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Table A.1.
Parameters extracted from the pyPipe3D VAC included in the analysis.
| Name | Unit | Description |
|---|---|---|
| mangaid | – | MaNGA ID |
| log_SFR_Hα | log(M⊙ yr−1) | Integrated star-formation rate derived from the integrate Hα luminosity |
| FoV | – | Ratio between the diagonal radius of the cube and Re |
| Re_kpc | kpc | Effective radius in kpc |
| log_Mass | log(M⊙) | Integrated stellar mass in units of the solar mass in logarithm scale |
| log_SFR_ssp | log(M⊙ yr−1) | Integrated SFR derived from the SSP analysis t< 32Myr |
| ZH_LW_Re_fit | dex | LW metallicity of the stellar population at Re, normalised to the solar value, |
| in logarithm scales | ||
| alpha_ZH_LW_Re_fit | dex/Re | Slope of the gradient of the LW metallicity of the stellar population |
| ZH_MW_Re_fit | dex | MW metallicity of the stellar population at Re, normalised to the solar value, |
| in logarithm scales | ||
| alpha_ZH_MW_Re_fit | dex/Re | Slope of the gradient of the MW log-metallicity of the stellar population |
| Age_LW_Re_fit | log(yr) | Luminosity weighted age of the stellar population in logarithm scale |
| alpha_Age_LW_Re_fit | log(yr)/Re | Slope of the gradient of the LW log-age of the stellar population |
| Age_MW_Re_fit | log(yr) | Mass weighted age of the stellar population in logarithm |
| alpha_Age_MW_Re_fit | log(yr)/Re | Slope of the gradient of the MW log-age of the stellar population |
| Re_arc | arcsec | Adopted effective radius in arcsec |
| DL | Mpc | Adopted luminosity distance |
| DA | Mpc | Adopted angular-diameter distance |
| PA | degrees | Adopted position angle in degrees |
| ellip | – | Adopted ellipticity |
| log_Mass_gas | log(M⊙) | Integrated gas mass in units of the solar mass in logarithm scale |
| vel_sigma_Re | – | Velocity/dispersion ratio for the stellar populations within 1.5 Re |
| log_SFR_SF | log(M⊙ yr−1) | Integrated SFR using only the spaxels compatible with SF |
| log_SFR_D_C | log(M⊙ yr−1) | Integrated SFR diffuse corrected |
| Sigma_Mass_cen | log(M⊙ pc−2) | Stellar Mass surface density in the central aperture |
| Sigma_Mass_Re | log(M⊙ pc−2) | Stellar Mass surface density at 1Re |
| Sigma_Mass_ALL | log(M⊙ pc−2) | Average Stellar Mass surface density within the entire FoV |
| T30 | Gyr | Lookback time at which the galaxy has formed 30% of its stellar mass |
| ZH_T30 | dex | Stellar metallicity, normalised by the solar value, in logarithm-scale at T30 time |
| ZH_Re_T30 | dex | Stellar metallicity, normalised by the solar value, in logarithm-scale at Re at T30 time |
| a_ZH_T30 | dex/Re | Slope of the ZH gradient at T30 time |
| T40 | Gyr | Lookback time at which the galaxy has formed 40% of its stellar mass |
| ZH_T40 | dex | Stellar metallicity, normalised by the solar value, in logarithm-scale at T40 time |
| ZH_Re_T40 | dex | Stellar metallicity, normalised by the solar value, in logarithm-scale at Re at T40 time |
| a_ZH_T40 | dex/Re | Slope of the ZH gradient at T40 time |
| T50 | Gyr | Lookback time at which the galaxy has formed 50% of its stellar mass |
| ZH_T50 | dex | Stellar metallicity, normalised by the solar value, in logarithm-scale at T50 time |
| ZH_Re_T50 | dex | Stellar metallicity, normalised by the solar value, in logarithm-scale at Re at T50 time |
| a_ZH_T50 | dex/Re | Slope of the ZH gradient at T50 time |
| T60 | Gyr | Lookback time at which the galaxy has formed 60% of its stellar mass |
| ZH_T60 | dex | Stellar metallicity, normalised by the solar value, in logarithm-scale at T60 time |
| ZH_Re_T60 | dex | Stellar metallicity, normalised by the solar value, in logarithm-scale at Re at T60 time |
| a_ZH_T60 | dex/Re | Slope of the ZH gradient at T60 time |
| T70 | Gyr | Lookback time at which the galaxy has formed 70% of its stellar mass |
| ZH_T70 | dex | Stellar metallicity, normalized by the solar value, in logarithm-scale at T70 time |
| ZH_Re_T70 | dex | Stellar metallicity, normalized by the solar value, in logarithm-scale at Re at T70 time |
