Comparison of the constraints on $S_8={\sigma }_8\times \sqrt{{\mathrm{\Omega }}_{\mathrm{m}}/0.3}$ with literature results from SPT-SZ (Bocquet et al. 2019), from SPT-SZ, SPTpol ECS, and SPTpol 500d cluster counts (Bocquet et al. 2024), from XXL cluster number counts and clustering (Garrel et al. 2022), from Planck CMB 2020 (Planck Collaboration VI 2020), from WMAP CMB (Hinshaw et al. 2013), from ACT lensing (Qu et al. 2024), from ACT lensing (Madhavacheril et al. 2024), from Planck lensing (Planck Collaboration VIII 2020), from DES 3x2 correlation function (Dark Energy Survey Collaboration 2022), from HSC 3x2 correlation function (Sugiyama et al. 2023), from DES cosmic shear (Amon et al. 2022; Secco et al. 2022), from HSC cosmic shear (Li et al. 2023), from KiDS cosmic shear (van den Busch et al. 2022), from joint DES and KiDS cosmic shear (Dark Energy Survey and Kilo-Degree Survey Collaboration 2023), from SDSS BAO and RSD (Alam et al. 2021). All the errors shown are at the 1σ level. The vertical line and grey shaded areas represent our measurement’s location and 1–2σ confidence level.