cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Deutonura gisini Deharveng 1982
Creators: name: Thibaud, Jean-Marc
Publisher: name: Zenodo
Year: 2017
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Collembola
Poduromorpha
Neanuridae
Deutonura
Deutonura gisini

description: Deutonura gisini Deharveng, 1982 **
Deutonura gisini Deharveng, 1982b: 8.
DISTRIBUTION. — Gard. Conqueyrac, Les Claris (Deharveng 1982b).
description: Published as part of Thibaud, Jean-Marc, 2017, Catalogue des collemboles de France, pp. 297-436 in Zoosystema 39 (3) on page 320, DOI: 10.5252/z2017n3a1, http://zenodo.org/record/5496272
A multi-stop time-of-flight spectrometer for the measurement of positron annihilation-induced electrons in coincidence with the Doppler-shifted annihilation gamma photon
Creators: name: Chirayath, V. A.
name: Gladen, R. W.
name: McDonald, A. D.
name: Fairchild, A. J.
name: Joglekar, P. V.
name: Satyal, S.
name: Lim, Z. H.
name: Shead, T. N.
name: Chrysler, M. D.
name: Mukherjee, S.
name: Barnett, B. M.
name: Byrnes, N. K.
name: Koymen, A. R.
name: Greaves, R. G.
name: Weiss, A. H.
Publisher: name: arXiv
Year: 2020
Subjects: subject: Instrumentation and Detectors (physics.ins-det)
subject: Materials Science (cond-mat.mtrl-sci)
subject: FOS: Physical sciences

description: Here we describe an advanced multi functional, variable-energy positron beam system capable of measuring the energies of multiple positron-induced electrons in coincidence with the Doppler-shifted gamma photon resulting from the annihilation of the correlated positron. The measurements were carried out using the unique characteristics of the digital time-of-flight spectrometer and the gamma spectrometer available with the advanced positron beam system. These measurements have resulted in (i) the first digital time of flight spectrum of positron annihilation-induced Auger electrons generated using coincident signals from a high-purity Ge detector and a micro-channel plate; (ii) a two-dimensional array of the energy of Doppler-broadened annihilation gamma and the time of flight of positron-annihilation induced Auger electrons or secondary electrons measured in coincidence with the annihilation gamma photon; and (iii) the time of flight spectra of multiple secondary electrons ejected from a bilayer graphene surface as a result of the impact and(or) annihilation of positrons. The novelty of the gamma electron coincidence spectroscopy has been demonstrated by extracting the Doppler-broadened spectrum of gamma photons emitted due to the annihilation of positrons exclusively with 1s electrons of carbon. The width of the extracted Doppler-broadened gamma spectrum has been found to be consistent with the expected broadening of the annihilation gamma spectrum due to the momentum of the 1s electrons in carbon.
description: The following article has been submitted to Review of Scientific Instruments. After it is published, it will be found at https://publishing.aip.org/resources/librarians/products/journals/
Clytia paulensis
Creators: name: Galea, Horia R.
Publisher: name: Zenodo
Year: 2007
Subjects: Biodiversity
Taxonomy
Animalia
Cnidaria
Hydrozoa
Leptothecata
Campanulariidae
Clytia
Clytia paulensis

description: Clytia paulensis (Vanhöffen, 1910)
(fig. 20J–L, table 38)
 Campanularia paulensis Vanhöffen, 1910: 272, 298, fig. 19A–B.
 Clytia ? paulensis: Stechow, 1919: 45.
 Clytia paulensis: Stechow, 1923: 110, fig. N; Calder, 1971: 51, pl. 3I; Millard, 1975: 221, fig. 73A–D; Cornelius, 1982: 88, fig. 14; Gili et al., 1989: 106, fig. 31A; Ramil & Vervoort, 1992: 239, fig. 67C–D; Cornelius, 1995b: 258, fig. 59; Hirohito, 1995 (English text): 68, fig. 20A–B, pl. 4 fig. D; Ramil et al., 1998a: 199; Medel & Vervoort, 2000: 39; Peña Cantero & García Carrascosa, 2002: 152, fig. 29A–C; Bouillon et al., 2004: 196, fig. 100F–J; Calder & Kirkendale, 2005: 486; Vervoort, 2006: 271.
 Material examined. Stn. MEL 02 —06.iii. 2005, 15 m, S81: several fertile colonies, epizoic on Symplectoscyphus filiformis and Obelia dichotoma; S78: one sterile colony, epizoic on Symplectoscyphus subdichotomus (MHNG INVE 53274). Stn. MEL 03 —08.iii.2005, 20– 30 m, S90: small, infertile colony, epizoic on Symplectoscyphus filiformis.
 Type locality. Saint Paul, southern Indian Ocean.
 Remarks. The present material from Chile agrees well with the redescription provided by Ramil & Vervoort (1992) and needs no further comment. An extensive synonymy of this species is given in Medel & Vervoort (2000). The medusa stage is still undescribed (Cornelius 1995b).
 World distribution. Temperate to warm-waters of Atlantic and Indo-Pacific Oceans (Medel & Vervoort 2000, Vervoort 2006).
 Records from Chile. The present material was collected around Melinka, Guaitecas Archipelago. This is the first record of the species for Chile.
description: Published as part of Galea, Horia R., 2007, Hydroids and hydromedusae (Cnidaria: Hydrozoa) from the fjords region of southern Chile, pp. 1-116 in Zootaxa 1597 (1) on pages 89-90, DOI: 10.11646/zootaxa.1650.1.4, http://zenodo.org/record/5097970
Deutonura inopinata Deharveng 1979
Creators: name: Thibaud, Jean-Marc
Publisher: name: Zenodo
Year: 2017
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Collembola
Poduromorpha
Neanuridae
Deutonura
Deutonura inopinata

