1 Spectral types from Burgasser et al. (2006a) except for 2MASS J0756, 2MASS J1036 , 2MASS J1626 and SIMP J0136.
2 Target photometry from 2MASS (Skrutskie et al. 2006).
3 Kirkpatrick et al. (2000).
4 Tinney et al. (2005).
5 Gizis (2002).
6 Knapp et al. (2004).
7 Burgasser (2004).
8 Burgasser et al. (2007)
9 The distance is based on the K magnitude only, as the parallax measurement of sdL7 subdwarf revealed a MK similar to the solar-metallicity L7 dwarfs, while the subdwarf is more than 1 magnitude brighter in the J band (Burgasser et al. 2008).
10 Artigau et al. (2006). They report a distance of
pc.
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