bluuebunny/crossref_metadata_2025_split huggingface dataset:
ASSESSMENT OF THE LEVEL OF IMPLEMENTATION OF SUSTAINABLE FOREST MANAGEMENT PRINCIPLES IN THE IRKUTSK REGION
Authors: Горбунова Ольга Ивановна , Кулагина Анна Николаевна 
Published: August 2022

Лесное хозяйство России на современном этапе развития находится в состоянии серьезной трансформации. Одна из ключевых задача стратегического развития лесного сектора страны - это реализация механизма устойчивого лесоуправления и лесопользования. Проведена оценка устойчивости уровня лесопользования в Иркутской области, в результате чего были разработаны рекомендации для повышения общего уровня лесоуправления в регионе.
Forestry in Russia at the present stage of development is in a state of serious transformation. One of the key tasks of the strategic development of the country's forest sector is the implementation of the mechanism of sustainable forest management. An assessment of the sustainability of the level of forest management in the Irkutsk region was carried out, as a result of which recommendations were developed to improve the overall level of forest management in the region.
SOCIO-ECONOMIC CONSEQUENCES OF UNEMPLOYMENT AND METHODS OF OVERCOMING IT
Authors: Выводцев Даниил Владимирович , Недорезова Елена Сергеевна 
Published: August 2022

В данной статье рассматривается социально-экономическое явление безработицы, факторы, к ней приводящие, так же, как и последствия этого явления в социальной и экономической сферах отдельно. В качестве практических примеров для выстраивания взаимосвязей в работе используется статистика последних лет. Потому, данная статья является актуальной в свете текущего состояния социально-экономической сферы Российской Федерации.
This article examines the socio-economic phenomenon of unemployment, the factors leading to it, as well as the consequences of this phenomenon in the social and economic spheres separately. The statistics of recent years are used as practical examples for building relationships in the work. Therefore, this article is relevant in the light of the current state of the socio-economic sphere of the Russian Federation.
THE ESSENCE AND ROLE OF THE RUSSIAN ECONOMIC CRISIS OF 2022
Authors: Недорезова Елена Сергеевна , Савельева Валерия Сергеевна 
Published: August 2022

Статья посвящена такому актуальному многогранному и непредсказуемому явлению, как экономический кризис, во время которого существующие средства достижения целей становятся неадекватными, зачастую возникают непредсказуемые ситуации и проблемы, на которые просто необходимо своевременно реагировать. В статье рассматривается влияние современного экономического кризиса на российскую экономику.
The article is devoted to such an urgent multifaceted and unpredictable phenomenon as the economic crisis, during which the existing means of achieving goals become inadequate, unpredictable situations and problems often arise, to which it is simply necessary to respond in a timely manner. The article examines the impact of the current economic crisis on the Russian economy.
THE PROBLEM OF UNEMPLOYMENT AND IT’S IMPACT ON THE ECONOMY OF THE RUSSIAN FEDERATION
Authors: Матюшкова Валерия Сергеевна , Недорезова Елена Сергеевна 
Published: August 2022

Проблема безработицы выступает одним из основных факторов становления и развития экономики любой страны мира. Целью статьи является рассмотрение положительного и отрицательного влияния безработицы на экономическую систему России, анализ ее современного уровня, а также поиск возможностей для ее сокращения на основании имеющегося международного опыта.
The problem of unemployment is one of the main factors in the formation and development of the economy of any country in the world. The purpose of the article is to consider the positive and negative impact of unemployment on the Russian economic system, to analyze its current level, as well as to search for opportunities to reduce it based on existing international experience.
FROM THE HISTORY OF THE FORMATION AND DEVELOPMENT OF HARMONIC HEARING IN MUSIC EDUCATION
Authors: Румянцева Маргарита Алексеевна 
Published: August 2022

