cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Additional file 3: of Multimorbidity patterns with K-means nonhierarchical cluster analysis
Creators: name: Violán, Concepción
name: Roso-Llorach, Albert
name: Quintí Foguet-Boreu
name: Guisado-Clavero, Marina
name: Mariona Pons-Vigués
name: Pujol-Ribera, Enriqueta
name: Valderas, Jose
Publisher: name: figshare
Year: 2018
Subjects: subject: Molecular Biology
subject: Biotechnology
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: Developmental Biology
subject: Science Policy

description: Diagnosis blocks (ICD 10) included in the Multimorbidity patterns in women and men aged 45–65 years, Catalonia, 2010. (DOCX 26 kb)
Chern classes and extraspecial groups
Creators: name: Green, David J
name: Leary, Ian J
Publisher: name: arXiv
Year: 2007
Subjects: subject: Group Theory (math.GR)
subject: Algebraic Topology (math.AT)
subject: FOS: Mathematics
subject: 20J06

description: The mod-p cohomology ring of the extraspecial p-group of exponent p is studied for odd p. We investigate the subquotient ch(G) generated by Chern classes modulo the nilradical. The subring of ch(G) generated by Chern classes of one-dimensional representations was studied by Tezuka and Yagita. The subring generated by the Chern classes of the faithful irreducible representations is a polynomial algebra. We study the interplay between these two families of generators, and obtain some relations between them.
Constraints on the properties of macroscopic transport in the Sun from combined lithium and beryllium depletion
Creators: name: Buldgen, G.
name: Noels, A.
name: Amarsi, A. M.
name: Nandal, D.
name: Pezzotti, C.
name: Scuflaire, R.
name: Deal, M.
name: Grevesse, N.
Publisher: name: arXiv
Year: 2025
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: Context. The Sun is a privileged laboratory of stellar evolution, thanks to the quality and complementary nature of available constraints. Using these observations, we are able to draw a detailed picture of its internal structure and dynamics which form the basis of the successes of solar modelling. Amongst such constraints, the depletion of lithium and beryllium are key tracers of the required efficiency and extent of macroscopic mixing just below the solar convective envelope. Thanks to revised determinations of these abundances, we may use them in conjunction with other existing spectroscopic and helioseismic constraints to study in detail the properties of macroscopic transport. Aims. We aim at constraining the efficiency of macroscopic transport at the base of the convective envelope and determining the compatibility of the observations with a suggested candidate linked with the transport of angular momentum in the solar radiative interior. Methods. We use recent spectroscopic observations of lithium and beryllium abundance and include them in solar evolutionary model calibrations. We test the agreement of such models in terms of position of the convective envelope, helium mass fraction in convective zone, sound speed profile inversions and neutrino fluxes. Results. We constrain the required efficiency and extent of the macroscopic mixing at the base of the solar convective envelope, finding that a power law of density with an index n between 3 and 6 would reproduce the data, with efficiencies at the base of the envelope of about 6000 cm2 /s, depending on the value of n. We also confirm that macroscopic mixing worsens the agreement with neutrino fluxes and that the current implementations of the magnetic Tayler instability are unable to explain the observations.
description: Accepted for publication in Astronomy and Astrophysics
Quantum fields during black hole formation: How good an approximation is the Unruh state?
Creators: name: Juárez-Aubry, Benito A.
name: Louko, Jorma
Publisher: name: arXiv
Year: 2018
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We study the quantum effects of a test Klein-Gordon field in a Vaidya spacetime consisting of a collapsing null shell that forms a Schwazschild black hole, by explicitly obtaining, in a $(1+1)$-dimensional model, the Wightman function, the renormalised stress-energy tensor, and by analysing particle detector rates along stationary orbits in the exterior black hole region, and make a comparison with the folklore that the Unruh state is the state that emerges from black hole formation. In the causal future of the shell, we find a negative ingoing flux at the horizon that agrees precisely with the Unruh state calculation, and is the source of black hole radiation, while in the future null infinity we find that the radiation flux output in the Unruh state is an upper bound for the positive outgoing flux in the collapsing null shell spacetime. This indicates that back-reaction estimates based on Unruh state calculations over-estimate the energy output carried by so-called pre-Hawking radiation. The value of the output predicted by the Unruh state is however approached exponentially fast. Finally, we find that at late times, stationary observers in the exterior black hole region in the collapsing shell spacetime detect the local Hawking temperature, which is also well characterised by the Unruh state, coming from right-movers. Early-time discrepancies between the detector rates for the Unruh state and for the state in the collapsing shell spacetime are explored numerically.
description: V2. 25 pages, 7 figures. Minor errors and typos fixed. Added references. Expanded discussion in Sec. 2.2 and 4.3
The evolution of the flux-size relationship in protoplanetary discs by viscous evolution and radial pebble drift
Creators: name: Appelgren, Johan
name: Johansen, Anders
name: Lambrechts, Michiel
name: Jørgensen, Jes
name: van der Marel, Nienke
name: Ohashi, Nagayoshi
name: Tobin, John
Publisher: name: arXiv
Year: 2025
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: FOS: Physical sciences

