bluuebunny/crossref_metadata_2025_split huggingface dataset:
Author Contribution in Manuscript Creation: Description and Announcement
Authors: Ryabova Anastasia Evgenievna 
Published: January 2024

Introduction: The topic of publication ethics is increasingly important in scientific discussions, especially the issues of accurate and honest representation of author contributions in the creation of scientific articles.Description of the CREDIT System: The contribution to authorship of an article is determined not only by participation in writing the text but also by the overall contribution of the participant in conducting the research itself. The CREDIT authorship model allows for precise tracking of each participant's contribution to the research project, describing various author roles, some of which may be independent, while others complement more significant roles.Conclusion: Detailed coverage of the CREDIT taxonomy and the procedure for documenting author contribution enhances the transparency of scientific communication.
Analytical Assessment of the System for Confirming Compliance of Milk and Dairy Products with Mandatory Legal Requirements
Authors: Abdullaeva Larisa Vladimirovna , Bedretdinova Sophia Andreevna 
Published: January 2024

Introduction: The safety and quality of dairy products produced and in circulation on the territory of the EAEU is ensured by compliance with legislation on technical regulation, sanitary, hygienic and veterinary safety. One of the important sections of technical regulation is the rules for confirming product compliance with mandatory legal requirements.Purpose: The purpose of this review is analysis of the current legislative framework in the Russian Federation in the field of confirming compliance of milk and dairy products with the requirements of regulatory legal acts and systematization of the data obtained on the applicable forms assessing and confirming compliance of products in the Russian Federation. Materials and Methods: As materials for the analytical study were used regulatory legal acts (hereinafter - RLA) in the field of technical regulation, sanitary, hygienic and veterinary safety of food products and raw materials. The documents were obtained on the official legal portals of the Government of the Russian Federation, the Eurasian Economic Commission, the Ministry of Agriculture of the Russian Federation, the Ministry of Industry and Trade of the Russian Federation, the Ministry of Health of the Russian Federation. As a research method, the analysis of the current legislation with the subsequent systematization of expert opinions on the law enforcement practice of the regulated rules for products confirming conformity, generalization and analysis of the most common arbitration situations in the raw milk and finished dairy products turnover at the stage of their compliance with mandatory requirements confirming (assessment) were used. The appeals and documents of the technical regulation and standardization services of dairy industry enterprises on the subject research field were also analyzed.Results: Based on the regulated in RLA requirements for confirming (assessment) compliance of raw milk and dairy products, as well as based on the generalized results of a product manufacturers survey, have been established the conformity assessment schemes most often used by manufacturers. Taking into account the analysis and systematization of material on arbitration issues in confirming (assessment) compliance, recommendations are proposed for optimizing the process of confirming (assessment) compliance of raw milk and dairy products with the requirements of the legislation of the EAEU and the Russian Federation, including the feasibility of its updating.Conclusion: According to the results of the research have been identified a number of problems in the field of confirming (assessment) of milk and dairy products compliance with the requirements of the RLA, which producers and regulatory authorities bodies in their professional activities, and appropriate solutions to these problems have been proposed.
ANALYSIS OF THE MAIN METHODS OF DUST CONTROL ON QUARRY ROADS
Authors: Орлов Федор Александрович , Полушкина Татьяна Олеговна 
Published: January 2024

Авторами приведен анализ основных методов борьбы с пылью на карьерных дорогах и влияние пыли на работников, занятых во вредных условиях труда. Рассмотрены основные факторы снижения пылеобразования на карьерных дорогах при добыче полезных ископаемых открытым способом.
The authors analyze the main methods of dust control on quarry roads and the impact of dust on workers employed in hazardous working conditions. The main factors of reduction of dust formation on quarry roads during open-pit mining are considered.
Are there “weak” definites in bare classifier languages?
Authors: Yip Ka-Fai , Banerjee Ushasi , Lee Margaret Chui Yi 
Published: January 2024