description: Deutonura inopinata Deharveng, 1979 **
Deutonura inopinata Deharveng, 1979a: 30.
DISTRIBUTION. — Tarn. Forêtdela Grésigne (Deharveng 1979a).
description: Published as part of Thibaud, Jean-Marc, 2017, Catalogue des collemboles de France, pp. 297-436 in Zoosystema 39 (3) on page 321, DOI: 10.5252/z2017n3a1, http://zenodo.org/record/5496272
A Diffusion-Based Embedding of the Stochastic Simulation Algorithm in Continuous Space
Creators: name: Thomas, Marcus
name: Schwartz, Russell
Publisher: name: arXiv
Year: 2020
Subjects: subject: Chemical Physics (physics.chem-ph)
subject: Quantitative Methods (q-bio.QM)
subject: FOS: Physical sciences
subject: FOS: Biological sciences

description: A variety of simulation methodologies have been used for modeling reaction-diffusion dynamics -- including approaches based on Differential Equations (DE), the Stochastic Simulation Algorithm (SSA), Brownian Dynamics (BD), Green's Function Reaction Dynamics (GFRD), and variations thereon -- each offering trade-offs with respect to the ranges of phenomena they can model, their computational tractability, and the difficulty of fitting them to experimental measurements. Here, we develop a multiscale approach combining efficient SSA-like sampling suitable for well-mixed systems with aspects of the slower but space-aware GFRD model, assuming as with GFRD that reactions occur in a spatially heterogeneous environment that must be explicitly modeled. Our method extends the SSA approach in two major ways. First, we sample bimolecular association reactions following diffusive motion with a time-dependent reaction propensity. Second, reaction locations are sampled from within overlapping diffusion spheres describing the spatial probability densities of individual reactants. We show the approach to provide efficient simulation of spatially heterogeneous biochemistry in comparison to alternative methods via application to a Michaelis-Menten model.
Suppressing Roughness of Virtual Times in Parallel Discrete-Event Simulations
Creators: name: Korniss, G.
name: Novotny, M. A.
name: Guclu, H.
name: Toroczkai, Z.
name: Rikvold, P. A.
Publisher: name: arXiv
Year: 2003
Subjects: subject: Statistical Mechanics (cond-mat.stat-mech)
subject: Disordered Systems and Neural Networks (cond-mat.dis-nn)
subject: Distributed, Parallel, and Cluster Computing (cs.DC)
subject: Computational Physics (physics.comp-ph)
subject: FOS: Physical sciences
subject: FOS: Computer and information sciences

description: In a parallel discrete-event simulation (PDES) scheme, tasks are distributed among processing elements (PEs), whose progress is controlled by a synchronization scheme. For lattice systems with short-range interactions, the progress of the conservative PDES scheme is governed by the Kardar-Parisi-Zhang equation from the theory of non-equilibrium surface growth. Although the simulated (virtual) times of the PEs progress at a nonzero rate, their standard deviation (spread) diverges with the number of PEs, hindering efficient data collection. We show that weak random interactions among the PEs can make this spread nondivergent. The PEs then progress at a nonzero, near-uniform rate without requiring global synchronizations.
Additional file 3 of The effects of external Mn2+ concentration on hyphal morphology and citric acid production are mediated primarily by the NRAMP-family transporter DmtA in Aspergillus niger
Creators: name: Fejes, Balázs
name: Ouedraogo, Jean-Paul
name: Fekete, Erzsébet
name: Sándor, Erzsébet
name: Flipphi, Michel
name: Soós, Áron
name: Molnár, Ákos
name: Kovács, Béla
name: Kubicek, Christian
name: Tsang, Adrian
name: Karaffa, Levente
Publisher: name: figshare
Year: 2020
Subjects: subject: Biochemistry
subject: Microbiology
subject: FOS: Biological sciences
subject: Genetics
subject: Molecular Biology
subject: Pharmacology
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: Developmental Biology
subject: Cancer
subject: Inorganic Chemistry
subject: FOS: Chemical sciences

description: Additional file 3: Table S2: Aspergillus niger strains used in this study.
Selfsynchronization and dissipation-induced threshold in collective atomic recoil lasing
Creators: name: von Cube, C.
name: Slama, S.
name: Kruse, D.
name: Zimmermann, C.
name: Courteille, Ph. W.
name: Robb, G. R. M.
name: Piovella, N.
name: Bonifacio, R.
Publisher: name: arXiv
Year: 2004
Subjects: subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: Networks of globally coupled oscillators exhibit phase transitions from incoherent to coherent states. Atoms interacting with the counterpropagating modes of a unidirectionally pumped high-finesse ring cavity form such a globally coupled network. The coupling mechanism is provided by collective atomic recoil lasing (CARL), i.e. cooperative Bragg scattering of laser light at an atomic density grating, which is self-induced by the laser light. Under the rule of an additional friction force, the atomic ensemble is expected to undergo a phase transition to a state of synchronized atomic motion. We present the experimental investigation of this phase transition by studying the threshold behavior of the CARL process.
description: 4 pages, 3 figures
Magnetic fields in isolated and interacting white dwarfs
Creators: name: Ferrario, Lilia
name: Wickramasinghe, D. T.
name: Kawka, Adela
Publisher: name: arXiv
Year: 2020
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: The magnetic white dwarfs (MWDs) are found either isolated or in interacting binaries. They divide into two groups: a high field group (0.1-1,000MegaGauss) comprising some 13% of all white dwarfs (WDs), and a low field group (B<0.1MG) whose incidence is currently under investigation. The situation may be similar in magnetic binaries because the bright accretion discs in low field systems hide the photosphere of their WDs thus preventing the study of their magnetic fields' strength and structure. Considerable research has been devoted to the vexed question on the origin of magnetic fields. One hypothesis is that WD magnetic fields are of fossil origin. The other is that magnetic fields arise from binary interaction, through differential rotation, during common envelope evolution. The recently discovered population of hot, carbon-rich WDs exhibiting an incidence of magnetism of up to about 70% and a variability from a few minutes to a couple of days may support the merging binary hypothesis. Several studies have raised the possibility of the detection of planets around MWDs. Rocky planets may be discovered by the detection of anomalous atmospheric heating of the MWD. Planetary remains have recently revealed themselves in the atmospheres of about 25% of WDs that are polluted by elements such as Ca, Si, and often also Mg, Fe, Na. This pollution has been explained by ongoing accretion of planetary debris. The study of isolated and accreting MWDs is likely to continue to yield exciting discoveries for many years to come.
description: Invited, refereed review paper to appear in the COSPAR 2018 special issue of Advances in Space Research (Elsevier) entitled Nova Eruptions, Cataclysmic Variables and related systems: Observational vs. theoretical challenges in the 2020 era, 98 pages, 30 figures
Novel Families of Fractional Quantum Hall States: Pairing of Composite Fermions
Creators: name: Quinn, John J.
name: Wojs, Arkadiusz
name: Yi, Kyung-Soo
Publisher: name: arXiv
Year: 2003
Subjects: subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: FOS: Physical sciences

