cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Silene quadrifida Linnaeus 1759
Creators: name: Jarvis, Charlie
Publisher: name: Linnaean Society of London in association with the Natural History Museum
Year: 2007
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Magnoliopsida
Caryophyllales
Caryophyllaceae
Silene
Silene quadrifida

description: Silene quadrifida (Linnaeus) Linnaeus, Systema Naturae, ed. 10, 2: 1032. 1759.
["Habitat in Styriae monte ad oppidum Eisenertz."] Sp. Pl. 1: 415 (1753). RCN: 3268.
 Basionym: Cucubalus quadrifidus L. (1753).
 Lectotype (Melzheimer & Polatschek in Phyton (Horn) 31: 285. 1992): [icon] "Caryophyllus minimus humilis alter exoticus flore candido amoeno" in Plantin, Pl. Stirp. Icon.: 445. 1581.
 Current name:  Silene quadrifida  (L.) L. (Caryophyllaceae).
description: Published as part of Jarvis, Charlie, 2007, Chapter 7: Linnaean Plant Names and their Types (part S), pp. 806-877 in Order out of Chaos. Linnaean Plant Types and their Types, London :Linnaean Society of London in association with the Natural History Museum on page 852, DOI: 10.5281/zenodo.291971
Spot distribution and fast surface evolution on Vega
Creators: name: Petit, P.
name: Hébrard, E. M.
name: Böhm, T.
name: Folsom, C. P.
name: Lignières, F.
Publisher: name: arXiv
Year: 2017
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: Spectral signatures of surface spots were recently discovered from high cadence observations of the A star Vega. We aim at constraining the surface distribution of these photospheric inhomogeneities, and investigating a possible short term evolution of the spot pattern. Using data collected over five consecutive nights, we employ the Doppler Imaging method to reconstruct three different maps of the stellar surface, from three consecutive subsets of the whole time-series. The surface maps display a complex distribution of dark and bright spots, covering most of the visible fraction of the stellar surface. A number of surface features are consistently recovered in all three maps, but other features seem to evolve over the time span of observations, suggesting that fast changes can affect the surface of Vega within a few days at most. The short-term evolution is observed as emergence or disappearance of individual spots, and may also show up as zonal flows, with low-latitude and high latitude belts rotating faster than intermediate latitudes. It is tempting to relate the surface brightness activity to the complex magnetic field topology previously reconstructed for Vega, although strictly simultaneous brightness and magnetic maps will be necessary to assess this potential link.
description: MNRAS Letters, in press
Additional file 4: of Including gene networks to predict calving difficulty in Holstein, Brown Swiss and Jersey cattle
Creators: name: Tiezzi, Francesco
name: Arceo, Maria
name: Cole, John
name: Maltecca, Christian
Publisher: name: figshare
Year: 2018
Subjects: subject: Microbiology
subject: FOS: Biological sciences
subject: Cell Biology
subject: Genetics
subject: Molecular Biology
subject: Physiology
subject: 69999 Biological Sciences not elsewhere classified
subject: 80699 Information Systems not elsewhere classified
subject: FOS: Computer and information sciences
subject: 19999 Mathematical Sciences not elsewhere classified
subject: FOS: Mathematics
subject: Developmental Biology
subject: Hematology
subject: 110309 Infectious Diseases
subject: FOS: Health sciences
subject: 60506 Virology
subject: Computational Biology

description: Figure S4. Network diagrams for HO, BS and JE respectively. Green dots correspond to genes enriching significant GO terms. Red dots correspond to genes enriching significant GO terms and located within dystocia QTLs. Blue dots correspond to the remaining of the genes highly correlated among them (rxy|z ≥ 0.98). Yellow circles correspond to the most connected genes within dystocia QTL (see Table 3). (PDF 819 kb)
Driven-dissipative, non-equilibrium Bose-Einstein condensation of just a few photons
Creators: name: Walker, Benjamin T.
name: Flatten, Lucas C.
name: Hesten, Henry J.
name: Mintert, Florian
name: Hunger, David
name: Trichet, Aurélien A. P.
name: Smith, Jason M.
name: Nyman, Robert A.
Publisher: name: arXiv
Year: 2017
Subjects: subject: Quantum Physics (quant-ph)
subject: Quantum Gases (cond-mat.quant-gas)
subject: Statistical Mechanics (cond-mat.stat-mech)
subject: FOS: Physical sciences

