Bayesian frequency analysis of HD 201433 observations with BRITE
- Autor(en)
- T. Kallinger, W. W. Weiss
- Abstrakt
Multiple oscillation frequencies separated by close to or less than the
formal frequency resolution of a data set are a serious problem in the
frequency analysis of time series data. We present a new and fully
automated Bayesian approach that searches for close frequencies in time
series data and assesses their significance by comparison to no signal
and a mono-periodic signal. We extensively test the approach with
synthetic data sets and apply it to the 156 days-long high-precision
BRITE photometry of the SPB star HD 201433, for which we find a sequence
of nine statistically significant rotationally split dipole modes.
- Organisation(en)
- Institut für Astrophysik
- Journal
- Proceedings of the Polish Astronomical Society
- Publikationsdatum
- 11-2016
- ÖFOS 2012
- 103004 Astrophysik
- Schlagwörter
- Link zum Portal
- https://ucrisportal.univie.ac.at/de/publications/dd7c87a2-c85e-4bf6-9a42-2d7ffb0c2d70