description: Fractional quantum Hall (FQH) states have recently been observed at unexpected values of the filling factor nu. Here we interpret these states as a novel family of FQH states involving pairing correlations rather than Laughlin correlations among the quasiparticles (QP's). The correlations depend upon the behavior of the QP-QP pseudopotential V_QP(L'), the interaction energy of a pair as a function of the pair angular momentum L'. This behavior, known from numerical studies of small systems, is used to demonstrate that pairing correlations give rise to FQH states at the experimentally observed values of nu.
description: to appear in Physics Letters A
MOESM1 of Discovery of the Agrobacterium growth inhibition sequence in virus and its application to recombinant clone screening
Creators: name: Yin, Jinlong
name: Liu, Hui
name: Xiang, Wenyang
name: Jin, Tongtong
name: Guo, Dongquan
name: Wang, Liqun
name: Zhi, Haijian
Publisher: name: figshare
Year: 2019
Subjects: subject: Space Science
subject: Medicine
subject: Microbiology
subject: FOS: Biological sciences
subject: Biotechnology
subject: Evolutionary Biology
subject: Biological Sciences not elsewhere classified
subject: Mathematical Sciences not elsewhere classified
subject: Infectious Diseases
subject: FOS: Health sciences
subject: Plant Biology
subject: Virology

description: Additional file 1: Table S1. Primers used for vectors construction. Figure S1. Phenotypes of Soybean cultivar Nannong 1138-2 leaves infected by different virus clones. Figure S2. Apply SC15P in efficient recombinant chones screening in Agrobacterium. Figure S3. P1 coding sequences alignment of three SMV strains.
Spectral Structures of Type II Solar Radio Bursts and Solar Energetic Particles
Creators: name: Iwai, Kazumasa
name: Yashiro, Seiji
name: Nitta, Nariaki V.
name: Kubo, Yuki
Publisher: name: arXiv
Year: 2019
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: Space Physics (physics.space-ph)
subject: FOS: Physical sciences

description: We investigated the relationship between the spectral structures of type II solar radio bursts in the hectometric and kilometric wavelength ranges and solar energetic particles (SEPs). To examine the statistical relationship between type II bursts and SEPs, we selected 26 coronal mass ejection (CME) events with similar characteristics (e.g., initial speed, angular width, and location) observed by the Large Angle and Spectrometric Coronagraph (LASCO), regardless of the characteristics of the corresponding type II bursts and the SEP flux. Then, we compared associated type II bursts observed by the Radio and Plasma Wave Experiment (WAVES) onboard the Wind spacecraft and the SEP flux observed by the Geostationary Operational Environmental Satellite (GOES) orbiting around the Earth. We found that the bandwidth of the hectometric type II bursts and the peak flux of the SEPs has a positive correlation (with a correlation coefficient of 0.64). This result supports the idea that the nonthermal electrons of type II bursts and the nonthermal ions of SEPs are generated by the same shock and suggests that more SEPs may be generated for a wider or stronger CME shock with a longer duration. Our result also suggests that considering the spectral structures of type II bursts can improve the forecasting accuracy for the peak flux of gradual SEPs.
description: 24 pages, 6 figures, accepted for publication in ApJ
Numerical verification of Beilinson's conjecture for K2 of hyperelliptic curves
Creators: name: Dokchitser, Tim
name: de Jeu, Rob
name: Zagier, Don
Publisher: name: arXiv
Year: 2004
Subjects: subject: Algebraic Geometry (math.AG)
subject: K-Theory and Homology (math.KT)
subject: Number Theory (math.NT)
subject: FOS: Mathematics
subject: 19E08, 11G40 (primary), 11G30 (secondary)

description: We construct families of hyperelliptic curves over Q of arbitrary genus g with (at least) g integral elements in K_2. We also verify the Beilinson conjectures about K_2 numerically for several curves with g=2, 3, 4 and 5. The paper is essentially self-contained and may serve as an elementary introduction to Beilinson's conjectures for K_2 of curves.
description: 39 pages; to appear in Compositio Math
Evolution of superconductivity and antiferromagnetic order in Ba(Fe$_{0.92-x}$Co$_{0.08}$V$_x$)$_2$As$_2$
Creators: name: Sheng, Jieming
name: Li, Xingguang
name: Tian, Congkuan
name: Song, Jianming
name: Li, Xin
name: Sun, Guangai
name: Xia, Tianlong
name: Wang, Jinchen
name: Liu, Juanjuan
name: Xu, Daye
name: Zhang, Hongxia
name: Tong, Xin
name: Luo, Wei
name: Wu, Liusuo
name: Bao, Wei
name: Cheng, Peng
Publisher: name: arXiv
Year: 2020
Subjects: subject: Superconductivity (cond-mat.supr-con)
subject: FOS: Physical sciences

