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Erratum: “The Flare Catalog and the Flare Activity in the Kepler Mission” (2019, ApJS, 241, 29)

  • Authors: Huiqin Yang, and Jifeng Liu

2020 The Astrophysical Journal Supplement Series 250 25.

  • Provider: AAS Journals

Caption: Figure 9.

The flare activity of C stars as a function of the temperature. This figure comprises stars whose rotation periods are shorter than the corresponding period of the 30 Myr ischrone of the I sequence. The temperature range is 3000 < Teff < 6400. Most of those stars are C stars, although a small part of them may be I stars that are younger than 30 Myr. The green dashed line is a polynomial fitting and the red dashed line is a Gaussian fitting.

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