eRASSl X-ray sources in the fourth galactic quadrant between −10° < b < 30°. The nominal regions of the Sco-Cen subgroups as defined by Preibisch & Mamajek (2008) are indicated. The colored sources indicates the sources identified with Gaia stars in the distance range 60–200 pc. Blue sources indicate US member candidates, red sources show UCC member candidates, and green sources represent LCC member candidates. Typical eRASS1 position errors are 4 arcsec.