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Fig. 10.

image

Magnification distribution for all background sources. We overlay a theoretical μ−2 relation to guide the eye. We observe a significant drop in the number of sources at low magnifications (μ <  1.5), due to the limits set by the FoV of the MUSE observations, and at very high magnifications (μ >  25) due to the very small statistics and possibly the resolved nature of Lyman-α emitters.

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