description: In this paper we study the evolution of radiative fluxes, flux radii and observable dust masses in protoplanetary discs, in order to understand how these depend on the angular momentum budget and on the assumed heat sources. We use a model that includes the formation and viscous evolution of protoplanetary gas discs, together with the growth and radial drift of the dust component. We find that we are best able to match the observed fluxes and radii of class 0/I discs when we assume (i) an initial total angular momentum budget corresponding to a centrifugal radius of 40 au around solar-like stars, and (ii) inefficient viscous heating. Fluxes and radii of class II discs appear consistent with disc models with angular momentum budgets equivalent to centrifugal radii of both 40 au or 10 au for solar like stars, and with models where viscous heating occurs at either full efficiency or at reduced efficiency. During the first 0.5 Myr of their evolution discs are generally optically thick at a wavelength of 1.3 mm. However, after this discs are optically thin at mm-wavelengths, supporting standard means of dust mass estimates. Using a disc population synthesis model, we then show that the evolution of the cumulative evolution of the observable dust masses agrees well with that observed in young star forming clusters of different ages.
description: 12 pagers, 12 figures
title: ADCO, Cartulaire général de Cîteaux, dit de Jean de Cirey, (XVe siècle), tome I, Cart. 185 (11 H 70), f. 0058r
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: cartulaire
subject: Corpus Burgundiae Medii Aevi
subject: Chartes de la Bourgogne du Moyen Âge
subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris

description: Cartulaire général de Cîteaux, dit de Jean de Cirey, (XVe siècle), tome I, Archives départementales de la Côte-d'Or, Cart. 185 (11 H 70), f. 0058r, 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 I, Archives départementales de la Côte-d'Or, Cart. 185 (11 H 70), f. 0058r, in Projet CBMA - Corpus Burgundiae Medii Aevi [Ressource en ligne], https:// manuscrits.cbma-project.eu/
description: Provenance: abbaye de Cîteaux
description: Provenance: http://www.wikidata.org/entity/Q843261
description: Provenance: https://www.geonames.org/3024876
description: Provenance: http://www.idref.fr/030974844/id
description: Provenance: https://catalogue.bnf.fr/ark:/12148/cb12228351v
Trends in Large Scale Structure Observations and the Likelihood of Early Reionization
Creators: name: Liddle, Andrew R
name: Lyth, David H
Publisher: name: arXiv
Year: 1994
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: With the imminent promise of constraints on the epoch of reionization from observations of microwave background anisotropies, the question of whether or not the standard Cold Dark Matter (CDM) model permits early reionization has been subjected to detailed investigation by various authors, with the conclusion that reionization may occur at quite high redshift. However, it is widely accepted that this model is excluded, as when normalised to the COBE observations it possesses excessive galaxy clustering on scales below tens of megaparsecs. We examine the trends of observations, first in a fairly model independent way, and second by considering variants on the standard CDM model introduced to resolve the observational conflicts. We conclude that the epoch of reionization favoured by the observational data is typically considerably later than the standard CDM model suggests, and amongst models which may fit the observational data only the introduction of a cosmological constant leads to a reionization redshift close to that of standard CDM.
description: 8 pages uuencoded postscript (LaTeX file available from ARL), changes include correction of the previously mishandled cosmological constant case (leading also to slight changes in abstract and conclusions) plus an update of the COBE normalisation
Additional file 5: of Phylogeography and genetics of the globally invasive snail Physa acuta Draparnaud 1805, and its potential to serve as an intermediate host to larval digenetic trematodes
Creators: name: Ebbs, Erika
name: Loker, Eric
name: Brant, Sara
Publisher: name: figshare
Year: 2018
Subjects: subject: Microbiology
subject: FOS: Biological sciences
subject: Genetics
subject: Molecular Biology
subject: 59999 Environmental Sciences not elsewhere classified
subject: FOS: Earth and related environmental sciences
subject: Ecology
subject: 69999 Biological Sciences not elsewhere classified

description: ITS1 phylogeny estimated using Bayesian inference. Physa acuta samples are colored according to the clade they were recovered from based on mitochondrial gene tree analysis: pink = Clade A, green = Clade B. Physa acuta taxa labeled as black did not group within P. acuta based on mitochondrial gene trees, and were excluded from all in-group analyses (S17, S120 and all P. zionis samples). ITS1 data only exists for HQ283259 and Pacuta_18S/ITS and were therefore not included in mitochondrial gene tree analyses. Posterior probabilities are illustrated as branch support values. (PDF 143 kb)
title: Populism, extremism and cultural change as traceable in the European Value Study and the European Social Survey, Supplementary Material
title: VALUES AND CLEAVAGES IN EUROPEAN poliTICAL CULTURES IN THE PAST FOUR DECADES
titleType: AlternativeTitle
Creators: name: Troitzsch, Klaus G.
Publisher: name: Springer
Year: 2024
Subjects: value change, populism, extremism, polarisation, skewed distribution, political culture, European Value Study

description: The three versions of the supplementary material collects some additional information beyond the data and methods used in the main paper (DOI:10.1007/978-3-031-43440-2_7) and in two talks given in the ECPR Standing Group on Political Culture Political Culture Lecture Series on April 10, 2024 and November 13, 2024, respectively, and all the tables and figures for individual countries on which the interpretations and conclusions of the talk are based.
RETURN To an Address of the Legislative Assembly for a Return of all moneys paid in connection with the dispatch of Volunteers, or Militia, to Nanaimo, relative to the Miners' Strike, in the Spring of 1877, showing to whom paid and the amount in each case, together with the authority for such payment.
Creators: name: British Columbia. Legislative Assembly
Publisher: name: Victoria, BC : Government Printer
Year: 2016

