cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Additional file 5: of Association between cognitive function and life-space mobility in older adults: results from the FRéLE longitudinal study
Creators: name: Béland, François
name: Julien, Dominic
name: Bier, Nathalie
name: Desrosiers, Johanne
name: Marie-Jeanne Kergoat
name: Demers, Louise
Publisher: name: figshare
Year: 2018
Subjects: subject: Space Science
subject: Medicine
subject: 59999 Environmental Sciences not elsewhere classified
subject: FOS: Earth and related environmental sciences
subject: Sociology
subject: FOS: Sociology
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences

description: Table S1. Characteristics of FRéLE participants. Table presenting descriptives of the FRéLE sample. (DOCX 26 kb)
SCUBA imaging of NGC 7331 dust ring
Creators: name: Bianchi, S.
name: Alton, P. B.
name: Davies, J. I.
name: Trewhella, M.
Publisher: name: arXiv
Year: 1998
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present observations of the spiral galaxy NGC 7331 using the Sub-millimetre Common User Bolometer Array (SCUBA) on the James Clark Maxwell Telescope. We have detected a dust ring of 45 arcsec radius (3.3 kpc) at wavelengths of 450 and 850-micron. The dust ring is in good correspondence with other observations of the ring in the mid-infrared (MIR), CO and radio-continuum, suggesting that the observed dust is associated with the molecular gas and star formation. A B-K colour map shows an analogous ring structure with an asymmetry about the major axis, consistent with the extinction being produced by a dust ring. The derived temperature of the dust lies between 16 and 31 K and the gas-to-dust ratio between 150 and 570, depending on the assumed dust emission efficiency index (beta=1.5 or 2.).
description: 5 pages, 6 figures, to be published in MNRAS
Experimental realization of quantum algorithms for linear system inspired by adiabatic quantum computing
Creators: name: Wen, Jingwei
name: Kong, Xiangyu
name: Wei, Shijie
name: Wang, Bixue
name: Xin, Tao
name: Long, Guilu
Publisher: name: arXiv
Year: 2018
Subjects: subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: Quantum adiabatic algorithm is of vital importance in quantum computation field. It offers us an alternative approach to manipulate the system instead of quantum gate model. Recently, an interesting work arXiv:1805.10549 indicated that we can solve linear equation system via algorithm inspired by adiabatic quantum computing. Here we demonstrate the algorithm and realize the solution of 8-dimensional linear equations $A\textbf{x}=\textbf{b}$ in a 4-qubit nuclear magnetic resonance system. The result is by far the solution of maximum-dimensional linear equation with a limited number of qubits in experiments, which includes some ingenious simplifications. Our experiment provides the new possibility of solving so many practical problems related to linear equations systems and has the potential applications in designing the future quantum algorithms.
Bioengineering of novel carbon-based biosensors for real-time biomedical use
Creators: name: Phairatana, Tonghathai
Publisher: name: Imperial College London
Year: 2015

description: The aim of this thesis was to develop novel carbon-based biosensors and sensors for real-time metabolite and drug detection, to provide the next generation of medical devices which can give clinicians relevant chemical information in real-time at the patient bedside. An autocalibration system was developed using LabSmith programmable components to give precise fluid delivery and excellent temporal control of multiple liquid streams. This enables a 5-point calibration to be carried out using two solutions in 12 minutes. Systems using chitosan, poly(ethylene glycol)diglycidyl ether hydrogel, electrodeposition and selfassembly to immobilise enzymes on a combined needle electrode surface were studied and their performances were investigated using a microfluidic platform. The autocalibration system was combined with the graphene oxide-based biosensors in a microchip coupled with a microdialysis probe and was examined as a proof-of-concept clinical on-line analysis system. A reduced graphene oxide-based sensor was fabricated using a combined needle electrode for on-line neurotransmitter detection of dopamine. Its performance was compared with that of a platinum electrode. A microfluidic sensor based on a carbon nanotube-epoxy composite was fabricated to detect the presence of carboplatin (anti-cancer drug) in healthy tissue in real time during chemotherapy. Detection of carboplatin was carried out using differential pulse voltammetry firstly in a beaker, in which carbon nanotube-epoxy composite electrodes performed better than glassy carbon electrodes for oxidation of free purine bases and than DNA-modified carbon nanotube-epoxy composite sensors for detection of carboplatin. Carboplatin detection was then performed in a microfluidic platform. The methodology for on-line carboplatin detection was optimised in terms of the analysis time and for the repeated determination of carboplatin using the same electrode. Microdialysis and microfluidic techniques have been combined to give a proof-of-concept system real-time carboplatin detection using the carbon nanotube-epoxy composite sensors.
Near-Term Detectability of Terrestrial Extrasolar Planets: TEP Network Observations of CM Draconis
Creators: name: Network, TEP
name: :
name: Deeg, H. J.
name: Doyle, L. R.
name: Kozhevnikov, V. P.
name: Martin, E. L.
name: Oetiker, B.
name: Palaiologou, E.
name: Schneider, J.
name: Afonso, C.
name: Dunham, E. W.
name: Jenkins, J. M.
name: Ninkov, Z.
name: Stone, R. P. S.
name: Zakharova, P. E.
Publisher: name: arXiv
Year: 1998
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Results from a photometric search for extrasolar planetary transits across the eclipsing binary CM Dra are presented. The TEP (Transits of Extrasolar Planets) network has observed this star since 1994, and a lightcurve with 617 hours of coverage has been obtained. The data give a complete phase coverage of the CM Dra system at each of the 3 years of observations, with a noise of less than 5 mmag. New epoch and period values for CM Dra are derived, and a low flare rate of 0.025/hr has been confirmed. The absence of periodic variations in eclipse minimum times excludes the presence of very massive planets with periods of less than a few years. The lightcurve was visually scanned for the presence of unusual events which may be indicative of transits of extrasolar planets with 'massive earth' sizes. Six suspicious events were found which are being followed up for future transits, by planets with sizes between 1.5 and 2.5 RE (Earth Radii). However, none of these events has amplitudes compatible with planets larger than 2.5 RE. Coplanar planets larger than 2.5 RE and with orbital periods of less than 60 days can therefore be ruled out with a confidence of about 80%. Planets smaller than 1.5 RE cannot be detected in the data without a sub-noise detection algorithm. A preliminary signal detection analysis shows that there is a 50% detection confidence for 2 RE planets with a period from 10 to 30 days with the current data. This data-set demonstrates that it is possible to detect terrestrial sized planets with ground based photometry, and that strong constraints on the sizes of planets orbiting in the plane of the CM Dra system can be set.
description: 12 pages, 8 figures (in 11 individual ps or eps files), to be published in A&A
ЎЗБЕКИСТОН РЕСПУБЛИКАСИДА ИМПОРТ ҚИЛИНГАН ХИЗМАТЛАР УЧУН ТЎЛАНГАН СОЛИҚЛАР ТАХЛИЛИ
Creators: name: Саидова Ўғилой Рустамжон қизи ТДИУ таянч докторанти
Publisher: name: Zenodo
Year: 2024

