cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
title: ADCO, Cartulaire de l'office de la Porte de l'abbaye de Cîteaux, Registrum possessionum porte Cistercii (début XVe siècle), Cart. 172 (11 H 69), 115 folios, f. 0055
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: cartulaire
subject: Corpus Burgundiae Medii Aevi
subject: Chartes de la Bourgogne du Moyen Âge
subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris

description: Cartulaire de l'office de la Porte de l'abbaye de Cîteaux, Registrum possessionum porte Cistercii (début XVe siècle), Archives départementales de la Côte-d'Or, Cart. 172 (11 H 69), 115 folios, f. 0055, Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Cartulaire de l'office de la Porte de l'abbaye de Cîteaux, Registrum possessionum porte Cistercii (début XVe siècle), Archives départementales de la Côte-d'Or, Cart. 172 (11 H 69), 115 folios, f. 0055, 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
Galaxy Formation by Galactic Magnetic Fields
Creators: name: Totani, Tomonori
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Galaxies exhibit a sequence of various morphological types, i.e., the Hubble sequence, and they are basically composed of spheroidal components (elliptical galaxies and bulges in spiral galaxies) and disks. It is known that spheroidal components are found only in relatively massive galaxies with M=10^{10-12} M_sun, and all stellar populations in them are very old, but there is no clear explanation for these facts. Here we present a speculative scenario for the origin of the Hubble sequence, in which magnetic fields ubiquitously seen in galaxies have played a crucial role. We first start from a strange observational fact that magnetic field strengths observed in spiral galaxies sharply concentrate at a few microgauss, for a wide range of galaxy luminosity and types. We then argue that this fact and the observed correlation between star formation activity and magnetic field strength in spiral galaxies suggest that spheroidal galaxies have formed by starbursts induced by strong magnetic fields. Then we show that this idea naturally leads to the formation of spheroidal systems only in massive and high-redshift objects in hierarchically clustering universe, giving a simple explanation for various observations.
description: 7 pages including 2 figures. Accepted by ApJ Letters
Musca roralis Linnaeus, 1758, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1758
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Diptera
Anthomyiidae
Musca
Musca roralis

description: Musca roralis [spec. nov.]
M. antennis setariis pilosa aterrima.
Habitat in Europa.
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 597, DOI: 10.5962/bhl.title.542, http://zenodo.org/record/3922206
Metal Deficiency in Two Massive Dead Galaxies at $z\sim2$
Creators: name: Morishita, T.
name: Abramson, L. E.
name: Treu, T.
name: Wang, X.
name: Brammer, G. B.
name: Kelly, P.
name: Stiavelli, M.
name: Jones, T.
name: Schmidt, K. B.
name: Trenti, M.
name: Vulcani, B.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: Local massive early-type galaxies are believed to have completed most of their star formation $\sim10$Gyr ago and evolved without having substantial star formation since. If so, their progenitors should have roughly solar stellar metallicities ($Z_*$), comparable to their values today. We report the discovery of two lensed massive ($\log M_*/M_\odot\sim11$), $z\sim2.2$ dead galaxies, that appear markedly metal deficient given this scenario. Using 17-band $HST$+$K_{s}$+$Spitzer$ photometry and deep $HST$ grism spectra from the GLASS and SN Refsdal follow-up campaigns covering features near $λ_{\rm rest}\sim4000$Å, we find these systems to be dominated by A-type stars with $\log Z_*/Z_\odot=-0.40\pm0.02$ and $-0.49\pm0.03$ ($30$-$40\%$ solar) under standard assumptions. The second system's lower metallicity is robust to isochrone changes, though this choice can drive the first system's from $\log Z_*/Z_\odot=-0.6$ to 0.1. If these two galaxies are representative of larger samples, this finding suggests that evolutionary paths other than dry minor-merging are required for these massive galaxies. Future analyses with direct metallicity measurements-e.g., by the $James\ Webb\ Space\ Telescope$-will provide critical insight into the nature of such phenomena.
description: Accepted for publication in Astrophysical Journal Letters; 6 pages, 3 figures, 1 table
Musca serrata Linnaeus, 1758, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1758
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Diptera
Anthomyiidae
Musca
Musca serrata

description: Musca serrata [spec. nov.]
M. antennis setariis pilosa fusca, alarum costa pilis brevissimis serrata, abdomine pedibusque ferrugineis.
Habitat in Europa.
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 597, DOI: 10.5962/bhl.title.542, http://zenodo.org/record/3922206
Autoxidation and its Inhibition in Both Industrial and Biological Contexts: New Molecules, Methods & Mechanisms
Creators: name: Shah, Ronak
Publisher: name: Université d'Ottawa / University of Ottawa
Year: 2019
Subjects: Ferroptosis
Autoxidation
Antioxidant
Lipoxygenase
Antioxidant Assay
Diarylamines

