cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
ПРАВОВАЯ КУЛЬТУРА И ОСОБЕННОСТИ ЕЕ ФОРМИРОВАНИЯ В РОССИИ НА РУБЕЖЕ XIX И XX ВЕКОВ
Creators: name: Владимир Владимирович Сушков
Publisher: name: Революция и эволюция: модели развития в науке, культуре, обществе
Year: 2019
Subjects: право
нравственность
естественное право
позитивное право
право-вой нигилизм
правовая культура
свобода личности
нравственный поступок

description: В данной статье рассмотрены особенности формирования правовой культуры в Рос-сии после проведения ряда либеральных реформ второй половины XIX века. Изучение мораль-ных оснований права нашей страны является актуальным в связи с необходимостью динамич-ного развития общества и избегания социальных конфликтов. Правовые ценности всегда опре-деляют своеобразие правовой культуры того или иного государства, логика развития которой складывается в правовую традицию и объясняет сложности реализации современных правовых концепций. Социальное и индивидуальное измерение приобретают вопросы справедливости, свободы, долга, которые становятся центральными в политических и идеологических дискус-сиях, определяющих развитие правовой культуры России. С этой целью изучены и проанали-зированы работы философов-правоведов, которые затрагивали вопросы соотношения права и нравственности, различие и сходство естественного и позитивного права, правовой нигилизм и его влияние на настроения общества того периода. Сделана попытка проследить своеобразие эволюции правовой культуры России на рубеже XIX и XX веков, вычленить идеи, носящие эволюционный характер, и идеи, носящие революционный характер, совокупность которых определила вторичность концепции прав личности по отношению к государственному и соци-альному праву.
Additional file 10 of Phylogenetic signal from rearrangements in 18 Anopheles species by joint scaffolding extant and ancestral genomes
Creators: name: Anselmetti, Yoann
name: Duchemin, Wandrille
name: Tannier, Eric
name: Chauve, Cedric
name: SĂ¨Verine BĂŠrard
Publisher: name: figshare
Year: 2018
Subjects: subject: Space Science
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Evolutionary Biology
subject: 59999 Environmental Sciences not elsewhere classified
subject: FOS: Earth and related environmental sciences
subject: Sociology
subject: FOS: Sociology
subject: 69999 Biological Sciences not elsewhere classified
subject: 80699 Information Systems not elsewhere classified
subject: FOS: Computer and information sciences
subject: Marine Biology
subject: 110309 Infectious Diseases
subject: FOS: Health sciences

description: Figure S9. Subfigures zooming of Additional fileÂ 9: Figure S8 to compare precision and recall statistics between ADseq and AD. Upper graphs: zoom of results with 50% of reads. Lower graphs: results with all reads. (PDF 154 kb)
The H alpha Galaxy Survey I. The galaxy sample, H alpha narrow-band observations and star formation parameters for 334 galaxies
Creators: name: James, P. A.
name: Shane, N. S.
name: Beckman, J. E.
name: Cardwell, A.
name: Collins, C. A.
name: Etherton, J.
name: de Jong, R. S.
name: Fathi, K.
name: Knapen, J. H.
name: Peletier, R. F.
name: Percival, S. M.
name: Pollacco, D. L.
name: Seigar, M. S.
name: Stedman, S.
name: Steele, I. A.
Publisher: name: arXiv
Year: 2003
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We discuss the selection and observations of a large sample of nearby galaxies, which we are using to quantify the star formation activity in the local Universe. The sample consists of 334 galaxies across all Hubble types from S0/a to Im and with recession velocities of between 0 and 3000 km/s. The basic data for each galaxy are narrow band H alpha plus [NII] and R-band imaging, from which we derive star formation rates, H alpha plus [NII] equivalent widths and surface brightnesses, and R-band total magnitudes. A strong correlation is found between total star formation rate and Hubble type, with the strongest star formation in isolated galaxies occurring in Sc and Sbc types. More surprisingly, no significant trend is found between H alpha plus [NII] equivalent width and galaxy R-band luminosity. More detailed analyses of the data set presented here will be described in subsequent papers.
description: 28 pages, 19 figures. Accepted for publication in Astronomy and Astrophysics. FITS-format R-band and H alpha plus [NII] images for all galaxies, and a version of the paper with full resolution figures, are available at http://www.astro.livjm.ac.uk/HaGS/
Humococcus mackenziei Ezzat 1959
Creators: name: Evans, Gregory A.
name: Abd-Rabou, Shaaban
Publisher: name: Zenodo
Year: 2023
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hemiptera
Pseudococcidae
Humococcus
Humococcus mackenziei

description: Humococcus mackenziei Ezzat, 1959
(Figure 20, after Ezzat 1959b)
 Taxonomy. Humococcus mackenziei Ezzat 1959b: 409. Type data. EGYPT: Alexandria, El-Max, on Zygophyllum album.
 Hosts in Egypt. Sarcocornia cellulose, Zygophyllum album, Zygophyllum sp. (Ezzat 1959b).
 Distribution in Egypt. Alexandria, El-Max (Ezzat 1959b).
 Remarks. This species has only been found in Egypt on these hosts. Ezzat (1959b) provided a description and illustration of the species.
description: Published as part of Evans, Gregory A. & Abd-Rabou, Shaaban, 2023, The mealybugs (Hemiptera: Coccoidea: Pseudococcidae) of Egypt, pp. 1-83 in Insecta Mundi 2023 (999) on page 19, DOI: 10.5281/zenodo.10832115
A tight-binding investigation of biaxial strain induced topological phase transition in GeCH$_3$
Creators: name: Rezaei, Mohsen
name: Sisakht, Esmaeil Taghizadeh
name: Fazileh, Farhad
name: Aslani, Zahra
name: Peeters, F. M.
Publisher: name: arXiv
Year: 2017
Subjects: subject: Materials Science (cond-mat.mtrl-sci)
subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: FOS: Physical sciences

