bluuebunny/crossref_metadata_2025_split huggingface dataset:
MINDFULNESS AS A NEW APPROACH TO SELF-REGULATION: PSYCHOLOGICAL AND PSYCHOPHYSIOLOGICAL EFFECTS OF MINDFULNESS MEDITATION
Authors: Гайдукова Ольга Леонидовна 
Published: May 2021

В статье раскрывается феномен медитации осознанности как инструмент психотерапевтических интервенций в отношении взрослых индивидов с нарушениями умственного развития (умственной отсталостью). Также рассматриваются некоторые наиболее распространенные техники данного подхода, чья эффективность применительно к данной группе популяции была доказана в приведенных в статье результатах экспериментальных исследований за последние годы.
The article describes the phenomenon of mindfulness meditation as a possible tool for psychotherapeutic interventions toward adult individuals with disorders of intellectual development (mental retardation). It also reviews some of the most common techniques of this approach, whose effectiveness for the considered group of the population has been proven by the results of experimental studies within recent years.
DRUG-INDUCED ITSENKO-CUSHING SYNDROME AS AN IMPORTANT PROBLEM OF MODERN MEDICINE
Authors: Власюк Ангелина Александровна , Федорцов Александр Александрович , Васильева Людмила Валентиновна , Малюков Дмитрий Андреевич 
Published: May 2021

В данной статье представлена информация о медикаментозном синдроме Иценко-Кушинга, развивающегося у пациентов вследствие употребления глюкокортикойдов при различных заболеваниях, а также зависимость развития осложнений от методик получаемого лечения.
The article presents information about the Itsenko-Cushing drug syndrome, which develops in patients as a result of the use of glucocorticoids for various diseases, as well as the dependence of the development of complications on the received treatment methods.
THE IMPACT OF A COURSE OF THE AUTHOR'S METHOD OF VIBROACOUSTIC MASSAGE ON THE PSYCHO-EMOTIONAL STATE OF A PERSON
Authors: Огуй Виктор Олегович 
Published: May 2021

В исследовании изучались изменения показателей психоэмоциальных характеристик в результате воздействия курсом виброакустического массажа поющими чашами (8-12 процедур ежедневно), выполненного по протоколу государственного патента на изобретение RU 2 687 006 C1. Автор и патентообладатель - Огуй Виктор Олегович. Полученные результаты свидетельствуют о том, что под воздействием виброакустического массажа поющими чашами, выполненного курсом из 8-12 процедур у испытуемых, значительно улучшаются психоэмоциональные характеристики. Кроме того, отмечалось статистически значимое снижение уровня депрессии, уменьшение уровня личностной и ситуативной тревожности. Представленный метод можно рекомендовать к использованию в санаторно-курортных и СПА-учреждениях.
The research studied changes in psycho-emotional characteristics as a result of exposure to a course of vibroacoustic massage with singing bowls (8-12 procedures daily), performed under the protocol of the state patent for invention RU 2 687 006 C1. Author and patentee - Oguy Viktor Olegovich. Conducting vibroacoustic massage according to the "singing bowls" method in a course of 8-12 sessions contributed to a significant improvement in the psycho-emotional characteristics of the subjects. In addition, there was a statistically significant decrease in the level of depression, a decrease in the level of personal and situational anxiety. The presented method is recommended for use in health resorts and SPA-institutions.
JUDGING OF THE COMPETITIONS IN MEN'S ARTISTIC GYMNASTICS
Authors: Семенова Лиана Олеговна 
Published: May 2021

Статья посвящена описанию судейства соревнований по мужской художественной гимнастике. В работе проведен анализ правил соревнований и сравнение судейства мальчиков и девочек в художественной гимнастике. Данные в статье помогут точно и грамотно разобраться в системе подсчета оценок на соревнованиях по художественной гимнастике у мальчиков, так как данный вид программы представлен на официальных стартах Чемпионата и Первенства России [1].
The article is devoted to the description of judging competitions in men's rhythmic gymnastics. The paper analyzes the rules of competitions and compares the judging of boys and girls in rhythmic gymnastics. The data in the article will help you accurately and competently understand the system of scoring in rhythmic gymnastics competitions for boys, as this type of program is presented at the official starts of the Championship and the Championship of Russia.
HELICOBACTER PYLORI INFECTION AND ITS ROLE IN THE PATHOGENESIS OF NONALCOHOLIC FATTY LIVER DISEASE
Authors: Абрамян Мария Владимировна , Свиридова Алина Викторовна , Веселова Елена Николаевна 
Published: May 2021

