cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Optical Counterparts to Galaxies in the Cen A Group Discovered by HIPASS
Creators: name: Knezek, Patricia M.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We have completed a 21-cm survey of a 600 square degree region of the Centaurus A group of galaxies at a redshift of ~500 km/s as part of a larger survey of the entire southern sky. This group of galaxies was recently the subject of a separate and thorough optical survey (Cote et al. 1997), and thus presented an ideal comparison for us to test the survey performance. We have identified 10 new group members to add to the 21 already known in our survey area. Six of the new members are previously uncatalogued galaxies, while four were catalogued but assumed not to be group members. Including the 7 known members outside of our survey area, this brings the total known number of Cen A members to 38. All of the new HI detections have optical counterparts, most being intrinsically very faint (M(B) > -13.0), late-type low surface brightness dwarfs. Most of the new members have HI masses only a few times our survey limit of 10(7) M(solar) at an assumed distance for the group of 3.5 Mpc, and are extremely gas-rich, with a median M(HI)/L(B) > 1. Our limiting HI sensitivity was actually slightly worse than the HI follow-up observations of the Cote et al. optical survey, yet we have already increased the known number of group members by 50% using an HI survey technique. While we have increased the known NUMBER of members by ~50%, these new members contribute < 4% to its light.
description: 8 pages, including 4 eps figures, to be published in PASA, vol. 16, in press
Additional file 1: of Enhancement of Glen Moy x Latham raspberry linkage map using GbS to further understand control of developmental processes leading to fruit ripening
Creators: name: Hackett, Christine
name: Milne, Linda
name: Smith, Kay
name: Hedley, Pete
name: Morris, Jenny
name: Simpson, Craig
name: Preedy, Katharine
name: Graham, Julie
Publisher: name: figshare
Year: 2018
Subjects: subject: Biochemistry
subject: Space Science
subject: Medicine
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Neuroscience
subject: 59999 Environmental Sciences not elsewhere classified
subject: FOS: Earth and related environmental sciences
subject: Ecology
subject: Sociology
subject: FOS: Sociology
subject: 69999 Biological Sciences not elsewhere classified
subject: 80699 Information Systems not elsewhere classified
subject: FOS: Computer and information sciences
subject: Developmental Biology
subject: 110309 Infectious Diseases
subject: FOS: Health sciences
subject: Computational Biology

description: Appendix A. Workflow for the linkage mapping procedure. (DOCX 15Â kb)
$\boldsymbol{\mathcalα}$ decay properties of $\boldsymbol{^{296}}$Og within the two-potential approach
Creators: name: Deng, Jun-Gang
name: Zhao, Jie-Cheng
name: Chen, Jiu-Long
name: Wu, Xi-Jun
name: Li, Xiao-Hua
Publisher: name: arXiv
Year: 2018
Subjects: subject: Nuclear Theory (nucl-th)
subject: Nuclear Experiment (nucl-ex)
subject: FOS: Physical sciences

description: The present work is a continuations of our previous paper [J.-G. Deng, et al., Chin. Phys. C, {\bf41}: 124109 (2017)]. In present work, the $\mathcalα$ decay half-life of unknown nucleus $^{296}$Og is predicted within the two-potential approach and the hindrance factors of all 20 even-even nuclei in the same region with $^{296}$Og, i.e. proton number $82
description: 2 figures, 2 tables. arXiv admin note: text overlap with arXiv:1710.03008
Multi-variate correlation and mixtures of product measures
Creators: name: Austin, Tim
Publisher: name: arXiv
Year: 2018
Subjects: subject: Probability (math.PR)
subject: Information Theory (cs.IT)
subject: Statistics Theory (math.ST)
subject: FOS: Mathematics
subject: FOS: Computer and information sciences
subject: 60B99 (primary), 60G99, 62B10, 94A17

description: Total correlation (`TC') and dual total correlation (`DTC') are two classical ways to quantify the correlation among an $n$-tuple of random variables. They both reduce to mutual information when $n=2$. The first part of this paper sets up the theory of TC and DTC for general random variables, not necessarily finite-valued. This generality has not been exposed in the literature before. The second part considers the structural implications when a joint distribution $μ$ has small TC or DTC. If $\mathrm{TC}(μ) = o(n)$, then $μ$ is close to a product measure according to a suitable transportation metric: this follows directly from Marton's classical transportation-entropy inequality. If $\mathrm{DTC}(μ) = o(n)$, then the structural consequence is more complicated: $μ$ is a mixture of a controlled number of terms, most of them close to product measures in the transportation metric. This is the main new result of the paper.
description: 39 pages [v2:] Slight changes in presentation based on feedback from colleagues [v3, v4:] Small revisions during preparation for journal
Nonlinear Schrodinger equation and classical-field description of the Lamb-Retherford experiment
Creators: name: Rashkovskiy, Sergey A.
Publisher: name: arXiv
Year: 2018
Subjects: subject: General Physics (physics.gen-ph)
subject: FOS: Physical sciences
subject: 81P10, 81Q05, 81V45

