Cosmological parameters for the set of end-to-end simulations cases discussed in Sect. 3.12.2. In all cases the input for the simulations is the same input CMB (and in some cases foreground) map(s). Error bars correspond to the uncertainty for a single realization (including noise variance, even in cases where the simulations contains no noise). The horizontal lines corresponds to the best-fit values of the refTT case.
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