cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Particle re-acceleration and diffuse radio sources in the galaxy cluster Abell 1550
Creators: name: Pasini, T.
name: Edler, H. W.
name: Brüggen, M.
name: de Gasperin, F.
name: Botteon, A.
name: Rajpurohit, K.
name: van Weeren, R. J.
name: Gastaldello, F.
name: Gaspari, M.
name: Brunetti, G.
name: Cuciti, V.
name: Nanci, C.
name: di Gennaro, G.
name: Rossetti, M.
name: Hoang, D. Dallacasa. D. N.
name: Riseley, C. J.
Publisher: name: arXiv
Year: 2022
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: We study diffuse radio emission in the galaxy cluster A1550, with the aim of constraining particle re-acceleration in the intra-cluster medium. We exploit observations at four different frequencies: 54, 144, 400 and 1400 MHz. To complement our analysis, we make use of archival Chandra X-ray data. At all frequencies we detect an ultra-steep spectrum radio halo ($S_ν\propto ν^{-1.6}$) with an extent of 1.2 Mpc at 54 MHz. Its morphology follows the distribution of the thermal intra-cluster medium inferred from the Chandra observation. West of the centrally located head-tail radio galaxy, we detect a radio relic with projected extent of 500 kpc. From the relic, a 600 kpc long bridge departs and connect it to the halo. Between the relic and the radio galaxy, we observe what is most likely a radio phoenix, given its curved spectrum. The phoenix is connected to the tail of the radio galaxy through two arms, which show a nearly constant spectral index for 300 kpc. The halo could be produced by turbulence induced by a major merger, with its axis lying in the NE-SW direction. This is supported by the position of the relic, whose origin could be attributed to a shock propagating along the merger axis. It is possible that the same shock has also produced the phoenix through adiabatic compression, while the bridge could be generated by electrons which were pre-accelerated by the shock, and then re-accelerated by turbulence. Finally, we detect hints of gentle re-energisation in the two arms which depart from the tail of the radio galaxy.
description: 16 pages, 10 figures
The 2022 Encounter of the Outburst Material from Comet 73P/Schwassmann--Wachmann~3
Creators: name: Ye, Quanzhi
name: Vaubaillon, Jérémie
Publisher: name: arXiv
Year: 2022
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: FOS: Physical sciences

description: The encounter of the meteoric material from 73P/Schmassmann--Wachmann~3 produced during the comet's 1995 outburst in May 2022 provides a rare and valuable opportunity to understand a fragmenting comet. Here we explore various ejection configurations and their impact on the meteor outburst detected in the early hours of UT 2022 May 31. We show that the dust must have been ejected $\sim4$ to $5\times$ faster than calculated by water-ice sublimation model to best match the observed meteor activity. As only a small subset of particles with a narrow range of cross-section is expected to have reached the Earth, the large spread of meteor brightness likely indicates the presence of large but porous meteoroids in the trail. Other effects such as an enhanced lunar sodium tail and a visible glow from the meteoroid trail may have also occurred during the encounter.
description: MNRAS in press
The Effects of Integrated Psychotherapy in Patients who have experienced Trauma: a Pre-Post Design during the Covid-19 Health Emergency
Creators: name: Tirinnanzi, Paolo
name: Bianchi, Alice
Publisher: name: Journal of Clinical & Developmental Psychology
Year: 2020

description: Background: A pandemic from a bio-psycho-social perspective represents for many people both a traumatic event and a risk factor for the onset of traumatic responses. These light up in the present but in reality, they represent the activation of peritraumatic networks dating back to the past to which the person can react both by the appearance of symptomatic pictures and the disintegration of the self into dissociated parts. Starting from this reading of trauma, Integrative Psychotherapy sets itself the challenge of accompanying people in an integrative work of the parts of the self by combining the emotional, somatic, and cognitive levels. Methods: The subjects were 31 patients, 15 of the control group and 16 of the experimental group. An online survey collected information on demographic data. Furthermore, anxiety, depression, and insomnia symptoms were assessed in pre and post-tests. The experimental group continued Integrative Psychotherapy during the health emergency. To analyze data, descriptive statistics, paired and independent two-sample t-tests were used. Results: The results indicated that there was a significant difference between the experimental group (patients that continued Integrative Psychotherapy sessions during the health emergency) and control group (patients that stopped therapy). Conclusions: The best performance of the experimental group shows the impact that Integrative Psychotherapy sessions have had in dealing with, managing, and overcoming the crises that patients were experiencing during the health emergency. Keywords: Integrative Psychotherapy; Self Integration; Trauma; Dissociation; COVID-19 pandemic
description: Journal of Clinical & Developmental Psychology, Online First Articles
Cloud-cloud collision and star formation in G323.18+0.15
Creators: name: Ma, Yingxiu.
name: Zhou, Jianjun.
name: Esimbek, Jarken.
name: Baan, Willem.
name: Li, Dalei.
name: He, Yuxin.
name: Tang, Xindi.
name: Ji, Weiguang.
name: Zhou, Dongdong.
name: Wu, Gang.
name: Xu, Ye.
Publisher: name: arXiv
Year: 2022
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We studied the cloud-cloud collision candidate G323.18+0.15 based on signatures of induced filaments, clumps, and star formation. We used archival molecular spectrum line data from the SEDIGISM $^{13}$CO($J$\,=\,2--1) survey, from the Mopra southern Galactic plane CO survey, and infrared to radio data from the GLIMPSE, MIPS, Hi-GAL, and SGPS surveys. Our new result shows that the G323.18+0.15 complex is 3.55kpc away from us and consists of three cloud components, G323.18a, G323.18b, and G323.18c. G323.18b shows a perfect U-shape structure, which can be fully complemented by G323.18a, suggesting a collision between G323.18a and the combined G323.18bc filamentary structure. One dense compressed layer (filament) is formed at the bottom of G323.18b, where we detect a greatly increased velocity dispersion. The bridge with an intermediate velocity in a position-velocity diagram appears between G323.18a and G323.18b, which corresponds to the compressed layer. G323.18a plus G323.18b as a whole are probably not gravitationally bound. This indicates that high-mass star formation in the compressed layer may have been caused by an accidental event. The column density in the compressed layer of about $1.36 \times 10^{22}$cm$^{-2}$ and most of the dense clumps and high-mass stars are located there. The average surface density of classI and classII young stellar objects (YSOs) inside the G323.18+0.15 complex is much higher than the density in the surroundings. The timescale of the collision between G323.18a and G323.18b is $1.59$Myr. This is longer than the typical lifetime of classI YSOs and is comparable to the lifetime of classII YSOs.
Andreas Anter: Theorien der Macht zur Einführung
Creators: name: Selk, Veith
Publisher: name: UB Tübingen
Year: 2015

