Direct-imaging discovery of a 12–14 Jupiter-mass object orbiting a young binary system of very low-mass stars

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Table 2

Host system absolute magnitudes compared with BT-Settl isochrones at 30 Myr absolute magnitudes (2MASS for JHK and NACO for L′).

Filter	M_J	M_H	M _{K_s}	M_L′


2M0103A	7.36 ± 0.05	6.78 ± 0.05	6.44 ± 0.05	6.04^*
2M0103B	7.56 ± 0.05	6.98 ± 0.05	6.64 ± 0.05	6.24^*
Model 0.2 M_⊙	7.31	6.75	6.50	6.1
– 0.175 M_⊙	7.51	6.95	6.70	6.3

Notes.

^(*)

Since no calibrated photometry is available in L′, these magnitudes are derived from the modelled K_S − L′.

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