of PEPR1. Values are means + standard deviations (n=3 technical replicates from the same cDNA), normalized against the relative average expression of UBOX from the same sample. Three independent biological replicates were performed with similar results. Statistically significant groups (p < 0.05) are indicated with lower-case letters based on a one-way ANOVA followed by Tukey’s post-test.
Additional file 1 of Inhibition of KIF20A by transcription factor IRF6 affects the progression of renal clear cell carcinoma
Creators: name: Ma, Xinwei
name: Wang, Xiaoqi
name: Dong, Qian
name: Pang, Hongquan
name: Xu, Jianming
name: Shen, Junkang
name: Zhu, Jianbing
Publisher: name: figshare
Year: 2021
Subjects: subject: Biochemistry
subject: Cell Biology
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Pharmacology
subject: Chemical Sciences not elsewhere classified
subject: Biological Sciences not elsewhere classified
subject: Developmental Biology
subject: Marine Biology
subject: Cancer

description: Additional file 1. Role of KIF20A in ccRCC.
Monomorium modestum var. boerorum Santschi, 1915, n. var.
Creators: name: Santschi, F.
Publisher: name: Zenodo
Year: 1915
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hymenoptera
Formicidae
Monomorium
Monomorium modestum
Var. boerorum

description: var. boerorum, n. var.
[[worker]]. Long. 1,9 - 2 mm. D'un jaune plus ocrace que le type de l'espece et un peu moins luisant en arriere. Pilosite plus faible. Tete un peu plus large, les cotes plus distinctement convexes et le bord posterieur legerement concave. Les lobes frontaux plus arrondis. Pronotum un peu plus convexe. Epinotum et pedicule un peu plus allonges. Du resto semblable au type.
Transvaal: Pretoria.
description: Published as part of Santschi, F., 1915, Nouvelles fourmis d'Afrique., pp. 244-282 in Annales de la Société Entomologique de France 84 on page 260
Angular Correlations and Light Gluinos in Multi-jet Photoproduction at HERA
Creators: name: Muñoz-Tapia, R.
name: Stirling, W. J.
Publisher: name: arXiv
Year: 1994
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: A study of $3+1$ jet event photoproduction at HERA is presented. We define an angular variable which is sensitive to the topology of the final state jets and is therefore able to discriminate between the different contributing subprocesses, and between QCD and an abelian gluon model. We also investigate the contribution from the direct production of light gluinos to the $3+1$ cross section.
description: 13 pag + 8 figures, Durham preprint DTP/94/50, (LATEX)
Pulsar Constraints on Neutron Star Structure and Equation of State
Creators: name: Link, B.
name: Epstein, R. I.
name: Lattimer, J. M.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: With the aim of constraining the structural properties of neutron stars and the equation of state of dense matter, we study sudden spin-ups, glitches, occurring in the Vela pulsar and in six other pulsars. We present evidence that glitches represent a self-regulating instability for which the star prepares over a waiting time. The angular momentum requirements of glitches in Vela indicate that at least 1.4% of the star's moment of inertia drives these events. If glitches originate in the liquid of the inner crust, Vela's `radiation radius' must exceed ~12 km for a mass of 1.4 solar masses. Observational tests of whether other neutron stars obey this constraint will be possible in the near future.
description: 5 pages, including figures. To appear in Physical Review Letters
Sub 20 meV Schottky barriers in metal/MoTe2 junctions
Creators: name: Townsend, Nicola J.
name: Amit, Iddo
name: Craciun, Monica F.
name: Russo, Saverio
Publisher: name: arXiv
Year: 2018
Subjects: subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: FOS: Physical sciences

