<?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%">Vasilopoulos, Georgios</style></author></authors></contributors><titles><title><style face="normal" font="default" size="100%">Measure spin-up of NGC 300 ULX-1</style></title><short-title><style face="normal" font="default" size="100%">Chandra Proposal</style></short-title></titles><dates><year><style  face="normal" font="default" size="100%">2017</style></year><pub-dates><date><style  face="normal" font="default" size="100%">2017/09/1</style></date></pub-dates></dates><urls><web-urls><url><style face="normal" font="default" size="100%">https://ui.adsabs.harvard.edu/abs/2017cxo..prop.5280V</style></url></web-urls></urls><pages><style face="normal" font="default" size="100%">5280</style></pages><language><style face="normal" font="default" size="100%">eng</style></language><abstract><style face="normal" font="default" size="100%">NGC 300 ULX-1 is a newly identified ULX pulsar. The system has shown a extraordinary spin up rate within the last year, when it spun-up from 31 sec to 20 sec. We request 2x10 ks chandra observations separated by 2-4 days in order to accurately measure the spin up rate of the pulsar.</style></abstract></record></records></xml>