cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Runaway electron deconfinement in SPARC and DIII-D by a passive 3D coil
Creators: name: Izzo, V. A.
name: Pusztai, I.
name: Särkimäki, K.
name: Sundström, A.
name: Garnier, D.
name: Weisberg, D.
name: Tinguely, R. A.
name: Paz-Soldan, C.
name: Granetz, R. S.
name: Sweeney, R.
Publisher: name: arXiv
Year: 2022
Subjects: subject: Plasma Physics (physics.plasm-ph)
subject: FOS: Physical sciences

description: The operation of a 3D coil--passively driven by the current quench loop voltage--for the deconfinement of runaway electrons is modeled for disruption scenarios in the SPARC and DIII-D tokamaks. Nonlinear MHD modeling is carried out with the NIMROD code including time-dependent magnetic field boundary conditions to simulate the effect of the coil. Further modeling in some cases uses the ASCOT5 code to calculate advection and diffusion coefficients for runaway electrons based on the NIMROD-calculated fields, and the DREAM code to compute the runaway evolution in the presence of these transport coefficients. Compared with similar modeling in Tinguely, et al [2021 Nucl. Fusion 61 124003], considerably more conservative assumptions are made with the ASCOT5 results, zeroing low levels of transport, particularly in regions in which closed flux surfaces have reformed. Of three coil geometries considered in SPARC, only the $n=1$ coil is found to have sufficient resonant components to suppress the runaway current growth. Without the new conservative transport assumptions, full suppression of the RE current is maintained when the TQ MHD is included in the simulation or when the RE current is limited to 250kA, but when transport in closed flux regions is fully suppressed, these scenarios allow RE beams on the order of 1-2MA to appear. Additional modeling is performed to consider the effects of the close ideal wall. In DIII-D, the current quench is modeled for both limited and diverted equilibrium shapes. In the limited shape, the onset of stochasticity is found to be insensitive to the coil current amplitude and governed largely by the evolution of the safety-factor profile. In both devices, prediction of the q-profile evolution is seen to be critical to predicting the later time effects of the coil.
Diffusion in the presence of a chiral topological defect
Creators: name: Manapany, Andy
name: Moueddene, Leila
name: Berche, Bertrand
name: Fumeron, Sébastien
Publisher: name: arXiv
Year: 2022
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: We study the diffusion processes of a real scalar field in the presence of the distorsion field induced by a chiral topological defect. The defect modifies the usual Euclidean background geometry into a non-diagonal Riemann-Cartan geometry characterized by a singular torsion field. The new form of the diffusion equation is established and the scalar field distribution in the vicinity of the defect is investigated numerically. Results show a high sensitivity to the boundary conditions. In the transient regime, we find that the defect vorticity generates an angular momentum associated to the diffusion flow and we discuss its main properties.
Additional file 1 of Histone deacetylase III interactions with BK polyomavirus large tumor antigen may affect protein stability
Creators: name: Hsu, Yueh-Han
name: Chao, Chun-Nun
name: Huang, Hsin-Yi
name: Zhao, Pei-Wen
name: Hsu, Pang-Hung
name: Shen, Cheng-Huang
name: Chen, San-Yuan
name: Fang, Chiung-Yao
Publisher: name: figshare
Year: 2023
Subjects: subject: Biochemistry
subject: Medicine
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
classificationCode: 69999
subject: Biological Sciences not elsewhere classified
subject: Cancer

description: Supplementary Material 1
РАСЧЕТ СИСТЕМЫ ВОДОСНАБЖЕНИЯ И ВОДООТВЕДЕНИЯ ЗДАНИЯ КОМБИНАТА БЫТОВОГО ОБСЛУЖИВАНИЯ
Creators: name: САФРОНОВА ТАТЬЯНА ИВАНОВНА
name: СВЕТЛИЦКАЯ ВАЛЕРИЯ ЕВГЕНЬЕВНА
Publisher: name: StudNet
Year: 2020
Subjects: СИСТЕМЫ ВОДОСНАБЖЕНИЯ И ВОДООТВЕДЕНИЯ
ВОДОЗАБОРНАЯ СКВАЖИНА
УРОВЕНЬ ВОДЫ
ПОЛИЭТИЛЕНОВЫЕ ТРУБЫ
WATER SUPPLY AND SANITATION SYSTEMS
WATER WELL
WATER LEVEL
POLYETHYLENE PIPES

description: В статье приведен расчет водопотребления и водоотведения здания комбината бытового обслуживания пос. Ильского Северского района Краснодарского края. Использование современного оборудования и материалов во многом улучшает работу сетей водоснабжения и водоотведения, увеличивает срок службы сетей и оборудования и уменьшает их стоимость. Применение запроектированных труб позволит увеличить срок эксплуатации сети водоснабжения и водоотведения, а также уменьшить затраты на материалы и стоимость монтажа.The article presents the calculation of water consumption and water disposal of the building of the consumer services plant in the village. Ilsky Seversky district of Krasnodar territory. The use of modern equipment and materials greatly improves the operation of water supply and sanitation networks, increases the service life of networks and equipment and reduces their cost. The use of designed pipes will increase the service life of the water supply and sanitation network, as well as reduce the cost of materials and installation costs.
СИСТЕМЫ ДИСТАНЦИОННОГО ОБУЧЕНИЯ КАК ИНСТРУМЕНТ ПРЕДАТТЕСТАЦИОННОЙ ПОДГОТОВКИ ПРОИЗВОДСТВЕННОГО ПЕРСОНАЛА
Creators: name: МОЛЯРЕНКО АНДРЕЙ АНДРЕЕВИЧ
Publisher: name: StudNet
Year: 2020
Subjects: ЭЛЕКТРОЭНЕРГЕТИКА
ОХРАНА ТРУДА
РАБОТА С ПЕРСОНАЛОМ
ОБУЧЕНИЕ ПЕРСОНАЛА
ДИСТАНЦИОННОЕ ОБУЧЕНИЕ
ELECTRIC POWER INDUSTRY
LABOR PROTECTION
PERSONNEL MANAGEMENT
PERSONNEL TRAINING
DISTANCE LEARNING