description: The newly emerging class of atomically-thin materials has shown a high potential for the realisation of novel electronic and optoelectronic components. Amongst this family, semiconducting transition metal dichalcogenides (TMDCs) are of particular interest. While their band gaps are compatible with those of conventional solid state devices, they present a wide range of exciting new properties that is bound to become a crucial ingredient in the future of electronics. To utilise these properties for the prospect of electronics in general, and long-wavelength-based photodetectors in particular, the Schottky barriers formed upon contact with a metal and the contact resistance that arises at these interfaces have to be measured and controlled. We present experimental evidence for the formation of Schottky barriers as low as 10 meV between MoTe2 and metal electrodes. By varying the electrode work functions, we demonstrate that Fermi level pinning due to metal induced gap states at the interfaces occurs at 0.14 eV above the valence band maximum. In this configuration, thermionic emission is observed for the first time at temperatures between 40 K and 75 K. Finally, we discuss the ability to tune the barrier height using a gate electrode.
description: 26 pages, 13 figures, 2D Materials (2018)
Updating the Unitarity Triangle: Top Quark Mass Versus Nonperturbative Uncertainties
Creators: name: Pich, A.
name: Prades, J.
Publisher: name: arXiv
Year: 1994
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We summarize the present knowledge on the non-perturbative hadronic inputs needed in the analysis of $B^0$-$\bar B^0$ mixing and the CP-violating parameter $\varepsilon$ of the $K^0$-$\bar K^0$ system. Using this information, together with the recently determined value of the top-quark mass, we update the phenomenological constraints on the unitarity triangle.
description: 21 pages, Plain LateX, 7 figures included, preprint FTUV/94-37, IFIC/94-32, NBI-94-32
title: ADCO, Grènetier de Cîteaux : comptes (1497-1504) (11 H 1172), f. 00743
Creators: name: de la Côte-d'Or, Archives départementales
name: Archives Départementales De La Côte-D'Or
name: Petot, Frédérique
name: Projet CBMA
name: CBMA/CG21/F.PETOT/2019
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2020
Subjects: subject: Corpus Burgundiae Medii Aevi
subject: Chartes de la Bourgogne du Moyen Âge
subject: comptes
subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris

description: Grènetier de Cîteaux : comptes (1497-1504), Archives départementales de la Côte-d'Or, (11 H 1172). Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Grènetier de Cîteaux : comptes (1497-1504), Archives départementales de la Côte-d'Or, (11 H 1172), f. 00743, 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
The Role of Screening Corrections in High Energy Photoproduction
Creators: name: Gotsman, E.
name: Levin, E. M.
name: Maor, U.
Publisher: name: arXiv
Year: 1994
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: The role of screening corrections, calculated using the eikonal model, is discussed in the context of soft photoproduction. We present a comprehensive calculation considering the total,elastic and diffractive cross sections jointly. We examine the differences between our results and those obtained from the supercritical Pomeron-Reggeon model with no unitarity corrections.
description: 12 pages (Replacement due to PostScript file problem in previous posting)
Additional file 2: of Effects of hyperoxia on vascular tone in animal models: systematic review and meta-analysis
Creators: name: Smit, Bob
name: Smulders, Yvo
name: Eringa, Etto
name: Straaten, Heleen Oudemans-Van
name: Girbes, Armand
name: Wever, Kimberley
name: Hooijmans, Carlijn
name: Man, Angelique Spoelstra-De
Publisher: name: figshare
Year: 2018
Subjects: subject: Medicine
subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: Developmental Biology
subject: Science Policy

description: Quality checklist. Modified quality checklist used to assess the quality of the included studies. (PDF 14 kb)
MOESM2 of The jasmonate receptor COI1 is required for AtPep1-induced immune responses in Arabidopsis thaliana
Creators: name: Danalyn Holmes
name: Grubb, Lauren
name: Monaghan, Jacqueline
Publisher: name: figshare
Year: 2018
Subjects: subject: Cell Biology
subject: Genetics
subject: FOS: Biological sciences
subject: Ecology
subject: Immunology
subject: FOS: Clinical medicine
subject: 69999 Biological Sciences not elsewhere classified
subject: Plant Biology

