cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
On the Interaction Between Cosmic Rays and Dark Matter Molecular Clouds - II. The Age Distribution of Cosmic Ray Electrons
Creators: name: Sciama, D. W.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We explore further the proposal in paper I of this series that the confinement time of cosmic ray nuclei in the Milky Way is determined by their interaction with dark matter molecular clouds rather than by their escape from the halo, as is assumed in conventional models of cosmic ray propagation. The same proposal can be made for cosmic ray electrons. This proposal leads to a specific age distribution for the electrons which is in agreement with Tang's (1984) observations of the electron spectrum at high energies but not with Nishimura et al's (1980) earlier data, which lead to a flatter spectrum. However, the simplest leaky box and diffusion models disagree with both sets of data so that our trapping model is supported if Tang's data are correct.
description: 7 pages, no figures, using MNRAS latex style
title: ADCO, Cartulaire de Cîteaux pour les possessions d'Aloxe (XVe siècle), Cart. 182 (11 H 233), 105 folios, f. 0197
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/2017
name: Petot, Frédéric
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2020
Subjects: subject: cartulaire
subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris
subject: Corpus Burgundiae Medii Aevi
subject: Chartes de la Bourgogne du Moyen Âge

description: Cartulaire de Cîteaux pour les possessions d'Aloxe (XVe siècle), Archives départementales de la Côte-d'Or, Cart. 182 (11 H 233), 105 folios, f. 0197, Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Cartulaire de Cîteaux pour les possessions d'Aloxe (XVe siècle), Archives départementales de la Côte-d'Or, Cart. 182 (11 H 233), 105 folios, f. 0197, 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
Orientational ordering of lamellar structures on closed surfaces
Creators: name: Pękalski, Jakub
name: Ciach, Alina
Publisher: name: arXiv
Year: 2018
Subjects: subject: Soft Condensed Matter (cond-mat.soft)
subject: FOS: Physical sciences

description: Self-assembly of particles with short-range attraction and long-range repulsion (SALR) interactions on a flat and on a spherical surface is compared. Molecular dynamics (MD) simulations are performed for the two systems having the same area and the density optimal for formation of stripes of particles. Structural characteristics, e.g. a cluster size distribution, a number of defects and an orientational order parameter (OP), as well as the specific heat, are obtained for a range of temperature. In both cases, the cluster size distribution becomes bimodal and elongated clusters appear at the temperature corresponding to the maximum of the specific heat. When the temperature decreases, orientational ordering of the stripes takes place, and the number of particles per cluster or stripe increases in both cases. However, only on the flat surface the specific heat has another maximum at the temperature corresponding to a rapid change of the OP. On the sphere, the crossover between the isotropic and anisotropic structures occurs in a much broader temperature interval, the orientational order is weaker, and occurs at significantly lower temperature. At low temperature the stripes on the sphere form spirals, and the defects resemble defects in the nematic phase of rods adsorbed at a sphere.
Calibration of the MACHO Photometry Database
Creators: name: Alcock, C.
name: Allsman, R. A.
name: Alves, D. R.
name: Axelrod, T. S.
name: Becker, A. C.
name: Bennett, D. P.
name: Cook, K. H.
name: Drake, A. J.
name: Freeman, K. C.
name: Griest, K.
name: Lehner, M. J.
name: Marshall, S. L.
name: Minniti, D.
name: Peterson, B. A.
name: Pratt, M. R.
name: Nelson, C. A.
name: Quinn, P. J.
name: Stubbs, C. W.
name: Sutherland, W.
name: Tomaney, A. B.
name: Welch, D. L.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: The MACHO Project is a microlensing survey that monitors the brightnesses of 60 million stars in the Large Magellanic Cloud (LMC), Small Magellanic Cloud, and Galactic bulge. Our database presently contains about 80 billion photometric measurements, a significant fraction of all astronomical photometry. We describe the calibration of MACHO two-color photometry and transformation to the standard Kron-Cousins V and R system. Calibrated MACHO photometry may be properly compared with all other observations on the Kron-Cousins standard system, enhancing the astrophysical value of these data. For 9 million stars in the LMC bar, independent photometric measurements of 20,000 stars with V < 18 mag in field-overlap regions demonstrate an internal precision sigV = 0.021, sigR = 0.019, and sig(V-R) = 0.028 mag. The accuracy of the zero-point in this calibration is estimated to be +-0.035 mag for stars with colors in the range -0.1 < (V-R) < 1.2 mag. A comparison of calibrated MACHO photometry with published photometric sequences and new Hubble Space Telescope observations shows agreement. The current calibration zero-point uncertainty for the remainder of the MACHO photometry database is estimated to be +- 0.10 mag in V or R and +-0.04 mag in (V-R). We describe the first application of calibrated MACHO photometry data: the construction of a color-magnitude diagram used to calculate our experimental sensitivity to detect microlensing in the LMC.
description: to appear in PASP, 11pt aaspp4.sty, 47 pages, includes 21 figures (4 are bitmapped)
How Do Women Experience Navigating Support After Domestic Abuse?
Creators: name: Eassom, Erica
Publisher: name: University of East London
Year: 2018
Subjects: Domestic violence
Support
Services
Help-Secondary victimisation
Secondary victimisation

