Figure 14: Mass two-point correlation functions on the light-cone for particles with redshift-dependent selection functions in the SCDM model, for (upper panels) and (lower panels). Left panels: with selection function whose shape is the same as that of the B-band magnitude limit of 19 for galaxies (upper) and 21 for QSOs (lower); right panels: randomly selected particles from the particles in the results from the left panels. (Figure taken from [28].)