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