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 Metcalfe

CK Middour, J Molenda-Zakowicz, MJPF Monteiro, JC Smith, MJ Thompson

Research output: Contribution to journal › Article

177 Citations (Scopus)

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.",

keywords = "asteroseismology, methods: data analysis",

author = "RA Garc{\'i}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 William Chaplin and Yvonne Elsworth and S Mathur and J Ballot and J Christensen-Dalsgaard and RL Gilliland and G Houdek and JM Jenkins and H Kjeldsen and S McCauliff and T Metcalfe and CK Middour and J Molenda-Zakowicz and MJPF Monteiro and JC Smith and MJ Thompson",

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month = jun,

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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

Abstract

Keywords

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