Table 2: Summary of IRAC observations of the sources in the environment of SGR 1806-20. We give their name and their MIR fluxes (in Jy). Uncertainties are given at 1$\sigma $.
Sources $3.6~{\mu}$m $4.5~{\mu}$m $5.8~{\mu}$m $8.0~{\mu}$m
  October 2004
LBV 1806-20 (A) $0.306\pm0.010$ $0.316\pm0.008$ $0.283\pm0.008$ $0.175\pm0.005$
WC9 (B) $0.165\pm0.005$ $0.208\pm0.006$ $0.218\pm0.007$ $0.141\pm0.003$
Supergiant (C) $0.041\pm0.002$ $0.036\pm0.002$ $0.028\pm0.002$ $0.027\pm0.002$
  September 2005
LBV 1806-20 (A) $0.337\pm0.015$ $0.332\pm0.016$ $0.299\pm0.014$ $0.199\pm0.007$
WC9 (B) $0.172\pm0.009$ $0.218\pm0.011$ $0.224\pm0.011$ $0.140\pm0.005$
Supergiant (C) $0.037\pm0.003$ $0.037\pm0.003$ $0.031\pm0.003$ $0.027\pm0.001$
  April 2006
LBV 1806-20 (A) $0.297\pm0.010$ $0.304\pm0.001$ $0.272\pm0.011$ $0.174\pm0.005$
WC9 (B) $0.170\pm0.006$ $0.207\pm0.007$ $0.225\pm0.009$ $0.140\pm0.006$
Supergiant (C) $0.041\pm0.003$ $0.038\pm0.002$ $0.030\pm0.003$ $0.025\pm0.002$

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