the second trough behind a slightly stronger trough close to 3000 days. The signal was found to have an eccentricity of 0.03, but to within the limits it can be considered as circular.

Given the mass of HD68402 is 1.12 , we compute a minimum mass of just over 3  for the planet. The phase folded velocities for the planetary signal are shown in Fig. \[phased3\]. Since the log-Bayesian evidence is 49.4, strongly confirming the existence of a signal, and it was also found in the MMSE analysis, and by a manual fitting approach, the solution is significantly well constrained, even though there is a small gap in the phase folded curve.

HD72892
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This G5V star is located at a distance of 73 pc from the Sun and has a metallicity of +0.25 dex. The star is also very inactive (log$R'_{\rm{HK}}$ = -5.02) and a slow rotator (= 2.5 ) representing an excellent target to search for planets. We have detected a signal with a period of nearly 40 days and semi-amplitude of 320 . The signal has a log Bayesian evidence value of 903.0, confirming the signal at very high significance. Given the S/N ratio between the signal 