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Table 12.

Total [O III]5007 Å line fluxes (Col. 2), the [O III] observed (Col. 3) and dust corrected (Col. 4) luminosities, and the AGN bolometric luminosities calculated following the Lamastra et al. (2009) (Col. 5) and the Heckman et al. (2004) (Col. 6) calibrations.

Object F[O III]T L[O III]obs L[O III]intr LBOL L09 LBOL H04
PKS 0023–26 (3.3±0.2) × 10−15 (1.1±0.1) × 1042 (5.4±1.8) × 1042 (2.5±0.8) × 1045 (4.0±0.2) × 1045
PKS 0252–71 (3.1±0.2) × 10−15 (4.1±0.2) × 1042 (4.1±0.6) × 1042 (1.8±0.3) × 1045 (1.4±0.1) × 1046
PKS 1151–34 (1.2±0.1) × 10−14 (2.5±0.2) × 1042 (5.8±3.4) × 1042 (2.6±1.6) × 1045 (8.7±0.6) × 1045
PKS 1306–09 (1.5±0.1) × 10−15 (1.3±0.1) × 1042 (2.6±1.0) × 1042 (1.2±0.5) × 1045 (4.5±0.3) × 1045
PKS 1549–79 (4.3±0.3) × 10−14 (2.7±0.2) × 1042 (1.3±0.5) × 1043 (6.0±2.4) × 1045 (9.6±0.6) × 1045
PKS 1814–63 (3.5±0.2) × 10−15 (3.4±0.2) × 1040 (5.7±2.3) × 1041 (8.1±3.2) × 1043 (1.2±0.1) × 1044
PKS 1934–63 (1.0±0.1) × 10−14 (9.5±0.9) × 1041 (2.1±0.6) × 1042 (9.4±2.6) × 1044 (3.3±0.3) × 1045
PKS 2135–209 (5.9±0.4) × 10−15 (1.0±0.1) × 1043 (2.9±1.0) × 1043 (1.3±0.4) × 1046 (3.6±0.3) × 1046
PKS 2314+03 (4.7±0.1) × 10−15 (6.8±0.1) × 1041 (1.7±0.8) × 1042 (7.7±3.5) × 1044 (2.4±0.04) × 1045

Notes. Fluxes are given in units of erg s−1 cm−2 Å−1 while luminosities are in erg s−1. The distances of the targets were estimated using the redshifts reported in Table 4, and to apply the dust extinction correction we used the DDD-derived E(B − V) values for total line fluxes reported in Col. 5 of Table 11.

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