description: Autoxidation, a radical chain reaction, is largely responsible for the degradation of most man-made and biological materials. These include chemical products such as lubricants, plastics and rubber; as well as biological molecules and membranes within our bodies. The development of means to hinder this process has been a major focus of the petroleum, chemical, pharmaceutical and biotechnology industry over the past century. The two most common strategies to emerge from these efforts have been the use of compounds that either prevent the initiation of autoxidation or trap the propagating radicals, so-called radical-trapping antioxidants (RTAs). Herein, we describe our efforts towards the design and development of extremely potent heterocyclic diarylamine RTAs, and their activity in a variety of applications ranging from isotropic organic solution to mammalian cells. We have elucidated the important structural motifs and mechanistic considerations necessary for the development of next-generation arylamine RTAs. Some of the substituted heterocyclic diarylamines analogs we disclose are among the best inhibitors of high temperature autoxidations described to date. Alongside, we developed novel analytical tools to facilitate the studies and acquisition of results for characterizing RTA activity in organic solutions and lipid bilayers. These fluorescent probes are highly relevant and allow for the determination of hydroperoxide and acid concentrations rapidly, as well as screen (or counter-screen) RTAs in liposomal membranes. Our methodologies address numerous drawbacks from frequently used ‘plug-and-play’ assays and we anticipate they will fill a current unmet need in both industrial and academic laboratories worldwide. Moreover, the recent characterization of ferroptosis – a novel regulated necrotic-like cell-death pathway associated with the accumulation of lipid hydroperoxides – has paved a way forward for studying oxidation induced damage in a biological context. Utilizing our expertise in lipid peroxidation and inhibition, we elucidated the prominent role of autoxidation in the execution of ferroptotic cell death. Alongside, our analytical tools and RTAs have also enabled the identification and characterization of novel ferroptosis inhibitors. Furthermore, this has prompted the development of a correlation to predict anti-ferroptosis activity of small-molecules using simple spectrophotometric assays.
Musca cellaris Linnaeus, 1758, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1758
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Diptera
Anthomyiidae
Musca
Musca cellaris

description: Musca cellaris [spec. nov.]
M. antennis setariis pilosa nigra, alis nervosis, oculis ferrugineis. Fn. svec. 1111.
Habitat in cellis vinariis aliisque.
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 597, DOI: 10.5962/bhl.title.542, http://zenodo.org/record/3922206
Reversible Pressure-Induced Amorphization in Solid C70 : Raman and Photoluminescence Study
Creators: name: Chandrabhas, N.
name: Sood, Ajay K.
name: Muthu, D. V. S.
name: Sundar, C. S.
name: Bharathi, A.
name: Hariharan, Y.
name: Rao, C. N. R.
Publisher: name: arXiv
Year: 1994
Subjects: subject: Condensed Matter (cond-mat)
subject: FOS: Physical sciences

description: We have studied single crystals of $C_{70}$ by Raman scattering and photoluminescence in the pressure range from 0 to 31.1 GPa. The Raman spectrum at 31.1 GPa shows only a broad band similar to that of the amorphous carbon without any trace of the Raman lines of $C_{70}$. After releasing the pressure from 31.1 GPa, the Raman and the photoluminescence spectra of the recovered sample are that of the starting $C_{70}$ crystal. These results indicate that the $C_{70}$ molecules are stable upto 31.1 GPa and the amorphous carbon high pressure phase is reversible, in sharp contrast to the results on solid $C_{60}$. A qualitative explaination is suggested in terms of inter- versus intra-molecular interactions.
description: To appear in Phys. Rev. Lett., 12 pages, RevTeX (preprint format), 3 figures available upon request
Musca putris Linnaeus, 1758, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1758
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Diptera
Anthomyiidae
Musca
Musca putris

description: Musca putris [spec. nov.]
M. antennis setariis subpilosa atra, alarum costa nigra oculis ferrugineis.
Fn. svec. 1110.
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 597, DOI: 10.5962/bhl.title.542, http://zenodo.org/record/3922206
title: Подвижной состав железных дорог. Прогнозирование ресурса колес
title: Учебное пособие для СПО
titleType: Subtitle
Creators: name: Воробьев А.А.
Publisher: name: Профобразование, Ай Пи Ар Медиа
Year: 2020

