Table 4: Correction for seeing effects, for apertures $2''\times 6''$ and $2.5''\times 6''$. Columns: 1 - seeing intervals in arcsec; 2 - mean seeing in arcsec; 3 - our seeing correction for the emission lines fluxes, ks(our); 4 - estimated seeing correction error, e(ks); 5 - Peterson's seeing correction for the emission lines fluxes from Peterson et al. (1995), ks(Pet); 6 - our host galaxy seeing correction for the continuum fluxes, in units of 10-14 erg s-1 cm-2 Å-1, Gs(our); 7 - estimated host galaxy seeing correction error, e(Gs); 8 - Peterson's host galaxy seeing correction Gs(Pet) for the continuum fluxes from Peterson et al. (1995).
Interval Mean ks(our) $\pm$e ks(Pet) Gs(our) $\pm$e Gs(Pet)
seeings seeing ( $2''\times 6''$)   ( $2''\times10''$) ( $2''\times 6''$)   ( $2''\times10''$)
arcsec arcsec H$\beta $ wings   H$\beta $ 10-14   10-14

1''-1.5''		 1.25'' 0.965 0.046   -0.160 0.197 -0.070 (1.3'')
  1.5'' 0.977*   0.973      
1.5''-2.5'' 2.0'' 1.000   1.000 0   0
2.5''-3.5'' 3.0'' 1.042 0.030 1.052 -0.039   0.130
3.5''-4.5'' 4.0'' 1.069 0.063 1.086      
3.5''-5.2''         0.329 0.203  
  5'' 1.096   1.105     0.31


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