Preparation of Kepler light curves for asteroseismic analyses

Bibcode
2011MNRAS.414L...6G
DOI
10.1111/j.1745-3933.2011.01042.x
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 autores
25
Número de autores del IAC
0
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.
Tipo
Con árbitro
Asterosismología
Métodos

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