Abstract
Soils or sediments? The role of Roger Langohr's process-oriented approach in understanding carbonate-related palaeosols of the stratigraphic record.
Creators: name: Mindszenty, Andrea
Publisher: name: Zenodo
Year: 2019
Subjects: carbonate palaeosols, soil-maturity, climate signal, Late Triassic, Hungary

description: ABSTRACT This paper is a summary of palaeopedologically-oriented research on and the interpretation of subaerial exposure-related features in cyclically organised shallow marine carbonates. We point out that the structure of soil profiles in such environments cannot be interpreted simply in terms of pedogenesis. Apparent soil-thickness is not necessarily proportional with soil-maturity and clays and secondary carbonates are not always direct indicators of climate, either.
description: This article is part of a book edited at the occasion of the Geoarchaeological meeting of Bruges: Soils as records of Past and Present: the geoarchaeological approach. Focus on: is there time for fieldwork today? - Bruges (Belgium), 6 and 7.11.2019. Editors Judit Deák, Carole Ampe and Jari Hinsch Mikkelsen Technical editor Mariebelle Deceuninck English language reviewer Caroline Landsheere Graphic design Frederick Moyaert Printing and binding Die Keure, Bruges
Milky Way Cepheid Standards for Measuring Cosmic Distances and Application to Gaia DR2: Implications for the Hubble Constant
Creators: name: Riess, Adam G.
name: Casertano, Stefano
name: Yuan, Wenlong
name: Macri, Lucas
name: Bucciarelli, Beatrice
name: Lattanzi, Mario G.
name: MacKenty, John W.
name: Bowers, J. Bradley
name: Zheng, Weikang
name: Filippenko, Alexei V.
name: Huang, Caroline
name: Anderson, Richard I.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: We present HST photometry of a selected sample of 50 long-period, low-extinction Milky Way Cepheids measured on the same WFC3 F555W, F814W, and F160W-band photometric system as extragalactic Cepheids in SN Ia hosts. These bright Cepheids were observed with the WFC3 spatial scanning mode in the optical and near-infrared to mitigate saturation and reduce pixel-to-pixel calibration errors to reach a mean photometric error of 5 millimags per observation. We use the new Gaia DR2 parallaxes and HST photometry to simultaneously constrain the cosmic distance scale and to measure the DR2 parallax zeropoint offset appropriate for Cepheids. We find a value for the zeropoint offset of -46 +/- 13 muas or +/- 6 muas for a fixed distance scale, higher than found from quasars, as expected, for these brighter and redder sources. The precision of the distance scale from DR2 has been reduced by a factor of 2.5 due to the need to independently determine the parallax offset. The best fit distance scale is 1.006 +/- 0.033, relative to the scale from Riess et al 2016 with H0=73.24 km/s/Mpc used to predict the parallaxes photometrically, and is inconsistent with the scale needed to match the Planck 2016 CMB data combined with LCDM at the 2.9 sigma confidence level (99.6%). At 96.5% confidence we find that the formal DR2 errors may be underestimated as indicated. We identify additional error associated with the use of augmented Cepheid samples utilizing ground-based photometry and discuss their likely origins. Including the DR2 parallaxes with all prior distance ladder data raises the current tension between the late and early Universe route to the Hubble constant to 3.8 sigma (99.99 %). With the final expected precision from Gaia, the sample of 50 Cepheids with HST photometry will limit to 0.5% the contribution of the first rung of the distance ladder to the uncertainty in the Hubble constant.
description: accepted to ApJ, 14 pages, 7 figures
Curbing the tide: The discovery of a Roman terp along the Heistlaan in Ramskapelle (Knokke-Heist, Belgium)
Creators: name: Verwerft, Dieter
name: Hinsch Mikkelsen, Jari
name: De Clerq, Win
Publisher: name: Zenodo
Year: 2019
Subjects: Roman archaeology, coastal plain of Flanders, terp, soil science, micromorphology

description: ABSTRACT: Archaeologists have long struggled trying to understand the nature of the Roman-period occupation of the coastal plain of Flanders. From the start of the 21st century, following academic and development-led projects, knowledge on the nature of the Roman occupation in the coastal plain has gradually been expanding. To assess the possible destruction of archaeological remains in the area along the A11-highway connection between Damme, Knokke-Heist, and Bruges, a different methodology was implemented. This resulted in the discovery of a 2nd to 3rd century AD site along the Heistlaan in Ramskapelle (Knokke-Heist). Based on geo-archaeological and sedimentological observations, coupled with micromorphological data, the site is interpreted as an artificial dwelling mound or terp. This discovery is a significant step in understanding the impact of human activities on the landscape in the coastal plain. The results help reinterpret older excavation data and aid future research projects.
description: This article is part of a book edited at the occasion of the Geoarchaeological meeting of Bruges: Soils as records of Past and Present: the geoarchaeological approach. Focus on: is there time for fieldwork today? - Bruges (Belgium), 6 and 7.11.2019. Editors Judit Deák, Carole Ampe and Jari Hinsch Mikkelsen Technical editor Mariebelle Deceuninck English language reviewer Caroline Landsheere Graphic design Frederick Moyaert Printing and binding Die Keure, Bruges
Additional file 3: of Understanding the implementation and efficacy of a home-based strength and balance fall prevention intervention in people aged 50Â years or over with vision impairment: a process evaluation protocol
Creators: name: Dillon, Lisa
name: Clemson, Lindy
name: Coxon, Kristy
name: Keay, Lisa
Publisher: name: figshare
Year: 2018
Subjects: subject: Medicine
subject: Sociology
subject: FOS: Sociology
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: Science Policy
subject: Computational Biology

