cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
title: ADCO, Cartulaire de Cîteaux pour les domaines de Beaune (XVe siècle), Cart. 177 (11 H 289), 197 folios, f. 0033
Creators: name: de la Côte d'Or, Archives départementales
name: Archives Départementales De La Côte-D'Or
name: Petot, Frédérique
name: Projet CBMA
name: CG21/F.PETOT/2015
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2020
Subjects: subject: 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 Beaune (XVe siècle), Archives départementales de la Côte-d'Or, Cart. 177 (11 H 289), 197 folios, f. 0033, Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Cartulaire de Cîteaux pour les possessions d’Izeure (XVe siècle), Archives départementales de la Côte-d'Or, Cart. 177 (11 H 289), 197 folios, f. 0033, 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
The MEMO project: Combining all microlensing surveys to search for intermediate-mass Galactic black holes
Creators: name: Mirhosseini, Arash
name: Moniez, Marc
Publisher: name: arXiv
Year: 2017
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: The microlensing surveys MACHO, EROS, MOA and OGLE (hereafter called MEMO) have searched for microlensing toward the Large Magellanic Cloud for a cumulated duration of 27 years. We study the potential of joining these databases to search for very massive objects, that produce microlensing events with a duration of several years. We identified the overlaps between the different catalogs and compiled their time coverage to identify common regions where a joint microlensing detection algorithm can operate. We extrapolated a conservative global microlensing detection efficiency based on simple hypotheses, and estimated detection rates for multi-year duration events. Compared with the individual survey searches, we show that a combined search for long timescale microlensing should detect about ten more events caused by $100.M_{\odot}$ black holes if these objects have a major contribution to the Milky Way halo. Assuming that a common analysis is feasible, meaning that the difficulties that arise from using different passbands can be overcome, we show that the sensitivity of such an analysis might enable us to quantify the Galactic black hole component.
description: 5 pages, 4 figures. Accepted for publication in Astronomy & Astrophysics
Formation of freely floating sub-stellar objects via close encounters
Creators: name: Vorobyov, Eduard I.
name: Steinrueck, Maria
name: Elbakyan, Vardan
name: Guedel, Manuel
Publisher: name: arXiv
Year: 2017
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: FOS: Physical sciences

description: We numerically studied close encounters between a young stellar system hosting a massive, gravitationally fragmenting disk and an intruder diskless star with the purpose to determine the evolution of fragments that have formed in the disk prior to the encounter. Numerical hydrodynamics simulations in the non-inertial frame of reference of the host star were employed to simulate the prograde and retrograde co-planar encounters. The initial configuration of the target system (star plus disk) was obtained via a separate numerical simulation featuring the gravitational collapse of a solar-mass pre-stellar core. We found that close encounters can lead to the ejection of fragments that have formed in the disk of the target prior to collision. In particular, prograde encounters are more efficient in ejecting the fragments than the retrograde encounters. The masses of ejected fragments are in the brown-dwarf mass regime. They also carry away an appreciable amount of gas in their gravitational radius of influence, implying that these objects may possess extended disks or envelopes, as also suggested by Thies et al. (2015). Close encounters can also lead to the ejection of entire spiral arms, followed by fragmentation and formation of freely-floating objects straddling the planetary mass limit. However, numerical simulations with a higher resolution are needed to confirm this finding.
description: 12 pages, 7 figures, accepted for publication by Astronomy & Astrophysics
Additional file 1 of BTNET : boosted tree based gene regulatory network inference algorithm using time-course measurement data
Creators: name: Sungjoon Park
name: Kim, Jung Min
name: Wonho Shin
name: Han, Sung Won
name: Minji Jeon
name: Jang, Hyun Jin
name: Ik-Soon Jang
name: Jaewoo Kang
Publisher: name: figshare
Year: 2018
Subjects: 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: FOS: Biological sciences
subject: 80699 Information Systems not elsewhere classified
subject: FOS: Computer and information sciences
subject: 19999 Mathematical Sciences not elsewhere classified
subject: FOS: Mathematics

description: Supplementary file of BTNET. The file contains the URL of the source code and dataset used in this study, evaluation results on individual benchmark datasets and materials and methods used for the qualitative analysis. (PDF 263 kb)
Intensity speckle presents the density matrix of light
Creators: name: Lee, KyeoReh
name: Park, YongKeun
Publisher: name: arXiv
Year: 2017
Subjects: subject: Optics (physics.optics)
subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: We show that an intensity speckle can be directly interpreted as the properties of incident light - amplitude, phase, polarization, and coherency over spatial positions. Revisiting the speckle-correlation scattering matrix (SSM) method [Lee and Park, Nat. Comm. 7, 13359 (2016)], we successfully extract the intact information of incident light from an intensity speckle snapshot as the form of coherency matrix. The idea is verified experimentally by introducing the peculiar states of light that exhibit uneven amplitude, phase, polarization, and coherency features. We also find substantial practical advantage of the proposed method compared to the conventional coherency matrix measuring techniques such as Stokes polarimetry. We believe this physical interpretation of an intensity speckle could open a new avenue to study and to utilize the speckle phenomenon in vast subfields of wave physics.
Electrochemical Investigation of Slurry Electrode-Electrolyte for Electrical Energy Storage Systems
Creators: name: Sodiq, Ahmed
Publisher: name: Manara - Qatar Research Repository
Year: 2025
Subjects: classificationCode: 40
subject: Engineering

