VizieR Online Data Catalog: Solar-like oscillations in Kepler red giants (Hekker+, 2011)

S. Hekker; Y. Elsworth; J. De Ridder; B. Mosser; R. A. Garcia; T. Kallinger; S. Mathur; D. Huber; D. L. Buzasi; H. L. Preston; S. J. Hale; J. Ballot; W. J. Chaplin; C. Regulo; T. R. Bedding; D. Stello; W. J. Borucki; D. G. Koch; J. Jenkins; C. Allen; R. L. Gilliland; H. Kjeldsen; J. Christensen-Dalsgaard

VizieR Online Data Catalog: Solar-like oscillations in Kepler red giants (Hekker+, 2011)

S. Hekker
, Y. Elsworth
, J. De Ridder
, B. Mosser
, R. A. Garcia
, T. Kallinger
, S. Mathur
, D. Huber
, D. L. Buzasi
, H. L. Preston
, S. J. Hale
, J. Ballot
, W. J. Chaplin
, C. Regulo
, T. R. Bedding
, D. Stello
, W. J. Borucki
, D. G. Koch
, J. Jenkins
, C. Allen

R. L. Gilliland, H. Kjeldsen, J. Christensen-Dalsgaard

Publications: Electronic/multimedia output › Web publication

Abstract

For this investigation we use Kepler data obtained during the first four months of operation. These data have been analysed by different groups using already published methods and the results are compared. We also performed simulations to investigate the uncertainty on the resulting parameters due to different realizations of the stochastic signal.(1 data file).

Original language	English
Publication status	Published - 2011

Austrian Fields of Science 2012

103004 Astrophysics

Keywords

Stars: giant
Stars: late-type
Photometry

Access to Document

http://adsabs.harvard.edu/abs/2011yCat..35250131H

Cite this

Hekker, S., Elsworth, Y., De Ridder, J., Mosser, B., Garcia, R. A., Kallinger, T., Mathur, S., Huber, D., Buzasi, D. L., Preston, H. L., Hale, S. J., Ballot, J., Chaplin, W. J., Regulo, C., Bedding, T. R., Stello, D., Borucki, W. J., Koch, D. G., Jenkins, J., ... Christensen-Dalsgaard, J. (2011). VizieR Online Data Catalog: Solar-like oscillations in Kepler red giants (Hekker+, 2011). Web publication http://adsabs.harvard.edu/abs/2011yCat..35250131H

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title = "VizieR Online Data Catalog: Solar-like oscillations in Kepler red giants (Hekker+, 2011)",

abstract = "For this investigation we use Kepler data obtained during the first four months of operation. These data have been analysed by different groups using already published methods and the results are compared. We also performed simulations to investigate the uncertainty on the resulting parameters due to different realizations of the stochastic signal.(1 data file).",

keywords = "Stars: giant, Stars: late-type, Photometry",

author = "S. Hekker and Y. Elsworth and \{De Ridder\}, J. and B. Mosser and Garcia, \{R. A.\} and T. Kallinger and S. Mathur and D. Huber and Buzasi, \{D. L.\} and Preston, \{H. L.\} and Hale, \{S. J.\} and J. Ballot and Chaplin, \{W. J.\} and C. Regulo and Bedding, \{T. R.\} and D. Stello and Borucki, \{W. J.\} and Koch, \{D. G.\} and J. Jenkins and C. Allen and Gilliland, \{R. L.\} and H. Kjeldsen and J. Christensen-Dalsgaard",

year = "2011",

language = "English",

}

Hekker, S, Elsworth, Y, De Ridder, J, Mosser, B, Garcia, RA, Kallinger, T, Mathur, S, Huber, D, Buzasi, DL, Preston, HL, Hale, SJ, Ballot, J, Chaplin, WJ, Regulo, C, Bedding, TR, Stello, D, Borucki, WJ, Koch, DG, Jenkins, J, Allen, C, Gilliland, RL, Kjeldsen, H & Christensen-Dalsgaard, J, VizieR Online Data Catalog: Solar-like oscillations in Kepler red giants (Hekker+, 2011), 2011, Web publication. <http://adsabs.harvard.edu/abs/2011yCat..35250131H>

TY - ADVS

T1 - VizieR Online Data Catalog: Solar-like oscillations in Kepler red giants (Hekker+, 2011)

AU - Hekker, S.

AU - Elsworth, Y.

AU - De Ridder, J.

AU - Mosser, B.

AU - Garcia, R. A.

AU - Kallinger, T.

AU - Mathur, S.

AU - Huber, D.

AU - Buzasi, D. L.

AU - Preston, H. L.

AU - Hale, S. J.

AU - Ballot, J.

AU - Chaplin, W. J.

AU - Regulo, C.

AU - Bedding, T. R.

AU - Stello, D.

AU - Borucki, W. J.

AU - Koch, D. G.

AU - Jenkins, J.

AU - Allen, C.

AU - Gilliland, R. L.

AU - Kjeldsen, H.

AU - Christensen-Dalsgaard, J.

PY - 2011

Y1 - 2011

N2 - For this investigation we use Kepler data obtained during the first four months of operation. These data have been analysed by different groups using already published methods and the results are compared. We also performed simulations to investigate the uncertainty on the resulting parameters due to different realizations of the stochastic signal.(1 data file).

AB - For this investigation we use Kepler data obtained during the first four months of operation. These data have been analysed by different groups using already published methods and the results are compared. We also performed simulations to investigate the uncertainty on the resulting parameters due to different realizations of the stochastic signal.(1 data file).

KW - Stars: giant

KW - Stars: late-type

KW - Photometry

M3 - Web publication

ER -