cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Odontomachus assiniensis subsp. fauconneti Forel, 1910, n. subsp.
Creators: name: Forel, A.
Publisher: name: Zenodo
Year: 1910
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hymenoptera
Formicidae
Odontomachus
Odontomachus assiniensis
Odontomachus assiniensis em. subsp. fauconneti

description: Odontomachus assiniensis Em. subsp. Fauconneti n. subsp. -
[[worker]]. - Long. 8,5 a 11 mill. - Beaucoup plus etroit et grele que le type de l'espece. Mandibules plus courbees en dedans, avec les deux dents apicales pointues, et la 3 me seule tronquee. Brun; pattes, thorax, mandibules, funicules, base et lisiere posterieure des segments abdominaux d'un jaune un peu roussatre, sauf le dos du thorax qui est brunatre. La base de l' ecaille est aussi jaunatre. Du reste comme le type de l'espece.
La difference la plus frappante est l'etroitesse de la tete, du thorax et de l'abdomen. La largeur de la tete est de 1,7 mill. (2,2 chez le type), du pronotum 0,9 (1,4 chez le type), de l'abdomen 1,3 (1,5 chez le type ou il est tres ratatine, tandis que chez les exemplaires du Fauconneti il est assez distendu).
Bakaie, entre Nyangwe et Stanleyville, Haut-Congo, recolte par M. Fauconnet. M. Fauconnet a trouve le veritable assiniensis dans les memes parages.
description: Published as part of Forel, A., 1910, Glanures myrmecologiques., pp. 6-32 in Annales de la Societe Entomologique de Belgique 54 on page 22
NuSTAR observations of the ultraluminous X-ray source M33 X-8: a black hole in a very high state?
Creators: name: Krivonos, Roman
name: Sazonov, Sergey
name: Tsygankov, Sergey
name: Poutanen, Juri
Publisher: name: arXiv
Year: 2018
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: The closest known ultraluminous X-ray source (ULX), M33 X-8, has been recently observed with NuSTAR during its Extragalactic Legacy program, which includes a hard X-ray survey of the M33 galaxy. We present results of two long observations of M33 taken in 2017 March and July, with M33 X-8 in the field of view. The source demonstrates a nearly constant flux during the observations, and its 3-20 keV spectrum can be well described by two distinct components: a standard accretion disc with a temperature of ~1 keV at the inner radius and a power law with a photon index ~3, which is significantly detected up to 20 keV. There is also an indication of a high-energy cutoff in the spectrum, corresponding to a temperature of the Comptonizing medium of >10 keV. The broad-band spectral properties of M33 X-8 resemble black hole X-ray binaries in their very high states, suggesting that M33 X-8 is a black hole accreting at a nearly Eddington rate, in contrast to super-Eddington accretion believed to take place in more luminous ULXs.
Localizing Gravity on a String-Like Defect in Six Dimensions
Creators: name: Gherghetta, Tony
name: Shaposhnikov, Mikhail
Publisher: name: arXiv
Year: 2000
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We present a metric solution in six dimensions where gravity is localized on a four-dimensional singular string-like defect. The corrections to four-dimensional gravity from the bulk continuum modes are suppressed by ${\cal O}(1/r^3)$. No tuning of the bulk cosmological constant to the brane tension is required in order to cancel the four-dimensional cosmological constant.
description: 9 pages, LaTeX ; v2: several equations corrected; v3: minor typos corrected, reference added, version to be published in Phys.Rev.Lett; v4: Eq.(16) modified
Additional file 1: of Cost-effectiveness analysis of umeclidinium bromide/vilanterol 62.5/25 mcg versus tiotropium/olodaterol 5/5 mcg in symptomatic patients with chronic obstructive pulmonary disease: a Spanish National Healthcare System perspective
Creators: name: M. Driessen
name: J. Whalen
name: B. Seewoodharry Buguth
name: L. Vallejo-Aparicio
name: I. Naya
name: Y. Asukai
name: B. Alcázar-Navarrete
name: M. Miravitlles
name: F. García-Río
name: N. Risebrough
Publisher: name: figshare
Year: 2018
Subjects: subject: Medicine
subject: Ecology
subject: FOS: Biological sciences
subject: 69999 Biological Sciences not elsewhere classified
subject: Marine Biology
subject: Science Policy

description: Improvement in COPD disease factors in the model at time = 0. Description of the improvements in COPD disease factors built into the model at time 0 (i.e. the beginning of the cycle), when FEV1 benefit has been included. (DOCX 13 kb)
Additional file 8: of Transcriptome analysis of atemoya pericarp elucidates the role of polysaccharide metabolism in fruit ripening and cracking after harvest
Creators: name: Chen, Jingjing
name: Duan, Yajie
name: Hu, Yulin
name: Li, Weiming
name: Sun, Dequan
name: Hu, Huigang
name: Xie, Jianghui
Publisher: name: figshare
Year: 2019
Subjects: subject: Biochemistry
subject: Cell Biology
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Physiology
subject: Biological Sciences not elsewhere classified
subject: Developmental Biology
subject: Plant Biology

description: Figure S5. Enriched starch and sucrose metabolism pathway. The components marked with red rectangles were considered differentially expressed. (DOC 32 kb)
Anochetus princeps var. laeta Forel, 1910, n. var.
Creators: name: Forel, A.
Publisher: name: Zenodo
Year: 1910
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hymenoptera
Formicidae
Anochetus
Anochetus princeps
Anochetus princeps em. var. laeta

