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Fig. 12.

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Forecast constraints with future experiments. Red: Forecast constraints when the first stellar mass bin from a CMASS survey is cross correlated with full overlap with the future SO CMB experiment, using the noise curves provided by the SO collaboration. Blue: Same, but using the galaxy shot noise and sky coverage of a DESI-like experiment with full overlap with SO (see text for details). The dashed lines show the fiducial parameter values we used for the forecast.

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