description: Andreas Anter (2013): Theorien der Macht zur Einführung, 2., korrigierte Auflage, Hamburg: Junius. 176 S., ISBN 978-3-88506-062-8, EUR 13,90.
description: Ethik und Gesellschaft, Nr. 2 (2015): Burn, baby, burn... Subjektivierte Arbeit und depressive Erschöpfung
Intramolecular Vibrational Redistribution in Formic Acid and its Deuterated Forms
Creators: name: Aerts, Antoine
name: Brown, Alex
name: Gatti, Fabien
Publisher: name: arXiv
Year: 2022
Subjects: subject: Chemical Physics (physics.chem-ph)
subject: FOS: Physical sciences

description: The intramolecular vibrational relaxation dynamics of formic acid and its deuterated isotopologues is simulated on the full-dimensional potential energy surface of Richter and Carbonniere [F. Richter and P. Carbonniere, J. Chem. Phys., 148, 064303 (2018)] using the Heidelberg MCTDH package. Mode couplings with the torsion coordinate capturing most of the trans-cis isomerisation are identified in the dynamics of artificially excited vibrational mode overtones. The C-O stretch bright vibrational mode is coupled to the out-of-the plane torsion mode in HCOOH, where this coupling could be exploited for laser-induced trans-to-cis isomerisation. Strong isotopic effects are observed: deuteration of the hydroxyl group, i.e., in HCOOD and DCOOD, destroys the C-O stretch to torsion mode coupling whereas in DCOOH, little to no effect is observed.
description: 28 pages, 7 figures
Additional file 7 of [18F]PSMA-1007 PET for biochemical recurrence of prostate cancer, a comparison with [18F]Fluciclovine
Creators: name: Loeff, Cato C.
name: van Gemert, Willemijn
name: Privé, Bastiaan M.
name: van Oort, Inge M.
name: Hermsen, Rick
name: Somford, Diederik M.
name: Nagarajah, James
name: Heijmen, Linda
name: Janssen, Marcel J. R.
Publisher: name: figshare
Year: 2024
Subjects: Medicine
Cell Biology
Cancer

description: Additional file 7
Detection of eccentric close-binary supermassive black holes with incomplete interferometric data
Creators: name: Kovacevic, Andjelka
name: Songsheng, Yu-Yang
name: Wang, Jian-Min
name: Popovic, Luka C.
Publisher: name: arXiv
Year: 2022
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: Recent studies have proposed that GRAVITY+ instrument is able to trace the circular orbit of the subparsec close-binary supermassive black holes (CB-SMBHs) by measuring the photocentre variation of the hot dust emission. However, the CB-SMBHs orbit may become highly eccentric throughout the evolution of these objects, and the orbital period may be far longer than the observational time baseline. We investigate the problem of detecting the CB-SMBH with hot dust emission and high eccentricity (eCBSMBH, e=0.5) when the observed time baselines of their astrometric data and radial velocities are considerably shorter than the orbital period. The parameter space of the Keplerian model of the eCBSMBH is large for exploratory purposes. We therefore applied the Bayesian method to fit orbital elements of the eCBSMBH to combined radial velocity and astrometric data covering a small fraction of the orbital period. We estimate that a number of potential eCBSMBH systems within reach of GRAVITY + will be similar to the number of the planned circular targets. We show that using observational time baselines that cover ~ 10% of the orbit increases the possibility of determining the period, eccentricity, and total mass of an eCBSMBH. When the observational time baseline becomes too short (~ 5%), the quality of the retrieved eCBSMBH parameters degrades. We also illustrate how interferometry may be used to estimate the photo-centre at the eCBSMBH emission line, which could be relevant for GRAVITY+ successors. Even if the astrometric signal for eCBSMBH systems is reduced by a factor of sqrt{1-e^{2}} compared to circular ones, we find that the hot dust emission of eCBSMBHs can be traced by GRAVITY+ at the elementary level.
description: accepted for publication in the journal Astronomy & Astrophysics
Supplementary Material from Divergence in brain size and brain region volumes across wild guppy populations
Creators: name: Reyes, Angie S.
name: Bittar, Amaury
name: Ávila, Laura C.
name: Botia, Catalina
name: Esmeral, Natalia P.
name: Bloch, Natasha I.
Publisher: name: The Royal Society
Year: 2022
Subjects: subject: Neuroscience
subject: Evolutionary Biology
subject: FOS: Biological sciences

description: This file contains supplementary methods, figures and tables
ИНКОТЕРМС 2020: ОСНОВНЫЕ ИЗМЕНЕНИЯ ДЛЯ ЗАКЛЮЧЕНИЯИ ИСПОЛНЕНИЯ ДОГОВОРОВ МЕЖДУНАРОДНОЙ КУПЛИ-ПРОДАЖИ ТОВАРОВ
Creators: name: ХОЛОПОВ КОНСТАНТИН ВЛАДИМИРОВИЧ
Publisher: name: Российский внешнеэкономический вестник
Year: 2020
Subjects: ПРАВИЛА ICC ПО ИСПОЛЬЗОВАНИЮ НАЦИОНАЛЬНЫХ И МЕЖДУНАРОДНЫХ ТОРГОВЫХ ТЕРМИНОВ
ИНКОТЕРМС 2020
ИНКОТЕРМС 2010
ИЗМЕНЕНИЯ В ИНКОТЕРМС
ТЕРМИНЫ ПОСТАВКИ ТОВАРОВ
БОРТОВОЙ КОНОСАМЕНТ
СТРАХОВОЕ ПОКРЫТИЕ ПО ТРАНСПОРТНОМУ СТРАХОВАНИЮ ГРУЗОВ
МЕЖДУНАРОДНАЯ ПОСТАВКА ТОВАРОВ В КОНТЕЙНЕРАХ МОРЕМ
СОЛАС
БАЗИСНЫЕ УСЛОВИЯ ПОСТАВКИ ТОВАРОВ
ICC RULES FOR THE USE OF DOMESTIC AND INTERNATIONAL TRADE TERMS
INCOTERMS 2020
INCOTERMS 2010
CHANGES IN INCOTERMS
TERMS OF DELIVERY
ON-BOARD BILL OF LADING
INSURANCE COVERAGE
DPU
INTERNATIONAL CONTAINER SHIPPING
SOLAS

