bluuebunny/crossref_metadata_2025_split huggingface dataset:
Проксемная сравнительно-сопоставительная модель арабского мира в публицистических текстах (на материале статей об архитектуре в журналах «Вокруг света» и National Geographic)
Authors: А.В. Колядин 
Published: November 2024

В статье рассматриваются проксемы как лексические компоненты дискурсивного информативного кода, интерпретируемого в качестве совокупности лексико-грамматических и синтаксических информативов в публицистическом дискурсе. Лингвистический анализ разноязычных публицистических форматов — статей А. Егорина «Ворота Востока» и С. Талреджа Cairo beyond the pyramids: The ultimate itinerary — позволил рассмотреть дискурсивную проекцию пространственного культурного кода в его англоязычной и русскоязычной формах, что способствовало созданию авторской классификации проксемических единиц, которая представляет собой совокупность пяти типов проксем: 1) проксемы, характеризующие расстояние между объектами; 2) проксемы, характеризующие направление движения; 3) проксемы, описывающие пространственную трансформацию объектов; 4) проксемы, определяющие размеры объектов (высота, ширина); 5) проксемы, характеризующие расположение объектов относительно друг друга.
The article deals with proxemes as the lexical components of a discursive informative code, interpreted as a set of lexico-grammatical and syntactic informatives in the journalistic discourse. The linguistic analysis of multilingual journalistic formats as well as of the journalistic articles Gate of the East by A. Egorin and Cairo beyond the pyramids: The ultimate itinerary by S. Talrej made it possible to consider the discursive projection of the spatial cultural code in its English and Russian forms, which contributed to the creation of the author’s classification of proxemes. This set includes 5 types of proxemes: proxemes characterizing the distance between objects, proxemes that characterize the direction of movement — 4 units, proxemes that describe the spatial transformation of objects, proxemes that determine the dimensions of objects (height, width), proxemes that characterize the location of objects relative to each other.
Overview of the Fiber System for the Dark Energy Spectroscopic Instrument
Authors: Poppett Claire , Tyas Luke , Aguilar J. , Bebek Christopher , Bramall D. , Claybaugh T. , Edelstein J. , Fagrelius P. , Heetderks H. , Jelinsky P. , Jelinsky S. , Lafever Robin , Lambert A. , Lampton M. , Levi Michael E. , Martini P. , Rockosi C. , Schmoll J. , Sharples Ray M. , Sirk Martin , Wishnow Edward , Yu Jiaxi , Ahlen S. , Bault A. , BenZvi S. , Brooks D. , Cole S. , de la Macorra A. , Dey Arjun , Doel P. , Fanning K. , Font-Ribera A. , Forero-Romero J. E. , Gaztañaga E. , Gontcho A Gontcho S. , Gonzalez-Morales A. X. , Hahn C. , Honscheid K. , Jimenez J. , Juneau S. , Kirkby D. , Kremin A. , Landriau M. , Le Guillou L. , Manera M. , Meisner A. , Miquel R. , Moustakas J. , Mueller E. , Muñoz-Gutiérrez A. , Myers A. D. , Nie J. , Niz G. , Palanque-Delabrouille N. , Percival W. J. , Prada F. , Rabinowitz D. , Rezaie M. , Rossi G. , Sanchez E. , Schlafly Edward F. , Schlegel D. , Schubnell M. , Seo H. , Sprayberry D. , Tarlé G. , Vargas-Magaña M. , Weaver B. A. , Zhou R. 
Published: November 2024

Abstract
The Dark Energy Spectroscopic Instrument (DESI) is a revolutionary instrument designed for precise measurements of cosmic distances and the investigation of dark energy. DESI utilizes 5000 optical fibers to simultaneously measure the spectra of distant objects and aims to measure 40 million galaxies and quasars in a 5 yr survey. One of the critical challenges to DESI’s success was ensuring that the fiber system was not only highly efficient but also delivered a highly stable beam enabling more reliable sky subtraction for measurements of faint objects. We achieved this stability by minimizing the stress on the fiber system during the manufacture and operation of the telescope and fiber positioning robots. We installed the DESI fiber system on the 4 m Mayall telescope with ≥99% of fibers intact, and the instrument has delivered superb optical performance throughout the initial years of the DESI survey, including ≥90% average throughput when injected with a focal ratio of ∼f/3.9 as delivered by the primary focus corrector, excluding fiber absorption losses. The design of DESI required multiple innovations to achieve these requirements, such as cleaved fibers bonded with a UV-curing epoxy to glass ferrules in the focal plane and fusion splicing instead of physical connectors. In this paper, we describe the development, delivery, and installation of the fiber system, the innovations that made the state-of-the-art performance possible, and the key lessons learned that could benefit future projects.
Migration of Accreting Planets and Black Holes in Disks
Authors: Laune JT , Li 李 Rixin 日新 , Lai Dong 
Published: November 2024

