The host galaxies of radio-loud quasars at z > 5 with ALMA

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Table 6.

Mean, median and standard deviation of the [C II] emission line properties shown in Fig. 7, for the RQ and RL high−z quasars samples.

	RQ quasars			RL quasars ^(⋆)			KS-test
	Mean	Median	st.dev	Mean	Median	st.dev	p-value
FWHM_[CII] [km s⁻¹]	387	379	133	272	290	110	0.14
EW_[CII] [km s⁻¹]	2362	1691	2013	1848	1180	1441	0.24
L_[CII] [10⁹ L_⊙]	2.9	1.8	2.6	1.5	0.8	1.2	0.04
SFR_[CII] [M_⊙ yr⁻¹]	466	258	498	211	95	194	0.04

Notes. We also report the p-values obtained with a Kolmogorov-Smirnov test, to assess if the observed quantities for RQ and RL quasars were obtained from the same underlying distribution.

^(⋆)

We only consider sources with [C II] emission lines detection, i.e., we excluded PSO172+18 from this comparison.

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