cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
title: ADCO, Cartulaire de Cîteaux pour les domaines de Beaune (XVe siècle), Cart. 177 (11 H 289), 197 folios, f. 0306
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/2015
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: cartulaire

description: Cartulaire de Cîteaux pour les domaines de Beaune (XVe siècle), Archives départementales de la Côte-d'Or, Cart. 177 (11 H 289), 197 folios, f. 0306, Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Cartulaire de Cîteaux pour les possessions d’Izeure (XVe siècle), Archives départementales de la Côte-d'Or, Cart. 177 (11 H 289), 197 folios, f. 0306, 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
CLASS B1152+199 and B1359+154: Two New Gravitational Lens Systems Discovered in the Cosmic Lens All-Sky Survey
Creators: name: Myers, S. T.
name: Rusin, D.
name: Fassnacht, C. D.
name: Blandford, R. D.
name: Pearson, T. J.
name: Readhead, A. C. S.
name: Jackson, N.
name: Browne, I. W. A.
name: Marlow, D. R.
name: Wilkinson, P. N.
name: Koopmans, L. V. E.
name: de Bruyn, A. G.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: The third phase of the Cosmic Lens All-Sky Survey (CLASS) has recently been completed, bringing the total number of sources imaged to over 15000 in the CLASS and JVAS combined survey. In the VLA observations carried out in March and April of 1998, two new candidate lensed systems were discovered: CLASS B1152+199 and B1359+154. B1152+199 is a 1.6 arcsecond double, with a background quasar at z=1.019 lensed by a foreground galaxy at z=0.439. The relatively flat radio spectra of the lensed images, combined with a previous ROSAT detection of the source, make B1152+199 a strong candidate for time delay studies at both radio and X-ray wavelengths. B1359+154 is a quadruply lensed quasar at z=3.235, with a maximum image separation of 1.7 arcseconds. As yet, the redshift of the lensing object in this system is undetermined. The steep spectral index of the source suggests that B1359+154 will not exhibit strong variability, and is therefore unlikely to be useful for determining the Hubble constant from measured time delays.
description: accepted for publication in The Astronomical Journal
Study of the Decay $Λ_c \to Λl^+ ν_{l}
Creators: name: The CLEO Collaboration
Publisher: name: arXiv
Year: 1994
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: High Energy Physics - Experiment (hep-ex)
subject: FOS: Physical sciences

description: Using the CLEO II detector at CESR, we observe 500 $Λl^+$ pairs consistent with the semileptonic decay $Λ_c \to Λl^+ ν_{l}$. We measure $σ(e^+ e^- \to Λ_c X) \dot {cal B}(Λ_c^+ \to Λl ν_{l}) =4.77 \pm 0.25 \pm 0.66 $pb. Combining with the charm semileptonic width and the lifetime of the $Λ_c$, we also obtain ${\cal B}(Λ_c \to p K^- π^+)$. We find no evidence for $Λl^+ ν_{l}$ final states in which there are additional $Λ_c^+$ decay products. We measure the decay asymmetry parameter of $Λ_c \to Λl^+ ν_{l}$ to be $α_{Λ_c} =-0.89\pm{^{0.17}_{0.11}}\pm{^{0.09}_{0.06}}.
description: 18 pages uuencoded compressed postscript (process with uudecode then gunzip). hardcopies with figures can be obtained by sending mail to: preprints@lns62.lns.cornell.edu
Design and test of 704 MHz and 2.1 GHz normal conducting cavities for Low Energy RHIC electron Cooler
Creators: name: Xiao, Binping
name: Belomestnykh, S.
name: Brennan, J. M.
name: Brutus, J. C.
name: McIntyre, G.
name: Mernick, K.
name: Pai, C.
name: Smith, K.
name: Xin, T.
name: Zaltsman, A.
name: Veshcherevich, V.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Accelerator Physics (physics.acc-ph)
subject: FOS: Physical sciences

description: The Low Energy RHIC electron Cooler (LEReC) is currently under commissioning at BNL to improve RHIC luminosity for heavy ion beam energies below 10 GeV/nucleon. The linac of LEReC consists of a DC photoemission gun, one 704 MHz superconducting radio frequency (SRF) booster cavity, and three normal conducting cavities. It is designed to deliver a 1.6 MeV to 2.6 MeV electron beam, with peak-to-peak momentum spread dp/p of less than 7e4. Two of the three normal conducting cavities will be used in LEReC for energy spread correction. A single-cell 704 MHz cavity for energy de-chirping and a three-cell 2.1 GHz third harmonic cavity for RF curvature correction. In this paper, we present the designs and RF test results of these two cavities.
description: 10 pages, 10 figures
Meganola tenebrosa
Creators: name: László, Gyula M.
name: Sterling, Mark
Publisher: name: Zenodo
Year: 2020
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Lepidoptera
Nolidae
Meganola
Meganola tenebrosa

description: Meganola tenebrosa (Hampson, 1896) (Figs 14, 77)
Nola tenebrosa Hampson, 1896, Fauna of British India, Moths 4: 504. Type-locality: Bhutan. Holotype: female, in coll. NHMUK.
Material examined:
China, Hong Kong. 1 male, Tai Yeung Che, Lam Tsuen, Tai Po, New Territories, 22.4472°N, 114.1285°E, 65m a.s.l., 125W Robinson, 15.5.2016, leg. M.J. Sterling, slide No.: LGN 2888 (coll. M. Sterling).
description: Published as part of László, Gyula M. & Sterling, Mark, 2020, Illustrated checklist of Nolinae (Lepidoptera, Nolidae) of Hong Kong, China, with description of two new species, pp. 35-58 in Ecologica Montenegrina 33 on page 55, DOI: 10.37828/em.2020.33.6, http://zenodo.org/record/8029131
Cancer araneus Linnaeus, 1758, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1758
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Malacostraca
Decapoda
Cancridae
Cancer
Cancer araneus