description: I show that Lamb-Retherford experiment can be fully described within the framework of classical field theory without using concepts such as the discrete states of the atom and jump-like electron transitions between them. The rate of stimulated decay of the metastable state of a hydrogen atom in an external periodic electric field is determined. The dependence of this rate on the frequency and amplitude of the external electric field, as well as on the parameters of the atom, has been obtained. It is shown that the maximum value of the stimulated decay rate of the metastable state of a hydrogen atom is achieved at an external electric field frequency equal to the frequency shift corresponding to either the fine structure of the hydrogen atom or the Lamb shift.
description: 25 pages, 2 figures
Quenching of the radio jet during the X-ray high state of GX 339-4
Creators: name: Fender, Robert
name: Corbel, Stephane
name: Tzioumis, Tasso
name: McIntyre, Vince
name: Campbell-Wilson, Duncan
name: Nowak, Mike
name: Sood, Ravi
name: Hunstead, Richard
name: Harmon, Alan
name: Durouchoux, Philippe
name: Heindl, William
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We have observed the black hole candidate X-ray binary GX 339-4 at radio wavelengths before, during and after the 1998 high/soft X-ray state transition. We find that the radio emission from the system is strongly correlated with the hard X-ray emission and is reduced by a factor > 25 during the high/soft state compared to the more usual low/hard state. At the points of state transition we note brief periods of unusually optically-thin radio emission which may correspond to discrete ejection events. We propose that in the low/hard state black hole X-ray binaries produce a quasi-continuous outflow, in the high/soft state this outflow is suppressed, and that state transitions often result in one or more discrete ejection events. Future models for low/hard states, such as ADAF/ADIOS solutions, need to take into account strong outflow of relativistic electrons from the system. We propose that the inferred Comptonising corona and the base of the jet-like outflow are the same thing, based upon the strong correlation between radio and hard X-ray emission in GX 339-4 and other X-ray binaries, and the similarity in inferred location and composition of these two components.
description: Accepted for publication in ApJ Letters
Cancer cancharus Linnaeus, 1758, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1758
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Malacostraca
Decapoda
Cancridae
Cancer
Cancer cancharus

description: Cancer cancharus [spec. nov.]
C. macrourus, thorace rugoso ovali, manibus compressis margine spinosis. M. L. U.
Habitat in Indiis.
* i * Macrouri thorace aculeato.
description: Published as part of Linnaeus, Carolus, 1758, Systema Naturae per regna tria naturae: secundum classes, ordines, genera, species, cum characteribus, differentiis, synonymis, locis, Stockholm :Laurentius Salvius on page 632, DOI: 10.5962/bhl.title.542, http://zenodo.org/record/3922206
Additional file 5 of Developing guideline-based key performance indicators for recurrent miscarriage care: lessons from a multi-stage consensus process with a diverse stakeholder group
Creators: name: Hennessy, Marita
name: Linehan, Laura
name: Dennehy, Rebecca
name: Devane, Declan
name: Rice, Rachel
name: Meaney, Sarah
name: O’Donoghue, Keelin
Publisher: name: figshare
Year: 2022
Subjects: subject: Medicine
subject: Genetics
subject: FOS: Biological sciences
subject: Environmental Sciences not elsewhere classified
subject: Biological Sciences not elsewhere classified
subject: Developmental Biology
subject: Cancer
subject: Science Policy
subject: Infectious Diseases
subject: FOS: Health sciences

description: Additional file 5. Sample item, Final survey.
Hypergraph expanders of all uniformities from Cayley graphs
Creators: name: Conlon, David
name: Tidor, Jonathan
name: Zhao, Yufei
Publisher: name: arXiv
Year: 2018
Subjects: subject: Combinatorics (math.CO)
subject: FOS: Mathematics
subject: 05C65, 05C81

description: Hypergraph expanders are hypergraphs with surprising, non-intuitive expansion properties. In a recent paper, the first author gave a simple construction, which can be randomized, of $3$-uniform hypergraph expanders with polylogarithmic degree. We generalize this construction, giving a simple construction of $r$-uniform hypergraph expanders for all $r \geq 3$.
description: 32 pages
Cosmic Rays, Radio Halos and Non-Thermal X-ray Emission in Clusters of Galaxies
Creators: name: Blasi, P.
name: Colafrancesco, S.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We calculate the flux of radio, hard X-ray and UV radiation from clusters of galaxies as produced by synchrotron emission and Inverse Compton Scattering of electrons generated as secondaries in cosmic ray interactions in the intracluster medium. Both the spatial distribution of cosmic rays due to their diffusion and the spatial distribution of the intracluster gas are taken into account. Our calculations are specifically applied to the case of the Coma cluster. The fluxes and spectra of the radio halo emission and of the hard X-ray excess from Coma can be explained in this model if an average magnetic field $B \sim 0.1μG$ is assumed. However, such a low value for the intracluster magnetic field implies a large cosmic ray energy density which in turn is responsible, through neutral pion decay, for a gamma ray flux above 100 MeV which exceeds the EGRET upper limit. This gamma ray bound can be relaxed if the hard X-ray excess and the radio halo emission from Coma are not due to the same population of electrons. We finally stress the unique role that the new generation gamma ray satellites will play to discriminate among different models for the non thermal emission in clusters of galaxies.
description: 25 pages, 3 Figures, Latex (using epsfig,elsart), to appear in Astroparticle Physics. Astroparticle Physics, in press
Statistical-mechanical analysis of compressed sensing for Hamiltonian estimation of Ising spin glass
Creators: name: Takahashi, Chako
name: Ohzeki, Masayuki
name: Okada, Shuntaro
name: Terabe, Masayoshi
name: Taguchi, Shinichiro
name: Tanaka, Kazuyuki
Publisher: name: arXiv
Year: 2018
Subjects: subject: Statistical Mechanics (cond-mat.stat-mech)
subject: FOS: Physical sciences

