cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Time-domain effective-one-body gravitational waveforms for coalescing compact binaries with nonprecessing spins, tides and self-spin effects
Creators: name: Nagar, Alessandro
name: Bernuzzi, Sebastiano
name: Del Pozzo, Walter
name: Riemenschneider, Gunnar
name: Akcay, Sarp
name: Carullo, Gregorio
name: Fleig, Philipp
name: Babak, Stanislav
name: Tsang, Ka Wa
name: Colleoni, Marta
name: Messina, Francesco
name: Pratten, Geraint
name: Radice, David
name: Rettegno, Piero
name: Agathos, Michalis
name: Fauchon-Jones, Edward
name: Hannam, Mark
name: Husa, Sascha
name: Dietrich, Tim
name: Cerda-Duran, Pablo
name: Font, Jose A.
name: Pannarale, Francesco
name: Schmidt, Patricia
name: Damour, Thibault
Publisher: name: arXiv
Year: 2018
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: We present TEOBResumS, a new effective-one-body (EOB) waveform model for nonprecessing (spin-aligned) and tidally interacting compact binaries.Spin-orbit and spin-spin effects are blended together by making use of the concept of centrifugal EOB radius. The point-mass sector through merger and ringdown is informed by numerical relativity (NR) simulations of binary black holes (BBH) computed with the SpEC and BAM codes. An improved, NR-based phenomenological description of the postmerger waveform is developed.The tidal sector of TEOBResumS describes the dynamics of neutron star binaries up to merger and incorporates a resummed attractive potential motivated by recent advances in the post-Newtonian and gravitational self-force description of relativistic tidal interactions. Equation-of-state dependent self-spin interactions (monopole-quadrupole effects) are incorporated in the model using leading-order post-Newtonian results in a new expression of the centrifugal radius. TEOBResumS is compared to 135 SpEC and 19 BAM BBH waveforms. The maximum unfaithfulness to SpEC data $\bar{F}$ -- at design Advanced-LIGO sensitivity and evaluated with total mass $M$ varying between $10M_\odot \leq M \leq 200 M_\odot$ --is always below $2.5 \times 10^{-3}$ except for a single outlier that grazes the $7.1 \times 10^{-3}$ level. When compared to BAM data, $\bar{F}$ is smaller than $0.01$ except for a single outlier in one of the corners of the NR-covered parameter space, that reaches the $0.052$ level.TEOBResumS is also compatible, up to merger, to high end NR waveforms from binary neutron stars with spin effects and reduced initial eccentricity computed with the BAM and THC codes. The model is designed to generate accurate templates for the analysis of LIGO-Virgo data through merger and ringdown. We demonstrate its use by analyzing the publicly available data for GW150914.
description: 39 pages, 36 figures. Extended appendix with discussion of the postmerger fits. Version accepted for publication in Phys. Rev. D
Circular polarization in pulsar integrated profiles
Creators: name: Han, J. L.
name: Manchester, R. N.
name: Xu, R. X.
name: Qiao, G. J.
Publisher: name: arXiv
Year: 1998
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present a systematic study of the circular polarization in pulsar integrated profiles, based on published polarization data. For core components, we find no significant correlation between the sense-change of circular polarization and the sense of linear position angle variation. Circular polarization is not restricted to core components and, in some cases, reversals of circular polarization sense are observed across the conal emission. In conal double profiles, the sense of circular polarization is found to be correlated with the sense of position-angle variation. Pulsars with a high degree of linear polarization often have one hand of circular polarization across the whole profile. For most pulsars, the sign of circular polarization is the same at 50-cm and 20-cm wavelength, and the degree of polarization is similar, albeit with a wide scatter. However, at least two cases of frequency-dependent sign reversals are known. This diverse behaviour may require more than one mechanism to generate circular polarization.
description: Will apear in MNRAS. 15 pages, 9 figures. One big table. 1.6MB PS file: ftp://ftp.mpifr-bonn.mpg.de/user/jhan/PS/98HMXQ_MN.ps
Centranthera indica Gamble 1924
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
Lamiales
Orobanchaceae
Centranthera
Centranthera indica

description: Rhinanthus indicus Linnaeus, Species Plantarum 2: 603. 1753.
"Habitat in Zeylona." RCN: 4377.
Lectotype (Cramer in Dassanayake & Fosberg, Revised Handb. Fl. Ceylon 3: 396. 1981): Herb. Hermann 2: 22, No. 238 (BM-000621584).
Current name: Centranthera indica (L.) Gamble (Scrophulariaceae).
Note: Specific epithet spelled “indica” in the protologue.
Although Cramer indicated the type in the Hermann herbarium (BM) as "Mus. No. 20", the only material that could have been intended is that in vol. 2: 22, comprising two closely associated specimens and this material is therefore accepted as the type.
description: Published as part of Jarvis, Charlie, 2007, Chapter 7: Linnaean Plant Names and their Types (part R), pp. 785-805 in Order out of Chaos. Linnaean Plant Types and their Types, London :Linnaean Society of London in association with the Natural History Museum on page 793, DOI: 10.5281/zenodo.291971
title: ADCO, Cartulaire de l'abbaye de Cîteaux dit Cartulare Antiquum t.3 (2e moitié XIIIe siècle), Cart. 168 (11 H 66), f. 0157v
Creators: name: de la Côte d'Or, Archives départementales
name: Archives Départementales De La Côte-D'Or
name: Petot, Frédérique
name: Projet CBMA
name: Petot, Frédéric
name: CG21/F.PETOT/2010
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2020
Subjects: subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris
subject: Corpus Burgundiae Medii Aevi
subject: Chartes de la Bourgogne du Moyen Âge
subject: cartulaire

