cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Random Frustration in two-dimensional spin-1/2 Heisenberg antiferromagnet
Creators: name: Rodriguez, J. P.
name: Bonca, J.
name: Ferrer, J.
Publisher: name: arXiv
Year: 1994
Subjects: subject: Condensed Matter (cond-mat)
subject: FOS: Physical sciences

description: The square lattice spin-1/2 antiferromagnet containing a dilute concentration, $δ$, of randomly placed ferromagnetic nearest-neighbor bonds is studied at low-temperature via non-linear $σ$-model techniques and by exact diagonalization. We generally find that long-range N\' eel order is destroyed above a critical strength in the defective ferromagnetic exchange coupling-constant given by $|K_c|/J\sim δ^{-1/2}$. We also observe large statistical fluctuations both in the spin-stiffness and in the antiferromagnetic structure-factor near this critical point, suggesting the onset of a spin-glass phase.
description: 13 pgs, TeX, submitted to Phys. Rev. Feb. 22, 1994. (Correct set of figures follow)
Centaurus A: multiple outbursts or bursting bubble?
Creators: name: Morganti, R.
name: Killeen, N. E. B.
name: Ekers, R. D.
name: Oosterloo, T. A.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present new radio observations of the brighter region of the northern lobe (the Northern Middle Lobe, NML) of Centaurus A obtained at 20 cm with the Australia Telescope Compact Array. The angular resolutions are ~50 and ~130 arcsec, therefore much higher than for the previously available radio images of this region. The most interesting feature detected is a large-scale jet that connects the inner radio lobe and the NML and that is imaged for the first time. The NML itself appears as diffuse emission with a relatively bright ridge on the eastern side. The radio morphology of Centaurus A and, in particular, its NML could be the result of a precessing jet that has undergone a strong interaction with the environment at least in the northern side. The very big drop in intensity between the inner jet and the large-scale jet can be explained with a sequence of bursts of activity at different epochs in the life of the source. Alternatively (or additionally) a ``bursting bubble'' model is proposed which could also explain the good collimation of the large-scale jet. In this model, the plasma accumulated in the inner lobe would be able to ``burst'' out only through one nozzle that would be the region where the large-scale jet forms. From the comparison between the radio emission and the regions of ionized gas we find that the inner optical filament falls about 2 arcmin (~2 kpc) away from the large-scale radio jet. Thus, this filament does not seem to have experienced a direct interaction with the radio plasma. The outer filaments appear to be, in projection, closer to the radio emission, arguing for a direct interaction with the radio jet. However, also in this case a more complicated interaction than assumed so far has to be occuring.
description: To appear in MNRAS; 11 pages, LateX, 7 figures. Fig 1 is available at http://www.ira.bo.cnr.it/~rmorgant/CentaurusA
J plots: a new method for characterizing structures in the interstellar medium
Creators: name: Jaffa, S. E.
name: Whitworth, A. P.
name: Clarke, S. D.
name: Howard, A. D. P.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: Large scale surveys have brought about a revolution in astronomy. To analyse the resulting wealth of data, we need automated tools to identify, classify, and quantify the important underlying structures. We present here a method for classifying and quantifying a pixelated structure, based on its principal moments of inertia. The method enables us to automatically detect, and objectively compare, centrally condensed cores, elongated filaments and hollow rings. We illustrate the method by applying it to (i) observations of surface-density from Hi-GAL, and (ii) simulations of filament growth in a turbulent medium. We limit the discussion here to 2D data; in a future paper we will extend the method to 3D data.
description: 10 pages, 9 figures
Protocol : Implementation of Thermal Infrared Camera for Non-Contact Physiological Measurement A Systematic Review
Creators: name: Manullang, Martin Clinton Tosima
Publisher: name: figshare
Year: 2021
Subjects: subject: 90303 Biomedical Instrumentation
subject: FOS: Medical engineering
subject: 90399 Biomedical Engineering not elsewhere classified
subject: 90699 Electrical and Electronic Engineering not elsewhere classified
subject: FOS: Electrical engineering, electronic engineering, information engineering

description: This is a protocol for prisma systematic literature review
Gravitational instability caused by the weight of heat
Creators: name: Roupas, Zacharias
Publisher: name: arXiv
Year: 2018
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: Statistical Mechanics (cond-mat.stat-mech)
subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: Thermal energy points toward a disordered, completely uniform state acting counter to gravity's tendency to generate order and structure through gravitational collapse. It is, therefore, expected to contribute to the stabilization of a self-gravitating, classical ideal gas over collapse. However, I identified an instability that always occurs at sufficiently high energies: the high-energy or relativistic gravothermal instability. I argue here that this instability presents an analogous core--halo structure as its Newtonian counterpart, the Antonov instability. The main difference is that in the former case the core is dominated by the gravitation of thermal energy and not rest mass energy. A relativistic generalization of Antonov's instability---the low-energy gravothermal instability---also occurs. The two turning points, which make themselves evident as a double spiral of the caloric curve, approach each other as relativistic effects become more intense and eventually merge in a single point. Thus, the high and low-energy cases may be realized as two aspects of a single phenomenon---the gravothermal instability---which involves a core--halo separation and an intrinsic heat flow. Finally, I argue that the core formed during a core-collapse supernova is subject to the relativistic gravothermal instability if it becomes sufficiently hot and compactified at the time of the bounce. In this case, it will continue to collapse towards the formation of a black hole.
description: Typos corrected in last update
Additional file 1: of Assessment of effectiveness and safety of repeat administration of proinflammatory primed allogeneic mesenchymal stem cells in an equine model of chemically induced osteoarthritis
Creators: name: Barrachina, Laura
name: Remacha, Ana
name: Romero, Antonio
name: Vitoria, Arantza
name: Albareda, Jorge
name: Prades, Marta
name: Roca, Mercedes
name: Zaragoza, Pilar
name: VĂĄzquez, Francisco
name: Rodellar, Clementina
Publisher: name: figshare
Year: 2018
Subjects: subject: Genetics
subject: FOS: Biological sciences
subject: Evolutionary Biology
subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences
subject: Ecology
subject: 69999 Biological Sciences not elsewhere classified
subject: Developmental Biology
subject: Science Policy
subject: Hematology

