cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
A possible binary AGN in Mrk\,622?
Creators: name: Benítez, E.
name: Rodríguez-Espinosa, J. M.
name: Cruz-González, I.
name: González-Martín, O.
name: Negrete, C. A.
name: Ruschel-Dutra, D.
name: Gutiérrez, L.
name: Jiménez-Bailón, E.
Publisher: name: arXiv
Year: 2017
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: Mrk\,622 is a Compton Thick AGN and a double-peaked narrow emission line galaxy, thus a dual AGN candidate. In this work, new optical long-slit spectroscopic observations clearly show that this object is rather a triple peaked narrow emission line galaxy, with both blue and red shifted narrow emission lines, as well as a much narrower emission line centred at the host galaxy systemic velocity. The average velocity offset between the blue and red shifted components is $\sim$500 km\,s$^{-1}$, which is producing the apparent double-peaked emission lines. These two components are in the loci of AGN in the Baldwin, Phillips \& Terlevich (BPT) diagrams and are found to be spatially separated by $\sim$76 pc. Analysis of the optical spatially resolved spectroscopic observations presented in this work favours that Mrk\,622 is a system consisting of a Composite AGN amidst a binary AGN candidate, likely the result of a recent merger. This notwithstanding, outflows from a starburst, or single AGN could also explain the triple nature of the emission lines.
description: 5 pages, 3 figures, 3 tables. Accepted in MNRAS Letters. 5 pages, 3 tables, 3 figures
Additional file 1 of METHimpute: imputation-guided construction of complete methylomes from WGBS data
Creators: name: Taudt, Aaron
name: Roquis, David
name: Amaryllis Vidalis
name: Wardenaar, René
name: Johannes, Frank
name: Colome-Tatché́-Tatché, Maria
Publisher: name: figshare
Year: 2018
Subjects: subject: Space Science
subject: Molecular Biology
subject: Sociology
subject: FOS: Sociology
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: 80699 Information Systems not elsewhere classified
subject: FOS: Computer and information sciences
subject: Developmental Biology

description: Figures S1-S12. (PDF 1832 kb)
Super-Gaussian, super-diffusive transport of multi-mode active matter
Creators: name: Hahn, Seungsoo
name: Song, Sanggeun
name: Kim, Dae Hyun
name: Yang, Gil-Suk
name: Lee, Kang Taek
name: Sung, Jaeyoung
Publisher: name: arXiv
Year: 2017
Subjects: subject: Biological Physics (physics.bio-ph)
subject: Soft Condensed Matter (cond-mat.soft)
subject: FOS: Physical sciences

description: Living cells exhibit multi-mode transport that switches between an active, self-propelled motion and a seemingly passive, random motion. Cellular decision-making over transport mode switching is a stochastic process that depends on the dynamics of the intracellular chemical network regulating the cell migration process. Here, we propose a theory and an exactly solvable model of multi-mode active matter. Our exact model study shows that the reversible transition between a passive mode and an active mode is the origin of the anomalous, super-Gaussian transport dynamics, which has been observed in various experiments for multi-mode active matter. We also present the generalization of our model to encompass complex multi-mode matter with arbitrary internal state chemical dynamics and internal state dependent transport dynamics.
description: 34 pages
Additional file 1: of Global prevalence and distribution of coinfection of malaria, dengue and chikungunya: a systematic review
Creators: name: Salam, Nasir
name: Shoeb Mustafa
name: Hafiz, Abdul
name: Chaudhary, Anis
name: Deeba, Farah
name: Shama Parveen
Publisher: name: figshare
Year: 2018
Subjects: subject: Medicine
subject: Microbiology
subject: FOS: Biological sciences
subject: Molecular Biology
subject: 80699 Information Systems not elsewhere classified
subject: FOS: Computer and information sciences
subject: 110309 Infectious Diseases
subject: FOS: Health sciences
subject: Computational Biology

description: Table S1. Detailed search strategy. (DOCX 14 kb)
Switching Times in Fabry-Perot Measurements
Creators: name: Addesso, P.
name: Pierro, V.
name: Filatrella, G.
Publisher: name: arXiv
Year: 2017
Subjects: subject: Instrumentation and Detectors (physics.ins-det)
subject: Chaotic Dynamics (nlin.CD)
subject: Data Analysis, Statistics and Probability (physics.data-an)
subject: FOS: Physical sciences

description: We show how to analyze the motion of very low dissipation suspended mirrors in a Fabry-Perot. The very precise measurements of the mirrors motion can be determined, also in the presence of a disturbing noise, by means of the sudden reflectivity changes in special points of the mirrors positions. When the mirrors cross such positions, the effective opto-mechanical potential that arises in the device is (roughly) at a maximum. We show that the motion cross such potential maxima is not only confused by the presence of noise, but also favoured by noise itself that induces hoppings. Thus, the measurements of the times at which the crossings occur can be exploited to identify the properties of the applied signal. We also show how to circumvent the difficulty of the extremely long transient that occur in the system analyzing the escape average time with two different methods: a direct sample average and the indirect estimate from the tail distribution. Numerical simulations and physical insight suggest that the indirect estimate, through the analysis of the distribution tails with an appropriated cut off is robust against the disturbances that arise from the presence of transient dynamics.
O'SMIRLIK YOSHIDA ADDIKTIV XULQNING SHAKLLANISHIDA O'Z-O'ZIGA BAHO BERISHNING  TA'SIRI
Creators: name: Mamajonova, Shoxista
Publisher: name: Zenodo
Year: 2024

