A new model to predict weak-lensing peak counts - III. Filtering technique comparisons

Chieh-An Lin; Martin Kilbinger; Sandrine Pires

doi:10.1051/0004-6361/201628565

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Volume 593 (September 2016)

A&A, 593 (2016) A88

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Fig. 9

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ABC constraints on Ω_m, σ₈, and using starlet. The distance D₂ is used for this run. On each panel, the ABC posterior is marginalized over one of the three parameters. Black stars are the input cosmology.

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