cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Additional file 8 of Prognostic value of CSN5 in patients with digestive system cancers: a systematic review and meta-analysis
Creators: name: Guo, Yonghua
name: Gao, Meng
name: Yao, Ye
name: Li, Jinghua
name: Chen, Xi
name: Wang, Xingxing
name: Chen, Zhang
name: Yuan, Yufeng
name: Ma, Weijie
Publisher: name: figshare
Year: 2022
Subjects: Medicine
Cell Biology
Biotechnology
Biological Sciences not elsewhere classified
Mathematical Sciences not elsewhere classified
Cancer
Science Policy

description: Additional file 8.
Additional file 1: of Using qualitative and community-based engagement approaches to gain access and to develop a culturally appropriate STI prevention intervention for foreign female entertainment workers in Singapore
Creators: name: Lim, Raymond
name: Cheung, Olive
name: Tham, Dede
name: La, Hanh
name: Thein Win
name: Chan, Roy
name: Wong, Mee
Publisher: name: figshare
Year: 2018
Subjects: subject: Biotechnology
subject: Ecology
subject: FOS: Biological sciences
subject: Sociology
subject: FOS: Sociology
subject: 69999 Biological Sciences not elsewhere classified
subject: 19999 Mathematical Sciences not elsewhere classified
subject: FOS: Mathematics
subject: Developmental Biology
subject: Marine Biology

description: Table S1. Results of the estimated foreign female entertainment worker (FEW) population sizes using the census enumeration technique. (PDF 1054 kb)
Distribution of extinction and star formation in NGC1569
Creators: name: Relano, M.
name: Lisenfeld, U.
name: Battaner, E.
name: Vilchez, J. M.
name: Perez-Gonzalez, P.
Publisher: name: arXiv
Year: 2006
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We investigate the distribution of the intrinsic extinction in NGC1569 using an extinction map derived from the H_alpha/H_beta emission line ratio. We compare the extinction distribution to that of the dust emission traced by SPITZER IRAC(8microns) and MIPS (24microns) maps. The intrinsic extinction shows spatial variations, from zones with negligible extinction to zones with values up to A(V)=0.8mag. We find an extinction shell and establish a relation between this shell and the interstellar expanding structure produced by the stellar winds comig from the Super Star Cluster (SSCs) A and B in the center of the galaxy. We suggest that the extinction shell has been produced by the accumulation of dust at the border of the shell. Although we find a good spatial correlation between the Balmer extinction and infrared emission, there is a spatial displacement between the 8microns and 24microns maxima and the maximum in Balmer extinction which needs further investigation.
description: 4 pages, presented at the Spitzer Conference Infrared Diagnostics of Galaxy Evolution, 14-16 November 2005
The quantum pigeonhole principle as a violation of the principle of bivalence
Creators: name: Bolotin, Arkady
Publisher: name: arXiv
Year: 2017
Subjects: subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: In the paper, it is argued that the phenomenon known as the quantum pigeonhole principle (namely, three quantum particles are put in two boxes, yet no two particles are in the same box) can be explained not as a violation of Dirichlet's box principle in the case of quantum particles but as a nonvalidness of a bivalent logic for describing not-yet verified propositions relating to quantum mechanical experiments.
description: This is a pre-print of an article published in Quantum Studies: Mathematics and Foundations. The final authenticated version is available online at: https://doi.org/10.1007/s40509-018-0157-y
Combining freeform optics and curved detectors for wide field imaging: a polynomial approach over squared aperture
Creators: name: Muslimov, Eduard
name: Hugot, Emmanuel
name: Jahn, Wilfried
name: Vives, Sebastien
name: Ferrari, Marc
name: Chambion, Bertrand
name: Henry, David
name: Gaschet, Cristophe
Publisher: name: arXiv
Year: 2017
Subjects: subject: Instrumentation and Methods for Astrophysics (astro-ph.IM)
subject: FOS: Physical sciences

