Astronomy and Astrophysics – Astronomy
Scientific paper
Dec 2002
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002aas...201.2112p&link_type=abstract
American Astronomical Society, 201st AAS Meeting, #21.12; Bulletin of the American Astronomical Society, Vol. 34, p.1139
Astronomy and Astrophysics
Astronomy
Scientific paper
Transits of bright stars offer a unique opportunity to study detailed properties of extrasolar planets that cannot be determined through radial-velocity observations. We propose a new technique to find such systems using all-sky small-aperture transit surveys. We derive a general formula for the number of stars that can be probed for such systems as a function of the characteristics of the star, the planet, and the survey. We use this formula to derive the optimal telescope design for finding transits of bright stars: a 1'' to 2'' ''telescope'' with a 4k by 4k camera. This work was supported in part by grant AST 02-01266 from the NSF.
DePoy Darren L.
Gould Andrew
Pepper Joshua
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