Properties of z ~ 3–6 Lyman break galaxies - II. Impact of nebular emission at high redshift

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Table 3

Summary of other studies in the literature as compared with our results.

Redshift	Authors	SFH^a	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	6^b	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	Calzetti^c	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.

^(a)

SSP: single stellar population, burst.

^(b)

Stack of 1913 objects in 6 UV magnitude bins.

^(c)

Yan et al. (2006) assume A_V = 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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