Histogram of derived astrophysical parameters for our sample BSSs. Top, middle and bottom left panels are the distributions for effective temperatures derived from color-temperature relations, isochrone fittings, and the XPP method (from Gaia DR3 spectroscopy, if available), respectively. Top, middle and bottom right panels are the distributions obtained from isochrone fitting, for BSS ages, luminosities and masses, respectively. GCs are denoted as a red dotted-dashed line, OCs as a dashed blue line and the distribution for all clusters (GCs + OCs) is depicted as a solid green line.