cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Orthogonality relations in Quantum Tomography
Creators: name: D'Ariano, G. M.
name: Maccone, L.
name: Paris, M. G. A.
Publisher: name: arXiv
Year: 2000
Subjects: subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: Quantum estimation of the operators of a system is investigated by analyzing its Liouville space of operators. In this way it is possible to easily derive some general characterization for the sets of observables (i.e. the possible quorums) that are measured for the quantum estimation. In particular we analyze the reconstruction of operators of spin systems.
description: 10 pages, 2 figures
title: Management options for reversing depressed maturation-size in Baltic Cod
Creators: name: Andersen, Ken H.
name: Farnsworth, K.
name: Thygesen, U.H.
name: Beyer, J.E.
Publisher: name: ASC 2006 - Theme session H
Year: 2024
Subjects: Fisheries and aquaculture
Pressures, impacts, conservation, and management

description: No abstracts are to be cited without prior reference to the author.The Baltic cod has been heavily exploited for several decades. Therefore there is reason to suspect that ﬁshing may select for a smaller maturation-size, leading to earlier maturation. We develop a general model to determine the optimal maturation size and rate of evolution in ﬁsh stocks, based on size spectrum theory and quantitative genetics. The model is simple and uses only few parameters, which are well known for many ﬁsh stocks, namely von Bertalanﬀy growth parameters, maturity ogives and ﬁshing mortality. Parameters are ﬁtted to Baltic cod, and the eﬀect of three diﬀerent management options are explored: 1) lowering the ﬁshing mortality; 2) ﬁshing only on the mature individuals and 3) reducing ﬁshing on the large individuals only.
Sensitivity analysis for unobserved confounding of direct and indirect effects using uncertainty intervals
Creators: name: Lindmark, Anita
name: de Luna, Xavier
name: Eriksson, Marie
Publisher: name: arXiv
Year: 2017
Subjects: subject: Statistics Theory (math.ST)
subject: FOS: Mathematics

description: To estimate direct and indirect effects of an exposure on an outcome from observed data strong assumptions about unconfoundedness are required. Since these assumptions cannot be tested using the observed data, a mediation analysis should always be accompanied by a sensitivity analysis of the resulting estimates. In this article we propose a sensitivity analysis method for parametric estimation of direct and indirect effects when the exposure, mediator and outcome are all binary. The sensitivity parameters consist of the correlation between the error terms of the mediator and outcome models, the correlation between the error terms of the mediator model and the model for the exposure assignment mechanism, and the correlation between the error terms of the exposure assignment and outcome models. These correlations are incorporated into the estimation of the model parameters and identification sets are then obtained for the direct and indirect effects for a range of plausible correlation values. We take the sampling variability into account through the construction of uncertainty intervals. The proposed method is able to assess sensitivity to both mediator-outcome confounding and confounding involving the exposure. To illustrate the method we apply it to a mediation study based on data from the Swedish Stroke Register (Riksstroke).
description: 22 pages, 5 figures
Additional file 2: of Inactivation of the tight junction gene CLDN11 by aberrant hypermethylation modulates tubulins polymerization and promotes cell migration in nasopharyngeal carcinoma
Creators: name: Hsin-Pai Li
name: Chen-Ching Peng
name: Chih-Ching Wu
name: Chien-Hsun Chen
name: Meng-Jhe Shih
name: Mei-Yuan Huang
name: Lai, Yi-Ru
name: Yung-Li Chen
name: Ting-Wen Chen
name: Tang, Petrus
name: Yu-Sun Chang
name: Chang, Kai-Ping
name: Cheng-Lung Hsu
Publisher: name: figshare
Year: 2018
Subjects: subject: Microbiology
subject: FOS: Biological sciences
subject: Cell Biology
subject: Genetics
subject: Molecular Biology
subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences
subject: 69999 Biological Sciences not elsewhere classified
subject: Developmental Biology

