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Table 1.

Summary statistics accounting for the mass distribution of our group and cluster sample.

⟨X⟩ Xmin X2.5% X16% X50% X84% X97.5% Xmax
log 10 ( M 200 m DM / M ⊙ ) $ \log_{10} (M_{200m}^{\mathrm{DM}}/M_\odot) $ 13.48 13.02 13.07 13.15 13.42 13.81 14.30 14.74
log 10 ( M 200 m gas / M ⊙ ) $ \log_{10} (M_{200m}^{\mathrm{gas}}/M_\odot) $ 12.65 12.06 12.20 12.31 12.58 12.99 13.49 13.95
log 10 ( M 200 m tot / M ⊙ ) $ \log_{10} (M_{200m}^{\mathrm{tot}}/M_\odot) $ 13.54 13.08 13.13 13.20 13.48 13.87 14.36 14.81
f gas 200 m $ f_{\mathrm{gas}}^{200m} $ 0.128 0.091 0.107 0.119 0.129 0.137 0.147 0.162
log 10 ( M 200 m hot gas / M ⊙ ) $ \log_{10} (M_{200m}^{\mathrm{hot\;gas}}/M_\odot) $ 12.59 11.97 12.06 12.23 12.53 12.96 13.45 13.93
f hot gas 200 m $ f_{\mathrm{hot\;gas}}^{200m} $ 0.112 0.066 0.078 0.093 0.113 0.130 0.141 0.162
f hot gas 200 m / f gas 200 m $ f_{\mathrm{hot\;gas}}^{200m}/f_{\mathrm{gas}}^{200m} $ 0.875 0.521 0.620 0.742 0.899 0.995 1.000 1.000

Notes. Each row in the first block corresponds to a different quantity, namely the DM, gas, and total masses within R200m (in logarithmic scale), and the baryon fraction within the same aperture. The second block contains the information relative to the hot gas (defined with a temperature threshold of Tthr = 106 K, similar to e.g. Rasia et al. 2025). Shown from left to right are the arithmetic mean ⟨X⟩, minimum Xmin, several percentiles Xp%, and maximum Xmax of each quantity X.

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