description: Автор рассматривает и анализирует основные изменения, внесённые в Инкотермс 2020 по сравнению с предыдущей редакцией документа. Акцент сделан на те изменения, которые существенно влияют на процессы заключения и процедуры исполнения договоров международной купли-продажи товаров. Особое внимание уделяется вопросам транспортно-логистического и документарного обеспечения внешнеторговых контрактов. Комментируются возможности подтверждения поставок товаров на термине FCA бортовыми коносаментами, доставка товаров во внутреннем и международном сообщениях своими силами без привлечения перевозчиков, последствия изменения уровня страхового покрытия на термине CIP, изменения аббревиатуры термина DAT на DPU, а также новые обязательства и расходы сторон при поставках товаров морем в контейнерах в международных сообщениях.
SDSS-IV MaNGA: How the stellar populations of passive central galaxies depend on stellar and halo mass
Creators: name: Oyarzun, Grecco A.
name: Bundy, Kevin
name: Westfall, Kyle B.
name: Tinker, Jeremy L.
name: Belfiore, Francesco
name: Argudo-Fernandez, Maria
name: Zheng, Zheng
name: Conroy, Charlie
name: Masters, Karen L.
name: Wake, David
name: Law, David R.
name: McDermid, Richard M.
name: Aragon-Salamanca, Alfonso
name: Parikh, Taniya
name: Yan, Renbin
name: Bershady, Matthew
name: Sanchez, Sebastian F.
name: Andrews, Brett H.
name: Fernandez-Trincado, Jose G.
name: Lane, Richard R.
name: Bizyaev, D.
name: Boardman, Nicholas Fraser
name: Lacerna, Ivan
name: Brownstein, J. R.
name: Drory, Niv
name: Zhang, Kai
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 analyze spatially resolved and co-added SDSS-IV MaNGA spectra with signal-to-noise ~100 from 2200 passive central galaxies (z~0.05) to understand how central galaxy assembly depends on stellar mass (M*) and halo mass (Mh). We control for systematic errors in Mh by employing a new group catalog from Tinker (2020a,b) and the widely-used Yang et al. (2007) catalog. At fixed M*, the strength of several stellar absorption features varies systematically with Mh. Completely model-free, this is one of the first indications that the stellar populations of centrals with identical M* are affected by the properties of their host halos. To interpret these variations, we applied full spectral fitting with the code alf. At fixed M*, centrals in more massive halos are older, show lower [Fe/H], and have higher [Mg/Fe] with 3.5 sigma confidence. We conclude that halos not only dictate how much M* galaxies assemble, but also modulate their chemical enrichment histories. Turning to our analysis at fixed Mh, high-M* centrals are older, show lower [Fe/H], and have higher [Mg/Fe] for Mh>10^{12}Msun/h with confidence > 4 sigma. While massive passive galaxies are thought to form early and rapidly, our results are among the first to distinguish these trends at fixed Mh. They suggest that high-M* centrals experienced unique early formation histories, either through enhanced collapse and gas fueling, or because their halos were early-forming and highly concentrated, a possible signal of galaxy assembly bias.
description: Accepted for publication in ApJ. 28 pages and 12 figures
НАПРАВЛЕНИЯ РАЗВИТИЯРЫНКА УСЛУГ ПО ОБСЛУЖИВАНИЮ ВОЗДУШНЫХ СУДОВ
Creators: name: НИКИТЕНКО АЛЕКСАНДР АЛЕКСЕЕВИЧ
Publisher: name: Российский внешнеэкономический вестник
Year: 2020
Subjects: ГРАЖДАНСКАЯ АВИАТЕХНИКА
ПРОИЗВОДСТВО ВОЗДУШНЫХ СУДОВ
ТЕХНИЧЕСКОЕ ОБСЛУЖИВАНИЕ И РЕМОНТ
ЭКСПОРТ
УСЛУГИ ПО ОБЕСПЕЧЕНИЮ ЛЕТНОЙ ГОДНОСТИ САМОЛЕТОВ
CIVIL AIRCRAFT
PRODUCTION OF AIRCRAFTS
MAINTENANCE AND REPAIR
EXPORTS
AIRCRAFT OVERHAUL SERVICES

description: Развитие международной торговли гражданской авиатехникой в последние годы характеризуется усилением конкурентной борьбы между двумя крупнейшими монополиями корпорациями «Boeing» и «Airbus». Автор рассматривает тенденции взаимного соперничества этих двух компаний и анализирует изменение производственной и сбытовой политики этих компаний. Главное внимание уделяется развитию практики технического обслуживания и ремонта гражданской авиатехники, предложение услуг по обеспечению летной годности со стороны специализированных компаний и фирм-производителей воздушных судов. Он доказывает, что расширение сети технического обслуживания существенно влияет на успех в конкуренции на рынке гражданских самолетов.
ОСОБЕННОСТИ МЕЖДУНАРОДНОГО РЫНКА СТРОИТЕЛЬСТВА АЭС
Creators: name: МАРЧЕНКО АНДРЕЙ СЕРГЕЕВИЧ
Publisher: name: Российский внешнеэкономический вестник
Year: 2020
Subjects: АТОМНАЯ ЭНЕРГЕТИКА
СТРОИТЕЛЬСТВО АЭС
МЕЖДУНАРОДНАЯ СТАТИСТИКА ТОРГОВЛИ РЕАКТОРНЫМ ОБОРУДОВАНИЕМ
МЕЖДУНАРОДНЫЙ РЫНОК СТРОИТЕЛЬСТВА АЭС
РОСАТОМ
NUCLEAR POWER
NUCLEAR POWER PLANT CONSTRUCTION
STATISTICS ON INTERNATIONAL TRADE IN NUCLEAR POWER PLANT EQUIPMENT
INTERNATIONAL MARKET FOR NUCLEAR POWER PLANT CONSTRUCTION
ROSATOM

description: В данной статье представлены основные особенности атомной энергетики, влияющие на формирование и развитие международного рынка строительства атомных станций. Автором рассмотрены крупнейшие компании на рынке строительства атомных станций, являющиеся держателями ядерных технологий. Отдельно рассмотрено положение России на этом рынке в лице государственной корпорации «Росатом». Для дополнения картины рассмотрена международная статистика торговли реакторным оборудованием. Данная статистика позволяет выделить основных поставщиков реакторного оборудования и определить страны, в которых ведется сооружение атомных станций.
Additional file 8 of [18F]PSMA-1007 PET for biochemical recurrence of prostate cancer, a comparison with [18F]Fluciclovine
Creators: name: Loeff, Cato C.
name: van Gemert, Willemijn
name: Privé, Bastiaan M.
name: van Oort, Inge M.
name: Hermsen, Rick
name: Somford, Diederik M.
name: Nagarajah, James
name: Heijmen, Linda
name: Janssen, Marcel J. R.
Publisher: name: figshare
Year: 2024
Subjects: Medicine
Cell Biology
Cancer

