Table 1.
Analysis of the amount of galaxies for which there is significant difference between the FADO and STARLIGHT estimates of the currently and total ever-formed stellar mass, light- and mass-weighted stellar age, and metallicity.
| EWHα < 100 | 100 ≤ EWHα < 500 | 500 ≤ EWHα < 1000 | EWHα ≥ 1000 | ||
|---|---|---|---|---|---|
| Mcurr | FD | 5% | 21% | 5% | 2% |
| ST | 9% | 34% | 71% | 82% | |
| Mever | FD | 5% | 22% | 7% | 4% |
| ST | 9% | 35% | 70% | 84% | |
| tL | FD | 87% | 78% | 66% | 35% |
| ST | 3% | 5% | 17% | 38% | |
| tM | FD | 11% | 34% | 25% | 13% |
| ST | 13% | 35% | 54% | 65% | |
| ZL | FD | 2% | 7% | 39% | 38% |
| ST | 2% | 12% | 12% | 13% | |
| ZM | FD | 0% | 13% | 24% | 31% |
| ST | 10% | 16% | 16% | 18% | |
| Total number | 87 | 171 | 187 | 55 | |
Notes. We present the percentage of galaxies for which either FADO or STARLIGHT obtains an estimate which is significantly different relative to the estimate of the other code, considering an error uncertainty of 0.2 dex. We divide the analysis in four intervals of EW(Hα), in angstroms, and provide the number of objects in each interval.
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