Table 5
Synoptic table containing the main results for the seven low-redshift narrow emission-line AGNs (Fig. 8) and for the two XBONGs (Fig. 9) identified or observed in the present sample of INTEGRAL sources.
| Object | F Hα | F Hβ | F [OIII] | Class | z | D L | E(B − V) | L X | |
|
|
|||||||||
| (Mpc) | Gal. | AGN | |||||||
|
|
|||||||||
| IGR J02045−1156 | 196 ± 10 | 32 ± 3 | 31 ± 3 | LINER | 0.0727 | 353.7 | 0.023 | 0.68 | 0.61 (0.1–2.4; R) |
| [196 ± 10] | [35 ± 4] | [33 ± 3] | 4.3 (0.2–12; N) | ||||||
| 1.4 (0.3–10; X) | |||||||||
| 24 (17–80; I) | |||||||||
| Swift J0250.2+4650 | 31.4 ± 1.6 | 6.5 ± 0.7 | 67 ± 2 | Sy2 | 0.021 | 98.4 | 0.194 | 0.20 | 0.20 (0.2–12; N) |
| [48 ± 3] | [13.7 ± 1.4] | [124 ± 4] | 1.7 (17–60; I) | ||||||
| 2.3 (14–195; B) | |||||||||
| 2.0 (15–150; B) | |||||||||
| IGR J05048−7340 | in abs. | in abs. | <8 | XBONG | 0.014 | 69.0 | 0.127 | – | 0.31 (20–60; I) |
| [in abs.] | [in abs.] | [<12] | 0.48 (14–195; B) | ||||||
| 0.43 (15–150; B) | |||||||||
| IGR J05470+5034 | 29 ± 3 | 3.4 ± 1.0 | 20 ± 2 | Sy2 | 0.036 | 170.6 | 0.233 | 0.83 | 0.006 (0.1–2.4; R) |
| [48 ± 5] | [7 ± 2] | [40 ± 4] | 5.9 (17–60; I) | ||||||
| 8.3 (14–195; B) | |||||||||
| 5.6 (15–150; B) | |||||||||
| IGR J10200−1436 | – | <0.03 | <0.07 | XBONG | 0.391 | 2277.2 | 0.104 | – | 6.8 (0.1–2.4; X) |
| – | [<0.05] | [<0.08] | 740 (20–40; I) | ||||||
| <810 (40–100; I) | |||||||||
| IGR J15415−5029 | 12.1 ± 1.8 | <0.17 | 4.7 ± 0.7 | likely Sy2 | 0.032 | 151.2 | 0.862 | >0.85 | 0.15 (0.3–10; C) |
| [86 ± 13] | [<13] | [66 ± 10] | 1.7 (17–60; I) | ||||||
| 3.0 (20–100; I) | |||||||||
| 2.5 (15–150; B) | |||||||||
| IGR J16058−7253* | |||||||||
| (LEDA 259433) | 4.6 ± 0.5 | in abs. | 7.6 ± 0.7 | likely Sy2 | 0.069 | 334.8 | 0.094 | – | 4.4 (2–10; X) |
| [8.5 ± 0.9] | [in abs.] | [9.4 ± 0.9] | |||||||
| (LEDA 259580) | 5.7 ± 0.5 | <2 | 7.8 ± 0.8 | Sy2 | 0.090 | 373.0 | 0.094 | >0 | 4.8 (2–10; X) |
| [6.4 ± 0.6] | [<3] | [1.05 ± 0.11] | |||||||
| IGR J17520−6018 | 2.7 ± 0.8 | in abs. | 4.4 ± 1.1 | likely Sy2 | 0.112 | 559.6 | 0.091 | – | 9.7 (2–10; X) |
| [3.2 ± 0.9] | [in abs.] | [5.4 ± 1.4] | 86 (20–100; I) | ||||||
| 56 (14–195; B) | |||||||||
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, 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). The typical error of the redshift measurement is ±0.001 except for the 6dFGS spectrum of IGR J02045−1156, for which an uncertainty of ±0.0003 can be assumed.
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