| a_ZH_T70 | dex/Re | Slope of the ZH gradient at T70 time |
| T80 | Gyr | Lookback time at which the galaxy has formed 80% of its stellar mass |
| ZH_T80 | dex | Stellar metallicity, normalized by the solar value, in logarithm-scale at T80 time |
| ZH_Re_T80 | dex | Stellar metallicity, normalized by the solar value, in logarithm-scale at Re at T80 time |
| a_ZH_T80 | dex/Re | Slope of the ZH gradient at T80 time |
| T90 | Gyr | Lookback time at which the galaxy has formed 90% of its stellar mass |
| ZH_T90 | dex | Stellar metallicity, normalized by the solar value, in logarithm-scale at T90 time |
| ZH_Re_T90 | dex | Stellar metallicity, normalized by the solar value, in logarithm-scale at Re at T90 time |
| a_ZH_T90 | dex/Re | Slope of the ZH gradient at T90 time |
| T95 | Gyr | Lookback time at which the galaxy has formed 95% of its stellar mass |
| ZH_T95 | dex | Stellar metallicity, normalized by the solar value, in logarithm-scale at T95 time |
| ZH_Re_T95 | dex | Stellar metallicity, normalised by the solar value, in logarithm-scale at Re |
| at T95 time | ||
| a_ZH_T95 | dex/Re | Slope of the ZH gradient at T95 time |
| T99 | Gyr | Lookback time at which the galaxy has formed 99% of its stellar mass |
| ZH_T99 | dex | Stellar metallicity, normalised by the solar value, in logarithm-scale at T99 time |
| ZH_Re_T99 | dex | Stellar metallicity, normalised by the solar value, in logarithm-scale at Re |
| at T99 time | ||
| a_ZH_T99 | dex/Re | Slope of the ZH gradient at T99 time |
| log_Mass_gas_Av_gas_OH | log(M⊙) | Integrated gas mass using the calibrator log_Mass_gas_Av_gas_OH, |
| in logarithm-scale | ||
| log_Mass_gas_Av_ssp_OH | log(M⊙) | Integrated gas mass using the calibrator log_Mass_gas_Av_ssp_OH, |
| in logarithm-scale | ||
| vel_ssp_2 | km s−1 | Stellar velocity at 2 Re |
| vel_Ha_2 | km s−1 | Hα velocity at 2 Re |
| vel_ssp_1 | km s−1 | Stellar velocity at 1 Re |
| vel_Ha_1 | km/s | Hα velocity at 1 Re |
| log_SFR_ssp_100Myr | log(M⊙ yr−1) | Integrated SFR derived from the SSP analysis for t< 100Myr |
| log_SFR_ssp_10Myr | log(M⊙ yr−1) | Integrated SFR derived from the SSP analysis for t< 10Myr |
| vel_disp_Ha_cen | km/s | Hα Velocity dispersion at the central aperture |
| vel_disp_ssp_cen | km/s | Stellar velocity dispersion at the central aperture |
| vel_disp_Ha_1Re | km/s | Hα velocity dispersion at 1 Re |
| vel_disp_ssp_1Re | km/s | Stellar velocity dispersion at 1 Re |
| log_Mass_in_Re | log(M⊙) | Integrated stellar mass within one optical Re |
| ML_int | M⊙/L⊙ | V-band mass-to-light ratio from integrated quantities |
| ML_avg | M⊙/L⊙ | V-band mass-to-light ratio averaged across the FoV |
| R50_kpc_V | kpc | Radius at which it is integrated half of the light in the V-band within the FoV |
| R50_kpc_Mass | kpc | Radius at which is integrated half of the stellar mass within the FoV |
| log_Mass_corr_in_R50_V | log(M⊙) | Integrated stellar mass within R50_kpc_V |
| log_Mass_gas_Av_gas_log_log | log(M⊙) | Molecular gas mass derived from the dust extinction using the log-log calibration |
| Av_gas_Re | mag | Dust extinction in the V-band derived from the Hα/Hβ line ratio at 1 Re |
| Av_ssp_Re | mag | Dust extinction in the V-band derived from the analysis of the stellar population |
| Lambda_Re | – | Specific angular momentum (λ-parameter) for the stellar populations within 1 Re |
| nsa_redshift | – | Redshift derived by the NSA collaboration |
| nsa_mstar | log(M⊙) | Stellar Mass derived by the NSA collaboration |
| nsa_inclination | deg | Inclination derived by the NSA collaboration |
| O/H_Re | dex | Oxygen abundance at the effective radius (Re) using the M13 O3N2-calibrator or |
| one of the alternative calibrators described in Table B.1 | ||
| OH_alpha_fit | dex/Re | Slope of the O/H gradient using the same calibrator adopted for the |
| oxygen abundance determination | ||
| Ne_Oster_S_Re_fit | dex | Electron density using the Oster_S estimator at 1Re |
