... bias[*]
The work presented here is based in part on data obtained with the ESO facilities on La Silla (EFOSC/3.6-m) and Paranal (FORS1/UT1).
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
...[*]
Figure 1 is only available in electronic form at http://www.edpsciences.org
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
...(H I)[*]
One of the observed QSOs actually has $z_{\rm em}$ < 2.2 due to an incorrect redshift in our original list, see Table 3.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
... IRAF[*]
IRAF is distributed by the National Optical Astronomy Observatories, which are operated by the Association of Universities for Research in Astronomy, Inc, under cooperative agreement with the National Science Foundation.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
...$z_{\min} = 1.8$[*]
We note that although most surveys calculate $z_{\min}$ for each QSO on a case by case basis, depending on wavelength coverage and S/N, we have designed the CORALS survey to have adequate spectral range and S/N to achieve a uniform lower redshift cut-off.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
Copyright ESO 2001