Published in

Cambridge University Press (CUP), Proceedings of the International Astronomical Union, S249(3), p. 111-114, 2007

DOI: 10.1017/s1743921308016475

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Selection effects in Doppler velocity planet searches

Journal article published in 2007 by Simon O'Toole ORCID, Chris Tinney, Hugh Jones
This paper was not found in any repository, but could be made available legally by the author.
This paper was not found in any repository, but could be made available legally by the author.

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Data provided by SHERPA/RoMEO

Abstract

AbstractThe majority of extra-solar planets have been discovered by measuring the Doppler velocities of the host star. Like all exoplanet detection methods, the Doppler method is rife with observational biases. Before any robust comparison of mass, orbital period and eccentricity distributions can be made with theory, a detailed understanding of these selection effects is required, something which up to now is lacking. We present here a progress report on our analysis of the selection effects present in Anglo-Australian Planet Search data, including the methodology used and some preliminary results.

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