Galaxy cluster mass bias from projected mass maps - THE THREE HUNDRED-NIKA2 LPSZ twin samples

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Table C.2.

Mean bias and variance due to projection effect for the 4 clusters studied with 100 maps.

Density model	Snapshot	z	Cluster	< b^κ>		< b^κ>		< b^κ>
				100 random	100 random	3 main	3 main	3 inertia	3 inertia
NFW

	101	0.817	0306	0.1155	0.0229	0.1490	0.0219	0.1314	0.0426
	104	0.700	0206	0.1233	0.0453	0.2036	0.0151	0.0671	0.1442
	107	0.592	0046	-0.0450	0.0212	-0.0317	0.0176	-0.0344	0.0350
	110	0.490	0198	0.0484	0.0355	0.0231	0.0495	0.1161	0.0281

Einasto

	101	0.817	0306	0.1047	0.0359	0.1712	0.0266	0.1259	0.0613
	104	0.700	0206	0.1312	0.0500	0.2162	0.0158	0.0735	0.1527
	107	0.592	0046	-0.0618	0.0212	-0.0545	0.0184	-0.0447	0.0301
	110	0.490	0198	0.0716	0.0387	0.0771	0.0378	0.1393	0.0373

Notes. The three main projections are the so-called 0, 1, and 2 or x, y, and z projections. The 3 intertia projections are: 0_pr_axes, 1_pr_axes, and 2_pr_axes.

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