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An Empirical Template Library for FGK and Late-type A Stars Using LAMOST Observed Spectra

  • Authors: Bing Du, A-Li Luo, F. Zuo, Z-R. Bai, R. Wang, Y-H. Song, W. Hou, Y-B. Li, J-N. Zhang, Y-X. Guo, J-J. Chen, M-X. Wang, Y-F. Wang, X. Kong, K-F. Wu, X. Wang, Y. Wu, Y.-H Hou, and Y-H. Zhao

2019 The Astrophysical Journal Supplement Series 240 10.

  • Provider: AAS Journals

Caption: Figure 19.

Distributions of the uncertainty levels of this library and LASP in the Teff bins in steps of 150 K, left: Teff uncertainty levels; middle: [Fe/H] uncertainty levels; right: log g uncertainty levels. The blue (red) lines represent the results of LASP (our library), whereas the solid (dashed) lines represent the results of roughly dwarfs (giants).

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