Table 2: The ISOCAM flux densities for MIR clumps in Mkn 297. The photometry was performed before deconvolution and is accurate to about $\pm $15%.

$\lambda$
Total flux Source flux densities
  density        
($\mu $m) (mJy) (mJy)
    1 2 3 4

6.7
141 19.5 16.0 14.0 19.0
7.7 246 30.5 19.5 19.0 29.5
12.0 269 42.5 28.0 24.5 31.5
14.3 289 66.5 48.5 30.5 43.5


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