Fig. 7.

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Percentage fraction in total marginal posterior error of fδ, mn due to uncertainties in the lensing kernel and IA parameter. Shown is the statistical error relative to the full marginal error (RMS variance of posterior) as a function of k in three redshift bins without marginalisation (solid lines), with marginalisation over errors in the source redshift distributions only (dashed lines), Ωm in the lensing kernel only (dash-dotted lines), and for the AIA error only (dotted lines).
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