Clusters position, redshift, mass, and cross-identifications.
|ID||RA||Dec||z||log M/M⊙||n200||err||Piffaretti et al. (2011) ID||Planck (2015) ID||Abell (1958) ID||NED ID|
|GCwM 1||0.8380||4.6440||0.098||14.05||24||5||ABELL2698 (1.9)||ABELL2698 (1.9,17)|
|GCwM 2||0.9235||2.0678||0.092||14.26||34||6||MCXCJ0003.8+0203 (2.3)||PSZ2G099.57-58.64 (1.5)||ABELL2700 (2.6)||ABELL2700 (2.3,66)|
|GCwM 3||1.3754||16.2435||0.116||14.29||36||7||MCXCJ0005.3+1612 (2.7)||WHLJ000524.0+161309 (2.1,21)|
|GCwM 4||1.5851||10.8613||0.170||14.49||52||8||MCXCJ0006.3+1052 (0.5)||PSZ2G105.40-50.43 (2.0)||NSCSJ000619+105206 (0.5,10)|
|GCwM 5||2.5753||17.7496||0.173||14.47||51||8||PSZ2G109.22-44.01 (1.2)||ABELL6 (4.2)|
|GCwM 6||2.9235||32.4316||0.107||14.61||64||9||MCXCJ0011.7+3225 (1.1)||PSZ2G113.29-29.69 (0.8)||ABELL7 (1.2)|
Notes. The table lists cluster coordinates (J2000), redshift z, log mass M200 estimated from the richness, the richness n200 and its error, followed by the id of clusters from a few bibliographic sources, with angular offsets reported in parentheses. The last column also lists the number of references to the cluster in May 2015, as given by NED. Masses have 0.16 dex errors. The table is entirely available at the CDS, and also accessible at http://www.brera.mi.astro.it/~andreon/famous.html. A portion is shown here for guidance regarding its form and content.
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