cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
The distribution of nearby stars in phase space mapped by Hipparcos III. Clustering and streaming among A-F type stars
Creators: name: Chereul, E.
name: Crézé, M.
name: Bienaymé, O.
Publisher: name: arXiv
Year: 1998
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: This paper presents the detailed results obtained in the search of density- velocity inhomogeneities in a volume limited and absolute magnitude limited sample of A-F type dwarfs within 125 parsecs of the Sun. A 3-D wavelet analysis is used to extract inhomogeneities, both in the density and velocity distributions. Having established a real picture of the phase space without assumption we come back to previously known observational facts regarding clusters and associations, superclusters. In the 3-D position space, well known open clusters (Hyades, Coma Berenices and Ursa Major), associations (parts of the Scorpio-Centaurus association) as well as the Hyades evaporation track are retrieved. Three new probably loose clusters are identified (Bootes, Pegasus 1 and 2). The sample is relatively well mixed in the position space since less than 7 per cent of the stars belong to structures with coherent kinematics, most likely gravitationally bound. In the velocity space, the majority of large scale velocity structures ($σ$ ~ 6.3 $km s-1$) are Eggen's superclusters (Pleiades SCl, Hyades SCl and Sirius SCl) with the whole Centaurus association. A new supercluster-like structure is found with a mean velocity between the Sun and Sirius SCl velocities. These structures are all characterized by a large age range which reflects the overall sample age distribution. Moreover, a few old streams of ~ 2 Gyr are also extracted at this scale with high U components. We show that all these large velocity dispersion structures represent 46% of the sample. Smaller scales (σ~ 3.8 and 2.4 $km s-1$) reveal that superclusters are always substructured by 2 or more streams which generally exhibit a coherent age distribution. Percentages of stars in these streams are 38% and 18% respectively.
description: 25 pages, Latex, 29 figures, 4 tables to be published in A&A Supplements Series
Triaxial Galaxies with Cusps
Creators: name: Merritt, David
name: Fridman, Tema
Publisher: name: arXiv
Year: 1995
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We have constructed fully self-consistent models of triaxial galaxies with central density cusps. The triaxial generalizations of Dehnen's spherical models are presented, which have densities that vary as 1/r^gamma near the center and 1/r^4 at large radii. We computed libraries of about 7000 orbits in each of two triaxial models with gamma=1 (weak cusp) and gamma=2 (strong cusp); these two models have density profiles similar to those of the core and power-law galaxies observed by HST. Both mass models have short-to-long axis ratios of 1:2 and are maximally triaxial. A large fraction of the orbits in both model potentials are stochastic, as evidenced by their non-zero Liapunov exponents. We show that most of the stochastic orbits in the strong- cusp potential diffuse relatively quickly through their allowed phase-space volumes, on time scales of 100 - 1000 dynamical times. Stochastic orbits in the weak-cusp potential diffuse more slowly, often retaining their box-like shapes for 1000 dynamical times or longer. Attempts to construct self- consistent solutions using just the regular orbits failed for both mass models. Quasi-equilibrium solutions that include the stochastic orbits exist for both models; however, real galaxies constructed in this way would evolve near the center due to the continued mixing of the stochastic orbits. We attempted to construct more nearly stationary models in which stochastic phase space was uniformly populated at low energies. These ``fully mixed'' solutions were found to exist only for the weak-cusp potential. No significant fraction of the mass could be placed on fully-mixed stochastic orbits in the strong-cusp model, demonstrating that strong triaxiality can be inconsistent with a high central density.
description: 58 TEX pages, 14 PostScript figures, uses epsf.sty
title: ADCO, Cartulaire des Dominicains de Dijon (1286), Cart. 221 (H 53), 170 folios, f. 0321
Creators: name: de la Côte d'Or, Archives départementales
name: Petot, Frédéric
name: Archives Départementales De La Côte-D'Or
name: Petot, Frédérique
name: Projet CBMA
name: CG21/F.PETOT/2012
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2020
Subjects: subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris
subject: Corpus Burgundiae Medii Aevi
subject: Chartes de la Bourgogne du Moyen Âge
subject: cartulaire

description: Cartulaire des Dominicains de Dijon (1286), Archives départementales de la Côte-d'Or, Cart. 221 (H 53), 170 folios. Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Cartulaire des Dominicains de Dijon (1286), Archives départementales de la Côte-d'Or, Cart. 221 (H 53), 170 folios, f. 0321, in Projet CBMA - Corpus Burgundiae Medii Aevi [Ressource en ligne], https:// manuscrits.cbma-project.eu/
description: Provenance: Dijon
description: Provenance: http://www.wikidata.org/entity/Q7003
description: Provenance: https://catalogue.bnf.fr/ark:/12148/cb15250518p
description: Provenance: http://www.idref.fr/02643413X/id
description: Provenance: https://www.geonames.org/6453767
A Note on Slant and Hemislant Submanifolds of an (ε)-Para Sasakian Manifold
Creators: name: Laha, Barnali
name: Arindam Bhattacharyya
Publisher: name: figshare
Year: 2018
Subjects: Algebra

