The DOI matches its Crossref record; 8 of the 8 references it cites were found in a registry or an index.
FUNDAMENTAL PROPERTIES OF KEPLER PLANET-CANDIDATE HOST STARS USING ASTEROSEISMOLOGY
Open accessAbstract
We have used asteroseismology to determine fundamental properties for 66 Kepler planet-candidate host stars, with typical uncertainties of 3% and 7% in radius and mass, respectively. The results include new asteroseismic solutions for four host stars with confirmed planets (Kepler-4, Kepler-14, Kepler-23 and Kepler-25) and increase the total number of Kepler host stars with asteroseismic solutions to 77. A comparison with stellar properties in the planet-candidate catalog by Batalha et al. shows that radii for subgiants and giants obtained from spectroscopic follow-up are systematically too low by up to a factor of 1.5, while the properties for unevolved stars are in good agreement. We furthermore apply asteroseismology to confirm that a large majority of cool main-sequence hosts are indeed dwarfs and not misclassified giants. Using the revised stellar properties, we recalculate the radii for 107 planet candidates in our sample, and comment on candidates for which the radii change from a previously giant-planet/brown-dwarf/stellar regime to a sub-Jupiter size or vice versa. A comparison of stellar densities from asteroseismology with densities derived from transit models in Batalha et al. assuming circular orbits shows significant disagreement for more than half of the sample due to systematics in the modeled impact parameters or due to planet candidates that may be in eccentric orbits. Finally, we investigate tentative correlations between host-star masses and planet-candidate radii, orbital periods, and multiplicity, but caution that these results may be influenced by the small sample size and detection biases.
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Cites
Kepler planet-detection mission: Introduction and first results
Borucki, W. J., Koch, D., Basri, G., Batalha, N., Brown, T., Caldwell, D., Caldwell, J., Christensen-Dalsgaard, J., Cochran, W. D., DeVore, E., et al. (2010) · Science · doi:10.1126/science.1185402 · Cited by 4,035
Self-citationBorucki, W. J., Koch, D. G., Basri, G., Batalha, N., Brown, T. M., Bryson, S. T., Caldwell, D., Christensen-Dalsgaard, J., Cochran, W. D., DeVore, E., et al. (2011) · The Astrophysical Journal · doi:10.1088/0004-637x/736/1/19 · Cited by 1,042
Self-citationGiant Planet Occurrence in the Stellar Mass-Metallicity Plane
Johnson, J. A., Aller, K. M., Howard, A. W., & Crepp, J. R. (2010) · Publications of the Astronomical Society of the Pacific · doi:10.1086/655775 · Cited by 782
Self-citationMiglio, A., Brogaard, K., Stello, D., Chaplin, W. J., D’Antona, F., Montalbán, J., Basu, S., Bressan, A., Grundahl, F., Pinsonneault, M., et al. (2012) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2011.19859.x · Cited by 342
Self-citationKepler constraints on planets near hot Jupiters
Steffen, J. H., Ragozzine, D., Fabrycky, D. C., Carter, J. A., Ford, E. B., Holman, M. J., Rowe, J. F., Welsh, W. F., Borucki, W. J., Boss, A. P., et al. (2012) · Proceedings of the National Academy of Sciences · doi:10.1073/pnas.1120970109 · Cited by 255
Self-citationKepler-22b: A 2.4 EARTH-RADIUS PLANET IN THE HABITABLE ZONE OF A SUN-LIKE STAR
Borucki, W. J., Koch, D. G., Batalha, N., Bryson, S. T., Rowe, J., Fressin, F., Torres, G., Caldwell, D. A., Christensen-Dalsgaard, J., Cochran, W. D., et al. (2012) · The Astrophysical Journal · doi:10.1088/0004-637x/745/2/120 · Cited by 241
Self-citationA FIRST COMPARISON OF KEPLER PLANET CANDIDATES IN SINGLE AND MULTIPLE SYSTEMS
