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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Table 1

Number of stars in the different samples of main-sequence M dwarfs.

Sample name	‘full’	‘validated’
LG11-Gaia	8229	7319
LG11-Gaia/eFEDS	14	13
LG11-Gaia/eRASS1	673	580
LG11-Gaia/eFEDS/TESS ⁽¹⁾	3	3
LG11-Gaia/eRASS1/TESS ⁽¹⁾	172	135

Notes. See Sects. 3, 4.2, and 5.2 for the definitions. ⁽¹⁾Only stars with reliable TESS rotation period are included in these samples.

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