Fig. 13.
Measurement forecasts on cosmological parameters from an LSST Y10-like survey, obtained with different estimates for the covariance matrix, and for different input cosmology. Curves show the 95.4% confidence intervals. Measurement are shown relative to the input value (hence the “Δ” in the axis labels) in order to align the different cosmologies to the origin and highlight the change in size of the error contours caused by variations in cosmology.
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