Table 1. Open in new tab The assumed... | Oxford Academic

Table 1.

Open in new tab

The assumed ranges and distributions of the model parameters in equation (19). For more details the readers are referred to Section 3.1 or Allen et al. (2008).

Param	Physical effect described	Mean ± stddev	Prior
K	Overall calibration	1.000 ± 0.100	Gaussian
γ	Non-thermal pressure	1.050 ± 0.050	Uniform
b₀	Gas bias: normalization	0.825 ± 0.175	Uniform
α_b	Gas bias: evolution	0.000 ± 0.100	Uniform
s₀	Stellar fraction: normalization	0.160 ± 0.048	Gaussian
α_s	Stellar fraction: evolution	0.000 ± 0.200	Uniform

Param	Physical effect described	Mean ± stddev	Prior
K	Overall calibration	1.000 ± 0.100	Gaussian
γ	Non-thermal pressure	1.050 ± 0.050	Uniform
b₀	Gas bias: normalization	0.825 ± 0.175	Uniform
α_b	Gas bias: evolution	0.000 ± 0.100	Uniform
s₀	Stellar fraction: normalization	0.160 ± 0.048	Gaussian
α_s	Stellar fraction: evolution	0.000 ± 0.200	Uniform

Table 1.

Open in new tab

The assumed ranges and distributions of the model parameters in equation (19). For more details the readers are referred to Section 3.1 or Allen et al. (2008).

Param	Physical effect described	Mean ± stddev	Prior
K	Overall calibration	1.000 ± 0.100	Gaussian
γ	Non-thermal pressure	1.050 ± 0.050	Uniform
b₀	Gas bias: normalization	0.825 ± 0.175	Uniform
α_b	Gas bias: evolution	0.000 ± 0.100	Uniform
s₀	Stellar fraction: normalization	0.160 ± 0.048	Gaussian
α_s	Stellar fraction: evolution	0.000 ± 0.200	Uniform

Param	Physical effect described	Mean ± stddev	Prior
K	Overall calibration	1.000 ± 0.100	Gaussian
γ	Non-thermal pressure	1.050 ± 0.050	Uniform
b₀	Gas bias: normalization	0.825 ± 0.175	Uniform
α_b	Gas bias: evolution	0.000 ± 0.100	Uniform
s₀	Stellar fraction: normalization	0.160 ± 0.048	Gaussian
α_s	Stellar fraction: evolution	0.000 ± 0.200	Uniform