Table 1: Reddening corrected line fluxes, relative to H$\beta $ = 100, and corresponding extinction coefficients for the sample of galaxies.
Galaxy [OI] [SIII] [OI] [NII] H$\alpha $ [NII] HeI [SII] [SII] HeI [ArIII] [OII] [OII] Pa12 Pa11 Pa10 Pa9 [SIII] Pa8 C(H$\beta $)
  6300 6312 6364 6548 6563 6584 6678 6717 6731 7065 7136 7320 7330 8750 8865 9014 9229 9069 9548  
(1) (2) (3) (4) (5) (6) (7) (8) (9) (10) (11) (12) (13) (14) (15) (16) (17) (18) (19) (20) (21)
UM238 - - - 5.7 286.0 8.6 - 17.2 13.4 5.8 6.8 3.2 1.8 - - - - 3.7 4.7 0.26
  - - - $\pm$ 1.1 $\pm$ 5.5 $\pm$ 1.3 - $\pm$ 1.8 $\pm$ 1.9 $\pm$ 0.9 $\pm$ 0.3 $\pm$ 0.7 $\pm$ 0.5 - - - - $\pm$ 0.5 $\pm$ 1.0  
UM69(E) - - - 9.4 286.0 28.9 - 40.5 30.0 - 8.4 7.2 3.4 - - - - 16.7 4.7 0.74
  - - - $\pm$ 1.4 $\pm$ 2.3 $\pm$ 1.4 - $\pm$ 1.6 $\pm$ 1.4 - $\pm$ 0.9 $\pm$ 0.7 $\pm$ 0.6 - - - - $\pm$ 1.2 $\pm$ 0.9  
UM69(W) - - - 15.4 286.0 39.2 - 56.2 40.0 - 6.4 - - - - - - 14.7 3.5 0.74
  - - - $\pm$ 1.4 $\pm$ 1.6 $\pm$ 1.2 - $\pm$ 2.2 $\pm$ 2.0 - $\pm$ 0.5 - - - - - - $\pm$ 1.0 $\pm$ 0.7  
Tol0104-388 7.1 - - 8.3 286.0 22.1 3.3 29.7 21.9 - 9.0 3.6 2.8 - 2.0 1.9 - 48.8a 4.0 0.18
  $\pm$ 0.2 - - $\pm$ 0.5 $\pm$ 0.6 $\pm$ 0.2 $\pm$ 0.3 $\pm$ 0.3 $\pm$ 0.1 - $\pm$ 0.4 $\pm$ 0.1 $\pm$ 0.1 - $\pm$ 0.3 $\pm$ 0.3 - $\pm$ 6.5 $\pm$ 0.9  
UM306 - - - 6.1 286.0 16.3 - 23.1 17.9 - 7.0 - - - - - - 22.7 3.7 0.21
  - - - $\pm$ 0.9 $\pm$ 1.3 $\pm$ 0.7 - $\pm$ 1.3 $\pm$ 1.2 - $\pm$ 0.9 - - - - - - $\pm$ 6.0 $\pm$ 2.1  
UM307 - - - 15.4 286.0 46.5 4.3 24.0 27.3 - 4.8 2.4 1.5 - - 2.1 - 18.5 3.7 0.25
  - - - $\pm$ 0.5 $\pm$ 1.0 $\pm$ 0.7 $\pm$ 1.0 $\pm$ 0.7 $\pm$ 0.6 - $\pm$ 0.7 $\pm$ 0.4 $\pm$ 0.4 - - $\pm$ 0.7 - $\pm$ 1.7 $\pm$ 0.6  
Tol0117-414NS(S) - - - 21.3 286.0 35.6 - 40.3 31.1 - - - - - - - - 32.5 - 0.10
  - - - $\pm$ 1.8 $\pm$ 2.6 $\pm$ 1.8 - $\pm$ 1.6 $\pm$ 1.6 - - - - - - - - $\pm$ 12.0 -  