description: Anochetus princeps Em. var. laeta n. var.
- D'un jaunatre assez pale et sale, avec les cotes de la tete brunatres. Pilosite un peu plus abondante que chez le type de l'espece, surtout sur les membres. Denticules du bord interne des mandibules plus aigus et plus longs. Ecaille moins elevee et moins acuminee. La partie posterieure de la tete, des yeux a l'occiput, est aussi un peu plus allongee et plus retrecie. Du reste identique au type de l'espece. Sumatra. Recu de M. Seeldrayers.
description: Published as part of Forel, A., 1910, Glanures myrmecologiques., pp. 6-32 in Annales de la Societe Entomologique de Belgique 54 on page 22
Additional file 1: of Clinical implications of fracture-associated vascular damage in extremity and pelvic trauma
Creators: name: F. Gilbert
name: C. Schneemann
name: C. Scholz
name: R. Kickuth
name: R. Meffert
name: R. Wildenauer
name: U. Lorenz
name: R. Kellersmann
name: A. Busch
Publisher: name: figshare
Year: 2018
Subjects: subject: Biochemistry
subject: Medicine
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Physiology
subject: 59999 Environmental Sciences not elsewhere classified
subject: FOS: Earth and related environmental sciences
subject: Ecology
subject: 19999 Mathematical Sciences not elsewhere classified
subject: FOS: Mathematics
subject: Developmental Biology
subject: Computational Biology

description: Table S1. Baseline characteristics of vascular and control trauma populations. Both populations have a similar size and show no differences in age, sex and trauma type distribution. The number of patients with multiple fractures is slightly higher in the control trauma population. (DOC 31 kb)
Minimum Spanning Tree cluster analysis of the LMC region above 10 GeV: detection of the SNRs N 49B and N 63A
Creators: name: Campana, R.
name: Massaro, E.
name: Bernieri, E.
Publisher: name: arXiv
Year: 2018
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: Astrophysics of Galaxies (astro-ph.GA)
subject: Instrumentation and Methods for Astrophysics (astro-ph.IM)
subject: FOS: Physical sciences

description: We present the results of a cluster search in the gamma-ray sky images of the Large Magellanic Cloud region by means of the Minimum Spanning Tree algorithm at energies higher than 10 GeV, using 9 years of Fermi-LAT data. Several significant clusters were found, the majority of which associated with previously known gamma-ray sources. New significant clusters associated with the supernova remnants N 49B and N 63A are also found, and confirmed with a Maximum Likelihood analysis of the Fermi-LAT data.
description: 11 pages, 3 figures. Accepted for publication in Astrophysics and Space Science
Additional file 1: of A multi-centre, double-blind, placebo-controlled, randomised trial of combination methotrexate and gefitinib versus methotrexate alone to treat tubal ectopic pregnancies (GEM3): trial protocol
Creators: name: May, James
name: Duncan, Colin
name: Mol, Ben
name: Siladitya Bhattacharya
name: Daniels, Jane
name: Middleton, Lee
name: Hewitt, Catherine
name: Arri Coomarasamy
name: Jurkovic, Davor
name: Bourne, Tom
name: Bottomley, Cecilia
name: Peace-Gadsby, Alexandra
name: Doust, Ann
name: Tong, Stephen
name: Horne, Andrew
Publisher: name: figshare
Year: 2018
Subjects: subject: Medicine
subject: Cell Biology
subject: Pharmacology
subject: Developmental Biology
subject: Cancer
subject: Science Policy
subject: 110309 Infectious Diseases
subject: FOS: Health sciences

description: SPIRIT 2013 checklist: recommended items to address in a clinical trial protocol and related documents. (DOC 125 kb)
Using the Fundamental Plane to Estimate the Total Binding Mass in A2626
Creators: name: Mohr, Joseph J.
name: Wegner, Gary
Publisher: name: arXiv
Year: 1997
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We use fundamental plane (FP) distance estimates to the components of the double cluster A2626 (cz~17,500 km/s) to constrain cluster kinematics and estimate total binding mass. The FP coefficients for a sample of 24 early type and S0 cluster members (alpha=1.30+/-0.36 and beta=0.31+/-0.06) are consistent with others reported in the literature. We examine the Mg_b distributions within both subclusters and find them to be indistinguishable. Lacking evidence for stellar population differences, we interpret the FP zeropoint offset (\log(D_B/D_A)=-0.037+/-0.046, where D_{cl} is distance to subcluster cl) as a measure of the distance difference. This measurement is consistent with the subclusters being at the same distance, and it rules out the Hubble flow hypothesis (distances proportional to velocity) with 99% confidence; analysis of the subcluster galaxy magnitude distributions rules out Hubble flow at 93% confidence. Both results favor a kinematic model where the subclusters are bound and infalling. We estimate the total cluster binding mass by modelling the subcluster merger as radial infall. The minimum possible total binding mass is 1.65 times higher than the sum of the standard virial masses, a difference statistically significant at the ~3sigma level. We discuss explanations for the inconsistency including (1) biases in the standard virial mass estimator, (2) biases in our radial infall mass estimate, and (3) mass beyond the virialized cluster region; if the standard virial mass is significantly in error, the cluster has an unusually high mass to light ratio (~1000h). Because observational signatures of departures from radial infall are absent, we explore the implications of mass beyond the virialized, core regions. (abridged)
description: 14 pages and 5 figures, Latex, Accepted for publication in AJ
Large-p_T Inclusive pi^0 Cross Sections and Next-to-Leading-Order QCD Predictions
Creators: name: Aurenche, P.
name: Fontannaz, M.
name: Guillet, J. -Ph.
name: Kniehl, B. A.
name: Werlen, M.
Publisher: name: arXiv
Year: 1999
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We review the phenomenology of pi^0 production at large transverse momentum in proton-induced collisions. Uncertainties in the next-to-leading-order predictions of Quantum Chromodynamics are discussed. The comparison with data reveals that the disagreement between theory and experiment lies essentially in an overall normalization factor. The situation for pi^0 production is contrasted with that of prompt-photon production in hadronic collisions.
description: 21 pages (Latex), 13 figures (Postscript)
Elastic pp and $\bar pp$ scattering in the Modified Additive Quark Model
Creators: name: Desgrolard, P.
name: Giffon, M.
name: Martynov, E.
Publisher: name: arXiv
Year: 2000
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: The modified additive quark model, proposed recently, allows to improve agreement of the standard additive quark model with the data on the $pp, \bar pp, π^{\pm} p, γp$ and $γγ$ total cross-sections, as well as on the ratios of real to imaginary part of $pp$ and $\bar pp$ amplitudes at $t=0$. Here, we extend this model to non forward elastic scattering of protons and antiprotons. A high quality reproduction of angular distributions at 19.4 GeV $\leq \sqrt{s}\leq $ 1800 Gev is obtained. A zero at small $|t|$ in the real part of even amplitude in accordance with a recently proved high energy general theorem is found.
description: 14 pages, LaTeX2e, 4 eps figures. Revised version accepted for publication in European Physical Journal C
Additional file 1: of Treatment-duration is related to changes in peripheral lymphocyte counts during definitive radiotherapy for unresectable stage III NSCLC
Creators: name: Zhao, Qianqian
name: Chen, Gang
name: Ye, Luxi
name: Shi, Shiming
name: Du, Shisuo
name: Zeng, Zhaochong
name: He, Jian
Publisher: name: figshare
Year: 2019
Subjects: subject: Molecular Biology
subject: Evolutionary Biology
subject: FOS: Biological sciences
subject: Ecology
subject: Sociology
subject: FOS: Sociology
subject: Biological Sciences not elsewhere classified
subject: Mathematical Sciences not elsewhere classified
subject: Developmental Biology
subject: Cancer
subject: Computational Biology

