Fig. 4.
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Distribution of the 1 − 10 TeV luminosities for all classes of objects as a function of age, distance, and over the population. Overlaid in the middle panel for comparison are the luminosities corresponding to a 1, 10, or 100 mCrab flux. In the bottom panel, the dashed lines are power-law fits to the high-luminosity ends of the distributions.
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