Fig. 1.

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Example luminosity functions ϕ(L) = dP/dln(L) induced by a Gaussian apparent structure model (Eqs. (10), left-hand panel) and a power law apparent structure model (Eqs. (13)) with a luminosity profile slope α = 3 (right-hand panel), both with a core half-opening angle θc = 0.1 rad and = 1053 erg s−1. In each panel, the luminosity function corresponding to a population with zero core dispersion (A → ∞ in Eq. (2)) is shown in grey, and three cases with different core luminosity distributions (slopes reported in the legend) are shown with coloured lines. The corresponding Lc distributions (arbitrarily scaled) are shown with dashed lines. In the right-hand panel, the dashed black line shows the trend ϕ(L)∝L−2/αL expected at intermediate luminosities.
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