description: Cancer araneus [spec. nov.]
C. brachyurus, thorace hirsuto ovato tuberculato, rostro bifido, manibus ovatis.
Fn. svec. 1246.
Iter. scanic. 312. @/ Jonst. exsangu. t. 5. f. 13.
Habitat in Oceano Europaeo.
description: Published as part of Linnaeus, Carolus, 1758, Systema Naturae per regna tria naturae: secundum classes, ordines, genera, species, cum characteribus, differentiis, synonymis, locis, Stockholm :Laurentius Salvius on page 628, DOI: 10.5962/bhl.title.542, http://zenodo.org/record/3922206
Additional file 2: of How do the experiences and beliefs of adults and children with heterozygous familial hypercholesterolaemia influence their adherence to treatment? A systematic review of qualitative evidence protocol
Creators: name: Kinnear, Fiona
name: Perry, Rachel
name: Searle, Aidan
name: Hamilton-Shield, Julian
name: Lithander, Fiona
Publisher: name: figshare
Year: 2018
Subjects: subject: Medicine
subject: Pharmacology
subject: Developmental Biology
subject: 111714 Mental Health
subject: FOS: Health sciences
subject: 110309 Infectious Diseases

description: Draft MEDLINE search strategy. (DOCX 14Â kb)
Flux Sensitivity of VERITAS
Creators: name: Vassiliev, Vladimir V.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: VERITAS is a new major ground-based gamma-ray observatory with an array of seven 10 m optical reflectors to be built at the Whipple Observatory in southern Arizona, USA. It will consist of an array of imaging Cherenkov telescopes designed to conduct critical measurements of AGNs and SNRs in the energy range of 50 GeV - 50 TeV. The design of the array has been optimized for the highest sensitivity to point sources in the 100 GeV - 10 TeV band when the stereoscopic imaging technique is employed. Maximum versatility of the array has been another major optimization criterion. We present the flux sensitivity of the baseline VERITAS configuration.
description: 5 pages, 1 figure, presented at VERITAS Workshop on TeV Astrophysics of Extragalactic Sources, Cambridge, MA, Oct. 23-24, 1998. In press, Astroparticle Physics, ed. M. Catanese, J. Quinn, T. Weekes
Sharp quantization for Lane-Emden problems in dimension two
Creators: name: Thizy, Pierre-Damien
Publisher: name: arXiv
Year: 2018
Subjects: subject: Analysis of PDEs (math.AP)
subject: FOS: Mathematics

description: In this short note, we prove a sharp quantization for positive solutions of Lane-Emden problems in a bounded planar domain. This result has been conjectured by De Marchis, Ianni and Pacella [6, Remark 1.2].
Precision Measurement of the $D_s^{*+}- D_s^+$ Mass Difference
Creators: name: The CLEO Collaboration
Publisher: name: arXiv
Year: 1994
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: High Energy Physics - Experiment (hep-ex)
subject: FOS: Physical sciences

description: We have measured the vector-pseudoscalar mass splitting $M(D_s^{*+})-M(D_s^+) = 144.22\pm 0.47\pm 0.37 MeV$, significantly more precise than the previous world average. We minimize the systematic errors by also measuring the vector-pseudoscalar mass difference $M(D^{*0})-M(D^0)$ using the radiative decay $D^{*0}\rightarrow D^0γ$, obtaining $[M(D_s^{*+})-M(D_s^+)]-[M(D^{*0})-M(D^0)] = 2.09\pm 0.47\pm 0.37 MeV$. This is then combined with our previous high-precision measurement of $M(D^{*0})-M(D^0)$, which used the decay $D^{*0}\rightarrow D^0π^0$. We also measure the mass difference $M(D_s^+)-M(D^+)=99.5\pm 0.6\pm 0.3$ MeV, using the $ϕπ^+$ decay modes of the $D_s^+$ and $D^+$ mesons.
description: 18 pages uuencoded compressed postscript (process with uudecode then gunzip). hardcopies with figures can be obtained by sending mail to: preprints@lns62.lns.cornell.edu
title: ADCO, Ordre cistercien et abbaye de Cîteaux : comptes pour l'ordre (1337-1347), comptes du boursier (1377-1402) (11 H 1160), f. 00482
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/2017
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2020
Subjects: subject: comptes
subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris
subject: Corpus Burgundiae Medii Aevi
subject: Chartes de la Bourgogne du Moyen Âge

description: Ordre cistercien et abbaye de Cîteaux : comptes pour l'ordre (1337-1347), comptes du boursier (1377-1402), Archives départementales de la Côte-d'Or, (11 H 1160). Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Ordre cistercien et abbaye de Cîteaux : comptes pour l'ordre (1337-1347), comptes du boursier (1377-1402), Archives départementales de la Côte-d'Or, (11 H 1160), f. 00482, 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
Cancer cuphaeus Linnaeus, 1758, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1758
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Malacostraca
Decapoda
Cancridae
Cancer
Cancer cuphaeus

