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Mikkel Nørup Lund

Limits on Surface Gravities of Kepler Planet-candidate Host Stars from Non-detection of Solar-like Oscillations

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Limits on Surface Gravities of Kepler Planet-candidate Host Stars from Non-detection of Solar-like Oscillations. / Campante, T. L.; Chaplin, W. J.; Lund, M. N.; Huber, D.; Hekker, S.; García, R. A.; Corsaro, E.; Handberg, R.; Miglio, A.; Arentoft, T.; Basu, S.; Bedding, T. R.; Christensen-Dalsgaard, J.; Davies, G. R.; Elsworth, Y. P.; Gilliland, R. L.; Karoff, C.; Kawaler, S. D.; Kjeldsen, H.; Lundkvist, M.; Metcalfe, T. S.; Silva Aguirre, V.; Stello, D.

I: Astrophysical Journal, Bind 783, Nr. 2, 123, 01.03.2014.

Publikation: Bidrag til tidsskrift/Konferencebidrag i tidsskrift /Bidrag til avisTidsskriftartikelForskningpeer review

Harvard

Campante, TL, Chaplin, WJ, Lund, MN, Huber, D, Hekker, S, García, RA, Corsaro, E, Handberg, R, Miglio, A, Arentoft, T, Basu, S, Bedding, TR, Christensen-Dalsgaard, J, Davies, GR, Elsworth, YP, Gilliland, RL, Karoff, C, Kawaler, SD, Kjeldsen, H, Lundkvist, M, Metcalfe, TS, Silva Aguirre, V & Stello, D 2014, 'Limits on Surface Gravities of Kepler Planet-candidate Host Stars from Non-detection of Solar-like Oscillations', Astrophysical Journal, bind 783, nr. 2, 123. https://doi.org/10.1088/0004-637X/783/2/123

APA

Campante, T. L., Chaplin, W. J., Lund, M. N., Huber, D., Hekker, S., García, R. A., Corsaro, E., Handberg, R., Miglio, A., Arentoft, T., Basu, S., Bedding, T. R., Christensen-Dalsgaard, J., Davies, G. R., Elsworth, Y. P., Gilliland, R. L., Karoff, C., Kawaler, S. D., Kjeldsen, H., ... Stello, D. (2014). Limits on Surface Gravities of Kepler Planet-candidate Host Stars from Non-detection of Solar-like Oscillations. Astrophysical Journal, 783(2), [123]. https://doi.org/10.1088/0004-637X/783/2/123

CBE

Campante TL, Chaplin WJ, Lund MN, Huber D, Hekker S, García RA, Corsaro E, Handberg R, Miglio A, Arentoft T, Basu S, Bedding TR, Christensen-Dalsgaard J, Davies GR, Elsworth YP, Gilliland RL, Karoff C, Kawaler SD, Kjeldsen H, Lundkvist M, Metcalfe TS, Silva Aguirre V, Stello D. 2014. Limits on Surface Gravities of Kepler Planet-candidate Host Stars from Non-detection of Solar-like Oscillations. Astrophysical Journal. 783(2):Article 123. https://doi.org/10.1088/0004-637X/783/2/123

MLA

Vancouver

Campante TL, Chaplin WJ, Lund MN, Huber D, Hekker S, García RA o.a. Limits on Surface Gravities of Kepler Planet-candidate Host Stars from Non-detection of Solar-like Oscillations. Astrophysical Journal. 2014 mar 1;783(2). 123. https://doi.org/10.1088/0004-637X/783/2/123

Author

Campante, T. L. ; Chaplin, W. J. ; Lund, M. N. ; Huber, D. ; Hekker, S. ; García, R. A. ; Corsaro, E. ; Handberg, R. ; Miglio, A. ; Arentoft, T. ; Basu, S. ; Bedding, T. R. ; Christensen-Dalsgaard, J. ; Davies, G. R. ; Elsworth, Y. P. ; Gilliland, R. L. ; Karoff, C. ; Kawaler, S. D. ; Kjeldsen, H. ; Lundkvist, M. ; Metcalfe, T. S. ; Silva Aguirre, V. ; Stello, D. / Limits on Surface Gravities of Kepler Planet-candidate Host Stars from Non-detection of Solar-like Oscillations. I: Astrophysical Journal. 2014 ; Bind 783, Nr. 2.

