The Hawaii Infrared Parallax Program. IV. A Comprehensive Parallax Survey of L0-T8 dwarfs with UKIRT
arXiv:2010.15850 · doi:10.3847/1538-3881/ab84f4
Abstract
We present parallaxes, proper motions, and -band photometry for 348 L and T dwarfs measured using the wide-field near-infrared camera WFCAM on the United Kingdom Infrared Telescope. This is the largest single batch of infrared parallaxes for brown dwarfs to date. Our parallaxes have a median uncertainty of 3.5 mas, similar to most previous ground-based infrared parallax surveys. Our target list was designed to complete a volume-limited parallax sample of L0-T8 dwarfs out to 25 pc spanning declinations to (68% of the sky). We report the first parallaxes for 165 objects, and we improve on previous measurements for another 53 objects. Our targets include 104 objects (mostly early-L dwarfs) having DR2 parallax measurements, with which our parallaxes are consistent. We include an extensive comparison of previous literature parallaxes for L and T dwarfs with both our results and DR2 measurements, identifying systematic offsets for some previous surveys. Our parallaxes confirm that 14 objects previously identified as wide common proper motion companions to main-sequence stars have distances consistent with companionship. We also report new photometry for our targets, including the first measurements for 193 of our targets and improvements over previously published photometry for another 60 targets. Altogether, our parallaxes will enable the first population studies using a volume-limited sample spanning spectral types L0-T8 defined entirely by parallaxes.
arXiv commentPublished in AJ. 54 pages, 17 figures, 7 tables. Data for all parallax survey targets can be found in the UltracoolSheet at http://bit.ly/UltracoolSheet , a compilation of 3000+ ultracool dwarfs and imaged exoplanets, including photometry, J2000 positions, parallaxes, proper motions, multiplicity, and spectroscopic classifications from multiple surveys and numerous sources
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