Table 4
Synopsis of cluster parameters and resulting weak lensing masses.
| Cluster | r 200 | c NFW |
|
r 200, B01 | c B01, NFW |
|
r 200, B12 | c B12, NFW |
|
| [Mpc] | [1014 M⊙] | [Mpc] | [1014 M⊙] | [Mpc] | [1014 M⊙] | ||||
| (1) | (2) | (3) | (4) | (5) | (6) | (7) | (8) | (9) | |
|
|
|||||||||
| CL 0030+2618 |
|
|
|
|
|
|
|
|
|
| CL 0159+0030 |
|
> 20 |
|
|
|
|
|
|
|
| CL 0230+1836 |
|
|
|
|
|
|
|
|
|
| CL 0809+2811 |
|
|
|
|
|
|
|
|
|
| CL 1357+6232 |
|
|
|
|
|
|
|
|
|
| CL 1416+4446 |
|
|
|
|
|
|
|
|
|
| CL 1641+4001 |
|
|
|
|
|
|
|
|
|
| CL 1701+6414† |
|
|
|
|
|
|
|
|
|
Notes. Columns (1) to (3) give r200 and
cNFW from the default cluster models, and the
corresponding mass, .
Fixing the concentration to the value cB01 expected from
the Bullock et al. (2001) mass-concentration
relation, we obtain the best-fit radius
r200,B01 and mass
, in Cols. (4) to (6).
Columns (7) to (9) contain the respective quantities calculated assuming the Bhattacharya et al. (2011) mass-concentration
relation.
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