bluuebunny/crossref_metadata_2025_split huggingface dataset:
Катойконимия Донбасса в словаре и медиатекстах
Authors: И.А. Герасименко 
Published: November 2024

Актуальность данной статьи обусловлена тем, что описание регионального своеобразия языка отра-жает особенности истории и культуры изучаемого края. Необходимость фиксации и сохранения линг-вокраеведческих фактов способствует расширению представлений о русском языке как о лингво-культурно-историческом феномене. Цель статьи — описание состава и способов номинации лиц Донецкого края по месту их жительства или рождения. Для данного анализа были привлечены лексикографические данные (в числе которых словарь-справочник Е. А. Левашова) и материалы со-временных региональных медиатекстов. Объектом исследования выступили катойконимы Донбасса, предметом — их состав и способы номинации. В статье дано толкование термина «катойконим», ко-торый понимается как название жителей по названию места жительства и выступает оттопонимиче-ским дериватом с обобщенным значением ‘названия лиц по месту жительства’. Было указано, что ка-тойконимия (катойконимикон) — это совокупность всех локальных катойконимов, функционирующих на определенной территории, а катойконимика — наука о названиях жителей этой территории. Анализ материала позволил прийти к заключению, что катойконимы Донецкого края являются дериватами в словообразовательных гнездах ойконимов, в формировании которых в течение длительного времени участвовали многие народы, говорившие на разных языках. Также анализ материала способствовал установлению наиболее и наименее распространенных словообразовательных типов среди рассмат-риваемых катойконимов.
The relevance of this article is due to the fact that the description of the regional uniqueness of the language reflects the specific history and culture of this region. The necessity of fixing and preserving culture-oriented facts contributes to the expansion of ideas about the Russian language as a linguistic, cultural and historical phenomenon. The aim of the article is to describe the composition and ways of identifying inhabitants of the Donetsk Region by their place of residence or birth. The paper includes an analysis of lexicographic data (including the reference dictionary compiled by E. A. Levashov) and materials of modern regional media. The object of the study is the demonyms of Donbas, and the subject is their composition and ways of naming the residents. The article defines the term demonym as the name of residents formed by the name of their place of residence and acts as an toponymic derivative with the generalized meaning of names of persons by place of residence. It states that demonymy (demonymikon) is a set of all local demonyms functioning in a certain territory, and demonymy is the study of names of the inhabitants of this territory. The analysis of the material brought us to the conclusion that the demonyms of the Donetsk Region are derivatives in word-forming nests of oikonyms, developed by many ethnic groups speaking different languages participated over a long time. The analysis of the material also contributed to the establishment of the most common and rarer word-forming types of the demonyms.
Методика, промежуточные результаты и перспективы полустационарных наблюдений на эрозионных берегах реки Оки в Рязанском расширении ее поймы
Authors: А.С. Кадыров , А.Ю. Воробьев 
Published: November 2024

Рассматриваются промежуточные результаты и потенциальные возможности получения новой геолого-геоморфологической информации при заложении учетных площадок на наиболее динамичных объектах днища долины реки Оки — эрозионных берегах ее излучин. Представлена методика тематических исследований, проводившихся разными методами в пределах Рязанского расширения окской поймы (743–660 км от устья реки) в 2013–2023 годах. Раскрыты причинно-следственные связи береговой морфолитодинамики и ее пространственной приуроченности с геологическими, гидрологическими и топологическими факторами рельефообразования. На примере полустационара «Дядьково» показано соотношение одно-, двух- и трехмерной составляющей эрозии. Также обсуждаются возможности расширения методологии подобных исследований с привлечением новых и традиционных подходов из смежных с геоморфологией географических дисциплин.
The article considers intermediate research results and opportunities for obtaining new geological and geomorphological data when establishing survey sites on the most dynamic objects of the Oka River valley bottom — the erosional banks of the river bends. The article presents a methodology of thematic studies using various methods applied to the Ryazan extension of the Oka floodplain (which is 743–660 km from the river mouth) over the past decade (2013–2023). It accounts for the cause-and-effect relationships of coastal morpholithodynamics and the spatial relation with the geological, hydrological and topological factors of relief formation. Using data from the Dyadkovo semi-stationary observation site, the research reveals the relationship between one-, two- and three-dimensional erosive components. It also discusses the possibilities of expanding this methodology, involving novel and traditional approaches from geographical disciplines related to geomorphology.
Strategi Penginjilan Kontekstual Rasul Paulus Berdasarkan 1 Korintus 9:19-27
Authors: Pasa Iskandar Dinata , Andi Yusuf Etni Grace 
Published: November 2024