description: Appendix 3. Participant Enactment. Survey questions, adapted from the Self-Report Habit Index. (DOCX 13 kb)
Populism, extremism and cultural change as traceable in the European Value Study Supplementary Material
Creators: name: Troitzsch, Klaus G.
Publisher: name: Zenodo
Year: 2023
Subjects: value change, populism, extremism, polarisation, skewed distribution, political culture, European Value Study

description: This supplementary material collects some additional information about the methods used in the main paper (DOI:10.1007/978-3-031-43440-2_7) and all the tables and figures for individual countries on which the interpretations and conclusions of the main paper are based.
Additional file 1 of The genetic architecture of temperature adaptation is shaped by population ancestry and not by selection regime
Creators: name: Otte, Kathrin A.
name: Nolte, Viola
name: Mallard, François
name: Schlötterer, Christian
Publisher: name: figshare
Year: 2021
Subjects: subject: Genetics
subject: FOS: Biological sciences

description: Additional file 1: Figure S1. Female fecundity as proxy for fitness in the ancestral population and for each evolved replicate in the Florida and Portugal populations. Figure S2. The inverse relationship between starting allele frequency and selection coefficient is robust to the definition of the selected allele. Figure S3. Histogram of the number of genes per reconstructed haplotype block in the cold-evolved Portugal population. Figure S4. Selected haplotype blocks from replicated D. simulans populations from Portugal evolving in a novel hot environment. Figure S5. Allele frequency changes between the founder and the evolved populations. Figure S6. Selected haplotype blocks from replicated D. simulans populations from Florida evolving in a novel hot environment. Figure S7. The adaptive architecture is population-specific but does not depend on the temperature regime. Figure S8. Replicate populations derived from Portugal founders show a more similar selection response than those with Florida ancestry. Figure S9. Linkage disequilibrium in the ancestral Florida population.
Neutron stars with spin polarized self-interacting dark matter
Creators: name: Rezaei, Zeinab
Publisher: name: arXiv
Year: 2018
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: Dark matter, one of the important portion of the universe, could affect the visible matter in neutron stars. An important physical feature of dark matter is due to the spin of dark matter particles. Here, applying the piecewise polytropic equation of state for the neutron star matter and the equation of state of spin polarized self-interacting dark matter, we investigate the structure of neutron stars which are influenced by the spin polarized self-interacting dark matter. The behavior of the neutron star matter and dark matter portions for the stars with different values of the interaction between dark matter particles and spin polarization of dark matter is considered. In addition, we present the value of the gravitational redshift of these stars in different cases of spin polarized and self-interacting dark matter.
description: 16 pages, 7 figures. Accepted for publication in Astroparticle Physics
The byres tale: farming nutrient-poor coversands at the edge of the Roman Empire (NW-Belgium)
Creators: name: Hinsch Mikkelsen, Jari
name: Langohr, Roger
name: Vanwesenbeeck, Veerle
name: Bourgeois, Ignace
name: De Clercq, Wim
Publisher: name: Zenodo
Year: 2019
Subjects: byre, potstal, cover sands, Gallo-Roman period, northern Belgium, soil micromorphology, archaeopedology

description: ABSTRACT Prior to the construction of a highABSTRACT-speed railway track (TGV) between Antwerp (Belgium) and the Dutch border, archaeological and geoarchaeological research was conducted at several archaeological sites. All are situated in the northern Campine, a region characterised by quartz-rich, nutrient-poor cover sands. On the site of Brecht-Zoegweg, two well preserved deepened byres (‘potstallen’) were uncovered in Roman stable-houses. Stables with sunken floors are commonly recorded on Roman-period farms in the sandy part of northern Belgium. Following medieval to sub-recent parallels in the area, they are considered to be features serving agricultural fertilising purposes through the intentional accumulation of dung and the creation of manure by mixing with added organic matter (sods or ‘plaggen’). This archaeopedological research investigates several questions concerning the origin and the infill process of these remarkable features. Field observations, analytical and micromorphological data point to a gradual succession of events leading to a byre with a sunken floor, rather than an intentional digging out of the floor concomitant with the house construction and a post-occupational filling or levelling. It is furthermore suggested that plaggen fertilisation could indeed have been applied, at least in some of the phases of the byre use.
description: This article is part of a book edited at the occasion of the Geoarchaeological meeting of Bruges: Soils as records of Past and Present: the geoarchaeological approach. Focus on: is there time for fieldwork today? - Bruges (Belgium), 6 and 7.11.2019. Editors Judit Deák, Carole Ampe and Jari Hinsch Mikkelsen Technical editor Mariebelle Deceuninck English language reviewer Caroline Landsheere Graphic design Frederick Moyaert Printing and binding Die Keure, Bruges
Dyson's Brownian Motion and Universal Dynamics of Quantum Systems
Creators: name: Narayan, Onuttom
name: Shastry, B. Sriram
Publisher: name: arXiv
Year: 1993
Subjects: subject: Condensed Matter (cond-mat)
subject: FOS: Physical sciences