description: We propose a tight-binding (TB) model, that includes spin-orbit coupling (SOC), to describe the electronic properties of methyl-substituted germanane (GeCH$_3$). This model gives an electronic spectrum in agreement with first principle results close to the Fermi level. Using the $\mathbb{Z}_2$ formalism, we show that a topological phase transition from a normal insulator (NI) to a quantum spin Hall (QSH) phase occurs at 11.6\% biaxial tensile strain. The sensitivity of the electronic properties of this system on strain, in particular its transition to the topological insulating phase, makes it very attractive for applications in strain sensors and other microelectronic applications.
description: 8 pages, 10 figures
Massive Klein--Gordon equation from a BEC-based analogue spacetime
Creators: name: Visser, Matt
name: Weinfurtner, Silke
Publisher: name: arXiv
Year: 2005
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: We extend the "analogue spacetime" programme by investigating a condensed-matter system that is in principle capable of simulating the massive Klein--Gordon equation in curved spacetime. Since many elementary particles have mass, this is an essential step in building realistic analogue models, and a first step towards simulating quantum gravity phenomenology. Specifically, we consider the class of two-component BECs subject to laser-induced transitions between the components. This system exhibits a complicated spectrum of normal mode excitations, which can be viewed as two interacting phonon modes that exhibit the phenomenon of "refringence". We study the conditions required to make these two phonon modes decouple. Once decoupled, the two distinct phonons generically couple to distinct effective spacetimes, representing a bi-metric model, with one of the modes acquiring a mass. In the eikonal limit the massive mode exhibits the dispersion relation of a massive relativistic particle: omega = sqrt[omega_0^2 + c^2 k^2], plus curved-space modifications. Furthermore, it is possible to tune the system so that both modes can be arranged to travel at the same speed, in which case the two phonon excitations couple to the same effective metric. From the analogue spacetime perspective this situation corresponds to the Einstein equivalence principle being satisfied.
description: V1: 10 pages; uses revtex4; V2: two references and brief comments added
Ricci tensor on smooth metric measure space with boundary
Creators: name: Han, Bang-Xian
Publisher: name: arXiv
Year: 2017
Subjects: subject: Metric Geometry (math.MG)
subject: Differential Geometry (math.DG)
subject: Functional Analysis (math.FA)
subject: FOS: Mathematics

description: The aim of this note is to study the measure-valued Ricci tensor on smooth metric measure space with boundary, which is a generalization of Bakry-Emery's modified Ricci tensor on weighted Riemannian manifold. As an application, we offer a new approach to study curvature-dimension condition of smooth metric measure space with boundary.
description: 7 pages
Bell State Preparation using Pulsed Non-Degenerate Two-Photon Entanglement
Creators: name: Kim, Yoon-Ho
name: Kulik, Sergei P.
name: Shih, Yanhua
Publisher: name: arXiv
Year: 2000
Subjects: subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: We report a novel Bell state preparation experiment. High-purity Bell states are prepared by using femtosecond pulse pumped \emph{nondegenerate} collinear spontaneous parametric down-conversion. The use of femtosecond pump pulse {\em does not} result in reduction of quantum interference visibility in our scheme in which post-selection of amplitudes and other traditional mechanisms, such as, using thin nonlinear crystals or narrow-band spectral filters are not used. Another distinct feature of this scheme is that the pump, the signal, and the idler wavelengths are all distinguishable, which is very useful for quantum communications.
description: 4 pages, submitted to PRL
LOFAR-Boötes: Properties of high- and low-excitation radio galaxies at $0.5 < z < 2.0$
Creators: name: Williams, W. L.
name: Rivera, G. Calistro
name: Best, P. N.
name: Hardcastle, M. J.
name: Röttgering, H. J. A.
name: Duncan, K. J.
name: de Gasperin, F.
name: Jarvis, M. J.
name: Miley, G. K.
name: Mahony, E. K.
name: Morabito, L. K.
name: Nisbet, D. M.
name: Prandoni, I.
name: Smith, D. J. B.
name: Tasse, C.
name: White, G. J.
Publisher: name: arXiv
Year: 2017
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: This paper presents a study of the redshift evolution of radio-loud active galactic nuclei (AGN) as a function of the properties of their galaxy hosts in the Boötes field. To achieve this we match low-frequency radio sources from deep $150$-MHz LOFAR observations to an $I$-band-selected catalogue of galaxies, for which we have derived photometric redshifts, stellar masses and rest-frame colours. We present spectral energy distribution (SED) fitting to determine the mid-infrared AGN contribution for the radio sources and use this information to classify them as High- versus Low-Excitation Radio Galaxies (HERGs and LERGs) or Star-Forming galaxies. Based on these classifications we construct luminosity functions for the separate redshift ranges going out to $z = 2$. From the matched radio-optical catalogues, we select a sub-sample of $624$ high power ($P_{150\mathrm{\,MHz}}>10^{25}$ W Hz$^{-1}$) radio sources between $0.5 \leq z < 2$. For this sample, we study the fraction of galaxies hosting HERGs and LERGs as a function of stellar mass and host galaxy colour. The fraction of HERGs increases with redshift, as does the fraction of sources in galaxies with lower stellar masses. We find that the fraction of galaxies that host LERGs is a strong function of stellar mass as it is in the local Universe. This, combined with the strong negative evolution of the LERG luminosity functions over this redshift range, is consistent with LERGs being fuelled by hot gas in quiescent galaxies.
description: 25 pages, 21 figures, accepted for publication in MNRAS
Additional file 2: of Predictive biomarkers for death and rehospitalization in comorbid frail elderly heart failure patients
Creators: name: Pacho, Cristina
name: Domingo, Mar
name: Núñez, Raquel
name: Lupón, Josep
name: Núñez, Julio
name: Barallat, Jaume
name: Moliner, Pedro
name: Antonio, Marta De
name: Santesmases, Javier
name: Cediel, Germán
name: Roura, Santiago
name: M. Pastor
name: Tor, Jordi
name: Bayes-Genis, Antoni
Publisher: name: figshare
Year: 2018
Subjects: subject: Medicine
subject: Pharmacology
subject: Biotechnology
subject: 19999 Mathematical Sciences not elsewhere classified
subject: FOS: Mathematics
subject: Developmental Biology
subject: 60506 Virology
subject: FOS: Biological sciences
subject: Computational Biology