description: Schematic representation of the study design. (DOCX 62Â kb)
Vespa rufa Linnaeus, 1758, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1758
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hymenoptera
Vespidae
Vespa
Vespa rufa

description: Vespa rufa [spec. nov.]
V. thorace lineolis punctisque duobus flavis, abdomine flavo antice ferrugineo.
Fn. svec. 998.
Reaum. ins. 6. t. 14?
Habitat in Europa.
description: Published as part of Linnaeus, Carolus, 1758, Systema Naturae per regna tria naturae: secundum classes, ordines, genera, species, cum characteribus, differentiis, synonymis, locis, Stockholm :Laurentius Salvius on page 572, DOI: 10.5962/bhl.title.542, http://zenodo.org/record/3922206
Effect of a Voltage Probe on the Phase-Coherent Conductance of a Ballistic Chaotic Cavity
Creators: name: Brouwer, P. W.
name: Beenakker, C. W. J.
Publisher: name: arXiv
Year: 1994
Subjects: subject: Condensed Matter (cond-mat)
subject: FOS: Physical sciences

description: The effect of an invasive voltage probe on the phase-coherent conduction through a ballistic chaotic cavity is investigated by random-matrix theory. The entire distribution P(G) of the conductance G is computed for the case that the cavity is coupled to source and drain by two point contacts with a quantized conductance of 2 e^2/h, both in the presence (beta = 1) and absence (beta = 2) of time-reversal symmetry. The loss of phase-coherence induced by the voltage probe causes a crossover from P(G) ~ G^(-1 + beta/2) to a Gaussian centered at G = e^2/h with a beta-dependent width. ***Submitted to Physical Review B.***
description: 9 pages, REVTeX-3.0, 4 postscript figures appended as self-extracting archive, INLO-PUB-941020b
Women's Candidacy and the Power of Incumbency in the 2019 Solomon Islands Election
Creators: name: Baker, Kerryn
Publisher: name: Canberra, ACT: Dept. of Pacific Affairs, Research School of Pacific and Asian Studies, The Australian National University
Year: 2019

description: The 2019 Solomon Islands election marked the first time in the country’s history that two women were elected to parliament in a general election. Lanelle Tanangada, who had been elected in the 2018 by-election for the Gizo/Kolombangara seat formerly held by her husband, fended off another strong challenge from former prime minister Gordon Darcy Lilo to keep the seat. Freda Tuki Soriacomua, who won the Temotu Vatud seat in 2014 but was removed from office in 2018 following a court challenge, regained her seat in 2019. While this is a milestone, the under-representation of women in Solomon Islands politics is a continued tradition. As of October 2019, women make up just 4% of members of the national parliament, and around 2% of provincial assembly members. This In Brief examines trends and patterns from the 2019 Solomon Islands election and their effect on women’s representation.
Artificial intelligence-based model for dose prediction of sertraline in adolescents: a real-world study
Creators: name: Fu, Ran
name: Yu, Ze
name: Zhou, Chunhua
name: Zhang, Jinyuan
name: Gao, Fei
name: Wang, Donghan
name: Hao, Xin
name: Pang, Xiaolu
name: Yu, Jing
Publisher: name: Taylor & Francis
Year: 2024
Subjects: subject: Biochemistry
subject: Medicine
subject: Microbiology
subject: FOS: Biological sciences
subject: Pharmacology
subject: Biotechnology
subject: Biological Sciences not elsewhere classified
subject: Mental Health
subject: Plant Biology

description: Variability exists in sertraline pharmacokinetic parameters in individuals, especially obvious in adolescents. We aimed to establish an individualized dosing model of sertraline for adolescents with depression based on artificial intelligence (AI) techniques. Data were collected from 258 adolescent patients treated at the First Hospital of Hebei Medical University between December 2019 to July 2022. Nine different algorithms were used for modeling to compare the prediction abilities on sertraline daily dose, including XGBoost, LGBM, CatBoost, GBDT, SVM, ANN, TabNet, KNN, and DT. Performance of four dose subgroups (50 mg, 100 mg, 150 mg, and 200 mg) were analyzed. CatBoost was chosen to establish the individualized medication model with the best performance. Six important variables were found to be correlated with sertraline dose, including plasma concentration, PLT, MPV, GL, A/G, and LDH. The ROC curve and confusion matrix exhibited the good prediction performance of CatBoost model in four dose subgroups (the AUC of 50 mg, 100 mg, 150 mg, and 200 mg were 0.93, 0.81, 0.93, and 0.93, respectively). The AI-based dose prediction model of sertraline in adolescents with depression had a good prediction ability, which provides guidance for clinicians to propose the optimal medication regimen.
Liquid-vapour asymmetry in pure fluids: A Monte Carlo simulation study
Creators: name: Wilding, Nigel B.
name: Mueller, Marcus
Publisher: name: arXiv
Year: 1994
Subjects: subject: Condensed Matter (cond-mat)
subject: FOS: Physical sciences