description: Ushbu maqolada  o’smirning  o’zini o’zi baholashi dastavval individ faoliyati natijalari ta’sirida shakllanishi, atrofdagilarning baholashi,o’ziga bo’lgan ishonch boshqalarning unga bildirgan fikri tufayli shakllananishi va mustahkamlanishi bu esa addiktiv xulq shakllanishini oldini olish uchun samarali psixoprofilaktik vosita ekanligi haqida fikr bildirilgan.
title: 01_0512
Creators: name: Wesley Baldwin, John
name: Baldwin, John W.
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2018
Subjects: subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris

description: L'ensemble de ces notes ont été crée par John Baldwin lors d'une de ses premières périodes de résidence à Paris. Ces documents comprennent tous les magistri qu’il avait pu rencontrer dans ses sources. Aux XIIème et XIIIème siècles, les universités n'existant pas encore, le titre de magister s'il évoque certainement une compétence n'est pas rattaché de façon systématique au passage par les écoles. De surcroît, les magistris sont le plus souvent désignés par leur seul prénom. La lecture de ces données est donc difficile et suppose un long travail pour tenter d'identifier un individu auquel on pourrait rattacher plusieurs mentions. John Baldwin avait donc renoncé à utiliser ces données pour donner un prolongement à sa magnifique étude sur les gradués d'université et leur emploi par les Capétiens et les Plantagenêts. Néanmoins, il a conservé ces données et elles sont potentiellement très utile dans le cadre de Studium, comme le sont toutes les mentions dans les volumes des Fasti Ecclesiae Gallicanae de chanoines portant ce titre de magister sans autres précisions. L'ampleur des dépouillements rend ces données très utiles et nous devons une grande reconnaissance à John Baldwin pour avoir pris la peine de faire photocopier ses fiches et de nous les avoir transmises amicalement.
Les données ainsi que les images des fiches sont accessibles sur le site Internet à l'adresse suivante : http://studium-baldwin.lamop.fr/.
Les transcriptions des fiches ont été effectuées par des étudiants de Paris 1 Panthéon - Sorbonne mais elles n'ont pas été corrigées par la suite.
description: Relation: https://lamop.hypotheses.org/
Tricritical Behavior in Charge-Order System
Creators: name: Misawa, Takahiro
name: Yamaji, Youhei
name: Imada, Masatoshi
Publisher: name: arXiv
Year: 2006
Subjects: subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: FOS: Physical sciences

description: Tricritical point in charge-order systems and its criticality are studied for a microscopic model by using the mean-field approximation and exchange Monte Carlo method in the classical limit as well as by using the Hartree-Fock approximation for the quantum model. We study the extended Hubbard model and show that the tricritical point emerges as an endpoint of the first-order transition line between the disordered phase and the charge-ordered phase at finite temperatures. Strong divergences of several fluctuations at zero wavenumber are found and analyzed around the tricritical point. Especially, the charge susceptibility chi_c and the susceptibility of the next-nearest-neighbor correlation chi_R are shown to diverge and their critical exponents are derived to be the same as the criticality of the susceptibility of the double occupancy chi_D0. The singularity of conductivity at the tricritical point is clarified. We show that the singularity of the conductivity sigma is governed by that of the carrier density and is given as |sigma-sigma_c|=|g-g_c|^{p_t}Alog{|g-g_{c}|}+B), where g is the effective interaction of the Hubbard model, sigma_c g_c represents the critical conductivity(interaction) and A and B are constants, respectively. Here, in the canonical ensemble, we obtain p_t=2beta_t=1/2 at the tricritical point. We also show that p_t changes into p_{t}'=2beta=1 at the tricritical point in the grand-canonical ensemble when the tricritical point in the canonical ensemble is involved within the phase separation region. The results are compared with available experimental results of organic conductor (DI-DCNQI)2Ag.
description: 20 pages, 32 figures, to appear in J. Phys. Soc. Jpn. Vol.75(2006)No.6
Additional file 1: of A qualitative study examining the benefits and challenges of incorporating patient-reported outcome substance use and mental health questionnaires into clinical practice to improve outcomes on the HIV care continuum
Creators: name: Monroe, Anne
name: Jabour, Sarah
name: PeĂąa, Sebastian
name: Keruly, Jeanne
name: Moore, Richard
name: Geetanjali Chander
name: Riekert, Kristin
Publisher: name: figshare
Year: 2018
Subjects: subject: Medicine
subject: Sociology
subject: FOS: Sociology
subject: Cancer
subject: Science Policy
subject: Computational Biology

description: Interview Guides. Interview guides used for patient and provider interviews. (DOCX 20 kb)
title: Control Effect of Peracetic Acid on Chlorinated DBP Formation and the Application of PAA Pre-oxidation in Drinking Water Treatment
Creators: name: Sun, Yue
Publisher: name: University of Massachusetts Amherst
Year: 2021
Subjects: subject: disinfection byproduct
subject: peracetic acid
subject: DBP control
subject: kinetics
subject: Civil and Environmental Engineering
subject: Environmental Engineering
subject: FOS: Environmental engineering

