Journal
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
Volume 414, Issue 1, Pages L6-L10Publisher
WILEY-BLACKWELL
DOI: 10.1111/j.1745-3933.2011.01042.x
Keywords
asteroseismology; methods: data analysis
Categories
Funding
- NASA's Science Mission
- Kepler team
- French PNPS programme
- UK Science and Technology Facilities Council
- Netherlands Organization for Scientific Research
- STFC [ST/F002041/1] Funding Source: UKRI
- Science and Technology Facilities Council [ST/F002041/1] Funding Source: researchfish
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The Kepler mission is providing photometric data of exquisite quality for the asteroseismic study of different classes of pulsating stars. These analyses place particular demands on the pre-processing of the data, over a range of time-scales from minutes to months. Here, we describe processing procedures developed by the Kepler Asteroseismic Science Consortium to prepare light curves that are optimized for the asteroseismic study of solar-like oscillating stars in which outliers, jumps and drifts are corrected.
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