cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Precise Temporal Action Localization by Evolving Temporal Proposals
Creators: name: Qiu, Haonan
name: Zheng, Yingbin
name: Ye, Hao
name: Lu, Yao
name: Wang, Feng
name: He, Liang
Publisher: name: arXiv
Year: 2018
Subjects: subject: Computer Vision and Pattern Recognition (cs.CV)
subject: FOS: Computer and information sciences

description: Locating actions in long untrimmed videos has been a challenging problem in video content analysis. The performances of existing action localization approaches remain unsatisfactory in precisely determining the beginning and the end of an action. Imitating the human perception procedure with observations and refinements, we propose a novel three-phase action localization framework. Our framework is embedded with an Actionness Network to generate initial proposals through frame-wise similarity grouping, and then a Refinement Network to conduct boundary adjustment on these proposals. Finally, the refined proposals are sent to a Localization Network for further fine-grained location regression. The whole process can be deemed as multi-stage refinement using a novel non-local pyramid feature under various temporal granularities. We evaluate our framework on THUMOS14 benchmark and obtain a significant improvement over the state-of-the-arts approaches. Specifically, the performance gain is remarkable under precise localization with high IoU thresholds. Our proposed framework achieves mAP@IoU=0.5 of 34.2%.
An Ultraviolet-Selected Galaxy Redshift Survey - II: The Physical Nature of Star Formation in an Enlarged Sample
Creators: name: Sullivan, M.
name: Treyer, M. A.
name: Ellis, R. S.
name: Bridges, T. J.
name: Milliard, B.
name: Donas, J.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present further spectroscopic observations for a sample of galaxies selected in the vacuum ultraviolet (UV) at 2000 Åfrom the FOCA balloon-borne imaging camera of Milliard et al. (1992). This work represents an extension of the initial study of Treyer et al. (1998). Our enlarged catalogue contains 433 sources; 273 of these are galaxies, nearly all with redshifts z=0-0.4. Nebular emission line measurements are available for 216 galaxies, allowing us to address issues of reddening and metallicity. The UV and Halpha luminosity functions strengthen our earlier assertions that the local volume-averaged star formation rate is higher than indicated from earlier surveys. Moreover, internally within our sample, we do not find a steep rise in the UV luminosity density with redshift over 0
description: 27 pages, 19 figures, accepted for publication in MNRAS
Dark-Matter Distribution inferred from High-accuracy Rotation Curves
Creators: name: Sofue, Yoshiaki
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Using high-accuracy rotation curves of spiral galaxies, we derive distributions of the surface mass density. Comparing with the luminosity profiles, we show that the dark mass in disk and bulge distributions follows those of luminous (stellar) mass, while luminous mass in halos does not follow dark mass. The dark-mass fraction (DMF) increases with the radius in the disk, and rapidly toward edge in the halo. In some galaxies, DMF increases toward the center,
description: Latex 4 pages with 5 figures; Conf. proc. "A new millennium of galaxy morphology" Johannesburg 1999 Sep
Momentum-space indirect interlayer excitons in transition metal dichalcogenide van der Waals heterostructures
Creators: name: Kunstmann, Jens
name: Mooshammer, Fabian
name: Nagler, Philipp
name: Chaves, Andrey
name: Stein, Frederick
name: Paradiso, Nicola
name: Plechinger, Gerd
name: Strunk, Christoph
name: Schüller, Christian
name: Seifert, Gotthard
name: Reichman, David R.
name: Korn, Tobias
Publisher: name: arXiv
Year: 2018
Subjects: subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: FOS: Physical sciences

description: Monolayers of transition metal dichalcogenides (TMDCs) feature exceptional optical properties that are dominated by excitons, tightly bound electron-hole pairs. Forming van der Waals heterostructures by deterministically stacking individual monolayers allows to tune various properties via choice of materials and relative orientation of the layers. In these structures, a new type of exciton emerges, where electron and hole are spatially separated. These interlayer excitons allow exploration of many-body quantum phenomena and are ideally suited for valleytronic applications. Mostly, a basic model of fully spatially-separated electron and hole stemming from the $K$ valleys of the monolayer Brillouin zones is applied to describe such excitons. Here, we combine photoluminescence spectroscopy and first principle calculations to expand the concept of interlayer excitons. We identify a partially charge-separated electron-hole pair in MoS$_2$/WSe$_2$ heterostructures residing at the $Γ$ and $K$ valleys. We control the emission energy of this new type of momentum-space indirect, yet strongly-bound exciton by variation of the relative orientation of the layers. These findings represent a crucial step towards the understanding and control of excitonic effects in TMDC heterostructures and devices.
description: Nature Physics (2018), in press [main article (letter) and Supporting Information]
Additional file 1: of Virulence-related comparative transcriptomics of infectious and non-infectious chlamydial particles
Creators: name: Beder, Thomas
name: Saluz, Hans
Publisher: name: figshare
Year: 2018
Subjects: subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Immunology
subject: FOS: Clinical medicine
subject: 69999 Biological Sciences not elsewhere classified
subject: 80699 Information Systems not elsewhere classified
subject: FOS: Computer and information sciences
subject: Marine Biology
subject: Cancer
subject: 110309 Infectious Diseases
subject: FOS: Health sciences