description: Cartulaire de l'abbaye de Cîteaux dit Cartulare Antiquum t.3 (2e moitié XIIIe siècle), Archives départementales de la Côte-d'Or, Cart. 168 (11 H 66), f. 0157v, Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Cartulaire de l'abbaye de Cîteaux dit Cartulare Antiquum t.3 (2e moitié XIIIe siècle), Archives départementales de la Côte-d'Or, Cart. 168 (11 H 66), f. 0157v, 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
Cosmic Microwave Background Polarization
Creators: name: Kosowsky, Arthur
Publisher: name: arXiv
Year: 1995
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Polarization of the cosmic microwave background, though not yet detected, provides a source of information about cosmological parameters complementary to temperature fluctuations. This paper provides a complete theoretical treatment of polarization fluctuations. After a discussion of the physics of polarization, the Boltzmann equation governing the evolution of the photon density matrix is derived from quantum theory and applied to microwave background fluctuations, resulting in a complete set of transport equations for the Stokes parameters from both scalar and tensor metric perturbations. This approach is equivalent at lowest order in scattering kinematics to classical radiative transfer, and provides a general framework for treating the cosmological evolution of density matrices. The metric perturbations are treated in the physically appealing longitudinal gauge. Expressions for various temperature and polarization correlation functions are derived. Detection prospects and theoretical utility of microwave background polarization are briefly discussed.
description: Replaced version corrects factor of 2 error in the Liouville equation. 24 pages, Postscript
Dark matter in elliptical galaxies
Creators: name: Carollo, M.
name: de Zeeuw, T.
name: van der Marel, R.
name: Danziger, J.
name: Qian, E.
Publisher: name: arXiv
Year: 1995
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present measurements of the shape of the stellar line-of-sight velocity distribution out to two effective radii along the major axes of the four elliptical galaxies NGC 2434, 2663, 3706, and 5018. The velocity dispersion profiles are flat or decline gently with radius. We compare the data to the predictions of f=f(E,L_z) axisymmetric models with and without dark matter. Strong tangential anisotropy is ruled out at large radii. We conclude from our measurements that massive dark halos must be present in three of the four galaxies, while for the fourth galaxy (NGC 2663) the case is inconclusive.
description: 15 pages, uuencoded compressed PostScript, includes 3 figures
Bicomponent polymeric micelles for pH-controlled delivery of doxorubicin
Creators: name: Wang, Chunyun
name: Qi, Peilan
name: Lu, Yan
name: Liu, Lei
name: Zhang, Yanan
name: Sheng, Qianli
name: Wang, Tianshun
name: Zhang, Mengying
name: Wang, Rui
name: Song, Shiyong
Publisher: name: Taylor & Francis
Year: 2020
Subjects: subject: Biophysics
subject: Biochemistry
subject: Space Science
subject: Microbiology
subject: FOS: Biological sciences
subject: Pharmacology
subject: Biotechnology
subject: Chemical Sciences not elsewhere classified
subject: Biological Sciences not elsewhere classified
subject: Cancer

description: Stimuli-responsive drug delivery systems (DDSs) are expected to realize site-specific drug release and kill cancer cells selectively. In this study, a pH-responsive micelle was designed utilizing the pH-sensitivity of borate bonds formed between dopamine and boronic acid. First, methyl (polyethylene glycol)-block-polycaprolactone (mPEG-PCL) was conjugated with 4-cyano-4-(thiobenzoylthio)pentanoic acid (CTP) to obtain a macroinitiator. Two different segments poly(dopamine methacrylamide) (PDMA) and poly(vinylphenylboronic acid) (PVBA) were then grafted to the end of mPEG-PCL. Two triblock copolymers, mPEG-PCL-PDMA and mPEG-PCL-PVBA, were then obtained by reversible addition–fragmentation transfer (RAFT) polymerization. These copolymers and their mixture self-assembled in aqueous solution to form micelles that were able to load hydrophobic anticancer drug doxorubicin (DOX). These two-component micelles were found to be pH-sensitive, in contrast to the one-component micelles. Furthermore, MTT studies showed that the micelles were almost nontoxic. The DOX-loaded micelles showed cytotoxicity equivalent to that of DOX at high concentration. In vivo antitumor experiments showed that this pH-sensitive polymeric micellar system had an enhanced therapeutic effect on tumors. These two-component boronate-based pH micelles are universally applicable to the delivery of anticancer drugs, showing great potential for cancer therapy.
FluidNET Abstract NAC - The sub- to supersolidus transition in the Lys-Caillaouas massif and Gavarnie-Héas valleys, central Pyrenees
Creators: name: Noor de Leijer
name: Dörte Jordan
name: Leo Kriegsman
Publisher: name: Zenodo
Year: 2023

description: The sub- to supersolidus transition in the Lys-Caillaouas massif and Gavarnie-Héas valleys, central Pyrenees

 

De Leijer N.J.M.1, Jordan D.A.A.2 and Kriegsman L.M.1,2*

1. Naturalis Biodiversity Center, Dept. of Research & Education, Leiden, Netherlands

2. Utrecht University, Faculty of Geosciences, Dept. of Earth Sciences, Netherlands

 

Partial melting is the key factor in crustal differentiation processes and in the transfer of many critical metals from the deepest continental crust to shallower levels via granitoids. These processes are documented in deeply exposed migmatite and granulite domains of former mountain belts. Migmatites are sites of melt production, but they are also affected by melt influx from deeper (granulite-dominated) levels. Additionally, the restitic units and the crystallizing melts frequently react at microscale and outcrop scale, which leaves a retrograde overprint on the peak mineral assemblages. Well-exposed areas showing the transition from subsolidus to supersolidus processes are required in order to quantify element transfers.

