Combining WASP and Kepler data: the case of the Sct star KIC 7106205
arXiv:1502.05555 · doi:10.1093/mnras/stv364
Abstract
Ground-based photometric observations from WASP have been calibrated, scaled and combined with Kepler observations of the Sct star KIC 7106205, allowing us to extend the time base of the study of the unexplained amplitude and frequency variation of a single pressure mode at d by 2 yr. Analysis of the combined data sets, spanning 6 yr, show that the amplitude modulation in KIC 7106205 has a much larger range than a previous study of the Kepler data alone indicated. The single pressure mode decreased from mmag in 2007, to mmag in 2009, and to mmag in 2013. Observations of the decrease in mode amplitude have now been extended back 2 yr before the launch of Kepler. With observations over a longer time span, we have been able to further investigate the decrease in mode amplitude in KIC 7106205 to address the question of mode amplitude stability in Sct stars. This study highlights the usefulness of the WASP data set for extending studies of some Kepler variable stars.
arXiv commentAccepted for publication in MNRAS
References in corpus (13)
- The WASP Project and the SuperWASP Cameras
- Kepler Mission Design, Realized Photometric Performance, and Early Science
- Kepler Input Catalog: Photometric Calibration and Stellar Classification
- Correcting systematic effects in a large set of photometric lightcurves
- Kepler Asteroseismology Program: Introduction and First Results
- Revised Stellar Properties of Kepler Targets for the Quarter 1-16 Transit Detection Run
- The Kepler characterization of the variability among A- and F-type stars. I. General overview
- High frequency A-type pulsators discovered using SuperWASP
- On the incidence of eclipsing Am binary systems in the SuperWASP survey
- Evidence of resonant mode coupling and the relationship between low and high frequencies in a rapidly rotating A star
- Pulsational Frequency and Amplitude Modulation in the \,Sct star KIC\,7106205
- KIC 7582608: A new Kepler roAp star with frequency variability
- Multimode Resonant Coupling in Pulsating Stars
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- Highlights of Discoveries for Scuti Variable Stars From the Kepler Era
- KIC5950759: a high-amplitude Sct star with amplitude and frequency modulation near the terminal age main sequence
- Suppressed phase variations in a high amplitude rapidly oscillating Ap star pulsating in a distorted quadrupole mode
- HD 41641: A classical Sct-type pulsator with chemical signatures of an Ap star
- Discovery and Characterization of Three New High-amplitude delta Scuti Stars from TESS Observations