description: Chlorine has been applied as the main disinfectant in US drinking water treatment for a century. Chlorination is low cost and effective, yet there are problems with this technology, including disagreeable taste of treated drinking water and formation of toxic and potentially carcinogenic disinfection byproducts (DBPs). Alternative disinfection methods including ozone, ferrate and UV light have been studied. They are not widely applied in drinking water treatment because of problems such as the costly generation process or no residual in the system. Peracetic acid, an easy-to-use and economic friendly oxidant, has been applied as an alternative disinfectant to chlorine in wastewater treatment. However, the study and application of PAA in drinking water treatment is limited. In this research, PAA disinfection and its use to control DBP formation during subsequent chlorination was examined. Different PAA operation scenarios were tested: disinfection in the dark at 20 C with contact times up to 72 hours, decay under direct sunlight up to 18 hours and decay in the dark at 20 C with different short contact times. Best DBP control effect was observed in the 72-hour PAA pre-oxidation test. Direct sunlight accelerated PAA decomposition and shown higher ability to drop the amount of DBPs formed during subsequent chlorination. Among the scenarios tested in this study, the optimum disinfection condition for PAA was 2 hours of PAA pre-disinfection in the dark at 20 C.
Exact solution of the deformed biquadratic spin 1 hamiltonian
Creators: name: Koberle, R.
name: Santos, A. Lima -
Publisher: name: arXiv
Year: 1993
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: Remarks about highest weight states of the underlying quantum group are corrected.
description: 9
title: jiquanbuning
Creators: name: Jacques, Guillaume
Publisher: name: COCOON - https://cocoon.huma-num.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2020
Subjects: subject: Japhug
subject: jya

description: Conforms to: doi:10.34847/cocoon.49aefa90-8c1f-3ba8-a099-0ebefc6a2aa7
Strong magnetization and Chern insulators in compressed graphene/CrI$_{3}$ van der Waals heterostructures
Creators: name: Zhang, Jiayong
name: Zhao, Bao
name: Zhou, Tong
name: Xue, Yang
name: Ma, Chunlan
name: Yang, Zhongqin
Publisher: name: arXiv
Year: 2017
Subjects: subject: Materials Science (cond-mat.mtrl-sci)
subject: FOS: Physical sciences

description: Graphene-based heterostructures are a promising material system for designing the topologically nontrivial Chern insulating devices. Recently, a two-dimensional (2D) monolayer ferromagnetic insulator CrI$_{3}$ was successfully synthesized in experiments [Huang et al., Nature 546, 270 (2017)]. Here, these two interesting materials are proposed to build a heterostructure (Gr/CrI$_{3}$). Our first-principles calculations show that the system forms a van der Waals (vdW) heterostructure, relatively facilely fabricated in experiments. A Chern insulating state is acquired in the Gr/CrI$_{3}$ heterostructure if the vdW gap is compressed to certain extents by applying an external pressure. Amazingly, very strong magnetization (about 150 meV) is found in graphene, induced by the substrate CrI$_{3}$, despite the vdW interactions between them. A low-energy effective model is employed to understand the mechanism. The work functions, contact types, and band alignments of the Gr/CrI$_{3}$ heterostructure system are also studied. Our work demonstrates that the Gr/CrI$_{3}$ heterostructure is a promising system to observe the quantum anomalous Hall effect at high temperatures (up to 45 K) in experiments.
description: 9 pages, 5 figures
The impact of chemical evolution on the observable properties of stellar populations
Creators: name: Tosi, M.
Publisher: name: arXiv
Year: 2000
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: The major effects of the chemical evolution of galaxies on the characteristics of their stellar populations are reviewed. A few examples of how the observed stellar properties derived from colour--magnitude diagrams can constrain chemical evolution models are given.
description: 10 pages, 7 encapsulated figs. Review paper to appear in 'The Evolution of Galaxies. I. Observational Clues', J.M. Vilchez, G.Stasinska and E. Perez eds. (Kluwer, Dordrecht) in press
A measurement of Lorentz Angle of radiation-hard Pixel Sensors
Creators: name: Aleppo, M.
Publisher: name: arXiv
Year: 2000
Subjects: subject: Instrumentation and Detectors (physics.ins-det)
subject: FOS: Physical sciences

description: Silicon pixel detectors developed to meet LHC requirements were tested in a beam at CERN in the framework of the ATLAS collaboration. The experimental behaviour of irradiated and not-irradiated sensors in a magnetic field is discussed. The measurement of the Lorentz angle for these sensors at different operating conditions is presented. A simple model of the charge drift in silicon before and after irradiation is presented. The good agreement between the model predictions and the experimental results is shown.
description: 6 pages, 5 figures. Presented at Pixel 2000 conference (Genoa, Italy, june 2000). To be published in the Prooceedings of the conference on NIM
Exploring self-similarity of complex cellular networks: The edge-covering method with simulated annealing and log-periodic sampling
Creators: name: Zhou, Wei-Xing
name: Jiang, Zhi-Qiang
name: Sornette, Didier
Publisher: name: arXiv
Year: 2006
Subjects: subject: Disordered Systems and Neural Networks (cond-mat.dis-nn)
subject: Statistical Mechanics (cond-mat.stat-mech)
subject: FOS: Physical sciences

