cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
On the use of variability time-scales as an early classifier of radio transients and variables
Creators: name: Pietka, M.
name: Staley, T. D.
name: Pretorius, M. L.
name: Fender, R. P.
Publisher: name: arXiv
Year: 2017
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: We have shown previously that a broad correlation between the peak radio luminosity and the variability time-scales, approximately L ~ t^5, exists for variable synchrotron emitting sources and that different classes of astrophysical source occupy different regions of luminosity and time-scale space. Based on those results, we investigate whether the most basic information available for a newly discovered radio variable or transient - their rise and/or decline rate - can be used to set initial constraints on the class of events from which they originate. We have analysed a sample of ~ 800 synchrotron flares, selected from light-curves of ~ 90 sources observed at 5-8 GHz, representing a wide range of astrophysical phenomena, from flare stars to supermassive black holes. Selection of outbursts from the noisy radio light-curves has been done automatically in order to ensure reproducibility of results. The distribution of rise/decline rates for the selected flares is modelled as a Gaussian probability distribution for each class of object, and further convolved with estimated areal density of that class in order to correct for the strong bias in our sample. We show in this way that comparing the measured variability time-scale of a radio transient/variable of unknown origin can provide an early, albeit approximate, classification of the object, and could form part of a suite of measurements used to provide early categorisation of such events. Finally, we also discuss the effect scintillating sources will have on our ability to classify events based on their variability time-scales.
description: Accepted for publication in MNRAS
Numerical Experiments on The Capacity of Quantum Channel with Entangled Input States
Creators: name: Osawa, Susumu
name: Nagaoka, Hiroshi
Publisher: name: arXiv
Year: 2000
Subjects: subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: The capacity of quantum channel with product input states was formulated by the quantum coding theorem. However, whether entangled input states can enhance the quantum channel is still open. It turns out that this problem is reduced to aspecial case of the more general problem whether the capacity of product quantum channel exhibits additivity. In the present study, we apply one of the quantum Arimoto-Blahut type algorithms to the latter problem. The results suggest that the additivity of product quantum channel capacity always holds and that entangled input states cannot enhance the quantum channel capacity.
description: Latex, 13 pages, partly presented at the second QIT and the 22nd SITA. Final version to appear in IEICE Trans. Fundamentals
Design and Performance of the Wide-Field X-Ray Monitor on Board the High-Energy Transient Explorer 2
Creators: name: Shirasaki, Y.
name: Kawai, N.
name: Yoshida, A.
name: Matsuoka, M.
name: Tamagawa, T.
name: Torii, K.
name: Sakamoto, T.
name: Suzuki, M.
name: Urata, Y.
name: Sato, R.
name: Nakagawa, Y.
name: Takahashi, D.
name: Fenimore, E. E.
name: Galassi, M.
name: Lamb, D. Q.
name: Graziani, C.
name: Donaghy, T. Q.
name: Vanderspek, R.
name: Yamauchi, M.
name: Takagishi, K.
name: Hatsukade, I.
Publisher: name: arXiv
Year: 2003
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: The Wide-field X-ray Monitor (WXM) is one of the scientific instruments carried on the High Energy Transient Explorer 2 (HETE-2) satellite launched on 2000 October 9. HETE-2 is an international mission consisting of a small satellite dedicated to provide broad-band observations and accurate localizations of gamma-ray bursts (GRBs). A unique feature of this mission is its capability to determine and transmit GRB coordinates in almost real-time through the burst alert network. The WXM consists of three elements: four identical Xe-filled one-dimensional position-sensitive proportional counters, two sets of one-dimensional coded apertures, and the main electronics. The WXM counters are sensitive to X-rays between 2 keV and 25 keV within a field-of-view of about 1.5 sr, with a total detector area of about 350 cm$^2$. The in-flight triggering and localization capability can produce a real-time GRB location of several to 30 arcmin accuracy, with a limiting sensitivity of $10^{-7}$ erg cm$^{-2}$. In this report, the details of the mechanical structure, electronics, on-board software, ground and in-flight calibration, and in-flight performance of the WXM are discussed.
description: 28 pages, 24 figures
Half polarized U(1) symmetric vacuum spacetimes with AVTD behavior
Creators: name: Choquet-Bruhat, Yvonne
name: Isenberg, James
Publisher: name: arXiv
Year: 2005
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: In a previous work, we used a polarization condition to show that there is a family of U(1) symmetric solutions of the vacuum Einstein equations such that each exhibits AVTD (Asymptotic Velocity Term Dominated) behavior in the neighborhood of its singularity. Here we consider the general case of U(1) bundles and determine a condition, called the half polarization condition, necessary and sufficient in our context, for AVTD behavior near the singularity.
Additional file 1 of Systematically analysis of decompensated cirrhotic patients with spontaneous bacterial peritonitis to identify diagnostic and prognostic indexes
Creators: name: Du, Tao
name: Li, Qing-ping
name: Jiang, Gui-xiang
name: Tan, Hui-yuan
name: Wu, Jiao-hua
name: Qin, Shan-yu
name: Yu, Bing
name: Jiang, Hai-xing
name: Luo, Wei
Publisher: name: figshare
Year: 2023
Subjects: subject: Medicine
subject: Cell Biology
subject: Genetics
subject: FOS: Biological sciences
subject: Immunology
subject: FOS: Clinical medicine
subject: Biological Sciences not elsewhere classified
subject: Mathematical Sciences not elsewhere classified
subject: Science Policy
subject: Hematology
subject: Virology

