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 8:

H $\beta$ Line centroids at different fractional heights of spectral types.
Source	c(0/4)^a	$\Delta^{{a,b}}$	c(1/4)^a	$\Delta^{{a,b}}$	c(1/2)^a	$\Delta^{{a,b}}$	c(3/4)^a	$\Delta^{{a,b}}$	c(0.9)^a	$\Delta^{{a,b}}$
(1)	(2)	(3)	(4)	(5)	(6)	(7)	(8)	(9)	(10)	(11)
A1	0	6900	0	300	-30	130	-30	100	-30	60
A2	-100	8200	-200	300	-170	150	-170	110	-170	70
B1	2400	3000	2100	700	130	280	-130	150	-170	100
B2	2200	2600	1700	600	380	230	170	150	130	100
A	-100	7400	-100	300	-70	130	-70	100	-70	60
M	0	8700	0	400	-40	160	-40	120	-40	70
BM	2400	2900	2200	700	270	330	-60	160	-120	100
43A	100	3900	100	200	90	70	90	50	90	30
44A	200	4100	100	200	130	70	130	60	130	40
45A	0	5400	0	200	30	100	30	80	30	50
46A	100	6200	100	300	120	110	120	90	110	50
47A	0	7900	0	300	-20	140	-20	110	-20	70
48A	-100	8100	-200	300	-170	150	-170	110	-170	70
43B	2100	3200	200	300	40	150	0	140	-10	100
44B	1200	3300	200	500	10	170	-30	150	-40	100
45B	1700	3200	1200	800	140	210	40	160	20	100
46B	2400	3000	1600	700	370	230	190	170	150	110
47B	2100	3200	2000	800	220	260	30	160	0	100
48B	3100	2300	2700	400	1550	440	-20	240	-230	120

^a In units of km s^-1. ^b 2 $\sigma$ confidence level uncertainty.

Source LaTeX | All tables | In the text

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