cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Additional file 2: of Decision modelling of non-pharmacological interventions for individuals with dementia: a systematic review of methodologies
Creators: name: Sopina, Elizaveta
name: SĂ¸Rensen, Jan
Publisher: name: figshare
Year: 2018
Subjects: subject: Medicine
subject: Physiology
subject: FOS: Biological sciences
subject: Developmental Biology

description: Summary of included studies. (DOCX 48 kb)
Galium tinctorium Linnaeus, 1753, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1753
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Magnoliopsida
Gentianales
Rubiaceae
Galium
Galium tinctorium

description: Galium tinctorium, spec. nov.
5. Galium foliis linearibus: caulinis senis; ramorum quaternis, caule flaccido, pedunculis subbifloris, fructibus glabris.
 Habitat in America septentrionali. Kalm.
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 106, DOI: 10.5281/zenodo.3931989
Intermittency in a single event
Creators: name: Bialas, A.
name: Ziaja, B.
Publisher: name: arXiv
Year: 1996
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: The possibility to study intermittency in a single event of high multiplicity is investigated in the framework of the $α-$model. It is found that, for cascade long enough, the dispersion of intermittency exponents obtained from individual events is fairly small. This fact opens the possibility to study the distribution of the intermittency parameters characterizing the cascades seen (by observing intermittency) in particle spectra.
description: 7 pages, latex, 2 figures available on request by e-mail
Modular architectures for quantum networks
Creators: name: Pirker, A.
name: Wallnöfer, J.
name: Dür, W.
Publisher: name: arXiv
Year: 2017
Subjects: subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: We consider the problem of generating multipartite entangled states in a quantum network upon request. We follow a top-down approach, where the required entanglement is initially present in the network in form of network states shared between network devices, and then manipulated in such a way that the desired target state is generated. This minimizes generation times, and allows for network structures that are in principle independent of physical links. We present a modular and flexible architecture, where a multi-layer network consists of devices of varying complexity, including quantum network routers, switches and clients, that share certain resource states. We concentrate on the generation of graph states among clients, which are resources for numerous distributed quantum tasks. We assume minimal functionality for clients, i.e. they do not participate in the complex and distributed generation process of the target state. We present architectures based on shared multipartite entangled Greenberger-Horne-Zeilinger (GHZ) states of different size, and fully connected decorated graph states respectively. We compare the features of these architectures to an approach that is based on bipartite entanglement, and identify advantages of the multipartite approach in terms of memory requirements and complexity of state manipulation. The architectures can handle parallel requests, and are designed in such a way that the network state can be dynamically extended if new clients or devices join the network. For generation or dynamical extension of the network states, we propose a quantum network configuration protocol, where entanglement purification is used to establish high-fidelity states. The latter also allows one to show that the entanglement generated among clients is private, i.e. the network is secure.
description: replaced with accepted version, 20+4 pages, 28+9 figures
title: ADCO, Cart. 186 (11 H 71), f. 0164v
Creators: name: de la Côte d'Or, Archives départementales
name: CBMA/CG21/F.PETOT/2012
name: Petot, Frédéric
name: Archives Départementales De La Côte-D'Or
name: Petot, Frédérique
name: Projet CBMA
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, t. II (XVe siècle), tome II, Archives départementales de la Côte-d'Or, C
art. 186 (11 H 71). Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Cartulaire général de Cîteaux, dit de Jean de Cirey, t. II (XVe siècle), tome II, Archives départementales de la
 Côte-d'Or, Cart. 186 (11 H 71), f. 0164v, 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
Galium uliginosum Linnaeus, 1753, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1753
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Magnoliopsida
Gentianales
Rubiaceae
Galium
Galium uliginosum

