cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Time-Resolved Mechanical Spectroscopy of Soft Materials via Optimally Windowed Chirps
Creators: name: Geri, Michela
name: Keshavarz, Bavand
name: Divoux, Thibaut
name: Clasen, Christian
name: Curtis, Dan J.
name: McKinley, Gareth H.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Soft Condensed Matter (cond-mat.soft)
subject: Materials Science (cond-mat.mtrl-sci)
subject: FOS: Physical sciences

description: The ability to measure the bulk dynamic behavior of soft materials with combined time- and frequency-resolution is instrumental for improving our fundamental understanding of connections between the microstructural dynamics and the macroscopic mechanical response. Current state-of-the-art techniques are often limited by a compromise between resolution in the time and frequency domain, mainly due to the use of elementary input signals that have not been designed for fast time-evolving systems such as materials undergoing gelation, curing or self-healing. In this work, we develop an optimized and robust excitation signal for time-resolved mechanical spectroscopy through the introduction of joint frequency- and amplitude-modulated exponential chirps. Inspired by the biosonar signals of bats and dolphins, we optimize the signal profile to maximize the signal-to-noise ratio while minimizing spectral leakage with a carefully-designed modulation of the envelope of the chirp. A combined experimental and numerical investigation reveals that there exists an optimal range of window profiles that minimizes the error with respect to standard single frequency sweep methods. The minimum error is set by the noise floor of the instrument, suggesting that the accuracy of an optimally windowed chirp signal is directly comparable to that achievable with a standard frequency sweep, while the acquisition time can be reduced by up to two orders of magnitude, for comparable spectral content. Finally, we demonstrate the ability of this optimized signal to provide time- and frequency-resolved rheometric data by studying the fast gelation process of an acid-induced protein gel. The use of optimally windowed chirps enables a robust rheological characterization of a wide range of soft materials undergoing rapid mutation and has the potential to become an invaluable tool for researchers across different disciplines.
A catalog of Nearby Poor Clusters of Galaxies
Creators: name: White, R. A.
name: Bliton, M.
name: Bhavsar, S. P.
name: Bornmann, P.
name: Burns, J. O.
name: Ledlow, M. J.
name: Loken, C.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: A catalog of 732 optically selected, nearby poor clusters of galaxies covering the entire sky north of $\rm -3^{\circ}$ declination is presented. The poor clusters, called WBL clusters, were identified as concentrations of 3 or more galaxies with photographic magnitudes brighter than 15.7, possessing a galaxy surface overdensity of $10^{4/3}$. These criteria are consistent with those used in the identification of the original Yerkes poor clusters, and this new catalog substantially increases the sample size of such objects. These poor clusters cover the entire range of galaxy associations up to and including Abell clusters, systematically including poor and rich galaxy systems spanning over three orders of magnitude in the cluster mass function. As a result, this new catalog contains a greater diversity of richness and structures than other group catalogs, such as the Hickson or Yerkes catalogs. The information on individual galaxies includes redshifts and cross-references to other galaxy catalogs. The entries for the clusters include redshift (where available) and cross-references to other group and cluster catalogs.
description: 27 pages, 7 figures, + one 20-page landscape table, accepted for publication in AJ
Spin excitations and thermodynamics of the t-J model on the honeycomb lattice
Creators: name: Vladimirov, A. A.
name: Ihle, D.
name: Plakida, N. M.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: FOS: Physical sciences

description: We present a spin-rotation-invariant Green-function theory for the dynamic spin susceptibility in the spin-1/2 antiferromagnetic t-J Heisenberg model on the honeycomb lattice. Employing a generalized mean-field approximation for arbitrary temperatures and hole dopings, the electronic spectrum of excitations, the spin-excitation spectrum and thermodynamic quantities (two-spin correlation functions, staggered magnetization, magnetic susceptibility, correlation length) are calculated by solving a coupled system of self-consistency equations for the correlation functions. The temperature and doping dependence of the magnetic (uniform static) susceptibility is ascribed to antiferromagnetic short-range order. Our results on the doping dependencies of the magnetization and susceptibility are analyzed in comparison with previous results for the t_J model on the square lattice.
description: 9 pages, 7 figures, submitted to European Physical Journal B. arXiv admin note: text overlap with arXiv:1703.08391
Low Energy Nucleon-Nucleon Scattering with the Skyrme Model in the Geodetic Approximation
Creators: name: Gisiger, T.
name: Paranjape, M. B.
Publisher: name: arXiv
Year: 1994
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We calculate nucleon-nucleon scattering at low energies and large impact parameter in the Skyrme model within the framework for soliton scattering proposed by Manton. This corresponds to a truncation of the degrees of freedom to the twelve collective coordinates which essentially describe the rigid body motion of the pair of Skyrmions. We take to its logical conclusion the result that the induced kinetic energy for these collective coordinates in the product ansatz behaves as one over the separation and hence can dominate over the potential. This behaviour implies to leading order that we can drop the potential and the resulting motion reduces simply to geodesic motion on the manifold parametrized by the variables of the product ansatz. We formulate the semi-classical quantization of these variables to obtain the motion corresponding to the nucleonic states of the Skyrme model. This is the appropriate description for the nucleons in order to consider their scattering within Manton's framework in the semi-classical approximation. We investigate the implications for the scattering of nucleons with various initial polarizations using the approximation method of ``variation of constants''.
description: 18 pages, UDEM-LPN-TH-94-196
SERVERLESS CLOUD COMPUTING: A COMPARISON BETWEEN "FUNCTION AS A SERVICE" PLATFORMS
Creators: name: Jiménez, Víctor Juan Expósito
name: Zeiner, Herwig
Publisher: name: figshare
Year: 2018
Subjects: Computer Engineering

