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Table 2:

Color-corrected fluxes of EX Lupi*.
$\lambda $[$\mu $m] 1983 1997 Feb. 5 1997 Mar. 18 1997 Aug. 24 1997 Sept. 19 2005 Mar. 29
  IRAS ISOPHOT ISOPHOT ISOPHOT ISOPHOT Spitzer/IRAC
3.6   $0.17\pm0.03$ $0.18\pm0.03$ $0.15\pm0.02$ $0.16\pm0.03$ $0.190 \pm 0.004$
4.5           $0.206\pm 0.004$
5.8           $0.236\pm 0.005$
8.0           $0.317\pm 0.007$
12 $0.76\pm 0.1$ $0.73\pm0.11$ $0.78\pm0.12$ $0.76\pm0.12$ $0.68\pm0.11$  
15   $0.54\pm0.08$ $0.43\pm0.07$ $0.47\pm0.07$ $0.48\pm0.07$  
20   $1.06\pm0.15$ $1.30\pm0.18$ $0.91\pm0.13$ $1.12\pm0.16$  
25 $1.04\pm 0.1$ $0.78\pm0.12$ $0.87\pm0.14$ $0.66\pm0.11$ $1.29\pm0.21$  
60 $1.35\pm 0.4$ $1.52\pm0.32$        
100 $0.97\pm 0.5$   $1.27\pm0.17 $      
200       $1.23\pm 0.35$    
* For the ISOPHOT data we adopted a conservative formal uncertainty of 15%.

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