description: Coherence is a defining feature of quantum condensates. These condensates are inherently multimode phenomena and in the macroscopic limit it becomes extremely difficult to resolve populations of individual modes and the coherence between them. In this work we demonstrate non-equilibrium Bose-Einstein condensation (BEC) of photons in a sculpted dye-filled microcavity, where threshold is found for $8\pm 2$ photons. With this nanocondensate we are able to measure occupancies and coherences of individual energy levels of the bosonic field. Coherence of individual modes generally increases with increasing photon number, but at the breakdown of thermal equilibrium we observe multimode-condensation phase transitions wherein coherence unexpectedly decreases with increasing population, suggesting that the photons show strong inter-mode phase or number correlations despite the absence of a direct nonlinearity. Experiments are well-matched to a detailed non-equilibrium model. We find that microlaser and Bose-Einstein statistics each describe complementary parts of our data and are limits of our model in appropriate regimes, which informs the debate on the differences between the two.
The Cosmic Evolution Survey (COSMOS): Subaru Observations of the HST COSMOS Field
Creators: name: Taniguchi, Y.
name: Scoville, N.
name: Murayama, T.
name: Sanders, D. B.
name: Mobasher, B.
name: Aussel, H.
name: Capak, P.
name: Ajiki, M.
name: Miyazaki, S.
name: Komiyama, Y.
name: Shioya, Y.
name: Nagao, T.
name: Sasaki, S. S.
name: Koda, J.
name: Carilli, C.
name: Giavalisco, M.
name: Guzzo, L.
name: Hasinger, G.
name: Impey, C.
name: LeFevre, O.
name: Lilly, S.
name: Renzini, A.
name: Rich, M.
name: Schinnerer, E.
name: Shopbell, P.
name: Kaifu, N.
name: Karoji, H.
name: Arimoto, N.
name: Okamura, S.
name: Ohta, K.
Publisher: name: arXiv
Year: 2006
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present deep optical imaging observations of 2 square degree area, covered by the Cosmic Evolution Survey (COSMOS), made by the prime-focus Camera (Supreme-Cam) on the 8.2m Subaru Telescope. Observations were done in six broad-band [B (4459.7 AA), g' (4723.1 AA), V (5483.8 AA), r' (6213.0 AA), i' (7640.8 AA), z' (8855.0 AA)], and one narrow-band (NB816) filters. A total of 10^6 galaxies were detected to i'~26.5 mag. These data, combined with observations at u* and K-band are used to construct the photometric catalogs for the COSMOS and to measure their photometric redshifts, multi-band spectral energy distributions, stellar masses and identification of high redshift candidates. This catalog provides multi-waveband data for scientific analysis of the COSMOS survey.
description: 46 pages, 32 figures, accepted for the COSMOS special issue of ApJS
Entretien auprès de Kamal Al-Sharif, natif de Mafraq, à propos de la rue Ali Abdiyeh depuis les années 1960
Creators: name: Al-Sharif, Kamal
name: Anass Al-Amush (Enquêteur)
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2020

description: Source: http://www.calames.abes.fr/pub/ms/FileId-3139
description: Coverage: Mafraq, Jordanie
Photon helicity in Lambda_b --> p K gamma decays
Creators: name: Legger, Federica
name: Schietinger, Thomas
Publisher: name: arXiv
Year: 2006
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: Radiative decays of polarized Lambda_b baryons represent an attractive possibility to measure the helicity of the photon emitted in the b --> s gamma quark transition and thus to subject the Standard Model to a stringent test at existing and future hadron colliders. The most abundant mode, Lambda(1116) gamma, is experimentally very challenging because of the long decay length of the Lambda(1116). We show that the experimentally more accessible Lambda_b --> p K gamma decays proceeding via Lambda resonances may be used to extract the photon helicity for sufficient Lambda_b polarization, if the resonance spin does not exceed 3/2. A direct comparison of the potential of such resonance decays to assess the photon polarization at a hadron collider with respect to the decay to Lambda(1116) is given.
description: elsart, 17 pages, 4 figures; corrected sensitivity estimates
Thermodynamics of strongly interacting matter in a hybrid model
Creators: name: Bhattacharyya, Abhijit
name: Ghosh, Sanjay K.
name: Maity, Soumitra
name: Raha, Sibaji
name: Ray, Rajarshi
name: Saha, Kinkar
name: Samanta, Subhasis
name: Upadhaya, Sudipa
Publisher: name: arXiv
Year: 2017
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: The equation of state and fluctuations of conserved charges in a strongly interacting medium under equilibrium conditions form the baseline upon which various possible scenarios in relativistic heavy-ion collision experiments are built. Many of these quantities have been obtained in the lattice QCD framework with reliable continuum extrapolations. Recently the Polyakov$-$Nambu$-$Jona-Lasinio model has been reparametrized to some extent to reproduce quantitatively the lattice QCD equation of state at vanishing chemical potentials. The agreement was precise except at low temperatures, possibly due to inadequate representation of the hadronic degrees of freedom in the model. This disagreement was also observed for some of the fluctuation and correlations considered. Here we address this issue by introducing the effects of hadrons through the Hadron Resonance Gas model. The total thermodynamic potential is now a weighted sum of the thermodynamic potential of the Polyakov$-$Nambu$-$Jona-Lasinio model and that of the Hadron Resonance Gas model. We find that the equation of state and the fluctuations and correlations obtained in this hybrid model agrees satisfactorily with the lattice QCD data in the low temperature regime.
description: 17 pages, 10 figures. arXiv admin note: text overlap with arXiv:1609.07882
Silene gallica Linnaeus 1753
Creators: name: Jarvis, Charlie
Publisher: name: Linnaean Society of London in association with the Natural History Museum
Year: 2007
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Magnoliopsida
Caryophyllales
Caryophyllaceae
Silene
Silene gallica

