Fig. A.6.
X-ray surface brightness profile of NGC 410 traced by the MOS detectors of XMM-Newton (data points with error bars). Also shown is the profile of the point spread function (dotted curve). The red lines show the best fit of a beta-model, where the dashed line gives the source profile convolved with the point spread function, which was fitted, and the solid line the deconvolved profile.
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