Table 6
Best-fit parameters of joint XIS spectral fits with modified contaminant.
| Name | kT a | Abundb | χ2/d.o.f.c |
| [keV] | Solar | ||
|
|
|||
| A1060 | 2.8 [2.7–2.9] | 0.37 [0.35–0.39] | 748.18/613 |
| A1795 | 4.2 [3.0–4.8] | 0.16 [0.12–0.24] | 242.37/246 |
| A262 | 2.1 [2.1–2.2] | 0.55 [0.52–0.59] | 444.91/380 |
| A3112 | 3.9 [3.7–4.1] | 0.33 [0.29–0.37] | 334.84/326 |
| A496 | 3.4 [3.2–3.6] | 0.29 [0.26–0.36] | 506.83/501 |
Notes. and of the 0.5–2.0 keV band spectral fits when forcing the temperatures and metal abundances to be equal in all instruments for a given cluster and allowing the oxygen column density of the contaminant to be a free parameter for all sources and instruments. The uncertainties are the statistical ones given at 1σ level.
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