description: Monte Carlo simulations within the grand canonical ensemble are used to obtain the joint distribution of density and energy fluctuations $p_L(ρ,u)$ for two model fluids: a decorated lattice gas and a polymer system. In the near critical region the form of $p_L(ρ,u)$ is analysed using a mixed field finite-size-scaling theory that takes account of liquid-vapour asymmetry. Field mixing transformations are performed that map $p_L(ρ,u)$ onto the joint distribution of critical scaling operators \ptMEstar\ appropriate to the Ising fixed point. Carrying out this procedure permits a very accurate determination of the critical point parameters. By forming various projections of \ptMEstar , the full universal finite-size spectrum of the critical density and energy distributions of fluids is also obtained. In the sub-critical coexistence region, an examination is made of the influence of field mixing on the asymmetry of the density distribution.
description: 19 pages Latex, 15 Figures available on request. Report Number #IP-94.153
Learning from Richer Human Guidance: Augmenting Comparison-Based Learning with Feature Queries
Creators: name: Basu, Chandrayee
name: Singhal, Mukesh
name: Dragan, Anca D.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Artificial Intelligence (cs.AI)
subject: FOS: Computer and information sciences

description: We focus on learning the desired objective function for a robot. Although trajectory demonstrations can be very informative of the desired objective, they can also be difficult for users to provide. Answers to comparison queries, asking which of two trajectories is preferable, are much easier for users, and have emerged as an effective alternative. Unfortunately, comparisons are far less informative. We propose that there is much richer information that users can easily provide and that robots ought to leverage. We focus on augmenting comparisons with feature queries, and introduce a unified formalism for treating all answers as observations about the true desired reward. We derive an active query selection algorithm, and test these queries in simulation and on real users. We find that richer, feature-augmented queries can extract more information faster, leading to robots that better match user preferences in their behavior.
description: 8 pages, 8 figures, HRI 2018
Vespa cribraria Linnaeus, 1758, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1758
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hymenoptera
Vespidae
Vespa
Vespa cribraria

description: Vespa cribraria [spec. nov.]
V. nigra, abdomine fasciis sex flavis: intermediis tribus interruptis, tibiis anticis clypeis cribriformibus.
Raj. ins. 255. Vespa ichneumon pedibus anterioribus velut clypeatis.
Roland. Act. Stockh. 1751. p. 56. t. 3. f. 1.
Uddm. diss. 94. Apis tibiis anticis lamella cribriformi.
Habitat in Europa.
description: Published as part of Linnaeus, Carolus, 1758, Systema Naturae per regna tria naturae: secundum classes, ordines, genera, species, cum characteribus, differentiis, synonymis, locis, Stockholm :Laurentius Salvius on page 573, DOI: 10.5962/bhl.title.542, http://zenodo.org/record/3922206
title: ADCO, Cinquième cartulaire de Saint-Étienne de Dijon (1664), Cart. 28 (G 132), 258 folios, f. 00169
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: cartulaire
subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris
subject: Corpus Burgundiae Medii Aevi
subject: Chartes de la Bourgogne du Moyen Âge

description: Cinquième cartulaire de Saint-Étienne de Dijon (1664), Archives départementales de la Côte-d'Or, Cart. 28 (G 132), 258 folios, f. 00169, Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Cinquième cartulaire de Saint-Étienne de Dijon (1664), Archives départementales de la Côte-d'Or, Cart. 28 (G 132), 258 folios, f. 00169, 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
Galactic chemical evolution of heavy elements: from Barium to Europium
Creators: name: Travaglio, C.
name: Galli, D.
name: Gallino, R.
name: Busso, M.
name: Ferrini, F.
name: Straniero, O.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We follow the chemical evolution of the Galaxy for elements from Ba to Eu, using an evolutionary model suitable to reproduce a large set of Galactic (local and non local) and extragalactic constraints. Input stellar yields for neutron-rich nuclei have been separated into their s-process and r-process components. The production of s-process elements in thermally pulsing asymptotic giant branch stars of low mass proceeds from the combined operation of two neutron sources: the dominant reaction 13C(alpha,n)16O, which releases neutrons in radiative conditions during the interpulse phase, and the reaction 22Ne(alpha,n)25Mg, marginally activated during thermal instabilities. The resulting s-process distribution is strongly dependent on the stellar metallicity. For the standard model discussed in this paper, it shows a sharp production of the Ba-peak elements around Z = Z_sun/4. Concerning the r-process yields, we assume that the production of r-nuclei is a primary process occurring in stars near the lowest mass limit for Type II supernova progenitors. The r-contribution to each nucleus is computed as the difference between its solar abundance and its s-contribution given by the Galactic chemical evolution model at the epoch of the solar system formation. We compare our results with spectroscopic abundances of elements from Ba to Eu at various metallicities (mainly from F and G stars) showing that the observed trends can be understood in the light of the present knowledge of neutron capture nucleosynthesis. Finally, we discuss a number of emerging features that deserve further scrutiny.
description: 34 pages, 13 figures. accepted by ApJ
Scaling of polarization amplitude in quantum many-body systems in one dimension
Creators: name: Kobayashi, Ryohei
name: Nakagawa, Yuya O.
name: Fukusumi, Yoshiki
name: Oshikawa, Masaki
Publisher: name: arXiv
Year: 2018
Subjects: subject: Statistical Mechanics (cond-mat.stat-mech)
subject: FOS: Physical sciences

