The figure for HIP 67593 is almost certainly an error, probably because the star has a relatively nearby brighter visual binary companion; the movement between the DSS2 and SDSS9 images is less than it. Gaia measured a much smaller proper motion for its Data Release 2, yet a 15-fold parallax between it and its likely common-proper-motion companion HIP 67594. Reconciling its distance and motion will have to wait for Data Release 3 expected to analyse well very high proper motion objects.