<?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%">Haberl, F.</style></author><author><style face="normal" font="default" size="100%">Vasilopoulos, G.</style></author><author><style face="normal" font="default" size="100%">Sturm, R.</style></author><author><style face="normal" font="default" size="100%">Maggi, P.</style></author></authors></contributors><titles><title><style face="normal" font="default" size="100%">Identification of IGR J01217-7257 with the transient pulsar XTE J0119-731 (SXP2.16) using XMM-Newton</style></title><short-title><style face="normal" font="default" size="100%">The Astronomer's Telegram</style></short-title></titles><keywords><keyword><style  face="normal" font="default" size="100%">Binary</style></keyword><keyword><style  face="normal" font="default" size="100%">Neutron Star</style></keyword><keyword><style  face="normal" font="default" size="100%">Pulsar</style></keyword><keyword><style  face="normal" font="default" size="100%">Transient</style></keyword></keywords><dates><year><style  face="normal" font="default" size="100%">2015</style></year><pub-dates><date><style  face="normal" font="default" size="100%">2015/11/1</style></date></pub-dates></dates><urls><web-urls><url><style face="normal" font="default" size="100%">https://ui.adsabs.harvard.edu/abs/2015ATel.8305....1H</style></url></web-urls></urls><volume><style face="normal" font="default" size="100%">8305</style></volume><pages><style face="normal" font="default" size="100%">1</style></pages><language><style face="normal" font="default" size="100%">eng</style></language><abstract><style face="normal" font="default" size="100%">We report first results from our XMM-Newton observation of IGR J01217-7257 performed on November 7, 2015. This transient in the Small Magellanic Cloud (Coe et al. 2014, ATel #5806) was found to be in a new outburst during Integral observations end of October 2015 (Coe et al. 2015, ATel #8246).</style></abstract></record></records></xml>