cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
SN 2012fr: Ultraviolet, Optical, and Near-Infrared Light Curves of a Type Ia Supernova Observed Within a Day of Explosion
Creators: name: Contreras, Carlos
name: Phillips, M. M.
name: Burns, Christopher R.
name: Piro, Anthony L.
name: Shappee, B. J.
name: Stritzinger, Maximilian D.
name: Baltay, C.
name: Brown, Peter J.
name: Conseil, Emmanuel
name: Klotz, Alain
name: Nugent, Peter E.
name: Turpin, Damien
name: Parker, Stu
name: Rabinowitz, D.
name: Hsiao, Eric Y.
name: Morrell, Nidia
name: Campillay, Abdo
name: Castellón, Sergio
name: Corco, Carlos
name: González, Consuelo
name: Krisciunas, Kevin
name: Serón, Jacqueline
name: Tucker, Brad E.
name: Walker, E. S.
name: Baron, E.
name: Cain, C.
name: Childress, Michael J.
name: Folatelli, Gastón
name: Freedman, Wendy L.
name: Hamuy, Mario
name: Hoeflich, P.
name: Persson, S. E.
name: Scalzo, Richard
name: Schmidt, Brian
name: Suntzeff, Nicholas B.
Publisher: name: arXiv
Year: 2018
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: We present detailed ultraviolet, optical and near-infrared light curves of the Type Ia supernova (SN) 2012fr, which exploded in the Fornax cluster member NGC 1365. These precise high-cadence light curves provide a dense coverage of the flux evolution from $-$12 to $+$140 days with respect to the epoch of $B$-band maximum (\tmax). Supplementary imaging at the earliest epochs reveals an initial slow, nearly linear rise in luminosity with a duration of $\sim$2.5 days, followed by a faster rising phase that is well reproduced by an explosion model with a moderate amount of $^{56}$Ni mixing in the ejecta. From an analysis of the light curves, we conclude: $(i)$ explosion occurred $< 22$ hours before the first detection of the supernova, $(ii)$ the rise time to peak bolometric ($λ> 1800 $Å) luminosity was $16.5 \pm 0.6$ days, $(iii)$ the supernova suffered little or no host-galaxy dust reddening, $(iv)$ the peak luminosity in both the optical and near-infrared was consistent with the bright end of normal Type Ia diversity, and $(v)$ $0.60 \pm 0.15 M_{\odot}$ of $^{56}$Ni was synthesized in the explosion. Despite its normal luminosity, SN 2012fr displayed unusually prevalent high-velocity \ion{Ca}{2} and \ion{Si}{2} absorption features, and a nearly constant photospheric velocity of the \ion{Si}{2} $λ$6355 line at $\sim$12,000 \kms\ beginning $\sim$5 days before \tmax. Other peculiarities in the early phase photometry and the spectral evolution are highlighted. SN 2012fr also adds to a growing number of Type Ia supernovae hosted by galaxies with direct Cepheid distance measurements.
description: 88 pages, 29 figures, 12 tables
Towards Precision Constraints on Gravity with the Effective Field Theory of Large-Scale Structure
Creators: name: Bose, Benjamin
name: Koyama, Kazuya
name: Lewandowski, Matthew
name: Vernizzi, Filippo
name: Winther, Hans A.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: We compare analytical computations with numerical simulations for dark-matter clustering, in general relativity and in the normal branch of DGP gravity (nDGP). Our analytical frameword is the Effective Field Theory of Large-Scale Structure (EFTofLSS), which we use to compute the one-loop dark-matter power spectrum, including the resummation of infrared bulk displacement effects. We compare this to a set of 20 COLA simulations at redshifts $z = 0$, $z=0.5$, and $z =1$, and fit the free parameter of the EFTofLSS, called the speed of sound, in both $Λ$CDM and nDGP at each redshift. At one-loop at $z = 0$, the reach of the EFTofLSS is $k_{\rm reach}\approx 0.14 \, h { \rm Mpc^{-1}}$ for both $Λ$CDM and nDGP. Along the way, we compare two different infrared resummation schemes and two different treatments of the time dependence of the perturbative expansion, concluding that they agree to approximately $1\%$ over the scales of interest. Finally, we use the ratio of the COLA power spectra to make a precision measurement of the difference between the speeds of sound in $Λ$CDM and nDGP, and verify that this is proportional to the modification of the linear coupling constant of the Poisson equation.
description: 34 pages, 12 figures; v2: JCAP published version, small improvements and additions
Additional file 5: of Reproducibility of domain-specific physical activity over two seasons in children
Creators: name: Aadland, Eivind
name: Andersen, Lars
name: Ekelund, Ulf
name: Anderssen, Sigmund
name: Resaland, Geir
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: Ecology
subject: FOS: Biological sciences
subject: Immunology
subject: FOS: Clinical medicine
subject: 69999 Biological Sciences not elsewhere classified
subject: Science Policy
subject: 110309 Infectious Diseases
subject: FOS: Health sciences
subject: 60506 Virology
subject: Computational Biology

