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The script files bestfit....xcm will set up the best fit. In more detail:
- The scripts use a 1-temperature phabs x mekal model.
- The column density is from Kalberla et al. (2005) and the absorption cross-sections are from Balucinska-Church & McCammon (1992).
- The scripts use the metal abundance table from Grevesse & Sauval (1998).
- 2. and 3. term in the script file name are the inner and outer radii of the spectrum extraction annulus in arcmin.
- *hard*, *soft* and *wide* refer to the fits done in 2.0-7.0 keV, 0.5-2.0 keV and 0.5-7.0 keV bands, respectively.
Wiki Markup *\*fe\** refers to the Fe XXV/XXVI fit in \[6.45 - 7.25\]/(1+z) band.
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Cluster Instrument
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