description: Table S2. Cox regression analyses for 30-day rehospitalization. A competing risk strategy using the Gray method was adopted, considering death as the competing risk in both univariate and multivariate Cox regression analyses. (DOCX 27 kb)
Additional file 4 of An integrated study of Violae Herba (Viola philippica) and five adulterants by morphology, chemical compositions and chloroplast genomes: insights into its certified plant origin
Creators: name: Lu, Gengyu
name: Qiao, Juanjuan
name: Wang, Long
name: Liu, Hui
name: Wu, Gang
name: Zhu, Yan
name: Zhao, Yucheng
name: Xie, Guoyong
name: Qin, Minjian
Publisher: name: figshare
Year: 2022
Subjects: subject: Genetics
subject: FOS: Biological sciences

description: Additional file 4: Figure S1. The distribution schematic of the six Viola species. Figure S2. Leaf morphology of the 18 commercial VH for tentative identification. Figure S3. The HPLC chromatograms of the wild-collected samples of 6 Viola species. Figure S4. The total ion current chromatograms of six Viola species in negative and positive ion mode. Figure S5. The distribution of RNA editing sites. Figure S6. Codon numbers for each amino acid of the six Viola species.
Why do millisecond pulsars have weaker magnetic fields compared to ordinary pulsars?
Creators: name: Choudhuri, Arnab Rai
name: Konar, Sushan
Publisher: name: arXiv
Year: 2003
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Millisecond pulsars, with magnetic fields weaker by three to four orders compared to those of ordinary pulsars, are presumed to be neutron stars spun up by binary accretion. We expect the magnetic field to get screened by the accreted material. Our simulation of this screening mechanism shows, for the first time, that the field decreases by a purely geometric factor $\sin^{-7/2} θ_{\rm P,i}$ before freezing to an asymptotic value, where $ θ_{\rm P,i}$ is the initial angular width of the polar cap. If $ θ_{\rm P,i}$ lies in the range $5^o$--$10^o$, then the magnetic field diminution factor turns out to be $\sim 10^3$--$10^4$ in conformity with observational data.
description: 11 pages, 3 figures, submitted to Current Science
Maconellicoccus hirsutus
Creators: name: Evans, Gregory A.
name: Abd-Rabou, Shaaban
Publisher: name: Zenodo
Year: 2023
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hemiptera
Pseudococcidae
Maconellicoccus
Maconellicoccus hirsutus

description: Maconellicoccus hirsutus (Green, 1908)
(Figure 23, after Williams 2004)
 Taxonomy. Phenacoccus hirsutus Green 1908 a: 25. Type data. INDIA, on undetermined shrub; Hosny 1939: 2.
 Maconellicoccus hirsutus (Green); Hall 1926c; Ezzat 1958: 380, change of combination; Ezzat 1962d: 161.
 Host plants in Egypt. Acacia nilotica, Acalypha sp., Albizia lebbeck, Annona sp., Arachis hypogaea, Asparagus officinalis, Bauhinia sp., Bougainvillea sp., Cajanus cajan, Calostemma sp., Ceratonia siliqua, Chenopodium album, Cosmos sp., Dahlia sp., Ficus platyphylla, Glebionis coronaria, Grevillea robusta, Helianthus annuus, Hibiscus schizopetalus, Jacaranda mimosifolia, Opuntia sp., Psidium guajava, Robinia pseudoacacia, Tecoma sp., Vitis vinifera, Zea mays.
 Distribution in Egypt. Alexandria in 1924 (Hall 1921), Mattariah, Maadi, Bilbeis, El-Saff, Barrage (Hosny 1939).
 Remarks. This is a very polyphagous, cosmopolitan species. Hall (1921) first reported its presence in Egypt. Hosny (1939) reported a heavy infestation of this species on the roots of beans in Maadi and on Arachis hypogaea (peanuts) from Sharkieh.
description: Published as part of Evans, Gregory A. & Abd-Rabou, Shaaban, 2023, The mealybugs (Hemiptera: Coccoidea: Pseudococcidae) of Egypt, pp. 1-83 in Insecta Mundi 2023 (999) on page 20, DOI: 10.5281/zenodo.10832115
Mirococcus inermis
Creators: name: Evans, Gregory A.
name: Abd-Rabou, Shaaban
Publisher: name: Zenodo
Year: 2023
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hemiptera
Pseudococcidae
Mirococcus
Mirococcus inermis