description: Table S2a. The reliability for different outcome variables for one out of two weeks of measurement for a 7-d week, weekdays and weekend days, applying a ≥ 4 weekdays and 2 weekend days wear time criterion (n = 257 (38%) children). Table S2b. The reliability for different outcome variables for one out of two weeks of measurement for school hours, afternoon and total leisure time, applying a ≥ 4 weekdays and 2 weekend days wear time criterion (n = 257 (38%) children). (DOCX 20 kb)
Poynting's theorem and energy conservation in the propagation of light in bounded media
Creators: name: Richter, Felix
name: Florian, Matthias
name: Henneberger, Klaus
Publisher: name: arXiv
Year: 2007
Subjects: subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: Optics (physics.optics)
subject: FOS: Physical sciences

description: Starting from the Maxwell-Lorentz equations, Poynting's theorem is reconsidered. The energy flux vector is introduced as S_e=(E x B)/mu_0 instead of E x H, because only by this choice the energy dissipation can be related to the balance of the kinetic energy of the matter subsystem. Conservation of the total energy as the sum of kinetic and electromagnetic energy follows. In our discussion, media and their microscopic nature are represented exactly by their susceptibility functions, which do not necessarily have to be known. On this footing, it can be shown that energy conservation in the propagation of light through bounded media is ensured by Maxwell's boundary conditions alone, even for some frequently used approximations. This is demonstrated for approaches using additional boundary conditions and the dielectric approximation in detail, the latter of which suspected to violate energy conservation for decades.
description: 5 pages, RevTeX4, changes: complete rewrite
title: ADCO, Cartulaire de Cîteaux pour les domaines de Saint-Jean de Losne et Losne (XVIIIe siècle), Cart. 198-01 (11 H 1055), 185 folios, f. 0246
Creators: name: de la Côte d'Or, Archives départementales
name: Petot, Frédéric
name: Archives Départementales De La Côte-D'Or
name: Petot, Frédérique
name: Projet CBMA
name: CG21/F.PETOT/2019
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2020
Subjects: subject: Corpus Burgundiae Medii Aevi
subject: Chartes de la Bourgogne du Moyen Âge
subject: cartulaire
subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris

description: Cartulaire de Cîteaux pour les domaines de Saint-Jean de Losne et Losne (XVIIIe siècle), Archives départementales de la Côte-d'Or, Cart. 198-01 (11 H 1055), 185 folios, f. 0246, Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Cartulaire de Cîteaux pour les domaines de Saint-Jean de Losne et Losne (XVIIIe siècle), Archives départementales de la Côte-d'Or, Cart. 198-01 (11 H 1055), 185 folios, f. 0246, in Projet CBMA - Corpus Burgundiae Medii Aevi [Ressource en ligne], https://manuscrits.cbma-project.eu/
description: Provenance: https://www.geonames.org/3024876
description: Provenance: http://www.idref.fr/030974844/id
description: Provenance: https://catalogue.bnf.fr/ark:/12148/cb12228351v
description: Provenance: abbaye de Cîteaux
description: Provenance: http://www.wikidata.org/entity/Q843261
Additional file 1: of Predicting environmentally suitable areas for Anopheles superpictus Grassi (s.l.), Anopheles maculipennis Meigen (s.l.) and Anopheles sacharovi Favre (Diptera: Culicidae) in Iran
Creators: name: Hanafi-Bojd, Ahmad
name: Sedaghat, Mohammad
name: Vatandoost, Hassan
name: Shahyad Azari-Hamidian
name: Pakdad, Kamran
Publisher: name: figshare
Year: 2018
Subjects: subject: 29999 Physical Sciences not elsewhere classified
subject: FOS: Physical sciences
subject: Medicine
subject: Ecology
subject: FOS: Biological sciences
subject: 69999 Biological Sciences not elsewhere classified
subject: 19999 Mathematical Sciences not elsewhere classified
subject: FOS: Mathematics
subject: Marine Biology

description: Coordinates for collection sites. (DOCX 17 kb)
Lettre de Guillaume-Emmanuel-Joseph de Guilhem de Clermont-Lodève, baron de Sainte-Croix à Jean-François Séguier, 1781-07-28
Creators: name: baron de Sainte-Croix, Guillaume-Emmanuel-Joseph de Guilhem de Clermont-Lodève
name: Guillaume-Emmanuel-Joseph De Guilhem De Clermont-Lodève, Baron De Sainte-Croix
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2021
Subjects: Antiquités (général)

description: [transcription] Il y a des siècles, Monsieur, et respectable ami que je n'ai reçu de vos nouvelles. Je viens rompre ce silence qui coûte tant à mon coeur. Donnez-moi des nouvelles de vos travaux et ce qui m'intéresse davantage de votre santé. J'ai eu beaucoup d'affaires et je suis depuis quelques jours assez incommodé. Cela n'a pas ralenti mon ardeur pour achever un ouvrage auquel je travaille depuis quelque temps, et qui n'est point relatif à mes études chéries, mais à un autre genre, peut-être plus inné chez moi et certainement plus ancien que celui de l'antiquité. Dès que je l'aurai achevé, je retournerai dans les vastes champs de celle-ci, et je glanerai ce qu'on y trouve sur les mystères et vous enverrai ensuite les livres que vous avez eu la bonté de me prêter. Ce sera la besogne de l'hiver. Ces sortes de recherches demandent une saison sédentaire. Vous avez de moi, un ou deux volumes du Journal des savants qui me sont précieux parce qu'il il y est parlé de mon oncle. Il suffit que vous vous en rappeliez. Monsieur de Rochefort m'écrivit, il y a peu de temps, pour me demander de vos nouvelles et les moyens de vous faire faire passer deux de ses ouvrages, une tragédie intitulée Ulysse et un poème sur la mort de l'Impératrice. Monsieur de Villoison vient de publier à Venise deux gros volumes de pièces, quelques inédites. Je les attends mais cela n'arrive pas sitôt. Donnez-moi des nouvelles d'Aubais. Je le répète, surtout des vôtres, ce qui convainc du vif intérêt que j'y prend et du tendre attachement avec lequel j'ai l'honneur d'être,

