bluuebunny/crossref_metadata_2025_split huggingface dataset:
Features of assessing the quality of medical care for patients with chronic heart failure of older age groups ()
Authors: Яковлев А.А. , Хавинсон В.Х. 
Published: March 2022

В обзоре представлен анализ литературы по качеству медицинской помощи в целом и критериям их оценки. Основная дискуссия ведется в нескольких направлениях: какие индикаторы качества медицинской помощи существуют в настоящий момент, какие из них можно использовать у больных старших возрастных групп, какие индикаторы следует применять у данной категории пациентов. На основании обзора следует вывод о том, что существующие индикаторы качества не отражают особенностей оказания помощи лицам пожилого и старческого возраста с ХСН. Делается заключение, что многие вопросы до настоящего времени не решены и необходимы дальнейшие исследования по данной проблеме. Оценка качества медицинской помощи при ХСН, прежде всего у пациентов пожилого и старческого возраста, на наш взгляд, должна проводится с учётом возрастных особенностей и с применением дополнительных индикаторов качества, которые следует ввести в профильный приказ отдельным пунктом.
The review presents a literature analysis on the quality of medical care in general and the criteria for their assessment. The main discussion is conducted in several areas: what indicators are currently available; which of them can be used in elderly and senile age groups; what indicators should be used in this category of patients. Based on the review, it should be concluded, that the existing quality indicators do not reflect the specifics of providing care to elderly and senile people with chronic heart failure. It is concluded, that many issues have not yet been resolved and further research is needed on this issue. In our opinion, the assessment of the quality of medical care for chronic heart failure, primarily in elderly and senile patients, should be carried out taking into account age characteristics and using additional quality indicators, which should be introduced in a separate paragraph in the profile order.
Graphene/AlGaN Schottky barrier photodiodes and its application for array devices
Authors: Nakagawa Yoshinori , Okauchi Shigeki , Sano Masahiko , Mukai Takashi , Ohno Yasuhide , Nagase Masao 
Published: March 2022

Abstract
This study evaluated the characteristics of graphene/AlGaN Schottky barrier photodiodes using graphene as a transparent electrode film and AlGaN as a light-absorbing sensor layer. It was found that the Schottky barrier height of graphene/AlGaN ranged within 1.2–1.7 eV depending on the Al composition ratio. By forming an array of photodiodes, an 8 × 8 pixels ultraviolet image sensor was fabricated.
Structural design optimization of 279 nm wavelength AlGaN homojunction tunnel junction deep-UV light-emitting diode
Authors: Nagata Kengo , Anada Satoshi , Miwa Hiroshi , Matsui Shinichi , Boyama Shinya , Saito Yoshiki , Kushimoto Maki , Honda Yoshio , Takeuchi Tetsuya , Amano Hiroshi 
Published: March 2022

Abstract
We demonstrated the structural optimization of AlGaN tunnel junction (TJ) deep-ultraviolet light-emitting diodes by changing the thickness and impurity concentrations of p+-type and n+-type AlGaN constituting the TJ. By decreasing the total thickness of the TJ to 23 nm, the operating voltage reached a minimum of 8.8 V at 63 A cm−2. Further decrease in TJ thickness markedly increases the operating voltage. This finding implies that the depletion layer width becomes greater than the TJ thickness if it is smaller than 12 nm. Therefore, we conclude that the TJ thickness must be greater than the depletion layer width.
A GAME-THEORETIC APPROACH FOR THE PROCESS OF A MULTI-NODE DECENTRALIZED COMPUTING SYSTEM SIMULATING
Authors: Рожкова Т.С. 
Published: March 2022

