Predicting the detectability of oscillations in solar-type stars observed by Kepler

W. J. Chaplin, H. Kjeldsen, T. R. Bedding, J. Christensen-Dalsgaard, Ronald Lynn Gilliland, S. D. Kawaler, T. Appourchaux, Y. Elsworth, R. A. García, G. Houdek, C. Karoff, T. S. Metcalfe, J. Molenda-Akowicz, M. J.P.F.G. Monteiro, M. J. Thompson, G. A. Verner, N. Batalha, W. J. Borucki, T. M. Brown, S. T. BrysonJ. L. Christiansen, B. D. Clarke, J. M. Jenkins, T. C. Klaus, D. Koch, D. An, J. Ballot, S. Basu, O. Benomar, A. Bonanno, A. M. Broomhall, T. L. Campante, E. Corsaro, O. L. Creevey, L. Esch, N. Gai, P. Gaulme, S. J. Hale, R. Handberg, S. Hekker, D. Huber, S. Mathur, B. Mosser, R. New, M. H. Pinsonneault, D. Pricopi, P. O. Quirion, C. Régulo, I. W. Roxburgh, D. Salabert, D. Stello, M. D. Suran

Research output: Contribution to journalArticle

69 Citations (Scopus)

Abstract

Asteroseismology of solar-type stars has an important part to play in the exoplanet program of the NASA Kepler Mission. Precise and accurate inferences on the stellar properties that are made possible by the seismic data allow very tight constraints to be placed on the exoplanetary systems. Here, we outline how to make an estimate of the detectability of solar-like oscillations in any given Kepler target, using rough estimates of the temperature and radius, and the Kepler apparent magnitude.

Original languageEnglish (US)
Article number54
JournalAstrophysical Journal
Volume732
Issue number1
DOIs
StatePublished - May 1 2011

Fingerprint

seismic data
oscillation
Kepler mission
solar oscillations
asteroseismology
stars
oscillations
extrasolar planets
estimates
inference
temperature
radii
programme