This project* focuses on the western Lys-Caillaouas massif and the adjacent Gavarnie-Héas valleys in the central Pyrenees, that expose a Hercynian window below an Alpine nappe stack. The area shows the transition from medium-grade metasediments to migmatites along a steep geothermal gradient. The presentation will highlight petrological and microtextural features of this transition, and addresses the geochemical link between in-situ melts in the migmatites and cross-cutting cordierite-bearing (leuco-)granites. The complexities of prograde melt-producing reactions and retrograde melt-consuming reactions will be summarized in a conceptual model for melt-mediated fluid transfer and recycling at sample and outcrop scale. This model serves as the foundation for quantifying element fluxes, including trace element redistribution.

(*Part of the FluidNET research and training network on fluid-rock interaction, funded by EU’s Horizon 2020 Marie Sklodowska-Curie grant 956127.)
HST Colour-Magnitude Diagrams of Six Old Globular Clusters in the LMC
Creators: name: Olsen, K. A. G.
name: Hodge, P. W.
name: Mateo, M.
name: Olszewski, E. W.
name: Schommer, R. A.
name: Suntzeff, N. B.
name: Walker, A. R.
Publisher: name: arXiv
Year: 1998
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We report on HST observations of six candidate old globular clusters in the Large Magellanic Cloud: NGC 1754, NGC 1835, NGC 1898, NGC 1916, NGC 2005 and NGC 2019. Deep exposures with the F555W and F814W filters provide us with colour-magnitude diagrams that reach to an apparent magnitude in V of ~25, well below the main sequence turnoff. These particular clusters are involved with significantly high LMC field star densities and care was taken to subtract the field stars from the cluster colour-magnitude diagrams accurately. In two cases there is significant variable reddening across at least part of the image, but only for NGC 1916 does the differential reddening preclude accurate measurements of the CMD characteristics. The morphologies of the colour- magnitude diagrams match well those of Galactic globular clusters of similar metallicity. All six have well-developed horizontal branches, while four clearly have stars on both sides of the RR Lyrae gap. The abundances obtained from measurements of the height of the red giant branch above the level of the horizontal branch are 0.3 dex higher, on average, than previously measured spectroscopic abundances. Detailed comparisons with Galactic globular cluster fiducials show that all six clusters are old objects, very similar in age to classical Galactic globulars such as M5, with little age spread among the clusters. This result is consistent with ages derived by measuring the magnitude difference between the horizontal branch and main sequence turnoff. We also find a similar chronology by comparing the horizontal branch morphologies and abundances with the horizontal branch evolutionary tracks of Lee, Demarque, & Zinn (1994). Our results imply that the LMC formed at the same time as the Milky Way Galaxy.
description: 23 pages, 18 PostScript figures, LaTeX, accepted by MNRAS. Uses mn.sty and epsf.sty. Requires ols.sty (included)
Rhinanthus alectorolophus Pollich 1777
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
Lamiales
Orobanchaceae
Rhinanthus
Rhinanthus alectorolophus

description: Rhinanthus major Linnaeus, Amoenitates Academicae 3: 53. 1756.
RCN: 4374.
Type not designated.
Original material: none traced.
Current name: Rhinanthus alectorolophus (Scop.) Pollich (Scrophulariaceae).
Note: This has been treated as a nomen ambiguum by many authors but no formal rejection proposal has been made.
description: Published as part of Jarvis, Charlie, 2007, Chapter 7: Linnaean Plant Names and their Types (part R), pp. 785-805 in Order out of Chaos. Linnaean Plant Types and their Types, London :Linnaean Society of London in association with the Natural History Museum on page 793, DOI: 10.5281/zenodo.291971
The Evolution of Correlation Functions and Power Spectra in Gravitational Clustering
Creators: name: Jain, B.
name: Mo, H. J.
name: White, S. D. M.
Publisher: name: arXiv
Year: 1995
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Hamilton et al. (1991) proposed a simple formula relating the nonlinear autocorrelation function of the mass distribution to the primordial spectrum of density fluctuations for gravitational clustering in an $Ω=1$ universe. High resolution N-body simulations show this formula to work well for scale-free spectra $P(k) \propto k^n$ when the spectral index $n\sim 0$, but not when $n \lsim -1$. We show that a modified version of the formula can work well provided its form depends on $n$. This dependence can be derived from a simple physical model for collapse from Gaussian initial conditions. Our modified formula is easy to apply and is an excellent fit to N-body simulations with $0 \leq n \leq -2$. It can also be applied to non-power law initial spectra such as that of the standard Cold Dark Matter model by using the local spectral index at the current nonlinear scale as the effective value of $n$ at any given redshift. We give analytic expressions both for the nonlinear correlation function and for the nonlinear power spectrum.
description: 6 pages, uuencoded compressed postscript file, including 2 figures. Significantly revised, matches published version
Additional file 4 of Whole-genome resequencing of three Coilia nasus population reveals genetic variations in genes related to immune, vision, migration, and osmoregulation
Creators: name: Gao, Jun
name: Xu, Gangchun
name: Xu, Pao
Publisher: name: figshare
Year: 2021
Subjects: subject: Genetics
subject: FOS: Biological sciences

