Table 4
Synoptic table containing the main results for the 3 narrow emission-line AGNs (Fig. 6) identified or observed in the present sample of INTEGRAL sources.
| Object | FHα | FHβ | F [OIII] | Class | z | DL | E(B − V) | LX | |
|
|
|||||||||
| (Mpc) | Gal. | AGN | |||||||
|
|
|||||||||
| IGR J03249+4041 | 14 (14–150; B) | ||||||||
| 14 (14–195; B) | |||||||||
| 8.5 (17–60; I) | |||||||||
| (LEDA 4678815) | 30.4 ± 1.5 | 3.9 ± 0.6 | 27.2 ± 1.4 | Sy2 | 0.049 | 234.4 | 0.206 | 0.77 | 2.8 (0.2–12; N) |
| [48 ± 3] | [7.8 ± 1.2] | [51 ± 3] | |||||||
| (LEDA 97012) | 29 ± 3 | 1.3 ± 0.3 | 17.3 ± 1.2 | Sy2 | 0.049 | 234.4 | 0.206 | 1.98 | 0.059 (0.2–12; N) |
| [46 ± 5] | [2.3 ± 0.6] | [33 ± 2] | |||||||
| IGR J13550−7218 | 26 ± 2 | 8.7 ± 0.9 | 77 ± 2 | Sy2 | 0.071 | 345.0 | 0.360 | 0 | 3.0 (0.5–10; X) |
| [56 ± 5] | [25 ± 4] | [218 ± 7] | 21 (20–100; I) | ||||||
Notes. Emission-line fluxes are reported both as observed and (between square brackets) corrected for the intervening Galactic absorption E(B − V)Gal along the object line of sight (from Schlegel et al. 1998). Line fluxes are in units of 10-15 erg cm-2 s-1, whereas X-ray luminosities are in units of 1043 erg s-1 and the reference band (between round brackets) is expressed in keV. In the last column, the upper-case letter indicates the satellite and/or the instrument with which the corresponding X-ray flux measurement was obtained (see text).
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