description: Cancer cuphaeus [spec. nov.]
C. brachyurus, thorace villoso ovato antice obtuso, postice tridentato.
Rumph. mus. t. 10. f. D?
Habitat in Asia.
description: Published as part of Linnaeus, Carolus, 1758, Systema Naturae per regna tria naturae: secundum classes, ordines, genera, species, cum characteribus, differentiis, synonymis, locis, Stockholm :Laurentius Salvius on page 628, DOI: 10.5962/bhl.title.542, http://zenodo.org/record/3922206
Biological arsenite oxidation with nitrate as sole electron acceptor
Creators: name: Wang, Jie
name: Wan, Junfeng
name: Li, Haisong
name: Li, Hongli
name: Dagot, Christophe
name: Wang, Yan
Publisher: name: Taylor & Francis
Year: 2016
Subjects: subject: Biochemistry
subject: Space Science
subject: Molecular Biology
subject: Environmental Sciences not elsewhere classified
subject: Chemical Sciences not elsewhere classified
subject: Ecology
subject: FOS: Biological sciences
subject: Biological Sciences not elsewhere classified
subject: Inorganic Chemistry
subject: FOS: Chemical sciences

description: The potential of anoxic biological arsenite oxidation with nitrate as the sole electron acceptor was tested by using the acclimatized activated sludge which was chronically exposed under arsenite and nitrate coexisted aquatic environment. The activated sludge cultivated in a sequencing batch reactor was fed with arsenite and nitrate as the main substrates over six months. A series of batch experiments were conducted with acclimated sludge. Results showed that no obvious inhibition was observed in the anoxic arsenite oxidation linked to nitrate and nitrite reduction at the concentration of arsenite up to 35 mg AsIII L−1. Moreover, it was found that nitrite was accumulated over the reaction probably due to limited availability of arsenite. The kinetic study further suggested that the maximum specific arsenite oxidation rates (qobs, max) with nitrate and nitrite as the electron acceptors were found to be 0.55 ± 0.10 mg AsIII g−1VSS min−1 and 0.40 ± 0.04 mg AsIII g−1VSS min−1, respectively.
Meganola basisignata Inoue 1991
Creators: name: Yu, Yong
name: Xu, Wen
name: Huang, Zhen-Fu
name: Hu, Yan-Qing
Publisher: name: Zenodo
Year: 2025
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Lepidoptera
Nolidae
Meganola
Meganola basisignata

description: Meganola basisignata Inoue, 1991
Meganola basisignata Inoue, 1991: 69. Type locality: Japan, Honshu, Miyagi pref., Sakunami Spa.
Distribution. Japan (Honshu).
description: Published as part of Yu, Yong, Xu, Wen, Huang, Zhen-Fu & Hu, Yan-Qing, 2025, Description of a new species of the Meganola tenebrosa (Hampson, 1896) species-group from China (Lepidoptera: Noctuoidea: Nolidae), pp. 396-400 in Zootaxa 5588 (2) on page 397, DOI: 10.11646/zootaxa.5588.2.13, http://zenodo.org/record/14896420
A Successive-Elimination Approach to Adaptive Robotic Sensing
Creators: name: Rolf, Esther
name: Fridovich-Keil, David
name: Simchowitz, Max
name: Recht, Benjamin
name: Tomlin, Claire
Publisher: name: arXiv
Year: 2018
Subjects: subject: Machine Learning (cs.LG)
subject: Robotics (cs.RO)
subject: Machine Learning (stat.ML)
subject: FOS: Computer and information sciences

description: We study an adaptive source seeking problem, in which a mobile robot must identify the strongest emitter(s) of a signal in an environment with background emissions. Background signals may be highly heterogeneous and can mislead algorithms that are based on receding horizon control. We propose AdaSearch, a general algorithm for adaptive source seeking in the face of heterogeneous background noise. AdaSearch combines global trajectory planning with principled confidence intervals in order to concentrate measurements in promising regions while guaranteeing sufficient coverage of the entire area. Theoretical analysis shows that AdaSearch confers gains over a uniform sampling strategy when the distribution of background signals is highly variable. Simulation experiments demonstrate that when applied to the problem of radioactive source seeking, AdaSearch outperforms both uniform sampling and a receding time horizon information-maximization approach based on the current literature. We also demonstrate AdaSearch in hardware, providing further evidence of its potential for real-time implementation.
Additional file 1: of How do the experiences and beliefs of adults and children with heterozygous familial hypercholesterolaemia influence their adherence to treatment? A systematic review of qualitative evidence protocol
Creators: name: Kinnear, Fiona
name: Perry, Rachel
name: Searle, Aidan
name: Hamilton-Shield, Julian
name: Lithander, Fiona
Publisher: name: figshare
Year: 2018
Subjects: subject: Medicine
subject: Pharmacology
subject: Biotechnology
subject: Science Policy
subject: 110309 Infectious Diseases
subject: FOS: Health sciences

description: PRISMA-P (Preferred Reporting Terms for Systematic Review and Meta-analysis Protocol(s) 2015 checklist: recommended items to address in a systematic review protocol. PRISMA (Preferred Reporting Terms for Systematic Review and Meta-Analysis) is an evidence-based minimum set of terms for reporting in systematic reviews and meta-analyses. (DOCX 29Â kb)
When does a perturbed Moser-Trudinger inequality admit an extremal?
Creators: name: Thizy, Pierre-Damien
Publisher: name: arXiv
Year: 2018
Subjects: subject: Analysis of PDEs (math.AP)
subject: FOS: Mathematics

