During the observations 13 doppler velocity tests were conducted, which showed this object's mass was at least 7.8 Jovian-masses and its orbit has a high eccentricity.
The exoplanet takes 3.53 years to complete a full stellar orbit.
[5][1][6] An astrometric measurement of the planet's inclination and true mass was published in 2022 as part of Gaia DR3.
[7] A number of subsequent studies in 2022 and 2023 have determined astrometric orbits for HD 175167 b,[2] estimating masses ranging from 6.4 MJ[8] to 15 MJ,[9][4] the latter of which would put it at the borderline of being a brown dwarf.
The most recent and accurate mass measurement is 10 MJ, making it a massive super-Jovian planet.