Abstract
Nascent planets are thought to lose angular momentum (AM) to the gaseous protoplanetary disk via gravitational interactions, leading to inward migration. A similar migration process also applies to stellar-mass black holes (BHs) embedded in the disks of active galactic nuclei. However, AM exchange via accretion onto the planet/BH may strongly influence the migration torque. In this study, we perform 2D global hydrodynamic simulations of an accreting planet/BH embedded in a disk, where AM exchange between the planet/BH and disk via gravity, accretion, pressure, and viscosity are considered. When accretion is turned off, we recover the linear estimate for Type I migration torque. However, for the two planet masses we investigated with our accreting simulations, we find outward migration due to the positive AM deposited onto the accreting body by the disk gas. Our simulations achieve the global steady state for the transport of mass and AM: The mass and AM fluxes are constant across the disk except for jumps (

Δ

M

̇

and

Δ

J

̇

) at the planet’s location, and the jumps match the accretion rate and torque on the planet. Our findings suggest that caution is needed when applying the standard results of disk migration to accreting planets and BHs.
Spectroscopic Study of Heating Distributions and Mechanisms Using Hinode/EIS
Authors: Ishigami Shun , Hara Hirohisa , Oba Takayoshi 
Published: November 2024

Abstract
Heating distributions along coronal loops are obtained from spectroscopic data with the Hinode/EUV Imaging Spectrometer. The loop half-lengths L
half are in the range of 24–107 Mm for our analysis of 18 loops. By using the analytical approximations to 1D hydrostatic numerical calculations of electron temperature T

e
(s) and density distributions n

e
(s) along a loop, the heating distribution that decreases with a heating scale height s

H
toward the loop top with a heating rate E
0 at the height of the transition region is estimated by applying a Bayesian analysis to the observed T

e
(s) and n

e
(s) derived by emission line ratios. We obtain s

H
= 10 ± 4 Mm increasing with L
half, E
0 = 10−2.0±0.5 erg cm−3 s−1 decreasing with L
half, and the heating flux F

H
= 107.0±0.4 erg cm−2 s−1. These loops show s

H
/L
half = 0.21 ± 0.07, suggesting the concentration of the heating near the lower part. Compared to the previous study using imaging data, s

H
is comparable, while E
0 and F

H
are about an order of magnitude larger. We find that using the imaging data leads to the underestimation of the electron density and consequently the underestimation of E
0 and F

H
. We examine heating mechanisms using the power-law relation for F

H
, the field strength B
base and L
half:

F

H

∝

B

base

β

L

half

λ

. We find

β
=

1.04

−
0.36

+
0.18

and

λ
=
−

0.99

−
0.05

+
0.04

, which show that the reconnection heating model is the most plausible.
Ensemble Kalman Filter Data Assimilation into the Surface Flux Transport Model to Infer Surface Flows: An Observing System Simulation Experiment
Authors: Dash Soumyaranjan , DeRosa Marc L. , Dikpati Mausumi , Sun 孙 Xudong 旭东 , Mahajan Sushant S. , Liu 刘 Yang 扬 , Hoeksema J. Todd 
Published: November 2024

Abstract
Knowledge of the global magnetic field distribution and its evolution on the Sun’s surface is crucial for modeling the coronal magnetic field, understanding the solar wind dynamics, computing the heliospheric open flux distribution, and predicting the solar cycle strength. As the far side of the Sun cannot be observed directly and high-latitude observations always suffer from projection effects, we often rely on surface flux transport (SFT) simulations to model the long-term global magnetic field distribution. Meridional circulation, the large-scale north–south component of the surface flow profile, is one of the key components of the SFT simulation that requires further constraints near high latitudes. Prediction of the photospheric magnetic field distribution requires knowledge of the flow profile in the future, which demands reconstruction of that same flow at the current time so that it can be estimated at a later time. By performing Observing System Simulation Experiments, we demonstrate how the ensemble Kalman filter technique, when used with an SFT model, can be utilized to make “posterior” estimates of flow profiles into the future that can be used to drive the model forward to forecast the photospheric magnetic field distribution.
Astrometric Jitter as a Detection Diagnostic for Recoiling and Slingshot Supermassive Black Hole Candidates
Authors: Uppal Anavi , Ward Charlotte , Gezari Suvi , Natarajan Priyamvada , Chen Nianyi , LaChance Patrick , Di Matteo Tiziana 
Published: November 2024