Monsieur,

votre très humble et très

obéissant serviteur, Sainte-Croix

Mormoiron ce 28 juillet 1781.
description: [personnes citées] Guillaume Dubois de Rochefort, Jean-Baptiste-Gaspard d'Anse de Villoison
description: [reférence bibliographique citée] Rochefort, Guillaume Du Bois de, Ulysse tragédie, Paris, 1781.
. Rochefort, Guillaume Du Bois de, Poème sur la mort de l'impératrice-reine, Paris, 1780.
. Villoison, Jean-Baptiste Gaspard d'Ansse de, Anecdota graeca e regia Parisiensi, & Veneta S. Marci bibliothecis deprompta edidit Johannes Baptista Caspar d'Ansse de Villoison
description: Source: [lieu de Conservation] Nîmes, Bibliothèque Carré d'Art [cote]ms. 141_19, fol. 136
description: Source: ark:/12148/btv1b100152047
Light-Cone Gauge for 1+1 Strings
Creators: name: Smith, Eric
Publisher: name: arXiv
Year: 1992
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: Explicit construction of the light-cone gauge quantum theory of bosonic strings in 1+1 spacetime dimensions reveals unexpected structures. One is the existence of a gauge choice that gives a free action at the price of propagating ghosts and a nontrivial BRST charge. Fixing this gauge leaves a U(1) Kac-Moody algebra of residual symmetry, generated by a conformal tensor of rank two and a conformal scalar. Another is that the BRST charge made from these currents is nilpotent when the action includes a linear dilaton background, independent of the particular value of the dilaton gradient. Spacetime Lorentz invariance in this theory is still elusive, however, because of the linear dilaton background and the nature of the gauge symmetries.
description: 22 pages
Okubo-Zweig-Iizuka-rule violation and B\to η^{(\prime)}K branching ratios
Creators: name: Hsu, Jen-Feng
name: Charng, Yeo-Yie
name: Li, Hsiang-nan
Publisher: name: arXiv
Year: 2007
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We show that few-percent Okubo-Zweig-Iizuka-rule violating effects in the quark-flavor basis for the $η$-$η'$ mixing can enhance the chiral scale associated with the $η_q$ meson few times. This enhancement is sufficient for accommodating the dramatically different data of the $B\toη^{\prime} K$ and $B\toηK$ branching ratios. We comment on other proposals for resolving this problem, including flavor-singlet contributions, axial U(1) anomaly, and nonperturbative charming penguins. Discrimination of the above proposals by means of the $B\toη^{(\prime)}\ellν$ and $B_s\toη^{(\prime)}\ell\ell$ data is suggested.
description: 7 pages, 2 figures, discussion on B\to\eta^{(\prime)}K* added, more references added
Measuring the neutron star tidal deformability with equation-of-state-independent relations and gravitational waves
Creators: name: Chatziioannou, Katerina
name: Haster, Carl-Johan
name: Zimmerman, Aaron
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: Gravitational wave measurements of binary neutron star coalescences offer information about the properties of the extreme matter that comprises the stars. Despite our expectation that all neutron stars in the Universe obey the same equation of state, i.e. the properties of the matter that forms them are universal, current tidal inference analyses treat the two bodies as independent. We present a method to measure the effect of tidal interactions in the gravitational wave signal -- and hence constrain the equation of state -- that assumes that the two binary components obey the same equation of state. Our method makes use of a relation between the tidal deformabilities of the two stars given the ratio of their masses, a relation that has been shown to only have a weak dependance on the equation of state. We use this relation to link the tidal deformabilities of the two stars in a realistic parameter inference study while simultaneously marginalizing over the error in the relation. This approach incorporates more physical information into our analysis, thus leading to a better measurement of tidal effects in gravitational wave signals. Through simulated signals we estimate that uncertainties in the measured tidal parameters are reduced by a factor of at least 2 -- and in some cases up to 10 -- depending on the equation of state and mass ratio of the system.
description: 9 pages, 8 figures, final published version
Selective Phonon Damping in Topological Semimetals
Creators: name: Gordon, Jacob S.
name: Kee, Hae-Young
Publisher: name: arXiv
Year: 2018
Subjects: subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: FOS: Physical sciences

