Table 1: The spectrograph characteristics.
Telescope Run Spectrograph Disp Disp ${\Delta\lambda}$ CCD Pix Spat. scale Slit
    Å/mm Å/pix Å   ${\rm\mu m}$ ''/pix arcsec
OHP/1.93 1998 CARELEC 260 7.0 3600-7200 $512 \times512~TEK$ 27 1.17 $300 \times 2.5$
OHP/1.93 1999 CARELEC 133 1.8 3400-7000 $2048 \times1024~EEV$ 13.5 0.58 $300 \times 2.5$
OHP/1.93 2000 CARELEC 133 1.8 3400-7000 $2048 \times1024~EEV$ 13.5 0.58 $300 \times 2.5$
OHP/1.93 2001 CARELEC 133 1.8 3400-7000 $2048 \times1024~EEV$ 13.5 0.58 $300 \times 2.5$
OHP/1.93 2002 CARELEC 133 1.8 3400-7000 $2048 \times1024~EEV$ 13.5 0.58 $300 \times 2.5$
OHP/1.93 2003 CARELEC 133 1.8 3400-7000 $2048 \times1024~EEV$ 13.5 0.58 $300 \times 2.5$
ESO/3.6(LD) 2001 EFOSC2 135 4.0 3380-7520 $2048 \times2048~LOR $ 15 0.16 $300 \times 1.5$
ESO/3.6(HD) 2001 EFOSC2 67 2.0 4700-6770 $2048 \times2048~LOR $ 15 0.16 $300 \times 1.5$
ESO/3.6(LD) 2002 EFOSC2 135 4.0 3380-7520 $2048 \times2048~LOR $ 15 0.16 $300 \times 1.5$
SPM/2.1 2002 $Boller\&Chivens$ 125 3.0 3900-7000 $1024 \times1024~SITE3$ 24 0.96 $300 \times 2.0$
LOI/1.52 2003 BFOSC 198 4.0 3600-8900 $1300 \times1340~EEV$ 20 0.58 $300 \times 2.0$


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