Exoplanet CoRoT-1 b is intriguing because we predict it to be a transitional planet between hot Jupiters (equilibrium temperatures ∼1500 K) and ultrahot Jupiters (equilibrium temperatures >2000 K). In 2012, observations of CoRoT-1 b included one primary transit and three secondary eclipses with the Hubble Space Telescope (HST) Wide Field Camera 3 (WFC3) combined with the G141 grism (1.1-1.7 μm) in stare mode. We aimed to further investigate CoRoT-1 b through its secondary eclipses, producing spectrophotometric light curves corrected for charge trapping, also known as the ramp effect in time-series observations with the WFC3. We found that, when correcting for the ramp effect and using the typically discarded first orbit, we are better capab...
International audienceContext. Transit detection from space using ultra-precise photometry led to th...
Context. Gas giants orbiting close to hot and massive early-type stars can reach dayside temperature...
International audienceContext. Gas giants orbiting close to hot and massive early-type stars can rea...
We have used Hubble/WFC3 and the G141 grism to measure the secondary eclipse of the transiting, very...
We probe the structure and composition of the atmospheres of five hot Jupiter exoplanets using the H...
We have used Hubble/WFC3 and the G141 grism to measure the secondary eclipse of the transiting, very...
We have used Hubble/WFC3 and the G141 grism to measure the secondary eclipse of the transiting, very...
International audienceWe report the detection in Ks-band of the secondary eclipse of the hot Jupiter...
We have used Hubble/WFC3 and the G141 grism to measure the secondary eclipse of the transiting, very...
We present our analysis of the red-channel CoRoT data of extrasolar planet CoRoT-2b. A deep secondar...
We present new photometric data of 11 hot Jupiter transiting exoplanets (CoRoT-12b, HATP-5b, HAT-P-1...
Spectroscopy of transiting exoplanets has revealed a wealth of information about their atmospheric c...
We measure secondary eclipses of the hot giant exoplanets CoRoT-1 at 3.6 and 4.5 μm, and CoRoT-2 at ...
By observing the occultation (secondary eclipse) of a transiting exoplanet by its host star inthe (n...
International audienceContext. Transit detection from space using ultra-precise photometry led to th...
International audienceContext. Transit detection from space using ultra-precise photometry led to th...
Context. Gas giants orbiting close to hot and massive early-type stars can reach dayside temperature...
International audienceContext. Gas giants orbiting close to hot and massive early-type stars can rea...
We have used Hubble/WFC3 and the G141 grism to measure the secondary eclipse of the transiting, very...
We probe the structure and composition of the atmospheres of five hot Jupiter exoplanets using the H...
We have used Hubble/WFC3 and the G141 grism to measure the secondary eclipse of the transiting, very...
We have used Hubble/WFC3 and the G141 grism to measure the secondary eclipse of the transiting, very...
International audienceWe report the detection in Ks-band of the secondary eclipse of the hot Jupiter...
We have used Hubble/WFC3 and the G141 grism to measure the secondary eclipse of the transiting, very...
We present our analysis of the red-channel CoRoT data of extrasolar planet CoRoT-2b. A deep secondar...
We present new photometric data of 11 hot Jupiter transiting exoplanets (CoRoT-12b, HATP-5b, HAT-P-1...
Spectroscopy of transiting exoplanets has revealed a wealth of information about their atmospheric c...
We measure secondary eclipses of the hot giant exoplanets CoRoT-1 at 3.6 and 4.5 μm, and CoRoT-2 at ...
By observing the occultation (secondary eclipse) of a transiting exoplanet by its host star inthe (n...
International audienceContext. Transit detection from space using ultra-precise photometry led to th...
International audienceContext. Transit detection from space using ultra-precise photometry led to th...
Context. Gas giants orbiting close to hot and massive early-type stars can reach dayside temperature...
International audienceContext. Gas giants orbiting close to hot and massive early-type stars can rea...