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supported by the Astronomical Project for the Chinese Antarctic Inland Station;the SOC Program(CHINARE2012-02-03;CHINARE2013-02-03;CHINARE2014-02-03;and CHINARE2015-02-03);the National Basic Research Program of China(2013CB834905 and 2015CB857005);Q.Tian is supported by the National Natural Science Foundation of China(11503023);the Natural Science Foundation of Shanghai(14ZR1444100);the Polar Science Innovation Fund for Young Scientists of Polar Research Institute of China(CX20130201);P.Jiang is supported by the National Natural Science Foundation of China(11233002 and11203022);H.Zhou is supported by the National Natural Science Foundation of China(11473025;11421303 and 11033007);S.Zhang is supported by the National Natural Science Foundation of China(11573024);T.Ji is supported by the National Natural Science Foundation of China(11503022);the Natural Science Foundation of Shanghai(15ZR1444200)
Transiting extrasolar planets(exoplanets),especially those orbiting bright stars, are desired for study of the diversity of planetary compositions, internal structures and atmospheres beyond our solar system. Dome A a...
ASTEROSEISMOLOGY of pulsating white dwarfs is an effective tool for us to infer their internal structures and the activities of stars on the final stages of stellar evolution. DA-type pulsating white dwarfs, with hydr...
Monochromatic photometry of comets is one of the important methods for investigating gasses and dust of comets. Because comets often are very faint, the observations of them are quite difficult; and in addition, the d...
Photographic observations of several comets were undertaken at the Zo-So Observatory (at present the Sheshan Station of Shanghai Observatory) around 1910, and Comet Halley was one of them. Those original data are not ...