Fig. 6 from The Mass of the Candidate Exoplanet Companion to HD 33636 from Hubble Space Telescope Astrometry and High‐Precision Radial Velocities

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The Mass of the Candidate Exoplanet Companion to HD 33636 from Hubble Space Telescope Astrometry and High‐Precision Radial Velocities

Authors: Jacob L. Bean, Barbara E. McArthur, G. Fritz Benedict, Thomas E. Harrison, Dmitry Bizyaev, Edmund Nelan, and Verne V. Smith

Bean et al. 2007 The Astronomical Journal 134 749.

Provider: AAS Journals

Caption: Fig. 6.

Results from the detection limit simulations converted to hypothetical companion minimum masses (﹩M\mathrm{sin}\,i﹩, top) and minimum astrometric perturbation size of HD 33636 (﹩a_{A}\mathrm{sin}\,i﹩, bottom). The different lines represent the different assumed eccentricity values. Values above the lines would have been detected with a periodogram analysis of the radial velocity data.

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