description: Song, Havlin and Makse (2005) have recently used a version of the box-counting method, called the node-covering method, to quantify the self-similar properties of 43 cellular networks: the minimal number $N_V$ of boxes of size $\ell$ needed to cover all the nodes of a cellular network was found to scale as the power law $N_V \sim (\ell+1)^{-D_V}$ with a fractal dimension $D_V=3.53\pm0.26$. We propose a new box-counting method based on edge-covering, which outperforms the node-covering approach when applied to strictly self-similar model networks, such as the Sierpinski network. The minimal number $N_E$ of boxes of size $\ell$ in the edge-covering method is obtained with the simulated annealing algorithm. We take into account the possible discrete scale symmetry of networks (artifactual and/or real), which is visualized in terms of log-periodic oscillations in the dependence of the logarithm of $N_E$ as a function of the logarithm of $\ell$. In this way, we are able to remove the bias of the estimator of the fractal dimension, existing for finite networks. With this new methodology, we find that $N_E$ scales with respect to $\ell$ as a power law $N_E \sim \ell^{-D_E}$ with $D_E=2.67\pm0.15$ for the 43 cellular networks previously analyzed by Song, Havlin and Makse (2005). Bootstrap tests suggest that the analyzed cellular networks may have a significant log-periodicity qualifying a discrete hierarchy with a scaling ratio close to 2. In sum, we propose that our method of edge-covering with simulated annealing and log-periodic sampling minimizes the significant bias in the determination of fractal dimensions in log-log regressions.
description: 19 elsart pages including 9 eps figures
Cosmological Relativity: A General-Relativistic Theory for the Accelerating Expanding Universe
Creators: name: Carmeli, M.
name: Behar, S.
Publisher: name: arXiv
Year: 2000
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Recent observations of distant supernovae imply, in defiance of expectations, that the universe growth is accelerating, contrary to what has always been assumed that the expansion is slowing down due to gravity. In this paper a general-relativistic cosmological theory that gives a direct relationship between distances and redshifts in an expanding universe is presented. The theory is actually a generalization of Hubble's law taking gravity into account by means of Einstein's theory of general relativity. The theory predicts that the universe can have three phases of expansion, decelerating, constant and accelerating, but it is shown that at present the first two cases are excluded, although in the past it had experienced them. Our theory shows that the universe now is definitely in the stage of accelerating expansion, confirming the recent experimental results.
Are better conducting molecules more rigid?
Creators: name: Eom, Young-Ho
name: Jeong, Hawoong
name: Yi, Juyeon
name: Orland, Henri
Publisher: name: arXiv
Year: 2006
Subjects: subject: Soft Condensed Matter (cond-mat.soft)
subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: FOS: Physical sciences

description: We investigate the electronic origin of the bending stiffness of conducting molecules. It is found that the bending stiffness associated with electronic motion, which we refer to as electro-stiffness, $κ_{e}$, is governed by the molecular orbital overlap $t$ and the gap width $u$ between HOMO and LUMO levels, and behaves as $κ_{e}\sim t^{2}/\sqrt{u^2+t^{2}}$. To study the effect of doping, we analyze the electron filling-fraction dependence on $κ_{e}$ and show that doped molecules are more flexible. In addition, to estimate the contribution of $κ_{e}$ to the total stiffness, we consider molecules under a voltage bias, and study the length contraction ratio as a function of the voltage. The molecules are shown to be contracted or dilated, with $κ_{e}$ increasing nonlinearly with the applied bias.
International Food Security Assessment 2021-31
Creators: name: Baquedano, Felix G.
name: Zereyesus, Yacob Abrehe
name: Valdes, Constanza
name: Ajewole, Kayode
name: Baquedano, Felix G.
name: Zereyesus, Yacob Abrehe
name: Valdes, Constanza
name: Ajewole, Kayode
Publisher: name: Unknown
Year: 2021
Subjects: subject: Community/Rural/Urban Development
subject: Consumer/Household Economics
subject: Food Consumption/Nutrition/Food Safety
subject: Food Security and Poverty
subject: International Development
subject: International Relations/Trade
subject: Public Economics
subject: Research Methods/ Statistical Methods
subject: Calories
subject: Coronavirus
subject: COVID-19
subject: food demand
subject: food insecurity
subject: food prices
subject: food security
subject: income
subject: nutritional target
subject: pandemic
subject: Asia
subject: Latin America and the Caribbean
subject: North Africa
subject: Sub-Saharan Africa

description: This report presents results from the United States Department of Agriculture (USDA), Economic Research Service’s (ERS) International Food Security Assessment (IFSA) analysis, which uses a demand-driven framework that evaluates consumer responsiveness to changes in prices and incomes for 76 low- and middle-income countries. Reflecting 2021’s anticipated lower income levels, despite anticipated growth for most countries, the number of food insecure people is estimated at 1.2 billion, almost 291 million higher than in 2020. A sharp increase in global food security was experienced in 2020, as compared to 2019, due to the COVID-19 pandemic. Most of the additional food insecure people in 2021 are located in the Central and South Asia (64.1 percent or 186.8 million) sub-region—including India, which drives food security trends in the Asia region. While the Sub-Saharan Africa region is projected to account for 20.6 percent (60 million) of the additional food insecure population. The remaining additional 15.3 percent (44.7 million) food insecure people in 2021 are located in other Asian sub-regions, Latin America and the Caribbean, and North Africa. The prevalence of food insecurity in 2021 for the countries in the assessment is estimated at 30.8 percent of the overall population in the countries, an increase of 6.8 percentage points relative to the 2020 estimate. In 2031, the number of food insecure people is projected to decline from the 2021 estimate by 47.4 percent (637.7 million people), which is 14.0 percent of the projected population of the countries included in this assessment. Given the evolving nature of the impacts from the COVID-19 pandemic and the long-term effects on individual country economies, the estimation results presented in this report contain a high degree of uncertainty. It is important to note the projections do not consider the impacts of unknown future events—such as climate change, armed conflict, and political and economic instability.
Superconducting Nb-film LC resonator
Creators: name: Finne, A.
name: Groenberg, L.
name: Blaauwgeers, R.
name: Eltsov, V. B.
name: Eska, G.
name: Krusius, M.
name: Ruohio, J. J.
name: Schanen, R.
name: Suni, I.
Publisher: name: arXiv
Year: 2000
Subjects: subject: Instrumentation and Detectors (physics.ins-det)
subject: FOS: Physical sciences