Tol0117-414NS(N) - - - 20.2 286.0 36.9 - 43.0 31.5 - - - - - - - - 31.7 - 0.22
  - - - $\pm$ 2.3 $\pm$ 6.8 $\pm$ 1.4 - $\pm$ 2.0 $\pm$ 0.9 - - - - - - - - $\pm$ 12.4 -  
Tol0117-414NS - - - 20.0 286.0 38.1 - 42.9 32.0 - - - - - - - - 27.9 - 0.10
  - - - $\pm$ 2.4 $\pm$ 2.9 $\pm$ 1.4 - $\pm$ 0.5 $\pm$ 1.1 - - - - - - - - $\pm$ 9.6 -  
Tol0117-414EW(EW) 12.1 - - 17.8 286.0 50.1 - 58.5 43.3 - - - - - - - - 28.2 - 0.31
  $\pm$ 1.1 - - $\pm$ 1.0 $\pm$ 1.9 $\pm$ 1.2 - $\pm$ 1.7 $\pm$ 2.9 - - - - - - - - $\pm$ 10.5 -  
Tol0117-414EW 16.1 - - 7.8 286.0 39.2 - 57.8 45.1 - - - - - - - - 25.9 - 0.31
  $\pm$ 1.3 - - $\pm$ 0.3 $\pm$ 6.6 $\pm$ 1.0 - $\pm$ 1.2 $\pm$ 1.4 - - - - - - - - $\pm$ 9.0 -  
UM323 - - - 9.9 286.0 17.3 - 26.9 20.1 - - - - - - - - 9.6 4.8 0.88
  - - - $\pm$ 5.1 $\pm$ 7.4 $\pm$ 4.7 - $\pm$ 6.6 $\pm$ 5.3 - - - - - - - - $\pm$ 1.3 $\pm$ 1.2  
Tol0140-420 - - - - 286.0 12.4 - 29.7 20.8 - - - - - - - - 16.5 - 0.02
  - - - - $\pm$ 5.9 $\pm$ 1.0 - $\pm$ 2.4 $\pm$ 2.4 - - - - - - - - $\pm$ 5.4 -  
UM137 - - - - 286.0 18.1 - 32.1 28.1 4.8 2.2 - - - - 5.1 - 5.3 4.4 1.47
  - - - - $\pm$ 2.8 $\pm$ 1.8 - $\pm$ 3.2 $\pm$ 2.8 $\pm$ 1.1 $\pm$ 0.7 - - - - $\pm$ 1.0 - $\pm$ 1.2 $\pm$ 1.5  
UM151 - - - 13.4 286.0 37.6 - 48.2 33.4 - 7.7 - - - - 1.9 - 28.5 2.8 0.41
  - - - $\pm$ 2.1 $\pm$ 3.5 $\pm$ 2.3 - $\pm$ 3.1 $\pm$ 2.5 - $\pm$ 2.7 - - - - $\pm$ 0.6 - $\pm$ 6.4 $\pm$ 0.6  
UM391 7.6 - 4.2 26.2 286.0 79.6 - 64.5 25.5 - 5.4 - - - - - - 19.5 - 0.53
  $\pm$ 2.0 - $\pm$ 1.5 $\pm$ 1.3 $\pm$ 1.6 $\pm$ 0.8 - $\pm$ 0.8 $\pm$ 0.7 $\pm$ 0. $\pm$ 1.2 - - - - - - $\pm$ 2.9 -  
UM396 - - - 7.3 286.0 9.0 3.1 13.4 7.3 3.7 10.2 - - - 3.0 6.7 - 27.3 3.9 0.35
  - - - $\pm$ 1.4 $\pm$ 1.9 $\pm$ 1.3 $\pm$ 0.4 $\pm$ 0.6 $\pm$ 0.5 $\pm$ 0.5 $\pm$ 0.6 - - - $\pm$ 0.5 $\pm$ 1.0 - $\pm$ 5.2 $\pm$ 0.3  
