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Table 1.
Examples of the analysed parameters from the pyPipe3D VAC.
| Name | Unit | Description |
|---|---|---|
| O/HRe | dex | Oxygen abundance at the effective radius (Re) using the M13 O3N2-calibrator |
| Φbaryon | log(M⊙ kpc−1) | Baryonic gravitational potential at Re estimated as M⋆, phot/Re |
| M⋆, phot | log(M⊙) | Integrated stellar mass obtained from photometry |
| LW–[Z/H]Re | dex | Luminosity weighted (LW) stellar metallicity at Re, normalised to the solar value, |
| in logarithmic scale | ||
| MW–[Z/H]Re | dex | Mass weighted (MW) stellar metallicity at Re, normalised to the solar value, in |
| logarithmic scale | ||
| g − r | mag | g − r colour extracted from the NSA catalogue |
| T99–[Z/H]Re | dex | Stellar metallicity at Re, normalised to the solar value, in logarithmic scale at T99 |
| (look-back time at which the galaxy has formed 99% of its mass) | ||
| B − R | mag | B − R colour computed from the MaNGA data |
| T95–[Z/H]Re | dex | Stellar metallicity at Re, normalised to the solar value, in logarithmic scale at T95 |
| (look-back time at which the galaxy has formed 95% of its mass) | ||
| B − V | mag | B − V colour computed from the MaNGA data |
| AV, Re | mag | Dust attenuation in the V-band derived from the Hα/Hβ line ratio at Re |
Notes. The table only displays the most relevant analysed parameters (see Sect. 4.1, Fig. 2) from the pyPipe3D VAC. The complete list is provided in Appendix A. We refer to Sánchez et al. (2022) for more details of the derivation of the parameters.
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