description: The vanadium doping effects on superconductivity and magnetism of iron pnictides are investigated in Ba(Fe$_{0.92-x}$Co$_{0.08}$V$_x$)$_2$As$_2$ by transport, susceptibility and neutron scattering measurements. The doping of magnetic impurity V causes a fast suppression of superconductivity with T$_c$ reduced at a rate of 7.4~K/1\%V. On the other hand, the long-range commensurate $C$-type antiferromagnetic order is recovered upon the V doping. The value of ordered magnetic moments of Ba(Fe$_{0.92-x}$Co$_{0.08}$V$_x$)$_2$As$_2$ follows a dome-like evolution versus doping concentration x. A possible Griffiths-type antiferromagnetic region of multiple coexisting phases in the phase diagram of Ba(Fe$_{0.92-x}$Co$_{0.08}$V$_x$)$_2$As$_2$ is identified, in accordance with previous theoretical predictions based on a cooperative behavior of the magnetic impurities and the conduction electrons mediating the Ruderman-Kittel-Kasuya-Yosida interactions between them.
description: 6 pages, 5 figures
title: 02_0952
Creators: name: Wesley Baldwin, John
name: Baldwin, John W.
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2018
Subjects: subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris

description: L'ensemble de ces notes ont été crée par John Baldwin lors d'une de ses premières périodes de résidence à Paris. Ces documents comprennent tous les magistri qu’il avait pu rencontrer dans ses sources. Aux XIIème et XIIIème siècles, les universités n'existant pas encore, le titre de magister s'il évoque certainement une compétence n'est pas rattaché de façon systématique au passage par les écoles. De surcroît, les magistris sont le plus souvent désignés par leur seul prénom. La lecture de ces données est donc difficile et suppose un long travail pour tenter d'identifier un individu auquel on pourrait rattacher plusieurs mentions. John Baldwin avait donc renoncé à utiliser ces données pour donner un prolongement à sa magnifique étude sur les gradués d'université et leur emploi par les Capétiens et les Plantagenêts. Néanmoins, il a conservé ces données et elles sont potentiellement très utile dans le cadre de Studium, comme le sont toutes les mentions dans les volumes des Fasti Ecclesiae Gallicanae de chanoines portant ce titre de magister sans autres précisions. L'ampleur des dépouillements rend ces données très utiles et nous devons une grande reconnaissance à John Baldwin pour avoir pris la peine de faire photocopier ses fiches et de nous les avoir transmises amicalement.
Les données ainsi que les images des fiches sont accessibles sur le site Internet à l'adresse suivante : http://studium-baldwin.lamop.fr/.
Les transcriptions des fiches ont été effectuées par des étudiants de Paris 1 Panthéon - Sorbonne mais elles n'ont pas été corrigées par la suite.
description: Relation: https://lamop.hypotheses.org/
Ferroelectric ordering and electroclinic effect in chiral smectic liquid crystals
Creators: name: Fokin, Yu. G.
name: Murzina, T. V.
name: Aktsipetrov, O. A.
name: Soria, S.
name: Marowsky, G.
Publisher: name: arXiv
Year: 2003
Subjects: subject: Optics (physics.optics)
subject: FOS: Physical sciences

description: Ferroelectric ordering, the electroclinic effect and chiral smectic C (SmC*) - smectic A (SmA*) phase transitions in thin planar ferroelectric liquid crystal (FLC) cells are studied by means of linear electrooptic and second harmonic generation techniques. The ferroelectric switching is detected in biased FLC cells by measuring azimuthal dependences of linear and nonlinear responses. The applied DC-electric field rotates the FLC symmetry axis with initial and final orientations in the cell plane. Comparative studies of the switching behavior in reflection and transmission allows to distinguish the contributions from the bulk and the sub-surface layers of the cell. The analysis of temperature dependence shows the existence of a strong surface coupling. The temperature dependent nonlinear polarization shows a critical behavior corresponding to the superfluid model.
description: 6 pages, 4 figures
Cunina octonaria McCrady 1859
Creators: name: Galea, Horia R.
Publisher: name: Zenodo
Year: 2007
Subjects: Biodiversity
Taxonomy
Animalia
Cnidaria
Hydrozoa
Narcomedusae
Cuninidae
Cunina
Cunina octonaria

description: Cunina octonaria McCrady, 1859
(fig. 21O)
 Cunina octonaria McCrady, 1859: 211, pl. 12 fig 4–5; Kramp, 1959: 199, fig. 307; 1961: 282; 1968: 128, fig. 347; Calder, 1971: 77, pl. 8I; Goy et al., 1991: 121, fig. 51; Bouillon et al., 2004: 234, figs 144E, 145A, 149A–H.
 Material examined. Plankton —off the Huinay Scientific Field Station, 18.ii.2006, 04.xi.2006, 45–0 m, two medusae, partly damaged (MHNG INVE 53569).
 Type locality. Charleston Harbor, South Carolina, USA.
 Remarks. For descriptions of this species, see Kramp (1959, 1968). The present material consists of two medusae, relatively poorly preserved, with the bell diameter of ca 2.3 mm.
 World distribution. This species is widely distributed in the warm parts of all oceans, including the Mediterranean (Kramp 1959).
 Records from Chile. The present specimens originate from fjord Comau. This is the first record of this species for Chile.
description: Published as part of Galea, Horia R., 2007, Hydroids and hydromedusae (Cnidaria: Hydrozoa) from the fjords region of southern Chile, pp. 1-116 in Zootaxa 1597 (1) on page 97, DOI: 10.11646/zootaxa.1650.1.4, http://zenodo.org/record/5097970
Anomalous thermal fluctuation distribution sustains proto-metabolic cycles and biomolecule synthesis
Creators: name: Ball, Rowena
name: Brindley, John
Publisher: name: arXiv
Year: 2019
Subjects: subject: Molecular Networks (q-bio.MN)
subject: FOS: Biological sciences

