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Table 1.

General properties of the QSO2 sample observed with OSIRIS/GTC.

Galaxy ID Short name z Scale log(L[OIII]) log(P5 GHz) Radio Extended radio emission
SDSS code SDSS_PA in the annular ring (FIRST–NVSS)
(kpc/″) (erg s−1) (erg s−1 Hz−1) (%)
(1) (2) (3) (4) (5) (6) (7) (8)
J074130.50+302005.1 0741+3020_148 0.476 5.922 41.93 30.69 RQ 38
J081858.36+395839.7 0818+3958_90 0.406 5.392 41.83 30.96 RI 36
J083454.90+553421.1 0834+5534_34 0.241 3.773 42.27 33.84 RL 3
J083454.90+553421.1 0834+5534_145 0.241 3.773 = =
J090226.73+545952.2 0902+5459_83 0.401 5.356 42.03 31.18 RI 8 (a)
J090226.73+545952.2 0902+5459_138 0.401 5.356 = =
J095629.03+573508.8 0956+5735_160 0.361 5.007 41.98 30.49 RQ 41 (b)
J110140.53+400422.9 1101+4004_111 0.456 5.780 43.29 32.26 RI 29

Notes. Column (1): SDSS galaxy ID. Column (2): short name galaxy ID with the information of the slit PA used (angle given from north to east). Column (3): redshift of the SDSS sources from the NASA Extragalactic Database (NED). Column (4): scale. Column (5): total luminosity of the [OIII]λ5007Å line (logarithmic scale). Column (6): radio power at 5 GHz. Column (7): radio loudness (RQ: radio-quiet; RI: radio-intermediate; and RL: radio-loud). Column (8): percentage of extended radio flux emission at 1.4 GHz between the FIRST and the NVSS beams (5″ vs. 45″ resolution, respectively).

(a)

The FIRST image shows that almost all the emission is in the lobes with marginal evidence for a radio core (Fig. 1).

(b)

This value is quite uncertain because the source is detected at only 3σ level in NVSS.

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