description: Sputtered Nb thin-film LC resonators for low frequencies at 0.5 MHz have been fabricated and tested in the temperature range 0.05--1 K in magnetic fields up to 30 mT. Their Q value increases towards decreasing temperature as sqrt(T) and reaches 10^3 at 0.05 K. As a function of magnetic field Q is unstable and displays variations up to 50%, which are reproducible from one field sweep to the next. These instabilities are attributed to dielectric losses in the plasma deposited SiO_2 insulation layer, since the thin-film coil alone reaches a Q > 10^5 at 0.05 K.
description: 6 pages, 7 figures, submitted to Review of Scientific Instruments
Giant quantized Goos-Hänchen effect on the surface of graphene in quantum Hall regime
Creators: name: Wu, Weijie
name: Chen, Shizhen
name: Mi, Chengquan
name: Zhang, Wenshuai
name: Luo, Hailu
name: Wen, Shuangchun
Publisher: name: arXiv
Year: 2017
Subjects: subject: Optics (physics.optics)
subject: FOS: Physical sciences

description: We theoretically predict a giant quantized Goos-Hänchen (GH) effect on the surface of graphene in quantum Hall regime. The giant quantized GH effect manifests itself as an angular shift whose quantized step reaches the order of mrad for light beams impinging on a graphene-on-substrate system. The quantized GH effect can be attributed to quantized Hall conductivity, which corresponds to the discrete Landau levels in quantum Hall regime. We find that the quantized step can be greatly enhanced for incident angles near the Brewster angle. Moreover, the Brewster angle is sensitive to the Hall conductivity, and therefore the quantized GH effect can be modulated by the Fermi energy and the external magnetic field. The giant quantized GH effect offers a convenient way to determine the quantized Hall conductivity and the discrete Landau levels by a direct optical measurement.
description: 6 pages, 6 figures
Additional file 1 of Matrix methods in health demography: a new approach to the stochastic analysis of healthy longevity and DALYs
Creators: name: Caswell, Hal
name: Zarulli, Virginia
Publisher: name: figshare
Year: 2018
Subjects: subject: Space Science
subject: Medicine
subject: Sociology
subject: FOS: Sociology
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: 19999 Mathematical Sciences not elsewhere classified
subject: FOS: Mathematics

description: The second set of figures displays the age schedules of the same statistics of healthy longevity measured by grip strength, for each of the countries in the SHARE dataset. (PDF 384 kb)
Ferramenta da Terapia Centrada na Pessoa (TCP): Exploração de Expectativas Futuras
Creators: name: Brandl, Edenilson
Publisher: name: Zenodo
Year: 2024
Subjects: Ferramenta da Terapia Centrada na Pessoa (TCP)
Terapia Centrada na Pessoa (TCP)
Exploração de Expectativas Futuras
Enciclopédia da Conscienciologia

description: Definologia: A exploração de expectativas futuras é uma ferramenta da Terapia Centrada na Pessoa (TCP) que consiste na análise e investigação das projeções, desejos e metas que o cliente possui em relação ao seu futuro, visando compreender suas motivações, aspirações e possíveis obstáculos que possam surgir no processo de alcançar tais expectativas.
title: lhasa
Creators: name: Jacques, Guillaume
Publisher: name: COCOON - https://cocoon.huma-num.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2020
Subjects: subject: Japhug
subject: jya

description: Conforms to: doi:10.34847/cocoon.49aefa90-8c1f-3ba8-a099-0ebefc6a2aa7
Improved model of the triple system V746 Cas that has a bipolar magnetic field associated with the tertiary
Creators: name: Harmanec, P.
name: Brož, M.
name: Mayer, P.
name: Zasche, P.
name: Kotková, L.
name: Nemravová, J. A.
name: Dukes, R. J.
name: Korčáková, D.
name: Šlechta, M.
name: Kıran, E.
name: Kříček, R.
name: Juryšek, J.
Publisher: name: arXiv
Year: 2017
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: V746 Cas is known to be a triple system composed of a close binary with an alternatively reported period of either 25.4d or 27.8d and a third component in a 62000d orbit. The object was also reported to exhibit multiperiodic light variations with periods from 0.83d to 2.50d, on the basis of which it was classified as a slowly pulsating B star. Interest in further investigation of this system was raised by the detection of a variable magnetic field. Analysing spectra from four instruments, earlier published radial velocities, and several sets of photometric observations, we arrived at the following conclusions: (1) The optical spectrum is dominated by the lines of the B-type primary (Teff1~16500(100) K), contributing 70% of the light in the optical region, and a slightly cooler B tertiary (Teff3~13620(150) K). The lines of the low-mass secondary are below our detection threshold; we estimate that it could be a normal A or F star. (2) We resolved the ambiguity in the value of the inner binary period and arrived at a linear ephemeris of T_super.conj.=HJD 2443838.78(81)+25.41569(42)xE. (3) The intensity of the magnetic field undergoes a~sinusoidal variation in phase with one of the known photometric periods, namely 2.503867(19)d, which we identify with the rotational period of the tertiary. (4) The second photometric 1.0649524(40)d period is identified with the rotational period of the B-type primary, but this interpretation is much less certain and needs further verification. (5) If our interpretation of photometric periods is confirmed, the classification of the object as a slowly pulsating B star should be revised. (6) Applying an N-body model to different types of available observational data, we constrain the orbital inclination of the inner orbit to ~60 deg to 85 deg even in the absence of eclipses, and estimate the probable properties of the triple system and its components.
description: Accepted for publication in Astronomy and Astrophysics
title: ADCO, Cartulaire général de Cîteaux, dit de Jean de Cirey, (XVe siècle), tome VI, Cart. 190 (11 H 75), 316 folios, f. 0173r
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: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris
subject: Corpus Burgundiae Medii Aevi
subject: Chartes de la Bourgogne du Moyen Âge
subject: cartulaire