Велика ли роль инфекции Helicobacter pylori на патогенез неалкогольной жировой болезни печени (НАЖБП)? Последние данные свидетельствуют о наличии их взаимосвязи [1, 2]. Однако до сих пор данная тема остается под вопросом. Цель данной работы - исследовать возможную связь и клиническое значение Helicobacter pylori в патогенезе неалкогольной жировой болезни печени.
Is the role of Helicobacter pylori infection on the pathogenesis of non-alcoholic fatty liver disease (NAFLD) significant? Recent data indicate the presence of their relationship [1, 2]. However, until now, this topic remains in question. The aim of this work is to investigate the possible relationship and clinical significance of Helicobacter pylori in the pathogenesis of non-alcoholic fatty liver disease
THE STRUCTURE OF CADETS' READINESS FOR PROFESSIONAL INTERACTION IN A POLYCULTURAL ENVIRONMENT
Authors: Пинчукова Оксана Сергеевна 
Published: May 2021

В данной статье рассматривается структура готовности курсантов военных вузов к профессиональному взаимодействию в поликультурной среде. Описан ряд компонентов и выделены базовые характеристики данного взаимодействия.
This article discusses the structure of cadets’ readiness of military universities for professional interaction in a multicultural environment. A number of components are described and the basic characteristics of this interaction are highlighted.
ANALYSIS OF NATO STANDARDS PERTAINING TO THE CONFORMANCE ASSESSMENT OF PIECES OF ARMAMENT AND MILITARY EQUIPMENT WITH THE REQUIREMENTS OF RESISTANCE TO CLIMATIC FACTORS
Authors: Lappo I. , Chervotoka О. , Herashchenko M. 
Published: May 2021

The strategic course towards the integration of Ukraine into the European economic space provides for the introduction of appropriate quality standards in the production of domestic products, including military ones. The state leadership has declared the transition of the Ukrainian defense–industrial complex to the standards of the European Union and NATO until 2022. The introduction of these standards should ensure the compatibility of the Armed Forces of Ukraine and the NATO countries armies. Since the development of high-precision armament and military equipment leads to the need to create a new generation of specialized systems for monitoring their characteristics and parameters during testing, the primary need is to improve the testing system, the normative base of which is the system of standards. As a result, first of all, the standards governing the preparation and testing of new and modernized armament and military equipment are subject to revision.
In order to intensify the work on the revision of standards, as well as to ensure regulatory support of the life cycle of armament and military equipment for a full transition to the use in production of international, European and NATO standards, amendments are being made to the national legislation of Ukraine. The purpose of this process is to create a mechanism for the implementation of NATO standards or their provisions in the Armed Forces of Ukraine.
The purpose of the article is to analyze the main provisions in NATO standards for testing the impact of climatic factors in order to implement them in the system of testing pieces of armament and military equipment.
During the research general scientific methods of processing and systematization of information, in particular system analysis and synthesis of organizational and technical systems, were applied.
In connection with the abolition of the state military standards of the GOST B system, which established the values quality level and the composition, sequence, general requirements for testing equipment, instruments, devices for military purposes, there was an urgent need for regulatory support for the organization and testing of armament and military equipment. It was determined that one of the main directions of solving the problem of normative support for the organization and testing of armament and military equipment is the adoption of international military standards as the state ones.
The main provisions of the standards that ensure the organization and conducting of military equipment climatic tests were analysed, the structure and content of these standards were considered.
Pelatihan Strategi E-Commerce Bagi Pelaku Usaha Mikro, Kecil dan Menengah di Kecamatan Bubutan Kota Surabaya
Authors: Yani Prawita , Susila Muktar Redy , Nugroho Wawan Cahyo , Putri Rizfanni Cahya 
Published: May 2021

