supported by the National SKA Program of China(2022SKA0120101,2022SKA0130100,2022SKA 0130104);the National Natural Science Foundation of China(NSFC,grant No.12103013);the Foundation of Science and Technology of Guizhou Province(Nos.(2021)023);the Foundation of Guizhou Provincial Education Department(Nos.KY(2021)303,KY(2020)003,KY(2023)059);supported by the National Natural Science Foundation of China(NSFC,grant Nos.12103076 and 12233005);the National Key R&D Program of China(2020YFE0202100);the Shanghai Sailing Program(21YF1455300);the China Postdoctoral Science Foundation(2021M693267)。
We present an independent catalog(FRIIRGcat)of 45,241 Fanaroff–Riley TypeⅡ(FR-Ⅱ)radio galaxies compiled from the Very Large Array Faint Images of the Radio Sky at Twenty-centimeters(FIRST)survey and employed the de...
supported by the National SKA Program of China(Nos.2022SKA0110201 and 2022SKA0110200);CAS Project for Young Scientists in Basic Research grant No.YSBR-062;the National Natural Science Foundation of China(NSFC)(grant Nos.12033008,11622325,11988101);the K.C.Wong Education Foundation;the science research grants from the China Manned Space Project(CMSP)with NO.CMS-CSST-2021-A03 and NO.CMS-CSST-2021-A07;support of the Tsinghua Shui Mu Scholarship;NSFC(grant No.12073014);the science research grants from the China Manned Space Project with No.CMS-CSST2021-A05;Tsinghua University Initiative Scientific Research Program(No.20223080023);supported by NSFC(grant Nos.11988101,12041302,and U1931110);supported by the science research grant from the China Manned Space Project with grant No.CMS-CSST-2021-A08;support from the European Union's Horizon 2020 Research and Innovation Programme under the Marie Sk?odowska-Curie grant agreement No.101086388;supported by the Cultivation Project for FAST Scientific Payoff and Research Achievement of CAMS-CAS;supported by the Key Research Project of Zhejiang Lab(No.2021PE0AC03)。
Environments play an important role in galaxy formation and evolution,particularly in regulating the content of neutral gas.However,current HI surveys have limitations in their depth,which prevents them from adequatel...
the support by the Russian Science Foundation grant 23-22-00090。
We study the origin of X-ray emission from OB stars due to collisions of stellar winds and/or inhomogeneities in the winds. The low-resolution X-ray spectra of a big sample of OB stars were fitted by both the stationa...
supported by the National Natural Science Foundation of China(NSFC,grant Nos.11988101 and 12073043);National Key Research and Development Program of China No.2019YFA0405500;the support from CAS Project for Young Scientists in Basic Research grant No.YSBR-062。
The specific angular momenta(j_(t))of stars,baryons as a whole and dark matter halos contain clues of vital importance about how galaxies form and evolve.Using a sample of 70 spiral galaxies,we perform a preliminary a...
supported by the National SKA Program of China No.2020SKA0120100;the National Natural Science Foundation of China(NSFC,Grant Nos.11963002,11703047,11773041,U2031119,12173052,12003047 and 12173053);the fostering project of Guizhou University with No.201911;Cultivation Project for FAST Scientific Payoff and Research Achievement of CAMS-CAS;supported by the Specialized Research Fund for State Key Laboratories;supported by the CAS“Light of West China”Program;the Youth Innovation Promotion Association of CAS(id 2023064);supported by the Youth Innovation Promotion Association of CAS(id.2018075 and Y2022027);supported by Guizhou Provincial Basic Research Program(Natural Science)(ZK[2023]039);Key Technology R&D Program([2023]352)。
Up to 2022 November,267 pulsars had been discovered in 36 globular clusters(GCs).In this paper,we present our studies on the distribution of GC pulsar parameters and the detection efficiency.The power law relation bet...
In a study that attempted to relate solar and human activity to Earth's recent temperature change,Connolly et al.committed a basic error in the choice of statistical methods and so overreported the effect of the Sun.A...
supported by the Natural Science Foundation of China(NSFC,Grant Nos.11733008,12090040,12090043,11521303,12125303);Yunnan Province and the National Tenthousand Talents Program;National Key R&D Program of China No.2019YFA0405500;the NSFC with Grant No.11835057;The Guoshoujing Telescope(the Large Sky Area MultiObject Fiber Spectroscopic Telescope,LAMOST)is a National Major Scientific Project built by the Chinese Academy of Sciences;Funding for the project has been provided by the National Development and Reform Commission;LAMOST is operated and managed by the National Astronomical Observatories,Chinese Academy of Sciences;supported by the Key Research Program of Frontier Sciences,CAS,Grant No.QYZDY-SSW-SLH007;the science research grants from the China Manned Space Project with No.CMS-CSST-2021-A10。
Massive binaries play significant roles in many fields.Identifying massive stars,particularly massive binaries,is of great importance.In this paper,by adopting the technique of measuring the equivalent widths of sever...
supported by the National Key R&D Program of China(Grant No.2017YFA0402704);the National Natural Science Foundation of China(Grant Nos.11803044 and 11933003);the China Manned Space Project with No.CMSCSST-2021-A05;sponsored(in part)by the Chinese Academy of Sciences(CAS);through a grant to the CAS South America Center for Astronomy(CASSACA)。
The Spitzer Extended Deep Survey(SEDS)as a deep and wide mid-infrared(MIR)survey project provides a sample of 500000+sources spreading 1.46 square degree and a depth of 26 AB mag(3σ).Combining with the previous avail...
supported by National Key R&D Program of China(No.2019YFA0405500);the National Natural Science Foundation of China(NSFC,Grant No.11835057);the State Natural Sciences Foundation Monumental Projects(Nos.12090040.Z.W.H,12090041.H.W.);The Guoshoujing Telescope(the Large Sky Area Multi-Object Fiber Spectroscopic Telescope,LAMOST)is a National Major Scientific Project built by the Chinese Academy of Sciencesprovided by the National Development and Reform Commission。
The Large Sky Area Multi-Object Fiber Spectroscopic Telescope(LAMOST)started a medianresolution spectroscopic(MRS,R~7500)survey since October 2018.The main scientific goals of MRS,including binary stars,pulsators and ...
supported by National Key R&D Program of China(Grant No.2019YFA0405502);the Key Research Program of the Chinese Academy of Sciences(Grant No.XDPB09-02);the National Natural Science Foundation of China(Grant Nos.11833006,11473033,11603037,11973049,and 11973052);the international partnership program’s key foreign cooperation project,Bureau of International Cooperation,Chinese Academy of Sciences(Grant No.114A32KYSB20160049);the Strategic Priority Research Program of Chinese Academy of Sciences(Grant No.XDB34020205);supported by the Astronomical Big Data Joint Research Center,co-founded by the National Astronomical Observatories,Chinese Academy of Sciences and Alibaba Cloud;partial support for this work from grant PHY 14-30152;Physics Frontier Center/JINA Center for the Evolution of the Element(JINA-CEE),awarded by the US National Science Foundation;partially supported by the Open Project Program of the Key Laboratory of Optical Astronomy,National Astronomical Observatories,Chinese Academy of Sciences;Funding for the project has been provided by the National Development and Reform Commission。
The abundance patterns of r-process-enhanced stars contain key information required to constrain the astrophysical site(s)of r-process nucleosynthesis,and to deepen our understanding of the chemical evolution of our G...