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Cadence optimisation and exoplanetary parameter sensitivity

Published online by Cambridge University Press:  01 October 2007

Stephen R. Kane ,
Eric B. Ford  and
Jian Ge
Stephen R. Kane
Affiliation:
Department of Astronomy, University of Florida, 211 Bryant Space Science Center, Gainesville, FL 32611-2055, U.S.A.
Eric B. Ford
Affiliation:
Department of Astronomy, University of Florida, 211 Bryant Space Science Center, Gainesville, FL 32611-2055, U.S.A.
Jian Ge
Affiliation:
Department of Astronomy, University of Florida, 211 Bryant Space Science Center, Gainesville, FL 32611-2055, U.S.A.
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Abstract

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To achieve maximum planet yield for a given radial velocity survey, the observing strategy must be carefully considered. In particular, the adopted cadence can greatly affect the sensitivity to exoplanetary parameters such as period and eccentricity. Here we describe simulations which aim to maximise detections based upon the target parameter space of the survey.

Keywords

methods: data analysis – planetary systems – techniques: radial velocities
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 3 , Symposium S249: Exoplanets: Detection, Formation and Dynamics , October 2007 , pp. 115 - 118
Copyright
Copyright © International Astronomical Union 2008

References

Ge, J., et al. 2006, Proc. SPIE, 6269, 75Google Scholar
Kane, S. R., Schneider, D. P., & Ge, J. 2007, MNRAS, 377, 1610Google Scholar