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Table 4

Model selection results for the stars without significant periodogram peaks.

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Notes. For each star and each model, we show the logarithm of the evidence, the odds ratio with respect to the constant model, the (normalised) value of the posterior distribution p(n | d) and the AICC and BIC for the maximum-likelihood solution.

(1)

The bars represent the posterior distribution for the number of Keplerians in the model. For each star, this posterior is normalized to the value in the most probable bin.

(2)

Calculated using maximum likelihood value from all MultiNest samples and the number of free parameters for each model.

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