Table 3: Line identifications and redshifts.
Name ID Line Wavelength (Å) Redshift Mean Flux FWHM Log Power 5 GHz
B0008-421 G [Ne V] 3425? 7294 1.130 1.130* 0.3 29 26.7
    [O II] 3727? 7940 1.130   0.7 39  
B0316+161 G [O II] 3727 7102 0.906 0.907 5.4 21 27.6
    [Ne III] 3869 7381 0.908   1.8 32  
    H$_\beta$ 4861 9277 0.908   4.7 49  
    [O III] 4959 9464 0.908   8.3 35  
    [O III] 5007 9544 0.906   33 51  
B0407-658 G [Ne V] 3425 6721 0.962 0.962 11 25 27.7
    [O II] 3727 7314 0.962   6.9 29  
    [Ne III] 3869 7595 0.963   2.0 44  
    [Ne III] 3967 7787 0.963   0.7 29  
    H$_\gamma$ 4102 8048 0.962   0.3 18  
    H$_\beta$ 4861 9538 0.962   4.4 52  
    [O III] 4959 9731 0.962   43 51  
    [O III] 5007 9823 0.962   16 54  
B0904+039 G [O II] 3727 6822 0.830 0.830 1.9 17 24.9
    [O III] 4959 9078 0.831   1.8 26  
    [O III] 5007 9162 0.830   4.4 26  
B0914+114 G Break 4000 4711 0.178 0.178 - - -
    H$\beta$ 4861 5690? 0.171? $\pm$0.005 - -  
    Mg b 5200 6115 0.183   - -  
    [N II] 6548 7667 0.171   - -  
    H$\alpha$ 6563 7772 0.184   - -  
    [S II] 6716 7952 0.184   - -  
B1045+019   [O II] 3727 6297 0.689 0.689* 0.4 12 26.6
    H$_\gamma$ 4102 7327 0.688   0.3 12  
    [He II] 4686 7918 0.689   0.3 29  
PMN J1300-1059 Q? Mg II 2799 6385 1.283 1.283* 10 125 -
B1433-040 Q [O II] 3727 6694 0.796 0.795 17 19 26.3
    [Ne III] 3869 6949 0.796   32 54  
    [Ne III] 3967 7122 0.795   10 21  
    H$_\delta$ 4102 7355 0.794   23 84  
    H$_\gamma$ 4341 7790 0.795   76 113  
    H$_\beta$ 4861 8724 0.795   347 192  
    [O III] 4959 8900 0.795   63 30  
    [O III] 5007 8987 0.795   121 27  
For B1433-040, the redshift is measured with the narrow emission profiles. The * means the redshift estimation is uncertain for that source, see text for details. The FWHM listed is the observed FWHM corrected for the FWHM of the instrumental spectrum. Fluxes in 10-16 erg/cm2/s. A conservative error for z is $\pm$0.001. The B0914+114 results correspond to the unrelated galaxy. It shows emission and absorption lines mixed so the centers are more uncertain than in the other sources (the 1$\sigma$ error in z is listed below the mean value) and line properties will depend on the stellar population model. The last column lists the radio power in W/Hz of the source for the redshifts listed. The 5 GHz fluxes are from O'Dea (1998) and Wright & Otrupcek (1990).

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