Table A.2:

The local sample: Seyfert 1.8 to 2.0 and narrow line radio galaxies (NLRGs).

Name	Type	z	log	f2-10			A
(1)	(2)	(3)	(4)	(5)	(6)	(7)	(8)	(9)
NGC 1068	2.0	0.0038	25.00	-11.34	1	-11.94	M	1
NGC 1275	NLRG	0.0175	20.00	-10.91	2a	-12.70	L	2
NGC 1320	2.0	0.0089	24.00	-12.24	3	-13.15	S	3
NGC 1667	2.0	0.0152	24.00	-13.00	4	-14.00	L	4
NGC 2992	1.9	0.0077	21.95	-10.13	5	-14.52	S	5
NGC 3081	2.0	0.0079	23.85	-11.89	6	-12.66	L	6
NGC 3281	2.0	0.0106	24.18	-11.54	7	-14.52	S	5
NGC 3393	2.0	0.0125	25.00	-12.68	8	-13.25	L	4
NGC 4074	2.0	0.0224	23.38	-11.59	3	-14.05	S	7
NGC 4507	2.0	0.0118	23.63	-10.89	9	-13.26	L	6
NGC 5135	2.0	0.0136	24.00	-12.80	10	-13.54	L	4
NGC 5506	1.9	0.0062	22.50	-10.10	11	-13.96	M	8
NGC 5643	2.0	0.0040	23.80	-12.08	12	-13.33	M	8
NGC 5728	2.0	0.0093	24.30	-11.89	13	-13.66	L	4
NGC 7130	2.0	0.0161	24.00	-12.29	14	-14.00	S	9
NGC 7314	1.9	0.0048	22.02	-10.39	15	-14.30	M	8
NGC 7582	2.0	0.0052	24.00	-11.64	16	-12.48	M	10
NGC 7674	2.0	0.0289	25.00	-12.12	17	-13.40	L	11
Mrk 1	2.0	0.0159	24.00	-12.89	18	-13.49	L	11
Mrk 34	2.0	0.0505	24.00	-12.74	19	-13.55	L	11
Mrk 78	2.0	0.0371	23.76	-12.23	3	-13.85	L	11
Mrk 348	2.0	0.0150	23.13	-10.56	20	-13.64	L	11
Mrk 463E	2.0	0.0500	23.85	-12.39	21	-13.89	L	11
Mrk 477	2.0	0.0377	23.38	-11.92	22	-13.14	L	4
Mrk 573	2.0	0.0171	24.00	-12.92	23	-13.00	S	3
Mrk 609	1.8	0.0344	20.00	-11.83	24	-14.40	S	12
Mrk 612	2.0	0.0204	23.81	-12.44	18	-13.66	L	11
3C 33	NLRG	0.0597	23.59	-11.13	25	-14.70	M	1
MCG-5-23-16	2.0	0.0085	22.15	-10.10	26	-13.89	S	5
WAS 49b	2.0	0.0630	22.80	-12.20	20	-14.30	S	13
Cygnus A	NLRG	0.0560	23.23	-10.89	25	-14.40	M	14
IC 3639	2.0	0.0109	24.00	-13.10	18	-13.60	L	4
Tol 0109-383	2.0	0.0117	24.30	-11.80	27	-13.62	S	15

Notes. Column description: (1) Source name. (2) Spectroscopic classification (1.8, 1.9 and 2.0 refer to Seyfert types). (3) Redshift. (4) Logarithm of the cold X-ray absorbing column density. For those objects in which no cold absorption is measured in excess of the Galactic value, the column has been fixed to log  = 20. (5) Observed 2-10 keV flux in units of erg cm^-2 s^-1. (6) Reference for the X-ray data. (7) [Ne V]3426 flux in units of erg cm^-2 s^-1. (8) Aperture used to measure the [Ne V] flux, defined following Schmitt (1998): S (small), M (medium) and L (large) correspond to apertures in the ranges 1-3'', 3-7'', and >7'', respectively. (9) Reference for the [Ne V] data.
X-ray references: (1) Cappi et al. (2006); (2) Panessa et al. (2006); (3) this work; (4) Bianchi et al. (2005); (5) Gilli et al. (2000); (6) Bassani et al. (1999); (7) Vignali & Comastri (2002); (8) Maiolino et al. (1998); (9) Matt et al. (2004); (10) Guainazzi et al. (2005a); (11) Bianchi et al. (2003); (12) Guainazzi et al. (2004); (13) Comastri et al. (2010); (14) Risaliti et al. (1999); (15) Dewangan & Griffiths (2005); (16) Piconcelli et al. (2007a); (17) Malaguti et al. (1998); (18) Guainazzi et al. (2005b); (19) Greenhill et al. (2008); (20) Awaki et al. (2000); (21) Bianchi et al. (2008); (22) Levenson et al. (2001); (23) Shu et al. (2007); (24) Gallo et al. (2006); (25) Evans et al. (2006); (26) Balestra et al. (2004); (27) Iwasawa et al. (2001b)
^(a) The column density of NGC 1275, which is at the center within the Perseus cluster, is difficult to measure: Evans et al. (2006) do not find absorption in excess of the Galactic one based on Chandra data.
[Ne V] references: (1) Koski (1978); (2) Anderson (1970); (3) Erkens et al. 1997; (4) This work (based on the catalog of UV-optical spectra of nearby galaxies by Storchi-Bergmann et al., see text); (5) Durret & Bergeron (1988); (6) Durret & Bergeron (1986); (7) Shuder & Osterbrock (1981); (8) Morris & Ward (1988); (9) Shields & Filippenko (1990); (10) Ward et al. (1980); (11) Malkan (1986); (12) Osterbrock (1981a); (13) Moran et al. (1992); (14) Osterbrock & Miller (1975); (15) Fosbury & Sansom (1983).