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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 15.

A few typical examples that exhibit abnormal residuals between the LAMOST spectrum and the PCA reconstruction. The top panel shows a spectrum with problematic fluxes over the wavelength range of λ4700–5000 Å, leading to poor PCA reconstruction. The middle panel shows a spectrum with artifacts in the LAMOST spectra across λ5000–7000 Å. The PCA reconstruction is visually reasonable, but the χ2 between the LAMOST and PCA-reconstructed spectra is suboptimal. The bottom panel shows a spectrum that has a problematic wavelength calibration from the LAMOST pipeline in the wavelength range of λ5800–7000 Å.

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