Published February 16, 2011
| Published
Journal Article
Open
Improving Transit Predictions of Known Exoplanets with TERMS
Abstract
Transiting planet discoveries have largely been restricted to the short-period or low-periastron distance regimes due to the bias inherent in the geometric transit probability. Through the refinement of planetary orbital parameters, and hence reducing the size of transit windows, long-period planets become feasible targets for photometric follow-up. Here we describe the TERMS project that is monitoring these host stars at predicted transit times.
Additional Information
© 2011 Owned by the authors, published by EDP Sciences. This is an Open Access article distributed under the terms of the Creative Commons Attribution-Noncommercial License 3.0, which permits unrestricted use, distribution, and reproduction in any noncommercial medium, provided the original work is properly cited. Published online: 16 February 2011.Attached Files
Published - Kane2011p13995Detection_And_Dynamics_Of_Transiting_Exoplanets.pdf
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Kane2011p13995Detection_And_Dynamics_Of_Transiting_Exoplanets.pdf
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Additional details
- Eprint ID
- 23834
- Resolver ID
- CaltechAUTHORS:20110531-100634902
- Created
-
2011-05-31Created from EPrint's datestamp field
- Updated
-
2021-11-09Created from EPrint's last_modified field
- Caltech groups
- Infrared Processing and Analysis Center (IPAC)