description: Electrical Energy Storage (EES) is projected to play an important role in the integration of large-scale renewable energy sources with electricity grid or off-grid. Grid-scale EES, particularly for renewable energy applications, has been a challenging task due to its high capital cost. Electrochemical-based EES systems, specifically redox flow batteries (RFBs) among other options, are uniquely suited for large-scale EES due to many advantages they have over conventional sealed batteries (e.g., lead-acid and Li-ion batteries). Flow batteries can meet a wide range of commercial-scale EES applications with varying power-to-energy ratios. Flow batteries have excellent energy efficiency and competitive life-cycle cost. The present work focuses on electrochemical investigations of slurry electrodes for flow cell (e.g. flow batteries) applications, aiming at improving the energy density of the system. The investigation includes; development of slurry electrode-electrolyte composites and slurry property characterization, electrochemical studies of slurry electrode-electrolyte (three-electrode cell configuration), cell design, subscale cell performance evaluation. The findings revealed that; in terms of conductivity, reduction of charge transfer resistance when carbon particles are dispersed in electrolyte/redox solution is mainly due to carbon nature. In addition, increase in carbon particles loading leads to increase in conductivity. The corrosion/carbon oxidation largely depends on the number of defect sites on carbon surfaces, which is directly related to carbon surface area (BET surface area). Among all the carbons studied, Black Pearls carbon demonstrated the best redox kinetics in V+2/V+3, V+4/V+5, Fe2+/Fe3+, and S2-/S0 redox couples. The kinetics of slurry electrodes in acid and alkaline media mainly depend on surface chemistries of the carbons. The performance of slurry electrodes at cell level is a function of; slurry conductivities, channel dimensions, slurry percolation (particle-to-particle interaction) and type of membrane.
RG flows with supersymmetry enhancement and geometric engineering
Creators: name: Giacomelli, Simone
Publisher: name: arXiv
Year: 2017
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: In this paper we study a class of $\mathcal{N}=2$ SCFTs with ADE global symmetry defined via Type IIB compactification on a class of hypersurfaces in $\mathbb{C}^3\times\mathbb{C}^*$. These can also be constructed by compactifying the 6d (2,0) theory of type ADE on a sphere with an irregular and a full punctures. When we couple to the ADE moment map a chiral multiplet in the adjoint representation and turn on a (principal) nilpotent vev for it, all the theories in this family display enhancement of supersymmetry in the infrared. We observe that all known examples of lagrangian theories which flow, upon the same type of deformation, to strongly coupled $\mathcal{N}=2$ theories fit naturally in our framework, thus providing a new perspective on this topic. We propose an infrared equivalence between this RG flow and a manifestly $\mathcal{N}=2$ preserving one and, as a byproduct, we extract a precise prescription to relate the SW curves describing the UV and IR fixed points for all theories with A or D global symmetry. We also find, for a certain subclass, a simple relation between UV and IR theories at the level of chiral algebras.
description: clarifications added, version published in JHEP
Relativity grupoid insted of relativity group
Creators: name: Oziewicz, Zbigmiew
Publisher: name: arXiv
Year: 2006
Subjects: subject: Category Theory (math.CT)
subject: Mathematical Physics (math-ph)
subject: FOS: Mathematics
subject: FOS: Physical sciences

description: Minkowski in 1908 used space-like binary velocity-field of a medium, relative to an observer. Hestenes in 1974 introduced, within a Clifford algebra, an axiomatic binary relative velocity as a Minkowski bivector. We propose consider binary relative velocity as a traceless nilpotent endomorphism in an operator algebra. Any concept of a binary axiomatic relative velocity made possible the replacement of the Lorentz relativity group by the relativity groupoid. The relativity groupoid is a category of massive bodies in mutual relative motions, where a binary relative velocity is interpreted as a categorical morphism with the associative addition. This associative addition is to be contrasted with non-associative addition of (ternary) relative velocities in isometric special relativity (loop structure). We consider an algebra of many time-plus-space splits, as an operator algebra generated by idempotents. The kinematics of relativity groupoid is ruled by associative Frobenius operator algebra, whereas the dynamics of categorical relativity needs the non-associative Frölicher-Richardson operator algebra. The Lorentz covariance is the cornerstone of physical theory. Observer-dependence within relativity groupoid, and the Lorentz-covariance (within the Lorentz relativity group), are different concepts. Laws of Physics could be observer-free, rather than Lorentz-invariant.
description: 10 p., invitated lecture presented at the 42nd Karpacz Winter School of Theoretical Physics, Ladek, Poland, 6-11 February 2006, "Current mathematical topics in gravitation and cosmology". Added references, title changed. Version to be published in IJGMMP
The Casimir effect for pistons with transmittal boundary conditions
Creators: name: Fucci, Guglielmo
Publisher: name: arXiv
Year: 2017
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: This work focuses on the analysis of the Casimir effect for pistons subject to transmittal boundary conditions. In particular we consider, as piston configuration, a direct product manifold of the type $I\times N$ where $I$ is a closed interval of the real line and $N$ is a smooth compact Riemannian manifold. By utilizing the spectral zeta function regularization technique, we compute the Casimir energy of the system and the Casimir force acting on the piston. Explicit results for the force are provided when the manifold $N$ is a $d$-dimensional ball.
description: 20 pages, LaTeX
Flight Lieutenant William Henry Buckley time spent in the RAF
Creators: name: Project Team, Their Finest Hour
Publisher: name: University of Oxford
Year: 2024
Subjects: classificationCode: 430304
subject: British history
classificationCode: 430308
subject: European history (excl. British, classical Greek and Roman)
classificationCode: 430316
subject: International history