description: In this paper, we are interested in several questions raised mainly in [17]. We consider the perturbed Moser-Trudinger inequality $I\_α^g(Ω)$ below, at the critical level $α=4π$, where $g$, satisfying $g(t)\to 0$ as $t\to +\infty$, can be seen as a perturbation with respect to the original case $g\equiv 0$. Under some additional assumptions, ensuring basically that $g$ does not oscillates too fast as $t\to +\infty$, we identify a new condition on $g$ for this inequality to have an extremal. This condition covers the case $g\equiv 0$ studied in [3,12,23]. We prove also that this condition is sharp in the sense that, if it is not satisfied, $I\_{4π}^g(Ω)$ may have no extremal.
A Measurement of ${\cal B}(D_s \to ϕl^+ ν)/{cal B}(D_s\to ϕπ^+)$
Creators: name: The CLEO Collaboration
Publisher: name: arXiv
Year: 1994
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: High Energy Physics - Experiment (hep-ex)
subject: FOS: Physical sciences

description: Using the CLEO~II detector at CESR, we have measured the ratio of branching fractions ${\cal B}(D_s^+ \to ϕe^+ ν)/{\cal B}(D_s^+ \to ϕπ^+) = 0.54\pm 0.05\pm 0.04$. We use this measurement to obtain a model dependent estimate of ${\cal B}(D_s^+ \to ϕπ^+)$.
description: 19 pages uuencoded compressed postscript (process with uudecode then gunzip). hardcopies with figures can be obtained by sending mail to: preprints@lns62.lns.cornell.edu
Additional file 9 of Early-life exposures and age at thelarche in the Sister Study cohort
Creators: name: Goldberg, Mandy
name: D’Aloisio, Aimee A.
name: O’Brien, Katie M.
name: Zhao, Shanshan
name: Sandler, Dale P.
Publisher: name: figshare
Year: 2021
Subjects: Medicine
Biotechnology
Environmental Sciences not elsewhere classified
Developmental Biology
Cancer
Science Policy
Mental Health

description: Additional file 9: Table S6. Associations between early-life exposures and timing of thelarche in the Sister Study cohort by Bayesian family history score (BFHS) (N = 49,151)
The connection between X-ray Clusters and Star Formation
Creators: name: Tozzi, Paolo
name: Norman, Colin
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: The properties of X-ray clusters of galaxies can be well understood in terms of a competition between shock heating and adiabatic compression. Strong shocks are expected to be important for massive clusters, while adiabatic compression is dominant for small clusters and groups. The scale of the shock/adiabatic transition is marked by a change of slope of the L-T relation and in the global properties of the emitting plasma. This scale is connected to star formation processes. Two quantities are crucial: the average energy injected in the IGM from stars and SNe, and the epoch of the energy injection. We show how these quantities can be synthesized in terms of specific entropy, which ultimately determines the X-ray emission from groups and clusters.
description: 4 pages, including 2 figures, LaTex2e. To be published in the Proceedings of the ``VLT Opening Symposium'', Antofagasta (Chile), 1-4 March 1999. Typos changed in eq. (3)
Measurement of Cabibbo Suppressed Decays of the $τ$ Lepton
Creators: name: The CLEO Collaboration
Publisher: name: arXiv
Year: 1994
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: High Energy Physics - Experiment (hep-ex)
subject: FOS: Physical sciences

description: Branching ratios for the dominant Cabibbo-suppressed decays of the $τ$ lepton have been measured by CLEO~II in $e^+ e^-$ annihilation at CESR ($\sqrt{s} \sim 10.6$~GeV) using kaons with momenta below $0.7\ \rm GeV/c$. The inclusive branching ratio into one charged kaon is $(1.60 \pm 0.12 \pm 0.19)\%$. For the exclusive decays, $B(τ\to K^-) = (0.66 \pm 0.07 \pm 0.09)\%$, $B(τ\to K^- π^0) = (0.51 \pm 0.10 \pm 0.07)\%$, and, based on three events, $B(τ\to K^- π^0 π^0) < 0.3\%$ at the 90\% confidence level. These represent significant improvements over previous results. $B(τ\to K^- π^0)$ is measured for the first time with exclusive $π^0$ reconstruction.
description: 11 pages uuencoded compressed postscript (process with uudecode then gunzip). hardcopies with figures can be obtained by sending mail to: preprints@lns62.lns.cornell.edu
The specific entropy of elliptical galaxies: an explanation for profile-shape distance indicators?
Creators: name: Neto, Gastao B. Lima
name: Gerbal, Daniel
name: Marquez, Isabel
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Dynamical systems in equilibrium have a stationary entropy; we suggest that elliptical galaxies, as stellar systems in a stage of quasi-equilibrium, may have a unique specific entropy. This uniqueness, a priori unknown, should be reflected in correlations between the parameters describing the mass (light) distribution in galaxies. Following recent photometrical work (Caon et al. 1993; Graham & Colless 1997; Prugniel & Simien 1997), we use the Sersic law to describe the light profile of elliptical galaxies and an analytical approximation to its three dimensional deprojection. The specific entropy is calculated supposing that the galaxy behaves as a spherical, isotropic, one-component system in hydrostatic equilibrium, obeying the ideal gas state equations. We predict a relation between the 3 parameters of the Sersic, defining a surface in the parameter space, an `Entropic Plane', by analogy with the well-known Fundamental Plane. We have analysed elliptical galaxies in Coma and ABCG 85 clusters and a group of galaxies (associated with NGC 4839). We show that the galaxies in clusters follow closely a relation predicted by the constant specific entropy hypothesis with a one-sigma dispersion of 9.5% around the mean value of the specific entropy. Assuming that the specific entropy is also the same for galaxies of different clusters, we are able to derive relative distances between the studied clusters. If the errors are only due to the determination of the specific entropy (about 10%), then the error in the relative distance determination should be less than 20% for rich clusters. We suggest that the unique specific entropy may provide a physical explanation for the distance indicators based on the Sersic profile put forward by Young & Currie (1994, 1995) and discussed by Binggeli & Jerjen (1998).
description: Submitted to MNRAS (05/05/99), 15 pages, 10 figures
Meganola guentereberti Laszlo, Ronkay & Ronkay 2014
Creators: name: Yu, Yong
name: Xu, Wen
name: Huang, Zhen-Fu
name: Hu, Yan-Qing
Publisher: name: Zenodo
Year: 2025
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Lepidoptera
Nolidae
Meganola
Meganola guentereberti

