Investigating the origin of radio emission in candidate super-Eddington accreting black holes

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Table C.1.

Analysis of the Hβ and Fe IIλ4570 emission features

		Hβ full broad profile (BC + BLUE)									Fe IIλ4570	Hβ BC		Hβ BLUE

Object	f_λ, 5100	Flux	EW	FWHM	c( $\frac{1}{4}$ $Mathematical equation: $ \frac{1}{4} $$ )	c( $\frac{1}{2}$ $Mathematical equation: $ \frac{1}{2} $$ )	c( $\frac{3}{4}$ $Mathematical equation: $ \frac{3}{4} $$ )	c( $\frac{9}{10}$ $Mathematical equation: $ \frac{9}{10} $$ )	AI	KI	R_FeII	F/F(Hβ)	FWHM	F/F(Hβ)	FWHM	Shift	Skew
(1)	(2)	(3)	(4)	(5)	(6)	(7)	(8)	(9)	(10)	(11)	(12)	(13)	(14)	(15)	(16)	(17)	(18)
J00418+4021	3.59E-16	7.7E-15	23.2	1247	87	96	103	90	-0.002	0.336	1.32	0.8344	1257	0.166	3412	-2928	0.594
J00457+0410	7.03E-16	4.6E-14	67.6	4405	-668	-452	-162	-53	-0.175	0.355	1.18	0.6664	3413	0.334	5099	-1332	0.898
J00535+1241	5.77E-15	2.3E-13	41.0	1412	-83	-61	-60	-59	-0.019	0.327	1.83	0.9354	1408	0.065	1629	-2676	1.010
J10255+5140	1.44E-15	9.1E-14	60.1	1480	48	41	41	41	0.006	0.339	0.78	0.9970	1463	0.003	3634	-533	0.605
J11292-0424	1.56E-15	1.7E-13	115.9	2455	-55	-76	-53	-60	0.002	0.333	0.95	1.0000	2454	0.000	...	...	...
J11420+6030	2.75E-16	1.0E-14	41.7	1542	-625	-73	-78	-75	-0.293	0.243	2.12	0.9290	1522	0.071	4370	-2934	1.013
J12075+1506	1.20E-15	4.7E-14	66.4	2253	-11	98	112	95	-0.051	0.313	1.08	0.9515	2238	0.049	3775	-2598	0.393
J12091+5611	1.11E-16	2.7E-15	22.9	1186	-319	-265	-258	-266	-0.050	0.314	2.09	0.8363	1141	0.164	5069	-2095	1.010
J12366+5630	1.43E-16	3.5E-15	25.8	1973	-529	-289	-227	-201	-0.213	0.288	2.10	0.7662	1753	0.234	6200	-1158	0.392
J12562+5652	1.12E-14	4.3E-13	34.7	4480	-545	-321	-14	72	-0.165	0.316	1.93	0.8460	3599	0.154	3947	-2393	1.010
J13012+5902	1.91E-14	7.1E-13	56.8	3313	-601	-370	-89	-6	-0.215	0.319	1.37	0.7323	2523	0.268	3712	-1551	1.000
J14052+2555	2.26E-14	2.3E-12	105.7	2054	-94	-94	-94	-94	0.000	0.333	1.02	1.0000	2053	0.000	...	...	...
J14063+2223	5.80E-15	4.1E-13	58.9	1633	-132	-43	-24	-19	-0.077	0.301	1.10	0.9053	1528	0.095	3522	-1800	1.000
J14170+4456	1.02E-14	6.1E-13	66.0	2270	-448	-174	-59	3	-0.220	0.314	1.17	0.7320	1929	0.268	4098	-721	0.586
J14258+3946	1.07E-16	5.5E-15	49.4	1977	-148	13	2	-4	-0.093	0.368	1.10	1.0000	1975	0.000	...	...	...
J14475+3455	1.77E-15	3.7E-14	26.9	3862	-953	-863	-168	-122	-0.291	0.260	1.97	0.9981	2298	0.002	2572	-2957	0.459
J15455+4846	4.87E-16	3.5E-14	73.4	1794	-77	10	27	10	-0.052	0.310	1.06	0.8097	1723	0.190	6858	-3164	1.051
J17014+5149	2.62E-15	1.3E-13	46.9	2582	-329	-78	-71	-69	-0.105	0.296	1.19	0.9436	2528	0.056	4497	-2564	0.335

Notes. All measured quantities refer to rest-frame. Col. 1: Object coordinate name. Col. 2: specific flux at 5100 Å in units of erg s⁻¹ cm⁻² Å⁻¹. Cols. 3: flux in units of erg s⁻¹ cm⁻². Col. 4: equivalent width in Å. Cols. 5: FWHM of the Hβ full broad profile in km s⁻¹; Cols. 6-9: profile centroids at fractional peak intensity in km s⁻¹. Col. 10: asymmetry index; Col. 11: kurtosis index. See Zamfir et al. (2010) for definition. Col. 12: ratio R_FeII, see text for definition. Col. 13: fractional intensity of the Hβ BC; Col. 14: FWHM Hβ BC in km s⁻¹; Col. 15: fractional intensity of the blueshifted broad component BLUE; Col. 16: FWHM in km s⁻¹; Col. 17: peak shift (mode) of BLUE in km s⁻¹. Col. 18: skew of BLUE.

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