Resumen
A second step in the characterization of extrasolar planets has been achieved with the detection of the planetary thermal emission by observing the occultation-phase light curves of these objects. We use near-infrared high-cadence observations to detect the occultation and the primary transits of some southern extrasolar planets which produce a highly accurate characterization of these systems.
Idioma original | Inglés |
---|---|
Páginas (desde-hasta) | 291-292 |
Número de páginas | 2 |
Publicación | Revista Mexicana de Astronomia y Astrofisica: Serie de Conferencias |
Volumen | 40 |
Estado | Publicada - 2011 |
Áreas temáticas de ASJC Scopus
- Ciencias planetarias y espacial
- Astronomía y astrofísica