description: Сўнгги йилларда мамлакатимизда олиб борилаётган ислоҳотлар натижасида иқтисодий ривожланиш, шу билан биргаликда импорт операцияларида ҳам барқарор ўсиш кузатилинмоқда. Ушбу тезисда Ўзбекистон Республикасига импорт қилинган хизматлар учун тўланган солиқларни 2010 йилдан 2022 йилгача давр оралиғидаги ўзгаришларини кўриб чиқамиз.
MOESM2 of Is nodding syndrome in northern Uganda linked to consumption of mycotoxin contaminated food grains?
Creators: name: Echodu, Richard
name: Edema, Hilary
name: Malinga, Geoffrey
name: Hendy, Adam
name: Colebunders, Robert
name: Kaducu, Joyce Moriku
name: Ovuga, Emilio
name: Haesaert, Geert
Publisher: name: figshare
Year: 2018
Subjects: subject: Genetics
subject: FOS: Biological sciences
subject: 59999 Environmental Sciences not elsewhere classified
subject: FOS: Earth and related environmental sciences
subject: Ecology
subject: Sociology
subject: FOS: Sociology
subject: 69999 Biological Sciences not elsewhere classified
subject: Science Policy

description: Additional file 2: Table S2. Sampling sites for cereal grains.
Chebyshev polynomial representation of imaginary time response functions
Creators: name: Gull, Emanuel
name: Iskakov, Sergei
name: Krivenko, Igor
name: Rusakov, Alexander A.
name: Zgid, Dominika
Publisher: name: arXiv
Year: 2018
Subjects: subject: Statistical Mechanics (cond-mat.stat-mech)
subject: FOS: Physical sciences

description: Problems of finite-temperature quantum statistical mechanics can be formulated in terms of imaginary (Euclidean) -time Green's functions and self-energies. In the context of realistic Hamiltonians, the large energy scale of the Hamiltonian (as compared to temperature) necessitates a very precise representation of these functions. In this paper, we explore the representation of Green's functions and self-energies in terms of a series of Chebyshev polynomials. We show that many operations, including convolutions, Fourier transforms, and the solution of the Dyson equation, can straightforwardly be expressed in terms of the series expansion coefficients. We then compare the accuracy of the Chebyshev representation for realistic systems with the uniform-power grid representation, which is most commonly used in this context.
description: 11 pages, 8 figures
Rhamnus
Creators: name: Jarvis, Charlie
Publisher: name: Linnaean Society of London in association with the Natural History Museum
Year: 2007
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Magnoliopsida
Rosales
Rhamnaceae
Rhamnus

description: Rhamnus minor Linnaeus, Plantae Tinctoriae: 14. 1759.
Type not designated.
Original material: Herb. Burser XXV: 8? (UPS).
Current name: Rhamnus sp. (Rhamnaceae).
Note: The precise synonymy of this name is uncertain.
description: Published as part of Jarvis, Charlie, 2007, Chapter 7: Linnaean Plant Names and their Types (part R), pp. 785-805 in Order out of Chaos. Linnaean Plant Types and their Types, London :Linnaean Society of London in association with the Natural History Museum on page 791, DOI: 10.5281/zenodo.291971
Reminiscences of Mary Benson 1987
Publisher: name: Columbia University
Year: 2020
Subjects: Civil rights workers
African Americans--Civil rights
African Americans--Social conditions

