We introduce two kurt-spectra to probe fourth-order statistics of weak lensing convergence maps. Using state-of-the-art numerical simulations, we study the shapes of these kurt-spectra as a function of source redshifts and smoothing angular scales. We employ a pseudo-Cℓ approach to estimate the spectra from realistic convergence maps in the presence of an observational mask and noise for stage-IV large-scale structure surveys. We compare these results against theoretical predictions calculated using the FFTLog formalism, and find that a simple nonlinear clustering model — the hierarchical ansatz — can reproduce the numerical trends for the kurt-spectra in the nonlinear regime. In addition, we provide estimators for beyond fourth-order spectra where no definitive analytical results are available, and present corresponding results from numerical simulations.
CITATION STYLE
Munshi, D., Lee, H., Dvorkin, C., & McEwen, J. D. (2022). Weak lensing trispectrum and Kurt-spectra. Journal of Cosmology and Astroparticle Physics, 2022(11). https://doi.org/10.1088/1475-7516/2022/11/020
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