cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Broadband Photon Spectrum and its Radial Profile of Pulsar Wind Nebulae
Creators: name: Ishizaki, Wataru
name: Tanaka, Shuta J.
name: Asano, Katsuaki
name: Terasawa, Toshio
Publisher: name: arXiv
Year: 2017
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: The observed radial profiles of the X-ray emission from Pulsar Wind Nebulae (PWNe) have been claimed to conflict with the standard one-dimensional (1-D) steady model. However, the 1-D model has not been tested to reproduce both the volume-integrated spectrum and the radial profile of the surface brightness, simultaneously. We revisit the 1-D steady model and apply it to PWNe 3C 58 and G21.5-0.9. We find that the parameters of the pulsar wind, the radius of the termination shock $r_{\rm s}$ and magnetization $σ$, greatly affect both the photon spectrum and radial profile of the emission. We have shown that the parameters constrained by the entire spectrum lead to a smaller X-ray nebula than observed one. We have also tested the case that reproduces only the observations in X and gamma-rays, ignoring the radio and optical components. In this case, there are parameter sets that reproduce both the spectrum and emission profile, but the advection time to the edge of the nebula becomes much smaller than the age. Our detailed discussion clarifies that the standard 1-D steady model has severe difficulty to reproduce both the volume-integrated spectrum and the surface brightness simultaneously. This implies that the model should be improved by taking into account extra physical processes such as spatial diffusion of particles. Additionally, we calculate the surface brightness profile of the radio, optical and TeV gamma-rays. The future observations in these wavelengths are also important to probe the spatial distributions of the relativistic plasma and the magnetic field of PWNe.
description: 15 pages, 10 figures, accepted for publication in ApJ
Probing sub-GeV dark sectors via high energy proton beams at LBNF/DUNE and MiniBooNE
Creators: name: Frugiuele, Claudia
Publisher: name: arXiv
Year: 2017
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We study the sensitivity to sub-GeV dark sectors of high energy ($ \geq100$ GeV) proton fixed target experiments such as the Main Injector and the future Long-Baseline Neutrino Facility (LBNF). We focus on off-axis detectors since they have been shown to be the ideal location to reduce the neutrino background. We consider MiniBooNE as an off-axis detector for the NuMI facility and a hypotetical detector for LBNF located 200 m away from the target and 6.5 degrees off-axis. We find that with the existing data, MiniBoone can explore new regions of the parameter space for leptophobic dark forces in the 100 MeV- few GeV mass range. The dedicated MiniBooNE run in beam dump mode would further improve the reach for even lighter masses. Therefore, MiniBooNE has the potential to be one of the most sensitive probe of leptophobic dark forces for masses between 1 MeV-10 GeV.
description: 5 pages, 2 figures
Additional file 2 of Epigenome-wide DNA methylation profiling of conditioned pain modulation in individuals with non-specific chronic low back pain
Creators: name: Goodin, Burel R.
name: Overstreet, Demario S.
name: Penn, Terence M.
name: Bakshi, Rahm
name: Quinn, Tammie L.
name: Sims, Andrew
name: Ptacek, Travis
name: Jackson, Pamela
name: Long, D. Leann
name: Aroke, Edwin N.
Publisher: name: figshare
Year: 2022
Subjects: subject: Genetics
subject: FOS: Biological sciences

description: Additional file 2: Table S1. Top 10 KEGG pathways enriched by gene annotated with DMCs between efficient and less efficient conditioned pain modulation in participants with cLBP. Table S2. Top 10 Wiikipathway enriched by gene annotated with DMCs between efficient and less efficient conditioned pain modulation in participants with cLBP
Additional file 1 of Epigenome-wide DNA methylation profiling of conditioned pain modulation in individuals with non-specific chronic low back pain
Creators: name: Goodin, Burel R.
name: Overstreet, Demario S.
name: Penn, Terence M.
name: Bakshi, Rahm
name: Quinn, Tammie L.
name: Sims, Andrew
name: Ptacek, Travis
name: Jackson, Pamela
name: Long, D. Leann
name: Aroke, Edwin N.
Publisher: name: figshare
Year: 2022
Subjects: subject: Genetics
subject: FOS: Biological sciences

