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Theoretical Spectra of Terrestrial Exoplanet Surfaces http://arxiv.org/abs/1204.1544 We investigate spectra of airless rocky exoplanets with a theoretical framework that self-consistently treats reflection and thermal emission. We find that a silicate
Near-infrared integral-field spectra of the planet/brown dwarf companion AB Pic b http://arxiv.org/abs/1001.0470 Abstract wrote:Chauvin et al. 2005 imaged a co-moving companion at ~260 AU from the young star AB Pic A. Evolutionary models predictions
This might be of interest... 3 general classes of planetary spectra, "soil", "ice", "gas". Not all spectra get assigned to what you'd expect... Ganymede ends up in the "soil" class for example, despite the surface
Model Spectra of the First Potentially Habitable Super-Earth - Gl581d Assumes that it is a terrestrial planet with climate dominated by carbonate-silicate cycle. This may not necessarily be accurate for super-Earths though...
Detection of a Temperature Inversion in the Broadband Infrared Emission Spectrum of TrES-4 http://arxiv.org/abs/0810.0021 Abstract wrote:We estimate the strength of the bandpass-integrated thermal emission from the extrasolar planet TrES-4 at 3.6, 4.5
In frensh translation in english
The HARPS-TERRA project I. Description of the algorithms, performance and new measurements on a few remarkable stars observed by HARPS Includes amongst other things a new orbital solution for epsilon Eridani.