This paper motivates a new view on the typology of definiteness that integrates (quasi-)names. The primary data is drawn from Cantonese and Bangla, where both bare classifier constructions and bare nominals are recruited for definite expressions. We argue that these bare nominals, while often analyzed as the so-called “weak”/unique definites in other languages, are indeed name-like expressions akin to the quasi-name Mom in English, in contrast with the definite descriptions denoted by bare classifier constructions. We propose that quasi-names, as well as proper names, are derived by a definite determiner that encodes a functional relation between the discourse participants and the referent. We further discuss cases where quasi-names compete with definite descriptions and proper names. The findings not only suggest that names should be brought into the picture, but also shed light on how pragmatic principles interact and determine the choice of referring expressions.
Semifactives in comparatives
Authors: Fleisher Nicholas 
Published: January 2024

This is more complicated than I realized. How are we to understand the status of realize's complement in a sentence like this? What sort of relationship must this complement bear to its matrix environment, in light of realize's status as a cognitive factive or semifactive predicate (Kiparsky & Kiparsky 1970; Karttunen 1971)? Comparative constructions, I suggest, do much to illuminate the nature of semifactives and the semantic–pragmatic status of their clausal complements. Specifically, I propose that semifactives support graded awareness—knowledge of something less, but not more, than the full truth with respect to some question or issue—while requiring that their complement be informationally consistent with the matrix environment, rather than presupposed true. The picture that emerges fits naturally with pragmatic approaches to presupposition generation and projection (Beaver 2010; Simons, Beaver, Roberts & Tonhauser 2017; Degen & Tonhauser 2022) and depends on sensitivity to scalar polarity and orientation (Kennedy 2001).
Acts, occasions and multiplicatives: A mereotopological account
Authors: Wągiel Marcin 
Published: January 2024

In this paper, I argue for the relevance of structured part-whole configurations in the domain of events. The evidence comes from the well-known event-internal/external distinction, which concerns mutliplicative adverbials quantifying either over separate occasions or occasion-internal acts, respectively (e.g., Cusic 1981, Andrews 1983, Cinque 1999, Zhang 2017). In order to capture this distinction, I postulate that the relationship between the two categories is based on a part-whole relation. In particular, inspired by proposals advocating the role of eventive higher-order units (Landman 2006, Henderson 2017) and building on the theories of (Grimm 2012) and (Mazzola 2019), I propose to extend mereotopology to the domain of events. I argue that this allows for capturing acts as simplex events conceptualized as bounded integrated MSSC wholes, whereas occasions as clusters, i.e., temporally structured configurations, of such simplex events.
МЕЖДУНАРОДНАЯ НАУЧНАЯ КОНФЕРЕНЦИЯ, ПО МОНГОЛЬСКОМУ И ТЮРКСКОМУ ЯЗЫКОЗНАНИЮ, ПОСВЯЩЕННАЯ ПАМЯТИ В.И. РАССАДИНА
Authors: Алишина Ханиса Чавдатовна 
Published: January 2024

15–16 ноября 2022 г. на базе Бурятского государственного университета им. Д. Банзарова совместно с Калмыцким государственным университетом им. Б.Б. Городовикова прошла Международная научная конференция по монгольскому и тюркскому языкознанию, посвященная памяти Валентина Ивановича Рассадина, первого заведующего кафедрой филологии Центральной и Восточной Азии (ныне кафедра филологии Центральной Азии), отмечающей свое 30-летие. Организатором конференции выступила кафедра филологии Центральной Азии Восточного института Бурятского государственного университета им. Д. Банзарова.
Data-driven Modeling of a Coronal Magnetic Flux Rope: From Birth to Death
Authors: Guo J. H. , Ni Y. W. , Guo Y. , Xia C. , Schmieder B. , Poedts S. , Zhong Z. , Zhou Y. H. , Yu F. , Chen P. F. 
Published: January 2024

Abstract
Magnetic flux ropes are a bundle of twisted magnetic field lines produced by internal electric currents, which are responsible for solar eruptions and are the major drivers of geomagnetic storms. As such, it is crucial to develop a numerical model that can capture the entire evolution of a flux rope, from its birth to death, in order to predict whether adverse space weather events might occur or not. In this paper, we develop a data-driven modeling that combines a time-dependent magnetofrictional approach with a thermodynamic magnetohydrodynamic model. Our numerical modeling successfully reproduces the formation and confined eruption of an observed flux rope, and unveils the physical details behind the observations. Regarding the long-term evolution of the active region, our simulation results indicate that the flux cancellation due to collisional shearing plays a critical role in the formation of the flux rope, corresponding to a substantial increase in magnetic free energy and helicity. Regarding the eruption stage, the deformation of the flux rope during its eruption can cause an increase in the downward tension force, which suppresses it from further rising. This finding may shed light on why some torus-unstable flux ropes lead to failed eruptions after large-angle rotations. Moreover, we find that twisted fluxes can accumulate during confined eruptions, which would breed the subsequent eruptive flares.
Spectral and Jet Properties of the Quasi-thermal-dominated GRB 210121A, GRB 210610B, and GRB 221022B
Authors: Song Xin-Ying , Wang Ling-Jun , Zhang Shu 
Published: January 2024