description: Table S1. Sequence of primers in this study. (PDF 105Â kb)
Final Results from the Hubble Space Telescope Key Project to Measure the Hubble Constant
Creators: name: Freedman, W. L.
name: Madore, B. F.
name: Gibson, B. K.
name: Ferrarese, L.
name: Kelson, D. D.
name: Sakai, S.
name: Mould, J. R.
name: Kennicutt,, R. C.
name: Ford, H. C.
name: Graham, J. A.
name: Huchra, J. P.
name: Hughes, S. M. G.
name: Illingworth, G. D.
name: Macri, L. M.
name: Stetson, P. B.
Publisher: name: arXiv
Year: 2000
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present here the final results of the Hubble Space Telescope Key Project to measure the Hubble constant. We summarize our method, the results and the uncertainties, tabulate our revised distances, and give the implications of these results for cosmology. The analysis presented here benefits from a number of recent improvements and refinements, including (1) a larger LMC Cepheid sample to define the fiducial period-luminosity (PL) relations, (2) a more recent HST Wide Field and Planetary Camera 2 (WFPC2) photometric calibration, (3) a correction for Cepheid metallicity, and (4) a correction for incompleteness bias in the observed Cepheid PL samples. New, revised distances are given for the 18 spiral galaxies for which Cepheids have been discovered as part of the Key Project, as well as for 13 additional galaxies with published Cepheid data. The new calibration results in a Cepheid distance to NGC 4258 in better agreement with the maser distance to this galaxy. Based on these revised Cepheid distances, we find values (in km/sec/Mpc) of H0 = 71 +/- 2 (random) +/- 6 (systematic) (type Ia supernovae), 71 +/- 2 +/- 7 (Tully-Fisher relation), 70 +/- 5 +/- 6 (surface brightness fluctuations), 72 +/- 9 +/- 7 (type II supernovae), and 82 +/- 6 +/- 9 (fundamental plane). We combine these results for the different methods with 3 different weighting schemes, and find good agreement and consistency with H0 = 72 +/- 8. Finally, we compare these results with other, global methods for measuring the Hubble constant.
description: Accepted to the Astrophysical Journal, 10 figures
What distinguishes the host galaxies of radio-loud and radio-quiet AGNs?
Creators: name: Kozieł-Wierzbowska, D.
name: Asari, N. Vale
name: Stasińska, G.
name: Sikora, M.
name: Goettems, E. I.
name: Wójtowicz, A.
Publisher: name: arXiv
Year: 2017
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We compare the optical properties of the host galaxies of radio-quiet (RQ) and radio-loud (RL) Type 2 active galactic nuclei (AGNs) to infer whether the jet production efficiency depends on the host properties or is determined just by intrinsic properties of the accretion flows. We carefully select galaxies from SDSS, FIRST, and NVSS catalogs. We confirm previous findings that the fraction of RL AGNs depends on the black-hole (BH) masses, and on the Eddington ratio. The comparison of the nature of the hosts of RL and RQ AGNs, therefore, requires pair-matching techniques. Matching in BH mass and Eddington ratio allows us to study the differences between galaxies hosting RL and RQ AGNs that have the same basic accretion parameters. We show that these two samples differ predominantly in the host-galaxy concentration index, morphological type (in the RL sample the frequency of elliptical galaxies becoming larger with increasing radio loudness), and nebular extinction (galaxies with highest radio loudness showing only low nebular extinction). Contrary to some previous studies, we find no significant difference between our radio-loud and radio-quiet samples regarding merger/interaction features.
description: 16 pages, 13 figures, published in ApJ
Characterization of separable states and entanglement witnesses
Creators: name: Lewenstein, M.
name: Kraus, B.
name: Horodecki, P.
name: Cirac, J. I.
Publisher: name: arXiv
Year: 2000
Subjects: subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: We provide a canonical form of mixed states in bipartite quantum systems in terms of a convex combination of a separable state and a, so-called, edge state. We construct entanglement witnesses for all edge states. We present a canonical form of nondecomposable entanglement witnesses and the corresponding positive maps. We provide constructive methods for their optimization in a finite number of steps. We present a characterization of separable states using a special class of entanglement witnesses. Finally, we present a nontrivial necessary condition for entanglement witnesses and positive maps to be extremal.
description: 4 pages, 1 figure
Star-planet interactions. IV. Possibility of detecting the orbit-shrinking of a planet around a red giant
Creators: name: Meynet, Georges
name: Eggenberger, Patrick
name: Privitera, Giovanni
name: Georgy, Cyril
name: Ekstroem, Sylvia
name: Alibert, Yann
name: Lovis, Christophe
Publisher: name: arXiv
Year: 2017
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: FOS: Physical sciences

description: The surface rotations of some red giants are so fast that they must have been spun up by tidal interaction with a close companion, either another star, a brown dwarf, or a planet. We focus here on the case of red giants that are spun up by tidal interaction with a planet. When the distance between the planet and the star decreases, the spin period of the star decreases, the orbital period of the planet decreases, and the reflex motion of the star increases. We study the change rate of these three quantities when the circular orbit of a planet of 15 M$_{J}$ that initially orbits a 2 M$_\odot$ star at 1 au shrinks under the action of tidal forces during the red giant phase. We use stellar evolution models coupled with computations of the orbital evolution of the planet, which allows us to follow the exchanges of angular momentum between the star and the orbit in a consistent way. We obtain that the reflex motion of the red giant star increases by more than 1 m s$^{-1}$ per year in the last $\sim$40 years before the planet engulfment. During this phase, the reflex motion of the star is between 660 and 710 m s$^{-1}$. The spin period of the star increases by more than about 10 minutes per year in the last 3000 y before engulfment. During this period, the spin period of the star is shorter than 0.7 year. During this same period, the variation in orbital period, which is shorter than 0.18 year, is on the same order of magnitude. Changes in reflex-motion and spin velocities are very small and thus most likely out of reach of being observed. The most promising way of detecting this effect is through observations of transiting planets, that is, through{\it } changes of the beginning or end of the transit. A space mission like PLATO might be of great interest for detecting planets that are on the verge of being engulfed by red giants.
description: 4 pages, 4 figures
A revised Cepheid distance to NGC 4258 and a test of the distance scale
Creators: name: Newman, Jeffrey A.
name: Ferrarese, Laura
name: Stetson, Peter B.
name: Maoz, Eyal
name: Zepf, Stephen E.
name: Davis, Marc
name: Freedman, Wendy L.
name: Madore, Barry F.
Publisher: name: arXiv
Year: 2000
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: In a previous paper (Maoz et al. 1999), we reported a Hubble Space Telescope (HST) Cepheid distance to the galaxy NGC 4258 obtained using the calibrations and methods then standard for the Key Project on the Extragalactic Distance Scale. Here, we reevaluate the Cepheid distance using the revised Key Project procedures described in Freedman et al. (2001). These revisions alter the zero points and slopes of the Cepheid Period-Luminosity (P-L) relations derived at the Large Magellanic Cloud (LMC), the calibration of the HST WFPC2 camera, and the treatment of metallicity differences. We also provide herein full information on the Cepheids described in Maoz et al. 1999. Using the refined Key Project techniques and calibrations, we determine the distance modulus of NGC 4258 to be 29.47 +/- 0.09 mag (unique to this determination) +/- 0.15 mag (systematic uncertainties in Key Project distances), corresponding to a metric distance of 7.8 +/- 0.3 +/- 0.5 Mpc and 1.2 sigma from the maser distance of 7.2 +/- 0.5 Mpc. We also test the alternative Cepheid P-L relations of Feast (1999), which yield more discrepant results. Additionally, we place weak limits upon the distance to the LMC and upon the effect of metallicity in Cepheid distance determinations.
description: 26 pages in emulateapj5 format, including 6 figures and 5 tables. Accepted for publication in the Astrophysical Journal
Online linear optimization with the log-determinant regularizer
Creators: name: Moridomi, Ken-ichiro
name: Hatano, Kohei
name: Takimoto, Eiji
Publisher: name: arXiv
Year: 2017
Subjects: subject: Machine Learning (cs.LG)
subject: FOS: Computer and information sciences

