Comparison of peak abundance histograms between Camelus (red circles) and MICE (blue line) for 4650 deg2. Error bars for Camelus represent the standard deviation of 500 realizations for the associated S/N bin. There is good agreement between the mock observations and the Camelus predictions across all wavelet filtering scales, especially for ν lower than ~5. The shaded regions represent bins where the relative different between MICE and Camelus is larger than 50%. We apply a conservative cut and omit these higher-bias bins in our analysis.
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