description: Additional file 2: Fresh weight of seedlings grown in MS media. Fresh weight of seedlings 10 days after continual growth in sterile MS liquid media. Values are means + standard deviation (n=6 plants). Three biological replicates were performed with similar results. Statistically significant groups (p < 0.05) are indicated with lower-case letters based on a one-way ANOVA followed by Tukeyâ s post-test.
Circinus X-1: survivor of a highly asymmetric supernova
Creators: name: Tauris, T. M.
name: Fender, R. P.
name: Heuvel, E. P. J. van den
name: Johnston, H. M.
name: Wu, K.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We have analyzed the kinematical parameters of Cir X-1 to constrain the nature of its companion star, the eccentricity of the binary and the pre-supernova parameter space. We argue that the companion is most likely to be a low-mass (< 2.0 M_sun) unevolved star and that the eccentricity of the orbit is 0.94 +/- 0.04. We have evaluated the dynamical effects of the supernova explosion and we find it must have been asymmetric. On average, we find that a kick of 740 km/s is needed to account for the recently measured radial velocity of +430 km/s (Johnston, Fender & Wu) for this extreme system. The corresponding minimum kick velocity is 500 km/s. This is the largest kick needed to explain the motion of any observed binary system. If Cir X-1 is associated with the supernova remnant G321.9-0.3 then we find a limiting minimum age of this remnant of 60000 yr. Furthermore, we predict that the companion star has lost 10% of its mass as a result of stripping and ablation from the impact of the supernova shell shortly after the explosion.
description: 6 pages, 3 figues, 2 tables, accepted for publication in MNRAS
title: ADCO, Grènetier de Cîteaux : comptes (1497-1504) (11 H 1172), f. 00735
Creators: name: de la Côte-d'Or, Archives départementales
name: Archives Départementales De La Côte-D'Or
name: Petot, Frédérique
name: Projet CBMA
name: CBMA/CG21/F.PETOT/2019
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2020
Subjects: subject: Corpus Burgundiae Medii Aevi
subject: Chartes de la Bourgogne du Moyen Âge
subject: comptes
subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris

description: Grènetier de Cîteaux : comptes (1497-1504), Archives départementales de la Côte-d'Or, (11 H 1172). Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Grènetier de Cîteaux : comptes (1497-1504), Archives départementales de la Côte-d'Or, (11 H 1172), f. 00735, 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
Performance Loss Analysis and Design Space Optimization of Perovskite Solar Cells
Creators: name: Agarwal, Sumanshu
name: Nair, Pradeep R.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Applied Physics (physics.app-ph)
subject: FOS: Physical sciences

description: While the performance enhancement witnessed in the field of perovskite solar cells over the recent years has been impressive, it is now evident that further optimization beyond the existing literature would require detailed analysis of various loss mechanisms. Here we address the same through detailed numerical simulations of optical and electrical characteristics. We quantify the various losses like optical losses (5-6%), recombination losses (3-4%), and resistive losses against the Auger limited practical efficiency limits. Moreover, we illustrate the schemes that result in reduction of these losses and eventual increase in efficiency. In addition, we extend the analyses to identify the optimum thickness of perovskite and the factors affecting the optimum thickness have been discussed in detail.
A model calculation of the value of the electromagnetic coupling constant at $q^2 = m_{Z}^{2}$
Creators: name: Geshkenbein, B. V.
name: Morgunov, V. L.
Publisher: name: arXiv
Year: 1994
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: A QCD model with an infinite number of vector mesons suggested by one of the authors is used to derive the value of the correction $δα_{hadr}$ for $α(m_{Z}^{2})$ due to the strong interactions. The result is $δα_{hadr} = 0.0275(2)$ ; thus $α(m^{2}_{Z}) = (128.96(3))^{-1}$.
description: in LaTeX, 6 pages, 0 figures, ITEP Preprint 49-94
title: ADCO, Neuvième cartulaire de Saint-Étienne de Dijon (1661 - 1684), Cart. 32 (G 136), 745 folios, f. 0403
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: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris
subject: cartulaire

description: Neuvième cartulaire de Saint-Étienne de Dijon (1661 - 1684), Archives départementales de la Côte-d'Or, Cart. 32 (G 136), 745 folios, f. 0403, 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. 0403, 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
Additional file 1 of Infant rhesus macaques as a non-human primate model of Bordetella pertussis infection
Creators: name: Jiang, Wenwen
name: Wei, Chen
name: Mou, Dachao
name: Zuo, Weilun
name: Liang, Jiangli
name: Ma, Xiao
name: Wang, Lichan
name: Gao, Na
name: Gu, Qin
name: Luo, Peng
name: Ma, Yan
name: Li, Jingyan
name: Liu, Shuyuan
name: Shi, Li
name: Sun, Mingbo
Publisher: name: figshare
Year: 2021
Subjects: subject: Medicine
subject: Neuroscience
subject: Ecology
subject: FOS: Biological sciences
subject: Computational Biology