description: Additional file 1: Figure S1. Top 10 GO terms enrichment results of annotated genes with hypomethylated CpGs between efficient and less efficient conditioned pain modulation participants with cLBP. All depicted terms were statistically significant (p
ALMA reveals starburst-like interstellar medium conditions in a compact star-forming galaxy at z ~ 2 using [CI] and CO
Creators: name: Popping, Gergö
name: Decarli, Roberto
name: Man, Allison W. S.
name: Nelson, Erica J.
name: Béthermin, Matthieu
name: De Breuck, Carlos
name: Mainieri, Vincenzo
name: van Dokkum, Pieter G.
name: Gullberg, Bitten
name: van Kampen, Eelco
name: Spaans, Marco
name: Trager, Scott C.
Publisher: name: arXiv
Year: 2017
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We present ALMA detections of the [CI] 1-0, CO J=3-2, and CO J=4-3 emission lines, as well as the ALMA band 4 continuum for a compact star-forming galaxy (cSFG) at z=2.225, 3D-HST GS30274. As is typical for cSFGs, this galaxy has a stellar mass of $1.89 \pm 0.47\,\times 10^{11}\,\rm{M}_\odot$, with a star formation rate of $214\pm44\,\rm{M}_\odot\,\rm{yr}^{-1}$ putting it on the star-forming `main-sequence', but with an H-band effective radius of 2.5 kpc, making it much smaller than the bulk of `main-sequence' star-forming galaxies. The intensity ratio of the line detections yield an ISM density (~ 6 $\times 10^{4}\,\rm{cm}^{-3}$) and a UV-radiation field ( ~2 $\times 10^4\,\rm{G}_0$), similar to the values in local starburst and ultra-luminous infrared galaxy environments. A starburst phase is consistent with the short depletion times ($t_{\rm H2, dep} \leq 140$ Myr) we find using three different proxies for the H2 mass ([CI], CO, dust mass). This depletion time is significantly shorter than in more extended SFGs with similar stellar masses and SFRs. Moreover, the gas fraction of 3D-HST GS30274 is smaller than typically found in extended galaxies. We measure the CO and [CI] kinematics and find a FWHM line width of ~$750 \pm 41 $ km s$^{-1}$. The CO and [CI] FWHM are consistent with a previously measured H$α$ FWHM for this source. The line widths are consistent with gravitational motions, suggesting we are seeing a compact molecular gas reservoir. A previous merger event, as suggested by the asymmetric light profile, may be responsible for the compact distribution of gas and has triggered a central starburst event. This event gives rise to the starburst-like ISM properties and short depletion times. The centrally located and efficient star formation is quickly building up a dense core of stars, responsible for the compact distribution of stellar light in 3D-HST GS30274.
description: Accepted for publication in A&A
How to control Spin-Seebeck current in a metal-quantum dot-magnetic insulator junction
Creators: name: Gu, Lei
name: Fu, Hua-Hua
name: Wu, Ruqian
Publisher: name: arXiv
Year: 2016
Subjects: subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: FOS: Physical sciences

description: The control of the spin-Seebeck current is still a challenging task for the development of spin caloritronic devices. Here, we construct a spin-Seebeck device by inserting a strongly correlated quantum dot (QD) between the metal lead and magnetic insulator. Using the slave-particle approach and non-crossing approximation, we find that the spin-Seebeck effect increases significantly when the energy level of the QD locates near the Fermi level of the metal lead due to the enhancement of spin flipping and occurrences of quantum resonance. Since this can be easily realized by applying a gate voltage in experiments, the spin-Seebeck device proposed here can also work as a thermovoltaic transistor. Moreover, the optimal correlation strength and the energy level position of the QD are discussed to maximize the spin-Seebeck current as required for applications in controllable spin caloritronic devices.
description: 21 pages, 8 figures, published in PRB
Potential Fluctuations at Low Temperatures in Mesoscopic-Scale SmTiO$_{3}$/SrTiO$_{3}$/SmTiO$_{3}$ Quantum Well Structures
Creators: name: Hardy, Will J.
name: Isaac, Brandon
name: Marshall, Patrick
name: Mikheev, Evgeny
name: Zhou, Panpan
name: Stemmer, Susanne
name: Natelson, Douglas
Publisher: name: arXiv
Year: 2017
Subjects: subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: FOS: Physical sciences

description: Heterointerfaces of SrTiO$_{3}$ with other transition metal oxides make up an intriguing family of systems with a bounty of coexisting and competing physical orders. Some examples, such as LaAlO$_{3}$/SrTiO$_{3}$, support a high carrier density electron gas at the interface whose electronic properties are determined by a combination of lattice distortions, spin-orbit coupling, defects, and various regimes of magnetic and charge ordering. Here, we study electronic transport in mesoscale devices made with heterostructures of SrTiO$_{3}$ sandwiched between layers of SmTiO$_{3}$, in which the transport properties can be tuned from a regime of Fermi-liquid like resistivity ($ρ\sim T^{2}$) to a non-Fermi liquid ($ρ\sim T^{5/3}$) by controlling the SrTiO$_{3}$ thickness. In mesoscale devices at low temperatures, we find unexpected voltage fluctuations that grow in magnitude as $T$ is decreased below 20 K, are suppressed with increasing contact electrode size, and are independent of the drive current and contact spacing distance. Magnetoresistance fluctuations are also observed, which are reminiscent of universal conductance fluctuations but not entirely consistent with their conventional properties. Candidate explanations are considered, and a mechanism is suggested based on mesoscopic temporal fluctuations of the Seebeck coefficient. An improved understanding of charge transport in these model systems, especially their quantum coherent properties, may lead to insights into the nature of transport in strongly correlated materials that deviate from Fermi liquid theory.
description: 19 pages, 4 figures + 12 pages, 9 figures of supplemental material
Additional file 1 of Economic evaluation of community-based falls prevention interventions for older populations: a systematic methodological overview of systematic reviews
Creators: name: Kwon, Joseph
name: Squires, Hazel
name: Franklin, Matthew
name: Lee, Yujin
name: Young, Tracey
Publisher: name: figshare
Year: 2022
Subjects: subject: Medicine
subject: Biotechnology
subject: Sociology
subject: FOS: Sociology
subject: Cancer
subject: Science Policy
subject: Computational Biology

