Table 2: Line intensities relative to H ${\beta }$ , in apertures A, B and C of slit 1, and integrated in a 6 $^{\prime \prime }$ aperture in slit 2, that avoids the companion galaxy G1.
Line $\lambda~(\AA)$ A B C Slit 2

Ne V (3346) 0.26 - 0.15 -

Ne V (3426) 0.64 - 0.57 -

O II (3727) 1.46 3.42 2.06 -

Ne III (3869) 0.94 1.47 0.86 -

H ${{\rm 8}}$ (3889) 0.12 - 0.21 -

Ne III (3967) 0.44 - 0.34 -

H ${{\rm\delta}}$ (4101) 0.27 - 0.17 -

H ${{\rm\gamma}}$ (4341) 0.46 - 0.34 -

O III (4363) 0.32 - 0.29 -

He II (4686) 0.21 - 0.22 -

H ${{\rm\beta}}$ (4861) 1.00 1.00 1.00 1.00

O III (4959) 4.08 2.18 3.43 2.44

O III (5007) 12.14 6.72 10.12 4.40

H ${{\rm\alpha}}$ (6563) 4.10 8.95 3.88 3.38

N II (6583) 1.52 6.32 1.53 1.29

S II (6717) 0.44 0.53 0.41 0.34

S II (6731) 0.37 0.34 0.37 0.36

**Table 2:** Line intensities relative to H ${\beta }$ , in apertures A, B and C of *slit 1*, and integrated in a 6 $^{\prime \prime }$ aperture in *slit 2*, that avoids the companion galaxy G1.
Line	$\lambda~(\AA)$	A	B	C	Slit 2
Ne V	(3346)	0.26	-	0.15	-
Ne V	(3426)	0.64	-	0.57	-
O II	(3727)	1.46	3.42	2.06	-
Ne III	(3869)	0.94	1.47	0.86	-
H ${{\rm 8}}$	(3889)	0.12	-	0.21	-
Ne III	(3967)	0.44	-	0.34	-
H ${{\rm\delta}}$	(4101)	0.27	-	0.17	-
H ${{\rm\gamma}}$	(4341)	0.46	-	0.34	-
O III	(4363)	0.32	-	0.29	-
He II	(4686)	0.21	-	0.22	-
H ${{\rm\beta}}$	(4861)	1.00	1.00	1.00	1.00
O III	(4959)	4.08	2.18	3.43	2.44
O III	(5007)	12.14	6.72	10.12	4.40
H ${{\rm\alpha}}$	(6563)	4.10	8.95	3.88	3.38
N II	(6583)	1.52	6.32	1.53	1.29
S II	(6717)	0.44	0.53	0.41	0.34
S II	(6731)	0.37	0.34	0.37	0.36

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