description: Cartulaire général de Cîteaux, dit de Jean de Cirey, (XVe siècle), tome VI, Archives départementales de la Côte-d'Or, Cart. 190 (11 H 75), 316 folios, f. 0173r, Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Cartulaire général de Cîteaux, dit de Jean de Cirey, (XVe siècle), tome VI, Archives départementales de la Côte-d'Or, Cart. 190 (11 H 75), 316 folios, f. 0173r, in Projet CBMA - Corpus Burgundiae Medii Aevi [Ressource en ligne], https:// manuscrits.cbma-project.eu/
description: Provenance: https://www.geonames.org/3024876
description: Provenance: http://www.idref.fr/030974844/id
description: Provenance: https://catalogue.bnf.fr/ark:/12148/cb12228351v
description: Provenance: abbaye de Cîteaux
description: Provenance: http://www.wikidata.org/entity/Q843261
Additional file 1: of Using Normalization Process Theory in feasibility studies and process evaluations of complex healthcare interventions: a systematic review
Creators: name: May, Carl
name: Cummings, Amanda
name: Girling, Melissa
name: Bracher, Mike
name: Mair, Frances
name: May, Christine
name: Murray, Elizabeth
name: Myall, Michelle
name: Rapley, Tim
name: Finch, Tracy
Publisher: name: figshare
Year: 2018
Subjects: subject: Space Science
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: 80699 Information Systems not elsewhere classified
subject: FOS: Computer and information sciences

description: Appendix data extraction tool. (PDF 156Â kb)
title: 01_0040
Creators: name: Wesley Baldwin, John
name: Baldwin, John W.
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2018
Subjects: subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris

description: L'ensemble de ces notes ont été crée par John Baldwin lors d'une de ses premières périodes de résidence à Paris. Ces documents comprennent tous les magistri qu’il avait pu rencontrer dans ses sources. Aux XIIème et XIIIème siècles, les universités n'existant pas encore, le titre de magister s'il évoque certainement une compétence n'est pas rattaché de façon systématique au passage par les écoles. De surcroît, les magistris sont le plus souvent désignés par leur seul prénom. La lecture de ces données est donc difficile et suppose un long travail pour tenter d'identifier un individu auquel on pourrait rattacher plusieurs mentions. John Baldwin avait donc renoncé à utiliser ces données pour donner un prolongement à sa magnifique étude sur les gradués d'université et leur emploi par les Capétiens et les Plantagenêts. Néanmoins, il a conservé ces données et elles sont potentiellement très utile dans le cadre de Studium, comme le sont toutes les mentions dans les volumes des Fasti Ecclesiae Gallicanae de chanoines portant ce titre de magister sans autres précisions. L'ampleur des dépouillements rend ces données très utiles et nous devons une grande reconnaissance à John Baldwin pour avoir pris la peine de faire photocopier ses fiches et de nous les avoir transmises amicalement.
Les données ainsi que les images des fiches sont accessibles sur le site Internet à l'adresse suivante : http://studium-baldwin.lamop.fr/.
Les transcriptions des fiches ont été effectuées par des étudiants de Paris 1 Panthéon - Sorbonne mais elles n'ont pas été corrigées par la suite.
description: Relation: https://lamop.hypotheses.org/
Discovery of a New Supernova Remnant in the Direction of G69.7+1.0
Creators: name: Yoshita, Kumi
name: Miyata, Emi
name: Tsunemi, Hiroshi
Publisher: name: arXiv
Year: 2000
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We discovered a middle-aged supernova remnant (SNR) in the vicinity of G69.7+1.0 using the ASCA satellite. G69.7+1.0 was identified in the 2.7 GHz survey and classified as a shell-type SNR with a diameter of 16 arcmin. During the ROSAT all-sky survey, the X-ray emission was detected in the direction of G69.7+1.0. However, it extends beyond the radio shell, and an X-ray bright region was located outside of the radio shell. A spectral study with the ASCA and ROSAT shows a thin thermal plasma with an electron temperature of ~0.4 keV. There is no significant variation of the spectral parameters over the field of view, except for the lower column density of the eastern part. We also found a large shell structure which surrounds the X-ray bright region in both optical and radio images. We suggest that the observed X-ray emission is associated with the large optical and radio shell, and that they are part of a new SNR, different from the radio SNR G69.7+1.0, which we have named AX J2001+3235 or G69.4+1.2. The large shell and the electron temperature of ~0.4 keV indicate that AX J2001+3235 is an evolved SNR. From a comparison with the column density of CTB 80 (G69.0+2.7), we estimate that the distance of the SNR is about 2.5 kpc.
description: Accepted for publication in PASJ, 9 pages, 5 figures
Additional file 3: of Description and characterization of a novel live-attenuated tri-segmented Machupo virus in Guinea pigs
Creators: name: Zaza, Amélie
name: Herbreteau, Cécile
name: Peyrefitte, Christophe
Publisher: name: figshare
Year: 2018
Subjects: subject: Medicine
subject: Ecology
subject: FOS: Biological sciences
subject: Immunology
subject: FOS: Clinical medicine
subject: 110309 Infectious Diseases
subject: FOS: Health sciences
subject: 60506 Virology