description: Additional file 4.
Additional file 7: of Genome-wide diversity in temporal and regional populations of the betabaculovirus Erinnyis ello granulovirus (ErelGV)
Creators: name: A. Brito
name: F. Melo
name: D. Ardisson-Araújo
name: W. Sihler
name: M. Souza
name: B. Ribeiro
Publisher: name: figshare
Year: 2018
Subjects: subject: Biophysics
subject: 29999 Physical Sciences not elsewhere classified
subject: FOS: Physical sciences
subject: Microbiology
subject: FOS: Biological sciences
subject: Genetics
subject: Evolutionary Biology
subject: 59999 Environmental Sciences not elsewhere classified
subject: FOS: Earth and related environmental sciences
subject: Ecology
subject: 69999 Biological Sciences not elsewhere classified
subject: Plant Biology

description: Showing polymorphisms in lef genes. Non-synonymous mutations in lef-1 (A) and lef-2 (B) were mainly found on the C-terminal of the proteins they encode. For LEF-10, polymorphisms were found mainly on it N-terminal (C). The exception is a single non-synonymous substitution at a region overlapping with vp1054, which in turn causes a synonymous change (CTG → CTA) at the 5′ end of the latter. (PDF 1357 kb)
Evolution of the Power Spectrum and the Self-Similarity in the Expanding One-Dimensional Universe
Creators: name: Yano, Taihei
name: Gouda, Naoteru
Publisher: name: arXiv
Year: 1998
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We have investigated time evolutions of power spectra of density fluctuations for long time after the first appearance of caustics in the expanding one-dimensional universe. It is found that when an initial power spectrum is sale-free with a power index $n$, a self-similarity of the time evolution of the power spectrum is achieved. We find that the power spectrum can be separated roughly into three regimes according to the shape of the power spectrum: the linear regime ($k < k_{nl}$ : the regime {\cal 1}),the single-caustic regime($k_{nl} < k < k_{snl}$ : the regime 2), and the multi-caustics regime($k > k_{snl}$ : the regime 3). The power index of the power spectrum in each regime has the values of $n,-1$, and $μ$ which depends on $n$, respectively. Even in the case of an initial power-law spectrum with a cutoff scale, there might be the possibility of the self-similar evolution of the power spectrum after the appearance of the caustics. It is found, however, the self-similarity is not achieved in this case. The shape of the power spectrum on scales smaller than the cutoff scale can be separated roughly in two regimes: the virialized regime ($k_{cut}< k < k_{cs}$ : the regime 4), and the smallest-single-caustic regime ($ k > k_{cs}$ : the regime 5). The power index of the power spectrum is $ν$ which may be determined by the distribution of singular points in the regime 4. In the regime 5, the value of the power index is -1. Moreover we show the general property about the shape of a power spectrum with a general initial condition.
description: Accepted for pubrication in the ApJS, vol.118, October, 1998; 15pages, uses aaspp4.sty, 12figures
Apparatus design and experimental studies of XUV initiated HHG
Creators: name: Hutchinson, Simon
Publisher: name: Imperial College London
Year: 2014

description: This thesis presents the work on a new beamline for ultra-fast spectroscopy experiments, along with the study of a new ultra-fast spectroscopy technique for studying attosecond electron dynamics: XUV initiated high harmonic generation (XiHHG) XiHHG is an extension of the high harmonic generation (HHG) technique for ultra-fast spectroscopy. XiHHG replaces the tunnel ionisation in HHG with single photon ionisation, and thus an XUV field is used to ionise the electron and a colinear IR field is used to recombine the electron. A goal of this is that energetically deep levels of atoms and molecules can be probed without the need for a very strong IR field. The specifications of the new beamline required that it be entirely housed in a vacuum of pressures on the order of 1×10 −6 mbar. As all of the optics and experimental controls were also in vacuum, electronic feed-throughs were implemented and sophisticated data acquistion software was developed. As the nature of the data collected for these experiments is large in volume, significant time was also spent creating an analysis script to handle the data automatically. This enabled the data to be transmitted amongst experimenters with ease and accuracy. Preliminary experimental results are shown from the beamline, with some possible theoretical explanations investigated. Further theoretical work is required in order to fully interpret the experimental results.
title: Jahreshefte der Gesellschaft für Naturkunde in Württemberg, Bd. 157 (2001): Jahreshefte der Gesellschaft für Naturkunde in Württemberg, 157. Jahrgang
title: Jahreshefte der Gesellschaft für Naturkunde in Württemberg, 157. Jahrgang
titleType: AlternativeTitle
Creators: name: Jahreshefte Der Gesellschaft Für Naturkunde In Württemberg
Publisher: name: Jahreshefte der Gesellschaft für Naturkunde in Württemberg
Year: 2021

