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Table 13.

Hβ flux (Col.2), the observed and intrinsic Hβ luminosity of the total (Cols. 3–4) and the outflowing gas (Cols. 5–7).

Object F HβT L HβT obs L HβT intr F Hβout L Hβout obs L Hβout intr
PKS 0023–26 (1.1±0.1) × 10−15 (3.7±0.2) × 1041 (1.9±0.6) × 1042 (5.2±0.5) × 10−16 (1.8±0.2) × 1041 (1.1±0.5) × 1042
PKS 0252–71 (3.5±0.4) × 10−16 (4.7±0.5) × 1041 (4.7±0.8) × 1041 (2.3±0.3) × 10−16 (3.0±0.4) × 1041 (3.0±1.1) × 1041
PKS 1151–34 (7.3±0.8) × 10−16 (1.5±0.2) × 1041 (3.7±2.3) × 1041 (4.2±0.5) × 10−16 (8.9±1.1) × 1040 (2.1±1.3) × 1041
PKS 1306–09 (4.3±0.3) × 10−16 (3.6±0.3) × 1041 (7.6±3.2) × 1041 (4.0±0.3) × 10−16 (3.4±0.3) × 1041 (6.7±3.2) × 1041
PKS 1549–79 (3.2±0.2) × 10−15 (2.1±0.1) × 1041 (1.0±0.4) × 1042 (3.2±0.2) × 10−15 (2.1±0.1) × 1041 (1.0±0.4) × 1042
PKS 1814–63 (6.1±0.6) × 10−16 (6.1±0.6) × 1039 (1.1±0.5) × 1041 (4.2±0.5) × 10−16 (4.2±0.5) × 1039 (7.3±3.6) × 1040
PKS 1934–63 (1.2±0.1) × 10−15 (1.2±0.1) × 1041 (2.6±0.8) × 1041 (7.6±0.8) × 10−16 (7.2±0.7) × 1040 (1.4±0.3) × 1041
PKS 2135–209 (8.8±0.7) × 10−16 (1.6±0.1) × 1042 (4.6±1.6) × 1042 (8.8±0.7) × 10−16 (1.6±0.1) × 1042 (4.6±1.6) × 1042
PKS 2314+03 (1.4±0.1) × 10−15 (2.0±0.2) × 1041 (5.1±2.5) × 1041 (1.4±0.1) × 10−15 (2.0±0.2) × 1041 (5.1±1.8) × 1041

Notes. Fluxes are given in units of erg s−1 cm−2 Å−1 while luminosities in erg s−1. The distances of the targets have been estimated using the redshifts reported in Table 4, to apply the dust correction we use the DDD-derived E(B − V) values reported in Table 11.

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