UM408 - - - - 286.0 6.8 - 17.7 11.5 - 6.9 - - - - - - 5.5 - 1.32
  - - - - $\pm$ 4.3 $\pm$ 1.3 - $\pm$ 1.2 $\pm$ 1.1 - $\pm$ 0.7 - - - - - - $\pm$ 0.8 -  
UM417 - - - - 286.0 8.3 - 10.1 8.9 4.5 4.6 - - - - - - 1.8 - 0.47
  - - - - $\pm$ 4.1 $\pm$ 1.3 - $\pm$ 0.7 $\pm$ 0.7 $\pm$ 0.7 $\pm$ 1.2 - - - - - - $\pm$ 0.2 -  
Tol0226-390 9.8 2.5 4.1 15.8 286.0 31.2 3.3 25.9 21.9 4.2 8.8 3.5 3.0 - - - 2.1 20.4 5.5 0.34
  $\pm$ 0.3 $\pm$ 0.3 $\pm$ 0.5 $\pm$ 0.9 $\pm$ 1.3 $\pm$ 1.0 $\pm$ 0.3 $\pm$ 0.8 $\pm$ 0.7 $\pm$ 0.2 $\pm$ 0.4 $\pm$ 0.3 $\pm$ 0.2 - - - $\pm$ 0.5 $\pm$ 3.4 $\pm$ 2.6  
Tol0306-405 - - - - 286.0 14.1 - 24.3 20.9 - 8.4 - - - - - - 7.5 - 0.33
  - - - - $\pm$ 1.6 $\pm$ 0.9 - $\pm$ 0.7 $\pm$ 0.8 - $\pm$ 0.1 - - - - - - $\pm$ 3.5 -  
Tol0341-407(W) 5.2 - - 1.1 286.0 6.4 4.8 15.5 10.7 2.9 6.2 2.5 2.6 1.6 - - 3.0 19.1 - 0.06
  $\pm$ 0.4 - - $\pm$ 0.1 $\pm$ 4.0 $\pm$ 0.1 $\pm$ 0.5 $\pm$ 0.1 $\pm$ 0.1 $\pm$ 0.1 $\pm$ 0.1 $\pm$ 0.2 $\pm$ 0.1 $\pm$ 0.5 - - $\pm$ 0.6 $\pm$ 1.7 -  
Tol0341-407(E) - - - - 286.0 16.6 - 37.8 25.3 - - 4.8 3.8 - - - - 17.5 - 0.06
  - - - - $\pm$ 4.5 $\pm$ 3.2 - $\pm$ 3.0 $\pm$ 2.4 - - $\pm$ 1.2 $\pm$ 1.0 - - - - $\pm$ 2.0 -  
Cam0357-3915 2.5 - - 2.4 286.0 6.5 3.3 9.3 6.3 5.2 4.8 1.9 0.9 - - 2.2 - 11.5 - 0.15
  $\pm$ 0.2 - - $\pm$ 0.1 $\pm$ 5.1 $\pm$ 0.6 $\pm$ 0.2 $\pm$ 0.1 $\pm$ 0.6 $\pm$ 0.3 $\pm$ 0.1 $\pm$ 0.1 $\pm$ 0.1 - - $\pm$ 0.5 - $\pm$ 2.0 -  
CTS1006 - - - 4.9 286.0 13.7 3.6 21.3 10.8 3.2 7.2 2.4 1.8 0.9 0.9 1.2 2.3 15.2 5.1 0.15
  - - - $\pm$ 0.4 - $\pm$ 0.3 $\pm$ 0.4 $\pm$ 0.6 $\pm$ 0.5 $\pm$ 0.4 $\pm$ 0.3 $\pm$ 0.2 $\pm$ 0.2 $\pm$ 0.2 $\pm$ 0.1 $\pm$ 0.2 $\pm$ 0.5 $\pm$ 1.3 $\pm$ 0.6  
CTS1008 3.2 1.6 - 5.1 286.0 13.4 3.9 16.7 13.7 3.7 9.5 3.2 1.6 - - - 4.2 17.4 4.7 0.24
  $\pm$ 0.1 $\pm$ 0.4 - $\pm$ 0.3 $\pm$ 0.5 $\pm$ 0.3 $\pm$ 0.3 $\pm$ 0.4 $\pm$ 0.4 $\pm$ 0.3 $\pm$ 0.6 $\pm$ 0.5 $\pm$ 0.3 - - - $\pm$ 1.0 $\pm$ 3.3 $\pm$ 1.4  