description: We establish a correspondence between the evolution of the distribution of eigenvalues of a $N\times N$ matrix subject to a random Gaussian perturbing matrix, and a Fokker-Planck equation postulated by Dyson. Within this model, we prove the equivalence conjectured by Altshuler et al between the space-time correlations of the Sutherland-Calogero-Moser system in the thermodynamic limit and a set of two-variable correlations for disordered quantum systems calculated by them. Multiple variable correlation functions are, however, shown to be inequivalent for the two cases.
description: 10 pages, revtex
Nuclear skin emergence in Skyrme deformed Hartree-Fock calculations
Creators: name: Sarriguren, P.
name: Gaidarov, M. K.
name: de Guerra, E. Moya
name: Antonov, A. N.
Publisher: name: arXiv
Year: 2007
Subjects: subject: Nuclear Theory (nucl-th)
subject: FOS: Physical sciences

description: A study of the charge and matter densities and the corresponding rms radii for even-even isotopes of Ni, Kr, and Sn has been performed in the framework of deformed self-consistent mean field Skyrme HF+BCS method. The resulting charge radii and neutron skin thicknesses of these nuclei are compared with available experimental data, as well as with other theoretical predictions. The formation of a neutron skin, which manifests itself in an excess of neutrons at distances greater than the radius of the proton distribution, is analyzed in terms of various definitions. Formation of a proton skin is shown to be unlikely. The effects of deformation on the neutron skins in even-even deformed nuclei far from the stability line are discussed.
description: 16 pages, 17 figures, to be published in Physical Review C
Soil and archaeology groundwork for landscape development projects of the Flemish Land Agency – the case study of Assebroek.
Creators: name: Ampe, Carole
name: Korneel Gheysen, Korneel
Publisher: name: Zenodo
Year: 2019
Subjects: circular structure, peat, limnic material, land development project

description: ABSTRACT: This paper describes the preliminary soil and archaeological research carried out by the Flemish Land Agency, to achieve a well substantiated project design. At the circular structure of Ver-Assebroek (Bruges), the site of a former medieval castle, a landscape development project aims to increase the visibility of the structure while respecting the soil values and archaeological structures on the site.
description: This article is part of a book edited at the occasion of the Geoarchaeological meeting of Bruges: Soils as records of Past and Present: the geoarchaeological approach. Focus on: is there time for fieldwork today? - Bruges (Belgium), 6 and 7.11.2019. Editors Judit Deák, Carole Ampe and Jari Hinsch Mikkelsen Technical editor Mariebelle Deceuninck English language reviewer Caroline Landsheere Graphic design Frederick Moyaert Printing and binding Die Keure, Bruges
On universally stable elements
Creators: name: Leary, I. J.
name: Schuster, B.
name: Yagita, N.
Publisher: name: arXiv
Year: 2007
Subjects: subject: Group Theory (math.GR)
subject: Algebraic Topology (math.AT)
subject: FOS: Mathematics

description: We show that certain subrings of the cohomology of a finite p-group P may be realised as the images of restriction from suitable virtually free groups. We deduce that the cohomology of P is a finite module for any such subring. Examples include the ring of `universally stable elements' defined by Evens and Priddy, and rings of invariants such as the mod-2 Dickson algebras.
Additional file 3 of The genetic architecture of temperature adaptation is shaped by population ancestry and not by selection regime
Creators: name: Otte, Kathrin A.
name: Nolte, Viola
name: Mallard, François
name: Schlötterer, Christian
Publisher: name: figshare
Year: 2021
Subjects: subject: Genetics
subject: FOS: Biological sciences

description: Additional file 3. Review history.
The Hall Number of Strongly Correlated Metals
Creators: name: Auerbach, Assa
Publisher: name: arXiv
Year: 2018
Subjects: subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: FOS: Physical sciences

