Fig. 19
M• and M ∗ measurements of high-luminosity quasars at z ≈ 3 from Schramm et al. (2008). The black contours show the predicted M•-MBulgeprobability distribution using model 2 for the null hypothesis of no evolution in M• /MBulge . For comparison, the offset green contours show the expected distribution if M• /MBulge were to evolve as strongly as with γ = 2.
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