description: Contains supplementary figures referred to in the text. Here, raw data processing, alignment and read distribution results are shown. Furthermore, the heatmaps of differentially expressed genes in C. psittaci and C. abortus are presented in higher resolution and NCBI locus tags, gene names and the functional annotations are included. Finally, the file contains the confirmation of the RNA-seq results with RT-qPCR for dnaK, hctA, mip and omcB shared among C. psittaci, C. abortus and W. chondrophila. (PDF 3185 kb)
Additional file 9: of Transcriptional defects and reprogramming barriers in somatic cell nuclear reprogramming as revealed by single-embryo RNA sequencing
Creators: name: Liu, Yong
name: Wu, Fengrui
name: Zhang, Ling
name: Wu, Xiaoqing
name: Li, Dengkun
name: Xin, Jing
name: Xie, Juan
name: Kong, Feng
name: Wang, Wenying
name: Wu, Qiaoqin
name: Zhang, Di
name: Wang, Rong
name: Gao, Shaorong
name: Li, Wenyong
Publisher: name: figshare
Year: 2018
Subjects: subject: Biophysics
subject: Biochemistry
subject: Physical Sciences not elsewhere classified
subject: Medicine
subject: Cell Biology
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Developmental Biology
subject: Hematology
subject: Virology

description: Analysis of specific protein-protein interactions. (PDF 748 kb)
Modified Gravity (MOG) and its test on galaxy clusters
Creators: name: Nieuwenhuizen, Theodorus M.
name: Morandi, Andrea
name: Limousin, Marceau
Publisher: name: arXiv
Year: 2018
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: The MOdified Gravity (MOG) theory of J. Moffat assumes a massive vector particle which causes a repulsive contribution to the tensor gravitation. For the galaxy cluster A1689 new data for the X-ray gas and the strong lensing properties are presented. Fits to MOG are possible by adjusting the galaxy density profile. However, this appears to work as an effective dark matter component, posing a serious problem for MOG. New gas and strong lensing data for the cluster A1835 support these conclusions and point at a tendency of the gas-alone to overestimate the lensing effects in MOG theory.
description: 6 pages latex, 6 figures. MNRAS accepted
Comparative study of plasmonic antennas for strong coupling and quantum nonlinearities with single emitters
Creators: name: Rousseaux, Benjamin
name: Baranov, Denis G.
name: Käll, Mikael
name: Shegai, Timur
name: Johansson, Göran
Publisher: name: arXiv
Year: 2018
Subjects: subject: Optics (physics.optics)
subject: FOS: Physical sciences
subject: 78-02

description: Realizing strong coupling between a single quantum emitter (QE) and an optical cavity is of crucial importance in the context of various quantum optical applications. While Rabi splitting of single quantum emitters coupled to high-Q diffraction limited cavities have been reported in numerous configurations, attaining single emitter Rabi splitting with a plasmonic nanostructure is still elusive. Here, we establish the analytical condition for strong coupling between a single QE and a plasmonic nanocavity and apply it to study various plasmonic arrangements that were shown to enable Rabi splitting. We investigate numerically the optical response and the resulting Rabi splitting in metallic nanostructures such as bow-tie nanoantennas, nanosphere dimers and nanospheres on a surface and find the optimal geometries for emergence of the strong coupling regime with single QEs. We also provide a master equation approach to show the saturation of a single QE in the gap of a silver bow-tie nanoantenna. Our results will be useful for implementation of realistic quantum plasmonic nanosystems involving single QEs.
description: 9 pages, 7 figures
Entropy in the Mass-Energy Gravity Model: Energy Redistribution, Equilibrium, and the Nature of Disorder
Creators: name: Shreenan-Dyck, Chris
Publisher: name: figshare
Year: 2025
Subjects: classificationCode: 490203
subject: Mathematical aspects of classical mechanics, quantum mechanics and quantum information theory

description: This paper extends the Mass-Energy Gravity (MEG) model by redefining entropy as a process of energy redistribution rather than a universal increase in disorder. In MEG, entropy is not driven by an absolute arrow of time but emerges from the way energy-density gradients (EDGs) dissipate over cosmic scales. This perspective challenges traditional thermodynamic interpretations by suggesting that entropy evolution depends on local energy conditions rather than a fixed time progression.We explore how entropy influences cosmic structure formation, its role in black hole dynamics, and whether mass-energy can ever reach true equilibrium. Unlike conventional models predicting inevitable heat death, MEG suggests that entropy’s behavior varies based on EDGs, allowing for persistent large-scale structures.Finally, we propose observational tests to distinguish MEG’s entropy framework from standard thermodynamic models, including studies of black hole entropy limits, cosmic microwave background (CMB) fluctuations, and energy redistribution in large-scale structures.This work provides a novel perspective on entropy’s role in the universe, bridging gravitational dynamics, cosmology, and thermodynamics under a single, unified framework.
Vacuum oscillation solution to the solar neutrino problem in standard and non-standard pictures
Creators: name: Berezhiani, Z.
name: Rossi, A.
Publisher: name: arXiv
Year: 1994
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: The neutrino long wavelength (just-so) oscillation is revisited as a solution to the solar neutrino problem. We consider just-so scenario in various cases: in the framework of the solar models with relaxed prediction of the boron neutrino flux, as well as in the presence of the non-standard weak range interactions between neutrino and matter constituents. We show that the fit of the experimental data in the just-so scenario is not very good for any reasonable value of the $^8B$ neutrino flux, but it substantially improves if the non-standard $τ$-neutrino--electron interaction is included. These new interactions could also remove the conflict of the just-so picture with the shape of the SN 1987A neutrino spectrum. Special attention is devoted to the potential of the future real-time solar neutrino detectors as are Super-Kamiokande, SNO and BOREXINO, which could provide the model independent tests for the just-so scenario. In particular, these imply specific deformation of the original solar neutrino energy spectra, and time variation of the intermediate energy monochromatic neutrino ($^7Be$ and $pep$) signals.
description: Latex, 14 pages, 9 figures (avalilable by fax or postscript files requested to Rossi@fe.infn.it) -- some textual and Latex errors are corrected and few references added
title: ADCO, Cart. 186 (11 H 71), f. 0299v
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: Chartes de la Bourgogne du Moyen Âge
subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris
subject: cartulaire
subject: Corpus Burgundiae Medii Aevi

