\
14348$^{6}$ & 33.1$\pm$5.8 & 96.8$\pm$10.3 & & & & & & 2.9$\pm$0.6 &\
14348$^{\dag}$ & 37.9$\pm$1.6 & & 16.9$\pm$2.0 & 52.6$\pm$2.4 & 34.4$\pm$3.3 & 14.1$\pm$10.7 & & & 2.2$\pm$0.3\

**Table note:** For each interacting system, we have measured the integrated flux of the individual galaxies resolved by ISOCAM and marked the southern and the northern galaxies with (S) and (N) respectively. We used the same notations as in Table 2 for identifying the different sets of ISOCAM observations, labeled (1) through (6). As all three galaxies were also observed with ISOPHOT-S and one with the CVF, we also provide the equivalent broad-band filter flux estimates (using the known filter band-passes and transmission curves) based on those spectra marked with a $\dag$ for ISOPHOT-S and a (5) for the CVF. The errors given for each measurement are statistical derived by adding the 1$\sigma$ rms map to the systematic error of 10% commonly associated with the transient correction. Absolute flux uncertainties are estimated to be $\pm$ 20$\%$. For the cases where we present multiple measurements for a target their median value should be considered as its nominal flux density.

As it has been discussed in several papers describing ISO observations [i.e. 