description: Resta proposed a definition of the electric polarization in one-dimensional systems in terms of the ground-state expectation value of the large gauge transformation operator. Vanishing of the expectation value in the thermodynamic limit implies that the system is a conductor. We study Resta's polarization amplitude (expectation value) in the $S=1/2$ XXZ chain and its several generalizations, in the gapless conducting Tomonaga-Luttinger Liquid phase. We obtain an analytical expression in the lowest-order perturbation theory about the free fermion point (XY chain), and an exact result for the Haldane-Shastry model with long-range interactions. We also obtain numerical results, mostly using the exact diagonalization method. We find that the amplitude exhibits a power-law scaling in the system size (chain length) and vanishes in the thermodynamic limit. On the other hand, the exponent depends on the model even when the low-energy limit is described by the Tomonaga-Luttinger Liquid with the same Luttinger parameter. We find that a change in the exponent occurs when the Umklapp term(s) are eliminated, suggesting the importance of the Umklapp terms.
description: 30 pages, 3 figures
Additional file 3: of Chest radiography versus lung ultrasound for identification of acute respiratory distress syndrome: a retrospective observational study
Creators: name: See, Kay
name: Ong, Venetia
name: Tan, Yi
name: Sahagun, Juliet
name: Juvel Taculod
Publisher: name: figshare
Year: 2018
Subjects: subject: Space Science
subject: Medicine
subject: Cell Biology
subject: Sociology
subject: FOS: Sociology
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: Developmental Biology
subject: 60506 Virology

description: Table S3. Comparative analysis using lung ultrasound findings for ARDS identification. (DOCX 23 kb)
Unwinding Scaling Violations in Phase Ordering
Creators: name: Rutenberg, A. D.
name: Bray, A. J.
Publisher: name: arXiv
Year: 1994
Subjects: subject: Condensed Matter (cond-mat)
subject: FOS: Physical sciences

description: The one-dimensional $O(2)$ model is the simplest example of a system with topological textures. The model exhibits anomalous ordering dynamics due to the appearance of two characteristic length scales: the phase coherence length, $L \sim t^{1/z}$, and the phase winding length, $L_{w} \sim L^χ$. We derive the scaling law $z=2+μχ$, where $μ=0$ ($μ=2$) for nonconserved (conserved) dynamics and $χ=1/2$ for uncorrelated initial orientations. From hard-spin equations of motion, we consider the evolution of the topological defect density and recover a simple scaling description. (please email ar@v2.ph.man.ac.uk for a hard copy by mail)
description: 4 pages, LATeX, uuencoded figure file appended: needs epsf.sty, [resubmitted since postscript version did not work well], M/C.TH.94/21,NI94022
Compactness of molecular reaction paths in quantum mechanics
Creators: name: Anapolitanos, Ioannis
name: Lewin, Mathieu
Publisher: name: arXiv
Year: 2018
Subjects: subject: Mathematical Physics (math-ph)
subject: Analysis of PDEs (math.AP)
subject: Spectral Theory (math.SP)
subject: FOS: Physical sciences
subject: FOS: Mathematics

description: We study isomerizations in quantum mechanics. We consider a neutral molecule composed of N quantum electrons and M classical nuclei and assume that the first eigenvalue of the corresponding N-particle Schrödinger operator possesses two local minima with respect to the locations of the nuclei. An isomerization is a mountain pass problem between these two local configurations, where one minimizes over all possible paths the highest value of the energy along the paths. Here we state a conjecture about the compactness of min-maxing sequences of such paths, which we then partly solve in the particular case of a molecule composed of two rigid sub-molecules that can move freely in space. More precisely, under appropriate assumptions on the multipoles of the two molecules, we are able to prove that the distance between them stays bounded during the whole chemical reaction. We obtain a critical point at the mountain pass level, which is called a transition state in chemistry. Our method requires to study the critical points and the Morse indices of the classical multipole interactions, as well as to improve existing results about the van der Waals force. This paper generalizes previous works by the second author in several directions.
description: Final version to appear in Arch. Rat. Mech. Anal
The Pacific Islands Forum Fisheries Agency: 40 Years of Successful Regional Cooperation
Creators: name: Aqorau, Transform
name: Sokimi (Jnr), William
Publisher: name: Canberra, ACT: Dept. of Pacific Affairs, Research School of Pacific and Asian Studies, The Australian National University
Year: 2019

description: The fortieth anniversary of the Pacific Islands Forum’s most successful initiative went unnoticed by Forum leaders at their meeting in Tuvalu in early August. The Pacific Islands Forum Fisheries Agency (FFA) turned 40 on 8 August, a milestone in regional fisheries cooperation. Fisheries is a standing agenda item at the annual Forum leaders’ meeting, reflecting its economic importance to Pacific Island countries (PICs). The FFA is the focal point for the coordination of fisheries policies, and supported the Parties to the Nauru Agreement (PNA)1 until the PNA established a secretariat in 2010. The FFA laid the initial foundations for PICs to exercise their fishing rights, thereby creating the environment that has allowed PNA members to assert their rights through the Vessel Day Scheme (VDS) and dramatically increase revenue from their tuna in the past five years. The establishment of the PNA office in 2010 has tested the utility of the FFA, and questions are being asked if it is still an effective forum for the coordination of policies to manage the region’s tropical tuna fisheries.
Additional file 1 of Joint deep learning for batch effect removal and classification toward MALDI MS based metabolomics
Creators: name: Niu, Jingyang
name: Yang, Jing
name: Guo, Yuyu
name: Qian, Kun
name: Wang, Qian
Publisher: name: figshare
Year: 2022
Subjects: subject: Space Science
subject: Genetics
subject: FOS: Biological sciences
subject: Biotechnology
subject: Biological Sciences not elsewhere classified
subject: Mathematical Sciences not elsewhere classified
subject: Science Policy

