Discovery of a Methane Dwarf from the IfA-Deep Survey

Details Discovery of a Methane Dwarf from the IfA-Deep Survey Discovery of a Methane Dwarf from the IfA-Deep Survey

2002-02-28

arxiv.org/abs/astro-ph/0202508v1

Astrophys.J. 568 (2002) L107-L111

Astronomy and Astrophysics

Astrophysics

Astrophysical Journal Letters, in press

Scientific paper

10.1086/340375

We present the discovery of a distant methane dwarf, the first from the Institute for Astronomy (IfA) Deep Survey. The object ("IfA 0230-Z1") was identified from deep optical I and z'-band imaging, being conducted as an IfA-wide collaboration using the prime-focus imager Suprime-Cam on the Subaru 8.2-m Telescope. IfA 0230-Z1 is extremely red in the Iz'J (0.8--1.2 micron) bands but relatively blue in J-H; such colors are uniquely characteristic of T dwarfs. A near-IR spectrum taken with the Keck Telescope shows strong H2O absorption and a continuum break indicative of CH4, confirming the object has a very cool atmosphere. Comparison with nearby T dwarfs gives a spectral type of T3-T4 and a distance of ~45 pc. Simple estimates based on previous T dwarf discoveries suggest that the IfA survey will find a comparable number of T dwarfs as the 2MASS survey, albeit at a much larger average distance. We also discuss the survey's ability to probe the galactic scale height of ultracool (L and T) dwarfs.

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