В статье рассматривается подход к имитационному моделированию процесса функционирования многоузловой децентрализованной вычислительной системы, реализуемой совокупностью взаимодействующих вычислителей на базе мобильных терминалов.
The article considers an approach the process of functioning a multi-node decentralized computing system simulation implemented by a set of interacting computers based on mobile terminals. As a methodological basis for such simulation, is substantiated a game-theoretic approach implemented in the framework of reinforcement learning methods in multi-agent systems. A formalization of this process is given, taking into account the possibility of increasing the power of the set of possible actions of an individual compute node due to the cooperative and/or competitive interaction of a subset of compute nodes with each other. An approach to obtaining criteria for dynamic stability of a multi-node decentralized computing system used training of compute node the Nash equilibrium point is proposed.
The Effect Of Retailing Mix On Costumer Purchase Decision
Authors: Nurtanto Edy , Rusilawati Ermina , Hamzah Zulfadli , Anis Md Zohurul 
Published: March 2022

The pupose of this research was to find out the influence of price, merchandise assortment, communication mix, location, customer service, and store design and display on purchasing decisions at the supermarket CG Mart. The population that becomes the object of this research is all consumers of CG Mart supermarkets. The number of samples used in this study were 100 respondents. The method of analysis used in this study is multiple regression analysis. The results of the study partially show that price has a significant effect on purchasing decisions, merchandise assortment has a significant effect on purchasing decisions, communication mix has effect but not significant on purchasing decisions, location has effect but not significant on purchasing decisions, customer service has a significant effect on purchasing decisions. , the store design and display does have a effect but not significant on purchasing decisions. And the simultaneous research on price, merchandise assortment, communication mix, location, customer service, and store design and display have a significant influence on purchasing decisions at the supermarket CG Mart.

Keywords: Price, merchandise assortment, communication mix, location, customer service, store design and display, purchasing decision.
Retrieving the C and O Abundances of HR 7672 AB: A Solar-type Primary Star with a Benchmark Brown Dwarf
Authors: Wang 王 Ji 吉 , Kolecki Jared R. , Ruffio Jean-Baptiste , Wang 王劲 Jason J. 飞 , Mawet Dimitri , Baker Ashley , Bartos Randall , Blake Geoffrey A. , Bond Charlotte Z. , Calvin Benjamin , Cetre Sylvain , Delorme Jacques-Robert , Doppmann Greg , Echeverri Daniel , Finnerty Luke , Fitzgerald Michael P. , Jovanovic Nemanja , Liu Michael C. , Lopez Ronald , Morris Evan , Pai Asnodkar Anusha , Pezzato Jacklyn , Ragland Sam , Roy Arpita , Ruane Garreth , Sappey Ben , Schofield Tobias , Skemer Andrew , Venenciano Taylor , Kent Wallace J. , Wallack Nicole L. , Wizinowich Peter , Xuan Jerry W. 
Published: March 2022

