Spatial distribution of the A0085 galaxy cluster candidate members using our target selection process for the four different parent catalogues used, from left to right: T80S/S-PLUS, LS-DR9, LS-DR10 and LS-DR10-CBPF. We include the corresponding parent sample(grey circles), the A0085 galaxy cluster candidate members selected from our photometric method (blue), the spectroscopically confirmed members (yellow circles), and the confirmed spectroscopic cluster members and spectroscopic objects within the cluster redshift range (yellow crosses) that were not selected by our method. The cluster galaxy candidate members of the four different z_phot are homogeneously distributed and any significant differences are appreciated.