cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Multiple Scattering Error Propagation in Particle Track Reconstruction
Creators: name: Pentia, M.
name: Iorgovan, G.
name: Mihul, A.
Publisher: name: arXiv
Year: 1994
Subjects: subject: High Energy Physics - Experiment (hep-ex)
subject: FOS: Physical sciences

description: Particle track reconstruction capabilities of the silicon tracking detector system have been studied. As the multiple Coulomb scattering (MCS) induces unavoidable uncertainties on the coordinate measurement, the corresponding error estimates and the associated correlations have been used to find the best track fit parameters and their errors. Finally it permits to find the proper particle characteristics, as vertex position and resolution, flight direction and the error.
description: 12 pages, 4 Tables,(LaTex) and 4 Figures available upon request, IFA-HE-124-1994 June
Additional file 1: of Population genomics and morphometric assignment of western honey bees (Apis mellifera L.) in the Republic of South Africa
Creators: name: Eimanifar, Amin
name: Brooks, Samantha A.
name: Bustamante, Tomas
name: Ellis, James
Publisher: name: figshare
Year: 2018
Subjects: subject: Microbiology
subject: FOS: Biological sciences
subject: Cell Biology
subject: Genetics
subject: Molecular Biology
subject: 59999 Environmental Sciences not elsewhere classified
subject: FOS: Earth and related environmental sciences
subject: Ecology
subject: 69999 Biological Sciences not elsewhere classified
subject: 19999 Mathematical Sciences not elsewhere classified
subject: FOS: Mathematics
subject: 110309 Infectious Diseases
subject: FOS: Health sciences
subject: Plant Biology

description: Table S1. Bioclimatic variables used in the distribution model analysis for the two honey bee subspecies from the Republic of South Africa. (DOC 127 kb)
Additional file 2 of Developing guideline-based key performance indicators for recurrent miscarriage care: lessons from a multi-stage consensus process with a diverse stakeholder group
Creators: name: Hennessy, Marita
name: Linehan, Laura
name: Dennehy, Rebecca
name: Devane, Declan
name: Rice, Rachel
name: Meaney, Sarah
name: O’Donoghue, Keelin
Publisher: name: figshare
Year: 2022
Subjects: subject: Medicine
subject: Genetics
subject: FOS: Biological sciences
subject: Environmental Sciences not elsewhere classified
subject: Biological Sciences not elsewhere classified
subject: Developmental Biology
subject: Cancer
subject: Science Policy
subject: Infectious Diseases
subject: FOS: Health sciences

description: Additional file 2. Sample item, Delphi survey—Round 1.
A Deep Reinforcement Learning Based Approach for Cost- and Energy-Aware Multi-Flow Mobile Data Offloading
Creators: name: Zhang, Cheng
name: Liu, Zhi
name: Gu, Bo
name: Yamori, Kyoko
name: Tanaka, Yoshiaki
Publisher: name: arXiv
Year: 2018
Subjects: subject: Networking and Internet Architecture (cs.NI)
subject: FOS: Computer and information sciences

description: With the rapid increase in demand for mobile data, mobile network operators are trying to expand wireless network capacity by deploying wireless local area network (LAN) hotspots on to which they can offload their mobile traffic. However, these network-centric methods usually do not fulfill the interests of mobile users (MUs). Taking into consideration many issues such as different applications' deadlines, monetary cost and energy consumption, how the MU decides whether to offload their traffic to a complementary wireless LAN is an important issue. Previous studies assume the MU's mobility pattern is known in advance, which is not always true. In this paper, we study the MU's policy to minimize his monetary cost and energy consumption without known MU mobility pattern. We propose to use a kind of reinforcement learning technique called deep Q-network (DQN) for MU to learn the optimal offloading policy from past experiences. In the proposed DQN based offloading algorithm, MU's mobility pattern is no longer needed. Furthermore, MU's state of remaining data is directly fed into the convolution neural network in DQN without discretization. Therefore, not only does the discretization error present in previous work disappear, but also it makes the proposed algorithm has the ability to generalize the past experiences, which is especially effective when the number of states is large. Extensive simulations are conducted to validate our proposed offloading algorithms.
description: 9 pages, 8 figures. arXiv admin note: substantial text overlap with arXiv:1801.10152
Carnet nº 1 : description des travaux accomplis sur le tour de France (p. 7)
Creators: name: Péraire, Lucien
name: CNRS
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2023

description: created: 15-6-1925
Cancer dorsipes Linnaeus, 1758, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1758
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Malacostraca
Decapoda
Cancridae
Cancer
Cancer dorsipes

description: Cancer dorsipes [spec. nov.]
C. brachyurus, thorace rugoso ovali: antice serrato ciliato, pedibus posticis dorsalibus.
Habitat in India.
description: Published as part of Linnaeus, Carolus, 1758, Systema Naturae per regna tria naturae: secundum classes, ordines, genera, species, cum characteribus, differentiis, synonymis, locis, Stockholm :Laurentius Salvius on page 630, DOI: 10.5962/bhl.title.542, http://zenodo.org/record/3922206
Determination of the Strange Quark Content of the Nucleon from a Next-to-Leading-Order QCD Analysis of Neutrino Charm Production
Creators: name: Bazarko, A. O.
Publisher: name: arXiv
Year: 1994
Subjects: subject: High Energy Physics - Experiment (hep-ex)
subject: FOS: Physical sciences