description: В статье рассматривается вопрос автоматизации предаттестационной подготовки производственного персонала. Проблематика консервативных подходов к подготовке персонала в электроэнергетике. Острая необходимость в новых технологичных решениях для обеспечения доступа к актуальной информации. Системы дистанционного обучения как инструмент автоматизации процесса обучения, а также методика построения автоматизированного курса дистанционного обучения. Общее описание расходов на реализацию проекта по автоматизированной предаттестационной подготовке.The article deals with the issue of automation of pre-certification training of production personnel. Problems of generally accepted approaches to personnel training in the electric power industry. There is an urgent need for new technological solutions to ensure access to up-to-date information. Distance learning systems as a tool for automating the learning process, as well as methods for building a distance learning course. General description of the project implementation costs for automated pre-certification training.
Analytically Approximation Solution to Einstein-Cubic Gravity
Creators: name: Sajadi, S. N.
name: Hendi, S. H.
Publisher: name: arXiv
Year: 2022
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: In this work, we introduce an analytical approximate black hole solution in Einstein-Cubic gravity. To obtain complete solutions, we construct the near horizon and asymptotic solutions as the first step. Then, the approximate analytic solutions are obtained through continued fraction expansion. We also compute the thermodynamic quantities and use the first law and Smarr formula to obtain the analytic solutions for the near horizon quantities. Finally, we follow the same approach to obtain the new static black hole solutions with different metric functions.
description: 22 pages, 12 Figures, accepted in EPJC
Variations of $P_2$ in subpulse drifting pulsars
Creators: name: Yuen, R.
name: Melrose, D. B.
name: Samsuddin, M. A.
name: Tu, Z. Y.
name: Han, X. H.
Publisher: name: arXiv
Year: 2016
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: We develop a model for subpulse separation period, $P_2$, taking into account both the apparent motion of the visible point as a function of pulsar phase, $ψ$, and the possibility of abrupt jumps between different rotation states in non-corotating pulsar magnetospheres. We identify three frequencies: (i) the spin frequency of the star, (ii) the drift frequency of the magnetospheric plasma in the source region, and (iii) the angular frequency of the visible point around its trajectory. We show how the last of these, which is neglected in traditional models by implicitly assuming the line of sight through the center of the star, affects the interpretation of $P_2$. We attribute the subpulse structure to emission from $m$ anti-nodes distributed uniformly in azimuthal angle about the magnetic axis. We show that variations of $P_2$ as a function of rotational phase or observing frequency arise naturally when the motion of the visible point is taken into account. We discuss possible application of our model in signifying overall field-line distortion at the emitting region. Abrupt changes in $P_2$ can occur during state switching in the magnetosphere. We demonstrate that the unique value of $P_2$ in each rotation state can be used, in principle, to relate the rotation state of the magnetospheres to subpulse drifting.
description: Accepted for publication in MNRAS
САХАРНЫЙ ДИАБЕТ: ТЕХНИКА ИНЪЕКЦИЙ, САМОКОНТРОЛЬ И КАЧЕСТВО ЖИЗНИ ПАЦИЕНТОВ
Creators: name: АНКУШИНА КСЕНИЯ ДМИТРИЕВНА
name: КАРПОВА АЛЕНА ОЛЕГОВНА
Publisher: name: StudNet
Year: 2020
Subjects: САХАРНЫЙ ДИАБЕТ
ТЕХНИКА ИНЪЕКЦИЙ
САМОКОНТРОЛЬ
ИНЪЕКЦИИ ИНСУЛИНА
ЭФФЕКТИВНОСТЬ ЛЕЧЕНИЯ
УДОВЛЕТВОРЕННОСТЬ ЛЕЧЕНИЕМ
КАЧЕСТВО ЖИЗНИ
DIABETES
INJECTION TECHNIQUE
SELF-CONTROL
INSULIN INJECTION
TREATMENT EFFICACY
SATISFACTION WITH TREATMENT
QUALITY OF LIFE

