The presence of methane in the atmosphere of an extrasolar planet

[1]  C. Beichman,et al.  The Mid-Infrared Spectrum of the Transiting Exoplanet HD 209458b , 2007, astro-ph/0702593.

[2]  C. Moutou,et al.  Detection of atmospheric haze on an extrasolar planet: the 0.55–1.05 μm transmission spectrum of HD 189733b with the Hubble Space Telescope , 2007, 0712.1374.

[3]  C. Moutou,et al.  Hubble Space Telescope time-series photometry of the planetary transit of HD 189733: no moon, no rings, starspots , 2007, 0707.1940.

[4]  Jonathan Tennyson,et al.  Water vapour in the atmosphere of a transiting extrasolar planet , 2007, Nature.

[5]  Mark S. Marley,et al.  Analysis of Spitzer Spectra of Irradiated Planets: Evidence for Water Vapor? , 2007, 0705.2457.

[6]  David Charbonneau,et al.  A map of the day–night contrast of the extrasolar planet HD 189733b , 2007, Nature.

[7]  L. J. Richardson,et al.  A spectrum of an extrasolar planet , 2007, Nature.

[8]  A. Burrows,et al.  A Spitzer Spectrum of the Exoplanet HD 189733b , 2007, astro-ph/0702494.

[9]  Avi Shporer,et al.  The Transit Light Curve Project. V. System Parameters and Stellar Rotation Period of HD 189733 , 2006, astro-ph/0612224.

[10]  D. Ehrenreich,et al.  Infrared Transmission Spectra for Extrasolar Giant Planets , 2006, astro-ph/0611174.

[11]  A. P. Showman,et al.  The Influence of Atmospheric Dynamics on the Infrared Spectra and Light Curves of Hot Jupiters , 2006 .

[12]  I. Hubeny,et al.  Theory for the Secondary Eclipse Fluxes, Spectra, Atmospheres, and Light Curves of Transiting Extrasolar Giant Planets , 2006, astro-ph/0607014.

[13]  A. Showman,et al.  Dynamics and Disequilibrium Carbon Chemistry in Hot Jupiter Atmospheres, with Application to HD 209458b , 2006, astro-ph/0602477.

[14]  R. Tolchenov,et al.  A high-accuracy computed water line list , 2006, astro-ph/0601236.

[15]  Gang Li,et al.  The HITRAN 2008 molecular spectroscopic database , 2005 .

[16]  A. Burrows.  A theoretical look at the direct detection of giant planets outside the Solar System , 2005, Nature.

[17]  S. Seager,et al.  On the Insignificance of Photochemical Hydrocarbon Aerosols in the Atmospheres of Close-in Extrasolar Giant Planets , 2004, astro-ph/0402601.

[18]  P. Bernath,et al.  Hot methane spectra for astrophysical applications , 2003 .

[19]  R. Gilliland,et al.  High Signal-to-Noise, Differential NICMOS Spectrophotometry , 2002 .

[20]  U. Jørgensen,et al.  High-temperature (1000–7000 K) collision-induced absorption of H2 pairs computed from the first principles, with application to cool and dense stellar atmospheres , 2001 .

[21]  T. Brown.  Transmission Spectra as Diagnostics of Extrasolar Giant Planet Atmospheres , 2001, astro-ph/0101307.

[22]  A. Burrows,et al.  Theory of Extrasolar Giant Planet Transits , 2001, astro-ph/0101024.

[23]  A. Claret,et al.  A new non-linear limb-darkening law for LTE stellar atmosphere models. Calculations for -5.0 <= log[M/H ] <= +1, 2000 K <= Teff <= 50000 K at several surface gravities , 2000 .

[24]  A. Claret,et al.  A new non-linear limb-darkening law for LTE stellar atmosphere models III , 2000 .

[25]  Princeton,et al.  Theoretical Transmission Spectra during Extrasolar Giant Planet Transits , 1999, astro-ph/9912241.

[26]  F. Allard,et al.  The NextGen Model Atmosphere Grid for 3000 ≤ Teff ≤ 10,000 K , 1998, astro-ph/9807286.