description: Silene quinquevulnera Linnaeus, Species Plantarum 1: 416. 1753, nom. rej.
"Habitat in Hispania, Lusatia, Italia, Gallia." RCN: 3240.
 Lectotype (Talavera & Muñoz Garmendia in Anales Jard. Bot. Madrid 45: 409. 1989): Herb. Burser XI: 72 (UPS).
 Current name:  Silene gallica  L. (Caryophyllaceae).
description: Published as part of Jarvis, Charlie, 2007, Chapter 7: Linnaean Plant Names and their Types (part S), pp. 806-877 in Order out of Chaos. Linnaean Plant Types and their Types, London :Linnaean Society of London in association with the Natural History Museum on page 852, DOI: 10.5281/zenodo.291971
VLA and XMM-Newton observations of the SNR W41/TeV Gamma-ray source HESS J1834-087
Creators: name: Tian, W. W.
name: Li, Z.
name: Leahy, D. A.
name: Wang, Q. D.
Publisher: name: arXiv
Year: 2006
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: The recently discovered extended TeV source HESS J1834-087 is associated with both a diffuse X-ray enhancement and a molecular cloud, projected at the center of an old radio supernova remnant G23.3-0.3 (SNR W41). New HI observations from the VLA Galactic Plane Survey (VGPS) show unambiguous structures associated with W41 in the radial velocity range of 53 to 63 km/s, so we obtain for W41 a distance of 4+-0.2 kpc. A new higher sensitivity VGPS continuum image of W41 at 1420 MHz shows faint emission in its eastern part not detected by previous observations, so we give a new angular size of 36'x30' in b-l direction (average radius of 19 pc). We estimate for W41 a Sedov age of ~10e5 yr. New XMM-Newton observation reveals diffuse X-ray emission within the HESS source and suggests an association between the X-ray and Gamma-ray emission. The high-resolution ^{13}CO images of W41 further reveal a giant molecular cloud (GMC) located at the center of W41, likely associated with W41 in the the radial velocity range of 61 to 66 km/s. Altogether, the new observations can be interpreted as providing the first evidence that an old SNR encounters a GMC to emit TeV gamma-rays in the cloud material.
description: 11 page, 5 figs, 1 table, accepted by ApJ letters
Additional file 3: of Including gene networks to predict calving difficulty in Holstein, Brown Swiss and Jersey cattle
Creators: name: Tiezzi, Francesco
name: Arceo, Maria
name: Cole, John
name: Maltecca, Christian
Publisher: name: figshare
Year: 2018
Subjects: subject: Cell Biology
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: 69999 Biological Sciences not elsewhere classified
subject: Developmental Biology
subject: 110309 Infectious Diseases
subject: FOS: Health sciences
subject: Plant Biology
subject: 60506 Virology

description: Figure S3. Manhattan plots for PVg averaged across traits (Var). The green circles correspond to SNP that were declared significant in all the traits evaluated. (PDF 305Â kb)
Photography and the Irreal
Creators: name: MacCathie-Nevile, Maggie
Publisher: name: La Trobe
Year: 2024
Subjects: classificationCode: 360604
subject: Photography, video and lens-based practice
classificationCode: 5003
subject: Philosophy
subject: FOS: Philosophy, ethics and religion

description: Submission note: An exegesis submitted in partial fulfillment of the requirements for the degree of Master of Visual Arts, Visual Arts & Design Program, School of Communication, Arts and Critical Enquiry, Faculty of Humanities and Social Sciences, La Trobe University, Bundoora.
Silene gallica Linnaeus 1753
Creators: name: Jarvis, Charlie
Publisher: name: Linnaean Society of London in association with the Natural History Museum
Year: 2007
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Magnoliopsida
Caryophyllales
Caryophyllaceae
Silene
Silene gallica

description: Silene rigidula Linnaeus, Centuria II Plantarum: 16. 1756.
RCN: 3243.
 Lectotype (Talavera & Muñoz Garmendia in Anales Jard. Bot. Madrid 45: 408. 1989): Herb. Linn. No. 583.13 (LINN).
 Current name:  Silene gallica  L. (Caryophyllaceae).
description: Published as part of Jarvis, Charlie, 2007, Chapter 7: Linnaean Plant Names and their Types (part S), pp. 806-877 in Order out of Chaos. Linnaean Plant Types and their Types, London :Linnaean Society of London in association with the Natural History Museum on page 852, DOI: 10.5281/zenodo.291971
Particle production in field theories coupled to strong external sources. II: Generating functions
Creators: name: Gelis, Francois
name: Venugopalan, Raju
Publisher: name: arXiv
Year: 2006
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: High Energy Physics - Theory (hep-th)
subject: Nuclear Experiment (nucl-ex)
subject: Nuclear Theory (nucl-th)
subject: FOS: Physical sciences

description: We discuss a method for computing the generating function for the multiplicity distribution in field theories with strong time dependent external sources. At leading order, the computation of the generating function reduces to finding a pair of solutions of the classical equations of motion, with non-standard temporal boundary conditions.
description: 24 pages, 6 figures, version to appear in NPA
Additional file 2: of Including gene networks to predict calving difficulty in Holstein, Brown Swiss and Jersey cattle
Creators: name: Tiezzi, Francesco
name: Arceo, Maria
name: Cole, John
name: Maltecca, Christian
Publisher: name: figshare
Year: 2018
Subjects: subject: Cell Biology
subject: Genetics
subject: FOS: Biological sciences
subject: 69999 Biological Sciences not elsewhere classified
subject: Developmental Biology
subject: Science Policy
subject: 110309 Infectious Diseases
subject: FOS: Health sciences
subject: Plant Biology
subject: Computational Biology

description: Figure S2. Pearson correlation of de-regress PTA between the traits. Holstein, Brown Swiss and Jersey, respectively. (PDF 14Â kb)
Influence of C$_{6}$H$_{4}$(OH)$_{2}$ isomers on water disinfection by photocatalysis: a computational study
Creators: name: Elmenaouar, K.
name: Benbrik, R.
name: Aamouche, A.
Publisher: name: arXiv
Year: 2017
Subjects: subject: Soft Condensed Matter (cond-mat.soft)
subject: Chemical Physics (physics.chem-ph)
subject: FOS: Physical sciences

description: Solar disinfection by photocatalysis is one of the promising methods used for drinking water disinfection. It leads to the destruction of bacteria like $Escherichia$ $Coli$ ($E.$ $Coli$). In this paper, we compare our theoretical results with experimental ones done previously by A.G. Rincón and his colleagues concerning the order of decay of C$_{6}$H$_{4}$(OH)$_{2}$ isomers in the presence of titanium dioxide TiO$_{2}$, and show the influence of optical properties of those molecules on $E.$ $Coli$ inactivation. According to the adsorption energy parameter, we find that catechol has the highest adsorption degree on titanium dioxide, followed by resorcinol, and finally hydroquinone. Three dihydroxybenzene isomers absorb photons belonging to ultraviolet (UV) range. The lowest absorption energies of resorcinol, catechol and hydroquinone are respectively 3.42, 4.44 and 4.49 eV.
description: 7 pages, 3 figures, 1 table
Photography and the Irreal
Creators: name: MacCathie-Nevile, Maggie
Publisher: name: La Trobe
Year: 2023

