supported by the National Natural Science Foundation of China (Grant Nos.12222304,12192220,and 12192221);supported by the Guangxi Natural Science Foundation (Grant No.2024GXNSFDA010069);the National Natural Science Foundation of China (Grant No.12073007);the Scientific Research Project of Guangxi University for Nationalities (Grant No.2018KJQD01);the research grants from the China Manned Space Project (Grant Nos.CMSCSST-2021-A06,and CMSCSST-2021-A07);the National Natural Science Foundation of China (Grant No.11421303);the Fundamental Research Funds for the Central Universities (Grant No.WK3440000005);the K.C.Wong Education Foundation;supported by the National Science Foundation of China (Grant Nos.11721303,11991052,12011540375,and 12233001);the National Key R&D Program of China (Grant No.2022YFF0503401);the China Manned Space Project (Grant Nos.CMS-CSST-2021-A04,and CMS-CSST-2021-A06);supported by the National Science Foundation of China (Grant No.12033006);provided by the Alfred P.Sloan Foundation;the U.S.Department of Energy Office of Science,and the Participating Institutions;support and resources from the Center for High Performance Computing at the University of Utah。
Galactic-scale outflows driven by active galactic nuclei(AGNs) represent a commonly invoked feedback mechanism within galaxy evolution models.However,the interactions among interstellar gas on galactic scales,the prop...
Since the discovery of quasars in the 1960s,people have been curious and confused about quasars’characteristics such as high brightness,long distance,large redshift,high energy and wide spectral lines.Until the mid-1...
supported by the Youth Innovation Promotion Association CAS with Certificate Number 2022259;the grants from the Natural Science Foundation of Shanghai through grant 21ZR1474100;the National Natural Science Foundation of China(NSFC)through grants 12173069,and 11703065;the science research grants from the China Manned Space Project with NO.CMS-CSST-2021-A12 and NO.CMS-CSST-2021-B10。
Quasars are very important in materializing the reference frame.The excess emission of active galactic nuclei(AGNs) in the mid-infrared band can be used to identify quasar candidates.As extremely distant and point-lik...
science research grants from the China Manned Space Project with No.CMS-CSST-2021-A01。
Quasars can be used to measure baryon acoustic oscillations at high redshift, which are considered as direct tracers of the most distant large-scale structures in the universe. It is fundamental to select quasars from...
the support for this work from the National Key R&D Program of China under Grant No.2018YFA0404204;the National Natural Science Foundation of China(NSFC U1931113 and U1738211);the Foundations of Yunnan Province(2018IC059 and 2018FY001(-003));the scientific research fund of Yunnan Education Department(2020Y0039)。
The unknown γ-ray excess in the northwest region of Arp 220 was revisited by analyzing~11.8 years of the Fermi Large Area Telescope(Fermi-LAT) data in this study.We found that its photon flux was approximately three ...
The commonly held view by astronomers and cosmologists is that redshift indicates distance for both galaxies and quasars. However, data from over 750,000 quasars, and specifically about 9500 with high accuracy measure...