description: Additional file 8
Ensemble simulations of the 12 July 2012 Coronal Mass Ejection with the Constant Turn Flux Rope Model
Creators: name: Singh, Talwinder
name: Kim, Tae K.
name: Pogorelov, Nikolai V.
name: Arge, Charles N.
Publisher: name: arXiv
Year: 2022
Subjects: subject: Space Physics (physics.space-ph)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: Flux-rope-based magnetohydrodynamic modeling of coronal mass ejections (CMEs) is a promising tool for the prediction of the CME arrival time and magnetic field at Earth. In this work, we introduce a constant-turn flux rope model and use it to simulate the 12-July-2012 16:48 CME in the inner heliosphere. We constrain the initial parameters of this CME using the graduated cylindrical shell (GCS) model and the reconnected flux in post-eruption arcades. We correctly reproduce all the magnetic field components of the CME at Earth, with an arrival time error of approximately 1 hour. We further estimate the average subjective uncertainties in the GCS fittings, by comparing the GCS parameters of 56 CMEs reported in multiple studies and catalogs. We determined that the GCS estimates of the CME latitude, longitude, tilt, and speed have average uncertainties of 5.74 degrees, 11.23 degrees, 24.71 degrees, and 11.4% respectively. Using these, we have created 77 ensemble members for the 12-July-2012 CME. We found that 55% of our ensemble members correctly reproduce the sign of the magnetic field components at Earth. We also determined that the uncertainties in GCS fitting can widen the CME arrival time prediction window to about 12 hours for the 12-July-2012 CME. On investigating the forecast accuracy introduced by the uncertainties in individual GCS parameters, we conclude that the half-angle and aspect ratio have little impact on the predicted magnetic field of the 12-July-2012 CME, whereas the uncertainties in longitude and tilt can introduce a relatively large spread in the magnetic field predicted at Earth.
ЭКОЛОГИЧЕСКИЕ ПРОБЛЕМЫ ПРОМЫШЛЕННОГО РАЗВИТИЯ КИТАЯ
Creators: name: ЗАХАРОВ АЛЕКСАНДР НИКОЛАЕВИЧ
name: КАЛАШНИКОВ ДЕНИС БОРИСОВИЧ
Publisher: name: Российский внешнеэкономический вестник
Year: 2020
Subjects: «ОДИН ПОЯС ОДИН ПУТЬ»
УСТОЙЧИВОЕ РАЗВИТИЕ
«ЗЕЛЕНАЯ» ЭКОНОМИКА
ИНДУСТРИАЛИЗАЦИЯ
РЕИНДУСТРИАЛИЗАЦИЯ
ПРОМЫШЛЕННАЯ ПОЛИТИКА
ONE BELT ONE ROAD
SUSTAINABLE DEVELOPMENT
GREEN ECONOMY
INDUSTRIALIZATION
RE-INDUSTRIALIZATION
INDUSTRIAL POLICY

description: Новизна постановки проблемы в данной статье обусловлена грядущей волной индустриализации отсталых стран и угрозой всемирного экологического кризиса в связи с отказом Китая от роли «мировой фабрики», и его переходом к постиндустриальному обществу. В статье раскрываются причины и проблемы преодоления негативного воздействия промышленного развития на окружающую среду. Теоретически, устойчивое «зелёное» развитие возможно. Однако, на практике оно упирается в отсутствие финансирования. Мировой опыт свидетельствует о потребности в государственном регулировании «зелёного» развития. Проанализированы новейшие меры и достижения правительства Китая в области экологизации экономики. Раскрыты особенности китайской экономической модели, позволяющие осуществлять дорогостоящие «зелёные» проекты с длительными сроками окупаемости, в т.ч. частным бизнесом. Новизна статьи заключается в представлении китайской Инициативы «Один пояс один путь» как направления решения глобальной экологической проблемы и как новой модели «зелёной» индустриализации отсталых стран. Авторами обоснованно доказано, что Китай имеет и мотивы, и возможности разрешить противоречие между промышленным развитием и экологией. Выявлено значение китайского опыта перехода к «зелёной» экономике для России, выражена авторская позиция относительно опасностей участия России в Инициативе «Один пояс один путь» с точки зрения задач модернизации отечественной экономики.
Additional file 9 of [18F]PSMA-1007 PET for biochemical recurrence of prostate cancer, a comparison with [18F]Fluciclovine
Creators: name: Loeff, Cato C.
name: van Gemert, Willemijn
name: Privé, Bastiaan M.
name: van Oort, Inge M.
name: Hermsen, Rick
name: Somford, Diederik M.
name: Nagarajah, James
name: Heijmen, Linda
name: Janssen, Marcel J. R.
Publisher: name: figshare
Year: 2024
Subjects: Medicine
Cell Biology
Cancer

description: Additional file 9
title: Kinematics of the New Zealand plate boundary: field report on GNSS surveys of the Taupō Volcanic Zone and Hauraki Rift (TVZ2021)
Creators: name: Hart, Rory J. A.
name: Palmer, Neville G.
Publisher: name: GNS Science
Year: 2022

description: During February 2021, a combined team from GNS Science and Land Information New Zealand (LINZ) re-measured a network of 103 geodetic survey markers, using Global Navigation Satellite System (GNSS) methods, throughout the Taupō Volcanic Zone and Hauraki regions of New Zealand for monitoring regional deformation due to tectonic processes. Previous comprehensive GNSS surveys of these regions have been carried out in 2015 (TVZ2015 [unpublished]), 2011 (2011TARA-TVZ [unpublished]), 2007 (TVZ2007 [unpublished]), 2005 (TVZ2005 [Palmer 2005]), 1995 (TVZ1995 [Blick et al. 1995]), 1994 (TVZ1994 [Darby and Meertens 1995]), 1993 (TVZ1993 [Blick 1993]), 1992 (TVZ1992 [Blick et al. 1992]) and 1991 (TVZ1991 [Blick 1991]), primarily for the Taupō Volcanic Zone. The Hauraki region was included following GNSS surveys for LINZ in 2013 (2013NNI [Palmer 2015]) and 2017 (2017NNI [unpublished]), and by Earthquake-Commission-funded PhD work of Robert Pickle in 2015, 2016 and 2017 (Pickle 2019) to better constrain deformation rates in this area. This report documents the field operations of the TVZ2021 re-survey. It describes the logistics of the campaign, the sites occupied and the data collected. The observations and data collected during this survey are intended to fulfil GNS Science’s obligation to LINZ under the contract outlined below: Contract name: ‘Regional Deformation Monitoring Service’. (The authors)
Electronic supplementary material from Echiuran Hox genes provide new insights into the correspondence between Hox subcluster organization and collinearity pattern
Creators: name: Wei, Maokai
name: Qin, Zhenkui
name: Kong, Dexu
name: Liu, Danwen
name: Zheng, Qiaojun
name: Bai, Shumiao
name: Zhang, Zhifeng
name: Ma, Yubin
Publisher: name: The Royal Society
Year: 2022
Subjects: subject: Evolutionary Biology
subject: FOS: Biological sciences
subject: Developmental Biology