description: Galium uliginosum, spec. nov.
6. Galium foliis senis lanceolatis retrorsum serrato-aculeatis mucronatis rigidis, corollis fructu majoribus.
 Aparine foliis lineari-lanceolatis acuminatis rigidis, corollis fructu majoribus. Roy. lugdb. 255. Fl. svec. 121.
 Aparine minor palustris parisiensis, flore albo. Tournef. inst. 114. Vaill. paris. 14. Fl. lapp.58.
 Habitat in Europae pascuis aquosis sterilibus. ♃
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 106, DOI: 10.5281/zenodo.3931989
Effect of off-diagonal exciton-phonon coupling on intramolecular singlet fission
Creators: name: Huang, Zhongkai
name: Fujihashi, Yuta
name: Zhao, Yang
Publisher: name: arXiv
Year: 2017
Subjects: subject: Chemical Physics (physics.chem-ph)
subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: Intramolecular singlet fission (iSF) materials provide remarkable advantages in terms of tunable electronic structures, and quantum chemistry studies have indicated strong electronic coupling modulation by high frequency phonon modes. In this work, we formulate a microscopic model of iSF with simultaneous diagonal and off-diagonal coupling to high-frequency modes. A non-perturbative treatment, the Dirac-Frenkel time-dependent variational approach is adopted using the multiple Davydov trial states. It is shown that both diagonal and off-diagonal coupling can aid efficient singlet fission if excitonic coupling is weak, and fission is only facilitated by diagonal coupling if excitonic coupling is strong. In the presence of off-diagonal coupling, it is found that high frequency modes create additional fission channels for rapid iSF. Results presented here may help provide guiding principles for design of efficient singlet fission materials by directly tuning singlet-triplet interstate coupling.
Evolution of the Hubble Sequence in Hierarchical Models for Galaxy Formation
Creators: name: Baugh, C. M.
name: Cole, S.
name: Frenk, C. S.
Publisher: name: arXiv
Year: 1996
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present a model for the broad morphological distinction between the disk and spheroidal components of galaxies. Elaborating on the hierarchical clustering scheme of galaxy formation proposed by Cole et al., we assume that galaxies form stars quiescently in a disk until they are disrupted into a spheroidal configuration by mergers. We calculate formation and merging histories, and the evolution in colour, luminosity and morphology of the galaxy populations in different environments. Roughly $ 50\ %$ of ellipticals in our model have undergone a major merger since $z = 0.5$, yet in spite of this we find that cluster ellipticals have colour-magnitude diagrams with remarkably small scatter. The morphological mix of galaxies that become rich cluster members at high redshift is dominated by spiral galaxies, due to the long timescale for galaxy mergers compared with the timescale for cluster assembly at high redshift. The assembly of low redshift clusters is slower, allowing more galaxy mergers to occur in the progenitor halos. As a result $z=0$ rich clusters become E/S0 dominated and we find a ``Butcher-Oemler'' effect that becomes weaker for poorer groups at high redshift. The field luminosity function of red galaxies shows little evolution out to $z\simeq 1$ and the reddest galaxies at these redshifts are as bright as their local counterparts. The blue luminosity function, on the other hand, evolves rapidly with redshift, increasing its characteristic luminosity and becoming steeper at the faint end. These trends are similar to those recently observed in the Canada-France Redshift Survey.
description: Submitted to MNRAS. 20 pages containing 16 figures. Also available as gzipped postscript at ftp://star-ftp.dur.ac.uk/pub/preprints/morph.ps.gz
Galium spurium Linnaeus, 1753, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1753
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Magnoliopsida
Gentianales
Rubiaceae
Galium
Galium spurium

description: Galium spurium, spec. nov.
 7. Galium foliis senis lanceolatis carinatis scabris retrorsum aculeatis, geniculis simplicibus, fructibus glabris. Hort. ups. 28. *
 Aparine semine laeviore. Raj. hist. 484.
 Aparine foliis crebrioribus & semine laeviore. Moris. hist. 3. p.332.
 Habitat in Europae cultis. ☉
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 106, DOI: 10.5281/zenodo.3931989
Superpixels Based Marker Tracking Vs. Hue Thresholding In Rodent Biomechanics Application
Creators: name: Maghsoudi, Omid Haji
name: Tabrizi, Annie Vahedipour
name: Robertson, Benjamin
name: Spence, Andrew
Publisher: name: arXiv
Year: 2017
Subjects: subject: Computer Vision and Pattern Recognition (cs.CV)
subject: FOS: Computer and information sciences

description: Examining locomotion has improved our basic understanding of motor control and aided in treating motor impairment. Mice and rats are premier models of human disease and increasingly the model systems of choice for basic neuroscience. High frame rates (250 Hz) are needed to quantify the kinematics of these running rodents. Manual tracking, especially for multiple markers, becomes time-consuming and impossible for large sample sizes. Therefore, the need for automatic segmentation of these markers has grown in recent years. We propose two methods to segment and track these markers: first, using SLIC superpixels segmentation with a tracker based on position, speed, shape, and color information of the segmented region in the previous frame; second, using a thresholding on hue channel following up with the same tracker. The comparison showed that the SLIC superpixels method was superior because the segmentation was more reliable and based on both color and spatial information.
description: This paper has been accepted for 2017 Asilomar conference, IEEE
Physics of Quark--Gluon Plasma
Creators: name: Smilga, A. V.
Publisher: name: arXiv
Year: 1996
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: In this lecture, we give a brief review of what theorists now know, understand, or guess about static and kinetic properties of quark--gluon plasma. A particular attention is payed to the problem of physical observability, i.e. the physical meaningfulness of various characteristics of $QGP$ discussed in the literature.
description: 35 pages LaTeX, 3 Postscript figures included by epsf.sty are now fixed and printable, uses axodraw.sty included in the package. Some references added and minor stylistic changes made. Lecture at the XXIV ITEP Winter School (Snegiri, February 1996)
Additional file 16: of Local adaptation in European populations affected the genetics of psychiatric disorders and behavioral traits
Creators: name: Polimanti, Renato
name: Kayser, Manfred
name: Gelernter, Joel
Publisher: name: figshare
Year: 2018
Subjects: subject: Medicine
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Evolutionary Biology
subject: 69999 Biological Sciences not elsewhere classified

