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Fig. 9


Linear bias as a function of redshift for AKARI photometric redshift samples (filled circles). Dashed curves represent the theoretical linear halo bias evolution of dark matter halos of minimal masses: 1010, 1011, 1012, and 1013 (from bottom to top). As a reference we show results from the literature: triangles mark results from Starikova et al. (2012), squares the results from Magliocchetti et al. (2008), crossesthe results from Gilli & Daddi (2007), and asterisks from Dolley et al. (2014).

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