description: В статье рассмотрены вопросы осведомленности о своем заболевании пациентов с сахарным диабетом 1 и 2 типа, о правильности лечения и постановке инъекций. Чтобы оценить осведомленность о заболевании, пациентам эндокринологического отделения одной из больниц г. Кирова было предложено ответить на вопросы анкеты о правильности хранения инсулина, о технике инъекций и самоконтроле уровня глюкозы. В ходе исследования были выявлены различия отношения к своему заболеванию между пациентами 1 и 2 типа сахарного диабета. Частые посещения врача, ежедневные инъекции, стационарное лечение, ограничение в пище и другие строгие правила поддержания здоровья значительно снижают удовлетворенность жизнью пациентов с сахарным диабетом. При помощи соц-демографической анкеты ADDQoL и опросника DTSQ, проведенных среди пациентов эндокринологического отделения одной из больниц г.Кирова были выявлены показатели удовлетворенности лечением и качеством жизни пациентов с сахарным диабетом 1 и 2 типов.The article deals with the issues of awareness of patients with diabetes mellitus type 1 and type 2 about their disease, in particular, about the correctness of treatment and the setting of injections. In order to assess the awareness of the disease, the patients of the endocrinology department of one of the hospitals in Kirov were asked to answer questions from the questionnaire about the proper storage of insulin, the injection technique, and self-monitoring of glucose levels. During the study, differences in attitudes towards their disease between patients with type 1 and type 2 diabetes were identified. Frequent visits to the doctor, daily injections, inpatient treatment, restriction of food and other strict rules of maintaining health significantly reduce satisfaction with the life of patients with diabetes. Using the social-demographic questionnaire ADDQoL and questionnaire DTSQ, conducted among patients of the endocrinological department of a hospital in Kirov, indicators of satisfaction with treatment and quality of life of patients with type 1 and type 2 diabetes were identified.
МЕТОДИКА УПРАВЛЕНИЯ МАСТЕР-ДАННЫМИ ПРИ ВНЕДРЕНИИ УЧЕТНОЙ СИСТЕМЫ В СЛОЖНОМ ИНТЕГРАЦИОННОМ ИТ-ЛАНДШАФТЕ
Creators: name: СУХАНОВА ДАРЬЯ АЛЕКСАНДРОВНА
name: ДАНИЛОВ БАИР СЕРГЕЕВИЧ
Publisher: name: StudNet
Year: 2020
Subjects: МАСТЕР-ДАННЫЕ
ОСНОВНЫЕ ДАННЫЕ
НОРМАТИВНО-СПРАВОЧНАЯ ИНФОРМАЦИЯ
УЧЕТНАЯ СИСТЕМА
РЕЕСТР ЭКЗЕМПЛЯРОВ ОБЪЕКТОВ НОРМАТИВНО-СПРАВОЧНОЙ ИНФОРМАЦИИ
МЕТОДИКА УПРАВЛЕНИЯ МАСТЕР-ДАННЫМИ
MASTER DATA
REFERENCE INFORMATION
ACCOUNTING SYSTEM
REGISTRY OF INSTANCES OF REFERENCE INFORMATION
MASTER DATA MANAGEMENT TECHNIQUE

description: Статья посвящена разработке методики управления мастер-данными при внедрении учетной системы. В статье рассматривается необходимость обособления единой среды управления мастер-данными, в которой связи работ и документов реализуются на инструментальном уровне, а технологии работы с данными унифицируются, что позволяет повысить эффективность процессов управления данными, сократить количество передач управления и ответственности между функциональными направлениями путем максимального сосредоточения функций этого процесса в «одних руках», а именно в руках группы НСИ, которая имеет детальный план работ, собственный бюджет и систему маршрутизации для всех функциональных направлений.The article is devoted to the development of master data management techniques. The article discusses the need to isolate a single master data management environment in which work and document communications are implemented at the instrumental level, and data processing technologies are unified, which allows to increase the efficiency of data management processes, reduce the number of control transfers and responsibilities between functional areas by maximizing concentration The functions of this process are in the same hands, namely, in the hands of the NSI group, which has a detailed work plan, its own budget and a routing system for all functional areas.
Additional file 1 of New medicines for spontaneous preterm birth prevention and preterm labour management: landscape analysis of the medicine development pipeline
Creators: name: McDougall, Annie R. A.
name: Hastie, Roxanne
name: Goldstein, Maya
name: Tuttle, Andrew
name: Ammerdorffer, Anne
name: Gülmezoglu, A. Metin
name: Vogel, Joshua P.
Publisher: name: figshare
Year: 2023
Subjects: subject: Medicine
subject: Cell Biology
subject: Neuroscience
subject: Pharmacology
subject: Biotechnology
subject: Developmental Biology
subject: Cancer
subject: Science Policy
classificationCode: 111714
subject: Mental Health
subject: Hematology

description: Additional file 1: Appendix A. Supplementary tables. Table S1. Scoring of target product profile comparison, for quantification of potential of candidates. Table S2. Threshold for ranking of potential at each phase of the R&D development pipeline.
Convergence of many-body wavefunction expansions using a plane wave basis in the thermodynamic limit
Creators: name: Shepherd, James J.
Publisher: name: arXiv
Year: 2016
Subjects: subject: Chemical Physics (physics.chem-ph)
subject: FOS: Physical sciences

description: Basis set incompleteness error and finite size error can manifest concurrently in systems for which the two effects are phenomenologically well-separated in length scale. When this is true, we need not necessarily remove the two sources of error simultaneously. Instead, the errors can be found and remedied in different parts of the basis set. This would be of great benefit to a method such as coupled cluster theory since the combined cost of $n_{occ}^6 n_{virt}^4$ could be separated into $n_{occ}^6$ and $n_{virt}^4$ costs with smaller prefactors. In this Communication, we present analysis on a data set due to Baardsen and coworkers, containing coupled cluster doubles energies for the 2DEG for $r_s=$ 0.5, 1.0 and 2.0 a.u.~at a wide range of basis set sizes and particle numbers. In obtaining complete basis set limit thermodynamic limit results, we find that within a small and removable error the above assertion is correct for this simple system. This approach allows for the combination of methods which separately address finite size effects and basis set incompleteness error.
description: Submitted to JCP as a Communication. Questions and comments welcome. Data set will be published elsewhere
Photohadronic interpretation of the different incarnation of 1ES 2344+514
Creators: name: Sahu, Sarira
name: Polanco, Isabel Abigail Valadez
name: Rajpoot, Subhash
Publisher: name: arXiv
Year: 2022
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: Since its discovery in 1995, the high-energy peaked blazar 1ES 2344+514 has undergone several episodes of GeV-TeV flaring and has been observed in the multiwavelength by several other telescopes. The observed X-ray spectrum of 1996 and the flaring event of 2016 establish that 1ES 2344+514 has a temporary EHBL-like behavior. Such behavior has also been observed in several nearby high-energy peaked blazars. We use the photohadronic model to account for the GeV-TeV flaring observed events of 1995 and 2007. Also, a recently proposed two-zone photohadronic model, which is successful in explaining the multi-TeV flaring events of many transient EHBL-like source, is employed to explain the GeV-TeV flaring spectra of MJD 57611 and MJD 57612. We find that the zone-2 parameters of the two-zone photohadronic model play a central role in explaining these spectra. Probably this is an indication of a new type of transient EHBL-like source. We find that our fits to the observed spectra are comparable or better than the other leptonic and hadronic models employed in the literature to address the same issue.
description: 12 pages, 4 figures, to be published in MNRAS
Cosmic Acceleration and Geodesic Deviation in Chameleon Scalar Field Model
Creators: name: Zaregonbadi, Raziyeh
name: Saba, Nasim
name: Farhoudi, Mehrdad
Publisher: name: arXiv
Year: 2022
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: While considering the chameleon scalar field model with the spatially flat FLRW background, we investigate the late-time acceleration phase of the universe, wherein we apply the typical potential usually used in this model. Through setting some constraints on the free parameters of the model, we indicate that the non-minimal coupling between the matter and the scalar field in such a model should be strongly coupled in order to have an accelerated expansion of the universe at the late-time. We also investigate the relative acceleration of the parallel geodesics by obtaining the geodesic deviation equation in the context of chameleon model. Then, through the null deviation vector fields, we obtain the observer area-distance as a measurable quantity to compare the model with other relevant models.
description: 12 pages, 4 figures
Functional and phenotypic studies of the pulmonary alveolar macrophage in lung cancer
Creators: name: McDonald., Dr. Christine F.
Publisher: name: Monash University
Year: 2021