description: Several powerful machines, such as the D-Wave 2000Q, dedicated to solving combinatorial optimization problems through the Ising-model formulation have been developed. To input problems into the machines, the unknown parameters on the Ising model must be determined, and this is necessarily a nontrivial task. It could be beneficial to construct a method to estimate the parameters of the Ising model from several pairs of values of the energy and spin configurations. In the present paper, we propose a simple method employing the $L_1$-norm minimization, which is based on the concept of the compressed sensing. Moreover, we analyze the typical performance of our proposed method of the Hamiltonian estimation by using the replica method. We also compare our analytical results through several numerical experiments using the alternating direction method of multipliers.
description: 8 pages, 2 figures
Additional file 1: of Surgical treatment of children with total colonic aganglionosis: functional and metabolic long-term outcome
Creators: name: Urla, Cristian
name: Lieber, Justus
name: Obermayr, Florian
name: Busch, Andreas
name: Schweizer, Roland
name: Warmann, Steven
name: Hans-Joachim Kirschner
name: Jรถrg Fuchs
Publisher: name: figshare
Year: 2018
Subjects: subject: Space Science
subject: Medicine
subject: Physiology
subject: FOS: Biological sciences
subject: Biotechnology
subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences
subject: Cancer
subject: 110309 Infectious Diseases
subject: FOS: Health sciences

description: Classification of surgical complications after Dindo and Clavien. Ranking system proposed by Dindo and Clavien [15] for classification of postoperative complications. (DOCX 12 kb)
The Gaia-WISE Extragalactic Astrometric Catalog
Creators: name: Paine, Jennie
name: Darling, Jeremy
name: Truebenbach, Alexandra
Publisher: name: arXiv
Year: 2018
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: The Gaia mission has detected a large number of active galactic nuclei (AGN) and galaxies, but these objects must be identified among the 1000-fold more numerous stars. Extant astrometric AGN catalogs do not have the uniform sky coverage required to detect and characterize the all-sky low-multipole proper motion signals produced by the barycenter motion, gravitational waves, and cosmological effects. To remedy this, we present an all-sky sample of 567,721 AGN in Gaia Data Release 1, selected using WISE two-color criteria. The catalog has fairly uniform sky coverage beyond the Galactic plane, with a mean density of 12.8 AGN per square degree. The objects have magnitudes ranging from $G=8.8$ down to Gaia's magnitude limit, $G=20.7$. The catalog is approximately 50% complete but suffers from low stellar contamination, roughly 0.2%. We predict that the end-of-mission Gaia proper motions for this catalog will enable detection of the secular aberration drift to high significance (23$σ$) and will limit the anisotropy of the Hubble expansion to about 2%.
description: 11 pages, 7 figures; Submitted to ApJS
Lettre de Joseph Hilarius Eckhel à Jean-François Séguier, 1783-11-03
Creators: name: Eckhel, Joseph Hilarius
name: Eckhel, Joseph Hilarius
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2021

description: [transcription] Vienne ce 3 novembre 1783.

Monsieur !

J'ai reçu avec beaucoup de plaisir votre derniere avec celle de Mr de Puy Morin, que vous avez jointe. Je vous remercie infiniment de votre accuratesse et attention pour moi. Ce qui regarde mon ouvrage: Numi veteres anecdoti, dont vous desirez un exemplaire, j'y ai deja pensé, et concerté la maniere, de vous le faire parvenir. c'est le comte de Diesbach, qui s'est est chargé. Il se trouvera à Paris à la fin de novembre, et logera chez le comte d'Affry place Vendôme. Vous aurez donc la bonté, de charger quelqu'un de vos connoissances, pour le demander dudit comte Diesbach. Pour mieux l'engager, de ne pas manquer sa commission, je lui ai fait un présent d'un autre exemplaire du dit ouvrage. c'est pour vous informer dans l'affaire en question que je vous ecris la presente. Je vous prie, de me garder constamment votre precieux attachement, et je suis avec beaucoup de consideration