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. 0299v, in Projet CBMA - Corpus Burgundiae Medii Aevi [Ressource en ligne], https://manuscrits.cbma-
project.eu/
description: Provenance: abbaye de Cîteaux
description: Provenance: http://www.wikidata.org/entity/Q843261
description: Provenance: https://www.geonames.org/3024876
description: Provenance: http://www.idref.fr/030974844/id
description: Provenance: https://catalogue.bnf.fr/ark:/12148/cb12228351v
Additional file 1: of Impact of oropharyngeal dysphagia on healthcare cost and length of stay in hospital: a systematic review
Creators: name: Attrill, Stacie
name: Sarahlouise White
name: Murray, Joanne
name: Hammond, Sue
name: Doeltgen, Sebastian
Publisher: name: figshare
Year: 2018
Subjects: subject: Medicine
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: 80699 Information Systems not elsewhere classified
subject: FOS: Computer and information sciences
subject: Developmental Biology
subject: Science Policy

description: Search terms. (DOCX 20 kb)
What is quantum in quantum randomness?
Creators: name: Grangier, Philippe
name: Auffèves, Alexia
Publisher: name: arXiv
Year: 2018
Subjects: subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: It is often said that quantum and classical randomness are of different nature, the former being ontological and the latter epistemological. However, so far the question of "What is quantum in quantum randomness", i.e. what is the impact of quantization and discreteness on the nature of randomness, remains to answer. In a first part, we explicit the differences between quantum and classical randomness within a recently proposed ontology for quantum mechanics based on contextual objectivity. In this view, quantum randomness is the result of contextuality and quantization. We show that this approach strongly impacts the purposes of quantum theory as well as its areas of application. In particular, it challenges current programs inspired by classical reductionism, aiming at the emergence of the classical world from a large number of quantum systems. In a second part, we analyze quantum physics and thermodynamics as theories of randomness, unveiling their mutual influences. We finally consider new technological applications of quantum randomness opened in the emerging field of quantum thermodynamics.
description: This article will appear in Philosophical Transaction A, following the Royal Society Symposium "Foundations of quantum mechanics and their impact on Contemporary Society"
The effects of resistivity on oscillatory reconnection and consequences for solar flare Quasi Periodic Pulsations
Creators: name: Schiavo, Luiz A. C. A.
name: Stewart, James
name: Browning, Philippa K.
Publisher: name: arXiv
Year: 2024
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: Plasma Physics (physics.plasm-ph)
subject: Space Physics (physics.space-ph)
subject: FOS: Physical sciences

description: Quasi-periodic pulsations (QPPs) are often observed in flare emissions. While these may reveal much about the time-dependent reconnection involved in flare energy release, the underlying mechanisms are still poorly understood. In this paper, we use 2D magnetohydrodynamic simulations to investigate the magnetic reconnection in two merging flux ropes, focusing on the effects of the resistivity on the time variation of the reconnection. We consider both uniform resistivity and current-dependent anomalous resistivity profiles. Our findings reveal that resistivity plays a critical role in controlling the reconnection dynamics, including reconnection rate oscillations and the rate of decay of the reconnection rate. Resistivity also influences the oscillations in emitted gyrosynchrotron radiation. However, in contrast to this strong influence of resistivity on reconnection rates, we observed a different behaviour for the emitted waves, whose frequencies are almost independent of resistivity variations.
MOESM1 of Microbial communities and inflammatory response in the endometrium differ between normal and metritic dairy cows at 5–10 days post-partum
Creators: name: Sicsic, Ron
name: Goshen, Tamir
name: Dutta, Rahul
name: Kedem-Vaanunu, Noa
name: Kaplan-Shabtai, Veronica
name: Pasternak, Zohar
name: Gottlieb, Yuval
name: Shpigel, Nahum
name: Raz, Tal
Publisher: name: figshare
Year: 2018
Subjects: subject: Medicine
subject: Physiology
subject: FOS: Biological sciences
subject: Sociology
subject: FOS: Sociology
subject: Immunology
subject: FOS: Clinical medicine
subject: 69999 Biological Sciences not elsewhere classified
subject: 80699 Information Systems not elsewhere classified
subject: FOS: Computer and information sciences
subject: Science Policy