description: Research has highlighted the multiple barriers women who have experienced domestic violence and abuse (DVA) face in ‘disclosing’ abuse. However, ‘disclosure’ is but the first step in women accessing ‘support’ for a wide range of needs; less is known about women’s experiences once they have accessed ‘support’. Existing research has frequently identified what is termed ‘secondary victimisation’ within services, however this has typically been studied within separate spheres - medical, legal and so on – preventing a more integrated understanding of women’s experiences. This research applies a feminist perspective to explore how women experience accessing ‘support’ from formal and informal systems after DVA, and considers what constitutes support, for them. The research involved consultation and collaboration with service users and staff at a specialist DVA organisation. Nine women who were engaged with the organisation took part in semi-structured interviews. The interviews were analysed using thematic analysis within a critical realist contextualist epistemology. Three main themes were identified: theme one, “It’s the Seeing It and Acknowledging It”: Who, Where and How?; theme two, The Duality of Help, and theme three, “We’ve Had Enough”. Theme one considers how constructing experiences as abuse intersected with women’s experiences of ‘help’. The second theme explores the paradoxes associated with navigating ‘support systems’ and their possible harms. The final theme explores how women describe being impacted by and responding to their experiences, both of abuse and within ‘support systems’. Results of the analysis are discussed in relation to empirical and theoretical literature. In discussing findings, the use of power within services is explored and the importance of relational aspects of care. Implications are considered at a community, service and research level.
Aspects of Supersymmetry at LEP II
Creators: name: Matalliotakis, D.
name: Nilles, H. P.
Publisher: name: arXiv
Year: 1994
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We give a short introduction to the concept of low energy supersymmetric models and their phenomenological predictions. In view of the future LEP II results we have to parametrize these predictions in a model independent way without too many simplifying assumptions. The study must therefore include models with {\it non--universal} soft supersymmetry breaking terms. We show that such non--universalities might have significant influence on the properties of these models.
description: 10 pages, TUM-HEP-205/94 (Latex file plus uuencoded postscript file, please observe instructions). Talk presented by H.P. Nilles at the Zeuthen Workshop on Elementary Particle Theory--Physics at LEP200 and Beyond and Beyond,Teupitz/Brandenburg, Germany, 10--15 April, 1994
MOESM1 of Improving knowledge on the activation of bone marrow fibroblasts in MGUS and MM disease through the automatic extraction of genes via a nonnegative matrix factorization approach on gene expression profiles
Creators: name: Boccarelli, Angelina
name: Esposito, Flavia
name: Coluccia, Mauro
name: Frassanito, Maria
name: Vacca, Angelo
name: Buono, Nicoletta Del
Publisher: name: figshare
Year: 2018
Subjects: subject: Space Science
subject: Medicine
subject: Genetics
subject: FOS: Biological sciences
subject: Physiology
subject: Evolutionary Biology
subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences
subject: 69999 Biological Sciences not elsewhere classified
subject: 80699 Information Systems not elsewhere classified
subject: FOS: Computer and information sciences
subject: Cancer
subject: Plant Biology
subject: Computational Biology

description: Additional file 1: Tables S1 and S2. Genes and their corresponding median value of MGUS and MM.
Octet baryon magnetic moments at next-to-next-to-leading order in covariant chiral perturbation theory
Creators: name: Xiao, Yang
name: Ren, Xiu-Lei
name: Lu, Jun-Xu
name: Geng, Li-Sheng
name: Meißner, Ulf-G.
Publisher: name: arXiv
Year: 2018
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: High Energy Physics - Lattice (hep-lat)
subject: FOS: Physical sciences

description: We calculate the octet baryon magnetic moments in covariant baryon chiral perturbation theory with the extended-on-mass-shell renormalization scheme up to next-to-next-to-leading order. At this order, there are nine low-energy constants, which cannot be uniquely determined by the seven experimental data alone. We propose two strategies to circumvent this problem. First, we assume that chiral perturbation theory has a certain convergence rate and use this as one additional constraint to fix the low-energy constants by fitting to the experimental data. Second, we fit to lattice QCD simulations to determine the low-energy constants. We then compare the resulting predictions of the light and strange quark mass dependence of the octet baryon magnetic moments by the three mostly studied formulations of baryon chiral perturbation theory, namely, the extended-on-mass-shell, the infrared, and the heavy baryon approach. It is shown that once more precise lattice data become available, one will learn more about the convergence pattern of baryon chiral perturbation theory.
description: 22 pages, 7 figures, 6 tables
Additional file 8: of Community-based rehabilitation intervention for people with schizophrenia in Ethiopia (RISE): a 12 month mixed methods pilot study
Creators: name: Asher, Laura
name: Hanlon, Charlotte
name: Birhane, Rahel
name: Alehegn Habtamu
name: Eaton, Julian
name: Weiss, Helen
name: Patel, Vikram
name: Abebaw Fekadu
name: Silva, Mary De
Publisher: name: figshare
Year: 2018
Subjects: subject: Sociology
subject: FOS: Sociology
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: 80699 Information Systems not elsewhere classified
subject: FOS: Computer and information sciences

description: Individiual level process and outcome data. Word document. (DOCX 17 kb)
Cellular automaton models for time-correlated random walks: derivation and analysis
Creators: name: Nava-Sedeno, J. M.
name: Hatzikirou, H.
name: Klages, R.
name: Deutsch, A.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Statistical Mechanics (cond-mat.stat-mech)
subject: Biological Physics (physics.bio-ph)
subject: Computational Physics (physics.comp-ph)
subject: Cell Behavior (q-bio.CB)
subject: FOS: Physical sciences
subject: FOS: Biological sciences

