Resolved mass-metallicity relation using intrinsic values from the CIELO simulations (black solid lines) and the calibrations of N2, R23, $\hat{\mathrm{R}}$, N2O2, and O3N2 provided by PRISMA considering the sample of spectra non-attenuated by ISM dust (blue dashed lines) and the ISM dust-attenuated spectra considering the Calzetti law (pink dashed lines). The shaded regions are delimited by the 25–75th percentiles. The yellow, dashed line in the O3N2 panel shows the observational results from Barrera-Ballesteros et al. (2016) using MaNGA galaxies (where the error bar cores correspond to the standard deviations).