<?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%">Coley, J. B.</style></author><author><style face="normal" font="default" size="100%">Fuerst, F.</style></author><author><style face="normal" font="default" size="100%">Hemphill, P.</style></author><author><style face="normal" font="default" size="100%">Kretschmar, P.</style></author><author><style face="normal" font="default" size="100%">Pottschmidt, K.</style></author><author><style face="normal" font="default" size="100%">Jaisawal, G. K.</style></author><author><style face="normal" font="default" size="100%">Malacaria, C.</style></author><author><style face="normal" font="default" size="100%">Vasilopoulos, G.</style></author><author><style face="normal" font="default" size="100%">Wilms, J.</style></author><author><style face="normal" font="default" size="100%">Wolff, M.</style></author></authors></contributors><titles><title><style face="normal" font="default" size="100%">Possible discovery of a cyclotron line in 4U 1901+03 with NuSTAR</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%">Neutron Star</style></keyword><keyword><style  face="normal" font="default" size="100%">Pulsar</style></keyword></keywords><dates><year><style  face="normal" font="default" size="100%">2019</style></year><pub-dates><date><style  face="normal" font="default" size="100%">2019/04/1</style></date></pub-dates></dates><urls><web-urls><url><style face="normal" font="default" size="100%">https://ui.adsabs.harvard.edu/abs/2019ATel12684....1C</style></url></web-urls></urls><volume><style face="normal" font="default" size="100%">12684</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 on a NuSTAR observation of the Be X-ray binary 4U 1901+03 taken on 2019 April 11.95 (MJD 58584.95; ObsID 90502307004). It was performed during the decline of the source's current outburst, which began around 2019-02-08 (ATel #12498, GCN #23882).</style></abstract></record></records></xml>