description: Mirococcus inermis (Hall, 1925)
(Figure 24, after Ezzat 1965a)
 Taxonomy. Phenacoccus inermis Hall 1925: 7. Type data. EGYPT: Helwan, on roots of Zygophyllum simplex; Hosny 1939: 2.
 Aegyptococcus inermis (Hall); Ezzat 1965a: 163-167, change of combination.
 Hosts in Egypt. Cleome arabica, Cressa cretica, Frankenia pulverulenta, Polycarpaea repens, Zygophyllum simplex (Hall 1925).
 Distribution in Egypt. near Helwan in 1908 (Hall 1925), Alexandria, El-Max, Maadi, Helwan (Hosny 1939).
 Remarks. This is a polyphagous species recorded on 31 genera in 16 plant families, including some grasses; it is known from Europe and North Africa. In their discussion of the species, Mohammed et al. (1995) stated that Ezzat (1965a) redescribed and illustrated this species showing the presence of quinquelocular pores.
description: Published as part of Evans, Gregory A. & Abd-Rabou, Shaaban, 2023, The mealybugs (Hemiptera: Coccoidea: Pseudococcidae) of Egypt, pp. 1-83 in Insecta Mundi 2023 (999) on page 20, DOI: 10.5281/zenodo.10832115
title: ADCO, Cart. 186 (11 H 71), f. 0048r
Creators: name: de la Côte d'Or, Archives départementales
name: Petot, Frédéric
name: Archives Départementales De La Côte-D'Or
name: Petot, Frédérique
name: Projet CBMA
name: CBMA/CG21/F.PETOT/2012
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2020
Subjects: subject: cartulaire
subject: Corpus Burgundiae Medii Aevi
subject: Chartes de la Bourgogne du Moyen Âge
subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris

description: Cartulaire général de Cîteaux, dit de Jean de Cirey, t. II (XVe siècle), tome II, Archives départementales de la Côte-d'Or, C
art. 186 (11 H 71). Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Cartulaire général de Cîteaux, dit de Jean de Cirey, t. II (XVe siècle), tome II, Archives départementales de la
 Côte-d'Or, Cart. 186 (11 H 71), f. 0048r, 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
Additional file 1: of Predictive biomarkers for death and rehospitalization in comorbid frail elderly heart failure patients
Creators: name: Pacho, Cristina
name: Domingo, Mar
name: Núñez, Raquel
name: Lupón, Josep
name: Núñez, Julio
name: Barallat, Jaume
name: Moliner, Pedro
name: Antonio, Marta De
name: Santesmases, Javier
name: Cediel, Germán
name: Roura, Santiago
name: M. Pastor
name: Tor, Jordi
name: Bayes-Genis, Antoni
Publisher: name: figshare
Year: 2018
Subjects: subject: Space Science
subject: Medicine
subject: Cell Biology
subject: Physiology
subject: FOS: Biological sciences
subject: 69999 Biological Sciences not elsewhere classified
subject: 80699 Information Systems not elsewhere classified
subject: FOS: Computer and information sciences
subject: 19999 Mathematical Sciences not elsewhere classified
subject: FOS: Mathematics
subject: Developmental Biology

description: Table S1. Correlations between studied biomarkers. Correlation between the different studied biomarkers was performed using Pearson correlation test of log-transformed values of each biomarker. (DOCX 25 kb)
Polymorphism and the obstinate circularity of second order logic: a victims' tale
Creators: name: Pistone, Paolo
Publisher: name: arXiv
Year: 2017
Subjects: subject: Logic (math.LO)
subject: Logic in Computer Science (cs.LO)
subject: FOS: Mathematics
subject: FOS: Computer and information sciences
subject: 03F05, 03F35

description: The investigations on higher-order type theories and on the related notion of parametric polymorphism constitute the technical counterpart of the old foundational problem of the circularity (or impredicativity) of second and higher order logic. However, the epistemological significance of such investigations, and of their often non trivial results, has not received much attention in the contemporary foundational debate. The results recalled in this paper suggest that the question of the circularity of second order logic cannot be reduced to the simple assessment of a vicious circle. Through a comparison between the faulty consistency arguments given by Frege and Martin-Löf, respectively for the logical system of the Grundgesetze (shown inconsistent by Russell's paradox) and for the intuitionistic type theory with a type of all types (shown inconsistent by Girard's paradox), and the normalization argument for second order type theory (or System F), we indicate a bunch of subtle mathematical problems and logical concepts hidden behind the hazardous idea of impredicative quantification, constituting a vast (and largely unexplored) domain for foundational research.
Mehrsprachige Digital Literacy und Digital Humanities in der Lehre
Creators: name: Beers, Theodore
name: Kraneiß, Natalie
name: Müller-Laackman, Jonas
name: Thies, Antonia
name: Wagner, Cosima
Publisher: name: Zenodo
Year: 2024
Subjects: DHd2024
Vortrag
Lehre
Mehrsprachigkeit
Digital Literacy
Community-Bildung
Einführung
Sprache
Literatur
Text

description: In der akademischen Lehre - nicht nur, aber vor allem in den Geisteswissenschaften - werden zunehmend digitale Methoden und Quellen eingebunden. Dabei stellt sich die Frage, wie das bereits vorhandene Wissen über Methoden und Tools sinnvoll und zielführend vermittelt werden kann. Diese Vermittlung wird zu einem Problem, wenn Lehrkräfte nicht über das nötige Fachwissen verfügen, um Digital Humanities als Teil des wissenschaftlichen Methodenkasten lehren zu können und es keine ausgebildeten DH-Lehrkräfte im Fachbereich gibt, die diese Aufgaben übernehmen können. Oft sind besonders die sogenannten "Kleinen Fächern" davon betroffen. Wir möchten über die Erkenntnisse und Erfahrungen aus Veranstaltungen der AG Multilingual DH mit betroffenen Stakeholdern berichten. Auch möchten wir einen Ausblick geben über weitere Schritte der Vernetzung und Zusammenarbeit, auch mit Blick auf die mögliche Rolle des DHd-Verbandes in diesem Kontext.
Individual project on theme "Lens Mill" (MOOC: CompTech in biology)
Creators: name: Efremova Anna
Publisher: name: Zenodo
Year: 2025

