bluuebunny/crossref_metadata_2025_split huggingface dataset:
Diagnostic information in GP referral letters to a memory clinic: a retrospective cohort study
Authors: Ronner Demi , Oostra Dorien , Claassen Jurgen , Richard Edo , Perry Marieke 
Published: February 2025

BackgroundDementia diagnostics can often be performed in primary care, yet older people with memory complaints are frequently referred to memory clinics (MCs).AimTo compare diagnostic information in GP referral letters of patients with and without an eventual dementia diagnosis.Design & settingRetrospective cohort study in a Dutch academic MC.MethodWe collected electronic health record (EHR) data of consecutive patients aged ≥65 years referred by their GP between 2016 and 2020. EHR data included patient characteristics, diagnostic information in referral letters, ancillary investigations performed at the MC, and established diagnoses. We performed χ2tests to compare groups.ResultsOf 651 patients included, the average age was 78.0 years (standard deviation 6.8) and 348 (53.5%) were diagnosed with dementia. Most people with dementia were diagnosed without ancillary investigations (n= 235/348, 67.5%). In GP referral letters of people with dementia compared with people without dementia, a collateral history, any physical examination, a differential diagnosis including dementia, a Mini-Mental State Examination score, interference with daily functioning, and decline from previous levels of functioning were mentioned more often. Furthermore, the more diagnostic criteria mentioned in the referral letter, the more often dementia was diagnosed at the MC (no criteria: 35.4%; one criterion: 47.3%; two criteria: 53.4%; three criteria: 69.9%; and four or five criteria: 83.3%).ConclusionGPs often correctly mention diagnostic information and dementia criteria in referral letters of people with dementia, and they are often diagnosed without ancillary investigations. This suggests that referral is often unnecessary, and GPs can be empowered to diagnose dementia themselves.
Современные направления развития организации обслуживания пассажиров в железнодорожных вокзальных комплексах
Authors: Марущак Т.Б. 
Published: February 2025

В настоящее время продолжается активное развитие железнодорожных вокзалов с целью их превращения в современные транспортно-пересадочные узлы с развитой общественно-деловой функцией, направленной на удовлетворение многообразных потребностей всех категорий клиентов ОАО «РЖД». В статье представлены результаты анализа современных тенденций организации обслуживания пассажиров в вокзальных комплексах и определены приоритетные направления совершенствования сервисных зон на вокзалах.
At present, active development of railway stations continues with the aim of turning them into modern transport and interchange hubs with a developed social and business function aimed at satisfying the diverse needs of all categories of JSCo ‘Russian Railways’ customers. The article presents the results of the analysis of current trends in the organisation of passenger service in railway station complexes and identifies priority areas for improving service areas at railway stations.
Ключевые детерминанты цифровой трансформации агропромышленного комплекса: человеческий фактор
Authors: Неганова В.П. 
Published: February 2025

В статье анализируется роль человеческого фактора в процессе внедрения цифровых технологий на предприятиях российского агропромышленного комплекса. Представлены результаты пилотного исследования основных детерминант, которые негативно или позитивно влияют на отношения сотрудников к внедрению цифровых технологий. Доказана значимость оценки их восприятия и интерпретации процессов цифровой трансформации как ключевого условия эффективности происходящих изменений.
The article analyzes the role of the human factor in the process of implementing digital technologies at enterprises of the Russian agro-industrial complex. The results of a pilot study of the main determinants that negatively or positively affect employees' attitudes towards the implementation of digital technologies are presented. The importance of assessing their perception and interpretation of digital transformation processes as a key condition for the effectiveness of the ongoing changes is proven.
Эффективность региональной системы здравоохранения: рейтинг субъектов Российской Федерации
Authors: Боченина М.В. , Кургина С.М. , Музалевская С.А. , Янгиров Т.А. 
Published: February 2025