description: Many diffusion processes in nature and society were found to be anomalous, in the sense of being fundamentally different from conventional Brownian motion. An important example is the migration of biological cells, which exhibits non-trivial temporal decay of velocity autocorrelation functions. This means that the corresponding dynamics is characterized by memory effects that slowly decay in time. Motivated by this we construct non-Markovian lattice-gas cellular automata models for moving agents with memory. For this purpose the reorientation probabilities are derived from velocity autocorrelation functions that are given a priori; in that respect our approach is `data-driven'. Particular examples we consider are velocity correlations that decay exponentially or as power laws, where the latter functions generate anomalous diffusion. The computational efficiency of cellular automata combined with our analytical results paves the way to explore the relevance of memory and anomalous diffusion for the dynamics of interacting cell populations, like confluent cell monolayers and cell clustering.
description: 14 pages, 7 figures, 16 pages supplement
Additional file 1: of What is the impact of sensory practices on the quality of life of long-term care residents? A mixed-methods systematic review protocol
Creators: name: Backman, Chantal
name: Crick, Michelle
name: Cho-Young, Danielle
name: Scharf, Megan
name: Shea, Beverley
Publisher: name: figshare
Year: 2018
Subjects: subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: Developmental Biology
subject: Science Policy

description: á PRISMA-P checklist (DOCX 40 kb)
Additional file 7: of Community-based rehabilitation intervention for people with schizophrenia in Ethiopia (RISE): a 12 month mixed methods pilot study
Creators: name: Asher, Laura
name: Hanlon, Charlotte
name: Birhane, Rahel
name: Alehegn Habtamu
name: Eaton, Julian
name: Weiss, Helen
name: Patel, Vikram
name: Abebaw Fekadu
name: Silva, Mary De
Publisher: name: figshare
Year: 2018
Subjects: subject: Sociology
subject: FOS: Sociology
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: 80699 Information Systems not elsewhere classified
subject: FOS: Computer and information sciences
subject: Computational Biology

description: Supplementary qualitative data. Word document. Additional supporting quotations from qualitative data, by theme and sub-theme. (DOCX 42 kb)
Multi-band optical variability on diverse timescales of blazar 1E 1458.8+2249
Creators: name: Özdönmez, Aykut
name: Tekkeşinoğlu, Murat
Publisher: name: arXiv
Year: 2024
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: This study presents an analysis of the optical variability of the blazar 1E 1458.8+2249 on diverse timescales using multi-band observations, including observations in the optical BVRI bands carried out with the T60 and T100 telescopes from 2020 to 2023 and ZTF gri data from 2018 to 2023. On seven nights, we searched for intraday variability using the power-enhanced F-test and the nested ANOVA test, but no significant variability was found. The long-term light curve shows a variability behaviour in the optical BVRI bands with amplitudes of $\sim100\%$ and in the gri bands with amplitudes of $\sim120\%$, including short-term variability of up to $\sim1.1$ mag. Correlation analysis revealed a strong correlation between the optical multi-band emissions without any time lag.From 62 nightly SEDs, we obtained spectral indices between 0.826 and 1.360, with an average of $1.128\pm0.063$. The relationships of both spectral indices and colour with respect to brightness indicate a mild BWB trend throughout the observation period, both intraday and long-term. We also performed a periodicity search using the Weighted Wavelet Z-transform (WWZ) and Lomb-Scargle methods. A recurrent optical emission pattern with a quasi-periodicity of $\sim340$ days is detected in the combined V- and R-band light curves. The observational results indicate that the blazar 1E 1458.8+2249 has a complex variability, while emphasising the need for future observations to unravel its underlying mechanisms.
description: 10 pages, 9 figures, 4 tables; published in PASA
Programmable Metasurfaces: State of the Art and Prospects
Creators: name: Liu, Fu
name: Pitilakis, Alexandros
name: Mirmoosa, Mohammad Sajjad
name: Tsilipakos, Odysseas
name: Wang, Xuchen
name: Tasolamprou, Anna C.
name: Abadal, Sergi
name: Cabellos-Aparicio, Albert
name: Alarcón, Eduard
name: Liaskos, Christos
name: Kantartzis, Nikolaos V.
name: Kafesaki, Maria
name: Economou, Eleftherios N.
name: Soukoulis, Costas M.
name: Tretyakov, Sergei
Publisher: name: arXiv
Year: 2018
Subjects: subject: Applied Physics (physics.app-ph)
subject: FOS: Physical sciences