In the era of disruption, contextual evangelism is always needed as a model of approach for preaching the gospel. This article aims to study the Apostle Paul's contextual evangelism strategy in Corinth based on 1 Corinthians 9:19-27. Contextual can be interpreted as a persuasive approach in preaching the gospel that can be accepted according to the local context. Using a descriptive qualitative method, the author analyzes how the Apostle Paul's contextual service strategy in the city of Corinth is based on 1 Corinthians 9:19-27. The author collects various information using a literature approach and applies the principle of hermeneutics through an exegetical approach to the keywords contained in the text. Based on the analysis carried out, it is concluded that the Apostle Paul used several strategies in carrying out contextual evangelism in the city of Corinth. The strategies used are: interactive dialogue, evangelism by identifying culture, and lifestyle evangelism.Dalam era disrupsi, penginjilan kontekstual senantiasa diperlukan sebagai model pendekatan bagi pemberitaan Injil. Artikel ini bertujuan untuk mempelajari strategi penginjilan kontekstual Rasul Paulus di Korintus berdasarkan 1 Korintus 9:19-27. Kontekstual dapat diartikan pendekatan secara persuasif dalam pemberitaan Injil yang dapat diterima sesuai konteks setempat. Dengan menggunakan metode kualitatif deskriptif, penulis menganalisa bagaimana strategi pelayanan kontekstual Rasul Paulus di kota Korintus berdasarkan 1 Korintus 9:19-27. Penulis mengumpulkan berbagai informasi dengan menggunakan pendekatan literatur dan menerapkan prinsip hermeneutika melalui pendekatan eksegesa terhadap kata-kata kunci yang terdapat dalam teks. Berdasarkan analisa yang dilakukan diperoleh kesimpulan bahwa Rasul Paulus menggunakan beberapa strategi dalam melaksanakan penginjilan kontekstual di Kota Korintus. Strategi yang digunakan adalah: dialog interaktif, penginjilan dengan melakukan indentifikasi budaya, dan penginjilan gaya hidup.
The Société de Poitou et du Loudunois, 1714–1812: A Huguenot Fund in the Refuge
Authors: Julien Barbara 
Published: November 2024

Abstract
This article presents an overview of the philanthropic society set up in the first year of the Georgian era to assist Poitevin refugees in London: its records, housed at the Huguenot Library, offer colourful insights into refugee life in eighteenth-century London, with a broad canvas of wealthy donors and often desperately poor compatriots evolving alongside each other within a structure of annual sermons and general assemblies, benevolence and poor relief. Financial challenges and a major fraud were weathered, and the society played a significant role within the network of other Huguenot charities operating in London. Like similar organizations and indeed Huguenot churches in the capital, by the 1780s its existence was undermined by the very assimilation its strict rules had sought to avoid, and its closure in 1812, through a lack both of donors and recipients of relief, had become inevitable.
Combined JWST–MUSE Integral Field Spectroscopy of the Most Luminous Quasar in the Local Universe, PDS 456
Authors: Seebeck Jerome , Veilleux Sylvain , Liu Weizhe , Rupke David S. N. , Vayner Andrey , Wylezalek Dominika , Zakamska Nadia L. , Bertemes Caroline 
Published: November 2024

