On The Frequency Of Hot Jupiters Orbiting F, G, K Dwarfs In The Solar Neighborhood

Details On The Frequency Of Hot Jupiters Orbiting F, G, K Dwarfs In The Solar Neighborhood On The Frequency Of Hot Jupiters Orbiting F, G, K Dwarfs In The Solar Neighborhood

Jan 2012

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2012aas...21924516w&link_type=abstract

American Astronomical Society, AAS Meeting #219, #245.16

Astronomy and Astrophysics

Astronomy

Scientific paper

We estimate the fraction of F, G, K stars in the solar neighborhood hosting hot jupiters as measured by the California Planet Survey from the Lick and Keck planet searches. We compare this with the rate of reported by Howard et al. (2011) for Kepler stars, and with the rate reported from microlensing (Gould et al. 2006) and the HARPS and CORAIE surveys (Mayor et al. 2011). We explore some of the difficulties in estimating this rate from the existing radial velocity data sets and explore why previous works found significantly higher rates, in significant disagreement with Kepler.

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