description: Cloud computing is moving fast and continually progressing. Beyond the microservices architecture, a new paradigm appears to be evolving and complementing it. By using a serverless computing architecture, faster and more reliable developments are possible in several fields such as the Internet of Things, industrial or mobility applications. In this paper, a serverless computing architecture is described and, in addition, a comparison of the most important "Function as a Service" platforms is given.
ALISHER NAVOIYNING JAMIYAT TAMADDUNIDA TUTGAN O'RNI
Creators: name: Yuldasheva, O'g'iloy
Publisher: name: Zenodo
Year: 2024

description: Ushbu maqola ham turkiy ham forsiy tillarda ijod qilgan, yosh chog'idayoq o'sha davrning dongdor shori Lutfiyni ikki misra g'azali bilan lol qoldira olgan buyuk mutafakkir Alisher Navoiy haqidadir.
website designing company in Vasundhara
Creators: name: Digital Markeitng
Publisher: name: Zenodo
Year: 2025

description: DigitalBanegaIndia is a one of the best website designing company in Vasundhara that helps small or large businesses to build a strong online identity. We offer a wide range of services like SEO (Search Engine Optimization), SMO (Social Media Optimization), website design, e-commerce websites, web development, software development and digital marketing. We provide free-of-cost consultancy. Our team of professional website designing company in Vasundhara works diligently and hard to create fast, easy to use and SEO-optimized websites. We are committed to delivering quality services and original results. For more information, visit our website immediately
title: ADCO, Cartulaire des Dominicains de Dijon (1286), Cart. 221 (H 53), 170 folios, f. 0135
Creators: name: de la Côte d'Or, Archives départementales
name: Archives Départementales De La Côte-D'Or
name: Petot, Frédérique
name: Projet CBMA
name: CG21/F.PETOT/2012
name: Petot, Frédéric
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2020
Subjects: subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris
subject: cartulaire
subject: Corpus Burgundiae Medii Aevi
subject: Chartes de la Bourgogne du Moyen Âge

description: Cartulaire des Dominicains de Dijon (1286), Archives départementales de la Côte-d'Or, Cart. 221 (H 53), 170 folios. Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Cartulaire des Dominicains de Dijon (1286), Archives départementales de la Côte-d'Or, Cart. 221 (H 53), 170 folios, f. 0135, in Projet CBMA - Corpus Burgundiae Medii Aevi [Ressource en ligne], https:// manuscrits.cbma-project.eu/
description: Provenance: Dijon
description: Provenance: http://www.wikidata.org/entity/Q7003
description: Provenance: https://catalogue.bnf.fr/ark:/12148/cb15250518p
description: Provenance: http://www.idref.fr/02643413X/id
description: Provenance: https://www.geonames.org/6453767
Strombus canariu Linnaeus, 1758, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1758
Subjects: Biodiversity
Taxonomy
Animalia
Mollusca
Gastropoda
Littorinimorpha
Strombidae
Strombus
Strombus canariu

description: Strombus canariu [spec. nov.]
S. testae labro rotundato brevi retuso, spiraque laevi.
Petiv. gaz. t. 98. f. 11.
Rumph. mus. t. 36. f. X. N.
Gvalt. test. t. 32. f. N.
Argenv. conch. t. 17. f. Q.
Klein. ostr. t. 4. f. 73.
Habitat in O. Asiae.
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 745, DOI: 10.5962/bhl.title.542, http://zenodo.org/record/3922206
On marginal and conditional parameters in logistic regression models
Creators: name: Stanghellini, Elena
name: Doretti, Marco
Publisher: name: arXiv
Year: 2018
Subjects: subject: Statistics Theory (math.ST)
subject: FOS: Mathematics

