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Home All issues Volume 679 (November 2023) A&A, 679 (2023) A61 Full HTML
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Fig. 3.

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Validation of DLL simulations against high-resolution κTNG-Dark simulations before and after using the HPN correction model. Upper panel: angular power spectra. Lower panel: fractional angular power spectra. The power spectra and ratios are means over 100 independent map realizations and the shaded regions represent the standard deviation from 100 DLL realizations. The spectra are computed for the source redshift zs = 0.91.

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