В статье рассматриваются вопросы построения рейтинга субъектов Российской Федерации по эффективности региональных систем здравоохранения, что является актуальным в рамках национального проекта «Здравоохранение». Анализ исследуемых показателей проведен методами кластерного анализа, оболочечного анализа данных DEA (Data Envelopment Analysis). Предложена авторская методика построения рейтинга на основе многомерной средней, которая предполагает наличие однородной совокупности.
The article examines the issues of constructing a rating of subjects of the Russian Federation by the effectiveness of regional health care systems, which is relevant within the framework of the national project "Healthcare". The analysis of the studied indicators was carried out using the methods of cluster analysis, data envelopment analysis DEA (Data Envelopment Analysis). The author's methodology of rating construction based on the multidimensional average, which assumes the presence of a homogeneous population, is proposed.
Перспективы и возможности оптимизации процесса адаптации персонала в организации
Authors: Галина А.Э. , Абдуллин Р.В. , Абдуллина Д.А. 
Published: February 2025

В статье рассмотрена возможность оптимизации процесса адаптации персонала с учетом особенностей современного рынка труда. Разработан бизнес-процесс адаптации персонала с использованием современных инструментов.
The article considers the possibility of optimizing the process of personnel adaptation, taking into account the peculiarities of the modern labor market. The business process of personnel adaptation using modern tools has been developed.
Pour une modernité antimoderne
Authors: Jaccard Jean-Philippe 
Published: February 2025

Dans les dernières années du vingtième siècle, la tendance à faire le procès de l’avant-garde a connu un certain succès, en faisant de celle-ci le stade préparatoire de l’art totalitaire qui se développera dans les dictatures à partir des années trente. Cette tendance, qu’elle soit en partie convaincante et intelligente (I. Golomstock), ou alors tendancieuse et bancale (B. Groys), mérite d’être corrigée, ou en tout cas fortement nuancée. Tout est parti d’un malentendu au lendemain de 1917, quand certains acteurs de l’avant-garde se sont crus investis d’une mission d’accompagnement de la révolution politique (V. Majakovskij, N. Punin, le LEF, etc.). Toutefois, juger l’avant-garde à l’aune de sa variante politisée, en oubliant ceux qui sont restés des rebelles « en-dehors de la révolution », ne saurait donner un tableau complet. Les zaumniki de Tiflis et de Moscou (A. Kručënyh, I. Zdanevič, I. Terent’ev), ceux Leningrad (A. Tufanov et le Flanc de gauche) et, après eux, l’OBÈRIU, dernière association « de gauche », sont étrangement absents de ces démonstrations à charge. Pourtant, ce sont bien eux, et non pas les ralliés au pouvoir soviétique, qui marquent une étape dans le développement organique de l’avant-garde russe, laquelle se transformera, comme dans toute l’Europe, en cette littérature « de l’inquiétude » annonçant l’avènement de l’existentialisme et de la littérature de l’absurde. Et ceux-là méritent d’être qualifiés d’« antimodernes », selon l’expression introduite par A. Compagnon pour désigner ceux qui ont très vite compris que ce progrès dont se gargarisait la révolution était une notion dépourvue de sens dans les domaines de la littérature et de l’art. Le même terme peut s’appliquer aux acteurs de l’underground (1950-1980) et aux actionistes des dernières années, permettant de dresser un schéma plus convaincant de l’évolution de la littérature russe aux XXe-XXIe siècles.
Resistance reduction in laser-thermally transferred carbon nanotube wirings on plastic films via CuI doping
Authors: Matsunami Takahiro , Takanashi Kotaro , Ikuno Takashi 
Published: February 2025

Abstract
We present a straightforward method to dramatically reduce the resistance of multi-walled carbon nanotube (MWNT) wirings on polyethylene (PE) films. By introducing CuI doping during laser thermal transfer, we achieved a resistance as low as 166 Ω cm−1—an 80% reduction compared to non-doped samples—without altering the wiring geometry. This scalable approach enhances conductivity and allows precise resistivity control. With its simplicity, efficiency, and adaptability, this method addresses key challenges in flexible electronics, paving the way for lightweight, high-performance carbon-based devices in advanced applications.
Common sources of linguistic conflict engage domain-general conflict control mechanisms during language comprehension
Authors: Boudewyn Megan A. , Xu Yaqi , Rosenfeld Ashley R. , Caines Nathan P. 
Published: February 2025

