 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 not consistent with the high proper motion.Gaia measured a much smaller proper motion for DR2, but also a parallax difference of a factor fifteen between the star and its nearby apparently common-proper-motion companion HIP 67594.A resolution of this will have to wait for Gaia DR3; generally very-high-proper-motion stars do not show up in Gaia DR2.