Image Details
Caption: Figure 2.
Rest-frame UV (1450 Å) luminosity function of the GALEX full AGN sample in the redshift interval z = 0.65–1.25 (black squares with 1σ error bars from the observed number of sources in each bin). Red diamonds show the converted X-ray-selected BLAGN luminosity function in the same redshift interval from Yencho et al. (2009). The green curves (lower for z = 0.68–0.95; upper for z = 0.95–1.25) show the converted optically selected luminosity functions from Croom et al. (2004).
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