bluuebunny/crossref_metadata_2025_split huggingface dataset:
8.7. Improving the methodology for generating statistical information on social security in the Russian Federation taking into account the ESSPROS and SOCX standards
Authors: Балынин И.В. 
Published: July 2020

В статье представлены результаты проведенного автором исследования методологии формирования статистической информации о социальном обеспечении в Российской Федерации, обозначены пути ее совершенствования с учетом стандартов ESSPROSи SOCX. Особое внимание уделено маркировке структурных единиц отдельных отчетных и статистических форм, содержащих информацию о социальном обеспечении в РФ. Сделан вывод о необходимости увеличения объема и осуществления дополнительной детализации текстового и числового материала, что позволит сформировать полноценную базу данных о социальном обеспечении в РФ.
The article presents the results of a study by the author of the methodology for generating statistical information on social security in the Russian Federation, outlines ways to improve it taking into account the ESSPROS and SOCX standards. Particular attention is paid to marking the structural units of individual reporting and statistical forms containing information on social security in the Russian Federation. It is concluded that it is necessary to increase the volume and implement additional detailing of textual and numerical material, which will allow the formation of a complete database of social security in the Russian Federation.
2.2. THE FORMATION OF INDICATORS OF NON-FINANCIAL REPORTS ACCORDING TO ACCOUNTING AND MANAGEMENT ACCOUNTING
Authors: Лесина Т.В. , Филимонова Е.А. 
Published: July 2020

Актуальность исследуемых вопросов определена тем, что показатели нефинансовой отчетности приобретают все большее значение для стейкхолдеров. В формировании нефинансовой отчетности в Российской Федерации заинтересованность проявляется и на государственном уровне. Цель статьи заключается в демонстрации возможностей использования показателей бухгалтерского и управленческого учета для формирования отдельных показателей нефинансовой отчетности в разрезе экономической, экологической и социальной категории. Ведущим методом к исследованию данной проблемы является наблюдение, классификация, обобщение, систематизация. В статье представлены примерные показатели нефинансовой отчетности по стандартам GRI и раскрытие их в бухгалтерском учете организации. Материалы статьи могут быть полезными при подготовке информации для формирования нефинансовой отчетности руководителями и работниками экономических служб.
The Relevance of the studied issues is determined by the fact that the indicators of non-financial reporting are becoming increasingly important for stakeholders. In the formation of non-financial reporting in Russia, interest is manifested at the state level. The purpose of the article is to demonstrate the possibility of using indicators of accounting and management accounting for the formation of individual indicators of non-financial reporting. The leading method to study this problem is observation, classification, generalization, systematization. The article presents approximate indicators of non-financial reporting on GRI standards and their disclosure in the accounting of the organization. The materials of the article can be useful in the preparation of information for the formation of non-financial reporting to managers and employees of economic services.
6.1. Modern techniques of behavioral analysis of financial instruments on the stock market
Authors: Богатырев С.Ю. 
Published: July 2020

В статье рассматриваются диапазоны конкретных значений поправки к бэта-коэффициенту, используемому при расчете ставки дисконтирования по модели CAPM для получения поведенческой ставки дисконтирования и расчета рыночной стоимости акций на рынках с учетом поведенческих факторов. В статье продемонстрировано применение инструментария поведенческого ценообразования. Представлены конкретные расчеты, предложены ориентиры для расчета поправки компонентов формулы расчета ставки дисконтирования для расчета стоимости с учетом эмоционального настроения на фондовых рынках.
The article discusses the ranges of specific values of the beta correction ‒ the coefficient used in calculating the discount rate using the CAPM model to obtain a behavioral discount rate and calculating the market value of shares in the markets, taking into account behavioral factors. The article demonstrates the use of behavioral pricing tools. Specific calculations are presented, guidelines are proposed for calculating the amendments to the components of the formula for calculating the discount rate for calculating value, taking into account the emotional mood of stock markets.
3.1. Evaluation of the return on health capital in the Russian economy
Authors: Мельников Р.М. 
Published: July 2020

