GJ 3378 is a red dwarf and plantary system 7.73 parsecs from us, toward the "Camelopard" north-polar orthogonal to the galactic plane. Two years ago was floated that this was a system. This planet is now recovered - rather, a different planet is recovered. Hat-tip to Pixy Misa.
As usual, more data refines the estimate. I am somewhat intrigued by a planet which is refined to such a statistically-different orbit. Moutou et al. supposed over five Earth masses and orbiting 24.7 days, with a high eccentricity. This new solution from Paul Robertson et al. has two(-plus) masses, at 21.5 days and orbiting possibly circular.
We are dealing here with a spectrograph, not a transit. At this potential angle of separation, transits can be too much for to hope. Thus, above, the language of minima: masses are calculated in m sini, i being rather less than ninety degrees. I also don't know the inclination of the star. Nobody has detected additional planets here, either. Robertson's crew did manage to duplicate Moutou's result with the SPIRou - alone; blaming this instrument for leading them agley.
Will say this: a brown dwarf can be ruled out. For the star, Copilot is asking me about metallicity and rotation. It's slightly less metallic than our own Sun - the latter (circumstantially) suggesting it formed around when our Sun formed. We are not told of a moving-group for this system; suggesting, further, gigayear drift from origin. Rotation is consistent with a stellarish age of five billion or more years. Assuredly a brown dwarf won't have cooled enough for nondetection in Gaia at this distance.
As for other planets, if this star formed in its own nebula as it probably did, larger planets might not have formed at all. Given maybe three years to find other planetary signatures, I assume anything important up to 2 Earth masses and up to one year period should show up. Unless it... has? That "24.7 day" false-positive could signal a 49.4 day true periodicity. It would be too small to do the Von Zeipel.