Monsieur

Votre très humble et très obéissant serviteur

L'abbé Eckhel

[annotation de Séguier : ecrit a Paris le 21 9bre 1783 a Mr l'Heritier]
description: [personnes citées] comte d' Affry, Comte de Diesbach, Nicolas Joseph Marcassus de Puymaurin
description: [reférence bibliographique citée] Eckhel, Joseph Hilarius, Numi veteres anecdoti, Vienne, J. Kurzböck, 1775.
description: Source: [lieu de Conservation] Nîmes, Bibliothèque Carré d'Art [cote]ms. 143_1, fol. 6
description: Source: ark:/12148/btv1b10015225h
Searching for non-gaussianity: Statistical tests
Creators: name: Forni, O.
name: Aghanim, N.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Non-gaussianity represents the statistical signature of physical processes such as turbulence. It can also be used as a powerful tool to discriminate between competing cosmological scenarios. A canonical analysis of non-gaussianity is based on the study of the distribution of the signal in the real (or direct) space (e.g. brightness, temperature). This work presents an image processing method in which we propose statistical tests to indicate and quantify the non-gaussian nature of a signal. Our method is based on a wavelet analysis of a signal. Because the temperature or brightness distribution is a rather weak discriminator, the search for the statistical signature of non-gaussianity relies on the study of the coefficient distribution of an image in the wavelet decomposition basis which is much more sensitive. We develop two statistical tests for non-gaussianity. In order to test their reliability, we apply them to sets of test maps representing a combination of gaussian and non-gaussian signals. We deliberately choose a signal with a weak non-gaussian signature and we find that such a non-gaussian signature is easily detected using our statistical discriminators. In a second paper, we apply the tests in a cosmological context.
description: 14 pages, 7 figures, in press in Astronomy & Astrophysics Supplement Series
No One is Perfect: Analysing the Performance of Question Answering Components over the DBpedia Knowledge Graph
Creators: name: Singh, Kuldeep
name: Lytra, Ioanna
name: Radhakrishna, Arun Sethupat
name: Shekarpour, Saeedeh
name: Vidal, Maria-Esther
name: Lehmann, Jens
Publisher: name: arXiv
Year: 2018
Subjects: subject: Information Retrieval (cs.IR)
subject: Computation and Language (cs.CL)
subject: FOS: Computer and information sciences

description: Question answering (QA) over knowledge graphs has gained significant momentum over the past five years due to the increasing availability of large knowledge graphs and the rising importance of question answering for user interaction. DBpedia has been the most prominently used knowledge graph in this setting and most approaches currently use a pipeline of processing steps connecting a sequence of components. In this article, we analyse and micro evaluate the behaviour of 29 available QA components for DBpedia knowledge graph that were released by the research community since 2010. As a result, we provide a perspective on collective failure cases, suggest characteristics of QA components that prevent them from performing better and provide future challenges and research directions for the field.
description: Evaluation of State of the art Question Answering components performing entity linking, relation linking etc
Search for slowly moving magnetic monopoles
Creators: name: Hong, J. T.
Publisher: name: arXiv
Year: 1994
Subjects: subject: High Energy Physics - Experiment (hep-ex)
subject: FOS: Physical sciences

description: We report a search for slowly moving magnetic monopoles in the cosmic radiation with the first supermodule of the MACRO detector at Gran Sasso. The absence of candidates established an upper limit on the monopole flux of $5.6\times10^{-15}\mbox{cm}^{-2}\mbox{sr}^{-1}\mbox{s}^{-1}$ at 90\% confidence level for the velocity range of $1.8\times10^{-4}
description: 3 pages including 2 figures, uuencoded gz-compressed PostScript file, Talk given at TAUP '93, published in Nucl. Phys. B (Proc. Suppl.) 35 (1994) 261-263
Advancing Sustainable Development through Multi-Use: Insights from the European OLAMUR & SEADOTs projects
Creators: name: Dankel, Dorothy
Publisher: name: Zenodo
Year: 2025

description: At SINTEF, we develop tools and insights for sustainable development of wind energy to create a successful export industry, reduce cost and uncertainty, and address and resolve environmental and societal conflicts.

How can we support biodiversity at the same time as we develop offshore wind farms and technology for a better society?And how can this work be seen together with climate and sustainability goals?
Cancer pilosus Linnaeus, 1758, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1758
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Malacostraca
Decapoda
Cancridae
Cancer
Cancer pilosus

description: Cancer pilosus [spec. nov.]
C. macrourus, thorace chelisque angulatis hispidis.
Mus. Ad. Fr. 87.
Habitat in Indiis.
description: Published as part of Linnaeus, Carolus, 1758, Systema Naturae per regna tria naturae: secundum classes, ordines, genera, species, cum characteribus, differentiis, synonymis, locis, Stockholm :Laurentius Salvius on page 632, DOI: 10.5962/bhl.title.542, http://zenodo.org/record/3922206
SARA: Self-Aware Resource Allocation for Heterogeneous MPSoCs
Creators: name: Song, Yang
name: Alavoine, Olivier
name: Lin, Bill
Publisher: name: arXiv
Year: 2018
Subjects: subject: Distributed, Parallel, and Cluster Computing (cs.DC)
subject: Hardware Architecture (cs.AR)
subject: FOS: Computer and information sciences

description: In modern heterogeneous MPSoCs, the management of shared memory resources is crucial in delivering end-to-end QoS. Previous frameworks have either focused on singular QoS targets or the allocation of partitionable resources among CPU applications at relatively slow timescales. However, heterogeneous MPSoCs typically require instant response from the memory system where most resources cannot be partitioned. Moreover, the health of different cores in a heterogeneous MPSoC is often measured by diverse performance objectives. In this work, we propose a Self-Aware Resource Allocation (SARA) framework for heterogeneous MPSoCs. Priority-based adaptation allows cores to use different target performance and self-monitor their own intrinsic health. In response, the system allocates non-partitionable resources based on priorities. The proposed framework meets a diverse range of QoS demands from heterogeneous cores.
description: Accepted by the 55th annual Design Automation Conference 2018 (DAC'18)
Finitely forcible graphons with an almost arbitrary structure
Creators: name: Kral, Daniel
name: Lovász, László Miklós
name: Noel, Jonathan A.
name: Sosnovec, Jakub
Publisher: name: arXiv
Year: 2018
Subjects: subject: Combinatorics (math.CO)
subject: FOS: Mathematics

