Indi Ba, Bb: a detailed study of the nearest known brown dwarfs

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Table 4:

The 2MASS magnitudes adopted for $\ensuremath {\varepsilon }$ Indi Ba, Bb in different studies.
Passband	Ba
	McC04	K09	This work
2MASS J	12.29 $\pm$ 0.02	12.33 $\pm$ 0.02	12.29 $\pm$ 0.03
2MASS H	11.51 $\pm$ 0.02	11.54 $\pm$ 0.02	11.50 $\pm$ 0.03
2MASS $K_{\rm {S}}$	11.35 $\pm$ 0.02	11.37 $\pm$ 0.02	11.38 $\pm$ 0.03
Passband	Bb
	McC04	K09	This work
2MASS J	13.23 $\pm$ 0.02	13.19 $\pm$ 0.03	13.23 $\pm$ 0.03
2MASS H	13.27 $\pm$ 0.02	13.36 $\pm$ 0.03	13.19 $\pm$ 0.03
2MASS $K_{\rm {S}}$	13.53 $\pm$ 0.02	13.51 $\pm$ 0.02	13.49 $\pm$ 0.03

McC04 refers to McCaughrean et al. (2004) for which we have assumed the uncertainties on the photometry to be equal to the uncertainty on the 2MASS photometry of the unresolved system. K09 is the study of Kasper et al. (2009).

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