description: Additional file 1: Additional Figure 1. Simplified layout of aerosol apparatus.
Large Top and Bottom Yukawa Couplings in Minimal Supersymmetry
Creators: name: Floratos, E. G.
name: Leontaris, G. K.
Publisher: name: arXiv
Year: 1994
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We present analytic expressions for the top and bottom Yukawa couplings in the context of the minimal supersymmetric standard model when both couplings $h_{t,0},h_{b,0}$ are large at the unification scale. For sufficiently large $h_{t,0},h_{b,0}$, i.e. within $\sim (20-25)\% $ close to their fixed point values, using as input the central value of the bottom mass $m_b(m_b)=4.25GeV$, we find that the top mass lies in the range $m_t \approx (174-178)GeV$, while $tanβ\approx (55-58)$. Implications on the evolution of the scalar masses and the radiative symmetry breaking scenario are discussed. %
description: (LateX, 9p, CERN-TH.7366/94, typos in eq.13 corrected, results unchanged)
Additional file 1: of Effects of hyperoxia on vascular tone in animal models: systematic review and meta-analysis
Creators: name: Smit, Bob
name: Smulders, Yvo
name: Eringa, Etto
name: Straaten, Heleen Oudemans-Van
name: Girbes, Armand
name: Wever, Kimberley
name: Hooijmans, Carlijn
name: Man, Angelique Spoelstra-De
Publisher: name: figshare
Year: 2018
Subjects: subject: Medicine
subject: Sociology
subject: FOS: Sociology
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: Search strategy. The search strategies used to search Pubmed and Embase for eligible studies. (PDF 201 kb)
Giant graviton interactions and M2-branes ending on multiple M5-branes
Creators: name: Hirano, Shinji
name: Sato, Yuki
Publisher: name: arXiv
Year: 2018
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We study splitting and joining interactions of giant gravitons with angular momenta $N^{1/2}\ll J\ll N$ in the type IIB string theory on $AdS_5 \times S^5$ by describing them as instantons in the tiny graviton matrix model introduced by Sheikh-Jabbari. At large $J$ the instanton equation can be mapped to the four-dimensional Laplace equation and the Coulomb potential for $m$ point charges in an $n$-sheeted Riemann space corresponds to the $m$-to-$n$ interaction process of giant gravitons. These instantons provide the holographic dual of correlators of all semi-heavy operators and the instanton amplitudes exactly agree with the pp-wave limit of Schur polynomial correlators in ${\cal N}=4$ SYM computed by Corley, Jevicki and Ramgoolam. By making a slight change of variables the same instanton equation is mathematically transformed into the Basu-Harvey equation which describes the system of M$2$-branes ending on M$5$-branes. As it turns out, the solutions to the sourceless Laplace equation on an $n$-sheeted Riemann space correspond to $n$ M5-branes connected by M2-branes and we find general solutions representing M2-branes ending on multiple M5-branes. Among other solutions, the $n=3$ case describes an M2-branes junction ending on three M5-branes. The effective theory on the moduli space of our solutions might shed light on the low energy effective theory of multiple M5-branes.
description: 39 pages, 8 figures
Additional file 1 of Effervescent cannabidiol solid dispersion-doped dissolving microneedles for boosted melanoma therapy via the “TRPV1-NFATc1-ATF3” pathway and tumor microenvironment engineering
Creators: name: Shi, Jiachen
name: Ma, Qiuling
name: Su, Wenting
name: Liu, Congyan
name: Zhang, Huangqin
name: Liu, Yuping
name: Li, Xiaoqi
name: Jiang, Xi
name: Ge, Chang
name: Kong, Fei
name: Chen, Yan
name: Qu, Ding
Publisher: name: figshare
Year: 2023
Subjects: Biochemistry
Space Science
Medicine
Pharmacology
Biotechnology
Cancer