description: We consider online linear optimization over symmetric positive semi-definite matrices, which has various applications including the online collaborative filtering. The problem is formulated as a repeated game between the algorithm and the adversary, where in each round t the algorithm and the adversary choose matrices X_t and L_t, respectively, and then the algorithm suffers a loss given by the Frobenius inner product of X_t and L_t. The goal of the algorithm is to minimize the cumulative loss. We can employ a standard framework called Follow the Regularized Leader (FTRL) for designing algorithms, where we need to choose an appropriate regularization function to obtain a good performance guarantee. We show that the log-determinant regularization works better than other popular regularization functions in the case where the loss matrices L_t are all sparse. Using this property, we show that our algorithm achieves an optimal performance guarantee for the online collaborative filtering. The technical contribution of the paper is to develop a new technique of deriving performance bounds by exploiting the property of strong convexity of the log-determinant with respect to the loss matrices, while in the previous analysis the strong convexity is defined with respect to a norm. Intuitively, skipping the norm analysis results in the improved bound. Moreover, we apply our method to online linear optimization over vectors and show that the FTRL with the Burg entropy regularizer, which is the analogue of the log-determinant regularizer in the vector case, works well.
description: 18 pages
The magnetic and electric transverse spin density of spatially confined light
Creators: name: Neugebauer, Martin
name: Eismann, Jörg
name: Bauer, Thomas
name: Banzer, Peter
Publisher: name: arXiv
Year: 2017
Subjects: subject: Optics (physics.optics)
subject: FOS: Physical sciences

description: When a beam of light is laterally confined, its field distribution can exhibit points where the local magnetic and electric field vectors spin in a plane containing the propagation direction of the electromagnetic wave. The phenomenon indicates the presence of a non-zero transverse spin density. Here, we experimentally investigate this transverse spin density of both magnetic and electric fields, occurring in highly-confined structured fields of light. Our scheme relies on the utilization of a high-refractive-index nano-particle as local field probe, exhibiting magnetic and electric dipole resonances in the visible spectral range. Because of the directional emission of dipole moments which spin around an axis parallel to a nearby dielectric interface, such a probe particle is capable of locally sensing the magnetic and electric transverse spin density of a tightly focused beam impinging under normal incidence with respect to said interface. We exploit the achieved experimental results to emphasize the difference between magnetic and electric transverse spin densities.
description: 7 pages, 4 figures
Cinema é celebração: a cena de exibição de cinema e audiovisual independentes do Rio de Janeiro na virada dos anos 2000. Dissertação de Mestrado. Rio de Janeiro: UFRJ, 2022.
Creators: name: Nogueira Carvalho, Thiago
Publisher: name: figshare
Year: 2024
Subjects: classificationCode: 470214
subject: Screen and media culture
classificationCode: 470101
subject: Communication studies
classificationCode: 360102
subject: Art history
classificationCode: 360501
subject: Cinema studies
classificationCode: 360604
subject: Photography, video and lens-based practice
classificationCode: 390201
subject: Education policy