description: Metasurfaces, ultrathin and planar electromagnetic devices with sub-wavelength unit cells, have recently attracted enormous attention for their powerful control over electromagnetic waves, from microwave to visible range. With tunability added to the unit cells, the programmable metasurfaces enable us to benefit from multiple unique functionalities controlled by external stimuli. In this review paper, we will discuss the recent progress in the field of programmable metasurfaces and elaborate on different approaches to realize them, with the tunability from global aspects, to local aspects, and to software-defined metasurfaces.
description: 5 pages with 3 figures
The BeppoSAX view of the hot cluster Abell 2319
Creators: name: Molendi, S.
name: De Grandi, S.
name: Fusco-Femiano, R.
name: Colafrancesco, S.
name: Fiore, F.
name: Nesci, R.
name: Tamburelli, F.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present results from a BeppoSAX observation of the rich cluster Abell 2319. The broad band spectrum (2-50 keV) of the cluster can be adequately represented by an optically thin thermal emission model with a temperature of 9.6+/-0.3 keV and a metal abundance of 0.25+/-0.03 in solar units, and with no evidence of a hard X-ray excess in the PDS spectrum. From the upper limit to the hard tail component we derive a lower limit of ~0.04 \muG for the volume-averaged intracluster magnetic field. By performing spatially resolved spectroscopy in the medium energy band (2-10 keV), we find that the projected radial temperature and metal abundance profiles are constant out to a radius of 16 arcmin (1.4 Mpc). A reduction of the temperature of 1/3, when going from the cluster core out to 16 arcmin, can be excluded in the present data at the 99% confidence level. From the analysis of the temperature and abundance maps we find evidence of a temperature enhancement and of an abundance decrement in a region localized 6 arcmin--8 arcmin NE of the core, where a merger event may be taking place. Finally, the temperature map indicates that the subcluster located NW of the main cluster may be somewhat cooler than the rest of the cluster.
description: To appear in ApJ-Letters
Acantholepis capensis Mayr
Creators: name: Emery, C.
Publisher: name: Zenodo
Year: 1895
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hymenoptera
Formicidae
Acantholepis
Acantholepis capensis

description: Acantholepis capensis Mayr.
- Cape Town, Pretoria, Makapan, Matjesfontein.
Mayr a decrit cette espece sur l'ouvriere et le male. La femelle correspond exactement a la description de Plagiolepis capensis du meme auteur.
description: Published as part of Emery, C., 1895, Voyage de M. E. Simon dans l'Afrique australe (janvier-avril 1893). 3 e mémoire. Formicides., pp. 15-56 in Annales de la Société Entomologique de France 64 on page 32
Flow Study in Relativistic Nuclear Collisions by Fourier Expansion of Azimuthal Particle Distributions
Creators: name: Voloshin, S.
name: Zhang, Y.
Publisher: name: arXiv
Year: 1994
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We propose a new method to study transverse flow effects in relativistic nuclear collisions by Fourier analysis of the azimuthal distribution on an event-by-event basis in relatively narrow rapidity windows. The distributions of Fourier coefficients provide direct information on the magnitude and type of flow. Directivity and two dimensional sphericity tensor, widely used to analyze flow, emerge naturally in our approach, since they correspond to the distributions of the first and second harmonic coefficients, respectively. The role of finite particle fluctuations and particle correlations is discussed.
description: 14 pages, 3 figures included as figures.uu at the end, REVTEX
Additional file 6: of Community-based rehabilitation intervention for people with schizophrenia in Ethiopia (RISE): a 12 month mixed methods pilot study
Creators: name: Asher, Laura
name: Hanlon, Charlotte
name: Birhane, Rahel
name: Alehegn Habtamu
name: Eaton, Julian
name: Weiss, Helen
name: Patel, Vikram
name: Abebaw Fekadu
name: Silva, Mary De
Publisher: name: figshare
Year: 2018
Subjects: Computational Biology