Abstract
A benchmark brown dwarf (BD) is a BD whose properties (e.g., mass and chemical composition) are precisely and independently measured. Benchmark BDs are valuable in testing theoretical evolutionary tracks, spectral synthesis, and atmospheric retrievals for substellar objects. Here, we report results of atmospheric retrieval on a synthetic spectrum and a benchmark BD, HR 7672 B, with petitRADTRANS. First, we test the retrieval framework on a synthetic PHOENIX BT-Settl spectrum with a solar composition. We show that the retrieved C and O abundances are consistent with solar values, but the retrieved C/O is overestimated by 0.13–0.18, which is about four times higher than the formal error bar. Second, we perform retrieval on HR 7672 B using high spectral-resolution data (R = 35,000) from the Keck Planet Imager and Characterizer and near-infrared photometry. We retrieve [C/H], [O/H], and C/O to be −0.24 ± 0.05, −0.19 ± 0.04, and 0.52 ± 0.02. These values are consistent with those of HR 7672 A within 1.5σ. As such, HR 7672 B is among only a few benchmark BDs (along with Gl 570 D and HD 3651 B) that have been demonstrated to have consistent elemental abundances with their primary stars. Our work provides a practical procedure of testing and performing atmospheric retrieval, and sheds light on potential systematics of future retrievals using high- and low-resolution data.
The Observed Evolution of the Stellar Mass–Halo Mass Relation for Brightest Central Galaxies
Authors: Golden-Marx Jesse B. , Miller C. J. , Zhang Y. , Ogando R. L. C. , Palmese A. , Abbott T. M. C. , Aguena M. , Allam S. , Andrade-Oliveira F. , Annis J. , Bacon D. , Bertin E. , Brooks D. , Buckley-Geer E. , Carnero Rosell A. , Carrasco Kind M. , Castander F. J. , Costanzi M. , Crocce M. , da Costa L. N. , Pereira M. E. S. , De Vicente J. , Desai S. , Diehl H. T. , Doel P. , Drlica-Wagner A. , Everett S. , Evrard A. E. , Ferrero I. , Flaugher B. , Fosalba P. , Frieman J. , García-Bellido J. , Gaztanaga E. , Gerdes D. W. , Gruen D. , Gruendl R. A. , Gschwend J. , Gutierrez G. , Hartley W. G. , Hinton S. R. , Hollowood D. L. , Honscheid K. , Hoyle B. , James D. J. , Jeltema T. , Kim A. G. , Krause E. , Kuehn K. , Kuropatkin N. , Lahav O. , Lima M. , Maia M. A. G. , Marshall J. L. , Melchior P. , Menanteau F. , Miquel R. , Mohr J. J. , Morgan R. , Paz-Chinchón F. , Petravick D. , Pieres A. , Plazas Malagón A. A. , Prat J. , Romer A. K. , Sanchez E. , Santiago B. , Scarpine V. , Schubnell M. , Serrano S. , Sevilla-Noarbe I. , Smith M. , Soares-Santos M. , Suchyta E. , Tarle G. , Varga T. N. ,   (DES Collaboration)
Published: March 2022

Abstract
We quantify evolution in the cluster-scale stellar mass–halo mass (SMHM) relation’s parameters using 2323 clusters and brightest central galaxies (BCGs) over the redshift range 0.03 ≤ z ≤ 0.60. The precision on the inferred SMHM parameters is improved by including the magnitude gap (m
gap) between the BCG and fourth-brightest cluster member (M14) as a third parameter in the SMHM relation. At fixed halo mass, accounting for m
gap, through a stretch parameter, reduces the SMHM relation’s intrinsic scatter. To explore this redshift range, we use clusters, BCGs, and cluster members identified using the Sloan Digital Sky Survey C4 and redMaPPer cluster catalogs and the Dark Energy Survey redMaPPer catalog. Through this joint analysis, we detect no systematic differences in BCG stellar mass, m
gap, and cluster mass (inferred from richness) between the data sets. We utilize the Pareto function to quantify each parameter’s evolution. We confirm prior findings of negative evolution in the SMHM relation’s slope (3.5σ), and detect negative evolution in the stretch parameter (4.0σ) and positive evolution in the offset parameter (5.8σ). This observed evolution, combined with the absence of BCG growth, when stellar mass is measured within 50 kpc, suggests that this evolution results from changes in the cluster’s m
gap. For this to occur, late-term growth must be in the intracluster light surrounding the BCG. We also compare the observed results to IllustrisTNG 300-1 cosmological hydrodynamic simulations and find modest qualitative agreement. However, the simulations lack the evolutionary features detected in the real data.
On the Accuracy of Underground Muon Intensity Calculations
Authors: Fedynitch A. , Woodley W. , Piro M.-C. 
Published: March 2022

