  We report accurate redshifts of 110 active galaxies (mostly radio-loud
objects at z<0.4) observed in the course of a survey to find broad,
double-peaked emission lines. These redshifts are measured from the narrow
emission lines of these objects and are accurate to at least one part in 10^4 .
For each object we determine a redshift from high- and low-ionization lines
separately, as well as an average redshift from all the available lines. We
find that in about 15% of cases, the low-ionization lines yield a slightly
higher redshift than the high-ionization lines; the average redshift difference
amounts to a velocity difference of approximately 80 km/s. In addition to the
redshift measurements we also report revised redshifts for two objects as well
as new classifications for three narrow-line objects.
