The photometric follow-up observations for transiting exoplanet XO-2b

Details The photometric follow-up observations for transiting exoplanet XO-2b The photometric follow-up observations for transiting exoplanet XO-2b

Nov 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011iaus..276..426g&link_type=abstract

The Astrophysics of Planetary Systems: Formation, Structure, and Dynamical Evolution, Proceedings of the International Astronomi

Astronomy and Astrophysics

Astrophysics

Planetary Systems, Eclipses, Techniques: Photometric

Scientific paper

Four new transit light curves of XO-2b obtained in 2008 and 2009, are
analyzed by using MCMC algorithm, and the system parameters are derived.
The result demonstrates that the orbital period of the system obtained
from new observations is almost the same as Burke et al.'s one (2007),
which does not confirm the result of Fernandez et al. (2009).

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