Fig. 1.

The FUV and TIR LFs at z = 0.7 (left and right panel, respectively). Open squares are nonparametric LFs estimated from our CDFS multiwavelength data with GALEX NUV- and Spitzer MIPS 24 μm selections. Dotted lines represent the FUV LFs at this redshift bin taken from Arnouts et al. (2005). Dashed lines depict the TIR LFs derived from the evolutionary parameters at z = 0.7 given by Le Floc’h et al. (2005). Because of a well-known large density enhancement at this redshift, we renormalized the LF to remove the effect of the overdensity.