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For most clusters the Chandra data are obtained with ACIS-S, but for some ACIS-I is used, and marked accordingly.

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

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• *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.

• Wiki Markup*\*fe\** refers to the Fe XXV/XXVI "constr." fit in \ [6.45 - 7.25\]/(1+z) band, i.e. with a prior for the emission measure.

For flux comparison, scale the measured fluxes to the full annulus by dividing with the fraction of the covered full annulus

The following links provide a single tar file for each cluster-instrument combination, containing the spectral analysis material described above:

Cluster                                                  Instrument

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MKW3S          XMM-Newton/pn       XMM-Newton/MOS       Chandra/ACIS-I

The following links contain some tabulated data from Nevalainen et al., 2010 paper in electronic form.

The first column gives the number X the of the cluster name AX, except for non-Abell names:
Coma = 1111, HydraA = 2222, MKW3S = 3333

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XMM-Newton pn, MOS1 and MOS2 wide band temperatures with large XMM-only regions

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Attachments