description: This thesis was scanned from the print manuscript for digital preservation and is copyright the author.
 Researchers can access this thesis by asking their local university, institution or public library to
 make a request on their behalf. Monash staff and postgraduate students can use the link in the References field.
MPEC 2024-R48 : 2024 RD1
Creators: name: Minor Planet Center Staff
Publisher: name: The Minor Planet Center
Year: 2024
Subjects: subject: Small Solar System bodies
valueUri: http://astrothesaurus.org/uat/1469
subject: 2024 RD1

description: The Minor Planet Electronic Circulars contain information on unusual minor planets, routine data on comets and natural satellites, and occasional editorial announcements.  They are published on behalf of Division F of the International Astronomical Union by the Minor Planet Center, Smithsonian Astrophysical Observatory, Cambridge, MA 02138, U.S.A.
ИЗНОС КАНАЛА СТВОЛА И ПОВЫШЕНИЕ ЭФФЕКТИВНОСТИ ФУНКЦИОНИРОВАНИЯ ИМПУЛЬСНЫХ ТЕПЛОВЫХ МАШИН
Creators: name: МИТРОХИН ОЛЕГ ВИКТОРОВИЧ
name: БАБАЕВ ДЖАМИЛЬ ДЖОНИЕВИЧ
Publisher: name: StudNet
Year: 2020
Subjects: СТВОЛ АРТИЛЛЕРИЙСКОГО ОРУДИЯ
ТРИБОТЕХНИЧЕСКИЙ СОСТАВ
НАПРАВЛЕННАЯ ИОННАЯ ДИФФУЗИЯ
УСЛОВИЯ ЭКСПЛУАТАЦИИ
ЖИВУЧЕСТЬ СТВОЛА
ARTILLERY GUN BARREL
TRIBOLOGICAL COMPOSITION
DIRECTIONAL ION DIFFUSION
OPERATING CONDITIONS
BARREL SURVIVABILITY

description: В статье рассмотрены перспективные тактика применения и характеристики импульсных тепловых машин, условия и механизм износа канала ствола, его влияние на эффективность стрельбы, способы его учета при стрельбе для повышения эффективности боевого применения импульсных тепловых машин, способы борьбы с уменьшением баллистических параметров стрельбы и увеличением рассеивания снарядов.The article discusses the promising tactics of application and characteristics of pulsed heat engines, the conditions and mechanism of wear of the barrel channel, its effect on firing efficiency, ways of taking it into account when firing to increase the effectiveness of combat use of pulsed heat engines, ways to combat the reduction of ballistic parameters of firing and an increase in the dispersion of shells.
Performance Assessment of the KASI-Deep Rolling Imaging Fast-optics Telescope pathfinder
Creators: name: Byun, Woowon
name: Ko, Jongwan
name: Kim, Yunjong
name: Seon, Kwang-Il
name: Chang, Seunghyuk
name: Kim, Dohoon
name: Choi, Changsu
name: Chun, Sang-Hyun
name: Jeon, Young-Beom
name: Kim, Jae-Woo
name: Lee, Chung-Uk
name: Lee, Yongseok
name: Park, Hong Soo
name: Sung, Eon-Chang
name: Yoo, Jaewon
name: Lee, Gayoung
name: Lee, Hyoungkwon
Publisher: name: arXiv
Year: 2022
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: Instrumentation and Methods for Astrophysics (astro-ph.IM)
subject: FOS: Physical sciences