Untuk memperkuat daya saing Usaha Mikro Kecil dan Menengah (UMKM) diperlukan suatu strategi guna memperluas marketing dari penjualan produk. Salah satu jalur distribusi dari penjualan produk saat iniÂ adalah e-commerce. Di era modern ini, penjualan produk bisa dijual melalui platform digital atau atau yang biasa dikenal dengan sebutan e-commerce. Kecamatan Bubutan merupakan salah satu kecamatan yang ada di Kota Surabaya yang terdiri dari banyak para pelaku usaha yang usianya terbilang sudah tidak muda lagi. Oleh karena itu pelatihan e-commerce dan strateginya mutlak diperlukan bagi pengembangan dan kelangsungan usaha. Para pelaku usaha di Kecamatan Bubutan telah dilatih dengan materi strategi e-commerce untuk menjalankan usahanya. Setelah dilakukan monitoring dan evaluasi, para pelaku UMKM memiliki bekal yang cukup baik dalam memperluas jalur distribusi pemasarannya melalui media digital sehingga bisa menjual secara global. Namun, untuk bisa mendapatkan manfaat yang lebih berkesinambungan, pelatihan sejenis dan dengan materi yang lebih mendalam serta durasi yang lebih lama perlu dilakukan.
Identifying Planetary Transit Candidates in TESS Full-frame Image Light Curves via Convolutional Neural Networks
Authors: Olmschenk Greg , Ishitani Silva Stela , Rau Gioia , Barry Richard K. , Kruse Ethan , Cacciapuoti Luca , Kostov Veselin , Powell Brian P. , Wyrwas Edward , Schnittman Jeremy D. , Barclay Thomas 
Published: May 2021

Abstract
The Transiting Exoplanet Survey Satellite (TESS) mission measured light from stars in ∼75% of the sky throughout its 2 yr primary mission, resulting in millions of TESS 30-minute-cadence light curves to analyze in the search for transiting exoplanets. To search this vast data trove for transit signals, we aim to provide an approach that both is computationally efficient and produces highly performant predictions. This approach minimizes the required human search effort. We present a convolutional neural network, which we train to identify planetary transit signals and dismiss false positives. To make a prediction for a given light curve, our network requires no prior transit parameters identified using other methods. Our network performs inference on a TESS 30-minute-cadence light curve in ∼5 ms on a single GPU, enabling large-scale archival searches. We present 181 new planet candidates identified by our network, which pass subsequent human vetting designed to rule out false positives. Our neural network model is additionally provided as open-source code for public use and extension.
Calibration of the Hα Age–Activity Relation for M Dwarfs
Authors: Kiman Rocio , Faherty Jacqueline K. , Cruz Kelle L. , Gagné Jonathan , Angus Ruth , Schmidt Sarah J. , Mann Andrew W. , Bardalez Gagliuffi Daniella C. , Rice Emily 
Published: May 2021

Abstract
In this work, we calibrate the relationship between Hα emission and M dwarf ages. We compile a sample of 892 M dwarfs with Hα equivalent width (Hα EW) measurements from the literature that are either comoving with a white dwarf of known age (21 stars) or in a known young association (871 stars). In this sample we identify 7 M dwarfs that are new candidate members of known associations. By dividing the stars into active and inactive categories according to their Hα EW and spectral type (SpT), we find that the fraction of active dwarfs decreases with increasing age, and the form of the decline depends on SpT. Using the compiled sample of age calibrators, we find that Hα EW and fractional Hα luminosity (L
Hα
/L
bol) decrease with increasing age. Hα EW for SpT ≤ M7 decreases gradually up until ∼1 Gyr. For older ages, we found only two early M dwarfs that are both inactive and seem to continue the gradual decrease. We also found 14 mid-type M dwarfs, out of which 11 are inactive and present a significant decrease in Hα EW, suggesting that the magnetic activity decreases rapidly after ∼1 Gyr. We fit L
Hα
/L
bol versus age with a broken power law and find an index of

for ages ≲776 Myr. The index becomes much steeper at older ages, but a lack of field age-calibrators (≫1 Gyr) leaves this part of the relation far less constrained. Finally, from repeated independent measurements for the same stars, we find that 94% of them have a level of Hα EW variability ≤5 Å at young ages (<1 Gyr).
Reconstructing the Extreme Ultraviolet Emission of Cool Dwarfs Using Differential Emission Measure Polynomials
Authors: Duvvuri Girish M. , Sebastian Pineda J. , Berta-Thompson Zachory K. , Brown Alexander , France Kevin , Kowalski Adam F. , Redfield Seth , Tilipman Dennis , Vieytes Mariela C. , Wilson David J. , Youngblood Allison , Froning Cynthia S. , Linsky Jeffrey , Parke Loyd R. O. , Mauas Pablo , Miguel Yamila , Newton Elisabeth R. , Rugheimer Sarah , Christian Schneider P. 
Published: May 2021

