Table 1: Emission line fluxes in the SDSS galaxies1.
Spectrum [Ne III] [O III] [Fe III] [O III] He I [O I] [S III] [N II] [S II] [Ar III] EW F2 C(H$\beta $)
number 3869 4363 4658 4959 5876 6300 6312 6584 6725 7135 Å    
0266-51630-1003 0.370 0.116 0.005 1.911 0.117 0.024 0.017 0.036 0.142 0.055 262 502 0.00
  0.012 0.005 0.002 0.057 0.004 0.002 0.001 0.002 0.004 0.003      
0267-51608-3843 0.444 0.042 0.010 1.263 0.088 0.020 0.010 0.096 0.219 0.053 57 314 0.19
  0.018 0.006 0.004 0.042 0.005 0.003 0.003 0.005 0.008 0.003      
0270-51909-3063 0.175 0.015 ... 0.967 0.130 0.026 0.011 0.294 0.518 ... 55 104 0.10
  0.014 0.009 ... 0.037 0.010 0.006 0.006 0.015 0.019 ...      
0272-51941-3653 0.297 0.023 0.006 1.131 0.112 0.058 0.023 0.224 0.502 0.076 31 110 0.13
  0.019 0.012 0.011 0.042 0.010 0.009 0.008 0.013 0.020 0.008      
0275-51910-4293 0.430 0.094 ... 1.587 0.112 0.029 0.012 0.059 0.237 0.056 107 197 0.03
  0.017 0.007 ... 0.051 0.006 0.004 0.003 0.004 0.009 0.004      
1 Only the first five galaxies are shown here. The total list of galaxies is available in electronic form at the CDS. The hydrogen, [O  II] $\lambda $3727, He  II $\lambda $4686, [Ar IV] $\lambda $4740, [Fe  III] $\lambda $4988, [Cl III] $\lambda $5517,5531, [O  II] $\lambda $7320,7330 and [S III] $\lambda $9069 emission lines are not shown here for lack of space, but they are present in the electronic table.

2 In units 10-16 erg s-1 cm-2.

3 The first row are values, the second row are errors.


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