Adaptive elliptical aperture photometry: a software package for high-cadence ground-based photometry. I. Application to rapid oscillators observed from SAAO
arXiv:1907.04421 · doi:10.1051/0004-6361/201935640
Abstract
Context. Modern space telescopes are currently providing high-precision light curves for a large fraction of the sky, such that many new variable stars are being discovered. However, some stars have periodic variability with periods of order minutes and require high-cadence photometry to probe the physical mechanisms responsible. A cadence of less than a minute is often required to remove Nyquist ambiguities and confirm rapid variability which forces observers to obtain high-cadence ground-based photometry. Aims. We aim to provide a modern software package to reduce ground-based photometric time series data and deliver optimised (differential) light curves. To produce high-quality light curves, which maximise the amplitude signal-to-noise ratio of short-period variability in a Fourier spectrum, we require adaptive elliptical aperture photometry as this represents a significant advantage compared to aperture photometry using circular apertures of fixed radii. Methods. The methodology of our code and its advantages are demonstrated using high-cadence ground-based photometry from the South African Astronomical Observatory (SAAO) of a confirmed rapidly oscillating Ap (roAp) star. Furthermore, we employ our software package to search for rapid oscillations in three candidate roAp stars. Results. We demonstrate that our pipeline represents a significant improvement in the quality of light curves, and we make it available to the community for use with different instruments and observatories. We search for and demonstrate the lack of high-frequency roAp pulsations to a limit of 1 mmag using B data in the three Ap stars HD 158596, HD 166542 and HD 181810. Conclusions. We demonstrate the significant improvement in the extraction of short-period variability caused by high-frequency pulsation modes, and discuss the implication of null detections in three Ap stars.
arXiv comment8 pages, accepted for publication in A&A
References in corpus (20)
- Astropy: A Community Python Package for Astronomy
- The Transiting Exoplanet Survey Satellite
- The K2 Mission: Characterization and Early results
- The CoRoT satellite in flight : description and performance
- Pulsating White Dwarf Stars and Precision Asteroseismology
- White Dwarf Rotation as a Function of Mass and a Dichotomy of Mode Linewidths: Kepler Observations of 27 Pulsating DA White Dwarfs Through K2 Campaign 8
- First Kepler results on compact pulsators I. Survey target selection and the first pulsators
- Rotation and pulsation in Ap stars: first light results from TESS sectors 1 and 2
- Magnetic OB[A] Stars with TESS: probing their Evolutionary and Rotational properties (MOBSTER) - I. First-light observations of known magnetic B and A stars
- GJ1214: Rotation period, starspots, and uncertainty on the optical slope of the transmission spectrum
- K2 space photometry reveals rotational modulation and stellar pulsations in chemically peculiar A and B stars
- Testing excitation models of rapidly oscillating Ap stars with interferometry
- Discovery of the longest-period rapidly oscillating Ap star HD177765
- The Nainital-Cape Survey-IV
- Suppressed phase variations in a high amplitude rapidly oscillating Ap star pulsating in a distorted quadrupole mode
- Detection of magnetic fields in chemically peculiar stars observed with the K2 space mission
- Whole Earth Telescope discovery of a strongly distorted quadrupole pulsation in the largest amplitude rapidly oscillating Ap star
- K2 observations of the rapidly oscillating Ap star 33 Lib (HD 137949): new frequencies and unique non-linear interactions
- MAIA, a three-channel imager for asteroseismology: instrument design
- Pulsation of magnetic stars