Fig. 2.
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Top panel shows the angular power spectra Cℓgg, Cℓκg, and Cℓκκ (solid lines) for the baseline sample. The cosmological-only contribution is shown as dashed lines, while the noise contribution is shown as dotted lines. Bottom panel shows the signal-to-noise ratio, defined as the ratio of the cosmological-only term to the noise, for Cℓgg and Cℓκκ.
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