description: We present the first next-to-leading-order QCD analysis of neutrino charm production, using a sample of 6090 $ν_μ$- and $\barν_μ$-induced opposite-sign dimuon events observed in the CCFR detector at the Fermilab Tevatron. We find that the nucleon strange quark content is suppressed with respect to the non-strange sea quarks by a factor $κ= 0.477 \: ^{+\:0.063}_{-\:0.053}$, where the error includes statistical, systematic and QCD scale uncertainties. In contrast to previous leading order analyses, we find that the strange sea $x$-dependence is similar to that of the non-strange sea, and that the measured charm quark mass, $m_c = 1.70 \pm 0.19 \:{\rm GeV/c}^2$, is larger and consistent with that determined in other processes. Further analysis finds that the difference in $x$-distributions between $xs(x)$ and $x\bar s(x)$ is small. A measurement of the Cabibbo-Kobayashi-Maskawa matrix element $|V_{cd}|=0.232 ^{+\:0.018}_{-\:0.020}$ is also presented. uufile containing compressed postscript files of five Figures is appended at the end of the LaTeX source.
description: Nevis R#1502
Additional file 7 of Developing guideline-based key performance indicators for recurrent miscarriage care: lessons from a multi-stage consensus process with a diverse stakeholder group
Creators: name: Hennessy, Marita
name: Linehan, Laura
name: Dennehy, Rebecca
name: Devane, Declan
name: Rice, Rachel
name: Meaney, Sarah
name: O’Donoghue, Keelin
Publisher: name: figshare
Year: 2022
Subjects: subject: Medicine
subject: Genetics
subject: FOS: Biological sciences
subject: Environmental Sciences not elsewhere classified
subject: Biological Sciences not elsewhere classified
subject: Developmental Biology
subject: Cancer
subject: Science Policy
subject: Infectious Diseases
subject: FOS: Health sciences

description: Additional file 7. List of KPIs not retained.
Galaxy Clusters: Oblate or Prolate?
Creators: name: Cooray, Asantha R.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: It is now well known that a combined analysis of the Sunyaev-Zel'dovich (SZ) effect and the X-ray emission observations can be used to determine the angular diameter distance to galaxy clusters, from which the Hubble constant is derived. Given that the SZ/X-ray Hubble constant is determined through a geometrical description of clusters, the accuracy to which such distance measurements can be made depends on how well one can describe intrinsic cluster shapes. Using the observed X-ray isophotal axial ratio distribution for a sample of galaxy clusters, we discuss intrinsic cluster shapes and, in particular, if clusters can be described by axisymmetric models, such as oblate and prolate ellipsoids. These models are currently favored when determining the SZ/X-ray Hubble constant. We show that the current observational data on the asphericity of galaxy clusters suggest that clusters are more consistent with a prolate rather than an oblate distribution. We address the possibility that clusters are intrinsically triaxial by viewing triaxial ellipsoids at random angles with the intrinsic axial ratios following an isotropic Gaussian distribution. We discuss implications of our results on current attempts at measuring the Hubble constant using galaxy clusters and suggest that an unbiased estimate of the Hubble constant, not fundamentally limited by projection effects, would eventually be possible with the SZ/X-ray method.
description: 6 pages, 6 figures. MNRAS (in press)
Additional file 5: of Enhancement of Glen Moy x Latham raspberry linkage map using GbS to further understand control of developmental processes leading to fruit ripening
Creators: name: Hackett, Christine
name: Milne, Linda
name: Smith, Kay
name: Hedley, Pete
name: Morris, Jenny
name: Simpson, Craig
name: Preedy, Katharine
name: Graham, Julie
Publisher: name: figshare
Year: 2018
Subjects: subject: Cell Biology
subject: Genetics
subject: FOS: Biological sciences
subject: Neuroscience
subject: 59999 Environmental Sciences not elsewhere classified
subject: FOS: Earth and related environmental sciences
subject: Immunology
subject: FOS: Clinical medicine
subject: 69999 Biological Sciences not elsewhere classified
subject: Developmental Biology
subject: 110309 Infectious Diseases
subject: FOS: Health sciences
subject: Computational Biology

description: Table S2. Two non-related regions with associated scaffolds within 2Â cM and any potential developmentally/ripening related genes. This table examines regions not identified in ripening to ensure the ripening related genes are not chance associations. (DOCX 17Â kb)
Generalized one-band model based on Zhang-Rice singlets for Tetragonal CuO
Creators: name: Hamad, I. J.
name: Manuel, L. O.
name: Aligia, A. A.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Superconductivity (cond-mat.supr-con)
subject: FOS: Physical sciences

description: Tetragonal CuO (T-CuO) has attracted attention because of its structure similar to that of the cuprates. It has been recently proposed as a compound whose study can give an end to the long debate about the proper microscopic modeling for cuprates. In this work, we rigorously derive an effective one-band generalized $t\!-\!J$ model for T-CuO, based on orthogonalized Zhang-Rice singlets, and make an estimative calculation of its parameters, based on previous \textit{ab initio} calculations. By means of the self-consistent Born approximation, we then evaluate the spectral function and the quasiparticle dispersion for a single hole doped in antiferromagnetically ordered half-filled T-CuO. Our predictions show very good agreement with angle-resolved photoemission spectra and with theoretical multiband results. We conclude that a generalized $t\!-\!J$ model remains the minimal Hamiltonian for a correct description of single-hole dynamics in cuprates.
description: 5 pages, 4 figures. Supplemental Material. To be published in Physical Review Letters
CPT Tests in the Neutral Kaon System by FNAL E773
Creators: name: Schwingenheuer, B.
Publisher: name: arXiv
Year: 1994
Subjects: subject: High Energy Physics - Experiment (hep-ex)
subject: FOS: Physical sciences