В статье оценивается эластичность предложения труда и ставок часовой заработной платы по состоянию здоровья для различных профессий. Показано, что мужчинам хорошее здоровье обеспечивает премию к часовой ставке заработной платы, а для женщин состояние здоровья позволяет регулировать уровень рабочей нагрузки.
The article evaluates the elasticity of the labor supply and hourly wage rates on health condition for different occupations. It has been shown that men's good health provides a premium to the hourly wage, and women regulate the level of workload based on health status. The length of the working week is most sensitive to changes in health for workers and office workers. Investments in health contribute to the increase in labor income in most occupations and industries.
8.5. TRANSFORMATION OF THE PROPERTY INSTITUTION IN THE MODERN ECONOMY
Authors: Устюжанина Е.В. , Ходжа К. 
Published: July 2020

В статье обосновано, что развитие института собственности происходит путем расщепления целостной системы отношений на отдельные составляющие. Это расщепление осуществляется в трех направлениях: расщепление объекта собственности, расщепление субъекта собственности и ослабление связей между субъектом и объектом собственности. Научная новизна методологии проведенного исследования заключается в сочетании неоклассического и институционального подходов. В качестве методов исследования в работе использованы исторический метод, структурный и сравнительный анализ
The article justifies that the development of the ownership institution takes place by splitting the holistic system of relations into separate components. This splitting is carried out in three directions: splitting the object of ownership, splitting the subject of ownership, and weakening the links between the subject and the object of ownership. In this transformation we see the implementation of the dialectical law of unity (integration of property rights and roles of owners) and the struggle of opposites (increasing splitting of both objects and subjects of ownership). The scientific novelty of the methodology is based on the combination of neoclassical and institutional approaches. Historical method, structural and comparative analysis are used as research methods of this study.
9.3. High-performance computing technologies in the tasks of socio-economic development of regions
Authors: Черногорский С.А. , Швецов К.В. , Костин К.Б. 
Published: July 2020

В работе рассматриваются задачи описания социально-экономического развития регионов. Сам характер существа рассматриваемых проблем указывает на то обстоятельство, что единственным и незаменимым инструментом здесь являются технологии математического моделирования. В работе применение подходов математического моделирования на основе высокопроизводительных вычислительных технологий рассматриваются на примере решения модельной задачи об управлении развитием регионов. Представлены результаты расчетов поведения динамической модели региона, проходящей через иерархию неустойчивостей (соответствие одних и тех же стационарных точек модели различным параметрам), в которых развиваются все более и более сложные структуры.
The article deals with the problem of describing social and economic development of the regions. The nature of the merits issues points to the fact that the only and indispensable tool here is the technology of mathematical modeling. In the paper, the application of mathematical modeling approaches based on high-performance computing technologies is considered on the example of solving a model problem on the management of regional development. The results of calculations of the behavior of the dynamic model of the region passing through the hierarchy of instabilities (the correspondence of the same stationary points of the model to different parameters) are presented in which more and more complex structures develop.
7.3. STRATEGY OF DEVELOPMENT OF THE REGIONAL ECONOMIC SYSTEM OF THE SUBJECT OF THE RUSSIAN FEDERATION
Authors: Журавлев Д.М. 
Published: July 2020

В статье рассматриваются теоретические и практические аспекты управления развитием региона. Раскрывается содержание процесса стратегирования. Сформулированы требования к стратегии, отражающие специфику региона как объекта управления. Определен перечень этапов регионального стратегирования и формализованы требования для подготовки и разработки экономико-математической модели. Применяя на практике полученные результаты, реализуется возможность целеполагания, прогнозирования и управления развитием.
The article discusses the theoretical and practical aspects of regional development management. The content of the strategic process is disclosed. The requirements to the strategy are formulated, reflecting the specifics of the region as a management object. The list of stages of regional strategic planning is defined and the requirements for the preparation and development of an economic and mathematical model are formalized. Putting the results into practice, the possibility of goal-setting, forecasting and development management is realized.
3.3. Predicative modeling of current liquidity of a commercial bank based on multivariate correlation analysis
Authors: Шершнева Е.Г. , Алпатова Е.С. , Бабанова Ф.Р. , Хасан Б.Б.-Х. 
Published: July 2020