description: Graphons are analytic objects representing convergent sequences of large graphs. A graphon is said to be finitely forcible if it is determined by finitely many subgraph densities, i.e., if the asymptotic structure of graphs represented by such a graphon depends only on finitely many density constraints. Such graphons appear in various scenarios, particularly in extremal combinatorics. Lovasz and Szegedy conjectured that all finitely forcible graphons possess a simple structure. This was disproved in a strong sense by Cooper, Kral and Martins, who showed that any graphon is a subgraphon of a finitely forcible graphon. We strenghten this result by showing for every $\varepsilon>0$ that any graphon spans a $1-\varepsilon$ proportion of a finitely forcible graphon.
X-ray Spectroscopy of the Nearby, Classical T Tauri Star TW Hya
Creators: name: Kastner, Joel H.
name: Huenemoerder, David P.
name: Schulz, Norbert S.
name: Weintraub, David A.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present ASCA and ROSAT X-ray observations of the classical T Tauri star TW Hya, the namesake of a small association that, at a distance of ~ 50 pc, represents the nearest known region of recent star formation. Analysis of ASCA and ROSAT spectra indicates characteristic temperatures of ~ 1.7 MK and ~ 9.7 MK for the X-ray emitting region(s) of TW Hya, with emission lines of highly ionized Fe dominating the spectrum at energies ~1 keV. The X-ray data show variations in X-ray flux on
Evidence for Hybrid Inorganic–Organic Transitions at the WS2/Terrylene Interface
Creators: name: Tanda Bonkano, Boubacar
name: Palato, Samuel
name: Krumland, Jannis
name: Kovalenko, Sergey
name: Schwendke, Philipp
name: Guerrini, Michele
name: Li, Qiuyang
name: Cocchi, Caterina
name: Stähler, Julia
Publisher: name: Humboldt-Universität zu Berlin
Year: 2023
Subjects: subject: hybrid inorganic/organic system
subject: transient absorption
subject: transition metal dichalcogenides
subject: 530 Physik

description: The realization of the potential of hybrid inorganic organic systems requires an understanding of the coupling between the constituents: its nature and its strength. The observation of hybrid optical transitions in the monolayer WS2/terrylene hybrid is reported. The first-principle calculations, linear optical, and transient absorption spectroscopy are employed to investigate the optical spectrum of the hybrid, which exhibits a new transition that does not appear in the constituents’ spectra. The calculations indicate type II level alignment, with the highest occupied level of terrylene in the gap of WS2. Exploiting state-resolved transient absorption, the response of the hybrid interface to optical excitation is selectively probed. The dynamics reveal rapid hole transfer from WS2 to the terrylene layer, with a decay time of 88 ps. This hole transfer induces a bleach of the hybrid transition, which indicates that terrylene contributes to its initial state. Based on this, the hybrid resonance energy, and on our calculations, we assign the hybrid feature to a transition from the highest occupied molecular orbital of terrylene to the conduction band of WS2 close to the Γ point. The results indicate that the conditions for strong electronic coupling are met in this hybrid system.
Answering Mermin's Challenge with Conservation per No Preferred Reference Frame
Creators: name: Stuckey, W. M.
name: McDevitt, Timothy
name: Silberstein, Michael
name: Le, T. D.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: In 1981, Mermin published a now famous paper titled, "Bringing home the atomic world: Quantum mysteries for anybody" that Feynman called, "One of the most beautiful papers in physics that I know." Therein, he presented the "Mermin device" that illustrates the conundrum of quantum entanglement per the Bell spin states for the "general reader." He then challenged the "physicist reader" to explain the way the device works "in terms meaningful to a general reader struggling with the dilemma raised by the device." Herein, we show how "conservation per no preferred reference frame (NPRF)" answers that challenge. In short, the explicit conservation that obtains for Alice and Bob's Stern-Gerlach spin measurement outcomes in the same reference frame holds only on average in different reference frames, not on a trial-by-trial basis. This conservation is SO(3) invariant in the relevant symmetry plane in real space per the SU(2) invariance of its corresponding Bell spin state in Hilbert space. Since NPRF is also responsible for the postulates of special relativity, and therefore its counterintuitive aspects of time dilation and length contraction, we see that the symmetry group relating non-relativistic quantum mechanics and special relativity via their "mysteries" is the restricted Lorentz group.
description: 18 pages, 9 figures. This version as revised and resubmitted to Scientific Reports
Python I, II, and III CMB Anisotropy Measurement Constraints on Open and Flat-Lambda CDM Cosmogonies
Creators: name: Rocha, Graca
name: Stompor, Radoslaw
name: Ganga, Ken
name: Ratra, Bharat
name: Platt, Stephen R.
name: Sugiyama, Naoshi
name: Gorski, Krzysztof M.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We use Python I, II, and III cosmic microwave background anisotropy data to constrain cosmogonies. We account for the Python beamwidth and calibration uncertainties. We consider open and spatially-flat-Lambda cold dark matter cosmogonies, with nonrelativistic-mass density parameter Omega_0 in the range 0.1--1, baryonic-mass density parameter Omega_B in the range (0.005--0.029) h^{-2}, and age of the universe t_0 in the range (10--20) Gyr. Marginalizing over all parameters but Omega_0, the combined Python data favors an open (spatially-flat-Lambda) model with Omega_0 simeq 0.2 (0.1). At the 2 sigma confidence level model normalizations deduced from the combined Python data are mostly consistent with those drawn from the DMR, UCSB South Pole 1994, ARGO, MAX 4 and 5, White Dish, and SuZIE data sets.
description: 20 pages, 7 figures, accepted by ApJ
Additional file 2: of Pay for performance program reduces treatment needed diabetic retinopathy - a nationwide matched cohort study in Taiwan
Creators: name: Shwu-Jiuan Sheu
name: Lin, Wen-Liang
name: Yea-Huei Kao Yang
name: Chi-Min Hwu
name: Ching-Lan Cheng
Publisher: name: figshare
Year: 2018
Subjects: subject: Medicine
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: Developmental Biology
subject: Science Policy