description: Table S1. Details of chemotherapy used in our study population (nâ =â 115). (DOCX 16 kb)
Ultra-high energy cosmic ray sources and large scale magnetic fields
Creators: name: Lemoine, Martin
name: Sigl, Guenter
name: Olinto, Angela V.
name: Schramm, David N.
Publisher: name: arXiv
Year: 1997
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Protons of energies up to 10**20 eV can be subject to significant deflection and energy dependent time delay in lage scale extragalactic or halo magnetic fields of strengths comparable to current upper limits. By performing 3-dimensional Monte Carlo simulations of nucleon propagation, we show how observations of arrival direction and time distributions can be used to measure the structure and strength of large-scale magnetic fields, and constrain the nature of the source of ultra-high energy cosmic rays.
description: 12 latex pages, 3 encapsulated postscript figures included, uses aaspp4.sty, and psfig.sty. Submitted to ApJ Lett
Pachycondyla (Ectomomyrmex) leeuwenhoeki subsp. sumatrensis
Creators: name: Forel, A.
Publisher: name: Zenodo
Year: 1910
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hymenoptera
Formicidae
Pachycondyla
Pachycondyla leeuwenhoeki
Pachycondyla (ectomomyrmex) leeuwenhoeki for. subsp. sumatrensis

description: Pachycondyla (Ectomomyrmex) Leeuwenhoeki For. subsp. sumatrensis Forel.
Sumatra (coll. Seeldrayers). - Je crois devoir elever cette variete au rang de sous-espece. L'exemplaire de M. Seeldrayers a le l'rsegment abdominal moins densement ponctue et plus luisant que chez le type.
description: Published as part of Forel, A., 1910, Glanures myrmecologiques., pp. 6-32 in Annales de la Societe Entomologique de Belgique 54 on page 23
title: Ильяс Жансугуров
Creators: name: ELS IPR BOOKS
Publisher: name: EDP Hub (Идипи Хаб), Ай Пи Ар Медиа
Year: 2024

description: Монография посвящена неповторимой жизни и богатому, многогранному творчеству Ильяса Жансугурова. Ильяс Жансугуров был не только поэтом, он известен еще и как прозаик, драматург, сатирик и талантливый переводчик. Ильяс Жансугуров занимает огромное место в истории казахской культуры, литературы и журналистики. Своим творчеством он внес значительный вклад в формирование нового художественного метода в казахской литературе. Данная монография рекомендуется для студентов-филологов и журналистов, а также для широкого круга читателей.
Cosmic ray sputtering yield of interstellar H2O ice mantles : Ice mantle thickness dependence
Creators: name: Dartois, E.
name: Chabot, M.
name: Barkach, T. Id
name: Rothard, H.
name: Augé, B.
name: Agnihotri, A. N.
name: Domaracka, A.
name: Boduch, P.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: Interstellar grain mantles present in dense interstellar clouds are in constant exchange with the gas phase via accretion and desorption mechanisms such as UV, X-ray photodesorption, cosmic ray induced sputtering, grain thermal fluctuations, and chemical reaction energy release. The relative importance of the various desorption mechanisms is of uttermost importance for astrophysical models to constrain the chemical evolution in such high density dense cloud regions. In this experimental work we investigated the sputtering yield as a function of ice mantle thickness, exposed to Xe ions at 95MeV. The ion induced ice phase transformation and the sputtering yield were simultaneously monitored by IR spectroscopy and mass spec- trometry, respectively. The sputtering yield is constant above a characteristic ice layer thickness and starts to decrease below this thickness. An estimate of the sputtering depth corresponding to this length can be evaluated. In these experiments the measured desorption depth corresponds to 30 ice layers. Assuming an effective cylindrical shape for the volume of sputtered molecules, the aspect ratio is close to unity; in the semi-infinite ice film case this ratio is the diameter to height of the cylinder. This result shows that most ejected molecules arise from a rather compact volume. The measured infinite thickness sputtering yield for water ice mantles scales as the square of the ion electronic stopping power (Se). We expect that the desorption depth dependence varies with Se^a , where a=0.5. Astrophysical models should take into account the thickness dependence constraints of these ice mantles in the interface regions when ices are close to their extinction threshold. In the very dense cloud regions, most of the water ice mantles are above this limit for the bulk of the cosmic rays.
description: 6 pages, 5 figures
Multi-Photon Amplitudes for Next-to-Leading Order QCD
Creators: name: Del Duca, Vittorio
name: Kilgore, William B.
name: Maltoni, Fabio
Publisher: name: arXiv
Year: 1999
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We present the tree-level amplitudes involving one, two and three photons that are required for next-to-leading order QCD calculations of production rates of three final-state particles. We also present the required one-loop amplitudes in terms of previously published results.
description: LaTeX, 22 pages
title: ADCO, Neuvième cartulaire de Saint-Étienne de Dijon (1661 - 1684), Cart. 32 (G 136), 745 folios, f. 0484
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: Laboratoire de Médiévistique Occidentale de Paris
subject: Corpus Burgundiae Medii Aevi
subject: Chartes de la Bourgogne du Moyen Âge
subject: cartulaire
subject: LaMOP