description: Additional file 1. Reproductive performance of healthy and metritic cows. Reproductive management was based on artificial insemination (AI) with thawed-frozen semen from proven sires. AI was performed by highly trained technicians employed by Sion LTD., Israel’s leading company for dairy cow Artificial Insemination Service. Cows were bred on spontaneous estrus observed or detected by computerized pedometry system. Estrus was confirmed by trans-rectal palpation of the reproductive tract at the time of AI. For pregnancy diagnosis, trans-rectal palpation of the uterus was performed at 40–50 days post-insemination. Reproductive performance parameters included the following: number of AI to conception, open days (days from parturition to conception), waste days (days from first AI to AI leading to conception; i.e., equals 0 if cow is pregnant from first AI), and pregnancy rate at 180 DIM. Data were analyzed by Wilcoxon rank sum test, or a Pearson’s Chi square test analysis (to compare pregnancy rate at 180 DIM). Values presented in the table are mean ± SEM for each group, or percentages (%).
Simulating the Electroweak Phase Transition in the SU(2) Higgs Model
Creators: name: Fodor, Z.
name: Hein, J.
name: Jansen, K.
name: Jaster, A.
name: Montvay, I.
Publisher: name: arXiv
Year: 1994
Subjects: subject: High Energy Physics - Lattice (hep-lat)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: Numerical simulations are performed to study the finite temperature phase transition in the SU(2) Higgs model on the lattice. In the presently investigated range of the Higgs boson mass, below 50 GeV, the phase transition turns out to be of first order and its strength is rapidly decreasing with increasing Higgs boson mass. In order to control the systematic errors, we also perform studies of scaling violations and of finite volume effects.
description: 46 pages with 16 figures, DESY-94-159
The Fornax Cluster VLT Spectroscopic Survey II - Planetary Nebulae kinematics within 200 kpc of the cluster core
Creators: name: Spiniello, C.
name: Napolitano, N. R.
name: Arnaboldi, M.
name: Tortora, C.
name: Coccato, L.
name: Capaccioli, M.
name: Gerhard, O.
name: Iodice, E.
name: Spavone, M.
name: Cantiello, M.
name: Peletier, R.
name: Paolillo, M.
name: Schipani, P.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: We present the largest and most spatially extended planetary nebulae (PNe) catalog ever obtained for the Fornax cluster. We measured velocities of 1452 PNe out to 200 kpc in the cluster core using a counter-dispersed slitless spectroscopic technique with data from FORS2 on the VLT. With such extended spatial coverage, we can study separately the stellar halos of some of the cluster main galaxies and the intracluster light. In this second paper of the Fornax Cluster VLT Spectroscopic Survey (FVSS), we identify and classify the emission-line sources, describe the method to select PNe and calculate their coordinates and velocities from the dispersed slitless images. From the PN 2D velocity map we identify stellar streams that are possibly tracing the gravitational interaction of NGC1399 with NGC1404 and NGC1387. We also present the velocity dispersion profile out to $\sim 200$ kpc radii, which shows signatures of a superposition of the bright central galaxy and the cluster potential, with the latter clearly dominating the regions outside R $\sim 1000$" ($\sim 100$ kpc).
description: 13 pages, 8 figures, Accepted for publication in MNRAS, companion paper FVSS-I (Pota et al, 2018, submitted)
title: ADCO, Cartulaire général de Cîteaux, dit de Jean de Cirey, (XVe siècle), tome III, Cart. 187 (11 H 72), f. 0120r
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: Corpus Burgundiae Medii Aevi
subject: Chartes de la Bourgogne du Moyen Âge
subject: cartulaire

description: Cartulaire général de Cîteaux, dit de Jean de Cirey, (XVe siècle), tome III, Archives départementales de la Côte-d'Or, Cart. 187 (11 H 72), f. 0120r, Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Cartulaire général de Cîteaux, dit de Jean de Cirey, (XVe siècle), tome III, Archives départementales de la Côte-d'Or, Cart. 187 (11 H 72), f. 0120r, 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
O'ZBEKISTONDA RAQAMLI IQTISODIYOTNI RIVOJLANTIRISH TENDENSIYALARI: XALQARO TAJRIBALAR VA MAVJUD MUAMMOLAR
Creators: name: Urinboyev, Azizbek
name: Yodgorov, Dimirbek
name: G'aniyev, Shaxzod
Publisher: name: Zenodo
Year: 2025

description: Ushbu maqolada raqamli iqtisodiyot hamda raqamli texnologiyalarning O‘zbekiston iqtisodiyoti rivojlanishida tutgan o‘rni va mamlakatimizda raqamli iqtisodiyotni rivojlantirishning asosiy tendensiyalarini, xalqaro tajribalarning mamlakatimiz uchun ahamiyatini hamda mavjud muammolarni tahlil qilishga qaratilgan. Maqolada O‘zbekistonning raqamli iqtisodiyotga jadal suratlar bilan  o‘tish jarayonida amalga oshirilgan strategiyalar, raqamli infratuzilma, e-tijorat va kriptovalyutalar sohasidagi yutuqlar, shu bilan birga, davlatning raqamli iqtisodiyotdagi roli haqida ma’lumotlar keltirilgan. Xalqaro tajribalarga, jumladan, Estoniya, Singapur va Janubiy Koreya tajribalariga tayanib, O‘zbekistonning raqamli iqtisodiyotdagi muvaffaqiyatlari va mavjud kamchiliklarini bartaraf etish imkoniyatlari ko‘rsatilgan.
Additional file 2 of m6A demethylase ALKBH5 inhibits tumor growth and metastasis by reducing YTHDFs-mediated YAP expression and inhibiting miR-107/LATS2â€“mediated YAP activity in NSCLC
Creators: name: Jin, Dan
name: Guo, Jiwei
name: Wu, Yan
name: Yang, Lijuan
name: Wang, Xiaohong
name: Du, Jing
name: Dai, Juanjuan
name: Chen, Weiwei
name: Gong, Kaikai
name: Miao, Shuang
name: Li, Xuelin
name: Sun, Hongliang
Publisher: name: figshare
Year: 2020
Subjects: Biochemistry
Molecular Biology
Pharmacology
Biological Sciences not elsewhere classified
Developmental Biology
Cancer

