Table 3
Summary of other studies in the literature as compared with our results.
| Redshift | Authors | SFHa | Ext. law | N | Comparison model |
|
|
|||||
| z ~ 3 | S01 | constant SFR | Calzetti | 74 | REF |
| z ~ 3 | P01 | constant/exp. declining | Calzetti | 33 | DEC |
| z ~ 4 | PG07 | exp. declining | Calzetti & SMC | 47 | DEC |
| z ~ 4 | L11 | constant SFR | Calzetti | 6b | REF |
| z ~ 5 | S07 | SSP/constant/exp. declining | Calzetti | 14 | DEC |
| z ~ 5 | V07 | constant SFR | SMC | 21 | REF |
| z ~ 5 | Y09 | constant SFR | Calzetti | 105 | REF |
| z ~ 6 | Y06 | SSP/constant SFR | Calzettic | 53 | DEC |
| z ~ 6 | E07 | SSP/constant/exp. declining | Calzetti | 17 | DEC |
Notes. Column 3 indicates assumed star formation histories; Col. 4 the extinction law; Col. 5 the number of galaxies, and Col. 6 indicates our model used for comparison.
Yan et al. (2006) assume AV = 0. For a fair comparison, we run DEC model with the same assumption.
Reference. S01: Shapley et al. (2001), P01: Papovich et al. (2001), PG07: Pentericci et al. (2007), L11: Lee et al. (2011), S07: Stark et al. (2007), V07: Verma et al. (2007), Y09: Yabe et al. (2009),Y06: Yan et al. (2006), and E07: Eyles et al. (2007).
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