The tar files contain 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 XMM-Newton data with calibration information from December 2009.
XMM-Newton MOS1 and MOS2 spectra and responses are combined and referred to as MOS instrument.
For most clusters the Chandra data are obtained with ACIS-S, but for some ACIS-I is used, and marked accordingly.
Chandra data are processed with CIAO 4.2.
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.
For flux comparison, scale the measured fluxes to the full annulus by dividing with the fraction of the covered full annulus
Cluster Instrument
A1795 XMM-Newton/pn XMM-Newton/MOS Chandra/ACIS-S
A2029 XMM-Newton/pn XMM-Newton/MOS Chandra/ACIS-S
A2052 XMM-Newton/pn
A2199 XMM-Newton/pn
A262 XMM-Newton/pn
A3112 XMM-Newton/pn
A3571 XMM-Newton/pn
A85
Coma
HydraA
MKW3S