Name | Type | z | log ![]() |
log f2-10 |
![]() |
log
![]() |
A |
![]() |
(1) | (2) | (3) | (4) | (5) | (6) | (7) | (8) | (9) |
NGC 3227 | 1.5 | 0.0039 | 22.83 | -11.09 | 1 | -13.05 | L | 1 |
NGC 3516 | 1.5 | 0.0088 | 20.63 | -10.62 | 2 | -13.15 | L | 1 |
NGC 3783 | 1.0 | 0.0097 | 20.00 | -10.07 | 3 | -12.86 | M | 2 |
NGC 4051 | 1.5 | 0.0020 | 20.00 | -10.64 | 4 | -12.98 | L | 1 |
NGC 4151 | 1.5 | 0.0033 | 22.88 | -10.35 | 1 | -11.70 | L | 1 |
NGC 4253 | NLS1 | 0.0129 | 20.00 | -10.80 | 5 | -13.49 | M | 3 |
NGC 4395 | 1.0 | 0.0010 | 20.80 | -11.30 | 6 | -14.10 | S | 4 |
NGC 4593 | 1.0 | 0.0090 | 20.00 | -10.43 | 7 | -13.60 | M | 2 |
NGC 5548 | 1.5 | 0.0172 | 20.00 | -10.28 | 7 | -12.57 | L | 1 |
NGC 6814 | 1.5 | 0.0052 | 20.00 | -11.82 | 8 | -13.77 | M | 2 |
NGC 7469 | 1.2 | 0.0163 | 20.00 | -10.64 | 7 | -12.74 | L | 1 |
Mrk 42 | NLS1 | 0.0246 | 20.00 | -11.98 | 9 | -14.52 | L | 5 |
Mrk 359 | NLS1 | 0.0169 | 20.00 | -11.24 | 10 | -13.30 | S | 4 |
Mrk 486 | NLS1 | 0.0389 | 20.00 | -11.55 | 11 | -13.68 | S | 4 |
Mrk 493 | NLS1 | 0.0313 | 20.00 | -11.46 | 10 | -14.52 | M | 3 |
Mrk 509 | 1.2 | 0.0344 | 20.00 | -10.47 | 7 | -12.24 | M | 2 |
Mrk 704 | 1.5 | 0.0291 | 23.13 | -11.25 | 12 | -13.21 | S | 4 |
Mrk 705 | 1.2 | 0.0285 | 20.00 | -10.64 | 13 | -13.80 | S | 4 |
Mrk 841 | 1.5 | 0.0364 | 20.00 | -10.79 | 14 | -13.15 | M | 2 |
Mrk 896 | 1.0 | 0.0264 | 20.00 | -11.46 | 10 | -14.10 | M | 2 |
Mrk 926 | 1.5 | 0.0469 | 20.00 | -10.51 | 7 | -13.96 | S | 6 |
Mrk 1239 | NLS1 | 0.0194 | 23.52 | -11.82 | 15 | -13.31 | S | 4 |
3C 120 | BLRG | 0.0330 | 20.70 | -10.31 | 16 | -13.72 | S | 6 |
3C 227 | BLRG | 0.0858 | 22.10 | -11.70 | 17 | -14.40 | M | 7 |
3C 382 | BLRG | 0.0578 | 20.00 | -10.21 | 18 | -13.85 | M | 7 |
3C 390.3 | BLRG | 0.0561 | 20.60 | -10.40 | 19 | -13.59 | S | 4 |
3C 445 | BLRG | 0.0562 | 22.70 | -11.17 | 20 | -13.85 | M | 2 |
Fairall 9 | 1.2 | 0.0470 | 20.00 | -10.92 | 7 | -13.03 | M | 8 |
Fairall 51 | 1.0 | 0.0142 | 22.20 | -10.60 | 21 | -13.29 | M | 2 |
Fairall 1116 | 1.0 | 0.0582 | 20.00 | -11.27 | 22 | -13.54 | M | 8 |
Tol 1351-375 | 1.9 | 0.0520 | 22.20 | -11.42 | 23 | -13.48 | M | 2 |
Tol 1506.3-00 | 1.5 | 0.0543 | 21.85 | -11.11 | 24 | -14.00 | M | 2 |
H1143-182 | 1.5 | 0.0329 | 20.00 | -10.55 | 4 | -13.19 | M | 8 |
H1846-786 | 1.0 | 0.0743 | 20.00 | -11.10 | 7 | -13.49 | M | 2 |
Akn 120 | 1.0 | 0.0330 | 20.00 | -10.42 | 25 | -14.15 | S | 4 |
Akn 564 | NLS1 | 0.0247 | 20.00 | -10.80 | 26 | -13.33 | S | 4 |
MCG-6-30-15 | 1.2 | 0.0077 | 20.00 | -10.62 | 27 | -14.05 | M | 2 |
1ES1615+061 | 1.5 | 0.0380 | 20.00 | -11.10 | 28 | -14.22 | M | 2 |
IIIZw77 | 1.2 | 0.0342 | 23.90 | -12.22 | 24 | -13.55 | M | 9 |
ESO 141-G55 | 1.2 | 0.0360 | 20.00 | -10.57 | 29 | -13.17 | M | 8 |
POX 52 | 1.0 | 0.0218 | 20.70 | -12.11 | 30 | -13.35 | M | 10 |
Notes. Column
description: (1) Source name. (2) Spectroscopic classification (1.0,
1.2 and 1.5 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) Logarithm
of the observed 2-10 keV flux in erg cm-2 s-1.
(6) Reference for the X-ray data. (7) Logarithm of the
[Ne V]3426 flux in 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) Bianchi
et al. (2004); (3) Blustin
et al. (2002); (4) Bianchi
et al. (2009); (5) Landi
et al. (2005); (6) Iwasawa
et al. (2010); (7) Shinozaki
et al. (2006); (8) Vasudevan
& Fabian (2007); (9) Vaughan
et al. (1999); (10) Gallo
(2006); (11) Ballo
et al. (2008); (12) Landi
et al. (2007); (13) Gallo
et al. (2005); (14) Piconcelli
et al. (2005); (15) Grupe
et al. (2004); (16) Grandi
et al. (2006); (17) Hardcastle
et al. (2007); (18) Gliozzi
et al. (2007); (19) Evans
et al. (2006); (20) Sambruna
et al. (2007); (21) Jiménez-Bailón
et al. (2008) (22) D'Ammando
et al. (2008); (23) Risaliti
et al. (2000); (24) this work; (25) Vaughan et al. (2004);
(26) Vignali et al. (2004);
(27) Ponti et al. (2004);
(28) Guainazzi et al.
(1998); (29) Gondoin
et al. (2003); (30) Thornton
et al. (2008).
[Ne V] references: (1) Anderson (1970); (2) Morris & Ward (1988); (3) Osterbrock & Pogge (1985);
(4) Erkens et al. (1997);
(5) Malkan (1986); (6) Durret & Bergeron (1988); (7)
Osterbrock et al. (1976);
(8) Winkler (1992); (9) Osterbrock (1981b); (10) Kunth et al. (1987).
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