Notes. Bayes factors obtained for different model comparisons indicate how much the data favour the inclusion of a continuous gravitational wave (CGW) with Earth and the pulsar term. The first comparison considers adding a continuous gravitational wave to the pulsar custom noise (PSRN). The second and third model comparisons include an additional common uncorrelated red noise CURN modelled with a power-law with 3 or 9 frequency bins. The fourth and fifth model comparisons include a gravitational wave background GWB modelled with a power-law with 3 or 9 frequency bins.