description: An exact formula for the temperature dependent Hall number of metals is derived. It is valid for non-relativistic fermions or bosons, with arbitrary potential and interaction. This DC transport coefficient is proven to (remarkably) depend solely on equilibrium susceptibilities, which are more amenable to numerical algorithms than the conductivity. An application to strongly correlated phases is demonstrated by calculating the Hall sign in the vicinity of Mott phases of lattice bosons.
description: 2 Figures, including supplementary material
The $\texttt{MSG}$ model for cloudy substellar atmospheres: A grid of self-consistent substellar atmosphere models with microphysical cloud formation
Creators: name: Estrada, Beatriz Campos
name: Lewis, David A.
name: Helling, Christiane
name: Booth, Richard A.
name: Martínez, Francisco Ardévol
name: Jørgensen, Uffe G.
Publisher: name: arXiv
Year: 2025
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: State-of-the-art JWST observations are unveiling unprecedented views into the atmospheres of substellar objects in the infrared, further highlighting the importance of clouds. Current forward models struggle to fit the silicate clouds absorption feature at ~$10\,μ$m observed in substellar atmospheres. In the MSG model, we aim to couple the MARCS 1D radiative-convective equilibrium atmosphere model with the 1D kinetic, stationary, non-equilibrium, cloud formation model DRIFT, to create a new grid of self-consistent cloudy substellar atmosphere models with microphysical cloud formation. We aim to test if this new grid is able to reproduce the silicate cloud absorption feature at ~$10\,μ$m. We model substellar atmospheres with effective temperatures in the range 1200-2500 K and with $\log(g)=4.0$. We compute atmospheric structures that self-consistently account for condensate cloud opacities based on microphysical properties. We present an algorithm based on control theory to help converge such self-consistent models. Synthetic atmosphere spectra are computed for each model to explore the observable impact of the cloud microphysics. We additionally explore the impact of choosing different nucleation species (TiO$_2$ or SiO) and the effect of less efficient atmospheric mixing on these spectra. The new MSG cloudy grid using TiO$_2$ nucleation shows spectra which are redder in the near-infrared compared to the currently known population of substellar atmospheres. We find the models with SiO nucleation, and models with reduced mixing efficiency are less red in the near-infrared. The grid is unable to reproduce the silicate features similar to those found in recent JWST observations and Spitzer archival data. We thoroughly discuss further work that may better approximate the impact of convection in cloud-forming regions and steps that may help resolve the silicate cloud feature.
description: Accepted for publication in A&A
Imaging a non-singular rotating black hole at the center of the Galaxy
Creators: name: Lamy, Frédéric
name: Gourgoulhon, Eric
name: Paumard, Thibaut
name: Vincent, Frédéric H.
Publisher: name: arXiv
Year: 2018
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: We show that the rotating generalization of Hayward's non-singular black hole previously studied in the literature is geodesically incomplete, and that its straightforward extension leads to a singular spacetime. We present another extension, which is devoid of any curvature singularity. The obtained metric depends on three parameters and, depending on their values, yields an event horizon or not. These two regimes, named respectively regular rotating Hayward black hole and naked rotating wormhole, are studied both numerically and analytically. In preparation for the upcoming results of the Event Horizon Telescope, the images of an accretion torus around Sgr A*, the supermassive object at the center of the Galaxy, are computed. These images contain, even in the absence of a horizon, a central faint region which bears a resemblance to the shadow of Kerr black holes and emphasizes the difficulty of claiming the existence of an event horizon from the analysis of strong-field images. The frequencies of the co- and contra-rotating orbits at the innermost stable circular orbit (ISCO) in this geometry are also computed, in the hope that quasi-periodic oscillations may permit to compare this model with Kerr's black hole on observational grounds.
description: 25 pages, 31 figures; v2: two figures and some clarifications added, version published in CQG
Fusion and singular vectors in A1{(1)} highest weight cyclic modules
Creators: name: Bauer, M.
name: Sochen, N.
Publisher: name: arXiv
Year: 1992
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We show how the interplay between the fusion formalism of conformal field theory and the Knizhnik--Zamolodchikov equation leads to explicit formulae for the singular vectors in the highest weight representations of A1{(1)}.
description: 42 pages
SOLVENCY RATIO AND FINANCIAL PERFORMANCE OF LISTED INDUSTRIAL GOODS FIRM IN NIGERIA EXCHANGE GROUP
Creators: name: Dr. Obani, Chimaobi Desmond
name: Dr. Ozuomba, Chidinma Nwamaka
name: Dr.  Agu, Charles Ikechukwu
name: Dr. Ogujiofor, Magnus Nkemjika
Publisher: name: SADI JOURNALS
Year: 2024
Subjects: Solvency Ratio, Financial Performance, Industrial Goods Firms, Debt-to-Asset Ratio, Return on Assets

description: The study examined solvency ratio and financial performance of industrial goods firms in Nigeria. Three specific objectives and hypotheses were formulated. The study adopted ex-post facto research design. Cross sectional panel data secondarily sourced from the annual financial reports and accounts of nine (9) listed industrial goods firms in Nigeria, from 2013 to 2023 were analyzed using descriptive statistics, normality graph, hausman specification test, and ordinary least square regression analyses with the aid of E-view 9 at 5% level of significance. The study proxy Solvency using Interest coverage ratio, debt to asset ratio and debt to equity ratio as explanatory variables while financial performance proxy using return on asset as response variable. The findings shown that the coefficient of interest coverage ratio is -0.012 and has a negative relationship with return on asset. The coefficient for Debt to asset ratio is -0.76 and has insignificant relationship with return on asset while the coefficient for debt-to-equity ratio is 0.05 with a positive relationship with return on asset of industrial goods firms in Nigeria. The study concludes that debt to asset ratio is the only significant variable on return on asset of listed industrial goods firms in Nigeria Exchange Group. Although interest coverage ratio and debt to equity ratio financial maintain negative and positive coefficients respectively with insignificant effect on the return on asset of listed industrial goods firms in Nigeria Exchange Group and recommends that managers of industrial goods firms in Nigeria should proficiently strategize the interest coverage ratio of the firms, in a manner that the Operational efficiency of the firm takes comparative advantage over the exposure of investment risk.
On the Internal Structure of the Singlet d$_{X^2-Y^2}$ Hole Pair in an Antiferromagnet
Creators: name: Poilblanc, Didier
Publisher: name: arXiv
Year: 1993
Subjects: subject: Condensed Matter (cond-mat)
subject: FOS: Physical sciences