description: Table S12. Significant associations of rs10932966 with RP11-16P6.1 gene expression in multiple tissues. (DOCX 11 kb)
Galaxy Pairwise Velocity Distributions on Non-Linear Scales
Creators: name: Diaferio, Antonaldo
name: Geller, Margaret J.
Publisher: name: arXiv
Year: 1996
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: The redshift-space correlation function $ξ_s$ for projected galaxy separations $\simless 1h^{-1}$ Mpc can be expressed as the convolution of the real-space correlation function with the galaxy pairwise velocity distribution function (PVDF). An exponential PVDF yields the best fit to the $ξ_s$ measured from galaxy samples of different redshift surveys. We show that this exponential PVDF is not merely a fitting function but arises from well defined gravitational processes. Two ingredients conspire to yield a PVDF with a nearly exponential shape: (i) the number density $n(σ)$ of systems with velocity dispersion $σ$; (ii) the unrelaxed dynamical state of most galaxy systems. The former ingredient determines the exponential tail and the latter the central peak of the PVDF. We compare the $ξ_s$ measured on non-linear scales from galaxy samples of the CfA redshift surveys with different models of the PVDF convolved with the measured real-space correlation function. This preliminary comparison indicates that the agreement between model and observations depends strongly on both the underlying cosmological model and the internal dynamics of galaxy systems. Neither parameter dominates. Moreover, the agreement depends sensitively on the accuracy of the galaxy position and velocity measurements.
description: 28 pages, TeX, to appear in The Astrophysical Journal
How To Find Charm in Nuclear Collisions at RHIC and LHC
Creators: name: Gavin, S.
name: McGaughey, P. L.
name: Ruuskanen, P. V.
name: Vogt, R.
Publisher: name: arXiv
Year: 1996
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: Measurements of dilepton production from charm decay and Drell-Yan processes respectively probe the gluon and sea quark distributions in hadronic collisions. In nucleus-nucleus collisions, these hard scattering processes constitute a `background' to thermal contributions from the hot matter produced by the collision. To determine the magnitude and behavior of this background, we calculate the hard scattering contribution to dilepton production in nuclear collisions at RHIC and LHC at next to leading order in perturbative QCD. Invariant mass, rapidity and transverse momentum distributions are presented. We compare these results to optimistic hydrodynamic estimates of the thermal dilepton production. We find that charm production from hard scattering is by far the dominant contribution. Experiments therefore can measure the gluon distribution in the nuclear target and projectile and, consequently, can provide new information on gluon shadowing. We then illustrate how experimental cuts on the rapidity gap between the leptons can aid in reducing the charm background, thereby enhancing thermal information.
description: 32 pages, latex, 19 figures
Galium saxatile Linnaeus, 1753, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1753
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Magnoliopsida
Gentianales
Rubiaceae
Galium
Galium saxatile

description: Galium saxatile, spec. nov.
8. Galium foliis senis obovatis obtusis, caule ramosissimo procumbente.
 Galium caule ramosissimo, foliis quinis obverse ovatis. Hort. cliff. 34. Roy. lugdb. 257.
 Gallium saxatile supinum, molliore folio. Juss. act. 1714. p.492. t.15.
 Habitat in Hispaniae maritimis lapidosis.
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 106, DOI: 10.5281/zenodo.3931989
Galium minutum Linnaeus, 1753, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1753
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Magnoliopsida
Gentianales
Rubiaceae
Galium
Galium minutum

description: Galium minutum, spec. nov.
9. Galium foliis octonis lanceolatis mucronatis serato-aculeatis glabris incurvis.
 Galium foliis senis cuneiformi-lanceolatis mucronatis glabris. Hort. ups. 28. *
 Gallium saxatile minimum supinum & pumilum, flore luteo. Tournef. inst. 1152.
 Habitat in imperio Ruthenico . ♃
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 106, DOI: 10.5281/zenodo.3931989
Galium pusillum Linnaeus, 1753, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1753
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Magnoliopsida
Gentianales
Rubiaceae
Galium
Galium pusillum

