Fig. 10.

Rate of events (all sky and in the source frame) for a model that traces the star formation rate and normalized to 8 × 10−5 events per year per Mpc3 (dashed line). The SNe rate has been re-scaled by a factor 106 for presentation purposes. Also shown are the product of the rate times the optical depth for μ > 100 (solid line) and the rate of lensed events with the same apparent magnitude as a similar unlensed event at z = 0.3 (dotted line).
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