description: This is the story of my Grandad and his time served in the RAF during World War 2 as an air gunner/wireless operator. It's from when he enlisted in August 1939 to his time with 425 Squadron up to 1944. He spent time in South East Asia with ACSEA, and family rumours say he spent time flying with Lord Mountbatten around South East Asia, but to this day, I can find no evidence of his time served there other than what his record says and his personal photos. Most importantly, there is the leather-bound signed photo of Lord and Lady Mountbatten.
The Protogalactic Origin for Cosmic Magnetic Fields
Creators: name: Kulsrud, Russell M.
name: Cen, Renyue
name: Ostriker, Jeremiah P.
name: Ryu, Dongsu
Publisher: name: arXiv
Year: 1996
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: It is demonstrated that strong magnetic fields are produced from a zero initial magnetic field during the pregalactic era, when galaxies are first forming. Their development proceeds in three phases. In the first phase, weak magnetic fields are created by the Biermann battery mechanism, acting in shocked parts of the intergalactic medium where caustics form and intersect. In the second phase, these weak magnetic fields are amplified to strong magnetic fields by the Kolmogoroff turbulence endemic to gravitational structure formation of galaxies. During this second phase, the magnetic fields reach saturation with the turbulent power, but they are coherent only on the scale of the smallest eddy. In the third phase, the magnetic field strength increases to equipartition with the turbulent energy, and the coherence length of the magnetic fields increases to the scale of the largest turbulent eddy, comparable to the scale of the entire galaxy. The resulting magnetic field represents a galactic magnetic field of primordial origin. No further dynamo action is necessary, after the galaxy forms, to explain the origin of magnetic fields. However, the magnetic field may be altered by dynamo action once the galaxy and the galactic disk have formed. It is first shown by direct numerical simulations, that thermoelectric currentsassociated with the Biermann battery, build the field up from zero to $10^{-21}$ G in the regions about to collapse into galaxies, by $z\sim3$. For weak fields, in the absence of dissipation, the cyclotron frequency ${\bf ω_{cyc}}=e{\bf B } /m_H c $ and $ {\bf ω}/(1+ χ)$, where ${\bf ω= \nabla \times v }$ is the vorticity and $χ$ is the degree of ionization, satisfy the same equations, and initial conditions ${\bf ω_{cyc}=ω}=0$, so that, ${\bf ω_{cyc}}({\bf
description: Princeton Univ Obs, submitted to ApJ
title: ADCO, Neuvième cartulaire de Saint-Étienne de Dijon (1661 - 1684), Cart. 32 (G 136), 745 folios, f. 1498
Creators: name: de la Côte d'Or, Archives départementales
name: Petot, Frédéric
name: Archives Départementales De La Côte-D'Or
name: Petot, Frédérique
name: Projet CBMA
name: CG21/F.PETOT/2012
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2020
Subjects: subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris
subject: cartulaire
subject: Corpus Burgundiae Medii Aevi
subject: Chartes de la Bourgogne du Moyen Âge

description: Neuvième cartulaire de Saint-Étienne de Dijon (1661 - 1684), Archives départementales de la Côte-d'Or, Cart. 32 (G 136), 745 folios, f. 1498, Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Neuvième cartulaire de Saint-Étienne de Dijon (1661 - 1684), Archives départementales de la Côte-d'Or, Cart. 32 (G 136), 745 folios, f. 1498, in Projet CBMA - Corpus Burgundiae Medii Aevi [Ressource en ligne], https:// manuscrits.cbma-project.eu/
description: Provenance: abbaye Saint-Étienne de Dijon
description: Provenance: http://www.wikidata.org/entity/Q15945019
Edmund Sydney White and Joyce Cornall Hinde
Creators: name: Project Team, Their Finest Hour
Publisher: name: University of Oxford
Year: 2024
Subjects: classificationCode: 430304
subject: British history
classificationCode: 430308
subject: European history (excl. British, classical Greek and Roman)
classificationCode: 430316
subject: International history