description: Submission note: An exegesis submitted in partial fulfillment of the requirements for the degree of Master of Visual Arts, Visual Arts & Design Program, School of Communication, Arts and Critical Enquiry, Faculty of Humanities and Social Sciences, La Trobe University, Bundoora.
Spitzer Mid-Infrared Spectroscopy of Infrared Luminous Galaxies at z~2 I: the Spectra
Creators: name: Yan, Lin
name: Sajina, Anna
name: Fadda, Dario
name: Choi, Phil
name: Armus, Lee
name: Helou, George
name: Teplitz, Harry
name: Frayer, David
name: Surace, Jason
Publisher: name: arXiv
Year: 2006
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present the mid-infrared (MIR) spectra obtained with the Spitzer InfraRed Spectrograph (IRS) for a sample of 52 sources, selected as infrared luminous, z>1 candidates in the Extragalactic First Look Survey (XFLS). The sample selection criteria are f(24um) > 0.9mJy, nu fnu(24um)/nu fnu(8um) > 3.16 and nu fnu(24um)/nu fnu(0.7um) > 10. Of the 52 spectra, 47 (90%) produced measurable redshifts based solely on the mid-IR spectral features, with the majority (35/47=74%) at 1.5 1. Their $L_{1600Å}$ and $L_{\rm IR}$ suggest that our sample is among the most luminous and most dust enshrouded systems of its epoch . Our study has revealed a significant population of dust enshrouded galaxies at z~2, whose enormous energy output, comparable to that of quasars, is generated by AGN as well as starburst. This IR luminous population has very little overlap with sub-mm and UV-selected populations (Abridged).
description: Accepted by the ApJ. In vol. 658, March, 2007
title: ADCO, Cartulaire général de Cîteaux, dit de Jean de Cirey, (XVe siècle), tome III, Cart. 187 (11 H 72), f. 0033v
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: cartulaire
subject: Corpus Burgundiae Medii Aevi
subject: Chartes de la Bourgogne du Moyen Âge
subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris

description: Cartulaire général de Cîteaux, dit de Jean de Cirey, (XVe siècle), tome III, Archives départementales de la Côte-d'Or, Cart. 187 (11 H 72), f. 0033v, 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 III, Archives départementales de la Côte-d'Or, Cart. 187 (11 H 72), f. 0033v, in Projet CBMA - Corpus Burgundiae Medii Aevi [Ressource en ligne], https:// manuscrits.cbma-project.eu/
description: Provenance: https://www.geonames.org/3024876
description: Provenance: http://www.idref.fr/030974844/id
description: Provenance: https://catalogue.bnf.fr/ark:/12148/cb12228351v
description: Provenance: abbaye de Cîteaux
description: Provenance: http://www.wikidata.org/entity/Q843261
Strategies for Promoting Open Access in a Global Context
Creators: name: Dr Manon Ress
Publisher: name: Zenodo
Year: 2015
Subjects: Open Access, global, public goods, WTO

description: This presentation will focus on a new element within broader strategies to promote open access databases in the global context and also on the new role libraries can play in this Open Science effort. A proposal for a ‘World Trade Organization (WTO) Agreement on the Supply of Social/Public Goods’ is aimed at addressing an under supply of social and public goods including, but not limited to, those involving knowledge goods. The proposal, among other things, is to use the status of the WTO and its dispute resolution mechanism to enforce commitments from governments that would have the effect of expanding public access to knowledge goods. Some of the interest in the WTO proposal would involve social goods for health, development and security. However, the agreement would also be available to address important trade-related issues concerning access to governmentfunded research and databases, by providing a forum and an enforcement mechanism to address global free rider issues. As designed, the proposal would cover both funding commitments, to produce knowledge as a public good, and commitments regarding policies on global access to government-funded research. To progress the proposal, experts have recently convened meetings in Berlin and Washington DC to discuss draft language that will introduce social/public goods into the WTO environment. The terms ‘asks’ and ‘offers’ would no longer exclusively reference the private goods market, nor privatisation and the enclosure of knowledge itself. Librarians and other open data and open science advocates should participate in these negotiations, which are an important part of the movement to make openness more sustainable and consequential. Dr Manon Ress is Director of Information Society Projects at Knowledge Ecology International, a non-government organization with offices in Washington, DC, and Geneva. She is an active participant at the World Intellectual Property Organization’s meetings of the Standing Committee on Copyright and Related Rights, and other multilateral and regional forums that discuss intellectual property rights, innovation and related topics. She is active in the Trans Atlantic Consumer Dialogue (TACD) working groups on intellectual property and information society, including the proposal for a Paris Accord between consumers and creative and inventive communities. Dr Ress work has focused on the protection on consumer and user rights in intellectual property norm setting,the development and use of open standards, open access publishing, the development of open access user generated databases, the use of prizes and other alternative reward mechanism to reward creative and inventive activity, disputes over jurisdiction and the enforcement of intellectual property rights and speech torts, and the development of distance education technologies. Dr Ress holds a BA and a Master’s Degree from the Université de Nice, France as well as a Master’s and a PhD from Princeton University.
Silene diversifolia Otth 1824
Creators: name: Jarvis, Charlie
Publisher: name: Linnaean Society of London in association with the Natural History Museum
Year: 2007
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Magnoliopsida
Caryophyllales
Caryophyllaceae
Silene
Silene diversifolia

