Fig. 17
NILC–MILCA F/L cross-power spectrum after foreground subtraction (red points), compared to the Atacama Cosmology Telescope (ACT; cyan dot) and the South Pole Telescope (SPT; orange, George et al. 2015) power spectrum estimates. The black line shows the tSZ power spectrum template (EM12, Efstathiou & Migliaccio 2012) used in the Planck CMB cosmological analysis (Planck Collaboration XVI 2014; Planck Collaboration XI 2016) with its best fit amplitude AtSZ (Planck Collaboration XI 2016). The grey region allows comparison with the ±2σ interval.
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