The planetary parameters we find here are generally in good agreement with those published in @minniti09 and @jenkins09, however the period we quote is significantly larger than that found by Jenkins et al. by $\sim$80 days. The differences in the periods are attributed to the lower number of high precision HARPS data in that work, which was causing the fitting algorithm to weight heavily towards those data points, even though they were much fewer compared to the MIKE data. This had the effect of significantly increasing the precision of the fit compared to Minniti et al., but in the presence of a linear trend, it also skewed the orbital period to lower values. All other parameters are in excellent agreement within the uncertainties.

HD68402
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The star HD68402 is classed as G5IV/V, though since we find a $\Delta M_V$ of around 0.1 magnitudes, we believe the star to be a dwarf. The metallicity of HD68402 is found to be +0.29 dex. A signal with a semi-amplitude of over 50 was found at a period ($\sim$1100 days) similar to that in the HD9174 data. The MMSE shows two long period troughs for this data, with the detected signal found to be 