description: Учебное пособие посвящено вопросам прогнозирования ресурса колес железнодорожного подвижного состава. Представлены показатели работы железнодорожного транспорта, статистические данные по повреждаемости колесных пар вагонов эксплуатации, аналитический обзор данных по изнашиванию колес подвижного состава, изнашивание в системе «колесо — рельс» и его моделирование, расчет напряженно-деформированного состояния колесной пары грузового вагона. Подготовлено в соответствии с Федеральным государственным образовательным стандартом среднего профессионального образования. Издание будет полезно при изучении дисциплин «Технические средства», «Эксплуатация и техническое обслуживание подвижного состава» для студентов специальностей 23.02.01 «Организация перевозок и управление на транспорте (железнодорожный транспорт)», 23.02.06 «Техническая эксплуатация подвижного состава железных дорог», а также может представлять интерес для научных и инженерно-технических сотрудников предприятий и научно-исследовательских организаций, работающих в области проектирования и эксплуатации подвижного состава.
A Hubble Space Telescope Survey for Resolved Companions of Planetary-Nebula Nuclei
Creators: name: Ciardullo, Robin
name: Bond, Howard E.
name: Sipior, Michael S.
name: Fullton, Laura K.
name: Zhang, C. -Y.
name: Schaefer, Karen G.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We report results of an HST "snapshot" survey aimed at finding resolved binary companions of the central stars of Galactic planetary nebulae (PNe). Using WF/PC and WFPC2, we searched the fields of 113 PNe for stars whose close proximity to the central star suggests a physical association. We find 10 binary nuclei that are very likely to be physically associated, and another six that are possible binary associations. By correcting for interstellar extinction and placing the central stars' companions on the main sequence, we derive distances to the objects, and thereby significantly increase the number of PNe with reliable distances. Comparison of our derived distances with those obtained from various statistical methods shows that all of the latter have systematically overestimated the distances, by factors ranging up to a factor of two or more. We show that this error is most likely due to the fact that the properties of our PNe with binary nuclei are systematically different from those of PNe used heretofore to calibrate statistical methods. Specifically, our PNe tend to have lower surface brightnesses at the same physical radius than the traditional calibration objects. This difference may arise from a selection effect: the PNe in our survey are typically nearby, old nebulae, whereas most of the objects that calibrate statistical techniques are low-latitude, high-surface-brightness, and more distant nebulae. As a result, the statistical methods that seem to work well with samples of distant PNe, e.g., those in the Galactic bulge or external galaxies, may not be applicable to the more diverse population of local PNe.
description: 37 text pages, 17 table pages, 9 figures. Accepted by Astronomical Journal for June 1999 issue
Predictability and prefab status: The case of adjective + noun sequences in English
Creators: name: Bybee, Joan
name: De Souza, Ricardo Napoleão
Publisher: name: Zenodo
Year: 2021

description: The main arguments of the chapter are that frequency or predictability effects are most appropriately applied within constructions, and that prefab status can lead to phonetic effects independently of frequency. The analysis uses tokens of adjective-noun sequences taken from conversational corpora. Study 1 applies diagnostics for conventionalization to establish prefab vs. free combination status in 239 bigrams. As expected from previous research, the criterion of non-compositional meaning gives clear results, while the criterion of fixedness runs into difficulties, especially as clusters of related prefabs are revealed. Study 2 examines the effect of prefab status vs. the effect of bigram frequency on the duration of the vowel in the adjective. Both prefab status and high bigram frequency lead to a shorter vowel, though the effect is not statistically significant.
Musca putris subsp. casei Linnaeus, 1758, subspec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1758
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Diptera
Anthomyiidae
Musca
Musca putris
Musca putris subsp. casei

description: Musca putris subsp. casei [subspec. nov.]
Frisch. ins. 1. t. 7.
Habitat? in Fimetis,? in Caseo.
Hae tres species adeo affines, ut difficulter distingvantur.
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 597, DOI: 10.5962/bhl.title.542, http://zenodo.org/record/3922206
Quantum Interference of Coulomb Interaction and Disorder: Phase Shift of Friedel Oscillations and an Instability of the Fermi Sea
Creators: name: Kroha, Johann
name: Huck, Andrea
name: Kopp, Thilo
Publisher: name: arXiv
Year: 1994
Subjects: subject: Condensed Matter (cond-mat)
subject: FOS: Physical sciences

description: We investigate the influence of interference between Coulomb interaction and impurity scattering on the static electronic response $χ(0,q)$ in disordered metals to leading order in the effective Coulomb interaction. When the transport relaxation time $τ_{tr}$ is much shorter than the quasiparticle life time, we find a $\mbox{sgn}(2p_F-q)/\sqrt{|2p_F-q|}$ divergence of the polarization function at the Fermi surface ($q=2p_F$). It causes a phase shift of the Friedel oscillations as well as an enhancement of their amplitude. Our results are consistent with experiments and may be relevant for understanding the stability of the amorphous state of certain alloys against crystallization.
description: 11 pages, 4 PostScript figures appended as a self-extracting tar archive; includes output instructions
Additional file 3: of NAL8 encodes a prohibitin that contributes to leaf and spikelet development by regulating mitochondria and chloroplasts stability in rice
Creators: name: Chen, Ke
name: Guo, Tao
name: Li, Xin-Min
name: Yang, Yi-Bing
name: Dong, Nai-Qian
name: Shi, Chuan-Lin
name: Ye, Wang-Wei
name: Shan, Jun-Xiang
name: Lin, Hong-Xuan
Publisher: name: figshare
Year: 2019
Subjects: subject: Cell Biology
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Evolutionary Biology
subject: Ecology
subject: Developmental Biology
subject: Infectious Diseases
subject: FOS: Health sciences
subject: Plant Biology