Abstract
Cosmic-ray muons detected by deep underground and underwater detectors have served as an information source on the high-energy cosmic-ray spectrum and hadronic interactions in air showers for almost a century. The theoretical interest in underground muons has nearly faded away because space-borne experiments probe the cosmic-ray spectrum more directly, and accelerators provide precise measurements of hadron yields. However, underground muons probe unique hadron interaction energies and phase space, which are still inaccessible to present accelerator experiments. The cosmic-ray nucleon energies reach the hundred-TeV and PeV ranges, which are barely accessible with space-borne experiments. Our new calculation combines two modern computational tools: mceq for surface muon fluxes and proposal for underground transport. We demonstrate excellent agreement with measurements of cosmic-ray muon intensities underground within estimated errors. Beyond that, the precision of historical data turns out to be significantly smaller than our error estimates. This result shows that the sources of high-energy atmospheric lepton flux uncertainties at the surface or underground can be significantly constrained without taking more data or building new detectors. The reduction of uncertainties can be expected to impact data analyses at large-volume neutrino telescopes and be used for the design of future ton-scale direct dark matter detectors.
ALMA High-resolution Multiband Analysis for the Protoplanetary Disk around TW Hya
Authors: Tsukagoshi Takashi , Nomura Hideko , Muto Takayuki , Kawabe Ryohei , Kanagawa Kazuhiro D. , Okuzumi Satoshi , Ida Shigeru , Walsh Catherine , Millar Tom J. , Takahashi Sanemichi Z. , Hashimoto Jun , Uyama Taichi , Tamura Motohide 
Published: March 2022

Abstract
We present a high-resolution (2.5 au) multiband analysis of the protoplanetary disk around TW Hya using Atacama Large Millimeter/submillimeter Array (ALMA) long baseline data at Bands 3, 4, 6, and 7. We aim to reconstruct a high-sensitivity millimeter continuum image and revisit the spectral index distribution. The imaging is performed by combining new ALMA data at Bands 4 and 6 with available archive data. Two methods are employed to reconstruct the images: multifrequency synthesis (MFS) and the fiducial image-oriented method, where each band is imaged separately and the frequency dependence is fitted pixel by pixel. We find that MFS imaging with a second-order Taylor expansion can reproduce the frequency dependence of the continuum emission between Bands 3 and 7 in a manner consistent with previous studies, and that it is a reasonable method for reconstructing the spectral index map. The image-oriented method provides a spectral index map consistent with the MFS imaging, but with a two times lower resolution. Mock observations of an intensity model were conducted to validate the images from the two methods. We find that the MFS imaging provides a high-resolution spectral index distribution with an uncertainty of <10%. Using the submillimeter spectrum reproduced from our MFS images, we directly calculate the optical depth, power-law index of the dust opacity coefficient (β), and dust temperature. The derived parameters are consistent with previous works, and the enhancement of β within the intensity gaps is also confirmed, supporting a deficit of millimeter-sized grains within the gaps.
Galaxy Power Spectrum and Biasing Results from the LOFAR Two-meter Sky Survey (First Data Release)
Authors: Tiwari Prabhakar , Zhao Ruiyang , Zheng Jinglan , Zhao Gong-Bo , Bacon David , Schwarz Dominik J. 
Published: March 2022

Abstract
The Low-Frequency Array (LOFAR) Two-meter Sky Survey (LoTSS) is an ongoing survey aiming to observe the entire northern sky, providing an excellent opportunity to study the distribution and evolution of the large-scale structure of the universe. The source catalog from the public LoTSS first data release (DR1) covers 1% of the sky, and shows correlated noise or fluctuations of the flux density calibration on scales of a few degrees. We explore the LoTSS DR1 to understand the survey systematics and data quality of this first data release. We produce catalog mocks to estimate uncertainties, and measure the angular clustering statistics of LoTSS galaxies, which fit the Lambda cold dark matter cosmology reasonably well. We employ a Markov Chain Monte Carlo–based Bayesian analysis to recover the best galaxy biasing scheme and multicomponent source fraction for LoTSS DR1 above 1 mJy assuming different possible redshift templates. After masking some noisy and uneven patches and with suitable flux density cuts, the LOFAR survey appears qualified for large-scale cosmological studies. The upcoming data releases from LOFAR are expected to be deeper and wider, and will therefore provide improved cosmological measurements.
The First Insight-HXMT Gamma-Ray Burst Catalog: The First Four Years
Authors: Song Xin-Ying , Xiong Shao-Lin , Zhang Shuang-Nan , Li Cheng-Kui , Li Xiao-Bo , Huang Yue , Guidorzi Cristiano , Frontera Filippo , Liu Cong-Zhan , Li Xu-Fang , Li Gang , Liao Jin-Yuan , Cai Ce , Luo Qi , Xiao Shuo , Yi Qi-Bin , Zheng Yao-Guang , Zhou Deng-Ke , Liu Jia-Cong , Xue Wang-Chen , Zhang Yan-Qiu , Zheng Chao , Chang Zhi , Li Zheng-Wei , Lu Xue-Feng , Zhang Ai-Mei , Zhang Yi-Fei , Jin Yong-Jie , Li Ti-Pei , Lu Fang-Jun , Song Li-Ming , Wu Mei , Xu Yu-Peng , Ma Xiang , Ge Ming-Yu , Jia Shu-Mei , Li Bing , Nie Jian-Yin , Wang Ling-Jun , Zhang Juan , Zheng Shi-Jie , Yang Xue-Juan , Yang Rong-Jia 
Published: March 2022

