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Identifying Active Young Stars from the LAMOST MRS and TESS Survey

  • Authors: Fu-Kun Xu, Shenghong Gu, Yue Xiang

Fu-Kun Xu et al 2026 The Astrophysical Journal Supplement Series 287 .

  • Provider: AAS Journals

Caption: Figure 1.

Identifying spectral discontinuity. Spectra are excluded if ﹩{\rm{\max }}(\left|{\rm{\Delta }}f/p\right|)\gt 1.4﹩ (the red dotted lines), where Δf is the difference of flux f between adjacent points and p is the pixel size (p ∼ 0.16 Å for LAMOST MRS). The left panel shows the max(﹩\left|{\rm{\Delta }}f/p\right|﹩) over 4950–5350 and 6350–6750 Å versus the SNR. The right panels present example spectra with series of max(﹩\left|{\rm{\Delta }}f/p\right|﹩) values.

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