description: In the present note we have derived some basic results pertaining to the geometry of slant and hemislant submanifolds of an (ε)-para Sasakian manifold.
The art of modeling CO, [CI], and [CII] in cosmological galaxy formation models
Creators: name: Popping, Gergö
name: Narayanan, Desika
name: Somerville, Rachel S.
name: Faisst, Andreas L.
name: Krumholz, Mark R.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: The advent of new sub-millimeter observational facilities has stimulated the desire to model the sub-mm line emission of galaxies within cosmological galaxy formation models. This is typically done in post-processing by applying sub-resolution recipes to describe the properties of the unresolved interstellar medium. At the same time, while there is freedom in how one implements these sorts of recipes, the impact of various choices has yet to be systematically explored in simulations. In this paper, we do just that. We combine a semi-analytic model of galaxy formation with chemical equilibrium networks and numerical radiative transfer models and explore how different choices for the sub-grid modeling affect the predicted CO, [CI], and [CII] emission of galaxies. We find that a key component for a successful model includes a molecular cloud mass-size relation and scaling for the ultraviolet and cosmic ray radiation field that varies based on local ISM properties. Our most successful model adopts a Plummer profile for the radial density distribution of gas within molecular clouds. On the other hand, different assumptions for the clumping of gas within molecular clouds and changes in the slope of the molecular cloud mass distribution function hardly affect the CO, [CI], and [CII] luminosities of galaxies. At fixed star-formation rate the [CII]-SFR ratio of galaxies scales inversely with the pressure acting on molecular clouds, increasing the molecular clouds density and hence decreasing the importance of [CII] line cooling. Overall we find that it is essential that a wide range of sub-mm emission lines arising in vastly different phases of the ISM are used as model constraints in order to limit the freedom in sub-grid choices and we present the details of the most successful model variant.
description: accepted for publication in MNRAS
Detection of Surface Brightness Fluctuations in NGC 4373 Using the Hubble Space Telescope
Creators: name: Pahre, M. A.
name: Mould, J. R.
name: Dressler, A.
name: Team, the WFPC-2 Investigation Definition
Publisher: name: arXiv
Year: 1998
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Surface brightness fluctuations (SBF) have been detected for three elliptical galaxies-NGC 3379 in the Leo group, NGC 4406 in the Virgo cluster, and NGC 4373 in the Hydra-Centaurus supercluster-using marginally-sampled, deep images taken with the Planetary Camera of the WFPC-2 instrument on the Hubble Space Telescope (HST). The power spectrum of the fluctuations image is well-fit by an empirical model of the point-spread function (PSF) constructed using point sources identified in the field. The previous ground-based SBF measurements for NGC 3379 and NGC 4406 are recovered, thereby demonstrating the capability of the Planetary Camera of WFPC-2 to measure distances using the SBF technique despite the marginal sampling of the images. The residual variance due to unresolved sources in all three galaxies is only 2-5% of the detected fluctuations signal, which confirms the advantage of HST imaging in minimizing the uncertainty of this SBF correction. Extensive consistency checks, including an independent SBF analysis using an alternate software package, suggest that our internal uncertainties are < 0.02 mag. The fluctuations magnitude for NGC 4373 is I814bar = 31.31 +/- 0.05 mag, corresponding to a distance modulus of DM = 32.99 +/- 0.11. This implies a peculiar velocity for this galaxy of 415 +/- 330 km/s, which is smaller than derived from the D_n-sigma relation. These results demonstrate the power of the post-repair HST to measure distances to elliptical galaxies at significant redshifts using the SBF technique.
description: to appear in The Astrophysical Journal; 25 pages, including 7 Postscript figures and 2 tables; uses AAS LaTeX style files
Additional file 1 of Translation of the Debriefing Assessment for Simulation in Healthcare in Portuguese and cross-cultural adaptation for Portugal and Brazil
Creators: name: Couto, Thomaz Bittencourt
name: Matos, Francisco Maio
name: de Toledo Rodovalho, Paula Dias
name: Fey, Mary
name: Simon, Robert
name: Muller-Botti, Sacha
Publisher: name: figshare
Year: 2021
Subjects: subject: Medicine
subject: Molecular Biology
subject: Neuroscience
subject: Sociology
subject: FOS: Sociology

description: Additional file 1. Portuguese Rater Version.
Supporting the needs of pre- and primary school children in rural Victoria: Multidisciplinary views and experiences
Creators: name: Reid, Carol
name: Burrows, J
name: Sprunt, R
name: Dolar, A
Publisher: name: La Trobe
Year: 2024
Subjects: classificationCode: 5201
subject: Applied and developmental psychology
classificationCode: 42
subject: Health sciences
subject: FOS: Health sciences
classificationCode: 4201
subject: Allied health and rehabilitation science

