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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 5.

Comparisons of the Ba abundances calculated by our work ([Ba/Fe]LGBM) and values determined from N19 ([Ba/Fe]N19). The yellow line signifies that the predicted value is equal to the target value. The yellow dot represents the point at which ∣[Ba/Fe]4554 Å − [Ba/Fe]4934 Å∣ ≥ 0.5 in N19. The left shows the differences between [Ba/Fe]LGBM and [Ba/Fe]N19 in the prediction of 4554 Å (Ba II), and the right shows these differences in the prediction of 4934 Å (Ba II).

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