Abstract
Some quasi-thermal (QT)-dominated gamma-ray bursts (GRBs) could be well described by a multicolor blackbody (mBB) function or a combined model of a BB plus a nonthermal (NT) component. In this analysis, two QT radiation-dominated bursts with known emission properties (GRB 210610B, likely from a hybrid jet, and GRB 210121A, with a spectrum consistent with nondissipative photospheric emission from a pure hot fireball) are used to make a comparison between these two models. To diagnose the magnetization properties of the central engine, the “top-down” approach proposed by Gao and Zhang is adopted. It is found that diagnoses based on these two models provide similar conclusions qualitatively; however, the model with mBB (or mBB+NT) may give more reasonable physical explanations. This implies that impacts from the GRB jet structure and geometrical broadening on the observed spectrum should be considered. However, conservatively, these methods may be not sensitive enough to distinguish between a pure hot fireball and a mildly magnetized hybrid jet. Some other information is necessary to provide more evidence when determining the jet properties for similar GRBs. Based on these considerations, we suggest that the photospheric emission of GRB 221022B is from a hot jet, where dissipation is caused by an internal shock mechanism due to the increasing Lorentz factor with time, which makes its prompt emission display typical evolution from thermal to NT.
On the Role of Alfvénic Fluctuations as Mediators of Coherence within Interplanetary Coronal Mass Ejections: Investigation of Multi-spacecraft Measurements at 1 au
Authors: Scolini Camilla , Lugaz Noé , Winslow Réka M. , Farrugia Charles J. , Magyar Norbert , Bacchini Fabio 
Published: January 2024

Abstract
Interplanetary coronal mass ejections (ICMEs) are defined as “coherent” if they are capable of responding to external perturbations in a collective manner. This implies that information must be able to propagate across ICME structures, and if this is not the case, single-point in situ measurements cannot be considered as indicative of global ICME properties. Here, we investigate the role of Alfvénic fluctuations (AFs) as mediators of ICME coherence. We consider multipoint magnetic field and plasma measurements of 10 ICMEs observed by the ACE and Wind spacecraft at 1 au at longitudinal separations of 0.5°–0.7°. For each event, we analyze the Alfvénicity in terms of the residual energy and cross helicity of fluctuations, and the coherence in terms of the magnetic correlation between Wind and ACE. We find that ∼65% and 90% of ICME sheaths and magnetic ejecta (MEs), respectively, present extended AFs covering at least 20% of the structure. Cross helicity suggests AFs of solar and interplanetary origin may coexist in the ICME population at 1 au. AFs are mainly concentrated downstream of shocks and in the back of MEs. The magnetic field is poorly correlated within sheaths, while the correlation decreases from the front to the back of the MEs for most magnetic field components. AFs are also associated with lower magnetic field correlations. This suggests either that ICME coherence is not mediated by Alfvén waves, implying that the coherence scale may be smaller than previously predicted, or that the magnetic field correlation is not a measure of coherence.
Are Radio Minihalos Confined by Cold Fronts in Galaxy Clusters? Minihalos and Large-scale Sloshing in A3444 and MS 1455.0+2232
Authors: Giacintucci S. , Venturi T. , Markevitch M. , Brunetti G. , Clarke T. E. , Kale R. 
Published: January 2024