description: My father, Edmund Sydney White, was born in 1919 at Royal Farm, Eaton, Cheshire. His twin sister Dorothy died of diphtheria at 18 months old and all his life he felt that someone was missing. On the day war was declared, he went down to the bottom of the garden for a very sober contemplation as he knew he would be called up. He couldn't claim being in a reserved occupation as a farmer; the Depression meant that the farm could only support his two older brothers. He had never been further from home than Chester, 12 miles from his village. He said he felt a mixture of fear and excitement, as many young men must have done.He joined the Royal Engineers in December 1939 and was posted to 290 Army Troops Company in January 1940 (a Black Country-based Territorial Army unit). He was provisionally embarked for service in the Finnish-Soviet theatre of war, then speedily disembarked and reformed to proceed to the Western front as part of the British Expeditionary Force. After several months in France, he was evacuated in May 1940 after Dunkirk and redeployed in southern England (Aldershot), where the company was involved in a lot of engineering works including artificial landscape concealment from enemy air attack.In February 1941, the 290 ATC embarked for the Middle East, spending 14 weeks at sea, arriving at Port Tufic on the Suez Canal, before proceeding to Palestine and the Syrian campaign. He became a driver and remembered seeing a man in Arab dress and blue eyes herding goats. He slowed down, whereupon the man addressed him in a perfect Etonian accent, telling him "Move on, soldier." A spy? He attended the Middle East School of Hygiene, attaining distinction for camp layout and water treatment. He told me (his daughter) that the main thing he had to test water for was bilharzia.He served in Italy from 1943 to 1945, building bridges, and it was here he caught malaria, which lingered after the war. He remembered stopping in Cape Town on the way back to Italy and a lady on the quay singing Gracie Fields songs to the troops, and the wonderful welcome and hospitality in homes the soldiers were shown. Who was this lady who has been mentioned in other accounts? He also remembered the final journey home through France in spring 1945, with all the wild flowers blooming and girls waving white handkerchiefs at the train—it was a wonderful feeling, to be going home after six years.
Unveiling the bosonic nature of an ultrashort few-electron pulse
Creators: name: Roussely, Gregoire
name: Arrighi, Everton
name: Georgiou, Giorgos
name: Takada, Shintaro
name: Schalk, Martin
name: Urdampilleta, Matias
name: Ludwig, Arne
name: Wieck, Andreas D.
name: Armagnat, Pacome
name: Kloss, Thomas
name: Waintal, Xavier
name: Meunier, Tristan
name: Bauerle, Christopher
Publisher: name: arXiv
Year: 2017
Subjects: subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: FOS: Physical sciences

description: Quantum dynamics is very sensitive to dimensionality. While two-dimensional electronic systems form Fermi liquids, one-dimensional systems -- Tomonaga-Luttinger liquids -- are described by purely bosonic excitations, even though they are initially made of fermions. With the advent of coherent single-electron sources, the quantum dynamics of such a liquid is now accessible at the single-electron level. Here, we report on time-of-flight measurements of ultrashort few-electron charge pulses injected into a quasi one-dimensional quantum conductor. By changing the confinement potential we can tune the system from the one-dimensional Tomonaga-Luttinger liquid limit to the multi-channel Fermi liquid and show that the plasmon velocity can be varied over almost an order of magnitude. These results are in quantitative agreement with a parameter-free theory and demonstrate a powerful new probe for directly investigating real-time dynamics of fractionalisation phenomena in low-dimensional conductors.
description: In v2 we added 11 pages of Supplementary Information. In v3 we updated the manuscript after it was peer-reviewed and published
Additional file 3: of Clinical evaluation of outdoor cats exposed to ectoparasites and associated risk for vector-borne infections in southern Italy
Creators: name: Persichetti, Maria
name: Pennisi, Maria
name: Vullo, Angela
name: Masucci, Marisa
name: Migliazzo, Antonella
name: Solano-Gallego, Laia
Publisher: name: figshare
Year: 2018
Subjects: subject: Space Science
subject: Medicine
subject: Microbiology
subject: FOS: Biological sciences
subject: Biotechnology
subject: 19999 Mathematical Sciences not elsewhere classified
subject: FOS: Mathematics
subject: 60506 Virology
subject: Computational Biology

description: Table S3. Ordered logistic regression analysis of VBP. (DOCX 14 kb)
Categorizing and mapping the media landscape of children and adolescents - a scoping review - preregistration
Creators: name: Denessen, Eddie J.P.G.
name: Scholten, Hanneke
name: De Ruyter, Sara
name: J.A.M., Alexander
Publisher: name: Open Science Framework
Year: 2023
Subjects: subject: Social and Behavioral Sciences
subject: media
subject: children
subject: media landscape
subject: adolescents