Tol0528-383(E) - - - 10.3 286.0 18.0 - 39.9 30.4 - 11.3 - - - - - - 19.9 3.9 0.46
  - - - $\pm$ 2.9 $\pm$ 3.2 $\pm$ 2.9 - $\pm$ 2.1 $\pm$ 2.7 - $\pm$ 1.9 - - - - - - $\pm$ 3.0 $\pm$ 1.3  
Tol0528-383(W) - - - 10.2 286.0 16.4 - 31.6 22.0 - 9.2 - - - - - 2.7 13.5 5.0 0.46
  - - - $\pm$ 1.9 $\pm$ 2.0 $\pm$ 1.8 - $\pm$ 1.8 $\pm$ 1.4 - $\pm$ 1.6 - - - - - $\pm$ 0.9 $\pm$ 2.5 $\pm$ 1.5  
Tol0538-416 4.5 2.0 3.0 5.1 286.0 14.9 4.0 24.4 15.9 3.4 16.7 - - - 2.3 - - 19.2 4.7 0.14
  $\pm$ 0.4 $\pm$ 0.3 $\pm$ 0.4 $\pm$ 0.7 $\pm$ 0.9 $\pm$ 0.6 $\pm$ 0.4 $\pm$ 0.8 $\pm$0.6 $\pm$ 0.5 $\pm$ 0.5 - - - $\pm$ 0.6 - - $\pm$ 4.1 $\pm$ 2.9  
IIZw40 1.8 1.1 - - 286.0 6.4 3.5 7.6 6.2 4.6 8.3 1.4 1.1 1.1 1.3 1.9 2.7 15.3 4.3 1.29
  $\pm$ 0.2 $\pm$ 0.2 - - $\pm$ 0.3 $\pm$ 0.2 $\pm$ 0.3 $\pm$ 0.4 $\pm$ 0.3 $\pm$ 0.2 $\pm$ 0.3 $\pm$ 0.2 $\pm$ 0.2 $\pm$ 0.1 $\pm$ 0.1 $\pm$ 0.3 $\pm$ 0.3 $\pm$ 1.6 $\pm$ 1.4  
Cam0840+1201 4.4 2.2 - 5.2 286.0 12.5 - 21.9 16.0 3.4 7.1 3.2 2.7 1.1 - 1.8 - 16.2 7.3 0.02
  $\pm$ 0.4 $\pm$ 0.3 - $\pm$ 0.2 - $\pm$ 0.2 - $\pm$ 0.3 $\pm$ 0.3 $\pm$ 0.2 $\pm$ 0.3 $\pm$ 0.2 $\pm$ 0.2 $\pm$ 0.7 - $\pm$ 0.2 - $\pm$ 5.1 $\pm$ 1.3  
Tol1924-416 4.9 1.5 1.1 3.5 286.0 8.9 3.5 14.7 11.4 2.9 5.2 2.4 2.0 - 1.4 1.8 - 11.7 4.3 0.10
  $\pm$ 0.2 $\pm$ 0.2 $\pm$ 0.2 $\pm$ 0.2 $\pm$ 0.6 $\pm$ 0.3 $\pm$ 0.1 $\pm$ 0.1 $\pm$ 0.1 $\pm$ 0.1 $\pm$ 0.1 $\pm$ 0.2 $\pm$ 0.1 - $\pm$ 0.2 $\pm$ 0.3 - $\pm$ 1.4 $\pm$ 0.7  
Tol2019-405(NE) - - - 7.4 286.0 14.9 - 30.1 24.3 - 6.1 3.2 2.8 - - - - 29.4 8.7 0.10
  - - - $\pm$ 1.3 $\pm$ 2.0 $\pm$ 1.5 - $\pm$ 2.8 $\pm$ 2.8 - $\pm$ 1.2 $\pm$ 0.9 $\pm$ 1.0 - - - - $\pm$ 4.6 $\pm$ 2.5  
Tol2019-405 - - - 7.7 286.0 17.4 - 36.0 29.9 - 6.9 - - - - - - 30.2 8.3 0.10
  - - - $\pm$ 1.6 $\pm$ 2.6 $\pm$ 1.9 - $\pm$ 2.3 $\pm$ 2.7 - $\pm$ 1.6 - - - - - - $\pm$ 6.4 $\pm$ 1.9  