description: Additional file 2 Fig. S1. Ectopic expression of YAP and ALKBH5 regulates cell proliferation.
Additional file 1: of Regulatory role of heme oxygenase-1 in silica-induced lung injury
Creators: name: Nakashima, Kentaro
name: Sato, Takashi
name: Shigemori, Suguru
name: Shimosato, Takeshi
name: Shinkai, Masaharu
name: Kaneko, Takeshi
Publisher: name: figshare
Year: 2018
Subjects: subject: Biochemistry
subject: Space Science
subject: Medicine
subject: Microbiology
subject: FOS: Biological sciences
subject: Cell Biology
subject: Molecular Biology
subject: Pharmacology
subject: Biotechnology
subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences
subject: 69999 Biological Sciences not elsewhere classified
subject: Science Policy

description: Effect of ERK inhibitor on HO-1 induction in the lungs in murine silicosis.Mice were administered intraperitoneally with the ERK inhibitor, U0126, 2 h before and 6 h after 2.5 mg of silica particles instillation. A) Lung samples collected 2 days after silica instillation were analyzed as described in Fig. 2. B) Densitometric analysis of band intensity representing the mean ± SD level of HO-1 protein relative to actin (n = 3/group). Although not significant, U0126 attenuated HO-1 induction after silica exposure. * P
Accounting all contributions for the Van Vleck paramagnetism and the Langevin diamagnetism from first principles: application to diamond
Creators: name: Nikolaev, A. V.
name: Vlasov, I. I.
name: Tao, L. L.
Publisher: name: arXiv
Year: 2024
Subjects: subject: Materials Science (cond-mat.mtrl-sci)
subject: FOS: Physical sciences

description: A general method for calculating magnetic susceptibility ($χ$) in dielectrics within a single choice of magnetic gauge for the whole crystal is presented. On the basis of the method, accounting for all contributions to the Van Vleck paramagnetism and Langevin (Larmore) diamagnetism, a full-scale ab initio calculation of $χ$ in diamond is performed. Unfamiliar contributions to $χ$ includes a Van Vleck contribution from the interstitial region and an offset contribution from the muffin-tin (MT) sphere, appearing due to the change of the MT-sphere magnetic moment when the sphere is displaced from the origin. Although the Langevin diamagnetism explicitly depends on the choice of the origin, its sum with the Van Vleck term remains invariant, which is demonstrated on the basis of the gauge invariance of the magnetic vector potential. The derived expressions have been applied to ab initio calculations of magnetic susceptibility of the crystalline diamond within the linear augmented plane wave method (LAPW). With the diamond unit cell having the inversion symmetry, the magnetic (Van Vleck) calculations require the irreducible part of the Brillouin zone accounting for half of the whole zone, i.e. 24 times larger than that in the absence of magnetic field. Investigating possible anisotropy of $χ$, we calculate it for 74 different directions of H (belonging to Lebedev surface grid points), and demonstrate that the actual value of $χ$ remain isotropic. The obtained volume magnetic susceptibility in diamond lies in the range $16.27-16.72 (with the Langevin contribution -39.22-39.94 and the Van Vleck contribution -22.94-23.22), in units 10^{-7}, which compares well with the experimental data and other calculations.
MATHÉMATIQUES ET RÉALITÉ : ÉMILE MEYERSON CONTRE LE PANMATHÉMATISME
Creators: name: AKA Pancrace
Publisher: name: Zenodo
Year: 2024

