Preparation of Kepler light curves for asteroseismic analyses
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| Titre | Preparation of Kepler light curves for asteroseismic analyses |
| Type de publication | Journal Article |
| Year of Publication | 2011 |
| Auteurs | Garcia, RA, Hekker, S, Stello, D, Gutierrez-Soto, J, Handberg, R, Huber, D, Karoff, C, Uytterhoeven, K, Appourchaux, T, Chaplin, WJ, Elsworth, Y, Mathur, S, Ballot, J, Christensen-Dalsgaard, J, Gilliland, RL, Houdek, G, Jenkins, JM, Kjeldsen, H, McCauliff, S, Metcalfe, T, Middour, CK, Molenda-Zakowicz, J, Monteiro, M, Smith, JC, Thompson, MJ |
| Journal | Monthly Notices of the Royal Astronomical Society |
| Volume | 414 |
| Pagination | L6-L10 |
| Date Published | Jun |
| ISBN Number | 0035-8711 |
| Numéro d'accès | WOS:000292141600002 |
| Résumé | 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. |
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