description: Assumptions table. Word document. Summary of main findings, adjustments to intervention and conclusion relating to each theory of change assumption. (DOCX 20 kb)
Kinematic Distances: A Monte Carlo Method
Creators: name: Wenger, Trey V.
name: Balser, Dana S.
name: Anderson, L. D.
name: Bania, T. M.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: Distances to high mass star forming regions (HMSFRs) in the Milky Way are a crucial constraint on the structure of the Galaxy. Only kinematic distances are available for a majority of the HMSFRs in the Milky Way. Here we compare the kinematic and parallax distances of 75 Galactic HMSFRs to assess the accuracy of kinematic distances. We derive the kinematic distances using three different methods: the traditional method using the Brand & Blitz (1993) rotation curve (Method A), the traditional method using the Reid et al. (2014) rotation curve and updated Solar motion parameters (Method B), and a Monte Carlo technique (Method C). Methods B and C produce kinematic distances closest to the parallax distances, with median differences of 13% (0.43 kpc) and 17% (0.42 kpc), respectively. Except in the vicinity of the tangent point, the kinematic distance uncertainties derived by Method C are smaller than those of Methods A and B. In a large region of the Galaxy, the Method C kinematic distances constrain both the distances and the Galactocentric positions of HMSFRs more accurately than parallax distances. Beyond the tangent point along longitude=30 degrees, for example, the Method C kinematic distance uncertainties reach a minimum of 10% of the parallax distance uncertainty at a distance of 14 kpc. We develop a prescription for deriving and applying the Method C kinematic distances and distance uncertainties. The code to generate the Method C kinematic distances is publicly available and may be utilized through an on-line tool.
description: 30 pages, 4 tables, 20 figures, accepted for publication in ApJ. Code available online here: https://github.com/tvwenger/kd -- Online tool available here: http://www.treywenger.com/kd/
Spectroscopy of Globular Clusters in the Sculptor Group Galaxies NGC 253 and NGC 55
Creators: name: Beasley, M. A.
name: Sharples, R. M.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We have obtained spectra for 103 published globular cluster candidates in the Sculptor Group galaxies NGC 253 and NGC 55. On the basis of radial velocities and digitized plate images, 14 globular clusters are identified in NGC 253 and one probable globular cluster is identified in NGC 55. The majority of the objects in the sample appear to be background galaxies. We have obtained and analysed COSMOS plate scans of NGC 253 and NGC 55 and use these along with the spectroscopically identified clusters to define new samples of globular cluster candidates in the two galaxies which should have reduced contamination.
description: 11 pages, 9 postscript figures, accepted for publication in MNRAS
Neutrinos propagating in curved spacetimes
Creators: name: Zhang, Fan
Publisher: name: arXiv
Year: 2018
Subjects: subject: General Physics (physics.gen-ph)
subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: In the Dirac-Weyl equation that describes massless neutrino propagation in the minimal Standard Model, the ($2\times 2$ equivalence of the) gamma matrices convert Weyl spinors into spacetime tensors, and vice versa. They can thus be regarded as amalgamations of three different types of mappings, one that connects particle spinors directly forming representations to internal gauge symmetries to their spacetime counterparts that are embodied by null flags, another that translates the spacetime spinors into their corresponding tensors expressed in an orthonormal tetrad, and finally a purely tensorial transformation into the coordinate tetrad. The splitting of spinors into particle and spacetime varieties is not usually practised, but we advocate its adoption for better physical clarity, in terms of distinguishing internal and spacetime transformations, and also for understanding the scattering of neutrinos by spacetime curvature. We construct the basic infrastructure required for this task, and provide a worked example for the Schwarzschild spacetime. Our investigation also uncovers a possible under-determinacy in the flavoured Dirac-Weyl equation, which could serve as a new incision point for introducing flavour oscillation mechanisms.
description: 21 pages, 3 figures
On the Derivative Expansion at Finite Temperature
Creators: name: Das, Ashok
name: Hott, Marcelo
Publisher: name: arXiv
Year: 1994
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: In this short note, we indicate the origin of nonanalyticity in the method of derivative expansion at finite temperature and discuss some of its consequences.
description: 7 pages, UR-1363, ER40685-813
Lead-free Hybrid Perovskite: An Efficient Room Temperature Spin Generator via Large Interfacial Rashba effect
Creators: name: Han, Lei
name: Wang, Qian
name: Lu, Ying
name: Tao, Sheng
name: Zhu, Wenxuan
name: Feng, Xiaoyu
name: Liang, Shixuan
name: Bai, Hua
name: Chen, Chong
name: Wang, Kai
name: Yang, Zhou
name: Fan, Xiaolong
name: Song, Cheng
name: Pan, Feng
Publisher: name: arXiv
Year: 2024
Subjects: subject: Materials Science (cond-mat.mtrl-sci)
subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: Applied Physics (physics.app-ph)
subject: Chemical Physics (physics.chem-ph)
subject: FOS: Physical sciences

description: Two-dimensional (2D) hybrid organic-inorganic perovskite (HOIP) demonstates great potential for developing flexible and wearable spintronic devices, by serving as spin sources via the bulk Rashba effect (BRE). However, the practical application of BRE in 2D HOIP faces huge challenges, particularly due to the toxicity of lead, which is crucial for achieving large spin-orbit coupling, and the restrictions in 2D HOIP candidates to meet specific symmetry-breaking requirements. To overcome these obstacles, we design a strategy to exploit the interfacial Rashba effect (IRE) of lead-free 2D HOIP (C6H5CH2CH2NH3)2CuCl4 (PEA-CuCl), manifesting as an efficient spin generator at room temperature. IRE of PEA-CuCl originates from the large orbital hybridization at the interface between PEA-CuCl and adjacent ferromagnetic layers. Spin-torque ferromagnetic resonance measurements further quantify a large Rashba effective field of 14.04 Oe per 10^11 A m-2, surpassing those of lead-based HOIP and traditional all-inorganic heterojunctions with noble metals. Our lead-free 2D HOIP PEA-CuCl, which harnesses large IRE for spin generation, is efficient, nontoxic, and economic, offering huge promise for future flexible and wearable spintronic devices.
Angular Sizes of $μ$Jy Radio Sources
Creators: name: Cotton, W. D.
name: Condon, J. J.
name: Kellermann, K. I.
name: Lacy, M.
name: Perley, R. A.
name: Matthews, A. M.
name: Vernstrom, T.
name: Scott, Douglas
name: Wall, J. V.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We made two new sensitive (rms noise sigma_n ~ 1 microJy/beam) high resolution (theta = 3.0" and theta = 0.66" FWHM) S--band (2 < nu < 4 GHz) images covering a single JVLA primary beam (FWHM ~ 14') centered on J2000 RA = 10 46, Dec = 59 01 in the Lockman Hole. These images yielded a catalog of 792 radio sources, 97.7 +/- 0.8% of which have infrared counterparts stronger than S ~ 2 microJy at lambda = 4.5 micron. About 91% of the radio sources found in our previously published, comparably sensitive low resolution (theta = 8" FWHM) image covering the same area were also detected at 0.66" resolution, so most radio sources with S_3GHz >~ 5 microJy have angular structure phi = 0.3" +/- 0.1" FWHM and an rms scatter sigma_phi ~ /2.43 ~ 0.12", so the median effective radius of star-forming galaxies at redshifts z~1 is ~ 1.0 kpc.
description: 20 pages, 8 figures
title: ADCO, Huitième cartulaire de Saint-Étienne de Dijon (1661-1667), Cart. 31 (G 135), 549 folios, f. 1087
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: Corpus Burgundiae Medii Aevi
subject: Chartes de la Bourgogne du Moyen Âge
subject: cartulaire
subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris

