The impact of baryons on the sparsity of simulated galaxy clusters from THE THREE HUNDRED Project - Astrophysical and cosmological implications

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Table 7.

Linear regression coefficients of the HE bias model.

	$b_{200, 500}^{HE}$ $b^{\mathrm{HE}}_{200,500}$	$b_{200, 2500}^{HE}$ $b^{\mathrm{HE}}_{200,2500}$	$b_{500, 2500}^{HE}$ $b^{\mathrm{HE}}_{500,2500}$
b₀^X	0.00 ± 0.28	0.17 ± 0.58	0.14 ± 0.43
b₁^X	−0.04 ± 0.40	−0.11 ± 0.79	0.01 ± 0.63

b₀^SZ	−0.08 ± 0.16	0.14 ± 0.58	0.21 ± 0.46
b₁^SZ	−0.05 ± 0.28	−0.12 ± 0.77	−0.08 ± 0.61

Notes. The different rows show the average and 1σ uncertainties of the intercept and slope of the linear HE bias model obtained from the X-ray and SZ calibration sample for different sparsity configurations (columns left to right).

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