description: Topological semimetals are characterized by their intriguing Fermi surfaces (FSs) such as Weyl and Dirac points, or nodal FS, and their associated surface states. Among them, topological crystalline semimetals, in the presence of strong spin-orbit coupling, possess a nodal FS protected by non-symmorphic lattice symmetries. In particular, it was theoretically proposed that $\mathrm{SrIrO}_{3}$ exhibits a bulk nodal ring due to glide symmetries, as well as flat two-dimensional surface states related to chiral and mirror symmetries. However, due to the semimetallic nature of the bulk, direct observation of these surface states is difficult. Here we study the effect of flat-surface states on phonon modes for $\mathrm{SrIrO}_{3}$ side surfaces. We show that particular phonon modes, based on mirror symmetry, have qualitatively different damping mechanisms due to the surface states which could be used to infer their existence. Experimental techniques for such measurements are also discussed.
description: 12 pages, 2 tables, 7 figures. Published version
Testing Cosmogonic Models with Gravitational Lensing
Creators: name: Wambsganss, Joachim
name: Cen, Renyue
name: Ostriker, Jeremiah P.
name: Turner, Edwin L.
Publisher: name: arXiv
Year: 1994
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Gravitational lensing provides a strict test of cosmogonic models. Detailed numerical propagation of light rays through a universe having a distribution of inhomogeneities derived from the standard CDM (cold dark matter) scenario with the aid of massive, fully nonlinear computer simulations is used to test the model. It predicts that we should have seen far more widely split quasar images than have been found. These and other inconsistencies rule out the COBE normalized CDM model with $Ω=1$ and $H_0=50$km/s/Mpc; but variants of this model might be constructed, which could pass the stringent tests provided by strong gravitational lensing.
description: 7p postscript file, submitted to Nature, local report#940916
RETURN To an Address of the Legislative Assembly, praying for copies of all correspondence (if any) which has taken place between the Government and the Commission appointed to enquire into the truth of the allegations of the Members for Kootenay:--"That the leader of the Government had, through his Kootenay Agents or otherwise, and alone or in connection with any other Members of the House" (of Assembly) "virtually endeavoured to influence the representatives or electors of the district by offering him, Mr. Gallagher, $1,000 and the Government constableship, filled by George A. Kelly, worth $1,400 a year and, inside of three months, the best position in the gift of the Government." Also, copies of all correspondence which has taken place between the Commission and Mr. Elliott in regard to the enquiry.
Creators: name: British Columbia. Legislative Assembly
Publisher: name: Victoria, BC : Government Printer
Year: 2016

Abstract
Digital Humanities and Legal History Can the computer read and classify ordinances?
Creators: name: Romein, Christel Annemieke
Publisher: name: Zenodo
Year: 2019
Subjects: digital scholarship
KB Lab
Digital Humanities
Computational linguistics
Entangled Histories
Police Ordinances

description: As Researcher-in-Residence at the KB National Library of the Netherlands (The Hague), I – Annemieke Romein – I look for early modern norms in books of ordinances (‘plakkaatboeken’). These books hold mainly administrative laws, varying from norms against beggars, safety, but also laws intended to stimulate the economy, and international treaties are frequently included too. Together with colleagues at the library, we are looking for means to have the computer take over the process of categorising these texts. The question is: Can a computer recognise the texts containing rules, and distinguish between texts on religion, maintenance of dykes, colonial affairs, etc.? (Full blog in English) Published at: http://esclh.blogspot.com/2019/08/project-presentation-digital-humanities.html?m=1 (30 August 2019) https://lab.kb.nl/about-us/blog/digital-humanities-and-legal-history-can-computer-read-and-classify-ordinances (10 October 2019)
description: {"references": ["http://esclh.blogspot.com/2019/08/project-presentation-digital-humanities.html?m=1", "https://lab.kb.nl/about-us/blog/digital-humanities-and-legal-history-can-computer-read-and-classify-ordinances"]}
Hadronic Superpartners from Superconformal and Supersymmetric Algebra
Creators: name: Nielsen, Marina
name: Brodsky, Stanley J.
Publisher: name: arXiv
Year: 2018
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: Through the embedding of superconformal quantum mechanics into AdS space, it is possible to construct an effective supersymmetric QCD light-front Hamiltonian for hadrons, which includes a spin-spin interaction between the hadronic constituents. A specific breaking of conformal symmetry determines a unique effective quark-confining potential for light hadrons, as well as remarkable connections between the meson, baryon, and tetraquark spectra. The pion is massless in the chiral limit and has no supersymmetric partner. The excitation spectra of relativistic light-quark meson, baryon and tetraquark bound states lie on linear Regge trajectories with identical slopes in the radial and orbital quantum numbers. Although conformal symmetry is strongly broken by the heavy quark mass, the basic underlying supersymmetric mechanism, which transforms mesons to baryons (and baryons to tetraquarks) into each other, still holds and gives remarkable connections across the entire spectrum of light, heavy-light and double-heavy hadrons. Here we show that all the observed hadrons can be related through this effective supersymmetric QCD, and that it can be used to identify the structure of the new charmonium states.
description: revised version accepted for publication at Phys. Rev. D
Integrable versus Non-Integrable Spin Chain Impurity Models
Creators: name: Sorensen, E. S.
name: Eggert, S.
name: Affleck, I.
Publisher: name: arXiv
Year: 1993
Subjects: subject: Condensed Matter (cond-mat)
subject: FOS: Physical sciences