description: Bericht der Gesellschaft für Naturkunde in Württemberg 2001...333-337 Bericht des Staatlichen Museums für Naturkunde Stuttgart 2000...293-331 Nachruf Fritz Weidenbach (1901-2000)...253-291 Nachruf Josef Kratochvil (1915-2001)...249-251 Nachruf Albert Kley (1907-2000)...245-247 Nachruf Elsbeth Keppler (1906-2001)...241-243 Neunachweise von Prosobranchia und Heterostropha (Mollusca, Gastropoda) in der Deutschen Bucht...211-239 Langzeitpopulationsdynamik des Siebenschläfers Myoxus glis in Baden-Württemberg – Ein Kleinsäuger als Gewinner der heutigen Waldwirtschaft und des gesellschaftlichen Wandels...181-210 Georg Friedrich Jägers Besuch bei Justinus Kerner – ein Bilddokument aus dem Jahre 1860...165-179 Neues zu Leonhart Fuchs...139-163 Die Mallomonas-Arten (Synurophyceae) des Federsees (Baden-Württemberg)...129-137 Ein Kieselholz aus der Wutachschlucht bei Ewattingen, SW-Deutschland...121-128 Erstnachweis eines Käfers im Nusplinger Plattenkalk (Oberjura, Schwäbische Alb)...115-120 Schildkröten (Reptilia: Testudines) aus dem Brenztaloolith des Oberen Jura der Schwäbischen Alb (SW-Deutschland) in der Tübinger Sammlung...099-114 Über das süddeutsche Pliozän und Pleistozän in ihren europäischen Zusammenhängen. Teil I. Das Pleistozän...043-097 Der Nusplinger Plattenkalk (Weisser Jura ζ) – Grabungskampagne 2000...021-042 Auswirkungen der Stickoxide als Luftschadstoffe auf die Vegetation...005-020
title: ADCO, Grènetier de Cîteaux : comptes (1499-1503) (11 H 1173), f. 00188
Creators: name: de la Côte-d'Or, Archives départementales
name: CBMA/CG21/F.PETOT/2019
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: Corpus Burgundiae Medii Aevi
subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris
subject: Chartes de la Bourgogne du Moyen Âge
subject: comptes

description: Grènetier de Cîteaux : comptes (1499-1503), Archives départementales de la Côte-d'Or, (11 H 1173). Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Grènetier de Cîteaux : comptes (1499-1503), Archives départementales de la Côte-d'Or, (11 H 1173), f. 00188, 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
Rhinanthus minor Linnaeus 1756
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
Lamiales
Orobanchaceae
Rhinanthus
Rhinanthus minor

description: Rhinanthus minor Linnaeus, Amoenitates Academicae 3: 54. 1756.
RCN: 4374.
Type not designated.
Original material: none traced.
Current name: Rhinanthus minor L. (Scrophulariaceae).
description: Published as part of Jarvis, Charlie, 2007, Chapter 7: Linnaean Plant Names and their Types (part R), pp. 785-805 in Order out of Chaos. Linnaean Plant Types and their Types, London :Linnaean Society of London in association with the Natural History Museum on page 793, DOI: 10.5281/zenodo.291971
Investigating the Role of COX-1 and COX-2 in Toll-Like Receptor Responses
Creators: name: Wright, William
Publisher: name: Imperial College London
Year: 2014

description: COX is the rate-limiting enzyme in the conversion of arachidonic acid to the prostanoids. It is present in humans as two isoforms, COX-1 and COX-2. COX-1 is constitutively expressed and involved in homeostatic functions, while COX-2 expression is mostly limited to sites of inflammation. The precise function of COX isoforms is a subject of debate, particularly with respect to nonsterodial anti-inflammatory drug (NSAID)-induced toxicity. Toll-like receptors (TLRs) trigger the immune response following recognition of pathogen-associated molecular patterns (PAMPs), such as bacterial lipopolysaccharide (LPS), which activates TLR4. The role of COX-1 and COX-2 in responses to different TLRs is incompletely understood. The main focus of my PhD was to investigate COX-1 and COX-2 function in innate immunity, using TLR agonists in mice lacking COX-1 or COX-2. I also studied this in relation to lung inflammation using lung fibroblasts, and isolated pulmonary arteries to examine the effect of prostanoids on pulmonary vascular responses. Lung fibroblasts isolated from COX-2-/- mice were more proliferative than lung fibroblasts from wild-type or COX-1-/- mice. They also released greater amounts of cytokines when stimulated with various TLR agonists. Human lung fibroblasts were particularly sensitive to TLR3 agonists, and cytokine release was enhanced in the presence of NSAIDs. The effect of diclofenac may have been caused by inhibition of COX-related prostaglandin (PG) E2. In in vivo studies, Cox2 gene expression was strongly induced by TLR4 activation in all organs and less so by TLR3 activation, where induction was restricted to the spleen and stomach. Mice lacking COX-2 released higher amounts of anti-viral proteins following TLR3 activation with poly (I:C). This suggests that COX-2-specific NSAIDs may boost the anti-viral response, thus proving beneficial over traditional NSAIDs during viral infection. In the pulmonary vasculature, I found that most prostacyclin drugs were limited by actions on EP3 receptors, but that selective peroxisome proliferator-activated receptor (PPAR)β/δ agonists were active as dilators under all conditions. Deletion of COX-1 or COX-2 affected the ability of mouse pulmonary arteries to release endothelial-derived nitric oxide but not to respond to IP or PPARβ/δ agonists. Finally, activation of adenosine monophosphate kinase (AMPK) had no direct dilator effect on pulmonary vessels. However, preliminary data suggest that pretreatment of vessels with an AMPK activator enhanced (additive) dilation induced by PPARβ/δ, indicating a potential benefit in pulmonary arterial hypertension (PAH). In summary, my in vitro and in vivo experiments using mice lacking COX-1 or COX-2 provide insight into the role of COX in immunity and the pulmonary vasculature.
Additional file 1: of Resurrection of Nalidixic Acid: Evaluation of Water-Based Nanoformulations as Potential Nanomedicine
Creators: name: Pandey, Alka
name: Aggarwal, Nisha
name: Adholeya, Alok
name: Mandira Kochar
Publisher: name: figshare
Year: 2018
Subjects: subject: Biochemistry
subject: Space Science
subject: Medicine
subject: Microbiology
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Pharmacology
subject: Biotechnology
subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences
subject: Immunology
subject: FOS: Clinical medicine
subject: 69999 Biological Sciences not elsewhere classified
subject: Cancer
subject: Hematology
subject: 110309 Infectious Diseases
subject: FOS: Health sciences