Статья посвящена историческому аспекту в области изучения музыкального слуха. Рассматривается вопрос становления и развития гармонического слуха в западноевропейской и отечественной музыкальной культуре. Затрагиваются также методические вопросы, связанные с формированием гармонического слуха, с принципами обучения, начиная с древней Руси и останавливаясь на современном этапе. Раскрывается постепенный процесс развития гармонического сознания в России.
The article is devoted to the historical aspect in the field of studying the musical ear. The question of the formation and development of harmonic hearing in Western European and domestic musical culture is considered. Methodological issues related to the formation of harmonic hearing, with the principles of teaching, starting from ancient Russia and stopping at the present stage, are also touched upon. The gradual process of development of harmonic consciousness in Russia is revealed.
VERBALIZATION OF THE CONCEPT RELIGION IN THE ENGLISH AND RUSSIAN LANGUAGES
Authors: Тасуева Седа Исаевна 
Published: August 2022

Данная статья посвящена рассмотрению лексем-вербализаторов концепта RELIGION/РЕЛИГИЯ согласно их диахронической динамике в английском и русском языках. Приведены основные составляющие семантического поля рассматриваемого концепта.
This article is devoted to the consideration of lexemes-verbalizers of the concept RELIGION according to their diachronic dynamics in English and Russian. The main components of the semantic field of the concept under consideration are given.
INFORMATION SECURITY IN MODERN RUSSIA
Authors: Михнева Анастасия Ильинична , Ванина Дарья Александровна 
Published: August 2022

В статье рассмотрены нормативные основы информационной безопасности в рамках Стратегии национальной безопасности России 2021 г. Отдельное внимание уделено анализу понятия и значения информационной безопасности в современных правовых условиях. Обоснован вывод о том, что субъектами системы обеспечения информационной безопасности являются органы всей системы единой публичной власти.
The article discusses the regulatory framework of information security in the framework of the National Security Strategy of Russia 2021. Special attention is paid to the analysis of the concept and meaning of information security in modern legal conditions. The conclusion is substantiated that the subjects of the information security system are the bodies of the entire system of unified public authority.
Cognitive and social well-being in older adulthood: The CoSoWELL corpus of written life stories
Authors: Kyröläinen Aki-Juhani , Gillett James , Karabin Megan , Sonnadara Ranil , Kuperman Victor 
Published: August 2022

AbstractThis paper presents the Cognitive and Social WELL-being (CoSoWELL) project that consists of two components. One is a large corpus of narratives written by over 1000 North American older adults (55+ years old) in five test sessions before and during the first year of the COVID-19 pandemic. The other component is a rich collection of socio-demographic data collected through a survey from the same participants. This paper introduces the first release of the corpus consisting of 1.3 million tokens and the survey data (CoSoWELL version 1.0). It also presents a series of analyses validating design decisions for creating the corpus of narratives written about personal life events that took place in the distant past, recent past (yesterday) and future, along with control narratives. We report results of computational topic modeling and linguistic analyses of the narratives in the corpus, which track the time-locked impact of the COVID-19 pandemic on the content of autobiographical memories before and during the COVID-19 pandemic. The main findings demonstrate a high validity of our analytical approach to unique narrative data and point to both the locus of topical shifts (narratives about recent past and future) and their detailed timeline. We make the CoSoWELL corpus and survey data available to researchers and discuss implications of our findings in the framework of research on aging and autobiographical memories under stress.
Analytic Light Curve for Mutual Transits of Two Bodies Across a Limb-darkened Star
Authors: Gordon Tyler A. , Agol Eric 
Published: August 2022

Abstract
We present a solution for the light curve of two bodies mutually transiting a star with polynomial limb darkening. The term “mutual transit” in this work refers to a transit of the star during which overlap occurs between the two transiting bodies. These could be an exoplanet with an exomoon companion, two exoplanets, an eclipsing binary and a planet, or two stars eclipsing a third in a triple-star system. We include analytic derivatives of the light curve with respect to the positions and radii of both bodies. We provide code that implements a photodynamical model for a mutual transit. We include two dynamical models, one for hierarchical systems in which a secondary body orbits a larger primary (e.g., an exomoon system) and a second for confocal systems in which two bodies independently orbit a central mass (e.g., two planets in widely separated orbits). Our code is fast enough to enable inference with Markov Chain Monte Carlo algorithms, and the inclusion of derivatives allows for the use of gradient-based inference methods such as Hamiltonian Monte Carlo. While applicable to a variety of systems, this work was undertaken primarily with exomoons in mind. It is our hope that making this code publicly available will reduce barriers for the community to assess the detectability of exomoons, conduct searches for exomoons, and attempt to validate existing exomoon candidates. We also anticipate that our code will be useful for studies of planet–planet transits in exoplanetary systems, transits of circumbinary planets, and eclipses in triple-star systems.
Mass–Velocity Dispersion Relation by Using the Gaia Data and Its Effect on Interpreting Short-duration and Degenerate Microlensing Events
Authors: Sajadian Sedighe , Rahvar Sohrab , Kazemian Fatemeh 
Published: August 2022

