Abstract
Recent wide field photometric surveys, which target a specific field for long durations, are ideal for studying both long- and short-period stellar variability. Here, we report on 75 variable stars detected during the observations of a field in Pegasus using the Wide Angle Search for Planets Prototype (WASP0) instrument, 73 of which are new discoveries. The variables detected include 16 δ Scuti stars, 34 eclipsing binaries, 3 BY Draconis stars and 4 RR Lyraes. We estimate that the fraction of stars in the field brighter than V ∼ 13.5 exhibiting variable behaviour with an amplitude greater than 0.6 per cent rms is ∼0.4 per cent. These results are compared with other wide field stellar variability surveys, and implications for detecting transits due to extra-solar planets are discussed. © 2005 RAS.
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Kane, S. R., Lister, T. A., Cameron, A. C., Home, K., James, D., Pollacco, D. L., … Tsapras, Y. (2005). Results from the Wide Angle Search for Planets Prototype (WASP0) - II. Stellar variability in the pegasus field. Monthly Notices of the Royal Astronomical Society, 362(1), 117–126. https://doi.org/10.1111/j.1365-2966.2005.09286.x
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