Image Details

Choose export citation format:

Searching for Barium Stars from the LAMOST Spectra Using the Machine-learning Method: I

  • Authors: Fengyue Guo, Zhongding Cheng, Xiaoming Kong, Yatao Zhang, Yude Bu, Zhenping Yi, Bing Du, Jingchang Pan

Fengyue Guo et al 2023 The Astronomical Journal 165 .

  • Provider: AAS Journals

Caption: Figure 4.

Comparisons of the Sr abundances calculated by our work ([Sr/Fe]LGBM) and values determined from N19 ([Sr/Fe]N19). The yellow line represents that the predicted value is equal to the target value. The yellow dot represents the point at which ∣[Sr/Fe]4077 Å − [Sr/Fe]4215 Å∣ ≥ 0.5 in N19. The left shows the differences between [Sr/Fe]LGBM and [Sr/Fe]N19 in the prediction of 4077 Å (Sr II), and the right shows these differences in the prediction of 4215 Å (Sr II).

Other Images in This Article
Copyright and Terms & Conditions

Additional terms of reuse