The signature of orbital motion from the dayside of the planet τ Boötis b

Matteo Brogi (), Ignas A. G. Snellen, Remco J. de Kok, Simon Albrecht, Jayne Birkby and Ernst J. W. de Mooij
Additional contact information
Matteo Brogi: Leiden Observatory, Leiden University, Postbus 9513, 2300RA Leiden, The Netherlands
Ignas A. G. Snellen: Leiden Observatory, Leiden University, Postbus 9513, 2300RA Leiden, The Netherlands
Remco J. de Kok: SRON, Sorbonnelaan 2, 3584 CA Utrecht, The Netherlands
Simon Albrecht: and Kavli Institute for Astrophysics and Space Research, Massachusetts Institute of Technology
Jayne Birkby: Leiden Observatory, Leiden University, Postbus 9513, 2300RA Leiden, The Netherlands
Ernst J. W. de Mooij: Leiden Observatory, Leiden University, Postbus 9513, 2300RA Leiden, The Netherlands

Nature, 2012, vol. 486, issue 7404, 502-504

Abstract: The detection of carbon monoxide absorption in the spectrum of the extrasolar planet τ Boötis b, and its tracing of the change in the radial velocity of the planet, demonstrates that atmospheric characterization is possible for non-transiting planets.

Date: 2012
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DOI: 10.1038/nature11161

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