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Table 2
Best-fit (multi-)temperature model for each cluster.
| Source | Model | Source | Model |
|
|
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| 2A0335 | 2CIE | HCG62 | 2CIE |
| A85 | 2CIE | HYDRA | 2CIE |
| A133 | 2CIE | M 49 | 1CIE |
| A189 | 1CIE | M 86 | 2CIE |
| A262 | 2CIE | M 87 | 2CIE+PL |
| A496 | 2CIE | M 89 | 1CIE |
| A1795 | 2CIE | MKW3s | 2CIE |
| A1991 | 2CIE | MKW4 | 1CIE |
| A2029 | 2CIE | NGC 507 | 2CIE |
| A2052 | 2CIE | NGC 1316 | 2CIE |
| A2199 | 2CIE | NGC 1404 | 2CIE |
| A2597 | 2CIE | NGC 1550 | 2CIE |
| A2626 | 1CIE | NGC 3411 | 1CIE |
| A3112 | 2CIE | NGC 4261 | 1CIE |
| A3526 | 2CIE | NGC 4325 | 2CIE |
| A3581 | 2CIE | NGC 4374 | 2CIE |
| A4038 | 2CIE | NGC 4636 | 2CIE |
| A4059 | 2CIE | NGC 4649 | 1CIE |
| AS1101 | 2CIE | NGC 5044 | GDEM |
| AWM7 | 2CIE | NGC 5813 | 1CIE |
| EXO0422 | 2CIE | NGC 5846 | 2CIE |
| Fornax | 2CIE | Perseus | 2CIE+NH+PL |
Notes. CIE: single-temperature collisional ionization equilibrium model. GDEM: Gaussian differential emission measure model. PL: power-law model. NH: NH left free in fitting.
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