The Flaring Activity Of M Dwarfs In Kepler Field
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The Kepler flux, M dwarfs that include flares,the format consist of four columns:<br> <br> BKJD Relative Flux Fit line Flare Flux the Relative flux wil be empty when flares occur, the flares flux will be empty when quiescent flux. the file lamost_obsid is the spectra used in this work, one can use the obsid to download the fits through the following website: http://dr4.lamost.org/
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Zenodo创建时间：
2017-09-20
