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THE FREQUENCY OF HOT JUPITERS ORBITING NEARBY SOLAR-TYPE STARS
Open accessAbstract
We determine the fraction of F, G, and K dwarfs in the solar neighborhood hosting hot Jupiters as measured by the California Planet Survey from the Lick and Keck planet searches. We find the rate to be 1.2% ± 0.38%, which is consistent with the rate reported by Mayor et al. from the HARPS and CORALIE radial velocity (RV) surveys. These numbers are more than double the rate reported by Howard et al. for Kepler stars and the rate of Gould et al. from the OGLE-III transit search; however, due to small number statistics these differences are of only marginal statistical significance. We explore some of the difficulties in estimating this rate from the existing RV data sets and comparing RV rates to rates from other techniques.
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“Discovery and characterization of thousands of hot Jupiters in exoplanetary systems via the transit method ( Wright et al. 2012 ) .”
From LSST: From Science Drivers to Reference Design and Anticipated Data Products (2019) · cites this paper as Wright et al. 2012
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Self-citation
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Cited by
Sorted by citations
LSST: From Science Drivers to Reference Design and Anticipated Data Products
Ivezić, Ž., Kahn, S. M., Tyson, J. A., Abel, B., Acosta, E., Allsman, R., Alonso, D., AlSayyad, Y., Anderson, S. F., Andrew, J., et al. (2019) · The Astrophysical Journal · doi:10.3847/1538-4357/ab042c · Cited by 4,357
“• Discovery and characterization of thousands of hot Jupiters in exoplanetary systems via the transit method (Wright et al. 2012).”
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“The discrepancy might be attributable to differences in metallicity or the frequency of multiple-star systems between the two samples (Gould et al. 2006, Bayliss & Sackett 2011, Wright et al. 2012).”
BackgroundThe NASA Exoplanet Archive: Data and Tools for Exoplanet Research
Akeson, R., Chen, X., Ciardi, D. R., Crane, M. K., Good, J., Harbut, M., Jackson, E. S., Kane, S. R., Laity, A. C., Leifer, S. D., et al. (2013) · Publications of the Astronomical Society of the Pacific · doi:10.1086/672273 · Cited by 906
“This includes high-resolution spectra from the N2K Consortium (Fischer et al. 2007), the M2K program (Fischer et al. 2012), and the California Planet search team (Wright et al. 2012).”
MethodDawson, R. I., & Johnson, J. A. (2018) · Annual Review of Astronomy and Astrophysics · doi:10.1146/annurev-astro-081817-051853 · Cited by 622
Self-citationImaging Extrasolar Giant Planets
Bowler, B. P. (2016) · Publications of the Astronomical Society of the Pacific · doi:10.1088/1538-3873/128/968/102001 · Cited by 450
“…stellar host mass, the overall giant planet occurrence rate for the full sample of 384 stars is 0.6+0.7 −0.5%, which happens to be comparable to the frequency of hot Jupiters around FGK stars in the field (1.2 ± 0.4%; Wright et al. 2012) and in the Kepler sample (0.5 ± 0.1%; Howard et al. 2012).”
BackgroundInfluential
Metadata
- Authors
- Wright, J. T., Marcy, G. W., Howard, A. W., Johnson, J. A., Morton, T. D., & Fischer, D. A.
- Affiliations
- Pennsylvania State University (US)
- University of California, Berkeley (US)
- California Institute of Technology (US)
- Yale University (US)
- Corresponding author
- Wright, J. T.
- Venue
- The Astrophysical Journal
- Publisher
- American Astronomical Society
- Published
- 2012-06-25
- Volume
- 753
- Issue
- 2
- Pages
- 160
- ISSN
- 0004-637X (ISSN-L)
- 1538-4357
- OpenAlex
- W2158240367
- Cited by
- 371
- References
- 40
- Citations by year
- 2026: 15 · 2025: 21 · 2024: 24 · 2023: 16 · 2022: 20 · 2021: 22 · 2020: 27 · 2019: 32 · 2018: 41 · 2017: 34 · 2016: 35 · 2015: 28 · 2014: 25 · 2013: 18 · 2012: 10
- FWCI
- 14.18
- Type
- journal article
- Language
- en
- Open access
- bronze
- doi.org
- Locations
- The Astrophysical Journal (publishedVersion)
- arXiv (Cornell University) (submittedVersion)
- CaltechAUTHORS (California Institute of Technology) (submittedVersion)
- arXiv (Cornell University)
- Topics
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Stellar, planetary, and galactic studies
- Physical Sciences › Physics and Astronomy › Instrumentation › Astronomy and Astrophysical Research
- Physical Sciences › Earth and Planetary Sciences › Space and Planetary Science › Astro and Planetary Science
- Keywords
- hot Jupiters, solar-type stars, planet occurrence rate, radial velocity surveys, transit surveys, Kepler, OGLE-III, Lick Observatory, Keck Observatory, nearby stars
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