Table 5.
Properties of the stellar populations of the sample obtained by FADO using the new SSP models.
| MaNGA Id | log M* | 〈log(τ)〉L | 〈log(τ)〉M | 〈log(Z/Z⊙)〉L | 〈log(Z/Z⊙)〉M |
|---|---|---|---|---|---|
| 7815-6101 | 9.11 | 8.58 | 9.66 | −0.29 | −0.41 |
| 7992-12703 | 8.75 | 8.44 | 9.17 | −0.36 | −0.27 |
| 8135-6101 | 8.42 | 8.62 | 9.51 | −0.38 | −0.23 |
| 8150-3701 | 6.77 | 8.03 | 9.61 | −0.64 | −0.86 |
| 8152-12702 | 8.14 | 9.01 | 9.58 | −1.01 | −1.26 |
| 8449-6101 | 8.83 | 8.11 | 8.93 | −0.29 | −0.29 |
Notes. Column 1 is the MaNGA Id, column 2 corresponds to the stellar mass, columns 3 and 4 are the mean stellar age weighted by mass and light and columns 5 and 6 are the mean stellar metallicity weighted by mass and light. The whole table is available at the CDS.
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