description: Figure S3. Phylogenetic analysis of rice NAL8 and related proteins from plants, animals, and one species of insect. The species names are shown at the ends of the branches. The phylogenetic tree was constructed using the Neighbor-Joining tree method as implemented in MEGA7.0 and embellished with iTOL ( http://itol.embl.de/ ). The numbers shown on each branch indicate protein substitution rate. The NAL8 homologous proteins are highly consistent with the species evolution relationship. (PDF 117 kb)
Cascading collocations: Collocades as correlates of formulaic language
Creators: name: Forsyth, Richard
Publisher: name: Zenodo
Year: 2021
Subjects: collocades
corpus
driven research
formulaic language
linguistic statistics
multi
word units
phraseology

description: This chapter focuses on a technique for detecting, measuring and displaying traces
 of formulaic language. For this purpose, a suite of computational procedures has
 been developed in order to quantify the degree to which individual texts and text
 types incorporate inflexible sequences of words. This development is predicated on
 the assumption that, even if we have no precise definition of formulaic language,
 it is widely accepted that it is characterized by repetition of fixed sequences. The
 method involves compiling a formulexicon from a corpus of two or more text types
 and then using coverage by elements of that formulexicon as an index of the degree
 to which a text, possibly absent from the training corpus, is pervaded by formulaic
 sequences. The problem of deciding what lengths of n-grams are warranted by the
 data is dealt with by the simple expedient of binarizing coverage counts by n-grams
 of various lengths. Trials on a variety of text types show that this allows collocades
 – cascades of collocations, whose lengths are not pre-determined – to emerge from
 the data. Here the term collocation is used in its broader sense, as in “collocations are
 co-occurrences of words” (Gries 2009: 14). Software in Python 3 that implements
 this approach is available online under a Creative Commons licence. Examples of
 applying these procedures to a number of corpora illustrate some of the uses of
 this approach.
Detailed Structure of a CDW in a Quenched Random Field
Creators: name: Brock, J. D.
name: Finnefrock, A. C.
name: Ringland, K. L.
name: Sweetland, E.
Publisher: name: arXiv
Year: 1994
Subjects: subject: Condensed Matter (cond-mat)
subject: FOS: Physical sciences

description: Using high resolution x-ray scattering, we have measured the structure of the Q_1 CDW in Ta-doped NbSe_3. Detailed line shape analysis of the data demonstrates that two length scales are required to describe the phase-phase correlation function. Phase fluctuations with wavelengths less than a new length scale $a$ are suppressed and this $a$ is identified with the amplitude coherence length. We find that xi_a* = 34.4 \pm 10.3 angstroms. Implications for the physical mechanisms responsible for pinning are discussed.
description: revtex 3.0, 3 postscript uuencoded figures
Additional file 1: of Comparison of crystalloid resuscitation fluids for treatment of acute brain injury: a clinical and pre-clinical systematic review and network meta-analysis protocol
Creators: name: Thompson, Mary
name: Lauralyn McIntyre
name: Hutton, Brian
name: Tran, Alexandre
name: Wolfe, Dianna
name: Hutchison, Jamie
name: Fergusson, Dean
name: Turgeon, Alexis
name: English, Shane
Publisher: name: figshare
Year: 2018
Subjects: subject: Medicine
subject: Molecular Biology
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: Developmental Biology
subject: Hematology

description: PRISMA-P checklist. (DOCX 18 kb)
Diffusion and scaling in escapes from two-degree-of-freedom Hamiltonian systems
Creators: name: Kandrup, Henry E.
name: Siopis, Christos
name: Contopoulos, George
name: Dvorak, Rudolf
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: This paper summarises an investigation of the statistical properties of orbits escaping from three different two-degree-of-freedom Hamiltonian systems which exhibit global stochasticity. Each H=H_{0}+eH', with H_{0} integrable and eH' a nonintegrable correction, not necessarily small. For e below a critical e_{0} escapes are impossible energetically. For somewhat higher values, escape is allowed energetically but many orbits never escape and the escape probability P for a generic orbit ensemble decays exponentially. At or near a critical e_{1}>e_{0}, there is an abrupt qualitative change in behaviour. Above e_{1}, P typically exhibits (1) a rapid evolution towards a nonzero P_{0}(e) followed by (2) a much slower subsequent decay towards zero which, in at least one case, is well fit by a power law P=const x t^{m}, with m=0.35-0.40. In all three cases, P_{0} and the time T required to converge towards P_{0} scales in e-e_{1}, i.e., P_{0}=const x (e-e_{1})^{a} and T=const x (e-e_{1})^{b}, and T also scales in the size r of the region sampled for initial conditions, i.e., T=const x r^{-d}. To within statistical uncertainties, the best fit values of the critical exponents are the same for all three potentials, namely: a=0.5, b=0.4, and d=0.1, and satisfy a-b-d=0. The transitional behaviour observed near e_{1} is attributed to the breakdown of some especially significant KAM tori or cantori. The power law behaviour at late times is interpreted as reflecting intrinsic diffusion of chaotic orbits through cantori surrounding islands of regular orbits.
description: 15 pages, including 8 figures (figure 5 has 6 parts), to appear in: Chaos
Musca frit Linnaeus, 1758, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1758
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Diptera
Anthomyiidae
Musca
Musca frit