description: Данный кейс является результатом реализации индивидуального проекта Ефремовой Анны по теме "Lens Mill" в рамках онлайн курса "Компьютерные технологии в биологии" (автор – А.В. Ваганов) (https://stepik.org/course/60859/promo)
Electrostatic self-energy and Bekenstein entropy bound in the massive Schwinger model
Creators: name: Sadjadi, H. Mohseni
name: Alimohammadi, M.
Publisher: name: arXiv
Year: 2005
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We obtain the electrostatic energy of two opposite charges near the horizon of stationary black-holes in the massive Schwinger model. Besides the confining aspects of the model, we discuss the Bekenstein entropy upper bound of a charged object using the generalized second law. We show that despite the massless case, in the massive Schwinger model the entropy of the black hole and consequently the Bekenstein bound are altered by the vacuum polarization.
description: 14 pages, accepted for publication in "Gen. Rel. Grav. (2005)"
Turbulent Structure of the Interstellar Medium
Creators: name: Mac Low, Mordecai-Mark
Publisher: name: arXiv
Year: 2003
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: How does turbulence contribute to the formation and structure of the dense interstellar medium (ISM)? Molecular clouds are dense, high-pressure objects. It is usually argued that gravitational confinement causes the high pressures, and that the clouds are (magneto)hydrostaticobjects supported by a balance between magnetic and turbulent pressures and gravity. However, magnetic pressures appear too weak, and MHD turbulent support not only requires driving, but also results in continuing gravitational collapse, as has now been demonstrated in simulations reaching 512^3 zones. Models of supernova-driven, magnetized turbulence readily form transient, high-pressure, dense regions that may form molecular clouds. They are contained not by self-gravity, but by turbulent ram pressures from the larger flow. Apparent virialization may actually be a geometrical effect. Turbulent clouds are unlikely to be in hydrostatic equilibrium, instead either collapsing or expanding, although they may appear well-fit by projected equilibrium Bonnor-Ebert spheres. Collapsing clouds probably form stars efficiently, while expanding ones can still form stars by turbulent compression, but rather inefficiently.
description: 8 pages, 4 figures, for publication in The Dense ISM in Galaxies, eds. S. Pfalzner, C. Kramer, C. Straubmeier, & A. Heithausen (Springer Verlag, Heidelberg)
Gene essentiality profiling reveals a novel determinant of stresses preventing protein aggregation in Salmonella
Creators: name: Wang, Zuoqiang
name: Zhu, Siqi
name: Li, Congcong
name: Lyu, Lin
name: Yu, Jingchen
name: Wang, Danni
name: Xu, Zhihong
name: Ni, Jinjing
name: Gao, Beile
name: Lu, Jie
name: Yao, Yu-Feng
Publisher: name: Taylor & Francis
Year: 2022
Subjects: subject: Biochemistry
subject: Microbiology
subject: FOS: Biological sciences
subject: Genetics
subject: Environmental Sciences not elsewhere classified
subject: Immunology
subject: FOS: Clinical medicine
subject: Biological Sciences not elsewhere classified
subject: Infectious Diseases
subject: FOS: Health sciences

description: Adaptation to various stresses during infection is important for Salmonella Typhimurium virulence, while the fitness determinants under infection-relevant stress conditions remain unknown. Here, we simulated conditions Salmonella encountered within the host or in the environment by 15 individual stresses as well as two model cell lines (epithelium and macrophage) to decipher the genes and pathways required for fitness. By high-resolution Tn-seq analysis, a total of 1242 genes were identified essential for fitness under at least one stress condition. The comparative analysis of fitness determinants in 17 stress conditions indicated the essentiality of genes varied in different mimicking host niches. A total of 12 genes were identified as fitness determinants in all stress conditions, including recB, recC and xseA (encode three exonuclease subunits necessary for DNA recombination repair) and a novel essential fitness gene yheM. YheM is a putative sulfurtransferase subunit that responsible for tRNA modification, and our results showed that Salmonella lacking yheM accumulated more aggregates of endogenous protein than wild-type. Moreover, we established a scoring scheme for sRNA essentiality analysis and found STnc2080 of unknown function was essential for resistance to LL-37. In summary, we systematically dissected Salmonella gene essentiality profiling and demonstrated the general and specific adaptive requirements in infection-relevant niches. Our data not only provide valuable insights on how Salmonella respond to environmental stresses during infections, but also highlight the potential clinical application of fitness determinants in vaccine development.
Additional file 1: of Male partner attendance at antenatal care and adherence to antenatal care guidelines: secondary analysis of 2011 Ethiopian demographic and health survey data
Creators: name: Forbes, Faye
name: Wynter, Karen
name: Wade, Catherine
name: Berihun Zeleke
name: Fisher, Jane
Publisher: name: figshare
Year: 2018
Subjects: subject: Sociology
subject: FOS: Sociology
subject: Science Policy

description: pdf contains a supplementary table listing original survey items, response categories and coding for analysis. (PDF 367Â kb)
mRNA based vaccines provide broad protection against different SARS-CoV-2 variants of concern
Creators: name: Wang, Haomeng
name: Chen, Zhao
name: Wang, Zhenghua
name: Li, Jin
name: Yan, Zhihong
name: Yuan, Jinbo
name: Zhu, Airu
name: Chen, Lan
name: Liu, Ye
name: Hu, Chenlong
name: Zhu, Ali
name: Li, Guowei
name: Li, Yuehu
name: Deng, Jie
name: Ma, Liqiao
name: Sui, Xiuwen
name: Miao, Wei
name: Li, Junqiang
name: Zheng, Xiuyu
name: Piao, Jinhua
name: Yao, Yanfeng
name: Rao, Juhong
name: Shan, Chao
name: Yuan, Zhiming
name: Zhao, Jincun
name: Zhu, Tao
Publisher: name: Taylor & Francis
Year: 2022
Subjects: subject: Microbiology
subject: FOS: Biological sciences
subject: Genetics
subject: Molecular Biology
subject: Environmental Sciences not elsewhere classified
subject: Ecology
subject: Sociology
subject: FOS: Sociology
subject: Immunology
subject: FOS: Clinical medicine
subject: Biological Sciences not elsewhere classified
subject: Mathematical Sciences not elsewhere classified
subject: Infectious Diseases
subject: FOS: Health sciences
subject: Computational Biology