description: Additional file 1: Supplementary Table S1. The laboratory indicators of ascites and serum PCT in 52 patients with SBP. Supplementary Table S2. The clinical characteristics of 12 patients with PMN < 250×106/L and PCT≤0.5 ng/ml.
Access control management for e-Healthcare in cloud environment
Creators: name: Sun, Lili
name: Yong, Jianming
name: Soar, Jeffrey
Publisher: name: arXiv
Year: 2017
Subjects: subject: Cryptography and Security (cs.CR)
subject: Computers and Society (cs.CY)
subject: FOS: Computer and information sciences

description: Semantic web technologies represent much richer forms of relationships among users, resources and actions among different web applications such as clouding computing. However, Semantic web applications pose new requirements for security mechanisms especially in the access control models. This paper addresses existing access control methods and presents a semantic based access control model which considers semantic relations among different entities in cloud computing environment. We have enriched the research for semantic web technology with role-based access control that is able to be applied in the field of medical information system or e-Healthcare system. This work shows how the semantic web technology provides efficient solutions for the management of complex and distributed data in heterogeneous systems, and it can be used in the medical information systems as well.
description: 11 pages
On Titanium Carbide Nanoparticles as the Origin of the 21 Micron Emission Feature in Post-Asymptotic Giant Branch Stars
Creators: name: Li, Aigen
Publisher: name: arXiv
Year: 2003
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Titanium carbide (TiC) nanocrystals were recently proposed as the carrier of the mysterious 21$\mum$ emission feature observed in post-asymptotic giant branch stars, based on their close spectral match and the presolar nature of meteoritic TiC nanograins (which reveals their stellar ejecta origin). But we show in this {\it Letter} that the Kramers-Kronig dispersion relations, which relate the wavelength-integrated extinction cross section to the total dust mass, would impose a lower bound on the TiC mass. This Kramers-Kronig lower limit exceeds the maximum available TiC mass by a factor of at least $\simali$50, independent of the absolute value of the ultraviolet/visible absorptivity of nano TiC. The TiC model is therefore readily ruled out by the Kramers-Kronig physical principle.
description: To appear in The Astrophysical Journal Letters; 10 pages, 3 figures
title: ADCO, Neuvième cartulaire de Saint-Étienne de Dijon (1661 - 1684), Cart. 32 (G 136), 745 folios, f. 0010
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
name: Petot, Frédéric
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2020
Subjects: subject: Chartes de la Bourgogne du Moyen Âge
subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris
subject: cartulaire
subject: Corpus Burgundiae Medii Aevi

description: Neuvième cartulaire de Saint-Étienne de Dijon (1661 - 1684), Archives départementales de la Côte-d'Or, Cart. 32 (G 136), 745 folios, f. 0010, 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. 0010, 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
Predicting Structures in the Zone of Avoidance
Creators: name: Sorce, Jenny G.
name: Colless, Matthew
name: Kraan-Korteweg, Renee C.
name: Gottloeber, Stefan
Publisher: name: arXiv
Year: 2017
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: The Zone of Avoidance (ZOA), whose emptiness is an artifact of our Galaxy dust, has been challenging observers as well as theorists for many years. Multiple attempts have been made on the observational side to map this region in order to better understand the local flows. On the theoretical side, however, this region is often simply statistically populated with structures but no real attempt has been made to confront theoretical and observed matter distributions. This paper takes a step forward using constrained realizations of the local Universe shown to be perfect substitutes of local Universe-like simulations for smoothed high density peak studies. Far from generating completely `random' structures in the ZOA, the reconstruction technique arranges matter according to the surrounding environment of this region. More precisely, the mean distributions of structures in a series of constrained and random realizations differ: while densities annihilate each other when averaging over 200 random realizations, structures persist when summing 200 constrained realizations. The probability distribution function of ZOA grid cells to be highly overdense is a Gaussian with a 15% mean in the random case, while that of the constrained case exhibits large tails. This implies that areas with the largest probabilities host most likely a structure. Comparisons between these predictions and observations, like those of the Puppis 3 cluster, show a remarkable agreement and allow us to assert the presence of the, recently highlighted by observations, Vela supercluster at about 180 Mpc/h, right behind the thickest dust layers of our Galaxy.
description: Accepted for publication in MNRAS, 11 pages, 6 figures, 1 table
Pedestrian navigation and public transit training interventions for youth with disabilities: a systematic review
Creators: name: Lindsay, Sally
name: De-Lawrence Lamptey
Publisher: name: Taylor & Francis
Year: 2018
Subjects: subject: Medicine
subject: Neuroscience
subject: Sociology
subject: FOS: Sociology
subject: Science Policy
subject: 111714 Mental Health
subject: FOS: Health sciences

