cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
title: ADCO, Troisième cartulaire de Saint-Étienne de Dijon (XVIe), Cart. 23 (G 127), 310 folios, f. 00525
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/2011
name: Petot, Frédéric
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2020
Subjects: subject: Corpus Burgundiae Medii Aevi
subject: Chartes de la Bourgogne du Moyen Âge
subject: cartulaire
subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris

description: Troisième cartulaire de Saint-Étienne de Dijon (XVIe), Archives départementales de la Côte-d'Or, Cart. 23 (G 127), 310 folios, f. 00525, Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Troisième cartulaire de Saint-Étienne de Dijon (XVIe), Archives départementales de la Côte-d'Or, Cart. 23 (G 127), 310 folios, f. 00525, 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
Cancer homarus Linnaeus, 1758, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1758
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Malacostraca
Decapoda
Cancridae
Cancer
Cancer homarus

description: Cancer homarus [spec. nov.]
C. macrourus, thorace antrorsum aculeato, manibus adactylis.
Habitat in Mari Asiatico.
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 633, DOI: 10.5962/bhl.title.542, http://zenodo.org/record/3922206
Charge density wave behavior and order-disorder in the antiferromagnetic metallic series Eu(Ga_1-xAl_x)_4
Creators: name: Stavinoha, Macy
name: Cooley, Joya A.
name: Minasian, Stefan G.
name: McQueen, Tyrel M.
name: Kauzlarich, Susan M.
name: Huang, C. -L.
name: Morosan, E.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: FOS: Physical sciences

description: The solid solution Eu(Ga_1-xAl_x)_4 was grown in single crystal form to reveal a rich variety of crystallographic, magnetic, and electronic properties that differ from the isostructural end compounds EuGa_4 and EuAl_4, despite the similar covalent radii and electronic configurations of Ga and Al. Here we report the onset of magnetic spin reorientation and metamagnetic transitions for x = 0 - 1 evidenced by magnetization and temperature-dependent specific heat measurements. T_N changes non-monotonously with x, and it reaches a maximum around 20 K for x = 0.50, where the a lattice parameter also shows an extreme (minimum) value. Anomalies in the temperature-dependent resistivity consistent with charge density wave behavior exist for x = 0.50 and 1 only. Density functional theory calculations show increased polarization between the Ga-Al covalent bonds in the x = 0.50 structure compared to the end compounds, such that crystallographic order and chemical pressure are proposed as the causes of the charge density wave behavior.
Additional file 2 of Sarcopenia predicts adverse outcomes in an elderly population with coronary artery disease: a systematic review and meta-analysis
Creators: name: Xue, Qiqi
name: Wu, Jie
name: Ren, Yan
name: Hu, Jiaan
name: Yang, Ke
name: Cao, Jiumei
Publisher: name: figshare
Year: 2021
Subjects: subject: Medicine
subject: Cell Biology
subject: Genetics
subject: FOS: Biological sciences
subject: Biological Sciences not elsewhere classified
subject: Cancer
subject: Science Policy

description: Additional file 2: Supplementary Table S2. Literature search and study characteristic.
The Core Structure of Galaxy Clusters from Gravitational Lensing
Creators: name: Williams, Liliya L. R.
name: Navarro, Julio F.
name: Bartelmann, Matthias
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We examine gravitational lensing constraints on the structure of galaxy clusters and compare them with the results of cosmological N-body simulations of cluster formation in cold dark matter (CDM) dominated universes. We find that cluster core masses, as measured by the observed location of giant tangential arcs, generally exceed those of dark matter halos of similar velocity dispersion. The magnitude of the discrepancy is a strong function of cluster mass. Arc properties in the most massive clusters in the sample (i.e. those with velocity dispersion, σ\sim 1500-2000 km/s) are essentially consistent with the N-body predictions. On the other hand, giant arcs in σ\sim 1000 km/s clusters can only be reconciled with CDM cluster halos if their lensing power has been increased substantially by the presence of a massive (\sim 3 \times 10^{12} h^{-1} M_{\odot}) central galaxy and of significant substructure. Best agreement is found if the mass of the central galaxy and the effects of substructure are approximately independent of cluster mass. Massive central galaxies with steep inner density profiles are also needed to explain a clear trend observed in our dataset between the radial thickness of giant tangential arcs and the velocity dispersion of the cluster lens. The position and redshift of radial arcs may be used as independent tests of these results, but at present the dataset available is too limited to have a significant impact on these conclusions. Our results depend only weakly on the cosmological model adopted, and suggest that structural parameters of clusters derived from strong lensing studies cannot usefully constrain the values of cosmological parameters.
description: 26 pages, including 7 figs, LaTeX
Cancer arctus Linnaeus, 1758, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1758
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Malacostraca
Decapoda
Cancridae
Cancer
Cancer arctus

