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| RR 143 | RR 210 | RR 216 | RR 242 | |
| Candidate sample | 171 | 190 | 178 | 118 |
| Observed | 106 (62%) | 55 (29%) | 24 (13%) | 73 (62%) |
| Measured z total | 84 (79%) | 52 (95%) | 22 (92%) | 55 (75%) |
| Measured z xcsao | 69 | 50 | 22 | 45 |
| Measured z splot | 15 | 2 | - | 10 |
| Members | 2 (2%) | 2 (4%) | 3 (14%) | 10 (18%) |
| Members corr. | 4.4 | 4.9 | 15 | 15.4 |
| Total number of spectroscopically observed objects: | 258 | |||
| Total number of measured redshifts: | 213 (83%) | |||
| Row 1: number of galaxies in the candidate sample; row 2: number of galaxies observed with VIMOS, in brackets the percentage of spectroscopically observed galaxies out of the candidate sample; row 3: number of galaxies for which a redshift could be measured, in brackets the percentage of galaxies with measured redshift out of all spectroscopically observed galaxies; row 4: number of redshifts obtained by cross-correlation with xcsao; row 5: number of redshifts obtained by fitting single lines with splot; row 6: number of newly discovered members, in brackets the percentage of newly found member galaxies out of all galaxies with measured redshifts; row 7: completeness corrected number of members (see Sect. 3). |
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