description: Additional file1: TableA1. Medline search strategyfor systematic overview and systematic review. Table A2. Embase search strategy for systematic overview ofsystematic reviews of falls prevention economic evaluation. Table A3. PubMed search strategy for systematic overview andsystematic review. Table A4. Cochrane Library (CSDR and CENTRAL) searchstrategy for systematic overview and systematic review. Table A5. EconLit search strategy for systematic overviewand systematic review. Table A6. CINAHL search strategy for systematic overview andsystematic review. Table A7. PsycInfo search strategy for systematic overviewand systematic review. Table A8. ASSIA search strategy for systematic overview andsystematic review. Table B. Studies excluded from systematic overview at fulltext screening and exclusion reason. Table C. Primary economic evaluations of community-basedfalls prevention interventions included in previous systematic reviews. Table D. Items contained in checklists used for qualityassessment of economic evaluations included in systematic reviews. Table E. Results of quality assessment by previoussystematic reviews of community-based falls prevention economic evaluations. Table F. AMSTAR 2 checklist for reporting andmethodological quality of systematic reviews (56).
Observation of spin-charge separation and boundary bound states via the local density of states
Creators: name: Schoenauer, Benedikt
name: Schmitteckert, Peter
name: Schuricht, Dirk
Publisher: name: arXiv
Year: 2016
Subjects: subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: FOS: Physical sciences

description: We numerically calculate the local density of states (LDOS) of a one-dimensional Mott insulator with open boundaries, which is modelled microscopically by a (extended) Hubbard chain at half filling. In the Fourier transform of the LDOS we identify several dispersing features corresponding to propagating charge and spin degrees of freedom, thus providing a visualisation of the spin-charge separation in the system. We also consider the effect of an additional boundary potential, which, if sufficiently strong, leads to the formation of a boundary bound state which is clearly visible in the LDOS as a non-dispersing feature inside the Mott gap.
A modular set of synthetic spectral energy distributions for young stellar objects
Creators: name: Robitaille, Thomas P.
Publisher: name: arXiv
Year: 2017
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: In this paper, I present a new set of synthetic spectral energy distributions (SEDs) for young stellar objects (YSOs) spanning a wide range of evolutionary stages, from the youngest deeply embedded protostars to pre-main-sequence stars with few or no disks. These models include significant improvements on the previous generation of published models: in particular, the new models cover a much wider and more uniform region of parameter space, do not include highly model-dependent parameters, and include a number of improvements that make them more suited to modeling far-infrared and sub-mm observations of forming stars. Rather than all being part of a single monolithic set of models, the new models are split up into sets of varying complexity. The aim of the new set of models is not to provide the most physically realistic models for young stars, but rather to provide deliberately simplified models for initial modeling, which allows a wide range of parameter space to be explored. I present the design of the model set, and show examples of fitting these models to real observations to show how the new grid design can help us better understand what can be determined from limited unresolved observations. The models, as well as a Python-based fitting tool are publicly available to the community.
description: Accepted for publication in Astronomy and Astrophysics. The models are available at http://doi.org/10.5281/zenodo.166732
Additional file 1 of Soil microbial communities following 20 years of fertilization and crop rotation practices in the Czech Republic
Creators: name: Kracmarova, Martina
name: Uhlik, Ondrej
name: Strejcek, Michal
name: Szakova, Jirina
name: Cerny, Jindrich
name: Balik, Jiri
name: Tlustos, Pavel
name: Kohout, Petr
name: Demnerova, Katerina
name: Stiborova, Hana
Publisher: name: figshare
Year: 2022
Subjects: subject: Microbiology
subject: FOS: Biological sciences

description: Additional file 1: Table S1. Table of soil physicochemical parameters. Fig. S1. Scatter plot of each pair of physicochemical parameters showing Pearson’s correlation coefficients. Table S2. The influence of location, soil type, fertilization and crop rotation on soil chemical properties analysed with Kruskal-Wallis test.
title: ADCO, Cartulaire général de Cîteaux, dit de Jean de Cirey, (XVe siècle), tome IV, Cart. 188 (11 H 73), f. 0108v
Creators: name: de la Côte d'Or, Archives départementales
name: Archives Départementales De La Côte-D'Or
name: Petot, Frédérique
name: Projet CBMA
name: CG21/F.PETOT/2012
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2020
Subjects: subject: Chartes de la Bourgogne du Moyen Âge
subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris
subject: cartulaire
subject: Corpus Burgundiae Medii Aevi

description: Cartulaire général de Cîteaux, dit de Jean de Cirey, (XVe siècle), tome IV, Archives départementales de la Côte-d'Or, Cart. 188 (11 H 73), f. 0108v, Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Cartulaire général de Cîteaux, dit de Jean de Cirey, (XVe siècle), tome IV, Archives départementales de la Côte-d'Or, Cart. 188 (11 H 73), f. 0108v, 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
Additional file 1 of Clinical feasibility and impact of data-driven respiratory motion compensation studied in 200 whole-body 18F-FDG PET/CT scans
Creators: name: Dias, André H.
name: Schleyer, Paul
name: Vendelbo, Mikkel H.
name: Hjorthaug, Karin
name: Gormsen, Lars C.
name: Munk, Ole L.
Publisher: name: figshare
Year: 2022
Subjects: Space Science
Medicine
Cell Biology
Cancer
Computational Biology

description: Additional file 1. Table S1: Scan indications and demographic distribution of full patient population. Table S2: Characteristics of all 200 “most blurry” lesions for all reconstructions using 3 different thresholds for isocontouring. Figure S1: Bland–Altman plots of the “most blurry” lesion (N = 200), representing the differences between SUVmean values. Figure S2: Bland–Altman plots for the fixed liver VOI, representing the differences between SUVmean values.
Heuristics for the refinement of assumptions in generalized reactivity formulae
Creators: name: Cavezza, Davide Giacomo
Publisher: name: Imperial College London
Year: 2020