Несмотря на то, что базовые экономические модели показывают свою жизнеспособность, прогрессивные информационные технологии требуют все более тонких инструментов воздействия на процессы регулирования денежных потоков в банковском секторе. Одним из таких инструментов традиционно выступает управление ликвидностью коммерческого банка. Вместе с тем, процессы управления ликвидностью сопровождаются кризисными явлениями и внутрибанковскими слабыми звеньями в коммуникациях и технологиях.В искомом ключе авторы предлагают методический подход по синхронизации целевых ориентиров и релевантных показателей деятельности банка на основе метода парных корреляций. Проанализированы факторы, влияющие на ликвидность современного банка с точки зрения тактических преференций. Обосновано заключение по применению политики рационального управления ликвидностью, включающей осмотрительное целеполагание, финансовое планирование и рисковую сдержанность.
The article presents a study of dependence of short-term bank`s liquidity on a number of economic indicators based on correlation and regression modeling. It is established that the dynamics of current liquidity of banks is significantly influenced by such parameters as non-performant loans, short-term liabilities and equity. The proposed approach can be used by commercial banks` analysts in the development of models for assessing the financial condition.
7.1. METHODICAL ASPECTS OF EVALUATING THE INFORMATION OPENNESS OF A LOCAL SELF-GOVERNMENT BODY
Authors: Атаева А.Г. , Дунаева А.В. 
Published: July 2020

В статье анализируется опыт регионов Российской Федерации по оценке информационной открытости органов государственной власти и органов местного самоуправления. Предлагается комплексный показатель информационной открытости органа местного самоуправления, который включает в себя сводные показатели работы органа власти с населением, качества и посещаемости официального сайта, активности работы органа власти в социальных сетях, качества организации работы со средствами массовой информации, удовлетворенности населения информационной открытостью.
The article analyzes the experience of Russian regions in assessing the informational openness of state authorities and local governments. A comprehensive indicator of the information openness of the local government is proposed, which includes summary indicators of the work of the government with the population, the quality and attendance of the official website, the activity of the government on social networks, the quality of the organization of work with the media, and public satisfaction with information openness.
Search for TiO and Optical Nightside Emission from the Exoplanet WASP-33b
Authors: Herman Miranda K. , Mooij Ernst J. W. de , Jayawardhana Ray , Brogi Matteo 
Published: July 2020

Abstract
With a temperature akin to an M dwarf, WASP-33b is among the hottest Jupiters known, making it an ideal target for high-resolution optical spectroscopy. By analyzing both transmission and emission spectra, we aim to substantiate previous reports of atmospheric TiO and a thermal inversion within the planet’s atmosphere. We observed two transits and six arcs of the phase curve with the Echelle SpectroPolarimetric Device for the Observation of Stars (ESPaDOnS) on the Canada–France–Hawaii Telescope and High Resolution Echelle Spectrometer (HIRES) on the Keck telescope, which provide high spectral resolution and ample wavelength coverage. We employ the Doppler cross-correlation technique to search for the molecular signatures of TiO and H2O in these spectra, using models based on the TiO line list of Plez. Though we cannot exclude line-list-dependent effects, our data do not corroborate previous indications of a thermal inversion. Instead we place a 3σ upper limit of 10−9 on the volume mixing ratio of TiO for the T–P profile we consider. While we are unable to constrain the volume mixing ratio of water, our strongest constraint on TiO comes from dayside emission spectra. This apparent absence of a stratosphere sits in stark contrast to previous observations of WASP-33b as well as theoretical predictions for the atmospheres of highly irradiated planets. The discrepancy could be due to variances between line lists, and we stress that detection limits are only as good as the line list employed, and are only valid for the specific T–P profile considered due to the strong degeneracy between lapse rate (

) and molecular abundance.
Scaling K2. III. Comparable Planet Occurrence in the FGK Samples of Campaign 5 and Kepler
Authors: Zink Jon K. , Hardegree-Ullman Kevin K. , Christiansen Jessie L. , Petigura Erik A. , Dressing Courtney D. , Schlieder Joshua E. , Ciardi David R. , Crossfield Ian J. M. 
Published: July 2020