description: Silene rubella Linnaeus, Species Plantarum 1: 419. 1753, nom. utique rej.
"Habitat in Lusitania." RCN: 3261.
 Lectotype (Oxelman & Lidén in Taxon 36: 477. 1987): Herb. Linn. No. 583.43 (LINN).
 Current name:  Silene diversifolia  Otth (Caryophyllaceae).
description: Published as part of Jarvis, Charlie, 2007, Chapter 7: Linnaean Plant Names and their Types (part S), pp. 806-877 in Order out of Chaos. Linnaean Plant Types and their Types, London :Linnaean Society of London in association with the Natural History Museum on page 852, DOI: 10.5281/zenodo.291971
Effective restoration of chiral symmetry in excited mesons
Creators: name: Wagenbrunn, R. F.
name: Glozman, L. Ya.
Publisher: name: arXiv
Year: 2006
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: High Energy Physics - Lattice (hep-lat)
subject: High Energy Physics - Theory (hep-th)
subject: Nuclear Theory (nucl-th)
subject: FOS: Physical sciences

description: A fast restoration of chiral symmetry in excited mesons is demonstrated. A minimal "realistic" chirally symmetric confining model is used, where the only interaction between quarks is the linear instantaneous Lorentz-vector confining potential. Chiral symmetry breaking is generated via the nonperturbative resummation of valence quarks self-energy loops and the meson bound states are obtained from the Bethe-Salpeter equation. The excited mesons fall into approximate chiral multiplets and lie on the approximately linear radial and angular Regge trajectories, though a significant deviation from the linearity of the angular trajectory is observed.
description: 12 pp. One more clarifying paragraph has been added. To appear in Phys. Lett. B
A Photometric and Spectroscopic Study of the Cataclysmic Variable ST LMi during 2005-2006
Creators: name: Kafka, S.
name: Howell, S. B.
name: Honeycutt, R. K.
name: Robertson, J. W.
Publisher: name: arXiv
Year: 2006
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present orbit-resolved spectroscopic and photometric observations of the polar ST LMi during its recent low and high states. In the low state spectra, we report the presence of blue and red satellites to the H-alpha emission line; the velocities and visibility of the satellites vary with phase. This behavior is similar to emission line profile variations recently reported in the low state of AM Her, which were interpreted as being due to magnetically-confined gas motions in large loops near the secondary. Our low-state spectroscopy of ST LMi is discussed in terms of extreme chromospheric activity on the secondary star. Concurrent photometry indicates that occasional low-level accretion may be present, as well as cool regions on the secondary near L1. Furthermore, we report a new ``extreme low-state'' of the system at V~18.5mag. Our orbital high-state spectroscopy reveals changes in the emission line profiles with orbital phases that are similar to those reported by earlier high-state studies. The complicated emission line profiles generally consist of two main components. The first has radial velocity variations identical to that of the major emission H-alpha component seen in the low state. The second is an additional red-shifted component appearing at the phases of maximum visibility of the accreting column of the white dwarf; it is interpreted as being due to infall velocities on the accreting magnetic pole of the white dwarf. At the opposite phases, an extended blue emission wing appears on the emission line profiles. We confirm the presence of a broad absorption feature near 6275Ang which has been previously identified as Zeeman sigma(-) absorption component to H-alpha. This feature appears at just those phases when the accretion pole region is mostly directly visible and most nearly face-on to the observer.
description: 16 pages, 1 table, 17 figures. To appear in the Astronomical Journal
Improving isotopic identification with \emph{INDRA} Silicon-CsI(\emph{Tl}) telescopes
Creators: name: Lopez, O.
name: Parlog, M.
name: Borderie, B.
name: Rivet, M. F.
name: Lehaut, G.
name: Tabacaru, G.
name: Tassan-got, L.
name: Pawlowski, P.
name: Bonnet, E.
name: Bougault, R.
name: Chbihi, A.
name: Dell'Aquila, D.
name: Frankland, J. D.
name: Galichet, E.
name: Gruyer, D.
name: La Commara, M.
name: Neindre, N. Le
name: Lombardo, I.
name: Manduci, L.
name: Marini, P.
name: Steckmeyer, J. C.
name: Verde, G.
name: Vient, E.
name: Wieleczko, J. P.
Publisher: name: arXiv
Year: 2017
Subjects: subject: Instrumentation and Detectors (physics.ins-det)
subject: Nuclear Experiment (nucl-ex)
subject: FOS: Physical sciences

description: Profiting from previous works done with the \emph{INDRA} multidetector on the description of the light response $\mathcal L$ of the CsI(\emph{Tl}) crystals to different impinging nuclei, we propose an improved $ΔE - \mathcal L$ identification-calibration procedure for Silicon-Cesium Iodide (Si-CsI) telescopes, namely an Advanced Mass Estimate (\emph{AME}) method. \emph{AME} is compared to the usual, %$"ΔE - E"$ simple visual analysis of the corresponding two-dimensional map of $ΔE - E$ type, by using \emph{INDRA} experimental data from nuclear reactions induced by heavy ions in the Fermi energy regime. We show that the capability of such telescopes to identify both the atomic $Z$ and the mass $A$ numbers of light and heavy reaction products, can be quantitatively improved thanks to the proposed approach. This conclusion opens new possibilities to use \emph{INDRA} for studying these reactions especially with radioactive beams. Indeed, the determination of the mass for charged reaction products becomes of paramount importance to shed light on the role of the isospin degree of freedom in the nuclear equation of state.
description: 19 pages, 10 figures, submitted to NIM A
Additional file 1: of Stereotactic body-radiotherapy boost dose of 18 Gy vs 21 Gy in combination with androgen-deprivation therapy and whole-pelvic radiotherapy for intermediate- or high-risk prostate cancer: a study protocol for a randomized controlled, pilot trial
Creators: name: Kim, Yeon
name: Hanjong Ahn
name: Choung-Soo Kim
name: Jae-Lyun Lee
name: Kim, Young
Publisher: name: figshare
Year: 2018
Subjects: subject: Biophysics
subject: 29999 Physical Sciences not elsewhere classified
subject: FOS: Physical sciences
subject: Medicine
subject: Cancer
subject: 110309 Infectious Diseases
subject: FOS: Health sciences