description: Reactive synthesis is concerned with automatically generating implementations from formal specifications. These specifications are typically written in the language of generalized reactivity (GR(1)), a subset of linear temporal logic capable of expressing the most common industrial specification patterns, and describe the requirements about the behavior of a system under assumptions about the environment where the system is to be deployed. Oftentimes no implementation exists which guarantees the required behavior under all possible environments, typically due to missing assumptions (this is usually referred to as unrealizability). To address this issue, new assumptions need to be added to complete the specification, a problem known as assumptions refinement. Since the space of candidate assumptions is intractably large, searching for the best solutions is inherently hard. In particular, new methods are needed to (i) increase the effectiveness of the search procedures, measured as the ratio between the number of solutions found and of refinements explored; and (ii) improve the results' quality, defined as the weakness of the solutions. In this thesis we propose a set of heuristics to meet these goals, and a methodology to assess and compare assumptions refinement methods based on quantitative metrics. The heuristics are in the form of algorithms to generate candidate refinements during the search, and quantitative measures to assess the quality of the candidates. We first discuss a heuristic method to generate assumptions that target the cause of unrealizability. This is done by selecting candidate refinement formulas based on Craig's interpolation. We provide a formal underpinning of the technique and evaluate it in terms of our new metric of effectiveness, as defined above, whose value is improved with respect to the state of the art. We demonstrate this on a set of popular benchmarks of embedded software. We then provide a formal, quantitative characterization of the permissiveness of environment assumptions in the form of a weakness measure. We prove that the partial order induced by this measure is consistent with the one induced by implication. The key advantage of this measure is that it allows for prioritizing candidate solutions, as we show experimentally. Lastly, we propose a notion of minimal refinements with respect to the observed counterstrategies. We demonstrate that exploring minimal refinements produces weaker solutions, and reduces the amount of computations needed to explore each refinement. However, this may come at the cost of reducing the effectiveness of the search. To counteract this effect, we propose a hybrid search approach in which both minimal and non-minimal refinements are explored.
QUEDAS EM IDOSOS E CUIDADOS ESSENCIAIS
Creators: name: Aurilene Josefa Cartaxo de Arruda Cavalcanti
name: GRACIMARY ALVES TEXEIRA
name: SÔNIA MARIA JOSINO DOS SANTOS
name: BEATRIZ DA SILVA VASCONCELOS PEREIRA
name: ARLLA MILENE CIRINO SOARES
name: ANA CAROLINA DOS SANTOS
Publisher: name: Zenodo
Year: 2023
Subjects: Idoso
Queda
Cuidado

description: Esta cartilha foi elaborada com o intuito de fornecer informações e facilitar o entendimento acerca dos riscos de queda, em especial, frente ao processo de senescência. Está destinada aos discentes do Curso Técnico em Cuidados de Idosos do Centro Profissional e Tecnológico - Escola Técnica de Saúde da Universidade Federal da Paraíba (CPT-ETS/UFPB).
A continuum of accretion burst behavior in young stars observed by K2
Creators: name: Cody, Ann Marie
name: Hillenbrand, Lynne A.
name: David, Trevor J.
name: Carpenter, John M.
name: Everett, Mark E.
name: Howell, Steve B.
Publisher: name: arXiv
Year: 2016
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: We present 29 likely members of the young $ρ$ Oph or Upper Sco regions of recent star formation that exhibit "accretion burst" type light curves in $K2$ time series photometry. The bursters were identified by visual examination of their ~80 day light curves, though all satisfy the $M < -0.25$ flux asymmetry criterion for burst behavior defined by Cody et al. (2014). The burst sources represent $\approx$9% of cluster members with strong infrared excess indicative of circumstellar material. Higher amplitude burster behavior is correlated with larger inner disk infrared excesses, as inferred from $WISE$ $W1-W2$ color. The burst sources are also outliers in their large H$α$ emission equivalent widths. No distinction between bursters and non-bursters is seen in stellar properties such as multiplicity or spectral type. The frequency of bursters is similar between the younger, more compact $ρ$ Oph region, and the older, more dispersed Upper Sco region. The bursts exhibit a range of shapes, amplitudes (~10-700%), durations (~1-10 days), repeat time scales (~3-80 days), and duty cycles (~10-100%). Our results provide important input to models of magnetospheric accretion, in particular by elucidating the properties of accretion-related variability in the low state between major longer duration events such as EX Lup and FU Ori type accretion outbursts. We demonstrate the broad continuum of accretion burst behavior in young stars -- extending the phenomenon to lower amplitudes and shorter timescales than traditionally considered in the theory of pre-main sequence accretion history.
description: refereed version re-submitted to AAS journals, 31 pages, 14 figures, 2 tables
title: ADCO, Cartulaire de Cîteaux pour les domaines de Saint-Jean de Losne et Losne (XVIIIe siècle), Cart. 198-01 (11 H 1055), 185 folios, f. 0199
Creators: name: de la Côte d'Or, Archives départementales
name: Petot, Frédéric
name: Archives Départementales De La Côte-D'Or
name: Petot, Frédérique
name: Projet CBMA
name: CG21/F.PETOT/2019
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2020
Subjects: subject: Corpus Burgundiae Medii Aevi
subject: Chartes de la Bourgogne du Moyen Âge
subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris
subject: cartulaire

