Enhancing cosmic shear with the multi-scale lensing PDF

We quantify the cosmological constraining power of the lensing PDF' - the one-point probability density of weak lensing convergence maps - by modelling this statistic numerically with an emulator trained on $w$CDM cosmic shear simulations. After validating our methods on Gaussian and lognormal fields, we show that multi-scale’ PDFs - measured from maps with multiple levels of smoothing - offer considerable gains over two-point statistics, owing to their ability to extract non-Gaussian information: for a mock Stage-III survey, lensing PDFs yield 33% tighter constraints on the clustering parameter $S_8={\sigma }_8\sqrt{{\mathrm{\Omega }}_{\mathrm{m}}\mathrm{/}0.3}$ than the two-point shear correlation functions. For Stage-IV surveys, we achieve $>$90% tighter constraints on $S_8$, but also on the Hubble and dark energy equation of state parameters. Interestingly, we find improvements when combining these two probes only in our Stage-III setup; in the Stage-IV scenario the lensing PDFs contain all information from the standard two-point statistics and more. This suggests that while these two probes are currently complementary, the lower noise levels of upcoming surveys will unleash the constraining power of the PDF.