Fig. 5 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. 5.

Periodogram of the radial velocity residuals from the best‐fit, single‐companion orbit with 1% and 10% FAP limits indicated. No periodicity is detected with ﹩\mathrm{FAP}\,< 70\% ﹩, which indicates that there are no additional companions in the system for our detection limits (see § 6).

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