description: In many bilaterians, Hox genes are generally clustered along the chromosomes and expressed in spatial and temporal order. In vertebrates, the expression of Hox genes follows a whole-cluster spatio-temporal collinearity (WSTC) pattern, whereas in some invertebrates the expression of Hox genes exhibits a subcluster-level spatio-temporal collinearity pattern. In bilaterians, the diversity of collinearity pattern and the cause of collinearity difference in Hox gene expression remain poorly understood. Here, we investigate genomic organization and expression pattern of Hox genes in the echiuran worm Urechis unicinctus (Annelid, Echiura). Urechis unicinctus has a split cluster with four subclusters divided by non-Hox genes: first subcluster (Hox1 and Hox2), second subcluster (Hox3), third subcluster (Hox4, Hox5, Lox5, Antp and Lox4), fourth subcluster (Lox2 and Post2). The expression of U. unicinctus Hox genes shows a subcluster-based whole-cluster spatio-temporal collinearity (S-WSTC) pattern: the anterior-most genes in each subcluster are activated in a spatially and temporally colinear manner (reminiscent of WSTC), with the subsequent genes in each subcluster then being very similar to their respective anterior-most subcluster gene. Combining genomic organization and expression profiles of Hox genes in different invertebrate lineages, we propose that the spatio-temporal collinearity of invertebrate Hox is subcluster-based.
КОНКУРЕНЦИЯ МЕЖДУ ВЛАДЕЛЬЦАМИ ЦИФРОВЫХ ПЛАТФОРМ В МИРОВОЙ ЭКОНОМИКЕ
Creators: name: АСАДУЛЛИНА АННА ВИКТОРОВНА
Publisher: name: Российский внешнеэкономический вестник
Year: 2020
Subjects: ЦИФРОВЫЕ ПЛАТФОРМЫ
РЫНКИ С ДВУСТОРОННИМИ СЕТЕВЫМИ ЭФФЕКТАМИ
ЭФФЕКТ МАСШТАБА
ЭКСПРОПРИАЦИЯ ЗОНЫ УНИЧТОЖЕНИЯ
ПРИОБРЕТЕНИЕ ЗАРОЖДАЮЩИХСЯ КОНКУРЕНТОВ
ОТКАЗ В ДОСТУПЕ К ДАННЫМ
АНТИМОНОПОЛЬНОЕ РЕГУЛИРОВАНИЕ
GAFA
DIGITAL PLATFORM
TWO-SIDED MARKETS
SCALE EFFECT
KILL ZONE EXPROPRIATION
ACQUISITION OF NASCENT RIVALS
DENIAL OF ACCESS OF DATA
ANTITRUST REGULATION

description: Интенсивное развитие цифровых технологий вызвало появление феномена, собирательно именуемого GAFA компаний Google, Apple, Facebook и Amazon, которые продемонстрировали в последнее десятилетие экспоненциальный рост рыночной капитализации и растущую рыночную власть. Существует два подхода к объяснению причин доминирования крупнейших цифровых платформ. Первый в основу рыночной концентрации на рассматриваемых типах рынка ставит эффекты масштаба и сетевые эффекты, характерные для рынков с двусторонними сетевыми эффектами. Второй подход указывает в первую очередь на антимонопольное поведение компаний, владеющих цифровыми платформами.Ввиду отсутствия надлежащих инструментов для оценки антиконкурентных эффектов поведения цифровых гигантов наблюдаются разные подходы в деятельности антимонопольных органов.
ОБЪЕДИНЁННЫЕ АРАБСКИЕ ЭМИРАТЫ: СОСТОЯНИЕ И ПЕРСПЕКТИВЫ ЭКОНОМИКИ И ВНЕШНЕЭКОНОМИЧЕСКИХ СВЯЗЕЙ
Creators: name: РУДЕНКО ЛЮДМИЛА НИКОЛАЕВНА
Publisher: name: Российский внешнеэкономический вестник
Year: 2020
Subjects: ОБЪЕДИНЁННЫЕ АРАБСКИЕ ЭМИРАТЫ
ЭКОНОМИЧЕСКОЕ РАЗВИТИЕ
2010Е ГОДЫ
ПАДЕНИЕ НЕФТЯНЫХ ЦЕН
ЭКОНОМИЧЕСКАЯ ДИВЕРСИФИКАЦИЯ
ЦИФРОВИЗАЦИЯ
РОССИЯОАЭ
ТОРГОВО-ЭКОНОМИЧЕСКОЕ И ИНВЕСТИЦИОННОЕ СОТРУДНИЧЕСТВО
UNITED ARAB EMIRATES
2010S
FALLING OIL PRICES
ECONOMIC DIVERSIFICATION
RUSSIA-UAE
TRADE
ECONOMIC AND INVESTMENT COOPERATION