| Ne_Oster_S_alpha_fit | dex/Re | Slope of the n_e gradient using the Oster_S estimator |
| Hd_Re_fit | Å | Value of the Hd stellar index at 1Re |
| Hd_alpha_fit | Å/Re | Slope of the gradient of the Hd index |
| Hb_Re_fit | Å | Value of the Hβ stellar index at 1Re |
| Hb_alpha_fit | Å/Re | Slope of the gradient of the Hβ index |
| Mgb_Re_fit | Å | Value of the Mgb stellar index at 1Re |
| Mgb_alpha_fit | Å/Re | Slope of the gradient of the Mgb index |
| Fe5270_Re_fit | Å | Value of the Fe5270 stellar index at 1Re |
| Fe5270_alpha_fit | Å/Re | Slope of the gradient of the Fe5270 index |
| Fe5335_Re_fit | Å | Value of the Fe5335 stellar index at 1Re |
| Fe5335_alpha_fit | Å/Re | Slope of the gradient of the Fe5335 index |
| D4000_Re_fit1 | – | Value of the D4000 stellar index at 1Re |
| D4000_alpha_fit | – | Slope of the gradient of the D4000 index |
| Hdmod_Re_fit | Å | Value of the Hdmod stellar index at 1Re |
| Hdmod_alpha_fit | Å/Re | Slope of the gradient of the Hdmod index |
| Hg_Re_fit | Å | Value of the Hg stellar index at 1Re |
| Hg_alpha_fit | Å/Re | Slope of the gradient of the Hg index |
| u_band_mag | mag | u-band magnitude derived from the original cube |
| u_band_abs_mag | mag | u-band absolute magnitude derived from the original cube |
| g_band_mag | mag | g-band magnitude derived from the original cube |
| g_band_abs_mag | mag | g-band abs. magnitude derived from the original cube |
| r_band_mag | mag | r-band magnitude derived from the original cube |
| r_band_abs_mag | mag | r-band abs. magnitude derived from the original cube |
| i_band_mag | mag | i-band magnitude derived from the original cube |
| i_band_abs_mag | mag | i-band abs. magnitude derived from the original cube |
| B_band_mag | mag | B-band magnitude derived from the original cube |
| B_band_abs_mag | mag | B-band abs. magnitude derived from the original cube |
| V_band_mag | mag | V-band magnitude derived from the original cube |
| V_band_abs_mag | mag | V-band abs. magnitude derived from the original cube |
| RJ_band_mag | mag | R-band magnitude derived from the original cube |
| RJ_band_abs_mag | mag | R-band abs. magnitude derived from the original cube |
| R50 | arcsec | Radius at which it is integrated half of the light within the FoV in the g-band |
| R90 | arcsec | Radius at which it is integrated 90% of the light within the FoV in the g-band |
| C | – | R90/R50 concentration index |
| B-V | mag | B-V color |
| B-R | mag | B-R color |
| log_Mass_phot | log(M⊙) | stellar masses derived from the photometric data within the FoV |
| V-band_SB_at_Re | mag/arcsec2 | V-band surface brightness at 1Re |
| V-band_SB_at_R_50 | mag/arcsec2 | V-band surface brightness at R50 |
| nsa_sersic_n_morph | – | NSA sersic index |
| u-g | mag | u-g NSA color |
| g-r | mag | g-r NSA color |
| r-i | mag | r-i NSA color |
| i-z | mag | i-z NSA color |
| P(CD) | – | Probability of being a CD galaxy |
| P(E) | – | Probability of being a E galaxy |
| P(S0) | – | Probability of being a S0 galaxy |
| P(Sa) | – | Probability of being a Sa galaxy |
| P(Sab) | – | Probability of being a Sab galaxy |
| P(Sb) | – | Probability of being a Sb galaxy |
| P(Sbc) | – | Probability of being a Sbc galaxy |
| P(Sc) | – | Probability of being a Sc galaxy |
| P(Scd) | – | Probability of being a Scd galaxy |
| P(Sd) | – | Probability of being a Sd galaxy |
| P(Sdm) | – | Probability of being a Sdm galaxy |
| P(Sm) | – | Probability of being a Sm galaxy |
| P(Irr) | – | Probability of being a Irr galaxy |
| best_type_n | – | Best morphological type index based on the NN analysis |
| Φbaryon | log(M⊙ kpc−1) | Baryonic gravitational potential at Re estimated as M⋆, phot/Re |
| Σ⋆ | log(M⊙ kpc−2) | Average stellar mass surface density within Re estimated as  |
Notes. The MaNGA ID is included in the table only for identification. We refer to Sánchez et al. (2022) for more details of the derivation of the parameters.
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