Abstract
The current study tested the hypothesis that lexical ambiguity, a common source of representational conflict during language comprehension, engages domain-general cognitive control processes that are reflected by theta-band oscillations in scalp-recorded electroencephalograms (EEG). In Experiment 1, we examined the neural signature elicited by lexically ambiguous compared to unambiguous words during sentence comprehension. The results showed that midfrontal theta activity was increased in response to linguistic conflict (lexical ambiguity). In Experiment 2, we examined postconflict adaptation effects by comparing temporarily ambiguous sentences that followed previous instances of conflict (other temporarily ambiguous sentences) to those that followed a previous low-conflict (unambiguous) sentence. A midfrontal theta effect associated with linguistic conflict was again found in Experiment 2, such that theta was increased for temporarily ambiguous sentences that followed previous low-conflict (unambiguous) sentences compared with those that followed previous high-conflict (temporarily ambiguous) sentences. In both experiments, facilitated lexical semantic processing was also observed for words that came after the point of conflict, which may reflect a downstream “benefit” of cognitive control engagement. Overall, our results provide novel insights into the neurocognitive mechanisms underlying conflict processing in language comprehension and suggest that the same neural computations are involved in processing nonlinguistic and linguistic conflict.
Tiered honorification in Eastern Indo-Aryan: A [HON]-less proposal
Authors: Wang Ruoan 
Published: February 2025

Longstanding tradition in the literature uses a [HON] feature to analyze tiered honorification systems of Indo-Aryan. This work presents a stark opposition to that tradition, using Wang’s (2023) framework based on a pragmatic calculus, which crucially does not make use of [HON]. I adapt such a framework to show how it can explain both the diachronic and synchronic properties of tiered systems.
High-Quality Sound Recovery of Moving Sound Source Using Millimeter-Wave Radio
Authors: Xiong Yuyong , Liu Zhaoyu , Tang Xiangyi , Meng Haibin , Peng Zhike 
Published: February 2025

The emerging millimeter-wave microphones have garnered considerable attention in recent years due to their potential for sound detection in various applications, particularly in situations where traditional microphones may be impractical. However, despite their promise, there is a notable lack of evidence demonstrating high-quality sound recovery of moving sources, which remains a significant challenge in the field. This paper addresses this critical gap by proposing a novel method for displacement alignment that improves the detection and recovery of sound signals from moving sources. The proposed method works by first aligning the displacement of the sound source over time, which ensures that the signals are synchronized and avoids interference from movement of sources. Subsequently, precise surface vibrations are extracted from the aligned signals, providing data for sound recovery. A finite impulse response (FIR) filter is applied to remove low-frequency motion, which often interferes with the clarity of the detected sound. Experimental results demonstrate the method’s effectiveness in recovering high-quality sound from moving sources, offering a promising solution for advancing the emerging millimeter-wave microphone technology in real-world applications. This work could pave the way for more accurate and reliable sound detection systems, particularly in dynamic environments.

Conflict of Interest Statement
The authors declare no conflicts of interest.
PAH Feature Ratios around Stellar Clusters and Associations in 19 Nearby Galaxies
Authors: Dale Daniel A. , Graham Gabrielle B. , Barnes Ashley T. , Baron Dalya , Bigiel Frank , Boquien Médéric , Chandar Rupali , Chastenet Jérémy , Chown Ryan , Egorov Oleg V. , Glover Simon C. O. , Hands Lindsey , Henny Kiana F. , Indebetouw Remy , Klessen Ralf S. , Larson Kirsten L. , Lee Janice C. , Leroy Adam K. , Maschmann Daniel , Pathak Debosmita , Rodríguez M. Jimena , Rosolowsky Erik , Sandstrom Karin , Schinnerer Eva , Sutter Jessica , Thilker David A. , Weinbeck Tony D. , Whitmore Bradley C. , Williams Thomas G. , Wofford Aida 
Published: February 2025