Abstract
Supermassive black holes (SMBHs) can be ejected from their galactic centers due to gravitational wave recoil or the slingshot mechanism following a galaxy merger. If an ejected SMBH retains its inner accretion disk, it may be visible as an off-nuclear active galactic nucleus (AGN). At present, only a handful of offset AGNs that are recoil or slingshot candidates have been found, and none have been robustly confirmed. Compiling a large sample of runaway SMBHs would enable us to constrain the mass and spin evolution of binary SMBHs and study feedback effects of displaced AGNs. We adapt the method of varstrometry—which was developed for Gaia observations to identify off-center, dual, and lensed AGNs—in order to quickly identify off-nuclear AGNs in optical survey data by looking for an excess of blue versus red astrometric jitter. We apply this to the Pan-STARRS1 3π Survey and report on five new runaway AGN candidates. We focus on ZTF18aajyzfv: a luminous quasar offset by 6.7 ± 0.2 kpc from an adjacent galaxy at z = 0.224, and conclude after Keck LRIS spectroscopy and comparison to ASTRID simulation analogs that it is likely a dual AGN. This selection method can be easily adapted to work with data from the soon-to-be commissioned Vera C. Rubin Telescope Legacy Survey of Space and Time (LSST). LSST will have a higher cadence and deeper magnitude limit than Pan-STARRS1, and should permit detection of many more runaway SMBH candidates.
Thermodynamics of Giant Molecular Clouds: The Effects of Dust Grain Size
Authors: Soliman Nadine H. , Hopkins Philip F. , Grudić Michael Y. 
Published: November 2024

Abstract
The dust grain size distribution (GSD) likely varies significantly across star-forming environments in the Universe, but its impact on star formation remains unclear. This ambiguity arises because the GSD interacts nonlinearly with processes like heating, cooling, radiation, and chemistry, which have competing effects and varying environmental dependencies. Processes such as grain coagulation, expected to be efficient in dense star-forming regions, reduce the abundance of small grains and increase that of larger grains. Motivated by this, we investigate the effects of similar GSD variations on the thermochemistry and evolution of giant molecular clouds (GMCs) using magnetohydrodynamic simulations spanning a range of cloud masses and grain sizes, which explicitly incorporate the dynamics of dust grains within the full-physics framework of the STARFORGE project. We find that grain size variations significantly alter GMC thermochemistry: the leading-order effect is that larger grains, under fixed dust mass, GSD dynamic range, and dust-to-gas ratio, result in lower dust opacities. This reduced opacity permits interstellar radiation field and internal radiation photons to penetrate more deeply. This leads to rapid gas heating and inhibited star formation. Star formation efficiency is highly sensitive to grain size, with an order-of-magnitude reduction when grain size dynamic range increases from 10−3–0.1 μm to 0.1–10 μm. Additionally, warmer gas suppresses low-mass star formation, and decreased opacities result in a greater proportion of gas in diffuse ionized structures.
Alleviating H
0 and S
8 Tensions Simultaneously in K-essence Cosmology
Authors: Hosseini Mansoori Seyed Ali , Moshafi Hossein 
Published: November 2024

Abstract
The present work begins by examining the early-Universe inflationary epoch of a special K-essence model, which incorporates a linear coupling term between the scalar field potential and the canonical Lagrangian. For the power-law potential, we both numerically and analytically prove that the inflationary parameters such as the spectral index and tensor-to-scalar ratio are compatible with the recent BICEP/Keck observations. Continuing this work, our analysis based on comparing early-Universe observations with late-Universe measurements indicates that the tension on the Hubble parameter H
0 and the growth of structure parameter S
8 can be alleviated simultaneously. More precisely, compared to the standard ΛCDM model, our model can reduce H
0 tension to roughly 2.2σ, and the S
8 discrepancy diminishes to 0.82σ.
FluxCT V2.0: Updates to a Web Tool Identifying Contaminating Flux in Space Telescope Data
Authors: Dong Zilin , Schonhut-Stasik Jessica , Stassun Keivan 
Published: November 2024

