Table 2: Log of the observations. The last two columns show the average seeing during the integrations and the photometric conditions, respectively.

QSO		 Date Exposure time Grating $\lambda$ coverage Seeing Conditions
    (s)   (Å)    

Q0953+4749		 2004-04-16 $4\times1800$ V300 3630-6980 0.9 stable
  2004-04-21 $5\times1800$ V300 3630-6980 1.0 non phot.
Q1347+112 2004-04-20 $7\times1800$ V300 3630-6980 0.6 non phot.
Q1425+606 2004-04-19 $6\times1800$ V300 3630-6750 1.0 stable
Q1451+1223 2004-04-17 $7\times1800$ V300 3630-6980 0.8 non phot.
Q1759+7539 2004-04-21 $7\times1800$ V300 3630-6980 1.0-1.5 non phot.
Q1802+5616 2003-06-18 $2\times1800$ V600 5100-6650 1.0 non phot.
  2003-06-20 $3\times1800$ V600   1.0 non phot.
  2003-06-21 $4\times1800$ V600   1.8 non phot.
  2003-06-22 $6\times1800$ V600   0.9 stable
Q2233+131 2003-08-24 $6\times1800$ V600 4000-5600 0.6 stable
  2003-08-25 $4\times1800$ V600   0.7 non phot.


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