Table 2
Characteristics of L and T dwarfs.
Spectral type spt | MYmod (mag) | n⊙ (10−3 pc−3 spt−1) | dYmod=22.5 (pc) |
|||
---|---|---|---|---|---|---|
W1 | W2 | W3 | W4 | |||
L0 | 13.21 | 0.637 | 695 | 702 | 687 | 666 |
L1 | 13.62 | 0.861 | 579 | 584 | 573 | 558 |
L2 | 14.09 | 1.000 | 470 | 473 | 466 | 456 |
L3 | 14.54 | 0.834 | 383 | 385 | 380 | 374 |
L4 | 15.00 | 0.819 | 311 | 312 | 309 | 305 |
L5 | 15.40 | 0.869 | 259 | 260 | 258 | 255 |
L6 | 15.76 | 0.785 | 220 | 221 | 220 | 217 |
L7 | 16.09 | 0.644 | 190 | 191 | 190 | 188 |
L8 | 16.21 | 0.462 | 180 | 180 | 179 | 178 |
L9 | 16.36 | 0.308 | 167 | 168 | 167 | 166 |
T0 | 16.39 | 0.22 | 165 | 166 | 165 | 163 |
T1 | 16.39 | 0.241 | 166 | 166 | 165 | 164 |
T2 | 16.36 | 0.406 | 167 | 168 | 167 | 165 |
T3 | 16.23 | 0.788 | 178 | 178 | 177 | 176 |
T4 | 16.32 | 1.42 | 171 | 171 | 170 | 169 |
T5 | 16.35 | 2.38 | 168 | 169 | 168 | 166 |
T6 | 16.60 | 3.45 | 150 | 151 | 150 | 149 |
T7 | 17.11 | 4.82 | 119 | 119 | 119 | 118 |
T8 | 17.96 | 6.19 | 81 | 81 | 81 | 81 |
T9 | 19.25 | 7.56 | 45 | 45 | 45 | 44 |
Notes. d is the maximum heliocentric distance for which a brown dwarf of a given spectral type and with an apparent magnitude Ymod = 22.5 can be detected. The absolute magnitudes MYmod were computed by combining the absolute magnitude in the 2MASS J filter MJ2MASS derived by Dupuy & Liu (2012) for each spectral type, with the observed colours Ymod − J2MASS measured on the 813 brown dwarf spectra used in this study. We also reference the local spatial density n⊙.
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