<?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%">Hofmann, F.</style></author><author><style face="normal" font="default" size="100%">Sturm, R.</style></author><author><style face="normal" font="default" size="100%">Greiner, J.</style></author><author><style face="normal" font="default" size="100%">Vasilopoulos, G.</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%">New Swift UVOT transient SWIFT J004255.6+411412 in M 31</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%">Nova</style></keyword><keyword><style  face="normal" font="default" size="100%">Star</style></keyword><keyword><style  face="normal" font="default" size="100%">Transient</style></keyword><keyword><style  face="normal" font="default" size="100%">Ultra-Violet</style></keyword></keywords><dates><year><style  face="normal" font="default" size="100%">2013</style></year><pub-dates><date><style  face="normal" font="default" size="100%">2013/05/1</style></date></pub-dates></dates><urls><web-urls><url><style face="normal" font="default" size="100%">https://ui.adsabs.harvard.edu/abs/2013ATel.5091....1H</style></url></web-urls></urls><volume><style face="normal" font="default" size="100%">5091</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%">In a monitoring observation of the central region of the Andromeda Galaxy (M 31) with the Ultra-violet/Optical Telescope (UVOT) on board the Swift satellite (ObsID 00035336102, starting 2013-05-27.15 UT), we detected a new UV transient (UVW1 filter, 181-321 nm). The source is located at RA 00h 42m 55.62s, Dec +41d 14' 12.3&quot; (± 0.5&quot;, J2000, 90% confidence level). The following table lists the Swift ObsID, the MJD at the beginning of the exposure, UVW1 magnitudes (Vega system), and 1σ statistical uncertainties.</style></abstract></record></records></xml>