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Probing the Outskirts of an Extrasolar Planet with HST Time-Series Photometry

Published online by Cambridge University Press:  26 May 2016

David Charbonneau ,
Timothy M. Brown ,
Ronald L. Gilliland ,
Robert W. Noyes  and
Adam Burrows
David Charbonneau
Affiliation:
Harvard-Smithsonian Center for Astrophysics, 60 Garden St., Cambridge, MA 02138, USA High Altitude Observatory, National Center for Atmospheric Research, 3450 Mitchell Lane, Boulder, CO 80301, USA
Timothy M. Brown
Affiliation:
High Altitude Observatory, National Center for Atmospheric Research, 3450 Mitchell Lane, Boulder, CO 80301, USA
Ronald L. Gilliland
Affiliation:
Space Telescope Science Institute, 3700 San Martin Dr., Baltimore, MD 21218, USA
Robert W. Noyes
Affiliation:
Harvard-Smithsonian Center for Astrophysics, 60 Garden St., Cambridge, MA 02138, USA
Adam Burrows
Affiliation:
Department of Astronomy, University of Arizona, 933 North Cherry Ave., Tucson, AZ 85121, USA

Abstract

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We observed 4 planetary transits of HD 209458 with the STIS spectrograph on HST, and generated a photometric time series with extremely rapid cadence and high precision. We use these data to better constrain the orbital, stellar, and planetary parameters, and to search for circumplanetary rings and planetary satellites.

Type
Part I: Discovery and study of extrasolar planets - current
Information
Symposium - International Astronomical Union , Volume 202: Planetary Systems in the Universe – Observation, Formation and Evolution , 2004 , pp. 72 - 74
Copyright
Copyright © Astronomical Society of the Pacific 2004 

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