description: Musca frit [spec. nov.]
M. antennis setariis pilosa nigra, halteribus plantis posticis abdomineque virescenti-pallidis.
Linn. act Stockh. 1750. p. 128.
Habitat in glumis Hordei, decimum quodque granum Hordeaceum apud nos destruens.
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 598, DOI: 10.5962/bhl.title.542, http://zenodo.org/record/3922206
Compatibility of quantum measurements and inclusion constants for the matrix jewel
Creators: name: Bluhm, Andreas
name: Nechita, Ion
Publisher: name: arXiv
Year: 2018
Subjects: subject: Quantum Physics (quant-ph)
subject: Mathematical Physics (math-ph)
subject: Operator Algebras (math.OA)
subject: FOS: Physical sciences
subject: FOS: Mathematics

description: In this work, we establish the connection between the study of free spectrahedra and the compatibility of quantum measurements with an arbitrary number of outcomes. This generalizes previous results by the authors for measurements with two outcomes. Free spectrahedra arise from matricial relaxations of linear matrix inequalities. A particular free spectrahedron which we define in this work is the matrix jewel. We find that the compatibility of arbitrary measurements corresponds to the inclusion of the matrix jewel into a free spectrahedron defined by the effect operators of the measurements under study. We subsequently use this connection to bound the set of (asymmetric) inclusion constants for the matrix jewel using results from quantum information theory and symmetrization. The latter translate to new lower bounds on the compatibility of quantum measurements. Among the techniques we employ are approximate quantum cloning and mutually unbiased bases.
description: v5: section 3.3 has been expanded significantly to incorporate the generalization of the Cartesian product and the direct sum to matrix convex sets. Many other minor modifications. Closed to the published version
Additional file 4: of Identification of heat-tolerance QTLs and high-temperature stress-responsive genes through conventional QTL mapping, QTL-seq and RNA-seq in tomato
Creators: name: Wen, Junqin
name: Jiang, Fangling
name: Weng, Yiqun
name: Sun, Mintao
name: Shi, Xiaopu
name: Zhou, Yanzhao
name: Yu, Lu
name: Wu, Zhen
Publisher: name: figshare
Year: 2019
Subjects: subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Evolutionary Biology
subject: Biological Sciences not elsewhere classified
subject: Marine Biology
subject: Plant Biology

description: Table S4. The statistics of sequencing data and genome comparison with the reference SL 2.50 in RNA-seq. (DOCX 16 kb)
Update of the global electroweak fit and constraints on two-Higgs-doublet models
Creators: name: Haller, Johannes
name: Hoecker, Andreas
name: Kogler, Roman
name: Mönig, Klaus
name: Peiffer, Thomas
name: Stelzer, Jörg
Publisher: name: arXiv
Year: 2018
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: High Energy Physics - Experiment (hep-ex)
subject: FOS: Physical sciences

description: We present an update of the global fit of the Standard Model electroweak sector to latest experimental results. We include new kinematic top quark and $W$ boson mass measurements from the LHC, a $\sin^2θ^{\ell}_{\mathrm{eff}}$ result from the Tevatron, and a new evaluation of the hadronic contribution to $α(M_Z^2)$. We present tests of the internal consistency of the electroweak Standard Model and updated numerical predictions of key observables. The electroweak data combined with measurements of the Higgs boson coupling strengths and flavour physics observables are used to constrain parameters of two-Higgs-doublet models.
description: 33 pages, 13 figures, submitted to EPJC
Exploring the valency of collocational chains
Creators: name: Pęzik, Piotr
Publisher: name: Zenodo
Year: 2021

description: Whereas the prefabricated status of idioms or restricted collocations is relatively self-evident in their context of use, the “underlying rigidity” (Sinclair 1991: 110) of other types of phraseological units may only become evident through large-scale analyses of reference corpora. This chapter focuses on the identification of subtle lexico-grammatical petrification of multiword units in dependency-annotated corpora. More specifically, it investigates restrictions on the valency of binary collocations and their tendency to be regularly subsumed by larger collocational chains. For example, the binary collocation deep breath is almost invariably a direct object of a small set of verbs: take, draw, let out. This restriction can be contrasted with collocational chains in which other adjectival collocations of breath (e.g. bad breath) have a wider range of syntactic roles determined mainly by the potential valency of their head noun (i.e. its propensity to function as subject, object etc.). Apart from discussing examples of such constructions from Polish and English corpus data, the chapter also attempts to show how lexico-syntactic properties of multiword units can be systematically accounted for and explored using a dependency-based approach to phraseology extraction.
title: ADCO, Ordre cistercien et abbaye de Cîteaux : comptes pour l'ordre (1337-1347), comptes du boursier (1377-1402) (11 H 1160), f. 00290
Creators: name: de la Côte-d'Or, Archives départementales
name: Archives Départementales De La Côte-D'Or
name: Petot, Frédérique
name: Projet CBMA
name: CBMA/CG21/F.PETOT/2017
name: Petot, Frédéric
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2020
Subjects: subject: Corpus Burgundiae Medii Aevi
subject: Chartes de la Bourgogne du Moyen Âge
subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris
subject: comptes