description: Cancer arctus [spec. nov.]
C. macrourus, thorace subaculeato hirto, manibus adactylis.
Marcgr. bras. 186. Poliquiquyixe.
Jonst. exsangu. t. 4. f. 3, 4, 8, 12.
Barrel. rar. t. 1288. f. 2.
Rumph. mus. t. 2. f. C. D.
Brown. jam. t. 41. f. 1.
Habitat in M. Europae, Asiae, Africae, Americae.
* l * Macrouri manibus adactylis, testa thoracis brevissima, nec thoracem totum tegente.
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 633, DOI: 10.5962/bhl.title.542, http://zenodo.org/record/3922206
Advancing the archaeology of architecture : a GIS-based approach to the organization of built space in the castros of Northwest Iberia
Creators: name: Hurt, John Duncan
name: 0000-0001-6384-9157
Publisher: name: The University of Texas at Austin
Year: 2019
Subjects: subject: Archaeology
subject: Architecture
subject: FOS: Civil engineering
subject: Northwest Iberia
subject: Castro
subject: GIS
subject: Spatial analysis

description: This thesis is framed as a contribution to the study of spatial organization at the scale of the individual settlement, specifically in the context of the castros of Northwest Iberia. I argue that new approaches to the description and analysis of organizational properties are needed to improve the current state of research on this topic. I propose a new methodology toward this end by applying concepts and methods from spatial statistics in a GIS environment. I demonstrate the potential of my proposition through a preliminary case study involving two castro sites from northwestern Portugal: Cividade de Terroso and Castro de Romariz. I conclude by discussing the implications of my work for the study of architecture and spatial organization in castro settlements, suggesting that there is much to be gained by further pursuit and expansion of this new methodological approach
Search for High Mass Top Quark Production in p anti-p Collisions at S**(1/2) = 1.8 TeV
Creators: name: Abachi, S.
Publisher: name: arXiv
Year: 1994
Subjects: subject: High Energy Physics - Experiment (hep-ex)
subject: FOS: Physical sciences

description: We present new results on the search for the top quark in p anti-p collisions at S**(1/2) = 1.8 TeV with an integrated luminosity of 13.5 +- 1.6 pb**(-1). We have considered t anti-t production in the Standard Model using electron and muon dilepton decay channels (t anti-t -> e mu + jets, e e + jets, and mu mu + jets) and single-lepton decay channels (t anti-t -> e + jets and mu + jets) with and without tagging of b quark jets. From all channels, we have 9 events with an expected background of 3.8 +- 0.9. If we assume that the excess is due to t anti-t production, and assuming a top mass of 180 GeV/c**2, we obtain a cross section of 8.2 +- 5.1 pb.
description: 12 pages FERMILAB-PUB-94/354-E (submitted to Phys. Rev. Lett.), http://d0wop.fnal.gov/d0pubs/journals/PRLTOP/PRLTOP.html
Noise-resistant Deep Learning for Object Classification in 3D Point Clouds Using a Point Pair Descriptor
Creators: name: Bobkov, Dmytro
name: Chen, Sili
name: Jian, Ruiqing
name: Iqbal, Muhammad
name: Steinbach, Eckehard
Publisher: name: arXiv
Year: 2018
Subjects: subject: Computer Vision and Pattern Recognition (cs.CV)
subject: Artificial Intelligence (cs.AI)
subject: Robotics (cs.RO)
subject: FOS: Computer and information sciences

description: Object retrieval and classification in point cloud data is challenged by noise, irregular sampling density and occlusion. To address this issue, we propose a point pair descriptor that is robust to noise and occlusion and achieves high retrieval accuracy. We further show how the proposed descriptor can be used in a 4D convolutional neural network for the task of object classification. We propose a novel 4D convolutional layer that is able to learn class-specific clusters in the descriptor histograms. Finally, we provide experimental validation on 3 benchmark datasets, which confirms the superiority of the proposed approach.
description: 8 pages
Implication of Dark Matter in Dwarf Spheroidal Galaxies
Creators: name: Hirashita, H.
name: Kamaya, H.
name: Takeuchi, T. T.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We examine the correlation between physical quantities to explore the existence of dark matter (DM) in the Local Group dwarf spheroidal galaxies (dSphs). In order to clarify whether DM exists in the dSphs we compare two extreme models of their internal kinematics: [1] a tidal model (the mass of a dSph is estimated with the luminous mass, since the observed large velocity dispersions of the dSphs are attributed to the tidal force by the Galaxy), and [2] a DM model (the mass of a dSph is estimated with the virial mass, since the velocity dispersion is considered to reflect the DM potential). In both models, we find that the relation between the surface brightness of the dSphs and the tidal force by the Galaxy is consistently interpreted. This makes a critical remark about the previous studies that concluded that the tidal force is effective for the dSphs based only on model [1]. We also check the correlation between the Galactocentric distance and the tidal force. Consequently, both models are also supported in this test. Thus, we are unable to judge which of the two is more promising for the dSphs in correlation investigations. The physical process of tidal disruption is also considered. Since the timescale for the tidally perturbed stars to escape is much shorter than the orbital periods of the dSphs, it is difficult for the tidally perturbed dSphs to exist as an assembly. Thus, we suggest that the gravitational field of DM is necessary to bind the dSphs with a large velocity dispersion.
description: 15 pages LaTeX, 4 figures, to appear in PASJ
On reverse-order law of tensors and its application to additive results on Moore-Penrose inverse
Creators: name: Panigrahy, Krushnachandra
name: Mishra, Debasisha
Publisher: name: arXiv
Year: 2018
Subjects: subject: Rings and Algebras (math.RA)
subject: FOS: Mathematics
subject: 15A69, 15A09

