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Fig. 8

image

Comparison of the supernova rates limits measured from our survey and those obtained from the SFR published in Riehm et al. (2011). The limits represent 90% C.L. The numbers label the background galaxies shown in Fig. 9. Only the galaxies with multiple images and delay time less than five years (i.e. less than the duration of the survey) are considered here.

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