Abstract
We present radio and X-ray studies of A3444 and MS1455.0+2232, two galaxy clusters with radio minihalos in their cool cores. A3444 is imaged using the Giant Metrewave Radio Telescope (GMRT) at 333, 607, and 1300 MHz and the Very Large Array at 1435 MHz. Most of the minihalo is contained within r < 120 kpc, but a fainter extension, stretching out to 380 kpc southwest of the center, is detected at 607 MHz. Using Chandra, we detect four X-ray sloshing cold fronts: three in the cool core at r = 60, 120, and 230 kpc, and a fourth one at r = 400 kpc—in the region of the southwestern radio extension—suggesting that the intracluster medium (ICM) is sloshing on a cluster-wide scale. The radio emission is contained within the envelope defined by these fronts. We also analyzed archival 383 MHz GMRT and Chandra observations of MS 1455.0+2232, which exhibits a known minihalo with its bright part delineated by cold fronts inside the cool core, but with a faint extension beyond the core. Similarly to A3444, we find a cold front at r ∼ 425 kpc, containing the radio emission. Thus the entire diffuse radio emission seen in these clusters appears to be related to large-scale sloshing of the ICM. The radio spectrum of the A3444 minihalo is a power law with a steep index α = 1.0 ± 0.1. The spectrum steepens with increasing distance from the center, as expected if the minihalo originates from reacceleration of relativistic particles by the sloshing-induced turbulence in the ICM.
The Effective Field Theory of Large-scale Structures of a Fuzzy Dark Matter Universe
Authors: Manouchehri Kousha Hamed , Hooshangi Sina , Abolhasani Aliakbar 
Published: January 2024

Abstract
Ultralight scalar fields and their noninteracting class, i.e., the so-called fuzzy dark matter (FDM), are dark matter candidates introduced to solve the small-scale problems of the standard cold dark matter. In this paper, we investigate whether the physics of FDM, particularly the quantum pressure that leads to the suppression of structure formation on small scales, could leave significant imprints on the large-scale statistics of matter fluctuations. For this purpose, we utilize the Effective Field Theory of Large Scale Structures (EFT of LSS), wherein small-scale physics is integrated and represented on large scales by only a set of free parameters. These parameters can be determined by fitting them into the cosmological simulations. By fitting the EFT predictions to the simulation data, we determine the value of the speed of sound as a quantitative measure of how UV physics affects large-scale perturbation. We use the Gadget-2 code to study the evolution of 5123 particles in a box with a side length 250 h
−1 Mpc. We exploit the suppressed FDM initial power for the FDM universe and perform N-body simulation sufficient to produce accurate—enough for our purpose—results on large scales. In particular, we perform three FDM simulations with different masses and compare their sound speed with the standard cold dark matter (CDM) simulation. We found no difference between the FDM and CDM sound speeds beyond the confidence intervals. However, a consistently increasing trend can be seen in the sound speed for lower masses. This result suggests further investigations using higher-resolution simulations.
Uncovering a Massive z ∼ 7.7 Galaxy Hosting a Heavily Obscured Radio-loud Active Galactic Nucleus Candidate in COSMOS-Web
Authors: Lambrides Erini , Chiaberge Marco , Long Arianna S. , Liu Daizhong , Akins Hollis B. , Ptak Andrew F. , Andika Irham Taufik , Capetti Alessandro , Casey Caitlin M. , Champagne Jaclyn B. , Chworowsky Katherine , Clarke Tracy E. , Cooper Olivia R. , Ding Xuheng , Dong Dillon Z. , Faisst Andreas L. , Forman Jordan Y. , Franco Maximilien , Gillman Steven , Gozaliasl Ghassem , Hall Kirsten R. , Harish Santosh , Hayward Christopher C. , Hirschmann Michaela , Hutchison Taylor A. , Jahnke Knud , Jin Shuowen , Kartaltepe Jeyhan S. , Kleiner Emma T. , Koekemoer Anton M. , Kokorev Vasily , Manning Sinclaire M. , Martin Crystal L. , McKinney Jed , Norman Colin , Nyland Kristina , Onoue Masafusa , Robertson Brant E. , Shuntov Marko , Silverman John D. , Stiavelli Massimo , Trakhtenbrot Benny , Vardoulaki Eleni , Zavala Jorge A. , Allen Natalie , Ilbert Olivier , McCracken Henry Joy , Paquereau Louise , Rhodes Jason , Toft Sune 
Published: January 2024

