Fig. 7
Measured radial velocity variation of GJ 9827 from FIES (circles) and HARPS (diamonds) and HARPS-N (triangles). The red solid line is the best-fit model including the signal of the planets and the Gaussian Process model of the correlated stellar noise. The colored dashed line shows the signal of the planets. The blue dotted line shows the Gaussian Process model of correlated stellar noise.
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