description: Meganola guentereberti László, Ronkay & Ronkay, 2014
Meganola guentereberti László, Ronkay & Ronkay, 2014: 38. Type locality: Nepal, Annapurna Himal, Tadapani.
Distribution. Nepal, Pakistan, Afghanistan.
description: Published as part of Yu, Yong, Xu, Wen, Huang, Zhen-Fu & Hu, Yan-Qing, 2025, Description of a new species of the Meganola tenebrosa (Hampson, 1896) species-group from China (Lepidoptera: Noctuoidea: Nolidae), pp. 396-400 in Zootaxa 5588 (2) on page 397, DOI: 10.11646/zootaxa.5588.2.13, http://zenodo.org/record/14896420
Additional file 1: of A systematic review and meta-analysis of epidemiology of depression in people living with HIV in east Africa
Creators: name: Getinet Ayano
name: Melat Solomon
name: Mebratu Abraha
Publisher: name: figshare
Year: 2018
Subjects: subject: Medicine
subject: Biotechnology
subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences
subject: 19999 Mathematical Sciences not elsewhere classified
subject: FOS: Mathematics
subject: Science Policy

description: Table S1. Summary of agreed level of bias and level of agreement on the methodological qualities of included studies in meta-analysis based on sampling, outcome, response rate and method of analysis. (DOCX 15 kb)
Cancer muscosus Linnaeus, 1758, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1758
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Malacostraca
Decapoda
Cancridae
Cancer
Cancer muscosus

description: Cancer muscosus [spec. nov.]
C. brachyurus, thorace villoso utrinque tridentato, rostro bidentato: lateribus unidentato.
Habitat in M. Mediterraneo. E. Brander.
Magnitudo glandis. Testa obovata, villis mollissimis incurvis hirsuta, ad utrumqae latus spinis 3 subulatis. Rostrum spinis 2 subulatis parallelis cum dente compresso ad utrumque latus rostri. Ungues pedum subulati, curvi, introrsum dentati. Chelae laeves, lineares, carpo utrinque dente obtuso retrorsum spectante.
description: Published as part of Linnaeus, Carolus, 1758, Systema Naturae per regna tria naturae: secundum classes, ordines, genera, species, cum characteribus, differentiis, synonymis, locis, Stockholm :Laurentius Salvius on page 628, DOI: 10.5962/bhl.title.542, http://zenodo.org/record/3922206
Production and Decay of D_1(2420)^0 and D_2^*(2460)^0
Creators: name: The CLEO Collaboration
Publisher: name: arXiv
Year: 1994
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: High Energy Physics - Experiment (hep-ex)
subject: FOS: Physical sciences

description: We have investigated $D^{+}π^{-}$ and $D^{*+}π^{-}$ final states and observed the two established $L=1$ charmed mesons, the $D_1(2420)^0$ with mass $2421^{+1+2}_{-2-2}$ MeV/c$^{2}$ and width $20^{+6+3}_{-5-3}$ MeV/c$^{2}$ and the $D_2^*(2460)^0$ with mass $2465 \pm 3 \pm 3$ MeV/c$^{2}$ and width $28^{+8+6}_{-7-6}$ MeV/c$^{2}$. Properties of these final states, including their decay angular distributions and spin-parity assignments, have been studied. We identify these two mesons as the $j_{light}=3/2$ doublet predicted by HQET. We also obtain constraints on {\footnotesize $Γ_S/(Γ_S + Γ_D)$} as a function of the cosine of the relative phase of the two amplitudes in the $D_1(2420)^0$ decay.
description: 15 pages in REVTEX format. hardcopies with figures can be obtained by sending mail to: preprints@lns62.lns.cornell.edu
Two-Photon Production of Charged Pion and Kaon Pairs
Creators: name: The CLEO Collaboration
Publisher: name: arXiv
Year: 1994
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: High Energy Physics - Experiment (hep-ex)
subject: FOS: Physical sciences

description: A measurement of the cross section for the combined two-photon production of charged pion and kaon pairs is performed using 1.2~$\rm fb^{-1}$ of data collected by the CLEO~II detector at the Cornell Electron Storage Ring. The cross section is measured at invariant masses of the two-photon system between 1.5 and 5.0 GeV/$c^2$, and at scattering angles more than $53^\circ$ away from the $γγ$ collision axis in the $γγ$ center-of-mass frame. The large background of leptonic events is suppressed by utilizing the CsI calorimeter in conjunction with the muon chamber system. The reported cross section is compared with leading order QCD models as well as previous experiments. In particular, although the functional dependence of the measured cross section disagrees with leading order QCD at small values of the two-photon invariant mass, the data show a transition to perturbative behavior at an invariant mass of approximately 2.5 GeV/$c^2$. hardcopies with figures can be obtained by writing to to: Pam Morehouse preprint secretary Newman Lab Cornell University Ithaca, NY 14853 or by sending mail to: preprints@lns62.lns.cornell.edu
description: 15 pages (in REVTEX format)
Two-level systems and growth-induced metastability in hydrogenated amorphous silicon
Creators: name: Molina-Ruiz, M.
name: Jacks, H. C.
name: Queen, D. R.
name: Wang, Q.
name: Crandall, R. S.
name: Hellman, F.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Materials Science (cond-mat.mtrl-sci)
subject: FOS: Physical sciences

