Predicting the Detectability of Oscillations in Solar-type Stars Observed by Kepler

W.~J. Chaplin; H. Kjeldsen; T.~R. Bedding; J. Christensen-Dalsgaard; R.~L. Gilliland; S.~D. Kawaler; T. Appourchaux; Y. Elsworth; R.~A. García; G. Houdek; C. Karoff; T.~S. Metcalfe; J. Molenda-Zakowicz; M.~J.~P.~F.~G. Monteiro; M.~J. Thompson; G.~A. Verner; N. Batalha; W.~J. Borucki; T.~M. Brown; S.~T. Bryson; J.~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

doi:10.1088/0004-637X/732/1/54

Predicting the Detectability of Oscillations in Solar-type Stars Observed by Kepler

W.~J. Chaplin, H. Kjeldsen, T.~R. Bedding, J. Christensen-Dalsgaard, R.~L. Gilliland, S.~D. Kawaler, T. Appourchaux, Y. Elsworth, R.~A. García, G. Houdek, C. Karoff, T.~S. Metcalfe, J. Molenda-Zakowicz, 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

Physics and Astronomy

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

91 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 language	English
Pages (from-to)	54
Number of pages	1
Journal	The Astrophysical Journal
Volume	732
Issue number	1
DOIs	https://doi.org/10.1088/0004-637X/732/1/54
Publication status	Published - 1 May 2011

Keywords

stars: interiors, stars: late-type, stars: oscillations

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

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Chaplin, W. J., Kjeldsen, H., Bedding, T. R., Christensen-Dalsgaard, J., Gilliland, R. L., Kawaler, S. D., Appourchaux, T., Elsworth, Y., García, R. A., Houdek, G., Karoff, C., Metcalfe, T. S., Molenda-Zakowicz, J., Monteiro, M. J. P. F. G., Thompson, M. J., Verner, G. A., Batalha, N., Borucki, W. J., Brown, T. M., ... Suran, M. D. (2011). Predicting the Detectability of Oscillations in Solar-type Stars Observed by Kepler. The Astrophysical Journal, 732(1), 54. https://doi.org/10.1088/0004-637X/732/1/54

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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.",

keywords = "stars: interiors, stars: late-type, stars: oscillations",

author = "W.~J. Chaplin and H. Kjeldsen and T.~R. Bedding and J. Christensen-Dalsgaard and R.~L. Gilliland and S.~D. Kawaler and T. Appourchaux and Y. Elsworth and R.~A. Garc{\'i}a and G. Houdek and C. Karoff and T.~S. Metcalfe and J. Molenda-Zakowicz and M.~J.~P.~F.~G. Monteiro and M.~J. Thompson and G.~A. Verner and N. Batalha and W.~J. Borucki and T.~M. Brown and S.~T. Bryson and J.~L. Christiansen and B.~D. Clarke and J.~M. Jenkins and T.~C. Klaus and D. Koch and D. An and J. Ballot and S. Basu and O. Benomar and A. Bonanno and A.-M. Broomhall and T.~L. Campante and E. Corsaro and O.~L. Creevey and L. Esch and N. Gai and P. Gaulme and S.~J. Hale and R. Handberg and S. Hekker and D. Huber and S. Mathur and B. Mosser and R. New and M.~H. Pinsonneault and D. Pricopi and P.-O. Quirion and C. R{\'e}gulo and I.~W. Roxburgh and D. Salabert and D. Stello and M.~D. Suran",

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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-Zakowicz, 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, A-M, 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, P-O, Régulo, C, Roxburgh, IW, Salabert, D, Stello, D & Suran, MD 2011, 'Predicting the Detectability of Oscillations in Solar-type Stars Observed by Kepler', The Astrophysical Journal, vol. 732, no. 1, pp. 54. https://doi.org/10.1088/0004-637X/732/1/54

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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, R.~L.

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-Zakowicz, 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.

KW - stars: interiors, stars: late-type, stars: oscillations

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

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

M3 - Article

SN - 1538-4357

VL - 732

SP - 54

JO - The Astrophysical Journal

JF - The Astrophysical Journal

IS - 1

ER -

Predicting the Detectability of Oscillations in Solar-type Stars Observed by Kepler

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Keywords

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