Table 1: The sample and the journal of observationsa.
Name z V $M_{\rm B}$ Date $T_{\rm exp}$ Seeing $\varepsilon$
          min  arcsec  
(1) (2) (3) (4) (5) (6) (7) (8)
HS 0010+3611 0.530 18.2 -24.4 27/08/2004 45 0.80 0.05
1E 0112+3256 0.764 18.9 -26.0 27/08/2004 55 0.80 0.22
PB 6708 0.868 18.6 -26.6 24/01/2005 64 0.95 0.08
KUV 03086-0447 0.755 17.5 -25.7 23/01/2005 106 0.95 0.03
US 3828 0.515 16.9 -25.1 22/01/2005 92 0.95 0.06
MS 08287+6614 0.610 18.0 -26.3 23/01/2005 73 0.85 0.10
TON 392 0.654 16.0 -25.6 24/01/2005 44 1.00 0.11
US 971 0.703 18.1 -27.1 22/01/2005 61 0.80 0.07
HE 0955-0009 0.597 16.9 -25.4 23/01/2005 104 0.90 0.04
HE 1100-1109 0.994 17.5 -25.2 22/01/2005 73 0.90 0.10
CSO 769 0.850 16.9 -24.4 23/01/2005 53 0.85 0.15
HS 1623+7313 0.621 16.3 -27.0 28/08/2004 75 0.85 0.04
HS 2138+1313 0.810 18.1 -24.9 28/08/2004 60 1.00 0.16
LBQS 2249-0154 0.832 18.7 -26.0 28/08/2004 64 0.90 0.10
ZC 2351+010B 0.810 17.5 -26.7 28/08/2004 40 1.00 0.16
a Column (1) gives the name of the object; (2) the redshift; (3) theV-band apparent magnitude; (4) the B-band absolute magnitude; (5) the date of observation; (6) total exposure time; (7) seeing FWHM (arcsec); and (8) the average ellipticity of the field stars.

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