J/A+AS/116/203 J/A+AS/116/203 The redshift catalogue for galaxy clusters P Stein Astron. Astrophys. Suppl. Ser. 116 203 1996 1996A&AS..116..203S Clusters, galaxy Redshifts catalogs galaxies: clusters: general galaxies: distances and redshifts An extensive redshift survey has been conducted on a sample of 15 nearby (0.01<~z<~0.05) clusters of galaxies. A total number of 860 redshifts were determined by fitting of emission-lines and/or cross-correlation techniques. Of this sample, 735 galaxies are within 0.2-0.8Mpc (H_0_=50km/s/Mpc) of the center of clusters. Approximate morphological types are available for most of the galaxies. A comparison of the present redshifts with published data allows an extensive error analysis. The agreement is excellent with the most modern data, showing a zero point error of 5km/s and an overall consistency of the measurements and their uncertainties. We estimate our redshifts to have mean random errors around 30km/s. A population analysis of the clusters will be given in a forthcoming paper.

Name Cluster or field name: --- Seq Sequential identification of objects --- RAh Right ascension (1950) h RAm Right ascension (1950) min RAs Right ascension (1950) s DE- Declination sign --- DEd Declination (1950) deg DEm Declination (1950) arcmin DEs Declination (1950) arcsec HRVem Heliocentric radial velocity from emission lines km/s e_HRVem Error on radial velocity from emission lines km/s HRVabs Heliocentric radial velocity from absorption lines (cross-correlation) km/s e_HRVabs Error on radial velocity from absorption lines km/s HRV Combined heliocentric radial velocity km/s e_HRV Error on radial velocity km/s Nem Number of emission lines from which `HRVem' was determined --- MType Morphological class for the galaxy --- r_MType Source number=1 Morphological types were taken either from the literature or determined directly on ESO-survey plates --- Simona Mei CDS 1995Sep07 J_A+AS_116_203.xml