J/A+A/629/A21           TEA-Phot python code                     (Bowman+, 2019)

Adaptive elliptical aperture photometry: A software package for high-cadence ground-based photometry? I. Application to rapid oscillators observed from SAAO. Bowman D.M., Holdsworth D.L. <Astron. Astrophys. 629, A21 (2019)> =2019A&A...629A..21B 2019A&A...629A..21B (SIMBAD/NED BibCode)
ADC_Keywords: Models Keywords: techniques: photometric - stars: chemically peculiar - stars: oscillations - stars: early-type - Abstract: 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 on the order of 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. 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. 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 employed our software package to search for rapid oscillations in three candidate roAp stars. 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. 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. Description: This is the [adapTive Elliptical Aperture PHOTometry (TEA-Phot)](https://bitbucket.org/DominicBowman/tea-phot) repository **TEA-Phot** is a user-friendly pipeline to process ground-based photometry and extract light curves of stars for the purpose of variability and asteroseismology. **TEA-Phot** is coded in python and has no external software dependencies such as IRAF, DS9 or Gaia, and utilises the flexible python module [SEP](https://sep.readthedocs.io/en/v1.0.x/) at its core. The code is optimised for high-cadence ground-based photometry, such as that provided by the SHOC and STE instruments at the [South African Astronomical Observatory (SAAO)](https://www.saao.ac.za), but can be easily modified for different instruments at different observatories. **TEA-Phot** is an open-source package, GNU-licensed, and any improvements provided by the users are well accepted. See disclaimer below and GNU License in gpl-3.0.txt. Get **TEA-Phot** **TEA-Phot** is available on https://bitbucket.org/DominicBowman/tea-phot You can quickly clone this repository by typing "git clone https://bitbucket.org/DominicBowman/tea-phot.git" Authors: Written and developed by Dominic Bowman, dominic.bowman(at)kuleuven.be, Instituut voor Sterrenkunde, KU Leuven, Belgium and Daniel Holdsworth, dlholdsworth(at)uclan.ac.uk, Jeremiah Horrocks Institute, University of Central Lancashire, UK Disclaimer **TEA-Phot** is provided "as it is", without any warranty. The Authors assume no liability for any damages of any kind (direct or indirect damages, contractual or non-contractual damages, pecuniary or non-pecuniary damages), directly or indirectly derived or arising from the correct or incorrect usage of **TEA-Phot**, in any possible environment, or arising from the impossibility to use, fully or partially, the software, or any bug or malfunction. Such exclusion of liability expressly includes any damages including the loss of data of any kind (including personal data). File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file TEA-Phot.py 185 1897 TEA-Phot python code -------------------------------------------------------------------------------- Acknowledgements: Dominic Bowman, dominic.bowman(at)kuleuven.be
(End) Patricia Vannier [CDS] 02-Aug-2019
The document above follows the rules of the Standard Description for Astronomical Catalogues; from this documentation it is possible to generate f77 program to load files into arrays or line by line