Constraining cosmology with a new all-sky Compton parameter map from the Planck PR4 data

Abstract

ABSTRACT We constructed a new all-sky Compton parameter map (y-map) of the thermal Sunyaev-Zel’dovich (tSZ) effect from the 100–857 GHz frequency channel maps delivered within the Planck data release 4. The improvements in terms of noise and systematic effects translated into a y-map with a noise level smaller by ∼7 per cent compared to the maps released in 2015, and with significantly reduced survey stripes. The produced 2020 y-map is also characterized by residual foreground contamination, mainly due to thermal dust emission at large angular scales and to cosmic infrared background and extragalactic point sources at small angular scales. Using the new Planck data, we computed the tSZ angular power spectrum and found that the tSZ signal dominates the y-map in the multipole range, 60 < ℓ < 600. We performed the cosmological analysis with the tSZ angular power spectrum and found $S_8 = 0.764 \, _{-0.018}^{+0.015} \, (stat) \, _{-0.016}^{+0.031} \, (sys)$, including systematic uncertainties from a hydrostatic mass bias and pressure profile model. The S8 value may differ by ±0.016 depending on the hydrostatic mass bias model and by +0.021 depending on the pressure profile model used for the analysis. The obtained value is fully consistent with recent Kilo-Degree Survey and Dark Energy Survey weak-lensing observations. While our result is slightly lower than the Planck CMB one, it is consistent with the latter within 2σ.