description: Problem: Predicted effects on children from the COVID-19 pandemic include poorer mental health and increased behavioural and developmental concerns. Rural children are at higher risk due to socio-economic factors, isolation and reduced access to services. Investigation by health services into the physical, social and emotional needs of children in rural areas is critical to inform local health promotion planning, service delivery priorities and workforce capacity building. Setting: Located in a Modified Monash Model category 5, our northern Victorian health service undertook a child-focused needs assessment in order to be strategically responsive to community issues. Key measures: The project utilised a quantitative community profiling approach and qualitative interviews with a purposive sample (n = 17) of multidisciplinary professionals. Strategies for change: Three main themes emerged: (1) Perpetual navigation of rural access limitations highlighted professionals' exhaustion in working in environments with ongoing unmet needs. (2) Cycles of disadvantage and early intervention gaps identified flow-on negative effects, with concerning trends in poorer child outcomes. (3) Solutions through collaboration grouped ideas to improve support for children. Effects of change: Community-level enablement strategies could increase contact with allied health professionals for rural children and reduce reliance on individualised treatment approaches. Lessons learnt: One collaborative action is to pilot and evaluate allied health student placement models to deliver group programs for rural children.
First-principles study of the anisotropic magneto-Peltier effect
Creators: name: Masuda, Keisuke
name: Uchida, Ken-ichi
name: Iguchi, Ryo
name: Miura, Yoshio
Publisher: name: arXiv
Year: 2018
Subjects: subject: Materials Science (cond-mat.mtrl-sci)
subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: FOS: Physical sciences

description: We study theoretically the anisotropic magneto-Peltier effect, which was recently demonstrated experimentally. A first-principles-based Boltzmann transport approach including the spin-orbit interaction shows that Ni has a larger anisotropy of the Peltier coefficient ($ΔΠ$) than Fe, consistent with experiments. It is clarified that spin-flip electron transitions due to the spin-orbit interaction are the key in the mechanism of the large anisotropic magneto-Peltier effect. Using our method, we further predict several ferromagnetic metals with much larger $ΔΠ$ than that of Ni.
description: 7 pages, 6 figures
Jynx torquilla Linnaeus, 1758, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1758
Subjects: Biodiversity
Taxonomy
Animalia
Chordata
Aves
Piciformes
Picidae
Jynx
Jynx torquilla

description: Jynx torquilla [spec. nov.]
Jynx.
Cuculus subgriseus maculatus, rectricibus nigris fasciis undulatis. Fn. svec. 78. t. 1. f. 78.
Jynx s. Torquilla. Bell. av. 76. a. Gesn. av. 573. Aldr. ornith. l. 12. c. 42. Jonst. av... t. 42. Will. orn. 95. t. 22. Raj. av. 44. Rudb. lapp. 66. t. 66. Alb. av. 1. p. 11. t. 21. Frisch. av... t. 38.
Habitat in Europa.
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 112, DOI: 10.5962/bhl.title.542, http://zenodo.org/record/3922206
Analytical Approximation to the Nonlinear Power Spectrum of Gravitational Clustering
Creators: name: Ma, Chung-Pei
Publisher: name: arXiv
Year: 1998
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: This paper presents an analytical formula that closely approximates the fully nonlinear power spectrum of matter fluctuations for redshift $z\approx 5$ to 0 over a wide range of cosmologically interesting flat models with varying matter density $Ω_m$ and neutrino fraction $Ω_ν$. The functional form is motivated by analytical solutions in asymptotic regimes, but in order to obtain accurate approximations, the coefficients are calculated from fits to the nonlinear power spectrum computed from numerical simulations of four cosmological models. The transformation from the linear to nonlinear power spectrum depends on $Ω_m, Ω_ν$, and time. A simple scaling rule is introduced, which greatly simplifies the construction of the functional form and allows the formula to depend directly on the rms linear mass fluctuation $σ_8$ instead of on an effective spectral index as in earlier work.
description: 16 pages, 4 postscript figures, AAS LaTeX v4.0. Accepted for publication in The Astrophysical Journal Letters
Additional file 2 of Translation of the Debriefing Assessment for Simulation in Healthcare in Portuguese and cross-cultural adaptation for Portugal and Brazil
Creators: name: Couto, Thomaz Bittencourt
name: Matos, Francisco Maio
name: de Toledo Rodovalho, Paula Dias
name: Fey, Mary
name: Simon, Robert
name: Muller-Botti, Sacha
Publisher: name: figshare
Year: 2021
Subjects: subject: Medicine
subject: Molecular Biology
subject: Neuroscience
subject: Sociology
subject: FOS: Sociology

