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.
Referencia bibliográfica
Monthly Notices of the Royal Astronomical Society: Letters, Volume 414, Issue 1, pp. L6-L10.
Fecha de publicación:
6
2011
Número de citas
271
Número de citas referidas
219
Descripción
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.