Abstract
Fast accreting, extremely luminous quasars contribute heavily to the feedback process within galaxies. While these systems are most common at cosmic noon (z ∼ 2), here we choose to study PDS 456, an extremely luminous (L
bol ∼ 1047 erg s−1) but nearby (z ∼ 0.185) quasar where the physics of feedback can be studied in greater detail. We present the results from our analysis of the JWST MIRI/Medium Resolution Spectroscopy (MRS) integral field spectroscopic (IFS) data of this object. The extreme brightness of PDS 456 makes it challenging to study the extended emission even in this nearby object. MIRI/MRS instrumental effects are mitigated by using complementary NIRSpec and MUSE IFS data cubes. We show clear evidence of a multiphase gas outflow extending up to 15 kpc from the central source. This includes emission from warm molecular (H2
ν = 0–0 and 1–0) and ionized (e.g., Paα, [O iii], [Ne iii], and [Ne vi]) gas with typical blueshifted velocities down to −500 km s−1. We are also able to probe the nuclear dust emission in this source through silicate and polycyclic aromatic hydrocarbon emission features but are unable to spatially resolve it. Our results are consistent with this powerful quasar driving a radiatively driven wind over a broad range of distances and altering the ionization structure of the host galaxy.
Unlocking Discovery Potential for Decaying Dark Matter and Faint X-Ray Sources with XRISM
Authors: Zhou Yu , Takhistov Volodymyr , Mitsuda Kazuhisa 
Published: November 2024

Abstract
Astrophysical emission lines arising from particle decays can offer unique insights into the nature of dark matter (DM). Using dedicated simulations with background and foreground modeling, we comprehensively demonstrate that the recently launched X-Ray Imaging and Spectroscopy Mission (XRISM) space telescope with powerful X-ray spectroscopy capabilities is particularly well suited to probe decaying DM, such as sterile neutrinos and axion-like particles, in the mass range of a few to tens of keV. We analyze and map XRISM’s DM discovery potential parameter space by considering the Milky Way Galactic DM halo, including establishing an optimal line-of-sight search, as well as dwarf galaxies, where we identify Segue 1 as a remarkably promising target. We demonstrate that with only 100 ks exposure, the XRISM/Resolve instrument is capable of probing the underexplored DM parameter window around a few keV and testing DM couplings with a sensitivity that exceeds by two orders existing Segue 1 limits. Further, we demonstrate that XRISM/Xtend instrument sensitivity enables discovery of the nature of faint astrophysical X-ray sources, especially in Segue 1, which could shed light on star formation history. We discuss implications for decaying DM searches with improved detector energy resolution in future experiments.
Impacting Atmospheres: How Late-stage Pollution Alters Exoplanet Composition
Authors: Vlahos Emilia , Chachan Yayaati , Savignac Vincent , Lee Eve J. 
Published: November 2024

Abstract
The atmospheric composition of exoplanets is often considered as a probe of the planet’s formation conditions. How exactly the initial chemical memory may be altered from the birth to the final state of the planet, however, remains unknown. Here, we develop a simple model of pollution of planetary atmosphere by the vaporization of infalling planetesimals of varying sizes and composition (SiO2 inside 1 au and H2O outside 1 au), following their trajectory and thermal evolution through the upper advective and radiative layers of a sub-Neptune-class planet during the late stage of disk evolution. We vary the rate of pollution by changing the solid content of the disk and by dialing the level of disk gas depletion, which in turn determines the rate of planetary migration. We find that pollution by silicate grains will always be limited by the saturation limit set by the thermal state of the atmosphere. By contrast, pollution by water ice can lead to ∼2–4 orders of magnitude variation in the atmospheric water mass fraction depending on the solid and gas content of the disk. Both cases suggest that post-formation pollution can erase the initial compositional memory of formation. Post-formation pollution can potentially transform sub-Neptunes with H/He-dominated envelopes that initially formed beyond the ice line to water worlds (i.e., with a water-enriched envelope) when the disk gas is depleted by ≳2 orders of magnitude, allowing gentle migration. We additionally discuss the expected C/O ratio profile under pollution by water and refractory carbon species.
Thermal Evolution of the Intergalactic Medium due to Lyα Photons during the Cosmic Dawn
Authors: Raste Janakee , Sarkar Anjan Kumar , Sethi Shiv K. 
Published: November 2024

