Zoomed-in view of CMD of NGC 2516 showing how binarity and rotation lead a star deviating from the main sequence. The ranges of the x- and y-axes are 0.2 mag < G_BP − G_RP < 0.6 mag and 2.0 mag < M_G < 3.5 mag. The stars are colour-coded by RUWE (showing binarity) and line broadening (representing rotation rates), respectively. The small black dots are stars without broadening values in the Gaia DR3 database.