description: Neuvième cartulaire de Saint-Étienne de Dijon (1661 - 1684), Archives départementales de la Côte-d'Or, Cart. 32 (G 136), 745 folios, f. 0484, Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Neuvième cartulaire de Saint-Étienne de Dijon (1661 - 1684), Archives départementales de la Côte-d'Or, Cart. 32 (G 136), 745 folios, f. 0484, in Projet CBMA - Corpus Burgundiae Medii Aevi [Ressource en ligne], https:// manuscrits.cbma-project.eu/
description: Provenance: abbaye Saint-Étienne de Dijon
description: Provenance: http://www.wikidata.org/entity/Q15945019
Additional file 7: of Disruption of ureide degradation affects plant growth and development during and after transition from vegetative to reproductive stages
Creators: name: Takagi, Hiroshi
name: Watanabe, Shunsuke
name: Shoma Tanaka
name: Matsuura, Takakazu
name: Mori, Izumi
name: Hirayama, Takashi
name: Shimada, Hiroshi
name: Sakamoto, Atsushi
Publisher: name: figshare
Year: 2018
Subjects: subject: Microbiology
subject: FOS: Biological sciences
subject: Cell Biology
subject: Genetics
subject: Molecular Biology
subject: Developmental Biology
subject: 110309 Infectious Diseases
subject: FOS: Health sciences
subject: Plant Biology

description: Figure S6. Characterization of ups1 and ups2 mutants. (a) Diagram of the T-DNA insertion in AtUPS1 in the ups1 mutant. Arrows indicate PCR primers; white boxes indicate untranslated regions; black boxes indicate exons; black lines indicate introns. (b) PCR-based genotyping of the ups1 mutant using primers specific to AtUPS1 (F1 and R1) and the left border sequence of the T-DNA (SAIL LB1). (c) Diagram of the T-DNA insertion in AtUPS2 in the ups2 mutant. Arrows indicate PCR primers; white boxes indicate untranslated regions; black boxes indicate exons; black lines indicate introns. (d) PCR-based genotyping of the ups1 mutant using primers specific to AtUPS2 (F2 and R2) and the left border sequence of the T-DNA (LBa1). (e) Semi-quantitative reverse transcription-PCR for estimating AtUPS1 and AtUPS2 mRNA levels in the mutant lines. VHA-A expression was simultaneously analyzed as an internal control. (PDF 865 kb)
Additional file 2: of Treatment-duration is related to changes in peripheral lymphocyte counts during definitive radiotherapy for unresectable stage III NSCLC
Creators: name: Zhao, Qianqian
name: Chen, Gang
name: Ye, Luxi
name: Shi, Shiming
name: Du, Shisuo
name: Zeng, Zhaochong
name: He, Jian
Publisher: name: figshare
Year: 2019
Subjects: subject: Biochemistry
subject: Physical Sciences not elsewhere classified
subject: Medicine
subject: Molecular Biology
subject: Pharmacology
subject: Sociology
subject: FOS: Sociology
subject: Biological Sciences not elsewhere classified
subject: Developmental Biology
subject: Cancer
subject: Computational Biology

description: Table S2. Correlation between TLCs nadir and percentage of lung or heart dose. (DOCX 14 kb)
Meranoplus castaneus Sm.
Creators: name: Forel, A.
Publisher: name: Zenodo
Year: 1910
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hymenoptera
Formicidae
Meranoplus
Meranoplus castaneus