Abstract
Using our K2 Campaign 5 fully automated planet-detection data set (43 planets), which has corresponding measures of completeness and reliability, we infer an underlying planet population model for the FGK dwarf sample (9257 stars). Implementing a broken power law for both the period and radius distributions, we find an overall planet occurrence of

planets per star within a period range of 0.5–38 days. Making similar cuts and running a comparable analysis on the Kepler sample (2318 planets; 94,222 stars), we find an overall occurrence of 1.10 ± 0.05 planets per star. Since the Campaign 5 field is nearly 120 angular degrees away from the Kepler field, this occurrence similarity offers evidence that the Kepler sample may provide a good baseline for Galactic inferences. Furthermore, the Kepler stellar sample is metal-rich compared to the K2 Campaign 5 sample, so a finding of occurrence parity may reduce the role of metallicity in planet formation. However, a weak (1.5σ) difference, in agreement with metal-driven formation, is found when assuming the Kepler model power laws for the K2 Campaign 5 sample and optimizing only the planet occurrence factor. This weak trend indicates that further investigation of metallicity-dependent occurrence is warranted once a larger sample of uniformly vetted K2 planet candidates is made available.
Synchrotron Self-Compton Scattering in Sgr A* Derived from NIR and X-Ray Flare Statistics
Authors: Subroweit Matthias , Mossoux Enmanuelle , Eckart Andreas 
Published: July 2020

Abstract
The flaring activity of Sagittarius A* (Sgr A*) can be analyzed by statistical means to test emission models for its accretion flow. A particular modeling question is whether the observed X-ray flares are the high-energy end of a synchrotron spectrum or if they arise from self-Comptonized photons of a lower-energy synchrotron process. We use already published Chandra X-ray Visionary Project data to statistically investigate the X-ray count-rate distribution of Sgr A*. Two previous workgroups have already undertaken such an analysis on that data. They modeled the flaring part of the emission with a bounded power law, i.e., a power-law distribution with a hard cutoff at the highest measured count rate. With this model, both teams obtain a power-law index

. We show that the flare count-rate distribution can also be well described by a truncated, i.e., an exponentially decaying power law. We argue that an exponential truncation is a more natural model than a hard cutoff. With this alternate model, our fit yields a power-law index

. We find that this slope can be canonically explained by a synchrotron self-Compton (SSC) process. Therefore, we argue that SSC models are the best ones suitable to explain the observed X-ray count-rate distribution.
Solar Vortex Tubes: Vortex Dynamics in the Solar Atmosphere
Authors: Silva Suzana S. A. , Fedun Viktor , Verth Gary , Rempel Erico L. , Shelyag Sergiy 
Published: July 2020

Abstract
In this work, a state-of-the-art vortex detection method, Instantaneous Vorticity Deviation, is applied to locate three-dimensional vortex tube boundaries in numerical simulations of solar photospheric magnetoconvection performed by the MURaM code. We detected three-dimensional vortices distributed along intergranular regions and displaying coned shapes that extend from the photosphere to the low chromosphere. Based on a well-defined vortex center and boundary, we were able to determine averaged radial profiles and thereby investigate the dynamics across the vortical flows at different height levels. The solar vortex tubes present nonuniform angular rotational velocity, and, at all height levels, there are eddy viscosity effects within the vortices, which slow down the plasma as it moves toward the center. The vortices impact the magnetic field as they help to intensify the magnetic field at the sinking points, and in turn, the magnetic field ends up playing an essential role in the vortex dynamics. The magnetic field was found to be especially important to the vorticity evolution. On the other hand, it is shown that, in general, kinematic vortices do not give rise to magnetic vortices unless their tangential velocities at different height levels are high enough to overcome the magnetic tension.
KIC 12268220: A δ Scuti Pulsating Star and an Active Protohelium White Dwarf in an Eclipsing Binary System
Authors: Cui Kaiming , Guo Zhao , Gao Qing , Ren Juanjuan , Zhang Junbo , Zhou Yutao , Liu Jifeng 
Published: July 2020