description: Galium pusillum, spec. nov.
10. Galium foliis octonis hispidis linearibus acuminaris subimbricatis, pedunculis dichotomis.
 Rubeola saxatilis. Bauh. pin. 334. prodr. 145.
 Habitat in montibus Galloprovinciae .
 Caules numerosi, digitales, angulati; Folia verticillata foliolis 8. s.6, lanceolato-linearibus vel linearibus, acutis, uti caulis undique pilis patentibus hispida. Rami rariores, alterni; Foliorum verticilli saepe ita conferti, ut folia imbricatim digesta conspiciantur. Panicula rarior, fere terminalis ex pedunculis bis dichotomis.
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 pages 106-107, DOI: 10.5281/zenodo.3931989
Precessional dynamics of black hole triples: binary mergers with near-zero effective spin
Creators: name: Antonini, Fabio
name: Rodriguez, Carl L.
name: Petrovich, Cristobal
name: Fischer, Caitlin L.
Publisher: name: arXiv
Year: 2017
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: The binary black hole mergers detected by Advanced LIGO/Virgo have shown no evidence of large black hole spins. However, because LIGO/Virgo best measures the effective combination of the two spins along the orbital angular momentum ($χ_{\rm eff}$), it is difficult to distinguish between binaries with slowly-spinning black holes and binaries with spins lying in the orbital plane. Here, we study the spin dynamics for binaries with a distant black hole companion. For spins initially aligned with the orbital angular momentum of the binary, we find that $χ_{\rm eff}$ "freezes" near zero as the orbit decays through the emission of gravitational waves. Through a population study, we show that this process predominantly leads to merging black hole binaries with near-zero $χ_{\rm eff}$. We conclude that if the detected black hole binaries were formed in triples, then this would explain their low $χ_{\rm eff}$ without the need to invoke near-zero spins or initially large spin-orbit angles.
description: 6 pages, 4 figure. Letter accepted for publication in MNRAS
Flat optical conductivity in ZrSiS due to two-dimensional Dirac bands
Creators: name: Schilling, M. B.
name: Schoop, L. M.
name: Lotsch, B. V.
name: Dressel, M.
name: Pronin, A. V.
Publisher: name: arXiv
Year: 2017
Subjects: subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: Materials Science (cond-mat.mtrl-sci)
subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: FOS: Physical sciences

description: ZrSiS exhibits a frequency-independent interband conductivity $σ(ω) = \rm{const}(ω) \equiv σ_{\rm{flat}}$ in a broad range from 250 to 2500 cm$^{-1}$ (30 - 300 meV). This makes ZrSiS similar to (quasi)two-dimensional Dirac electron systems, such as graphite and graphene. We assign the flat optical conductivity to the transitions between quasi-two-dimensional Dirac bands near the Fermi level. In contrast to graphene, $σ_{\rm{flat}}$ is not supposed to be universal but related to the length of the nodal line in the reciprocal space, $k_{0}$. When $σ_{\rm{flat}}$ and $k_{0}$ are connected by a simple model, we find good agreement between experiment and theory. Due to the spin-orbit coupling, the discussed Dirac bands in ZrSiS possess a small gap $Δ$, for which we determine an upper bound max($Δ$) = 30 meV from our optical measurements. At low temperatures the momentum-relaxation rate collapses, and the characteristic length scale of momentum relaxation is of the order of microns below 50 K.
description: 5 pages
The Jacobi orientation and the two-variable elliptic genus
Creators: name: Ando, Matthew
name: French, Christopher P.
name: Ganter, Nora
Publisher: name: arXiv
Year: 2006
Subjects: subject: Algebraic Topology (math.AT)
subject: Algebraic Geometry (math.AG)
subject: FOS: Mathematics
subject: 55N34

description: We explain the relationship between the sigma orientation and Witten genus on the one hand and the two-variable elliptic genus on the other. We show that if E is an elliptic spectrum, then the Theorem of the Cube implies the existence of canonical SU-orientation of the associated spectrum of Jacobi forms. In the case of the elliptic spectrum associated to the Tate curve, this gives the two-variable elliptic genus. We also show that the two-variable genus arises as an instance of the circle-equivariant sigma orientation.
description: Revised to better exhibit complex orientation of MSU^(CP^\infty_{-infty})
3D magneto-hydrodynamic models of non-thermal photon emission in the binary system $γ^2$ Velorum
Creators: name: Reitberger, K.
name: Kissmann, R.
name: Reimer, A.
name: Reimer, O.
Publisher: name: arXiv
Year: 2017
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: Recent reports claiming association of the massive star binary system $γ^2 $Velorum (WR 11) with a high-energy $γ$-ray source observed by \textit{Fermi}-LAT contrast the so-far exclusive role of $η$ Carinae as the hitherto only detected $γ$-ray emitter in the source class of particle-accelerating colliding-wind binary (CWB) systems. We offer support to this claim of association by providing dedicated model predictions for the nonthermal photon emission spectrum of $γ^2$ Velorum. We use three-dimensional magneto-hydrodynamic modeling (MHD) to investigate the structure and conditions of the wind-collision region (WCR) of $γ^2$ Velorum including the important effect of radiative braking in the stellar winds. A transport equation is then solved throughout the computational domain to study the propagation of relativistic electrons and protons. The resulting distributions of particles are subsequently used to compute nonthermal photon emission components. In agreement with observation in X-ray spectroscopy, our simulations yield a large shock-cone opening angle. We find the nonthermal $γ$-ray emission of $γ^2$ Velorum to be of hadronic origin owing to the strong radiation fields in the binary system which inhibit the acceleration of electrons to energies sufficiently high for efficient inverse Compton radiation. We also discuss the strong dependence of a hadronic $γ$-ray component on the energy-dependent diffusion used in the simulations. Of two mass-loss rates for the WR star found in literature, only the higher one is able to accommodate the observed $γ$-ray spectrum with reasonable values for important simulation parameters such as the injection ratio of high-energy particles within the WCR.
description: accepted for publication by The Astrophysical Journal
Additional file 1: of Decision modelling of non-pharmacological interventions for individuals with dementia: a systematic review of methodologies
Creators: name: Sopina, Elizaveta
name: SĂ¸Rensen, Jan
Publisher: name: figshare
Year: 2018
Subjects: subject: Medicine
subject: Sociology
subject: FOS: Sociology
subject: Developmental Biology