description: Additional file 2. Portuguese Student Version.
Galactic Rotation Curves vs. Ultra-Light Dark Matter: Implications of the Soliton -- Host Halo Relation
Creators: name: Bar, Nitsan
name: Blas, Diego
name: Blum, Kfir
name: Sibiryakov, Sergey
Publisher: name: arXiv
Year: 2018
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: Astrophysics of Galaxies (astro-ph.GA)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: Bosonic ultra-light dark matter (ULDM) would form cored density distributions at the center of galaxies. These cores, seen in numerical simulations, admit analytic description as the lowest energy bound state solution ("soliton") of the Schroedinger-Poisson equations. Numerical simulations of ULDM galactic halos found empirical scaling relations between the mass of the large-scale host halo and the mass of the central soliton. We discuss how the simulation results of different groups can be understood in terms of the basic properties of the soliton. Importantly, simulations imply that the energy per unit mass in the soliton and in the virialised host halo should be approximately equal. This relation lends itself to observational tests, because it predicts that the peak circular velocity, measured for the host halo in the outskirts of the galaxy, should approximately repeat itself in the central region. Contrasting this prediction to the measured rotation curves of well-resolved near-by galaxies, we show that ULDM in the mass range $m\sim (10^{-22}÷10^{-21})$ eV, which has been invoked as a possible solution to the small-scale puzzles of $Λ$CDM, is in tension with the data. We suggest that a dedicated analysis of the Milky Way inner gravitational potential could probe ULDM up to $m\lesssim 10^{-19}$ eV.
description: 22 pages, 19 figures. v2: added clarifications, match journal version
A Study on Set-Valuations of Signed Graphs
Creators: name: P.K. Ashraf
name: K.A. Germina
name: N.K. Sudev
Publisher: name: figshare
Year: 2018
Subjects: Algebra

description: In this paper, we define the notion of set-valuations of signed graphs and discuss certain properties of signed graphs which admits certain types of set-valuations.
Tracing the Dynamics of Disk Galaxies with Optical and IR Surface Photometry: Color Gradients in M99
Creators: name: Gonzalez, Rosa A.
name: Graham, James R.
Publisher: name: arXiv
Year: 1995
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present optical and IR surface photometry of M99 (NGC 4254) at g, r_S i, J and K'. We also present a K' image of M51 (NGC 5194) for comparison. Fourier decomposition of the disk light reveals that the radial distribution of power depends on wavelength, which in turn implies that the spiral structure traced in the visual (i.e. young population I and dust) is different from the one detected at 2 microns (i.e. old stellar disk). We observe radial modulation of the power and a dependency of power with wavelength that are consistent with modal theory of spiral structure. A central motivation for our research is the fundamental idea of density wave theory that the passage of a spiral density wave triggers star formation. We have found a stellar population age gradient consistent with this scenario in a reddening-free, red supergiant-sensitive, Q-like photometric parameter at 6 kpc galactocentric distance across one of the arms of M99. We rule out that the change in this parameter, Q(r_SJgi), across the arm is mainly due to dust. The difference in Q(r_SJgi) going from the interarm regions to the arms also indicates that arms cannot be due exclusively to crowding of stellar orbits. We present the first measurement of Omega_p, the angular speed of the spiral pattern, and of the location of the corotation radius, derived from the drift velocity of the young stars away from their birth site. The measured Q(r_SJgi) implies a star formation rate for M99 within the range of 10-20 M_odot/yr; a disk stellar mass surface density of ~80 M_odot/pc^2; and a maximum contribution of ~20 percent from red supergiants to the K' light in a small region, and much smaller on average. We measure a K' arm--interarm contrast of 2-3, too high for M99 to be a truly isolated galaxy.
description: 25 pages of uuencoded, compressed Postscript (text only). To appear in 1 April 1996 issue of The Astrophysical Journal. Also available, together with 2 uuencoded, compressed PostScript files with 10 figures each, at http://astro.berkeley.edu/preprints.html
On the cosmological evolution of the FRII radio source population
Creators: name: Kaiser, Christian R.
name: Alexander, Paul
Publisher: name: arXiv
Year: 1998
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present an analytical model for the cosmological evolution of the FRII source population. Based on an earlier model for the intrinsic radio luminosity - linear size evolution of these objects, we construct theoretical source samples. The source distributions in the radio power - linear size plane of these samples are then compared with that of an observed flux-limited sample. We find that the source parameters determining the radio luminosity of FRII objects can not be independent of each other. The best-fitting models predict the jet power to be correlated either with the life time of the source or with the shape of the density distribution of the source environment. The latter case is consistent with the observed tendency of the most luminous radio sources at high redshift to be located in richer and more extended environments than their low redshift counterparts. We also find evidence for a class of FRII sources distinctly different from the main population. These sources are extremely old and/or are located in very underdense environments. The luminosity function of FRII sources resulting from the model is in good agreement with previous results for high luminosity sources. The apparent luminosity evolution of the radio luminosity function is not reproduced because of the high flux limit of the used comparison sample. The cosmological evolution of the median linear size of FRII sources is found to be mild.
description: 15 pages, 5 ps-figures, uses mn-style, accepted by MNRAS, corrects typographical errors and updates the references
Additional file 1 of Duration of basic and attenuated-psychotic symptoms in individuals at clinical high risk for psychosis: pattern of symptom onset and effects of duration on functioning and cognition
Creators: name: Staines, Lorna
name: Gajwani, Ruchika
name: Gross, Joachim
name: Gumley, Andrew I.
name: Lawrie, Stephen M.
name: Schwannauer, Matthias
name: Schultze-Lutter, Frauke
name: Uhlhaas, Peter J.
Publisher: name: figshare
Year: 2021
Subjects: subject: Medicine
subject: Neuroscience
subject: Physiology
subject: FOS: Biological sciences
subject: Sociology
subject: FOS: Sociology
subject: 111714 Mental Health
subject: FOS: Health sciences