description: Ordre cistercien et abbaye de Cîteaux : comptes pour l'ordre (1337-1347), comptes du boursier (1377-1402), Archives départementales de la Côte-d'Or, (11 H 1160). Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Ordre cistercien et abbaye de Cîteaux : comptes pour l'ordre (1337-1347), comptes du boursier (1377-1402), Archives départementales de la Côte-d'Or, (11 H 1160), f. 00290, 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
Coherent lepton pair production in hadronic heavy ion collisions
Creators: name: Zha, W.
name: Ruan, L.
name: Tang, Z.
name: Xu, Z.
name: Yang, S.
Publisher: name: arXiv
Year: 2018
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: Recently, significant enhancements of $e^{+} e^{-}$ pair production at very low transverse momentum ($p_{T} < 0.15$ GeV/c) were observed by the STAR collaboration in peripheral hadronic A+A collisions. This excesses can not be described by the QGP thermal radiation and $ρ$ in-medium broadening calculations. This is a sign of coherent photon-photon interactions, which were conventionally studied only in ultra-peripheral collisions. In this article, we present calculations of lepton pair ($e^{+}e^{-}$ and $μ^{+}μ^{-}$) production from coherent photon-photon interactions in hadronic A+A collisions at RHIC and LHC energies within the STAR and ALICE acceptance.
The Galactic Center Isolated Nonthermal Filaments as Analogs of Cometary Plasma Tails
Creators: name: Shore, Steven N.
name: LaRosa, T. N.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We propose a model for the origin of the isolated nonthermal filaments observed at the Galactic center based on an analogy to cometary plasma tails. We invoke the interaction between a large scale magnetized galactic wind and embedded molecular clouds. As the advected wind magnetic field encounters a dense molecular cloud, it is impeded and drapes around the cloud, ultimately forming a current sheet in the wake. This draped field is further stretched by the wind flow into a long, thin filament whose aspect ratio is determined by the balance between the dynamical wind and amplified magnetic field pressures. The key feature of this cometary model is that the filaments are dynamic configurations, and not static structures. As such, they are local amplifications of an otherwise weak field and not directly connected to any static global field. The derived field strengths for the wind and wake are consistent with observational estimates. Finally, the observed synchrotron emission is naturally explained by the acceleration of electrons to high energy by plasma and MHD turbulence generated in the cloud wake.
description: Uses AAS aasms4.sty macros. ApJ (in press, vol. 521, 20 Aug)
Paths to formulaicity: How do L2 speakers internalise new formulaic material?
Creators: name: Cutler, Stephen F.
Publisher: name: Zenodo
Year: 2021

description: How are new formulaic expressions acquired and stored by L2 learners? Defining formulaicity with respect to the individual speaker’s storage and processing of a given expression as a single holistic unit (Myles & Cordier 2017; Wray 2002), two potential routes are explored: the “fusion” over time of individual words and “holistic acquisition”, where an expression is internalised as a single unit from the start. Two studies exploring the route to acquisition are reported. L2 speakers are presented with novel target expressions to memorise, and their ease of recall, accuracy and fluency over time is monitored. These delivery features are used in combination to indicate particular stages of acquisition that may be associated with each route. Study 1 contrasts analytical and holistic methods for introducing the targets. Study 2 explores methods for determining the holisticity and processing automaticity of the target expressions in the learners’ output. Drawing on the results of these, a model for the acquisition and storage of formulaic expressions based on the “superlemma” model of Sprenger et al. (2006) is presented and discussed in relation to fusion and holistic acquisition.
The Unified Limit: The Ultimate Constraint on Energy-Density in the Universe
Creators: name: Shreenan-Dyck, Chris
Publisher: name: figshare
Year: 2025
Subjects: classificationCode: 490204
subject: Mathematical aspects of general relativity

description: The Unified Limit (U) is a fundamental concept within the Mass-Energy Gravity (MEG) model, representing the upper bound on energy density that governs mass-energy interactions, gravitational effects, and cosmic expansion. This paper explores how U serves as the ultimate energy threshold, unifying the speed of light limit and black hole energy density under a single principle.

By constraining energy-density variations, U prevents singularities, maintains cosmic stability, and naturally explains phenomena such as gravitational lensing, galaxy rotation curves, and large-scale structure formation without requiring dark matter or dark energy. The implications of U extend beyond gravity, offering a framework that integrates inertia, entropy, and energy redistribution into a coherent, testable model.

