  Studies of the properties of low-redshift cluster galaxies suffer, in
general, from small spatial coverage of the cluster area. WINGS, the most
homogeneous and complete study of galaxies in dense environments to date,
obtained spectroscopic redshifts for 48 clusters at a median redshift of 0.05,
out to an average distance of approximately 0.5 cluster virial radii. The WINGS
photometric survey was recently extended by the VST survey OmegaWINGS to cover
the outskirts of a subset of the original cluster sample. In this work, we
present the spectroscopic follow-up of 33 of the 46 clusters of galaxies
observed with VST over 1 square degree. The aim of this spectroscopic survey is
to enlarge the number of cluster members and study the galaxy characteristics
and the cluster dynamical properties out to large radii, reaching the virial
radius and beyond. We used the AAOmega spectrograph at AAT to obtain
fiber-integrated spectra covering the wavelength region between 3800 and 9000
A, with a spectral resolution of 3.5-6 A full width at half maximum (FWHM).
Observations were performed using two different configurations and exposure
times per cluster. We measured redshifts using both absorption and emission
lines and used them to derive the cluster redshifts and velocity dispersions.
We present here the redshift measurements for 17985 galaxies, 7497 of which
turned out to be cluster members. The sample magnitude completeness is 80% at
V=20. Thanks to the observing strategy, the radial completeness turned out to
be relatively constant (90%) within the AAOmega field of view. The success rate
in measuring redshifts is 95%, at all radii. We provide redshifts for the full
sample of galaxies in OmegaWINGS clusters together with updated and robust
cluster redshift and velocity dispersions. These data will be publicly
accessible through the CDS and VO archives.