description: Meranoplus castaneus Sm.
- [[worker]]. - Long. 3 a 3.2 mill. - Mandibules striees. Tete un peu plus large que longue et plus large derriere que devant, echancree derriere. Yeux fort convexes. Antennes de 9 articles; ceux du funicule plus longs qu'epais. Dos du thorax borde; pronotum avec deux larges epines plates, courtes. Mesonotum avec 2 epines laterales, echancre derriere. Epinotum avec 2 epines greles. Premier n oe ud vu de cote cuneiforme, tranchant au sommet ou il est largement et faiblement echancre. Vu de devant il est un peu plus large en bas devant qu'au sommet. Second n oe ud arrondi, aussi long que large, prolonge au milieu de son bord posterieur superieur par une epine pointue, grele, horizontale, dirigee en arriere. En dessous, devant, il porte une dent dirigee en avant que Smith a evidemment attribuee au 1 er n oe ud.
Subopaque. Tete assez finement ridee en long, et reticulee entre les rides. Thorax et pedicule grossierement reticules et finement reticules dans les mailles. Epinotum lisse, avec quelques rides. Abdomen densement et finement reticule, avec une tendance a former de fines rides longitudinales. Pattes et scapes stries. Pilosite dressee abondante partout, jaunatre, pointue, inegale de longueur.
Entierement ferrugineux.
Sumatra. Collection C Seeldrayers
description: Published as part of Forel, A., 1910, Glanures myrmecologiques., pp. 6-32 in Annales de la Societe Entomologique de Belgique 54 on page 24
Device independent quantum random number generation
Creators: name: Liu, Yang
name: Zhao, Qi
name: Li, Ming-Han
name: Guan, Jian-Yu
name: Zhang, Yanbao
name: Bai, Bing
name: Zhang, Weijun
name: Liu, Wen-Zhao
name: Wu, Cheng
name: Yuan, Xiao
name: Li, Hao
name: Munro, W. J.
name: Wang, Zhen
name: You, Lixing
name: Zhang, Jun
name: Ma, Xiongfeng
name: Fan, Jingyun
name: Zhang, Qiang
name: Pan, Jian-Wei
Publisher: name: arXiv
Year: 2018
Subjects: subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: Randomness is critical for many information processing applications, including numerical modeling and cryptography. Device-independent quantum random number generation (DIQRNG) based on the loophole free violation of Bell inequality produces unpredictable genuine randomness without any device assumption and is therefore an ultimate goal in the field of quantum information science. However, due to formidable technical challenges, there were very few reported experimental studies of DIQRNG, which were vulnerable to the adversaries. Here we present a fully functional DIQRNG against the most general quantum adversaries. We construct a robust experimental platform that realizes Bell inequality violation with entangled photons with detection and locality loopholes closed simultaneously. This platform enables a continuous recording of a large volume of data sufficient for security analysis against the general quantum side information and without assuming independent and identical distribution. Lastly, by developing a large Toeplitz matrix (137.90 Gb $\times$ 62.469 Mb) hashing technique, we demonstrate that this DIQRNG generates $6.2469\times 10^7$ quantum-certified random bits in 96 hours (or 181 bits/s) with uniformity within $10^{-5}$. We anticipate this DIQRNG may have profound impact on the research of quantum randomness and information-secured applications.
description: 35 pages, 10 figures. The section "randomness extraction" in supplementary is revised in order to avoid text overlap
Maximum Likelihood Analysis of Clusters of Ultra-High Energy Cosmic Rays
Creators: name: Sigl, Guenter
name: Lemoine, Martin
name: Olinto, Angela V.
Publisher: name: arXiv
Year: 1997
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present a numerical code designed to conduct a likelihood analysis for clusters of nucleons above 10**19 eV originating from discrete astrophysical sources such as powerful radio galaxies, gamma-ray bursts or topological defects. The code simulates the propagation of nucleons in a large-scale magnetic field and constructs the likelihood of a given observed event cluster as a function of the average time delay due to deflection in the magnetic field, the source activity time scale, the total fluence of the source, and the power law index of the particle injection spectrum. Other parameters such as the coherence length and the power spectrum of the magnetic field are also considered. We apply it to the three pairs of events above 4X10**19 eV recently reported by the Akeno Giant Air Shower Array (AGASA) experiment, assuming that these pairs were caused by nucleon primaries which originated from a common source. Although current data are too sparse to fully constrain each of the parameters considered, and/or to discriminate models of the origin of ultra-high energy cosmic rays, several tendencies are indicated. If the clustering suggested by AGASA is real, next generation experiments with their increased exposure should detect more than 10 particles per source over a few years and our method will put strong constraints on both the large-scale magnetic field parameters and the nature of these sources.
description: 11 latex pages, 8 postscript figures included, uses revtex.sty in two-column format and epsf.sty. Submitted to Physical Review D
Additional file 8: of Disruption of ureide degradation affects plant growth and development during and after transition from vegetative to reproductive stages
Creators: name: Takagi, Hiroshi
name: Watanabe, Shunsuke
name: Shoma Tanaka
name: Matsuura, Takakazu
name: Mori, Izumi
name: Hirayama, Takashi
name: Shimada, Hiroshi
name: Sakamoto, Atsushi
Publisher: name: figshare
Year: 2018
Subjects: subject: Medicine
subject: Microbiology
subject: FOS: Biological sciences
subject: Ecology
subject: 69999 Biological Sciences not elsewhere classified
subject: Developmental Biology
subject: Plant Biology

description: Figure S7. Growth of representative ups1 and ups2 mutants. Plants were grown at 23Â Â°C in soil for 7Â weeks under long-day conditions. (PDF 257 kb)
Myrmica myrmicoxena Forel
Creators: name: Forel, A.
Publisher: name: Zenodo
Year: 1910
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hymenoptera
Formicidae
Myrmica
Myrmica myrmicoxena