description: A fundamental research question is how much a variation in a covariate influences a binary response variable in a logistic regression model, both directly or through mediators. We derive the exact formula linking the parameters of marginal and conditional regression models with binary mediators when no conditional independence assumptions can be made. The formula has the appealing property of being the sum of terms that vanish whenever parameters of the conditional models vanish, thereby recovering well-known results as particular cases. It also permits to quantify the distortion induced by omission of some relevant covariates, opening the way to sensitivity analysis. Also in this case, as the parameters of the conditional models are multiplied by terms that are always positive or bounded, the formula may be used to construct reasonable bounds on the parameters of interest. We assume that, conditionally on a set of covariates, the data-generating process can be represented by a Directed Acyclic Graph. We also show how the results here presented lead to the extension of path analysis to a system of binary random variables.
description: 12 pages, 2 figures
The Emission from Post-Shock Flows in mCVs
Creators: name: Cropper, Mark
name: Wu, Kinwah
name: Ramsay, Gavin
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We re-examine the vertical structure of the post-shock flow in the accretion region of mCVs, and the X-ray emission as a function of height. We then predict X-ray light curves and phase-resolved spectra, taking into account the vertical structure, examine the implications and check whether the predicted heights are compatible with observation.
description: 6 pages, to be published in the Proc of the Symp. to mark the 60th birthday of Brian Warner
Additional file 1 of Biochar-mediated enhanced ethanol fermentation (BMEEF) in Zymomonas mobilis under furfural and acetic acid stress
Creators: name: Wang, Wei-ting
name: Dai, Li-chun
name: Wu, Bo
name: Qi, Bu-fan
name: Huang, Tian-fang
name: Hu, Guo-quan
name: He, Ming-xiong
Publisher: name: figshare
Year: 2020
Subjects: subject: Biochemistry
subject: Space Science
subject: Medicine
subject: Microbiology
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Neuroscience
subject: Environmental Sciences not elsewhere classified
subject: Sociology
subject: FOS: Sociology
subject: Biological Sciences not elsewhere classified

description: Additional file 1: Figure S1. Biochar-facilitated ethanol fermentation in acetic acid stress conditions. No acetic acid removal (a), and little pH changes (b). Figure S2. Effects of biochar on ethanol fermentation by Z. mobilis ZM4 in the presence of RM medium. “RM” indicates Z. mobilis ZM4 fermented in RM medium. “RMC” indicates Z. mobilis ZM4 co-cultured with 3.5‰ biochar fermented in RM medium.
AN INTEROPERABLE CLOUD-BASED GEOPORTAL FOR DISCOVERY AND MANAGEMENT OF EARTH OBSERVATIONPRODUCTS
Creators: name: Sánchez-Gallegos, Dante D.
name: Gonzalez-Compean, J.L.
name: SosaSosa, Victor J.
name: Marin-Castro, Heidy M.
name: Tuxpan-Vargas, José
Publisher: name: figshare
Year: 2018
Subjects: Computer Engineering

description: This paper presents the design and development of an interoperable geoportal service for discovery and management of earth observation products (EOPs). In this service, the geoportal components are encapsulated into virtual containers that are launched into the cloud by using a microservice scheme to solve issues such as interoperability (with other systems) and implementation (over different platforms). A search microservice that analyses the preferences of end-users (settings of spatiotemporal and polygon shapes) and builds clusters of users sharing preferences was included into the geoportal for recommending/delivering, in advance, products matching with end-user preferences. The geoportal service also enables end-users to organize EOPs on-the-fly by using spatiotemporal parameters. A prototype of this service was implemented in a private cloud and connected to a satellite imagery repository of an antenna (ERIS) managed by Mexican Space Agency in a proof of concept. Learned lessons and performance assessments are described through an experimental evaluation with real users' participation.
Strombus ater Linnaeus, 1758, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1758
Subjects: Biodiversity
Taxonomy
Animalia
Mollusca
Gastropoda
Littorinimorpha
Strombidae
Strombus
Strombus ater

description: Strombus ater [spec. nov.]
S. testa turrita laevi, labro antice posticeque soluto.
Rumph. mus. t. 30. f. R.
Habitat in Asiae paludibus.
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 746, DOI: 10.5962/bhl.title.542, http://zenodo.org/record/3922206
title: ADCO, Cartulaire de Fontenay, second fragment (XIIIe siècle), Cart. 201 (15 H 9), folios 47-142, f. 040v
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/2009
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2020
Subjects: subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris
subject: cartulaire
subject: Corpus Burgundiae Medii Aevi
subject: Chartes de la Bourgogne du Moyen Âge

description: Cartulaire de Fontenay, second fragment (XIIIe siècle), Archives départementales de la Côte-d'Or, Cart. 201 (15 H 9), folios 47-142. Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Cartulaire de Fontenay, second fragment (XIIIe siècle), Archives départementales de la Côte-d'Or, Cart. 201 (15 H 9), folios 47-142, f. 040v, in Projet CBMA - Corpus Burgundiae Medii Aevi [Ressource en ligne], https:// manuscrits.cbma-project.eu/
description: Provenance: abbaye de Fontenay
description: Provenance: http://www.wikidata.org/entity/Q464918
description: Provenance: https://catalogue.bnf.fr/ark:/12148/cb119679755
description: Provenance: https://www.geonames.org/7874015
description: Provenance: http://www.idref.fr/027691802/id
Leptoquark Pair Production at $ep$ Colliders
Creators: name: Blümlein, Johannes
name: Boos, Edward
name: Pukhov, Alexander
Publisher: name: arXiv
Year: 1994
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: The pair production cross section for scalar and vector leptoquarks at $ep$ colliders is calculated for the case of photon--gluon fusion. In a model independent analysis we consider the most general $C$ and $P$ conserving couplings of gluons and photons to both scalar and vector leptoquarks described by an effective low--energy Lagangian which obeys $U(1)_{em} \times SU(3)_c$ invariance. Numerical predictions are given for the kinematical regime at HERA and LEP~$\otimes$~LHC.
description: 15 p., postscript encoded with uufiles; DESY 94--072
Additional file 5 of Large-scale public data reuse to model immunotherapy response and resistance
Creators: name: Fu, Jingxin
name: Li, Karen
name: Zhang, Wubing
name: Wan, Changxin
name: Zhang, Jing
name: Jiang, Peng
name: Liu, X.
Publisher: name: figshare
Year: 2020
Subjects: subject: Genetics
subject: FOS: Biological sciences
subject: Pharmacology
subject: Evolutionary Biology
subject: Biological Sciences not elsewhere classified
subject: Information Systems not elsewhere classified
subject: Mathematical Sciences not elsewhere classified
subject: Cancer
subject: Plant Biology

