Image Details
Caption: Fig. 1.
Keck Doppler velocities, with error bars, for HD 16141. The solid line through the points shows the best Keplerian fit. The residuals having ﹩\mathrm{rms}\,=3.24﹩ m s﹩^{-1}﹩ are shown at the bottom (crosses) with arbitrary zero point (horizontal dashed line).
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