Photometric redshift versus spectroscopic redshift for each set of photometric redshifts, 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 solid black vertical-line indicates the cluster redshift obtained from the mean spectroscopic redshift distribution, while the dashed vertical-lines indicate the cluster lower and upper limits.