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.
| Original language | English (US) |
|---|---|
| Pages (from-to) | 99-109 |
| Number of pages | 11 |
| Journal | Proceedings of the International Astronomical Union |
| Volume | 4 |
| Issue number | S253 |
| DOIs | |
| State | Published - May 2008 |
| Externally published | Yes |
All Science Journal Classification (ASJC) codes
- Astronomy and Astrophysics
- Space and Planetary Science