Table 2: Radio flux densities of the Coronet sources.

Source ID		 2005 flux density1 1998 flux density2
  [mJy] [mJy]
IRS 2 $0.49 \pm 0.02$ 0.29-0.36
Source 5 $1.14 \pm 0.02$ 0.40-1.21
IRS 5N $0.06 \pm 0.02$ 0.103
IRS 5 $0.68 \pm 0.02$ 0.75-3.28
IRS 6 $0.07 \pm 0.02$ 0.15
IRS 1 $0.42 \pm 0.02$ 0.36-0.59
R CrA $0.30 \pm 0.02$ 0.16-0.26
IRS 7W4 $5.33 \pm 0.02$ 4.11-5.29
IRS 7E $1.77 \pm 0.02$ 1.38-2.10
1 Quoted errors are from Gaussian fitting. Our flux scale has an absolute uncertainty of $\sim$15%;
2 minima and maxima (if source detected in single epochs), see Forbrich et al. (2006);
3 note that this source is not called IRS 5N in Forbrich et al. (2006) but is No. 5 in the tables;
4 blended with Source 9.

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