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Cadence optimisation and exoplanetary parameter sensitivity

Published online by Cambridge University Press:  01 October 2007

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.

Type
Contributed Papers
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