description: Recollections of Allard K. Lowenstein: first meeting, 1959, his concern over Communist infiltration of Student Nonviolent Coordinating Committee, his visits to London, his speeches, family life, his death; her position as secretary to Michael Scott, her trip to southern United States in the 1960s, sit-ins, 1963
STELLAR POPULATION GRADIENTS IN BRIGHT CLUSTER GALAXIES AT z=0.2
Creators: name: Davidge, T. J.
name: Grinder, M.
Publisher: name: arXiv
Year: 1995
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Slit spectra, covering the rest frame near-ultraviolet and blue wavelength regions, are combined with moderately deep g and R images to investigate radial population gradients in the brightest components of six z=0.2 galaxy clusters selected by x-ray brightness. We conclude that the brightest cluster galaxies (BCGs) of the EMSS0440+02, EMSS0906+11 and EMSS1231+15 clusters have global stellar contents resembling nearby elliptical galaxies. The BCGs in the clusters EMSS0839+29, EMSS1455+22 and Abell2390 are complicated by ionized gas, which is detected over large portions of all three systems. Radial color variations are detected in the majority of galaxies and, for those systems not showing extended [OII] emission, the weakening of D4000 (which measures the 4000 Angstrom break in magnitudes) with radius falls in the upper range of what is seen among nearby ellipticals. However, there is no correlation between local D4000 values and (g-r), suggesting that these quantities are sensitive to different parameters. We estimate the metallicity sensitivity of D4000 using a combination of observational and theoretical data, and find metallicity gradients for BCGs which are relatively steep, and in qualitative agreement with predictions for galaxies which experience a single monolithic dissipative collapse. Line gradients measured with respect to g surface brightness show excellent galaxy-to-galaxy consistency, and are in good agreement with what has been measured in Coma cluster galaxies. The presence of significant stellar population gradients in the BCGs suggests that the material from which they formed experienced dissipation during the collapse phases, and it seems likely that these galaxies could not have formed solely from the merging of gas-poor galaxies.
description: 48 pages, latex, figures available upon request to first author (davidge@dao.nrc.ca). To appear in the Astronomical Journal.
The Stochastic Axion Scenario
Creators: name: Graham, Peter W.
name: Scherlis, Adam
Publisher: name: arXiv
Year: 2018
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: For the minimal QCD axion model it is generally believed that overproduction of dark matter constrains the axion mass to be above a certain threshold, or at least that the initial misalignment angle must be tuned if the mass is below that threshold. We demonstrate that this is incorrect. During inflation, if the Hubble scale is low, the axion tends toward an equilibrium. This means the minimal QCD axion can naturally give the observed dark matter abundance in the entire lower part of the mass range, down to masses $\sim 10^{-12}$ eV (or $f_a$ up to almost the Planck scale). The axion abundance is generated by quantum fluctuations of the field during inflation. This mechanism generates cold dark matter with negligible isocurvature perturbations. In addition to the QCD axion, this mechanism can also generate a cosmological abundance of axion-like particles and other light fields.
description: 19 pages, 3 figures. v2: minor changes made to agree with published version
Additional file 3: of Comparative transcriptome analysis of Eimeria maxima (Apicomplexa: Eimeriidae) suggests DNA replication activities correlating with its fecundity
Creators: name: Dandan Hu
name: Chaoyue Wang
name: Wang, Si
name: Xinming Tang
name: Chunhui Duan
name: Sixin Zhang
name: Jinxia Suo
name: Miner Deng
name: Yanli Lv
name: Suo, Xun
name: Xianyong Liu
Publisher: name: figshare
Year: 2018
Subjects: subject: Biochemistry
subject: Microbiology
subject: FOS: Biological sciences
subject: Cell Biology
subject: Genetics
subject: Ecology
subject: 69999 Biological Sciences not elsewhere classified
subject: Developmental Biology

description: Comparative endogenous development for the E. maxima wild strain and its precocious line. Chickens were sacrificed after indicated times post-inoculation with the E. maxima wild strain BJ-WT-130 and the precocious line BJ-PL-98. The small intestines were used for H&E staining. Black, white and red arrows indicate the schizonts, gametocytes and unsporulated oocysts, respectively. Black arrowhead indicates microgametocytes. Bar = 20 μm. (PDF 52347 kb)
Uncertainties and array geometry selection
Creators: name: Akindoyin, Akinbiyi Olaposi
Publisher: name: Imperial College London
Year: 2017

