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Despite its utility in identifying patterns in celestial objects, the Hertzsprung-Russell diagram is not supported in dim or small stars;it struggles to provide insights into certain celestial objects such as brown dw...
supported by Higher Education and Science Committee of the Republic of Armenia(23LCG-1C011);Australian Research Council and Research(DP200101792,DP210101900,DP210102831,DE220100462,LE210100098,LE230100085);Austrian Federal Ministry of Education,Science and Research,Austrian Science Fund(P 34529,J 4731,J 4625,M 3153);Horizon 2020 ERC Starting(947006)“InterLeptons”;Natural Sciences and Engineering Research Council of Canada,Compute Canada and CANARIE;National Key R&D Program of China(2022YFA1601903);National Natural Science Foundation of China(11575017,11761141009,11705209,11975076,12135005,12150004,12161141008,12175041);Natural Science Foundation Project of Shandong Province,China(ZR2022JQ02);the Czech Science Foundation(22-18469S)and Charles University Grant Agency(246122);European Research Council,Seventh Framework(PIEF-GA-2013-622527);Horizon 2020 ERC-Advanced(Grant Nos.267104 and 884719);Horizon 2020 ERC-Consolidator(819127);Horizon 2020 Marie Sklodowska-Curie Grant Agreement(700525)“NIOBE”and(101026516);Horizon 2020 Marie Sklodowska-Curie RISE project JENNIFER2 Grant Agreement(822070)(European grants);L'Institut National de Physique Nucléaire et de Physique des Particules(IN2P3)du CNRS and L'Agence Nationale de la Recherche(ANR)(ANR-21-CE31-0009)(France);BMBF,DFG,HGF,MPG,and AvH Foundation(Germany);Department of Atomic Energy under Project Identification(RTI 4002);Department of Science and Technology,and UPES SEED funding programs(UPES/R&D-SEED-INFRA/17052023/01,UPES/R&D-SOE/20062022/06)(India);Israel Science Foundation(2476/17);U.S.-Israel Binational Science Foundation(2016113);Israel Ministry of Science(3-16543);Istituto Nazionale di Fisica Nucleare and the Research Grants BELLE2;Japan Society for the Promotion of Science,Grant-in-Aid for Scientific Research(16H03968,16H03993,16H06492,16K05323,17H01133,17H05405,18K03621,18H03710,18H05226,19H00682,20H05850,20H05858,22H00144,22K14056,22K21347,23H05433,26220706,26400255);the Ministry of Education,Culture,Sports,Science,and Technology(MEXT)of Japan;Nat
series of data samples was collected with the Belle Ⅱ detector at the SuperKEKB collider from March 2019 to June 2022.We determine the integrated luminosities of these data samples using three distinct methodologies ...
This article concerns the integral related to the transverse comoving distance and, in turn, to the luminosity distance both in the standard non-flat and flat cosmology. The purpose is to determine a straightforward m...
project funded by China National Space Administration(CNSA);the Chinese Academy of Sciences(CAS);supported by the National Key R&D Program of China(2021YFA0718500 and 2023YFE0101200)from the Minister of Science and Technology of China(MOST);supports from the National Natural Science Foundation of China under grants 12373051 and 12333007;supported by International Partnership Program of Chinese Academy of Sciences(grant No.113111KYSB20190020)。
Owing to the broad energy coverage of Insight-HXMT in the hard X-ray band,we detected the highest energy of pulsation exceeding 200 keV around the 2017–2018 outburst peak of the first Galactic pulsating ultraluminous...
the Russian Science Foundation(project No.22-12-00021)。
Luminosity monitoring at e^(+)e^(−)colliders was investigated using SANC Monte Carlo event generator ReneSANCe and integrator MCSANC for simulation of Bhabha scattering at low angles.Results are presented for center-o...
supported by the National Key R&D Program of China under Contract No.2022YFA1602200;the International Partnership Program of the Chineses Academy of Sciences under Grant No.211134KYSB20200057;the STCF Key Technology Research and Development Project.
The superτ-charm facility(STCF)is an electron–positron collider proposed by the Chinese particle physics community.It is designed to operate in a center-of-mass energy range from 2 to 7 GeV with a peak luminosity of...
Empirically standardised peak luminosity of Type Ia supernovae(SNe Ia)as a standard candle has become one of the most powerful probes of the expansion history of the late universe.Although the existence of such a cons...
supported by the National SKA Program of China(Grant No.2020SKA0110402);the National Natural Science Foundation of China(Grant No.12073088);the National Key R&D Program of China(Grant No.2020YFC2201600);the Guangdong Major Project of Basic and Applied Basic Research(Grant No.2019B030302001)。
Much of the research in supernova cosmology is based on an assumption that the peak luminosity of type Ia supernovae(SNe Ia),after a standardization process,is independent of the galactic environment.A series of recen...
support from the National Program on Key Research and Development Project(Grant No.2021YFA0718500)from the Minister of Science and Technology of China(MOST);supports from the National Natural Science Foundation of China under Grants U1938102,12273043,U1838201,U1838202,U1938109 and U1938108;supported by International Partnership Program of Chinese Academy of Sciences(Grant No.113111KYSB20190020).
Purpose In order to carry out in-orbit calibration,the hard X-ray modulation telescope satellite(HXMT)has made a number of observations of Crab pulsar.We study the long-term evolution of the X-ray flux of the Crab pul...
In the warm dark matter scenario, the Press-Schechter formalism is valid only for galaxy masses greater than the “velocity dispersion cut-off”. In this work we extend the predictions to masses below the velocity dis...
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