description: Table S1. SPIRIT 2013 Checklist. (DOCX 62 kb)
Heavy meson semileptonic differential decay rate in two dimensions in the large Nc
Creators: name: Mondejar, Jorge
name: Pineda, Antonio
name: Rojo, Joan
Publisher: name: arXiv
Year: 2006
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: High Energy Physics - Theory (hep-th)
subject: Nuclear Theory (nucl-th)
subject: FOS: Physical sciences

description: We study QCD in 1+1 dimensions in the large $N_c$ limit using light-front Hamiltonian perturbation theory in the $1/N_c$ expansion. We use this formalism to exactly compute hadronic transition matrix elements for arbitrary currents at leading order in $1/N_c$. We compute the semileptonic differential decay rate of a heavy meson, $dΓ/dx$, and its moments, $M_N$, using the hadronic matrix elements obtained previously. We put some emphasis in trying to understand parity invariance. We also study with special care the kinematic region where the operator product expansion ($1/N \sim 1-x \sim 1$) or non-local effective field theories ($1/N \sim 1-x \sim Λ_{QCD}/m_Q$) can be applied. We then compare with the results obtained using an effective field theory approach based on perturbative factorization, with the focus to better understand quark-hadron duality. At the end of the day, using effective field theories, we have been able to obtain expressions for the moments with relative accuracy of $O(Λ_{QCD}^2/m_Q^2)$ in the kinematic region where the operator product expansion can be applied, and with relative accuracy of $O(Λ_{QCD}/m_Q)$ in the kinematic region where non-local effective field theories can be applied. These expressions agree, within this precision, with those obtained from the hadronic result using the layer-function approximation plus Euler-McLaurin expansion. Very good numerical agreement for the moments is obtained between the exact result and the result using effective field theories.
description: 52 pages, 30 figures, references added, small modifications, some discussion of the four dimensional case changed, journal version
Performance of the upgraded H.E.S.S. cameras
Creators: name: Bonnefoy, S.
name: Ashton, T.
name: Backes, M.
name: Balzer, A.
name: Berge, D.
name: Brun, F.
name: Chaminade, T.
name: Delagnes, E.
name: Fontaine, G.
name: Füßling, M.
name: Giavitto, G.
name: Giebels, B.
name: Glicenstein, J. F.
name: Gräber, T.
name: Hinton, J. A.
name: Jahnke, A.
name: Klepser, S.
name: Kossatz, M.
name: Kretzschmann, A.
name: Lefranc, V.
name: Leich, H.
name: Lenain, J. P.
name: Lüdecke, H.
name: Lypova, I.
name: Manigot, P.
name: Marandon, V.
name: Moulin, E.
name: de Naurois, M.
name: Nayman, P.
name: Ohm, S.
name: Penno, M.
name: Ross, D.
name: Salek, D.
name: Schade, M.
name: Schwab, T.
name: Shiningayamwe, K.
name: Stegmann, C.
name: Steppa, C.
name: Thornhill, J.
name: Toussenel, F.
Publisher: name: arXiv
Year: 2017
Subjects: subject: Instrumentation and Methods for Astrophysics (astro-ph.IM)
subject: FOS: Physical sciences

description: The 14 years old cameras of the H.E.S.S. 12-m telescopes have been upgraded in 2015/2016, with the goals of reducing the system failure rate, reducing the dead time and improving the overall performance of the array. This conference contribution describes the various tests that were carried out on the cameras and their sub-components both in the lab and on site. It also gives an overview of the commissioning and calibration procedures adopted during and after the installation, including e.g. flat-fielding and trigger threshold scans. Finally, it reports in detail about the overall performance of the four new H.E.S.S. I cameras, using very recent data.
Silene rupestris Linnaeus 1753
Creators: name: Jarvis, Charlie
Publisher: name: Linnaean Society of London in association with the Natural History Museum
Year: 2007
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Magnoliopsida
Caryophyllales
Caryophyllaceae
Silene
Silene rupestris

description: Silene rupestris Linnaeus, Species Plantarum 1: 421. 1753.
"Habitat in montibus aridis Sueciae, Helvetiae." RCN: 3269.
 Lectotype (Talavera & Munoz Garmendia in Anales Jard. Bot. Madrid 45: 445. 1989): Herb. Linn. No. 583.50 (LINN).
 Current name:  Silene rupestris  L. (Caryophyllaceae).
description: Published as part of Jarvis, Charlie, 2007, Chapter 7: Linnaean Plant Names and their Types (part S), pp. 806-877 in Order out of Chaos. Linnaean Plant Types and their Types, London :Linnaean Society of London in association with the Natural History Museum on page 852, DOI: 10.5281/zenodo.291971
Additional file 1: of Including gene networks to predict calving difficulty in Holstein, Brown Swiss and Jersey cattle
Creators: name: Tiezzi, Francesco
name: Arceo, Maria
name: Cole, John
name: Maltecca, Christian
Publisher: name: figshare
Year: 2018
Subjects: subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: 59999 Environmental Sciences not elsewhere classified
subject: FOS: Earth and related environmental sciences
subject: 69999 Biological Sciences not elsewhere classified
subject: Developmental Biology
subject: Science Policy