description: An environment far from equilibrium is thought to be a necessary condition for the origin and persistence of life. In this context we report open-flow simulations of a non-enzymic proto-metabolic system, in which hydrogen peroxide acts both as oxidant and driver of thermochemical cycling. We find that a Gaussian perturbed input produces a non-Boltzmann output fluctuation distribution around the mean oscillation maximum. Our main result is that net biosynthesis can occur under fluctuating cyclical but not steady drive. Consequently we may revise the necessary condition to "dynamically far from equilibrium".
description: 4 pages, 3 figures
Curation, Trust, and Impact: Making Social Science Research Transparent and Reproducible
Creators: name: Peer, Limor
name: Arguillas, Florio
name: Christian, Thu-Mai
Publisher: name: Zenodo
Year: 2021
Subjects: curation, reproducibility, transparency

description: The scientific enterprise, as a form of knowledge that can be applied to better the world, relies on public trust. That trust is earned in part because the scientific method is predicated on being open to scrutiny and primed for correction. With increased reliance on computation in every aspect of science and inquiry, there are more opportunities for close examination of the scientific record. Such examination depends on research practices as well as on the practices of those who are entrusted with keeping, logging, and stewarding the artifacts that comprise the scientific record. Data professionals, including curators, can help ensure the transparency and reproducibility of these artifacts, and shore up the public’s trust in science. In this lightning talk, we will explain why and how traditional curation and stewardship responsibilities must evolve to meet the moment. We will focus on the ways in which a transparency mindset informs curation practices that concretely enhance the quality of scientific artifacts. First, we frame the object of curation as the entirety of the data collection and analysis process, not only its component parts. That is, the activities that verify (to the extent possible) that statistical and analytic claims about given data can be reproduced with that data. Second, we explore how statistical and programming skills can be useful for curators and other data professionals. To illustrate, we will focus on the curation of social science research. The social sciences are concerned with understanding, and improving conditions for, society and individuals, and curation can contribute to public trust in this research by enhancing its transparency and reproducibility. Through a series of examples from social science research, we will highlight the skills and the actions data professionals bring to bear. We will also discuss the benefits reaped as a result of these actions – for science and society, as well as for the researchers and curators
Testing White Dwarf Crystallization Theory with Asteroseismology of the Massive Pulsating DA Star BPM 37093
Creators: name: Metcalfe, T. S.
name: Montgomery, M. H.
name: Kanaan, A.
Publisher: name: arXiv
Year: 2004
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: It was predicted more than 40 years ago that the cores of the coolest white dwarf stars should eventually crystallize. This effect is one of the largest sources of uncertainty in white dwarf cooling models, which are now routinely used to estimate the ages of stellar populations in both the Galactic disk and the halo. We are attempting to minimize this source of uncertainty by calibrating the models, using observations of pulsating white dwarfs. In a typical mass white dwarf model, crystallization does not begin until the surface temperature reaches 6000-8000 K. In more massive white dwarf models the effect begins at higher surface temperatures, where pulsations are observed in the ZZ Ceti (DAV) stars. We use the observed pulsation periods of BPM 37093, the most massive DAV white dwarf presently known, to probe the interior and determine the size of the crystallized core empirically. Our initial exploration of the models strongly suggests the presence of a solid core containing about 90% of the stellar mass, which is consistent with our theoretical expectations.
description: minor changes for length, accepted for ApJ Letters
A New Monomeric Interpretation of Intrinsic Optical Bistability Observed in Yb3+ - Doped Bromide Materials
Creators: name: Ciccarello, F.
name: Napoli, A.
name: Messina, A.
name: Luthi, S. R.
Publisher: name: arXiv
Year: 2003
Subjects: subject: Chemical Physics (physics.chem-ph)
subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: We present a mechanism able to show intrinsic bistable behaviour involving single Yb3+ ions embedded into bromide lattices, in which intrinsic optical bistability (IOB) has been observed. The mechanism is based on the experimentally found coupling between the Yb3+ ion and the totally symmetric local mode of vibration of the [YbBr6]3- coordination unit. The model reproduces the IOB observed in CsCdBr3:1% Yb3+ and allows to understand the experimentally found presence of the phenomenon in the other bromides, but its absence in Cs3Lu2Cl9:Yb3+.
description: 1 figure
Additional file 2 of The effects of external Mn2+ concentration on hyphal morphology and citric acid production are mediated primarily by the NRAMP-family transporter DmtA in Aspergillus niger
Creators: name: Fejes, Balázs
name: Ouedraogo, Jean-Paul
name: Fekete, Erzsébet
name: Sándor, Erzsébet
name: Flipphi, Michel
name: Soós, Áron
name: Molnár, Ákos
name: Kovács, Béla
name: Kubicek, Christian
name: Tsang, Adrian
name: Karaffa, Levente
Publisher: name: figshare
Year: 2020
Subjects: subject: Biochemistry
subject: Microbiology
subject: FOS: Biological sciences
subject: Genetics
subject: Molecular Biology
subject: Pharmacology
subject: Evolutionary Biology
subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences
subject: Ecology
subject: 69999 Biological Sciences not elsewhere classified
subject: Developmental Biology
subject: Inorganic Chemistry
subject: Plant Biology

description: Additional file 2: Table S1. Distribution of Mn2+ ions in a liquid culture of Aspergillus niger NRRL 2270.
THE ROLE OF KLOTHO IN INFLAMMATION AND VASCULAR CALCIFICATION IN CHRONIC KIDNEY DISEASE
Creators: name: Abdujabborov, Jamshidbek
name: Omonov, Jamshid
name: Tursunboev, Ulugbek
name: Kushboeva, Shabnam
name: Abdurakhmanova, Sayyora
Publisher: name: Zenodo
Year: 2025

