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Table 1.

Priors adopted in the fit and the corresponding fiducial values.

Parameter Prior Fiducial
fconc [0.1, 1] 0 . 98 0.054 + 0.017 $ 0.98_{-0.054}^{+0.017} $ (0.999)
log(L0/[h−2 L]) [7, 13] 9 . 95 0.577 + 0.331 $ 9.95_{-0.577}^{+0.331} $ (10.357)
4log(M1/[h−1 M]) [9.0, 14.0] 11 . 66 0.434 + 0.341 $ 11.66_{-0.434}^{+0.341} $ (12.070)
γ1 𝒩(3.18, 2) 4 . 22 1.863 + 1.888 $ 4.22_{-1.863}^{+1.888} $ (3.146)
γ2 [0, 2] 0 . 42 0.140 + 0.174 $ 0.42_{-0.140}^{+0.174} $ (0.266)
σc [0.1, 0.3] 0 . 13 0.022 + 0.060 $ 0.13_{-0.022}^{+0.060} $ (0.115)
αs 𝒩(−1.1, 0.9) 1 . 73 0.404 + 0.524 $ -1.73_{-0.404}^{+0.524} $ (−1.478)
b0 𝒩(0, 1.5) 1 . 36 0.456 + 0.491 $ -1.36_{-0.456}^{+0.491} $ (−1.607)
b1 𝒩(1.5, 2.0) 0 . 86 0.359 + 0.287 $ 0.86_{-0.359}^{+0.287} $ (1.056)

Notes. Fiducial values are here reported as the median of the marginal posteriors, while the best fit values are reported in brackets. The error bars correspond to the 16th and 84th percentiles. 𝒩(μ, σ) indicates a normal distribution with mean μ and standard deviation σ. Parameter fconc is the normalisation of the concentration-halo mass relation, L0 the normalisation of Lc(M) relation, M1 the characteristic scale where Lc(M) changes the slope from γ1 to γ2. Furthermore σc is the scatter between luminosity and halo mass, while αs, b1, and b2 govern the slope and the normalisation of the Schechter function, respectively.

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