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Magnetic Activity in X-Ray Stars from eROSITA: Insights from the TESS and LAMOST Surveys

  • Authors: Lulu Xu, Li-yun Zhang, Yinpeng Wang, Tianhao Su, Xianming L. Han, Adriana M. Pires, Rui Guo, Xian Zhang, Prabhakar Misra, Qingfeng Pi, Hongpeng Lu

Lulu Xu et al 2026 The Astrophysical Journal Supplement Series 284 .

  • Provider: AAS Journals

Caption: Figure 11.

In the upper set of plots, the top left panel features an exposure count histogram, with a subplot presenting a cumulative bar chart of exposure counts. The top middle panel displays a δEWHα histogram, accompanied by a subplot showing an enlarged view of the region where δEWHα exceeds 0.4. The top right panel shows a histogram of the coefficient of variation for EWHα. Mirroring the layout and structure of the upper plots, the lower set utilizes medium-resolution data instead of low-resolution data. The third set of plots, also based on the medium-resolution sample, presents the relationships between the mean EWHα (〈EW〉) and its standard deviation (σEW) in the left panel, and between 〈EW〉 and σEW/〈EW〉 in the right panel. The red dots represent the median values within each bin.

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