description: Cartulaire de Cîteaux pour les domaines de Saint-Jean de Losne et Losne (XVIIIe siècle), Archives départementales de la Côte-d'Or, Cart. 198-01 (11 H 1055), 185 folios, f. 0199, Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Cartulaire de Cîteaux pour les domaines de Saint-Jean de Losne et Losne (XVIIIe siècle), Archives départementales de la Côte-d'Or, Cart. 198-01 (11 H 1055), 185 folios, f. 0199, 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
All Chern-Simons Invariants of 4D, N = 1 Gauged Superform Hierarchies
Creators: name: Becker, Katrin
name: Becker, Melanie
name: Linch, William D.
name: Randall, Stephen
name: Robbins, Daniel
Publisher: name: arXiv
Year: 2017
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We give a geometric description of supersymmetric gravity/(non-)abelian $p$-form hierarchies in superspaces with 4D, $N = 1$ super-Poincare invariance. These hierarchies give rise to Chern-Simons-like invariants, such as those of the 5D, $N = 1$ graviphoton and the eleven-dimensional 3-form but also generalizations such as Green-Schwarz-like/BF-type couplings. Previous constructions based on prepotential superfields are reinterpreted in terms of $p$-forms in superspace thereby elucidating the underlying geometry. This vastly simplifies the calculations of superspace field-strengths, Bianchi identities, and Chern-Simons invariants. Using this, we prove the validity of a recursive formula for the conditions defining these actions for any such tensor hierarchy. Solving it at quadratic and cubic orders, we recover the known results for the BF-type and cubic Chern-Simons actions. As an application, we compute the quartic invariant $\sim A dA dA dA + \ldots$ relevant, for example, to seven-dimensional supergravity compactifications.
description: 31 pages; v2: added references
Orbits of massive satellite galaxies: II. Bayesian Estimates of the Milky Way and Andromeda masses using high precision astrometry and cosmological simulations
Creators: name: Patel, Ekta
name: Besla, Gurtina
name: Mandel, Kaisey
Publisher: name: arXiv
Year: 2017
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: Space observatories like the Hubble Space Telescope and Gaia are providing unprecedented 6D phase space information of satellite galaxies. Such measurements can shed light on the structure and assembly history of the Local Group, but improved statistical methods are needed to use them efficiently. Here we illustrate such a method using analogs of the Local Group's two most massive satellite galaxies, the Large Magellanic Cloud (LMC) and Triangulum (M33), from the Illustris dark-matter-only cosmological simulation. We use a Bayesian inference scheme combining measurements of positions, velocities, and specific orbital angular momenta ( j ) of the LMC/M33 with importance sampling of their simulated analogs to compute posterior estimates of the Milky Way (MW) and Andromeda's (M31) halo masses. We conclude the resulting host halo mass is more susceptible to bias when using measurements of the current position and velocity of satellites, especially when satellites are at short-lived phases of their orbits (i.e. at pericentre). Instead, the j value of a satellite is well-conserved over time and provides a more reliable constraint on host mass. The inferred virial mass of the MW (M31) using j of the LMC (M33) is $\rm M_{vir, MW}=1.02^{+0.77}_{-0.55}\times10^{12}\; M_{\odot}$ ($\rm M_{vir, M31}=1.37^{+1.39}_{-0.75}\times10^{12}\; M_{\odot}$). Choosing simulated analogs whose j values are consistent with the conventional picture of a previous (< 3 Gyr ago), close encounter (< 100 kpc) of M33 about M31 results in a very low virial mass for M31 ($\rm\sim\!10^{12}\; M_{\odot}$). This supports the new scenario put forth in Patel et al. (2017), wherein M33 is on its first passage about M31 or on a long period orbit. We conclude that this Bayesian inference scheme, utilising satellite j, is a promising method to reduce the current factor of two spread in the mass range of the MW and M31 moving forward.
description: 24 pages, 9 figures. Submitted to MNRAS
Additional file 2 of “Like before, but not exactly”: the Qualy-REACT qualitative inquiry into the lived experience of long COVID
Creators: name: Schiavi, Margherita
name: Fugazzaro, Stefania
name: Bertolini, Anna
name: Denti, Monica
name: Mainini, Carlotta
name: Accogli, Monia Allisen
name: Bedogni, Ginevra
name: Ghizzoni, Daniele
name: Esseroukh, Otmen
name: Gualdi, Cecilia
name: Costi, Stefania
Publisher: name: figshare
Year: 2022
Subjects: subject: Medicine
subject: Science Policy
subject: Sociology
subject: FOS: Sociology
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: 111714 Mental Health
subject: FOS: Health sciences

description: Additional file 2. Study Consent Form.
Additional file 1 of “Like before, but not exactly”: the Qualy-REACT qualitative inquiry into the lived experience of long COVID
Creators: name: Schiavi, Margherita
name: Fugazzaro, Stefania
name: Bertolini, Anna
name: Denti, Monica
name: Mainini, Carlotta
name: Accogli, Monia Allisen
name: Bedogni, Ginevra
name: Ghizzoni, Daniele
name: Esseroukh, Otmen
name: Gualdi, Cecilia
name: Costi, Stefania
Publisher: name: figshare
Year: 2022
Subjects: subject: Medicine
subject: Science Policy
subject: Sociology
subject: FOS: Sociology
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: 111714 Mental Health
subject: FOS: Health sciences

description: Additional file 1. The COREQ checklist of the report.
Healing Data Loss Problems in Android Apps
Creators: name: Riganelli, Oliviero
name: Micucci, Daniela
name: Mariani, Leonardo
Publisher: name: arXiv
Year: 2017
Subjects: subject: Software Engineering (cs.SE)
subject: FOS: Computer and information sciences

