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. Metcalfe

C. K. Middour, J. Molenda-Zakowicz, M. J.P.F.G. Monteiro, J. C. Smith, M. J. Thompson

Astronomy & Astrophysics

Research output: Contribution to journal › Article › peer-review

245 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

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.\}",

year = "2011",

month = jun,

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

language = "English (US)",

volume = "414",

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journal = "Monthly Notices of the Royal Astronomical Society: Letters",

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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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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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IS - 1

ER -

Preparation of Kepler light curves for asteroseismic analyses

Abstract

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