Table 1: Parameters of the double Gaussian fit executed on the $\rm H\alpha $, [OIII] 5007, and [NII] 6583 emission lines. The flux of the components F is given in 10-16 erg/s/cm2, position with respect to the nominal center wavelength v and $\sigma $ are given in km s-1.
Name Line F1 v1 $\sigma_1$ F2 v2 $\sigma_2$
5253-1 $\rm H\alpha $ 96.9 4.3 22.0 38.3 -34.6 18.5
  [OIII] 90.6 3.3 22.3 23.6 -37.9 15.1
  [NII] 8.0 6.3 19.7 3.0 -33.0 15.5
5253-5 $\rm H\alpha $ 997.1 0.6 19.2 968.8 -10.9 49.9
  [OIII] 1496.8 0.7 16.2 1635.5 -8.7 48.6
  [NII] 43.5 2.3 14.2 93.1 -8.6 38.1
He 2-10 $\rm H\alpha $ 30.2 1.43 34.2 33.7 -19.0 93.5
  [OIII] 8.4 -1.03 33.9 8.7 -25.9 86.8
  [NII] 9.3 0.9 30.9 9.7 -17.7 87.4


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