description: Android apps should be designed to cope with stop-start events, which are the events that require stopping and restoring the execution of an app while leaving its state unaltered. These events can be caused by run-time configuration changes, such as a screen rotation, and by context-switches, such as a switch from one app to another. When a stop-start event occurs, Android saves the state of the app, handles the event, and finally restores the saved state. To let Android save and restore the state correctly, apps must provide the appropriate support. Unfortunately, Android developers often implement this support incorrectly, or do not implement it at all. This bad practice makes apps to incorrectly react to stop-start events, thus generating what we defined data loss problems, that is Android apps that lose user data, behave unexpectedly, and crash due to program variables that lost their values. Data loss problems are difficult to detect because they might be observed only when apps are in specific states and with specific inputs. Covering all the possible cases with testing may require a large number of test cases whose execution must be checked manually to discover whether the app under test has been correctly restored after each stop-start event. It is thus important to complement traditional in-house testing activities with mechanisms that can protect apps as soon as a data loss problem occurs in the field. In this paper we present DataLossHealer, a technique for automatically identifying and healing data loss problems in the field as soon as they occur. DataLossHealer is a technique that checks at run-time whether states are recovered correctly, and heals the app when needed. DataLossHealer can learn from experience, incrementally reducing the overhead that is introduced avoiding to monitor interactions that have been managed correctly by the app in the past.
description: IEEE International Symposium on Software Reliability Engineering Workshops (ISSREW), 2016
Impact of the Hubble tension on the $r$-$n_s$ contour
Creators: name: Jiang, Jun-Qian
name: Ye, Gen
name: Piao, Yun-Song
Publisher: name: arXiv
Year: 2023
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: General Relativity and Quantum Cosmology (gr-qc)
subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: The injection of early dark energy (EDE) before the recombination, a possible resolution of the Hubble tension, will not only shift the scalar spectral index $n_s$ towards $n_s=1$, but also be likely to tighten the current upper limit on tensor-to-scalar ratio $r$. In this work, with the latest CMB datasets (Planck PR4, ACT, SPT and BICEP/Keck), as well as BAO and SN, we confirm this result, and discuss its implication on inflation. We also show that if we happen to live with EDE, how the different inflation models currently allowed would be distinguished by planned CMB observations, such as CMB-S4 and LiteBIRD.
description: 17 pages, 6 figures
Rotation-driven phase transitions in the cores of pulsars
Creators: name: Mellinger, R. D.
name: Weber, F.
name: Spinella, W.
name: Contrera, G. A.
name: Orsaria, M.
Publisher: name: arXiv
Year: 2017
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: Nuclear Theory (nucl-th)
subject: FOS: Physical sciences

description: In this paper, we discuss the impact of rotation on the particle composition of rotating neutron stars (pulsars). Particular emphasis is put on the formation of quark matter during stellar spin-down, driven by continuous gravitational compression. Our study is based on modern models for the nuclear equation of state whose parameters are tightly constrained by nuclear data, neutron star masses, and the latest estimates of neutron star radii.
description: 7 pages, 5 figures; Paper presented at the 7th International Workshop on Astronomy and Relativistic Astrophysics, Gramado, Rio Grande do Sul, Brazil, October 9 - 13, 2016
Longitudinal Beam Dynamics and Coherent Synchrotron Radiation at cSTART
Creators: name: Schwarz, Markus
name: Bründermann, Erik
name: Härer, Bastian
name: El Khechen, Dima
name: Malygin, Anton
name: Müller, Anke-Susanne
name: Nasse, Michael J.
name: Papash, Alexander
name: Ruprecht, Robert
name: Schäfer, Jens
name: Schuh, Marcel
name: Wesolowski, Pawel
Publisher: name: JACoW Publishing
Year: 2021