Abstract
Gravitational microlensing, the lensing of stars in the Milky Way with other stars, has been used for exploring compact dark matter objects, exoplanets, and black holes. The duration of microlensing events, the so-called Einstein crossing time, is a function of distance, mass, and velocities of lens objects. Lenses with different ages and masses might have various characteristic velocities inside the Galaxy and this might lead to our misinterpretation of microlensing events. In this work, we use the Gaia archived data to find a relation between the velocity dispersion and mass, and the age of stars. This mass–velocity dispersion relation confirms the known age–velocity relation for early-type and massive stars, and additionally reveals a dependence of stellar velocity dispersion on the mass for low-mass and late-type stars at a 2σ–3σ level. By considering this correlation, we simulate short-duration microlensing events due to brown dwarfs. From this simulation, we conclude that lens masses are underestimated by ∼2.5%–5.5% while modeling short-duration and degenerate microlensing events with the Bayesian analysis.
Star Cluster Formation and Evolution in M101: An Investigation with the Legacy Extragalactic UV Survey
Authors: Linden S. T. , Perez G. , Calzetti D. , Maji S. , Messa M. , Whitmore B. C. , Chandar R. , Adamo A. , Grasha K. , Cook D. O. , Elmegreen B. G. , Dale D. A. , Sacchi E. , Sabbi E. , Grebel E. K. , Smith L. 
Published: August 2022

Abstract
We present Hubble Space Telescope WFC3/UVIS (F275W, F336W) and ACS/WFC optical (F435W, F555W, and F814W) observations of the nearby grand-design spiral galaxy M101 as part of the Legacy Extragalactic UV Survey (LEGUS). Compact sources detected in at least four bands were classified by both human experts and the convolutional neural network StarcNet. Human experts classified the 2351 brightest sources, retrieving N

c
= 965 star clusters. StarcNet, trained on LEGUS data not including M101, classified all 4725 sources detected in four bands, retrieving N

c
= 2270 star clusters. The combined catalog represents the most complete census to date of compact star clusters in M101. We find that for the 2351 sources with both a visual- and machine-learning classification StarcNet is able to reproduce the human classifications at high levels of accuracy (∼80%–90%), which is equivalent to the level of agreement between human classifiers in LEGUS. The derived cluster age distribution implies a disruption rate of

dN

/

d
τ
∝

τ

−
0.45
±
0.14

over 107 < τ < 108.5 yr for cluster masses ≥103.55
M
⊙ for the central region of M101 and

dN

/

d
τ
∝

τ

−
0.02
±
0.15

for cluster masses ≥103.38
M
⊙ in the northwest region of the galaxy. The trends we recover are weaker than those of other nearby spirals (e.g., M51) and starbursts, consistent with the M101 environment having a lower-density interstellar medium, and providing evidence in favor of environmentally dependent cluster disruption in the central, southeast, and northwest regions of M101.
Supercritical Growth Pathway to Overmassive Black Holes at Cosmic Dawn: Coevolution with Massive Quasar Hosts
Authors: Hu Haojie , Inayoshi Kohei , Haiman Zoltán , Li Wenxiu , Quataert Eliot , Kuiper Rolf 
Published: August 2022

