Abstract
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.
Original language | English (US) |
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Pages (from-to) | L6-L10 |
Journal | Monthly Notices of the Royal Astronomical Society: Letters |
Volume | 414 |
Issue number | 1 |
DOIs | |
State | Published - Jun 2011 |
All Science Journal Classification (ASJC) codes
- Astronomy and Astrophysics
- Space and Planetary Science