  The goal of the Complete Optical and Radio Absorption Line System (CORALS)
survey is to quantify the potential impact on QSO absorber statistics from dust
in intervening galaxies. Dust may introduce a selection bias in surveys which
are based on magnitude limited QSO samples, leading to an underestimate of
absorber number density, n(z). Here we present the results of the second phase
of the CORALS survey which extends our previous work on z > 1.8 damped Lyman
alpha systems (DLAs) to search for strong metal line systems (candidate DLAs)
in the range 0.6 < z < 1.7. We have identified 47 MgII systems with rest frame
equivalent widths EW(MgII lambda 2796) > 0.3 A in our sample of 75
radio-selected quasars. Our principal and most robust result is that the n(z)
of low redshift MgII systems determined for the CORALS survey is in excellent
agreement with that of optically-selected, magnitude limited QSO samples. The
statistically inferred number density of DLAs, n(z)=0.16^+0.08_-0.06, is
consistent with other low redshift samples, although the large 1 sigma error
bars permit up to a factor of 2.5 more DLAs in CORALS. However, confirmation of
the DLA candidates, precise evaluation of their n(z) and measurement of their
HI column densities awaits UV observations with the Hubble Space Telescope.
Finally, we report an excess of intermediate redshift MgII systems observed
towards bright QSOs which could be due to a lensing amplification bias.
However, there is also evidence that this excess could simply be due to more
sensitive EW detection limits towards brighter QSOs. We also emphasize that
absorber statistics determined from magnitude limited surveys reach a steady
value if the completeness limit is significantly fainter than the fiducial
value of the quasar luminosity function. (Abridged).