Abstract
The first star-forming objects that formed at high redshifts during the cosmic dawn (CD) also emitted photons between Lyα and Lyman-limit frequencies. These photons are instrumental in coupling the spin temperature of the neutral hydrogen (H i) atoms with the kinetic temperature of the intergalactic medium (IGM). Along with this coupling effect, these photons also impact the kinetic temperature by exchanging energy with the H i atoms. The injected Lyα photons in general cool the medium, while the continuum photons heat the medium. While studying this effect in the literature, a quasi-static profile around the Lyα frequency is assumed. In this paper, we solve the time-dependent coupled dynamics of the photon intensity profile along with the evolution of the thermal state of the IGM and H i spin temperature. It is expected that, during the CD era, the IGM has a mix of continuum photons with 10%–20% of injected photons. For this case, we show that the system reaches thermal equilibrium in around 1 Myr, with the final temperature in the range 50–100 K. This timescale is comparable to the source lifetime of Population III stars at high redshifts. One impact of switching off short-lived sources is that it can keep the system heated above the temperature of the quasi-static state. We also show that the quasi-static equilibrium for the continuum photons is only achieved on timescales of 100 Myr at z ≃ 20, comparable to the age of the Universe. We also briefly discuss how the Lyα induced heating can impact the 21 cm signal from CD.
Advection-nonlinear-diffusion Model of Flare Accelerated Electron Transport in Type III Solar Radio Bursts
Authors: Kontar Eduard P. , Azzollini Francesco , Lyubchyk Olena 
Published: November 2024

Abstract
Electrons accelerated by solar flares and observed as type III solar radio bursts are not only a crucial diagnostic tool for understanding electron transport in the inner heliosphere but also a possible early indication of potentially hazardous space weather events. The electron beams traveling in the solar corona and heliosphere along magnetic field lines generate Langmuir waves and quasilinearly relax toward a plateau in velocity space. The relaxation of the electron beam over the short distance in contrast to large beam-travel distances observed is often referred to as Sturrok’s dilemma. Here, we develop a new electron transport model with quasilinear distance/time self-consistently changing in space and time. This model results in a nonlinear advection-diffusion equation for the electron beam density with a nonlinear diffusion term that is inversely proportional to the beam density. The solution predicts slow super-diffusive (ballistic) spatial expansion of a fast-propagating electron beam. This model also provides the evolution of the spectral energy density of Langmuir waves, which determines brightness temperature of plasma radiation in solar bursts. The model solution is consistent with the results of numerical simulation using kinetic equations and can explain some characteristics of type III solar radio bursts.
A Photochemical Phosphorus-Hydrogen-Oxygen Network for Hydrogen-dominated Exoplanet Atmospheres
Authors: Lee Elspeth K. H. , Tsai Shang-Min , Moses Julianne I. , Plane John M. C. , Visscher Channon , Klippenstein Stephen J. 
Published: November 2024

Abstract
Due to the detection of phosphine (PH3) in the solar system gas giants Jupiter and Saturn, PH3 has long been suggested to be detectable in exosolar substellar atmospheres too. However, to date, direct detection of phosphine has proven to be elusive in exoplanet atmosphere surveys. We construct an updated phosphorus-hydrogen-oxygen (PHO) photochemical network suitable for the simulation of gas giant hydrogen-dominated atmospheres. Using this network, we examine PHO photochemistry in hot Jupiter and warm Neptune exoplanet atmospheres at solar and enriched metallicities. Our results show for HD 189733b-like hot Jupiters that HOPO, PO, and P2 are typically the dominant P carriers at pressures important for transit and emission spectra, rather than PH3. For GJ1214b-like warm Neptune atmospheres our results suggest that at solar metallicity PH3 is dominant in the absence of photochemistry, but is generally not in high abundance for all other chemical environments. At 10 and 100 times solar, small oxygenated phosphorus molecules such as HOPO and PO dominate for both thermochemical and photochemical simulations. The network is able to reproduce well the observed PH3 abundances on Jupiter and Saturn. Despite progress in improving the accuracy of the PHO network, large portions of the reaction rate data remain with approximate, uncertain, or missing values, which could change the conclusions of the current study significantly. Improving understanding of the kinetics of phosphorus-bearing chemical reactions will be a key undertaking for astronomers aiming to detect phosphine and other phosphorus species in both rocky and gaseous exoplanetary atmospheres in the near future.
Securing Arithmetical Determinacy
Authors: Speitel Sebastian G.W. 
Published: November 2024