This paper presents the mathematical formalism of U, discusses its role in cosmology and astrophysics, and outlines observational tests to distinguish MEG’s predictions from those of General Relativity.
Motion and collision of particles in rotating linear dilaton black hole
Creators: name: González, P. A.
name: Olivares, Marco
name: Papantonopoulos, Eleftherios
name: Vásquez, Yerko
Publisher: name: arXiv
Year: 2018
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We study the motion of particles in the background of a four-dimensional linear dilaton black hole. We solve analytically the equations of motion of the test particles and we describe their motion. We show that the dilaton black hole acts as a particle accelerator by analyzing the energy in the center of mass (CM) frame of two colliding particles in the vicinity of its horizon. In particular we find that there is a critical value of the angular momentum, which depends on the string coupling, and a particle with this critical angular momentum can reach the inner horizon with an arbitrarily high CM energy. This is known as the Bañados, Silk and West (BSW) process. We also show that the motion and collisions of particles have a similar behavior to the three-dimensional BTZ black hole. In fact, the photons can plunge into the horizon or escape to infinity, and they can not be deflected, while for massive particles there are no confined orbits of first kind, like planetary or circular orbits.
description: arXiv admin note: text overlap with arXiv:hep-th/0208225 by other authors
Additional file 4: of NAL8 encodes a prohibitin that contributes to leaf and spikelet development by regulating mitochondria and chloroplasts stability in rice
Creators: name: Chen, Ke
name: Guo, Tao
name: Li, Xin-Min
name: Yang, Yi-Bing
name: Dong, Nai-Qian
name: Shi, Chuan-Lin
name: Ye, Wang-Wei
name: Shan, Jun-Xiang
name: Lin, Hong-Xuan
Publisher: name: figshare
Year: 2019
Subjects: subject: Cell Biology
subject: Molecular Biology
subject: Biotechnology
subject: Ecology
subject: FOS: Biological sciences
subject: Developmental Biology
subject: Infectious Diseases
subject: FOS: Health sciences
subject: Plant Biology

description: Figure S4. Comparisons and statistical analysis of TQ, the nal8 mutant, and NAL8 complementation transgenic rice lines. (A) Spikelet phenotypes among TQ, nal8 and the transgenic complementation lines NAL8com#1 and #2. Scale bar = 5 cm. (B) Mature grains of TQ, nal8 and the complementation lines NAL8com#1 and #2. Scale bar = 2 mm. (C-H) Statistical analyses of average grain width (n = 20 plants) (C), average grain length (n = 20 plants) (D), average thousand seed weight (n = 20 plants) (E), average plant height (n = 20 plants) (F), average spikelet number (n = 20 plants) (G) and average flag leaf length (n = 20 plants) (H) in TQ, nal8 and the transgenic complementation lines NAL8com#1 and #2. Values in C-H are given as the mean ± SD. *P < 0.05; **P < 0.01 compared with the TQ control using Student’s t-test. (PDF 80 kb)
Kinematic Disturbances in Optical Rotation Curves among 89 Virgo Disk Galaxies
Creators: name: Rubin, Vera C.
name: Waterman, Andrew H.
name: Kenney, Jeffrey D. P.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: For 89 galaxies, mostly spirals, in the Virgo cluster region, we have obtained optical long-slit major axis spectra of the ionized gas. We find: (1) One-half of the Virgo galaxies we observed have regular rotation patterns, while the other 50% exhibit kinematic disturbances ranging from mild to major. Velocity complexities are generally consistent with those resulting from tidal encounters or accretion events. Since kinematic disturbances are expected to fade within ~10^9 years, many Virgo galaxies have experienced several significant kinematic disturbances during their lifetimes. (2) A few Virgo galaxies have ionized gas of limited extent, with velocities exceptionally low for their luminosities. In these galaxies the gas must be not rotationally supported. (3) There is a remarkable difference in the distribution of galaxy systemic velocity for galaxies with Regular rotation curves and galaxies with Disturbed rotation curves. Galaxies with regular rotation patterns show a flat distribution with systemic velocity, while galaxies with disturbed kinematics have a Gaussian distribution very similar to that for the elliptical galaxies in Virgo. This suggests that spirals with disturbed kinematics are preferentially on radial orbits, which bring them to the cluster core, where tidal interactions are strong and/or more common. These interactions may alter the morphology of the galaxy, and may also play a role in driving the Virgo cluster toward dynamical equilibrium.
description: to be published in the Astronomical Journal, 37 pages, 19 .ps figures, 4 .ps tables
Hour time-scale QPOs in the X-ray and radio emission of LS I +61$^{\circ}$303
Creators: name: Nösel, Silvia
name: Sharma, Richa
name: Massi, Maria
name: Cimò, Giuseppe
name: Chernyakova, Masha
Publisher: name: arXiv
Year: 2018
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: LS I +61$^{\circ}$303 is an X-ray binary with a radio outburst every ~27 days. Previous studies of the stellar system revealed radio microflares superimposed on the large radio outburst. We present here new radio observations of LS I +61$^{\circ}$303 at 2.2 GHz with the Westerbork Synthesis Radio Telescope (WSRT). Using various timing analysis methods we find significant Quasi-Periodic Oscillations (QPOs) of 55 minutes stable over the duration of 4 days. We also use archival data obtained from the Suzaku satellite at X-ray wavelengths. We report here for the first time significant X-ray QPOs of about 2 hours present over the time span of 21 hours. We compare our results with the previously reported QPO observations and we conclude that the QPOs seem to be associated with the radio outburst, independent of the amplitude of the outburst. Finally, the different QPO time-scales are discussed in the context of magnetic reconnection.
Topological Defects in the Abrikosov Lattice of Vortices in Type-II Superconductors
Creators: name: Dodgson, M. J. W.
name: Moore, M. A.
Publisher: name: arXiv
Year: 1994
Subjects: subject: Condensed Matter (cond-mat)
subject: FOS: Physical sciences