description: Exact diagonalizations of two dimensional small t--J clusters reveal dominant hole-hole correlations at distance $\sqrt{2}$ (ie between holes on next nearest neighbor sites). A new form of singlet $d_{x^2-y^2}$ pair operator is proposed to account for the spatial extention of the two hole-bound pair beyond nearest neighbor sites.
description: Report LPQTH-93/07, Latex file, 7 pages, 2 figures on request
RETURN To an Address of the Legislative Assembly for a Return showing the number of patients admitted into the Hospitals of Victoria, New Westminster, Nanaimo, and Cariboo, respectively, from January 1st, 1878, to January 1st, 1879, together with all other particulars in connection with each patient as entered in the record books or journals of each Hospital.
Creators: name: British Columbia. Legislative Assembly
Publisher: name: Victoria, BC : Government Printer
Year: 2016

Abstract
Additional file 1 of Automated closed-loop management of body temperature using forced-air blankets: preliminary feasibility study in a porcine model
Creators: name: Jรถrg Peter
name: Klingert, Kathrin
name: Klingert, Wilfried
name: Thiel, Karolin
name: Kรถnigsrainer, Alfred
name: Grasshoff, Christian
name: Rosenstiel, Wolfgang
name: Schenk, Martin
Publisher: name: figshare
Year: 2018
Subjects: subject: Space Science
subject: Medicine
subject: 59999 Environmental Sciences not elsewhere classified
subject: FOS: Earth and related environmental sciences
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: Computational Biology

description: Interface schematics. The additional file interface-schematic.pdf contains full electronic schematics for the presented hardware interface to the 3M Bair Hugger 755. (PDF 84.1 kb)
Bounds on the Light Quark Masses: the scalar channel revisited
Creators: name: Dominguez-Clarimon, Alexandre
name: de Rafael, Eduardo
name: Taron, Josep
Publisher: name: arXiv
Year: 2007
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We evaluate lower bounds on the sum of the up and down quark masses. The bounds follow from the constraints provided by the dispersion relation obeyed by the two--point function of the scalar current density when combined with properties of the scalar spectral function at long--distances and perturbative QCD at short--distances. Our results point to values of $m_u+m_d$ somewhat higher than those reported recently in the literature using lattice QCD simulations.
description: 7 pages, 3figures. A few sentences have been added to improve clarity. One reference added. To be published in PLB
Dwarf Elliptical Galaxies
Creators: name: Ferguson, Henry C.
name: Binggeli, Bruno
Publisher: name: arXiv
Year: 1994
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Dwarf elliptical (dE) galaxies, with blue absolute magnitudes typically fainter than $M_B = -16$, are the most numerous type of galaxy in the nearby universe. Tremendous advances have been made over the past several years in delineating the properties of both Local Group satellite dE's and the large dE populations of nearby clusters. We review some of these advances, with particular attention to how well currently available data can constrain 1) models for the formation of dE's, 2) the physical and evolutionary connections between different types of galaxies (nucleated and nonnucleated dE's, compact E's, irregulars, and blue compact dwarfs) that overlap in the same portion of the mass-spectrum of galaxies, 3) the contribution of dE's to the galaxy luminosity functions in clusters and the field, 4) the star-forming histories of dE's and their possible contribution to faint galaxy counts, and 5) the clustering properties of dE's. In addressing these issues, we highlight the extent to which selection effects temper these constraints, and outline areas where new data would be particularly valuable.
description: 63p, uuencoded compressed postscript, 2/8 figs included, A&A Review in press, request paper copies from ferguson@stsci.edu, STScI 866
Additional file 1 of “We are only looking at the tip of the iceberg in infertility”: perspectives of health providers about fertility issues and management among Aboriginal and Torres Strait Islander people
Creators: name: Gilbert, Emily
name: Walker, Ruth
name: Simon, David
name: Derkenne, Ruth
name: Rumbold, Alice
name: Campbell, Sandra
name: Boyle, Jacqueline A
Publisher: name: figshare
Year: 2021
Subjects: subject: Cell Biology
subject: Biotechnology
subject: Ecology
subject: FOS: Biological sciences
subject: 69999 Biological Sciences not elsewhere classified
subject: Cancer
subject: Science Policy

description: Additional file 1.
AGN astrometry: A powerful tool for galaxy kinematic studies
Creators: name: Kimani, Naftali
Publisher: name: Zenodo
Year: 2019

