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Li, Hjorth & Richard quantify the unlikelihood of seeing a multiply-imaged supernova in A1689, and other clusters.

Would be nice to make similar forecast for Euclid (~40 epochs in the Deep Caps)

This is a very interesting paper indeed - Karpenka et al are trying to detect the weak lensing effect on SNe Ia, using a halo model for the line of sight structure. The interesting part is that they infer the parameters of the halo model simultaneously with the cosmological parameters, with the individual convergences playing a fleeting role before being quickly marginalised out. This is the Right Thing To Do - very computationally intensive, but feasible, as they show!

Although, to qualify that comment about computational intensity: they do not include scatter in their assumed scaling relation between halo mass and galaxy luminosity. To do that properly needs a whole slew of additional parameters, one for the true mass of every galaxy in sight...

It is similar to what I wrote a paper about in 2001. It is good to see this idea is being pursued. It has always seemed to me that you would do better with galaxy-galaxy lensing because of the much larger numbers.