description: Additional file 1: Supplementary Table 1. Summary of between group differences of onset of basic symptoms compared to onset of attenuated psychotic symptoms.
MPEC 2025-D175 : 2025 DX6
Creators: name: Minor Planet Center Staff
Publisher: name: The Minor Planet Center
Year: 2025
Subjects: subject: Small Solar System bodies
valueUri: http://astrothesaurus.org/uat/1469
subject: 2025 DX6

description: The Minor Planet Electronic Circulars contain information on unusual minor planets, routine data on comets and natural satellites, and occasional editorial announcements.  They are published on behalf of Division F of the International Astronomical Union by the Minor Planet Center, Smithsonian Astrophysical Observatory, Cambridge, MA 02138, U.S.A.
Metal-rich globular clusters of the Galaxy: morphology of the helium-burning "clump," and the determination of relative ages through the "$ΔV$" method
Creators: name: Catelan, M.
name: Pacheco, J. A. de Freitas
Publisher: name: arXiv
Year: 1995
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Morphological aspects of the $V, \bv$ diagram of metal-rich globular clusters are analyzed, on the basis of stellar evolution models for horizontal-branch (HB) and red giant branch stars. These have been incorporated into detailed synthetic HB models, the influence of differential reddening upon which is also discussed. The synthetic HB models are found to be very clumpy in the colour-magnitude diagram, though more extended structures occasionally result due to the effect of evolution away from the zero-age HB. In particular, "sloped" clumps may be naturally expected for sufficiently high helium abundances. Differential reddening is found to have a smaller influence than evolution itself upon the morphology of the clump. The synthetic HB models are also used to study the age difference between metal-rich clusters on the basis of the "$ΔV$" method. We emphasize the importance of knowing in advance the relative abundances of helium and metals in order to estimate this age difference quantitatively. We present chemical evolution models that serve to illustrate the effect, and show that, for two clusters of identical [Fe/H] and $ΔV$, the one enriched predominantly by ejecta from supernovae type II explosions will appear younger than the other which also suffered enrichment from supernovae type Ia ejecta. The implied locations of the red giant branch feature known as the "bump" are also discussed on the basis of recent observational and theoretical results. Our corresponding predictions should be checked against accurate observational data obtained with the Hubble Space Telescope.
description: 18 pages, LaTeX file (requires AAS LaTeX macro v4.0). Two tables and five figures available upon request. To appear in PASP (February 1996 issue)
Imperfect Knowledge Management (IKM) in GEFRED (GENeralized model for Fuzzy RElational Databases)
Creators: name: Jimenez, Leoncio
name: Valdes, Yolanda
name: Vistoso, Jorge
name: Lacoste, Germain
Publisher: name: arXiv
Year: 2025
Subjects: subject: Databases (cs.DB)
subject: FOS: Computer and information sciences

description: Imperfect Knowledge Management (IKM) aids in managing imprecise, uncertain, or incomplete aspects of meaning. IKM acknowledges that an enterprise's knowledge is often imperfect, characterized by varying degrees of imprecision, uncertainty, or incompleteness. In this context, knowledge is viewed as an object described by attributes and values. Our focus is on the domain of competencies (know how) in the production of coated cardboard, particularly the process of converting finished products from the manufactured cardboard. This process involves both classic and fuzzy attributes that are used to assess the quality of the cardboard. This article introduces a set of protocols designed to model a fuzzy metaknowledge base using GEFRED (GENeralized model for Fuzzy RElational Databases) in an Oracle 8i relational database system.
description: in Spanish language. The authors express their gratitude to Dr. Angelica Urrutia and Dr. Jose Galindo for providing the Fuzzy EER conceptual model and the FSQL development environment, respectively, which were used to create the fuzzy relational database. IX Congreso Argentino de Ciencias de la Computacion (CACIC 2003), 3 al 5 de octubre de 2003, Buenos Aires, Argentina
title: ADCO, Cartulaire général de Cîteaux, dit de Jean de Cirey, (XVe siècle), tome I, Cart. 185 (11 H 70), f. 0111r
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: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris
subject: Corpus Burgundiae Medii Aevi
subject: Chartes de la Bourgogne du Moyen Âge
subject: cartulaire

description: Cartulaire général de Cîteaux, dit de Jean de Cirey, (XVe siècle), tome I, Archives départementales de la Côte-d'Or, Cart. 185 (11 H 70), f. 0111r, 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 I, Archives départementales de la Côte-d'Or, Cart. 185 (11 H 70), f. 0111r, in Projet CBMA - Corpus Burgundiae Medii Aevi [Ressource en ligne], https:// manuscrits.cbma-project.eu/
description: Provenance: abbaye de Cîteaux
description: Provenance: http://www.wikidata.org/entity/Q843261
description: Provenance: https://www.geonames.org/3024876
description: Provenance: http://www.idref.fr/030974844/id
description: Provenance: https://catalogue.bnf.fr/ark:/12148/cb12228351v
Additional file 3 of Translation of the Debriefing Assessment for Simulation in Healthcare in Portuguese and cross-cultural adaptation for Portugal and Brazil
Creators: name: Couto, Thomaz Bittencourt
name: Matos, Francisco Maio
name: de Toledo Rodovalho, Paula Dias
name: Fey, Mary
name: Simon, Robert
name: Muller-Botti, Sacha
Publisher: name: figshare
Year: 2021
Subjects: subject: Medicine
subject: Molecular Biology
subject: Neuroscience
subject: Sociology
subject: FOS: Sociology

