The SARS algorithm: detrending CoRoT light curves with Sysrem using simultaneous external parameters
(2010)
Ground-based detection of thermal emission from the exoplanet WASP-19b
(2010)
The spin-orbit angle of the transiting hot Jupiter CoRoT-1b
Monthly Notices of the Royal Astronomical Society: Letters 402:1 (2010)
Abstract:
We measure the angle between the planetary orbit and the stellar rotation axis in the transiting planetary system CoRoT-1, with new HIRES/Keck and FORS/VLT high-accuracy photometry. The data indicate a highly tilted system, with a projected spin-orbit angle λ = 77° ± 11°. Systematic uncertainties in the radial velocity data could cause the actual errors to be larger by an unknown amount, and this result needs to be confirmed with further high-accuracy spectroscopic transit measurements. Spin-orbit alignment has now been measured in a dozen extra-solar planetary systems, and several show strong misalignment. The first three misaligned planets were all much more massive than Jupiter and followed eccentric orbits. CoRoT-1, however, is a jovian-mass close-in planet on a circular orbit. If its strong misalignment is confirmed, it would break this pattern. The high occurrence of misaligned systems for several types of planets and orbits favours planet-planet scattering as a mechanism to bring gas giants on very close orbits. © 2009 The Authors. Journal compilation © 2009 RAS.Transiting exoplanets from the CoRoT space mission IX. CoRoT-6b: a transiting `hot Jupiter' planet in an 8.9d orbit around a low-metallicity star
(2010)
Erratum: The secondary eclipse of the transiting exoplanet CoRoT-2b * (Astronomy and Astrophysics (2009) 501 (L23-L26) DOI:10.1051/0004-6361/ 200912505)
Astronomy and Astrophysics 512:8 (2010)