description: In the recent years a significant progress was achieved in the field of design and fabrication of optical systems based on freeform optical surfaces. They provide a possibility to build fast, wide-angle and high-resolution systems, which are very compact and free of obscuration. However, the field of freeform surfaces design techniques still remains underexplored. In the present paper we use the mathematical apparatus of orthogonal polynomials defined over a square aperture, which was developed before for the tasks of wavefront reconstruction, to describe shape of a mirror surface. Two cases, namely Legendre polynomials and generalization of the Zernike polynomials on a square, are considered. The potential advantages of these polynomials sets are demonstrated on example of a three-mirror unobscured telescope with F/#=2.5 and FoV=7.2x7.2°. In addition, we discuss possibility of use of curved detectors in such a design.
description: 14 pages, 10 figures, 5 tables, to be published in Optics Express Vol. 25, Iss. 13 - June 26, 2017
Control of the geometric phase and pseudo-spin dynamics on coupled Bose-Einstein condensates
Creators: name: Duzzioni, E. I.
name: Sanz, L.
name: Mizrahi, S. S.
name: Moussa, M. H. Y.
Publisher: name: arXiv
Year: 2006
Subjects: subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: We describe the behavior of two coupled Bose-Einstein condensates in time-dependent (TD) trap potentials and TD Rabi (or tunneling) frequency, using the two-mode approach. Starting from Bloch states, we succeed to get analytical solutions for the TD Schroedinger equation and present a detailed analysis of the relative and geometric phases acquired by the wave function of the condensates, as well as their population imbalance. We also establish a connection between the geometric phases and constants of motion which characterize the dynamic of the system. Besides analyzing the affects of temporality on condensates that differs by hyperfine degrees of freedom (internal Josephson effect), we also do present a brief discussion of a one specie condensate in a double-well potential (external Josephson effect).
description: 1 tex file and 11 figures in pdf format
The possible submillimeter bump and accretion-jet in the central supermassive black hole of NGC 4993
Creators: name: Wu, Qingwen
name: Feng, Jianchao
name: Fan, Xuliang
Publisher: name: arXiv
Year: 2017
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: NGC 4993, as a host galaxy of the electromagnetic counterpart of the first gravitational-wave detection of a binary neutron-star merger, was observed by many powerful telescopes from radio to $γ$-ray waveband. The weak nuclear activities of NGC 4993 suggest that it is a low-luminosity active galactic nuclear (LLAGN). We build the multi-waveband spectral energy distributions (SEDs) of NGC 4993 from literatures. We find that the radio spectrum at $\sim 100-300$ GHz is much steeper than that of low-frequency waveband (e.g., 6-100 GHz), where this break was also found in the supermassive black holes in our galaxy center (Sgr A*), and in some other nearby AGNs. The radio emission above and below this break may has different physical origins, which provide an opportunity to probe the accretion and jet properties. We model the multi-waveband SEDs of NGC 4993 with an advection-dominated accretion flow (ADAF)-jet model. We find that the high-frequency steep radio emission at millimeter waveband is consistent with the prediction of the ADAF, while the low-frequency flat radio spectrum is better fitted by the jet. Further more, the X-ray emission can be also explained by the ADAF model simultaneously. From the model fits, we estimate important parameters of the central engine (e.g., accretion rate near the horizon of the black hole and mass-loss rate in jet) for NGC 4993. This result strengthen that the millimiter, submillimer and deep X-ray observations are crucial to understand the weak or quiescent activities in supermassive black-hole systems. Further simultaneous millimeter and X-ray monitoring of this kind of LLAGNs will help us to better understand the physical origin of multiwaveband emission.
description: 5 pages, 1 figure, ApJ in press
Order parameters and boundary effects in U(1) lattice gauge theory
Creators: name: Kerler, W.
name: Rebbi, C.
name: Weber, A.
Publisher: name: arXiv
Year: 1996
Subjects: subject: High Energy Physics - Lattice (hep-lat)
subject: FOS: Physical sciences

description: We show that, independently of the boundary conditions, the two phases of the 4-dimensional compact U(1) lattice gauge theory can be characterized by the presence or absence of an ``infinite'' current network, with an appropriate definition of ``infinite'' for the various types of boundary conditions imposed on the finite lattice. The probability for the occurrence of an ``infinite'' network takes values 0 or 1 in the cold and hot phase, respectively. It thus constitutes a very efficient order parameter, which allows one to determine the transition region at low computational cost. In addition, for open and fixed boundary conditions we address the question of the impact of inhomogeneities and give examples of the reappearance of an energy gap already at moderate lattice sizes.
description: 11 pages, Latex, 5 PostScript figures, uuencoded
Additional file 6: of Genome analysis of the freshwater planktonic Vulcanococcus limneticus sp. nov. reveals horizontal transfer of nitrogenase operon and alternative pathways of nitrogen utilization
Creators: name: Cesare, Andrea Di
name: Cabello-Yeves, Pedro
name: Chrismas, Nathan
name: Sánchez-Baracaldo, Patricia
name: Salcher, Michaela
name: Callieri, Cristiana
Publisher: name: figshare
Year: 2018
Subjects: subject: Medicine
subject: Microbiology
subject: FOS: Biological sciences
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: Inorganic Chemistry
subject: FOS: Chemical sciences
subject: Plant Biology
subject: 60506 Virology
subject: Computational Biology

description: Fig. S3. Microphotography at epifluorescence microscopy of V.limneticus sp. nov. cultures in the two treatments with (+N) and whithout (-N) nitrogen. Glycogen granules are clearly visible in the N limited culture. (Zeiss Axioplan, 1250×, blue excitation). V.limneticus sp. nov. monoclonal culture was isolated from a volcanic freshwater mesotrophic lake in central Italy, Lake Albano. Dimension of cells: 0.97 ± 0.21 × 0.76 ± 0.12 μm, Volume: 0.36 ± 0.19 μm3. (PDF 644 kb)
Additional file 9 of Prognostic value of CSN5 in patients with digestive system cancers: a systematic review and meta-analysis
Creators: name: Guo, Yonghua
name: Gao, Meng
name: Yao, Ye
name: Li, Jinghua
name: Chen, Xi
name: Wang, Xingxing
name: Chen, Zhang
name: Yuan, Yufeng
name: Ma, Weijie
Publisher: name: figshare
Year: 2022
Subjects: Medicine
Cell Biology
Biotechnology
Biological Sciences not elsewhere classified
Mathematical Sciences not elsewhere classified
Cancer
Science Policy

description: Additional file 9.
title: ADCO, Cartulaire de l'office de la Porte de l'abbaye de Cîteaux, Registrum possessionum porte Cistercii (début XVe siècle), Cart. 172 (11 H 69), 115 folios, f. 0215
Creators: name: de la Côte d'Or, Archives départementales
name: Archives Départementales De La Côte-D'Or
name: Petot, Frédérique
name: Projet CBMA
name: Petot, Frédéric
name: CG21/F.PETOT/2012
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2020
Subjects: subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris
subject: cartulaire
subject: Corpus Burgundiae Medii Aevi
subject: Chartes de la Bourgogne du Moyen Âge

