The REFLEX galaxy cluster survey VIII. Spectroscopic observations and optical atlas

Author(s): Guzzo, L.; Schuecker, P.; Boehringer, H.; et al.

Source: ASTRONOMY & ASTROPHYSICS  Volume: 499   Issue: 2   Pages: 357-369   DOI: 10.1051/0004-6361/200810838   Published: MAY 2009

We present the final data from the spectroscopic survey of the ROSAT-ESO Flux-Limited X-ray ( REFLEX) catalog of galaxy clusters. The REFLEX survey covers 4.24 steradians (34% of the entire sky) below a declination of delta = + 2.5 degrees and at high Galactic latitude (vertical bar b vertical bar > 20 degrees). The REFLEX catalog includes 447 entries with a median redshift of 0.08 and is better than 90% complete to a limiting flux f(X) = 3 x 10(-12) erg s(-1) cm(-2) (0.1 to 2.4 keV), representing the largest statistically homogeneous sample of clusters drawn from the ROSAT All-Sky Survey (RASS) to date. Here we describe the details of the spectroscopic observations carried out at the ESO 1.5 m, 2.2 m, and 3.6 m telescopes, as well as the data reduction and redshift measurement techniques. The spectra typically cover the wavelength range 3600-7500 angstrom at a two-pixel resolution of similar to 14 angstrom, and the measured redshifts have a total rms error of similar to 100 km s(-1). In total we present 1406 new galaxy redshifts in 192 clusters, most of which previously did not have any redshift measured. Finally, the luminosity/redshift distributions of the cluster sample and a comparison to the no-evolution expectations from the cluster X-ray luminosity function are presented.