Photometry of the Supersoft X Ray Source v Sagittae During Its Large Outburst in 2004

Abstract

New quadratic orbital elements of V Sge are presented. These was computed using 14 minima timings obtained in 2004. During this photometric campaing, the star was undergoing large outburst, which was measured in detail using CCD.

Publication
Open European Journal on Variable Stars, Vol. 23, Proceedings of the 37th Conference on Variable Stars Research, Edited by L. Brat., p.80
Ph.D. Candidate in Astrophysics and Research Assistant

My research interests include stellar astrophysics, data analysis and high-performance computing.