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We present positions, proper motions, and near-infrared photometry for 966known objects with spectral types later than M observed as part of the theUKIRT Hemisphere Survey (UHS). We augment the photometry and astrometry fromUHS with information from Gaia DR3, Pan-STARRS DR2, and CatWISE 2020 to producea database of homogeneous photometry and astrometry for this sample. Themulti-epoch survey strategy of UHS allows us to determine proper motions formost sources, with a median proper motion uncertainty of $\sim$3.6 masyr$^{-1}$. Our UHS proper motion measurements are generally in good agreementwith those from Gaia DR3, Pan-STARRS, and CatWISE 2020, with UHS proper motionstypically more precise than those from CatWISE 2020 and Pan-STARRS but not GaiaDR3. We critically analyze publicly available spectra for 406 members of thissample and provide updated near-infrared spectral types for $\sim$100 objects.We determine typical colors as a function of spectral type and provide absolutemagnitude vs. spectral type relations for UHS $J$- and $K$-band photometry.Using newly determined proper motions, we highlight several objects ofinterest, such as objects with large tangential velocities, widely separatedco-moving companions, and potential members of young nearby associations.

Astrometry and Photometry for $\approx$1000 L, T, and Y Dwarfs from the UKIRT Hemisphere Survey