description: Supplementary Material 1
Keplerian frequencies and innermost stable circular orbits of rapidly rotating strange stars
Creators: name: Stergioulas, N.
name: Kluzniak, W.
name: Bulik, T.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: It has been suggested that the frequency in the co-rotating innermost stable circular orbit (ISCO) about a compact stellar remnant can be determined through X-ray observations of low-mass X-ray binaries, and that its value can be used to constrain the equation of state of ultradense matter. Upon constructing numerical models of rapidly rotating strange (quark) stars in general relativity, we find that for stars rotating at the equatorial mass-shedding limit, the ISCO is indeed above the stellar surface, for a wide range of central energy densities at a height equal to 11% of the circumferential stellar radius, which scales inversely with the square root of the energy density, of self-bound quark matter at zero presure. In contrast to static stars, the ISCO frequencies of rapidly rotating strange stars can be as low as 0.9 kHz for a 1.3 solar mass strange star. Hence, the presence of strange stars in low-mass X-ray binaries cannot be excluded on the basis of the currently observed frequencies of kHz QPOs, such as the cut-off frequency of 1066 Hz in 4U 1820-30.
description: 5 pg., 4 figs
Additional file 1 of A four-hypoxia-genes-based prognostic signature for oral squamous cell carcinoma
Creators: name: Zhao, Chenguang
name: Zhou, Yingrui
name: Ma, Hongwei
name: Wang, Jinhui
name: Guo, Haoliang
name: Liu, Hao
Publisher: name: figshare
Year: 2021
Subjects: subject: Cell Biology
subject: Genetics
subject: FOS: Biological sciences
subject: Immunology
subject: FOS: Clinical medicine
subject: Biological Sciences not elsewhere classified
subject: Mathematical Sciences not elsewhere classified
subject: Cancer
subject: Science Policy

description: Additional file 1: Table S1. 26 hypoxia-related genes. Table S2. Analysis of correlations between risk score and immune checkpoints.
IN03041 Riṭigala Āṇḍiyā-kanda Cave Inscription 8a
Creators: name: Wickremasinghe, Don Martino de Zilva
Publisher: name: Zenodo
Year: 2019
Subjects: IN03041
Epigraphia Zeylanica
Riṭigala
Āṇḍiyā-kanda

description: IN03041 Riṭigala Āṇḍiyā-kanda Cave Inscription 8a - Transcript and Translation Source: Wickremasinghe, Don Martino de Zilva. (1904-12). ‘No. 10. Riṭigala Inscriptions,’ Epigraphia Zeylanica 1, pp. 135-153.
The magnitude of the gluon condensate and the masses of $c$ and $b$ quarks from the families of ${\cal J}$/$Ψ$ and $Υ$ mesons
Creators: name: Geshkenbein, B. V.
name: Morgunov, V. L.
Publisher: name: arXiv
Year: 1994
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: It is shown that the model used in [1] for the description of the experimental function $R_c (s)$ in the form of a sum of $δ$-functions and the plateau contradicts the Wilson operator expansion (O.E.) in the terms due to the gluon condensate. A QCD model with an infinite number of vector mesons [12,13] does satisfy the requirements of the O.E. for masses and electronic widths resonances close to the experimental values. The region of allowable values of the masses of $c$ and $b$-quarks and the gluon condensate compatible with the O.E. is obtained (Figs. 2,3).
description: in LaTeX, 12 pages, 3 figures available upon request, SSCL - preprint - 534, (1993)
Additional file 1 of Stage IIB-IVA cervix carcinoma in elderly patients treated with radiation therapy: a longitudinal cohort study by propensity score matching analysis
Creators: name: Shou, Huafeng
name: Wan, Qiuyan
name: Xu, Hong’en
name: Shi, Lei
name: Song, Tao
Publisher: name: figshare
Year: 2023
Subjects: subject: Space Science
subject: Medicine
subject: Immunology
subject: FOS: Clinical medicine
subject: Biological Sciences not elsewhere classified
subject: Cancer
subject: Science Policy
subject: Hematology