Abstract
The Hard X-ray Modulation Telescope (Insight-HXMT) is China’s first X-ray astronomy satellite. It was launched on 2017 June 15. The anticoincidence CsI detectors of the High Energy X-ray telescope (HE) on board Insight-HXMT could serve as an all-sky gamma-ray monitor in about 0.2–3 MeV. In its first four years of operation, Insight-HXMT has detected 322 gamma-ray bursts (GRBs) by the offline search pipeline, including blind search and targeted search. For the GOLDEN sample of Insight-HXMT GRBs, joint analyses were performed with other GRB missions, including the Fermi Gamma-ray Burst Monitor (Fermi/GBM), the Swift Burst Alert Telescope (Swift/BAT), and the Gravitational wave high-energy Electromagnetic Counterpart All-sky Monitor (GECAM). The analyses showed that Insight-HXMT can provide a better constraint on the GRB spectrum at a higher-energy band. The properties of Insight-HXMT GRBs are reported in detail, including their trigger time, duration, spectral parameters, peak fluxes of different timescales, and fluence. This catalog is an official product of the Insight-HXMT GRB team.
Ce que disent les mémoires de recherche des professeurs des écoles stagiaires sur leur appropriation des questions environnementales et de développement durable
Authors: Barroca-Paccard Marco 
Published: March 2022

Au-delà de la reconnaissance de son importance sociétale et scolaire, l’éducation environnementale et au développement durable pose des défis importants aux enseignants. Cependant, il existe peu de travaux qui se sont intéressés à cette question chez les enseignants fonctionnaires stagiaires professeurs des écoles. Ce travail utilise un corpus de plus de 398000 mots, constitué avec des mémoires de master d’étudiants issus de 11 Académies françaises qui se sont intéressés à l’enseignement de l’environnement et du développement durable. L’analyse lexicométrique a permis de montrer l’existence de 6 classes de sens qui représentent les idées et les thèmes dominants du corpus. L’ensemble montre la place centrale du mot élève ainsi que la centration sur les écogestes et sur les directives institutionnelles au détriment des dimensions critiques qui semblent très peu présentes. Le travail permet d’envisager des pistes pour mettre en œuvre une formation des professeurs des écoles conformément à la directive de généralisation de l’éducation au développement durable – EDD (MENJ, 2019).
Les Questions socialement vives et l’enseignement des sciences humaines et sociales au Québec : des visées délibératives confrontées au paradoxe curriculaire
Authors: Éthier Marc-André , Lefrançois David , Larocque Stéphanie 
Published: March 2022