description: In a $Λ$CDM universe, most galaxies evolve by mergers and accretions, leaving faint and/or diffuse structures, such as tidal streams and stellar halos. Although these structures are a good indicator of galaxies' recent mass assembly history, they have the disadvantage of being difficult to observe due to their low surface brightness (LSB). To recover these LSB features by minimizing the photometric uncertainties introduced by the optical system, we developed a new optimized telescope named K-DRIFT pathfinder, adopting a linear astigmatism free-three mirror system. Thanks to the off-axis design, it is expected to avoid the loss and scattering of light on the optical path within the telescope. To assess the performance of this prototype telescope, we investigate the photometric depth and capability to identify LSB features. We find that the surface brightness limit reaches down to $μ_{r,1σ}\sim28.5$ mag arcsec$^{-2}$ in $10^{\prime\prime}\times10^{\prime\prime}$ boxes, enabling us to identify a single stellar stream to the east of NGC 5907. We also examine the characteristics of the point spread function (PSF) and find that the PSF wing reaches a very low level. Still, however, some internal reflections appear within a radius of $\sim$6 arcmin from the center of sources. Despite a relatively small aperture (0.3 m) and short integration time (2 hr), this result demonstrates that our telescope is highly efficient in LSB detection.
description: 15 pages, 8 figures, accepted for publication in PASP
Low Spin-Axis Variations of Circumbinary Planets
Creators: name: Chen, Renyi
name: Li, Gongjie
name: Tao, Molei
Publisher: name: arXiv
Year: 2022
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: FOS: Physical sciences

description: Having a massive moon has been considered as a primary mechanism for stabilized planetary obliquity, an example of which being our Earth. This is, however, not always consistent with the exoplanetary cases. This article details the discovery of an alternative mechanism, namely that planets orbiting around binary stars tend to have low spin-axis variations. This is because the large quadrupole potential of the stellar binary could speed up the planetary orbital precession, and detune the system out of secular spin-orbit resonances. Consequently, habitable zone planets around the stellar binaries in low inclination orbits hold higher potential for regular seasonal changes comparing to their single star analogues.
description: 21 pages, 15 figures Accepted for publication in MNRAS
Kinematically Identified Recoiling Supermassive Black Hole Candidates in SDSS QSOs with z $
Creators: name: Kim, D. -C.
name: Evans, A. S.
name: Stierwalt, S.
name: Privon, G. C.
Publisher: name: arXiv
Year: 2016
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We have performed a spectral decomposition to search for recoiling supermassive black holes (rSMBH) in the SDSS QSOs with $z<0.25$. Out of 1271 QSOs, we have identified 26 rSMBH candidates that are recoiling toward us. The projected recoil velocities range from $-76\ \kms$ to $-307\ \kms$ with a mean of $-149\pm58\ \kms$. Most of the rSMBH candidates are hosted by gas-rich LIRGs/ULIRGs, but only 23\% of them shows signs of tidal features suggesting majority of them are advanced mergers. We find that the black hole masses $M_{BH}$ of the rSMBH candidates are on average $\sim$5 times smaller than that of their stationary counterparts and cause a scatter in $M_{BH}-σ_*$ relation. The Eddington ratios of all of the rSMBH candidates are larger than 0.1, with mean of 0.52$\pm$0.27, suggesting they are actively accreting mass. Velocity shifts in high-excitation coronal lines suggest that the rSMBH candidates are recoiling with an average velocity of about $-265\ \kms$. Electron density in the narrow line region of the H II rSMBH candidates is about 1/10 of that in AGN rSMBH candidates probably because AGN in the former was more spatially offset than that in the latter. The estimated spatial offsets between the rSMBH candidate and center of host galaxy range from 0.21\as \ to 1.97\as \ and need to be confirmed spatially with high-resolution adaptive optics imaging observations.
description: ApJ accepted
Additional file 2 of New medicines for spontaneous preterm birth prevention and preterm labour management: landscape analysis of the medicine development pipeline
Creators: name: McDougall, Annie R. A.
name: Hastie, Roxanne
name: Goldstein, Maya
name: Tuttle, Andrew
name: Ammerdorffer, Anne
name: Gülmezoglu, A. Metin
name: Vogel, Joshua P.
Publisher: name: figshare
Year: 2023
Subjects: subject: Medicine
subject: Cell Biology
subject: Neuroscience
subject: Pharmacology
subject: Biotechnology
subject: Developmental Biology
subject: Cancer
subject: Science Policy
classificationCode: 111714
subject: Mental Health
subject: Hematology

description: Additional file 2: Appendix B. Low rank candidates.
МОДЕРНИЗАЦИЯ СХЕМЫ С ДВУМЯ СИСТЕМАМИ СБОРНЫХ ШИН И С ОБХОДНОЙ СИСТЕМОЙ ШИН
Creators: name: ШИРОКОВ ИВАН СЕРГЕЕВИЧ
Publisher: name: StudNet
Year: 2020
Subjects: ОТКРЫТОЕ РАСПРЕДЕЛИТЕЛЬНОЕ УСТРОЙСТВО
ЭЛЕКТРИЧЕСКАЯ ЭНЕРГИЯ
АВТОТРАНСФОРМАТОР
СИСТЕМА СБОРНЫХ ШИН
МАТЕМАТИЧЕСКОЕ ОЖИДАНИЕ
OPEN SWITCHGEAR
ELECTRIC ENERGY
AUTOTRANSFORMER
EXPECTED VALUE

