Flare occultations observed with optical photometry can constrain the latitude of M dwarf flares, with an estimated 3 to 22 detectable events expected in existing TESS data.
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Identifying Flare Locations Through Exoplanet Transit Occultations
Flare occultations observed with optical photometry can constrain the latitude of M dwarf flares, with an estimated 3 to 22 detectable events expected in existing TESS data.