description: Purpose: Being able to travel independently, whether as a pedestrian or by taking public transportation, is a critical element to maintaining quality of life and participation in the community. The objective of this systematic review is to understand the best practices and effective components of pedestrian and public transit training interventions for youth with disabilities. Method: Systematic searches of seven international databases identified 29 studies meeting our inclusion criteria. We analyzed these studies based on participant characteristics, methods, results, and quality of evidence. Results: Among the 29 studies, 857 participants (aged 5–39, mean 18.3 years) were represented across 10 countries. Although the intervention outcomes varied across the studies, 24 of them reported an improvement in at least one of the following: pedestrian and general navigation skills, pedestrian safety, landmark recognition, route knowledge, and public transportation skills. Conclusions: Our findings highlight that pedestrian and public transit interventions have the potential to improve the participation and quality of life of children and youth with disabilities. More rigorous, theoretically informed interventions, using standardized measures are needed to enhance pedestrian and transit training skills among youth with disabilities.Implications for rehabilitationTravel training interventions have the potential to effectively support youth with disabilities in learning pedestrian and public transportation navigation skills.Clinicians and educators should encourage youth with disabilities to participate in travel training programs enhance their independence skills and participation in the community.Clinicians, educators, and program managers can help to build relevant content for travel training programs and connect youth to programs. Travel training interventions have the potential to effectively support youth with disabilities in learning pedestrian and public transportation navigation skills. Clinicians and educators should encourage youth with disabilities to participate in travel training programs enhance their independence skills and participation in the community. Clinicians, educators, and program managers can help to build relevant content for travel training programs and connect youth to programs.
Modeling the Infrared Emission from the Epsilon Eridani Disk
Creators: name: Li, Aigen
name: Lunine, J. I.
name: Bendo, G. J.
Publisher: name: arXiv
Year: 2003
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We model the infrared (IR) emission from the ring-like dust disk around the main-sequence (MS) star Epsilon Eridani, a young analog to our solar system, in terms of a porous dust model previously developed for the extended wedge-shaped disk around the MS star $β$ Pictoris and the sharply truncated ring-like disks around the Herbig Ae/Be stars HR 4796A and HD 141569A. It is shown that the porous dust model with a porosity of $\simali$90% is also successful in reproducing the IR to submillimeter dust emission spectral energy distribution as well as the 850$\mum$ flux radial profile of the dust ring around the more evolved MS star Epsilon Eridani. Predictions are made for future {\it SIRTF} observations which may allow a direct test of the porous dust model.
description: To appear in The Astrophysical Journal Letters (2003-November-20th issue); 11 pages; 2 figures
Systems Leadership for Learning
Creators: name: Haßler, Björn
Publisher: name: Zenodo
Year: 2019

description: The Google Doc for this article is available at https://docs.google.com/document/d/1YtDTd-YHXCO4eMTguu2rENDXdQFHq9Ct6w-_uXbI8ls/edit# and comments are welcome. Please cite as: Björn Haßler (2019). Systems Leadership for Learning — A framework for development cooperation in education. Open Development & Education, Cambridge, UK. DOI: 10.5281/zenodo.2626704. Available under Creative Commons Attribution 4.0 International, https://creativecommons.org/licenses/by/4.0/.
No urban malaise for Millennials
Creators: name: Okulicz-Kozaryn, Adam
name: Rubia R. Valente
Publisher: name: Taylor & Francis
Year: 2018
Subjects: subject: Genetics
subject: FOS: Biological sciences
subject: 59999 Environmental Sciences not elsewhere classified
subject: FOS: Earth and related environmental 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: Cancer
subject: Science Policy

description: Urban malaise or unhappiness with city life is common in developed countries. City dwellers, particularly those in the largest metropolitan areas, are reported to be the least satisfied with their lives. Using the US General Social Survey (1972–2016), this paper explores the latest happiness trends. The results confirm earlier findings of urban malaise: Americans in general are happiest in smaller cities and rural areas. However, the advantage of rural living is declining – rural Americans are becoming less happy relative to urbanites. Most interestingly, the results show that the latest generation, termed ‘Millennials’ (1982–2004), as opposed to earlier generations, are the happiest in large cities (an estimated magnitude larger than earning an additional US$100,000 in family income annually). The possible reasons for this trend are explored and directions for future research are discussed.
Is empty spacetime a physical thing?
Creators: name: Meschini, Diego
name: Lehto, Markku
Publisher: name: arXiv
Year: 2005
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: This article deals with empty spacetime and the question of its physical reality. By "empty spacetime" we mean a collection of bare spacetime points, the remains of ridding spacetime of all matter and fields. We ask whether these geometric objects--themselves intrinsic to the concept of field--might be observable through some physical test. By taking quantum-mechanical notions into account, we challenge the negative conclusion drawn from the diffeomorphism invariance postulate of general relativity, and we propose new foundational ideas regarding the possible observation--as well as conceptual overthrow--of this geometric ether.
description: 21 pages, Latex. v2: Section 5 expanded
Additional file 1 of Histone deacetylase 3 deletion in alveolar type 2 epithelial cells prevents bleomycin-induced pulmonary fibrosis
Creators: name: Xiong, Rui
name: Geng, Boxin
name: Jiang, Wenyang
name: Hu, Yong
name: Hu, Zhaoyu
name: Hao, Bo
name: Li, Ning
name: Geng, Qing
Publisher: name: figshare
Year: 2023
Subjects: subject: Biochemistry
subject: Medicine
subject: Cell Biology
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Pharmacology
subject: Biotechnology
subject: Chemical Sciences not elsewhere classified
subject: Immunology
subject: FOS: Clinical medicine
subject: Biological Sciences not elsewhere classified
subject: Marine Biology
subject: Cancer

