THESIS is a concept for a medium class mission designed for spectroscopic characterization of extrasolar planets between 2-14 microns. The concept leverage...
Charbonneau, D.: Detection of atmospheric haze on an extrasolar planet: the 0.55-1.05 μm transmission spectrum of HD 189733b with the HubbleSpaceTelescope...
Hubble Space Telescope (HST) observations of the nearby (3.22 pc) K2 V star ɛ Eridani have been combined with ground-based astrometric and radial veloci...
We report the first astrometrically determined mass of an extrasolar planet, a companion previously detected by Doppler spectroscopy. Radial velocities fir...
al (2008) Detection of atmospheric haze on an extrasolar planet: the 0.55-1.05 μm transmission spectrum of HD 189733 b with the Hubble Space Telescope...
Detecting extrasolar planets in reflected stellar radiation is an exceedingly challenging task due to the great faintness of planets as compared with stars...
We present recent observations from the Hubble Space Telescope-Cosmic Origins Spectrograph aimed at characterizing the auroral emission from the extrasolar...
We present observations of two occultations of the extrasolar planet WASP-33b using the Wide Field Camera 3 (WFC3) on the Hubble Space Telescope, which all...
The Hubble Space Telescope (HST) detection of an extrasolar planet atmosphere in 2001 was a landmark step forward for the characterization of extrasolar pl...