description: Search strategies. (DOCX 20 kb)
Galium verum Linnaeus, 1753, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1753
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Magnoliopsida
Gentianales
Rubiaceae
Galium
Galium verum

description: Galium verum, spec. nov.
 11. Galium foliis octonis linearibus sulcatis, ramis floriferis brevibus. Hort. cliff. 34. Fl. svec. 116. Mat. med. 46. Roy. lugdb. 256.
 Galium caule erecto, foliis plurimis verticillatis linearibus. Fl. lapp.61.
 Gallium luteum. Bauh. pin. 335.
 Habitat in Europa frequens. ♃
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 107, DOI: 10.5281/zenodo.3931989
Cortázar "Das besetzte Haus/ Erzählungen"
Creators: name: Walter, Boehlich
name: Boehlich, Walter
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2021
Subjects: Literatura argentina
"Bestiario"
"Casa tomada"

description: Anuncio de un programa de la radio-televisión Hessischer Rundfunk sobre "Casa tomada".
description: Notas: Sello "Für den Autor" ("Para el Autor") en la parte inferior izquierda de la primera página.
description: Source: Num.Ref. : JC-CAR-07.024
description: Source: Localización del archivo: Centre de Recherches Latino-Américaines (CRLA–Archivos, ITEM UMR8132). MSHS - Bât. A5, 1er étage 5 rue Théodore Lefebvre - TSA21103. 86073 Poitiers cedex 9.
title: ADCO, Cartulaire des Dominicains de Dijon (1286), Cart. 221 (H 53), 170 folios, f. 0168
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: Corpus Burgundiae Medii Aevi
subject: Chartes de la Bourgogne du Moyen Âge
subject: cartulaire
subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris

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. 0168, in Projet CBMA - Corpus Burgundiae Medii Aevi [Ressource en ligne], https:// manuscrits.cbma-project.eu/
description: Provenance: http://www.idref.fr/02643413X/id
description: Provenance: https://www.geonames.org/6453767
description: Provenance: Dijon
description: Provenance: http://www.wikidata.org/entity/Q7003
description: Provenance: https://catalogue.bnf.fr/ark:/12148/cb15250518p
Galium mollugo Linnaeus, 1753, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1753
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Magnoliopsida
Gentianales
Rubiaceae
Galium
Galium mollugo

description: Galium mollugo, spec. nov.
12. Galium foliis octonis ovatis linearibus subserratis patentissimis mucronatis, caule flaccido, ramis patentibus.
 Galium foliis pluribus acutis, caule flaccido, ramis patentissimis. Hort. cliff. 34. Roy. lugdb. 257. Fl. svec. 117.
 Mollugo montana latifolia ramosa. Bauh. pin. 334.
 Rubia sylvestris laevis. Bauh. pin. 333.
 Mollugo belgarum. Lob. ic. 802.
 Habitat in Europa mediterranea. ♃
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 107, DOI: 10.5281/zenodo.3931989
The Nuclear Level Density and the Determination of Thermonuclear Rates for Astrophysics
Creators: name: Rauscher, T.
name: Thielemann, F. -K.
name: Kratz, K. -L.
Publisher: name: arXiv
Year: 1996
Subjects: subject: Astrophysics (astro-ph)
subject: Nuclear Theory (nucl-th)
subject: FOS: Physical sciences