description: Table S4. Genes with approved drugs.
Revisiting the Phase Curves of WASP-43b: Confronting Reanalyzed Spitzer Data with Cloudy Atmospheres
Creators: name: Mendonça, João M.
name: Malik, Matej
name: Demory, Brice-Olivier
name: Heng, Kevin
Publisher: name: arXiv
Year: 2018
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: FOS: Physical sciences

description: Recently acquired Hubble and Spitzer phase curves of the short-period hot Jupiter WASP-43b make it an ideal target for confronting theory with data. On the observational front, we re-analyze the 3.6 and 4.5 $μ$m Spitzer phase curves and demonstrate that our improved analysis better removes residual red noise due to intra-pixel sensitivity, which leads to greater fluxes emanating from the nightside of WASP-43b, thus reducing the tension between theory and data. On the theoretical front, we construct cloudfree and cloudy atmospheres of WASP-43b using our Global Circulation Model (GCM), THOR, which solves the non-hydrostatic Euler equations (compared to GCMs that typically solve the hydrostatic primitive equations). The cloudfree atmosphere produces a reasonable fit to the dayside emission spectrum. The multi-phase emission spectra constrain the cloud deck to be confined to the nightside and have a finite cloud-top pressure. The multi-wavelength phase curves are naturally consistent with our cloudy atmospheres, except for the 4.5 $μ$m phase curve, which requires the presence of enhanced carbon dioxide in the atmosphere of WASP-43b. Multi-phase emission spectra at higher spectral resolution, as may be obtained using the James Webb Space Telescope, and a reflected-light phase curve at visible wavelengths would further constrain the properties of clouds in WASP-43b.
description: Accepted for publication in ApJ
High-z gamma-ray burst detection by SVOM/ECLAIRs: Impact of instrumental biases on the bursts' measured properties
Creators: name: Lanza, Miguel Llamas
name: Godet, Olivier
name: Arcier, Benjamin
name: Yassine, Manal
name: Atteia, Jean-Luc
name: Bouchet, Laurent
Publisher: name: arXiv
Year: 2024
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: Context. Gamma-ray bursts (GRBs) can be detected at cosmological distances and therefore can be used to study the contents and phases of the early Universe. The 4-150 keV wide-field trigger camera ECLAIRs to fly on board the Space-based multi-band Variable Object Monitor (SVOM) mission, dedicated to studying the high-energy transient sky in synergy with multi-messenger follow-up instruments, has been adapted to detect high-redshift (high-z) GRBs. Aims. Investigating the detection capabilities of ECLAIRs for high-z GRBs and estimating the impacts of instrumental biases in reconstructing some of the source measured properties, focusing on GRB duration biases as a function of redshift. Methods. We simulated realistic detection scenarios for a sample of 162 already observed GRBs with known redshift values as they would have been seen by ECLAIRs. We simulated them at redshift values equal and higher than their measured value. Then, we assessed whether they would be detected with a trigger algorithm resembling that on board of ECLAIRs, and derived quantities such as T90, for those that would have been detected. Results. We find that ECLAIRs would be capable of detecting GRBs up to very high redshift values (e.g. 20 GRBs in our sample are detectable within more than 0.4 of the ECLAIRs field of view for z > 12). The ECLAIRs low-energy threshold of 4 keV, contributes to this great detection capability, as it may enhance it at high redshift (z > 10) by over 10% compared to a 15 keV low-energy threshold. We also show that the detection of GRBs at high-z values may imprint tip-of-the-iceberg biases on the GRB duration measurements, which can affect the reconstruction of other source properties.
description: 13 pages, 14 Figures, 2 Tables. Accepted for publication on A&A on February 23, 2024
The X-Ray Spectrum and Global Structure of the Stellar Wind in Vela X-1
Creators: name: Sako, Masao
name: Liedahl, Duane A.
name: Kahn, Steven M.
name: Paerels, Frits
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present a quantitative analysis of the X-ray spectrum of the eclipsing high mass X-ray binary Vela X-1 (4U 0900-40) using archival data from ASCA. The observation covers a time interval centered on eclipse of the X-ray pulsar by the companion. The spectrum exhibits two distinct sets of discrete features: (1) recombination lines and radiative recombination continua from mostly H- and He-like species produced by photoionization in an extended stellar wind; and (2) fluorescent K-shell lines associated with near-neutral species also present in the circumsource medium. Using a detailed spectral model that explicitly accounts for the recombination cascade kinetics for each of the constituent charge states, we are able to obtain a statistically acceptable (chi_r^2=0.88) fit to the observed spectrum and to derive emission measures associated with the individual K-shell ions of several elements. We find a best-fit mass loss rate of ~2.7 x 10^-7 M-solar/yr, which is approximately a factor of 10 lower than previous estimates of the mass loss rate for the Vela X-1 companion star, which have primarily been determined from P Cygni profiles, and X-ray absorption measurements. We argue that this discrepancy can be reconciled if the X-ray irradiated portion of the wind in Vela X-1 is structurally inhomogeneous, consisting of hundreds of cool, dense clumps embedded in a hotter, more ionized gas. Most of the mass is contained in the clumps, while most of the wind volume (>95%) is occupied by the highly ionized component. We show quantitatively, that this interpretation is also consistent with the presence of the X-ray fluorescent lines in the ASCA spectrum, which are produced in the cooler, clumped component.
description: 45 pages, LaTeX, 9 PostScript figures. To be published in ApJ, November 20, 1999, Volume 526
title: Chrystal MacMillan and Elsie Bowerman: First Women Barristers' Negotiation of Professional and Political Identities
Creators: name: Noakes, Laura
Publisher: name: The Open University
Year: 2021

