Measuring accurate transit parameters
- 1 May 2008
- journal article
- research article
- Published by Cambridge University Press (CUP) in Proceedings of the International Astronomical Union
- Vol. 4 (S253) , 99-109
- https://doi.org/10.1017/s174392130802629x
Abstract
By observing the transits of exoplanets, one may determine many fundamental system parameters. I review current techniques and results for the parameters that can be measured with the greatest precision, specifically, the transit times, the planetary mass and radius, and the projected spin-orbit angle.Keywords
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This publication has 61 references indexed in Scilit:
- THE TRANSIT LIGHT CURVE PROJECT. VIII. SIX OCCULTATIONS OF THE EXOPLANET TrES-3The Astronomical Journal, 2008
- Hydrodynamic Simulations of Unevenly Irradiated Jovian PlanetsThe Astrophysical Journal, 2008
- A Determination of the Spin‐Orbit Alignment of the Anomalously Dense Planet Orbiting HD 149026The Astrophysical Journal, 2007
- The Transit Light Curve Project. VII. The Not-So-Bloated Exoplanet HAT-P-1bThe Astronomical Journal, 2007
- Spin-Orbit Alignment for the Eccentric Exoplanet HD 147506bThe Astrophysical Journal, 2007
- A method for the direct determination of the surface gravities of transiting extrasolar planetsMonthly Notices of the Royal Astronomical Society: Letters, 2007
- The Transit Light Curve Project. III. Tres Transits of TrES‐1The Astrophysical Journal, 2007
- Measurement of the Spin-Orbit Alignment in the Exoplanetary System HD 189733The Astrophysical Journal, 2006
- Method for Spot Detection on Solar-like StarsThe Astrophysical Journal, 2003
- On the detection of an effect of rotation during eclipse in the velocity of the brigher component of beta Lyrae, and on the constancy of velocity of this system.The Astrophysical Journal, 1924