Abstract:
Figure1
0.4-0.7keV.fits and Figure10.7-1.25keV XMM-Newton mosaic images of M 31 in the 0.4-0.7keV and 0.7-1.25keV range. We used all XMM-Newton data up to and including our new observations (early 2016). To produce these mosaics we used the the XMM-Newton Extended Source Analysis Software (XMM-ESAS), packaged in SAS1 15.0.0. XMM-ESAS is based on the software used for the background modelling described by Snowden et al. (2004ApJ...610.1182S). The units of the images are cts/s/deg
2. See Section 2.1.1 for more details.
Figure2_0.4-1.25keV.fits. XMM-Newton image of the northern disk of M 31 in the 0.4-1.25keV range produced as in Figure 1. See Sections 2.1.1 and 2.2 for more details.
(2 data files).
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