The imprint of AGN-driven outflows on the Circumgalactic Medium: The case of Lyα nebulae around high-z quasars

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Table 4.

Statistical parameters for the Spearman rank correlation test on the scaling relations in Figs. 8 and 9.

Exc. source	${\dot{E}}_{kin}^{[OIII]}$ $Mathematical equation: $ \dot{E}_{\mathrm{kin}}^{\mathrm{[OIII]}} $$ –D_Lyα		${\dot{E}}_{kin}^{[OIII]}$ $Mathematical equation: $ \dot{E}_{\mathrm{kin}}^{\mathrm{[OIII]}} $$ –L_Lyα

	ρ	p-value	ρ	p-value
None	0.60	0.21	−0.08	0.87
Q0050+0051	0.60	0.28	−0.09	0.87
Q0052+0140	0.89	0.03	0.60	0.28
Q2121+0052	0.60	0.28	−0.09	0.87
Q2123-0050	0.60	0.28	−0.39	0.50
SDSSJ2319-1040	0.39	0.50	−0.39	0.50
SDSSJ1427-0029	0.39	0.50	−0.09	0.87

Notes. From left to right, the columns report the source excluded in each run of the test and the test results for the scaling relation between outflow kinetic power and Lyα nebula size and luminosity.

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