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Transit Detection of Radial Velocity Planets

Published online by Cambridge University Press:  01 May 2008

Stephen R. Kane
Affiliation:
Michelson Science Center, Caltech, MS 100-22, 770 South Wilson Avenue Pasadena, CA 91125, USA email: skane@ipac.caltech.edu
Kaspar von Braun
Affiliation:
Michelson Science Center, Caltech, MS 100-22, 770 South Wilson Avenue Pasadena, CA 91125, USA email: skane@ipac.caltech.edu
Corresponding
E-mail address:
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Abstract

The orbital parameters of extra-solar planets have a significant impact on the probability that the planet will transit the host star. This was recently demonstrated by the transit detection of HD 17156b whose favourable eccentricity and argument of periastron dramatically increased its transit likelihood. We present a study which provides a quantitative analysis of how these two orbital parameters affect the geometric transit probability as a function of period. Further, we apply these results to known radial velocity planets and show that there are unexpectedly high transit probabilities for planets at relatively long periods. For a photometric monitoring campaign which aims to determine if the planet indeed transits, we calculate the significance of a null result and the subsequent constraints that may be applied to orbital parameters.

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2009

References

Barbieri, M., et al. , 2007, A&A, 476, L13Google Scholar
Barnes, J. W., et al. , 2007, PASP, 119, 986CrossRefGoogle Scholar
Burke, C. J., 2008, ApJ, 679, 1566CrossRefGoogle Scholar
Butler, R. P., et al. , 2006, ApJ, 646, 505CrossRefGoogle Scholar
Ford, E. B., Rasio, F. A., 2008, ApJ, in press (astro-ph/0703163)Google Scholar
Kane, S. R., 2007, MNRAS, 380, 1488CrossRefGoogle Scholar
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