Comparison between quantities for a sample of 18 massive quiescent galaxies from Baker et al. (2025a) compared with our work. Upper left: comparison of our photometric EAZY redshifts versus the spectroscopic redshifts. Lower left: comparison of photometric redshifts from EAZY and those from BAGPIPES. Upper middle: comparison between the stellar masses obtained via photometric fitting with bagpipes and those from combined spectrophotometric fitting. Lower middle: comparison between the stellar masses obtained from photometry with BAGPIPES vs EAZY. Upper right: comparison of the formation times (t₅₀) and lower right a comparison of the quenching times (t₉₀).