description: This scoping review will give an overview of existing categorizations of the media landscape for children and adolescents. In addition, it will map the media included in the current media landscape of children and adolescents.
On the Influence of Momentum Conservation upon the Scaling Behaviour of Factorial Moments in High Energy Multiparticle Production
Creators: name: Lianshou, Liu
name: Yang, Zhang
name: Yue, Deng
Publisher: name: arXiv
Year: 1996
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: The experimental results on the falling down of scaled factorial moments in azimuthal variable $ϕ$ is studied in some detail. It is shown that this phenomenon may be referred to the influence of transverse momentum conservation. The existing experimental data from DELPHI, EMU08, NA22 and UA1 are successfully explained. Various methods are proposed to partly eliminate this influence and rule out the 'falling down' of factorial moments.
description: Latex, 8 pages, 6 figures in 3 PS files, to appear in Z. Phys. C
Analytical Approximations to the Low-Order Statistics of Dark Matter Distribution
Creators: name: Mo, H. J.
name: Jing, Y. P.
name: Börner, G.
Publisher: name: arXiv
Year: 1996
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We show that in a hierarchical clustering model the low-order statistics of the density and the peculiar velocity fields can all be modelled semianalytically for a given cosmology and an initial density perturbation power spectrum $P(k)$. We present such models for the two-point correlation function $ξ(r)$, the amplitude $Q$ of the three-point correlation function, the mean pairwise peculiar velocity $< v_{12}(r)> $, the pairwise peculiar velocity dispersion $< v_{12}^2(r)>$, and the one-point peculiar velocity dispersion $< v_1^2 >$. We test our models against results derived from N-body simulations. These models allow us to understand in detail how these statistics depend on $P(k)$ and cosmological parameters. They can also help to interpret, and maybe correct for, sampling effects when these statistics are estimated from observations. The dependence of the small-scale pairwise peculiar velocity dispersion on rich clusters in the sample, for instance, can be studied quantitatively. There are also significant implications for the reconstruction of the cosmic density field from measurements in redshift space.
description: 32 pages, Latex, aaspp4.sty, 7 figs included, revised version to appear in MNRAS. In this version, a simple fitting formula is given for the pairwise peculiar velocity dispersion
Using planetary transits to estimate magnetic cycles lengths in Kepler stars
Creators: name: Estrela, Raissa
name: Valio, Adriana
Publisher: name: arXiv
Year: 2017
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: FOS: Physical sciences

description: Observations of various solar-type stars along decades revealed that they can have magnetic cycles, just like our Sun. An investigation of the relation between their cycle length and rotation period can shed light on the dynamo mechanisms operating in these stars. Previous works on this relation suggested that the stars could be separated into active and inactive branches, with the Sun falling between them. In this work, we determined short magnetic activity cycles for 6 active solar-type stars observed by the Kepler telescope. The method adopted here estimates the activity from the excess in the residuals of the transitlight curves. This excess is obtained by subtracting a spotless model transit from the light curve, and then integrating over all the residuals during the transit. The presence of long term periodicity is estimated from the analysis of a Lomb-Scargle periodogram of the complete time series. Finally, we investigate the rotation-cycle period relation for the stars analysed here and find that some active stars do not follow the behaviour proposed earlier, falling in the inactive branch. In addition, we also notice a considerable spread from other stars in the literature in the active/inactive branches.
description: 8 pages, 4 figures, Proceedings of the IAU Symposium No. 328: "Living Around Active Stars"
Additional file 4: of Hydrological features and the ecological niches of mammalian hosts delineate elevated risk for Ross River virus epidemics in anthropogenic landscapes in Australia
Creators: name: Walsh, Michael
name: Webb, Cameron
Publisher: name: figshare
Year: 2018
Subjects: subject: Evolutionary Biology
subject: FOS: Biological sciences
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
subject: 60506 Virology

description: Table S1. Description of the ecologic niche models for each of the predicted species distributions for mammalian hosts. (DOCX 15 kb)
QCD Sum-Rule Calculation of the Kinetic Energy and Chromo-Interaction of Heavy Quarks Inside Mesons
Creators: name: Neubert, Matthias
Publisher: name: arXiv
Year: 1996
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We present a QCD sum-rule determination of the heavy-quark kinetic energy inside a heavy meson, $-λ_1/2 m_Q$, which is consistent with the field-theory analog of the virial theorem. We obtain $-λ_1\approx (0.10\pm 0.05)~\mbox{GeV}^2$, significantly smaller than a previous sum-rule result, but in good agreement with recent determinations from the analysis of inclusive decays. We also present a new determination of the chromo-magnetic interaction, yielding $λ_2(m_b)=(0.15\pm 0.03)~\mbox{GeV}^2$. This implies $m_{B^*}^2-m_B^2=(0.60\pm 0.12)~\mbox{GeV}^2$, in good agreement with experiment. As a by-product of our analysis, we derive the QCD sum rules for the three form factors describing the meson matrix element of a velocity-changing current operator containing the gluon field-strength tensor.
description: 13 pages LaTeX (A4), 3 figures
Dispersion Measure Variation of Repeating Fast Radio Burst Sources
Creators: name: Yang, Yuan-Pei
name: Zhang, Bing
Publisher: name: arXiv
Year: 2017
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: The repeating fast radio burst (FRB) 121102 was recently localized in a dwarf galaxy at a cosmological distance. The dispersion measure (DM) derived for each burst from FRB 121102 so far has not shown significant evolution, even though an apparent increase was recently seen with newly detected VLA bursts. It is expected that more repeating FRB sources may be detected in the future. In this work, we investigate a list of possible astrophysical processes that might cause DM variation of a particular FRB source. The processes include (1) the cosmological scale effects such as Hubble expansion and large-scale structure fluctuations; (2) the FRB local effects such as gas density fluctuation, expansion of a supernova remnant, a pulsar wind nebula, and an HII region; and (3) the propagation effect due to plasma lensing. We find that the DM variations contributed by the large-scale structure are extremely small, and any observable DM variation is likely caused by the plasma local to the FRB source. Besides mechanisms that produce decreasing DM with time, we suggest that an FRB source in an expanding supernova remnant around a nearly neutral ambient medium during the deceleration (Sedov-Taylor and snowplow) phases or in a growing HII region can introduce DM increasing. Some effects (e.g. an FRB source moving in an HII region or plasma lensing) can give either positive or negative DM variations. Future observations of DM variations of FRB 121102 and other repeating FRB sources can bring important clues for the physical origin of these sources.
description: 12 pages. Accepted for publication in ApJ
title:  Opportunità e limiti dell’autonomia privata. Tra diritto comparato e D.I.P
Creators: name: Carbone, Sergio M.
Publisher: name: RomaTrE-Press
Year: 2018

