Plot of proper eccentricity vs. proper semi-major axis (left) for the members of asteroid dynamical families taken from the list of Milani et al. (2014), also available on the AstDyS web site. The sub-sample of family members whose Gaia DR3 photometric data pass the solution rejection filter described in this paper is displayed using a colour code to indicate their resulting sense of rotation. Right: the same, but for sine of proper inclination vs. proper semi-major axis. In these plots, red points indicate family members displaying retrograde sense of rotation, while blue symbols are used for objects displaying prograde rotation, according to the results of photometric inversion. Black symbols are used for family members for which we have not obtained a photometric inversion.