Characterising galaxy clusters’ completeness function in Planck with hydrodynamical simulations

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Table 2.

Constraints on cosmological parameters obtained from the analysis of Planck PSZ2 cluster number counts and BAO, using three different completeness functions, as described in the text.

	Simulation	ERF	PACT
	completeness	completeness	completeness
H₀	$68 . 4_{- 2.4}^{+ 2.0}$ $68.4^{+2.0}_{-2.4}$	$69 . 1_{- 2.4}^{+ 2.1}$ $69.1^{+2.1}_{-2.4}$	$70 . 3_{- 2.5}^{+ 2.2}$ $70.3^{+2.2}_{-2.5}$
Ω_m	$0 . 301_{- 0.023}^{+ 0.019}$ $0.301^{+0.019}_{-0.023}$	$0 . 314_{- 0.024}^{+ 0.020}$ $0.314^{+0.020}_{-0.024}$	0.337 ± 0.024
σ₈	$0 . 742_{- 0.033}^{+ 0.025}$ $0.742^{+0.025}_{-0.033}$	$0 . 770_{- 0.036}^{+ 0.027}$ $0.770^{+0.027}_{-0.036}$	$0 . 823_{- 0.039}^{+ 0.030}$ $0.823^{+0.030}_{-0.039}$

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