Cet article vise à analyser la formation disciplinaire en sciences sociales en s’inspirant de recherches empiriques menées à propos des enjeux controversés en classe – ou « questions publiques controversées » ou encore « questions socialement vives » (QSV). L’article synthétise des travaux sur les visées délibératives de l’enseignement des sciences sociales au moyen de QSV et les effets escomptés de cet enseignement sur les élèves. Il décrit, analyse et critique ensuite l’un des programmes québécois de l’ordre secondaire liés au domaine de l’« univers social », soit le cours d’éducation financière, en tant que cas de figure des prescriptions et contenus curriculaires pouvant faire obstacle au traitement délibératif des QSV en classe.
Traité du management socio-économique
Authors: Deville Norbert , Voyant Olivier 
Published: March 2022

Une crise est un prétexte utile pour activer la réelle, pour ne pas dire unique, source de différenciation de l’entreprise, à savoir le Potentiel Humain. Il y a 10 ans, le CETAF a été confronté à une crise institutionnelle, sociale et économique. Il a fait le choix de l’Humain. Ce chapitre retrace son parcours et la manière dont la transformation a permis aux collaborateurs d’écrire l’histoire de l’entreprise plutôt que de la subir.
Traité du management socio-économique
Authors: Pesqueux Yvon , Pigé Benoît 
Published: March 2022

Le conflit normatif est un enchevêtrement de normes qui place les personnes en situation de contradiction avec ce qu’elles ont à vivre avec la société qui les entoure. La non-prise-en-compte de la conflictualité possible des normes s’explique par le processus d’a-territorialisation des normes internationales. La référence à des « parties intéressées » marque le passage d’un statut de normes techniques a-territoriales (les ISO étaient des normes « industrielles ») à celui de normes politiques. Ce passage ouvre la question d’une gouvernance multi-niveaux au niveau du territoire par consensus avec les niveaux plus éloignés.
Traité du management socio-économique
Authors: Monod Emmanuel 
Published: March 2022

Le haut niveau d’échec des projets de transformation numérique est susceptible d’être réduit par l’approche socio-économique du management, qui n’est pas seulement un système holistique de management de la performance, mais également une méthode de transformation organisationnelle. Néanmoins, les dimensions numériques de SEAM mériteraient un développement, en particulier les méthodes de développement, l’infrastructure technologique et l’architecture d’entreprise, en cohérence avec l’approche « Human-Digital Competitiveness » (HDC). Mené en cohérence avec HDC, le management socio-économique a le potentiel d’être une approche de management de la performance orientée client et humaine, qui accroîtrait le succès des transformations numériques en entreprise.
L’Église aux périphéries : le dernier voyage de Paul (Ac 27,1–28,14)
Authors: Bernard Matthieu 
Published: March 2022

Le dernier voyage de Paul joue un rôle précis dans l’ecclésiologie narrative des Actes : esquisser, de manière proleptique, la mission de l’Église aux « périphéries », les « extrémités de la terre » du programme d’Ac 1,8. Sans annonce explicite et malgré sa captivité, Paul reste un héraut de l’Évangile : il partage angoisses et espérances, nourrit d’un pain de grâce, se fait tout à tous, bénit et guérit. Des gestes inspirants pour la mission de l’Église, encore aujourd’hui.
La déchéance de nationalité devant la Cour suprême du Royaume-Uni : déférence judiciaire et sécurité nationale
Authors: Pougnet Rachel 
Published: March 2022

Pour la troisième fois en l’espace de dix ans, la Cour suprême du Royaume-Uni a été confrontée à une mesure de déchéance de nationalité adoptée par le gouvernement britannique. Dans un arrêt « Begum » de février 2021, la Cour Suprême décide que Shamima Begum ne doit pas être autorisée à revenir sur le territoire britannique pour y conduire son appel contre sa déchéance de nationalité. La Cour suprême fait acte d’une importante déférence judiciaire face à des arguments de sécurité nationale. En effet, elle confère une large marge de manœuvre au gouvernement lors de l’examen des conditions de mise en œuvre de la déchéance de nationalité, à raison de la proximité de cette mesure avec des intérêts de sécurité nationale. La Cour suprême procède également à une mise en balance du droit à un recours effectif et du droit à un procès équitable face à des considérations sécuritaires.