Published April 19, 2010
| public
Journal Article
Detectability of Earth-like Planets in Multi-Planet Systems: Preliminary Report
- Creators
- Traub, W. A.
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Beichman, C.
- Boden, A. F.
- Boss, A. P.
- Casertano, S.
- Catanzarite, J.
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Fischer, D.
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Ford, E. B.
- Gould, A.
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Halverson, S.
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Howard, A.
- Ida, S.
- Kasdin, N. J.
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Laughlin, G. P.
- Levison, H. F.
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Lin, D.
- Makarov, V. V.
- Marr, J.
- Muterspaugh, M.
- Raymond, S. N.
- Savransky, D.
- Shao, M.
- Sozzetti, A.
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Zhai, C.
Abstract
We ask if Earth-like planets (terrestrial mass and habitable-zone orbit) can be detected in multi-planet systems, using astrometric and radial velocity observations. We report here the preliminary results of double-blind calculations designed to answer this question.
Additional Information
© 2010 EAS, EDP Sciences. Published online 19 April 2010.Additional details
- Eprint ID
- 78767
- Resolver ID
- CaltechAUTHORS:20170705-124700317
- Created
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2017-07-05Created from EPrint's datestamp field
- Updated
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2021-11-15Created from EPrint's last_modified field
- Caltech groups
- Infrared Processing and Analysis Center (IPAC)