description: L’articolo analizza, nella prospettiva del diritto internazionale privato, il ruolo della autonomia privata nella scelta del diritto applicabile ai contratti internazionali, con particolare riferimento alle controversie e alla esecuzione dei lodi arbitrali.
description: Dialoghi con Guido Alpa. Un volume offerto in occasione del suo LXXI compleanno
Origins of the Ambient Solar Wind: Implications for Space Weather
Creators: name: Cranmer, Steven R.
name: Gibson, Sarah E.
name: Riley, Pete
Publisher: name: arXiv
Year: 2017
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: The Sun's outer atmosphere is heated to temperatures of millions of degrees, and solar plasma flows out into interplanetary space at supersonic speeds. This paper reviews our current understanding of these interrelated problems: coronal heating and the acceleration of the ambient solar wind. We also discuss where the community stands in its ability to forecast how variations in the solar wind (i.e., fast and slow wind streams) impact the Earth. Although the last few decades have seen significant progress in observations and modeling, we still do not have a complete understanding of the relevant physical processes, nor do we have a quantitatively precise census of which coronal structures contribute to specific types of solar wind. Fast streams are known to be connected to the central regions of large coronal holes. Slow streams, however, appear to come from a wide range of sources, including streamers, pseudostreamers, coronal loops, active regions, and coronal hole boundaries. Complicating our understanding even more is the fact that processes such as turbulence, stream-stream interactions, and Coulomb collisions can make it difficult to unambiguously map a parcel measured at 1 AU back down to its coronal source. We also review recent progress -- in theoretical modeling, observational data analysis, and forecasting techniques that sit at the interface between data and theory -- that gives us hope that the above problems are indeed solvable.
description: Accepted for publication in Space Science Reviews. Special issue connected with a 2016 ISSI workshop on "The Scientific Foundations of Space Weather." 44 pages, 9 figures
Versality of the relative Fukaya category
Creators: name: Sheridan, Nick
Publisher: name: arXiv
Year: 2017
Subjects: subject: Symplectic Geometry (math.SG)
subject: FOS: Mathematics

description: Seidel introduced the notion of a Fukaya category `relative to an ample divisor', explained that it is a deformation of the Fukaya category of the affine variety that is the complement of the divisor, and showed how the relevant deformation theory is controlled by the symplectic cohomology of the complement. We elaborate on Seidel's definition of the relative Fukaya category, and give a criterion under which the deformation is versal.
description: 138 pages, minor changes
Additional file 2: of Clinical evaluation of outdoor cats exposed to ectoparasites and associated risk for vector-borne infections in southern Italy
Creators: name: Persichetti, Maria
name: Pennisi, Maria
name: Vullo, Angela
name: Masucci, Marisa
name: Migliazzo, Antonella
name: Solano-Gallego, Laia
Publisher: name: figshare
Year: 2018
Subjects: subject: Medicine
subject: Biotechnology
subject: 59999 Environmental Sciences not elsewhere classified
subject: FOS: Earth and related environmental sciences
subject: 19999 Mathematical Sciences not elsewhere classified
subject: FOS: Mathematics
subject: 110309 Infectious Diseases
subject: FOS: Health sciences
subject: 60506 Virology
subject: FOS: Biological sciences
subject: Computational Biology