description: The compact STorage ring for Accelerator Research and Technology (cSTART) project aims to store electron bunches of LWFA-like beams in a very large momentum acceptance storage ring. The project will be realized at the Karlsruhe Institute of Technology (KIT, Germany). Initially, the Ferninfrarot Linac- Und Test-Experiment (FLUTE), a source of ultra-short bunches, will serve as an injector for cSTART to benchmark and emulate laser-wakefield accelerator-like beams. In a second stage a laser-plasma accelerator will be used as an injector, which is being developed as part of the ATHENA project in collaboration with DESY and Helmholtz Institute Jena (HIJ). With an energy of 50 MeV and damping times of several seconds, the electron beam does not reach equilibrium emittance. Furthermore, the critical frequency of synchrotron radiation is 50 THz and in the same order as the bunch spectrum, which implies that the entire bunch radiates coherently. We perform longitudinal particle tracking simulations to investigate the evolution of the bunch length and spectrum as well as the emitted coherent synchrotron radiation. Finally, different options for the RF system are discussed.
CANDELS Multiwavelength Catalogs: Source Identification and Photometry in the CANDELS Extended Groth Strip
Creators: name: Stefanon, Mauro
name: Yan, Haojing
name: Mobasher, Bahram
name: Barro, Guillermo
name: Donley, Jennifer L.
name: Fontana, Adriano
name: Hemmati, Shoubaneh
name: Koekemoer, Anton M.
name: Lee, BoMee
name: Lee, Seong-Kook
name: Nayyeri, Hooshang
name: Peth, Michael
name: Pforr, Janine
name: Salvato, Mara
name: Wiklind, Tommy
name: Wuyts, Stijn
name: Ashby, Matthew L. N.
name: Castellano, Marco
name: Conselice, Christopher J.
name: Cooper, Michael C.
name: Cooray, Asantha R.
name: Dolch, Timothy
name: Ferguson, Henry
name: Galametz, Audrey
name: Giavalisco, Mauro
name: Guo, Yicheng
name: Willner, Steven P.
name: Dickinson, Mark E.
name: Faber, Sandra M.
name: Fazio, Giovanni G.
name: Gardner, Jonathan P.
name: Gawiser, Eric
name: Grazian, Andrea
name: Grogin, Norman A.
name: Kocevski, Dale
name: Koo, David C.
name: Lee, Kyoung-Soo
name: Lucas, Ray A.
name: McGrath, Elizabeth J.
name: Nandra, Kirpal
name: Newman, Jeffrey A.
name: van der Wel, Arjen
Publisher: name: arXiv
Year: 2017
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We present a 0.4-8$μ$m multi-wavelength photometric catalog in the Extended Groth Strip (EGS) field. This catalog is built on the Hubble Space Telescope (HST) WFC3 and ACS data from the Cosmic Assembly Near-infrared Deep Extragalactic Legacy Survey (CANDELS), and it incorporates the existing HST data from the All-wavelength Extended Groth strip International Survey (AEGIS) and the 3D-HST program. The catalog is based on detections in the F160W band reaching a depth of F160W=26.62 AB (90% completeness, point-sources). It includes the photometry for 41457 objects over an area of $\approx 206$ arcmin$^2$ in the following bands: HST ACS F606W and F814W; HST WFC3 F125W, F140W and F160W; CFHT/Megacam $u^*$, $g'$, $r'$, $i'$ and $z'$; CFHT/WIRCAM $J$, $H$ and $K_\mathrm{S}$; Mayall/NEWFIRM $J1$, $J2$, $J3$, $H1$, $H2$, $K$; Spitzer IRAC $3.6μ$m, $4.5μ$m, $5.8μ$m and $8.0μ$m. We are also releasing value-added catalogs that provide robust photometric redshifts and stellar mass measurements. The catalogs are publicly available through the CANDELS repository.
description: ApJS in press. Catalogs can be accessed through the MAST archive at https://archive.stsci.edu/prepds/candels/
Increasing the Single-Bunch Instability Threshold by Bunch Splitting Due to RF Phase Modulation
Creators: name: Steinmann, Johannes L.
name: Blomley, Edmund
name: Brosi, Miriam
name: Bruendermann, Erik
name: Mochihashi, Akira
name: Schönfeldt, Patrik
name: Schuh, Marcel
name: Mueller, Anke-Susanne
Publisher: name: JACoW Publishing
Year: 2021

description: RF phase modulation at twice the synchrotron frequency can be used to split a stored electron bunch into two or more bunchlets orbiting each other. We report on time-resolved measurements at the KArlsruhe Research Accelerator (KARA), where this bunch splitting was used to increase the threshold current of the microbunching instability, happening in the short-bunch operation mode. Switching the modulation on and off, reproducibly influences the sawtooth behaviour of the emitted coherent synchrotron radiation.
Crystal field excitations and magnons: their roles in oxyselenides Pr2O2M2OSe2 (M = Mn, Fe)
Creators: name: Oogarah, R. K.
name: Stockdale, C. P. J.
name: Stock, C.
name: Evans, J. S. O.
name: Wills, A. S.
name: Taylor, J. W.
name: McCabe, E. E.
Publisher: name: arXiv
Year: 2017
Subjects: subject: Materials Science (cond-mat.mtrl-sci)
subject: FOS: Physical sciences

description: We present the results of neutron scattering experiments to study the crystal and magnetic structures of the Mott-insulating transition metal oxyselenides Pr2O2M2OSe2 (M = Mn, Fe). The structural role of the non-Kramers Pr3+ ion is investigated and analysis of Pr3+ crystal field excitations performed. Long-range order of Pr3+ moments in Pr2O2Fe2OSe2 can be induced by an applied magnetic field.
Accessing the Republic. Entity extraction from the resolutions of the Dutch States-General.
Creators: name: Koolen, Marijn
name: Renkema, Esger
name: Groskamp, Nienke
name: Smit, Frank
name: Reinders, Jirsi
name: Sluijter, Ronald
name: Hoekstra, Rik
name: Oddens, Joris
Publisher: name: Zenodo
Year: 2024
Subjects: named entity recognition
digital history
digital source publication
political history
data curation

description: This repository contains the abstract and presentation of our paper presented at the Digital Humanities in the BeNeLux 2024 (DH Benelux 2024) conference, held 4-7 June at KU Leuven in Leuven Belgium.

