Table 2.
Sample properties and results of NFW fits.
| Cluster | z | NH | R500, TOT | M500, TOT | M200, TOT | c200, TOT | M200, DM | c200, DM |
|---|---|---|---|---|---|---|---|---|
| 1020 cm−2 | kpc | 1014 M⊙ | 1014 M⊙ | 1014 M⊙ | ||||
| A85 | 0.0555 | 2.8 |
 |
 |
 |
 |
– | – |
| A644 | 0.0704 | 7.5 |
 |
 |
 |
 |
 |
 |
| A1644 | 0.0473 | 4.1 |
 |
 |
 |
 |
– | – |
| A1795 | 0.0622 | 1.2 |
 |
 |
 |
 |
 |
 |
| A2029 | 0.0766 | 3.2 |
 |
 |
 |
 |
 |
 |
| A2142 | 0.09 | 3.8 |
 |
 |
 |
 |
 |
 |
| A2255 | 0.0809 | 2.5 |
 |
 |
 |
 |
– | – |
| A2319 | 0.0557 | 3.2 |
 |
 |
 |
 |
 |
 |
| A3158 | 0.059 | 1.4 |
 |
 |
 |
 |
– | – |
| A3266 | 0.0589 | 1.6 |
 |
 |
 |
 |
– | – |
| RXC1825 | 0.065 | 9.4 |
 |
 |
 |
 |
– | – |
| Zw1215 | 0.0766 | 1.7 |
 |
 |
 |
 |
– | – |
Notes. The columns labeled “DM” refer to the NFW fits to the DM only for the five systems with complete information on the baryonic components (see Sect. 5.4), whereas the “TOT” subscripts refer to the fits of the total gravitational field with an NFW model (see Fig. 3). In this case, the quoted total mass is computed from the sum of DM and baryonic density profiles.
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