description: Cartulaire de l'office de la Porte de l'abbaye de Cîteaux, Registrum possessionum porte Cistercii (début XVe siècle), Archives départementales de la Côte-d'Or, Cart. 172 (11 H 69), 115 folios, f. 0215, Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Cartulaire de l'office de la Porte de l'abbaye de Cîteaux, Registrum possessionum porte Cistercii (début XVe siècle), Archives départementales de la Côte-d'Or, Cart. 172 (11 H 69), 115 folios, f. 0215, in Projet CBMA - Corpus Burgundiae Medii Aevi [Ressource en ligne], https:// manuscrits.cbma-project.eu/
description: Provenance: https://www.geonames.org/3024876
description: Provenance: http://www.idref.fr/030974844/id
description: Provenance: https://catalogue.bnf.fr/ark:/12148/cb12228351v
description: Provenance: abbaye de Cîteaux
description: Provenance: http://www.wikidata.org/entity/Q843261
Ramp and periodic dynamics across non-Ising critical points
Creators: name: Ghosh, Roopayan
name: Sen, Arnab
name: Sengupta, K.
Publisher: name: arXiv
Year: 2017
Subjects: subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: FOS: Physical sciences

description: We study ramp and periodic dynamics of ultracold bosons in an one-dimensional (1D) optical lattice which supports quantum critical points separating a uniform and a $Z_3$ or $Z_4$ symmetry broken density-wave ground state. Our protocol involves both linear and periodic drives which takes the system from the uniform state to the quantum critical point (for linear drive protocol) or to the ordered state and back (for periodic drive protocols) via controlled variation of a parameter of the system Hamiltonian. We provide exact numerical computation, for finite-size boson chains with $L \le 24$ using exact-diagonalization (ED), of the excitation density $D$, the wavefunction overlap $F$, and the excess energy $Q$ at the end of the drive protocol. For the linear ramp protocol, we identify the range of ramp speeds for which $D$ and $Q$ shows Kibble-Zurek scaling. We find, based on numerical analysis with $L \le 24$, that such scaling is consistent with that expected from critical exponents of the $q$-state Potts universality class with $q=3,4$. For periodic protocol, we show that the model display near-perfect dynamical freezing at specific frequencies; at these frequencies $D, Q \to 0$ and $|F| \to 1$. We provide a semi-analytic explanation of such freezing behavior and relate this phenomenon to a many-body version of Stuckelberg interference. We suggest experiments which can test our theory.
description: v2,final version accepeted in PRB
0303 The Crystal Palace as the Parliament of Objects
Creators: name: Prange, Regine
Publisher: name: RIHA Journal
Year: 2024

description: In a sequence dedicated to the London World’s Fair in his collage film The Power of Emotion (1983), Alexander Kluge talks about how the suppression of prudent proletarian emotion by the aesthetic staging and emotionalisation of exchange value corrupted the departure of industrial modernity into happiness and affluence. Correspondent to the mode of the opera, which originated concurrently with the "parliament of objects" as the "power plant of emotions", the fairytale-like beginning of the collage with the Great Exhibition in London in 1851 is followed by the Crystal Palace fire in 1937, with which the Reichstag fire of 1935 is associated. What is crucial is the portrayal of the workers Kluge’s montages feature as the 'real' builders of the Crystal Palace and of societal prosperity. The artisanal sensitivity with which bolt and nut are connected in such a way that the construction is stable represents a social utopia, which in view of its loss requires a response at the artistic level that is appropriate to the wartime destruction. The technological construction of aesthetic semblance has to be laid bare, the artistic form has to become iconoclastic.
description: RIHA Journal, 2024: Special Issue "'Gesamtkunstwerk' World’s Fair. Revisioning International Exhibitions"
VLA observations of the disk around the young brown dwarf 2MASS J044427+2512
Creators: name: Ricci, L.
name: Rome, H.
name: Pinilla, P.
name: Facchini, S.
name: Birnstiel, T.
name: Testi, L.
Publisher: name: arXiv
Year: 2017
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: We present multi-wavelength radio observations obtained with the VLA of the protoplanetary disk surrounding the young brown dwarf 2MASS J04442713+2512164 (2M0444) in the Taurus star forming region. 2M0444 is the brightest known brown dwarf disk at millimeter wavelengths, making this an ideal target to probe radio emission from a young brown dwarf. Thermal emission from dust in the disk is detected at 6.8 and 9.1 mm, whereas the 1.36 cm measured flux is dominated by ionized gas emission. We combine these data with previous observations at shorter sub-mm and mm wavelengths to test the predictions of dust evolution models in gas-rich disks after adapting their parameters to the case of 2M0444. These models show that the radial drift mechanism affecting solids in a gaseous environment has to be either completely made inefficient, or significantly slowed down by very strong gas pressure bumps in order to explain the presence of mm/cm-sized grains in the outer regions of the 2M0444 disk. We also discuss the possible mechanisms for the origin of the ionized gas emission detected at 1.36 cm. The inferred radio luminosity for this emission is in line with the relation between radio and bolometric luminosity valid for for more massive and luminous young stellar objects, and extrapolated down to the very low luminosity of the 2M0444 brown dwarf.
description: 9 pages, 5 figures, accepted for publication in ApJ
La bande dessinée d'Ilan Manouach : l'héritage du cinéma, l'usage de repères et la place du sens
Creators: name: Manouach, Ilan
name: Boivin, Thomas
Publisher: name: Multitudes
Year: 2009