description: Survival rate and body weight of guinea pig inoculated with two doses of wt MACV. Four or five guinea pigs were infected intraperitoneally with 3 × 104 TCID50 (low dose) or 106 TCID50 (high dose) of wt MACV, respectively. The animals were observed for 24 days thereafter. (A) Their survival rate and (B) their weight were monitored. Animals infected with the high dose were heavier (515-610 g) than the ones used for the low dose experiment (250-300 g), explaining the differences of weight evolution between the two groups. (PDF 375 kb)
General Electric Quarterly Survey 69-04
Creators: name: Electric, General
Publisher: name: Roper Center for Public Opinion Research
Year: 2021

description: Most interested in, concerned about lately (1); local community interests (1); current and future race relations in United States (4); companies helping race relations (1); water pollution (3); transportation problem (3); air pollution (3); noise pollution (3); importance of various topics (10); local building approval (5); spending money (9); most important space developments (1); employment opportunities (2); chances of moving (1); moving for job opportunities (1); financial situation (2); price changes (1).
Gaia Data Release 1: The archive visualisation service
Creators: name: Moitinho, A.
name: Krone-Martins, A.
name: Savietto, H.
name: Barros, M.
name: Barata, C.
name: Falcão, A. J.
name: Fernandes, T.
name: Alves, J.
name: Silva, A. F.
name: Gomes, M.
name: Bakker, J.
name: Brown, A. G. A.
name: González-Núñez, J.
name: Gracia-Abril, G.
name: Gutiérrez-Sánchez, R.
name: Hernández, J.
name: Jordan, S.
name: Luri, X.
name: Merin, B.
name: Mignard, F.
name: Mora, A.
name: Navarro, V.
name: O'Mullane, W.
name: Sellés, T. Sagristà
name: Salgado, J.
name: Segovia, J. C.
name: Utrilla, E.
name: Arenou, F.
name: de Bruijne, J. H. J.
name: Jansen, F.
name: McCaughrean, M.
name: O'Flaherty, K. S.
name: Taylor, M. B.
name: Vallenari, A.
Publisher: name: arXiv
Year: 2017
Subjects: subject: Instrumentation and Methods for Astrophysics (astro-ph.IM)
subject: Astrophysics of Galaxies (astro-ph.GA)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: Context: The first Gaia data release (DR1) delivered a catalogue of astrometry and photometry for over a billion astronomical sources. Within the panoply of methods used for data exploration, visualisation is often the starting point and even the guiding reference for scientific thought. However, this is a volume of data that cannot be efficiently explored using traditional tools, techniques, and habits. Aims: We aim to provide a global visual exploration service for the Gaia archive, something that is not possible out of the box for most people. The service has two main goals. The first is to provide a software platform for interactive visual exploration of the archive contents, using common personal computers and mobile devices available to most users. The second aim is to produce intelligible and appealing visual representations of the enormous information content of the archive. Methods: The interactive exploration service follows a client-server design. The server runs close to the data, at the archive, and is responsible for hiding as far as possible the complexity and volume of the Gaia data from the client. This is achieved by serving visual detail on demand. Levels of detail are pre-computed using data aggregation and subsampling techniques. For DR1, the client is a web application that provides an interactive multi-panel visualisation workspace as well as a graphical user interface. Results: The Gaia archive Visualisation Service offers a web-based multi-panel interactive visualisation desktop in a browser tab. It currently provides highly configurable 1D histograms and 2D scatter plots of Gaia DR1 and the Tycho-Gaia Astrometric Solution (TGAS) with linked views. An innovative feature is the creation of ADQL queries from visually defined regions in plots. [abridged]
description: 16 pages, 9 figures, accepted for publication in Astronomy & Astrophysics. Abstract abridged for arXiv submission. The service and image gallery here described are accessible from the Gaia archive "visualization" tab at http://gea.esac.esa.int/archive/
title: riquet7-v2
Creators: name: Jacques, Guillaume
Publisher: name: COCOON - https://cocoon.huma-num.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2020
Subjects: subject: Japhug
subject: jya

description: Conforms to: doi:10.34847/cocoon.49aefa90-8c1f-3ba8-a099-0ebefc6a2aa7
Lettre de Alexandre-Xavier Panel à Jean-François Séguier, 1729-07-21
Creators: name: Panel, Alexandre-Xavier
name: Alexandre-Xavier Panel
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2021
Subjects: Numismatique

description: [transcription] Monsieur,

c'est avec regret que j'ay laissé partir M. Novy sans lui remettre ma lettre, et même sans avoir eu l'honneur de le voir dans son logis. Il m'avait dit que son séjour en cette ville serait de plusieurs jours, sur quoi j'avais compté d'être à temps de lui rendre une visite jeudi, c'est-à-dire aujourd'hui. J'ai été frustré de mon attente, son départ a été plus prompt qu'il ne le comptait lui-même, comme il m'a fait l'honneur de me le dire.

