The properties of XO-5b and WASP-82b redetermined using new high-precision transit photometry and global data analyses
This paper presents new transit photometry of two transiting exoplanetary systems, XO-5 and WASP-82. In each case the new transit light curve is more precise than any other of that system previously published. The new data are analysed alongside previously-published photometry and radial velocities, resulting in an improved orbital ephemeris and a refined set of system parameters in each case.
Tuesday, December 23, 2014
Hot Jupiters XO-5b and WASP-82b Reconsidered
Posted by Will Baird at 8:00 AM
Labels: exoplanet characteristics, hot jupiters, WASP-82b, XO-5b
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