description: Additional file 3. Portuguese Instructor Version.
Small-signal modelling of maximum power point tracking for photovoltaic systems
Creators: name: Sokolov, Michael
Publisher: name: Imperial College London
Year: 2013

description: In grid connected photovoltaic (PV) generation systems, inverters are used to convert the generated DC voltage to an AC voltage. An additional dc-dc converter is usually connected between the PV source and the inverter for Maximum Power Point Tracking (MPPT). An iterative MPPT algorithm searches for the optimum operating point of PV cells to maximise the output power under various atmospheric conditions. It is desirable to be able to represent the dynamics of the changing PV power yield within stability studies of the AC network. Unfortunately MPPT algorithms tend to be nonlinear and/or time-varying and cannot be easily combined with linear models of other system elements. In this work a new MPPT technique is developed in order to enable linear analysis of the PV system over reasonable time scales. The new MPPT method is based on interpolation and an emulated-load control technique. Numerical analysis and simulations are employed to develop and refine the MPPT. The small-signal modelling of the MPPT technique exploits the fact that the emulated-load control technique can be linearised and that short periods of interpolation can be neglected. A small-signal PV system model for variable irradiation conditions was developed. The PV system includes a PV module, a dc-dc boost converter, the proposed controller and a variety of possible loads. The new model was verified by component-level time-domain simulations. Be cause measured signals in PV systems contain noise, it is important to assess the impact of that noise on the MPPT and design an algorithm that operates effectively in pr esence of noise. For performance assessment of the new MPPT techniques, the efficiencies of various MPPT techniques in presence of noise were compared. This comparison showed superiority of the interpolation MPPT and led to conclusions about effective use of existing MPPT methods. The new MPPT method was also experimentally tested.
Additional file 4 of Translation of the Debriefing Assessment for Simulation in Healthcare in Portuguese and cross-cultural adaptation for Portugal and Brazil
Creators: name: Couto, Thomaz Bittencourt
name: Matos, Francisco Maio
name: de Toledo Rodovalho, Paula Dias
name: Fey, Mary
name: Simon, Robert
name: Muller-Botti, Sacha
Publisher: name: figshare
Year: 2021
Subjects: subject: Medicine
subject: Molecular Biology
subject: Neuroscience
subject: Sociology
subject: FOS: Sociology

description: Additional file 4. Portuguese DASH Rater's Handbook.
Numerical study of energy diffusion in King models
Creators: name: Theuns, Tom
Publisher: name: arXiv
Year: 1995
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: The energy diffusion coefficients D_n(E) (n=1,2) for a system of equal mass particles moving self-consistently in an N-body realisation of a King model are computed from the probability per unit time, P(E, Delta E), that a star with initial energy E will undergo an energy change Delta E. In turn, P is computed from the number of times during the simulation that a particle in a state of given energy undergoes a transition to another state. These particle states are defined directly from the time evolution of E by identifying them with the event occuring between two local maxima in the E(t) curve. If one assumes next that energy changes are uncorrelated between different states, one can use diffusion theory to compute D_n(E). The simulations employ N=512, 2048,... , 32768 particles and are performed using an implementation of Aarseth's direct integrator N-body1 on a massively parallel computer. The more than seven million transitions measured in the largest N simulation provide excellent statistics. The numerically determined D(E)'s are compared against their theoretical counterparts which are computed from phase-space averaged rates of energy change due to independent binary encounters. The overall agreement between them is impressive over most of the energy range, notwithstanding the very different type of approximations involved, giving considerable support to the valid usage of these theoretical expressions to simulate dynamical evolution in Fokker-Planck type calculations.
description: 10 pages, uuencoded .gz.ps, accepted by MNRAS
Control and characterisation of metal oxide/polymer morphologies for hybrid photovoltaic devices
Creators: name: Downing, Jonathan Mark
Publisher: name: Imperial College London
Year: 2013

