Footprints of the FoVs covered by the HST observations listed in Table 1. The underlying stars come from the Gaia DR3 dataset (Gaia Collaboration 2023) centred on NGC 362, obtained with a search radius of 1 degree and using the Gaia G-band magnitude to scale the size of the data points. Each FoV is colour-coded according to the GO proposal number, listed in Table 1. The black cross marks the centre (RA = 15.8087453, Dec = −70.8489012, Dalessandro et al. 2013) while the black circle represents the half-mass radius, r_h (63^′′.5, Dalessandro et al. 2013).