description: Additional file 1: Implementation details and supplementary results.
Restreindre l'Aide médicale d'État, une aberration sanitaire et économique ?
Creators: name: Liebart, Deborah
Publisher: name: Zenodo
Year: 2019
Subjects: aide médicale d'Etat, PUMA, CSS, CMU-C, aberration économique et sanitaire, système de soin, Etat Providence, épidémies, tuberculose, rougeole, solidarité

description: Alors que le nouveau Plan Immigration vient d’être dévoilé le 6 novembre dernier, je voudrais m’arrêter sur les modifications apportées à l’Aide médicale d’État (AME). Parfois présenté comme l’incarnation du laxisme français à l’égard de l’immigration clandestine, parfois présenté comme la porte ouverte au « tourisme médical », ce dispositif est destiné à prendre en charge les dépenses de santé des étrangers sans papiers vivant sur le territoire national. Le mythe du « tourisme médical du migrant » est un levier puissant des discours identitaires contemporains, bien que bien marginal au regard des études de Médecins du Monde : seulement 3 % des sans papiers citent la santé comme motif de migration, et 85 % des patients pris en charge par l’association et éligibles au dispositif ignorent jusqu’à son existence. L’AME, au-delà du soin individuel, représente un véritable dispositif de santé publique, l’une des sentinelles de la veille sanitaire nationale protégeant la société dans son ensemble. Au delà et contrairement au discours actuellement répandu, l’AME pourrait bien représenter une économie sur le budget total dédié au soin. Regardons de plus près.
Constraining Curvature Parameters via Topology
Creators: name: Roukema, Boudewijn F.
name: Luminet, Jean-Pierre
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: If the assumption that physical space has a trivial topology is dropped, then the Universe may be described by a multiply connected Friedmann-Lema\^ıtre model on a sub-horizon scale. Specific candidates for the multiply connected space manifold have already been suggested. How precisely would a significant detection of multiple topological images of a single object, or a region on the cosmic microwave background, (due to photons arriving at the observer by multiple paths which have crossed the Universe in different directions), constrain the values of the curvature parameters $Ω_0$ and $λ_0$? The way that the constraints on $Ω_0$ and $λ_0$ depend on the redshifts of multiple topological images and on their radial and tangential separations is presented and calculated. The tangential separations give the tighter constraints: multiple topological images of known types of astrophysical objects at redshifts $z \ltapprox 3$ would imply values of $Ω_0$ and $λ_0$ preciser than $\sim 1%$ and $\sim 10%$ respectively. Cosmic microwave background `spots' identified with lower redshift objects by the Planck or MAP satellites would provide similar precision. This method is purely geometrical: no dynamical assumptions (such as the virial theorem) are required and the constraints are independent of the Hubble constant, $H_0.$
description: 10 pages, 4 figures, accepted for Astronomy & Astrophysics; revised version - quantum epoch topology evolution reference added
title: Финансы
title: Учебное пособие
titleType: Subtitle
Creators: name: Дмитриева И.Е.
name:  Ярошенко Е.А.
Publisher: name: Ай Пи Ар Медиа
Year: 2020

description: Учебное пособие содержит информацию о сущности и функциях финансов, финансовой политике, управлении финансами, бюджетном устройстве в Российской Федерации, доходах и расходах бюджетов, государственных внебюджетных фондах и иные темы, предусмотренные программой дисциплины, а также практические задания. Подготовлено в соответствии с требованиями Федерального государственного образовательного стандарта высшего образования. Учебное пособие предназначено для изучения дисциплин «Финансы», «Финансы и кредит» по укрупненной группе специальностей и направлений подготовки 38.00.00 «Экономика и управление», а также будет полезно аспирантам, преподавателям, практическим работникам сферы финансов.
Coalescence driven self-organization of growing nanodroplets around a microcap
Creators: name: Dyett, Brendan
name: Hao, Hao
name: Lohse, Detlef
name: Zhang, Xuehua
Publisher: name: arXiv
Year: 2018
Subjects: subject: Soft Condensed Matter (cond-mat.soft)
subject: FOS: Physical sciences

