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Recent data from the WMAP, ACT and SPT experiments provide precise measurements of the cosmic microwave background temperature power spectrum over a wide range of angular scales.
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Here we use a slightly adapted binning of the spectra compared to those used in Dunkley:2013vu and Sievers:2013wk ; this is preferable as it gives the two ACT regions more similar bandpower window functions. Using the new binning alters cosmological parameters by ≲ 0.1 σ \lesssim 0.1\sigma . The lensing amplitude reduces of about 0.2 σ 0.2\sigma
Cited in the paper.
In the secondary model there are 6 common parameters: two for the thermal and kinematic SZ effects, three for the CIB clustered and Poisson power, and a cross-correlation between tSZ and clustered CIB power. There is a separate Poisson radio power each for ACT and SPT; two Galactic parameters for ACT; and four calibration parameters for ACT, as described in Dunkley:2013vu
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