description: The equality $(\mc{A}\n\mc{B})^\dagger = \mc{B}^\dagger \n \mc{A}^\dagger$ for any two complex tensors $\mc{A}$ and $\mc{B}$ of arbitrary order, is called as the {\it reverse-order law} for the Moore-Penrose inverse of arbitrary order tensors via the Einstein product. Panigrahy {\it et al.} [Linear Multilinear Algebra; 68 (2020), 246-264.] obtained several necessary and sufficient conditions to hold the reverse-order law for the Moore-Penrose inverse of even-order tensors via the Einstein product, very recently. This notion is revisited here among other results. In this context, we present several new characterizations of the reverse-order law of arbitrary order tensors via the same product. More importantly, we illustrate a result on the Moore-Penrose inverse of a sum of two tensors as an application of the reverse-order law which leaves an open problem. We recall the definition of the Frobenius norm and the spectral norm to illustrate a result for finding the additive perturbation bounds of the Moore-Penrose inverse under the Frobenius norm. We conclude our paper with the introduction of the notion of sub-proper splitting for tensors which may help to find an iterative solution of a tensor multilinear system.
Optimization of a solvent extraction route for the recovery of Mo from petroleum refinery spent catalyst using Cyphos IL 102
Creators: name: Singh, Rashmi
name: Harshit Mahandra
name: Gupta, Bina
Publisher: name: Taylor & Francis
Year: 2018
Subjects: subject: Biochemistry
subject: Cell Biology
subject: Biotechnology
subject: Evolutionary Biology
subject: FOS: Biological sciences
subject: 59999 Environmental Sciences not elsewhere classified
subject: FOS: Earth and related environmental sciences
subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences
subject: Ecology
subject: Immunology
subject: FOS: Clinical medicine

description: In this study, trihexyl(tetradecyl)phosphonium bromide (Cyphos IL 102) diluted in toluene has been explored for the first time as an organic phase for the extraction, separation, and recovery of Mo(VI) from hydrochloric acid medium. The study focuses on the recovery of metals from spent catalyst, a hazardous solid waste. The metal recovered in the form of metal oxide has further applications in various fields. The widespread use of solvent extraction for metal recovery can be assigned to its economic feasibility and the built-in concentration step thereby providing an appropriate commercial technology for the beneficiation of low-grade sources of metals and recovery of substances from complex matrices. The influence of fundamental extraction variables on Mo(VI) extraction and loading and recycling capacity of the extractant has also been evaluated. Binary separations of Mo(VI) from other associated metal ions have been achieved with high separation factors. Optimized conditions have been employed for the extraction and recovery of Mo(VI) from petroleum refinery spent catalyst leach liquor containing Mo-1141.18 ppm, Al-2158.42 ppm, Ni-270.39 ppm, and Co-61.82 ppm. Quantitative and selective extraction (98.4%) of Mo from spent petroleum refinery catalyst was achieved in two stages at A:O = 3:2 using 2.0 × 10−2 mol/L Cyphos IL 102. Almost 99% Mo was stripped with 1.0 mol/L (NH4)2CO3 in two stages at O:A = 1:1. MoO3, obtained from the stripped solution by thermal decomposition was characterized by XRD, FESEM, and EDX techniques. Economical and environmental aspect of present work is supported by high loading capacity and reusability of extractant.
Spectroscopy of $Ω_{ccb}$ baryon in Hypercentral Quark Model
Creators: name: Shah, Zalak
name: Rai, Ajay Kumar
Publisher: name: arXiv
Year: 2018
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We extract the mass spectra of triply heavy baryon $Ω_{ccb}$ using Hypercentral constituent quark model. The first order correction is also added to the potential term of Hamiltonian. The radial and orbital excited state masses are also determined. Moreover, the Regge trajectories and magnetic moments are also given for this baryon.
description: 6 pages, 2 figures, it is to be published in Chinese Physics C
A Measurement of the $D^{*\pm}$ Cross Section in Two-Photon Processes
Creators: name: Enomoto, R.
Publisher: name: arXiv
Year: 1994
Subjects: subject: High Energy Physics - Experiment (hep-ex)
subject: FOS: Physical sciences

description: We have measured the inclusive $D^{*\pm}$ production cross section in a two-photon collision at the TRISTAN $e^+e^-$ collider. The mean $\sqrt{s}$ of the collider was 57.16 GeV and the integrated luminosity was 150 $pb^{-1}$. The differential cross section ($dσ(D^{*\pm})/dP_T$) was obtained in the $P_T$ range between 1.6 and 6.6 GeV and compared with theoretical predictions, such as those involving direct and resolved photon processes.
description: 8 pages, Latex format (article), figures corrected, published in Phys. Rev. D 50 (1994) 1879
Lettre de Jean-François Séguier à Giovanni Bianchi , 1740-01-28
Creators: name: Séguier, Jean-François
name: Jean-François Séguier
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2021
Subjects: Antiquités (général)
Epigraphie
Fossiles
Sciences naturelles (général)