description: Table S2. Serum biochemistry reference intervals. (DOCX 15 kb)
The Ellipticity and Orientation of Clusters of Galaxies from N-Body Experiments
Creators: name: Splinter, Randall J.
name: Melott, Adrian L.
name: Linn, Angela
name: Buck, Charles
name: Tinker, Jeremy
Publisher: name: arXiv
Year: 1996
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: In this study we use simulations of 128$^3$ particles to study the ellipticity and orientation of clusters of galaxies in N-body simulations of differing power-law initial spectra (P(k) \propto k^n ,n = +1, 0, -1, -2$), and density parameters ($Ω_0 = 0.2$ to 1.0). Furthermore, unlike most theoretical studies we mimic most observers by removing all particles which lie at distances greater than 2 1/h Mpc from the cluster center of mass. We computed the axial ratio and the principal axes using the inertia tensor of each cluster. The mean ellipticity of clusters increases strongly with increasing $n$. We also find that clusters tend to become more spherical at smaller radii. We compared the orientation of a cluster to the orientation of neighboring clusters as a function of distance (correlation). In addition, we considered whether a cluster's major axis tends to lie along the line connecting it to a neighboring cluster, as a function of distance (alignment). Both alignments and correlations were computed in three dimensions and in projection to mimic observational surveys. Our results show that significant alignments exist for all spectra at small separations ($D < 15 h^{-1}$ Mpc) but drops off at larger distance in a strongly $n-$dependent way.
description: 22 pages, requires aaspp4.sty, flushrt.sty, and epsf.sty Revised manuscript, accepted for publication in ApJ
ความสัมพันธ์ระหว่างความรอบรู้ด้านสุขภาพกับพฤติกรรมการรับประทานยาและการมาตรวจตามนัดของผู้ป่วยโรคเบาหวานและโรคความดันโลหิตสูงในจังหวัดลำพูน
Creators: name: เอกชัย ชัยยาทา
name: ลภัสรดา หนุ่มคำ
name: ณิชมน รักกะเปา
Publisher: name: กองบริหารการวิจัย
Year: 2563
Subjects: ความรอบรู้ด้านสุขภาพ
พฤติกรรมการรับประทานยา
การมาตรวจตามนัด
โรคเรื้อรัง
เบาหวาน
ความดันโลหิตสูง

description: วารสารวิทยาศาสตร์และเทคโนโลยี, 28, 1, 182-196
The optimal particle-mesh interpolation basis
Creators: name: Wang, Han
name: Fang, Jun
name: Gao, Xingyu
Publisher: name: arXiv
Year: 2017
Subjects: subject: Chemical Physics (physics.chem-ph)
subject: Computational Physics (physics.comp-ph)
subject: FOS: Physical sciences

description: The fast Ewald methods are widely used to compute the point-charge electrostatic interactions in molecular simulations. The key step that introduces errors in the computation is the particle-mesh interpolation. In this work, the optimal interpolation basis is derived by minimizing the estimated error of the fast Ewald method. The basis can be either general or model specific, depending on whether or not the charge correlation has been taken into account. By using the TIP3P water as an example system, we demonstrate that the general optimal basis is always more accurate than the B-spline basis in the investigated parameter range, while the computational cost is at most 5\% more expensive. In some cases, the optimal basis is found to be two orders of magnitude more accurate. The model specific optimal basis further improves the accuracy of the general optimal basis, but requires more computational effort in the optimization, and may not be transferable to systems with different charge correlations. Therefore, the choice between the general and model specific optimal bases is a trade-off between the generality and the accuracy.
Little People in British Children's Books during the Cold War
Creators: name: Dubosarksy, Ursula
Publisher: name: Macquarie University
Year: 2024
Subjects: classificationCode: 399999
subject: Other education not elsewhere classified

description: This is a non-traditional thesis, comprising a research component and a creative component.
The research component is a study of works of British children's fiction published in the period 1945 to 1963 which all feature characters who, while otherwise being more or less ordinary human beings, are very small. A little person in art inevitably carries a variety of metaphoric and sometimes allegoric connotations, as found both in the recurring motif of the frequently magical little person in folk culture across the centuries and most famously in formal literature by Johnathan Swift in Gulliver's Travels (1726). In these mid-twentieth century works for children by T H White, Mary Norton, Rumer Godden and Helen Clare/Pauline Clarke, however, I argue that the post-1945 period of publication pivotally focused the metaphor so that the little person can be read as representing the perils and contradictions of belonging to a literal minority group within a dominant big culture. The little people here are versions of refugees diminished and displaced by trauma of war and persecution, standing like Paddington Bear on railway platforms, homeless, rootless and culturally anxious. The innocuous and fantastic miniature human becomes an almost secret metaphor to describe the consequences of war in the language and symbolism of children, and far more freely and indeed sometimes more grimly than writers of explicit war stories for children of the period.
The creative component is a novel, The Red Shoe, published by Allen & Unwin (2006). It concerns a family of three young daughters in Sydney in 1954, set during an event known as the "Petrov Affair", when Soviet spies Vladimir and Evdokia Petrov defected to Australia in a sudden flare of international Cold War publicity. The novel is linked to the research component by the period of its setting, its exploration of the meaning of public political events in the private lives of children, and by featuring a little person, an insidious individual named Floreal. In my novel, however, Floreal is more oppressive than oppressed, embodying less his minority status than those disturbing aspects of creativity which all the texts in the study touch on, most fully and explicitly in Clarke's The Twelve and the Genii (1962), in which the little people, as playthings of children, are conduits or instruments of creative expression over which the creator appears at times to have little of no control. It was this reading of the metaphor which had for me, as a creative writer, the most particularly vivid and unsettling attraction.
Differential Dynamic Microscopy microrheology of soft materials: a tracking-free determination of the frequency-dependent loss and storage moduli
Creators: name: Edera, Paolo
name: Bergamini, Davide
name: Trappe, Véronique
name: Giavazzi, Fabio
name: Cerbino, Roberto
Publisher: name: arXiv
Year: 2017
Subjects: subject: Soft Condensed Matter (cond-mat.soft)
subject: FOS: Physical sciences