description: Myrmica myrmicoxena Forel.
Cette curieuse espece est bien une Myrmica et tres probablement parasite ou hote de la lobicornis Nyl., malgre la presence des [[queen]] et. [[male]] lobicornis dans la meme fourmiliere. La tete de la [[queen]] est plus petite, plus arrondie et plus faiblement sculptee que chez la lobicornis. Chez le [[male]], le scape, fort court, est a peine un peu courbe a sa base; les mandibules ont 6 a 7 dents. Il ressemble du reste beaucoup a celui de la lobicornis; la sculpture est un peu plus faible et les n oe uds, ainsi que tout le corps et les pattes, plus courts. Les ailes ont les nervures absolument comme chez les autres Myrmica; elles sont seulement plus hyalines que chez la lobicornis, avec les nervures plus pales.
description: Published as part of Forel, A., 1910, Glanures myrmecologiques., pp. 6-32 in Annales de la Societe Entomologique de Belgique 54 on page 24
DRELL-YAN PROCESSES AS A PROBE OF CHARGE SYMMETRY VIOLATION IN THE PION AND NUCLEON
Creators: name: Londergan, J. T.
name: Garvey, G. T.
name: Liu, G. Q.
name: Rodionov, E. N.
name: Thomas, A. W.
Publisher: name: arXiv
Year: 1995
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We extend earlier investigations of charge symmetry violation in the valence quark distributions of the nucleon, and make similar estimates for the pion. The sensitivity of pion-induced Drell-Yan measurements to such effects is then examined. It is shown that combinations of $π^+$ and $π^-$ data on deuterium and hydrogen are sensitive to these violations, and that the pion and nucleon charge symmetry violating terms separate as a function of $x_π$ and $x_N$ respectively. We estimate the background terms which must be evaluated to extract charge symmetry violation.
description: 11 pages + uuencoded postscript file of 4 figures
Additional file 3: of Treatment-duration is related to changes in peripheral lymphocyte counts during definitive radiotherapy for unresectable stage III NSCLC
Creators: name: Zhao, Qianqian
name: Chen, Gang
name: Ye, Luxi
name: Shi, Shiming
name: Du, Shisuo
name: Zeng, Zhaochong
name: He, Jian
Publisher: name: figshare
Year: 2019
Subjects: subject: Molecular Biology
subject: Pharmacology
subject: Evolutionary Biology
subject: FOS: Biological sciences
subject: Sociology
subject: FOS: Sociology
subject: Developmental Biology
subject: Cancer

description: Table S3. Multivariate logistic regression associating baseline variables with SL during radiation treatment in subgroup patients treated with helical tomotherapy. (DOCX 14 kb)
Magnetic fields within color superconducting neutron star cores
Creators: name: Alford, M.
name: Berges, J.
name: Rajagopal, K.
Publisher: name: arXiv
Year: 1999
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We discuss the Meissner effect for a color superconductor formed by cold dense quark matter. Though color and ordinary electromagnetism are broken in a color superconductor, there is a linear combination of the photon and a gluon that remains massless. Consequently, a color superconducting region may be penetrated by an external magnetic field. We show that at most a small fraction of the magnetic field is expelled, and if the screening distance is the smallest length scale in the problem there is no expulsion at all. We calculate the behavior of the magnetic field for a spherical geometry relevant for compact stars. If a neutron star contains a quark matter core, this core is a color superconductor. Our results demonstrate that such cores admit magnetic fields without restricting them to quantized flux tubes. Such magnetic fields within color superconducting neutron star cores are stable on time scales longer than the age of the universe, even if the spin period of the neutron star is changing.
description: 22 pages, LaTeX with 2 eps figures; typos corrected, references added
Camponotus truebi Forel, 1910, n. sp.
Creators: name: Forel, A.
Publisher: name: Zenodo
Year: 1910
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hymenoptera
Formicidae
Camponotus
Camponotus truebi

