Preparation of Kepler light curves for asteroseismic analyses

R. A. García; S. Hekker; D. Stello; J. Gutiérrez-Soto; R. Handberg; D. Huber; C. Karoff; K. Uytterhoeven; T. Appourchaux; W. J. Chaplin; Y. Elsworth; S. Mathur; J. Ballot; J. Christensen-Dalsgaard; R. L. Gilliland; G. Houdek; J. M. Jenkins; H. Kjeldsen; S. McCauliff; T. Metcalfe; C. K. Middour; J. Molenda-Zakowicz; M. J.P.F.G. Monteiro; J. C. Smith; M. J. Thompson

doi:10.1111/j.1745-3933.2011.01042.x

Preparation of Kepler light curves for asteroseismic analyses

R. A. García, S. Hekker, D. Stello, J. Gutiérrez-Soto, R. Handberg, D. Huber, C. Karoff, K. Uytterhoeven, T. Appourchaux, W. J. Chaplin, Y. Elsworth, S. Mathur, J. Ballot, J. Christensen-Dalsgaard, R. L. Gilliland, G. Houdek, J. M. Jenkins, H. Kjeldsen, S. McCauliff, T. MetcalfeC. K. Middour, J. Molenda-Zakowicz, M. J.P.F.G. Monteiro, J. C. Smith, M. J. Thompson

Astronomy & Astrophysics

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162 Scopus citations

Abstract

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.

Original language	English (US)
Pages (from-to)	L6-L10
Journal	Monthly Notices of the Royal Astronomical Society: Letters
Volume	414
Issue number	1
DOIs	https://doi.org/10.1111/j.1745-3933.2011.01042.x
State	Published - Jun 2011

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All Science Journal Classification (ASJC) codes

Astronomy and Astrophysics
Space and Planetary Science

Cite this

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., ... Thompson, M. J. (2011). Preparation of Kepler light curves for asteroseismic analyses. Monthly Notices of the Royal Astronomical Society: Letters, 414(1), L6-L10. https://doi.org/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. / Preparation of Kepler light curves for asteroseismic analyses. In: Monthly Notices of the Royal Astronomical Society: Letters. 2011 ; Vol. 414, No. 1. pp. L6-L10.

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title = "Preparation of Kepler light curves for asteroseismic analyses",

abstract = "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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García, RA, Hekker, S, Stello, D, Gutiérrez-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, MJPFG, Smith, JC & Thompson, MJ 2011, 'Preparation of Kepler light curves for asteroseismic analyses', Monthly Notices of the Royal Astronomical Society: Letters, vol. 414, no. 1, pp. L6-L10. https://doi.org/10.1111/j.1745-3933.2011.01042.x

Preparation of Kepler light curves for asteroseismic analyses. / 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.

In: Monthly Notices of the Royal Astronomical Society: Letters, Vol. 414, No. 1, 06.2011, p. L6-L10.

Research output: Contribution to journal › Article

TY - JOUR

T1 - Preparation of Kepler light curves for asteroseismic analyses

AU - García, R. A.

AU - Hekker, S.

AU - Stello, D.

AU - Gutiérrez-Soto, J.

AU - Handberg, R.

AU - Huber, D.

AU - Karoff, C.

AU - Uytterhoeven, K.

AU - Appourchaux, T.

AU - Chaplin, W. J.

AU - Elsworth, Y.

AU - Mathur, S.

AU - Ballot, J.

AU - Christensen-Dalsgaard, J.

AU - Gilliland, R. L.

AU - Houdek, G.

AU - Jenkins, J. M.

AU - Kjeldsen, H.

AU - McCauliff, S.

AU - Metcalfe, T.

AU - Middour, C. K.

AU - Molenda-Zakowicz, J.

AU - Monteiro, M. J.P.F.G.

AU - Smith, J. C.

AU - Thompson, M. J.

PY - 2011/6

Y1 - 2011/6

N2 - 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.

AB - 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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SP - L6-L10

JO - Monthly Notices of the Royal Astronomical Society: Letters

JF - Monthly Notices of the Royal Astronomical Society: Letters

SN - 1745-3925

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10.1111/j.1745-3933.2011.01042.x