description: The free energy costs for various defects within an Abrikosov lattice of vortices are calculated using the lowest Landau level approximation (LLL). Defect solutions with boundary conditions for lines to meet at a point (crossing defect) and for lines to twist around each other (braid defect) are sought for 2, 3, 6, and 12 lines. Many results have been unexpected, including the nonexistence of a stable two- or three-line braid. This, and the high energy cost found for a six-line braid lead us to propose that the equilibrium vortex state is not entangled below the irreversibility line of the high-$T_c$ superconductors or in a large part of the vortex-liquid phase above this line. Also, the solution for an infinite straight screw dislocation is found, and used to give a limiting form for the free energy cost of very large braids. This depends on the area enclosed by the braid as well as its perimeter length.
description: 30 pages, 17 Encapsulated PostScript figures, uses Revtex (with epsf)
Radio Emission from Supernovae
Creators: name: Katz, J. I.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: I consider radio emission from the remarkable SN1998bw. Ni-56 and Co-56 decays produce a gamma-ray flux whose Compton-scattered electrons naturally explain the observed mildly relativistic exapnsion of the radio source and its double- peaked history. Such models require a surrounding plasma, perhaps produced by the supernova progenitor, whose interaction with the nonrelativistic debris may account for the observed X-ray source. The radio spectrum appears to be self- absorbed. This interpretation determines the brightness temperature, and hence the energy of the radiating electrons, implying a surprisingly large magnetic field. Attempts to avoid this conclusion by interpreting the spectrum as the result of inverse bremsstrahlung absorption do not lead to significantly lower fields. The large inferred field may have several explanations: radiation from a central pulsar, a turbulent hydrodynamic dynamo or an aspherical Compton current, but a frozen-in field from the supernova progenitor is not adequate. The electron-ion and particle-field equipartition problems are discussed. Compton electrons also explain the inferred expansion speed of SN1987A's spots.
description: 11 pp, aas latex, no figures. Application to new SN1987A data (astro-ph/9904109) added
Red and Blue Shifted Broad Lines in Luminous Quasars
Creators: name: McIntosh, D. H.
name: Rix, H. -W.
name: Rieke, M. J.
name: Foltz, C. B.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We have observed a sample of 22 luminous quasars, in the range 2.03.1 objects using NIR spectroscopy.
description: 12 pages, Latex, 2 figures, 2 tables, Accepted for publication in ApJ Letters
Musca leprae Linnaeus, 1758, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1758
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Diptera
Anthomyiidae
Musca
Musca leprae

description: Musca leprae [spec. nov.]
M. antennis setariis atra nitens, antennis pedibusque albis, oculis rufo inauratis.
Habitat in Elephantiasi Nigritarum Americae. Rolander.
Corpus pediculo minus. Abdomen subtus & basi album. Denticulus utrinque ad basin proboscidis.
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 598, DOI: 10.5962/bhl.title.542, http://zenodo.org/record/3922206
HI and OH absorption at z=0.89
Creators: name: Chengalur, Jayaram N.
name: de Bruyn, A. G.
name: Narasimha, D.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We report on WSRT observations of HI and OH absorption at z=0.885 towards the radio lens PKS 1830-21, mm wave transitions of several molecular species have already been observed at this redshift. At mm wavelengths the source structure is dominated by two extremely compact components, the northeast (NE) and southwest (SW) components. At lower frequencies the continuum emission is much more extended and there is also a broad Einstein ring connecting the NE and SW components. This means that the HI and OH spectra sample a much larger region of the absorber than the mm wave spectra. The HI spectrum that we obtain is asymmetric, with a peak at -147 km/s with respect to the main molecular line redshift of z=0.88582. Weak mm wave molecular absorption has also been detected towards the NE component at this same velocity. The HI absorption, however, covers a total velocity width of 300 km/sec, i.e. including velocities well to the red of molecular features suggesting that it is spatially widespread. In OH we detect both the 1667 and the 1665 MHz transitions. The OH spectrum has a velocity width comparable to that of the HI spectrum, suggesting that it too is widespread in the absorber. The lack of a prominent HI peak in the spectrum at the velocity corresponding to the SW component, suggests that the galaxy responsible for the absorption at z=0.885 has a central molecular disk many kpc in size, and that HI is deficient in this central region. Our observations are sensitive to the large scale kinematics of the absorber, and to first order the implied dynamical mass is consistent with the lens models of Nair et. al. (1993).
description: 4 pages, 3 figures