description: Camponotus Truebi n. sp.
- [[worker]]. - Long. 5 a 5,5 mill. - Mandibules epaisses, courtes, mates, densement et finement ridees, abondamment ponctuees, armees de 6 (ou 7?) dents. Portion mediane de l'epistome en carre arrondi, subcarene, sans lobe anterieur, mais avec une echancrure de chaque cote. Aire frontale rhombiforme; aretes frontales longues, sinueuses, fort divergentes. Tete en trapeze, retrecie devant, concave derriere, a cotes fort convexes, avec sa largeur maximum au tiers posterieur ou elle egale presque la longueur. Les scapes un peu deprimes (aplatis), mais pas larges, depassent le bord posterieur de 2 fois leur largeur. Dos du thorax assez convexe en long. Suture promesonotale distincte; suture meso-epinotale obsolete. La face basale de l'epinotum est assez large, environ deux fois plus longue que large, mais convexe transversalement, plus que longitudinalement, et plus longue que la face declive a laquelle elle passe par une courbe assez brusque. Ecaille assez large, epaisse, beaucoup plus convexe devant que derriere ou elle est presque plane, presque aussi epaisse a son sommet obtus qu'a sa base. Cuisses et tibias plutot courts, comprimes, mais non prismatiques, sans piquants au cote interne.
Luisant, finement et faiblement chagrine. Devant de la tete densement reticule et subopaque. Un groupe de soies blanchatres sur (epinotum, un autre sur l'ecaille, et une ou deux rangees de soie un peu plus courtes sur chaque segment abdominal. Ailleurs sur le corps, les soies sont tres eparses, courtes, d'un blanc jaunatre. Quelques soies fort courtes et eparses sur les joues, les tibias et les scapes. Pubescence presque nulle sur le corps, plus distincte sur les membres. Sur les tibias, les poils dresses sont extremement rares, mais il y a 3 ou 4 petits piquants a l'extremite inferieure.
Entierement noir; extremite des mandibules et funicules d'un brun noir; extremite des tarses roussatre; lisiere extreme des segments abdominaux jaunatre.
Une [[worker]] media differe de la [[worker]] major (maxima?) ci-dessus decrite par ses scapes depassant le bord posterieur d'un bon quart, enfin par sa tete moins elargie et moins concave derriere, moins mate devant, avec le milieu de l'epistome plutot trapeziforme.
Narits Districts, Formose, recu par M. Rolle. Cette espece est voisine du groupe fallax Nyl., mais en differe par son epistome entier au milieu, son epinotum plus lage et son ecaille plus epaisse.
description: Published as part of Forel, A., 1910, Glanures myrmecologiques., pp. 6-32 in Annales de la Societe Entomologique de Belgique 54 on pages 26-27
The role of ν_τ ultrahigh energy astrophysics in Km^3 detectors
Creators: name: Fargion, D.
Publisher: name: arXiv
Year: 1997
Subjects: subject: Astrophysics (astro-ph)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We show that the expected $ ν_τ $ signals, by their secondary tau tracks, in Km^3 detectors at highest cosmic ray energy window $ 1.7\cdot 10^{21} eV \gt E_τ \gt 1.6 x 10^{17} eV$, must overcome the corresponding $ ν_μ $ (or muonic) ones. Indeed, the Lorentz-boosted tau range length grows (linearly) above muon range, for $ E_τ \RAISE 1.6 x 10^8 GeV$ and reaches its maxima extension, $ R_{τ_{\max}} \simeq 191 km$, at energy $E_τ \simeq 3.8 x 10^9 GeV$. At this peak the tau range is nearly 20 times the corresponding muon range (at the same energy) implying a similar ratio in $ ν_τ $ over $ ν_μ $ detectability. This dominance, however may lead (at present most abundant $ ν_τ $ model fluxes) to just a rare spectacular event a year (if flavor mixing occurs). Lower energetic $ τ$ and $ ν_τ $ signals $ (\barν_e e\to \barν_τ τ, ν_τ N\to ...) $ at energy range ($ 10^5 ÷10^7 GeV$) may be more easily observed in km^3 detectors at a rate of a few $ (\barν_e e\to \barν_τ τ) $ to tens event $ (ν_τ N\to τ+ $ anything) a year.
description: 14 pages LaTex, 1 postscript figure
IR nebulae around bright massive stars as indicators for binary interactions
Creators: name: Bodensteiner, Julia
name: Baade, Dietrich
name: Greiner, Jochen
name: Langer, Norbert
Publisher: name: arXiv
Year: 2018
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: Recent studies show that more than 70% of massive stars do not evolve as effectively single stars, but as members of interacting binary systems. The evolution of these stars is thus strongly altered compared to similar but isolated objects. We investigate the occurrence of parsec-scale mid-infrared nebulae around early-type stars. If they exist over a wide range of stellar properties, one possible overarching explanation is non-conservative mass transfer in binary interactions, or stellar mergers. For ~3850 stars (all OBA stars in the Bright Star Catalogue [BSC], Be stars, BeXRBs, and Be+sdO systems), we visually inspect WISE 22 $μ$m images. Based on nebular shape and relative position, we distinguish five categories: offset bow shocks structurally aligned with the stellar space velocity, unaligned offset bow shocks, and centered, unresolved, and not classified nebulae. In the BSC, we find that 28%, 13%, and 0.4% of all O, B, and A stars, respectively, possess associated infrared (IR) nebulae. Additionally, 34/234 Be stars, 4/72 BeXRBs, and 3/17 Be+sdO systems are associated with IR nebulae. Aligned or unaligned bow shocks result from high relative velocities between star and interstellar medium (ISM) that are dominated by the star or the ISM, respectively. About 13% of the centered nebulae could be bow shocks seen head- or tail-on. For the rest, the data disfavor explanations as remains of parental disks, supernova remnants of a previous companion, and dust production in stellar winds. The existence of centered nebulae also at high Galactic latitudes strongly limits the global risk of coincidental alignments with condensations in the ISM. Mass loss during binary evolution seems a viable mechanism for the formation of at least some of these nebulae. In total, about 29% of the IR nebulae (2% of all OBA stars in the BSC) may find their explanation in the context of binary evolution.
description: 21 pages, 5 tables, 6 figures, accepted for publication in A&A
Nuclear Motion Is Classical: Spectrum of a Magic Protonated Water Cluster
Creators: name: Frank, Irmgard
Publisher: name: Basel : MDPI
Year: 2023
Subjects: subject: Car–Parrinello molecular dynamics
subject: classical nuclear motion
subject: spectra
subject: Dewey Decimal Classification::500 | Naturwissenschaften::540 | Chemie

description: The assumption that nuclear motion is classical explains many phenomena. The problems of Schrödinger’s cat and the EPR paradoxon do not exist in a perfectly deterministic theory. All it needs is to describe nuclear motion classically right from the beginning. To establish this simple idea, it must be tested for as many examples as possible. In the present paper, we use ab initio molecular dynamics to investigate the infrared spectrum of a ‘magic’ protonated water cluster H3O+(H2O)20 which exhibits some features that were believed to afford a quantum treatment of nuclear motion. The role of the temperature in contrast to a quantum mechanical description is discussed.
Gamma-Ray Burst Spectral Evolution Through Crosscorrelations of Discriminator Light Curves
Creators: name: Band, David L.
Publisher: name: arXiv
Year: 1997
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Gamma-ray burst spectra usually show hard-to-soft evolution within intensity spikes and from spike to spike. The techniques used to study spectral evolution often lack sufficient temporal resolution to determine the nature of this evolution. By comparing the auto- and crosscorrelations between the time histories of the BATSE Large Area Detector discriminator rates I have characterized the spectral evolution of a sample of 209 bursts. I find that hard-to-soft evolution is ubiquitous, and only ~10% of the bursts show clear soft-to-hard evolution.
description: 17 pages, AASTeX 4.0, 9 figures, to appear in Ap.J., vol 486
title: ADCO, Cartulaire de Cîteaux dit Cartulaire de France (début XVe), Cart. 171 (11 H 68), f. 0006
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: CG21/F.PETOT/2012
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 de Cîteaux dit Cartulaire de France (début XVe), Archives départementales de la Côte-d'Or, Cart. 171 (11 H 68), f. 0006, Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Cartulaire de Cîteaux dit Cartulaire de France (début XVe), Archives départementales de la Côte-d'Or, Cart. 171 (11 H 68), f. 0006, 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
Ponera inexorata var. inexpedita Forel, 1911, n. var.
Creators: name: Forel, A.
Publisher: name: Zenodo
Year: 1911
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hymenoptera
Formicidae
Ponera
Ponera inexorata
Ponera inexorata wheeler, v. inexpedita