Tol2138-397 - - - - 286.0 - - 14.8 7.5 - - 5.4 - - - - - 14.7 - 0.11
  - - - - $\pm$ 7.4 - - $\pm$ 0.8 $\pm$ 0.5 - - $\pm$ 0.4 - - - - - $\pm$ 2.8 -  
Tol2146-391 23.2 - - 3.4 286.0 5.5 - 11.0 7.5 4.5 8.5 2.9 2.6 - 1.5 2.4 - 28.2a - 0.12
  $\pm$ 1.0 - - $\pm$ 0.2 $\pm$188.6 $\pm$ 0.3 - $\pm$ 0.8 $\pm$ 0.5 $\pm$ 0.2 $\pm$ 0.5 $\pm$ 0.1 $\pm$ 0.1 - $\pm$ 0.3 $\pm$ 0.4 - $\pm$ 2.7 -  
MCG-05-52-065(E) - - - 25.5 286.0 59.1 5.6 67.4 46.5 - 8.4 - - - - - - 31.3 4.6 0.44
  - - - $\pm$ 2.8 $\pm$ 4.1 $\pm$ 2.9 $\pm$ 1.9 $\pm$ 2.8 $\pm$ 2.2 - $\pm$ 1.3 - - - - - - $\pm$ 3.6 $\pm$ 1.4  
MCG-05-52-065(W) - - - 24.1 286.0 89.4 - 88.8 69.8 - - - - - - - - 29.5 - 0.44
  - - - $\pm$ 4.5 $\pm$ 8.4 $\pm$ 6.7 - $\pm$ 8.7 $\pm$ 6.6 - - - - - - - - $\pm$ 4.5 -  
Tol2240-384 2.9 - - - 286.0 3.8 2.1 6.8 5.6 - 4.4 - - - - - 2.8 8.6 - 0.36
  $\pm$ 0.6 - - - - - $\pm$ 0.3 $\pm$ 0.4 $\pm$ 0.3 - $\pm$ 0.1 - - - - - $\pm$ 1.7 $\pm$ 3.2 -  
UM160(E) - - - 3.2 286.0 10.0 4.8 24.8 17.1 - 5.1 - - - - - - 13.6 - 0.26
  - - - $\pm$ 0.2 $\pm$ 3.6 $\pm$ 0.9 $\pm$ 1.6 $\pm$ 1.6 $\pm$ 0.5 - $\pm$ 0.4 - - - - - - $\pm$ 2.7 -  
UM160(W) - - - - 286.0 13.4 - 38.6 27.2 - - - - - - - - 23.6 - 0.26
  - - - - $\pm$ 1.6 $\pm$ 1.6 - $\pm$ 0.8 $\pm$ 1.4 - - - - - - - - $\pm$ 4.9 -  
UM166 - - - 17.4 286.0 58.3 - 34.4 31.7 - 6.2 - - - - - - 54.1a - 0.25
  - - - $\pm$ 1.6 $\pm$ 2.8 $\pm$ 1.7 - $\pm$ 2.3 $\pm$ 2.0 - $\pm$ 1.3 - - - - - - $\pm$ 5.8 -  
UM167 5.9 - 1.4 36.6 286.0 105.6 2.5 30.2 29.8 2.8 4.0 3.0 2.4 0.8 0.9 1.2 2.3 24.1 4.1 0.30
  $\pm$ 0.3 - $\pm$ 0.1 $\pm$ 1.1 $\pm$ 2.1 $\pm$ 0.6 $\pm$ 0.3 $\pm$ 0.5 $\pm$ 0.7 $\pm$ 0.3 $\pm$ 0.1 $\pm$ 0.2 $\pm$ 0.1 $\pm$ 0.1 $\pm$ 0.2 $\pm$ 0.2 $\pm$ 0.6 $\pm$ 2.8 $\pm$ 0.9  

a We have quoted the flux of [SIII]$\lambda$9532 Å instead of [SIII]$\lambda$9069 Å.


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