description: La bande dessinée d'Ilan Manouach : l'héritage du cinéma, l'usage de repères et la place du sens

https://www.multitudes.net/ilan-manouach/

https://www.cairn.info/revue-multitudes-2009-2-page-285.htm
On Evaluating Commercial Cloud Services: A Systematic Review
Creators: name: Li, Zheng
name: Zhang, He
name: O'Brien, Liam
name: Cai, Rainbow
name: Flint, Shayne
Publisher: name: arXiv
Year: 2017
Subjects: subject: Distributed, Parallel, and Cluster Computing (cs.DC)
subject: Performance (cs.PF)
subject: FOS: Computer and information sciences

description: Background: Cloud Computing is increasingly booming in industry with many competing providers and services. Accordingly, evaluation of commercial Cloud services is necessary. However, the existing evaluation studies are relatively chaotic. There exists tremendous confusion and gap between practices and theory about Cloud services evaluation. Aim: To facilitate relieving the aforementioned chaos, this work aims to synthesize the existing evaluation implementations to outline the state-of-the-practice and also identify research opportunities in Cloud services evaluation. Method: Based on a conceptual evaluation model comprising six steps, the Systematic Literature Review (SLR) method was employed to collect relevant evidence to investigate the Cloud services evaluation step by step. Results: This SLR identified 82 relevant evaluation studies. The overall data collected from these studies essentially represent the current practical landscape of implementing Cloud services evaluation, and in turn can be reused to facilitate future evaluation work. Conclusions: Evaluation of commercial Cloud services has become a world-wide research topic. Some of the findings of this SLR identify several research gaps in the area of Cloud services evaluation (e.g., the Elasticity and Security evaluation of commercial Cloud services could be a long-term challenge), while some other findings suggest the trend of applying commercial Cloud services (e.g., compared with PaaS, IaaS seems more suitable for customers and is particularly important in industry). This SLR study itself also confirms some previous experiences and reveals new Evidence-Based Software Engineering (EBSE) lessons.
Large-scale dynamos in rapidly rotating plane layer convection
Creators: name: Bushby, P. J.
name: Käpylä, P. J.
name: Masada, Y.
name: Brandenburg, A.
name: Favier, B.
name: Guervilly, C.
name: Käpylä, M. J.
Publisher: name: arXiv
Year: 2017
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: Fluid Dynamics (physics.flu-dyn)
subject: FOS: Physical sciences

description: Context: Convectively-driven flows play a crucial role in the dynamo processes that are responsible for producing magnetic activity in stars and planets. It is still not fully understood why many astrophysical magnetic fields have a significant large-scale component. Aims: Our aim is to investigate the dynamo properties of compressible convection in a rapidly rotating Cartesian domain, focusing upon a parameter regime in which the underlying hydrodynamic flow is known to be unstable to a large-scale vortex instability. Methods: The governing equations of three-dimensional nonlinear magnetohydrodynamics (MHD) are solved numerically. Different numerical schemes are compared and we propose a possible benchmark case for other similar codes. Results: In keeping with previous related studies, we find that convection in this parameter regime can drive a large-scale dynamo. The components of the mean horizontal magnetic field oscillate, leading to a continuous overall rotation of the mean field. Whilst the large-scale vortex instability dominates the early evolution of the system, it is suppressed by the magnetic field and makes a negligible contribution to the mean electromotive force that is responsible for driving the large-scale dynamo. The cycle period of the dynamo is comparable to the ohmic decay time, with longer cycles for dynamos in convective systems that are closer to onset. In these particular simulations, large-scale dynamo action is found only when vertical magnetic field boundary conditions are adopted at the upper and lower boundaries. Strongly modulated large-scale dynamos are found at higher Rayleigh numbers, with periods of reduced activity ("grand minima"-like events) occurring during transient phases in which the large-scale vortex temporarily re-establishes itself, before being suppressed again by the magnetic field.
description: 16 pages, 16 figures, to appear in Astronomy & Astrophysics. The material in the Appendix could form the basis for a possible benchmarking exercise; we would encourage anyone who might be interested in participating in such an exercise to contact the authors
Boosting Metrics for Cloud Services Evaluation -- The Last Mile of Using Benchmark Suites
Creators: name: Li, Zheng
name: O'Brien, Liam
name: Cai, Rainbow
name: Zhang, He
Publisher: name: arXiv
Year: 2017
Subjects: subject: Distributed, Parallel, and Cluster Computing (cs.DC)
subject: Performance (cs.PF)
subject: FOS: Computer and information sciences

