Color–magnitude diagram of confirmed or high-likelihood members of ABDMG (as defined by Faherty et al. 2016) with trigonometric distance measurements (red stars) compared with field (black diamonds) and young brown dwarfs (open purple circles and right-pointing blue triangles). Field brown dwarfs within one spectral subtype of 2MASS J1324+6358 are marked with a green open circle. The ABDMG members define a sequence redder than the field, with an L/T transition happening at a slightly fainter J-band magnitude. 2MASS J1324+6358 is both redder and fainter than field T1–T3 dwarfs in the near-infrared, similarly to young late-type L dwarfs. These data were compiled from Gagné et al. (2015b), Faherty et al. (2016), Liu et al. (2016), Vos et al. (2018), and other references therein.