description: Статья посвящена исследованию различных аспектов экономического развития Объединённых Арабских Эмиратов (ОАЭ) в 2010-е годы. Основное внимание при этом уделяется Абу-Даби и Дубаю, которые являются самыми крупными из семи эмиратов, входящих в это федеративное государство. Важное место в статье отведено изучению влияния ухудшения конъюнктуры глобального энергетического рынка на макроэкономическое и финансовое положение Эмиратов. В то же время автор анализирует особенности экономической диверсификации, а также рассматривает специфику цифровизации в экономике ОАЭ. Особое внимание в статье уделено перспективам расширения торгово-экономического и инвестиционного сотрудничества между Российской Федерацией и Объединёнными Арабскими Эмиратами.
New Photometric Calibration of the Wide Field Camera 3 Detectors
Creators: name: Calamida, A.
name: Bajaj, V.
name: Mack, J.
name: Marinelli, M.
name: Medina, J.
name: Pidgeon, A.
name: Kozhurina-Platais, V.
name: Shanahan, C.
name: Som, D.
Publisher: name: arXiv
Year: 2022
Subjects: subject: Instrumentation and Methods for Astrophysics (astro-ph.IM)
subject: Astrophysics of Galaxies (astro-ph.GA)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: We present a new photometric calibration of the WFC3-UVIS and WFC3-IR detectors based on observations collected from 2009 to 2020 for four white dwarfs, namely GRW+70~5824, GD~153, GD~71, G191B2B, and a G-type star, P330E. These calibrations include recent updates to the Hubble Space Telescope primary standard white dwarf models and a new reference flux for Vega. Time-dependent inverse sensitivities for the two WFC3-UVIS chips, UVIS1 and UVIS2, were calculated for all 42 full-frame filters, after accounting for temporal changes in the observed count rates with respect to a reference epoch in 2009. We also derived new encircled energy values for a few filters and improved sensitivity ratios for the two WFC3-UVIS chips by correcting for sensitivity changes with time. Updated inverse sensitivity values for the 20 WFC3-UVIS quad filters and for the 15 WF3-IR filters were derived by using the new models for the primary standards and the new Vega reference flux and, in the case of the IR detector, new flat fields. However, these values do not account for any sensitivity changes with time. The new calibration provides a photometric internal precision better than 0.5% for the wide-, medium-, and narrow-band WFC3-UVIS filters, 5% for the quad filters, and 1% for the WFC3-IR filters. As of October 15, 2020, an updated set of photometric keywords are populated in the WFC3 image headers.
description: 38 pages, 23 figures, accepted for publication on the Astronomical Journal
Supplementary material for 'Modelling the Arctic wave-affected marginal ice zone, a comparison with ICESat-2 observations'
Creators: name: Boutin, G.
name: Williams, T.
name: Horvat, C.
name: Brodeau, L.
Publisher: name: The Royal Society
Year: 2022
Subjects: subject: Oceanography
subject: FOS: Earth and related environmental sciences
subject: Geophysics
subject: 40602 Glaciology

description: Tables and Figures related to model evaluation
Additional file 10 of [18F]PSMA-1007 PET for biochemical recurrence of prostate cancer, a comparison with [18F]Fluciclovine
Creators: name: Loeff, Cato C.
name: van Gemert, Willemijn
name: Privé, Bastiaan M.
name: van Oort, Inge M.
name: Hermsen, Rick
name: Somford, Diederik M.
name: Nagarajah, James
name: Heijmen, Linda
name: Janssen, Marcel J. R.
Publisher: name: figshare
Year: 2024
Subjects: Medicine
Cell Biology
Cancer

description: Additional file 10
X-ray emission of contact binary variables within 1 kpc
Creators: name: Liu, Junhui
name: Wu, Jianfeng
name: Esamdin, Ali
name: Gu, Wei-Min
name: Sun, Mouyuan
name: Wang, Junfeng
Publisher: name: arXiv
Year: 2022
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: By assembling the largest sample to date of X-ray emitting EW-type binaries (EWXs), we carried out correlation analyses for the X-ray luminosity log$L_{\textrm{X}}$, and X-ray activity level log($L_{\textrm{X}}$/$L_{\textrm{bol}}$) versus the orbital period $P$ and effective temperature $T_{\rm eff}$. We find strong $P$-log$L_{\textrm{X}}$ and $P$-log($L_{\textrm{X}}$/$L_{\textrm{bol}}$) correlations for EWXs with $P$ < 0.44 days and we provide the linear parametrizations for these relations, on the basis of which the orbital period can be treated as a good predictor for log$L_{\textrm{X}}$ and log($L_{\textrm{X}}$/$L_{\textrm{bol}}$). The aforementioned binary stellar parameters are all correlated with log$L_{\textrm{X}}$, while only $T_{\rm eff}$ exhibits a strong correlation with log($L_{\textrm{X}}$/$L_{\textrm{bol}}$). Then, EWXs with higher temperature show lower X-ray activity level, which could indicate the thinning of the convective area related to the magnetic dynamo mechanism. The total X-ray luminosity of an EWX is essentially consistent with that of an X-ray saturated main sequence star with the same mass as its primary, which may imply that the primary star dominates the X-ray emission. The monotonically decreasing $P$-log($L_{\textrm{X}}$/$L_{\textrm{bol}}$) relation and the short orbital periods indicate that EWXs could all be in the X-ray saturated state, and they may inherit the changing trend of the saturated X-ray luminosities along with the mass shown by single stars. For EWXs, the orbital period, mass, and effective temperature increase in concordance. We demonstrate that the period $P=0.44$ days corresponds to the primary mass of $\sim1.1 \rm M_\odot$, beyond which the saturated X-ray luminosity of single stars will not continue to increase with mass. This explains the break in the positive $P$-log$L_{\textrm{X}}$ relation for EWXs with $P>0.44$ days.
description: 16 pages, 7 figures and 8 tables; accepted for publication in A&A
5 ЛЕТ ЕАЭС: ИТОГИ ВЗАИМНОЙ ТОРГОВЛИ
Creators: name: УШКАЛОВА ДАРЬЯ ИГОРЕВНА
Publisher: name: Российский внешнеэкономический вестник
Year: 2020
Subjects: ЕВРАЗИЙСКИЙ ЭКОНОМИЧЕСКИЙ СОЮЗ
СТРАНЫ ЕАЭС
ВЗАИМНАЯ ТОРГОВЛЯ В РАМКАХ ЕАЭС
ТОВАРНАЯ СТРУКТУРА ВЗАИМНОЙ ТОРГОВЛИ
МЕЖДУНАРОДНАЯ ЭКОНОМИЧЕСКАЯ ИНТЕГРАЦИЯ
EURASIAN ECONOMIC UNION
EAEU
EAEU MUTUAL TRADE
COMMODITY STRUCTURE OF MUTUAL TRADE
INTERNATIONAL ECONOMIC INTEGRATION

