@article {23773,
	title = {VizieR Online Data Catalog: Northern disk of M31 XMM-Newton images (Kavanagh+, 2020)},
	year = {2020},
	month = {2020/04/1},
	pages = {J/A+A/637/A12},
	abstract = {Figure1<SUB>0.4-0.7keV.fits and Figure1</SUB>0.7-1.25keV 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<SUP>2</SUP>. See Section 2.1.1 for more details. <P />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. <P />(2 data files).},
	keywords = {Galaxies: nearby, Interstellar medium, X-ray sources},
	url = {https://ui.adsabs.harvard.edu/abs/2020yCat..36370012K},
	author = {Kavanagh, P. J. and Sasaki, M. and Breitschwerdt, D. and de Avillez, M. A. and Filipovic, M. D. and Galvin, T. and Haberl, F. and Hatzidimitriou, D. and Henze, M. and Plucinsky, P. P. and Saeedi, S. and Sokolovsky, K. V. and Williams, B. F.}
}
