Figure 1.
Angular number density (left), clustering bias (centre), and magnification bias (right) as a function of redshift, for flux density thresholds 1, 5, 10, and 20 μJy, respectively.
Angular number density (left), clustering bias (centre), and magnification bias (right) as a function of redshift, for flux density thresholds 1, 5, 10, and 20 μJy, respectively.