Abstract
We present FluxCT V2.0, an updated web tool for identifying contaminating flux in Kepler and TESS target pixel files. FluxCT V2.0 focuses on enhancing functionality, user experience, and data processing capabilities. We resolved existing issues to allow for an extended user base, removed known bugs, and extended the tool to any TESS pixel file, allowing the user to search any TESS point object. A batch code for TESS is now available on the companion GitHub. Additional output parameters, such as amplitude dilution and a magnitude cut, have been added to the tool, allowing users more freedom to analyze the possible effects of target sources.
Health Literacy Directed Weight Loss Intervention in Primary Care Clinics
Authors: Davis Terry , Arnold Connie , Zhang Dachuan , Martin Corby K. , Newton Robert L. , Myers Candice , Denstel Kara D. , Mire Emily F. , Höchsmann Christoph , Apolzan John , Katzmarzyk Peter T. ,   for the PROPEL Research Group
Published: November 2024

Background
Low income and low health literacy are associated with poorer health knowledge, health behaviors and poor health outcomes. The effectiveness of health literacy-directed weight loss treatment interventions in primary care clinics is lacking.

Objective
The aim of this study was to conduct a pragmatic cluster-randomized trial (PROmoting Successful Weight Loss in Primary CarE in Louisiana ([PROPEL]) to test the effectiveness of a 24-month, patient-centered, literacy-directed obesity treatment program delivered within primary care in an underserved population. This study reports the association between health literacy and program effectiveness, examining potential correlates of weight loss related to patient adherence to the program.

Methods
We randomly assigned 18 clinics to usual care (UC) or a health literacy-directed lifestyle intervention (HLI). The primary outcome was percent weight loss at 24 months.

Key Results

Of 803 adult participants (84% women; 67% Black), 31% had limited health literacy. Patients in UC lost an average of 0.44%of their enrollment weight after 24 months. Those with adequate literacy lost 0.57% and those with limited literacy lost 0.30%, which was not significantly different. The HLI patient group lost an average of 4.9% of their enrollment weight. Those with adequate literacy lost 5.2% and those with limited literacy, 4.7%, which was not significantly different. The advantage of adequate health literacy was consistent across the 24-month study period, though not significant. Patients in the HLI group with adequate health literacy had greater percent weight loss by a margin of 0.50 ± 0.75 (
p
= .50), while the UC margin was 0.27 ± 0.84 (
p
= .74). The percent weight loss difference between HLI and UC groups was 4.6 ± 0.8 (
p
< .001) among patients with adequate health literacy and 4.4 ± 1.0 (
p
< .001) among patients with limited health literacy. The difference in percent weight loss between the HLI and UC groups was 0.2 ± 1.1 (
p
= .84) higher for adequate literacy patients.

Conclusions

A health literacy directed health coaching intervention in community clinics led to significant weight loss over 24 months but did not vary by level of patient health literacy. [

HLRP: Health Literacy Research and Practice
. 2024;8(4):e204–e211.

]
Péchés de jeunesse
Authors: Nuq Amélie 
Published: November 2024

Dans Los mares del Sur (1979), le détective Pepe Carvalho, héros des romans de l’écrivain Manuel Vázquez Montalbán, affirme faire partie de la génération de Barcelonais qui a grandi sous la menace d’un internement à l’Asilo Durán. Si elle est encore présente aujourd’hui dans la mémoire collective barcelonaise, cette institution corrective est, comme celles qui étaient réparties sur l’ensemble du territoire espagnol depuis le début du xxe siècle, très peu connue des historiens. L’ouvrage se propose de combler cette lacune et de documenter le sort des « voyous » et des « filles déchues » internés durant la période de la dictature franquiste (1939-1975) dans deux maisons de redressement, l’Asilo Durán et la Colonia San Vicente Ferrer de Valence. Il s’agit tout autant d’en franchir les murs pour documenter, malgré les silences des archives, la vie quotidienne des pensionnaires, que d’observer durant toute la durée de la dictature les rapports entre le pouvoir franquiste, l’Église catholique et les habitants des quartiers populaires et marginaux des grandes villes espagnoles.Même pendant la période de l’immédiat après-guerre civile, marquée par une répression impitoyable et par la volonté d’écraser les vaincus, les maisons de redressement ne constituent étonnamment pas un lieu de répression politique dans lequel les enfants de « rouges » seraient surreprésentés. En revanche, le caractère profondément traditionnaliste et religieux de la prise en charge de la jeunesse dangereuse et en danger est très clair, ce qui permet de caractériser plus finement encore la nature d’un régime qui ne cesse de poser question aux historiens.
De nouvelles données sur un sanctuaire diablinte : le site de la Fermerie à Juvigné (Mayenne) du iie s. av. n. è. au ive s. de n. è.
Authors: Bossard Stanislas , Dufay-Garel Yann , Aubin Gérard , Meissonnier Jacques , Reich Guillaume , Camus Adrien , Garnier Nicolas , Mathé Vivien , Mortreau Maxime , Rolland Joëlle 
Published: November 2024