description: The prediction of cross sections for nuclei far off stability is crucial in the field of nuclear astrophysics. In recent calculations the nuclear level density -- as an important ingredient to the statistical model (Hauser-Feshbach) -- has shown the highest uncertainties. We present a global parametrization of nuclear level densities based on the back-shifted Fermi-Gas formalism. Employment of an energy-dependent level density parameter $a$ and microscopic corrections from a recent FRDM mass formula by Möller et al.\ leads to a highly improved fit of level densities at the neutron-separation energy in the mass range $20\le A \le 245$. The importance of using proper microscopic corrections from mass formulae is emphasized. The resulting level description is well suited for astrophysical applications. The level density can also provide clues to the applicability of the statistical model which is only correct for a high density of excited states. Using the above description one can derive a ``map'' for the applicability of the model for reactions of stable and unstable nuclei with neutral and charged particles.
description: 12 pages, 4 Postcript figures, uses memsait.sty; preprint also available at http://quasar.physik.unibas.ch/ . to appear in Memorie della Societa Astronomica Italiana
Is Zee Model The Model of Neutrino Masses?
Creators: name: Smirnov, Alexei Yu.
name: Tanimoto, Morimitsu
Publisher: name: arXiv
Year: 1996
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: Zee model leads naturally to two heavy, strongly degenerate and almost maximally mixed neutrinos and to one light neutrino with small mixing. This pattern coincides with the one needed for a solution of the atmospheric neutrino problem by $\n_\m\A \n_τ$ oscillations and for existence of the two component hot dark matter in the Universe. Furthermore, the oscillations $\bar\n_\m\A \bar\n_e$ can be in the range of sensitivity of KARMEN, LSND experiments. Phenomenology of this scenario is considered and possibility to check it in the forthcoming experiments is discussed. Scenario implies large values and inverse flavour hierarchy of the couplings of the Zee boson with fermions: $f_{e τ} \ll f_{μτ} \leq f_{e μ} \sim 0.1$. Main signatures of scenario are: strongly suppressed signal of $\n_\m\A \n_τ$ oscillation in CHORUS and NOMAD experiments, so that positive result from these experiments will rule out the scenario; possibility of observation of $\n_e\A \n_τ$ oscillations by CHORUS and NOMAD; corrections to the muon decay, neutrino-electron scattering at the level of the experimental errors; branching ratio $B(μ\A e γ)$ bigger than $10^{-13}$. The solar neutrino problem can be solved by introduction of additional very light singlet fermion without appreciable changes of the active neutrino pattern.
description: 19 pages, latex, 6 figures available upon request from the author by fax
Galium glaucum Linnaeus, 1753, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1753
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Magnoliopsida
Gentianales
Rubiaceae
Galium
Galium glaucum

description: Galium glaucum, spec. nov.
 13. Galium foliis verticillatis linearibus, pedunculis dichotomis summo caule floriferis. Roy. lugdb. 256. Hort. ups. 27. Sauv. monsp. 161.
 Gallium saxatile, glauco folio. Bocc. mus. 2. p.172. t.116.
 Rubia montana angustifolia. Bauh. pin. 333. prodr. 145.
 Habitat in Tataria , Helvetia , Austria , Monspelii . ♃
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 107, DOI: 10.5281/zenodo.3931989
Ages of galaxy bulges and disks from optical and near-infrared colors
Creators: name: Peletier, R. F.
name: Balcells, M.
Publisher: name: arXiv
Year: 1996
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We compare optical and near-infrared colors of disks and bulges in a diameter-limited sample of inclined, bright, nearby, early-type spirals. Color profiles along wedge apertures at 15 degree from the major axis and on the minor axis on the side of the galaxy opposite to the dust lane are used to assign nominal colors for the inner disks (at 2 scale length) and for the bulges (~ 0.5 r_eff), respectively. We estimate that the effects of dust reddening and the cross-talk between the colors of the two components is negligible. We find that color differences (bulge -- disk) are very small: Delta(U-R)=0.126 +/- 0.165, Delta(R-K)=0.078 +/- 0.165. Disks tend to be bluer by an amount three times smaller than that reported by Bothun & Gregg (1990) for S0's. Color variations from galaxy to galaxy are much larger than color differences between disk and bulge in each galaxy. Probably, the underlying old population of disks and bulges is much more similar than the population paradigm would lead us to believe. Implied age differences, assuming identical metallicities, are less than 30%.
description: 12 pages, latex, including 3 figures (Fig. 1 missing). Fig. 1 can be obtained at ftp://iac.es/pub/rpelet/preprints/buldiskfig1.ps.gz Astronomical Journal, in press
Extensions of interpolation between the arithmetic-geometric mean inequality for matrices
Creators: name: Bakherad, Mojtaba
name: Lashkaripour, Rahmatollah
name: Hajmohamadi, Monire
Publisher: name: arXiv
Year: 2017
Subjects: subject: Functional Analysis (math.FA)
subject: Operator Algebras (math.OA)
subject: FOS: Mathematics

description: In this paper, we present some extensions of interpolation between the arithmetic-geometric means inequality. Among other inequalities, it is shown that if $A, B, X$ are $n\times n$ matrices, then \begin{align*} \|AXB^*\|^2\leq\|f_1(A^*A)Xg_1(B^*B)\|\,\|f_2(A^*A)Xg_2(B^*B)\|, \end{align*} where $f_1,f_2,g_1,g_2$ are non-negative continues functions such that $f_1(t)f_2(t)=t$ and $g_1(t)g_2(t)=t\,\,(t\geq0)$. We also obtain the inequality \begin{align*} \left|\left|\left|AB^*\right|\right|\right|^2\nonumber&\leq \left|\left|\left|p(A^*A)^{\frac{m}{p}}+ (1-p)(B^*B)^{\frac{s}{1-p}}\right|\right|\right|\,\left|\left|\left|(1-p)(A^*A)^{\frac{n}{1-p}}+ p(B^*B)^{\frac{t}{p}}\right|\right|\right|, \end{align*} in which $m,n,s,t$ are real numbers such that $m+n=s+t=1$, $|||\cdot|||$ is an arbitrary unitarily invariant norm and $p\in[0,1]$.
description: J. Inequal. Appl. 2017
title: ADCO, Sixième cartulaire de Saint-Étienne de Dijon (1662), Cart. 30 (G 133), 441 folios, f. 754
Creators: name: de la Côte d'Or, Archives départementales
name: Archives Départementales De La Côte-D'Or
name: Petot, Frédérique
name: Projet CBMA
name: CG21/F.PETOT/2012
name: Petot, Frédéric
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2020
Subjects: subject: Chartes de la Bourgogne du Moyen Âge
subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris
subject: cartulaire
subject: Corpus Burgundiae Medii Aevi

