Fig. 7.
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Constraints on parameters from the WL optimistic setting with baryons. We show the case where e-Mantis is used to create both the data and fitting and the case where FORGE is used to create the data and it is fitted by e-Mantis. We also include the case where we impose a Gaussian prior on log10 Mc with the width of 0.2 in the case of FORGE fiducial data. Left panel: Constraints on baryonic parameters. Right panel: Constraints on cosmological parameters.
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