Information Bulletin on Variable Stars, cilt.1, sa.6125, 2015 (Scopus)
Reduction of the CCD frames and differential photometry were performed with the standard tasks of IRAF package. The minima times of eclipsing binaries were calculated using Kwee & van Woerden’s (1956) method. Mid-transit times were calculated by making use of a model-fitting algorithm available via the Exoplanet Transit Database (Poddany et al. 2010).