  We report trigonometric parallaxes for 134 low mass stars and brown dwarfs,
of which 38 have no previously published measurement and 79 more have improved
uncertainties. Our survey targeted nearby targets, so 119 are closer than 30
pc. Of the 38 stars with new parallaxes, 14 are within 20 pc and seven are
likely brown dwarfs (spectral types later than L0). These parallaxes are useful
for studies of kinematics, multiplicity, and spectrophotometric calibration.
Two objects with new parallaxes are confirmed as young stars with membership in
nearby young moving groups: LP 870-65 in AB Doradus and G 161-71 in Argus. We
also report the first parallax for the planet-hosting star GJ 3470; this allows
us to refine the density of its Neptune-mass planet. One T-dwarf, 2MASS
J12590470-4336243, previously thought to lie within 4 pc, is found to be at 7.8
pc, and the M-type star 2MASS J01392170-3936088 joins the ranks of nearby stars
as it is found to be within 10 pc. Five stars that are over-luminous and/or too
red for their spectral types are identified and deserve further study as
possible young stars.