description: [transcription] Carissimo Signore e Padrone Colendissimo

Verona 28 gennaio

Ho mandato ieri al signor Pasquali franco di porto una scatola ripiena di alcuni impietramenti e l’ho pregato di farli capitare a Vostra Signoria Illustrissima quanto prima. Questo non è che picciol saggio di quello che potrò mandarle nella buona stagione, e in tanto mi faccia grazia di ricevergli in segno d’amicizia e di buona corrispondenza. Uno fra gli altri singolari fra cotesti è quello delle pietre volgarmente chiamate dalla loro forma Lenticolari. Queste sono d’una spezie molto particolare, e ve ne sono qui più campi così ripieni che altro non apparisce fuorché cotesti impietramenti. Maraviglia mi recano certamente e sono persuaso, che se gli autori dell’istoria naturale, parlando delle pietre lenticolari, avessero vedute queste, non avrebbero così francamente spacciate tante favole. Si quid novisti rectius istis si degni di farmene partecipe. Insieme vi troverà alcune Corna d’Ammone che sono della più piccola spezie di cotesti testacei: altra meraviglia, perché così fatti pesci in cotesti mari non si trovano punto. Venti dì fa andai a vedere un certo macigno dove si trovano gli echini, e questi le ritrovai sul dorso d’un monte assai alto. Fra quei ci trovai ancora dei trochiti mostruosi. Poco a poco piglio informazioni di tutte queste meraviglie: forse un giorno ne farò qualche uso.

/ Ho già messo ordine per andare nella bella stagione visitare gli monti di Zoppica e Boniolo che molti bei impietramenti nelle loro bucche riservano. Mi conservi la sua amicizia e mi creda di tutto cuore mio carissimo Signore

Il Giornale novo del signor Marchese esce dal torchio, e non vi è risposta alcuna al consaputo libro.
L’inscrione [sic] antica in piazza vostra ha ella la parola ultima così: STER o S?R?

Verona, 28 gennaio 1740
Suo Devotissimo ed Obligatissimo Servitore
Gianfrancesco Séguier
description: [personnes citées] Giovanni Battista Pasquali, Scipione Maffei
description: [reférence bibliographique citée]
Giornale de’ letterati d’Italia, Venezia, Gio. Gabbriello Ertz, 1710-1740, 42 vol., in-12
description: Source: [lieu de Conservation] Rimini, Biblioteca Gambalunga [cote]Fondo Gambetti, Lettere autografe al Dott. Giovanni Bianchi, pièce 3
Cancer mantis Linnaeus, 1758, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1758
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Malacostraca
Decapoda
Cancridae
Cancer
Cancer mantis

description: Cancer mantis [spec. nov.]
C. macrourus articularis, manibus adactylis compressis falcatis serrato-dentatis. Mus. Ad. Fr. 1. p. 86.
Rumph. mus. t. 3. f. E. C. Arenarius.
Marcgr. bras. 186. t 187. Tamaru-guacu.
Habitat in M. Asiatico, Indico, Mediterraneo.
Thoracis testa membranacea. Pedes utrinque 3. Pollex serrato-dontatus, terminalis. Dactyli sub abdomine trium parium. Antennae trifidae: lamina ovata ad oculos.
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 633, DOI: 10.5962/bhl.title.542, http://zenodo.org/record/3922206
Computable Aspects of the Bachmann-Howard Principle
Creators: name: Freund, Anton
Publisher: name: arXiv
Year: 2018
Subjects: subject: Logic (math.LO)
subject: FOS: Mathematics
subject: 03B30, 03D60, 03F15

description: We have previously established that $Π^1_1$-comprehension is equivalent to the statement that every dilator has a well-founded Bachmann-Howard fixed point, over $\mathbf{ATR_0}$. In the present paper we show that the base theory can be lowered to $\mathbf{RCA_0}$. We also show that the minimal Bachmann-Howard fixed point of a dilator $T$ can be represented by a notation system $\vartheta(T)$, which is computable relative to $T$. The statement that $\vartheta(T)$ is well-founded for any dilator $T$ will still be equivalent to $Π^1_1$-comprehension. Thus the latter is split into the computable transformation $T\mapsto\vartheta(T)$ and a statement about the preservation of well-foundedness, over a system of computable mathematics.
description: This is the submitted version (before peer review) of a paper published in the Journal of Mathematical Logic. Note, in particular, that the numbering of theorems differs from the published version
Cancer scyllarus Linnaeus, 1758, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1758
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Malacostraca
Decapoda
Cancridae
Cancer
Cancer scyllarus

