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Table 4

Synoptic table containing the main results for the eight low-z broad emission-line AGNs (Fig. 7) identified or observed in the present sample of INTEGRAL sources.

Object F Hβ F [OIII] Class z DL (Mpc) E(B − V)Gal L X
IGR J02447+7046 2.0 ± 0.2 0.66 ± 0.06 Sy1.2 0.306 1710.8 0.770 3.7 (20–100; I)
[11.6 ± 1.2] [3.9 ± 0.4]
IGR J02574−0303 5.5 ± 0.6 1.51 ± 0.15 Sy1.2 0.197 1037.8 0.047 0.13 (0.5–10; X)
[5.6 ± 0.6] [1.63 ± 0.16] 2.6 (17–80; I)
IGR J06293−1359 0.47 ± 0.07 0.31 ± 0.03 Sy1.5 0.376 2174.8 0.317 9.6 (20–40; I)
[1.2 ± 0.2] [0.62 ± 0.06] <7.9 (40–100; I)
IGR J14488−4008 120 ± 20 45 ± 4 Sy1.2 0.123 619.0 0.109 0.11 (2–10; X)
[160 ± 30] [58 ± 6] 0.17 (20–40; I)
<0.17 (40–100; I)
0.33 (17–60; I)
0.60 (14–195; B)
0.38 (15–150; B)
IGR J17476−2253 6.0 ± 0.6 5.73 ± 0.17 Sy1.5 0.047 224.5 1.009 0.016–0.030 (2–10; X)
[127 ± 13] [121 ± 4] 0.11 (20–100; I)
0.060 (17–60; I)
0.11 (14–195; B)
0.090 (15–150; B)
IGR J17488−2338 1.08 ± 0.16 1.13 ± 0.03 Sy1.5 0.240 1295.7 1.570 0.70 (0.2–12; N)
[62 ± 9] [54.8 ± 1.6] 0.46 (2–10; X)
2.8 (20–100; I)
2E 1923.7+5037 137 ± 10 27.9 ± 1.4 Sy1.2 0.068 329.8 0.093 0.013 (0.1–2.4; X)
[173 ± 12] [36.1 ± 1.8] 0.014 (0.16–3.5; E)
0.13 (0.2–12; N)
0.10 (18–55; I+B)
0.13 (14–195; B)
IGR J21565+5948 0.55 ± 0.06 2.8 ± 0.4 Sy1 0.209 1108.7 1.267 0.010 (0.1–2.4; R)
[68 ± 10] [13.7 ± 1.4] 0.21 (0.3–10; C)
0.18 (2–10; X)
1.4 (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, X-ray luminosities are in units of 1045 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.

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