We report the discovery of four field methane ("T"-type) brown dwarfs using
Two Micron All-Sky Survey (2MASS) data. One additional methane dwarf, prev
iously discovered by the Sloan Digital Sky Survey, was also identified. Nea
r-infrared spectra clearly show the 1.6 and 2.2 pm CH, absorption bands cha
racteristic of objects with T-eff less than or similar to 1300 K as well as
broadened H2O bands at 1.4 and 1.9 mu m. Comparing the spectra of these ob
jects with that of Gl 229B, we propose that all new 2MASS T dwarfs are warm
er than 950 K, in order from warmest to coolest: 2MASS J1217-03, 2MASS J122
5-27, 2MASS J1047+21, and 2MASS J1237+65. Based on this preliminary sample,
we find a warm T dwarf surface density of 0.0022 T dwarfs deg(-2), or simi
lar to 90 warm T dwarfs over the whole sky detectable to J < 16. The result
ing space density upper limit, 0.01 T dwarfs pc(-3), is comparable to that
of the first L dwarf sample from Kirkpatrick et al.