V light curve of V567 Oph (Kiss+, 2002)

Computer Science

Scientific paper

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Stars: Variable, Photometry

Scientific paper

We present differential CCD photometry for the high-amplitude delta Scuti star V567 Ophiuchi obtained in the Johnson V-band. It was observed on 15 nights in two consecutive years in order to resolve the long-standing ambiguity related to its secondary period. A frequency analysis of almost 5000 individual single-filtered measurements resulted in two independent frequencies (f1=6.6879c/d and f2=11.8266c/d) with a ratio of f1/f2=0.565. The presented photometric data are differential magnitudes relative to the comparison star C1 (GSC 00417-01714) from Powell et al. (1990PASP..102.1131P)
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