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Table 2.

Compiled results for the observed targets including photometry and astrometry for the binary candidates.

Object SpT type Distance Happ Kapp Age Mass Separation PA
[pc] [mag] [mag] [Myr] [MJup] [mas] [deg]
2M2033 L0γ ± 1 55.4 ± 3.6(a) 15.14 ± 0.11 14.24 ± 0.08 20−40
2M2117 T0 16.9 ± 1.7 (b) 14.53 ± 0.04 14.15 ± 0.07 21−26
2M22353 M9γ ± 1 46.42 ± 0.72 13.59 ± 0.04 13.17 ± 0.03 20−40
2M2322 L1γ ± 2 43.03 ± 1.94 14.54 ± 0.06 13.86 ± 0.04 20−40

2M1510A M9γ−1 36.74 ± 0.36 12.28 ±  0.04 11.82 ±  0.04 30−50
2M1510B L1β(?) 14.22 ±  0.06 14.09 ±  0.04 30−50 103.43 ± 13.43 64.96 ± 2.12
2M1547A 34.25 ± 0.46 13.67 ±  0.07 13.19 ±  0.04 30−50
2M1547B 14.55 ±  0.07 13.91 ±  0.04 30−50 173.66 ± 0.59 15.62 ± 0.50
2M2202A M9γ/β ± 1 69.97 ± 2.36 14.34 ±  0.07 13.91 ±  0.06 120−200
2M2202B M9γ/β ± 1 14.41 ±  0.08 13.92 ±  0.06 120−200 60.36 ± 2.67 59.51 ± 1.58

Notes. Masses are calculated from BT-Settl evolutionary models.

(a)

Distance measurement from Gagné et al. (2015).

(b)

Distance measurement from Best et al. (2015).

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