Preparation of Kepler light curves for asteroseismic analyses

RA García; S Hekker; D Stello; J Gutiérrez-Soto; R Handberg; D Huber; C Karoff; K Uytterhoeven; T Appourchaux; William Chaplin; Yvonne Elsworth; S Mathur; J Ballot; J Christensen-Dalsgaard; RL Gilliland; G Houdek; JM Jenkins; H Kjeldsen; S McCauliff; T Metcalfe; CK Middour; J Molenda-Zakowicz; MJPF Monteiro; JC Smith; MJ Thompson

doi:10.1111/j.1745-3933.2011.01042.x

Preparation of Kepler light curves for asteroseismic analyses

RA García, S Hekker, D Stello, J Gutiérrez-Soto, R Handberg, D Huber, C Karoff, K Uytterhoeven, T Appourchaux, William Chaplin, Yvonne Elsworth, S Mathur, J Ballot, J Christensen-Dalsgaard, RL Gilliland, G Houdek, JM Jenkins, H Kjeldsen, S McCauliff, T MetcalfeCK Middour, J Molenda-Zakowicz, MJPF Monteiro, JC Smith, MJ Thompson

Physics and Astronomy

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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
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
Publication status	Published - 11 Jun 2011

Keywords

asteroseismology
methods: data analysis

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10.1111/j.1745-3933.2011.01042.x

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García, RA., Hekker, S., Stello, D., Gutiérrez-Soto, J., Handberg, R., Huber, D., Karoff, C., Uytterhoeven, K., Appourchaux, T., Chaplin, W., Elsworth, Y., Mathur, S., Ballot, J., Christensen-Dalsgaard, J., Gilliland, RL., Houdek, G., Jenkins, JM., Kjeldsen, H., McCauliff, S., ... Thompson, MJ. (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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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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doi = "10.1111/j.1745-3933.2011.01042.x",

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García, RA, Hekker, S, Stello, D, Gutiérrez-Soto, J, Handberg, R, Huber, D, Karoff, C, Uytterhoeven, K, Appourchaux, T, Chaplin, W , 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, MJPF, 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

TY - JOUR

T1 - Preparation of Kepler light curves for asteroseismic analyses

AU - García, RA

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, William

AU - Elsworth, Yvonne

AU - Mathur, S

AU - Ballot, J

AU - Christensen-Dalsgaard, J

AU - Gilliland, RL

AU - Houdek, G

AU - Jenkins, JM

AU - Kjeldsen, H

AU - McCauliff, S

AU - Metcalfe, T

AU - Middour, CK

AU - Molenda-Zakowicz, J

AU - Monteiro, MJPF

AU - Smith, JC

AU - Thompson, MJ

PY - 2011/6/11

Y1 - 2011/6/11

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.

KW - asteroseismology

KW - methods: data analysis

U2 - 10.1111/j.1745-3933.2011.01042.x

DO - 10.1111/j.1745-3933.2011.01042.x

M3 - Article

VL - 414

SP - L6-L10

JO - Monthly Notices of the Royal Astronomical Society: Letters

JF - Monthly Notices of the Royal Astronomical Society: Letters

IS - 1

ER -

Preparation of Kepler light curves for asteroseismic analyses

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Keywords

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