description: Cancer scyllarus [spec. nov.]
C. macrourus articularis, manibus adactylis ventricosis rectis angulatis introrsum tridentatis. Mus. Ad. Fr. 1. p. 86. C. mirabilis.
Rumph. mus. t. 3. f. F. G.
Habitat in M. Asiatico.
Statura praecedentis. Thoracis testa latere postico emarginata. Mucronum par pone pedes.
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 633, DOI: 10.5962/bhl.title.542, http://zenodo.org/record/3922206
The K Band Luminosity Function in Galaxy Clusters to z ~ 1
Creators: name: De Propris, R.
name: Stanford, S. A.
name: Eisenhardt, P. R.
name: Dickinson, M. E.
name: Elston, R.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present $K$-band luminosity functions for galaxies in a heterogeneous sample of 38 clusters at $0.1 < z < 1$. Using infrared-selected galaxy samples which generally reach 2 magnitudes fainter than the characteristic galaxy luminosity $L^*$, we fit Schechter functions to background-corrected cluster galaxy counts to determine $K^*$ as a function of redshift. Because of the magnitude limit of our data, the faint-end slope $α$ is fixed at -0.9 in the fitting process. We find that $K^*(z)$ departs from no-evolution predictions at $z > 0.4$, and is consistent with the behavior of a simple, passive luminosity evolution model in which galaxies form all their stars in a single burst at $z_f = 2 (3)$ in an $H_0 = 65 km/s Mpc^{-1}, Ω_M = 0.3, Ω_Λ=0.7 (0)$ universe. This differs from the flat or negative infrared luminosity evolution which has been reported for high redshift field galaxy samples. We find that the observed evolution appears to be insensitive to cluster X-ray luminosity or optical richness, implying little variation in the evolutionary history of galaxies over the range of environmental densities spanned by our cluster sample. These results support and extend previous analyses based on the color evolution of high redshift cluster E/S0 galaxies, indicating not only that their stellar populations formed at high redshift, but that the assembly of the galaxies themselves was largely complete by $z \approx 1$, and that subsequent evolution down to the present epoch was primarily passive.
description: 35 pages, 10 figures; accepted by the Astronomical Journal (August 1999 issue)
Testing modified gravity with globular clusters: the case of NGC 2419
Creators: name: Llinares, Claudio
Publisher: name: arXiv
Year: 2018
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: Astrophysics of Galaxies (astro-ph.GA)
subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: The dynamics of globular clusters has been studied in great detail in the context of general relativity as well as with modifications of gravity that strongly depart from the standard paradigm such as MOND. However, at present there are no studies that aim to test the impact that less extreme modifications of gravity (e.g. models constructed as alternatives to dark energy) have on the behaviour of globular clusters. This Letter presents fits to the velocity dispersion profile of the cluster NGC 2419 under the symmetron modified gravity model. The data shows an increase in the velocity dispersion towards the centre of the cluster which could be difficult to explain within general relativity. By finding the best fitting solution associated with the symmetron model, we show that this tension does not exist in modified gravity. However, the best fitting parameters give a model that is inconsistent with the dynamics of the Solar System. Exploration of different screening mechanisms should give us the chance to understand if it is possible to maintain the appealing properties of the symmetron model when it comes to globular clusters and at the same time recover the Solar System dynamics properly.
description: 6 pages, 2 figures. Accepted for publication in MNRAS Letters
DUMAND and AMANDA: High Energy Neutrino Astrophysics
Creators: name: Wilkes, R. Jeffrey
Publisher: name: arXiv
Year: 1994
Subjects: subject: Astrophysics (astro-ph)
subject: High Energy Physics - Experiment (hep-ex)
subject: FOS: Physical sciences

description: The field of high energy neutrino astrophysics is entering an exciting new phase as two new large-scale observatories prepare to come on line. Both DUMAND (Deep Underwater Muon and Neutrino Detector) and AMANDA (Antarctic Muon and Neutrino Detector) had major deployment efforts in 12/93--1/94. Results were mixed, with both projects making substantial progress, but encountering setbacks that delayed full-scale operation. The achievements, status, and plans (as of 10/94) of these two projects will be discussed.
description: 30 pages, embedded Postscript (epsf) figures in separate file packaged by uufiles
DUMAND-II (Deep Underwater Muon and Neutrino Detector) PROGRESS Report
Creators: name: Young, Kenneth K.
Publisher: name: arXiv
Year: 1994
Subjects: subject: Astrophysics (astro-ph)
subject: High Energy Physics - Experiment (hep-ex)
subject: FOS: Physical sciences

description: The DUMAND-II detector will search for astronomical sources of high energy neutrinos. Successful deployment of the basic infrastructure, including the shore cable, the underwater junction box, and an environmental module was accomplished in December, 1993. One optical module string was also deployed and operated, logging data for about 10 hours. The underwater cable was connected to the shore station where we were able to successfully exercise system controls and log further environmental data. After this time, water leaking into the electronics control module for the deployed string disabled the string electrical system. The acquired data are consistent with the expected rate of downgoing muons, and our ability to reconstruct muons was demonstrated. The measured acoustical backgrounds are consistent with expectation, which should allow acoustical detection of nearby PeV particle cascades. The disabled string has been recovered and is undergoing repairs ashore. We have identified the source of the water leak and implemented additional testing and QC procedures to ensure no repetition in our next deployment. We will be ready to deploy three strings and begin continuous data taking in 1995.
description: 7 pp, figures available in separate file, requires file aip.sty available in /macros; to be published in Proc. 5th Conf. on Intersections of Particle and Nuclear Physics (AIP, New York)
Integrated restoration prioritization–A multi-discipline approach in the Greater Toronto Area
Creators: name: Stille, John
name: Namrata Shrestha
name: Toninger, Ralph
name: MacKenzie, Carissa
name: Ramesbottom, Andrew
name: Smith, Joel
Publisher: name: Taylor & Francis
Year: 2018
Subjects: subject: Space Science
subject: Molecular Biology
subject: Ecology
subject: FOS: Biological sciences
subject: Sociology
subject: FOS: Sociology
subject: 69999 Biological Sciences not elsewhere classified