description: Sixième cartulaire de Saint-Étienne de Dijon (1662), Archives départementales de la Côte-d'Or, Cart. 30 (G 133), 441 folios, f. 754, Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Sixième cartulaire de Saint-Étienne de Dijon (1662), Archives départementales de la Côte-d'Or, Cart. 30 (G 133), 441 folios, f. 754, in Projet CBMA - Corpus Burgundiae Medii Aevi [Ressource en ligne], https://manuscrits.cbma-project.eu/
description: Provenance: abbaye Saint-Étienne de Dijon
description: Provenance: http://www.wikidata.org/entity/Q15945019
Additional file 5: of The effect of Kenyaâ s free maternal health care policy on the utilization of health facility delivery services and maternal and neonatal mortality in public health facilities
Creators: name: C. Gitobu
name: P. Gichangi
name: W. Mwanda
Publisher: name: figshare
Year: 2018
Subjects: subject: Medicine
subject: Biotechnology
subject: Sociology
subject: FOS: Sociology
subject: 19999 Mathematical Sciences not elsewhere classified
subject: FOS: Mathematics
subject: Developmental Biology
subject: Cancer
subject: Computational Biology

description: Fitness of maternal mortality ratio model. This additional file is derived from an analysis of the mean absolute percentage error (MAPE) of neonatal mortality rate in all the 77 health facilities. (DOCX 13Â kb)
Squeezed States and Particle Production in High Energy Collisions
Creators: name: Bambah, Bindu A.
Publisher: name: arXiv
Year: 1996
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: Using the `quantum optical approach' we propose a model of multiplicity distributions in high energy collisions based on squeezed coherent states. We show that the k-mode squeezed coherent state is the most general one in describing hadronic mulitiplicity distributions in particle collision processes, describing not only $p \bar p$ collisions but $e^{+}e^{-}$, $νp$ and diffractive collisions as well. The reason for this phenomenological fit has been gained by working out a microscopic theory in which the squeezed coherent sources arise naturally if one considers the Lorentz squeezing of hadrons and works in the covariant phase space formalism .
description: 7 pages, 4 Figures (can be obtained from author by snail mail)
Superpixel Based Segmentation and Classification of Polyps in Wireless Capsule Endoscopy
Creators: name: Maghsoudi, Omid Haji
Publisher: name: arXiv
Year: 2017
Subjects: subject: Computer Vision and Pattern Recognition (cs.CV)
subject: FOS: Computer and information sciences

description: Wireless Capsule Endoscopy (WCE) is a relatively new technology to record the entire GI trace, in vivo. The large amounts of frames captured during an examination cause difficulties for physicians to review all these frames. The need for reducing the reviewing time using some intelligent methods has been a challenge. Polyps are considered as growing tissues on the surface of intestinal tract not inside of an organ. Most polyps are not cancerous, but if one becomes larger than a centimeter, it can turn into cancer by great chance. The WCE frames provide the early stage possibility for detection of polyps. Here, the application of simple linear iterative clustering (SLIC) superpixel for segmentation of polyps in WCE frames is evaluated. Different SLIC superpixel numbers are examined to find the highest sensitivity for detection of polyps. The SLIC superpixel segmentation is promising to improve the results of previous studies. Finally, the superpixels were classified using a support vector machine (SVM) by extracting some texture and color features. The classification results showed a sensitivity of 91%.
description: This paper has been published in SPMB 2017
Galium purpureum Linnaeus, 1753, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1753
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Magnoliopsida
Gentianales
Rubiaceae
Galium
Galium purpureum

