Abstract
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.
Original language | English (US) |
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Pages (from-to) | 115-118 |
Number of pages | 4 |
Journal | Proceedings of the International Astronomical Union |
Volume | 3 |
Issue number | S249 |
DOIs | |
State | Published - Oct 2007 |
All Science Journal Classification (ASJC) codes
- Medicine (miscellaneous)
- Astronomy and Astrophysics
- Nutrition and Dietetics
- Public Health, Environmental and Occupational Health
- Space and Planetary Science