description: Specific heat measurements from 2 to 300 K of hydrogenated amorphous silicon prepared by hot-wire chemical vapor deposition show a large excess specific heat at low temperature, significantly larger than the Debye specific heat calculated from the sound velocity. The as-prepared films have a Schottky anomaly that is associated with metastable hydrogen in the amorphous network, as well as large linear and excess cubic term commonly associated with tunneling two-level systems in amorphous solids. Annealing at 200 °C, a temperature that enables hydrogen mobility but not evaporation, irreversibly reduces the heat capacity, eliminating the Schottky anomaly and leaving a reduced linear heat capacity. A non-monotonic dependence on growth temperature and H content is observed in all effects, except for sound velocity, which suggests that the tunneling two-level systems and the Schottky anomaly are associated with atomic hydrogen and require low density regions to form, while sound velocity is associated with the silicon network and improves with increasing growth temperature.
description: 17 pages, 3 figures, 1 table
MOF-derived multi-interface carbon-based composites with enhanced polarization loss and efficient microwave absorption
Creators: name: Qu, Hongjiao
name: Zheng, Peng
name: Wang, Tao
name: Yu, Xingyu
name: Pan, Junjie
name: Fan, Xiaoli
name: Zhang, Tengfei
name: Sun, Xin
name: He, Jianping
Publisher: name: Taylor & Francis
Year: 2022
Subjects: Biochemistry
Space Science
Physical Sciences not elsewhere classified
Biotechnology
Chemical Sciences not elsewhere classified

description: Metal-organic framework materials (MOFs) have been widely studied because of their adjustable composition and controllable structure in the field of microwave absorption (MA). Therein, Prussian blue analogs (PBA) have attracted the attention of researchers with ultra-high metal content. However, the attenuation ability of microwave for PBA-based composites is still unsatisfactory up to now. Therefore, the NiFe/CoFe@C composites were prepared by carbonizing polymetallic PBA (NiCoFe PBA) materials in this work, and the influence of different metal alloy components on MA was explored by adjusting the ratio of metal ions (Ni2+/Co2+). Moreover, the NiFe/CoFe@C composites have rich interfaces and enhance the polarization loss due to the introduction of Ni and it has an optimal performance at 2.7 mm that is the reflection loss (RL) is −41.49 dB and an effective absorption bandwidth (EAB) is 7.12 GHz with 1/1 (Ni2+/Co2+). The above data provides a research idea for obtaining light and efficient absorbers.
Additional file 1: of Safer tattooing interventions in prisons: a systematic review and call to action
Creators: name: Nguyen Tran
name: CĂŠlestine Dubost
name: StĂŠphanie Baggio
name: GĂŠtaz, Laurent
name: Wolff, Hans
Publisher: name: figshare
Year: 2018
Subjects: subject: Medicine
subject: Sociology
subject: FOS: Sociology
subject: Developmental Biology

description: English translation of notes from in-depth interviews with nursing staff from the Luxemburg detention center. (DOCX 19 kb)
Hot fusion reactions with deformed nuclei for synthesis of superheavy nuclei: an extension of the fusion-by-diffusion model
Creators: name: Hagino, K.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Nuclear Theory (nucl-th)
subject: Nuclear Experiment (nucl-ex)
subject: FOS: Physical sciences

description: The fusion-by-diffusion model proposed by Swiatecki {\it et al.} [Phys. Rev. C71, 014602 (2005)] has provided a simple and convenient tool to estimate evaporation residue cross sections for superheavy nuclei. I extend this model by taking into account deformation of the target nucleus, and discuss the role of orientation of deformed target in hot fusion reactions at energies around the Coulomb barrier. To this end, I introduce an injection point for the diffusion process over an inner barrier which depends on the orientation angle. I apply this model to the $^{48}$Ca+$^{248}$Cm reaction and show that the maximum of evaporation residue cross section appears at an energy slightly above the height of the capture barrier for the side collision, for which the effective inner barrier is considerably lower than that for the tip collision, thus enhancing the diffusion probability. I also discuss the energy dependence of the injection point, and show that a large part of the energy dependence found in the previous analyses can be attributed to the deformation effect of a target nucleus.
description: 12 pages, 6 figures
Physical Conditions in Regions of Star Formation
Creators: name: Evans, Neal J.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: The physical conditions in molecular clouds control the nature and rate of star formation, with consequences for planet formation and galaxy evolution. The focus of this review is on the conditions that characterize regions of star formation in our Galaxy. A review of the tools and tracers for probing physical conditions includes summaries of generally applicable results. Further discussion distinguishes between the formation of low-mass stars in relative isolation and formation in a clustered environment. Evolutionary scenarios and theoretical predictions are more developed for isolated star formation, and observational tests are beginning to interact strongly with the theory. Observers have identified dense cores collapsing to form individual stars or binaries, and analysis of some of these support theoretical models of collapse. Stars of both low and high mass form in clustered environments, but massive stars form almost exclusively in clusters. The theoretical understanding of such regions is considerably less developed, but observations are providing the ground rules within which theory must operate. The most rich and massive star clusters form in massive, dense, turbulent cores, which provide models for star formation in other galaxies.
description: 48 pages, annual review latex, 4 figures supplied, 2 not supplied
Measurement of the Branching Fraction for D^+ \to K^- π^+ π^+
Creators: name: The CLEO Collaboration
Publisher: name: arXiv
Year: 1994
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: High Energy Physics - Experiment (hep-ex)
subject: FOS: Physical sciences