description: This thesis examines the relationship between first-wave feminist political activism and the professional identities of early women lawyers through a detailed contextual consideration of two women: Elsie Bowerman and Chrystal Macmillan. Bowerman was a keen member of the Women’s Social and Political Union (WSPU). She was Christabel Pankhurst’s election agent for the 1918 general election and founded the Women’s Guild of Empire (WGE) with fellow suffragette Flora Drummond. Bowerman was called to the Bar in 1924 and practised until 1938. Chrystal Macmillan was a leading member of the National Union of Women’s Suffrage Societies (NUWSS), the first woman to plead her case in the House of Lords, and a successful barrister whose feminist politics extended beyond the granting of suffrage to women. Much of her post-World War One activism focused on opposing the practice of assigning married women their husband’s identity. I argue that there were complex and multifaceted connections between these women’s activism, legal practice and the law, which originated during the fight for women’s votes. I will examine in depth the effect these connections had on their legal aspirations and their involvement with politics after 1918. In doing so my thesis calls attention to the complications encountered by both women within the legal profession as women and feminists, and also reveals their long-term dedication to facilitating legal change through their activism. This research illuminates the multiple links between Bowerman and Macmillan’s roles as barristers and political activists, by exploring how complex societal expectations of women’s behaviour interacted with their wish to challenge gendered inequality. Consequently, it complicates our understanding of women entering the professions, feminist activism, and the relationship between law and politics during the late-19th and 20th centuries.
Disk stars in the Milky Way detected beyond 25 kpc from its center
Creators: name: Lopez-Corredoira, M.
name: Prieto, C. Allende
name: Garzon, F.
name: Wang, H.
name: Liu, C.
name: Deng, L.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: CONTEXT. The maximum size of the Galactic stellar disk is not yet known. Some studies have suggested an abrupt drop-off of the stellar density of the disk at Galactocentric distances $R\gtrsim 15$ kpc, which means that in practice no disk stars or only very few of them should be found beyond this limit. However, stars in the Milky Way plane are detected at larger distances. In addition to the halo component, star counts have placed the end of the disk beyond 20 kpc, although this has not been spectroscopically confirmed so far. AIMS. Here, we aim to spectroscopically confirm the presence of the disk stars up to much larger distances. METHODS. With data from the LAMOST and SDSS-APOGEE spectroscopic surveys, we statistically derived the maximum distance at which the metallicity distribution of stars in the Galactic plane is distinct from that of the halo populations. RESULTS. Our analysis reveals the presence of disk stars at R>26 kpc (99.7% C.L.) and even at R>31 kpc (95.4% C.L.).
description: 4 pages, accepted to be published in A&A-Letters
Higher Twist Effects in the Drell-Yan Angular Distribution
Creators: name: Eskola, K. J.
name: Hoyer, P.
name: Vänttinen, M.
name: Vogt, R.
Publisher: name: arXiv
Year: 1994
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We study the Drell-Yan process $πN \rightarrow μ^+ μ^- X$ at large $x_F$ using perturbative QCD. A higher-twist mechanism suggested by Berger and Brodsky is known to qualitatively explain the observed $x_F$ dependence of the muon angular distribution, but the predicted large $x_F$ behavior differs quantitatively from observations. We have repeated the model calculation taking into account the effects of nonasymptotic kinematics. At fixed-target energies we find important corrections which improve the agreement with data. The asymptotic result of Berger and Brodsky is recovered only at much higher energies. We discuss the generic reasons for the large corrections at high $x_F$. A proper understanding of the $x_F \to 1$ data would give important information on the pion distribution amplitude and exclusive form factor.
description: 8 pages in Latex with 3 figures appended as Postscript files, HU-TFT-94-12, LBL-35430. (The introductory part has been slightly altered and three references have been added)
Strombus lividus Linnaeus, 1758, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1758
Subjects: Biodiversity
Taxonomy
Animalia
Mollusca
Gastropoda
Littorinimorpha
Strombidae
Strombus
Strombus lividus