Abstract
Characterizing the atmospheres of planets orbiting M dwarfs requires understanding the spectral energy distributions of M dwarfs over planetary lifetimes. Surveys like MUSCLES, HAZMAT, and FUMES have collected multiwavelength spectra across the spectral type’s range of T
eff and activity, but the extreme ultraviolet (EUV, 100–912 Å) flux of most of these stars remains unobserved because of obscuration by the interstellar medium compounded with limited detector sensitivity. While targets with observable EUV flux exist, there is no currently operational facility observing between 150 and 912 Å. Inferring the spectra of exoplanet hosts in this regime is critical to studying the evolution of planetary atmospheres because the EUV heats the top of the thermosphere and drives atmospheric escape. This paper presents our implementation of the differential emission measure technique to reconstruct the EUV spectra of cool dwarfs. We characterize our method’s accuracy and precision by applying it to the Sun and AU Mic. We then apply it to three fainter M dwarfs: GJ 832, Barnard’s star, and TRAPPIST-1. We demonstrate that with the strongest far-ultraviolet (FUV, 912–1700 Å) emission lines, observed with the Hubble Space Telescope and/or Far Ultraviolet Spectroscopic Explorer, and a coarse X-ray spectrum from either the Chandra X-ray Observatory or XMM-Newton, we can reconstruct the Sun’s EUV spectrum to within a factor of 1.8, with our model’s formal uncertainties encompassing the data. We report the integrated EUV flux of our M dwarf sample with uncertainties of a factor of 2–7 depending on available data quality.
Revisiting Attenuation Curves: The Case of NGC 3351*
Authors: Calzetti Daniela , Battisti Andrew J. , Shivaei Irene , Messa Matteo , Cignoni Michele , Adamo Angela , Dale Daniel A. , Gallagher John S. , Grasha Kathryn , Grebel Eva K. , Kennicutt Robert C. , Linden Sean T. , Östlin Göran , Sabbi Elena , Smith Linda J. , Tosi Monica , Wofford Aida 
Published: May 2021

Abstract
Multiwavelength images from the far-UV (∼0.15 μm) to the submillimeter of the central region of the galaxy NGC 3351 are analyzed to constrain its stellar populations and dust attenuation. Despite hosting a ∼1 kpc circumnuclear starburst ring, NGC 3351 deviates from the IRX–β relation, the relation between the infrared-to-UV luminosity ratio and the UV continuum slope β that other starburst galaxies follow. To understand the reason for the deviation, we leverage the high angular resolution of archival near-UV-to-near-IR Hubble Space Telescope images to divide the ring into ∼60–180 pc size regions and model each individually. We find that the UV slope of the combined intrinsic (dust-free) stellar populations in the central region is redder than what is expected for a young model population. This is due to the region’s complex star formation history, which boosts the near-UV emission relative to the far-UV. The resulting net attenuation curve has a UV slope that lies between those of the starburst attenuation curve (Calzetti et al. 2000) and the Small Magellanic Cloud extinction curve; the total-to-selective attenuation value,

R
′

(V) = 4.93, is larger than both. As found for other star-forming galaxies, the stellar continuum of NGC 3351 is less attenuated than the ionized gas, with E(B − V)star = 0.40 E(B − V)gas. The combination of the “red” intrinsic stellar population and the new attenuation curve fully accounts for the location of the central region of NGC 3351 on the IRX–β diagram. Thus, the observed characteristics result from the complex mixture of stellar populations and dust column densities in the circumnuclear region. Despite being a sample of one, these findings highlight the difficulty of defining attenuation curves of general applicability outside the regime of centrally concentrated starbursts.
The Mass and Age Distribution of Halo White Dwarfs in the Canada–France Imaging Survey
Authors: Fantin Nicholas J. , Côté Patrick , McConnachie Alan W. , Bergeron Pierre , Cuillandre Jean-Charles , Dufour Patrick , Gwyn Stephen D. J. , Ibata Rodrigo A. , Thomas Guillaume F. 
Published: May 2021

Abstract
We present optical spectroscopy for 18 halo white dwarfs identified using photometry from the Canada–France Imaging Survey and Pan-STARRS1 DR1 3π survey combined with astrometry from Gaia DR2. The sample contains 13 DA, 1 DZ, 2 DC, and 2 potentially exotic types of white dwarf. We fit both the spectrum and the spectral energy distribution in order to obtain the temperature and surface gravity, which we then convert into mass and then age using stellar isochrones and the initial-to-final mass relation. We find a large spread in ages that is not consistent with expected formation scenarios for the Galactic halo. We find a mean age of