description: Ecosystem restoration planning requires an integrated approach considering many components of the natural system when prioritizing where and what to restore. Toronto and Region Conservation Authority and partners have developed a multi-discipline and multi-benefit approach to restoration planning that facilitates effective restoration works, which contribute to realizing regional watershed objectives pertaining to natural system functions. Through various long term monitoring and modeling initiatives, Toronto and Region Conservation Authority has amassed a wealth of knowledge on terrestrial biodiversity, aquatic ecosystems, hydrology, and headwater conditions. The aim of Integrated Restoration Prioritization is to identify impairments and threats to ecosystem function as a means to improve the delivery of ecological goods and services. Consolidating data and comparing discrete areas based on different parameters and thresholds can help direct decision making for future restoration initiatives. The first iteration of the Integrated Restoration Prioritization analyzed existing datasets, identified gaps, and made recommendations for future monitoring. This approach will assist with delisting Beneficial Use Impairments #14 Loss of Fish and Wildlife Habitat and #3 Degradation of Fish and Wildlife Populations within the Toronto Remedial Action Plan area. Further, the Integrated Restoration Prioritization will assist in implementing the recommendations made in watershed planning documents pertaining to fisheries and natural heritage management. Specifically, the Integrated Restoration Prioritization will identify where impairments to ecological function are located, ensure habitats and corridor linkages are protected or restored, and prioritize local and upstream catchments that could contribute most to improving the natural system if restored.
title: ADCO, Cartulaire général de Cîteaux, dit de Jean de Cirey, (XVe siècle), tome IV, Cart. 188 (11 H 73), f. 0023v
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
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2020
Subjects: subject: cartulaire
subject: Corpus Burgundiae Medii Aevi
subject: Chartes de la Bourgogne du Moyen Âge
subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris

