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In the bottom of this page you find the spectra, responses and background files necessary to reproduce the spectral analysis in Kettula et al., 2013 (A&A, 552, 47) which yielded results summarised in Fig 1. The results correspond to public SUZAKU calibration information in June 2011, i.e. XIS CALDB release
20110608\ and XRT CALDB release 20080709\

Fig.1: The average relative difference (diamonds) +- the error of the mean of the temperatures for different instrument pairs using the public calibration in June 2011 (blue line) and the modified contaminate used in the paper (green line) in the soft band (left side of the plot) and in the hard band (right side of the plot). The corresponding values for the hard band flux using the public contaminate are shown with red symbols and lines.



SUZAKU data are processed with HEASoft3 release 6.11, containing Suzaku ftools version
18, see details.

XMM-Newton data are processed with xmmsas 20110223 1801-11.0.0, see details.



*Cluster*                                          *Instrument*

A1060            Suzaku/XIS0       Suzaku/XIS1      Suzaku/XIS3   

A1795            Suzaku/XIS0       Suzaku/XIS1      Suzaku/XIS3   

A262              Suzaku/XIS0       Suzaku/XIS1      Suzaku/XIS3   

A3112            Suzaku/XIS0       Suzaku/XIS1      Suzaku/XIS3   

A496              Suzaku/XIS0       Suzaku/XIS1      Suzaku/XIS3   

AWM7            Suzaku/XIS0       Suzaku/XIS1      Suzaku/XIS3   

Centaurus       Suzaku/XIS0       Suzaku/XIS1      Suzaku/XIS3   

Coma             Suzaku/XIS0       Suzaku/XIS1      Suzaku/XIS3   

Ophiuchus      Suzaku/XIS0       Suzaku/XIS1      Suzaku/XIS3   

Triangulum      Suzaku/XIS0       Suzaku/XIS1      Suzaku/XIS3   

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