Comparison of Ω_m − σ₈ posteriors obtained by different surveys. Top panel: 2500 deg² SPT-SZ cluster survey (Bocquet et al. 2019, blue contours), eROSITA (eFEDS) cluster survey (Chiu et al. 2023, yellow contours), DES-Y3 NC+3x2pt (Dark Energy Survey Collaboration 2022, green contours), and Planck TT,TE,EE+lowE with free m_ν (Planck Collaboration VI 2020, black countours), compared to our results in the NC+M_WL+CL (red contours) analyses. Bottom panel: DES-Y1 number counts and weak-lensing mass estimates (Dark Energy Survey Collaboration 2020, cyan contours), DES-Y1 cluster count data and SPT-SZ follow-up data (Costanzi 2021, orange contours), and DES-Y1 NC+4x2pt (To et al. 2021a, dark green contours), compared to our results from the NC+M_WL (dotted gray contours) and NC+M_WL+CL (red contours) results.