description: Huitième cartulaire de Saint-Étienne de Dijon (1661-1667), Archives départementales de la Côte-d'Or, Cart. 31 (G 135), 549 folios, f. 1087, Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Huitième cartulaire de Saint-Étienne de Dijon (1661-1667), Archives départementales de la Côte-d'Or, Cart. 31 (G 135), 549 folios, f. 1087, 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
The Classical-Quantum Duality of Nature. New Variables for Quantum Gravity
Creators: name: Sanchez, Norma G.
Publisher: name: arXiv
Year: 2018
Subjects: subject: General Physics (physics.gen-ph)
subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: The classical-quantum duality at the basis of quantum theory is here extended to the Planck scale domain. The classical/semiclassical gravity (G) domain is dual (in the precise sense of the classical-quantum duality) to the quantum (Q) elementary particle domain through the Planck scale. This duality is universal. From the gravity and quantum variables (G, Q), we define new (QG) quantum gravity variables QG = (1/2) (G + Q) which include all (classical, semiclassical and quantum gravity) domains and the elementary particle domain passing by the Planck scale. Two values of G or Q variables are necessary for each variable QG. The complete analytic extension of the QG variables is performed. This allows us to reveal the classical-quantum duality of the Schwarzschild-Kruskal space-time: The exterior regions are classical/semiclassical while the interior is totally quantum, its boundaries being the Planck scale. Exterior and interior lose their difference near the horizon which turns to be quantum dressed, " l'horizon habille' ". QG variables are naturally invariant under G --> Q and conversely. Space-time reflections, antipodal symmetry and PT or CPT symmetry are contained in the QG symmetry, which also shed insight into the global properties of the Kruskal manifold and its present renewed interest...(Abridged)
description: 22 pages, 3 figures, New original material
Additional file 5: of Community-based rehabilitation intervention for people with schizophrenia in Ethiopia (RISE): a 12 month mixed methods pilot study
Creators: name: Asher, Laura
name: Hanlon, Charlotte
name: Birhane, Rahel
name: Alehegn Habtamu
name: Eaton, Julian
name: Weiss, Helen
name: Patel, Vikram
name: Abebaw Fekadu
name: Silva, Mary De
Publisher: name: figshare
Year: 2018
Subjects: subject: Molecular Biology
subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences
subject: Sociology
subject: FOS: Sociology
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: 80699 Information Systems not elsewhere classified
subject: FOS: Computer and information sciences
subject: Developmental Biology
subject: Computational Biology

description: Instruments. Word document. Further details on quantitative data collection instruments. (DOCX 21 kb)
Rigid Single-Slice-in-Volume registration via rotation-equivariant 2D/3D feature matching
Creators: name: Brandstätter, Stefan
name: Seeböck, Philipp
name: Fürböck, Christoph
name: Pochepnia, Svitlana
name: Prosch, Helmut
name: Langs, Georg
Publisher: name: arXiv
Year: 2024
Subjects: subject: Computer Vision and Pattern Recognition (cs.CV)
subject: Machine Learning (cs.LG)
subject: FOS: Computer and information sciences

description: 2D to 3D registration is essential in tasks such as diagnosis, surgical navigation, environmental understanding, navigation in robotics, autonomous systems, or augmented reality. In medical imaging, the aim is often to place a 2D image in a 3D volumetric observation to w. Current approaches for rigid single slice in volume registration are limited by requirements such as pose initialization, stacks of adjacent slices, or reliable anatomical landmarks. Here, we propose a self-supervised 2D/3D registration approach to match a single 2D slice to the corresponding 3D volume. The method works in data without anatomical priors such as images of tumors. It addresses the dimensionality disparity and establishes correspondences between 2D in-plane and 3D out-of-plane rotation-equivariant features by using group equivariant CNNs. These rotation-equivariant features are extracted from the 2D query slice and aligned with their 3D counterparts. Results demonstrate the robustness of the proposed slice-in-volume registration on the NSCLC-Radiomics CT and KIRBY21 MRI datasets, attaining an absolute median angle error of less than 2 degrees and a mean-matching feature accuracy of 89% at a tolerance of 3 pixels.
Nitrifying bio-cord reactor: performance optimization and effects of substratum and air scouring
Creators: name: Tian, Xin
name: Ahmed, Warsama
name: Delatolla, Robert
Publisher: name: Taylor & Francis
Year: 2017
Subjects: subject: Biochemistry
subject: Neuroscience
subject: Physiology
subject: FOS: Biological sciences
subject: Biotechnology
subject: Evolutionary Biology
subject: Chemical Sciences not elsewhere classified
subject: Immunology
subject: FOS: Clinical medicine
subject: Biological Sciences not elsewhere classified
subject: Developmental Biology
subject: Marine Biology
subject: Infectious Diseases
subject: FOS: Health sciences