description: Additional file 1. Fig S1. Distribution of HDAC3 in the nucleus and cytoplasm. Fig S2. Knockout effect of HDAC3 in mouse AT2 cells. Fig S3. Under the background of bleomycin-induced PF in mice. (A) The effect of RGFP966 on the acetylation of GTAT3 (B) and the expression of HDAC3, HDAC2, HDAC4, and SIRT3 proteins. Fig S4. Expression of HDAC3 in M2 macrophages in IPF. Fig S5. The relative mRNA expression of AQP5, AGER, and HOPX in HDAC3-C and HDAC3-CKO mice in the presence of saline or bleomycin for 21d. Fig S6. (A–B) Expression of fibrotic markers and EMT markers in positive and negative EpCAM-isolated cells respectively (C) HDAC3 and vimentin immunofluorescence colocalization staining in bleomycin-induced PF in mice. Fig S7. Bioinformatics and immunofluorescence staining analysis of HDAC3 expression in fibroblasts from patients with IPF vs healthy controls. Fig S8. Culture and identification of primary mouse AT2 cells.
Higgs-Inflaton Mixing and Vacuum Stability
Creators: name: Ema, Yohei
name: Karciauskas, Mindaugas
name: Lebedev, Oleg
name: Rusak, Stanislav
name: Zatta, Marco
Publisher: name: arXiv
Year: 2017
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: The quartic and trilinear Higgs field couplings to an additional real scalar are renormalizable, gauge and Lorentz invariant. Thus, on general grounds, one expects such couplings between the Higgs and an inflaton in quantum field theory. In particular, the (often omitted) trilinear coupling is motivated by the need for reheating the Universe after inflation, whereby the inflaton decays into the Standard Model (SM) particles. Such a coupling necessarily leads to the Higgs-inflaton mixing, which could stabilize the electroweak vacuum by increasing the Higgs self-coupling. We find that the inflationary constraints on the trilinear coupling are weak such that the Higgs-inflaton mixing up to order one is allowed, making it accessible to colliders. This entails an exciting possibility of a direct inflaton search at the LHC.
description: 12 pages, 2 figures
The MUSE Hubble Ultra Deep Field Survey VIII : Extended Lyman-alpha haloes around high-redshift star-forming galaxies
Creators: name: Leclercq, Floriane
name: Bacon, Roland
name: Wisotzki, Lutz
name: Mitchell, Peter
name: Garel, Thibault
name: Verhamme, Anne
name: Blaizot, Jérémy
name: Hashimoto, Takuya
name: Herenz, Edmund Christian
name: Conseil, Simon
name: Cantalupo, Sebastiano
name: Inami, Hanae
name: Contini, Thierry
name: Richard, Johan
name: Maseda, Michael
name: Schaye, Joop
name: Marino, Raffaella Anna
name: Akhlaghi, Mohammad
name: Brinchmann, Jarle
name: Carollo, Marcella
Publisher: name: arXiv
Year: 2017
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We report the detection of extended Lyman-alpha (Lya) haloes around 145 individual star-forming galaxies at redshifts 3 M_{UV}> -22) Lya emitters (LAEs). Using a 2D, two-component decomposition of Lya emission assuming circular exponential distributions, we measure scale lengths and luminosities of Lya haloes. We find that 80% of our objects having reliable Lya halo measurements show Lya emission that is significantly more extended than the UV continuum detected by HST (by a factor ~4 to >20). The median exponential scale length of the Lya haloes in our sample is ~4.5 kpc. By comparing the maximal detected extent of the Lya emission with the predicted dark matter halo virial radii of simulated galaxies, we show that the detected Lya emission of our selected sample of LAEs probes a significant portion of the cold circum-galactic medium (CGM) of these galaxies (>50% in average). This result shows that there must be significant HI reservoirs in the CGM and reinforces the idea that Lya haloes are ubiquitous around high-redshift Lya emitting galaxies. Our characterization of the Lya haloes indicates that the majority of the Lya flux comes from the halo (~65%) and that their scale lengths seem to be linked to the UV properties of the galaxies. We do not observe a significant Lya halo size evolution with redshift. We also find that the Lya lines cover a large range of full width at half maximum (FWHM) from 118 to 512 km/s. While the FWHM does not seem to be correlated to the Lya scale length, most compact Lya haloes and those that are not detected with high significance tend to have narrower Lya profiles. Finally, we investigate the origin of the extended Lya emission but we conclude that our data do not allow us to disentangle the possible processes.
description: 24 pages, 18 figures, 1 table, accepted for publication in A&A
Factors affecting the adsorption of gaseous environmental odors by activated carbon: A critical review
Creators: name: Le-Minh, Nhat
name: Sivret, Eric C.
name: Shammay, Ari
name: Stuetz, Richard M.
Publisher: name: Taylor & Francis
Year: 2018
Subjects: subject: Space Science
subject: 59999 Environmental Sciences not elsewhere classified
subject: FOS: Earth and related environmental sciences
subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences
subject: Ecology
subject: FOS: Biological sciences
subject: Sociology
subject: FOS: Sociology
subject: 69999 Biological Sciences not elsewhere classified
subject: Science Policy

