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Sparse Bayesian mass-mapping with uncertainties: peak statistics and feature locations

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arxiv 1812.04018 v2 pith:UP5IITW5 submitted 2018-12-10 astro-ph.CO

classification astro-ph.CO
keywords bayesianpeakuncertaintyconvergencemapsrecoveredcumulativeinverse
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Weak lensing convergence maps - upon which higher order statistics can be calculated - can be recovered from observations of the shear field by solving the lensing inverse problem. For typical surveys this inverse problem is ill-posed (often seriously) leading to substantial uncertainty on the recovered convergence maps. In this paper we propose novel methods for quantifying the Bayesian uncertainty in the location of recovered features and the uncertainty in the cumulative peak statistic - the peak count as a function of signal to noise ratio (SNR). We adopt the sparse hierarchical Bayesian mass-mapping framework developed in previous work, which provides robust reconstructions and principled statistical interpretation of reconstructed convergence maps without the need to assume or impose Gaussianity. We demonstrate our uncertainty quantification techniques on both Bolshoi N-body (cluster scale) and Buzzard V-1.6 (large scale structure) N-body simulations. For the first time, this methodology allows one to recover approximate Bayesian upper and lower limits on the cumulative peak statistic at well defined confidence levels.

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  1. Cosmological studies from tomographic weak lensing peak abundances and impacts of photo-z errors

    astro-ph.CO 2019-08 conditional novelty 6.0 of 10

    For an LSST-like survey, four-bin tomographic weak lensing peak counts shrink the Omega_m-sigma_8 error contour by about a factor of five relative to 2D peak counts, and can simultaneously constrain photo-z bias to 10...

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