Computer Science
Scientific paper
Oct 2011
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011epsc.conf..249l&link_type=abstract
EPSC-DPS Joint Meeting 2011, held 2-7 October 2011 in Nantes, France. http://meetings.copernicus.org/epsc-dps2011, p.249
Computer Science
Scientific paper
Spectroscopy of exoplanet atmospheres has the potential to provide a wealth of information on their atmospheric properties such as temperature and composition. Here we present a non-linear optimal estimation approach to retrieving exoplanet atmosphere properties from their spectra through a cost function minimization based on the techniques pioneered by [1]. With these tools we can determine the information content and the degrees of freedom for a given spectra and in turn determine, realistically, how much information in terms of temperature and composition can be obtained. We apply these techniques to the well-studied atmospheres of HD189733b, HD209458b, and G436b.
Line Michael R.
Yung Yuk L.
Zhang Xinyu
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