Cluster Mass-to-Light Ratios from Weak Lensing
Ours:
| Cluster | Z | M/L | reference |
| A1689 | 0.18 | 400h +/- 40 | Kaiser et al 1996 |
| A1146 | 0.14 | 200h +/- 50 | Kaiser et al 1996 |
| A2218 | 0.18 | 440h +/- 80 | Squires et al 1996a |
| ms1224 | 0.35 | 800h +/- 200 | Fahlman et al 1994 |
| A2390 | 0.23 | 320h +/- 90 | Squires et al 1996b |
| A2163 | 0.18 | 300h +/- 100 | Squires et al 1996c |
| ms1054 | 0.83 | > 360h | Luppino and Kaiser 1996 |
Others:
| Cluster | Z | M/L | reference |
| 1455+22 | 0.26 | 460h | Smail etal 1994 |
| cl0016+16 | 0.55 | 430h | Smail etal 1994 |
| cl0024+17 | 0.38 | 430h | Bonnet etal 1994 |
| cl0939 | 0.41 | 200h | Seitz etal 1996 |
| A1689 | 0.18 | 450h +/- 50 | Tyson and Fisher 1995 |
Biggest discrepancy with virial mass
- A1689: M_vir ~ 2.5 x M_lens
- ms1224: M_vir ~ 0.33 x M_lens