description: Benchmark suites are significant for evaluating various aspects of Cloud services from a holistic view. However, there is still a gap between using benchmark suites and achieving holistic impression of the evaluated Cloud services. Most Cloud service evaluation work intended to report individual benchmarking results without delivering summary measures. As a result, it could be still hard for customers with such evaluation reports to understand an evaluated Cloud service from a global perspective. Inspired by the boosting approaches to machine learning, we proposed the concept Boosting Metrics to represent all the potential approaches that are able to integrate a suite of benchmarking results. This paper introduces two types of preliminary boosting metrics, and demonstrates how the boosting metrics can be used to supplement primary measures of individual Cloud service features. In particular, boosting metrics can play a summary Response role in applying experimental design to Cloud services evaluation. Although the concept Boosting Metrics was refined based on our work in the Cloud Computing domain, we believe it can be easily adapted to the evaluation work of other computing paradigms.
description: Proceedings of the 27th IEEE International Conference on Advanced Information Networking and Applications (AINA 2013), pp. 381-388, Barcelona, Spain, March 25-28, 2013
Telegram Regarding Recommendations for Warsaw and Stockholm Embassies
Creators: name: United States. Department Of State
Publisher: name: The University of Texas at Austin
Year: 1966
Subjects: Box 200 Folder 6
Box 200 Folder 06
Poland -- Politics and government -- 1945-1980
Poland -- Relations -- Soviet Union

description: Telegram conveying recommendations on Rapacki remarks for the Warsaw and Stockholm embassies.
$S$-wave $Kπ$ contributions to the hadronic charmonium $B$ decays in the perturbative QCD approach
Creators: name: Rui, Zhou
name: Wang, Wen-Fei
Publisher: name: arXiv
Year: 2017
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We extend our recent works on the two-pion $S$-wave resonance contributions to the kaon-pion ones in the $B$ meson hadronic charmonium decay modes based on the perturbative QCD approach. The $S$-wave $Kπ$ time-like form factor in its distribution amplitudes is described by the LASS parametrization, which consists of the $K^*_0(1430)$ resonant state together with an effective range nonresonant component. The predictions for the decays $B\rightarrow J/ψKπ$ in this work agree well with the experimental results from $BABAR$ and Belle Collaborations. We also discuss theoretical uncertainties, indicating the results of this work, which can be tested by the LHCb and Belle-II experiments, are reasonably accurate.
description: 8 pages,2 figures,2 tables
The Hubble Constant: A Summary of the HST Program for the Luminosity Calibration of Type Ia Supernovae by Means of Cepheids
Creators: name: Sandage, A.
name: Tammann, G. A.
name: Saha, A.
name: Reindl, B.
name: Macchetto, F. D.
name: Panagia, N.
Publisher: name: arXiv
Year: 2006
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: This is the fifth and final summary paper of our 15 year program using the Hubble Space Telescope (HST) to determine the Hubble constant using Type Ia supernovae, calibrated with Cepheid variables in nearby galaxies that hosted them. Several developments not contemplated at the start of the program in 1990 have made it necessary to put the summary on H_0 on a broader basis than originally thought, making four preparatory papers necessary. The new Cepheid distances of the subset of 10 galaxies, which were hosts of normal SNeIa, give weighted mean luminosities in B, V, and I at maximum light of -19.49, -19.46, and -19.22, respectively. These calibrate the adopted SNeIa Hubble diagram from Paper III to give a global value of H_0 = 62.3 +/- 1.3 (random) +/- 5.0 (systematic). Local values of H_0 between 4.4 and 30 Mpc from Cepheids, SNeIa, 21cm-line widths, and the tip of the red-giant branch (TRGB) all agree within 5% of our global value. This agreement of H_0 on all scales from 4 - 200 Mpc finds its most obvious explanation in the smoothing effect of vacuum energy on the otherwise lumpy gravitational field due to the non-uniform distribution of the local galaxies. The physical methods of time delay of gravitational lenses and the Sunyaev-Zeldovich effect are consistent (but with large errors) with our global value. The present result is also not in contradiction with existing analyses of CMB data, because they either lead to wide error margins of H_0 or depend on the choice of unwarrented priors that couple the value of H_0 with a number of otherwise free parameters in the CMB acoustic waves. Our value of H_0 is 14% smaller than the value of H_0 found by Freedman et al. (2001) because our independent Cepheid distances to the six SNeIa-calibrating galaxies used in that analysis average 0.35mag larger than those used earlier.
description: 52 pages, 9 figures, 8 tables, accepted for publication in ApJ
Additional file 3: of MTH1 deficiency selectively increases non-cytotoxic oxidative DNA damage in lung cancer cells: more bad news than good?
Creators: name: Abbas, Hussein
name: Kheloud Alhamoudi
name: Evans, Mark
name: Jones, George
name: Foster, Steven
Publisher: name: figshare
Year: 2018
Subjects: subject: Biophysics
subject: Biochemistry
subject: Space Science
subject: 29999 Physical Sciences not elsewhere classified
subject: FOS: Physical sciences
subject: Cell Biology
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Biotechnology
subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences
subject: 69999 Biological Sciences not elsewhere classified
subject: Cancer
subject: Hematology

description: Representative images of “Comets” and the corresponding intensity profiles, showing (i) ~ 5% Tail DNA damage, typical of the NSCLC cells treated with no siRNA or scramble siRNA, and analysed by regular Fpg-modified alkaline comet assay (0.8 U Fpg/gel); and (ii) comets showing ~ 10% tail DNA, typical of the NSCLC cells treated with MTH1 siRNA. Superimposed on the Comet images are the image analysis software (Komet 5.5, Andor Technology) determined boundaries demarcating the ‘Comet head’ (pink circle) and ‘tail extent’ (vertical orange line) (Barber RC, Hickenbotham P, Hatch T, Kelly D, Topchiy N, Almeida GM, et al. Radiation-induced transgenerational alterations in genome stability and DNA damage. Oncogene. 2006;25(56):7336–7342). % tail DNA = 100 - % head DNA; % head DNA = (integrated optical head intensity / (integrated optical head intensity + integrated optical tail intensity)) × 100. (PDF 1431 kb)
Coboundary dynamical Poisson groupoids and integrable systems
Creators: name: Li, Luen-Chau
Publisher: name: arXiv
Year: 2005
Subjects: subject: Mathematical Physics (math-ph)
subject: Symplectic Geometry (math.SG)
subject: FOS: Physical sciences
subject: FOS: Mathematics