description: В статье рассматриваются пути снижения числа аварий в энергетической системе и годового недоотпуска электроэнергии в результате аварий. Для решения проблем с перерывами в подаче электроэнергии требуется рассматривать каждый элемент энергосистемы в отдельности. Необходимо производить оценку надёжности отдельных видов оборудования и установок, искать пути повышения надёжности, как в ходе эксплуатации, так и при проектировании. В качестве примера выполняется оценка надёжности открытого распределительного устройства (ОРУ) напряжением 110 кВ подстанции «Котельнич», которое относится к Западным электрическим сетям филиала «Кировэнерго» ПАО «МРСК Центра и Приволжья».The article discusses ways to reduce the number of accidents in the energy system and annual undersupply of electricity as a result of accidents. To solve problems with interruptions in the supply of electricity, it is required to consider each element of the power system separately. It is necessary to assess the reliability of certain types of equipment and installations, to look for ways to increase reliability, both during operation and during design. As an example, the reliability assessment of an open switchgear with a voltage of 110 kV of the substation "Kotelnich", Kirov region.
Tracking the ice mantle history in the Solar-type Protostars of NGC 1333 IRAS 4
Creators: name: De Simone, Marta
name: Ceccarelli, Cecilia
name: Codella, Claudio
name: Svoboda, Brian E.
name: Chandler, Claire J.
name: Bouvier, Mathilde
name: Yamamoto, Satoshi
name: Sakai, Nami
name: Yang, Yao-Lun
name: Caselli, Paola
name: Lefloch, Bertrand
name: Liu, Hauyu Baobab
name: López-Sepulcre, Ana
name: Loinard, Laurent
name: Pineda, Jaime E.
name: Testi, Leonardo
Publisher: name: arXiv
Year: 2022
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: To understand the origin of the diversity observed in exoplanetary systems, it is crucial to characterize the early stages of their formation, represented by Solar-type protostars. Likely, the gaseous chemical content of these objects directly depends on the composition of the dust grain mantles formed before the collapse. Directly retrieving the ice mantle composition is challenging, but it can be done indirectly by observing the major components, such as NH3 and CH3OH at cm wavelengths, once they are released into the gas-phase during the warm protostellar stage. We observed several CH3OH and NH3 lines toward three Class 0 protostars in NGC1333 (IRAS 4A1, IRAS 4A2, and IRAS 4B), at high angular resolution (1"; ~300 au) with the VLA interferometer at 24-26 GHz. Using a non-LTE LVG analysis, we derived a similar NH3/CH3OH abundance ratio in the three protostars (<0.5, 0.015-0.5, and 0.003-0.3 for IRAS 4A1, 4A2, and 4B, respectively). Hence, we infer they were born from pre-collapse material with similar physical conditions. Comparing the observed abundance ratios with astrochemical model predictions, we constrained the dust temperature at the time of the mantle formation to be ~17 K, which coincides with the average temperature of the southern NGC 1333 diffuse cloud. We suggest that a brutal event started the collapse that eventually formed IRAS 4A1, 4A2 and 4B, which,therefore, did not experience the usual pre-stellar core phase. This event could be the clash of a bubble with NGC 1333 south, that has previously been evoked in the literature.
description: accepted in ApJ Letters
Cluster-lensing: A Python Package for Galaxy Clusters & Miscentering
Creators: name: Ford, Jes
name: VanderPlas, Jake
Publisher: name: arXiv
Year: 2016
Subjects: subject: Instrumentation and Methods for Astrophysics (astro-ph.IM)
subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We describe a new open source package for calculating properties of galaxy clusters, including NFW halo profiles with and without the effects of cluster miscentering. This pure-Python package, cluster-lensing, provides well-documented and easy-to-use classes and functions for calculating cluster scaling relations, including mass-richness and mass-concentration relations from the literature, as well as the surface mass density $Σ(R)$ and differential surface mass density $ΔΣ(R)$ profiles, probed by weak lensing magnification and shear. Galaxy cluster miscentering is especially a concern for stacked weak lensing shear studies of galaxy clusters, where offsets between the assumed and the true underlying matter distribution can lead to a significant bias in the mass estimates if not accounted for. This software has been developed and released in a public GitHub repository, and is licensed under the permissive MIT license. The cluster-lensing package is archived on Zenodo (Ford 2016). Full documentation, source code, and installation instructions are available at http://jesford.github.io/cluster-lensing/.
description: 11 pages, 3 figures. Feedback on this paper is welcome here: http://jesford.github.io/paper-on-cluster-lensing/. Software documentation, installation instructions, and source code are here: http://jesford.github.io/cluster-lensing/
Role of angiotensin AT₂ receptor in stroke
Creators: name: McCarthy., Claudia
Publisher: name: Monash University
Year: 2021

description: This thesis was scanned from the print manuscript for digital preservation and is copyright the author.
 Researchers can access this thesis by asking their local university, institution or public library to
 make a request on their behalf. Monash staff and postgraduate students can use the link in the References field.
D2.9 Harmonization framework
Creators: name: Hernandez Palencia, Ignacio
name: Cabezas Rodríguez, José
name: Gimenez Celdran, Angel
name: Amodeo Gonzalez, Gustavo
Publisher: name: Zenodo
Year: 2023
Subjects: OODA
SWOT

