Euclid Preparation. XXVIII. Forecasts for ten different higher-order weak lensing statistics
Collaboration
33 pages
Published in:
- Astron.Astrophys. 675 (2023) A120
- Published: Jul, 2023
e-Print:
- 2301.12890 [astro-ph.CO]
DOI:
- 10.1051/0004-6361/202346017 (publication)
Experiments:
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Abstract: (arXiv)
Recent cosmic shear studies have shown that higher-order statistics (HOS) developed by independent teams now outperform standard two-point estimators in terms of statistical precision thanks to their sensitivity to the non-Gaussian features of large-scale structure. The aim of the Higher-Order Weak Lensing Statistics (HOWLS) project is to assess, compare, and combine the constraining power of ten different HOS on a common set of -like mocks, derived from N-body simulations. In this first paper of the HOWLS series, we computed the nontomographic (, ) Fisher information for the one-point probability distribution function, peak counts, Minkowski functionals, Betti numbers, persistent homology Betti numbers and heatmap, and scattering transform coefficients, and we compare them to the shear and convergence two-point correlation functions in the absence of any systematic bias. We also include forecasts for three implementations of higher-order moments, but these cannot be robustly interpreted as the Gaussian likelihood assumption breaks down for these statistics. Taken individually, we find that each HOS outperforms the two-point statistics by a factor of around two in the precision of the forecasts with some variations across statistics and cosmological parameters. When combining all the HOS, this increases to a times improvement, highlighting the immense potential of HOS for cosmic shear cosmological analyses with . The data used in this analysis are publicly released with the paper.Note:
- 33 pages, 24 figures, main results in Fig. 19 & Table 5, version published in A&A
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