<?xml version="1.0" encoding="UTF-8"?><xml><records><record><source-app name="Biblio" version="7.x">Drupal-Biblio</source-app><ref-type>17</ref-type><contributors><authors><author><style face="normal" font="default" size="100%">Kavanagh, P. J.</style></author><author><style face="normal" font="default" size="100%">Sasaki, M.</style></author><author><style face="normal" font="default" size="100%">Breitschwerdt, D.</style></author><author><style face="normal" font="default" size="100%">de Avillez, M. A.</style></author><author><style face="normal" font="default" size="100%">Filipovic, M. D.</style></author><author><style face="normal" font="default" size="100%">Galvin, T.</style></author><author><style face="normal" font="default" size="100%">Haberl, F.</style></author><author><style face="normal" font="default" size="100%">Hatzidimitriou, D.</style></author><author><style face="normal" font="default" size="100%">Henze, M.</style></author><author><style face="normal" font="default" size="100%">Plucinsky, P. P.</style></author><author><style face="normal" font="default" size="100%">Saeedi, S.</style></author><author><style face="normal" font="default" size="100%">Sokolovsky, K. V.</style></author><author><style face="normal" font="default" size="100%">Williams, B. F.</style></author></authors></contributors><titles><title><style face="normal" font="default" size="100%">VizieR Online Data Catalog: Northern disk of M31 XMM-Newton images (Kavanagh+, 2020)</style></title><short-title><style face="normal" font="default" size="100%">VizieR Online Data Catalog</style></short-title></titles><keywords><keyword><style  face="normal" font="default" size="100%">Galaxies: nearby</style></keyword><keyword><style  face="normal" font="default" size="100%">Interstellar medium</style></keyword><keyword><style  face="normal" font="default" size="100%">X-ray sources</style></keyword></keywords><dates><year><style  face="normal" font="default" size="100%">2020</style></year><pub-dates><date><style  face="normal" font="default" size="100%">2020/04/1</style></date></pub-dates></dates><urls><web-urls><url><style face="normal" font="default" size="100%">https://ui.adsabs.harvard.edu/abs/2020yCat..36370012K</style></url></web-urls></urls><pages><style face="normal" font="default" size="100%">J/A+A/637/A12</style></pages><language><style face="normal" font="default" size="100%">eng</style></language><abstract><style face="normal" font="default" size="100%">Figure1&lt;SUB&gt;0.4-0.7keV.fits and Figure1&lt;/SUB&gt;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&lt;SUP&gt;2&lt;/SUP&gt;. See Section 2.1.1 for more details. &lt;P /&gt;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. &lt;P /&gt;(2 data files).</style></abstract></record></records></xml>