First eROSITA study of nearby M dwarfs and the rotation-activity relation in combination with TESS

The Early Data Release of eROSITA and Mikhail Pavlinsky ART-XC on the SRG mission

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Fig. 12

Comparison between X-ray luminosities observed during eFEDS (log L_x,eFEDs) and eRASS1 (log L_x,eRAss1). L_x,eRAss1 is more than twice higher than L_x,eFEDS for the two stars above the dashed red line.

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