description: The FNAL experiment E773 has measured the phases Phi_{+-} = (43.35 +- 0.70 +- 0.79) degree and Phi_{00}-Phi_{+-} = (0.67 +- 0.85 +- 1.1) degree of the CP violating parameters eta_{+-} and eta_{00} in the decay of neutral kaons into two charged or neutral pions. These preliminary results test CPT symmetry and show no evidence for a violation. In addition we present a preliminary measurement of Delta m = m_L - m_S = (0.5286 +- 0.0029 +- 0.0022)*E+10 hbar/sec and tau_S = (0.8929 +- 0.0014 +- 0.0014)*E-10 sec. The first errors are statistical and the second errors are systematic for above results.
description: 9 pages, EFI 94-31 (replaced postscript file by uuencoded compressed postscript file)
title: ADCO, Grènetier de Cîteaux : comptes (1497-1504) (11 H 1172), f. 00603
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. 00603, 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
Cancer symmysta Linnaeus, 1758, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1758
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Malacostraca
Decapoda
Cancridae
Cancer
Cancer symmysta

description: Cancer symmysta [spec. nov.]
C. subbrachyurus, thorace subcylindrico ciliato-serrato, chelis cordatis, antennis ciliato-pilosis.
Habitat in Asia.
* f * Macrouri parasitici, cauda setacea aphylla.
description: Published as part of Linnaeus, Carolus, 1758, Systema Naturae per regna tria naturae: secundum classes, ordines, genera, species, cum characteribus, differentiis, synonymis, locis, Stockholm :Laurentius Salvius on pages 630-631, DOI: 10.5962/bhl.title.542, http://zenodo.org/record/3922206
Additional file 1: of Comparison of logistic regression with machine learning methods for the prediction of fetal growth abnormalities: a retrospective cohort study
Creators: name: Kuhle, Stefan
name: Maguire, Bryan
name: Hongqun Zhang
name: Hamilton, David
name: Allen, Alexander
name: K. Joseph
name: Allen, Victoria
Publisher: name: figshare
Year: 2018
Subjects: subject: Medicine
subject: Microbiology
subject: FOS: Biological sciences
subject: Sociology
subject: FOS: Sociology
subject: 69999 Biological Sciences not elsewhere classified
subject: 19999 Mathematical Sciences not elsewhere classified
subject: FOS: Mathematics
subject: Developmental Biology
subject: 60506 Virology

description: Table S1. Predictors of fetal growth abnormalities and their use in the prediction models. (PDF 71 kb)
An SZ Temperature Decrement - X-ray Luminosity Relation for Galaxy Clusters
Creators: name: Cooray, Asantha R.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present the observed relation between the cosmic microwave background (CMB) temperature decrement due to the Sunyaev-Zeldovich (SZ) effect and the X-ray luminosity of galaxy clusters. We discuss this relation in terms of the cluster properties, and show that the slope of the observed relation is in agreement with both the L-T relation based on numerical simulations and X-ray emission observations, and the M_gas-L relation based on observations. The slope of the Delta T_SZ-L relation is also consistent with the M_tot-L relation, where M_tot is the cluster total mass based on gravitational lensing observations. This agreement may be taken to imply a constant gas mass fraction within galaxy clusters, however, there are large uncertainties, dominated by observational errors, associated with these relations. Using the Delta T_SZ-L relation and the cluster X-ray luminosity function, we evaluate the local cluster contribution to arcminute scale cosmic microwave background anisotropies. The Compton distortion y-parameter produced by massive galaxy clusters through SZ effect is roughly two orders of magnitude lower than the current upper limit based on FIRAS observations.
description: 7 pages, 8 figures. MNRAS (in press)
On the Nuclear Rotation Curve of M31
Creators: name: Statler, Thomas S.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: The nuclear rotation curve of M31, as observed by the Hubble Space Telescope Faint Object Camera Spectrograph, shows a significant disturbance coinciding with the off-center brightness peak, P1. This +/- 60 km/s feature is distinguished by a local velocity maximum centered on P1 and a local minimum approxmately 0.08" closer to P2. If the M31 double nucleus is an eccentric disk with an off-center density concentration, as suggested by Tremaine, then the self-gravity of the disk can produce just such a disturbance. The expected kinematic signature is calculated approximately by examining sequences of closed periodic orbits in a Kepler potential perturbed by a model disk potential that precesses at constant frequency. The perturbation forces a steep negative eccentricity gradient in the sequence of closed orbits through the densest part of the disk, which reverses the arrangement of periapsis and apoapsis with respect to the central mass. Stars making up the inner part of the density concentration are at apoapsis, while stars making up the outer part are at periapsis, producing a steep local velocity gradient. This result is independent of the details of the mass distribution. The projected rotation curve of the model is shown to closely resemble that of M31, giving strong support to the eccentric disk picture.
description: 10 pages, 4 eps figures, LaTeX, AASTeX 4.0. Submitted to ApJ Letters
Supersymmetric dynamics and zeta-functions
Creators: name: Makhaldiani, Nugzar
Publisher: name: arXiv
Year: 2018
Subjects: subject: General Physics (physics.gen-ph)
subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: Boson, fermion, and super oscillators and (statistical) mechanism of cosmological constant; finite approximation of the zeta-function and fermion factorization of the bosonic statistical sum considered.
Nuclear Broadening of Out-of-Plane Transverse Momentum in Di-Jet Production
Creators: name: Kopeliovich, Boris
Publisher: name: arXiv
Year: 1994
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: High Energy Physics - Experiment (hep-ex)
subject: FOS: Physical sciences