description: Activated carbon has a long history of application to abate gaseous environmental odors; however, design and operating decisions are primarily based on empirical relations and pilot testing, with limited use of fundamental mechanistic knowledge. To support improved abatement outcomes, environmental odorant adsorption was reviewed. While influenced by a range of adsorbate and adsorbent properties and process operating conditions, information about their impacts is often limited or unavailable. Current research has focused on volatile sulfur compounds, with lesser focus on volatile organic compounds and volatile nitrogen compounds. Even within volatile sulfur compounds, most work has focused on hydrogen sulfide and the full range of reduced sulfur compounds (important environmental odorants) remain to be studied. The current narrow window of knowledge does not reflect the complexity of environmental odorants and is limiting development and systematic application of this technology. It has been demonstrated that single component adsorbent characterization does not reflect the adsorption of the complex mixture of odorants and non-odorous compounds that make up environmental odor emissions. Studies to explore adsorption competition in multi-compound systems and develop methods/guidance to account for this in abatement system selection and design are required to achieve cost effective and reliable outcomes.
State-dependent interactions in ultracold $^{174}$Yb probed by optical clock spectroscopy
Creators: name: Franchi, L.
name: Livi, L. F.
name: Cappellini, G.
name: Binella, G.
name: Inguscio, M.
name: Catani, J.
name: Fallani, L.
Publisher: name: arXiv
Year: 2017
Subjects: subject: Quantum Gases (cond-mat.quant-gas)
subject: Atomic Physics (physics.atom-ph)
subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: We report on the measurement of the scattering properties of ultracold $^{174}$Yb bosons in a three-dimensional (3D) optical lattice. Site occupancy in an atomic Mott insulator is resolved with high-precision spectroscopy on an ultranarrow optical clock transition. Scattering lengths and loss rate coefficients for $^{174}$Yb atoms in different collisional channels involving the ground state $^1$S$_0$ and the metastable $^3$P$_0$ are derived. These studies set important constraints for future experimental studies of two-electron atoms for quantum-technological applications.
description: 14 pages, 6 figures
Relativistic Aharonov-Casher Phase in Spin One
Creators: name: Swansson, James A
name: McKellar, Bruce H J
Publisher: name: arXiv
Year: 2000
Subjects: subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: The Aharonov-Casher (AC) phase is calculated in relativistic wave equations of spin one. The AC phase has previously been calculated from the Dirac-Pauli equation using a gauge-like technique \cite{MK1,MK2}. In the spin-one case, we use Kemmer theory (a Dirac-like particle theory) to calculate the phase in a similar manner. However the vector formalism, the Proca theory, is more widely known and used. In the presence of an electromagnetic field, the two theories are `equivalent' and may be transformed into one another. We adapt these transformations to show that the Kemmer theory results apply to the Proca theory. Then we calculate the Aharonov-Casher phase for spin-one particles directly in the Proca formalism.
description: 12 pages
Modeling the Infrared Emission from the HD 141569A Disk
Creators: name: Li, Aigen
name: Lunine, J. I.
Publisher: name: arXiv
Year: 2003
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We model the infrared (IR) emission from the double-ring disk of HD 141569A, using a porous dust model that was previously shown successful in reproducing the spectral energy distributions (SEDs) of the disks around $β$ Pictoris and HR 4796A. The dust consists of either unaltered or highly processed interstellar materials and vacuum with a volume fraction of ~90%. Together with a population of polycyclic aromatic hydrocarbon (PAH) molecules of which a large fraction is charged, the porous dust model made of coagulated but otherwise unaltered protostellar interstellar grains provides an excellent fit to the entire SED from the mid-IR to millimeter wavelengths including the PAH mid-IR emission features. The nondetection of the 21 micron crystalline silicate feature predicted from the porous dust model composed of highly-processed grains (mainly crystalline silicate dust) imposes an upper limit of ~10% on the mass fraction of crystalline silicates. Spectroscopic and broadband photometric predictions are made for SIRTF observations which will provide further tests of the applicability of the porous dust model to circumstellar disks.
description: published in The Astrophysical Journal, vol. 594, pp. 987--1010; 46 pages; 12 figures
Additional file 1: of Cytomegalovirus infection and outcome in immunocompetent patients in the intensive care unit: a systematic review and meta-analysis
Creators: name: Li, Xi
name: Huang, Yongbo
name: Xu, Zhiheng
name: Zhang, Rong
name: Liu, Xiaoqing
name: Li, Yimin
name: Mao, Pu
Publisher: name: figshare
Year: 2018
Subjects: subject: Space Science
subject: Medicine
subject: Science Policy
subject: Infectious Diseases
subject: FOS: Health sciences