description: A presente pesquisa aplicada tem como resultados um texto dissertativo e um produto técnico audiovisual no formato de uma série documental de oito episódios, e investiga, através de abordagem qualitativa, a cena de exibição de cinema e audiovisual independentes do Rio de Janeiro na virada dos anos 2000, a partir de cinco de seus principais eventos constituintes: Festival Brasileiro de Cinema Universitário, O Incinerasta, Cachaça Cinema Clube, Mostra do Filme Livre, e Cineclube Mate Com Angu. Realizada a partir de entrevistas com integrantes dos eventos estudados, a série documental aborda aspectos como: o papel das escolas e cursos de cinema na formação dos grupos; as transformações tecnológicas da época; a importância do curta-metragem na cena; o movimento cineclubista no Rio de Janeiro nos anos 2000; a expansão do audiovisual para a periferia; e a relação com a institucionalidade existente na região. Além das motivações e retrospecto, também é abordada a importância do movimento para a constituição da identidade geracional dos novos ingressantes no campo do cinema brasileiro. Por meio da circulação da série, pretende-se também dar visibilidade para a cena estudada, assim como promover um diálogo entre diferentes gerações, incitando o debate e a reflexão sobre os desafios do cinema e audiovisual brasileiro na atualidade.
title: How does stochasticity affect evolutionary regime shifts in ageand size at maturation?
Creators: name: Boukal, David S.
name: de Roos, André M.
name: Persson, Lennart
Publisher: name: ASC 2006 - Theme session H
Year: 2024
Subjects: Fisheries and aquaculture
Pressures, impacts, conservation, and management

description: No abstracts are to be cited without prior reference to the author.Fish in many exploited stocks grow faster and mature earlier at either larger or smaller sizes in comparison to pre-exploitation periods. These changes can be driven by both genetic and phenotypic responses. We have shown recently that their interplay can lead to irreversible evo-lutionary regime shifts in individual life histories and stock properties. Our results were based on a model which assumed annual spawning and size- and density-dependent individual growth in a deterministic environment. We now extend the analysis to cover stochasticity in recruit-ment, survival after recruitment and harvesting pressure, including the possibility of bycatch and illegal fishing after fishing moratoria or reduced harvest rates are imposed. We show that under low and moderate stochasticity, early maturation at small sizes and late maturation at large sizes can still persist as alternative, evolutionary and ecologically stable states under otherwise identical environmental conditions. Typically, maturation sizes of the late-maturing phenotypes decrease with increasing stochasticity, while those of the early-maturing phenotypes remain nearly constant. Consequently, we confirm that even in stochastic environments, exploitation of late-maturing populations can induce rapid evolution to smaller maturation sizes associated with stepwise decreases in mean age at first reproduction. These changes can be reversed by fishing moratoria; more stochastic environments and/or harvesting pressure require faster clo-sure of the fishery. Unless stochasticity is too strong, incomplete closure of the fishery may also lead to the counterintuitive, accelerated evolution towards smaller sizes at maturation which we reported for the deterministic system.
title: ADCO, Deuxième cartulaire ou Grand cartulaire de l'abbaye de Molesme, Cart. 143 (7 H 7), 153 fol, f. 0112v
Creators: name: de la Côte d'Or, Archives départementales
name: Petot, Frédéric
name: Archives Départementales De La Côte-D'Or
name: Petot, Frédérique
name: Projet CBMA
name: CG21/F.PETOT/2009
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2020
Subjects: subject: Corpus Burgundiae Medii Aevi
subject: Chartes de la Bourgogne du Moyen Âge
subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris
subject: cartulaire

description: Deuxième cartulaire ou Grand cartulaire de l'abbaye de Molesme, Archives départementales de la Côte-d'Or, Cart. 143 (7 H 7), 153 fol, f. 0112v, Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Deuxième cartulaire ou Grand cartulaire de l'abbaye de Molesme, Archives départementales de la Côte-d'Or, Cart. 143 (7 H 7), 153 fol, f. 0112v, in Projet CBMA - Corpus Burgundiae Medii Aevi [Ressource en ligne], https:// manuscrits.cbma-project.eu/
description: Provenance: http://www.wikidata.org/entity/Q334044
description: Provenance: https://catalogue.bnf.fr/ark:/12148/cb137389344
description: Provenance: abbaye de Molesme
Multiphoton Label-Free ex-vivo imaging using a custom-built dual-wavelength microscope with chromatic aberrations compensation
Creators: name: Filippi, Andrea
name: Borile, Giulia
name: Sasso, Eleonora Dal
name: Iop, Laura
name: Armani, Andrea
name: Gintoli, Michele
name: Sandri, Marco
name: Gerosa, Gino
name: Romanato, Filippo
Publisher: name: arXiv
Year: 2017
Subjects: subject: Biological Physics (physics.bio-ph)
subject: Optics (physics.optics)
subject: FOS: Physical sciences