description: Recently claimed \cite{dj1,dj2,FC} anomalous nuclear effects in di-jet production are analyzed in view of multiple interaction of projectile/ejectile partons in nuclear matter. We derive model--independent relations between A-dependence of the cross section and nuclear broadening of transverse momentum. Comparison with the data show that initial/final state interaction of partons participating in hard process is hard as well. This is a solid argument in favor of smallness of a color neutralization radius of a hadronizing highly virtual quark.
description: 6 pages, Talk presented at the 5th Conference on the Intersection of Particle and Nuclear Physics, St. Petersburg, Florida, 1994
Evolution of the cluster abundance in non-Gaussian models
Creators: name: Robinson, James
name: Baker, Jonathan E.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We carry out N-body simulations of several non-Gaussian structure formation models, including Peebles' isocurvature cold dark matter model, cosmic string models, and a model with primordial voids. We compare the evolution of the cluster mass function in these simulations with that predicted by a modified version of the Press-Schechter formalism. We find that the Press-Schechter formula can accurately fit the cluster evolution over a wide range of redshifts for all of the models considered, with typical errors in the mass function of less than 25%, considerably smaller than the amount by which predictions for different models may differ. This work demonstrates that the Press-Schechter formalism can be used to place strong model independent constraints on non-Gaussianity in the universe.
description: 11 pages, 12 postscipt figures
How Much SETI Has Been Done? Finding Needles in the n-Dimensional Cosmic Haystack
Creators: name: Wright, Jason T.
name: Kanodia, Shubham
name: Lubar, Emily G.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Instrumentation and Methods for Astrophysics (astro-ph.IM)
subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: FOS: Physical sciences

description: Many articulations of the Fermi Paradox have as a premise, implicitly or explicitly, that humanity has searched for signs of extraterrestrial radio transmissions and concluded that there are few or no obvious ones to be found. Tarter et al. (2010) and others have argued strongly to the contrary: bright and obvious radio beacons might be quite common in the sky, but we would not know it yet because our search completeness to date is so low, akin to having searched a drinking glass's worth of seawater for evidence of fish in all of Earth's oceans. Here, we develop the metaphor of the multidimensional "Cosmic Haystack" through which SETI hunts for alien "needles" into a quantitative, eight-dimensional model and perform an analytic integral to compute the fraction of this haystack that several large radio SETI programs have collectively examined. Although this model haystack has many qualitative differences from the Tarter et al. (2010) haystack, we conclude that the fraction of it searched to date is also very small: similar to the ratio of the volume of a large hot tub or small swimming pool to that of the Earth's oceans. With this article we provide a Python script to calculate haystack volumes for future searches and for similar haystacks with different boundaries. We hope this formalism will aid in the development of a common parameter space for the computation of upper limits and completeness fractions of search programs for radio and other technosignatures.
description: 20 pages, 4 figures. Submitted to The Astronomical Journal on 17th August 2018, Accepted on 11th September 2018. Published on 14th November 2018 v2 includes a correction to Eq. 11. Thanks to Bart Wlodarczyk-Sroka and Michael Garrett for spotting the typographical error (a missing factor of 4pi), which has no effect on the rest of the paper or the associated code
ZAMONAVIY TURIZMNING VUJUDGA KELISHI  JARAYONLARI VA BOSQICHLARI
Creators: name: Tashov, Mizrob
Publisher: name: Zenodo
Year: 2025

description: Turizmni, ilmiy asoslangan holda amalga oshirish g‘oyasini ro‘yobga chiqarish XIX asrning o‘rtalariga to‘g‘ri kelgan bo‘lib, bu jarayon sanoatning rivojlanishi va ishlab chiqarishning takomillashuvi bilan bog‘liqdir. Muallif maqolada  zamonaviy turizmning vujudga kelishi  jarayonlari va bosqichlarini  ilmiy isbotlab bergan.
Detecting Tau Neutrino Oscillations at PeV Energies
Creators: name: Learned, John G.
name: Pakvasa, Sandip
Publisher: name: arXiv
Year: 1994
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: Astrophysics (astro-ph)
subject: High Energy Physics - Experiment (hep-ex)
subject: FOS: Physical sciences