description: In order to overcome the pandemic of COVID-19, messenger RNA (mRNA)-based vaccine has been extensively researched as a rapid and versatile strategy. Herein, we described the immunogenicity of mRNA-based vaccines for Beta and the most recent Omicron variants. The homologous mRNA-Beta and mRNA-Omicron and heterologous Ad5-nCoV plus mRNA vaccine exhibited high level cross-reactive neutralization for Beta, original, Delta and Omicron variants. It indicated that the COVID-19 mRNA vaccines have great potential in the clinical use against different SARS-CoV-2 variants.
Inflows, Outflows, and a Giant Donor in the Remarkable Recurrent Nova M31N 2008-12a? - Hubble Space Telescope Photometry of the 2015 Eruption
Creators: name: Darnley, M. J.
name: Hounsell, R.
name: Godon, P.
name: Perley, D. A.
name: Henze, M.
name: Kuin, N. P. M.
name: Williams, B. F.
name: Williams, S. C.
name: Bode, M. F.
name: Harman, D. J.
name: Hornoch, K.
name: Link, M.
name: Ness, J. -U.
name: Ribeiro, V. A. R. M.
name: Sion, E. M.
name: Shafter, A. W.
name: Shara, M. M.
Publisher: name: arXiv
Year: 2017
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: The recurrent nova M31N 2008-12a experiences annual eruptions, contains a near-Chandrasekhar mass white dwarf, and has the largest mass accretion rate in any nova system. In this paper, we present Hubble Space Telescope (HST) WFC3/UVIS photometry of the late decline of the 2015 eruption. We couple these new data with archival HST observations of the quiescent system and Keck spectroscopy of the 2014 eruption. The late-time photometry reveals a rapid decline to a minimum luminosity state, before a possible recovery / re-brightening in the run-up to the next eruption. Comparison with accretion disk models supports the survival of the accretion disk during the eruptions, and uncovers a quiescent disk mass accretion rate of the order of $10^{-6}\,M_\odot\,\mathrm{yr}^{-1}$, which may rise beyond $10^{-5}\,M_\odot\,\mathrm{yr}^{-1}$ during the super-soft source phase - both of which could be problematic for a number of well-established nova eruption models. Such large accretion rates, close to the Eddington limit, might be expected to be accompanied by additional mass loss from the disk through a wind and even collimated outflows. The archival HST observations, combined with the disk modeling, provide the first constraints on the mass donor; $L_\mathrm{donor}=103^{+12}_{-11}\,L_\odot$, $R_\mathrm{donor}=14.14^{+0.46}_{-0.47}\,R_\odot$, and $T_\mathrm{eff, donor}=4890\pm110$ K, which may be consistent with an irradiated M31 red-clump star. Such a donor would require a system orbital period $\gtrsim5$ days. Our updated analysis predicts that the M31N 2008-12a WD could reach the Chandrasekhar mass in < 20 kyr.
description: 20 pages, 8 figures, 5 tables, accepted for publication in The Astrophysical Journal
Auffinden und Analysieren komplexer Textvarianten in Hannah Arendts Denk- und Schreibwerkstatt mit LERA
Creators: name: Etling, Fabian
name: Pöckelmann, Marcus
name: Grote, Brigitte
Publisher: name: Zenodo
Year: 2024
Subjects: DHd2024
Posterpräsentation
Digitale Edition
Kollationierung
textgenetischer Vergleich
interaktive Textsynopse
Close Reading
Distant Reading
Annotieren
Webentwicklung
Visualisierung
Text
Werkzeuge
virtuelle Forschungsumgebungen

