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Cambridge University Press (CUP), Proceedings of the International Astronomical Union, S253(4), p. 121-127, 2008

DOI: 10.1017/s1743921308026318

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Towards the Albedo of an Exoplanet: MOST Satellite Observations of Bright Transiting Exoplanetary Systems

Journal article published in 2008 by Jason F. Rowe ORCID, Jaymie M. Matthews, Sara Seager, Dimitar Sasselov, Rainer Kuschnig, David B. Guenther, Anthony F. J. Moffat, Slavek M. Rucinski, Gordon A. H. Walker, Werner W. Weiss
This paper was not found in any repository, but could be made available legally by the author.
This paper was not found in any repository, but could be made available legally by the author.

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Abstract

AbstractThe Canadian MOST satellite is a unique platform for observations of bright transiting exoplanetary systems. Providing nearly continuous photometric observations for up to 4 weeks, MOST can produce important observational data to help us learn about the properties of exosolar planets. We review our current observations of HD 209458 and HD 189733 with implications for the albedo and our progress towards detecting reflected light from an exoplanet.

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