description: Table S2. Incidence of diabetic retinopathy in eye examination groups compared with no eye examination groups among non-P4P population (check detection bias) (DOCX 15 kb)
The augmentation of Knowledge Management through Industry 4.0: case of Aviation sector of emerging economy
Creators: name: Miao, Miao
name: Zaman, Syed Imran
name: Zafar, Arooba
name: Rodriguez, Cristian Garcia
name: Zaman, Syed Ahsan Ali
Publisher: name: Taylor & Francis
Year: 2022
Subjects: subject: Genetics
subject: FOS: Biological sciences
subject: Ecology
subject: Sociology
subject: FOS: Sociology
subject: Biological Sciences not elsewhere classified
subject: Science Policy
subject: Plant Biology

description: This research examines critical elements of knowledge management and industry 4.0 that assist human resources in the air transport industry. In addition, we look at the essential components that connect the divide between Industry 4.0 and knowledge management. This paper uses the Grey- DEMATEL technique to comprehend the cause-and-effect factors and their interrelationships. A seven-scale ranking, and sensitivity analysis was further applied for better results. It was observed from the findings that information sharing (F15) was the most significant factor for the aviation sector as the causal factor was ranked as the top criterion. Joint knowledge creation (F15) was ranked as the second topmost criteria as effect factor. E-learning (F9) is the third-ranking effect factor. This paper showed that information sharing assists in management performance and efficiency performance in the aviation sector.
Extrapolation of Galactic Dust Emission at 100 Microns to CMBR Frequencies Using FIRAS
Creators: name: Finkbeiner, Douglas P.
name: Davis, Marc
name: Schlegel, David J.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present predicted full-sky maps of submillimeter and microwave emission from the diffuse interstellar dust in the Galaxy. These maps are extrapolated from the 100 micron emission and 100/240 micron flux ratio maps that Schlegel, Finkbeiner, & Davis (1998; SFD98) generated from IRAS and COBE/DIRBE data. Results are presented for a number of physically plausible emissivity models. We find that no power law emissivity function fits the FIRAS data from 200 - 2100 GHz. In this paper we provide a formalism for a multi-component model for the dust emission. A two-component model with a mixture of silicate and carbon-dominated grains (motivated by Pollack et al., 1994}) provides a fit to an accuracy of about 15% to all the FIRAS data over the entire high-latitude sky. Small systematic differences are found between the atomic and molecular phases of the ISM. Our predictions for the thermal (vibrational) emission from Galactic dust at ν< 3000 GHz are available for general use. These full-sky predictions can be made at the DIRBE resolution of 40' or at the higher resolution of 6.1 arcmin from the SFD98 DIRBE-corrected IRAS maps.
description: 48 pages, AAS LaTeX, 6 figures, ApJ (accepted). Data described in the text, as well as 4 additional figures, are available at http://astro.berkeley.edu/dust
Additional file 1 of Co-deficiency of B7-H3 and B7-H4 identifies high CD8 + T cell infiltration and better prognosis in pancreatic cancer
Creators: name: Si, Shuping
name: Wang, Lei
name: Cao, Hui
name: Xu, Yuhua
name: Zhan, Qiang
Publisher: name: figshare
Year: 2022
Subjects: subject: Biochemistry
subject: Cell Biology
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Biotechnology
subject: Chemical Sciences not elsewhere classified
subject: Immunology
subject: FOS: Clinical medicine
subject: Biological Sciences not elsewhere classified
subject: Developmental Biology
subject: Cancer

description: Additional file 1: Figure S1. Expression levels of B7-H3 and B7-H4 PAAD tissues based on public data.
Additional file 1: of Pay for performance program reduces treatment needed diabetic retinopathy - a nationwide matched cohort study in Taiwan
Creators: name: Shwu-Jiuan Sheu
name: Lin, Wen-Liang
name: Yea-Huei Kao Yang
name: Chi-Min Hwu
name: Ching-Lan Cheng
Publisher: name: figshare
Year: 2018
Subjects: subject: Biochemistry
subject: Medicine
subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: Science Policy
subject: 110309 Infectious Diseases
subject: FOS: Health sciences

description: Table S1. Baseline characteristics of the cohort patients with type 2 diabetes using propensity score (DOCX 16 kb)
Finite Large Antenna Arrays for Massive MIMO: Characterization and System Impact
Creators: name: Chen, Cheng-Ming
name: Volski, Vladimir
name: Van der Perre, Liesbet
name: Vandenbosch, Guy A. E.
name: Pollin, Sofie
Publisher: name: arXiv
Year: 2018
Subjects: subject: Signal Processing (eess.SP)
subject: FOS: Electrical engineering, electronic engineering, information engineering