description: The coalescence between growing droplets is important for the surface coverage and spatial arrangements of droplets on surfaces. In this work, total internal reflection fluorescence (TIRF) microscopy is utilized to in-situ investigate the formation of nanodroplets around the rim of a polymer microcap, with sub-micron spatial and millisecond temporal resolution. We observe that the coalescence among droplets occurs frequently during their growth by solvent exchange. Our experimental results show that the position of the droplet from two merged droplets is related to the size of the parent droplets. The position of the coalesced droplet and the ratio of parent droplet sizes obey a scaling law, reflecting a coalescence preference based on the size inequality. As a result of droplet coalescence, the angles between the centroids of two neighbouring droplets increase with time, obeying a nearly symmetrical arrangement of droplets at various time intervals. The evolution of the position and number from coalescence of growing droplets is modelled. The mechanism for coalescence driven self-organization of growing droplets is general, applicable to microcaps of different sizes and droplets of different liquids. The understanding from this work may be valuable for positioning nanodroplets by nucleation and growth without using templates.
description: 10 pages, 9 figures
The Spectral Correlation Function -- A New Tool for Analyzing Spectral-Line Maps
Creators: name: Rosolowsky, Erik W.
name: Goodman, Alyssa A.
name: Wilner, David J.
name: Williams, Jonathan P.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: The "spectral correlation function" analysis we introduce in this paper is a new tool for analyzing spectral-line data cubes. Our initial tests, carried out on a suite of observed and simulated data cubes, indicate that the spectral correlation function [SCF] is likely to be a more discriminating statistic than other statistical methods normally applied. The SCF is a measure of similarity between neighboring spectra in the data cube. When the SCF is used to compare a data cube consisting of spectral-line observations of the ISM with a data cube derived from MHD simulations of molecular clouds, it can find differences that are not found by other analyses. The initial results presented here suggest that the inclusion of self-gravity in numerical simulations is critical for reproducing the correlation behavior of spectra in star-forming molecular clouds.
description: 29 pages, including 4 figures (tar file submitted as source) See also: http://cfa-www.harvard.edu/~agoodman/scf/velocity_methods.html
Vespa rupestris Linnaeus, 1758, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1758
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hymenoptera
Vespidae
Vespa
Vespa rupestris

description: Vespa rupestris [spec. nov.]
V. abdominis segmento secundo majore maculis duabus ovatis albidis, pedibus antennisque ferrugineis.
Habitat ad Lapidum latera australia, nidum ex fistulis aggregatis conficiens. Rolander.
description: Published as part of Linnaeus, Carolus, 1758, Systema Naturae per regna tria naturae: secundum classes, ordines, genera, species, cum characteribus, differentiis, synonymis, locis, Stockholm :Laurentius Salvius on page 573, DOI: 10.5962/bhl.title.542, http://zenodo.org/record/3922206
ANALGETIK-ANTIPIRETIK GURUHIGA KIRIVCHI PREPARATLARNING ASSORTIMENT TAHLILI
Creators: name: Xomidova, N.B.
name: Anvarova, F.J.
name: Jaloliddinova, M.Sh.
Publisher: name: Zenodo
Year: 2024

description: Ushbu maqolada O‘zbekiston Respublikasi farmatsevtika bozoridagi xorijiy, MDH davlatlari hamda mahalliy ishlab chiqaruvchi farmatsevtik korxonalardagi analgetik-antipiretik ta’sirga ega preparatlarning dori shakllari bo‘yicha assortiment tahlili 2019-2023 yillar kesimida o’rganish natijalari keltirildi.
Pressure Tuning of the Charge Density Wave in the Halogen-Bridged Transition-Metal (MX) Solid $Pt_2Br_6(NH_3)_4$
Creators: name: Kanner, G. S.
name: Gammel, J. Tinka
name: Love, S. P.
name: Johnson, S. R.
name: Scott, B.
name: Swanson, B. I.
Publisher: name: arXiv
Year: 1994
Subjects: subject: Condensed Matter (cond-mat)
subject: FOS: Physical sciences

description: We report the pressure dependence up to 95 kbar of Raman active stretching modes in the quasi-one-dimensional MX chain solid $Pt_2Br_6(NH_3)_4$. The data indicate that a predicted pressure-induced insulator-to-metal transition does not occur, but are consistent with the solid undergoing either a three-dimensional structural distortion, or a transition from a charge-density wave to another broken-symmetry ground state. We show that such a transition cacan be well-modeled within a Peierls-Hubbard Hamiltonian. 1993 PACS: 71.30.+h, 71.45.Lr, 75.30.Fv, 78.30.-j, 81.40.Vw
description: 4 pages, ReVTeX 3.0, figures available from the authors on request (Gary Kanner, 111456@INCDP3.Lanl.GOV), to be published in Phys Rev B Rapid Commun, REVISION: minor typos corrected, LA-UR-94-2462
Additional file 2: of Objectively measured physical activity in population-representative parent-child pairs: parental modelling matters and is context-specific
Creators: name: Bringolf-Isler, Bettina
name: Schindler, Christian
name: Kayser, Bengt
name: L. Suzanne Suggs
name: Probst-Hensch, Nicole
Publisher: name: figshare
Year: 2018
Subjects: subject: Genetics
subject: FOS: Biological sciences
subject: 69999 Biological Sciences not elsewhere classified
subject: Science Policy

description: Comparison of children with and without valid parental measurements. (DOCX 15Â kb)
MPEC 2024-E130 : 2024 ES2
Creators: name: Minor Planet Center Staff
Publisher: name: The Minor Planet Center
Year: 2024
Subjects: subject: Small Solar System bodies
valueUri: http://astrothesaurus.org/uat/1469
subject: 2024 ES2

description: The Minor Planet Electronic Circulars contain information on unusual minor planets, routine data on comets and natural satellites, and occasional editorial announcements.  They are published on behalf of Division F of the International Astronomical Union by the Minor Planet Center, Smithsonian Astrophysical Observatory, Cambridge, MA 02138, U.S.A.
Supplementary document for Spatially resolved measurements of optical properties in microscale biological samples from 450nm to 1624nm - 5423646.pdf
Creators: name: Mok, Aaron
name: Shea, Jamien
name: Wu, Chunyan
name: Xia, Fei
name: Tatarsky, Rose
name: Yapici, Nilay
name: Xu, Chris
Publisher: name: Optica Publishing Group
Year: 2021
Subjects: Biomedical Instrumentation