description: Ammonia removal kinetics and solids’ production performance of the bio-cord technology are studied in this research. Three nitrifying reactors housing different bio-cord substratum were operated at five different ammonia loading rates. All of the bio-cord substrata demonstrated stable and high ammonia-nitrogen removal efficiencies of 96.8 ± 0.9%, 97.0 ± 0.6% and 92.0 ± 0.4% at loading rates of 0.8, 1.6 and 1.8 g NH4+-N/m2 d, respectively. At these same loading rates, the bio-cord reactors housing the three substrata also showed low solids’ production rates of 0.19 ± 0.03, 0.23 ± 0.02, 0.25 ± 0.03 g total suspended solids/d. A reduction of system stability, identified via fluctuating ammonia removal rates, was however observed for all substrata at loading rates of 2.1 and 2.4 g NH4+-N/m2 d. Further, the solids’ production rates at these higher loading conditions were also observed to fluctuate for all substrata, likely indicating intermediate sloughing events. The effects of enhancing the air scouring of the bio-cord on the ammonia removal rate was shown to be dependent upon the substratum, while enhanced air scouring of the bio-cord was shown to stabilize the production of solids for all substrata. This study represents the first performance and optimization study of the bio-cord technology for low-carbon nitrification and shows that air scouring of the substratum reduces sloughing events at elevated loading and that the bio-cord technology achieves stable kinetics above conventional rates of 1 g NH4+-N/m2 d to values of 1.8 g NH4+-N/m2 d.
Evidence of H alpha periodicities in LS I+61303
Creators: name: Zamanov, R. K.
name: Marti, J.
name: Paredes, J. M.
name: Fabregat, J.
name: Ribo, M.
name: Tarasov, A. E.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present the results of analyzing H$α$ spectra of the radio emitting X-ray binary LS I+61303. For the first time, the same 26.5 d radio period is clearly detected in the H$α$ emission line. Moreover, the equivalent width and the peak separation of the H$α$ emission line seem also to vary over a time scale of 1600 days. This points towards the $\sim4$ yr modulation, detected in the radio outburst amplitude, being probably a result of variations in the mass loss rate of the Be star and/or density variability in the circumstellar disk. In addition, the dependence of the peak separation from the equivalent width informs us that the LS I+61303 circumstellar disk is among the densest of Be-stars.
description: 8 pages, 5 figures, LaTeX, uses aa.cls. Accepted for publication in A&A
A SUSY SO(10) Model with Large $tan β$
Creators: name: Lazarides, G.
name: Panagiotakopoulos, C.
Publisher: name: arXiv
Year: 1994
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We construct a supersymmetric SO(10) model with the asymptotic relation tan$β\simeq m_t/m_b$ automatically arising from its structure. The model retains the significant Minimal Supersymmetric Standard Model predictions for $sin^2 θ_w$ and $α_s$ and contains an automatic $Z_2$ matter parity. Proton decay through $d=5$ operators is sufficiently suppressed. It is remarkable that no global symmetries need to be imposed on the model.
description: 11 pages, LaTeX, UT-STPD-2-94
Extended X-ray emission in PKS 1718$-$649
Creators: name: Beuchert, T.
name: Rodríguez-Ardila, A.
name: Moss, V. A.
name: Schulz, R.
name: Kadler, M.
name: Wilms, J.
name: Angioni, R.
name: Callingham, J. R.
name: Gräfe, C.
name: Krauß, F.
name: Kreikenbohm, A.
name: Langejahn, M.
name: Leiter, K.
name: Maccagni, F. M.
name: Müller, C.
name: Ojha, R.
name: Ros, E.
name: Tingay, S. J.
Publisher: name: arXiv
Year: 2018
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: PKS 1718$-$649 is one of the closest and most comprehensively studied candidates of a young active galactic nucleus (AGN) that is still embedded in its optical host galaxy. The compact radio structure, with a maximal extent of a few parsecs, makes it a member of the group of compact symmetric objects (CSO). Its environment imposes a turnover of the radio synchrotron spectrum towards lower frequencies, also classifying PKS 1718$-$649 as gigahertz-peaked radio spectrum (GPS) source. Its close proximity has allowed the first detection of extended X-ray emission in a GPS/CSO source with Chandra that is for the most part unrelated to nuclear feedback. However, not much is known about the nature of this emission. By co-adding all archival Chandra data and complementing these datasets with the large effective area of XMM-Newton, we are able to study the detailed physics of the environment of PKS 1718$-$649. Not only can we confirm that the bulk of the $\lesssim$kiloparsec-scale environment emits in the soft X-rays, but we also identify the emitting gas to form a hot, collisionally ionized medium. While the feedback of the central AGN still seems to be constrained to the inner few parsecs, we argue that supernovae are capable of producing the observed large-scale X-ray emission at a rate inferred from its estimated star formation rate.
description: 5 pages, 2 figures, 2 tables, accepted for publication by A&A
The Distribution of X-ray Dips with Orbital Phase in Cygnus X-1
Creators: name: Balucinska-Church, M.
name: Church, M. J.
name: Charles, P. A.
name: Nagase, F.
name: LaSala, J.
name: Barnard, R.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present results of a comprehensive study of the distribution of absorption dips with orbital phase in Cygnus X-1. Firstly, the distribution was obtained using archival data from all major X-ray observatories and corrected for the selection effect that phase zero (superior conjunction of the black hole) has been preferentially observed. Dip occurrence was seen to vary strongly with orbital phase ϕ, with a peak at ϕ~ 0.95, i.e. was not symmetric about phase zero. Secondly, the RXTE ASM has provided continuous coverage of the Low State of Cygnus X-1 since Sept. 1996, and we have selected dip data based on increases in hardness ratio. The distribution, with much increased numbers of dip events, confirms that the peak is at ϕ~ 0.95, and we report the discovery of a second peak at ϕ~ 0.6. We attribute this peak to absorption in an accretion stream from the companion star HDE 226868. We have estimated the ionization parameter at different positions showing that radiative acceleration of the wind is suppressed by photoionization in particular regions in the binary system. To obtain the variation of column density with phase, we make estimates of neutral wind density for the extreme cases that acceleration of the wind is totally suppressed, or not suppressed at all. An accurate description will lie between these extremes. In each case, a strong variation of column density with orbital phase resulted, similar to the variation of dip occurrence. This provides evidence that formation of the blobs in the wind which lead to absorption dips depends on the density of the neutral component in the wind, suggesting possible mechanisms for blob growth.
description: 9 pages, Latex, 7 ps figures. accepted by MNRAS
Alfaria Emery, 1896, nov. gen
Creators: name: Emery, C.
Publisher: name: Zenodo
Year: 1896
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hymenoptera
Formicidae
Alfaria