description: Massive MIMO is considered a key technology for 5G. Various studies analyze the impact of the number of antennas, relying on channel properties only and assuming uniform antenna gains in very large arrays. In this paper, we investigate the impact of mutual coupling and edge effects on the gain pattern variation in the array. Our analysis focuses on the comparison of patch antennas versus dipoles, representative for the antennas typically used in massive MIMO experiments today. Through simulations and measurements, we show that the finite patch array has a lower gain pattern variation compared with a dipole array. The impact of a large gain pattern variation on the massive MIMO system is that not all antennas contribute equally for all users, and the effective number of antennas seen for a single user is reduced. We show that the effect of this at system level is a decreased rate for all users for the zero-forcing MIMO detector, up to 20% for the patch array and 35% for the dipole array. The maximum ratio combining on the other hand, introduces user unfairness.
description: 9 pages, IEEE Transactions on Antennas and Propagation
Inter-Eclipse Spectroscopic Snapshot of Epsilon Aurigae with HST
Creators: name: Sheffer, Yaron
name: Lambert, David L.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: A single-epoch low resolution GHRS spectrum of the eclipsing binary Epsilon Aurigae was obtained while the secondary was orbiting towards eclipse by the primary. The detected emission line profiles have the appearance of double- peaked emission with a stronger red component at a radial velocity of +108 km/s, and a weaker blue emission bump at ca. -92 km/s. We compare these observational results with known orbital properties of the epsilon Aur binary system, and propose that the emission originates at the inner radius of the disk surrounding the enigmatic secondary. We interpret the kinematic data as a possible means to uncover the underlying stellar masses and we speculate about the binary's relationship to other "high-mass" models.
description: 27 pages, 4 (separate) figures, plain TeX (aasms4.sty)
Polarized Bhabha Scattering and a Precision Measurement of the Electron Neutral Current Couplings
Creators: name: The SLD Collaboration
Publisher: name: arXiv
Year: 1994
Subjects: subject: High Energy Physics - Experiment (hep-ex)
subject: FOS: Physical sciences

description: We present the first measurement of the left-right asymmetry in Bhabha scattering with a polarized electron beam. The effective electron vector and axial vector couplings to the Z0 are extracted from a combined analysis of the polarized Bhabha scattering data and the left-right asymmetry previously published by this collaboration.
description: PHYZZX, 17 pages, SLAC-PUB-6605
The power spectrum of the Lyman-alpha clouds
Creators: name: Amendola, Luca
name: Savaglio, Sandra
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We investigate the clustering properties of 13 QSO lines of sight in flat space, with average redshifts from z~2 to 4. We estimate the 1-D power spectrum and the integral density of neighbours, and discuss their variation with respect to redshift and column density. We compare the results with standard CDM models, and estimate the power spectrum of Lyman-alpha clustering as a function both of redshift and column density. We find that a) there is no significant periodicity or characteristic scale; b) the clustering depends both on column density and redshift; c) the clustering increases linearly only if at the same time the HI column density decreases strongly with redshift. The results remain qualitatively the same assuming an open cosmological model.
description: Accepted for publication in MNRAS
Cancer norvegicus Linnaeus, 1758, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1758
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Malacostraca
Decapoda
Cancridae
Cancer
Cancer norvegicus

description: Cancer norvegicus [spec. nov.]
C. macrourus, thorace antrorsum aculeato, manibus prismaticis: angulis spinosis. Fn. svec. 1247.
It. scanic. 307.
Mus. Ad. Fr. 1. p. 88.
Aldr. exsangu. 113. Astacus mediae magnitudinis prior.
Habitat in Mari Norvegico.
* k * Macrouri, manibus adactylis, thorace oblongo.
description: Published as part of Linnaeus, Carolus, 1758, Systema Naturae per regna tria naturae: secundum classes, ordines, genera, species, cum characteribus, differentiis, synonymis, locis, Stockholm :Laurentius Salvius on pages 632-633, DOI: 10.5962/bhl.title.542, http://zenodo.org/record/3922206
The Role of Kinetic Energy Flux in the Convective Urca Process
Creators: name: Stein, J.
name: Barkat, Z.
name: Wheeler, J. C.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: The previous analysis of the convective Urca neutrino loss process in degenerate, convective, quasi-static, carbon-burning cores by Barkat and Wheeler omitted specific consideration of the role of the kinetic energy flux. The arguments of Barkat and Wheeler that steady-state composition gradients exist are correct, but chemical equilibrium does not result in net cooling. Barkat and Wheeler included a "work" term that effectively removed energy from the total energy budget that could only have come from the kinetic energy, which must remain positive. Consideration of the kinetic energy in the thermodynamics of the convective Urca process shows that the convective Urca neutrinos reduce the rate of increase of entropy that would otherwise be associated with the input of nuclear energy and slow down the convective current, but, unlike the "thermal" Urca process do not reduce the entropy or temperature.
description: 16 pages, AAS LaTex, in press, Astrophysical Journal, September 20, Vol 523
Effects of CaO on nitrogen transformation during pyrolysis of soybean protein
Creators: name: Lihong Wei
name: Meijia Liu
name: Faguang Liang
name: Tianhua Yang
name: Wen, Lina
Publisher: name: Taylor & Francis
Year: 2018
Subjects: subject: Biochemistry
subject: Medicine
subject: Pharmacology
subject: Biotechnology
subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences
subject: Ecology
subject: FOS: Biological sciences
subject: 69999 Biological Sciences not elsewhere classified
subject: Developmental Biology
subject: Plant Biology

