Exploring the links between quasar winds and radio emission along the main sequence at high redshift

Open Access

Table 14.

Least-squares linear relations (y = a + b * x) between different outflow properties and the bolometric luminosity.

y	x	Sources	a ± δa	b ± δb	RMSE	CC	ρ-value
(1)	(2)	(3)	(4)	(5)	(6)	(7)	(8)
[O III]λ5007

$log {\dot{E}}_{kin, 44}$ $\log \dot{E}_{\mathrm{kin,44}}$	log L_bol, 44	45	−4.09±0.44	0.86±0.14	0.009	0.69	1.7×10⁻⁶
$log {\dot{M}}_{out} v_{o, 34}$ $\log \dot{M}_{\mathrm{out}}v_{\mathrm{o,34}}$	log L_bol, 44	45	−1.62±0.31	0.79±0.09	0.017	0.78	2.7×10⁻¹⁰

C IVλ1549

$log {\dot{E}}_{kin, 44}$ $\log \dot{E}_{\mathrm{kin,44}}$	log L_bol, 44	68	−3.59±0.25	1.24±0.08	0.075	0.87	2.1×10⁻²²
$log {\dot{M}}_{out} v_{o, 34}$ $\log \dot{M}_{\mathrm{out}}v_{\mathrm{o,34}}$	log L_bol, 44	68	−2.08±0.22	1.19±0.07	0.069	0.90	3.7×10⁻²⁵

Notes. (1), (2) Fitted parameters. (3) Number of sources. (4), (5) Linear correlation coefficients. (6) Root mean square error. (7), (8) Pearson r score and its associated null hypothesis probability value.

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.