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Fig. 8

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Luminosity in the 100 MeV100 GeV band as a function of total infrared luminosity and SFR for the complete sample of models. The orange region is the uncertainty range of the correlation determined experimentally. The top panel shows the result for the basic model, and the middle panel shows the result obtained with larger halos for the small galaxies and using a correction for starlight leakage. The bottom panel shows the ratio of 100 MeV100 GeV to total infrared luminosities.

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