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Table 1:

Emission line identification and fluxes, relative to $F_{\rm H\beta }=100$.

Identification
$\lambda [\AA]$ $F_{\rm obs}$
     
I 4340.5 18
  4363.2 $^\star$
He  II 4685.7 26
I 4861.4 100
  4958.9 24
  5006.8 81
He  II 5411.5 5
  5720.9 11
He  I 5875.6 80
/[Fe  VII] 6086 26

[O  I]

6300.3 11

[S  III]

6312.1 4

I

6562.8 5500:

[N  II]

6583.4 60:

He  I

6678.2 55

[S  II]

6716.4 5

[S  II]

6730.8 4

Raman

6825 19

He  I

7065 218

Raman

7082 6

[Ar  III]

7135.8 20

[Fe  II]

7155.1 11

[Fe  II]

7172.0 9

[Ar  IV]

7236.0 4

He  I

7281.4 21

[O  II]

7319 16

[O  II]

7330 13

Notes.  $^{(\star)}$ Marginal detection; (:) uncertain flux because of blending.


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