Abstract
We present a photometric, spectroscopic, asteroseismic, and evolutionary analysis of the Algol-type eclipsing binary KIC 12268220. We find the O’Connell effect and anticorrelated eclipse timing variations in the Kepler light curve, revealing the presence of large starspots. Radial velocities and atmospheric parameters are obtained from ground-based spectroscopic observations. Combined with the radial velocity measurements and Gaia-derived total luminosity, our light-curve modeling yields the solution of the physical parameters for both the primary and secondary components. We find 14 independent frequencies arising from the δ Scuti primary, and the observed frequencies agree with the frequency range of unstable modes from nonadiabatic calculations. Based on the conclusion from previous literature, we run a grid of models to study the evolution process of our system. The evolutionary tracks of our model suggest that the low-mass (

∼
0.23

M

⊙

) evolved secondary shows a similar evolutionary state to the R CMa-type system, which might evolve to an EL CVn system.
Heuristic Description of Perpendicular Particle Transport in Turbulence with Super-diffusive Magnetic Field Lines
Authors: Shalchi A. 
Published: July 2020

Abstract
Recently a heuristic description of collisionless perpendicular diffusion of energetic particles was presented. The latter approach describes the transport of energetic particles across a mean magnetic field based on simple physical arguments. Although this approach was developed with the intention to improve our understanding of perpendicular diffusion, this heuristic approach also provided some interesting quantitative results such as an explanation of the factor a
2 used in the past to balance out inaccuracies of systematic analytical theories. However, the aforementioned heuristic approach is based on the assumption that magnetic field lines become diffusive after overcoming the initial free-streaming regime. In the current paper we alter the heuristic approach to make it applicable for turbulence spectra leading to super-diffusive magnetic fields lines. It is argued that particle diffusion is still restored in the late time limit. In the high-energy limit this recovery of diffusion is based on a hybrid model in which particles move half ballistically and half diffusively in the parallel direction. Furthermore, this leads to the relation

between perpendicular and parallel mean free paths of the energetic particles. This type of transport was obtained in the past from test-particle simulations as well as systematic analytical theories. In the current paper we present the first time an explanation of this behavior based on simple physical arguments.
Emergence of an Ultrared, Ultramassive Galaxy Cluster Core at z = 4
Authors: Long Arianna S. , Cooray Asantha , Ma Jingzhe , Casey Caitlin M. , Wardlow Julie L , Nayyeri Hooshang , Ivison R. J. , Farrah Duncan , Dannerbauer Helmut 
Published: July 2020

Abstract
Recent simulations and observations of massive galaxy cluster evolution predict that the majority of stellar mass buildup happens within cluster members by z = 2, before cluster virialization. Protoclusters rich with dusty, star-forming galaxies (DSFGs) at z > 3 are the favored candidate progenitors for these massive galaxy clusters at z ∼ 0. We present here the first study analyzing stellar emission along with cold dust and gas continuum emission in a spectroscopically confirmed z = 4.002 protocluster core rich with DSFGs, the Distant Red Core (DRC). We combine new Hubble Space Telescope and Spitzer data with existing Gemini, Herschel, and Atacama Large Millimeter/submillimeter Array observations to derive individual galaxy-level properties and compare them to coeval field and other protocluster galaxies. All of the protocluster members are massive (>1010
M
⊙), but not significantly more so than their coeval field counterparts. Within uncertainty, all are nearly indistinguishable from galaxies on the star-forming versus stellar mass main-sequence relationship and the star formation efficiency plane. Assuming no future major influx of fresh gas, we estimate that these gaseous DSFGs will deplete their gas reservoirs in ∼300 Myr, becoming the massive quiescent ellipticals dominating cluster cores by z ∼ 3. Using various methodologies, we derive a total z = 4 halo mass of ∼1014
M
⊙ and estimate that the DRC will evolve to become an ultramassive cluster core of mass ≳1015
M
⊙ by z = 0.