Table 2: Rest-frame optical emission line widths.
Line id NEP 1239 NEP 1640 NEP 2131

km s^-1 km s^-1 km s^-1

[NeV] 819

[OII] 801

[NIII] 460

H $\gamma$ 633

H $\beta$ 453 270

[OIII $]\lambda$ 4958 458 480 741

[OIII $]\lambda$ 5007 457 623 707

[NeI] 608

H $\alpha$ 726

**Table 2:** Rest-frame optical emission line widths.
Line id	NEP 1239	NEP 1640	NEP 2131
	km s^-1	km s^-1	km s^-1
[NeV]			819
[OII]			801
[NIII]			460
H $\gamma$			633
H $\beta$	453	270
[OIII $]\lambda$ 4958	458	480	741
[OIII $]\lambda$ 5007	457	623	707
[NeI]		608
H $\alpha$			726

Source LaTeX | All tables | In the text

	1 Introduction
	2 The NEP sample of QSO 2 candidates
	3 Observations and data analysis
	4 Discussion and conclusions
	References