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| Paper: |
A Spectroscopic Method for Direct Detection of Exoplanets |
| Volume: |
450, Molecules in the Atmospheres of Extrasolar Planets |
| Page: |
229 |
| Authors: |
Cubillos, P.; Rojo, P.; Fortney, J. |
| Abstract: |
In this work we have revisited a method to directly search the signature
of a known non-transiting extrasolar planet in the IR spectrum of a
star-planet system. We present preliminary results on the planetary
system HD 217107 observed with Phoenix spectrograph in 2007, and also
present an optimized strategy to maximize our future success considering the
best conditions and best candidates to observe after performing
simulations to predict sensitivity limits of the method.
With positive results this method could add new information of
nontransiting exoplanets and validate the high
resolution models of their atmospheres. |
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