In this appendix we present a few ELGs that were selected from our Region 1 (see Paper I) (the region of the Pisces-Perseus Supercluster) and Region 2. These objects were observed after the publication of the first catalogue and therefore were missed from our "List 1".
The observations were done in August 1995 with the Cassegrain Twin
Spectrograph at the 3.5m telescope at Calar Alto, as a back-up of
an observational campaign not dedicated to our project. The details of the
observations are given in Table 6
while in Table 7 we list the name of the ELGs, alternative
designations (for those objects contained in other catalogues), their
coordinates (equinox 1950.0),
heliocentric redshifts and emission-lines seen in their spectra. The
abbreviations for alternative designations can be found in the List of
Abbreviations used for the Table 2. The data
reduction follows the same procedure as described in Sect. 2. The errors in
the redshifts are around 
. In order to have an
external check of our redshift determination we also observed a few candidates
that had redshifts in the literature. In Table 8 we give the names
of the galaxies observed together with their velocities, both measured and
from literature. In the last column we indicate the difference between our
values and the reference one. Besides UM27, for which we obtained a big
difference, the rest show differences up to 0.0001 in z. The finding
charts of the newly discovered objects can be found in Fig. 2,
upper panel.
 |
We would like to thank the Calar Alto staff for their support during the observations. U. Hopp acknowledge the support by the SFB 375 by the Deutsche For-schungsgemeinschaft.
This research has made use of the NASA/IPAC Extragalactic Database (NED) which is operated by the Jet Propulsion Laboratory, California Institute of Technology, under contract with the National Aeronautics and Space Administration.
Copyright The European Southern Observatory (ESO)
