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

A3571

A85

Coma

HydraA

MKW3S

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