description: The ready formation of nanostructures, combined with excellent optoelectronic properties has shown zinc oxide (ZnO) to be a promising material for use in photovoltaic devices. Hybrid photovoltaic (h-PV) devices composed of metal oxide-organic pairings are currently limited by ineffective charge transfer between the materials and by poor transport of free charge out of the active layer. Control of interfacial properties, and the structure and morphology of each component is key to device optimisation. In this thesis, ZnO nanorods are paired with the photoactive polymer, poly 3-hexlythiophene (P3HT) with two areas studied: i) nanorod alignment to aid polymer infiltration, and ii) elucidating optimum polymer processing conditions to prepare efficient devices. Aligned nanorods are synthesised from ZnO coated substrates by a hydrothermal method. To understand the influence of ionic additives on morphological control, the addition of potassium chloride (KCl) to growth solutions is investigated. Films have been studied by SEM and XRD, with the correlation of these results (nanorod length, width, density vs (002) diffraction peak area) used to examine alignment, which increases at higher concentrations. This ordering is explained via a geometrical selection argument. Effective polymer infiltration into nanorod arrays is found to be possible by spin coating and annealing above the polymer melting point. Extended annealing (> 60 seconds) is seen to reduce device performance. Small angle X-ray scattering and X-ray diffraction as a function of temperature was conducted to investigate polymer orientation and the kinetics of crystallisation within nanostructured films. These results are combined with device measurements to aid in understanding the relationship between morphological characteristics of the constituent materials and h-PV performance.
Deep Learning with Convolutional Neural Network for Objective Skill Evaluation in Robot-assisted Surgery
Creators: name: Wang, Ziheng
name: Fey, Ann Majewicz
Publisher: name: arXiv
Year: 2018
Subjects: subject: Computer Vision and Pattern Recognition (cs.CV)
subject: Robotics (cs.RO)
subject: FOS: Computer and information sciences

description: With the advent of robot-assisted surgery, the role of data-driven approaches to integrate statistics and machine learning is growing rapidly with prominent interests in objective surgical skill assessment. However, most existing work requires translating robot motion kinematics into intermediate features or gesture segments that are expensive to extract, lack efficiency, and require significant domain-specific knowledge. We propose an analytical deep learning framework for skill assessment in surgical training. A deep convolutional neural network is implemented to map multivariate time series data of the motion kinematics to individual skill levels. We perform experiments on the public minimally invasive surgical robotic dataset, JHU-ISI Gesture and Skill Assessment Working Set (JIGSAWS). Our proposed learning model achieved a competitive accuracy of 92.5%, 95.4%, and 91.3%, in the standard training tasks: Suturing, Needle-passing, and Knot-tying, respectively. Without the need of engineered features or carefully-tuned gesture segmentation, our model can successfully decode skill information from raw motion profiles via end-to-end learning. Meanwhile, the proposed model is able to reliably interpret skills within 1-3 second window, without needing an observation of entire training trial. This study highlights the potentials of deep architectures for an proficient online skill assessment in modern surgical training.
description: Manuscript published. For reference, see https://link.springer.com/article/10.1007/s11548-018-1860-1
title: ADCO, Grènetier de Cîteaux : comptes (1497-1504) (11 H 1172), f. 00682
Creators: name: de la Côte-d'Or, Archives départementales
name: Archives Départementales De La Côte-D'Or
name: Petot, Frédérique
name: Projet CBMA
name: CBMA/CG21/F.PETOT/2019
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: comptes
subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris

description: Grènetier de Cîteaux : comptes (1497-1504), Archives départementales de la Côte-d'Or, (11 H 1172). Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Grènetier de Cîteaux : comptes (1497-1504), Archives départementales de la Côte-d'Or, (11 H 1172), f. 00682, in Projet CBMA - Corpus Burgundiae Medii Aevi \[Ressource en ligne\], https:// manuscrits.cbma-project.eu/
description: Provenance: abbaye de Cîteaux
description: Provenance: http://www.wikidata.org/entity/Q843261
description: Provenance: https://www.geonames.org/3024876
description: Provenance: http://www.idref.fr/030974844/id
description: Provenance: https://catalogue.bnf.fr/ark:/12148/cb12228351v
Picus Linnaeus, 1758, gen. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1758
Subjects: Biodiversity
Taxonomy
Animalia
Chordata
Aves
Piciformes
Picidae
Picus

description: Picus [gen. nov.]
Rostrum polyedrum, rectum: apice cuneato.
Nares pennis setaceis obtectae.
Lingua teres, lumbriciformis, longissima, mucronata, apice retrorsum aculeata setis.
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 112, DOI: 10.5962/bhl.title.542, http://zenodo.org/record/3922206
One machine, one minute, three billion tetrahedra
Creators: name: Marot, Célestin
name: Pellerin, Jeanne
name: Remacle, Jean-François
Publisher: name: arXiv
Year: 2018
Subjects: subject: Computational Geometry (cs.CG)
subject: Graphics (cs.GR)
subject: FOS: Computer and information sciences

description: This paper presents a new scalable parallelization scheme to generate the 3D Delaunay triangulation of a given set of points. Our first contribution is an efficient serial implementation of the incremental Delaunay insertion algorithm. A simple dedicated data structure, an efficient sorting of the points and the optimization of the insertion algorithm have permitted to accelerate reference implementations by a factor three. Our second contribution is a multi-threaded version of the Delaunay kernel that is able to concurrently insert vertices. Moore curve coordinates are used to partition the point set, avoiding heavy synchronization overheads. Conflicts are managed by modifying the partitions with a simple rescaling of the space-filling curve. The performances of our implementation have been measured on three different processors, an Intel core-i7, an Intel Xeon Phi and an AMD EPYC, on which we have been able to compute 3 billion tetrahedra in 53 seconds. This corresponds to a generation rate of over 55 million tetrahedra per second. We finally show how this very efficient parallel Delaunay triangulation can be integrated in a Delaunay refinement mesh generator which takes as input the triangulated surface boundary of the volume to mesh.
A Note on Hyperstructres and Some Applications
Creators: name: B.O. Onasanya
Publisher: name: figshare
Year: 2018
Subjects: Algebra

