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Stellar noise and planet detection. II. Radial-velocity noise induced by magnetic cycles

Published online by Cambridge University Press:  10 November 2011

Xavier Dumusque
Affiliation:
Observatoire de Genève, 51 ch. des Maillettes, 1290 Sauverny, Switzerland email: xavier.dumusque@unige.ch Centro de Astrofísica, Universidade do Porto, Rua das Estrelas, 4150-762 Porto, Portugal
Cristophe Lovis
Affiliation:
Observatoire de Genève, 51 ch. des Maillettes, 1290 Sauverny, Switzerland email: xavier.dumusque@unige.ch
Stephane Udry
Affiliation:
Observatoire de Genève, 51 ch. des Maillettes, 1290 Sauverny, Switzerland email: xavier.dumusque@unige.ch
Nuno C. Santos
Affiliation:
Centro de Astrofísica, Universidade do Porto, Rua das Estrelas, 4150-762 Porto, Portugal
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Abstract

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For the 451 stars of the HARPS high precision program, we study correlations between the radial-velocity (RV) variation and other parameters of the Cross Correlated Function (CCF). After a careful target selection, we found a very good correlation between the slope of the RV-activity index (log(R'HK)) correlation and the Teff for dwarf stars. This correlation allow us to correct RV from magnetic cycles given the activity index and the Teff.

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2011

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