description: WP2 provides the design, specifications, and requirements that need to be taken into account throughout the project life cycle. This includes an in-depth review of system requirements, out comes from consultations with stakeholders, and pre-standardization research. The Deliverable 2.9 Harmonization framework presents the results over the methodology for agile harmonization and standardization based in all information analysed. This deliverable is the second harmonization framework and represents the final framework at the end of the project. The harmonization and standardization process is a multidisciplinary process where cross-sectoral experts with heterogeneous knowledge shall contribute, providing support in multiple initiatives, such as literature identification, specific procedures (and their differences between regions/countries), evaluation and information exchange. This deliverable is an update of the previously submitted document D2.5 - Harmonization framework. The new content with respect to the last version submitted has been highlighted in yellow for easy review. This deliverable D2.9 "Harmonisation framework" expose the methodology followed in the project, the tasks elaborated to select the priorities and the pre-harmonisation in these points. Neither partial nor final results are shown. The results are part of the deliverable D2.12 “Harmonization and Standardization Reports”.
MIGHTEE-HI: Evolution of HI scaling relations of star-forming galaxies at $z<0.5$
Creators: name: Sinigaglia, Francesco
name: Rodighiero, Giulia
name: Elson, Ed
name: Vaccari, Mattia
name: Maddox, Natasha
name: Frank, Bradley S.
name: Jarvis, Matt J.
name: Oosterloo, Tom
name: Davé, Romeel
name: Salvato, Mara
name: Baes, Maarten
name: Bellstedt, Sabine
name: Bisigello, Laura
name: Collier, Jordan D.
name: Cook, Robin H. W.
name: Davies, Luke J. M.
name: Delhaize, Jacinta
name: Driver, Simon P.
name: Foster, Caroline
name: Kurapati, Sushma
name: Lagos, Claudia del P.
name: Lidman, Christopher
name: Piña, Pavel E. Mancera
name: Meyer, Martin J.
name: Mogotsi, K. Moses
name: Pan, Hengxing
name: Ponomareva, Anastasia A.
name: Prandoni, Isabella
name: Rajohnson, Sambatriniaina H. A.
name: Robotham, Aaron S. G.
name: Santos, Mario G.
name: Sekhar, Srikrishna
name: Spekkens, Kristine
name: Thorne, Jessica E.
name: van der Hulst, Jan M.
name: Wong, O. Ivy
Publisher: name: arXiv
Year: 2022
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: We present the first measurements of HI galaxy scaling relations from a blind survey at $z>0.15$. We perform spectral stacking of 9023 spectra of star-forming galaxies undetected in HI at $0.23
description: 12 pages, 5 figures. Accepted for publication in ApJ Letters on 30 July 2022
ПАНДЕМИЯ И НЕФТЯНОЙ РЫНОК. ЭКОНОМИЧЕСКИЕ И ПОЛИТИЧЕСКИЕ АСПЕКТЫ
Creators: name: АЛИКОВ АРТЕМ РУСТЕМОВИЧ
name: КАЗАНСКИЙ НИКИТА АЛЕКСЕЕВИЧ
name: КУЗЬМИНА НАТАЛИЯ ВИТАЛЬЕВНА
name: ШАХОВСКИЙ РОМАН АНАТОЛЬЕВИЧ
Publisher: name: StudNet
Year: 2020
Subjects: ПАНДЕМИЯ
НЕФТЯНОЙ РЫНОК
ОПЕК
БАНКОВСКАЯ СФЕРА
ЭКОНОМИЧЕСКИЙ КРИЗИС
PANDEMIC
OIL MARKET
OPEC
BANKING
ECONOMIC CRISIS

description: Целью данной статьи является анализ экономических событий, произошедших в конце 2019 начале 2020 годов, а именно разразившаяся пандемия Covid-19, а также внезапно возникшие проблемы с подписанием очередного договора ОПЕК+ которые оказали непосредственное серьезное влияние на экономики многих государств, и очень серьезно ударили по экономике России .В ходе исследования проведен анализ состояния отдельных секторов и элементов экономики России в настоящее время, и в динамике последних нескольких лет. Рассмотрены и проанализированы политические и экономические стороны обозначенной проблемы. Авторами сделаны выводы о влиянии недавней разрушительной пандемии и разрыва нефтяной сделки на некоторые, наиболее уязвимые и важные для экономического развития, сферы экономики, в том числе на банковскую. А также выдвинуты прогнозы о возможном развитии ситуации.The purpose of this article is to analyze the economic events that occurred in late 2019 early 2020, namely the outbreak of the Covid-19 pandemic, as well as sudden problems with the signing of the next OPEC + agreement that had a direct serious impact on the economies of many countries, and it hit very seriously on the Russian economy. The study analyzes the state of individual sectors and elements of the Russian economy at present, and in the dynamics of the past few years. The political and economic aspects of the indicated problem are considered and analyzed. The authors draw conclusions about the impact of the recent devastating pandemic and the breakdown of the oil deal on some of the most vulnerable and important sectors of the economy for economic development, including banking. And also predictions about the possible development of the situation are put forward
Exponentially amplified magnetic field eliminates disk fragmentation around the Population III protostar
Creators: name: Hirano, Shingo
name: Machida, Masahiro N.
Publisher: name: arXiv
Year: 2022
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: One critical remaining issue to unclear the initial mass function of the first (Population III) stars is the final fate of secondary protostars formed in the accretion disk, specifically whether they merge or survive. We focus on the magnetic effects on the first star formation under the cosmological magnetic field. We perform a suite of ideal magnetohydrodynamic simulations until 1000 years after the first protostar formation. Instead of the sink particle technique, we employ a stiff equation of state approach to represent the magnetic field structure connecting to protostars. Ten years after the first protostar formation in the cloud initialized with $B_0 = 10^{-20}$ G at $n_0 = 10^4\,{\rm cm^{-3}}$, the magnetic field strength around protostars amplifies from pico- to kilo-gauss, which is the same strength as the present-day star. The magnetic field rapidly winds up since the gas in the vicinity of the protostar ($\leq\!10$ au) has undergone several tens orbital rotations in the first decade after protostar formation. As the mass accretion progresses, the vital magnetic field region extends outward, and the magnetic braking eliminates fragmentation of the disk that would form in the unmagnetized model. On the other hand, assuming a gas cloud with small angular momentum, this amplification might not work because the rotation would be slower. However, disk fragmentation would not occur in that case. We conclude that the exponential amplification of the cosmological magnetic field strength, about $10^{-18}$ G, eliminates disk fragmentation around the Population III protostars.
description: 9 pages, 5 figures, accepted for publication in ApJL
ИНТЕРНЕТ-ЭКОНОМИКА И ИНТЕРНЕТ-БИЗНЕС
Creators: name: КУШМАНОВА АЛЕКСАНДРА АНДРЕЕВНА
name: БАРБАШЕВА ОКСАНА ДМИТРИЕВНА
Publisher: name: StudNet
Year: 2020
Subjects: ИНТЕРНЕТ
БИЗНЕС
ТЕХНОЛОГИИ
ЭКОНОМИКА
ИНТЕРНЕТ-КОМПАНИИ
INTERNET
BUSINESS
TECHNOLOGY
ECONOMY
INTERNET COMPANIES