description: Label-Free Multiphoton Microscopy is a very powerful optical microscopy that can be applied to study samples with no need for exogenous fluorescent probes, keeping the main benefits of a Multiphoton approach, like longer penetration depths and intrinsic optical sectioning, while opening the possibility of serial examinations with different kinds of techniques. Among the many variations of Label-Free MPM, Higher Harmonic Generation (HHG) is one of the most intriguing due to its generally low photo-toxicity, which enables the examination of specimens particularly susceptible to photo-damages. HHG and common Two-Photon Microscopy (TPM) are well-established techniques, routinely used in several research fields. However, they require a significant amount of fine-tuning in order to be fully exploited and, usually, the optimized conditions greatly differ, making them quite difficult to perform in parallel without any compromise on the extractable information. Here we present our custom-built Multiphoton microscope capable of performing simultaneously TPM and HHG without any kind of compromise on the results thanks to two, separate, individually optimized laser sources with full chromatic aberration compensation. We also apply our setup to the examination of a plethora of ex vivo samples in order to prove the significant advantages of our approach.
Additional file 2: of Fibrocytes are increased in lung and peripheral blood of patients with idiopathic pulmonary fibrosis
Creators: name: P. Heukels
name: J. Van Hulst
name: M. Van Nimwegen
name: C. Boorsma
name: B. Melgert
name: L. Van Den Toorn
name: K. Boomars
name: M. Wijsenbeek
name: H. Hoogsteden
name: J. Von Der ThĂźsen
name: R. Hendriks
name: M. Kool
name: B. Van Den Blink
Publisher: name: figshare
Year: 2018
Subjects: subject: Microbiology
subject: FOS: Biological sciences
subject: Cell Biology
subject: Genetics
subject: Biotechnology
subject: Immunology
subject: FOS: Clinical medicine
subject: 69999 Biological Sciences not elsewhere classified
subject: Developmental Biology
subject: Cancer
subject: Hematology
subject: Computational Biology

description: Sort strategy for CD45+/Col-1+ cells. (A) The conventional strategy with the CD45+/Col-1+ cells in red. (B) Position of the same fibrocytes when employing a gating strategy based on additional extracellular markers. The sort strategy is based on extracellular markers and with some modifications previously published [16] (of note: for our research question we did not exclude SSChi cells). CD45+ cells were analyzed for HLA-DR expression and lineage markers to exclude B-cells (CD19), NK cells (CD56) and T-cells (CD3). Lineage negative cells were plotted as CD14 versus CD16 to create a distinct group of cells enriched for CD45+/Col-1+ cells (red box). (PDF 75 kb)
Cooling a Hot Disk Around a Supermassive Black Hole by a Star
Creators: name: Chang, Heon-Young
Publisher: name: arXiv
Year: 2000
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: If a supermassive black hole resides in the centers of galaxies, there are several effects expected to be observed. It is likely that accretion disks are around the supermassive black hole. Stellar interactions with the accretion flows around the supermassive black hole play a role in that an flying-by star may cool a hot accretion disk as a result of Comptonization. It is shown that the Comptonization of the stellar emission will take place in a hot accretion disk such as the ADAFs around the supermassive black hole and become a relatively important source of the accretion disk cooling when the mass accretion rate is low, and stars are passing outer parts of the hot accretion disk. We suggest that such a stellar cooling can be observed in the radio frequency regime since synchrotron luminosity of the ADAFs depends strongly on the electron temperature and occurs much more frequently than a tidal disruption event.
description: Submitted to ApJL, 13 pages, 2 postscript figures
Effect of Composition Gradient on Magnetothermal Instability Modified by Shear and Rotation
Creators: name: Gupta, Himanshu
name: Chaudhuri, Anya
name: Sadhukhan, Shubhadeep
name: Chakraborty, Sagar
Publisher: name: arXiv
Year: 2017
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: Fluid Dynamics (physics.flu-dyn)
subject: Plasma Physics (physics.plasm-ph)
subject: FOS: Physical sciences

description: We model the intracluster medium as a weakly collisional plasma that is a binary mixture of the hydrogen and the helium ions, along with free electrons. When, owing to the helium sedimentation, the gradient of the mean molecular weight (or equivalently, composition or helium ions' concentration) of the plasma is not negligible, it can have appreciable influence on the stability criteria of the thermal convective instabilities, e.g., the heat-flux-buoyancy instability and the magnetothermal instability (MTI). These instabilities are consequences of the anisotropic heat conduction occurring preferentially along the magnetic field lines. In this paper, without ignoring the magnetic tension, we first present the mathematical criterion for the onset of composition gradient modified MTI. Subsequently, we relax the commonly adopted equilibrium state in which the plasma is at rest, and assume that the plasma is in a sheared state which may be due to differential rotation. We discuss how the concentration gradient affects the coupling between the Kelvin--Helmholtz instability and the MTI in rendering the plasma unstable or stable. We derive exact stability criterion by working with the sharp boundary case in which the physical variables---temperature, mean molecular weight, density, and magnetic field---change discontinuously from one constant value to another on crossing the boundary. Finally, we perform the linear stability analysis for the case of the differentially rotating plasma that is thermally and compositionally stratified as well. By assuming axisymmetric perturbations, we find the corresponding dispersion relation and the explicit mathematical expression determining the onset of the modified MTI.
description: 11 pages, 1 figure, Accepted in MNRAS
title: Article_L'Indispensable Agenda de l'amateur photographe pour 1889-90
Creators: name: AmateurS
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2020

description: ID_ARTI_00187
title: ADCO, Neuvième cartulaire de Saint-Étienne de Dijon (1661 - 1684), Cart. 32 (G 136), 745 folios, f. 0029
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: Corpus Burgundiae Medii Aevi
subject: Chartes de la Bourgogne du Moyen Âge
subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris
subject: cartulaire