description: In this paper, we present a general scheme to construct integrable systems based on realization in the coboundary dynamical Poisson groupoids of Etingof and Varchenko. We also present a factorization method for solving the Hamiltonian flows. To illustrate our scheme and factorization theory, we consider a family of hyperbolic spin Ruijsenaars-Schneider models related to affine Toda field theories and solve the equations of motion in a simple case.
description: 22 pages. This version has additional typo corrections
Telegram Regarding Suggestions for Gronouski-Wang Talks
Creators: name: United States. Department Of State
Publisher: name: The University of Texas at Austin
Year: 1966
Subjects: Box 200 Folder 6
Box 200 Folder 06
Poland -- Politics and government -- 1945-1980
Poland -- Relations -- Soviet Union

description: Telegram concerning Ambassador Granouski's upcoming talk with Ambassador Wang.
Note Regarding Draft Instructions for Gronouski-Wang Talks
Creators: name: United States. Department Of State
Publisher: name: The University of Texas at Austin
Year: 1966
Subjects: Box 200 Folder 6
Box 200 Folder 06
Poland -- Politics and government -- 1945-1980
Poland -- Relations -- Soviet Union

description: Note for the President concerning recommendations for Ambassador Gronouski's talks with Chinese communists.
Manipulation of the quantum state by Majorana transition in spinor Bose-Einstein condensates
Creators: name: Xia, Lin
name: Xu, Xu
name: Yang, Fan
name: Xiong, Wei
name: Li, Juntao
name: Ma, Qianli
name: Zhou, Xiaoji
name: Guo, Hong
name: Chen, Xuzong
Publisher: name: arXiv
Year: 2006
Subjects: subject: Quantum Physics (quant-ph)
subject: Other Condensed Matter (cond-mat.other)
subject: FOS: Physical sciences

description: Manipulation of the quantum state by the Majorana transition in spinor BEC system has been realized by altering the rotation frequency of the magnetic field's direction. This kind of manipulation method has no limitation on the transition speed in principle and the system is well closed, which provides a new and superior tool to manipulate quantum states. Using this methord on pulsed atom laser, multicomponent spinor atom laser is generated. We demonstrate that the experiment results are agreed with the theoretical predication.
description: 5 pages, 5 figures
Correlations of Energy-Momentum Tensor via Gradient Flow in SU(3) Yang-Mills Theory at Finite Temperature
Creators: name: Kitazawa, Masakiyo
name: Iritani, Takumi
name: Asakawa, Masayuki
name: Hatsuda, Tetsuo
Publisher: name: arXiv
Year: 2017
Subjects: subject: High Energy Physics - Lattice (hep-lat)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: Euclidean two-point correlators of the energy-momentum tensor (EMT) in SU(3) gauge theory on the lattice are studied on the basis of the Yang-Mills gradient flow. The entropy density and the specific heat obtained from the two-point correlators are shown to be in good agreement with those from the one-point functions of EMT. These results constitute a first step toward the first principle simulations of the transport coefficients with the gradient flow.
description: 5 pages, 12 figures
A Family of Hyperbolic Spin Calogero-Moser Systems and the Spin Toda Lattices
Creators: name: Li, Luen-Chau
Publisher: name: arXiv
Year: 2005
Subjects: subject: Mathematical Physics (math-ph)
subject: Symplectic Geometry (math.SG)
subject: FOS: Physical sciences
subject: FOS: Mathematics

description: In this paper, we continue to develop a general scheme to study a broad class of integrable systems naturally associated with the coboundary dynamical Lie algebroids. In particular, we present a factorization method for solving the Hamiltonian flows. We also present two important class of new examples, a family of hyperbolic spin Calogero-Moser systems and the spin Toda lattices. To illustrate our factorization theory, we show how to solve these Hamiltonian systems explicitly.
description: 47 pages. References have been updated. This version has additional typo corrections
title: Crimes Amendment (Non-fatal Strangulation) Bill 2023: Bill Brief
Creators: name: Otter, Caley
Publisher: name: Parliamentary Library and Information Service (Vic)
Year: 2023