Des prospections pédestres (2015), suivies d’une campagne de fouille programmée et d’investigations géophysiques (2016), ont fourni de multiples informations inédites sur un sanctuaire de l’âge du Fer et de l’époque romaine découvert et sondé dans les années 1980 à Juvigné (Mayenne). Cet article présente les résultats de ces récentes interventions, en décrivant d’abord le mode de clôture de l’aire sacrée, puis en s’intéressant à son organisation interne et à ses équipements. Un imposant fossé, des trous de poteau, témoins de probables constructions en matériaux périssables, et une série de fosses, ayant notamment servi à enfouir des objets manipulés dans le cadre des activités religieuses, constituent les aménagements d’un premier sanctuaire de l’époque gauloise. À ces structures succèdent ensuite, au cours du Haut-Empire, un péribole maçonné et un temple, d’abord de plan circulaire, puis à cella centrale et galerie périphérique de plan quadrangulaire. Aussi, l’examen du mobilier est riche en enseignements au sujet des pratiques rituelles, en particulier pour l’âge du Fer, période à laquelle peut être rattaché un grand nombre d’objets (armes, parures et accessoires vestimentaires, outils, monnaies, céramique et plaques foyères). Quelques fibules, des monnaies, une figurine de cervidé et de rares fragments de céramique, renvoient à la phase romaine du site et peuvent correspondre, en tout ou partie, à des offrandes. Ce sanctuaire, dont l’évolution peut être retracée dans les grandes lignes à partir des données recueillies depuis les années 1980, devait constituer l’un des espaces cultuels les plus importants de la cité dont il relevait, que l’on suppose avoir été celle des Aulerques Diablintes, dont il occupait vraisemblablement les confins occidentaux. Au regard de sa longévité, de son ampleur, de ses équipements et de son évolution, il semble alors probable d’y voir l’un des lieux de culte publics de la civitas, mais on ignore encore s’il intégrait une agglomération de son territoire ou s’il était isolé dans les campagnes diablintes.
Harnessing Regulatory invariant Natural Killer T cells in Autoimmune Liver Disease Treatment
Authors: Sokke Umeshappa Channakeshava , Hebbandi Nanjundappa Roopa , Babu Kolla Harish 
Published: November 2024

Abstract
Invariant Natural Killer T cells (iNKTs) are pivotal innate T cells that regulate immunity through cytokine secretion. In extra-hepatic autoimmunity, distinct regulatory iNKT cell types (iNKTR) play crucial roles. Recently, we identified a novel liver-specific subset, Maf+LiNKTR1 cells, characterized by its CD4+ TR1-like transcriptional signature. This subset responds to lipid-antigen-presenting nanomedicines, suppressing liver autoimmunity; however, its role under homeostatic conditions, in autoimmunity development, and responsiveness to other iNKT-directed therapies are not known. Using mouse models of Primary Biliary Cholangitis (PBC), here we explored the immunoregulatory role and therapeutic potential of Maf+LiNKTR1 cells. We observed a significant decrease in Maf+LiNKTR1 in PBC, accompanied by increased proinflammatory LiNKT1 subset. Biliary epithelial IL-10 signaling and gut-derived short-chain fatty acids contributed to Maf+LiNKTR1 generation. The reduced Maf+LiNKTR1 frequency correlated with loss of regulatory networks, suggesting a role in maintaining liver tolerance. Importantly, the subset responded to other iNKT-directed drugs, significantly suppressing PBC. Our study extended to the broader regulatory network of Maf+LiNKTR1. Further, it enhances our understanding of Maf+LiNKTR1 in liver health and autoimmunity development, offering potential therapeutic insights for autoimmune and other inflammatory liver conditions.