The tar file contains spectra, responses and background files necessary to reproduce the spectral analysis in Nevalainen et al., 2010, A&A, 523, 22.
SASv9.0 was used for processing the data. Calibration information is from December 2009.
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.
*fe* refers to the Fe XXV/XXVI fit in [6.45 - 7.25]/(1+z) band.
Cluster Instrument
A1795 XMM-Newton/pn XMM-Newton/MOS1 XMM-Newton/MOS2 Chandra/ACIS-S Chandra/ACIS-I
A2029
A2052
A2199
A262
A3112
A3571
A85
Coma
HydraA
MKW3S