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How to use the Phoebe code to solve transiting exoplanet light curve

Published online by Cambridge University Press:  01 May 2008

Stanislav Poddaný
Stanislav Poddaný*
Affiliation:
Astronomical Institute, Charles University, Faculty of Mathematics and Physics, V Holešovičkách 2, Prague, Czech Republic Štefánik observatory, Observatory and Planetárium of Prague, Petřín 205, Prague, Czech Republic email: [email protected]
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Abstract

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A brief demonstration of photometric light curves solutions for eight transiting exoplanets using the Phoebe 0.29c code is presented. We determined radii and inclinations for TrES-1b, TrES-2b, Wasp-1b, XO-1b, XO-2b, OGLE-TR-10b, OGLE-TR-111b and HD 189733b. All our results are in good agreement with the last results published.

Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 4 , Symposium S253: Transiting Planets , May 2008 , pp. 398 - 401
Copyright
Copyright © International Astronomical Union 2009

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