 In 2016, data collected during the extended K2 mission of the Kepler space telescope was used to identify two transiting exoplanet candidates orbiting this star, designated HD 3167 b and HD 3167 c. This makes it one of the closest and brightest such multi-transiting stars known.The lack of chromospheric activity makes it ideal for the precise radial velocity (RV) measurements needed to estimate the masses of its planets.Follow-up RV observations showed additional perturbation signals beyond the two planets already identified.