La condition que vous mettez dans l'échange de vos médailles est trop onéreuse. A la place du Gordien Pie, vous demandez un Auguste grand bronze, c'est-à-dire une médaille de 15 à 20 lt., car on en trouve pas au dessous de ce prix à Rome d'où j'ai fait venir la plupart de celles que j'ai. Je vous avais proposé d'ailleurs en échange six médailles; vous ne m'en avez envoyé que cinq. La Pomponia s'est trouvée à redire [fol. 42 v] mais quand même vous m'auriez envoyé cette consulaire, et, que les autres seraient à fleur de coin, toutes ensembles elles n'égaleraient jamais un Auguste. Ainsi, comme l'échange que j'avais eu l'honneur de vous proposer ne vous convient pas, et que je ne puis admettre la condition que vous exigez, j'ai pris le parti qui m'a paru le plus sage, c'est de vous les renvoyer. Une autrefois, je serai sans doute plus heureux. La difficulté d'avoir le Justinien d'or m'est un motif assez pressant pour ne pas y penser. Peut-être qu'après vous être donné bien de la peine pour l'acquérir, vous n'en viendrez pas à bout puisque comme vous me le marquez le possesseur ne veut pas s'en défaire. Après tout, les médailles de cet empereur sont plus communes en ce métal qu'en aucun autre. J'ai l'honneur d'être avec respect,

Monsieur,

Votre très humble et très obéissant serviteur

Panel, jésuite.

Avignon, 21 juillet 1729.
description: [personnes citées] Raymond Novi de Caveirac
description: Source: [lieu de Conservation] Nîmes, Bibliothèque Carré d'Art [cote]ms. 147_4, fol. 42
description: Source: ark:/12148/btv1b100152922
Finding the Needles in the Haystacks: High-Fidelity Models of the Modern and Archean Solar System for Simulating Exoplanet Observations
Creators: name: Roberge, Aki
name: Rizzo, Maxime J.
name: Lincowski, Andrew P.
name: Arney, Giada N.
name: Stark, Christopher C.
name: Robinson, Tyler D.
name: Snyder, Gregory F.
name: Pueyo, Laurent
name: Zimmerman, Neil T.
name: Jansen, Tiffany
name: Nesvold, Erika R.
name: Meadows, Victoria S.
name: Turnbull, Margaret C.
Publisher: name: arXiv
Year: 2017
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: FOS: Physical sciences

description: We present two state-of-the-art models of the solar system, one corresponding to the present day and one to the Archean Eon 3.5 billion years ago. Each model contains spatial and spectral information for the star, the planets, and the interplanetary dust, extending to 50 AU from the sun and covering the wavelength range 0.3 to 2.5 micron. In addition, we created a spectral image cube representative of the astronomical backgrounds that will be seen behind deep observations of extrasolar planetary systems, including galaxies and Milky Way stars. These models are intended as inputs to high-fidelity simulations of direct observations of exoplanetary systems using telescopes equipped with high-contrast capability. They will help improve the realism of observation and instrument parameters that are required inputs to statistical observatory yield calculations, as well as guide development of post-processing algorithms for telescopes capable of directly imaging Earth-like planets.
description: Accepted for publication in PASP
Energy cost of entanglement extraction in complex quantum systems
Creators: name: Beny, Cedric
name: Chubb, Christopher T.
name: Farrelly, Terry
name: Osborne, Tobias J.
Publisher: name: arXiv
Year: 2017
Subjects: subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: What is the energy cost of extracting entanglement from complex quantum systems? In other words, given a state of a quantum system, how much energy does it cost to extract m EPR pairs? This is an important question, particularly for quantum field theories where the vacuum is generally highly entangled. Here we build a theory to understand the energy cost of entanglement extraction. First, we apply it to a toy model, and then we define the entanglement temperature, which relates the energy cost to the amount of extracted entanglement. Next, we give a physical argument to find the energy cost of entanglement extraction in some condensed matter and quantum field systems. The energy cost for those quantum field theories depends on the spatial dimension, and in one dimension, for example, it grows exponentially with the number of EPR pairs extracted. Next, we outline some approaches for bounding the energy cost of extracting entanglement in general quantum systems. Finally, we look at the antiferromagnetic Heisenberg and transverse field Ising models numerically to calculate the entanglement temperature using matrix product states.
description: 10 pages (8 for main text and 2 for appendices); 4 figures
Single-mode heat conduction by photons
Creators: name: Meschke, M.
name: Guichard, W.
name: Pekola, J. P.
Publisher: name: arXiv
Year: 2006
Subjects: subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: FOS: Physical sciences

description: Electrical conductance is quantized in units of $σ_{\rm Q}=2e^2/h$ in ballistic one-dimensional conductors. Similarly, thermal conductance at temperature $T$ is expected to be limited by the quantum of thermal conductance of one mode, $G_{\rm Q} = \frac{πk_{\rm B}^2}{6\hbar}T$, when physical dimensions are small in comparison to characteristic wavelength of the carriers. The relation between $σ_{\rm Q}$ and $G_{\rm Q}$ obeys the Wiedemann-Franz law for ballistic electrons (apart from factor 2 in $σ_{\rm Q}$ due to spin degeneracy), but somewhat amazingly the same expression of $G_{\rm Q}$ is expected to hold also for phonons and photons, or any other particles with arbitrary exclusion statistics. The single-mode heat conductance is particularly relevant in nano-structures, e.g., when studying heat conduction by phonons in dielectric materials, or cooling of electrons in metals at very low temperatures. Here we show, based on our experimental results, that at low temperatures heat is transferred by photon radiation, in our case along a superconducting line, when electron-phonon as well as normal electronic heat conduction are frozen out. Thermal conductance is limited by $G_{\rm Q}$, approaching this value towards low temperatures. Our observation has implications on, e.g., performance and design of ultra-sensitive bolometers and electronic micro-refrigerators, whose operation is largely dependent on weak thermal coupling between the device and its environment.
description: 5 pages, 3 figures