VLT/ISAAC spectra of the Hβ region in intermediate-redshift quasars - III. Hβ broad-line profile analysis and inferences about BLR structure

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Table 4:

H $\beta$ Line profile measurements.
Source	FWZI^a	$\Delta^{{a,b}}$	FWHM^a	$\Delta^{{a,b}}$	A.I.^c	$\Delta^{{b}}$	Kurt.^d	$\Delta^{{b}}$
(1)	(2)	(3)	(4)	(5)	(6)	(7)	(8)	(9)
HE 0035-2853	23 300	3600	7400	500	0.19	0.07	0.37	0.04
HE 0043-2300	25 000	4500	4600	300	-0.03	0.10	0.33	0.06
HE 0058-3231	25 200	4400	5800	500	0.22	0.08	0.30	0.04
HE 0105-3006	20 700	5000	5200	400	0.10	0.17	0.28	0.08
HE 0109-3518	24 400	5900	4000	300	-0.01	0.10	0.33	0.06
HE 0119-3325	25 300	6800	4500	300	0.03	0.09	0.41	0.06
HE 0142-4619	26 900	4200	3600	300	0.24	0.17	0.26	0.08
HE 0203-4627	27 800	5100	7200	500	0.12	0.09	0.32	0.05
HE 0205-3756	20 700	4400	4400	400	0.41	0.06	0.16	0.03
HE 0224-3826	20 800	2900	6500	400	0.10	0.07	0.40	0.05
HE 0229-5603	26 500	6300	4000	300	0.03	0.10	0.31	0.06
HE 0239-4809	19 700	3900	4700	400	0.19	0.14	0.27	0.06
HE 0248-3628	22 200	4400	3900	300	-0.19	0.10	0.30	0.05
HE 0251-5550	25 700	4400	4500	400	0.47	0.07	0.19	0.03
HE 0349-5249	26 500	4000	5900	800	0.37	0.07	0.27	0.04
HE 0359-3959	18 500	4800	4300	400	-0.15	0.09	0.30	0.05
HE 0435-4312	25 300	6100	5500	300	0.08	0.14	0.38	0.08
HE 0436-3709	26 700	4300	6600	500	0.26	0.09	0.32	0.05
HE 0940-1050	15 400	1400	3500	200	0.53	0.04	0.22	0.02
HE 1039-0724	22 900	3300	11 300	500	0.63	0.04	0.48	0.03
HE 1120+0154	25 800	4300	6900	500	0.33	0.07	0.35	0.04
HE 1347-2457	24 700	3600	6800	500	0.20	0.09	0.31	0.05
HE 1348+0118	23 600	4400	3700	200	0.08	0.15	0.38	0.08
HE 1349+0007	23 400	3500	6200	400	0.27	0.10	0.34	0.06
HE 1409+0101	21 600	4600	8300	900	0.48	0.07	0.28	0.03
HE 1430-0041	19 100	3600	4700	300	-0.05	0.10	0.33	0.06
HE 1505+0212	18 400	2300	5200	200	-0.02	0.25	0.37	0.11
HE 2147-3212	25 900	3900	5800	400	0.01	0.10	0.33	0.05
HE 2156-4020	26 200	4400	5000	500	0.27	0.10	0.26	0.05
HE 2335-3029	18 100	4000	3100	200	0.04	0.11	0.38	0.07

^a In units of km s^-1; ^b 2 $\sigma$ confidence level uncertainty; ^c asymmetry index defined as in Marziani et al. (1996); ^d Kurtosis parameter as in Marziani et al. (1996).

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