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].)
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