description: Cartulaire général de Cîteaux, dit de Jean de Cirey, (XVe siècle), tome IV, Archives départementales de la Côte-d'Or, Cart. 188 (11 H 73), f. 0023v, Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Cartulaire général de Cîteaux, dit de Jean de Cirey, (XVe siècle), tome IV, Archives départementales de la Côte-d'Or, Cart. 188 (11 H 73), f. 0023v, 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
ISOCAM 15um Search for Distant Infrared Galaxies Lensed by Clusters
Creators: name: Barvainis, Richard
name: Antonucci, Robert
name: Helou, George
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: In a search for lensed infrared galaxies, ISOCAM images have been obtained toward the rich clusters Abell 2218 and Abell 2219 at 15um. Nine galaxies (four in Abell 2218 and five in Abell 2219) were detected with flux levels in the range 530-1100 microJy. Three of the galaxies detected in Abell 2218 have previously known redshifts; of these one is a foreground galaxy and the other two are lensed background galaxies at z=0.474 and z=1.032. One of the objects detected in the field of Abell 2219 is a faint, optically red, extreme infrared-dominated galaxy with a probable redshift of 1.048.
description: 10 pages of text, 6 figures. Requires aaspp4.sty. To be published in the Astronomical Journal, July 1999
On the Intrinsic Bias in detecting Caustic Crossings between Galactic Halo and Self-lensing Events in the Magellanic Clouds
Creators: name: Han, Cheongho
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: In this paper, we investigate the intrinsic bias in detecting caustic crossings between Galactic halo and self-lensing events in the Magellanic Clouds. For this, we determine the region for optimal caustic-crossing detection in the parameter space of the physical binary separations, $\ell$, and the total binary lens mass, $M$, and find that the optimal regions for both populations of events are similar to each other. In particular, if the Galactic halo is composed of lenses with the claimed average mass of $\sim 0.5 M_\odot$, the optimal binary separation range of Galactic halo events of $3.5 AU\lesssim \ell\lesssim 14 AU$ matches well with that of a Magellanic Cloud self-lensing event caused by a binary lens with a total mass $M\sim 1 M_\odot$; well within the mass range of the most probable lens population of stars in the Magellanic Clouds. Therefore, our computation implies that if the binary fractions and the distributions of binary separations of the two populations of lenses are not significantly different from each other, there is no strong detection bias against Galactic halo caustic-crossing events.
description: total 4 pages, including 3 Figures and no Table, accepted for publication in MNRAS
$W^+Z$ and $W^+γ^*$ Backgrounds to Strong $W^+W^+$ Scattering at the LHC
Creators: name: Chanowitz, Michael S.
name: Kilgore, William B.
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: Because of inevitable blind spots at high rapidity and low transverse momentum, the process $\overline qq \rightarrow l^+ l^- \ l^{+} ν$ provides a surprisingly large background to the $W^+W^+ \rightarrow l^+ ν\ l^+ ν$ signal associated with strong $WW$ scattering. Previous calculations of the total background are approximately doubled, and the estimate of the ``no-lose'' luminosity at the LHC to observe manifestations of the electroweak symmetry breaking mechanism is increased to between $\sim 100$ and $\sim 140$ fb$^{-1}$.
description: 13 pages, Latex, uuencoded figures
Non-thermal Radiation of Cosmological gamma-ray Bursters
Creators: name: Smolsky, M. V.
name: Usov, V. V.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We use 1+1/2 dimensional particle-in-cell plasma simulations to study the interaction of a relativistic, strongly magnetized wind with an ambient medium. Such an interaction is a plausible mechanism which leads to generation of cosmological gamma-ray bursts. We confirm the idea of Meszaros and Rees (1992) that an essential part (about 20%) of the energy that is lost by the wind in the process of its deceleration may be transferred to high-energy electrons and then to high-frequency (X-ray and gamma-ray) emission. We show that in the wind frame the spectrum of electrons which are accelerated at the wind front and move ahead of the front is nearly a two-dimensional relativistic Maxwellian with a relativistic temperature $T=6*10^9Γ_T$ K, where $Γ_T=200Γ_0$ with the accuracy of ~20%, and $Γ_0$ is the Lorentz factor of the wind, $Γ_0>100$ for winds outflowing from cosmological gamma-ray bursters. Our simulations point to an existence of a high-energy tail of accelerated electrons with a Lorentz factor of more than $700Γ_0$. Large-amplitude electromagnetic waves are generated by the oscillating currents at the wind front. The mean field of these waves ahead of the wind front is an order of magnitude less than the magnetic field of the wind. High-energy electrons which are accelerated at the wind front and injected into the region ahead of the front generate synchro-Compton radiation in the fields of large-amplitude electromagnetic waves. This radiation closely resembles synchrotron radiation and can reproduce the non-thermal radiation of gamma-ray bursts observed in the Ginga and BATSE ranges (from a few keV to a few MeV).
description: 37 pages, 11 figures, submitted to ApJ
Additional file 1 of Sarcopenia predicts adverse outcomes in an elderly population with coronary artery disease: a systematic review and meta-analysis
Creators: name: Xue, Qiqi
name: Wu, Jie
name: Ren, Yan
name: Hu, Jiaan
name: Yang, Ke
name: Cao, Jiumei
Publisher: name: figshare
Year: 2021
Subjects: subject: Medicine
subject: Cell Biology
subject: Genetics
subject: FOS: Biological sciences
subject: Biological Sciences not elsewhere classified
subject: Cancer
subject: Science Policy

description: Additional file 1: Supplementary Table S1. Search terms and strategy.
Integrated restoration prioritization – A multi-discipline approach in the Greater Toronto Area
Creators: name: Stille, John
name: Namrata Shrestha
name: Toninger, Ralph
name: MacKenzie, Carissa
name: Ramesbottom, Andrew
name: Smith, Joel
Publisher: name: Taylor & Francis
Year: 2018
Subjects: subject: Space Science
subject: Molecular Biology
subject: Ecology
subject: FOS: Biological sciences
subject: Sociology
subject: FOS: Sociology
subject: 69999 Biological Sciences not elsewhere classified

description: Ecosystem restoration planning requires an integrated approach considering many components of the natural system when prioritizing where and what to restore. Toronto and Region Conservation Authority and partners have developed a multi-discipline and multi-benefit approach to restoration planning that facilitates effective restoration works, which contribute to realizing regional watershed objectives pertaining to natural system functions. Through various long term monitoring and modeling initiatives, Toronto and Region Conservation Authority has amassed a wealth of knowledge on terrestrial biodiversity, aquatic ecosystems, hydrology, and headwater conditions. The aim of Integrated Restoration Prioritization is to identify impairments and threats to ecosystem function as a means to improve the delivery of ecological goods and services. Consolidating data and comparing discrete areas based on different parameters and thresholds can help direct decision making for future restoration initiatives. The first iteration of the Integrated Restoration Prioritization analyzed existing datasets, identified gaps, and made recommendations for future monitoring. This approach will assist with delisting Beneficial Use Impairments #14 Loss of Fish and Wildlife Habitat and #3 Degradation of Fish and Wildlife Populations within the Toronto Remedial Action Plan area. Further, the Integrated Restoration Prioritization will assist in implementing the recommendations made in watershed planning documents pertaining to fisheries and natural heritage management. Specifically, the Integrated Restoration Prioritization will identify where impairments to ecological function are located, ensure habitats and corridor linkages are protected or restored, and prioritize local and upstream catchments that could contribute most to improving the natural system if restored.
Cancer pulex Linnaeus, 1758, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1758
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Malacostraca
Decapoda
Cancridae
Cancer
Cancer pulex