description: Table S1. The Newcastleâ Ottawa scale (PDF 17Â kb)
Rigorous steps towards holography in asymptotically flat spacetimes
Creators: name: Dappiaggi, C.
name: Moretti, V.
name: Pinamonti, N.
Publisher: name: arXiv
Year: 2005
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: High Energy Physics - Theory (hep-th)
subject: Mathematical Physics (math-ph)
subject: FOS: Physical sciences

description: Scalar QFT on the boundary $\Im^+$ at null infinity of a general asymptotically flat 4D spacetime is constructed using the algebraic approach based on Weyl algebra associated to a BMS-invariant symplectic form. The constructed theory is invariant under a suitable unitary representation of the BMS group with manifest meaning when the fields are interpreted as suitable extensions to $\Im^+$ of massless minimally coupled fields propagating in the bulk. The analysis of the found unitary BMS representation proves that such a field on $\Im^+$ coincides with the natural wave function constructed out of the unitary BMS irreducible representation induced from the little group $Δ$, the semidirect product between SO(2) and the two dimensional translational group. The result proposes a natural criterion to solve the long standing problem of the topology of BMS group. Indeed the found natural correspondence of quantum field theories holds only if the BMS group is equipped with the nuclear topology rejecting instead the Hilbert one. Eventually some theorems towards a holographic description on $\Im^+$ of QFT in the bulk are established at level of $C^*$ algebras of fields for strongly asymptotically predictable spacetimes. It is proved that preservation of a certain symplectic form implies the existence of an injective $*$-homomorphism from the Weyl algebra of fields of the bulk into that associated with the boundary $\Im^+$. Those results are, in particular, applied to 4D Minkowski spacetime where a nice interplay between Poincaré invariance in the bulk and BMS invariance on the boundary at $\Im^+$ is established at level of QFT. It arises that the $*$-homomorphism admits unitary implementation and Minkowski vacuum is mapped into the BMS invariant vacuum on $\Im^+$.
description: 62 pages, amslatex, xy package; revised section 2 and the conclusions; corrected some typos; added some references; accepted for pubblication on Rev. Math. Phys
title: 03_0587
Creators: name: Wesley Baldwin, John
name: Baldwin, John W.
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2018
Subjects: subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris

description: L'ensemble de ces notes ont été crée par John Baldwin lors d'une de ses premières périodes de résidence à Paris. Ces documents comprennent tous les magistri qu’il avait pu rencontrer dans ses sources. Aux XIIème et XIIIème siècles, les universités n'existant pas encore, le titre de magister s'il évoque certainement une compétence n'est pas rattaché de façon systématique au passage par les écoles. De surcroît, les magistris sont le plus souvent désignés par leur seul prénom. La lecture de ces données est donc difficile et suppose un long travail pour tenter d'identifier un individu auquel on pourrait rattacher plusieurs mentions. John Baldwin avait donc renoncé à utiliser ces données pour donner un prolongement à sa magnifique étude sur les gradués d'université et leur emploi par les Capétiens et les Plantagenêts. Néanmoins, il a conservé ces données et elles sont potentiellement très utile dans le cadre de Studium, comme le sont toutes les mentions dans les volumes des Fasti Ecclesiae Gallicanae de chanoines portant ce titre de magister sans autres précisions. L'ampleur des dépouillements rend ces données très utiles et nous devons une grande reconnaissance à John Baldwin pour avoir pris la peine de faire photocopier ses fiches et de nous les avoir transmises amicalement.
Les données ainsi que les images des fiches sont accessibles sur le site Internet à l'adresse suivante : http://studium-baldwin.lamop.fr/.
Les transcriptions des fiches ont été effectuées par des étudiants de Paris 1 Panthéon - Sorbonne mais elles n'ont pas été corrigées par la suite.
description: Relation: https://lamop.hypotheses.org/
Microscopic theory for electron hydrodynamics in monolayer and bilayer graphene
Creators: name: Ho, Derek Y. H.
name: Yudhistira, Indra
name: Chakraborty, Nilotpal
name: Adam, Shaffique
Publisher: name: arXiv
Year: 2017
Subjects: subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: FOS: Physical sciences

