The cosmological analysis of X-ray cluster surveys - IV. Testing ASpiX with template-based cosmological simulations

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Volume 614 (June 2018)

A&A, 614 (2018) A72

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This article has an erratum: [https://doi.org/10.1051/0004-6361/201731445e]

Table 8

Cosmological analysis performed on the Aardvark C1 CLEAN samples corresponding to the 39 × 18.22 deg² sub-maps (effective area).

ID	Parameter		Ω_m	σ₈	x_c,0	w₀

S5	cat x 39	CR-HR₁-r_c-z
	< p_best−10> Amoeba		0.222 ± 0.046	0.857 ± 0.080	0.240 ± 0.024	–1.023 ± 0.209
S6	cat x 39	CR-HR₁-HR₂-r_c
	< p_best10 > Amoeba		0.222 ± 0.055	0.855 ± 0.075	0.246 ± 0.041	–1.103 ± 0.506

	Fisher	CR-HR₁-r_c-z	0.23 ± 0.031	0.83 ± 0.060	0.24 ± 0.021	–1.00 ± 0.175
	analysis	CR-HR₁-HR₂-r_c	0.23 ± 0.050	0.83 ± 0.063	0.24 ± 0.051	–1.00 ± 0.705

Notes.Two XOD are considered: CR-HR₁-r_c-z and CR-HR₁-HR₂-r_c. The displayed statistics are the average of the best-10 values obtained for each of the 39 small fields and associated standard deviation. The last two rows give the predictions from the FA.

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