SIMBAD references

2011MNRAS.414L...6G - Mon. Not. R. Astron. Soc., 414, L6-L10 (2011/June-2)

Preparation of Kepler light curves for asteroseismic analyses.

GARCIA R.A., HEKKER S., STELLO D., GUTIERREZ-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. and THOMPSON M.J.

Abstract (from CDS):

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.

Abstract Copyright: 2011 The Authors Monthly Notices of the Royal Astronomical Society2011 RAS

Journal keyword(s): asteroseismology - methods: data analysis

Simbad objects: 2

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