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We present the Late-Type Extension to the Motion Verified Red Stars(LaTE-MoVeRS) catalog, containing 46,463 photometric late-type ($>$ M5) dwarfswithin the Sloan Digital Sky Survey (SDSS) footprint. Proper motions werecomputed for objects combining astrometry from the SDSS Data Release 12 (DR12),the Two-Micron All-Sky Survey (2MASS) Point Source Catalog (PSC), and the\emph{Wide-field Infrared Survey Explorer} (\emph{WISE}) AllWISE datasets.LaTE-MoVeRS objects were required to have significant proper motion($\mu_\mathrm{tot} \geqslant 2\sigma_{\mu_\mathrm{tot}}$). Using theLaTE-MoVeRS sample and \emph{Gaia} Data Release 1, we estimate \emph{Gaia} willbe $\sim$64\% complete for very-low-mass objects ($>$ M5) in comparison to thecombined SDSS+2MASS+\emph{WISE} dataset ($i < 21.3$). We computed photometricdistances and estimated stellar effective temperatures for the LaTE-MoVeRScatalog. The majority of the dwarfs in the sample have distances $< 150$ pc and$T_\mathrm{eff} < 3000$ K. Thirteen objects were identified within LaTE-MoVeRSwith estimated photometric distances within 25 pc that have not been previouslyidentified as nearby objects. We also identified one new object with a largeamount of excess mid-infrared flux that has not been previously identified(2MASS J11151597$+$1937266). This object appears to be an L2$\gamma$ at$\sim$50 pc showing spectroscopic signs of a flaring event (e.g., strongHydrogen Balmer emission lines). This object does not exhibit kinematicssimilar to any known kinematic association. The LaTE-MoVeRS catalog isavailable through SDSS CasJobs and VizieR.

The Late-Type Extension to MoVeRS (LaTE-MoVeRS): Proper motion verified low-mass stars and brown dwarfs from SDSS, 2MASS, and WISE