description: In classical group theory, two elements composed yield another element. This theory, definitely, has limitations in its use in the study of atomic reactions and reproduction in organisms where two elements composed can yield more than one. In this paper, we partly give a review of some properties of hyperstructures with some examples in chemical sciences. On the other hand, we also construct some examples of hyperstructures in genotype, extending the works of Davvaz (2007) to blood genotype. This is to motivate new and collaborative researches in the use of hyperstructures in these related fields.
The Angular Correlation Function of K=19.5 Galaxies and the Detection of a Cluster at z=0.775
Creators: name: Roche, Nathan
name: Eales, Steve
name: Hippelein, Hans
name: Willott, Chris
Publisher: name: arXiv
Year: 1998
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: On five K-band Omega camera images, covering a total of 162.2 sq. arcmin to K=19.5, we investigate (i) the clustering environment of 5 radio galaxies at 0.71.5) redshifts. We also find a significant excess of 1.5--5.0 arcsec separation pairs of galaxies compared to the expectation from the inward extrapolation of omega(theta). To K=19.5, we estimate that 11.0\pm 3.4 per cent of galaxies are in close pairs in excess of omega(theta). This can be explained if the local rate of galaxy mergers and interactions increases with redshift as $\sim (1+z)^m$ with $m=1.33_{-0.51}^{+0.36}$.
description: 14 pages, latex, 8 figures, submitted to MNRAS
Strain-controlled high harmonic generation with Dirac fermions in silicene
Creators: name: Qin, Rui
name: Chen, Zi-Yu
Publisher: name: arXiv
Year: 2018
Subjects: subject: Optics (physics.optics)
subject: FOS: Physical sciences

description: Two-dimensional (2D) materials with zero band gap exhibit remarkable electronic properties with wide tunability. High harmonic generation (HHG) in such materials offers unique platforms to develop novel optoelectronic devices at nanoscale, as well as to investigate strong-field and ultrafast nonlinear behaviour of massless Dirac fermions. However, control of HHG by modulating electronic structure of materials remains largerly unexplored to date. Here we report controllable HHG by tuning the electronic structures via mechanical engineering. Using an \textit{ab initio} approach based on time-dependent density-functional theory (TDDFT), we show that the HHG process is sensitive to the modulation of band structures of monolayer silicene while preserving the Dirac cones under biaxial and uniaxial strains, which can lead to significant enhancement of harmonic intensity up to an order of magnitude. With the additional advantage of silicene in compatibility and integration into the current silicon-based electronic industry, this study may open a new avenue to develop efficient solid-state optoelectronic nano-devices, and provide a valuable tool to understand the strong-field and mechanically induced ultrafast nonlinear response of Dirac carriers in 2D materials.
description: 24pages, 7 figures
Low Mass Companions to T~Tauri Stars: a Mechanism for Rapid-rise FU~Orionis Outbursts
Creators: name: Clarke, Cathie
name: Syer, Dave
Publisher: name: arXiv
Year: 1995
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We show that outside-in disc instabilities, which can produce rapid-\null rise FU Orionis outbursts in T~Tauri systems, are a natural consequence of the existence of protoplanetary protostellar companions. The \pcomp{} would be formed through gravitational instability on a dynamical timescale ($\sim 10^5\y$), and provided it was formed at less than a few \AU{}, it would be swept in to $\sim15\Rsun$ in less than $10^5\y$. A companion of mass $10^{-2}$\Msun at this radius would act as a flood gate which stores material upstream and periodically releases it following the ignition of the thermal ionisation instability.
description: To appear in MNRAS, 5 pages, uuencoded PostScript (figures included) also available at http://www.mpa-garching.mpg.de/~syer/papers/
A Class of Lie-admissible Algebras
Creators: name: Qiuhui Mo
name: Xiangui Zhao
name: Qingnian Pan
Publisher: name: figshare
Year: 2018
Subjects: Algebra

description: In this paper, we study nonassociative algebras which satisfy the following identities: (xy)z = (yx)z,x(yz) = x(zy). These algebras are Lie-admissible algebras.
Additional file 5 of Translation of the Debriefing Assessment for Simulation in Healthcare in Portuguese and cross-cultural adaptation for Portugal and Brazil
Creators: name: Couto, Thomaz Bittencourt
name: Matos, Francisco Maio
name: de Toledo Rodovalho, Paula Dias
name: Fey, Mary
name: Simon, Robert
name: Muller-Botti, Sacha
Publisher: name: figshare
Year: 2021
Subjects: subject: Medicine
subject: Molecular Biology
subject: Neuroscience
subject: Sociology
subject: FOS: Sociology

description: Additional file 5. Different translations of DASH rater, student and instructor version.