Table 3
Lyα luminosity of the quasars in the BLR, compared with the luminosity of the extended envelopes.
| Object | L(BLR) | L(Lyα) | Lcorrected(Lyα) |
| [erg s-1] | [erg s-1] | [erg s-1] | |
|
|
|||
| SDSS J0939+0039 | 4.1(±0.2) × 1044 | <7.4 × 1041a | <2.0 × 1042a |
| BR 1033−0327 | 7.2(±0.4) × 1045 | 2.7(±0.2) × 1042 | (1.1 ± 0.1) × 1043 |
| SDSS J14472+0401 | 2.1(±0.1) × 1045 | 8.6(±1.4) × 1041 | (2.0 ± 0.3) × 1042 |
| Q 2139−4324 | 4.6(±0.2) × 1044 | <4.1 × 1041a | <1.1 × 1042a |
| SDSS J21474−0838 | 6.8(±0.3) × 1045 | 6.2(±0.4) × 1043 | 1.9(±0.1) × 1044 |
| BR 2237−0607 | 1.4(±0.1) × 1046 | 5.1(±1.6) × 1041 | 8.0(±2.5) × 1041 |
Notes. The flux in the quasar BLR is measured in the wavelength interval 1200 − 1230 Å (rest-frame). The last column gives the Lyα flux of the envelope, after correction for slit-clipping (see text). The objects published in Courbin et al. (2008) are included for the sake of completeness.
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