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QuasarEvolutionData

Compiled outputs from the semi-empirical model described in Ren+21

One way to compute the QLF from LcMh is to use Eqn3 from Ren+21, with zc=4 and the parameters (Sigma, k) given in the manuscript.
Alternatively, one can use the precomputed LcMh at different z (Eqn2).

Contains:

Lc(Mh) for 1 < z < 10 as shown in Fig1+2
QLFs for 1 < z < 10 as shown in Fig1+2
HMF for 1 < z < 10
Halo Assembly Times, t(M) for 1 < z < 10 as computed using Giocoli+07


Paper plots for reference:

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Compiled outputs from the semi-empirical model described in Ren+21

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