description: It is suggested that a large deep underocean (or ice) neutrino detector, given the presence of significant numbers of neutrinos in the PeV energy range as predicted by various models of Active Galactic Nuclei, can make unique measurements of the properties of neutrinos. It will be possible to observe the existence of the tau neutrino, measure its mixing with other flavors, in fact test the mixing pattern for all three flavors based upon the mixing parameters suggested by the atmospheric and solar neutrino data, and measure the tau neutrino cross section. The key signature is the charged current tau neutrino interaction, which produces a double cascade, one at either end of a lightly radiating track. At a few PeV these cascades would be separated by roughly 100 m, and thus be easily resolvable in next generation DUMAND-like detectors. First examples might be found in detectors presently under construction. Future applications are precise neutrino astronomy and earth tomography. This paper is an expanded version of hep-ph/9405296, for publication.
description: 18 pages latex, incl 3 figs, UH-511-799-94
title: ADCO, Sixième cartulaire de Saint-Étienne de Dijon (1662), Cart. 30 (G 133), 441 folios, f. 625
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: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris
subject: cartulaire
subject: Corpus Burgundiae Medii Aevi
subject: Chartes de la Bourgogne du Moyen Âge

description: Sixième cartulaire de Saint-Étienne de Dijon (1662), Archives départementales de la Côte-d'Or, Cart. 30 (G 133), 441 folios, f. 625, Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Sixième cartulaire de Saint-Étienne de Dijon (1662), Archives départementales de la Côte-d'Or, Cart. 30 (G 133), 441 folios, f. 625, 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 Peroxiredoxin I maintains luteal function by regulating unfolded protein response
Creators: name: Park, Hyo-Jin
name: Lee, Dong
name: Seong, Jung
name: Hyun-Shik Lee
name: Oh-Shin Kwon
name: Kang, Beom
name: Jeen-Woo Park
name: Sang-Rae Lee
name: Dong-Seok Lee
Publisher: name: figshare
Year: 2018
Subjects: subject: Biochemistry
subject: Cell Biology
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Physiology
subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences
subject: Developmental Biology
subject: Cancer

description: Figure S1. Changes in PRDX family (2–6) protein levels in luteal phase of WT mice. Protein levels of PRDX 2–6 were confirmed in CL tissue by western blot analysis (A). The relative levels of PRDX proteins were obtained after normalization to β-actin levels. The histogram values of densitometry analysis were obtained using the Image J software. The bar graph data represent the least-squares means ± SEM of three independent experiments. *P
title: Untersuchung der Lösungsmittelatmosphäre von verdunstenden, gedruckten Fluidfilmen mittels digitaler, holographischer Interferometrie
Creators: name: Braig, Felix
Publisher: name: UNSPECIFIED
Year: 2024