description: Using the CLEO-II detector at CESR we have measured the ratio of branching fractions, ${\cal B}(D^+\rightarrow K^- π^+ π^+)/{\cal B}(D^0 \rightarrow K^-π^+) = 2.35 \pm 0.16 \pm 0.16$. Our recent measurement of ${\cal B}(D^0 \rightarrow K^-π^+)$ then gives ${\cal B}(D^+\rightarrow K^- π^+ π^+) = (9.3 \pm 0.6 \pm 0.8)\%$.
description: 6 pages (in REVTEX format). hardcopies with figures can be obtained by sending mail to: preprints@lns62.lns.cornell.edu
Workflow for designing instructional videos to support place-based geoscience education for geoscience majors
Creators: name: Wang, Ning
name: Stern, Robert J.
name: Waite, Lowell
Publisher: name: Taylor & Francis
Year: 2022
Subjects: subject: Space Science
subject: Microbiology
subject: FOS: Biological sciences
subject: Genetics
subject: Neuroscience
subject: Environmental Sciences not elsewhere classified
subject: Biological Sciences not elsewhere classified
subject: Science Policy
subject: Plant Biology

description: Geographic context is important for Earth Science education but different places have different geological complexities and effectively establishing geoscientific context can be difficult. Well-designed videos can help geoscience educators introduce geologically significant places to undergraduate geoscience students. However, there is no established framework to guide geoscientists who want to create instructional videos for place-based geoscience education. In this commentary, we share a framework including writing a narrative and generating visual materials as well as considering key psychological principles and universal design elements to improve geoscience video effectiveness. The design framework was created based on the place-based education framework, salient elements of cognitive theory of multimedia learning, and the framework of motivational design. More design recommendations were given by summarizing our experience of making and assessing a 6-minute geosicence video about the Permian Basin of W. Texas and SE New Mexico and other best practice of making the same type of videos in peer reviewed articles. We find that well-designed geoscience videos can improve geoscience majors’ knowledge about local geology and understanding of connections between place and people. The generalized video-making workflow and design recommendations can help geoscientists make their own geoscientific videos for undergraduates.
MOESM1 of Unhealthy weight among children in Spain and the role of the home environment
Creators: name: Vaquera, Elizabeth
name: Jones, Rebecca
name: Marí-Klose, Pau
name: Marí-Klose, Marga
name: Cunningham, Solveig
Publisher: name: figshare
Year: 2018
Subjects: subject: Medicine
subject: Ecology
subject: FOS: Biological sciences
subject: Sociology
subject: FOS: Sociology
subject: 69999 Biological Sciences not elsewhere classified
subject: Science Policy
subject: 110309 Infectious Diseases
subject: FOS: Health sciences
subject: Computational Biology

description: Additional file 1. Encuesta de Relaciones Inter e Intrageneracionales en la Infancia 2010. Questionnaire for Children 5–10 years. This is the full questionnaire for families with children 5–10 used for data collection in Spanish.
title: ADCO, Comptes du Petit-Cîteaux (1477-1491) (11 H 1179), f. 00051
Creators: name: de la Côte d'Or, Archives départementales
name: Archives Départementales De La Côte D'Or
name: Petot, Frédérique
name: Projet CBMA
name: Petot, Frédéric
name: Archives Départementales De La Côte-D'Or
name: CBMA/CG21/F.PETOT/2019
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2020
Subjects: subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris
subject: Corpus Burgundiae Medii Aevi
subject: Chartes de la Bourgogne du Moyen Âge
subject: cartulaire
subject: comptes