In this paper we report on our approach to extracting entities from the REPUBLIC corpus of the resolutions of the States General of the Dutch Republic 1576-1796. We describe 1) the construction of ground truth data for different types of entities, 2) the evaluation of NER taggers based on various types of embeddings for historical Dutch, 3) our findings from curating millions of occurrences of the different entity types, and 4) how the curation gives insights into the characteristics of the corpus.
Additional file 4 of Non-medical factors in prehospital resuscitation decision-making: a mixed-methods systematic review
Creators: name: Milling, Louise
name: Kjær, Jeannett
name: Binderup, Lars Grassmé
name: de Muckadell, Caroline Schaffalitzky
name: Havshøj, Ulrik
name: Christensen, Helle Collatz
name: Christensen, Erika Frischknecht
name: Lassen, Annmarie Touborg
name: Mikkelsen, Søren
name: Nielsen, Dorthe
Publisher: name: figshare
Year: 2022
Subjects: Medicine
Biotechnology
Science Policy
Computational Biology

description: Additional file 4. Overview of the synthesis process.
Additional file 1 of Pediatric biorepository participation during the COVID-19 pandemic: predictors of enrollment and biospecimen donation
Creators: name: Neilan, Anne M.
name: Tyagi, Anisha
name: Tong, Yao
name: Farkas, Eva J.
name: Burns, Madeleine D.
name: Fialkowski, Allison
name: Park, Grace
name: Hardcastle, Margot
name: Gootkind, Elizabeth
name: Bassett, Ingrid V.
name: Shebl, Fatma M.
name: Yonker, Lael M.
Publisher: name: figshare
Year: 2022
Subjects: subject: Medicine
subject: Microbiology
subject: FOS: Biological sciences
subject: Biotechnology
subject: Immunology
subject: FOS: Clinical medicine
subject: Biological Sciences not elsewhere classified
subject: Developmental Biology
subject: Infectious Diseases
subject: FOS: Health sciences
subject: Virology
subject: Computational Biology

description: Additional file 1.
Tuning across the BCS-BEC crossover in the multiband superconductor Fe$_{1+y}$Se$_x$Te$_{1-x}$ : An angle-resolved photoemission study
Creators: name: Rinott, S.
name: Ribak, K. B. Chashka A.
name: Taleb-Ibrahimi, E. D. L. Rienks A.
name: Fevre, P. Le
name: Bertran, F.
name: Randeria, M.
name: Kanigel, A.
Publisher: name: arXiv
Year: 2017
Subjects: subject: Superconductivity (cond-mat.supr-con)
subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: FOS: Physical sciences

description: The crossover from Bardeen-Cooper-Schrieffer (BCS) superconductivity to Bose-Einstein condensation (BEC) is difficult to realize in quantum materials because, unlike in ultracold atoms, one cannot tune the pairing interaction. We realize the BCS-BEC crossover in a nearly compensated semimetal Fe$_{1+y}$Se$_x$Te$_{1-x}$ by tuning the Fermi energy, $ε_F$, via chemical doping, which permits us to systematically change $Δ/ ε_F$ from 0.16 to 0.5 were $Δ$ is the superconducting (SC) gap. We use angle-resolved photoemission spectroscopy to measure the Fermi energy, the SC gap and characteristic changes in the SC state electronic dispersion as the system evolves from a BCS to a BEC regime. Our results raise important questions about the crossover in multiband superconductors which go beyond those addressed in the context of cold atoms.
title: ADCO, Sixième cartulaire de Saint-Étienne de Dijon (1662), Cart. 30 (G 133), 441 folios, f. 229
Creators: name: de la Côte d'Or, Archives départementales
name: Archives Départementales De La Côte-D'Or
name: Petot, Frédérique
name: Projet CBMA
name: Petot, Frédéric
name: CG21/F.PETOT/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: Sixième cartulaire de Saint-Étienne de Dijon (1662), Archives départementales de la Côte-d'Or, Cart. 30 (G 133), 441 folios, f. 229, Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Sixième cartulaire de Saint-Étienne de Dijon (1662), Archives départementales de la Côte-d'Or, Cart. 30 (G 133), 441 folios, f. 229, 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
Vibrational two-photon emission from coherently excited solid parahydrogen
Creators: name: Miyamoto, Yuki
name: Hara, Hideaki
name: Masuda, Takahiko
name: Sasao, Noboru
name: Uetake, Satoshi
name: Yoshimi, Akihiro
name: Yoshimura, Koji
name: Yoshimura, Motohiko
Publisher: name: arXiv
Year: 2016
Subjects: subject: Chemical Physics (physics.chem-ph)
subject: Atomic Physics (physics.atom-ph)
subject: FOS: Physical sciences

description: We report observation of two-photon emission from coherently excited vibrational state of solid parahydrogen, known as one of quantum solids. The coherent state between the ground and the excited states is prepared by stimulated Raman scattering using two visible laser pulses. The two-photon emission is triggered by another mid-infrared laser pulse. The observed two-photon emission persists even when the trigger pulse is injected long after the excitation. The observed phenomenon is due to a long decoherence time of the vibrational states of solid parahydrogen, which is attributed to special nature as quantum solid. Dependence of the decoherence on target temperature and residual orthohydrogen concentration are studied along with its time evolution. It is found that the emission intensity increases even after the excitation pulses pass through the target completely. The coherence development is highly suppressed at high target temperature and high residual orthohydrogen concentration. Effects of target annealing and laser-induced damage on the target are also observed.
Additional file 3 of Non-medical factors in prehospital resuscitation decision-making: a mixed-methods systematic review
Creators: name: Milling, Louise
name: Kjær, Jeannett
name: Binderup, Lars Grassmé
name: de Muckadell, Caroline Schaffalitzky
name: Havshøj, Ulrik
name: Christensen, Helle Collatz
name: Christensen, Erika Frischknecht
name: Lassen, Annmarie Touborg
name: Mikkelsen, Søren
name: Nielsen, Dorthe
Publisher: name: figshare
Year: 2022
Subjects: Medicine
Biotechnology
Science Policy
Computational Biology

description: Additional file 3. List of search terms.