description: Um die qualitative und quantitative Verteilung des Lösungsmitteldampfs in der Umgebung von gedruckten Fluidfilmen zu bestimmen, werden eine Inkjet-Einheit und ein Laser-Michelson-Interferometer in die Roboterzelle eines Sechs-Achs-Roboters integriert. Die Inkjet-Druckeinheit und der Roboter werden genutzt, um linienförmige Fluidfilme eines binären Druckfluids aus Ethylenglykol und Ethanol mit unterschiedlichen Längen und Breiten zu drucken und diese automatisiert in den Messarm des Interferometers zu bewegen. Um den Einfluss der natürlichen Konvektion auf die Lösungsmittelkonzentration in der Umgebung der gedruckten Fluidfilme zu untersuchen, wird das Substrat sowohl horizontal als auch vertikal in dem Messarm platziert. Die Interferogramme des Interferometers werden mithilfe einer Kamera aufgenommen und die durch den Lösungsmitteldampf hervorgerufene Phasenverschiebung zwischen dem Messarm und Referenzarm des Interferometers mithilfe der Windowed-Fourier-Transform Methode bestimmt. Nachdem die Phasensprünge durch das Phase Unwrapping entfernt wurden, lässt sich der Gangunterschied berechnen, der durch den Lösungsmitteldampf verursacht wird. Bei dem Gangunterschied handelt es sich um eine in Lichtausbreitungsrichtung integrierte Größe, das heißt die dreidimensionale Konzentrationsverteilung des Lösungsmitteldampfs wird auf die Ebene des Kamerasensors projiziert. Indem die Gangunterschiede mehrerer linienförmiger Fluidfilme unterschiedlicher Länge kombiniert werden, kann eine zweidimensionale Konzentrationsverteilung des Lösungsmitteldampfs entlang eines Querschnitts durch den mittleren Bereich des linienförmigen Fluidfilms bestimmt werden. Die maximal ermittelten Stoffmengenkonzentrationen werden dabei an der Phasenkontaktfläche zwischen flüssiger und gasförmiger Phase erreicht. Die Temperatur, der Luftdruck und die Luftfeuchtigkeit werden während der Messungen aufgezeichnet, sodass die bestimmten Konzentrationswerte mit den theoretischen Sättigungsdampfkonzentrationen bei den jeweiligen Bedingungen verglichen werden können. Es zeigt sich für die linienförmigen Fluidfilme, dass der Einfluss der natürlichen Konvektion auf die Lösungsmitteldampfverteilung über den verdunstenden Fluidfilmen mit zunehmender Breite des Fluidfilms steigt. Das Messverfahren eignet sich, um die Randüberhohung der Verdunstungsrate zu identifizieren und zu quantifizieren. Während die horizontalen Substratpositionen eine symmetrische Randüberhöhung der Verdunstungsrate aufweisen, wird in der vertikalen Substratposition eine starke Asymmetrie deutlich. Um die Reproduzierbarkeit der bestimmten Gangunterschiede zu erhöhen und damit die Genauigkeit der bestimmten Konzentrationsverteilungen weiter zu verbessern, könnte die passive Überwachung der Luftparameter mit einer Überwachung der Substrattemperatur und einer aktiven Steuerung der Umgebungsparameter ergänzt werden.
Global Dynamics of Advection-Dominated Accretion Revisited
Creators: name: Lu, Ju-Fu
name: Gu, Wei-Min
name: Yuan, Feng
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We numerically solve the set of dynamical equations describing advection-dominated accretion flows (ADAF) around black holes, using a method similar to that of Chakrabarti (1996a). We choose the sonic radius of the flow $R_s$ and the integration constant in angular momentum equation $j$ as free parameters, and integrate the equations from the sonic point inwards to see if the solution can extend supersonically to the black hole horizon, and outwards to see if and where an acceptable outer boundary of the flow can be found. We recover the ADAF-thin disk solution constructed in Narayan, Kato, & Honma (1997, NKH97), an representative paper of the previous works on global ADAF solutions, although in that paper an apparently very different procedure was adopted. We obtain a complete picture in the form of $R_s-j$ parameter space which sums up the situation of ADAF solution at a glance. For comparison we also present the distribution of global solutions for inviscid flows in the $R_s-j$ space, which supports the view that there should be some similarities between the dynamical behavior of ADAF and that of adiabatic flows, and that there should be a continuous change from the properties of viscous flows to those of inviscid ones.
description: 24 pages with 15 figures, to appear in ApJ Vol. 523
Saturating the quantum Cramér-Rao bound using LOCC
Creators: name: Zhou, Sisi
name: Zou, Chang-Ling
name: Jiang, Liang
Publisher: name: arXiv
Year: 2018
Subjects: subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: The quantum Cramér-Rao bound (QCRB) provides an ultimate precision limit allowed by quantum mechanics in parameter estimation. Given any quantum state dependent on a single parameter, there is always a positive-operator valued measurement (POVM) saturating the QCRB. However, the QCRB-saturating POVM cannot always be implemented efficiently, especially in multipartite systems. In this paper, we show that the POVM based on local operations and classical communication (LOCC) is QCRB-saturating for arbitrary pure states or rank-two mixed states with varying probability distributions over fixed eigenbasis. Local measurements without classical communication, however, is not QCRB-saturating in general.
description: 13 pages, 2 figures, published version
A Measurement of the Angular Power Spectrum of the Microwave Background Made from the High Chilean Andes
Creators: name: Torbet, E.
name: Devlin, M. J.
name: Dorwart, W. B.
name: Herbig, T.
name: Miller, A. D.
name: Nolta, M. R.
name: Page, L.
name: Puchalla, J.
name: Tran, H. T.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We report on a measurement of the angular spectrum of the anisotropy of the microwave sky at 30 and 40 GHz between l=50 and l=200 over approximately 600 sq. deg. The data support a rise in the angular spectrum to a maximum with $δT_l \approx 85 μ$K at l=200. We also give a 2-sigma upper limit of $δT_l < 122 μ$K at l=432 at 144 GHz. These results come from the first campaign of the Mobile Anisotropy Telescope (MAT) on Cerro Toco, Chile. To assist in assessing the site, we present plots of the fluctuations in atmospheric emission at 30 and 144 GHz.
description: 5 pages, 3 figures, 2 tables; revised 10 June. Submitted to ApJL. Website at http://pupgg.princeton.edu/~cmb
Additional file 1 of Developing guideline-based key performance indicators for recurrent miscarriage care: lessons from a multi-stage consensus process with a diverse stakeholder group
Creators: name: Hennessy, Marita
name: Linehan, Laura
name: Dennehy, Rebecca
name: Devane, Declan
name: Rice, Rachel
name: Meaney, Sarah
name: O’Donoghue, Keelin
Publisher: name: figshare
Year: 2022
Subjects: subject: Medicine
subject: Genetics
subject: FOS: Biological sciences
subject: Environmental Sciences not elsewhere classified
subject: Biological Sciences not elsewhere classified
subject: Developmental Biology
subject: Cancer
subject: Science Policy
subject: Infectious Diseases
subject: FOS: Health sciences

description: Additional file 1. GRIPP2-SF Reporting Checklist.
Cancer bernhardus Linnaeus, 1758, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1758
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Malacostraca
Decapoda
Cancridae
Cancer
Cancer bernhardus

description: Cancer bernhardus [spec. nov.]
C. macrourus parasiticus, chelis cordatis laevibus: sinistra majore.
Gesn. aquat. 161.
Habitat in Oceano Europaeo, intra varias testas Concharum.
Chelae margine anteriore versus basin barbatae.
description: Published as part of Linnaeus, Carolus, 1758, Systema Naturae per regna tria naturae: secundum classes, ordines, genera, species, cum characteribus, differentiis, synonymis, locis, Stockholm :Laurentius Salvius on page 631, DOI: 10.5962/bhl.title.542, http://zenodo.org/record/3922206
Additional file 4: of Enhancement of Glen Moy x Latham raspberry linkage map using GbS to further understand control of developmental processes leading to fruit ripening
Creators: name: Hackett, Christine
name: Milne, Linda
name: Smith, Kay
name: Hedley, Pete
name: Morris, Jenny
name: Simpson, Craig
name: Preedy, Katharine
name: Graham, Julie
Publisher: name: figshare
Year: 2018
Subjects: subject: Space Science
subject: Cell Biology
subject: Genetics
subject: FOS: Biological sciences
subject: 59999 Environmental Sciences not elsewhere classified
subject: FOS: Earth and related environmental sciences
subject: Ecology
subject: Immunology
subject: FOS: Clinical medicine
subject: 69999 Biological Sciences not elsewhere classified
subject: Developmental Biology
subject: 110309 Infectious Diseases
subject: FOS: Health sciences

