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Dealing with activity in RV planet searches

Published online by Cambridge University Press:  27 October 2016

Isabelle Boisse
Isabelle Boisse*
Affiliation:
Aix Marseille Université, CNRS, LAM (Laboratoire d'Astrophysique de Marseille) UMR 7326, 13388, Marseille, Franceisabelle.boisse@lam.fr
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Abstract

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Precise radial velocity measurements of a star allow to search for planets. But this method has to face with irregularly time series. Stellar variabilities: pulsation, granulation, stellar activity on a short and long timescale, also modify the measure of the radial velocities. There is indeed a growing literature of controversies on how a signal is interpreted as a planet or due to stellar activity. I present how the star variations change the measured RVs, which techniques and indices are used by several teams to disentangle activity and planets, and the future options that are being studied.

Keywords

Stellar activitySpectroscopy
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 11 , General Assembly A29A: Astronomy in Focus , August 2015 , pp. 193 - 195
Copyright
Copyright © International Astronomical Union 2016 

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