Abstract
We present a comparison of observed polycyclic aromatic hydrocarbon (PAH) feature ratios in 19 nearby galaxies with a grid of theoretical expectations for near- and mid-infrared dust emission. The PAH feature ratios are drawn from Cycle 1 JWST observations and are measured for 7224 stellar clusters and 29,176 stellar associations for which we have robust ages and mass estimates from Hubble Space Telescope five-band photometry. Though there are galaxy-to-galaxy variations, the observed PAH feature ratios largely agree with the theoretical models, particularly those that are skewed toward more ionized and larger PAH size distributions. For each galaxy we also extract PAH feature ratios for 200 pc wide circular regions in the diffuse interstellar medium, which serve as a noncluster/association control sample. Compared to what we find for stellar clusters and associations, the 3.3 μm/7.7 μm and 3.3 μm/11.3 μm ratios from the diffuse interstellar medium are ∼0.10–0.15 dex smaller. When the observed PAH feature ratios are compared to the radiation field hardness as probed by the [O iii]/Hβ ratio, we find anticorrelations for nearly all galaxies in the sample. These results together suggest that the PAH feature ratios are driven by the shape and intensity of the radiation field and that the smallest PAHs—observed via JWST F335M imaging—are increasingly “processed” or destroyed in regions with the most intense and hard radiation fields.
Spin Evolution and Mass Distribution of Galactic Binary Neutron Stars
Authors: Chu Qingbo , Lu 陆 Youjun 由俊 , Yu Shenghua 
Published: February 2025

Abstract
Binary neutron stars (BNSs) detected in the Milky Way have total masses distributing narrowly around ∼2.6–2.7M
⊙, while the BNS merger GW190425 detected via a gravitational wave has a significantly larger mass (∼3.4M
⊙). This difference is not well understood, yet. In this paper, we investigate the BNS spin evolution via an improved binary star evolution model and its effects on the BNS observability, with the implementation of various relevant astrophysical processes. We find that the first-born neutron star component in low-mass BNSs can be spun up to millisecond pulsars by the accretion of Roche-lobe overflow from its companion and its radio lifetime can be comparable to the Hubble time. However, most high-mass BNSs have substantially shorter radio lifetimes than low-mass BNSs, and thus a smaller probability of being detected via radio emission. Adopting the star formation and metal enrichment history of the Milky Way given by observations, we obtain the survived Galactic BNSs with pulsar components from our population synthesis model and find that their distributions on the diagrams of the spin period versus the spin period time derivative (

P
−

P

̇

) and the orbital period versus the eccentricity (P
orb–e) can well match those of the observed Galactic BNSs. The total mass distribution of the observed Galactic BNSs can also be matched by the model. A significant fraction (∼19%–22%) of merging BNSs at redshift z ∼ 0 have masses ≳3M
⊙, which seems compatible with the GW observations. Future radio observations may detect many more Galactic BNSs, which will put strong constraints on the spin evolution of BNSs during their formation processes.
Toward Early-type Eclipsing Binaries as Extragalactic Milestones. IV. Physical Properties of Three Detached O/B-type Systems in the LMC
Authors: Taormina Mónica , Pietrzyński G. , Kudritzki R.-P. , Pilecki B. , Thompson I. B. , Puls J. , Górski M. , Zgirski B. , Graczyk D. , Urbaneja M. A. , Gieren W. , Narloch W. , Hajdu G. 
Published: February 2025

Abstract
We present a complete set of physical parameters for three early-type eclipsing binary systems in the Large Magellanic Cloud (LMC): OGLE LMC-ECL-17660, OGLE LMC-ECL-18794, and HV 2274, together with the orbital solutions. The first and third systems comprise B-type stars, while the second has O-type components and exhibits a total eclipse. We performed a complex analysis that included modeling light and radial velocity curves, O − C analysis, and additional non-LTE spectroscopic analysis for the O-type system. We found that OGLE LMC-ECL-17660 is at least a triple, and tentatively, a quadruple. A significant nonlinear period decrease was determined for HV 2274. Its origin is unclear, possibly due to a faint, low-mass companion on a wide orbit. The analyzed components have masses ranging from 11.7 M
⊙ to 22.1 M
⊙, radii from 7.0 R
⊙ to 14.2 R
⊙, and temperatures between 22,500 and 36,000 K. For HV 2274, the precision of our masses and radii is about six times higher than in previous studies. The position of the components of all six systems analyzed in this series on the mass–luminosity and mass–radius diagrams indicates they are evolutionarily advanced on the main sequence. Our sample contributes significantly to the knowledge of physical parameters of early-type stars in the mass range of 11 M
⊙–23 M
⊙. A new mass–luminosity relation for O- and B-type stars in the LMC is provided. Additionally, we used the measured apsidal motion of the systems to compare the observational and theoretical internal structure constant.
Prediction of Star Formation Rates Using an Artificial Neural Network
Authors: Ayubinia Ashraf , Woo Jong-Hak , Hafezianzadeh Fatemeh , Kim Taehwan , Kim Changseok 
Published: February 2025