All Science Journal Classification (ASJC) codes

  • Astronomy and Astrophysics
  • Space and Planetary Science

Cite this

Chaplin, W. J., Kjeldsen, H., Bedding, T. R., Christensen-Dalsgaard, J., Gilliland, R. L., Kawaler, S. D., ... Suran, M. D. (2011). Predicting the detectability of oscillations in solar-type stars observed by Kepler. Astrophysical Journal, 732(1), [54]. https://doi.org/10.1088/0004-637X/732/1/54
Chaplin, W. J. ; Kjeldsen, H. ; Bedding, T. R. ; Christensen-Dalsgaard, J. ; Gilliland, Ronald Lynn ; Kawaler, S. D. ; Appourchaux, T. ; Elsworth, Y. ; García, R. A. ; Houdek, G. ; Karoff, C. ; Metcalfe, T. S. ; Molenda-Akowicz, J. ; Monteiro, M. J.P.F.G. ; Thompson, M. J. ; Verner, G. A. ; Batalha, N. ; Borucki, W. J. ; Brown, T. M. ; Bryson, S. T. ; Christiansen, J. L. ; Clarke, B. D. ; Jenkins, J. M. ; Klaus, T. C. ; Koch, D. ; An, D. ; Ballot, J. ; Basu, S. ; Benomar, O. ; Bonanno, A. ; Broomhall, A. M. ; Campante, T. L. ; Corsaro, E. ; Creevey, O. L. ; Esch, L. ; Gai, N. ; Gaulme, P. ; Hale, S. J. ; Handberg, R. ; Hekker, S. ; Huber, D. ; Mathur, S. ; Mosser, B. ; New, R. ; Pinsonneault, M. H. ; Pricopi, D. ; Quirion, P. O. ; Régulo, C. ; Roxburgh, I. W. ; Salabert, D. ; Stello, D. ; Suran, M. D. / Predicting the detectability of oscillations in solar-type stars observed by Kepler. In: Astrophysical Journal. 2011 ; Vol. 732, No. 1.
@article{af3fa4517ef5480fa718bcbba6bc52b1,
title = "Predicting the detectability of oscillations in solar-type stars observed by Kepler",
abstract = "Asteroseismology of solar-type stars has an important part to play in the exoplanet program of the NASA Kepler Mission. Precise and accurate inferences on the stellar properties that are made possible by the seismic data allow very tight constraints to be placed on the exoplanetary systems. Here, we outline how to make an estimate of the detectability of solar-like oscillations in any given Kepler target, using rough estimates of the temperature and radius, and the Kepler apparent magnitude.",
author = "Chaplin, {W. J.} and H. Kjeldsen and Bedding, {T. R.} and J. Christensen-Dalsgaard and Gilliland, {Ronald Lynn} and Kawaler, {S. D.} and T. Appourchaux and Y. Elsworth and Garc{\'i}a, {R. A.} and G. Houdek and C. Karoff and Metcalfe, {T. S.} and J. Molenda-Akowicz and Monteiro, {M. J.P.F.G.} and Thompson, {M. J.} and Verner, {G. A.} and N. Batalha and Borucki, {W. J.} and Brown, {T. M.} and Bryson, {S. T.} and Christiansen, {J. L.} and Clarke, {B. D.} and Jenkins, {J. M.} and Klaus, {T. C.} and D. Koch and D. An and J. Ballot and S. Basu and O. Benomar and A. Bonanno and Broomhall, {A. M.} and Campante, {T. L.} and E. Corsaro and Creevey, {O. L.} and L. Esch and N. Gai and P. Gaulme and Hale, {S. J.} and R. Handberg and S. Hekker and D. Huber and S. Mathur and B. Mosser and R. New and Pinsonneault, {M. H.} and D. Pricopi and Quirion, {P. O.} and C. R{\'e}gulo and Roxburgh, {I. W.} and D. Salabert and D. Stello and Suran, {M. D.}",
year = "2011",
month = "5",
day = "1",
doi = "10.1088/0004-637X/732/1/54",
language = "English (US)",
volume = "732",
journal = "Astrophysical Journal",
issn = "0004-637X",
publisher = "IOP Publishing Ltd.",
number = "1",

}

Chaplin, WJ, Kjeldsen, H, Bedding, TR, Christensen-Dalsgaard, J, Gilliland, RL, Kawaler, SD, Appourchaux, T, Elsworth, Y, García, RA, Houdek, G, Karoff, C, Metcalfe, TS, Molenda-Akowicz, J, Monteiro, MJPFG, Thompson, MJ, Verner, GA, Batalha, N, Borucki, WJ, Brown, TM, Bryson, ST, Christiansen, JL, Clarke, BD, Jenkins, JM, Klaus, TC, Koch, D, An, D, Ballot, J, Basu, S, Benomar, O, Bonanno, A, Broomhall, AM, Campante, TL, Corsaro, E, Creevey, OL, Esch, L, Gai, N, Gaulme, P, Hale, SJ, Handberg, R, Hekker, S, Huber, D, Mathur, S, Mosser, B, New, R, Pinsonneault, MH, Pricopi, D, Quirion, PO, Régulo, C, Roxburgh, IW, Salabert, D, Stello, D & Suran, MD 2011, 'Predicting the detectability of oscillations in solar-type stars observed by Kepler', Astrophysical Journal, vol. 732, no. 1, 54. https://doi.org/10.1088/0004-637X/732/1/54

Predicting the detectability of oscillations in solar-type stars observed by Kepler. / Chaplin, W. J.; Kjeldsen, H.; Bedding, T. R.; Christensen-Dalsgaard, J.; Gilliland, Ronald Lynn; Kawaler, S. D.; Appourchaux, T.; Elsworth, Y.; García, R. A.; Houdek, G.; Karoff, C.; Metcalfe, T. S.; Molenda-Akowicz, J.; Monteiro, M. J.P.F.G.; Thompson, M. J.; Verner, G. A.; Batalha, N.; Borucki, W. J.; Brown, T. M.; Bryson, S. T.; Christiansen, J. L.; Clarke, B. D.; Jenkins, J. M.; Klaus, T. C.; Koch, D.; An, D.; Ballot, J.; Basu, S.; Benomar, O.; Bonanno, A.; Broomhall, A. M.; Campante, T. L.; Corsaro, E.; Creevey, O. L.; Esch, L.; Gai, N.; Gaulme, P.; Hale, S. J.; Handberg, R.; Hekker, S.; Huber, D.; Mathur, S.; Mosser, B.; New, R.; Pinsonneault, M. H.; Pricopi, D.; Quirion, P. O.; Régulo, C.; Roxburgh, I. W.; Salabert, D.; Stello, D.; Suran, M. D.