description: В статье представлен анализ развития взаимной торговли стран Евразийского экономического союза в ходе интеграционного процесса. Подробно анализируется динамика и факторы развития многостороннего торгового взаимодействия в рамках ЕАЭС, важнейшие тенденции эволюции товарной структуры взаимной торговли его членов. В результате исследования делается вывод о преобладании позитивного влияния интеграционного процесса на товарную структуру взаимной торговли стран ЕАЭС: в ходе интеграционного процесса в рамках ТС-ЕЭП-ЕАЭС удельный вес минеральных продуктов в общем объеме экспорта сократился на треть; существенно возросла доля продовольственных товаров и сельскохозяйственного сырья; наметилось повышение удельного веса поставок машин, оборудования и транспортных средств.
Nova Sagittarii 1943 (V1148 Sgr): A Luminous Red Nova?
Creators: name: Bond, Howard E.
name: Mink, Jessica
name: Doane, Allison
name: Lavallee, Sarah
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: Nova Sagittarii 1943 (V1148 Sgr) was an 8th-mag optical transient that was unusual in having a late-type spectrum during its outburst, in striking contrast to the normal high-excitation spectra seen in classical novae. Unfortunately, only an approximate position was given in the discovery announcement, hampering follow-up attempts to observe its remnant. We have identified the nova on two photographic plates in the Harvard archive, allowing us to determine a precise astrometric position. Apart from these two plates, obtained in 1943 and 1944, none of the photographs in the Harvard collection, from 1897 to 1950, show V1148 Sgr to limits as faint as g ~ 18.3. Modern deep images show a candidate remnant at i ~ 19.2, lying only 0".26 from the site of the nova. V1148 Sgr may have been a luminous red nova (LRN), only the sixth one known in the Milky Way. However, it lacks the near- and mid-infrared excesses, and millimeter-wave emission, seen in other LRNe, leaving its nature uncertain. We urge spectroscopy of the candidate remnant.
description: Accepted by Astronomical Journal
ОСОБЫЕ ЭКОНОМИЧЕСКИЕ ЗОНЫ В РАЗВИТИИ МИРОВОЙ ЭКОНОМИКИ
Creators: name: КРАВЧЕНКО ЮЛИЯ БОРИСОВНА
Publisher: name: Российский внешнеэкономический вестник
Year: 2020
Subjects: ОСОБЫЕ ЭКОНОМИЧЕСКИЕ ЗОНЫ
ПРИВЛЕЧЕНИЕ ИНВЕСТИЦИЙ
СТИМУЛИРОВАНИЕ ЭКСПОРТА
СОЗДАНИЕ РАБОЧИХ МЕСТ
ЭКОНОМИЧЕСКИЙ РОСТ
SPECIAL ECONOMIC ZONES
INVESTMENT ATTRACTION
EXPORT GENERATION
MENT CEMPLOYREATION
ECONOMIC GROWTH

description: В статье автор рассматривает динамику количества особых экономических зон и их вклад в развитие мировой экономики. Выявлено, что особые экономические зоны могут содействовать привлечению инвестиций, стимулированию экспорта и созданию рабочих мест только в тех случаях, когда удается наладить связи между зонами и остальной экономикой. Установлено, что там, где особые экономические зоны способствуют экономическому росту, динамика, как правило, носит временный характер. При этом слишком многие зоны действуют как анклавы и оказывают ограниченное воздействие вне своих пределов. В конце статьи автор приводит новые вызовы, с которыми в будущем могут столкнуться особые экономические зоны.
Effects of CO-dark Gas on Measurements of Molecular Cloud Stability and the Size-Linewidth Relationship
Creators: name: O'Neill, Theo J.
name: Indebetouw, Remy
name: Bolatto, Alberto D.
name: Madden, Suzanne C.
name: Wong, Tony
Publisher: name: arXiv
Year: 2022
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: Stars form within molecular clouds, so characterizing the physical states of molecular clouds is key in understanding the process of star formation. Cloud structure and stability is frequently assessed using metrics including the virial parameter and Larson (1981) scaling relationships between cloud radius, velocity dispersion, and surface density. Departures from the typical Galactic relationships between these quantities have been observed in low-metallicity environments. The amount of H$_2$ gas in cloud envelopes without corresponding CO emission is expected to be high under these conditions; therefore, this "CO-dark" gas could plausibly be responsible for the observed variations in cloud properties. We derive simple corrections that can be applied to empirical clump properties (mass, radius, velocity dispersion, surface density, and virial parameter) to account for CO-dark gas in clumps following power-law and Plummer mass density profiles. We find that CO-dark gas is not likely to be the cause of departures from Larson's relationships in low-metallicity regions, but that virial parameters may be systematically overestimated. We demonstrate that correcting for CO-dark gas is critical for accurately comparing the dynamical state and evolution of molecular clouds across diverse environments.
description: 19 pages, 5 figures, accepted for publication in ApJ
ВНЕШНЕТОРГОВАЯ ДЕЯТЕЛЬНОСТЬ КНР
Creators: name: ЧЖЭН ВЭЙ
Publisher: name: Российский внешнеэкономический вестник
Year: 2020
Subjects: ТАМОЖЕННО-ТАРИФНОЕ РЕГУЛИРОВАНИЕ
НЕТАРИФНОЕ РЕГУЛИРОВАНИЕ
ОБЪЕМЫ ЭКСПОРТА
ТОРГОВЫЕ КОНФЛИКТЫ
ВТО
ВНЕШНЕТОРГОВАЯ ДЕЯТЕЛЬНОСТЬ
США
CUSTOMS TARIFF REGULATION
NON-TARIFF REGULATION
EXPORT VOLUMES
TRADE CONFLICTS
WTO
FOREIGN TRADE ACTIVITIES
USA

description: В данной статье представлены инструменты управления внешнеторговой деятельностью Китая, в том числе таможенно-тарифные и нетарифные. В статье представлены основные принципы внешней торговли, направленные на эффективную модернизацию национальной экономики Китая. Дана оценка угроз, влияющих на внешнеэкономическую деятельность Китая в связи с введением высоких импортных пошлин со стороны США. Проанализированы текущее внутреннее потребление Китая, объем экспорта при текущих импортных таможенных ставках США. Выявлено, что внешнеторговая деятельность является ключевым фактором стабильного экономического развития Китая.
LibOCS BESPOC Implementation
Creators: name: Ignat, Tiberius
Publisher: name: Zenodo
Year: 2024
Subjects: libocs
citizen science
open science
bespoc
academic libraries
baltics

description: Slides from Multiplier Event "Strengthening the Role of Libraries for Rising Citizen Science: LibOCS shares knowledge and experience", took place at Kaunas University of Technology Campus Library (Studentų St. 48, Kaunas, Lithuania). 