description: Chronic Kidney Disease (CKD) is a progressive condition that significantly impacts renal function and leads to a variety of complications, including vascular calcification (VC) and fibrosis. Recent studies have highlighted the potential role of the klotho protein in mitigating some of these pathological processes. Klotho is an anti-aging protein that has been implicated in regulating various physiological functions, including mineral metabolism, oxidative stress, and inflammation. This mini-thesis explores the dual role of klotho in regulating inflammation via the NF-κB pathway and its contribution to preventing VC and renal fibrosis in CKD.
Real-Time Well Log Prediction From Drilling Data Using Deep Learning
Creators: name: Kanfar, Rayan
name: Shaikh, Obai
name: Yousefzadeh, Mehrdad
name: Mukerji, Tapan
Publisher: name: arXiv
Year: 2020
Subjects: subject: Geophysics (physics.geo-ph)
subject: Machine Learning (cs.LG)
subject: Applications (stat.AP)
subject: FOS: Physical sciences
subject: FOS: Computer and information sciences

description: The objective is to study the feasibility of predicting subsurface rock properties in wells from real-time drilling data. Geophysical logs, namely, density, porosity and sonic logs are of paramount importance for subsurface resource estimation and exploitation. These wireline petro-physical measurements are selectively deployed as they are expensive to acquire; meanwhile, drilling information is recorded in every drilled well. Hence a predictive tool for wireline log prediction from drilling data can help management make decisions about data acquisition, especially for delineation and production wells. This problem is non-linear with strong ineractions between drilling parameters; hence the potential for deep learning to address this problem is explored. We present a workflow for data augmentation and feature engineering using Distance-based Global Sensitivity Analysis. We propose an Inception-based Convolutional Neural Network combined with a Temporal Convolutional Network as the deep learning model. The model is designed to learn both low and high frequency content of the data. 12 wells from the Equinor dataset for the Volve field in the North Sea are used for learning. The model predictions not only capture trends but are also physically consistent across density, porosity, and sonic logs. On the test data, the mean square error reaches a low value of 0.04 but the correlation coefficient plateaus around 0.6. The model is able however to differentiate between different types of rocks such as cemented sandstone, unconsolidated sands, and shale.
Additional file 9: of Evaluating the profound effect of gut microbiome on host appetite in pigs
Creators: name: Yang, Hui
name: Yang, Ming
name: Fang, Shaoming
name: Huang, Xiaochang
name: He, Maozhang
name: Ke, Shanlin
name: Gao, Jun
name: Wu, Jinyuan
name: Zhou, Yunyan
name: Fu, Hao
name: Chen, Congying
name: Huang, Lusheng
Publisher: name: figshare
Year: 2018
Subjects: subject: Biochemistry
subject: Medicine
subject: Microbiology
subject: FOS: Biological sciences
subject: Genetics
subject: Ecology
subject: Biological Sciences not elsewhere classified
subject: Inorganic Chemistry
subject: FOS: Chemical sciences

description: Table S5. The ARRIVE Guidelines Checklist. (DOC 59 kb)
Structure functions of 2d integrable asymptotically free models
Creators: name: Balog, Janos
name: Weisz, Peter
Publisher: name: arXiv
Year: 2004
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We investigate structure functions in the 2--dimensional (asymptotically free) non--linear O$(n) σ$--models using the non--perturbative S--matrix bootstrap program. In particular the {\it exact small (Bjorken) $x$ behavior is exhibited}; the structure is rather universal and is probably the same in a wide class of (integrable) asymptotically free models. Structurally similar universal formulae may also hold for the small $x$ behavior of QCD in 4--dimensions. Structure functions in the special case of the $n=3$ model are accurately computed over the whole $x$ range for $-q^2/M^2<10^5$, and some moments are compared with results from renormalized perturbation theory. Some remarks concerning the structure functions in the $1/n$ approximation are also made.
description: 16 pages, 6 figures
Amphogona apicata Kramp 1957
Creators: name: Galea, Horia R.
Publisher: name: Zenodo
Year: 2007
Subjects: Biodiversity
Taxonomy
Animalia
Cnidaria
Hydrozoa
Trachymedusae
Rhopalonematidae
Amphogona
Amphogona apicata

description: Amphogona apicata Kramp, 1957
(fig. 21P, pl. 2P)
 Amphogona apicata Kramp, 1957: 59, pl. 5 fig. 7; 1959: 188, fig. 281; 1961: 252; 1968: 119, fig. 321; Palma et al., 2007: 70, 73.
 Material examined. Plankton — off the Huinay Scientific Field Station, 12–13.i.2006, 09.ii.2006, 04.xi.2006, 50–0 m, several medusae (MHNG INVE 49041).
 Type locality. Southern Atlantic and Mozambique Channel.
 Description. Umbrella bell-shaped, higher than wide (3.8 mm high and 2.75 mm in diameter), with a distinct apical knob of thick mesoglea; elsewhere, mesoglea thin. With eight radial canals bearing eight gonads in middle part of their upper halves; gonads sac-shaped, pendent. With about 60 short, solid tentacles, borne on nearly indistinguishable marginal bulbs; no statocysts. Velum broad, velar opening wide. Manubrium relatively long, borne on conical peduncle of nearly the same length as manubrium itself; distal end of manubrium projecting slightly below the upper halve of umbrella. Mouth with four lips.
 Remarks. Present specimens differ only slightly from Kramp’s (1959, 1968) accounts: he described the gonads as being near the middle points of radial canals while in the present material they are found on upper third of radial canals.
 World distribution. This species was recorded from the Strait of Magellan (Pagès & Orejas 1999), Falkland Islands, South Georgia, Cape of Good Hope, and Mozambique Channel (Kramp 1959).
 Records from Chile. The present material was collected from fjord Comau. Additional records are those of Palma et al. (2007) from the southern channels (between the Gulf of Corcovado and the Pulluche-Chacabuco Channels).
description: Published as part of Galea, Horia R., 2007, Hydroids and hydromedusae (Cnidaria: Hydrozoa) from the fjords region of southern Chile, pp. 1-116 in Zootaxa 1597 (1) on page 97, DOI: 10.11646/zootaxa.1650.1.4, http://zenodo.org/record/5097970
Can high-velocity stars reveal black holes in globular clusters?
Creators: name: Drukier, G. A.
name: Bailyn, C. D.
Publisher: name: arXiv
Year: 2003
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We estimate the number of individual, fast-moving stars observable in globular clusters under the assumption that the clusters contain massive central black holes which follow the galactic black-hole mass vs. sigma relationship. We find that radial velocity measurements are unlikely to detect such stars, but that proper motion studies could reveal such stars, if they exist, in the most likely clusters. Thus, HST proper motion studies can test this hypothesis in a few nearby clusters.
description: 10 pages, 1 figure in AASTeX v5.0. Accepted for publication in ApJ Letters
Deutonura phlegraea
Creators: name: Thibaud, Jean-Marc
Publisher: name: Zenodo
Year: 2017
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Collembola
Poduromorpha
Neanuridae
Deutonura
Deutonura phlegraea

