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How AGN feedback drives the size growth of the first quasars

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Figure

Figure 1. Illustration of the typical cosmological environment of the targeted haloes with AGN feedback in the simulation
Table 2. Main properties of the sample of the 6 haloes followed by our simulations, evaluated at z = 6.2 and z = 3.3 in, respectively, the top and bottom table
Figure 2. Total stellar mass-halo mass ratio versus halo mass for the five haloes shown with the abundance matching constraints of Moster et al
Figure 3. The left-hand panel shows the black hole mass versus total stellar mass for all haloes compared to the relation for elliptical galaxies of Reines & Volonteri (2015)
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