description: This thesis investigates several issues associated with antenna array uncertainties, antenna array geometries and antenna selection approaches. In particular, initially this thesis is concerned with problem of using separate units of cheap SDR with independent local oscillator (LO) in a multi-antenna system. In such a system, each of these SDR boards which forms the receiving array elements has slightly different carrier frequency and phase uncertainties even if all the local oscillators are using similar hardware. In order to form a fully coherent array testbed, two synchronisation methods are proposed to remove these uncertainties/errors. The first is a hardware synchronisation approach while the second is based on a novel algorithm which operates on the non-synchronous data to transform them to a new set of synchronous data by removing the local oscillator uncertainties. Finally the problem of antenna array selection is studied. Initially, this is based on the selection metrics that are based on various performance criteria. Then a qualitative study of the impact of the array geometry on the overall system performance is investigated with emphasis given to the family of 2D grid antenna array.Antenna array selection is suitable for systems with large number of antenna array and limited number of processors and RF units where, there is a strong motivation to develop an efficient and optimal antenna subset selection algorithm. Antenna selection is a signal processing technique that can help to reduce the number of RF chains, while preserving the system performance at a certain required level. Then, a different antenna array selection approach is proposed which is based on the concept of sensor locator polynomial (SLP) in conjunction with two equivalent linear arrays (ELA) and sensitivity analysis of the array geometry and its associated manifold, thus selecting the best subset of antennas that satisfies a predefined criterion.
Deflection angle of light for an observer and source at finite distance from a rotating wormhole
Creators: name: Ono, Toshiaki
name: Ishihara, Asahi
name: Asada, Hideki
Publisher: name: arXiv
Year: 2018
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: By using a method improved with a generalized optical metric, the deflection of light for an observer and source at finite distance from a lens object in a stationary, axisymmetric and asymptotically flat spacetime has been recently discussed [Ono, Ishihara, Asada, Phys. Rev. D 96, 104037 (2017)]. By using this method, in the weak field approximation, we study the deflection angle of light for an observer and source at finite distance from a rotating Teo wormhole, especially by taking account of the contribution from the geodesic curvature of the light ray in a space associated with the generalized optical metric. Our result of the deflection angle of light is compared with a recent work on the same wormhole but limited within the asymptotic source and observer [Jusufi, Ovgun, Phys. Rev. D 97, 024042, (2018)], in which they employ another approach proposed by Werner with using the Nazim's osculating Riemannian construction method via the Randers-Finsler metric. We show that the two different methods give the same result in the asymptotic limit. We obtain also the corrections to the deflection angle due to the finite distance from the rotating wormhole.
description: 11 pages, no figures, text improved, accepted by PRD
X-ray Properties of B2 1028+313: A Quasar at the Center of the Abell Cluster A1030
Creators: name: Sarazin, C. L.
name: Koekemoer, A. M.
name: Baum, S. A.
name: O'Dea, C. P.
name: Owen, F. N.
name: Wise, M. W.
Publisher: name: arXiv
Year: 1998
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: X-ray observations with the ROSAT HRI and with ASCA are presented for the nearby radio quasar B2 1028+313, which is located in the cD galaxy at the center of the Abell cluster A1030. We also analyze archival ROSAT PSPC observations. We find that the X-ray emission is dominated by the quasar. The flux varied by a factor of about two between the ROSAT HRI and ASCA observations, which were about one year apart. The X-ray spectrum of the quasar is fit by a single power-law, except at low energies where there is a soft excess. Although the shape of the soft excess is not strongly constrained, it can be fit by a blackbody with a temperature of about 30 eV. There was evidence for extended X-ray emission, which contributed about 25% of the total flux. However, this emission does not appear to be normal X-ray emission from intracluster gas or a central cooling flow. The extended X-ray emission appears to be quite soft; if its spectrum is modeled as thermal emission, the temperature is ~0.2 keV, rather than the 5-10 keV expected for ICM emission. The radial surface distribution of the emission was not fit by either the beta model which usually describes ICM emission, or by a cooling flow model. The ASCA and ROSAT spectra showed no convincing evidence for a thermal component with a cluster-like temperature, either in the overall spectral shape or in emission lines. In addition, the ROSAT PSPC image showed that the extended X-ray emission was highly elongated to the NNW and SSE, in the same direction as the extended radio emission from the quasar. We suggest that the extended emission is inverse Compton emission from the extended radio lobes.
description: ApJ, in press, 16 pages with 11 imbedded figures, Latex in the emulateapj style
title: ADCO, Cartulaire de Fontenay, premier fragment (XIIIe siècle), Cart. 201 (15 H 9), 175 folios, f. 025r
Creators: name: de la Côte d'Or, Archives départementales
name: Petot, Frédéric
name: Archives Départementales De La Côte-D'Or
name: Petot, Frédérique
name: Projet CBMA
name: CG21/F.PETOT/2009
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2020
Subjects: subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris
subject: Corpus Burgundiae Medii Aevi
subject: Chartes de la Bourgogne du Moyen Âge
subject: cartulaire

description: Cartulaire de Fontenay, premier fragment (XIIIe siècle), Archives départementales de la Côte-d'Or, Cart. 201 (15 H 9), 175 folios. Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Cartulaire de Fontenay, premier fragment (XIIIe siècle), Archives départementales de la Côte-d'Or, Cart. 201 (15 H 9), 175 folios, f. 025r, in Projet CBMA - Corpus Burgundiae Medii Aevi [Ressource en ligne], https:// manuscrits.cbma-project.eu/
description: Provenance: https://catalogue.bnf.fr/ark:/12148/cb119679755
description: Provenance: https://www.geonames.org/7874015
description: Provenance: http://www.idref.fr/027691802/id
description: Provenance: abbaye de Fontenay
description: Provenance: http://www.wikidata.org/entity/Q464918
Rhamnus napeca Linnaeus, 1753, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1753
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Magnoliopsida
Rosales
Rhamnaceae
Rhamnus
Rhamnus napeca

description: Rhamnus napeca, spec. nov.
 7. Rhamnus aculeis subgeminatis recurvis, pedunculis corymbosis, floribus semidigynis, foliis serratis utrinque laevibus. Fl. zeyl. 87. *
 Habitat in Zeylona . ♄
description: Published as part of Linnaeus, Carolus, 1753, Species plantarum: exhibentes plantas rite cognitas, ad genera relatas, cum differentiis specificis, nominibus trivialibus, synonymis selectis, locis natalibus, secundum systema sexuale digestas, Stockholm :Laurentius Salvius on page 194, DOI: 10.5281/zenodo.3931989
Recovering missing information when projecting 3D points or unprojecting image pixels
Creators: name: Chen, Wayne
Publisher: name: The Australian National University
Year: 2024