description: Recent renormalization group studies of impurities in spin-1/2 chains appear to be inconsistent with Bethe ansatz results for a special integrable model. We study this system in more detail around the integrable point in parameter space and argue that this integrable impurity model corresponds to a non-generic multi-critical point. Using previous results on impurities in half-integer spin chains, a consistent renormalization group flow and phase diagram is proposed.
description: 20 pages 11 figures obtainable from authors, REVTEX 3.0
Simulating realistic self-interacting dark matter models including small and large-angle scattering
Creators: name: Arido, Cenanda
name: Fischer, Moritz S.
name: Garny, Mathias
Publisher: name: arXiv
Year: 2024
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: Astrophysics of Galaxies (astro-ph.GA)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: Dark matter (DM) self-interactions alter the matter distribution on galactic scales and alleviate tensions with observations. A feature of the self-interaction cross section is its angular dependence, influencing offsets between galaxies and DM halos in merging galaxy clusters. While algorithms for modelling mostly forward-dominated or mostly large-angle scatterings exist, incorporating realistic angular dependencies, such as light mediator models, within $N$-body simulations remains challenging. We develop, validate and apply a novel and efficient method, combining existing approaches to describe small- and large-angle scattering regimes within a hybrid scheme. Below a critical angle the effective description via a drag force combined with transverse momentum diffusion is used, while above the angle dependence is sampled explicitly. First, we verify the scheme using a test set-up with known analytical solutions, and check that our results are insensitive to the choice of the critical angle within an expected range. Next, we demonstrate that our scheme speeds up the computations by multiple orders of magnitude for realistic light mediator models. Finally, we apply the method to galaxy cluster mergers and discuss the sensitivity of the offset between galaxies and DM to the angle dependence of the cross section. Our scheme ensures accurate offsets for mediator mass $m_ϕ$ and DM mass $m_χ$ within the range $0.1v/c\lesssim m_ϕ/m_χ\lesssim v/c$, while for larger (smaller) mass ratios the offsets obtained for isotropic (forward-dominated) self-scattering are approached. Here $v$ is the typical velocity scale. Equivalently, the upper condition can be expressed as $1.1\lesssim σ_{\rm tot}/σ_{\mathrm{\widetilde{T}}}\lesssim 10$ for the ratio of the total and momentum transfer cross sections, with the ratio being $1$ ($\infty$) in the isotropic (forward-dominated) limits.
description: 23 pages, 13 figures + appendix, accepted for publication in A&A
An Investigation of the Interstellar Environment of Supernova Remnant CTB 87
Creators: name: Liu, Qian-Cheng
name: Chen, Yang
name: Chen, Bing-Qiu
name: Zhou, Ping
name: Wang, Xiao-Tao
name: Su, Yang
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: We present a new millimeter CO-line observation towards supernova remnant (SNR) CTB 87, which was regarded purely as a pulsar wind nebula (PWN), and an optical investigation of a coincident surrounding superbubble. The CO observation shows that the SNR delineated by the radio emission is projectively covered by a molecular cloud (MC) complex at V$_{\rm {LSR}}$ = $-60$ to $-54$ km s$^{-1}$. Both the symmetric axis of the radio emission and the trailing X-ray PWN appear projectively to be along a gap between two molecular gas patches at $-58$ to $-57$ km s$^{-1}$. Asymmetric broad profiles of $^{12}$CO lines peaked at $-58$ km s$^{-1}$ are found at the eastern and southwestern edges of the radio emission. This represents a kinematic signature consistent with an SNR-MC interaction. We also find that a superbubble, $\sim 37'$ in radius, appears to surround the SNR from HI 21cm (V$_{\rm {LSR}} \sim -61$ to $-68$ km s$^{-1}$), WISE mid-IR, and optical extinction data. We build a multi-band photometric stellar sample of stars within the superbubble region and find 82 OB star candidates. The likely peak distance in the stars' distribution seems consistent with the distance previously suggested for CTB 87. We suggest the arc-like radio emission is mainly the relic of the part of blastwave that propagates into the MC complex and is now in a radiative stage while the other part of blastwave has been expanding into the low-density region in the superbubble. This scenario naturally explains the lack of the X-ray emission related to the ejecta and blastwave. The SNR-MC interaction also favours a hadronic contribution to the γ-ray emission from the CTB 87 region.
description: 25 pages, 9 figures, 2 tables. Accepted to the Astrophysical Journal
Essential curves in handlebodies and topological contractions
Creators: name: Grines, Viatcheslav
name: Laudenbach, François
Publisher: name: arXiv
Year: 2007
Subjects: subject: Geometric Topology (math.GT)
subject: FOS: Mathematics
subject: 57M25, 37D15

description: If $X$ is a compact set, a {\it topological contraction} is a self-embedding $f$ such that the intersection of the successive images $f^k(X)$, $k>0$, consists of one point. In dimension 3, we prove that there are smooth topological contractions of the handlebodies of genus $\geq 2$ whose image is essential. Our proof is based on an easy criterion for a simple curve to be essential in a handlebody.
title: ADCO, Grènetier de Cîteaux : comptes (1497-1504) (11 H 1172), f. 00611
Creators: name: de la Côte-d'Or, Archives départementales
name: Archives Départementales De La Côte-D'Or
name: Petot, Frédérique
name: Projet CBMA
name: CBMA/CG21/F.PETOT/2019
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2020
Subjects: subject: comptes
subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris
subject: Corpus Burgundiae Medii Aevi
subject: Chartes de la Bourgogne du Moyen Âge

