No CrossRef data available.
Article contents
Analysis of the light and radial velocity curves of transiting extra-solar planets
Published online by Cambridge University Press: 01 May 2008
Abstract
Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.
Several approaches have been followed for the analysis of the light curves of transiting extra-solar planets. From simple approximate algorithms and synthetic models to semi-analytical complete solutions. The different alternatives are discussed with their strengths and weaknesses. Analytical expressions can also provide a deeper insight into the main system parameters from the measurement of a few strategic points describing the shape of the light curve.
- Type
- Contributed Papers
- Information
- Proceedings of the International Astronomical Union , Volume 4 , Symposium S253: Transiting Planets , May 2008 , pp. 394 - 397
- Copyright
- Copyright © International Astronomical Union 2009
References
Etzel, P. B. 1993. In “Light curve modeling of eclipsing binary stars” (Ed. Milone, E. F.), p. 113, Springer Verlag, New York.CrossRefGoogle Scholar
Giménez, A. & Diaz-Cordovés, J. 1993. In “Light curve modeling of eclipsing binary stars” (Ed. Milone, E.F.), p. 125, Springer Verlag, New York.CrossRefGoogle Scholar