description: Computer vision aims to bridge the divide between 2D and 3D spaces. With the significant advance- ments in computational resources and deep learning techniques, neural networks have become the cornerstone for solving computer vision tasks. As the training of a neural network is data-driven, both input and ground truth data play pivotal roles in the network training process. However, 2D data is usually dense but involves a projection operation that loses 3D information; 3D data is often sparse due to sensor limitations. Addressing this challenge, our research focuses on the recovery of missing information when pro- jecting 3D points or unprojecting image pixels, exploring this problem across three different tasks: novel view synthesis, uncertainty-aware monocular depth estimation, and latent space analyses for the deepSDF model. Novel view synthesis from sparse coloured point clouds aims to generate dense RGB images given a sparse XYZRGB input Uncertainty-aware Monocular Depth Estimation (MDE) targets the generation of dense depth es- timation given a dense RGB input and sparse depth ground truth. We propose a novel network with an encoder-decoder structure and a novel loss function that enables joint training of depth and uncertainty estimation. This model competes closely with state-of-the-art solutions on depth estimation evaluation metrics and outperforms them on uncertainty estimation. The latent space analysis for the deepSDF model explores the connections among latent represent- ations of different 3D models. Our experiments reveal that these latent codes are not independent; latent codes generated from linear interpolation between each pair of latent codes represent the transformation from one model to another. Our findings confirm the existence and impact of sparsity within input data. However, our proposed methods demonstrate not only how to overcome these challenges but also how to evaluate their impact on the accuracy of the generated results. This work contributes significantly to enhancing the accuracy and reliability of models tackling data sparsity in the field of computer vision.
Doctoral thesis recital (horn)
Creators: name: Holmes, Rust
Publisher: name: The University of Texas at Austin
Year: 2019
Subjects: Sonatas (Horn and piano)
Horn and piano music.
Trios (Piano, horns (2))
Variations (Horn and piano)
Horn music.

description: Scherzo concertante (1966) / Vaclav Nelhybel -- Sonata in B minor for horn and piano, op. 27 (1955) / Kurt Atterberg -- Canto serioso (1913) / Carl Nielsen -- Introduction, theme, and variations, op. 13 (1875) / Franz Strauss -- Pange lingue : (2017) / Patrick Hughes (Patrick Hughes, horn) -- Tanguito : (1964) / Dante Yenque.
The NOT GL survey for multiply imaged quasars
Creators: name: Jaunsen, A. O.
name: Jablonski, M.
name: Pettersen, B. R.
name: Stabell, R.
Publisher: name: arXiv
Year: 1995
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: A gravitational lens (GL)-search program, initiated in 1990 at the Nordic Optical Telescope (NOT), has revealed several possible GL-candidates among a sample of 168 quasars (QSOs), chosen from three lists compiled by C. Hazard, D. Reimers and J. Surdej, respectively. Some of these candidates, selected for having close companions (within 5 arcseconds), were imaged in several filters and their colours compared. Low dispersion spectra of the most promising candidates were also obtained at the NOT and ESO New Technology Telescope (NTT). None of these has proved to be strong candidates of gravitational lensing effects. We present this new sample of QSOs and combine it with previously published optical QSO samples in a statistical analysis to yield constraints on flat cosmologies and galaxy velocity dispersions. Finally, by simulating larger samples of quasars and gravitational lenses, we discuss how the uncertainties affecting our present results would be changed.
description: 12 pages (including figures) uuencoded compressed Postscript file. Accepted for publication in Astronomy & Astrophysics.
Ziziphus napeca Willd.
Creators: name: Jarvis, Charlie
Publisher: name: Linnaean Society of London in association with the Natural History Museum
Year: 2007
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Magnoliopsida
Rosales
Rhamnaceae
Ziziphus
Ziziphus napeca

description: Rhamnus napeca Linnaeus, Species Plantarum 1: 194. 1753.
"Habitat in Zeylona." RCN: 1569.
Lectotype (Wadhwa in Dassanayake & Clayton, Revised Handb. Fl. Ceylon 10: 365. 1996): Herb. Hermann 3: 43, No. 87 (BM-000594685).
Current name: Ziziphus napeca (L.) Willd. (Rhamnaceae).
description: Published as part of Jarvis, Charlie, 2007, Chapter 7: Linnaean Plant Names and their Types (part R), pp. 785-805 in Order out of Chaos. Linnaean Plant Types and their Types, London :Linnaean Society of London in association with the Natural History Museum on page 791, DOI: 10.5281/zenodo.291971
Fuel cell performance prediction using an Auto-Regressive Moving-Average Model
Creators: name: A.H. Detti
name: N. Yousfi Steiner
name: L. Bouillaut
name: A.B. Same
name: S. Jemei
Publisher: name: Zenodo
Year: 2019
Subjects: PEMFC Systems, prognostic, ARMA