description: Neuvième cartulaire de Saint-Étienne de Dijon (1661 - 1684), Archives départementales de la Côte-d'Or, Cart. 32 (G 136), 745 folios, f. 0029, Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Neuvième cartulaire de Saint-Étienne de Dijon (1661 - 1684), Archives départementales de la Côte-d'Or, Cart. 32 (G 136), 745 folios, f. 0029, 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
Atomic coherence and interference phenomena in resonant nonlinear optical interactions
Creators: name: Popov, A. K.
name: Rautian, S. G.
Publisher: name: arXiv
Year: 2000
Subjects: subject: Quantum Physics (quant-ph)
subject: Optics (physics.optics)
subject: FOS: Physical sciences

description: Interference effects in quantum transitions, giving rise to amplification without inversion, optical transparency and to enhancements in nonlinear optical frequency conversions are considered. Review of the relevant early theoretical and experimental results is given. The role of relaxation processes, spontaneous cascade of polarizations, local field effects, Doppler-broadening, as well as specific features of the interference in the spectral continuum are discussed.
description: 13 pages, 13 eps figures, review paper, Proceedings of the 15th International Conference on Nonlinear Optics - ICONO'95
Additional file 2: of Construction and pilot test of a set of indicators to assess the implementation and effectiveness of the who safe childbirth checklist
Creators: name: Saturno-Hernández, Pedro
name: Fernández-Elorriaga, María
name: Martínez-Nicolás, Ismael
name: Poblano-Verástegui, Ofelia
Publisher: name: figshare
Year: 2018
Subjects: subject: Cell Biology
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences

description: Mexico Safe Childbirth Checklist for mother and newborn (english). The original WHO Safe Childbirth Checklist was refined and adapted to the Mexican context and translated to english language. (PDF 458 kb)
Sergio Secondiano Sacchi (Hg.): Multifilter. Mito e memoria del padre nella canzone. Roma: Squi(libri), 2017. ISBN 978-8885571020. 208 Seiten, 2 CDs.
Creators: name: Ankli, Ruedi
Publisher: name: ATeM Archiv für Textmusikforschung
Year: 2019

description: ATeM Archiv für Textmusikforschung, No 3,2
The standstill luminosity in Z Cam systems
Creators: name: Stehle, R.
name: King, A.
name: Rudge, C.
Publisher: name: arXiv
Year: 2000
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We consider accretion discs in close binary systems. We show that heating of a disc at the impact point of the accretion stream contributes significantly to the local energy budget at its outer edge. As a result the thermal balance relation between local accretion rate and surface density (the `S-curve') changes; the critical mass transfer rate above which no dwarf nova outbursts occur can be up to 40% smaller than without impact heating. Standstills in ZCam systems thus occur at smaller mass transfer rates than otherwise expected, and are rather fainter than the peak luminosity during the dwarf nova phase as a result.
description: 3 pages, 3 figures. Accepted for publication in MNRAS
Self-reflection interventions to promote well-being
Creators: name: Burns, Shannon
name: Falk, Emily
name: Cosme, Danielle
name: Mesquiti, Steven
Publisher: name: Open Science Framework
Year: 2023
Subjects: subject: Psychology
subject: FOS: Psychology
subject: Social Psychology
subject: Social and Behavioral Sciences
subject: journaling
subject: well-being
subject: self-reflection
subject: mental health
subject: audio
subject: intervention

description: Encouraging individuals to practice self-reflection has the potential to improve long-term well-being, potentially by increasing self-insight. Through better understanding of the self, individuals can learn to make better decisions and achieve a greater sense of autonomy (Ryan et al., 2021). Indeed, a variety of frameworks provide converging evidence for the benefits of self-reflection, including expressive writing to process emotional experiences (Pennebaker & Chung, 2011), reminiscence-based therapies that involve reflecting on autobiographical memories (Hallford & Meller, 2016; Hallford et al., 2022), and mindfulness techniques that enhance self-awareness (Vago & Silbersweig, 2012). We conducted an initial study to examine potential links between self-reflection, self-insight, and well-being. Participants (N = 222) engaged in self-reflection through audio journaling (i.e., making audio-recorded responses to self-reflection prompts) for four days across one week. All participants engaged in the intervention and there was no control condition. We looked at pre-post changes on the following well-being and mental health dimensions: anxiety, depression, positive and negative emotion, satisfaction with life, and psychological well-being (sub-scales: autonomy, environmental mastery, personal growth, purpose, relationships, and self-acceptance). Across these dimensions, we observed subjective decreases in depression (b = -0.17 [-0.23, -0.11]), anxiety (b = -0.20 [-0.27, -0.12]), and negative emotions (b = -0.08 [-0.15, -0.01]); and increases in satisfaction with life (b = 0.23 [0.10, 0.36]), environmental mastery (b = 0.17 [0.05, 0.29]), personal growth (b = 0.23 [0.11, 0.34]), relationships (b = 0.18 [0.04, 0.31]), purpose (b = 0.15 [0.02, 0.28]), self-acceptance (b = 0.26 [0.12, 0.40]), and weak increases in autonomy (b = 0.09 [-0.04, 0.21]). The only dimension that was not affected by the intervention was positive emotion. The present study builds on these promising initial findings. In this study, we test the effects of a within-person self-reflection intervention on various dimensions of mental health and well-being.
Probability distribution and statistical properties of spherically compensated cosmic regions in $Λ$CDM cosmology
Creators: name: Alimi, Jean-Michel
name: de Fromont, Paul
Publisher: name: arXiv
Year: 2017
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences
subject: 83F05

