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Fig. 7

image

Evolution of the bias factor, calculated with the variance at 8 h-1 Mpc, for samples of star-forming galaxies. Red diamonds indicate the BJGKn< 6 samples. At z ~ 2, the gray, blue, red, green, and light green squares show the sBzK samples of Hayashi et al. (2007), Blanc et al. (2008), Hartley et al. (2008), Lin et al. (2012), and McCracken et al. (2010), respectively. Yellow squares show the BMandBX selected galaxies of Adelberger et al. (2005). At z ~ 3, the blue, green, and red squares indicate the LBGs selected by Yoshida et al. (2008), Kashikawa et al. (2006), Hildebrandt et al. (2007), Ouchi et al. (2005), respectively. Gray squares show the Ly-α emitters selected by Guaita et al. (2010), Gawiser et al. (2007). The lines show the bias evolution for different halo masses (Sheth et al. 2001), which are indicated below each line at the right side of the panel.

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