description: Table S1. Genome scaffolds within 2Â cM of most significant marker containing genes with a potential role in ripening related developmental processes. This table examines genes within the QTL regions which may have a role in developmental processes leading to fruit ripening. (DOCX 30Â kb)
Spin Asymmetry in Muon--Proton Deep Inelastic Scattering on a Transversely-Polarized Target
Creators: name: The Spin Muon Collaboration
Publisher: name: arXiv
Year: 1994
Subjects: subject: High Energy Physics - Experiment (hep-ex)
subject: FOS: Physical sciences

description: We measured the spin asymmetry in the scattering of 100 GeV longitudinally-polarized muons on transversely polarized protons. The asymmetry was found to be compatible with zero in the kinematic range $0.006
description: 10 pages CERN-PPE/94-116
What makes a theory of infinitesimals useful? A view by Klein and Fraenkel
Creators: name: Kanovei, Vladimir
name: Katz, Karin U.
name: Katz, Mikhail G.
name: Mormann, Thomas
Publisher: name: arXiv
Year: 2018
Subjects: subject: History and Overview (math.HO)
subject: Classical Analysis and ODEs (math.CA)
subject: Logic (math.LO)
subject: FOS: Mathematics
subject: 26E35, 03A05

description: Felix Klein and Abraham Fraenkel each formulated a criterion for a theory of infinitesimals to be successful, in terms of the feasibility of implementation of the Mean Value Theorem. We explore the evolution of the idea over the past century, and the role of Abraham Robinson's framework therein.
description: 10 pages, published in Journal of Humanistic Mathematics http://scholarship.claremont.edu/jhm/vol8/iss1/7/
Additional file 8 of Developing guideline-based key performance indicators for recurrent miscarriage care: lessons from a multi-stage consensus process with a diverse stakeholder group
Creators: name: Hennessy, Marita
name: Linehan, Laura
name: Dennehy, Rebecca
name: Devane, Declan
name: Rice, Rachel
name: Meaney, Sarah
name: O’Donoghue, Keelin
Publisher: name: figshare
Year: 2022
Subjects: subject: Medicine
subject: Genetics
subject: FOS: Biological sciences
subject: Environmental Sciences not elsewhere classified
subject: Biological Sciences not elsewhere classified
subject: Developmental Biology
subject: Cancer
subject: Science Policy
subject: Infectious Diseases
subject: FOS: Health sciences

description: Additional file 8. Overview of item rating during final survey, by stakeholder category, KPI category.
A Stellar Population Gradient in VII Zw 403 - Implications for the Formation of Blue Compact Dwarf Galaxies
Creators: name: Schulte-Ladbeck, Regina E.
name: Hopp, Ulrich
name: Crone, Mary M.
name: Greggio, Laura
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present evidence for the existence of an old stellar halo in the Blue Compact Dwarf galaxy VII Zw 403. VII Zw 403 is the first Blue Compact Dwarf galaxy for which a clear spatial segregation of the resolved stellar content into a "core-halo" structure is detected. Multicolor HST/WFPC2 observations indicate that active star formation occurs in the central region, but is strikingly absent at large radii. Instead, a globular-cluster-like red giant branch suggests the presence of an old (> 10 Gyr) and metal poor (=-1.92) stellar population in the halo. While the vast majority of Blue Compact Dwarf galaxies has been recognized to possess halos of red color in ground-based surface photometry, our observations of VII Zw 403 establish for the first time a direct correspondence between a red halo color and the presence of old, red giant stars. If the halos of Blue Compact Dwarf galaxies are all home to such ancient stellar populations, then the fossil record conflicts with delayed-formation scenarios for dwarfs.
description: Accepted for publication in the ApJ
Echo trains in pulsed electron spin resonance of a strongly coupled spin ensemble
Creators: name: Weichselbaumer, Stefan
name: Zens, Matthias
name: Zollitsch, Christoph W.
name: Brandt, Martin S.
name: Rotter, Stefan
name: Gross, Rudolf
name: Huebl, Hans
Publisher: name: arXiv
Year: 2018
Subjects: subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: We report on a novel dynamical phenomenon in electron spin resonance experiments of phosphorus donors. When strongly coupling the paramagnetic ensemble to a superconducting lumped element resonator, the coherent exchange between these two subsystems leads to a train of periodic, self-stimulated echos after a conventional Hahn echo pulse sequence. The presence of these multi-echo signatures is explained using a simple model based on spins rotating on the Bloch sphere, backed up by numerical calculations using the inhomogeneous Tavis-Cummings Hamiltonian.
The swansong in context: long-timescale X-ray variability of NGC 4051
Creators: name: Uttley, P.
name: McHardy, I. M.
name: Papadakis, I. E.
name: Guainazzi, M.
name: Fruscione, A.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: On 9-11 May 1998, the highly-variable, low luminosity Seyfert 1 galaxy NGC4051 was observed in an unusual low flux state by BeppoSAX (Guainazzi et al. 1998) RXTE and EUVE. We present fits of the 4-15 keV RXTE spectrum and BeppoSAX MECS spectrum obtained during this observation, which are consistent with the interpretation that the source had switched off, leaving only the spectrum of pure reflection from distant cold matter. We place this result in context by showing the X-ray lightcurve of NGC4051 obtained by our RXTE monitoring campaign over the past two and a half years, which shows that the low state lasted for ~150 days before the May observations (implying that the reflecting material is > 10^17 cm from the continuum source) and forms part of a lightcurve showing distinct variations in long-term average flux over timescales > months. We show that the long-timescale component to X-ray variability is intrinsic to the primary continuum and is probably distinct from the variability at shorter timescales, possibly associated with variations in the accretion flow of matter onto the central black hole. As the source approaches the low state, the variability process becomes non-linear. NGC4051 may represent a microcosm of all X-ray variability in radio quiet active galactic nuclei (AGNs), displaying in a few years a variety of flux states and variability properties which more luminous AGNs may pass through on timescales of decades to thousands of years.
description: 5 pages, accepted for publication in MNRAS
Additional file 1: of Miglustat in Niemann-Pick disease type C patients: a review
Creators: name: MercĂ¨ Pineda
name: Walterfang, Mark
name: Patterson, Marc
Publisher: name: figshare
Year: 2018
Subjects: subject: Space Science
subject: Medicine
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Sociology
subject: FOS: Sociology
subject: Developmental Biology
subject: Marine Biology
subject: Science Policy