description: Presentation given at the IEEE Vehicle and propulsion Conference VPPC 2019, October 14th-17th, 2019 Hanoi Vietnam
New mechanism producing axions in the AQN model and how the CAST can discover them
Creators: name: Fischer, H.
name: Liang, X.
name: Semertzidis, Y.
name: Zhitnitsky, A.
name: Zioutas, K.
Publisher: name: arXiv
Year: 2018
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: Astrophysics of Galaxies (astro-ph.GA)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: We advocate the idea that there is a fundamentally new mechanism for the axion production in the Sun, which has never been discussed previously in the literature. This novel mechanism of the axion production is based on the so-called Axion Quark Nugget (AQN) Dark Matter Model. These axions will be produced in addition to well studied axions emitted due to the Primakoff effect. The AQN model was originally invented as a natural explanation of the observed ratio $Ω_{\rm dark} \sim Ω_{\rm visible}$ when the DM and visible matter densities assume the same order of magnitude values, irrespectively to the axion mass $m_a$ or initial misalignment angle $θ_0$. This model, without adjustment of any parameters, reproduces reasonably the intensity of the extreme UV (EUV) radiation from the solar corona as a result of the AQN annihilation events with the solar material. This extra energy released in corona represents a resolution, within AQN framework, a long standing puzzle known in the literature as the "solar corona heating mystery". The same annihilation events also produce the relativistic axions. This represents a new mechanism of the axion production, and constitutes the main subject of this work. The flux of these axions is unambiguously fixed in this model and expressed in terms of the EUV luminosity from corona. We also compute the spectral properties of these axions and make few comments on the potentials for the discovery of these solar axions by the upgraded CAST (CERN Axion Solar Axion) experiment.
description: matches the published version
Enhanced photon coupling of ALP dark matter adiabatically converted from the QCD axion
Creators: name: Ho, Shu-Yu
name: Saikawa, Ken'ichi
name: Takahashi, Fuminobu
Publisher: name: arXiv
Year: 2018
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We revisit the adiabatic conversion between the QCD axion and axion-like particle (ALP) at level crossing, which can occur in the early universe as a result of the existence of a hypothetical mass mixing. This is similar to the Mikheyev-Smirnov-Wolfenstein effect in neutrino oscillations. After refining the conditions for the adiabatic conversion to occur, we focus on a scenario where the ALP produced by the adiabatic conversion of the QCD axion explains the observed dark matter abundance. Interestingly, we find that the ALP decay constant can be much smaller than the ordinary case in which the ALP is produced by the realignment mechanism. As a consequence, the ALP-photon coupling is enhanced by a few orders of magnitude, which is advantageous for the future ALP and axion-search experiments using the ALP-photon coupling.
description: 24 pages, 9 figures, 1 table;references added, typo fixed, matches the version published in JCAP
Description of the data set for the manuscript "A machine learning approach to quantifying the specificity of color-emotion associations and their cultural differences".
Creators: name: Jonauskaite, Domicele
name: Wicker, Jörg
name: Mohr, Christine
name: Dael, Nele
name: Havelka, Jelena
name: Papadatou-Pastou, Marietta
name: Zhang, Meng
name: Oberfeld, Daniel
Publisher: name: The Royal Society
Year: 2019

description: Description of the data set
Reminiscences of Mary Lee Hu 1985
Publisher: name: Columbia University
Year: 2019
Subjects: Jewelers
Jewelry
Jewelry making
Wire craft

