Fig. 9.
Correspondence between observational overdensity significances of quasars and their z = 0 descendant halo masses of quasars and simulated g-dropouts. The blue histogram shows the distribution of maximum overdensity significances centered on quasars with a radius of 1΄, which is exactly the same as figure 3a. The orange, red, and green lines indicate the simulated g-dropout overdensity significance distributions with z = 0 descendant halo masses Mh, z = 0 = 1012 M⊙ –1013 M⊙ , Mh, z = 0 = 1013 M⊙ –1014 M⊙ , and Mh, z = 0 > 1014 M⊙ , respectively. Their overdensity significances are those simulated for z ∼ 4. (Color online)

Correspondence between observational overdensity significances of quasars and their z = 0 descendant halo masses of quasars and simulated g-dropouts. The blue histogram shows the distribution of maximum overdensity significances centered on quasars with a radius of 1΄, which is exactly the same as figure 3a. The orange, red, and green lines indicate the simulated g-dropout overdensity significance distributions with z = 0 descendant halo masses Mh, z = 0 = 1012M–1013M, Mh, z = 0 = 1013M–1014M, and Mh, z = 0 > 1014M, respectively. Their overdensity significances are those simulated for z ∼ 4. (Color online)

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