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 (blue line) and the modified contaminate (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.
*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