Abstract
In this study we develop an artificial neural network to estimate the infrared (IR) luminosity and star formation rates (SFR) of galaxies. Our network is trained using “true” IR luminosity values derived from modeling the IR spectral energy distributions of FIR-detected galaxies. We explore five different sets of input features, each incorporating optical, mid-infrared, near-infrared, ultraviolet, and emission line data, along with spectroscopic redshifts and uncertainties. All feature sets yield similar IR luminosity predictions, but including all photometric data leads to slightly improved performance. This suggests that comprehensive photometric information enhances the accuracy of our predictions. Our network is applied to a sample of SDSS galaxies defined as unseen data, and the results are compared with three published catalogs of SFRs. Overall, our network demonstrates excellent performance for star-forming galaxies, while we observe discrepancies in composite and AGN samples. These inconsistencies may stem from uncertainties inherent in the compared catalogs or potential limitations in the performance of our network.
The Detection Rate of Associated Mg ii Absorption Lines in Quasars Depends on Their Radio Emission
Authors: Chen Zhi-Fu , Ho Luis C. 
Published: February 2025

Abstract
In active galactic nuclei, jet-driven feedback plays a significant role in influencing the properties of gas within their host galaxy and the circumgalactic medium. By combining observations from the Very Large Array Sky Survey, the Faint Images of the Radio Sky at Twenty-cm, the LOFAR Two Meter Sky Survey, and the Sloan Digital Sky Survey (SDSS), we assembled a sample of 3141 radio-loud quasars, among which 418 exhibit Mg ii-associated absorption lines in their SDSS spectra. We classify these quasars into evolutionary stages based on their radio spectral shapes. Our analysis reveals that evolved quasars exhibit a significantly higher incidence of Mg ii-associated absorption lines compared to younger sources, particularly among quasars with “nonpeaked” radio spectra, which show an incidence of Mg ii-associated absorbers approximately 1.7 times greater than that of gigahertz-peaked spectrum sources. This observation can be explained effectively by jet-driven feedback. As quasars age, their jets expand and expel substantial amounts of gas from smaller scales to larger scales, ultimately reaching the circumgalactic medium. The gas expelled from the inner regions and distributed over larger scales results in a greater coverage fraction of absorbing gas. Consequently, evolved quasars exhibit a higher incidence of Mg ii absorption lines.
Le Beatus de San Miguel de Escalada
Authors: Ramos Blassi Ricardo 
Published: February 2025

Le Beatus de San Miguel de Escalada (ms. New York, Pierpont Morgan Library, M 644) réalisé par Magius se trouve parmi les premiers de la seconde branche de la famille des Beatus selon la classification de P. Klein. Les miniaturistes qui se sont succédé dans cette même branche ii (a et b) vont prolonger le schéma illustratif mis en place par Magius qui y a introduit une vraie nouveauté. Les visions des folios 83 et surtout 87 – qui correspondent à la troisième Grande Vision de l’Apocalypse de Jean du Livre iii selon la division du Commentaire du Beatus (Ap 4-5) – rassemblent des traditions iconographiques extrêmement riches, tout en conservant les traditions les plus anciennes en ce qui concerne les coupoles ou les pavements ayant des représentations du thème du Ciel. L’une des caractéristiques du Beatus de Magius, ainsi que l’une de ses nouveautés par rapport aux autres Beatus, c’est la composition géométrique de ses images à valeur symbolique. Ceci est d’ailleurs fondamental, comme on pourra le constater, pour réussir à approfondir la signification de son œuvre. Cette géométrie permet en plus de relier la vision du folio 87 (circulaire) à celle du folio 222v, la Jérusalem Céleste (carrée), ce qui nous rapproche de l’ancien système romain de fondation d’une ville, et nous aide aussi à mieux comprendre quelques éléments de composition des visions. Dans ce sens, on arrivera à apprécier encore plus la personnalité de Magius comme un véritable archipictor.