Image Details
Caption: Figure 7.
Average FFD, combining all available quarters of Kepler data, for stars in the six g − i color bins defined in Davenport (2016a). Each track is colored as a function of the measured rotation period from McQuillan et al. (2014). A clear and coherent decrease in the total flare rates is observed as stars slow down (age) within each panel.
© 2019. The American Astronomical Society.