基于网格聚类分析LAMOST恒星光谱与理论模型的差异
[1] Cui X Q, Zhao Y H, Chu Y Q, et al. RAA, 2012, 12(9): 1197.
[2] GUO Ping, WANG Ke, LUO A-li, et al(郭 平, 王 可, 罗阿理, 等). Journal of Software(软件学报), 2015, 26(11): 3012.
[3] CUI Chen-zhou, YU Ce, XIAO Jian, et al(崔辰州, 于 策, 肖 健, 等). Chinese Science Bulletin(科学通报), 2015, 60(5-6): 447.
[4] Luo A L, Zhao Y H, Zhao G, et al. RAA, 2015, 15(8): 1095.
[5] Prieto C A, Beers T C, Wilhelm R, et al. The Astrophysical Journal, 2006, 636(2): 804.
[6] LI Hua-nan, XIAO Quan-bao, SHAO Zheng-yi(李化南, 肖泉宝, 邵正义). Annals of Shanghai Astronomical Observatory, Chinese Academy of Sciences(中国科学院上海天文台年刊), 2006, 26: 119.
[7] TU Liang-ping, WEI Hui-ming, WANG Zhi-heng, et al(屠良平, 魏会明, 王志衡, 等). Spectroscopy and Spectral Analysis(光谱学与光谱分析), 2015, 35(4): 1104.
[8] DING Yue-rong(丁月蓉). Astronomical Data Processing Methods(天文数据处理方法). Nanjing: Nanjing University Press(南京: 南京大学出版社), 1998. 88.
[9] Castelli F, Kurucz R L. Proc. of IAU Symp. 210, Modelling of Stellar Atonspheres, Poster A20, 2003, astro-ph/0405087.
陈淑鑫, 孙伟民, 孔啸. 基于网格聚类分析LAMOST恒星光谱与理论模型的差异[J]. 光谱学与光谱分析, 2017, 37(6): 1951. CHEN Shu-xin, SUN Wei-min, KONG Xiao. Difference Analysis of LAMOST Stellar Spectrum and Kurucz Model Based on Grid Clustering[J]. Spectroscopy and Spectral Analysis, 2017, 37(6): 1951.