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Article Contents
1 Introduction
2 How to resolve the CIRB into individual galaxies ?
3 The 15$\mu $m extragalactic background light
4 MIR, as a tracer of the bolometric IR luminosity
5 IR luminosities and star formation rates of ISOCAM galaxies
6 Contribution of ISOCAM galaxies to the cosmic infrared background
7 Conclusions

Copyright ESO 2002
Published by EDP Sciences