Morphology of Weak Lensing Convergence Maps
  We study the morphology of convergence maps by perturbatively reconstructing
their Minkowski Functionals (MFs). We present a systematics study using a set
of three generalised skew-spectra as a function of source redshift and
smoothing angular scale. Using an approach based on pseudo-$S_{\ell}$s (PSL) we
show how these spectra will allow reconstruction of MFs in the presence of an
arbitrary mask and inhomogeneous noise in an unbiased way. Our theoretical
predictions are based on a recently introduced fitting function to the
bispectrum. We compare our results against state-of-the art numerical
simulations and find an excellent agreement. The reconstruction can be carried
out in a controlled manner as a function of angular harmonics $\ell$ and source
redshift $z_s$ which allows for a greater handle on any possible sources of
non-Gaussianity. Our method has the advantage of estimating the topology of
convergence maps directly using shear data. We also study weak lensing
convergence maps inferred from Cosmic Microwave Background (CMB) observations;
and we find that, though less significant at low redshift, the post-Born
corrections play an important role in any modelling of the non-Gaussianity of
convergence maps at higher redshift. We also study the cross-correlations of
estimates from different tomographic bins.