description: Table S1. Comparison of disability scales. (DOCX 45 kb)
Additional file 11: of Comparison of logistic regression with machine learning methods for the prediction of fetal growth abnormalities: a retrospective cohort study
Creators: name: Kuhle, Stefan
name: Maguire, Bryan
name: Hongqun Zhang
name: Hamilton, David
name: Allen, Alexander
name: K. Joseph
name: Allen, Victoria
Publisher: name: figshare
Year: 2018
Subjects: subject: Medicine
subject: Molecular Biology
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: 19999 Mathematical Sciences not elsewhere classified
subject: FOS: Mathematics
subject: Developmental Biology

description: Figure S8. Receiver operating characteristic curves for the prediction of LGA among multiparous women (26Â weeks) using elastic net, classification trees, random forest, gradient boosting, and neural networks. (PDF 201 kb)
Sequences of consecutive squares on quartic elliptic curves
Creators: name: Sadek, Mohammad
name: Kamel, Mohamed
Publisher: name: arXiv
Year: 2018
Subjects: subject: Number Theory (math.NT)
subject: FOS: Mathematics

description: Let $C: y^2=ax^4+bx^2+c$, be an elliptic curve defined over $\mathbb Q$. A set of rational points $(x_i,y_i) \in C(\mathbb Q)$, $i=1,2,\cdots,$ is said to be a sequence of consecutive squares if $x_i= (u + i)^2$, $i=1,2,\cdots$, for some $u\in \mathbb Q$. Using ideas of Mestre, we construct infinitely many elliptic curves $C$ with sequences of consecutive squares of length at least $6$. It turns out that these 6 rational points are independent. We then strengthen this result by proving that for a fixed $6$-term sequence of consecutive squares, there are infinitely many elliptic curves $C$ with the latter sequence forming the $x$-coordinates of six rational points in $C(\mathbb Q)$.
Millimetric Astronomy from the High Antarctic Plateau: site testing at Dome C
Creators: name: Valenziano, L.
name: Dall'Oglio, G.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Preliminary site testing at Dome C (Antarctica) is presented, using both Automatic Weather Station (AWS) meteorological data (1986-1993) and Precipitable Water Vapor (PWV) measurements made by the authors. A comparison with South Pole and other sites is made. The South Pole is a well established astrophysical observing site, where extremely good conditions are reported for a large fraction of time during the year. Dome C, where Italy and France are building a new scientific station, is a potential observing site in the millimetric and sub-millimetric range. AWS are operating at both sites and they have been continuously monitoring temperature, pressure, wind speed and direction for more than ten years. Site testing instruments are already operating at the South Pole (AASTO, Automated Astrophysical Site-Testing Observatory), while ''light'' experiments have been running at Dome C (APACHE, Antarctic Plateau Anisotropy CHasing Experiment) during summertime. A direct comparison between the two sites is planned in the near future, using the AASTO. The present analysis shows that the average wind speed is lower at Dome C (~1 m/s) than at the South Pole (~2 m/s), while temperature and PWV are comparable.
description: 10 pages, 8 figures, se also http://www.atnf.csiro.au/pasa/16_2/
Asynchronous exponential growth of the growth-fragmentation equation with unbounded fragmentation rate
Creators: name: Bernard, Etienne
name: Gabriel, Pierre
Publisher: name: arXiv
Year: 2018
Subjects: subject: Analysis of PDEs (math.AP)
subject: FOS: Mathematics

description: The objective is to prove the asynchronous exponential growth of the growth-fragmentation equation in large weighted $L^1$ spaces and under general assumptions on the coefficients. The key argument is the creation of moments for the solutions to the Cauchy problem, resulting from the unboundedness of the total fragmentation rate. It allows us to prove the quasi-compactness of the associated (rescaled) semigroup, which in turn provides the exponential convergence toward the projector on the Perron eigenfunction.