description: Cancer pulex [spec. nov.]
C. macrourus articularis, manibus adactylis, cauda attenuata spinis bifidis. It. oel. 42, 96.
Habitat ad Maris littora.
Species 54-59 ob thoracem Lorica destitutum & singularem structuram corporis adeo a reliquis Cancris recedunt, ut facile genus distinctum constituerent.
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 633, DOI: 10.5962/bhl.title.542, http://zenodo.org/record/3922206
Weihrauch goes Brouwerian
Creators: name: Brattka, Vasco
name: Gherardi, Guido
Publisher: name: arXiv
Year: 2018
Subjects: subject: Logic (math.LO)
subject: Logic in Computer Science (cs.LO)
subject: FOS: Mathematics
subject: FOS: Computer and information sciences
subject: 03B30, 03D30, 03D78, 03F52, 03F60, 06D20

description: We prove that the Weihrauch lattice can be transformed into a Brouwer algebra by the consecutive application of two closure operators in the appropriate order: first completion and then parallelization. The closure operator of completion is a new closure operator that we introduce. It transforms any problem into a total problem on the completion of the respective types, where we allow any value outside of the original domain of the problem. This closure operator is of interest by itself, as it generates a total version of Weihrauch reducibility that is defined like the usual version of Weihrauch reducibility, but in terms of total realizers. From a logical perspective completion can be seen as a way to make problems independent of their premises. Alongside with the completion operator and total Weihrauch reducibility we need to study precomplete representations that are required to describe these concepts. In order to show that the parallelized total Weihrauch lattice forms a Brouwer algebra, we introduce a new multiplicative version of an implication. While the parallelized total Weihrauch lattice forms a Brouwer algebra with this implication, the total Weihrauch lattice fails to be a model of intuitionistic linear logic in two different ways. In order to pinpoint the algebraic reasons for this failure, we introduce the concept of a Weihrauch algebra that allows us to formulate the failure in precise and neat terms. Finally, we show that the Medvedev Brouwer algebra can be embedded into our Brouwer algebra, which also implies that the theory of our Brouwer algebra is Jankov logic.
description: 36 pages
Simulations of Supercollider Physics
Creators: name: Lane, K. D.
name: Paige, F. E.
name: Skwarnicki, T.
name: Womersley, W. J.
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: The Standard Model of particle physics makes it possible to simulate complete events for physics signatures and their backgrounds in high energy collisions. Knowledge of how the produced particles interact with the materials in a detector makes it possible to simulate the response of any particular detector design to these events and so determine whether the detector could observe the signal. The combination of these techniques has played an important role in the design of new detectors, particularly those for hadron supercolliders where the high rates and small signal cross sections make the experiments very difficult. The technique is reviewed here and illustrated using the simulations of the GEM detector proposed for the Superconducting Super Collider. Although the simulations and results described here are somewhat detector-specific, we believe that they can serve as a useful model for this component of detector design for future hadron supercolliders.
description: 99 pages, Plain TeX (macros included), includes gzipped tar file with 56/60 EPS figures for dvips. Get complete version from http://penguin.phy.bnl.gov/www/hetpapers.html or ftp://penguin.phy.bnl.gov/pub/papers/gemreview.ps.Z
[ENIC] Regulamento (2018).pdf
Creators: name: Cavalcante, Vinicius Holanda
Publisher: name: figshare
Year: 2018
Subjects: Education

description: Regulamento para os pesquisadores e alunos de Iniciação Científica interessados em participar do; Encontro de Iniciação Científica e Seminário Nacional de Pesquisa da Universidade Nove de Julho - UNINOVE
Mercury fluxes, budgets, and pools in forest ecosystems of China: A review
Creators: name: Zhou, Jun
name: Du, Buyun
name: Shang, Lihai
name: Wang, Zhangwei
name: Cui, Hongbiao
name: Fan, Xingjun
name: Zhou, Jing
Publisher: name: Taylor & Francis
Year: 2019
Subjects: subject: Medicine
subject: Environmental Sciences not elsewhere classified
subject: Ecology
subject: FOS: Biological sciences
subject: Biological Sciences not elsewhere classified

description: Mercury (Hg) retention in forest ecosystem plays a key role in global biogeochemical cycling. We present a comprehensive review of the research status of forest Hg in China to characterize the Hg budgets and pools. Averaged total Hg (THg) inputs at remote forests and rural and suburban forests in China are about 2–4-fold and 2.5–5-fold higher than the observed values in Europe and North America, respectively. The highly elevated THg inputs are mainly derived from the elevated atmospheric Hg concentrations and litterfall biomass. THg outputs from the forest ecosystems are much lower than the atmospheric depositions. The annual THg retentions range from 26.1 to 60.4 µg m−2 at subtropical forests and from 12.4 to 26.2 µg m−2 at temperate forests. Given the large areal coverage, THg retention in forest is ∼69 t year−1 in China and is much high than that in global scale estimated by models. The much higher THg retention has elevated the THg pools in Chinese subtropical forests. This study has implication for the role of China forests in the global Hg biogeochemical cycle and the optimization of atmospheric Hg transport and deposition models.