9.03

−
2.03

+
2.13

Gyr and a dispersion of

4.21

−
1.58

+
2.33

Gyr for the inner halo using a maximum-likelihood method. This result suggests an extended star formation history within the local halo population.
Magnetic Fields in Massive Star-forming Regions (MagMaR). I. Linear Polarized Imaging of the Ultracompact H ii Region G5.89–0.39
Authors: Fernández-López M. , Sanhueza P. , Zapata L. A. , Stephens I. , Hull C. , Zhang Q. , Girart J. M. , Koch P. M. , Cortés P. , Silva A. , Tatematsu K. , Nakamura F. , Guzmán A. E. , Nguyen Luong Q. , Guzmán Ccolque E. , Tang Y.-W. , Chen H.-R. V. 
Published: May 2021

Abstract
We report 1.2 mm polarized continuum emission observations carried out with the Atacama Large Millimeter/submillimeter Array toward the high-mass star formation region G5.89–0.39. The observations show a prominent 0.2 pc north–south filamentary structure. The ultracompact H ii region in G5.89–0.39 breaks the filament into two pieces. Its millimeter emission shows a dusty belt with a mass of 55–115 M
⊙ and 4500 au in radius, surrounding an inner part comprising mostly ionized gas, with dust emission only accounting for about 30% of the total millimeter emission. We also found a lattice of convex arches that may be produced by dragged dust and gas from the explosive dispersal event involving the O5 Feldt’s star. The north–south filament has a mass between 300 and 600 M
⊙ and harbors a cluster of about 20 mm envelopes with a median size and mass of 1700 au and 1.5 M
⊙, respectively, some of which are already forming protostars. We interpret the polarized emission in the filament as mainly coming from magnetically aligned dust grains. The polarization fraction is ∼4.4% in the filaments and 2.1% at the shell. The magnetic fields are along the North Filament and perpendicular to the South Filament. In the Central Shell, the magnetic fields are roughly radial in a ring surrounding the dusty belt between 4500 and 7500 au, similar to the pattern recently found in the surroundings of Orion BN/KL. This may be an independent observational signpost of explosive dispersal outflows and should be further investigated in other regions.
The Reconstruction of Dark Energy with the Ridge Regression Approach
Authors: Huang Long , Yang Xiaofeng , Liu Xiang 
Published: May 2021

Abstract
Whether or not dark energy evolves with time may be determined by the nonparametric method. In order to avoid instability of the derivative for the functional data, we linearize the luminosity-distance integral formula in near-flat space by adopting Lagrange interpolation for the numerical integral, and proposing a method of combining principal component analysis (PCA) and biased estimation on the basis of ridge regression analysis to reconstruct the regression parameters. We also present a principal component selection criterion to better distinguish between ΛCDM and w(z) ≠ −1 models by reconstruction. We define the type I error as the situation where w
true = −1 but w
recon ≠ −1, and the type II error as the situation where w
true ≠ −1 but w
recon = −1; we use the various w(z) functions to test the method. The preliminary test results demonstrate that the PCA-biased method can be used to determine the most probable behavior of w(z). Finally, we apply this method to recent supernova measurements, reconstructing the continuous history of w(z) out to redshift z = 1.5.
Chemical Tagging N-rich Field Stars with High-resolution Spectroscopy
Authors: Yu Jincheng , Tang Baitian , Fernández-Trincado José G. , Geisler Douglas , Yan Hongliang , Soto M. 
Published: May 2021

Abstract
We measure chemical abundances for over 20 elements of 15 N-rich field stars with high-resolution (R ∼ 30,000) optical spectra. We find that Na, Mg, Al, Si, and Ca abundances of our N-rich field stars are mostly consistent with those of stars from globular clusters (GCs). Seven stars are estimated to have [Al/Fe ] > 0.5, which is not found in most GC “first generation” stars. On the other hand, α element abundances (especially Ti) could show distinguishable differences between in situ stars and accreted stars. We discover that one interesting star, with consistently low [Mg/Fe], [Si/Fe], [Ca/Fe], [Ti/Fe], [Sc/Fe], [V/Fe], and [Co/Fe], show similar kinematics and [Ba/Eu] as other stars from the dissolved dwarf galaxy “Gaia–Sausage–Enceladus.” The α-element abundances and the iron-peak element abundances of the N-rich field stars with metallicities − 1.25 ≤ [Fe/H] ≤ − 0.95 show consistent values with Milky Way field stars (we refer to Milky Way field stars as Milky Way halo field stars unless otherwise specified in this paper) rather than stars from dwarf galaxies, indicating that they were formed in situ. In addition, the neutron-capture elements of N-rich field stars show that most of them could be enriched by asymptotic giant branch stars with masses around 3–5 M
⊙.