description: Eine umfangreiche Überlieferungslage, die verschiedene Textfassungen und Bearbeitungszustände aufweist, stellt Editionsprojekte vor eine doppelte Herausforderung. Zum einen ist die editorische Kollationierungsarbeit manuell in der erforderlichen Präzision zeitökonomisch kaum leistbar. Zum anderen sind die Anforderungen an die Visualisierung der Ergebnisse hoch, da den Nutzenden der Edition möglichst ein vollständiger Textvergleich geboten und alle textkritischen Entscheidungen transparent gemacht werden sollen. Auch das Editionsvorhaben Hannah Arendt. Kritische Gesamtausgabe (HAKG) sieht sich mit diesen Herausforderungen konfrontiert. Mit der Webanwendung LERA (Locate, Explore, Retrace and Apprehend) existiert ein Kollationierungswerkzeug, das die Berechnung von Textvarianten zwischen mehreren Textfassungen sowie interaktive Close- und Distant-Reading-Visualisierungen ermöglicht. Eine automatische Alignierung größerer Textsegmente sowie ein Detailvergleich auf Zeichenebene erlauben eine explorative Analyse der Abweichungen in synoptischer Gegenüberstellung. Dieser Beitrag zeigt, wie sich durch die Kooperation von HAKG und LERA nicht nur die Bedarfe des Editionsprojekts decken lassen, sondern für beide Seiten Mehrwerte entstehen, von denen auch Dritte profitieren können.
The Power of SOFIA/FORCAST in Estimating Internal Luminosities of Low Mass Class 0/I Protostars
Creators: name: Huard, Tracy L.
name: Terebey, Susan
Publisher: name: arXiv
Year: 2017
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: With the Stratospheric Observatory for Infrared Astronomy (SOFIA) routinely operating science flights, we demonstrate that observations with the Faint Object infraRed CAmera for the SOFIA Telescope (FORCAST) can provide reliable estimates of the internal luminosities, $L_{\rm int}$, of protostars. We have developed a technique to estimate $L_{\rm int}$ using a pair of FORCAST filters: one "short-wavelength" filter centered within 19.7-25.3 $μ$m, and one "long-wavelength" filter within 31.5-37.1 $μ$m. These $L_{\rm int}$ estimates are reliable to within 30-40% for 67% of protostars and to within a factor of 2.3-2.6 for 99% of protostars. The filter pair comprised of F25.3$μ$m and F37.1$μ$m achieves the best sensitivity and most constrained results. We evaluate several assumptions that could lead to systematic uncertainties. The OH5 dust opacity matches observational constraints for protostellar environments best, though not perfectly; we find that any improved dust model will have a small impact of 5-10% on the $L_{\rm int}$ estimates. For protostellar envelopes, the TSC84 model yields masses that are twice those of the Ulrich model, but we conclude this mass difference does not significantly impact results at the mid-infrared wavelengths probed by FORCAST. Thus, FORCAST is a powerful instrument for luminosity studies targeting newly discovered protostars or suspected protostars lacking detections longward of 24 $μ$m. Furthermore, with its dynamic range and greater angular resolution, FORCAST may be used to characterize protostars that were either saturated or merged with other sources in previous surveys using the Spitzer Space Telescope or Herschel Space Observatory.
description: 17 pages, 9 figures. Accepted for publication in ApJ
Intrinsic definitions of "relative velocity" in general relativity
Creators: name: Bolos, Vicente J.
Publisher: name: arXiv
Year: 2005
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: Differential Geometry (math.DG)
subject: FOS: Physical sciences
subject: FOS: Mathematics

description: Given two observers, we define the "relative velocity" of one observer with respect to the other in four different ways. All four definitions are given intrinsically, i.e. independently of any coordinate system. Two of them are given in the framework of spacelike simultaneity and, analogously, the other two are given in the framework of observed (lightlike) simultaneity. Properties and physical interpretations are discussed. Finally, we study relations between them in special relativity, and we give some examples in Schwarzschild and Robertson-Walker spacetimes.
description: 29 pages, 12 figures. New proofs in special relativity and a new open problem in general relativity (see Remark 5.2). An Appendix has been added, studying the relative velocities in Schwarzschild, with new figures. Some spelling erros fixed
Peliococcopsis priesneri
Creators: name: Evans, Gregory A.
name: Abd-Rabou, Shaaban
Publisher: name: Zenodo
Year: 2023
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hemiptera
Pseudococcidae
Peliococcopsis
Peliococcopsis priesneri

description: Peliococcopsis priesneri (Laing, 1936)
(Figure 26, after Ezzat 1960e)
 Taxonomy. Phenacoccus priesneri Laing 1936: 80. Type data. EGYPT: Giza, on grass. Peliococcus priesneri (Laing, 1936); Ezzat 1960d: 51, change of combination.
 Hosts in Egypt. Cynodon dactylon (Laing 1936).
 Distribution in Egypt. Dokki, Cairo (Laing 1936).
 Remarks. This is a European species known only to feed on grasses. Ezzat (1960d) provided an illustration and redescription of the species. Danzig (2001) and Danzig and Gavrilov-Zimin (2014) reviewed the Palearctic species of this genus.
description: Published as part of Evans, Gregory A. & Abd-Rabou, Shaaban, 2023, The mealybugs (Hemiptera: Coccoidea: Pseudococcidae) of Egypt, pp. 1-83 in Insecta Mundi 2023 (999) on page 21, DOI: 10.5281/zenodo.10832115
Additional file 6 of Lactobacillus murinus alleviate intestinal ischemia/reperfusion injury through promoting the release of interleukin-10 from M2 macrophages via Toll-like receptor 2 signaling
Creators: name: Hu, Jingjuan
name: Deng, Fan
name: Zhao, Bingcheng
name: Lin, Zebin
name: Sun, Qishun
name: Yang, Xiao
name: Wu, Mei
name: Qiu, Shida
name: Chen, Yu
name: Yan, Zhengzheng
name: Luo, Sidan
name: Zhao, Jin
name: Liu, Weifeng
name: Li, Cai
name: Liu, Ke Xuan
Publisher: name: figshare
Year: 2022
Subjects: subject: Biochemistry
subject: Medicine
subject: Microbiology
subject: FOS: Biological sciences
subject: Cell Biology
subject: Physiology
subject: Chemical Sciences not elsewhere classified
subject: Ecology
subject: Science Policy
subject: Immunology
subject: FOS: Clinical medicine
subject: Biological Sciences not elsewhere classified

description: Additional file 5: Figure S4. Lactobacillus murinus improves intestinal I/R-induced intestinal injury in antibiotic-treated mice. a. Experimental design. The WT mice were randomly divided into the following groups. Group ABX + I/R, in which ABX was administered 1w before intestinal ischemia; Group ABX + I/R + L. murinus, treatment of mice with ABX for a week, and then mice were gavaged daily for 7 days with L. murinus. b Relative abundance of L. murinus in the cecum after ABX clearance experiment. c-e HE staining and ZO-1 and occludin immunofluorescent staining in the ileum. Representative quantification on the right. Scale bar=100 μm. f Tight junction mRNA levels in the ileum. g FD-4 level in the plasma. The results are expressed as the mean ± SEM. n = 8. ***p<0.001, **p<0.01, *p<0.05 were determined by two-tailed Student’s t-test. ABX, antibiotic; FD-4, FITC Dextran 4-KD; I/R, ischemia/reperfusion; HE, hematoxylin-eosin; L. murinus, Lactobacillus murinus; SMA, superior mesenteric artery.
Nuclear pasta in hot dense matter and its implications for neutrino scattering
Creators: name: Roggero, Alessandro
name: Margueron, Jérôme
name: Roberts, Luke F.
name: Reddy, Sanjay
Publisher: name: arXiv
Year: 2017
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: Nuclear Theory (nucl-th)
subject: FOS: Physical sciences

