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The observations were carried out with the Ritchey-Chretien Spectrograph
attached to a Tektronix 2K2K CCD detector. We used a
2''
205'' slit with a KPC-10A grating (316 grooves mm-1)
in its first order, and a GG 375 order separation filter cutting
off second-order contamination for wavelengths blueward of
7400Å. This instrumental setup allows a spatial scale along the slit of
pixel-1, a scale perpendicular to the slit of
2.77Åpixel-1, a spectral range of 3700-8300Å and a spectral resolution of
7Å (FWHM).
Short exposures (3-5 minutes) were used in order to detect strong emission
lines to allow measurement of redshifts and a crude classification.
No orientation of the slit along the parallactic angle was done because
of the snap-shot observing mode.
Reference spectra of an Ar-Ne-He lamp were recorded to provide
wavelength calibration.
Spectrophotometric standard stars from Oke ([1990]) and Bohlin
([1996]) were observed at the beginning and at the end of each night
for flux calibration. The dome flats, bias, dark and twilight sky frames
were accumulated each night.
The weather conditions were photometric,
with seeing variations between 25 and 3 (FWHM).