Fig. 13
Posterior probability distributions of the three parameters defining p(λEdd) in Eq. (8) for the whole galaxy population (all galaxies) across 0.5 <z< 2.5 from the MCMC analysis. The solid lines denote the best-fit values for each parameter, which are also listed in Table 3. The density contours show the 68.3, 90, and 95 percent posterior confidence probabilities.
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