Abstract
Observations of the most luminous quasars at high redshifts (z > 6) have revealed that the largest supermassive black holes (SMBHs) at those epochs tend to be substantially overmassive relative to their host galaxies compared to the local relations, suggesting they experienced rapid early growth phases. We propose an assembly model for the SMBHs that end up in rare massive ∼1012
M
⊙ host halos at z ∼ 6–7, applying a kinetic feedback prescription for BHs accreting above the Eddington rate, provided by radiation hydrodynamic simulations for the long-term evolution of the accretion-flow structure. The large inflow rates into these halos during their assembly enable the formation of >109
M
⊙ SMBHs by z ∼ 6, even starting from stellar-mass seeds at z ∼ 30, and even in the presence of outflows that reduce the BH feeding rate, especially at early times. This mechanism also naturally yields a high BH-to-galaxy mass ratio of >0.01 before the SMBH mass reaches M
BH > 109
M
⊙ by z ∼ 6. These fast-growing SMBH progenitors are bright enough to be detected by upcoming observations with the James Webb Space Telescope over a wide range of redshift (7 < z < 15), regardless of how they were seeded.
Observing Scenarios for the Next Decade of Early Warning Detection of Binary Neutron Stars
Authors: Magee Ryan , Borhanian Ssohrab 
Published: August 2022

Abstract
We describe representative observing scenarios for early warning detection of binary neutron star mergers with the current generation of ground-based gravitational wave detectors as they approach design sensitivity. We incorporate recent estimates of the infrastructure latency and detector sensitivities to provide up-to-date predictions. We use Fisher analysis to approximate the associated localizations, and we directly compare to Bayestar to quantify biases inherited from this approach. In particular, we show that Advanced LIGO and Advanced Virgo will detect and distribute ≲1 signal with signal-to-noise ratio greater than 15 before a merger in their fourth observing run provided they maintain a 70% duty cycle. This is consistent with previous early warning detection estimates. We estimate that 60% of all observations and 8% of those detectable 20 s before a merger will be localized to ≲100 deg2. If KAGRA is able to achieve a 25 Mpc horizon, 70% of these binary neutron stars will be localized to ≲100 deg2 by a merger. As the Aundha–Hanford–KAGRA–Livingston–Virgo network approaches design sensitivity over the next ∼10 yr, we expect one (six) early warning alerts to be distributed 60 (0) s before a merger. Although adding detectors to the Hanford–Livingston–Virgo network at design sensitivity impacts the detection rate at ≲50% level, it significantly improves localization prospects. Given uncertainties in sensitivities, participating detectors, and duty cycles, we consider 103 future detector configurations so electromagnetic observers can tailor preparations toward their preferred models.
Ice Features of Low-luminosity Protostars in Near-infrared Spectra of AKARI/IRC
Authors: Kim Jaeyeong , Lee Jeong-Eun , Jeong Woong-Seob , Kim Il-Seok , Aikawa Yuri , Noble Jeniffer A. , Choi Minho , Lee Ho-Gyu , Dunham Michael M. , Kim Chul-Hwan , Koo Bon-Chul 
Published: August 2022

Abstract
We present near-infrared spectra of three low-luminosity protostars and one background star in the Perseus molecular cloud, acquired using the infrared camera on board the AKARI space telescope. For the comparison with different star-forming environments, we also present spectra of the massive protostar AFGL 7009S, where the protostellar envelope is heated significantly, and the low-mass protostar RNO 91, which is suspected to be undergoing an episodic burst. We detected ice absorption features of H2O, CO2, and CO in all spectra around the wavelengths of 3.05, 4.27, and 4.67 μm, respectively. For at least two low-luminosity protostars, we also detected the XCN ice feature at 4.62 μm. The presence of the crystalline H2O ice and XCN ice components indicates that the low-luminosity protostars experienced a hot phase via accretion bursts during the past mass accretion process. We compared the ice abundances of the low-luminosity protostars with those of embedded low-mass protostars and the dense molecular clouds and cores, suggesting that their ice abundances reflect the strength of prior bursts and the timescale after the last burst.
Chemical Differentiation and Temperature Distribution on a Few au Scale around the Protostellar Source B335
Authors: Okoda Yuki , Oya Yoko , Imai Muneaki , Sakai Nami , Watanabe Yoshimasa , López-Sepulcre Ana , Saigo Kazuya , Yamamoto Satoshi 
Published: August 2022

