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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 YmodJ2MASS measured on the 813 brown dwarf spectra used in this study. We also reference the local spatial density n.

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