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The Connection between Flares and Starspots on M Dwarfs Based on TESS Photometry

  • Authors: Chunxiang Wang, Jiaxin Wang, Yanjun He, Heyu Sun, Yu Pan, Xianju Zhou, Shichang Li, Yirong Ma

Chunxiang Wang et al 2026 The Astrophysical Journal Supplement Series 287 .

  • Provider: AAS Journals

Caption: Figure 6.

FFD for the detected M dwarf flares. The hollow circles represent the incomplete sample at lower energies, while the solid circles denote the high-completeness sample used for the fit. The blue dashed line indicates the best-fit power law with an index of α = 2.11 in the high-completeness regime (E > 1034 erg). The gray dotted line marks the fit cutoff.

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