International audienceWe observed the hot Jupiter HAT-P-32b (also known as HAT-P-32Ab) to determine its optical transmission spectrum by measuring the wavelength-dependent, planet-to-star radius ratios in the region between 518-918 nm. We used the OSIRIS instrument at the Gran Telescopio CANARIAS (GTC) in long-slit spectroscopy mode, placing HAT-P-32 and a reference star in the same slit and obtaining a time series of spectra covering two transit events. Using the best quality data set, we were able to yield 20 narrowband transit light curves, with each passband spanning a 20 nm wide interval. After removal of all systematic noise signals and light curve modeling, the uncertainties for the resulting radius ratios lie between 337 and 972 ppm...
Aims. We set out to study the atmosphere of WASP-80b, a warm inflated gas giant with an equilibrium ...
Aims. We set out to study the atmosphere of WASP-80b, a warm inflated gas giant with an equilibrium ...
We present a 0.3-5 μm transmission spectrum of the hot Jupiter HAT-P-32Ab observed with the Space Te...
International audienceWe observed the hot Jupiter HAT-P-32b (also known as HAT-P-32Ab) to determine ...
International audienceWe observed the hot Jupiter HAT-P-32b (also known as HAT-P-32Ab) to determine ...
International audienceWe observed the hot Jupiter HAT-P-32b (also known as HAT-P-32Ab) to determine ...
Context. Time-series spectrophotometric studies of exoplanets during transit using ground-based faci...
Context. Time-series spectrophotometric studies of exoplanets during transit using ground-based faci...
Context. Time-series spectrophotometric studies of exoplanets during transit using ground-based faci...
Context. Time-series spectrophotometric studies of exoplanets during transit using ground-based faci...
Context. Transiting planets offer an excellent opportunity for characterizing the atmospheres of ext...
Context. Transiting highly inflated giant planets offer the possibility of characterizing their atmo...
Context. Transiting highly inflated giant planets offer the possibility of characterizing their atmo...
Context. Transiting highly inflated giant planets offer the possibility of characterizing their atmo...
Context. Rayleigh scattering in a hydrogen-dominated exoplanet atmosphere can be detected using grou...
Aims. We set out to study the atmosphere of WASP-80b, a warm inflated gas giant with an equilibrium ...
Aims. We set out to study the atmosphere of WASP-80b, a warm inflated gas giant with an equilibrium ...
We present a 0.3-5 μm transmission spectrum of the hot Jupiter HAT-P-32Ab observed with the Space Te...
International audienceWe observed the hot Jupiter HAT-P-32b (also known as HAT-P-32Ab) to determine ...
International audienceWe observed the hot Jupiter HAT-P-32b (also known as HAT-P-32Ab) to determine ...
International audienceWe observed the hot Jupiter HAT-P-32b (also known as HAT-P-32Ab) to determine ...
Context. Time-series spectrophotometric studies of exoplanets during transit using ground-based faci...
Context. Time-series spectrophotometric studies of exoplanets during transit using ground-based faci...
Context. Time-series spectrophotometric studies of exoplanets during transit using ground-based faci...
Context. Time-series spectrophotometric studies of exoplanets during transit using ground-based faci...
Context. Transiting planets offer an excellent opportunity for characterizing the atmospheres of ext...
Context. Transiting highly inflated giant planets offer the possibility of characterizing their atmo...
Context. Transiting highly inflated giant planets offer the possibility of characterizing their atmo...
Context. Transiting highly inflated giant planets offer the possibility of characterizing their atmo...
Context. Rayleigh scattering in a hydrogen-dominated exoplanet atmosphere can be detected using grou...
Aims. We set out to study the atmosphere of WASP-80b, a warm inflated gas giant with an equilibrium ...
Aims. We set out to study the atmosphere of WASP-80b, a warm inflated gas giant with an equilibrium ...
We present a 0.3-5 μm transmission spectrum of the hot Jupiter HAT-P-32Ab observed with the Space Te...