description: Strombus lividus [spec. nov.]
S. testa turrita nodoso-spinosa, labro antice soluto.
Habitat ..
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 746, DOI: 10.5962/bhl.title.542, http://zenodo.org/record/3922206
Vers un modèle numérique pour une paléographie transversale
Creators: name: Stokes, Peter
Publisher: name: Zenodo
Year: 2024
Subjects: Paléographie
Linked Open Data
Modélisation
Humanités numériques

description: Cette présentation vise à aborder la question d'une terminologie commune pour l'écriture manuscrite qui peut être appliquée à toutes les écritures, langues et périodes, dans le but de relier les jeux de données existants et nouveaux en tant que "Linked Open Data", et de fournir une base plus rigoureuse pour l'analyse du polygraphisme (à savoir les scribes qui utilisaient des écritures entièrement différentes, par ex. le latin et l'arabe, ou le chinois et l'hébreu).
description: This presentation aims to begin addressing the question of a common terminology for handwriting that can be applied across all scripts, languages and periods, with the goal of being able to link existing and new datasets as Linked Open Data and provide a more rigorous foundation for the analysis of polygraphic scribes (namely those who wrote in entirely different scripts such as Latin and Arabic, or Chinese and Hebrew).
An Observational Test of Dark Matter as Cold Fractal Clouds
Creators: name: Irwin, Judith A.
name: Widrow, Lawrence M.
name: English, Jayanne
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Using the VLA, we have performed the first observational test of dark matter in the form of cold, primordial fractal clouds, as envisioned by Pfenniger, Combes, & Martinet (1994) and Pfenniger & Combes (1994). We show that, after a Hubble Time, primordial fractal clouds will convert most of their HI to H2, but a small fraction of HI remains which is optically thick. This opens up a new window for detecting dark matter which may exist in this form. The detectability of such gas depends on its filling factor and temperature and therefore should be observable in absorption against a background source, with observations of sufficient sensitivity and resolution. The current VLA observations have made a first step towards this goal by taking advantage of a fortuitous alignment between the extension of the HI disk of the nearby galaxy, NGC 3079, and a background quasar Q 0957+561. Our observations probe 28 independent beams against the quasar and all of velocity space between the extension of a flat rotation curve and a Keplerian decline for the halo region of NGC 3079. We do not detect any absorption features and investigate, in detail, the implication of this result for the hypothesis that dark matter is in the form of fractal clouds. While our analysis does not rule out fractal clouds as dark matter, it does lay out the groundwork for future, more sensitive observations and we consider what form these might take to probe the range of possible cloud properties more deeply. It is interesting that the observations can rule out cold optically thin HI gas, if it exists, to a limit of 0.001% of the dark matter. In contrast, the existence of cold HI in a fractal hierarchy would be an efficient way of hiding dark matter.
description: 41 pages including 8 figures and one table Submitted to the Astrophysical Journal
title: ADCO, Huitième cartulaire de Saint-Étienne de Dijon (1661-1667), Cart. 31 (G 135), 549 folios, f. 0647
Creators: name: de la Côte d'Or, Archives départementales
name: CG21/F.PETOT/2012
name: Archives Départementales De La Côte-D'Or
name: Petot, Frédérique
name: Projet CBMA
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2020
Subjects: subject: Chartes de la Bourgogne du Moyen Âge
subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris
subject: cartulaire
subject: Corpus Burgundiae Medii Aevi

description: Huitième cartulaire de Saint-Étienne de Dijon (1661-1667), Archives départementales de la Côte-d'Or, Cart. 31 (G 135), 549 folios, f. 0647, Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Huitième cartulaire de Saint-Étienne de Dijon (1661-1667), Archives départementales de la Côte-d'Or, Cart. 31 (G 135), 549 folios, f. 0647, in Projet CBMA - Corpus Burgundiae Medii Aevi [Ressource en ligne], https://manuscrits.cbma-project.eu/
description: Provenance: abbaye Saint-Étienne de Dijon
description: Provenance: http://www.wikidata.org/entity/Q15945019
The Physics of Z' bosons
Creators: name: del Aguila, F.
Publisher: name: arXiv
Year: 1994
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: In these lectures we review the simplest gauge extensions of the standard model, and the present and future limits on new weak interactions.
description: 17 UG-FT-35/94
Massive Stars: Their Environment and Formation
Creators: name: Garay, Guido
name: Lizano, Susana
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Cloud environment is thought to play a critical role in determining the mechanism of formation of massive stars. In this contribution we review the physical characteristics of the environment around recently formed massive stars. Particular emphasis is given to recent high angular resolution observations which have improved our knowledge of the physical conditions and kinematics of compact regions of ionized gas and of dense and hot molecular cores associated with luminous O and B stars. We will show that this large body of data, gathered during the last decade, has allowed significant progress in the understanding of the physical processes that take place during the formation and early evolution of massive stars.
description: Pub. Astron. Soc. of Pacific (Invited Review), 95 pages (Latex), 5 pages (tables, Latex), 11 postscript or gif figures
Eon Reverser Toward Temporal Bubble Radio Communication
Creators: name: Cacci, Marco
Publisher: name: Zenodo
Year: 2025