Latham, D. W., Rowe, J. F., Quinn, S. N., Batalha, N. M., Borucki, W. J., Brown, T. M., Bryson, S. T., Buchhave, L. A., Caldwell, D. A., Carter, J. A., et al. (2011) · The Astrophysical Journal · doi:10.1088/2041-8205/732/2/l24 · Cited by 188
Self-citationON THE RELATIVE SIZES OF PLANETS WITHIN KEPLER MULTIPLE-CANDIDATE SYSTEMS
Ciardi, D. R., Fabrycky, D. C., Ford, E. B., Gautier, T. N., Howell, S. B., Lissauer, J. J., Ragozzine, D., & Rowe, J. F. (2013) · The Astrophysical Journal · doi:10.1088/0004-637x/763/1/41 · Cited by 130
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Cited by
Accurate Empirical Radii and Masses of Planets and Their Host Stars with Gaia Parallaxes
Stassun, K. G., Collins, K. A., & Gaudi, B. S. (2017) · The Astronomical Journal · doi:10.3847/1538-3881/aa5df3 · Cited by 459
A chemical survey of exoplanets with ARIEL
Tinetti, G., Drossart, P., Eccleston, P., Hartogh, P., Heske, A., Leconte, J., Micela, G., Ollivier, M., Pilbratt, G., Puig, L., et al. (2018) · Experimental Astronomy · doi:10.1007/s10686-018-9598-x · Cited by 445
Stellar Spin-Orbit Misalignment in a Multiplanet System
Huber, D., Carter, J. A., Barbieri, M., Miglio, A., Deck, K. M., Fabrycky, D. C., Montet, B. T., Buchhave, L. A., Chaplin, W. J., Hekker, S., et al. (2013) · Science · doi:10.1126/science.1242066 · Cited by 315
Self-citationHot super-Earths stripped by their host stars
Lundkvist, M. S., Kjeldsen, H., Albrecht, S., Davies, G. R., Basu, S., Huber, D., Justesen, A. B., Karoff, C., Silva Aguirre, V., Van Eylen, V., et al. (2016) · Nature Communications · doi:10.1038/ncomms11201 · Cited by 258
Self-citationPLANETARY CANDIDATES OBSERVED BY KEPLER . VI. PLANET SAMPLE FROM Q1–Q16 (47 MONTHS)
Mullally, F., Coughlin, J. L., Thompson, S. E., Rowe, J., Burke, C., Latham, D. W., Batalha, N. M., Bryson, S. T., Christiansen, J., Henze, C. E., et al. (2015) · The Astrophysical Journal Supplement Series · doi:10.1088/0067-0049/217/2/31 · Cited by 254
Self-citation
Metadata
- Authors
- Huber, D., Chaplin, W. J., Christensen-Dalsgaard, J., Gilliland, R. L., Kjeldsen, H., Buchhave, L. A., Fischer, D. A., Lissauer, J. J., Rowe, J. F., Sanchis-Ojeda, R., Basu, S., Handberg, R., Hekker, S., Howard, A. W., Isaacson, H., Karoff, C., Latham, D. W., Lund, M. N., Lundkvist, M., Marcy, G. W., Miglio, A., Silva Aguirre, V., Stello, D., Arentoft, T., Barclay, T., Bedding, T. R., Burke, C. J., Christiansen, J. L., Elsworth, Y. P., Haas, M. R., Kawaler, S. D., Metcalfe, T. S., Mullally, F., & Thompson, S. E.
- Venue
- The Astrophysical Journal
- Publisher
- American Astronomical Society
- Published
- 2013-04-04
- Volume
- 767
- Issue
- 2
- Pages
- 127
- ISSN
- 0004-637X (ISSN-L)
- 1538-4357
- OpenAlex
- W2027724151
- Cited by
- 330
- References
- 8
- FWCI
- 24.80
- Type
- journal article
- Language
- en
- Open access
- bronze
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- CoChat. (2026). Citation check: FUNDAMENTAL PROPERTIES OF KEPLER PLANET-CANDIDATE HOST STARS USING ASTEROSEISMOLOGY. https://app.cochat.ai/papers/10.1088/0004-637x/767/2/127
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- Huber, D., Chaplin, W. J., Christensen-Dalsgaard, J., Gilliland, R. L., Kjeldsen, H., Buchhave, L. A., Fischer, D. A., Lissauer, J. J., Rowe, J. F., Sanchis-Ojeda, R., Basu, S., Handberg, R., Hekker, S., Howard, A. W., Isaacson, H., Karoff, C., Latham, D. W., Lund, M. N., Lundkvist, M., . . . Thompson, S. E. (2013). FUNDAMENTAL PROPERTIES OF KEPLER PLANET-CANDIDATE HOST STARS USING ASTEROSEISMOLOGY. The Astrophysical Journal. https://doi.org/10.1088/0004-637x/767/2/127
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