supported by the National Natural Science Foundation of China(Grant Nos.11533003,11673006,U1331202,U1931133 and U1938201);the Guangxi Science Foundation(2016GXNSFFA380006,AD17129006and 2018GXNSFGA281007);the Strategic Priority Research Program of the Chinese Academy of Sciences(XDB23040000);the Strategic Pioneer Program on Space Science,Chinese Academy of Sciences(XDA15052600);financial support from the Chinese Academy of Sciences PIFI post-doctoral fellowship program(program C);financial support of the Univ Earth S Labex program at Sorbonne Paris Cité(ANR-10-LABX-0023 and ANR-11-IDEX-0005-02)
The second(O2)observational campaign of gravitational waves(GWs)organized by the LIGO/Virgo Collaborations has led to several breakthroughs such as the detection of GW signals from merger systems involving black holes...
supported by the Strategic Priority Research Program “The Emergence of Cosmological Structures” of the Chinese Academy of Sciences (Grant No. XDB09000000);the National Key Basic Research Program of China (Grant 2014CB845700);the National Natural Science Foundation of China (NSFC, Grant Nos. 11503012, U1331202 and U1731124);NSFC (Grant Nos. 11373032 and 11333003);NSFC (Grant Nos. 11390372 and 11633004);NSFC (Grant No. 11403056);The Guo Shou Jing Telescope (the Large Sky Area Multi-Object 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 National Astronomical Observatories, Chinese Academy of Sciences
We present the peculiar in-plane velocities derived from LAMOST red clump stars, which are purified and separated by a novel approach into two groups with different ages. The samples are mostly contributed around the ...
supported by the National Basic Research Program of China (973 program,2014CB845800);the National Natural Science Foundation of China (NSFC,Grant No.U1331202);the NSFC (Nos.11103036 and U1331101);supported by the NSFC (No.U1231115)
We report the optical observations of GRB 121011 A by the 0.8m TNT facility at Xinglong observatory, China. The light curve of the optical afterglow shows a smooth and featureless bump during the epoch of;30 s and;000...