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Data-driven Spectroscopic Estimates of Absolute Magnitude, Distance, and Binarity: Method and Catalog of 16,002 O- and B-type Stars from LAMOST

  • Authors: Mao-Sheng Xiang, Hans-Walter Rix, Yuan-Sen Ting, Eleonora Zari, Kareem El-Badry, Hai-Bo Yuan, and Wen-Yuan Cui

2021 The Astrophysical Journal Supplement Series 253 22.

  • Provider: AAS Journals

Caption: Figure 8.

MCMC fitting of the intrinsic uncertainty and measurement uncertainty in our ﹩{M}_{K{\rm{s}}}﹩ estimates. Binaries were excluded iteratively. The intrinsic uncertainty σint indicates the epistemic uncertainty in ﹩{M}_{K{\rm{s}}}﹩ estimates, whereas the measurement uncertainty σs quantifies the aleatoric uncertainty induced by spectral noise. The MCMC results show an intrinsic uncertainty of σint = 0.25 mag and a typical measurement uncertainty of σs = 0.10 mag at S/N = 100.

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