Figure 6 from The Largest M Dwarf Flares from ASAS-SN

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The Largest M Dwarf Flares from ASAS-SN

Authors: Sarah J. Schmidt, Benjamin J. Shappee, Jennifer L. van Saders, K.Z. Stanek, Jonathan S. Brown, C.S. Kochanek, Subo Dong, Maria R. Drout, Stephan Frank, T.W.-S. Holoien, Sean Johnson, Barry F. Madore, J.L. Prieto, Mark Seibert, Marja K. Seidel, and Gregory V.A. Simonian

2019 The Astrophysical Journal 876 115.

Provider: AAS Journals

Caption: Figure 6.

Fraction of M dwarfs with activity (as defined by the presence of Hα emission) for the ASAS-SN flare dwarfs (black) compared to a sample selected based on colors (SDSS DR7 M dwarf and BUD ML dwarf samples; gray; West et al. 2011; Schmidt et al. 2015). The uncertainties are based on a binomial distribution. While the ASAS-SN flare sample is much smaller, it does also have a higher significantly active fraction than the comparison dwarfs.

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