description: Childhood, Olmsted Falls, Ohio; education at Cranbrook Academy of Art, Southern Illinois University; wire weaving and jewelry; marriage; teaching at Southern Illinois University and Bellingham, Washington; exhibitions; aesthetic and commercial aspects of jewelry making.
3D global simulations of RIAFs: convergence, effects of azimuthal extent and dynamo
Creators: name: Dhang, Prasun
name: Sharma, Prateek
Publisher: name: arXiv
Year: 2018
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: We study the long-term evolution of non-radiative geometrically thick ($H/R\approx 0.5$) accretion flows using 3D global ideal MHD simulations and a pseudo-Newtonian gravity. We find that resolving the scale height with 42 grid points is adequate to obtain convergence with the product of quality factors $\langle \langle Q_θ \rangle \rangle \langle \langle Q_ϕ \rangle \rangle \geq 300$ and magnetic tilt angle $θ_B \sim 13^{\circ}-14^{\circ}$. Like previous global isothermal thin disk simulations, we find stronger mean magnetic fields for the restricted azimuthal domains. Imposing periodic boundary conditions with the azimuthal extent smaller than $2π$ make the turbulent field at low $m$ appear as a mean field in the runs with smaller azimuthal extent. But unlike previous works, we do not find a monotonic trend in turbulence with the azimuthal extent. We conclude that the minimum azimuthal extent should be $\geq π/2$ to capture the flow structure, but a full $2 π$ extent is necessary to study the dynamo. We find an intermittent dynamo cycle, with $α$-quenching playing an important role in the nonlinear saturated state. Unlike previous local studies, we find almost similar values of kinetic and magnetic $α$-s, giving rise to an irregular distribution of dynamo-$α$. The effects of dynamical quenching are shown explicitly for the first time in global simulations of accretion flows.
description: 24 pages, 27 figures, 4 tables. Accepted in MNRAS. We welcome comments and suggestions
THE UNUSUAL X-RAY AND OPTICAL PROPERTIES OF THE ULTRASOFT AGN ZWICKY 159.034 (RE J 1237+264)
Creators: name: Brandt, W. N.
name: Pounds, K. A.
name: Fink, H.
Publisher: name: arXiv
Year: 1995
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Zwicky 159.034, one of the Seyfert galaxies identified with EUV sources detected during the ROSAT Wide Field Camera (WFC) all-sky survey, has unusual properties. The ROSAT Position Sensitive Proportional Counter (PSPC) 0.1--2.5 keV X-ray spectrum, obtained simultaneously with the WFC survey, appears extremely steep. Subsequent deeper pointed observations with ROSAT revealed that its 0.1--2.5 keV count rate had decreased by an extremely large amount (a factor of about 70). This is comparable to the variability amplitude seen in another ultrasoft Seyfert, E1615+061. There appears to be about 10 times as much flux in the soft component as in any expected hard tail suggesting that, in the absence of partial covering of the hard flux, the soft flux cannot arise via reprocessing of the hard tail. Its peculiar optical spectrum has permitted lines with widths about 1200--1500 km s^{-1}, and forbidden lines are weak or absent. Its optical spectrum shows evidence for variability, and might be used to study the role reprocessed X-rays play in the formation of optical lines.
description: 5 pages, uuencoded compressed postscript, ps figs available by email from wnb@mail.ast.cam.ac.uk, MNRAS in press
$s$-Process in Massive Carbon-Enhanced Metal-Poor Stars
Creators: name: Banerjee, Projjwal
name: Qian, Yong-Zhong
name: Heger, Alexander
Publisher: name: arXiv
Year: 2018
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: Observations suggest that the interstellar medium (ISM) might have been highly enriched in carbon at very early times. We explore nucleosynthesis in massive carbon-enhanced metal-poor (CEMP) stars of $12$--$40\,\mathrm{M}_\odot$ formed from such an ISM with ${\rm [Fe]}\leq-2$. We find substantial production of elements heavier than Fe, mostly up to Sr, by the weak \textsl{s}-process in stars with initial abundances of ${\rm [CNO]}\gtrsim-1.5$. Even heavier elements, up to Ba, can be produced for ${\rm [CNO]}\gtrsim-0.5$. The efficiency of this \textsl{s}-process is sensitive to the initial enhancement of C (or more generally, CNO) and mass of the star, with the yield increasing approximately linearly with the initial Fe abundance. The \textsl{s}-process in CEMP stars of $\gtrsim 20 \,\mathrm{M}_\odot$ with ${\rm [CNO]}\gtrsim -1.5$ can be an important source for heavy elements in the Early Galaxy.
description: 6 pages, 2 figures, and 3 tables, Accepted for publication in MNRAS
MOESM1 of Is nodding syndrome in northern Uganda linked to consumption of mycotoxin contaminated food grains?
Creators: name: Echodu, Richard
name: Edema, Hilary
name: Malinga, Geoffrey
name: Hendy, Adam
name: Colebunders, Robert
name: Kaducu, Joyce Moriku
name: Ovuga, Emilio
name: Haesaert, Geert
Publisher: name: figshare
Year: 2018
Subjects: subject: Biochemistry
subject: Biotechnology
subject: Ecology
subject: FOS: Biological sciences
subject: Sociology
subject: FOS: Sociology
subject: 69999 Biological Sciences not elsewhere classified
subject: Science Policy

description: Additional file 1: Table S1. Concentration of mycotoxins in grain samples from Lamwo and Kitgum in households with NS and without NS.
Introducing a new, robust galaxy finder algorithm for simulations
Creators: name: Cañas, Rodrigo
name: Elahi, Pascal J.
name: Welker, Charlotte
name: Lagos, Claudia del P.
name: Power, Chris
name: Dubois, Yohan
name: Pichon, Christophe
Publisher: name: arXiv
Year: 2018
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: Identifying galaxies in hydrodynamical simulations is a difficult task, particularly in regions of high density such as galaxy groups and clusters. We present a new scale-free shape-independent algorithm to robustly and accurately identify galaxies in simulation, implemented within the phase-space halo-finder code VELOCIraptor. This is achieved by using the full phase-space dispersion tensor for particle assignment and an iterative adjustment of search parameters, which help us overcome common structure finding problems. We apply our improved method to the Horizon-AGN simulation and compare galaxy stellar masses ($M_*$), star formation rates (SFR) and sizes with the elaborate configuration-space halo finder, HaloMaker. Galaxies living in halos with $> 1$ galaxy are the most affected by the shortcomings of real-space finders, with their mass, SFR, and sizes being $> 2$ times larger (smaller) in the case of host (satellite) galaxies. Thus, our ability to measure minor/major merger rates and disentangle environmental effects in simulations can be generally hindered if the identification of galaxies is not treated carefully. Though large systematic differences are obtained on a one-to-one basis, the overall Galaxy Stellar Mass Function, the Star Formation Rate Function and mass-size relations are not greatly affected. This is due to isolated galaxies being the most abundant population, dominating broad statistics.
description: Accepted for publication in MNRAS. 28 pages, 12 figures
title: ADCO, Cartulaire de Cîteaux pour les domaines de Beaune (XVe siècle), Cart. 177 (11 H 289), 197 folios, f. 0386
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: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris
subject: Corpus Burgundiae Medii Aevi
subject: Chartes de la Bourgogne du Moyen Âge
subject: cartulaire

