Members of the cluster obtained in Sect. 2 coloured by membership probability. Spectroscopic targets are marked with black circles. From left to right: proper motions distribution, proper motion-parallax distribution, spatial distribution in equatorial coordinates, and CMD in the Gaia EDR3 passbands. The isochrone from the PARSEC database (Bressan et al. 2012) of the cluster age and metallicity (2.5 Gyr and [M/H] = −0.1 as derived in Sect. 4.1 and shifted by d = 1778 pc and E_{(B − V)} = 0.12) is overplotted in the CMD to guide the eye.