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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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

All Science Journal Classification (ASJC) codes

Astronomy and Astrophysics
Space and Planetary Science

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10.1111/j.1745-3933.2011.01042.x

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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

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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.",

author = "Garc{\'i}a, {R. A.} and S. Hekker and D. Stello and J. Guti{\'e}rrez-Soto and R. Handberg and D. Huber and C. Karoff and K. Uytterhoeven and T. Appourchaux and Chaplin, {W. J.} and Y. Elsworth and S. Mathur and J. Ballot and J. Christensen-Dalsgaard and Gilliland, {R. L.} and G. Houdek and Jenkins, {J. M.} and H. Kjeldsen and S. McCauliff and T. Metcalfe and Middour, {C. K.} and J. Molenda-Zakowicz and Monteiro, {M. J.P.F.G.} and Smith, {J. C.} and Thompson, {M. J.}",

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doi = "10.1111/j.1745-3933.2011.01042.x",

language = "English (US)",

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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

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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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Preparation of Kepler light curves for asteroseismic analyses

Abstract

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