description: Cartulaire de Cîteaux pour les domaines de Beaune (XVe siècle), Archives départementales de la Côte-d'Or, Cart. 177 (11 H 289), 197 folios, f. 0386, 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. 0386, 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
ROSAT PSPC observations of the outer regions of the Perseus cluster of galaxies
Creators: name: Ettori, S.
name: Fabian, A. C.
name: White, D. A.
Publisher: name: arXiv
Year: 1998
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present an analysis of four off-axis ROSAT PSPC observations of the Perseus cluster of galaxies (Abell~426). We detect the surface brightness profile to a radius of 80 arcmin ($\sim 2.4 h_{50}^{-1}$ Mpc) from the X-ray peak. The profile is measured in various sectors and in three different energy bands. Firstly, a colour analysis highlights a slight variation of $N_{H}$ over the region, and cool components in the core and in the eastern sector. We apply the $β$-model to the profiles from different sectors and present a solution to the, so-called, $β$-problem. The residuals from an azimuthally-averaged profile highlight extended emission both in the East and in the West, with estimated luminosities of about 8 and 1 $\times 10^{43} erg/s$, respectively. We fit several models to the surface brightness profile, including the one obtained from the Navarro, Frenk and White (1995) potential. We obtain the best fit with the gas distribution described by a power law in the inner, cooling region and a $β$-model for the extended emission. Through the best-fit results and the constraints from the deprojection of the surface brightness profiles, we define the radius where the overdensity inside the cluster is 200 times the critical value, $r_{200}$, at $2.7 h_{50}^{-1}$ Mpc. Within $2.3 h_{50}^{-1}$ Mpc ($0.85 r_{200}$), the total mass in the Perseus cluster is $1.2 \times 10^{15} M_{\odot}$ and its gas fraction is about 30 per cent.
description: 21 pages, 23 figures; accepted for publication in MNRAS; also available at http://www-xray.ast.cam.ac.uk/~settori/paper.html
Additional file 4: of Association between cognitive function and life-space mobility in older adults: results from the FRĂŠLE longitudinal study
Creators: name: FranĂ§Ois BĂŠland
name: Julien, Dominic
name: Bier, Nathalie
name: Desrosiers, Johanne
name: Marie-Jeanne Kergoat
name: Demers, Louise
Publisher: name: figshare
Year: 2018
Subjects: subject: Biochemistry
subject: Space Science
subject: Medicine
subject: Molecular Biology
subject: 59999 Environmental Sciences not elsewhere classified
subject: FOS: Earth and related environmental sciences
subject: Sociology
subject: FOS: Sociology
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: 19999 Mathematical Sciences not elsewhere classified
subject: FOS: Mathematics

description: Part 4 Statistical significance and strength of association. Describes change in the predicted variable based on a 1-unit change in the predictor variable. (DOCX 23 kb)
COLLISIONAL VERSUS COLLISIONLESS MATTER: A ONE-DIMENSIONAL ANALYSIS OF GRAVITATIONAL CLUSTERING
Creators: name: Gheller, Claudio
name: Moscardini, Lauro
name: Pantano, Ornella
Publisher: name: arXiv
Year: 1995
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present the results of a series of one-dimensional N-body and hydrodynamical simulations which have been used for testing the different clustering properties of baryonic and dark matter in an expanding background. Initial Gaussian random density perturbations with a power-law spectrum $P(k) \propto k^n$ are assumed. We analyse the distribution of density fluctuations and thermodynamical quantities for different spectral indices $n$ and discuss the statistical properties of clustering in the corresponding simulations. At large scales the final distribution of the two components is very similar while at small scales the dark matter presents a lumpiness which is not found in the baryonic matter. The amplitude of density fluctuations in each component depends on the spectral index $n$ and only for $n=-1$ the amplitude of baryonic density fluctuations is larger than that in the dark component. This result is also confirmed by the behaviour of the bias factor, defined as the ratio between the r.m.s of baryonic and dark matter fluctuations at different scales: while for $n=1,\ 3$ it is always less than unity except at very large scales where it tends to one, for $n=-1$ it is above 1.4 at all scales. All simulations show also that there is not an exact correspondence between the positions of largest peaks in dark and baryonic components, as confirmed by a cross-correlation analysis. The final temperatures depend on the initial spectral index: the highest values are obtained for $n=-1$ and are in proximity of high density regions.
description: 7 pages Latex (MN style) + 10 figures in postscript files, uuencoded submitted to MNRAS
MEASURING SPIRAL ARM TORQUES: RESULTS FOR M100
Creators: name: Gnedin, Oleg Y.
name: Goodman, Jeremy
name: Frei, Zsolt
Publisher: name: arXiv
Year: 1995
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Spiral arms, if they are massive, exert gravitational torques that transport angular momentum radially within galactic disks. These torques depend not on the pattern speed or permanence of the arms but only on the nonaxisymmetric mass distribution. Hence the torques can be measured from photometry. We demonstrate this using $gri$ CCD data for M100 (NGC 4321). Since we find consistency among the three bands, we believe that dust and young stars in the arms do not seriously bias our results. If the present epoch is representative, the timescale for redistribution of angular momentum in M100 is $5-10$ Gyr, the main uncertainty being the mass-to-light ratio of the disk.
description: Uuencoded compressed PostScript (300k) - 26 pages, figs. 3-9; submitted to AJ. Full PostScript version (with all figures) is available through anonymous ftp at ftp://astro.princeton.edu/ognedin/Torque/paper.ps or ftp://astro.princeton.edu/library/preprints/pop613.ps.Z or through WWW http://www.astro.princeton.edu/~library/prep.html