CMD 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 bright-faint boundary at m_r = 18.5 is indicated by a vertical dotted line. The different CMDs evidence the out-striking differences of the selected cluster galaxy candidate members, specially at fainter magnitudes (m_r ≥ 18.5), where only T80S/S-PLUS- and LS-DR10-CBPF-z_phot effectively populate the red faint regime (m_g − m_r > 0.5).