<?xml version="1.0" encoding="UTF-8"?><xml><records><record><source-app name="Biblio" version="7.x">Drupal-Biblio</source-app><ref-type>47</ref-type><contributors><authors><author><style face="normal" font="default" size="100%">Ulaş, Burak</style></author><author><style face="normal" font="default" size="100%">Ulusoy, Ceren</style></author><author><style face="normal" font="default" size="100%">Gazeas, Kosmas</style></author><author><style face="normal" font="default" size="100%">Erkan, Naci</style></author><author><style face="normal" font="default" size="100%">Liakos, Alexios</style></author></authors></contributors><titles><title><style face="normal" font="default" size="100%">A search for pulsations in two Algol-type systems V1241 Tau and GQ Dra</style></title><short-title><style face="normal" font="default" size="100%">Precision Asteroseismology</style></short-title></titles><keywords><keyword><style  face="normal" font="default" size="100%">Astrophysics - Solar and Stellar Astrophysics</style></keyword><keyword><style  face="normal" font="default" size="100%">Stars: binaries: eclipsing</style></keyword><keyword><style  face="normal" font="default" size="100%">stars: oscillations (including pulsations)</style></keyword></keywords><dates><year><style  face="normal" font="default" size="100%">2014</style></year><pub-dates><date><style  face="normal" font="default" size="100%">2014/02/1</style></date></pub-dates></dates><urls><web-urls><url><style face="normal" font="default" size="100%">https://ui.adsabs.harvard.edu/abs/2014IAUS..301..507U</style></url></web-urls></urls><volume><style face="normal" font="default" size="100%">301</style></volume><pages><style face="normal" font="default" size="100%">507 - 508</style></pages><isbn><style face="normal" font="default" size="100%">1743-9221</style></isbn><language><style face="normal" font="default" size="100%">eng</style></language><abstract><style face="normal" font="default" size="100%">We present new photometric observations of two eclipsing binary systems, V1241 Tau and GQ Dra. We use the following methodology: initially, the Wilson-Devinney code is applied to the light curves in order to determine the photometric elements of the systems. Then, the residuals are analysed using Fourier techniques. The results are the following. One frequency can be possibly attributed to a real light variation of V1241 Tau, while there is no evidence of pulsations in the light curve of GQ Dra.</style></abstract></record></records></xml>