Evidence for a spectroscopic direct detection of reflected light from 51 Pegasi b

@article{Martins2015EvidenceFA,
  title={Evidence for a spectroscopic direct detection of reflected light from 51 Pegasi b},
  author={Jorge H. C. Martins and Nuno C. Santos and Pedro Figueira and Jo{\~a}o P. Faria and Michael Montalto and Isabelle Boisse and David Ehrenreich and Christophe Lovis and Michel Mayor and Claudio Melo and Francesco A. Pepe and S{\'e}rgio G. Sousa and St{\'e}phane Udry and D. Cunha},
  journal={Astronomy and Astrophysics},
  year={2015},
  volume={576}
}
Context. The detection of reflected light from an exoplanet is a difficult technical challenge at optical wavelengths. Even though this signal is expected to replicate the stellar signal, not only is it several orders of magnitude fainter, but it is also hidden among the stellar noise. Aims. We apply a variant of the cross-correlation technique to HARPS observations of 51 Peg to detect the reflected signal from planet 51 Peg b. Methods. Our method makes use of the cross-correlation function… 

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