description: This Bill Brief provides an overview of the Crimes Amendment (Non-fatal Strangulation) Bill 2023, which establishes two offences for non-fatal strangulation. It offers some background to the Bill’s introduction, considers the second reading speech delivered by the Minister and looks at the Bill in greater detail. It also considers the arguments in favour of and against the introduction of a standalone offence for non-fatal strangulation, including areas for further research, and compares similar offences in Australian and selected overseas jurisdictions.
Cosmic Evolution of Black Holes and Spheroids. I: The M_BH-sigma Relation at z=0.36
Creators: name: Woo, Jong-Hak
name: Treu, Tommaso
name: Malkan, Matthew A.
name: Blandford, Roger D.
Publisher: name: arXiv
Year: 2006
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We test the evolution of the correlation between black hole mass and bulge velocity dispersion (M$_{\rm BH}-σ$), using a carefully selected sample of 14 Seyfert 1 galaxies at $z=0.36\pm0.01$. We measure velocity dispersion from stellar absorption lines around Mgb (5175Å) and Fe (5270Å) using high S/N Keck spectra, and estimate black hole mass from the H$β$ line width and the optical luminosity at 5100Å, based on the empirically calibrated photo-ionization method. We find a significant offset from the local relation, in the sense that velocity dispersions were smaller for given black hole masses at $z=0.36$ than locally. We investigate various sources of systematic uncertainties and find that those cannot account for the observed offset. The measured offset is $Δ\log M_{\rm BH}=0.62 \pm 0.10 \pm 0.25$, i.e. $Δ\log σ=0.15 \pm 0.03 \pm 0.06$, where the error bars include a random component and an upper limit to the systematics. At face value, this result implies a substantial growth of bulges in the last 4 Gyr, assuming that the local M$_{\rm BH}-σ$ relation is the universal evolutionary end-point. Along with two samples of active galaxies with consistently determined black hole mass and stellar velocity dispersion taken from the literature, we quantify the observed evolution with the best fit linear relation, $Δ\log M_{\rm BH} = (1.66\pm0.43)z + (0.04\pm0.09)$ with respect to the local relationship of Tremaine et al. (2002), and $Δ\log M_{\rm BH} = (1.55\pm0.46)z + (0.01\pm0.12)$ with respect to that of Ferrarese (2002). This result is consistent with the growth of black holes predating the final growth of bulges at these mass scales ($$=170 km s$^{-1}$).
description: ApJ, accepted, 31 pages, 13 figures, minor typos corrected
title: ADCO, Neuvième cartulaire de Saint-Étienne de Dijon (1661 - 1684), Cart. 32 (G 136), 745 folios, f. 0844
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: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris
subject: cartulaire
subject: Corpus Burgundiae Medii Aevi
subject: Chartes de la Bourgogne du Moyen Âge

description: Neuvième cartulaire de Saint-Étienne de Dijon (1661 - 1684), Archives départementales de la Côte-d'Or, Cart. 32 (G 136), 745 folios, f. 0844, 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. 0844, 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
MarlinMT - parallelising the Marlin framework
Creators: name: Ete, Remi
name: Frank-Dieter Gaede
Publisher: name: Zenodo
Year: 2019

description: Marlin is the event processing framework of the iLCSoft ecosystem. Originally developed for the ILC more than 15 years ago, it is now widely used, e.g. by CLICdp, CEPC and many test beam projects such as Calice, LCTPC and EU-Telescope. While Marlin is lightweight and flexible it was originally designed for sequential processing only. With MarlinMT we now evolved Marlin for parallel processing of events on multi-core architectures based on multi-threading. We report on the necessary developments and issues encountered, within Marlin as well as with the underlying LCIO EDM. A focus will be put on the new parallel event processing (PEP) scheduler. We conclude with first performance estimates, such as application speedup and memory profiling, based on parts of the ILD reconstruction chain that have been ported to MarlinMT.
The Universe is Reionizing at z~7: Bayesian Inference of the IGM Neutral Fraction Using Ly$α$ Emission from Galaxies
Creators: name: Mason, Charlotte A.
name: Treu, Tommaso
name: Dijkstra, Mark
name: Mesinger, Andrei
name: Trenti, Michele
name: Pentericci, Laura
name: de Barros, Stephane
name: Vanzella, Eros
Publisher: name: arXiv
Year: 2017
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We present a new flexible Bayesian framework for directly inferring the fraction of neutral hydrogen in the intergalactic medium (IGM) during the Epoch of Reionization (EoR, z~6-10) from detections and non-detections of Lyman Alpha (Ly$α$) emission from Lyman break galaxies (LBGs). Our framework combines sophisticated reionization simulations with empirical models of the interstellar medium (ISM) radiative transfer effects on Ly$α$. We assert that the Ly$α$ line profile emerging from the ISM has an important impact on the resulting transmission of photons through the IGM, and that these line profiles depend on galaxy properties. We model this effect by considering the peak velocity offset of Ly$α$ lines from host galaxies' systemic redshifts, which are empirically correlated with UV luminosity and redshift (or halo mass at fixed redshift). We use our framework on the sample of LBGs presented in Pentericci et al. (2014) and infer a global neutral fraction at z~7 of $\overline{x}_\mathrm{HI} = 0.59_{-0.15}^{+0.11}$, consistent with other robust probes of the EoR and confirming reionization is on-going ~700 Myr after the Big Bang. We show that using the full distribution of Ly$α$ equivalent width detections and upper limits from LBGs places tighter constraints on the evolving IGM than the standard Ly$α$ emitter fraction, and that larger samples are within reach of deep spectroscopic surveys of gravitationally lensed fields and JWST NIRSpec.
description: 15 pages, 14 figures. Accepted for publication in ApJ
Implementing community paramedicine: A known player in a new role. A narrative review
Creators: name: Spelten, Evelien
name: Thomas, Brodie
name: Van-Vuuren, Julia
name: Hardman, Ruth
name: Burns, David
name: O'Meara, P
name: Reynolds, Louise
Publisher: name: La Trobe
Year: 2024
Subjects: classificationCode: 320219
subject: Paramedicine