description: Deutonura phlegraea (Caroli, 1912)
Achorutes phlegraeus Caroli, 1912a: 365.
Lathriopyga phlegraea – Cassagnau 1954c: 28.
Deutonura phlegraea – Deharveng 1982b: 10.
DISTRIBUTION. — Ardèche. Baume-Saint-Arnaudprèsde Les Assions (Stomp etal. 1982).
Ariège. Forêtde Belesta (Cassagnau 1954c).
Aude. Forêtde Ramondens (Cassagnau 1954c, L. phlegraea).
Corse. Pelouse du lac Nino (Denis 1947b). — Poinsot 1972a. — Poinsot-Balaguer 1978 (L. phlegraea; espèce douteusepour la Corse, plutôt Neanura [Deutonura] betica Deharveng 1980).
Est du Rhône. Deharveng 1982b.
Haute-Garonne. Forêt de Buzet, Saint-Jean-de-l’Union, forêts de Bouconne etde Sainte-Croix-Volvestre (Cassagnau 1954c). — Jardins à Toulouse (Cassagnau 1962a, b; Deharveng 1979a).
Hautes-Pyrénées. Fenouillet (Cassagnau & Delamare Deboutteville 1951).
Pyrénées-Orientales. Valléede la Bayorie près de Banyuls-sur-Mer (Denis 1932).
Sud-Ouest de la France. En plaine (Cassagnau 1961).
Tarn, Aude. Montagne Noire (Cassagnau 1965).
Tarn. Sidobre (Izarra 1969).
Var. Montrieux-le-Vieux (Denis 1932).
Vosges. Minede la Croix-aux-Minesprèsde Saint-Dié (Denis 1934a).
TAXONOMIE. — Denis 1947b (redescription); Deharveng 1982b (redescription).
ÉCOLOGIE. — Cassagnau 1965 (écologie, sol).
description: Published as part of Thibaud, Jean-Marc, 2017, Catalogue des collemboles de France, pp. 297-436 in Zoosystema 39 (3) on page 322, DOI: 10.5252/z2017n3a1, http://zenodo.org/record/5496272
ALP Constraints in Gauged $\mathcal{N}=2$ Supergravity
Creators: name: Aoki, Shuntaro
name: Liao, Henry
Publisher: name: arXiv
Year: 2020
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We discuss a possibility of restricting parameters in $\mathcal{N}=2$ supergravity based on axion observations. We derive conditions that prepotential and gauge couplings should satisfy. Such conditions not only allow us to constrain the theory but also provide the lower bound of $\mathcal{N}=2\rightarrow\mathcal{N}=1$ breaking scale.
description: 19 pages
Astrophysical magnetic fields and nonlinear dynamo theory
Creators: name: Brandenburg, Axel
name: Subramanian, Kandaswamy
Publisher: name: arXiv
Year: 2004
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: The current understanding of astrophysical magnetic fields is reviewed, focusing on their generation and maintenance by turbulence. In the astrophysical context this generation is usually explained by a self-excited dynamo, which involves flows that can amplify a weak 'seed' magnetic field exponentially fast. Particular emphasis is placed on the nonlinear saturation of the dynamo. Analytic and numerical results are discussed both for small scale dynamos, which are completely isotropic, and for large scale dynamos, where some form of parity breaking is crucial. Central to the discussion of large scale dynamos is the so-called alpha effect which explains the generation of a mean field if the turbulence lacks mirror symmetry, i.e. if the flow has kinetic helicity. Large scale dynamos produce small scale helical fields as a waste product that quench the large scale dynamo and hence the alpha effect. With this in mind, the microscopic theory of the alpha effect is revisited in full detail and recent results for the loss of helical magnetic fields are reviewed.
description: 285 pages, 72 figures, accepted by Phys. Rep
UV Perturbations in Brane Gas Cosmology
Creators: name: Watson, Scott
Publisher: name: arXiv
Year: 2004
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: Astrophysics (astro-ph)
subject: General Relativity and Quantum Cosmology (gr-qc)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We consider the effect of the ultraviolet (UV) or short wavelength modes on the background of Brane Gas Cosmology. We find that the string matter sources are negligible in the UV and that the evolution is given primarily by the dilaton perturbation. We also find that the linear perturbations are well behaved and the predictions of Brane Gas Cosmology are robust against the introduction of linear perturbations. In particular, we find that the stabilization of the extra dimensions (moduli) remains valid in the presence of dilaton and string perturbations.
description: 21 pages, 5 figures
Boudiennyia Girault
Creators: name: Huber, John T.
name: Read, Jennifer D.
name: Triapitsyn, Serguei V.
Publisher: name: Zenodo
Year: 2007
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hymenoptera
Mymaridae
Boudiennyia