description: Particle tracking microrheology (PT-$μ$r) exploits the thermal motion of embedded particles to probe the local mechanical properties of soft materials. Despite its appealing conceptual simplicity, PT-$μ$r requires calibration procedures and operating assumptions that constitute a practical barrier to a wider adoption. Here we demonstrate Differential Dynamic Microscopy microrheology (DDM-$μ$r), a tracking-free approach based on the multi-scale, temporal correlation study of the image intensity fluctuations that are observed in microscopy experiments as a consequence of the motion of the tracers. We show that the mechanical moduli of an arbitrary sample are determined correctly in a wide frequency range, provided that the standard DDM analysis is reinforced with a novel, iterative, self-consistent procedure that fully exploits the multi-scale information made available by DDM. Our approach to DDM-$μ$r does not require any prior calibration, is in agreement with both traditional rheology and Diffusing Wave Spectroscopy microrheology, and works in conditions where PT-$μ$r fails, providing thus an operationally simple, calibration-free probe of soft materials.
description: 10 pages, 5 figures
A Possible Signal for QGP Formation from the Minimum-Bias Data of Relativistic Large Heavy Ion Collisions
Creators: name: Lianshou, Liu
name: Yuan, Hu
name: Yue, Deng
Publisher: name: arXiv
Year: 1996
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: It is argued that the experimentally observed strong upward-bending of the logarithm of factorial moments versus that of phase space partition number in the higher-dimensional phase space of nucleus-nucleus collisions is due to the superposition of elementary collision processes in these collisions. A direct implication of this observation is that, at high enough energy and/or density, when the produced particles from individual elementary processes are melted into a unique system the above-mentioned superposition effect will disappear and the factorial moments will not be strongly upward-bending any more. So, the disappearance of strong upward-bending of higher-dimensional factorial moments in heavy ion collision may be taken as a signal for the formation of a unique system, or QGP, in this collision.
description: 5 pages 3 Postscript figures, Latex
title: ADCO, Comptes du Petit-Cîteaux (1477-1491) (11 H 1179), f. 00461
Creators: name: de la Côte d'Or, Archives départementales
name: Petot, Frédéric
name: Archives Départementales De La Côte-D'Or
name: Archives Départementales De La Côte D'Or
name: Petot, Frédérique
name: Projet CBMA
name: CBMA/CG21/F.PETOT/2019
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2020
Subjects: subject: cartulaire
subject: comptes
subject: Corpus Burgundiae Medii Aevi
subject: Chartes de la Bourgogne du Moyen Âge
subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris

description: Comptes du Petit-Cîteaux (1477-1491), Archives départementales de la Côte-d'Or, (11 H 1179). Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Comptes du Petit-Cîteaux (1477-1491), Archives départementales de la Côte-d'Or, (11 H 1179), f. 00461, 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
Rumex maritimus Linnaeus, 1753, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1753
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Magnoliopsida
Polygonales
Polygonaceae
Rumex
Rumex maritimus

description: Rumex maritimus, spec. nov.
 8. Rumex floribus hermaphroditis: valvulis dentatis graniferis, foliis linearibus. Lech. scan. 26. It. scan. 248.
 Lapathum aquaticum, luteolae folio. Tournef. inst. 504.
 Lapathum aquaticum, angustissimo acuminato folio. Bocc. mus. 2. p. 142. t.104.
 Habitat in Europae litoribus maritimis.
description: Published as part of Linnaeus, Carolus, 1753, Species plantarum: exhibentes plantas rite cognitas, ad genera relatas, cum differentiis specificis, nominibus trivialibus, synonymis selectis, locis natalibus, secundum systema sexuale digestas, Stockholm :Laurentius Salvius on page 335, DOI: 10.5281/zenodo.3931989
Additional file 1: of Clinical evaluation of outdoor cats exposed to ectoparasites and associated risk for vector-borne infections in southern Italy
Creators: name: Persichetti, Maria
name: Pennisi, Maria
name: Vullo, Angela
name: Masucci, Marisa
name: Migliazzo, Antonella
name: Solano-Gallego, Laia
Publisher: name: figshare
Year: 2018
Subjects: subject: Medicine
subject: Biotechnology
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: 110309 Infectious Diseases
subject: FOS: Health sciences
subject: 60506 Virology
subject: Computational Biology

description: Table S1. Feline CBC reference intervals. (DOCX 15 kb)