description: Alfaria nov. gen.
[[worker]] Capo subquadrato; mandibole trigone, col margine masticatorio munito di denti piccoli e numerosi; lamine frontali distanti Tuna dall'altra, dilatate e prolungate quasi fino alla meta del capo; clipeo trasversalmente convesso, col margine anteriore distante dalle mandibole; occhi piuttosto piccoli, ma con molte faccette, situati nel mezzo dei lati del capo; antenne di 12 articoli, senza clava distinta. Torace inerme, senza suture. Segmento peduncolare dell'addome appena ingrossato nel mezzo, col contorno dorsale arcuato, col contorno ventrale incavato, attaccato al segmento seguente per quasi tutta la sua grossezza; 2. ° segmento campaniforme, separato dal 3. ° per una forte strozzatura; questo ricopre quasi tutto il resto dell'addome, e subgloboso e fortemente curvato in basso, in modo che il piano del suo margine apicale forma con quello del margine basale un angolo quasi retto; i segmenti seguenti che costituiscono la punta dell'addome sono rivolti in basso e in avanti. Tibie medie e posteriori con un solo sperone. Unghie semplici.
[[queen]] Rassomiglia alla [[worker]]; quella dell' A. simulans ne differisce per gli occhi piu. grandi, un ocello sul vertice; le suture distinte fra i 3 segmenti del torace; lo scutello non e distinto dal resto del mesonoto; nessun vestigio di ali; peduncolo subgloboso; unghie con un piccolo dente. Nell'altra specie, vi sono tre ocelli, il torace e normale e le unghie non sono dentate.
? [[male]] Capo allungato, col clipeo piu sporgente che nella [[worker]]; mandibole trigone, allungate, un poco curvate; lamine frontali debolissime; scapo lungo circa 2 volte quanto il 1. ° articolo del flagello, piu breve del 2. °. Torace con profondi solchi parapsidiali. Peduncolo subcilindrico, un poco curvato; i due segmenti seguenti di forma ordinaria, subeguali, ricoprenti circa i 2 / 3 dell' addome, il primo di essi subcampaniforme. Tibie con un solo sperone; unghie con un forte dente. Ali con due celle cubitali.
Questo genere e molto affine a Ectatomma e particolarmente al sottogenere Rhytidoponera: la forma, singolare del 3. ° segmento addominale che ricorda i generi Proceratium e Sysphincta si trova gia distintamente accennata in varie specie di Ectatomma; anche la forma del peduncolo non e molto dissimile da quella dell' E. bispinosum, mentre l'assenza di suture si osserva in alcune Gnamptoyenys.
Il [[male]] non differisce da quello delle Rhytidoponera: non sono sicuro che sia stato preso con la [[worker]] e [[queen]]; lo trovai in un tubo che racchiudeva alcune [[worker]] di Alfaria con altre formiche.
description: Published as part of Emery, C., 1896, Studi sulle formiche della fauna Neotropica., pp. 33-107 in Bollettino della Societa Entomologica Italiana 28 on pages 9-10
MSSM and Large $tanβ$ from SUSY Trinification
Creators: name: Lazarides, G.
name: Panagiotakopoulos, C.
Publisher: name: arXiv
Year: 1994
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We construct a supersymmetric model based on the semi-simple gauge group $SU(3)_c \times SU(3)_L \times SU(3)_R$ with the relation $tanβ\simeq m_t/m_b$ automatically arising from its structure. The model below a scale $\sim 10^{16}$ GeV gives naturally rise just to the minimal supersymmetric standard model and therefore to the presently favored values for $sin^2 θ_w$ and $α_s$ without fields in representations higher than the fundamental.
description: 9 pages, LaTeX, UT-STPD-3-94
Additional file 2: of Epidemiology of patients presenting to a pediatric emergency department in Karachi, Pakistan
Creators: name: Ijaz, Nadir
name: Strehlow, Matthew
name: N. Ewen Wang
name: Pirrotta, Elizabeth
name: Areeba Tariq
name: Naseeruddin Mahmood
name: Swaminatha Mahadevan
Publisher: name: figshare
Year: 2018
Subjects: subject: Biotechnology
subject: Ecology
subject: FOS: Biological sciences
subject: 69999 Biological Sciences not elsewhere classified

description: Table S2. Logistic regression model for predictors of mortality for all patients (N = 679, c-statistic = 0.82): 85% of followed patients were included in this model, of which 17% of patients died. Model was controlled for gender. (DOCX 15 kb)