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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 http://heasarc.gsfc.nasa.gov/docs/heasarc/caldb/data/suzaku/xis/^{Image Added}
index/cif suzaku xis 20110608.html
and XRT CALDB release 20080709 http://heasarc.gsfc.nasa.gov/docs/heasarc/caldb/data/suzaku/xrt/^{Image Added}
index/cif suzaku xrt 20080709.html

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.

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