The RoPES project with HARPS and HARPS-N - II. A third planet in the multi-planet system HD 176986

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Table 2

Evidence of different models for HD 176986.

Model	∆lnZ YARARA	∆ln Z multi-dim GP
Two-sinusoidal	−16.1	−23.6
Three-sinusoidal	0.0	0.0
Three Keplerian	−6.0	+0.2
Four-sinusoidal	−1.5	−10.3

Notes. We see in the table the difference in evidence of different models. The three-sinusoidal model is favored compared to the two-sinusoidal model and the four-sinusoidal model. The circular solution is also favored compared to the solution with an eccentricity.

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