Table 1: Positions and magnitudes from Momany et al. (2003). For each star, the first line lists the original magnitudes while the second gives dereddened magnitudes and colours adopting the reddening law by Dean et al. (1978) and Rieke & Lebofsky (1985). Star I-36 could not be measured in the H frame. $(V-I)_{\rm J}$ is Johnson, $(V-I)_{\rm C}$is Cousins.

Star		 $\alpha_{2000}$ $\delta_{2000}$ $\Delta E(B-V)$ V I J H $K_{\rm s}$        
      E(B-V) V0 I0 J0 H0 $K_{\rm s0}$ $(V-I)_{\rm C0}$ $(V-I)_{\rm J0}$ (V-K)0 (J-K)0
I-16 18:04:49.5 -30:03:03.5 -0.039 16.73 14.94 13.41 12.57 12.40        
      0.421 15.42 14.19 13.12 12.34 12.25 1.23 1.58 3.17 0.87
I-18 18:04:49.7 -30:03:02.5 -0.039 16.73 15.06 13.79 13.03 12.96        
      0.421 15.42 14.31 13.50 12.80 12.81 1.11 1.43 2.61 0.69
I-24 18:04:50.3 -30:03:08.9 -0.039 17.19 15.40 14.12 13.39 13.22        
      0.421 15.88 14.65 13.83 13.16 13.07 1.23 1.58 2.81 0.76
I-36 18:04:50.9 -30:03:48.0 -0.026 16.39 14.42 12.90 - 11.86        
      0.434 15.04 13.65 12.59 99.75 11.71 1.39 1.79 3.34 0.89

I-42

 18:04:47.7 -30:03:46.5 -0.046 16.43 14.33 12.81 11.90 11.79        
      0.414 15.15 13.60 12.53 11.68 11.64 1.55 1.99 3.50 0.89


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