description: Transmission of UV curable resin
The 2dF Galaxy Redshift Survey: Spectral Types and Luminosity Functions
Creators: name: Folkes, S. R.
name: Ronen, S.
name: Price, I.
name: Lahav, O.
name: Colless, M.
name: Maddox, S. J.
name: Deeley, K. E.
name: Glazebrook, K.
name: Bland-Hawthorn, J.
name: Cannon, R. D.
name: Cole, S.
name: Collins, C. A.
name: Couch, W. J.
name: Driver, S. P.
name: Dalton, G.
name: Efstathiou, G.
name: Ellis, R. S.
name: Frenk, C. S.
name: Kaiser, N.
name: Lewis, I. J.
name: Lumsden, S. L.
name: Peacock, J. A.
name: Peterson, B. A.
name: Sutherland, W.
name: Taylor, K.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We describe the 2dF Galaxy Redshift Survey (2dFGRS), and the current status of the observations. In this exploratory paper, we apply a Principal Component Analysis to a preliminary sample of 5869 galaxy spectra and use the two most significant components to split the sample into five spectral classes. These classes are defined by considering visual classifications of a subset of the 2dF spectra, and also by comparing to high quality spectra of local galaxies. We calculate a luminosity function for each of the different classes and find that later-type galaxies have a fainter characteristic magnitude, and a steeper faint-end slope. For the whole sample we find M*=-19.7 (for Omega=1, H_0=100 km/sec/Mpc), alpha=-1.3, phi*=0.017. For class 1 (`early-type') we find M*=-19.6, alpha=-0.7, while for class 5 (`late-type') we find M*=-19.0, alpha=-1.7. The derived 2dF luminosity functions agree well with other recent luminosity function estimates.
description: 15 pages, 14 ps and eps figures, Latex, MNRAS, accepted
Additional file 2: of Chest radiography versus lung ultrasound for identification of acute respiratory distress syndrome: a retrospective observational study
Creators: name: See, Kay
name: Ong, Venetia
name: Tan, Yi
name: Sahagun, Juliet
name: Juvel Taculod
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: 60506 Virology

description: Table S2. Treatment parameters and clinical outcomes using various definitions of acute respiratory distress syndrome. (DOCX 21 kb)
CO-bandhead spectroscopy of IC 342: mass and age of the nuclear star cluster
Creators: name: Boeker, T.
name: van der Marel, R. P.
name: Vacca, W. D.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We have used the NASA Infra-Red Telescope Facility (IRTF) to observe the nuclear stellar cluster in the nearby, face-on, giant Scd spiral IC 342. From high resolution (R = 21500) spectra at the 12CO (2-0) bandhead at 2.3 micron we derive a line-of-sight stellar velocity dispersion sigma = (33 +- 3) km/s. To interpret this observation we construct dynamical models based on the Jeans equation for a spherical system. The light distribution of the cluster is modeled using an isophotal analysis of an HST V-band image from the HST Data Archive, combined with new ground-based K-band imaging. Under the assumption of an isotropic velocity distribution, the observed kinematics imply a K-band mass-to-light ratio M/L_K = 0.05, and a cluster mass M ~ 6 times 10^6 Msun. We model the mass-to-light ratio with the `starburst99' stellar population synthesis models of Leitherer and collaborators, and infer a best-fitting cluster age in the range 63-630 Myears. Although this result depends somewhat on a number of uncertainties in the modeling (e.g., the assumed extinction along the line-of-sight towards the nucleus, the IMF of the stellar population model, and the velocity dispersion anisotropy of the cluster), none of these can be plausibly modified to yield a significantly larger age. We discuss the implications of this result on possible scenarios for the frequency of nuclear starbursts and their impact on secular evolution of spiral galaxy nuclei. As a byproduct of our analysis, we infer that IC 342 cannot have any central black hole more massive than 0.5 million solar masses. This is ~ 6 times less massive than the black hole inferred to exist in our Galaxy, consistent with the accumulating evidence that galaxies with less massive bulges harbor less massive black holes.
description: 27 pages, incl. 9 figures, submitted to The Astronomical Journal
Additional file 1 of Clinical status of patients 1 year after hospital discharge following recovery from COVID-19: a prospective cohort study
Creators: name: Li, Dapeng
name: Liao, Xuejiao
name: Ma, Zhenghua
name: Zhang, Lina
name: Dong, Jingke
name: Zheng, Guoqin
name: Zi, Mei
name: Peng, Wujian
name: Wei, Lanlan
name: Li, Zhiyan
name: Kong, Yingjun
name: Wang, Lifei
name: Liu, Dongjing
name: Wang, Fang
name: He, Qing
name: Li, Guobao
name: Zhang, Zheng
name: Liu, Lei
Publisher: name: figshare
Year: 2022
Subjects: subject: Medicine
subject: Cell Biology
subject: Neuroscience
subject: Physiology
subject: FOS: Biological sciences
subject: Biotechnology
subject: Immunology
subject: FOS: Clinical medicine
subject: Mental Health

