<?xml version="1.0" encoding="UTF-8"?><xml><records><record><source-app name="Biblio" version="7.x">Drupal-Biblio</source-app><ref-type>13</ref-type><contributors><authors><author><style face="normal" font="default" size="100%">Maggi, P.</style></author><author><style face="normal" font="default" size="100%">Haberl, F.</style></author><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%">Bozzetto, L. M.</style></author><author><style face="normal" font="default" size="100%">Filipovic, M. D.</style></author><author><style face="normal" font="default" size="100%">Vasilopoulos, G.</style></author><author><style face="normal" font="default" size="100%">Pietsch, W.</style></author><author><style face="normal" font="default" size="100%">Points, S. D.</style></author><author><style face="normal" font="default" size="100%">Chu, Y. -H.</style></author><author><style face="normal" font="default" size="100%">Dickel, J.</style></author><author><style face="normal" font="default" size="100%">Ehle, M.</style></author><author><style face="normal" font="default" size="100%">Williams, R.</style></author><author><style face="normal" font="default" size="100%">Greiner, J.</style></author></authors></contributors><titles><title><style face="normal" font="default" size="100%">VizieR Online Data Catalog: X-ray supernova remnants in LMC (Maggi+, 2016)</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%">Magellanic Clouds</style></keyword><keyword><style  face="normal" font="default" size="100%">Supernova Remnants</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%">2016</style></year><pub-dates><date><style  face="normal" font="default" size="100%">2016/03/1</style></date></pub-dates></dates><urls><web-urls><url><style face="normal" font="default" size="100%">https://ui.adsabs.harvard.edu/abs/2016yCat..35850162M</style></url></web-urls></urls><volume><style face="normal" font="default" size="100%">358</style></volume><pages><style face="normal" font="default" size="100%">J/A+A/585/A162</style></pages><language><style face="normal" font="default" size="100%">eng</style></language><abstract><style face="normal" font="default" size="100%">The processing of all available XMM-Newton data in the LMC region, and those of the VLP survey in particular, was done with the data reduction pipeline developed in our research group over several years. Various non-X-ray data were used to supplement the XMM-Newton observations. They allow us to assess e.g. the relation between the population of SNRs and large scale structure of the LMC, or to evaluate doubtful candidates in the sample compilation. We compiled a sample of 59 definite SNRs, cleaned of misclassified objects and doubtful candidates. &lt;P /&gt;(2 data files).</style></abstract></record></records></xml>