description: The presentation highlights the successes of the high resolution astrometric VLBI observations used for measuring proper motion of galaxies in the Local group. The required high accuracies are only attainable through the use of the phase-referencing technique which require either a compact radio source (AGN) or strong maser emission in the target galaxy and, additionally, some compact extra-galactic radio sources (quasars) to serve as ideal background reference source. The derived proper motions can lead to lower limits on the orbital lower estimates to the mass of the host galaxy, promise a new handle on dynamical models of interacting galaxy systems and offer insights on the spatial distribution of dark matter in the near universe.
The PLATO field selection process. II. Characterization of LOPS2, the first long-pointing field
Creators: name: Nascimbeni, V.
name: Piotto, G.
name: Cabrera, J.
name: Montalto, M.
name: Marinoni, S.
name: Marrese, P. M.
name: Aerts, C.
name: Altavilla, G.
name: Benatti, S.
name: Börner, A.
name: Deleuil, M.
name: Desidera, S.
name: Gizon, L.
name: Goupil, M. J.
name: Granata, V.
name: Heras, A. M.
name: Magrin, D.
name: Malavolta, L.
name: Mas-Hesse, J. M.
name: Osborn, H. P.
name: Pagano, I.
name: Paproth, C.
name: Pollacco, D.
name: Prisinzano, L.
name: Ragazzoni, R.
name: Ramsay, G.
name: Rauer, H.
name: Tkachenko, A.
name: Udry, S.
Publisher: name: arXiv
Year: 2025
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: Instrumentation and Methods for Astrophysics (astro-ph.IM)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: PLAnetary Transits and Oscillations of stars (PLATO) is an ESA M-class mission to be launched by the end of 2026 to discover and characterize transiting planets around bright and nearby stars, and in particular habitable rocky planets hosted by solar-like stars. Over the mission lifetime, an average of 8% of the science data rate will be allocated to Guest Observer programs (GOs) selected by ESA through public calls, hence it is essential for the community to know in advance where the observing fields will be located. In a previous paper, we identified two preliminary long-pointing fields (LOPN1 and LOPS1) for PLATO, respectively in the northern and southern hemisphere. Here we present LOPS2, a slightly adjusted version of the southern field that has recently been selected by the PLATO Science Working Team as the first field to be observed by PLATO for at least two continuous years, following the scientific requirements. In this paper, we describe the astrophysical content of LOPS2 in detail, including known planetary systems, bright/variable/binary stars, clusters and synergies with other current and future facilities.
description: 40 pages, 23 figures, six tables. Accepted for publication in A&A on January 11, 2025. More typos corrected. Supplementary material available on https://zenodo.org/records/14720127
Additional file 1 of Fatores associados ao óbito em casos confirmados de COVID-19 no estado do Rio de Janeiro
Creators: name: Cini Oliveira, Marcella
name: de Araujo Eleuterio, Tatiana
name: de Andrade Corrêa, Allan Bruno
name: da Silva, Lucas Dalsenter Romano
name: Rodrigues, Renata Coelho
name: de Oliveira, Bruna Andrade
name: Martins, Marlos Melo
name: Raymundo, Carlos Eduardo
name: de Andrade Medronho, Roberto
Publisher: name: figshare
Year: 2021
Subjects: subject: Medicine
subject: Genetics
subject: FOS: Biological sciences
subject: Biotechnology
subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences
subject: Immunology
subject: FOS: Clinical medicine
subject: 19999 Mathematical Sciences not elsewhere classified
subject: FOS: Mathematics
subject: Cancer
subject: Computational Biology

description: Additional file 1.
title: ADCO, Cartulaire général de Cîteaux, dit de Jean de Cirey, (XVe siècle), tome I, Cart. 185 (11 H 70), f. 0308r
Creators: name: de la Côte d'Or, Archives départementales
name: Petot, Frédérique
name: Projet CBMA
name: CG21/F.PETOT/2012
name: Archives Départementales De La Côte-D'Or
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: Cartulaire général de Cîteaux, dit de Jean de Cirey, (XVe siècle), tome I, Archives départementales de la Côte-d'Or, Cart. 185 (11 H 70), f. 0308r, 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 I, Archives départementales de la Côte-d'Or, Cart. 185 (11 H 70), f. 0308r, in Projet CBMA - Corpus Burgundiae Medii Aevi [Ressource en ligne], https:// manuscrits.cbma-project.eu/
description: Provenance: abbaye de Cîteaux
description: Provenance: http://www.wikidata.org/entity/Q843261
description: Provenance: https://www.geonames.org/3024876
description: Provenance: http://www.idref.fr/030974844/id
description: Provenance: https://catalogue.bnf.fr/ark:/12148/cb12228351v
Solutions of the Knizhnik - Zamolodchikov Equation with Rational Isospins and the Reduction to the Minimal Models
Creators: name: Furlan, P.
name: Ganchev, A. Ch.
name: Paunov, R.
name: Petkova, V. B.
Publisher: name: arXiv
Year: 1992
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: In the spirit of the quantum Hamiltonian reduction we establish a relation between the chiral $n$-point functions, as well as the equations governing them, of the $A_1^{(1)}$ WZNW conformal theory and the corresponding Virasoro minimal models. The WZNW correlators are described as solutions of the Knizhnik - Zamolodchikov equations with rational levels and isospins. The technical tool exploited are certain relations in twisted cohomology. The results extend to arbitrary level $k+2 \neq 0$ and isospin values of the type $J=j-j'(k+2)$, $ \ 2j, 2j' \in Z\!\!\!Z_+$.
description: 40 pages