description: La modernité scientifique est consubstantielle à la mathématisation progressive des sciences et de la réalité. L’usage du langage mathématique semble être la voie idéale qui s’offre au savant désireux de rechercher la vérité et d’exprimer avec exactitude, rigueur, simplicité et objectivité la matière de son étude. Le paradigme mathématique, fondé sur l’usage de symboles abstraits et de méthode rigoureuse (la démonstration), tend à l’universalité. Les mathématiques s’universalisent, en raison de l’universalité de leur discours. De Galilée à A. Comte, un nombre notable de savants et de philosophes prônent sans arrêt un panmathématisme. Le panmathématisme est la tendance à faire prévaloir les méthodes mathématiques dans tous les domaines de la connaissance et dans la connaissance de l’univers. Toutefois, É. Meyerson s’insurge contre le panmathématisme ou l’idéal mathématique qui est mis en œuvre dans les sciences expérimentales. L’objectif de ce travail est de montrer qu’au sein de son épistémologie réaliste, la qualité joue un rôle prépondérant dans la science, en ce sens qu’elle nous éclaire sur son but véritable. Au cours de son investigation dans le labyrinthe des phénomènes naturels, le savant s’intéresse, dans un premier temps, à tout ce qui a trait à la qualité de la réalité et dans un second temps, il cherche à la quantifier, en empruntant aux mathématiques leur symbole, nombre, figure et méthode.
The impact hazard from small asteroids: current problems and open questions
Creators: name: Foschini, Luigi
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: The current philosophy of impact hazard considers the danger from small asteroids negligible. However, several facts claim for a revision of this philosophy. In this paper, some of these facts are reviewed and discussed. It is worth noting that while the impact frequency of Tunguska-like objects seems to be higher than previously estimated, the atmospheric fragmentation is more efficient than commonly thought. Indeed, data recorded from airbursts show that small asteroids breakup at dynamical pressures lower than their mechanical strength. This means that theoretical models are inconsistent with observations and new models and data are required in order to understand the phenomena.
description: 14 pages; no figures. To appear on the Proceedings of the Third National Meeting of Planetary Sciences (Bormio, Italy, January 24-30, 2000). Invited talk
Perturbative versus Lattice QCD Energy Density Correlators at High Temperatures
Creators: name: Rischke, Dirk H.
name: Gyulassy, Miklos
Publisher: name: arXiv
Year: 1994
Subjects: subject: Nuclear Theory (nucl-th)
subject: High Energy Physics - Lattice (hep-lat)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: Correlators of magnetic and electric field energy density are investigated for SU($N_c$) gauge theory at high temperatures $T$. At separations $z\leq 2/T$ the correlators are shown to be dominated by a power--law behavior even for finite gluon screening masses. This continuum behavior is well approximated on current $4\times 16^3$--lattices in the perturbative limit and leads to a considerable overestimate of screening masses deduced from fitting the lattice correlators with conventional exponential forms. The use of extended sources and sinks to enhance the signal improves the situation for screening masses $m\gg T$ but leads to a largely uncontrolled error for masses less than $T$. In fact, we show that recent lattice QCD data of Grossmann et al., from which a magnetic screening mass $m_M \approx 2.9 \, T$ was deduced, may even be consistent with a vanishing actual magnetic screening mass.
description: 23 pages, 10 figures (uuencoded), preprint CU-TP-639
The Massive Star-Forming Regions Omnibus X-Ray Catalog, Second Installment
Creators: name: Townsley, Leisa K.
name: Broos, Patrick S.
name: Garmire, Gordon P.
name: Anderson, Gemma E.
name: Feigelson, Eric D.
name: Naylor, Tim
name: Povich, Matthew S.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: Astrophysics of Galaxies (astro-ph.GA)
subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: We present the second installment of the Massive Star-forming Regions (MSFRs) Omnibus X-ray Catalog (MOXC2), a compilation of X-ray point sources detected in Chandra/ACIS observations of 16 Galactic MSFRs and surrounding fields. MOXC2 includes 13 ACIS mosaics, three containing a pair of unrelated MSFRs at different distances, with a total catalog of 18,396 point sources. The MSFRs sampled range over distances of 1.3 kpc to 6 kpc and populations varying from single massive protostars to the most massive Young Massive Cluster known in the Galaxy. By carefully detecting and removing X-ray point sources down to the faintest statistically-significant limit, we facilitate the study of the remaining unresolved X-ray emission. Through comparison with mid-infrared images that trace photon-dominated regions and ionization fronts, we see that the unresolved X-ray emission is due primarily to hot plasmas threading these MSFRs, the result of feedback from the winds and supernovae of massive stars. The 16 MSFRs studied in MOXC2 more than double the MOXC1 sample, broadening the parameter space of ACIS MSFR explorations and expanding Chandra's substantial contribution to contemporary star formation science.
description: 60 pages, 24 figures. Accepted by ApJS. Figures have been significantly downgraded to meet arXiv requirements. See https://doi.org/10.5281/zenodo.1067748 for higher-resolution versions of this paper and for supplemental data products
title: ADCO, Ordre cistercien : comptes (1499-1515) (11 H 1162), f. 00417
Creators: name: de la Côte-d'Or, Archives départementales
name: Archives Départementales De La Côte-D'Or
name: Petot, Frédérique
name: Projet CBMA
name: CBMA/CG21/F.PETOT/2019
name: Petot, Frédéric
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2020
Subjects: subject: Corpus Burgundiae Medii Aevi
subject: Chartes de la Bourgogne du Moyen Âge
subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris
subject: comptes

description: Ordre cistercien : 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. 00417, 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
Načrti za podatke o obnovljivih materialih in produktih
Creators: name: Slavec, Ana
Publisher: name: Zenodo
Year: 2019
Subjects: data management
upravljanje podatkov
renewable materials
obnovljivi materiali