description: Grènetier de Cîteaux : comptes (1497-1504), Archives départementales de la Côte-d'Or, (11 H 1172). Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Grènetier de Cîteaux : comptes (1497-1504), Archives départementales de la Côte-d'Or, (11 H 1172), f. 00611, 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
Additional file 6: of Estimating causal effects of time-dependent exposures on a binary endpoint in a high-dimensional setting
Creators: name: Vahé Asvatourian
name: Coutzac, Clélia
name: Chaput, Nathalie
name: Robert, Caroline
name: Michiels, Stefan
name: Lanoy, Emilie
Publisher: name: figshare
Year: 2018
Subjects: subject: Space Science
subject: Molecular Biology
subject: Pharmacology
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: 19999 Mathematical Sciences not elsewhere classified
subject: FOS: Mathematics
subject: 60506 Virology

description: Estimation of biomarkers’ median effect. It provides supplementary tables of the application results. (DOCX 31 kb)
Frozen and $β$-equilibrated $f$ and $p$ modes of cold neutron stars: nuclear metamodel predictions
Creators: name: Montefusco, Gabriele
name: Antonelli, Marco
name: Gulminelli, Francesca
Publisher: name: arXiv
Year: 2024
Subjects: subject: Nuclear Theory (nucl-th)
subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: When the chemical re-equilibration timescale is sufficiently long, the normal and quasi-normal mode frequencies of neutron stars should be calculated in the idealized limit that the internal composition of each fluid element is fixed over the oscillation period. However, many studies rely on a barotropic equation of state, which implicitly overlooks potential out-of-$β$-equilibrium effects. To investigate possible biases arising from this assumption, we calculate the non-radial fundamental ($f$) and first pressure ($p_1$) modes for a wide range of neutron star structures, each governed by different nucleonic equations of state. This ensemble is generated using the metamodel technique, a phenomenological framework that incorporates constraints from experimental nuclear physics and chiral effective field theory. The metamodel also provides the internal composition of $β$-equilibrated $npeμ$ matter, allowing us to calculate oscillation modes beyond those supported by a purely barotropic fluid. Thus, we systematically assess the impact of assuming a barotropic equation of state across various equations of state and provide a distribution of expected $f$ and $p_1$ mode frequencies that may be detectable by next-generation gravitational wave interferometers.
description: 11 pages, 7 figures
The Complete Spectrum of the $W_N$ String
Creators: name: Lu, H.
name: Pope, C. N.
name: Schrans, S.
name: Xu, K. W.
Publisher: name: arXiv
Year: 1992
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We obtain the complete physical spectrum of the $W_N$ string, for arbitrary $N$. The $W_N$ constraints freeze $N-2$ coordinates, while the remaining coordinates appear in the currents only {\it via} their energy-momentum tensor. The spectrum is then effectively described by a set of ordinary Virasoro-like string theories, but with a non-critical value for the central charge and a discrete set of non-standard values for the spin-2 intercepts. In particular, the physical spectrum of the $W_N$ string includes the usual massless states of the Virasoro string. By looking at the norms of low-lying states, we find strong indications that all the $W_N$ strings are unitary.
description: 28 pages
RETURN To an Address of the Legislative Assembly for copies of all correspondence, Orders in Council, and other documents whatsoever, in relation to the Miners' strike at Nanaimo, and to the dispatch of a body of armed volunteers, or militia, to the District of Nanaimo, in the spring of 1877.
Creators: name: British Columbia. Legislative Assembly
Publisher: name: Victoria, BC : Government Printer
Year: 2016

Abstract
Detection of an inner gaseous component in a Herbig Be star accretion disk: Near- and mid-infrared spectro-interferometry and radiative transfer modeling of MWC 147
Creators: name: Kraus, Stefan
name: Preibisch, Thomas
name: Ohnaka, Keiichi
Publisher: name: arXiv
Year: 2007
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We study the geometry and the physical conditions in the inner (AU-scale) circumstellar region around the young Herbig Be star MWC 147 using long-baseline spectro-interferometry in the near-infrared (NIR K-band, VLTI/AMBER observations and PTI archive data) as well as the mid-infrared (MIR N-band, VLTI/MIDIobservations). The emission from MWC 147 is clearly resolved and has a characteristic physical size of approx. 1.3 AU and 9 AU at 2.2 micron and 11 micron respectively (Gaussian diameter). The spectrally dispersed AMBER and MIDI interferograms both show a strong increase in the characteristic size towards longer wavelengths, much steeper than predicted by analytic disk models assuming power-law radial temperature distributions. We model the interferometric data and the spectral energy distribution of MWC 147 with 2-D, frequency-dependent radiation transfer simulations. This analysis shows that models of spherical envelopes or passive irradiated Keplerian disks (with vertical or curved puffed-up inner rim) can easily fit the SED, but predict much lower visibilities than observed; the angular size predicted by such models is 2 to 4 times larger than the size derived from the interferometric data, so these models can clearly be ruled out. Models of a Keplerian disk with optically thick gas emission from an active gaseous disk (inside the dust sublimation zone), however, yield a good fit of the SED and simultaneously reproduce the absolute level and the spectral dependence of the NIR and MIR visibilities. We conclude that the NIR continuum emission from MWC 147 is dominated by accretion luminosity emerging from an optically thick inner gaseous disk, while the MIR emission also contains contributions from the outer, irradiated dust disk.
description: 44 pages, 15 figures, accepted for publication in The Astrophysical Journal. The quality of the figures was slightly reduced in order to comply with the astro-ph file-size restrictions. You can find a high-quality version of the paper at http://www.mpifr-bonn.mpg.de/staff/skraus/papers/mwc147.pdf
Estimator of Prediction Error Based on Approximate Message Passing for Penalized Linear Regression
Creators: name: Sakata, Ayaka
Publisher: name: arXiv
Year: 2018
Subjects: subject: Machine Learning (stat.ML)
subject: Machine Learning (cs.LG)
subject: FOS: Computer and information sciences

