Table 2: Log of the observations. The last two columns show the average seeing during the integrations and the photometric conditions derived from the A&G camera images.
QSO Date Exp.time Grating $\lambda$ coverage Seeing Conditions
    (s)   (Å)    
Q0151+048A 2003-08-27 5 $\times$ 1800 V600 3500-5080 0.8-1.2 stable
Q0953+4749 2004-04-16 4 $\times$ 1800 V300 3630-6980 0.9 stable
  2004-04-21 5 $\times$ 1800 V300 3630-6980 1.0 non-phot.
Q1347+112 2004-04-20 7 $\times$ 1800 V300 3630-6980 0.6 non-phot.
Q1425+606 2004-04-19 6 $\times$ 1800 V300 3630-6750 1.0 stable
Q1451+1223 2004-04-17 7 $\times$ 1800 V300 3630-6980 0.8 non-phot.
Q1759+7539 2004-04-21 7 $\times$ 1800 V300 3630-6980 1.0-1.5 non-phot.
Q1802+5616 2003-06-18 2 $\times$ 1800 V600 5100-6650 1.0 non-phot.
  2003-06-20 3 $\times$ 1800 V600 5100-6650 1.0 non-phot.
  2003-06-21 4 $\times$ 1800 V600 5100-6650 1.8 non-phot.
  2003-06-22 6 $\times$ 1800 V600 5100-6650 0.9 stable
Q2155+1358 2003-08-26 7 $\times$ 1800 V600 4015-5610 0.7 stable
  2003-08-27 4 $\times$ 1800 V600 4015-5610 0.8 non-phot.
Q2233+131 2002-09-03$^\dagger$ 4 $\times$ 1800 V300 3930-7250 1.0-1.3  
  2003-08-24 6 $\times$ 1800 V600 4000-5600 0.6 stable
  2003-08-25 4 $\times$ 1800 V600 4000-5600 0.7 non-phot.

$^\dagger$ Results from these observations are published in Christensen et al. (2004).


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