description: Ponera inexorata Wheeler, v. inexpedita n. var.
[[worker]]. Unterscheidet sich vom Arttypus durch die etwas dunklere Farbe, die entschieden schwächere Behaarung, den etwas schwächer eingeschnuerten Hinterleib und durch die fast fehlenden (winzigen und ganz flachen) atrophischen Augen. Sie hat die Gröfse des Arttypus (viel gröfser als die Subsp. fallax Forel aus Guatemala).
Ein flügelloses [[queen]], 4,3 mm lang, braunrot, scheint dazu zu gehören.
Sao Paulo (v. Ihering).
description: Published as part of Forel, A., 1911, Ameisen des Herrn Prof. v. Ihering aus Brasilien (Sao Paulo usw.) nebst einigen anderen aus Südamerika und Afrika (Hym.)., pp. 285-312 in Deutsche Entomologische Zeitschrift 1911 on pages 285-286
BCP3: Summary of Theory
Creators: name: Peccei, R. D.
Publisher: name: arXiv
Year: 2000
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: I discuss a number of the highlights in theory presented at the BCP3 conference. These included new, and more stringent, CKM fits; a critical overview of heavy hadron lifetimes; progress in computing rates and CP-asymmetries in charmless B-decays; a thorough discussion of the implications of the new results on $ε^{\prime}/ε$; and, finally, a peek at the future, trying to estimate how well one is going to be able to measure the unitarity triangle angles.
description: To appear in the Proceedings of the Third International Conference on B Physics and CP Violation, Taipei, Taiwan, December 3-7, 1999
Evidence for the photoionization absorption edge in a photospheric radius expansion X-ray burst from GRS 1747$-$312 in Terzan 6
Creators: name: Li, Zhaosheng
name: Suleimanov, Valery F.
name: Poutanen, Juri
name: Salmi, Tuomo
name: Falanga, Maurizio
name: Nättilä, Joonas
name: Xu, Renxin
Publisher: name: arXiv
Year: 2018
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: Thermonuclear X-ray bursts on the surface of neutron stars (NSs) can enrich photosphere with metals, which may imprint the photoionization edges on the burst spectra. We report here the discovery of absorption edges in the spectra of the type I X-ray burst from the NS low-mass X-ray binary GRS 1747$-$312 in Terzan 6 during observations by the Rossi X-ray Timing Explorer. We find that the edge energy evolves from $9.45\pm0.51$ keV to $\sim6$ keV and then back to $9.44\pm0.40$ keV during the photospheric radius expansion phase and remains at $8.06\pm0.66$ keV in the cooling tail. The photoionization absorption edges of hydrogen-like Ni, Fe or Fe/Ni mixture and the bound-bound transitions of metals may be responsible for the observed spectral features. The ratio of the measured absorption edge energy in the cooling tail to the laboratory value of hydrogen-like Ni(Fe) edge energy allows us to estimate the gravitational redshift factor $1+z=1.34\pm0.11$($1+z=1.15\pm0.09$). The evolution of the spectral parameters during the cooling tail are well-described by the metal-rich atmosphere models. The combined constraints on the NS mass and radius from the direct cooling method and the tidal deformability strongly suggest very high atmospheric abundance of the iron group elements and limit the distance to the source to $11\pm1$ kpc.
description: matches the published version
Well-posedness and stability analysis of an epidemic model with infection age and spatial diffusion
Creators: name: Walker, Christoph
Publisher: name: Berlin ; Heidelberg ; New York : Springer
Year: 2023
Subjects: subject: Age-strucutre
subject: Spatial diffusion
subject: Stability of steady states
subject: Dewey Decimal Classification::500 | Naturwissenschaften::570 | Biowissenschaften, Biologie

description: A compartment epidemic model for infectious disease spreading is investigated, where movement of individuals is governed by spatial diffusion. The model includes infection age of the infected individuals and assumes a logistic growth of the susceptibles. Global well-posedness of the equations within the class of nonnegative smooth solutions is shown. Moreover, spectral properties of the linearization around a steady state are derived. This yields the notion of linear stability which is used to determine stability properties of the disease-free and the endemic steady state.
NON-EQUILIBRIUM DESCRIPTION OF BREMSSTRAHLUNG IN DENSE MATTER (Landau - Pomeranchuk - Migdal Effect)
Creators: name: Knoll, Jörn
name: Voskresensky, Dmitri N.
Publisher: name: arXiv
Year: 1995
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: The soft behavior of the bremsstrahlung from a source is discussed in terms of classical transport models and within a non--equilibrium quantum field theory (Schwinger - Kadanoff - Baym - Keldysh) formulation.
description: 8 pages, latex, no figures (diagrams in latex)