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Fig. 10

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Predicted maximum GRB rates observed by EXIST. We adopted Salpeter IMF, vwind = 100      km   s-1, fGRB = 0.01, f = 0.01; for Pop III.2 GRBs, dashed black line; and Gaussian IMF, vwind = 50      km   s-1, f = 0.1, fGRB = 0.1; for Pop III.1 GRBs, dotted blue line. Dotted red lines represent the same with LF’s bright end power law index 1.7 and 0.8.

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