Integral field spectroscopy of two radio galaxies at z 2.3 | A&A

EDP Sciences Journals List

Subscriber Authentication Point

Home

Free access article

Table 3:

Line ratios for the total emission and the perturbed and quiescent components with it was possible to decouple them.
Object	Dataset	Ly $\alpha$ /HeII	Ly $\alpha$ /CIV	Ly $\alpha$ /NV	NV/HeII	CIV/HeII	CIV/CIII]	CIII]/HeII
4C 40.36	V300	12.73 $\pm$ 0.23	6.97 $\pm$ 0.07	18.71 $\pm$ 0.48	0.68 $\pm$ 0.03	1.83 $\pm$ 0.05	1.90 $\pm$ 0.05	0.96 $\pm$ 0.03
	V600		6.57 $\pm$ 0.13	23.26 $\pm$ 1.45
	V01^*	14.7	8.4	39.2	0.37	1.8	1.8	1.0
	H05^**	11.6	7.1	19.3	0.6	1.6	2.2	0.7
4C48.48	V300	9.57 $\pm$ 0.13	9.04 $\pm$ 0.12	>17.9	<0.38	1.06 $\pm$ 0.03	1.05 $\pm$ 0.03	1.01 $\pm$ 0.03
Broader			9.07 $\pm$ 0.15
Narrower			11.36 $\pm$ 0.75
4C48.48	V600		11.21 $\pm$ 0.21	>65.2
Broader			8.33 $\pm$ 0.24
Narrower			16.59 $\pm$ 0.88
	V01^*	13.2	12.6	48.3	0.27	1.0	1.7	0.6
	H07^**	11.3	8.2	12.6	0.9	1.4	2.6	0.5

^* Vernet et al. (2001); ^** Humphrey (2005).

Source LaTeX | All tables | In the text