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TESS data for asteroseismology (T’DA) stellar variability classification pipeline : setup and application to the Kepler Q9 data
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Audenaert, J., Kuszlewicz, J. S., Handberg, R., Tkachenko, A., Armstrong, David J., Hon, M., Kgoadi, R., Lund, M. N., Bell, K. J., Bugnet, L., Bowman, D. M., Johnston, C., García, R. A., Stello, D., Molnár, L., Plachy, E., Buzasi, D. and Aerts, C. (2021) TESS data for asteroseismology (T’DA) stellar variability classification pipeline : setup and application to the Kepler Q9 data. The Astronomical Journal, 162 (5). 209. doi:10.3847/1538-3881/ac166a
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WRAP-TESS-data-asteroseismology-stellar-variability-classification-pipeline-set-up-2021.pdf - Accepted Version Embargoed item. Restricted access to Repository staff only until 21 October 2022. Contact author directly, specifying your specific needs. - Requires a PDF viewer. Download (4Mb) |
Official URL: https://doi.org/10.3847/1538-3881/ac166a
Abstract
The NASA Transiting Exoplanet Survey Satellite (TESS) is observing tens of millions of stars with time spans ranging from ∼27 days to about 1 yr of continuous observations. This vast amount of data contains a wealth of information for variability, exoplanet, and stellar astrophysics studies but requires a number of processing steps before it can be fully utilized. In order to efficiently process all the TESS data and make it available to the wider scientific community, the TESS Data for Asteroseismology working group, as part of the TESS Asteroseismic Science Consortium, has created an automated open-source processing pipeline to produce light curves corrected for systematics from the short- and long-cadence raw photometry data and to classify these according to stellar variability type. We will process all stars down to a TESS magnitude of 15. This paper is the next in a series detailing how the pipeline works. Here, we present our methodology for the automatic variability classification of TESS photometry using an ensemble of supervised learners that are combined into a metaclassifier. We successfully validate our method using a carefully constructed labeled sample of Kepler Q9 light curves with a 27.4 days time span mimicking single-sector TESS observations, on which we obtain an overall accuracy of 94.9%. We demonstrate that our methodology can successfully classify stars outside of our labeled sample by applying it to all ∼167,000 stars observed in Q9 of the Kepler space mission.
| Item Type: | Journal Article | |||||||||||||||||||||||||||||||||||||||||||||||||||
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| Subjects: | Q Science > QB Astronomy | |||||||||||||||||||||||||||||||||||||||||||||||||||
| Divisions: | Faculty of Science > Physics | |||||||||||||||||||||||||||||||||||||||||||||||||||
| SWORD Depositor: | Library Publications Router | |||||||||||||||||||||||||||||||||||||||||||||||||||
| Library of Congress Subject Headings (LCSH): | Astroseismology, Extrasolar planets, Machine learning | |||||||||||||||||||||||||||||||||||||||||||||||||||
| Journal or Publication Title: | The Astronomical Journal | |||||||||||||||||||||||||||||||||||||||||||||||||||
| Publisher: | American Astronomical Society | |||||||||||||||||||||||||||||||||||||||||||||||||||
| ISSN: | 1538-3881 | |||||||||||||||||||||||||||||||||||||||||||||||||||
| Official Date: | 21 October 2021 | |||||||||||||||||||||||||||||||||||||||||||||||||||
| Dates: |
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| Volume: | 162 | |||||||||||||||||||||||||||||||||||||||||||||||||||
| Number: | 5 | |||||||||||||||||||||||||||||||||||||||||||||||||||
| Article Number: | 209 | |||||||||||||||||||||||||||||||||||||||||||||||||||
| DOI: | 10.3847/1538-3881/ac166a | |||||||||||||||||||||||||||||||||||||||||||||||||||
| Status: | Peer Reviewed | |||||||||||||||||||||||||||||||||||||||||||||||||||
| Publication Status: | Published | |||||||||||||||||||||||||||||||||||||||||||||||||||
| Access rights to Published version: | Restricted or Subscription Access | |||||||||||||||||||||||||||||||||||||||||||||||||||
| Copyright Holders: | © 2021. The American Astronomical Society. All rights reserved. | |||||||||||||||||||||||||||||||||||||||||||||||||||
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