description: Figure S1. Schematic representation of the workflow used in this study. (PDF 11Â kb)
Barred CO emission in HE1029-1831
Creators: name: Krips, M.
name: Eckart, A.
name: Neri, R.
name: Bertram, T.
name: Straubmeier, C.
name: Fischer, S.
name: Staguhn, J. G.
name: Vogel, S. N.
Publisher: name: arXiv
Year: 2006
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present CO(1-0) and CO(2-1) line emission maps of the barred spiral active galaxy HE1029-1831 (z=0.0403) obtained with the IRAM Plateau de Bure Interferometer (PdBI) and in part by the Berkeley-Illinois-Maryland Association (BIMA) observatory. The CO emission is well associated with the optical bar and extended along it. The FWHM of the CO emission is estimated to be ~(6+-2)kpc. The CO emission shows a strong velocity gradient along the minor axis of the bar (PA=90degree). The molecular gas mass is estimated to be ~1.2x10^(10)Msun which indicates a very gas rich host galaxy. Most of the molecular gas appears to be subthermally excited and cold but we also find weak evidence for a warmer and/or denser gas component at the southern part of the bar emission, about \~4kpc from the galactic nucleus.
description: accepted for publication in A&A; 6 pages and 7 figures
Light Higgs Boson from a Pole Attractor
Creators: name: Matsedonskyi, Oleksii
name: Montull, Marc
Publisher: name: arXiv
Year: 2017
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We propose a new way of explaining the observed Higgs mass, within the cosmological relaxation framework. The key feature distinguishing it from other scanning scenarios is that the scanning field has a non-canonical kinetic term, whose role is to terminate the scan around the desired Higgs mass value. We propose a concrete realisation of this idea with two new singlet fields, one that scans the Higgs mass, and another that limits the time window in which the scan is possible. Within the provided time period, the scanning field does not significantly evolve after the Higgs field gets close to the Standard Model value, due to particle production friction.
description: version published in PRD
Additional file 1: of Dengue virus-like particles mimic the antigenic properties of the infectious dengue virus envelope
Creators: name: Metz, Stefan
name: Thomas, Ashlie
name: White, Laura
name: Stoops, Mark
name: Corten, Markus
name: Hannemann, Holger
name: Aravinda De Silva
Publisher: name: figshare
Year: 2018
Subjects: subject: Space Science
subject: Medicine
subject: Microbiology
subject: FOS: Biological sciences
subject: Cell Biology
subject: Molecular Biology
subject: Biotechnology
subject: Ecology
subject: Immunology
subject: FOS: Clinical medicine
subject: Cancer
subject: 110309 Infectious Diseases
subject: FOS: Health sciences
subject: 60506 Virology

description: Normalized antibody binding to DENV virus particles and VLPs. The binding of each mAb to virus (black bars) or VLPs (grey bars) within every DENV serotype was normalized to 1F4 (DENV1), 2D22 (DENV2), 5Â J7 (DENV3) and 5H2 (DENV4). (PDF 220 kb)
Identifying the Patient Barriers and Strategies to Improve Referral Compliance for Children after Abnormal Vision Screening Tests: A Scoping Review Protocol
Creators: name: Hicks, Patrice
name: Howard, Allison
name: Afua Asare
name: Amoah, Amy
name: Rodriguez, Aurora
Publisher: name: OSF Registries
Year: 2023
Subjects: subject: Medicine and Health Sciences
subject: Social and Behavioral Sciences

description: The scoping review will map the existing literature regarding patient barriers to referral compliance after abnormal vision screening tests in children, along with the strategies employed or recommended to overcome these barriers.
Neutrino masses and mixing parameters in a left-right model with mirror fermions
Creators: name: Gaitán, R.
name: Hernández-Galeana, A.
name: Rivera-Rebolledo, J. M.
name: de Córdoba, P. Fernández
Publisher: name: arXiv
Year: 2006
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: In this work we consider a left-right model containing mirror fermions with gauge group SU(3)$_{C} \otimes SU(2)_{L} \otimes SU(2)_{R} \otimes U(1)_{Y^\prime}$. The model has several free parameters which here we have calculated by using the recent values for the squared-neutrino mass differences. Lower bound for the mirror vacuum expectation value helped us to obtain crude estimations for some of these parameters. Also we estimate the order of magnitude of the masses of the standard and mirror neutrinos.
description: 13 pages, version submitted to European Physical Journal C
ЭПИСТЕМИЧЕСКАЯ ВОЗМОЖНОСТЬ И ЕЕ ВЫРАЖЕНИЕ В АНГЛИЙСКОМ И ТАТАРСКОМ ЯЗЫКАХ
Creators: name: Р. Р. Ахунзянова
Publisher: name: Мир науки, культуры, образования
Year: 2019
Subjects: модальность
эпистемическая модальность
эпистемическая возможность
английский язык
татарский язык
семантика

