Spectroscopy Sample
In the following table, we list the main properties of the clusters in the WINGS-SPE sample. The columns indicate: (1) cluster name, (2-3) coordinates of the image field center at epoch J 2000 [right ascension (2) in hours, minutes and seconds and declination (3) in degrees, arcminutes, arcseconds], (4) number of redshifts, which is equal to the number of entries in the spectroscopic catalog for that cluster, (5) mean cluster redshift, (6) number of member galaxies (used to compute mean redshift and velocity dispersion), (7) cluster velocity dispersion computed from the WINGS-SPE data, (8) cluster velocity dispersion available from the literature, (9) reference for the literature velocity dispersion, (10) logarithm of the X-ray luminosity in the 0.1 − 2.4 keV ROSAT RASS bandpass (from Ebeling et al. 1996), (11) virial radius in Mpc, (12) aperture in units of R200.
We also list in the following table the main properties of the 30 clusters not observed but for which literature data exist.The columns here indicate: (1) cluster name, (2-3) coordinates of the image field center at epoch J 2000 [right ascension (2) in hours, minutes and seconds and declination (3) in degrees, arcminutes, arcseconds], (4) cluster mean redshift, (5) number of member galaxies, (6) cluster velocity dispersion, (7) reference for the data reported in columns (4-6), (8) logarithm of the X-ray luminosity in the 0.1 − 2.4 keV ROSAT RASS bandpass (from Ebeling et al. 1996).
The details of the tables and more information can be found in the WINGS-SPE paper.