description: Figure S1. Synthetic scheme. Figure S2. Particle size distribution of nanoformulations: a) NF 1, b) NF 2, c) NF 3, d) NF 4, d) NF 5, e) NF 6, f) NF 7 and g) NF 8. Figure S3. TEM images of nanoformulation a) NF1, b) NF2, c) NF3, d) NF4 and e) NF5 after 3 months storage at room temperature (representative images shown, scale bar is shown at the bottom left corner of each figure and varied between 20 nm to 100 nm). Figure S4. Antibacterial activity of nanoformulations and non-nano derivatives against bacillus subtilis using CFU per mL. a) 800, b) 400, c) 200, d) 100, e) 50μgmL1 and f) Control. Figure S5. Antibacterial activity of nanoformulations and non-nano derivatives against Acinetobacter baumannii using CFU per mL. a) 800, b) 400, c) 200, d) 100, e) 50μgmL− 1 and f) Control. Figure S6. Anticandida activity of nanoformulations (NF) along with their non-nano derivatives (NN) showing zone of inhibition at each test concentration in μgmL− 1. Table S1a Stability of prepared nanoformulations stored at 4 °C. Table S1b. Stability of prepared nanoformulations stored at 25 °C. Table S2. Net change in OD (average of 3 readings) at 570 nm after 18 h of exposure to nanoformulations on Staphylococcus aureus. Table S3. Net change in OD (average of 3 readings) at 570 nm after 18 h of exposure to nanoformulations on Bacillus subtilis. Table S4. Net change in OD (average of 3 readings) at 570 nm after 18 h of exposure to nanoformulations on Pseudomonas aeruginosa. Table S5. Net change in OD (average of 3 readings) at 570 nm after 18 h of exposure to nanoformulations on Acinetobacter baumannii. (DOCX 14298 kb)
Radiatively Driven Mass Accretion onto Galactic Nuclei by Circumnuclear Starbursts
Creators: name: Umemura, Masayuki
name: Fukue, Jun
name: Mineshige, Shin
Publisher: name: arXiv
Year: 1998
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We examine the radiatively driven mass accretion onto galactic nuclei due to the intensive radiation from circumnuclear starbursts. The radiation from a starburst not only contracts an inner gas disk by the radiation flux force, but also extracts angular momenta due to the relativistic radiation drag, thereby inducing an avalanche of the surface layer of disk. The present radiatively driven mass accretion may provide a physical mechanism which enables mass accretion from 100 pc scales down to pc, and it can eventually link to an advection-dominated viscous accretion onto a massive black hole. The radiation-hydrodynamical and self-gravitational instabilities of the disk are briefly discussed. In particular, the radiative acceleration possibly builds up a dusty wall, which provides another version for the formation of an obscuring torus.
description: 25 Pages, Latex, 6 figures, accepted by MNRAS, email:umemura@rccp.tsukuba.ac.jp
Calcium-driven In Silico Inactivation of a Human Olfactory Receptor
Creators: name: Pirona, Lorenza
name: Ballabio, Federico
name: Alfonso-Prieto, Mercedes
name: Capelli, Riccardo
Publisher: name: Forschungzentrum Jülich
Year: 2024
Subjects: subject: 570

description: bioRxiv beta (2024). doi:10.1101/2024.01.31.578070
description: Conformational changes as well as molecular determinants related to the activation and inactivation of olfactory receptors are still poorly understood due to the intrinsic difficulties in the structural determination of this GPCR family. Here, we perform, for the first time, the in silico inactivation of the human olfactory receptor OR51E2, highlighting the possible role of calcium in this receptor state transition. Using molecular dynamics simulations, we show that a divalent ion in the ion binding site, coordinated by two acidic residues at positions 2.50 and 3.39 conserved across most ORs, stabilizes the receptor in its inactive state. In contrast, protonation of the same two acidic residues is not sufficient to drive inactivation within the µs timescale of our simulations. Our findings suggest a novel molecular mechanism for OR inactivation, potentially guiding experimental validation and offering insights into the possible broader role of divalent ions in GPCR signaling.
description: Published by Cold Spring Harbor Laboratory, NY, Cold Spring Harbor
Archaeological representations in the media: the dominance of pseudo-Archeology
Creators: name: SCHIELE (Israel), ALEXANDRE
name: SCHIELE (Canada), BERNARD
Publisher: name: Review of Science, Mathematics and ICT Education
Year: 2022
Subjects: Science, pseudoscience, expert, media, television, media format