description: InnoRenew CoE Center odličnosti za raziskave in inovacije na področju obnovljivih materialov in zdravega bivanjskega okolja je neodvisni raziskovalni inštitut, ki je bil ustanovljen februarja 2017 in je eden izmed devetih partnerjev v projektu InnoRenew v okviru programa Obzorja 2020 (H2020 WIDESPREAD-2-Teaming: #739574). Inštitut ima šest raziskovalnih skupin, ki pokrivajo zelo različna področja – od lesarstva, gradbeništva in kemije do računalništva, psihologije in drugih družbenih ved. Ker je projekt vključen v program Pilot odprtih raziskovalnih podatkov Obzorja 2020, smo septembra 2017 pripravil Načrta upravljanja z raziskovalnimi podatki na inštitutu InnoRenew CoE in partnerjev v projektu InnoRenew. Načrt sledi smernicam upravljanja raziskovalnih podatkov po načelih FAIR (najdljivost, dostopnost, interoperabilnost in ponovna uporabnost) in vključuje tudi poglavja o varstvu podatkov ter o pravnih in etičnih vidikih, saj se v določenih raziskavah zbirajo tudi raziskovalni podatki o ljudeh. Pri teh raziskavah je treba upoštevati še dodatno etično presojo raziskovalnih načrtov, ocenjevanje tveganj pri zbiranju podatkov ter Splošno uredbo o varstvu podatkov (GDPR). Večji del raziskav inštituta in projekta pa predstavljajo raziskave na področju tehnike, predvsem raziskave o obnovljivih materialih in proizvodih, kjer so izzivi upravljanja z raziskovalnimi podatki drugačni kot v družboslovnih raziskavah. Kot ambasadroka Združenja za raziskovalne podatke za področje tehnike – obnovljivih materialov sem ugotovila, da sta glavna tehnična izziva pomanjkanje standardov za metapodatke in ontologije ter pomanjkanje področnih repozitorijev, socialni izzivi pa strah pred izgubo konkurenčne prednosti, strah pred zlorabami in napačnimi interpretacijami podatkov ter nenaklonjenost industrijskih partnerjev do izmenjave podatkov. Na vseh področjih, tako naravoslovnih kot družboslovnih, pa sta izziv slaba seznanjenost raziskovalcev z načeli FAIR in pomanjkanje veščin, potrebnih za upravljanje raziskovalnih podatkov, zato naši načrti za prihodnje delo vključujejo izobraževalne delavnice in seminarje za raziskovalce. Pri sodelovanju z delovnimi skupinami RDA pa se bomo lotili tudi tehničnih ovir, kot so pomanjkanje metapodatkovnih shem in področnih repozitorijev.
Thermal photon production in high-energy nuclear collisions
Creators: name: Neumann, John J.
name: Seibert, David
name: Fai, George
Publisher: name: arXiv
Year: 1994
Subjects: subject: Nuclear Theory (nucl-th)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We use a boost-invariant one-dimensional (cylindrically symmetric) fluid dynamics code to calculate thermal photon production in the central rapidity region of S+Au and Pb+Pb collisions at SPS energy ($\sqrt{s}=20$ GeV/nucleon). We assume that the hot matter is in thermal equilibrium throughout the expansion, but consider deviations from chemical equilibrium in the high temperature (deconfined) phase. We use equations of state with a first-order phase transition between a massless pion gas and quark gluon plasma, with transition temperatures in the range $150 \leq T_c \leq 200$ MeV.
description: revised, now includes a_1 contribution. revtex, 10 pages plus 4 figures (uuencoded postscript)
Gamma-ray emission from novae related to positron annihilation: constraints on its observability posed by new experimental nuclear data
Creators: name: Hernanz, M.
name: Jose, J.
name: Coc, A.
name: Gomez-Gomar, J.
name: Isern, J.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Classical novae emit gamma-ray radiation at 511 keV and below, with a cut-off at around (20-30) keV, related to positron annihilation and its Comptonization in the expanding envelope. This emission has been elusive up to now, because it occurs at epochs well before the maximum in optical luminosity, but it could be detected by some sensitive intrument on board a satellite, provided that the nova is close enough and that it is observed at the right moment. The detection of this emission, which is a challenge for the now available and for the future gamma-ray instruments, would shed light into the physical processes occurring in the early phases of the explosion, which are invisible in other lower energy ranges. A good prediction of the emitted fluxes and of the corresponding detectability distances with different instruments relies critically on a good knowledge of reaction rates relevant to f18 destruction, which have been subject to a strong revision after recent nuclear spectroscopy measurements. With respect to previous results, smaller ejected masses of f18 are predicted, leading to smaller emitted fluxes in the (20-511) keV range and shorter detectability distances.
description: 9 pages, 2 figures, accepted for publication in Astrophys. J. Letters
Additional file 1: of Circulating levels of P-selectin and E-selectin relate to cardiovascular magnetic resonance-derived aortic characteristics in young adults from the general population, a cross-sectional study
Creators: name: Eikendal, Anouk
name: Bots, Michiel
name: Gohar, Aisha
name: Lutgens, Esther
name: Imo Hoefer
name: Ruijter, Hester Den
name: Leiner, Tim
Publisher: name: figshare
Year: 2018
Subjects: subject: Space Science
subject: Medicine
subject: 59999 Environmental Sciences not elsewhere classified
subject: FOS: Earth and related environmental sciences
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: Science Policy

description: Appendix 1. Characteristics of study population (N = 131). Appendix 2. MR Imaging parameters of 3D-T1-BB-VISTA and velocity encoded sequences. Appendix 3. Relation of circulating endothelial CAMs with aortic characteristics stratified for current/former smoking and never smoking. (DOCX 30 kb)
Steady distribution of the incremental model for bacteria proliferation
Creators: name: Gabriel, Pierre
name: Martin, Hugo
Publisher: name: arXiv
Year: 2018
Subjects: subject: Analysis of PDEs (math.AP)
subject: FOS: Mathematics
subject: 35Q92, 35P05, 45K05, 45P05, 92D25, 35A22, 35B40, 35B65

