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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 Figs. 1 and 2. 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 (red line) in the soft band.

 

Fig.2: The total amount of the hydrogen column density of the contaminant obtained by the spectral fits to the 0.5-2.0 kev band data when requiring consistent temperatures between the different XIS instruments (upper panel) and its difference from that implemented in the public calibration (lower panel).

Image Added

 

  • 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).

 

  • The spectra are extracted from 3-6 arcmin annulus, centered on the cluster center
  • 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).

 

                               INDIVIDUAL FITS

                ( Each cluster and instrument fitted separately , (see Table A.1 in Kettula et al., 2013)

...

Triangulum      Suzaku/XIS0       Suzaku/XIS1      Suzaku/XIS3   

 

The script files xisX_Y_3_6_am_circ_newcal_Z_mekalfit.xcm will set up the best fit. In more detail:

  • "X" refers to XIS unit (0,1, or 3)
  • "Y" is the cluster name
  • "Z" refers to the band used in the fit (0520 = 0.5-2.0 keV;  2070 = 2.0-7.0 keV

 

                                    JOINT

...

FITS

                (For each cluster all XIS instruments are fitted simultaneously, forcing the temperature and metal abundance equal between the instruments, and allowing Oxygen column density of the the  contaminant to vary , (see Tables 5 and 6 in Kettula et al., 2013)

 

Scripts

A1060

A1795

A262

A3112

A496

 

Unpack the files in the same directory.

Executing the Running XSPEC script do_mekalfit_simult_modcon.xcm performs file will run the spectral fits and produces

log files of the fit procedure  mekalfit_simult_modcon_Y.log

XSPEC session files mekalfit_simult_modcon_Y.xcm

and plots mekalfit_simult_modcon_Y.ps

of the best fits, where Y is the cluster name.

fits, assuming  your XSPEC has been installed from the source.

It will produce the log - files and ps - plots for each cluster. Due to an unfortunate XSPEC bug, saving the session does something wrong

and the resulting best-fit session (as reported in the log files) files are not available.

The local model for the contaminant is included in the distribution and will be set up automatically, provided your XSPEC has been installed from the source.