Times of minima of eclipsing binaries and mid-transit times of transiting exoplanets


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Baştürk Ö., Bahar E., Şenavcı H. V., Kılıçoğlu T., Özavcı İ., Burdanov A., ...Daha Fazla

Information Bulletin on Variable Stars, cilt.1, sa.6125, 2015 (Scopus) identifier

Özet

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).