
We present parallaxes of 11 mid-to-late T dwarfs observed in the UKIRT Infrared Deep Sky Survey. We use these results to test the reliability of model predictions in magnitude-color space, determine a reliable method for the estimation of the physical properties of T dwarfs, and provide a new set of parallax measurements for these objects. The results of this study will be useful for the understanding of the properties of T dwarfs and their place in the context of the late-type stellar population.
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