The secondary eclipse of the transiting exoplanet CoRoT-2b
Astronomy and Astrophysics 501:3 (2009)
Abstract:
We present a study of the light curve of the transiting exoplanet CoRoT-2b, aimed at detecting the secondary eclipse and measuring its depth. The data were obtained with the CoRoT satellite during its first run of more than 140 days. After filtering the low frequencies with a pre-whitening technique, we detect a 0.0060±0.0020% secondary eclipse centered on the orbital phase 0.494±0.006. Assuming a black-body emission of the planet, we estimate a surface brightness temperature of Tp,CoRoT = 1910+90-100 K. We provide the planet's equilibrium temperature and re-distribution factors as a function of the unknown amount of reflected light. The upper limit for the geometric albedo is 0.12. The detected secondary is the shallowest ever found. © 2009 ESO.Sensitivity of stable water isotopic values to convective parameterization schemes
Geophysical Research Letters American Geophysical Union (AGU) 36:23 (2009)
Global warming, convective threshold and false thermostats
Geophysical Research Letters American Geophysical Union (AGU) 36:21 (2009)
Pixel multiplexing for high-speed multi-resolution fluorescence imaging
ArXiv 0910.0789 (2009)