Table 3.
p-values from Monte Carlo calibrated KS and Kuiper tests of the observed distribution against maximum-likelihood LF models obtained by folding the maximum-likelihood Schechter (Eq. (19)) or power-law (Eq. (23)) parameterisations with the MW survey area and LAE selection function (RSSF), as well as the fc = 0.15 truncation criterion.
| Parameterisation |  |
 |
 |
 |
p2DKS |
|---|---|---|---|---|---|
| Schechter (logL* = 42.66, α = −1.84, logϕ* = −2.71) | 0.74 | 0.73 | 0.30 | 0.49 | 0.87 |
| Power Law (logL* = 42.5, β = −2.99, logϕ* = −2.932) | 0.08 | 0.04 | 0.17 | 0.35 | 0.23 |
| Power Law incl. AGN (logL* = 42.5, β = −2.94, logϕ* = −2.930) | 0.12 | 0.08 | 0.18 | 0.29 | 0.30 |
Notes. One-dimensional KS and Kuiper tests are performed in redshift and luminosities, while the 2D KS test operates directly in redshift-luminosity space (see Fig. 14). L* in erg s−1 and ϕ* in Mpc−3.
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