Abstract
Resolving physical and chemical structures in the vicinity of a protostar is of fundamental importance for elucidating their evolution to a planetary system. In this context, we have conducted 1.2 mm observations toward the low-mass protostellar source B335 at a resolution of 0.″03 with the Atacama Large Millimeter/submillimeter Array. More than 20 molecular species including HCOOH, NH2CHO, HNCO, CH3OH, CH2DOH, CHD2OH, and CH3OD are detected within a few tens au around the continuum peak. We find a systematic chemical differentiation between oxygen-bearing and nitrogen-bearing organic molecules by using the principal component analysis for the image cube data. The distributions of the nitrogen-bearing molecules are more compact than those of the oxygen-bearing ones except for HCOOH. The temperature distribution of the disk/envelope system is revealed by a multiline analysis for each of HCOOH, NH2CHO, CH3OH, and CH2DOH. The rotation temperatures of CH3OH and CH2DOH at the radius of 0.″06 along the envelope direction are derived to be 150–165 K. On the other hand, those of HCOOH and NH2CHO, which have a smaller distribution, are 75–112 K, and are significantly lower than those for CH3OH and CH2DOH. This means that the outer envelope traced by CH3OH and CH2DOH is heated by additional mechanisms rather than protostellar heating. We here propose the accretion shock as the heating mechanism. The chemical differentiation and the temperature structure on a scale of a few au provide us with key information to further understand chemical processes in protostellar sources.
Density and Refractive Index of Carbon Monoxide Ice at Different Temperatures
Authors: Luna Ramón , Millán Carlos , Domingo Manuel , Santonja Carmina , Satorre Miguel Á. 
Published: August 2022

Abstract
This paper is intended to study the density and the refractive index of the solid carbon monoxide in the interval 13–28 K to improve our understanding of the dynamics in the astrophysical environments where they are present. A series of deposition experiments have been performed under high vacuum conditions to study the properties of this ice under astrophysical conditions. Ice density has been experimentally calculated at different deposition temperatures of astrophysical interest, which complement the scarce values present in the literature. The refractive index has also been experimentally determined. The data have been used to obtain an experimental relationship between refractive index and density. Values of density are necessary to interpret observations of astrophysical objects or to design irradiation experiments to understand how irradiation affects ices present in these objects. The experimental relationship found between density and refractive index allows us to estimate density from a known refractive index, even for temperatures not reached using our experimental setup.
Thermal and Non-thermal Properties of Active Region Recurrent Coronal Jets
Authors: Paraschiv Alin R. , Donea Alina C. , Judge Philip G. 
Published: August 2022

Abstract
We present observations of recurrent active region coronal jets, and derive their thermal and non-thermal properties, by studying the physical properties of the plasma simultaneously at the base footpoint and along the outflow of jets. The sample of analyzed solar jets were observed by SDO-AIA in extreme ultraviolet and by RHESSI in the X-ray domain. The main thermal plasma physical parameters, such as temperature, density, energy flux contributions, etc., are calculated using multiple inversion techniques to obtain the differential emission measure from extreme-ultraviolet filtergrams. The underlying models are assessed, and their limitations and applicability are scrutinized. Complementarily, we perform source reconstruction and spectral analysis of higher energy X-ray observations to further assess the thermal structure and identify non-thermal plasma emission properties. We discuss a peculiar penumbral magnetic reconnection site, which we previously identified as a “Coronal Geyser.” Evidence supporting cool and hot thermal emission, as well as non-thermal emission, is presented for a subset of geyser jets. These active region jets are found to be energetically stronger than their polar counterparts, but we find their potential influence on heliospheric energetics and dynamics to be limited. We scrutinize whether the geyser does fit the non-thermal erupting microflare picture, finding that our observations at peak flaring times can only be explained by a combination of thermal and non-thermal emission models. This analysis of geysers provides new information and observational constraints applicable to theoretical modeling of solar jets.