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Fig. 7


SFRcorr(Hα) vs. stellar mass for LAEs and SFGs at z ≥ 2. Red and magenta colors indicate Lyα and Hα emitting galaxies, while blue indicate UV-continuum-selected SFGs without Lyα in emission. The blue star with cyan error bars represents BX16, which shows Lyα absorption. The SFR(Hα) upper limit is due to an upper limit in Hα flux, and lower limits are presented when it is not possible to estimate Eβ(B − V) from the rest-frame UV continuum slope for individual sources. The solid green line is the M − SFR relation by Talia et al. (2012) for SFGs at z ≃2. The black line is the same relation for z ~ 2 SFGs in the GOODS survey (Daddi et al. 2007). Dashed green and black lines indicate the 1σ range of those relations. Measured values from Nakajima et al. (2012b) (green square), Finkelstein et al. (2011) (orange dots), Atek et al. (2011) (brown triangle), and Erb et al. (2010) (violet triangle) are also shown.

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