description: Интернет полностью охватил различные области: промышленность, транспорт, образование и другие. Появляются телекоммуникационные сети, которые помогают легко получить необходимую информацию. В настоящее время всё зависит от инноваций и компьютеризации. Компании, которые найдут применение новейшим информационным технологиям, получат различные преимущества в плане плодотворности и продуктивности удовлетворения желаний потребителей. В статье анализируется интернет-экономика и интернет-бизнес и то, насколько они важны, в современном мире. Также рассмотрены конкретные примеры видов бизнеса в интернете, и разобраны примеры успешных интернет-бизнесов. Авторами сделаны выводы о прибыльности электронного бизнеса. Также рассмотрены основные причины банкротства интернет компаний. Интернет является неотъемлемой частью нашей жизни, и поэтому тема интернет-экономики и интернет-бизнеса актуальна.The Internet has completely covered various areas: industry, transport, education, and others. Telecommunications networks are emerging that help you easily get the necessary information. At present, everything depends on innovation and computerization. Companies that use the latest information technologies will have various advantages in terms of productivity and satisfaction of consumers ' desires. The article analyzes the Internet economy and Internet business and how important they are in the modern world. Specific examples of Internet business types are also considered, and examples of successful Internet businesses are analyzed. The authors draw conclusions about the profitability of e-business. The main reasons for the bankruptcy of Internet companies are also considered. The Internet is an integral part of our life, and therefore the topic of the Internet economy and Internet business is relevant.
A light-curve analysis of the X-ray flash first observed in classical novae
Creators: name: Kato, Mariko
name: Saio, Hideyuki
name: Hachisu, Izumi
Publisher: name: arXiv
Year: 2022
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: An X-ray flash, expected in a very early phase of a nova outburst, was at last detected with the {\it SRG}/eROSITA in the classical nova YZ Reticuli 2020. The observed flash timescale, luminosity, and blackbody temperature substantially constrain the nova model. We present light curve models of the X-ray flash for various white dwarf (WD) masses and mass accretion rates. We have found the WD mass in YZ Ret to be as massive as $M_{\rm WD}\sim 1.3 ~M_\odot$ with mass accretion rates of $\dot M_{\rm acc}\sim 5 \times 10^{-10}- 5\times 10^{-9} ~M_\odot$ yr$^{-1}$ including the case that the mass accretion rate is changing between them, to be consistent with the {\it SRG}/eROSITA observation. The X-ray observation confirms the luminosity to be close to the Eddington limit at the X-ray flash. The occurrence of optically thick winds, with the photospheric radius exceeding $\sim 0.1~R_\odot$, terminated the X-ray flash of YZ Ret by strong absorption. This sets a constrain on the starting time of wind mass loss. A slight contamination of the core material into the hydrogen rich envelope seems to be preferred to explain a very short duration of the X-ray flash.
description: minor typos corrected: 8 pages, 1 table, 3 figures
Multiprocessor Scheduling of a Multi-mode Dataflow Graph Considering Mode Transition Delay
Creators: name: Jung, Hanwoong
name: Oh, Hyunok
name: Ha, Soonhoi
Publisher: name: arXiv
Year: 2016
Subjects: subject: Other Computer Science (cs.OH)
subject: FOS: Computer and information sciences

description: Synchronous Data Flow (SDF) model is widely used for specifying signal processing or streaming applications. Since modern embedded applications become more complex with dynamic behavior changes at run-time, several extensions of the SDF model have been proposed to specify the dynamic behavior changes while preserving static analyzability of the SDF model. They assume that an application has a finite number of behaviors (or modes) and each behavior (mode) is represented by an SDF graph. They are classified as multi-mode dataflow models in this paper. While there exist several scheduling techniques for multi-mode dataflow models, no one allows task migration between modes. By observing that the resource requirement can be additionally reduced if task migration is allowed, we propose a multiprocessor scheduling technique of a multi-mode dataflow graph considering task migration between modes. Based on a genetic algorithm, the proposed technique schedules all SDF graphs in all modes simultaneously to minimize the resource requirement. To satisfy the throughput constraint, the proposed technique calculates the actual throughput requirement of each mode and the output buffer size for tolerating throughput jitter. We compare the proposed technique with a method which analyzes SDF graphs in each execution mode separately and a method that does not allow task migration for synthetic examples and three real applications: H.264 decoder, vocoder, and LTE receiver algorithms.
Additional file 1 of Patient-shared knowledge and information in clinical decision-making: an international survey of the perspectives and experiences of naturopathic practitioners
Creators: name: Steel, Amie
name: Brand, Sarah
name: Leach, Matthew
name: Lloyd, Iva
name: Ward, Vicky
Publisher: name: figshare
Year: 2023
Subjects: subject: Medicine
subject: Sociology
subject: FOS: Sociology
classificationCode: 69999
subject: Biological Sciences not elsewhere classified
subject: Science Policy
classificationCode: 110309
subject: Infectious Diseases
subject: FOS: Health sciences

description: Additional file 1.
Analysis of polyspecific naturally-occurring autoantibodies in healthy, unimmunized mice
Creators: name: McCall., Adrian
Publisher: name: Monash University
Year: 2021

description: This thesis was scanned from the print manuscript for digital preservation and is copyright the author.
 Researchers can access this thesis by asking their local university, institution or public library to
 make a request on their behalf. Monash staff and postgraduate students can use the link in the References field.