Image Details

Choose export citation format:

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 2.

Left: examples of phase-folded LCs with different significance (Sgnf, see Equation (1)). Different rotation cycles are highlighted in distinct colors. Right: the corresponding spectral analysis results. For each target, the LAMOST spectrum, VAE template, and residual spectrum + 1.05 are plotted as blue, red, and black lines, respectively, overlaid by horizontal red dotted lines at 1.00 and 1.05 and vertical black dotted lines denoting the Hα and Li I line centers.

Other Images in This Article
Copyright and Terms & Conditions

Additional terms of reuse