High - precision radial -
velocity measurements confirm a sinusoidal variation with the period and phase predicted by the photometry, and rule out the presence of line - bisector variations that would indicate that the spectroscopic orbit is spurious.
Not exact matches
Initially identified a decade ago through radial
velocity measurements, it was later
confirmed through transit observations with the MOST and Spitzer space telescopes.
Kepler 18 - b, c, and d: A System Of Three Planets
Confirmed by Transit Timing Variations, Lightcurve Validation, Spitzer Photometry and Radial
Velocity Measurements
We detected the transit light - curve signature in the course of the TrES multi-site transiting planet survey, and
confirmed the planetary nature of the companion via multicolor photometry and precise radial
velocity measurements.
This low - mass companion was discovered using radial
velocity measurements in 1996, possibly
confirming Louis Berman's discovery of a spectroscopic companion to Star B in 1931.
Kepler 10b was detected using the transit method from more than eight months of data collected by the spacecraft between May 2009 and early January 2010 and
confirmed by radial
velocity measurements, and there evidence for another planet (KOI 72.02) in an outer orbit with a period around 45.3 days (Kepler news release; images, animations, and discovery page; and Batalha et al, 2011).
It was discovered by J.B. Irwin in 1956, its membership was
confirmed by radial
velocity measurements conducted by M.W. Feast of Radcliffs Observatory (the common RV of the cluster members is +4 km / sec).