description: The Eon Reverser is your concept of an entropy bomb capable of manipulating spacetime locally but also on a planetary scale. The idea revolves around controlled time reversal effects, but only within a limited window-minutes or hours-to prevent catastrophic paradoxes or collapses in causality. At its core, the Eon Reverser operates by leveraging a mix of antimatter-based energy systems, exotic field interactions, and possibly even tachyonic resonance phenomena to induce localized temporal reversals. It's not about breaking causality entirely but rather about selectively rewinding events in a controlled manner.
A Comprehensive Spectral and Variability Study of Narrow-Line Seyfert 1 Galaxies Observed by ASCA: I. Observations and Time Series Analysis
Creators: name: Leighly, Karen M.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: (Abridged) I present a comprehensive and uniform analysis of 25 {\it ASCA} observations from 23 Narrow-line Seyfert 1 galaxies. The time series analysis is presented in this paper, Part 1, and the spectral analysis and correlations are presented in the companion paper, Part 2.
description: 51 pages, 32 figures, accepted for publication in ApJS. Report also available also at http://www.astro.columbia.edu/~leighly/research.html
The Proximal Chiral Phase Transition
Creators: name: Kapusta, Joseph I.
name: Srivastava, Ajit M.
Publisher: name: arXiv
Year: 1994
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: Nuclear Theory (nucl-th)
subject: FOS: Physical sciences

description: We consider the form of the chiral symmetry breaking piece of the effective potential in the linear sigma model. Surprisingly, it allows for a second local minimum at both zero and finite temperature. Even though chiral symmetry is not exact, and therefore is not restored in a true phase transition at finite temperature, this second minimum can nevertheless mimic many of the effects of a first order phase transition. We derive a lower limit on the height of the second minimum relative to the global minimum based on cosmological considerations; this limit is so weak as to be practically nonexistent. In high energy nuclear collisions, it may lead to observable effects in Bose-Einstein interferometry due to domain walls and to coherent pion emission.
description: 21 pages (LATEX), 6 figures in postscript (uuencoded, compressed tar file included at the end of the paper), NSF-ITP-94-28, NUC-MINN-94/3-T
Snapping of Bistable, Prestressed Cylindrical Shells
Creators: name: Jiang, Xin
name: Pezzulla, Matteo
name: Shao, Huiqi
name: Ghosh, Tushar K.
name: Holmes, Douglas P.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Soft Condensed Matter (cond-mat.soft)
subject: FOS: Physical sciences

description: Bistable shells can reversibly change between two stable configurations with very little energetic input. Understanding what governs the shape and snap-through criteria of these structures is crucial for designing devices that utilize instability for functionality. Bistable cylindrical shells fabricated by stretching and bonding multiple layers of elastic plates will contain residual stress that will impact the shell's shape and the magnitude of stimulus necessary to induce snapping. Using the framework of non-Euclidean shell theory, we first predict the mean curvature of a nearly cylindrical shell formed by arbitrarily prestretching one layer of a bilayer plate with respect to another. Then, beginning with a residually stressed cylinder, we determine the amount of the stimuli needed to trigger the snapping between two configurations through a combination of numerical simulations and theory. We demonstrate the role of prestress on the snap-through criteria, and highlight the important role that the Gaussian curvature in the boundary layer of the shell plays in dictating shell stability.
description: 8 pages, 8 figures
Quantum friction between oscillating crystal slabs: Graphene monolayers on dielectric substrates
Creators: name: Despoja, Vito
name: Echenique, Pedro M.
name: Sunjic, Marijan
Publisher: name: arXiv
Year: 2018
Subjects: subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: Materials Science (cond-mat.mtrl-sci)
subject: FOS: Physical sciences

description: We present a theoretical description of energy transfer processes between two noncontact quasi- twodimensional crystals separated by distance a, oscillating with frequency omega0 and amplitude rho0 , and compare it with the case of two quasi-twodimensional crystals in uniform parallel motion. We apply the theory to calculate van der Waals energy and dissipated energy in two oscillating slabs where each slab consists of a graphene monolayer deposited on SiO2 substrate. The graphene dielectric response is determined from first principles, and SiO2 surface response is described using empirical local dielectric function. We studied the modification of vdW attraction as function of the driving frequency and graphene doping. We propose the idea of controlling the sticking and unsticking of slabs by tuning the graphene dopings EF i and driving frequency omega0 . We found simple rho02 dependence of vdW and dissipated energy. As the Dirac plasmons are the dominant channels through which the energy between slabs can be transferred, the dissipated power in equally doped EF1 = EF2 = 0 graphenes shows strong omega0 = 2omegap peak. This peak is substantially reduceed when graphenes are deposited on SiO2 substrate. If only one graphene is pristine (EFi = 0) the 2omegap peak disappears. For larger separations a the phononic losses also become important and the doping causes shifts, appearance and disappearance of many peaks originating from resonant coupling between hybridized electronic-phononic excitations in graphene-substrate slabs.
Additional file 1 of Understanding intergenerational dynamics and social support’s impact on health and well-being of older adults in South Asia: a scoping review
Creators: name: Jahangir, Selim
name: Patil, Divya Sussana
name: Gangopadhyay, Jagriti
name: Vogt, Tobias C.
Publisher: name: figshare
Year: 2025
Subjects: subject: Medicine
subject: Geology
subject: FOS: Earth and related environmental sciences
subject: Sociology
subject: FOS: Sociology
subject: Cancer
subject: Science Policy
subject: Infectious Diseases
subject: FOS: Health sciences
subject: Computational Biology