description: We propose an estimator of prediction error using an approximate message passing (AMP) algorithm that can be applied to a broad range of sparse penalties. Following Stein's lemma, the estimator of the generalized degrees of freedom, which is a key quantity for the construction of the estimator of the prediction error, is calculated at the AMP fixed point. The resulting form of the AMP-based estimator does not depend on the penalty function, and its value can be further improved by considering the correlation between predictors. The proposed estimator is asymptotically unbiased when the components of the predictors and response variables are independently generated according to a Gaussian distribution. We examine the behaviour of the estimator for real data under nonconvex sparse penalties, where Akaike's information criterion does not correspond to an unbiased estimator of the prediction error. The model selected by the proposed estimator is close to that which minimizes the true prediction error.
title: ADCO, Neuvième cartulaire de Saint-Étienne de Dijon (1661 - 1684), Cart. 32 (G 136), 745 folios, f. 1408
Creators: name: de la Côte d'Or, Archives départementales
name: Petot, Frédéric
name: Archives Départementales De La Côte-D'Or
name: Petot, Frédérique
name: Projet CBMA
name: CG21/F.PETOT/2012
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2020
Subjects: subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris
subject: Corpus Burgundiae Medii Aevi
subject: Chartes de la Bourgogne du Moyen Âge
subject: cartulaire

description: Neuvième cartulaire de Saint-Étienne de Dijon (1661 - 1684), Archives départementales de la Côte-d'Or, Cart. 32 (G 136), 745 folios, f. 1408, Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Neuvième cartulaire de Saint-Étienne de Dijon (1661 - 1684), Archives départementales de la Côte-d'Or, Cart. 32 (G 136), 745 folios, f. 1408, 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
Distribution-free uncertainty quantification for inverse problems: application to weak lensing mass mapping
Creators: name: Leterme, Hubert
name: Fadili, Jalal
name: Starck, Jean-Luc
Publisher: name: arXiv
Year: 2024
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: Instrumentation and Methods for Astrophysics (astro-ph.IM)
subject: Methodology (stat.ME)
subject: FOS: Physical sciences
subject: FOS: Computer and information sciences

description: In inverse problems, distribution-free uncertainty quantification (UQ) aims to obtain error bars with coverage guarantees that are independent of any prior assumptions about the data distribution. In the context of mass mapping, uncertainties could lead to errors that affects our understanding of the underlying mass distribution, or could propagate to cosmological parameter estimation, thereby impacting the precision and reliability of cosmological models. Current surveys, such as Euclid or Rubin, will provide new weak lensing datasets of very high quality. Accurately quantifying uncertainties in mass maps is therefore critical to perform reliable cosmological parameter inference. In this paper, we extend the conformalized quantile regression (CQR) algorithm, initially proposed for scalar regression, to inverse problems. We compare our approach with another distribution-free approach based on risk-controlling prediction sets (RCPS). Both methods are based on a calibration dataset, and offer finite-sample coverage guarantees that are independent of the data distribution. Furthermore, they are applicable to any mass mapping method, including blackbox predictors. In our experiments, we apply UQ on three mass-mapping method: the Kaiser-Squires inversion, iterative Wiener filtering, and the MCALens algorithm. Our experiments reveal that RCPS tends to produce overconservative confidence bounds with small calibration sets, whereas CQR is designed to avoid this issue. Although the expected miscoverage rate is guaranteed to stay below a user-prescribed threshold regardless of the mass mapping method, selecting an appropriate reconstruction algorithm remains crucial for obtaining accurate estimates, especially around peak-like structures, which are particularly important for inferring cosmological parameters. Additionally, the choice of mass mapping method influences the size of the error bars.
description: Accepted for publication in Astronomy & Astrophysics
Conductivity of higher dimensional holographic superconductors with nonlinear electrodynamics
Creators: name: Sheykhi, Ahmad
name: Asl, Doa Hashemi
name: Dehyadegari, Amin
Publisher: name: arXiv
Year: 2018
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: We investigate analytically as well as numerically the properties of s-wave holographic superconductors in $d$-dimensional spacetime and in the presence of Logarithmic nonlinear electrodynamics. We study three aspects of these kind of superconductors. First, we obtain, by employing analytical Sturm-Liouville method as well as numerical shooting method, the relation between critical temperature and charge density, $ρ$, and disclose the effects of both nonlinear parameter $b$ and the dimensions of spacetime, $d$, on the critical temperature $T_c$. We find that in each dimension, $T_c/ρ^{1/(d-2)}$ decreases with increasing the nonlinear parameter $b$ while it increases with increasing the dimension of spacetime for a fixed value of $b$. Then, we calculate the condensation value and critical exponent of the system analytically and numerically and observe that in each dimension, the condensation get larger with increasing the nonlinear parameter $b$. Besides, for a fixed value of $b$, it increases with increasing the spacetime dimension. We confirm that the results obtained from our analytical method are in agreement with the results obtained from numerical shooting method. This fact may support the correctness of our analytical method. Finally, we explore the holographic conductivity of this system and find out that the superconducting gap increases with increasing either the nonlinear parameter or the spacetime dimension.
description: 25 pages
Spaceflight from Super-Earths is difficult
Creators: name: Hippke, Michael
Publisher: name: arXiv
Year: 2018
Subjects: subject: Popular Physics (physics.pop-ph)
subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: FOS: Physical sciences