description: Additional file 1: Table S1. Baseline characteristics of patients who received trimodal therapy before and after PSM. Table S2. Univariate and multivariate analyses of OS in stage IIB-IVA patients who received trimodal therapy before and after PSM.
LA Palma Night-Sky Brightness
Creators: name: Benn, Chris R.
name: Ellison, Sara L.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: The brightness of the moonless night sky above La Palma was measured on 427 CCD images taken with the Isaac Newton and Jacobus Kapteyn Telescopes on 63 nights during 1987 - 1996. The median sky brightness at high elevation, high galactic latitude and high ecliptic latitude, at sunspot minimum, is B = 22.7, V = 21.9, R = 21.0, similar to that at other dark sites. The main contributions to sky brightness are airglow and zodiacal light. The sky is brighter at low ecliptic latitude (by 0.4 mag); at solar maximum (by 0.4 mag); and at high airmass (0.25 mag brighter at airmass 1.5). Light pollution (line + continuum) contributes < 0.03 mag in U, approximately 0.02 mag in B, approximately 0.10 mag in V, approximately and 0.10 mag in R at the zenith. This paper is a summary of results which are presented in full elsewhere (Benn & Ellison 1998, La Palma Technical Note 115).
description: Accepted for publication in New Astronomy Reviews
TMOKE as efficient tool for the magneto-optic analysis of ultra-thin magnetic films
Creators: name: Borovkova, O. V.
name: Hashim, H.
name: Kozhaev, M. A.
name: Dagesyan, S. A.
name: Chakravarty, A.
name: Levy, M.
name: Belotelov, V. I.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Instrumentation and Detectors (physics.ins-det)
subject: Optics (physics.optics)
subject: FOS: Physical sciences

description: Ultra-thin magnetic dielectric films are of prime importance due to their applications for nanophotonics and spintronics. Here, we propose an efficient method for the magneto-optical investigation of ultra-thin magnetic films which allows one to access their state of magnetization and magneto-optical properties. It is based on the surface-plasmon-polariton-assisted transverse magneto-optical Kerr effect (TMOKE). In our experiments, sub-100 nm-thick bismuth-substituted lutetium iron-garnet films covered with a plasmonic gold grating have been analyzed. The excitation of surface plasmon-polaritons provides resonance enhancement of TMOKE up to 0.04 and makes it easily detectable in the experiment. For films thicker than 40 nm, the TMOKE marginally depends on the film thickness. A further decrease in the film thickness diminishes TMOKE since for such thicknesses the surface plasmon-polariton field partly penetrates inside the non-magnetic substrate. Nevertheless, the TMOKE remains measurable even for few-nm-thick films, which makes this technique unique for the magneto-optical study of ultra-thin films. Particularly, the proposed method reveals that the off-diagonal components of the magnetic film permittivity tensor grow slightly with the reduction of the film thickness.
description: 5 pages
MOESM1 of The jasmonate receptor COI1 is required for AtPep1-induced immune responses in Arabidopsis thaliana
Creators: name: Danalyn Holmes
name: Grubb, Lauren
name: Monaghan, Jacqueline
Publisher: name: figshare
Year: 2018
Subjects: subject: Biochemistry
subject: Pharmacology
subject: Evolutionary Biology
subject: FOS: Biological sciences
subject: Ecology
subject: Immunology
subject: FOS: Clinical medicine
subject: 69999 Biological Sciences not elsewhere classified
subject: Inorganic Chemistry
subject: FOS: Chemical sciences
subject: Science Policy
subject: Plant Biology

description: Additional file 1: Primers used in this study. A list of primers used for qPCR.
Physics at High Energy Photon Photon Colliders
Creators: name: Chanowitz, Michael S.
Publisher: name: arXiv
Year: 1994
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: I review the physics prospects for high energy photon photon colliders, emphasizing results presented at the LBL Gamma Gamma Collider Workshop. Advantages and difficulties are reported for studies of QCD, the electroweak gauge sector, supersymmetry, and electroweak symmetry breaking.
description: 18 pages, no figures, plain latex (run twice), LBL-35776