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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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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
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