Table A.1
Matching between Abell (Abell et al. 1989) and KiDS clusters.
| Abell | KiDS | |||||||||||||||
|
|
|
|||||||||||||||
| ID | RA* | Dec* | Richness** | z *** | RA | Dec | z | S/N | Sep. (″) | |||||||
|
|
||||||||||||||||
| A693 | 129.920 | 1.073 | 46 [0] | 0.16 (5) | 129.923 | 1.074 | 0.17 | 7.9 | 11 | |||||||
| A711 | 132.592 | 0.313 | 57 [1] | 0.19 (6) | 132.600 | 0.260 | 0.19 | 10.6 | 192 | |||||||
| A776 | 139.065 | –0.393 | 51 | 0.33 (7) | 139.073 | –0.402 | 0.37 | 16.4 | 43 | |||||||
| A1376 | 176.529 | –1.094 | 50 [1] | 0.12 (1) | 176.564 | –1.096 | 0.12 | 8.9 | 126 | |||||||
| A1386 | 177.090 | –1.945 | 66 [1] | 0.10 (2) | 177.062 | –1.932 | 0.18 | 9.4 | 112 | |||||||
| A1411 | 178.816 | –0.528 | 69 | 0.13 (3) | 178.807 | –0.526 | 0.15 | 8.5 | 33 | |||||||
| A1445 | 180.431 | –0.184 | 81 [2] | 0.17 (1) | 180.432 | –0.184 | 0.19 | 13.2 | 4 | |||||||
| A1533 | 186.140 | 0.906 | 119 [2] | 0.23 (1) | 186.122 | 0.898 | 0.25 | 7.2 | 73 | |||||||
| A1938 | 219.432 | –0.316 | 53 | 0.14 (4) | 219.433 | –0.316 | 0.14 | 10.1 | 2 | |||||||
| A1389 | 177.281 | –1.367 | 40 [0] | 0.08 (8) | 177.187 | –1.284 | 0.12 | 6.6 | 452 | |||||||
| A1419 | 179.083 | –0.206 | 73 [1] | 0.12 (3) | 179.041 | –0.326 | 0.27 | 12.7 | 457 | |||||||
Notes. The last column (Sep.) gives the distance in arcsec between the centers of the Abell cluster and the KiDS cluster.
RA and Dec for the clusters A1376, A1389, A1419, A1445 and A1938 are from De Propris et al. (2002). The others are from Abell et al. (1989).
Richness as defined in Abell et al. (1989) (number of cluster members between m3 and m3 + 2, corrected for background) and, in square brackets, richness class from Abell (1958).
Redshift from different references, indicated in brackets; (5), (6) and (7) are photometric redshifts.
Reference. (1) Struble & Rood (1999); (2) Quintana & Ramirez (1995); (3) Popesso et al. (2007); (4) Priv. comm., M. Merchan, and A. Zandivarez, unpublished Galaxy Groups catalog as described in Merchán & Zandivarez (2002) and sent to Dr. John Mulchaey in 2003. Received by NED in 2007; (5) Koester et al. (2007); (6) Wen et al. (2010); (7) Estrada et al. (2007); (8) Yoon et al. (2008).
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