Searching for hot subdwarf stars from the LAMOST Spectra. II. Pure spectroscopic identification method for hot subdwarfs-Reference-Cited by-同舟云学术

Searching for hot subdwarf stars from the LAMOST Spectra. II. Pure spectroscopic identification method for hot subdwarfs

Author:

Lei Zhenxin¹²,Bu Yude³,Zhao Jingkun¹,Németh Péter⁴⁵,Zhao Gang¹

Affiliation:

1. Key Laboratory of Optical Astronomy, National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100012, China

2. College of Science, Shaoyang University, Shaoyang 422000, China

3. School of Mathematics and Statistics, Shandong University, Weihai, 264209, Shandong, China

4. Astronomical Institute of the Czech Academy of Sciences, CZ-251 65, Ondřejov, Czech Republic

5. Astroserver.org, 8533 Malomsok, Hungary

Funder

National Natural Science Foundation of China

Natural Science Foundation of Hunan province

Youth Fund project of Hunan Provincial Education Department

Chinese Academy of Sciences

Young Scholars Program of Shandong University, Weihai

Natural Science Foundation of Shandong Province

China post-doctoral Science Foundation

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

Reference59 articles.

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