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  • "X" refers to XIS unit (0,1, or 3)
  • "Y" is the cluster name
  • "Z" refers to the band used in the fit (0520 = 0.5-2.0 keV;  2070 = 2.0-7.0 keV 
  •  The spectra are extracted from 3-6 arcmin annulus, centered on the cluster center
  • 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 "constr." fit in \[6.45 - 7.25\]/(1+z) band, i.e. with a prior for the emission measure.

                               INDIVIDUAL FITS

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