description: Many rocky exoplanets are heavier and larger than the Earth, and have higher surface gravity. This makes space-flight on these worlds very challenging, because the required fuel mass for a given payload is an exponential function of planetary surface gravity. We find that chemical rockets still allow for escape velocities on Super-Earths up to 10x Earth mass. More massive rocky worlds, if they exist, would require other means to leave the planet, such as nuclear propulsion.
description: Accepted for publication in the International Journal of Astrobiology. arXiv admin note: substantial text overlap with arXiv:1803.11384
The Superfluidity and Experimental Properties of Odd-Energy-Gap Superconductors
Creators: name: Dobroliubov, M.
name: Langmann, E.
name: Stamp, P. C. E.
Publisher: name: arXiv
Year: 1993
Subjects: subject: Condensed Matter (cond-mat)
subject: FOS: Physical sciences

description: We consider the experimental properties of superconductors with a gap which is an odd function of energy $\bepsk=\epsk - μ$, i.e.\ , a gap which vanishes everywhere on the Fermi surface; this is done within a in a BCS framework. Apart from the standard phenomenology (density of states, penetration depth, NMR, $C_V(T)$, $B_{c2}(T)$), we also look at the stability of the superconducting state. It is stable to finite supercurrents (although with a normal fluid density which increases with the supercurrent density), and is also very weakly affected by non-magnetic impurities. We find two classes of odd-gap superconductors, which strongly differ in their low-energy properties. For a certain parameter range, most of the results resemble those for d-wave superconductors (except for the effect of impurities).
description: LaTeX, 13pp plus 6 PS figures included in PSBOX format UBCTP CM1-1993
Additional file 5: of Trimodal distribution of arylamine N-acetyltransferase 1 mRNA in breast cancer tumors: association with overall survival and drug resistance
Creators: name: Minchin, Rodney
name: Butcher, Neville
Publisher: name: figshare
Year: 2018
Subjects: subject: Genetics
subject: FOS: Biological sciences
subject: Pharmacology
subject: Biotechnology
subject: Ecology
subject: 69999 Biological Sciences not elsewhere classified
subject: 19999 Mathematical Sciences not elsewhere classified
subject: FOS: Mathematics
subject: Cancer
subject: Plant Biology

description: Table S2. The Cox proportional hazard regression models based on survival for NAT1 sub-populations, tumour characteristics and treatment. (PDF 121 kb)
The notion of persistence applied to breathers in thermal equilibrium
Creators: name: Farago, Jean
Publisher: name: arXiv
Year: 2007
Subjects: subject: Statistical Mechanics (cond-mat.stat-mech)
subject: FOS: Physical sciences

description: We study the thermal equilibrium of nonlinear Klein-Gordon chains at the limit of small coupling (anticontinuum limit). We show that the persistence distribution associated to the local energy density is a useful tool to study the statistical distribution of so-called thermal breathers, mainly when the equilibrium is characterized by long-lived static excitations; in that case, the distribution of persistence intervals turns out to be a powerlaw. We demonstrate also that this generic behaviour has a counterpart in the power spectra, where the high frequencies domains nicely collapse if properly rescaled. These results are also compared to non linear Klein-Gordon chains with a soft nonlinearity, for which the thermal breathers are rather mobile entities. Finally, we discuss the possibility of a breather-induced anomalous diffusion law, and show that despite a strong slowing-down of the energy diffusion, there are numerical evidences for a normal asymptotic diffusion mechanism, but with exceptionnally small diffusion coefficients.
description: submitted to Physica D
IN03056 Slab-Inscription of Queen Līlāvatī
Creators: name: Wickremasinghe, Don Martino de Zilva
Publisher: name: Zenodo
Year: 2019
Subjects: IN03056
Epigraphia Zeylanica
Līlāvatī

description: IN03056 Slab-Inscription of Queen Līlāvatī - Transcript and Translation Source: Wickremasinghe, Don Martino de Zilva. (1904-12). ‘No. 14. The Slab-Inscription Marked D/8 of Queen Līlāvatī,’ Epigraphia Zeylanica 1, pp. 176-182.
Connections between Minkowski and Cosmological Correlation Functions
Creators: name: Chu, Shek Kit
name: Lee, Mang Hei Gordon
name: Lu, Shiyun
name: Tong, Xi
name: Wang, Yi
name: Zhou, Siyi
Publisher: name: arXiv
Year: 2018
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: We show how cosmological correlation functions of massless fields can be rewritten in terms of Minkowski correlation functions, by extracting symmetry-breaking operators from the cosmological correlators. This technique simplifies some cosmological calculations. Also, known properties of Minkowski correlation functions can be translated to non-trivial properties of cosmological correlations. To illustrate this idea, inflation to Minkowski and matter bounce to Minkowski relations are presented for the interactions of general single field inflation. And a Minkowski recursion relation is translated to a novel relation for inflation.
description: 19 pages, 2 figures