description: Galium purpureum, spec. nov.
 14. Galium foliis verticillatis lineari-setaceis pedunculis folio longioribus. Hort. cliff. 34. Roy. lugdb. 256.
 Gallium nigropurpureum montanum tenuifolium. Col. ecphr. 1. p.298. Bauh. pin. 335.
 Habitat in Italia .
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 107, DOI: 10.5281/zenodo.3931989
Wind accretion in binary stars II. Accretion rates
Creators: name: Theuns, Tom
name: Boffin, Henri
name: Jorissen, Alain
Publisher: name: arXiv
Year: 1996
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Smoothed particle hydrodynamics (SPH) is used to estimate accretion rates of mass, linear and angular momentum in a binary system where one component undergoes mass loss through a wind. Physical parameters are chosen such as to model the alleged binary precursors of barium stars, whose chemical peculiarities are believed to result from the accretion of the wind from a companion formerly on the asymptotic giant branch (AGB). The binary system modelled consists of a 3 solar masses AGB star on the main sequence, in a 3AU circular orbit. Three-dimensional simulations are performed for gases with polytropic indices gamma=1, 1.1 and 1.5, to bracket more realistic situations that would include radiative cooling. Mass accretion rates are found to depend on resolution and we estimate typical values of 1-2% for the gamma=1.5 case and 8% for the other models. The highest resolution obtained (with 400k particles) corresponds to an accretor of linear size 16 solar radii. Despite being (in the gamma = 1.5 case) about ten times smaller than theoretical estimates based on the Bondi-Hoyle prescription, the SPH accretion rates remain large enough to explain the pollution of barium stars. Uncertainties in the current SPH rates remain however, due to the simplified treatment of the wind acceleration mechanism, as well as to the absence of any cooling prescription and to the limited numerical resolution. Angular momentum transfer leads to significant spin up of the accretor and can account for the rapid rotation of HD165141, a barium star with a young white dwarf companion and a rotation rate unusually large among K giants.
description: 13 pages, mn style, 5 figures, to be published by MNRAS
Testing Modified Gravity Theories via Wide Binaries and GAIA
Creators: name: Pittordis, Charalambos
name: Sutherland, Will
Publisher: name: arXiv
Year: 2017
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: The standard LambdaCDM model based on General Relativity (GR) including cold dark matter (CDM) is very successful at fitting cosmological observations, but recent non-detections of candidate dark matter (DM) particles mean that various modified-gravity theories remain of significant interest. The latter generally involve modifications to GR below a critical acceleration scale $\sim 10^{-10} \, m \, s^{-2}$. Wide-binary (WB) star systems with separations $> 5 \, kAU$ provide an interesting test for modified gravity, due to being in or near the low-acceleration regime and presumably containing negligible DM. Here, we explore the prospects for new observations pending from the GAIA spacecraft to provide tests of GR against MOND or TeVes-like theories in a regime only partially explored to date. In particular, we find that a histogram of (3D) binary relative velocities against circular velocity predicted from the (2D) projected separations predicts a rather sharp feature in this distribution for standard gravity, with an 80th (90th) percentile value close to 1.025 (1.14) with rather weak dependence on the eccentricity distribution. However, MOND/TeVeS theories produce a shifted distribution, with a significant increase in these upper percentiles. In MOND-like theories {\em without} an external field effect, there are large shifts of order unity. With the external field effect included, the shifts are considerably reduced to $\sim 0.04 - 0.08$, but are still potentially detectable statistically given reasonably large samples and good control of contaminants. In principle, followup of GAIA-selected wide binaries with ground-based radial velocities accurate to < 0.03 km/s should be able to produce an interesting new constraint on modified-gravity theories.
description: LaTeX, 20 pages, 17 figures. v2 is author-produced version as accepted by MNRAS; results similar to v1, moderate clarifications
The search and investigation of the Large Groups of Quasars
Creators: name: Komberg, Boris V.
name: Kravtsov, Andrey V.
name: Lukash, Vladimir N.
Publisher: name: arXiv
Year: 1996
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Recently, it was suggested that large concentrations or groups of quasars may trace sites of enhanced matter density at medium and high redshifts analogous to how galaxy clusters trace them in nearby space. We have checked existing quasar data for the presence of such groups. Large Quasar Groups (LQGs) were identified using a well-known cluster analysis technique. Our final list consists of 12 groups, including one reported previously. Most of the quasars in these groups come from deep homogeneous surveys. We have found that: (i) the probability that the detected groups are random is rather small (generally a few per cent); (ii) their sizes range from $\sim 70$ to $\sim 160h^{-1} Mpc$, which is comparable to sizes of nearby rich superclusters; (iii) the detected groups all have redshifts $0.5
description: 11 pages, 2 tables, uses mn.sty, also available at http://charon.nmsu.edu/~akravtso/publications.html , accepted for publication in MNRAS
Convergence rates of solutions for a two-species chemotaxis-Navier-Stokes sytstem with competitive kinetics
Creators: name: Jin, Hai-Yang
name: Xiang, Tian
Publisher: name: arXiv
Year: 2017
Subjects: subject: Analysis of PDEs (math.AP)
subject: FOS: Mathematics
subject: 35B40, 35K47, 35K55

description: In this paper, we study the rates of convergence of supposedly given global bounded classical solutions to a two-species chemotaxis-Navier-Stokes system with Lotka-Volterra competitive kinetics. Except in one case where the rate of convergence for the fluid component is expressed in terms of the Poincare constant and the model parameters, all other rates of convergence are shown to be expressible only in terms of the model parameters and the underlying space dimension.
description: 16 pages, submitted