description: The statistical properties of cosmic structures are well known to be strong probes for cosmology. In particular, several studies tried to use the cosmic void counting number to obtain tight constrains on Dark Energy. In this paper we address this question by using the CoSphere model as introduced in de Fromont & Alimi (2017a). We derive their exact statistics in both primordial and non linearly evolved Universe for the standard $Λ$CDM model. We first compute the full joint Gaussian probability distribution for the various parameters describing these profiles in the Gaussian Random Field. We recover the results of Bardeen et al. (1986) only in the limit where the compensation radius becomes very large, i.e. when the central extremum decouples from its cosmic environment. We derive the probability distribution of the compensation size in this primordial field. We show that this distribution is redshift independent and can be used to model cosmic void size distribution. Interestingly, it can be used for central maximum such as DM haloes. We compute analytically the statistical distribution of the compensation density in both primordial and evolved Universe. We also derive the statistical distribution of the peak parameters already introduced by Bardeen et al. (1986) and discuss their correlation with the cosmic environment. We thus show that small central extrema with low density are associated with narrow compensation regions with a small $R_1$ and a deep compensation density $δ_1$ while higher central extrema are located in larger but smoother over/under massive regions.
description: 13 pages, 10 images, submitted to MNRAS
Additional file 1: of Inactivation of the tight junction gene CLDN11 by aberrant hypermethylation modulates tubulins polymerization and promotes cell migration in nasopharyngeal carcinoma
Creators: name: Hsin-Pai Li
name: Chen-Ching Peng
name: Chih-Ching Wu
name: Chien-Hsun Chen
name: Meng-Jhe Shih
name: Mei-Yuan Huang
name: Lai, Yi-Ru
name: Yung-Li Chen
name: Ting-Wen Chen
name: Tang, Petrus
name: Yu-Sun Chang
name: Chang, Kai-Ping
name: Cheng-Lung Hsu
Publisher: name: figshare
Year: 2018
Subjects: subject: Biophysics
subject: Biochemistry
subject: Cell Biology
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences
subject: Developmental Biology

description: Supplementary Materials and Methods. (DOC 39Â kb)
Spin-isospin excitation of ${}^3$He with three-proton final state
Creators: name: Ishikawa, Souichi
Publisher: name: arXiv
Year: 2017
Subjects: subject: Nuclear Theory (nucl-th)
subject: Nuclear Experiment (nucl-ex)
subject: FOS: Physical sciences

description: Spin-isospin excitation of ${}^3$He nucleus by proton-induced charge-exchange reaction, ${}^3\mathrm{He}(p,n)ppp$, at forward neutron scattering angle is studied in a plane wave impulse approximation (PWIA). In PWIA, cross sections of the reaction is written in terms of proton-neutron scattering amplitudes and response functions of the transition from ${}^{3}$He to three-proton state by spin-isospin transition operators. The response functions are calculated with realistic nucleon-nucleon potential models using a Faddeev three-body method. Calculated cross sections agree with available experimental data in substance. Possible effects arising from the uncertainty of proton-neutron amplitudes and three-nucleon interactions in three-proton system are examined.
description: 16 pages, 6 figures, accepted for publication in PTEP
title: Morphological features of walleye pollock individuals from the different parts of a trawl
Creators: name: Lapshin, Oleg M.
name: B. N. Kotenev, Y. G. Izumov
name: Gerasimov, Y. V.
Publisher: name: ASC 2006 - Theme session H
Year: 2024
Subjects: Fisheries and aquaculture
Pressures, impacts, conservation, and management