description: Background: Community Paramedicine is a model of care which is effective and accepted by health professionals and the community. Community paramedicine delivers low acuity primary care to disadvantaged communities and addresses service gaps. We aimed to identify successful implementation of community paramedicine models and signalled opportunities and challenges. Methods: A narrative review was conducted. We identified 14 literature reviews from four databases EMBASE, CINAHL, PubMed, Cochrane. The results from the thematic analysis were structured along the quadruple aim for healthcare redesign framework. Results: The reviews supported acceptability of the model. Patients are satisfied and there is evidence of cost reduction. Long term evidence of the positive effects of community paramedicine on patient, community health and the health system are lacking. Equally, there is unfamiliarity about the role and how it is part of an integrated health model. Conclusions: Community paramedicine could alleviate current stresses in the healthcare system and uses an available workforce of registered paramedics. To facilitate integration, we need more evidence on long-term effects for patients and the system. In addition, the unfamiliarity with the model needs to be addressed to enhance the uptake of the model.
Additional file 5: of Genome analysis of the freshwater planktonic Vulcanococcus limneticus sp. nov. reveals horizontal transfer of nitrogenase operon and alternative pathways of nitrogen utilization
Creators: name: Cesare, Andrea Di
name: Cabello-Yeves, Pedro
name: Chrismas, Nathan
name: SĂĄnchez-Baracaldo, Patricia
name: Salcher, Michaela
name: Callieri, Cristiana
Publisher: name: figshare
Year: 2018
Subjects: subject: Medicine
subject: Microbiology
subject: FOS: Biological sciences
subject: Genetics
subject: Molecular Biology
subject: Evolutionary Biology
subject: Ecology
subject: 69999 Biological Sciences not elsewhere classified
subject: Marine Biology
subject: 60506 Virology
subject: Computational Biology

description: Table S3. Abundance of the genes tested by real time PCR expressed as threshold cycle value. (PDF 83Â kb)
HYPE-Study (study-design preregistration)
Creators: name: Haehner, Peter
Publisher: name: Open Science Framework
Year: 2022
Subjects: subject: Cognition and Perception
subject: Psychology
subject: FOS: Psychology
subject: Personality and Social Contexts
subject: Social and Behavioral Sciences
subject: hypothetical events
subject: life events
subject: mental health
subject: missed events
subject: perceived event characteristics
subject: personality
subject: well-being

description: In this preregistration, only the design of the Hypothetical and Experience Events Study (HYPE-Study) will be preregistered. As the data collected in this study are intended to be used in different publications, the data analyses for these studies will be preregistered separately.
A multisite microcanonical updating method
Creators: name: Cruz, A.
name: Fernandez, L. A.
name: Iniguez, D.
name: Tarancon, A.
Publisher: name: arXiv
Year: 1996
Subjects: subject: High Energy Physics - Lattice (hep-lat)
subject: FOS: Physical sciences

description: We have made a study of several update algorithms using the XY model. We find that sequential local overrelaxation is not ergodic at the scale of typical Monte Carlo simulation time. We have introduced a new multisite microcanonical update method, which yields results compatible with those of random overrelaxation and the microcanonical demon algorithm, which are very much slower, all being incompatible with the sequential overrelaxation results.
description: 13 pages, 4 figures
title: Autorisation de captation, utilisation, diffusion et conservation de la voix d'une personne
Creators: name: Bureau, Eve
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2017

description: Source: T-4802
description: Source: C-4802
Effects of general relativity on glitch amplitudes and pulsar mass upper bounds
Creators: name: Antonelli, M.
name: Montoli, A.
name: Pizzochero, P. M.
Publisher: name: arXiv
Year: 2017
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: Pinning of vortex lines in the inner crust of a spinning neutron star may be the mechanism that enhances the differential rotation of the internal neutron superfluid, making it possible to freeze some amount of angular momentum which eventually can be released, thus causing a pulsar glitch. We investigate the general relativistic corrections to pulsar glitch amplitudes in the slow-rotation approximation, consistently with the stratified structure of the star. We thus provide a relativistic generalization of a previous Newtonian model that was recently used to estimate upper bounds on the masses of glitching pulsars. We find that the effect of general relativity on the glitch amplitudes obtained by emptying the whole angular momentum reservoir is less than 30\%. Moreover we show that the Newtonian upper bounds on the masses of large glitchers obtained from observations of their largest recorded event differ by less than a few percent from those calculated within the relativistic framework. This work can also serve as a basis to construct more sophisticated models of angular momentum reservoir in a relativistic context. In particular, we present two alternative scenarios for "rigid" and "slack" vortex lines, and we generalize the Feynman-Onsager relation to the case when both entrainment coupling between the fluids and a strong gravitational field are present.
description: 15 pages, accepted for publication in MNRAS
Additional file 2: of MTH1 deficiency selectively increases non-cytotoxic oxidative DNA damage in lung cancer cells: more bad news than good?
Creators: name: Abbas, Hussein
name: Kheloud Alhamoudi
name: Evans, Mark
name: Jones, George
name: Foster, Steven
Publisher: name: figshare
Year: 2018
Subjects: subject: Biochemistry
subject: Cell Biology
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Evolutionary Biology
subject: Developmental Biology
subject: Cancer

description: MTH2 levels are stable following MTH1 siRNA knockdown. Western blots from a single confirmation experiment performed to determine MTH2 protein levels in cell cultures grown in media without transfection reagent (no siRNA), or following transfection with MTH1 siRNA or scramble siRNA (nâ =â 1). (PDF 1128Â kb)