description: We find that the abundance of large clusters of nucleons in neutron-rich matter at sub-nuclear density is greatly reduced by finite temperature effects when matter is close to beta-equilibrium. Large nuclei and exotic non-spherical nuclear configurations called pasta, favored in the vicinity of the transition to uniform matter at $T=0$, dissolve at relatively low temperature. For matter close to beta-equilibrium we find that the pasta melting temperature is $T_m^β\simeq 4\pm 1$~MeV for realistic equations of state. The mechanism for pasta dissolution is discussed, and in general $T_m^β$ is shown to be sensitive to the proton fraction. We find that coherent neutrino scattering from nuclei and pasta makes a modest contribution to the opacity under the conditions encountered in supernovae and neutron star mergers. Implications for neutrino signals from galactic supernovae are briefly discussed.
description: 9 pages, 7 figures, 1 table
Searching for signs of triggered star formation toward IC 1848
Creators: name: Thompson, M. A.
name: White, G. J.
name: Morgan, L. K.
name: Miao, J.
name: Fridlund, C. V. M.
name: Huldtgren-White, M.
Publisher: name: arXiv
Year: 2003
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We have carried out an in-depth study of three bright-rimmed clouds SFO 11, SFO 11NE and SFO 11E associated with the HII region IC 1848, using observations carried out at the James Clerk Maxwell Telescope (JCMT) and the Nordic Optical Telescope (NOT), plus archival data from IRAS, 2MASS and the NVSS. We show that the overall morphology of the clouds is reasonably consistent with that of radiative-driven implosion (RDI) models developed to predict the evolution of cometary globules. There is evidence for a photoevaporated flow from the surface of each cloud and, based upon the morphology and pressure balance of the clouds, it is possible that D-critical ionisation fronts are propagating into the molecular gas. The primary O star responsible for ionising the surfaces of the clouds is the 06V star HD17505. Each cloud is associated with either recent or ongoing star formation: we have detected 8 sub-mm cores which possess the hallmarks of protostellar cores and identify YSO candidates from 2MASS data. We infer the past and future evolution of the clouds and demonstrate via a simple pressure-based argument that the UV illumination may have induced the collapse of the dense molecular cores found at the head of SFO 11 and SFO 11E.
description: Accepted by A&A. 27 pages. Note: figures presented here are low-resolution postscript. Please contact lead author for full-resolution images if required
Probing dark energy with large galaxy surveys: systematics quantification and mitigation
Creators: name: Awan, Humna
Publisher: name: No Publisher Supplied
Year: 2020

description: Dark energy is a leading theory to explain cosmic acceleration, and forthcoming astronomical surveys have been specifically designed to probe this mysterious energy component of our universe. This thesis addresses aspects of using large galaxy surveys to study dark energy, which requires an unprecedented understanding and mitigation of systematics -- a challenge that can be addressed on two fronts: quantification of the impacts of systematics, and new tools to mitigate them. Here, we specifically study the impacts of three key systematics: those induced by 1) the telescope observing strategy, 2) the Milky Way dust, and 3) uncertain photometric redshifts. Focusing on the Legacy Survey of Space and Time (LSST) carried out by the Vera C. Rubin Observatory, we quantify the impacts of LSST observing strategy on large-scale structure studies, which is a probe of dark energy. We demonstrate the effectiveness of large translational dithers -- telescope-pointing offsets -- in increasing LSST survey uniformity and reducing systematic uncertainties (Awan et al., 2016; LSST Science Collaboration et al., 2017) -- a result that has now been adopted for the baseline LSST observing strategy. We also study the impacts of Milky Way dust on dark energy science and demonstrate that ~25% of the default LSST survey area would not be useful for extragalactic static science given the Milky Way dust extinction, motivating the reconfiguration of the LSST survey footprint to avoid high-extinction regions of the sky (Lochner et al., 2018; Olsen et al., 2018). And finally, we present a new formalism that provides a novel way to correct for redshift contamination arising from photometric redshift estimation (Awan & Gawiser, 2020). Specifically, we first introduce a general formalism to correct for sample contamination for photometric galaxy samples when measuring two-point angular correlation functions, and then a new weighted estimator that assigns each galaxy a weight in each redshift bin based on its probability of being in that bin, thereby fully utilizing the probabilistic distance information available for photometric galaxies. While these techniques are motivated by preparations for LSST, they are applicable to other large galaxy surveys like Dark Energy Survey (DES), Dark Energy Spectroscopic Instrument (DESI), Hobby-Eberly Telescope Dark Energy Experiment (HETDEX), Euclid, and Wide-Field Infrared Survey Telescope (WFIRST).
title: ADCO, Ordre cistercien : comptes (1499-1515) (11 H 1162), f. 00262
Creators: name: de la Côte-d'Or, Archives départementales
name: Archives Départementales De La Côte-D'Or
name: Petot, Frédérique
name: Projet CBMA
name: Petot, Frédéric
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: comptes
subject: Corpus Burgundiae Medii Aevi
subject: Chartes de la Bourgogne du Moyen Âge
subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris

description: Ordre cistercien : comptes (1499-1515), Archives départementales de la Côte-d'Or, (11 H 1162). Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Ordre cistercien : comptes (1499-1515), Archives départementales de la Côte-d'Or, (11 H 1162), f. 00262, 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