Distribution of Gaia distances from (Bailer-Jones et al. 2018) and spectral types calculated from G_bp – G_rp. Top panel: gray histogram is the distribution for the stars from LG11-Gaia in the eFEDS fields. The green contours represent the distance and SpT distribution for those stars observed by TESS. We show the CPM pairs in yellow. Bottom panel: stars from the LG11-Gaia sample identified in the preliminary eRASS1 catalog. For simplicity, we do not show the four CPM pairs here because they represent only 4% of the sample.