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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