description: Contrary to a prevalent impression within the research community, pseudo-science is far from a marginal phenomenon, far from being a mere epiphenomenon in the mediascape. As this article shows, it constitutes a dominant trend since the 2010s, especially in historical and archeological television documentaries. These documentaries enjoy high ratings, which partly explains why producers continue to make them. Thus, omnipresent in the mediascape and beyond, they outcompete the scientific consensus and the worldview it projects, regardless of the debunking efforts of researchers and journalists. Furthermore, pseudoscience publications enjoy sales volumes that even the most renown researchers can only dream of. This omnipresence of pseudoscientific discourses in the social sphere transforms representations, increases beliefs in the paranormal and encourages conspiratorial mindsets. The comparative analysis of two documentaries: Lost World of the Maya (National Geographic) (NG) and Ancient Aliens©: Secret of the Maya (AA), has revealed a great number of similarities. Their format is identical, with the same number of segments, separated by synchronous commercial breaks of equal lengths (give or take a few seconds). If they somewhat differ in terms of treatment (AA proposes to uncover a conspiracy, and NG to solve an enigma) and the structure of the argumentation (AA: narration, assertion, speculation; NG: description, question, interpretation), they both show the same archetypal images of the Maya culture and mobilize the same enunciative modalities: a voice-over commentary ensures coherence throughout, interspaced with snippets from specifically invited “experts” whose task is to illustrate, specify, justify…. the overarching narrative. And yet, although many appear on screen, their speaking time is unequally distributed, with one (NG) or two (AA) speaking the most, and the others barely a minute each in total. Thus, their similarity is such that it is accurate to speak of variations within a media format. More precisely, we can only reaffirm Marshall McLuhan’s observation that “the medium is the message”, as, beyond the scientific or pseudoscientific narrative, the very dynamic of the media predominates, blurring the distinction between the two.
description: Review of Science, Mathematics and ICT Education, Forthcoming papers
Toughening mechanisms of block copolymer and graphene nanoplatelet modified epoxy polymers
Creators: name: Chong, Huang Ming
Publisher: name: Imperial College London
Year: 2015

description: Epoxies are thermosetting polymers that have uses in a multitude of industrial and consumer applications. The high crosslink density of epoxies gives rise to exceptional mechanical, chemical and heat resistance properties. However, this also results in low toughness, i.e. poor resistance to crack initiation and propagation. The present work discusses the toughening mechanisms of four epoxy polymers modified with several novel modifiers, which create different morphologies. Nanoscale core-shell rubber (CSR) particles are attractive as epoxy tougheners because they remain well dispersed even at high loadings, do not affect the Tg and most importantly, provide good toughness improvement (900% increase in GIC for a low Tg epoxy system). For a given weight percentage of modifiers, the tensile and compressive properties were better maintained for the much smaller CSR particles as these particles have a lower rubber content. However, the fracture performance of the CSR modified epoxies appear to be limited in low Tg epoxies. Examination of the fracture surfaces using high resolution scanning electron microscopy (SEM) show less plastic void growth due to the higher stresses required to initiate cavitation. Amphiphilic triblock copolymers (BCP) represent the next generation of phase separating materials for toughening epoxies. The structure/property relationships of epoxies modified with symmetric and asymmetric triblock copolymers were determined. The complex 3D nanostructures that were created offer greatly increased fracture performance over conventional toughening agents for very tough epoxies, while minimising the decrease in mechanical properties. A measured increase in GIC of 1600% was noted. This increased to 2250% when a further addition of silica nanoparticles was considered. This complex nanostructure allows for more gradual and extensive plastic deformation of the epoxy matrix as shear yielding and plastic void growth initiated by debonding at the BCP/epoxy interface. The morphology was further studied numerically using a phase field model which identified parameters that control the evolution of the microstructure. Graphene nanoplatelets (GNP) vary in size and quality depending on the method of preparation. Thus, a range of GNPs with different platelet sizes, thicknesses and aspect ratios were used to identify the properties that control the mechanical and fracture performance of GNP modified epoxies. The bulk GNP geometry and chemical makeup were first characterised. The optimum dispersion method was determined through systematic experiments using two solvents and an ultrasonic probe, and examined using SEM. Well dispersed GNPs improved the Young’s modulus, whereas the fracture energy increased for both well dispersed and poorly dispersed GNPs.
title: ADCO, Cartulaire de Cîteaux pour les domaines de Saint-Jean de Losne et Losne (XVIIIe siècle), Cart. 198-01 (11 H 1055), 185 folios, f. 0363
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/2019
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2020
Subjects: subject: cartulaire
subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris
subject: Corpus Burgundiae Medii Aevi
subject: Chartes de la Bourgogne du Moyen Âge