Bibtex

@article{ef454d0dd3e149429185ad1af5230757,
title = "Limits on Surface Gravities of Kepler Planet-candidate Host Stars from Non-detection of Solar-like Oscillations",
abstract = "We present a novel method for estimating lower-limit surface gravities (log g) of Kepler targets whose data do not allow the detection of solar-like oscillations. The method is tested using an ensemble of solar-type stars observed in the context of the Kepler Asteroseismic Science Consortium. We then proceed to estimate lower-limit log g for a cohort of Kepler solar-type planet-candidate host stars with no detected oscillations. Limits on fundamental stellar properties, as provided by this work, are likely to be useful in the characterization of the corresponding candidate planetary systems. Furthermore, an important byproduct of the current work is the confirmation that amplitudes of solar-like oscillations are suppressed in stars with increased levels of surface magnetic activity.",
keywords = "methods: statistical, planetary systems, stars: late-type, stars: oscillations, techniques: photometric",
author = "Campante, {T. L.} and Chaplin, {W. J.} and Lund, {M. N.} and D. Huber and S. Hekker and Garc{\'i}a, {R. A.} and E. Corsaro and R. Handberg and A. Miglio and T. Arentoft and S. Basu and Bedding, {T. R.} and J. Christensen-Dalsgaard and Davies, {G. R.} and Elsworth, {Y. P.} and Gilliland, {R. L.} and C. Karoff and Kawaler, {S. D.} and H. Kjeldsen and M. Lundkvist and Metcalfe, {T. S.} and {Silva Aguirre}, V. and D. Stello",
year = "2014",
month = mar,
day = "1",
doi = "10.1088/0004-637X/783/2/123",
language = "English",
volume = "783",
journal = "Astrophysical Journal",
issn = "0004-637X",
publisher = "Institute of Physics Publishing, Inc",
number = "2",

}

RIS

TY - JOUR

T1 - Limits on Surface Gravities of Kepler Planet-candidate Host Stars from Non-detection of Solar-like Oscillations

AU - Campante, T. L.

AU - Chaplin, W. J.

AU - Lund, M. N.

AU - Huber, D.

AU - Hekker, S.

AU - García, R. A.

AU - Corsaro, E.

AU - Handberg, R.

AU - Miglio, A.

AU - Arentoft, T.

AU - Basu, S.

AU - Bedding, T. R.

AU - Christensen-Dalsgaard, J.

AU - Davies, G. R.

AU - Elsworth, Y. P.

AU - Gilliland, R. L.

AU - Karoff, C.

AU - Kawaler, S. D.

AU - Kjeldsen, H.

AU - Lundkvist, M.

AU - Metcalfe, T. S.

AU - Silva Aguirre, V.

AU - Stello, D.

PY - 2014/3/1

Y1 - 2014/3/1

N2 - We present a novel method for estimating lower-limit surface gravities (log g) of Kepler targets whose data do not allow the detection of solar-like oscillations. The method is tested using an ensemble of solar-type stars observed in the context of the Kepler Asteroseismic Science Consortium. We then proceed to estimate lower-limit log g for a cohort of Kepler solar-type planet-candidate host stars with no detected oscillations. Limits on fundamental stellar properties, as provided by this work, are likely to be useful in the characterization of the corresponding candidate planetary systems. Furthermore, an important byproduct of the current work is the confirmation that amplitudes of solar-like oscillations are suppressed in stars with increased levels of surface magnetic activity.

AB - We present a novel method for estimating lower-limit surface gravities (log g) of Kepler targets whose data do not allow the detection of solar-like oscillations. The method is tested using an ensemble of solar-type stars observed in the context of the Kepler Asteroseismic Science Consortium. We then proceed to estimate lower-limit log g for a cohort of Kepler solar-type planet-candidate host stars with no detected oscillations. Limits on fundamental stellar properties, as provided by this work, are likely to be useful in the characterization of the corresponding candidate planetary systems. Furthermore, an important byproduct of the current work is the confirmation that amplitudes of solar-like oscillations are suppressed in stars with increased levels of surface magnetic activity.

KW - methods: statistical

KW - planetary systems

KW - stars: late-type

KW - stars: oscillations

KW - techniques: photometric

U2 - 10.1088/0004-637X/783/2/123

DO - 10.1088/0004-637X/783/2/123

M3 - Journal article

VL - 783

JO - Astrophysical Journal

JF - Astrophysical Journal

SN - 0004-637X

IS - 2

M1 - 123

ER -