description: No abstracts are to be cited without prior reference to the author.Our previous investigations revealed morphological and behavioral heterogeneity in walleye pollock aggregations. For its further investigation, a trawl fishing survey was conducted in the northern part of Sea of Okhotsk, with sampling fish from the different sections of the trawl. Sample A was taken from the terminal part of cod end (specimens caught first); sample B – from the nearer part of cod end (specimens caught last); sample C – from the catcher (along with specimens meshed in the belly part around the catcher). The number of vertebrae in the abdominal section (Va), caudal section (Vc), and the total number of vertebrae (Vert) were counted in each sample. Sample C is characterized by higher Va and Vert values in comparison with samples A and B. Modal Va value in sample A is shifted from 18 to 19. The percentage of “long-tail” fish in sample B is greater than in sample A. Sample C is notable for its maximum diversity and increased number of vertebrae in Va. Morphological features of fish in sample A are the most similar to the characteristics of the whole catch. Based on the results of trawl fishing, the following structure of walleye pollock aggregations is seen. Some fish in the aggregation will be inevitably caught in a trawl with no chance of escape (sample A). Another part of the aggregation consists of the individuals actively getting away from the approaching trawl (sample B). The tactics of fish in group C is rather to get out of the trawl than to escape from the approaching gear. “Short-tail” fish are numerous in sample C, while the “long-tail” specimens are abundant in sample B. Fish of groups C and B having avoided capture maintain the intrapopulation variation of walleye pollock.
Three qubits can be entangled in two inequivalent ways
Creators: name: Dür, W.
name: Vidal, G.
name: Cirac, J. I.
Publisher: name: arXiv
Year: 2000
Subjects: subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: Invertible local transformations of a multipartite system are used to define equivalence classes in the set of entangled states. This classification concerns the entanglement properties of a single copy of the state. Accordingly, we say that two states have the same kind of entanglement if both of them can be obtained from the other by means of local operations and classical communcication (LOCC) with nonzero probability. When applied to pure states of a three-qubit system, this approach reveals the existence of two inequivalent kinds of genuine tripartite entanglement, for which the GHZ state and a W state appear as remarkable representatives. In particular, we show that the W state retains maximally bipartite entanglement when any one of the three qubits is traced out. We generalize our results both to the case of higher dimensional subsystems and also to more than three subsystems, for all of which we show that, typically, two randomly chosen pure states cannot be converted into each other by means of LOCC, not even with a small probability of success.
description: 12 pages, 1 figure; replaced with revised version; terminology adapted to earlier work; reference added; results unchanged
Galactic Black HOle Binary Systems
Creators: name: Done, C.
Publisher: name: arXiv
Year: 2000
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: I review observations of the X-ray spectra of Galactic Black Hole Candidates, and theoretical ideas as to how these can be produced. X-ray reflection should enable different source geometries to be distinguished, but the ionisation instability of X-ray irradiated material in hydrostatic equilibrium gives rise to large ambiguities in interpretation. It is not currently possible to determine whether the underlying emission mechanism in the low state is an advective flow or magnetic reconnection above the disk, but more detailed modelling of the ionisation instability {\it may} allow us to distinguish between these scenarios.
description: Invited review at the COSPAR conference. Accepted for publication in Advances in Space Research
Rainer Simon: Konzert der Sinne. Dimensionen einer phänomenologischen Analyse der Wahrnehmung von Musikaufführungen. Freiburg i. Br./Berlin/Wien: Rombach Verlag, 2018. ISBN 978-3793098737. 423 Seiten.
Creators: name: Agnetta, Marco
Publisher: name: ATeM Archiv für Textmusikforschung
Year: 2019

description: ATeM Archiv für Textmusikforschung, No 3,2
Locating the QCD critical end point through the peaked baryon number susceptibilities along the freeze-out line
Creators: name: Li, Zhibin
name: Chen, Yidian
name: Li, Danning
name: Huang, Mei
Publisher: name: arXiv
Year: 2017
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: High Energy Physics - Lattice (hep-lat)
subject: High Energy Physics - Theory (hep-th)
subject: Nuclear Theory (nucl-th)
subject: FOS: Physical sciences

description: We investigate the baryon number susceptibilities up to fourth order along different freeze-out lines in a holographic QCD model with the critical end point (CEP), and we propose that the peaked baryon number susceptibilities along the freeze-out line can be used as a clean signature to locate the CEP in the QCD phase diagram. On the temperature and baryon chemical potential plane, the ratio of the baryon number susceptibilities (up to fourth order) forms a ridge along the phase boundary, and develops a sword shape mountain standing upright around the CEP in a narrow and oblate region. This feature is model independent and universal if the CEP exists. The measurement of the baryon number susceptibilities from heavy-ion collision experiment is along the freeze-out line. If the freeze-out line crosses the foot of the CEP mountain, then one can observe the peaked baryon number susceptibilities along the freeze-out line, and the kurtosis of the baryon number distributions has the tallest magnitude. The data from the first phase of beam energy scan program at the Relativistic Heavy Ion Collisions indicates that a peak of the kurtosis of the baryon number distribution would show up at the collision energy around 5 GeV, which suggests that the freeze-out line crosses the foot of the CEP mountain and the summit of the CEP would be located nearby around the collision energy of 3 GeV.
description: 5 pages, 3 figures
On Completeness of Logical Relations for Monadic Types
Creators: name: Lasota, Slawomir
name: Nowak, David
name: Zhang, Yu
Publisher: name: arXiv
Year: 2006
Subjects: subject: Logic in Computer Science (cs.LO)
subject: Programming Languages (cs.PL)
subject: FOS: Computer and information sciences
subject: D.3.1; F.3.1

description: Software security can be ensured by specifying and verifying security properties of software using formal methods with strong theoretical bases. In particular, programs can be modeled in the framework of lambda-calculi, and interesting properties can be expressed formally by contextual equivalence (a.k.a. observational equivalence). Furthermore, imperative features, which exist in most real-life software, can be nicely expressed in the so-called computational lambda-calculus. Contextual equivalence is difficult to prove directly, but we can often use logical relations as a tool to establish it in lambda-calculi. We have already defined logical relations for the computational lambda-calculus in previous work. We devote this paper to the study of their completeness w.r.t. contextual equivalence in the computational lambda-calculus.
description: 20 pages, full version of the paper published at ASIAN'2006, with the same title
Additional file 1: of Policies and clinical practices relating to the management of gestational diabetes mellitus in the public health sector, South Africa â a qualitative study
Creators: name: Lorrein Muhwava
name: Murphy, Katherine
name: Zarowsky, Christina
name: Levitt, Naomi
Publisher: name: figshare
Year: 2018
Subjects: subject: Cell Biology
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: Science Policy

description: Discussion guide for key informant interviews. Description of data: The discussion guide was used to direct discussions with key informants using probes. (PDF 62Â kb)