description: Genus Boudiennyia Girault (Figs. 54–59)
 Boudiennyia Girault, 1937 [448]: 2. Type species: Ooctonus saintpierrei Girault, by original designation.
 Diagnosis. Boudiennyia belongs to the Ooctonus group of genera. It is the only Australian genus of the group and is distinguished from the superficially similar genus Gonatocerus, whose species also have an 8-segmented funicle and entire clava, as follows: propodeum with a distinct transverse carina (costula) joining the longitudinal submedian carinae (Fig. 59); fore wing with venation more than half wing length and hypochaeta much closer to proximal macrochaeta than to distal macrochaeta (Fig. 55); gaster distincly petiolate, the petiole at least 3x as long as wide. Fore leg as in Fig. 54. Male flagellum 11-segmented (Fig. 58) and genitalia as in Fig. 57.
 Body length. 717–1203 µm.
 Hosts. Unknown.
 Distribution. Australia.
 Important Reference. Huber (2002).
Australian species (1):
 B. saintpierrei (Girault, 1913 [158]: 80) (Ooctonus); Girault, 1913 [165]: 107 (description); Girault, 1937 [448]: 2 (generic transfer); Dahms, 1986: 497 (types). TL: Qld, Kuranda.
description: Published as part of Huber, John T., Read, Jennifer D. & Triapitsyn, Serguei V., 2007, Paranaphoidea Girault 1913, pp. 1-111 in Zootaxa 1596 on page 27, DOI: 10.11646/zootaxa.1596.1.1, http://zenodo.org/record/5779298
Betweenness Centrality in Large Complex Networks
Creators: name: Barthelemy, Marc
Publisher: name: arXiv
Year: 2003
Subjects: subject: Disordered Systems and Neural Networks (cond-mat.dis-nn)
subject: Statistical Mechanics (cond-mat.stat-mech)
subject: FOS: Physical sciences

description: We analyze the betweenness centrality (BC) of nodes in large complex networks. In general, the BC is increasing with connectivity as a power law with an exponent $η$. We find that for trees or networks with a small loop density $η=2$ while a larger density of loops leads to $η<2$. For scale-free networks characterized by an exponent $γ$ which describes the connectivity distribution decay, the BC is also distributed according to a power law with a non universal exponent $δ$. We show that this exponent $δ$ must satisfy the exact bound $δ\geq (γ+1)/2$. If the scale free network is a tree, then we have the equality $δ=(γ+1)/2$.
description: 6 pages, 5 figures, revised version
Lettre de (Négociants de Lyon) Michel fils et Sablié à Jean-François Séguier, 1778-06-19
Creators: name: Sablié, Michel Fils Et
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2021

description: [transcription] M. Jean-François Séguier

Nîmes Lyon, le 19 juin 1778.

Monsieur,

Nous eûmes l'honneur de vous écrire à la date du 12 courant pour vous annoncer l'envoi d'un petit paquet reçu à notre adresse de Bergame et qui vous était destiné. Le voiturier à qui nous nous proposions de le remettre refusa de s'en charger, attendu les visites scrupuleuses qu'il essuyait ordinairement dans sa route, de sorte que nous avons été obligés de le consigner à la messagerie pour vous le faire parvenir. Veuillez donc vous le procurer suivant notre lettre de voiture que vous aurez s'il vous plaît la bonté de nous renvoyer entièrement acquittée, afin que nous puissions au moyen d'icelle nous faire remboyrser ici les 53 lt. 4 s. en question pour frais de transport.

Quoiqu'en cette affaire nous ne fassions sûrement qu'office d'ami, nous sommes fâchés du retard qui résulte et que nous n'avons pu prévoir ni empêcher.

Nous avons l'honneur d'être avec considération,

Monsieur,

Votre très humble serviteur

P. Michel fils et Sablié
description: Source: [lieu de Conservation] Nîmes, Bibliothèque Carré d'Art [cote]ms. 312_7, fol. 17r
description: Source: ark:/12148/btv1b10015928h
N-body self-consistent stars-halo modeling of the Fornax dwarf galaxy
Creators: name: Shchelkanova, Galina
name: Hayashi, Kohei
name: Blinnikov, Sergei
Publisher: name: arXiv
Year: 2020
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We present nearly self-consistent stellar-halo models of the Fornax dwarf spheroidal galaxy associated with the Milky Way galaxy. Such galaxies are dominated by dark matter and have almost no gas in the system. Therefore, they are excellent objects for N-body modeling that takes into account visible and dark matter halo components. In order to model the dark matter halo inferred from the analysis of the measured velocities of Fornax's stars, we constructed several self-consistent quasi-equilibrium models based on two source code sets. One of them (GalactICS Software, NEMO) deals with the self-consistent distribution function modeling which depends on energy $E$ and vertical component of the angular momentum $L_z$. The other is included in the AGAMA framework and is based on Schwarzschild's calculation of orbits. It can reproduce the non-spherical self-consistent structure of Fornax as the weighted sum of orbit contributions to the galactic density even though the inferred dark halo parameters come from Jeans analysis which does not require that any distribution functions should be positive. To guess the parameters which make the N-body models close to the visible object we use the stellar-dark matter model of the Fornax galaxy based on hydrodynamic axisymmetric Jeans equations taking into account the velocity anisotropy parameter. Then we studied the evolution of the models by performing N-body simulations with the falcON code in order to test their stability. The variability of the model parameters over time was obtained during simulations. The AGAMA models show the best agreement of the resulting velocity dispersion profiles with the observed data.
description: 26 pages, 15 figures