description: В статье рассматривается субъективный тип модальности – эпистемическая модальность, которая заключается в оценке пропозиции высказывания говорящим с точки зрения ее вероятности. Высказывания с эпистемической модальностью главным образом имеют характер логических умозаключений, в которых говорящий лично оценивает, насколько содержание пропозиции соответствует действительности, основываясь на своем знании ситуации. В центре данного исследования находится эпистемическая возможность, которая выражает низкую или среднюю степень вероятности соответствия содержания пропозиции действительности и является результатом недостаточной или ограниченной осведомленности говорящего относительно описываемой ситуации. Целью настоящего исследования является рассмотрение репрезентации семантики эпистемической возможности в разноструктурных языках, в частности в английском и татарском языках, которые принадлежат к аналитическому и агглютинативному языковым типам соответственно. Реализация данного вида модальных значений исследуется на различных (морфологическом, лексическом, синтаксическом) уровнях языковой системы.
Spathius magnus Chao. A 1978
Creators: name: Tang, Pu
name: Belokobylskij, Sergey
name: Chen, Xue-Xin
Publisher: name: Zenodo
Year: 2015
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hymenoptera
Braconidae
Spathius
Spathius magnus

description: Spathius magnus Chao, 1978
(Fig. 20)
Spathius magnus Chao, 1978: 178; Chen & Shi, 2004: 145; Yu et al., 2012.
Material examined. Female (holotype, IZCAS), Yunnan Prov., 27. VI.1957, Zang Linchao. China (ZJUH). Yunnan Prov.: 1 female, Jinghong, 31.VII.2003, Lu Jia, No. 20045948.
Distribution. China (Hubei, Yunnan).
description: Published as part of Tang, Pu, Belokobylskij, Sergey & Chen, Xue-Xin, 2015, Spathius Nees, 1818 (Hymenoptera: Braconidae, Doryctinae) from China with a key to species, pp. 1-132 in Zootaxa 3960 (1) on page 66, DOI: 10.11646/zootaxa.3960.1.1, http://zenodo.org/record/14951550
КОНЦЕПТ «ГОРА» КАК КОНСТРУКТ ТОПОНИМИЧЕСКОЙ КАРТИНЫ МИРА КАВКАЗСКИХ МИНЕРАЛЬНЫХ ВОД
Creators: name: Л. В. Васильева
name: И. В. Величко
Publisher: name: Мир науки, культуры, образования
Year: 2019
Subjects: концепт
языковая картина мира
топонимическая картина мира
ороним
оним
онимизация

description: В статье представлен анализ концепта «гора» на материале оронимии Кавказских Минеральных Вод. Охарактеризован процесс формирования топонимической лексики данного региона с точки зрения полиэтнического, поликонфессионального и полиязычного характера языковой картины мира Северного Кавказа. Рассмотрены на основе лексико-семантической характеристики онимы орографических объектов. Представлены две группы оронимов: первичные и непервичные. Каждая группа классифицирована: в первой выделено шесть тем, во второй – 4. Определено пропорциональное соотношение русскоязычных, тюркских и аборигенных названий. Указаны мотивы и основные способы онимизации. Обусловлено влияние паралингвистических факторов на формирование топонимической картины мира Кавказских Минеральных Вод.
Accretion Discs with Strong Toroidal Magnetic Fields
Creators: name: Begelman, M. C.
name: Pringle, J. E.
Publisher: name: arXiv
Year: 2006
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Simulations and analytic arguments suggest that the turbulence driven by magnetorotational instability (MRI) in accretion discs can amplify the toroidal (azimuthal) component of the magnetic field to a point at which magnetic pressure exceeds the combined gas + radiation pressure in the disc. Arguing from the recent analysis by Pessah and Psaltis, and other MRI results in the literature, we conjecture that the limiting field strength for a thin disc is such that the Alfven speed roughly equals the geometric mean of the Keplerian speed and the gas sound speed. We examine the properties of such magnetically-dominated discs, and show that they resolve a number of outstanding problems in accretion disc theory. The discs would be thicker than standard (Shakura-Sunyaev) discs at the same radius and accretion rate, and would tend to have higher colour temperatures. If they transport angular momentum according to an alpha-prescription, they would be stable against the thermal and viscous instabilities that are found in standard disc models. In discs fuelling active galactic nuclei, magnetic pressure support could also alleviate the restriction on accretion rate imposed by disc self-gravity.
description: 8 pages, no figures, to be published in Monthly Notices of the Royal Astronomical Society
Silene saxifraga Linnaeus 1753
Creators: name: Jarvis, Charlie
Publisher: name: Linnaean Society of London in association with the Natural History Museum
Year: 2007
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Magnoliopsida
Caryophyllales
Caryophyllaceae
Silene
Silene saxifraga

description: Silene saxifraga Linnaeus, Species Plantarum 1: 421. 1753.
"Habitat in montibus cretaceis Galliae, Italiae." RCN: 3270.
 Lectotype (Talavera & Munoz Garmendia in Anales Jard. Bot. Madrid 45: 443. 1989): Herb. Burser XI: 128 (UPS).
 Current name:  Silene saxifraga  L. (Caryophyllaceae).
description: Published as part of Jarvis, Charlie, 2007, Chapter 7: Linnaean Plant Names and their Types (part S), pp. 806-877 in Order out of Chaos. Linnaean Plant Types and their Types, London :Linnaean Society of London in association with the Natural History Museum on page 852, DOI: 10.5281/zenodo.291971
Quantum error correction using weak measurements
Creators: name: Kumar, Parveen
name: Patel, Apoorva
Publisher: name: arXiv
Year: 2017
Subjects: subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: The standard quantum error correction protocols use projective measurements to extract the error syndromes from the encoded states. We consider the more general scenario of weak measurements, where only partial information about the error syndrome can be extracted from the encoded state. We construct a feedback protocol that probabilistically corrects the error based on the extracted information. Using numerical simulations of one-qubit error correction codes, we show that our error correction succeeds for a range of the weak measurement strength, where (a) the error rate is below the threshold beyond which multiple errors dominate, and (b) the error rate is less than the rate at which weak measurement extracts information. It is also obvious that error correction with too small a measurement strength should be avoided.
description: 9 pages, 7 figures