Fig. 2.
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Comparison of MCMC runs with ‘true’ Cℓ’s and RF Cℓ’s for cosmological and scaling relation parameters. In grey, both Cℓ’s and the non-Gaussian contribution (σTℓℓ′) are computed as detailed in Sect. 2.1. In blue, σTℓℓ′ is approximated by a constant value over ℓ and cosmology. In orange, the Cℓ’s are computed with the RF and the sample variance noise is approximated by a constant.
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