Preparation of Kepler lightcurves for asteroseismic analyses

Details Preparation of Kepler lightcurves for asteroseismic analyses Preparation of Kepler lightcurves for asteroseismic analyses

2011-03-02

arxiv.org/abs/1103.0382v1

Astronomy and Astrophysics

Astrophysics

Solar and Stellar Astrophysics

Accepted for publication in MNRAS. 5 pages, 2 figures

Scientific paper

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 timescales from minutes to months. Here, we describe processing procedures developed by the Kepler Asteroseismic Science Consortium (KASC) 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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