description: Comptes du Petit-Cîteaux (1477-1491), Archives départementales de la Côte-d'Or, (11 H 1179). Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Comptes du Petit-Cîteaux (1477-1491), Archives départementales de la Côte-d'Or, (11 H 1179), f. 00051, 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
Schwarzschild black hole encircled by a rotating thin disc: Properties of perturbative solution
Creators: name: Kotlařík, P.
name: Semerák, O.
name: Čížek, P.
Publisher: name: arXiv
Year: 2018
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: In ApJ (1974), Will solved the perturbation of a Schwarzschild black hole due to a slowly rotating light concentric thin ring, using Green's functions expressed as infinite-sum expansions in multipoles and in the small mass and rotational parameters. In a previous paper (ApJS 2017, Paper I), we expressed the Green functions in closed form containing elliptic integrals, leaving just summation over the mass expansion. Such a form is more practical for numerical evaluation, but mainly for generalizing the problem to extended sources where the Green functions have to be integrated over the source. We exemplified the method by computing explicitly the first-order perturbation due to a slowly rotating thin disc lying between two finite radii. After finding basic parameters of the system -- mass and angular momentum of the black hole and of the disc -- we now add further properties, namely those which reveal how the disc gravity influences geometry of the black-hole horizon and those of circular equatorial geodesics (specifically, radii of the photon, marginally bound and marginally stable orbits). We also realize that, in the linear order, no ergosphere occurs and the central singularity remains point-like, and check the implications of natural physical requirements (energy conditions and subluminal restriction on orbital speed) for the single-stream as well as counter-rotating double-stream interpretations of the disc.
description: 14 pages, 7 figures
Hard X-ray emission from elliptical galaxies
Creators: name: Allen, S. W.
name: Di Matteo, T.
name: Fabian, A. C.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We report the detection of hard X-ray emission components in the spectra of six nearby, giant elliptical galaxies observed with the ASCA satellite. The systems studied, which exhibit strong dynamical evidence for supermassive black holes in their nuclei, are M87, NGC 1399 and NGC 4696 (the dominant galaxies of the Virgo, Fornax and Centaurus clusters, respectively) and NGC 4472, 4636 and 4649 (three further giant ellipticals in the Virgo cluster). The ASCA data for all six sources provide clear evidence for hard emission components, which can be parameterized by power-law models with photon indices in the range Γ= 0.6-1.5 (mean value 1.2) and intrinsic 1-10 keV luminosities of 2 \times 10^{40} - 2 \times 10^{42} erg/s. Our results imply the identification of a new class of accreting X-ray source, with X-ray spectra significantly harder than those of binary X-ray sources, Seyfert nuclei or low luminosity AGN, and bolometric luminosities relatively dominated by their X-ray emission. We discuss various possible origins for the hard X-ray emission and argue that it is most likely to be due to accretion onto the central supermassive black holes, via low-radiative efficiency accretion coupled with strong outflows. In the case of M87, our detected power-law flux is in good agreement with a previously-reported measurement from ROSAT High Resolution Imager observations, which were able to resolve the jet from the nuclear X-ray emission components. We confirm previous results showing that the use of multiphase models in the analysis of the ASCA data leads to determinations of approximately solar emission-weighted metallicities for the X-ray gas in the galaxies. We also present results on the individual element abundances in NGC 4636.
description: MNRAS in press. 15 pages, 3 figures in MNRAS LaTex style. Minor modifications. Some additional results supporting original conclusions
A Measurement of the Branching Fraction ${\cal B} τ^+ \to h^- π^0 ν_τ$
Creators: name: The CLEO Collaboration
Publisher: name: arXiv
Year: 1994
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: High Energy Physics - Experiment (hep-ex)
subject: FOS: Physical sciences

description: Using data from the CLEO II detector at CESR, we measure ${\cal B}(τ^\pm\rightarrow h^\pmπ^0ν_τ)$ where $h^\pm$ refers to either $π^\pm$ or $K^\pm$. We use three different methods to measure this branching fraction. The combined result is ${\cal B}(τ^\pm\rightarrow h^\pmπ^0ν_τ) = 0.2587 \pm 0.0012 \pm 0.0042$, in good agreement with Standard Model predictions. This result, in combination with other precision measurements, reduces the significance of the one-prong problem in tau decays. A postscript version is available through World-Wide-Web in http://w4.lns.cornell.edu/public/CLNS/1994/
description: 9 pages (in REVTEX format) Preprint CLNS94-1281, CLEO 94-11
Meganola margalla Laszlo, Ronkay and Ronkay 2014
Creators: name: Joshi, Rahul
name: Singh, Navneet
name: Laszlo, Gyula M.
Publisher: name: Zenodo
Year: 2019
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Lepidoptera
Nolidae
Meganola
Meganola margalla

description: 38. Meganola margalla László, Ronkay and Ronkay, 2014
 Meganola margalla László, Ronkay and Ronkay, 2014, Fibigeriana Supplement 2: 38.
TL: Margalla Hills, Islamabad, Pakistan. Holotype (♂).
TD: MWM.
 Distribution in India: Uttar Pradesh, Bhim valley (László et al., 2014). Elsewhere: Nepal (László et al., 2014).
description: Published as part of Joshi, Rahul, Singh, Navneet & Laszlo, Gyula M., 2019, An updated Checklist of subfamily Nolinae (Lepidoptera, Nolidae) from India, pp. 263-281 in Records of the Zoological Survey of India 119 (3) on page 270, DOI: 10.26515/rzsi/v119/i3/2019/142368, http://zenodo.org/record/13185704
Low radiative efficiency accretion in the nuclei of elliptical galaxies
Creators: name: Di Matteo, T.
name: Quataert, E.
name: Allen, S. W.
name: Narayan, R.
name: Fabian, A. C.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: The discovery of hard, power-law X-ray emission from a sample of six nearby elliptical galaxies, including the dominant galaxies of the Virgo,Fornax and Centaurus clusters (M87, NGC 1399 and NGC 4696, respectively), and NGC 4472, 4636 and 4649 in the Virgo cluster, has important implications for the study of quiescent supermassive black holes. We describe how the broad band spectral energy distributions of these galaxies, which accrete from their hot gaseous halos at rates comparable to their Bondi rates, can be explained by low-radiative efficiency accretion flows in which a significant fraction of the mass, angular momentum and energy is removed from the flows by winds. The observed suppression of the synchrotron component in the radio band and the systematically hard X-ray spectra, which are interpreted as thermal bremsstrahlung emission, support the conjecture that significant mass outflow is a natural consequence of systems accreting at low-radiative efficiencies. We briefly discuss an alternative model for the X-ray emission, namely that it is due to nonthermal synchrotron-self Compton processes in the accretion flow, or wind. This appears to require implausibly weak magnetic fields. Emission from a collimated jet viewed off axis should be distinguishable from the bremsstrahlung model by variability and thermal line emission studies. We argue that the difference in radiative efficiency between the nuclei of spiral and elliptical galaxies arises from the different manner in which interstellar gas is fed into the nuclei. In ellipticals, matter fed from the hot (slowly cooling) ISM is likely to be highly magnetized and with low specific angular momentum, both of which favor low-radiative efficiency accretion solutions and possibly the formation of the observed jets.
description: submitted to MNRAS, 16 pages, 3 figures in MNRAS LaTex style