Monthly Notices of the Royal Astronomical Society: Letters, Volume 414, Issue 1, pp. L6-L10.
Bibcode
García, R. A.; Hekker, S.; Stello, D.; Gutiérrez-Soto, J.; Handberg, R.; Huber, D.; Karoff, C.; Uytterhoeven, K.; Appourchaux, T.; Chaplin, W. J.; Elsworth, Y.; Mathur, S.; Ballot, J.; Christensen-Dalsgaard, J.; Gilliland, R. L.; Houdek, G.; Jenkins, J. M.; Kjeldsen, H.; McCauliff, S.; Metcalfe, T.; Middour, C. K.; Molenda-Zakowicz, J.; Monteiro, M. J. P. F. G.; Smith, J. C.; Thompson, M. J.
Bibliographical reference
Advertised on:
6
2011
Citations
268
Refereed citations
218
Description
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.