Integral field spectroscopy of two radio galaxies at z 2.3

Free Access

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

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.