description: Additional file 1: Fig S1. Correlation between total CT score and pulmonary function parameters. Table S1. Baseline characteristics of discharged patients with COVID-19 who were followed up compared with who were not. Table S2. General symptoms and psychological symptoms in recovery patients with COVID-19 at 1-year follow-up. Table S3. Pulmonary function test, 6-min walking test, and CT scan at 1-year follow-up. Table S4. Comparison of CT finding according to diffusion capacity of the lung for carbon monoxide. Table S5. The kidney function in recovery patients with COVID-19 at 1-year follow-up. Table S6. Laboratory biomarkers in recovery patients with COVID-19 at 1-year follow-up. Table S7. SARS-CoV-2 RBD-specific antibody levels and seropositive rate in recovery patients with COVID-19 at 1-year follow-up. Table S8. Risk factors associated with psychological symptoms, diffusion impairment, radiological abnormalities, decreased eGFR, and decreased IgG.
title: ADCO, Cartulaire de Cîteaux dit Cartularium Vetus (milieu XIIIe siècle) et Notices du XIIe siècle, Cart. 169 (11 H 63), f. 0070r
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/2011
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2020
Subjects: subject: Corpus Burgundiae Medii Aevi
subject: Chartes de la Bourgogne du Moyen Âge
subject: cartulaire
subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris

description: Cartulaire de Cîteaux dit Cartularium Vetus (milieu XIIIe siècle) et Notices du XIIe siècle, Archives départementales de la Côte-d'Or, Cart. 169 (11 H 63), f. 0070r, Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Cartulaire de Cîteaux dit Cartularium Vetus (milieu XIIIe siècle) et Notices du XIIe siècle, Archives départementales de la Côte-d'Or, Cart. 169 (11 H 63), f. 0070r, in Projet CBMA - Corpus Burgundiae Medii Aevi [Ressource en ligne], https:// manuscrits.cbma-project.eu/
description: Provenance: abbaye de Cîteaux
description: Provenance: http://www.wikidata.org/entity/Q843261
description: Provenance: https://www.geonames.org/3024876
description: Provenance: http://www.idref.fr/030974844/id
description: Provenance: https://catalogue.bnf.fr/ark:/12148/cb12228351v
An Argument Communication Model of Polarization and Ideological Alignment
Creators: name: Banisch, Sven
name: Olbrich, Eckehard
Publisher: name: arXiv
Year: 2018
Subjects: subject: Physics and Society (physics.soc-ph)
subject: Multiagent Systems (cs.MA)
subject: FOS: Physical sciences
subject: FOS: Computer and information sciences

description: A multi-level model of opinion formation is presented which takes into account that attitudes on different issues are usually not independent. In the model, agents exchange beliefs regarding a series of facts. A cognitive structure of evaluative associations links different (partially overlapping) sets of facts to different political issues and determines an agents' attitudinal positions in a way borrowed from expectancy value theory. If agents preferentially interact with other agents that hold similar attitudes on one or several issues, this leads to biased argument pools and polarization in the sense that groups of agents selectively belief in distinct subsets of facts. Besides the emergence of a bi-modal distribution of opinions on single issues that most previous opinion polarization models address, our model also accounts for the alignment of attitudes across several issues along ideological dimensions.
description: See www.universecity.de/demos/SCSIssueAlignment.html for an interactive online demonstration. This project has received funding from the European Union's Horizon 2020 research and innovation programme under grant agreement No 732942 (Opinion Dynamics and Cultural Conflict in European Spaces -- www.Odycceus.eu)
title: Финансы, денежное обращение и кредит
title: Учебное пособие для СПО
titleType: Subtitle
Creators: name: Дмитриева И.Е.
Publisher: name: Профобразование, Ай Пи Ар Медиа
Year: 2020

description: Учебное пособие содержит базовые теоретические сведения по дисциплине «Финансы, денежное обращение и кредит», а также практические задания, включающие тесты и расчетные задачи. Издание разработано в соответствии с требованиями Федерального государственного образовательного стандарта среднего профессионального образования по специальности 38.02.01 «Экономика и бухгалтерский учет (по отраслям)» и предназначено для обучающихся, преподавателей и практических работников.
A representative sample of Be Stars I: Sample Selection, Spectral Classification and Rotational Velocities
Creators: name: Steele, I. A.
name: Negueruela, I.
name: Clark, J. S.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present a sample of 58 Be stars containing objects of spectral types O9 to B8.5 and luminosity classes III to V. We have obtained 3670 - 5070 Angstrom spectra of the sample which are used to derive spectral types and rotational velocities. We discuss the distribution of spectral types and rotational velocities obtained and conclude that there are no significant selection effects in our sample.
description: 10 Pages, 9 Figures, Accepted for publication in A&AS
Exact Results for the Adsorption of a Flexible Self-Avoiding Polymer Chain in Two Dimensions
Creators: name: Batchelor, M. T.
name: Yung, C. M.
Publisher: name: arXiv
Year: 1994
Subjects: subject: Condensed Matter (cond-mat)
subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We derive the exact critical couplings ($x^*, y_{\rm a}^*$), where $y_{\rm a}^*/x^* = \sqrt{1+\sqrt2} = 1.533\ldots\,$, for the polymer adsorption transition on the honeycomb lattice, along with the universal critical exponents, from the Bethe Ansatz solution of the O($n$) loop model at the special transition. Our result for the thermal scaling dimension, and thus the crossover exponent $ϕ=\frac{1}{2}$, is in agreement with an earlier result based on conformal invariance arguments. Our result for the geometric scaling dimensions confirms recent conjectures that they are given by $h_{\ell+1,3}$ in the Kac formula.
description: 11 pages, REVTEX. Minor corrections made and a new reference added to the O(n) model with mixed boundary conditions - final version for publication in Physical Review Letters