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Transit Search for Exoplanets with the Vulcan Camera

Published online by Cambridge University Press:  26 May 2016

Douglas A. Caldwell
Affiliation:
NASA Ames Research Center, MS 245-3, Moffett Field, CA 94035-1000, USA
W. J. Borucki
Affiliation:
NASA Ames Research Center, MS 245-3, Moffett Field, CA 94035-1000, USA
J. M. Jenkins
Affiliation:
NASA Ames Research Center, MS 245-3, Moffett Field, CA 94035-1000, USA
D. G. Koch
Affiliation:
NASA Ames Research Center, MS 245-3, Moffett Field, CA 94035-1000, USA
L. Webster
Affiliation:
NASA Ames Research Center, MS 245-3, Moffett Field, CA 94035-1000, USA
R. L. Showen
Affiliation:
NASA Ames Research Center, MS 245-3, Moffett Field, CA 94035-1000, USA

Abstract

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The NASA Ames Research Center's Vulcan photometer is being used in a search for close–in giant extrasolar planets. With our current data reduction system we achieve 0.2–0.8% hour–to–hour relative photometric precision on ∽ 6000 stars brighter than 13th magnitude. Three Galactic-plane fields have so far yielded hundreds of variable stars, including ∽ 50 eclipsing or interacting binaries per field. Several candidate detections have been followed up with radial velocity observations. High-resolution spectroscopy revealed many of the strongest candidates to be grazing eclipsing binaries.

Type
Part I: Discovery and study of extrasolar planets - current
Copyright
Copyright © Astronomical Society of the Pacific 2004 

References

Caldwell, D. A., Borucki, W. J., Lissauer, J. J. 2000, Bioastronomy 99: A New Era in the Search for Life in the Universe, ed. Lemarchand, G. & Meech, K., ASP Conference Series, in press.Google Scholar
Jenkins, J.M., Doyle, L. R., & Cullers, D. K. 1996, Icarus, 119, 244.Google Scholar
Posson–Brown, J., Latham, D., Borucki, W. J. 2000, in preparation.Google Scholar