University of Hertfordshire

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From the same journal

A search for high proper motion T dwarfs with pan-starrs1 + 2MASS + wise

Research output: Contribution to journalArticle

  • Michael C. Liu
  • Niall R. Deacon
  • Eugene A. Magnier
  • Trent J. Dupuy
  • Kimberly M. Aller
  • Brendan P. Bowler
  • Joshua Redstone
  • Bertrand Goldman
  • W. S. Burgett
  • K. C. Chambers
  • K. W. Hodapp
  • N. Kaiser
  • R. P. Kudritzki
  • J. S. Morgan
  • P. A. Price
  • J. L. Tonry
  • R. J. Wainscoat
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Original languageEnglish
Article numberL32
Pages (from-to)1-6
Number of pages6
JournalAstrophysical Journal Letters
Volume740
Issue2
DOIs
Publication statusPublished - 23 Sep 2011

Abstract

We have searched 8200deg2 for high proper motion (05-27year -1) T dwarfs by combining first-epoch data from the Pan-STARRS1 (PS1) 3π Survey, the Two Micron All Sky Survey (2MASS) All-Sky Point Source Catalog, and the WISE Preliminary Data Release. We identified two high proper motion objects with the very red (W1 - W2) colors characteristic of T dwarfs, one being the known T7.5 dwarf GJ 570D. Near-IR spectroscopy of the other object (PSO J043.5395+02.3995 ≡ WISEP J025409.45+022359.1) reveals a spectral type of T8, leading to a photometric distance of 7.2 ± 0.7pc. The 256year-1 proper motion of PSO J043.5+02 is the second highest among field T dwarfs, corresponding to a tangential velocity of 87 ± 8kms -1. According to the Besançon galaxy model, this velocity indicates that its galactic membership is probably in the thin disk, with the thick disk an unlikely possibility. Such membership is in accord with the near-IR spectrum, which points to a surface gravity (age) and metallicity typical of the field population. We combine 2MASS, Sloan Digital Sky Survey, WISE, and PS1 astrometry to derive a preliminary parallax of 171 ± 45 mas (5.8+2.0 -1.2pc), the first such measurement using PS1 data. The proximity and brightness of PSO J043.5+02 will facilitate future characterization of its atmosphere, variability, multiplicity, distance, and kinematics. The modest number of candidates from our search suggests that the immediate (∼10pc) solar neighborhood does not contain a large reservoir of undiscovered T dwarfs earlier than about T8.

Notes

© 2011. The American Astronomical Society. All rights reserved. Printed in the U.S.A.

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