description: Electrons behave like a classical fluid with a momentum distribution function that varies slowly in space and time when the quantum mechanical carrier-carrier scattering dominates over all other scattering processes. Recent experiments in monolayer and bilayer graphene have reported signatures of such hydrodynamic electron behavior in ultra-clean devices. In this theoretical work, starting from a microscopic treatment of electron-electron, electron-phonon and electron-impurity interactions within the Random Phase Approximation, we demonstrate that monolayer and bilayer graphene both host two different hydrodynamic regimes. We predict that the hydrodynamic window in bilayer graphene is stronger than in monolayer graphene, and has a characteristic `v-shape' as opposed to a `lung-shape'. Finally, we collapse experimental data onto a universal disorder-limited theory, thereby proving that the observed violation of Wiedemann-Franz law in monolayers occurs in a regime dominated by impurity-induced electron-hole puddles.
description: 6 pages, 4 figures
title: ADCO, Cartulaire de Cîteaux pour les possessions de Chaugey et Maison-Dieu (Fin XVe siècle), Cart. 180 (11 H 755), 83 folios, f. 0046
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
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2020
Subjects: subject: Corpus Burgundiae Medii Aevi
subject: Chartes de la Bourgogne du Moyen Âge
subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris
subject: cartulaire

description: Cartulaire de Cîteaux pour les possessions de Chaugey et Maison-Dieu (Fin XVe siècle), Archives départementales de la Côte-d'Or, Cart. 180 (11 H 755), 83 folios, f. 0046, Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Cartulaire de Cîteaux pour les possessions de Chaugey et Maison-Dieu (Fin XVe siècle), Archives départementales de la Côte-d'Or, Cart. 180 (11 H 755), 83 folios, f. 0046, 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
SSHOC D1.1 Project Management Plan
Creators: name: Spahic, Amir
name: Versic, Ivana Ilijasic
name: Jong, Franciska De
name: Eijk, Cees Van Der
Publisher: name: Zenodo
Year: 2019
Subjects: SSHOC
Social Sciences and Humanities Open Cloud
European Open Science Cloud
EOSC
Interoperability
metadata interoperability
data interoperability
FAIR principles
metadata standards

description: This document is the deliverable “D1.1 – Project Management Plan” of the Horizon2020 project “Social Sciences & Humanities Open Cloud” (hereinafter also referred to as “SSHOC”, project reference: 823782). The SSHOC Project Management Plan is the central document describing major aspects of the project management process. It is intended to provide guidance and direction for specific management, planning, and control activities such as scheduling, reporting, communication, quality, etc. The focus of this document is to describe the approaches being taken in the project to manage the various work packages, share and store documents, communicate among consortium members, control the quality of project deliverables, and provide links to other important procedures i.e. related to governance, described in Grant Agreement and/or Consortium Agreement. The Project Management Plan is a living document and should be updated continuously throughout the project. Benefits of creating a Project Management Plan include: clearly define roles, responsibilities, processes and activities; increase probability that projects will be completed on-time, within budget, and with a high degree of quality; ensuring understanding of what was agreed upon; helping project teams identify and plan for how project activities will be managed (budget, quality, schedule, etc.). The intended audience of the SSHOC Project Management Plan consists of members of the SSHOC consortium and the Project Officer at the controlling and granting side.
description: This deliverable has been accepted by the European Commission on 18 November 2019
description: {"references": ["SSHOC Grant Agreement", "SSHOC Consortium Agreement", "SSHOC Overall Communication and Outreach Plan (D2.1)", "H2020 Online Manual http://ec.europa.eu/research/participants/docs/h2020-funding-guide/grants/grant- management_en.htm"]}
Figure S1 from Logical modelling uncovers developmental constraints for primary sex determination of chicken gonads
Creators: name: Sánchez, Lucas
name: Chaouiya, Claudine
Publisher: name: The Royal Society
Year: 2018
Subjects: subject: 60114 Systems Biology
subject: FOS: Biological sciences
subject: Computational Biology
subject: 10202 Biological Mathematics
subject: FOS: Mathematics

description: Gene regulatory network controlling chicken primary sex determination. Normal green (resp. blunt red) arrows represent positive (resp. negative) interactions, and dashed arrows indicate indirect or proposed interactions. Z1 and Z2 represent each a Z chromosome, whereas W denotes a W chromosome; sex chromosome constitution (ZW or ZZ) is thus specified by an adequate combination of these input nodes.
Intent-Aware Contextual Recommendation System
Creators: name: Bhattacharya, Biswarup
name: Burhanuddin, Iftikhar
name: Sancheti, Abhilasha
name: Satya, Kushal
Publisher: name: arXiv
Year: 2017
Subjects: subject: Information Retrieval (cs.IR)
subject: Artificial Intelligence (cs.AI)
subject: Machine Learning (cs.LG)
subject: Machine Learning (stat.ML)
subject: FOS: Computer and information sciences