description: To elucidate the effects of CaO on nitrogen transformation during sludge pyrolysis, transformation behavior from char N into NOx precursors during pyrolysis of soybean protein (SP) with CaO at 600–700°C was investigated. Results showed that CaO inhibited the transformation of pyridine N and quaternary N into HCN and promoted HCN conversion into NH3 at 600–700°C. CaO inhibited the conversion of protein N and tar N into NH3 at 600°C but promoted it at 700°C. NOx precursor yield was the lowest when SP was pyrolyzed with CaO/N of 5.5 at 600°C (reduced by 11.66% compared with raw SP pyrolysis).
A New Algorithm for Supernova Neutrino Transport and Some Applications
Creators: name: Burrows, A.
name: Young, T.
name: Pinto, P. A.
name: Eastman, R.
name: Thompson, T.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We have developed an implicit, multi-group, time-dependent, spherical neutrino transport code based on the Feautrier variables, the tangent-ray method, and accelerated ${\bf Λ}$ iteration. The code achieves high angular resolution, is good to O($v/c$), is equivalent to a Boltzmann solver (without gravitational redshifts), and solves the transport equation at all optical depths with precision. In this paper, we present our formulation of the relevant numerics and microphysics and explore protoneutron star atmospheres for snapshot post-bounce models. Our major focus is on spectra, neutrino-matter heating rates, Eddington factors, angular distributions, and phase-space occupancies. In addition, we investigate the influence on neutrino spectra and heating of final-state electron blocking, stimulated absorption, velocity terms in the transport equation, neutrino-nucleon scattering asymmetry, and weak magnetism and recoil effects. Furthermore, we compare the emergent spectra and heating rates obtained using full transport with those obtained using representative flux-limited transport formulations to gauge their accuracy and viability. Finally, we derive useful formulae for the neutrino source strength due to nucleon-nucleon bremsstrahlung and determine bremsstrahlung's influence on the emergent $ν_μ$ and $ν_τ$ neutrino spectra.
description: 58 pages, single-spaced LaTeX, 23 figures, revised title, also available at http://jupiter.as.arizona.edu/~burrows/papers, accepted for publication in the Ap.J
title: ADCO, Huitième cartulaire de Saint-Étienne de Dijon (1661-1667), Cart. 31 (G 135), 549 folios, f. 0909
Creators: name: de la Côte d'Or, Archives départementales
name: Archives Départementales De La Côte-D'Or
name: Petot, Frédérique
name: Projet CBMA
name: CG21/F.PETOT/2012
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2020
Subjects: subject: Corpus Burgundiae Medii Aevi
subject: Chartes de la Bourgogne du Moyen Âge
subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris
subject: cartulaire

description: Huitième cartulaire de Saint-Étienne de Dijon (1661-1667), Archives départementales de la Côte-d'Or, Cart. 31 (G 135), 549 folios, f. 0909, Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Huitième cartulaire de Saint-Étienne de Dijon (1661-1667), Archives départementales de la Côte-d'Or, Cart. 31 (G 135), 549 folios, f. 0909, in Projet CBMA - Corpus Burgundiae Medii Aevi [Ressource en ligne], https://manuscrits.cbma-project.eu/
description: Provenance: abbaye Saint-Étienne de Dijon
description: Provenance: http://www.wikidata.org/entity/Q15945019
The RGB Sample of Intermediate BL Lacs
Creators: name: Laurent-Muehleisen, S. A.
name: Kollgaard, R. I.
name: Feigelson, E. D.
name: Brinkmann, W.
name: Siebert, J.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Combining newly identified and previously known BL Lacs from the RASS-Green Bank (RGB) catalog, we present a sample of 127 BL Lacs, the largest ever derived from a single uniform survey. A Complete sample of 33 objects brighter than O=18.0 mag is also presented. These samples are compared to other known BL Lac samples and are generally found to exhibit properties intermediate between those of the previously disparate classes of High and Low energy peaked BL Lacs (HBLs and LBLs, respectively). This result is most dramatic in the distribution of the X-ray to radio logarithmic flux ratios, where the RGB BL Lacs are shown to peak precisely where the sharp dichotomy between the two subclasses was previously seen. The alpha_ro vs alpha_ox diagram also shows the RGB sample smoothly bridges the gap between the previously distinct subclasses of LBLs and HBLs. We also find a weak, but statistically significant correlation between the composite X-ray spectral index alpha_xox and alpha_ro. This implies that the more LBL-like RGB BL Lacs have a secondary source of X-ray emission, possibly from an inverse Compton component. We also present both the X-ray and radio logN-logS distributions for which the competing HBL/LBL unification scenarios have differing predictions. The unknown effects of the triple flux limit inherent in the RGB Complete sample makes quantitative analysis uncertain, but the characteristics of the RGB sample compare well both with results obtained from previous samples and with general theoretical predictions based on a simple Monte Carlo simulation. Our analysis indicates that the unimodal distribution of BL Lac properties found in the RGB sample likely reliably reflect the underlying population, while the bimodal distribution found in earlier studies arose primarily from observational selection effects.
description: 40 pages, 11 figures, 3 tables, Accepted for Publication in the Astrophysical Journal