Ly emitters in the GOODS-S field - A powerful pure nebular SED with N IV] emission at z = 5.563

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Table 3:

Fiducial model emission line spectrum.
$\lambda_{\rm rest}$	$\log$ (L [erg s^-1])	$I/I_{\mbox{H$\beta$ }}$
O VI 1035	40.984	0.007
Si III 1207	41.589	0.026
Ly $\alpha$ 1215	44.724	36.011
N V 1240	42.229	0.115
Si IV 1397	42.564	0.249
O IV 1402	42.416	0.177
N IV] 1486	42.938	0.590
C IV 1549	44.054	7.698
He II 1640	43.026	0.7217
C III] 1909	42.985	0.657
[O II] 3727	41.411	0.018
He II 4686	42.127	0.0911
[O III] 5007	43.936	5.865
H $\alpha$ 6563	43.625	2.867

Notes. Note that no resonance line absorption is accounted for in these values. For the doublets, including [O III] 4959, 5007 Å, the number represents the sum of the two lines.

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