description: Additional file 1: Search strategy.
The impact of HPV genotypes on survival in HPV-positive oropharyngeal squamous cell carcinomas: a systematic review
Creators: name: Skovvang, Anne
name: Jensen, Jakob Schmidt
name: Garset-Zamani, Martin
name: Carlander, Amanda
name: Grønhøj, Christian
name: von Buchwald, Christian
Publisher: name: Taylor & Francis
Year: 2021
Subjects: subject: Biotechnology
subject: Immunology
subject: FOS: Clinical medicine
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: Cancer
subject: Science Policy
subject: 110309 Infectious Diseases
subject: FOS: Health sciences

description: Patients with HPV-positive (HPV+) oropharyngeal squamous cell carcinomas (OPSCCs) are known to have a better prognosis compared to patients with HPV-negative OPSCCs. To investigate the impact of specific HPV genotypes on survival in HPV + OPSCC. A systematic search of PubMed and Embase for studies addressing the association between specific HPV genotypes and survival among patients with OPSCC was performed. Six studies (n = 1385 patients) published between 2013 and 2017 were included. Five studies (n = 1290 patients) found a better survival among HPV16 cases compared to other high-risk (HR) HPV genotypes (HPV 33, 18, 35, 31, 39, 52, 59, 45, 56, 67, 29, and 58), of which three studies (n = 933 patients) reached significant results. Two of these studies reported a five-year overall survival (OS) of 64.6% and 71.4% in HPV16 OPSCCs vs. 45.6% and 57.1% in HR non-HPV16 OPSCCs (p = .001 and p = .010, respectively), and the last study found a better OS among HPV16 cases with a hazard ratio (HR) of 0.35, 95%. CI [0.14;0.85], p = .02. Our findings indicate a favorable prognosis among patients with HPV16 OPSCC compared with HR non-HPV16 OPSCC. These results may be important when designing future trials and in the planning of follow-up regimes.
Standard map-like models for single and multiple walkers in an annular cavity
Creators: name: Rahman, Aminur
Publisher: name: arXiv
Year: 2018
Subjects: subject: Chaotic Dynamics (nlin.CD)
subject: FOS: Physical sciences

description: Recent experiments on walking droplets in an annular cavity showed the existence of complex dynamics including chaotically changing velocity. This article presents models, influenced by the kicked rotator/standard map, for both single and multiple droplets. The models are shown to achieve both qualitative and quantitative agreement with the experiments, and makes predictions about heretofore unobserved behavior. Using dynamical systems techniques and bifurcation theory, the single droplet model is analyzed to prove dynamics suggested by the numerical simulations.
description: 22 pages, 22 figures
Alcubierre-Cacci A New Frontier for Spacetime Propulsion and Interstellar Travel
Creators: name: Cacci, Marco
Publisher: name: Zenodo
Year: 2025

description: The Alcubierre-Cacci Drive represents an innovative theoretical advancement in faster-than-light propulsion, combining Alcubierre’s concept of spacetime curvature with novel enhancements for improved efficiency and stability. This model leverages the manipulation of spacetime through negative energy densities and exotic materials, hypothesizing a practical pathway for superluminal travel while minimizing the energy requirements traditionally associated with warp drives. Key innovations include a refined energy distribution system and adaptive field stabilization mechanisms, designed to address quantum fluctuations and mitigate potential causality violations. The Alcubierre-Cacci Drive integrates elements of quantum field theory, general relativity, and advanced material sciences, aiming to overcome significant barriers in spacetime engineering. This proposal not only extends the theoretical foundations of warp technology but also introduces a framework for experimental validation in the future, paving the way for a transformative era of interstellar exploration.
A Comprehensive Spectral and Variability Study of Narrow-Line Seyfert 1 Galaxies Observed by ASCA: II. Spectral Analysis and Correlations
Creators: name: Leighly, Karen M.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: (Abridged) I present a comprehensive and uniform analysis of 25 {\it ASCA} observations from 23 Narrow-line Seyfert 1 galaxies. The spectral analysis and correlations are presented in this paper, Part 2; the reduction and time series analysis is presented in the companion paper, Part 1.
description: 73 pages, 31 figures, accepted for publication in ApJS. Report also available at http://www.astro.columbia.edu/~leighly/research.html
АНАЛИЗ ФАРМАЦЕВТИЧЕСКОГО РЫНКА РК МЯГКИХ ЛЕКАРСТВЕННЫХ ФОРМ
Creators: name: Койлыбаева, М.К.
name: Жалғасқызы, Л.
Publisher: name: Zenodo
Year: 2024

description: Фармацевтический рынок – важнейший сектор экономики каждого государства, являющийся критерием экономического, социального развития общества и показателем уровня благосостояния населения. В фармацевтической индустрии важное внимание уделяется анализу ситуации на фармацевтическом рынке.