star is found to be a very slow rotator, having a of only 1.3$\pm$0.2 , and with a low chromospheric activity of log$R'_{\rm{HK}}$ of -4.8. We note that this activity level is significantly lower than the one reported in @jenkins11a, due to an updated $B-V$ colour used here. The colour used in Jenkins et al. was drawn from the Hipparcos catalogue ($B-V =$ 0.685), yet the Tycho-2 catalogue magnitudes ([@hog00]) give a colour $>1$, agreeing with what is expected for a mid-K star. Even if the star was moderately active, we would still expect the jitter to be low since mid-K type stars are not as $Doppler-noisy$ as earlier type stars for a given activity level (e.g. [@isaacson10]). This, combined with the very slow rotation of the star, indicates that it is likely a signal with a peak-to-peak amplitude of nearly 80 is not caused by modulated activity effects, especially with a period close to 300 days and eccentricity of 0.8.

The signal detected in our MCMC analysis is also clearly apparent in the MMSE, being the deepest trough, despite the high eccentricity. However, an additional trough at a much longer period is also approaching a similar level of significance. 