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Table 3.
Stellar masses of AGS24 assuming different SFHs and attenuation laws.
| FAST++4: | |
|---|---|
| Calzetti et al. (2000) attenuation law + vary SFHs | |
| Models | log M⋆ [log M⊙] |
| Delayed exponentially declining | 11.37 |
| Exponentialy declining | 11.31 |
| Truncated | 11.40 |
| A second burst | 11.33 |
| CIGALE: | |
| delayed exponentially declining SFH + vary attenuation laws | |
| Models | log M⋆ [log M⊙] |
| Calzetti et al. (2000) | 11.52 ± 0.57 |
| Charlot & Fall (2000) | 11.41 ± 0.21 |
| MAGPHYS (a) | 11.44 ± 0.22 |
Notes.
(a)
A modified Charlot & Fall (2000) law that is used in MAGPHYS (da Cunha et al. 2008).
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