Table D.2
Synoptic table containing the main results for the 18 narrow emission-line AGNs observed in the present sample of 2PBC sources.
| Object | F Hα | F Hβ | F [OIII] | Class | z | D L | E(B−V) | L X | |
|
|
|||||||||
| (Mpc) | Gal. | AGN | |||||||
|
|
|||||||||
| 2PBC J0128.5+1628 | 59 ± 1 | 9.0 ± 0.7 | 78 ± 1 | Sy2 | 0.038 | 167.5 | 0.062 | 0.82 | 4.03(15–150)C |
| [68 ± 2] | [11 ± 1] | [93 ± 1] | 0.29 (0.3–10)X | ||||||
| 4.9 (14–195)B | |||||||||
| 2PBC J0154.1−5034 | 1.7 ± 0.1 | 0.6 ± 0.2 | 4.0 ± 0.1 | Sy 2 | 0.101 | 465.2 | 0.017 | ~0.04 | 20.70 (15–150)C |
| [1.7 ± 0.1] | [0.6 ± 0.2] | [4.3 ± 0.1] | 1.0 (0.3–10)X | ||||||
| 2PBC J0252.3+4309 | 19.3 ± 0.3 | 4.9 ± 0.3 | 34.8 ± 0.1 | Sy2 | 0.051 | 226.9 | 0.093 | 0.27 | 7.39 (15–150)C |
| [24 ± 1] | [6.3 ± 0.3] | [46 ± 1] | 0.24 (0.3–10)X | ||||||
| 8.04 (14–195)B | |||||||||
| 2PBC J0356.6−6252 | 15.7 ± 0.3 | 5.7 ± 0.4 | 49.8 ± 0.3 | ”Naked” Sy2 | 0.107 | 494.8 | 0.039 | ~0.0 | 29.3 (15–150)C |
| [17 ± 5] | [6.1 ± 0.6] | [56 ± 1] | 0.67 (0.3–10)X | ||||||
| 36.1 (14–195)B | |||||||||
| 2PBC J0505.4−6734 | – | – | 2.5 ± 0.3 | likely Sy2 | 0.046 | 203.9 | 0.229 | – | 3.48 (15–150)C |
| [5.2 ± 0.6] | 0.65 (0.2–12)N | ||||||||
| 5.9 (14–195)B | |||||||||
| 2PBC J0608.0+5749 | 1.5 ± 0.4 | <3 | 6.7 ± 0.3 | ”Naked” Sy2 | 0.050 | 222.3 | 0.099 | ~0.0 | 5.91 (15–150)C |
| [4.9 ± 0.4] | [<5] | [8.9 ± 0.3] | 0.35 (0.3–10)X | ||||||
| 2PBC J0640.1−4740 | 17.7 ± 0.1 | 5.5 ± 0.6 | 36.5 ± 0.3 | Sy2 | 0.056 | 250.0 | 0.099 | 0.13 | 6.73 (15–150)C |
| [21.9 ± 0.1] | [7.1 ± 0.6] | [50 ± 1] | 1.92 (0.3–10)X | ||||||
| 10.3 (14–195)B | |||||||||
| 2PBC J0819.2−2508 | 193 ± 2 | 25 ± 4 | 453 ± 12 | Sy2 | 0.004 | 17.2 | 0.145 | 0.876 | 0.02 (15–150)C |
| [272 ± 10] | [40 ± 10] | [719 ± 12] | 0.006 (0.3–10)X | ||||||
| 2PBC J0838.7+2612 | 7.8 ± 0.1 | 0.8 ± 0.1 | 7.2 ± 0.1 | Sy2 | 0.052 | 231.5 | 0.048 | 1.220 | 6.41 (15–150)C |
| [9 ± 1] | [0.9 ± 0.2] | [8.3 ± 0.1] | 0.30 (0.3–10)X | ||||||
| 2PBC J1020.5−0235 | – | 0.2 ± 0.1 | 3.9 ± 0.1 | Sy2 | 0.294 | 1517.0 | 0.042 | – | 303.0 (15–150)C |
| [0.3 ± 0.1] | [4.3 ± 0.1] | 23.8 (0.3–10)X | |||||||
| 194.7 (14–195)B | |||||||||
| 2PBC J1042.2+0043 | 8.2 ± 0.2 | 1.9 ± 0.1 | 16.6 ± 0.2 | Sy2 | 0.096 | 440.7 | 0.056 | 0.350 | 23.2 (15–150)C |
| [9.3 ± 0.2] | [2.3 ± 0.1] | [19.5 ± 0.2] | 8.36 (0.3–10)X | ||||||
| 28.2 (14–195)B | |||||||||
| 2PBC J1332.1−7751 | – | – | – | XBONG | 0.009 | 38.8 | 0.210 | – | 0.25 (15–150)C |
| 0.02 (0.3–10)X | |||||||||
| 0.3 (14–195)B | |||||||||
| 2PBC J1555.0−6225 | 27.8 ± 4.1 | 4.1 ± 0.1 | 7.3 ± 0.3 | likely Starburst Galaxy | 0.022 | 95.8 | 0.271 | 0.599 | 1.1 (15–150)C |
| [52 ± 5] | [10.0 ± 0.3] | [17.1 ± 0.4] | 0.13 (0.3–10)X | ||||||
| 2PBC J1649.3−1739 | 1.3 ± 0.1 | – | 0.6 ± 0.1 | type 2 AGN | 0.023 | 100.2 | 0.938 | – | 1.68 (15–150)C |
| [11 ± 3] | [11 ± 2] | 0.58 (0.3–10)X | |||||||
| 2PBC J1832.8+3124 | 10.1 ± 0.6 | – | 15.9 ± 0.7 | Sy2 | 0.043 | 190.2 | 0.116 | – | 2.60 (15–150)C |
| [13 ± 1] | [22 ± 1] | 0.07 (0.3–10)X | |||||||
| 2PBC J2029.4−6146 | 6.5 ± 1.5 | 1.9 ± 0.1 | 21.0 ± 0.1 | ”Naked” Sy2 | 0.124 | 579.9 | 0.052 | ~0.0 | 44.3 (15–150)C |
| [8 ± 3] | [3.4 ± 0.2] | [24.0 ± 0.1] | 18.5 (0.3–10)X | ||||||
| 63.6 (14–195)B | |||||||||
| 2PBC J2238.9+4050 | 14.9 ± 0.2 | 3.4 ± 0.2 | 2.0 ± 0.1 | LINER | 0.055 | 245.4 | 0.242 | 0.296 | 5.04 (15–150)C |
| [28 ± 7] | [7.2 ± 0.6] | [4.0 ± 0.4] | 0.46 (0.3–10)X | ||||||
| 2PBC J2322.6+2903 | 6.5 ± 0.2 | – | 16.8 ± 0.4 | Sy2 | 0.019 | 82.6 | 0.154 | – | 0.74 (15–150)C |
| [8.9 ± 0.2] | [26.7 ± 0.4] | 0.06 (0.3–10)X | |||||||
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. The typical error of the redshift measurement is ±0.001.
From Swift-BAT, Cusumano et al. (2010).
From Swift-BAT, Baumgartner et al. (2013).
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