In: Astrophysical Journal, Vol. 732, No. 1, 54, 01.05.2011.

Research output: Contribution to journalArticle

TY - JOUR

T1 - Predicting the detectability of oscillations in solar-type stars observed by Kepler

AU - Chaplin, W. J.

AU - Kjeldsen, H.

AU - Bedding, T. R.

AU - Christensen-Dalsgaard, J.

AU - Gilliland, Ronald Lynn

AU - Kawaler, S. D.

AU - Appourchaux, T.

AU - Elsworth, Y.

AU - García, R. A.

AU - Houdek, G.

AU - Karoff, C.

AU - Metcalfe, T. S.

AU - Molenda-Akowicz, J.

AU - Monteiro, M. J.P.F.G.

AU - Thompson, M. J.

AU - Verner, G. A.

AU - Batalha, N.

AU - Borucki, W. J.

AU - Brown, T. M.

AU - Bryson, S. T.

AU - Christiansen, J. L.

AU - Clarke, B. D.

AU - Jenkins, J. M.

AU - Klaus, T. C.

AU - Koch, D.

AU - An, D.

AU - Ballot, J.

AU - Basu, S.

AU - Benomar, O.

AU - Bonanno, A.

AU - Broomhall, A. M.

AU - Campante, T. L.

AU - Corsaro, E.

AU - Creevey, O. L.

AU - Esch, L.

AU - Gai, N.

AU - Gaulme, P.

AU - Hale, S. J.

AU - Handberg, R.

AU - Hekker, S.

AU - Huber, D.

AU - Mathur, S.

AU - Mosser, B.

AU - New, R.

AU - Pinsonneault, M. H.

AU - Pricopi, D.

AU - Quirion, P. O.

AU - Régulo, C.

AU - Roxburgh, I. W.

AU - Salabert, D.

AU - Stello, D.

AU - Suran, M. D.

PY - 2011/5/1

Y1 - 2011/5/1

N2 - Asteroseismology of solar-type stars has an important part to play in the exoplanet program of the NASA Kepler Mission. Precise and accurate inferences on the stellar properties that are made possible by the seismic data allow very tight constraints to be placed on the exoplanetary systems. Here, we outline how to make an estimate of the detectability of solar-like oscillations in any given Kepler target, using rough estimates of the temperature and radius, and the Kepler apparent magnitude.

AB - Asteroseismology of solar-type stars has an important part to play in the exoplanet program of the NASA Kepler Mission. Precise and accurate inferences on the stellar properties that are made possible by the seismic data allow very tight constraints to be placed on the exoplanetary systems. Here, we outline how to make an estimate of the detectability of solar-like oscillations in any given Kepler target, using rough estimates of the temperature and radius, and the Kepler apparent magnitude.

UR - http://www.scopus.com/inward/record.url?scp=79955606117&partnerID=8YFLogxK

UR - http://www.scopus.com/inward/citedby.url?scp=79955606117&partnerID=8YFLogxK

U2 - 10.1088/0004-637X/732/1/54

DO - 10.1088/0004-637X/732/1/54

M3 - Article

AN - SCOPUS:79955606117

VL - 732

JO - Astrophysical Journal

JF - Astrophysical Journal

SN - 0004-637X

IS - 1

M1 - 54

ER -

Chaplin WJ, Kjeldsen H, Bedding TR, Christensen-Dalsgaard J, Gilliland RL, Kawaler SD et al. Predicting the detectability of oscillations in solar-type stars observed by Kepler. Astrophysical Journal. 2011 May 1;732(1). 54. https://doi.org/10.1088/0004-637X/732/1/54