 

Project Number: 2021-1-EE01-KA220-HED-000031125

Project Acronym: LibOCS

Project Title: University libraries strengthening the academia-society connection through citizen science in the Baltics

This project is funded under the Erasmus+ KA2 Strategic Partnerships program.
Evolution of Main-Sequence-like Surviving Companions in Type Ia Supernova Remnants
Creators: name: Rau, Shiau-Jie
name: Pan, Kuo-Chuan
Publisher: name: arXiv
Year: 2022
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: Recent theoretical and numerical studies of Type Ia supernova explosion within the single-degenerate scenario suggest that the non-degenerate companions could survive during the supernova impact and could be detectable in nearby supernova remnants. However, observational efforts show less promising evidence on the existence of surviving companions from the standard single-degenerate channels. The spin-up/spin-down models are possible mechanisms to explain the non-detection of surviving companions. In these models, the spin-up phase could increase the critical mass for explosion, leading to a super-Chandrasekhar mass explosion, and the spin-down phase could lead to extra mass loss and angular momentum redistribution. Since the spin-down timescale for the delayed explosion of a rotating white dwarf is unclear, in this paper, we explore a vast parameter space of main-sequence-like surviving companions via two-dimensional hydrodynamic simulations of supernova impact and the subsequent stellar evolution of surviving companions. Tight universal relations to describe the mass stripping effect, supernova kick, and depth of supernova heating are provided. Our results suggest that the not-yet detected surviving companions from observations of nearby Type Ia supernova remnants might favor low mass companions, short binary separation, or stronger supernova explosion energies than the standard singe-degenerate channels.
description: 11 pages, 9 figures. Accepted by ApJ
An Expanding Shell of Neutral Hydrogen Associated with SN 1006: Hints for the Single-Degenerate Origin and Faint Hadronic Gamma-Rays
Creators: name: Sano, H.
name: Yamaguchi, H.
name: Aruga, M.
name: Fukui, Y.
name: Tachihara, K.
name: Filipovic, M. D.
name: Rowell, G.
Publisher: name: arXiv
Year: 2022
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We report new HI observations of the Type Ia supernova remnant SN 1006 using the Australia Telescope Compact Array with an angular resolution of $4.5' \times 1.4'$ ($\sim$2 pc at the assumed SNR distance of 2.2 kpc). We find an expanding gas motion in position-velocity diagrams of HI with an expansion velocity of $\sim$4 km s$^{-1}$ and a mass of $\sim$1000 $M_\odot$. The spatial extent of the expanding shell is roughly the same as that of SN 1006. We here propose a hypothesis that SN 1006 exploded inside the wind-blown bubble formed by accretion winds from the progenitor system consisting of a white dwarf and a companion star, and then the forward shock has already reached the wind wall. This scenario is consistent with the single-degenerate model. We also derived the total energy of cosmic-ray protons $W_\mathrm{p}$ to be only $\sim$1.2-$2.0 \times 10^{47}$ erg by adopting the averaged interstellar proton density of $\sim$25 cm$^{-3}$. The small value is compatible with the relation between the age and $W_\mathrm{p}$ of other gamma-ray supernova remnants with ages below $\sim$6 kyr. The $W_\mathrm{p}$ value in SN 1006 will possibly increase up to several 10$^{49}$ erg in the next $\sim$5 kyr via the cosmic-ray diffusion into the HI wind-shell.
description: 12 pages, 4 figures, 1 table, accepted for publication in The Astrophysical Journal (ApJ)
ОЦЕНКА ПРОИЗВОДСТВЕННОЙ И ВНЕШНЕТОРГОВОЙ ДЕЯТЕЛЬНОСТИ ПРЕДПРИЯТИЙ КИТАЯ
Creators: name: ЯНЬ ЛЭЙ
Publisher: name: Российский внешнеэкономический вестник
Year: 2020
Subjects: ПРОИЗВОДСТВЕННАЯ ПРОГРАММА «СДЕЛАНО В КИТАЕ 2025»
ИННОВАЦИОННЫЕ ПРОЕКТЫ
ТОРГОВАЯ НАПРЯЖЕННОСТЬ
МИНИСТЕРСТВО ПРОМЫШЛЕННОСТИ И ИНФОРМАТИЗАЦИИ КИТАЯ
ВЫСОКИЕ ТЕХНОЛОГИИ
PRODUCTION PROGRAM “MADE IN CHINA-2025”
INNOVATIVE PROJECTS
TRADE TENSIONS
MINISTRY OF INDUSTRY AND INFORMATION TECHNOLOGY OF CHINA
HIGH TECHNOLOGY

description: В рамках статьи рассмотрены проблемы реализации производственных программ для развития промышленности Китая. Представлены ключевые особенности внешнеторговой деятельности Китая. Проведен обзор успешных производственных программ, реализованных в рамках приоритетных направлений экономического развития Китая в условиях торговой напряженности с США. Раскрыт потенциал реализуемых производственных программ с точки зрения экономического эффекта для страны. Проанализированы производственные программы Китая и Германии, обладающие взаимодополняемостью и взаимозаменяемостью.
Additional figures and detailed descriptions of analysis from Increased SERCA2a sub-cellular heterogeneity in right-ventricular heart failure inhibits excitation-contraction coupling and modulates arrhythmogenic dynamics
Creators: name: Holmes, M.
name: Hurley, M. E.
name: Sheard, T. M. D.
name: Benson, A. P.
name: Jayasinghe, I.
name: Colman, M. A.
Publisher: name: The Royal Society
Year: 2022
Subjects: subject: Cell Biology
subject: Physiology
subject: FOS: Biological sciences
subject: Computational Biology

description: The intracellular calcium handling system of cardiomyocytes is responsible for controlling excitation-contraction coupling (ECC) and has been linked to pro-arrhythmogenic cellular phenomena in conditions such as heart failure (HF). SERCA2a, responsible for intracellular uptake, is a primary regulator of calcium homeostasis, and remodelling of its function has been proposed as a causal factor underlying cellular and tissue dysfunction in disease. Whereas adaptations to the global (i.e. whole-cell) expression of SERCA2a have been previously investigated in the context of multiple diseases, the role of its spatial profile in the sub-cellular volume has yet to be elucidated. We present an approach to characterize the sub-cellular heterogeneity of SERCA2a and apply this approach to quantify adaptations to the length-scale of heterogeneity (the distance over which expression is correlated) associated with right-ventricular (RV) HF. These characterizations informed simulations to predict the functional implications of this heterogeneity, its remodelling in disease, on ECC, the dynamics of calcium-transient alternans and the emergence of spontaneous triggered activity. Image analysis reveals that RV-HF is associated with an increase in length-scale and its inter-cellular variability; simulations predict that this increase in length-scale can reduce ECC and critically modulate the vulnerability to both alternans and triggered activity.This article is part of the theme issue ‘The cardiomyocyte: new revelations on the interplay between architecture and function in growth, health and disease’.