Abstract
In this Letter, we report the discovery of the highest redshift, heavily obscured, radio-loud (RL) active galactic nucleus (AGN) candidate selected using JWST NIRCam/MIRI, mid-IR, submillimeter, and radio imaging in the COSMOS-Web field. Using multifrequency radio observations and mid-IR photometry, we identify a powerful, RL, growing supermassive black hole with significant spectral steepening of the radio spectral energy distribution (f
1.28 GHz ∼ 2 mJy, q
24 μm = −1.1, α
1.28−3 GHz = − 1.2, Δα = − 0.4). In conjunction with ALMA, deep ground-based observations, ancillary space-based data, and the unprecedented resolution and sensitivity of JWST, we find no evidence of AGN contribution to the UV/optical/near-infrared (NIR) data and thus infer heavy amounts of obscuration (N
H > 1023 cm−2). Using the wealth of deep UV to submillimeter photometric data, we report a singular solution photo-z of z
phot =

7.7

−
0.3

+
0.4

and estimate an extremely massive host galaxy

(
log

M

⋆

=
11.92
±
0.5

M

⊙

)

hosting a powerful, growing supermassive black hole​​​​​ (L
Bol = 4−12x × 1046 erg s−1). This source represents the farthest known obscured RL AGN candidate, and its level of obscuration aligns with the most representative but observationally scarce population of AGN at these epochs.
3 μm Phase Curves of Main-belt Asteroids from NEOWISE Photometry
Authors: Varakian Matthew , Chanover Nancy , Masiero Joseph , Oszkiewicz Dagmara 
Published: January 2024

Abstract
The shapes of asteroid phase curves are influenced by the physical properties of asteroid surfaces. The variation of an asteroid’s brightness as a function of the solar phase angle can tell us about surface properties such as grain size distribution, roughness, porosity, and composition. Phase curves are traditionally derived from photometric observations at visible wavelengths, but phase curves using infrared data can also provide useful information about an asteroid surface. Using photometric observations centered near ∼3.4 μm from the W1 band of the Near-Earth Object Wide-field Infrared Survey Explorer mission, we construct thermally and rotationally corrected infrared phase curves for a sample of main-belt asteroids, which includes asteroids observed by the AKARI satellite, as well as subsets of the Themis and Flora dynamical families. We calculate the linear slope of the phase curves as a measure of their shape and compare W1 phase slopes to band depths of absorption features associated with hydrated materials, spectral slopes, visible albedos, W1 albedos, and diameters. We observe a steepening of the W1 phase slope of C-type asteroids with increasing 2.7 μm band depth but little correlation between the phase slope and 3 μm band depth or 3 μm spectral slope. The C-types in our sample exhibit steeper average W1 phase slopes than M- or S-types, similar to visible-light phase slopes. We also observe steeper W1 phase slopes for smaller-diameter objects within the Themis family and explore comparisons to Jupiter-family comets in phase slope versus albedo space.
A non-adaptive radiation of viviparous skinks from the seasonal tropics of India: Systematics of Subdoluseps (Squamata: Scincidae), with description of a new genus and five cryptic new species
Authors: Agarwal Ishan , Thackeray Tejas , Khandekar Akshay 
Published: January 2024

AbstractSubdolusepsis a recently described genus of Lygosomine skinks distributed in peninsular India and Southeast Asia. We conduct the first revision of IndianSubdolusepsbased on range-wide sampling including 89 specimens from 33 localities. We use two mitochondrial and three nuclear markers, 58 morphological characters, and ecological data to reconstruct the evolutionary history of IndianSubdolusepsand assess their diversity and distribution, providing insights into lygosominin biogeography. We formally describe the Indian clade as a new genus,Dravidosepsgen. nov.and name five new species from Tamil Nadu, India in an integrative taxonomic framework –D. gingeeensissp. nov.,D. jawadhuensissp. nov.,D. kalakadensissp. nov.,D. srivilliputhurensissp. nov., andD. tamilnaduensissp. nov.. We transferRiopa goaensis,Subdoluseps pruthiandS. nilgiriensisto the new genus and designate neotypes for the former two. Members ofDravidosepsgen. nov.are the first known viviparous skinks from peninsular India and the only known viviparous lygosominins apart from a few species of east AfricanMochlus. The Lygosomini have a Southeast Asian origin and began diversifying in the Eocene with three dispersals between India and Southeast Asia. Species level diversification inDravidosepsgen. nov.was likely driven by a combination of niche conservatism, paleoclimate and past forest distribution. The discovery of a new genus and five new species reiterates the high levels of diversity and endemism present in peninsular India and how much more remains to be discovered.