description: Recommender systems take inputs from user history, use an internal ranking algorithm to generate results and possibly optimize this ranking based on feedback. However, often the recommender system is unaware of the actual intent of the user and simply provides recommendations dynamically without properly understanding the thought process of the user. An intelligent recommender system is not only useful for the user but also for businesses which want to learn the tendencies of their users. Finding out tendencies or intents of a user is a difficult problem to solve. Keeping this in mind, we sought out to create an intelligent system which will keep track of the user's activity on a web-application as well as determine the intent of the user in each session. We devised a way to encode the user's activity through the sessions. Then, we have represented the information seen by the user in a high dimensional format which is reduced to lower dimensions using tensor factorization techniques. The aspect of intent awareness (or scoring) is dealt with at this stage. Finally, combining the user activity data with the contextual information gives the recommendation score. The final recommendations are then ranked using filtering and collaborative recommendation techniques to show the top-k recommendations to the user. A provision for feedback is also envisioned in the current system which informs the model to update the various weights in the recommender system. Our overall model aims to combine both frequency-based and context-based recommendation systems and quantify the intent of a user to provide better recommendations. We ran experiments on real-world timestamped user activity data, in the setting of recommending reports to the users of a business analytics tool and the results are better than the baselines. We also tuned certain aspects of our model to arrive at optimized results.
description: Presented at the 5th International Workshop on Data Science and Big Data Analytics (DSBDA), 17th IEEE International Conference on Data Mining (ICDM) 2017; 8 pages; 4 figures; Due to the limitation "The abstract field cannot be longer than 1,920 characters," the abstract appearing here is slightly shorter than the one in the PDF file
Additional file 9: of Effects of vitamin D supplementation on the outcomes of patients with pulmonary tuberculosis: a systematic review and meta-analysis
Creators: name: Wu, Hong-xia
name: Xiong, Xiao-feng
name: Zhu, Min
name: Wei, Jia
name: Zhuo, Kai-quan
name: Cheng, De-yun
Publisher: name: figshare
Year: 2018
Subjects: subject: Medicine
subject: Science Policy
subject: Infectious Diseases
subject: FOS: Health sciences

description: Figure S9. Change of hemoglobin count after vitamin D supplementation. CI, confidence interval; SD, standard derivation; IV, Inverse Variance. (PDF 195 kb)
ESM (methods and additional results) from In ovo yolk carotenoid and testosterone levels interactively influence female transfer of yolk antioxidants to her eggs
Creators: name: Giraudeau, Mathieu
name: Ann-Kathrin Ziegler
name: Mcgraw, Kevin
name: Okuliarová, Monika
name: Zeman, Michal
name: Tschirren, Barbara
Publisher: name: The Royal Society
Year: 2018
Subjects: Developmental Biology

description: ESM
Investigating the diversity of supernovae type Iax: A MUSE and NOT spectroscopic study of their environments
Creators: name: Lyman, J. D.
name: Taddia, F.
name: Stritzinger, M. D.
name: Galbany, L.
name: Leloudas, G.
name: Anderson, J. P.
name: Eldridge, J. J.
name: James, P. A.
name: Krühler, T.
name: Levan, A. J.
name: Pignata, G.
name: Stanway, E. R.
Publisher: name: arXiv
Year: 2017
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: SN 2002cx-like Type Ia supernovae (also known as SNe Iax) represent one of the most numerous peculiar SN classes. They differ from normal SNe Ia by having fainter peak magnitudes, faster decline rates and lower photospheric velocities, displaying a wide diversity in these properties. We present both integral-field and long-slit visual-wavelength spectroscopy of the host galaxies and explosion sites of SNe Iax to provide constraints on their progenitor formation scenarios. The SN Iax explosion site metallicity distribution is similar to that of core-collapse (CC) SNe and metal-poor compared to normal SNe Ia. Fainter members, speculated to form distinctly from brighter SN Iax, are found at a range of metallicities, extending to very metal-poor environments. Although the SN Iax explosion sites' ages and star-formation rates are comparatively older and less intense than the distribution of star forming regions across their host galaxies, we confirm the presence of young stellar populations (SP) at explosion environments for most SNe Iax, expanded here to a larger sample. Ages of the young SP (several $\times 10^{7}$ to $10^8$~yrs) are consistent with predictions for young thermonuclear and electron-capture SN progenitors. The lack of extremely young SP at the explosion sites disfavours very massive progenitors such as Wolf-Rayet explosions with significant fall-back. We find weak ionised gas in the only SN Iax host without obvious signs of star-formation. The source of the ionisation remains ambiguous but appears unlikely to be mainly due to young, massive stars.
description: Submitted to MNRAS
Modeling the Infrared Emission from the HR 4796A Disk
Creators: name: Li, Aigen
name: Lunine, J. I.
Publisher: name: arXiv
Year: 2003
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We model the spectral energy distribution (SED) from the mid-infrared to submillimeter of the ring-like disk of HR 4796A, the dustiest A-type star. We consider dust made either of coagulated but otherwise unaltered protostellar interstellar grains, or grains that are highly-processed in a protostellar/protoplanetary nebula with silicate dust annealed and carbon dust oxidized. Both types of dust are successful in reproducing the observed SED, provided that the grains are highly fluffy, with a vacuum volume fraction of \~90%. We find no evidence for the existence of a hot ``zodiacal dust'' component a few AU from the star, which was suggested by previous workers to account for the 10 micron-wavelength emission.
description: published in The Astrophysical Journal, vol. 590, pp. 368--378; 26 pages; 9 figures