description: We study the mathematical properties of a model of cell division structured by two variables, the size and the size increment, in the case of a linear growth rate and a self-similar fragmentation kernel. We first show that one can construct a solution to the related two dimensional eigenproblem associated to the eigenvalue 1 from a solution of a certain one dimensional fixed point problem. Then we prove the existence and uniqueness of this fixed point in the appropriate $\mathrm{L}^1$ weighted space under general hypotheses on the division rate. Knowing such an eigenfunction proves useful as a first step in studying the long time asymptotic behaviour of the Cauchy problem.
description: 18 pages, 3 figures
Magnetic field topology from non-force free extrapolation and magnetohydrodynamic simulation of its eventual dynamics
Creators: name: Nayak, Sushree S.
name: Bhattacharyya, R.
name: Prasad, A.
name: Hu, Qiang
Publisher: name: arXiv
Year: 2018
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: Magnetic reconnections (MRs) for various magnetic field line (MFL) topologies are believed to be the initiators of various solar eruptive events like flares and coronal mass ejections (CMEs). Consequently, important is a thorough understanding and quantification of the MFL topology and their evolution which leads to MRs. Contemporary standard is to extrapolate the coronal MFLs using equilibrium models where the Lorentz force on the coronal plasma is zero everywhere, because either there is no current or the current is parallel to the magnetic field. In tandem, a non-force-free-field (NFFF) extrapolation scheme has evolved and allows for a Lorentz force which is non-zero only at the photosphere but asymptotically vanishes with height. The paper reports magnetohydrodynamic (MHD)- simulations initiated by NFFF extrapolation of the coronal MFLs for the active region NOAA 11158. Interestingly, quasi-separatrix layers (QSLs) which facilitate MRs are detected in the extrapolated MFLs. The AR 11158 is flare producing and, the paper makes an attempt to asses the role of QSLs in the flare onsets.
description: Proc. IAU Symp. 340. 2 pages, 3 figures, accepted for publication
Real-time Sub-milliwatt Epilepsy Detection Implemented on a Spiking Neural Network Edge Inference Processor
Creators: name: Lia, Ruixin
name: Zhaoa, Guoxu
name: Muir, Dylan Richard
name: Ling, Yuya
name: Burelo, Karla
name: Khoei, Mina
name: Wang, Dong
name: Xing, Yannan
name: Qiao, Ning
Publisher: name: arXiv
Year: 2024
Subjects: subject: Signal Processing (eess.SP)
subject: Artificial Intelligence (cs.AI)
subject: Machine Learning (cs.LG)
subject: Neural and Evolutionary Computing (cs.NE)
subject: Neurons and Cognition (q-bio.NC)
subject: FOS: Electrical engineering, electronic engineering, information engineering
subject: FOS: Computer and information sciences
subject: FOS: Biological sciences

description: Analyzing electroencephalogram (EEG) signals to detect the epileptic seizure status of a subject presents a challenge to existing technologies aimed at providing timely and efficient diagnosis. In this study, we aimed to detect interictal and ictal periods of epileptic seizures using a spiking neural network (SNN). Our proposed approach provides an online and real-time preliminary diagnosis of epileptic seizures and helps to detect possible pathological conditions.To validate our approach, we conducted experiments using multiple datasets. We utilized a trained SNN to identify the presence of epileptic seizures and compared our results with those of related studies. The SNN model was deployed on Xylo, a digital SNN neuromorphic processor designed to process temporal signals. Xylo efficiently simulates spiking leaky integrate-and-fire neurons with exponential input synapses. Xylo has much lower energy requirments than traditional approaches to signal processing, making it an ideal platform for developing low-power seizure detection systems.Our proposed method has a high test accuracy of 93.3% and 92.9% when classifying ictal and interictal periods. At the same time, the application has an average power consumption of 87.4 uW(IO power) + 287.9 uW(computational power) when deployed to Xylo. Our method demonstrates excellent low-latency performance when tested on multiple datasets. Our work provides a new solution for seizure detection, and it is expected to be widely used in portable and wearable devices in the future.
A homogeneous study of the s-process in the 21mic carbon-rich post-AGB objects
Creators: name: Van Winckel, H.
name: Reyniers, M.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present in this paper a homogeneous photospheric abundance study, on the basis of the analysis of high resolution optical spectra, of six post-AGB objects displaying a 21mic circumstellar dust feature in their IR spectrum. The F-G spectral type of the 21mic stars make that a large range of elements including a wide variety of s-process elements, can be studied by their atomic lines. The high C/O-ratios together with the large overabundance of s-process elements prove that the objects are descendants of field carbon stars. We discuss in detail the s-process abundance distribution displayed by these 21mic stars and conclude that the 3rd dredge-up efficiency is closely related to the strength of the integrated neutron irradiation. The expected anti-correlation of the neutron irradiation with metallicity, on the other hand, contains a large intrinsic scatter. Finally we compare our results with other intrinsic and extrinsic s-process enriched objects and conclude that the post-AGB stars offer very useful complementary data to constrain the evolutionary models of AGB nucleosynthesis and dredge-up processes.
description: 16 pages, 10 figures, accepted for publication in Astronomy and Astrophysics