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Table 2.
Properties of the complementary QSO2 sample observed with FORS2/VLT.
| Galaxy ID | Short name | z | Scale | log(L[OIII]) | log(P5 GHz) | Radio | Extended radio emission |
|---|---|---|---|---|---|---|---|
| SDSS code | SDSS | in the annular ring (FIRST–NVSS) | |||||
| (kpc/″) | (erg s−1) | (erg s−1 Hz−1) | (%) | ||||
| (1) | (2) | (3) | (4) | (5) | (6) | (7) | (8) |
| J092318.06+010144.8 | J0923+0101 | 0.386 | 5.226 | 42.36 | 30.6 | RQ | 51 |
| J095044.69+011127.2 | J0950+0111 | 0.404 | 5.376 | 41.80 | 30.9 | RI | – |
| J095514.11+034654.2 | J0955+0346 | 0.422 | 5.520 | 42.05 | 30.9 | RI | 12 |
| J101403.49+024416.4 | J1014+0244 | 0.573 | 6.526 | 41.87 | 31.5 | RI | – |
| J115314.36+032658.6 | J1153+0326 | 0.575 | 6.537 | 43.24 | 31.2 | RQ | – |
| J124749.79+015212.6 | J1247+0152 | 0.427 | 5.559 | 41.81 | 32.0 | RL | 28 |
| J130740.55–021455.2 | J1307–0214 | 0.424 | 5.536 | 42.59 | 30.9 | RQ | – |
| J133633.65–003936.4 | J1336–0039 | 0.416 | 5.473 | 42.22 | ≲30.4 | RQ | 34 |
| J133735.01–012815.6 | J1337–0128 | 0.328 | 4.700 | 42.31 | 30.9 | RQ | 21 |
| J140740.06+021748.3 | J1407+0217 | 0.309 | 4.512 | 42.58 | 30.4 | RQ | 27 |
| J141315.31–014221.0 | J1413–0142 | 0.380 | 5.175 | 42.76 | 31.1 | RQ | – |
| J143027.66–005614.8 | J1430–0050 | 0.318 | 4.602 | 42.02 | ≲30.1 | RQ | – |
| J154613.27–000513.5 | J1546–0005 | 0.383 | 5.200 | 41.76 | 30.8 | RI | – |
Notes. See Table 1. The minus means that it has not been possible to assign a value because the source is weak and it is only detected in FIRST.
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