The existence of non-standard models of first-order Peano-Arithmetic (PA) threatens to undermine the claim of the moderate mathematical realist that non-mysterious access to the natural number structure is possible on the basis of our best arithmetical theories. The move to logics stronger than FOL is denied to the moderate realist on the grounds that it merely shifts the indeterminacy “one level up” into the meta-theory by, illegitimately, assuming the determinacy of the notions needed to formulate such logics. This paper argues that the challenge can be met. We show how the quantifier “there are infinitely many” can be uniquely determined in a naturalistically acceptable fashion and thus be used in the formulation of a theory of arithmetic. We compare the approach pursued here with Field’s justification of the same device and the popular strategy of invoking a second-order formalism, and argue that it is more robust than either of the alternative proposals.
Seasonal abundance of key alfalfa (Fabaceae) seed production pests and their natural enemies in southern Alberta, Canada
Authors: Ríos Martínez Aldo F. , Reid Michelle , Frost Carol M. , Cárcamo Héctor A. , Mori Boyd A. 
Published: November 2024

Abstract
The economic importance of insect pests in agricultural fields and the potential biological control by their natural enemies warrant foundational studies for the development of integrated pest management strategies. An insect survey was conducted in alfalfa (Fabaceae) seed production fields in southern Alberta, Canada, during the bud, flowering, and seed crop stages in 2020 and 2021. We examined the seasonal abundance of Hypera postica (Gyllenhal) (Coleoptera: Curculionidae), Adelphocoris lineolatus (Goeze) (Hemiptera: Miridae), Lygus spp. Hahn (Hemiptera: Miridae), and 12 natural enemy taxa. We also examined the seasonal abundance, richness, and diversity of generalist predators and the seasonality of the two H. postica parasitoids, Bathyplectes curculionis (Thomson) (Hymenoptera: Ichneumonidae) and Oomyzus incertus (Ratzeburg) (Hymenoptera: Eulophidae). The seasonality of pests and natural enemies was inconsistent between years. Hypera postica larvae, B. curculionis, and O. incertus were present from mid-June to mid-August. However, we detected no correlations between H. postica larvae and its two parasitoids in either year. A number of generalist predators were correlated with A. lineolatus and Lygus spp. Further research is needed to understand the effects of environmental and biotic factors on the seasonality of pests and natural enemies in alfalfa seed production fields, and the insects’ trophic interactions.
Fasciola worm and egg-derived antigens: Exploring their diagnostic potential for urogenital schistosomiasis in resource-limited endemic regions
Authors: Adesida Adedayo , Oriade Tajudeen , Sulaiman Kabirat , Afolayan Funmilayo , Auta Timothy , Akanbi Ibikunle , Aladegboye Mercy , Nwuba Roseangela , Odaibo Alexander , Oyeyemi Oyetunde 
Published: November 2024

Objective:
To evaluate the immunodiagnostic potential of crude Fasciola gigantica-worm (FWA) and egg antigen (FEA) in detecting anti-Schistosoma (S.) haematobium antibodies in sera and urine samples.

Methods:
This is a cross-sectional diagnostic study. Employing an indirect ELISA, antibodies against these antigens were assessed in samples from infected and non-infected individuals in both schistosomiasis endemic (NE) and non-endemic (NNE) areas, using microscopy as the diagnostic standard.

Results:
FWA-sera exhibited excellent diagnostic accuracy with an area under the curve (AUC) of 0.957, a sensitivity of 93.75%, and a specificity of 85.42% for discriminating between infected and non-infected individuals in non-endemic areas. FWA-urine also demonstrated robust performance, achieving AUC>0.95, sensitivity>97.0%, and specificity>85.0% in both NE and NNE categories. Notably, S. haematobium-specific antibody levels against FWA were significantly elevated in infected individuals in both endemic and non-endemic areas. FEA-sera exhibited outstanding diagnostic performance with sensitivity exceeding 90% and an AUC of 0.968 in non-endemic samples but not in FEA-urine.

Conclusions:
FWA-based ELISAs, applicable to both sera and urine, emerge as promising tools for S. haematobium diagnosis in resource-limited settings, offering advantages of high sensitivity and specificity with shared antigens with Fasciola. The superior diagnostic metrics of urine samples suggest their potential as a noninvasive biological sample for diagnostic purposes.