description: Cartulaire de Cîteaux pour les domaines de Saint-Jean de Losne et Losne (XVIIIe siècle), Archives départementales de la Côte-d'Or, Cart. 198-01 (11 H 1055), 185 folios, f. 0363, Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Cartulaire de Cîteaux pour les domaines de Saint-Jean de Losne et Losne (XVIIIe siècle), Archives départementales de la Côte-d'Or, Cart. 198-01 (11 H 1055), 185 folios, f. 0363, 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
Rhynchocorys orientalis Benth.
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
Lamiales
Orobanchaceae
Rhynchocorys
Rhynchocorys orientalis

description: Rhinanthus orientalis Linnaeus, Species Plantarum 2: 603. 1753.
"Habitat in Oriente." RCN: 4372.
Type not designated.
Original material: [icon] in Tournefort, Rel. Voy. Levant (Paris ed.) 2: 299. 1717.
Current name: Rhynchocorys orientalis (L.) Benth. (Scrophulariaceae).
description: Published as part of Jarvis, Charlie, 2007, Chapter 7: Linnaean Plant Names and their Types (part R), pp. 785-805 in Order out of Chaos. Linnaean Plant Types and their Types, London :Linnaean Society of London in association with the Natural History Museum on page 793, DOI: 10.5281/zenodo.291971
Additional File 4:
Creators: name: Thobani Ntshiqa
name: Musekiwa, Alfred
name: Mandla Mlotshwa
name: Mangold, Kerry
name: Reddy, Carl
name: Williams, Seymour
Publisher: name: figshare
Year: 2018
Subjects: subject: Medicine
subject: Sociology
subject: FOS: Sociology
subject: Computational Biology

description: Figure S3. Male condom use at last sex by marital status among the sexually active young women aged 16â 24Â years, National HIV Communication Survey, South Africa, 2012, Graphical presentation of male condom use by marital status using percentages, Male condom use by marital status. (DOCX 32 kb)
Additional file 5 of Whole-genome resequencing of three Coilia nasus population reveals genetic variations in genes related to immune, vision, migration, and osmoregulation
Creators: name: Gao, Jun
name: Xu, Gangchun
name: Xu, Pao
Publisher: name: figshare
Year: 2021
Subjects: subject: Genetics
subject: FOS: Biological sciences

description: Additional file 5.
Large-scale bias in the Universe II: redshift space bispectrum
Creators: name: Verde, Licia
name: Heavens, Alan F.
name: Matarrese, Sabino
name: Moscardini, Lauro
Publisher: name: arXiv
Year: 1998
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: The determination of the density parameter $Ω_0$ from the large-scale distribution of galaxies is one of the major goals of modern cosmology. However, if galaxies are biased tracers of the underlying mass distribution, linear perturbation theory leads to a degeneracy between $Ω_0$ and the linear bias parameter $b$, and the density parameter cannot be estimated. In Matarrese, Verde & Heavens (1997) we developed a method based on second-order perturbation theory to use the bispectrum to lift this degeneracy by measuring the bias parameter in an $Ω_0$-independent way. The formalism was developed assuming that one has perfect information on the positions of galaxies in three dimensions. In galaxy redshift surveys, the three-dimensional information is imperfect, because of the contaminating effects of peculiar velocities, and the resulting clustering pattern in redshift space is distorted. In this paper, we combine second-order perturbation theory with a model for collapsed, virialised structures, to extend the method to redshift space, and demonstrate that the method should be successful in determining with reasonable accuracy the bias parameter from state-of-the-art surveys such as the Anglo-Australian 2 degree field survey and the Sloan digital sky survey.
description: To appear in MNRAS
Reminiscences of Nan Tucker McEvoy 1967
Publisher: name: Columbia University
Year: 2019
Subjects: Journalists

description: Recollections of Adlai E. Stevenson: at San Francisco founding of United Nations, in Washington; national political conventions 1952; Democratic Advisory Council; 1956 campaign; 1960 campaign, failure to be appointed Secretary of State, acceptance of ambassadorship to United Nations; relationship between Stevenson and John F. Kennedy.
Secondary Episode of Star Formation in Elliptical Galaxies
Creators: name: Kodama, Tadayuki
name: Arimoto, Nobuo
Publisher: name: arXiv
Year: 1998
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We put upper limits of secondary burst of star formation in elliptical galaxies of the Gonzalez's (1993) sample, most of which locates in small groups, based on the colour dispersion around the U-V versus central velocity dispersion relation, and the equivalent width of Hbeta absorption. There are significant number of Hbeta strong galaxies which have EW(Hbeta)>2A, however they do not always have bluer colours in U-V. To be consistent with small colour dispersion of U-V, the mass fraction of secondary burst to the total mass should be less than only 10% at the maximum within recent 2Gyr. This result suggests that even if recent galaxy merging produce some ellipticals, it should not have been accompanied by an intensive star burst, and hence it could not involve large gas-rich systems. A capture of dwarf galaxy is more likely to explain dynamical disturbances observed in some elliptical galaxies. The above analysis based on the U-V is not compatible with the one based on the line indices, which requires that more than 10% of mass is present in a 2Gyr old star burst to cover the full range of the observed Hbeta (de Jong & Davies 1997). The discrepancy might be partly explained by the internal extinction localized at the region where young stars form. However, considering that the Hbeta index might have great uncertainties both in models and in observational data, we basically rely on U-V analysis.
description: 8 pages, 8 figures, Accepted for publication in MNRAS