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Table 1:

Log of imaging observations with FORS1 and 2 of the three surveyed fields. The $5\sigma $ detection limits are computed for a 3 $^{\prime \prime }$ diameter aperture. The data for BRI 1346-0322 and Q 2138-4427 are reproduced from Paper I.
Filter $z_{\rm qso}$, $z_{\rm abs}$ Total Exp. PSF FWHM 5$\sigma $
    time (h) ( $\hbox{$^{\prime\prime}$ }$) limit
BRI 1202-0725 4.70, 3.20      
N   8.3 1.02 25.6
Va   2.9 0.96 26.6
R   1.6 0.95 26.1
BRI 1346-0322 3.99, 3.15      
N   8.9 0.93 25.6
B   2.5 1.02 26.6
R   1.7 0.94 26.0
Q 2138-4427 3.17, 2.85      
N   10.0 0.96 26.5
B   2.5 1.04 26.9
R   1.7 0.93 26.3
a Due to the higher target redshift of this field the wavelength
of the Ly$\alpha $-line was matched by the V-band rather than B.

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