Table 6: Fluxes of the most prominent emission lines of the galaxies in the comparison sample. The unit is 10^-19 W m^-2. Positive numbers are emission lines and negative are absorption lines. Only galaxies with detected emission lines are included.
ESO-nr H $\alpha$ H $\beta$ H $\gamma$ [OII] [O III] [N II] [S II] [S II]

6563 4861 4340 3727 5007 6584 6717 6731

015- G05 9.9 -5.1 -2.3 - - 23 - -

026- G04 - -1.1 - - - 11 - -

027- G14 35 5.4 - - - 14 3.9 1.9

048- G25 7.9 - - - - 1.2 - -

074- G26 17 - - - - 6.8 - -

106- G08 10 - - - - 5.5 - -

151- G43 2.8 - - - - 0.3 - -

153- G33 3.5 - - - - 2.9 1.1 0.8

201- G12 13 - - - - - - -

200- G36 22 -4.6 - - - 12 4.3 2.9

240- G12 21 3.6 - 14 5.9 7.0 7.6 2.7

287- G21 8.7 - - - - - - -

293- G04 11 - -8.1 24 3.1 3.3 2.5 1.9

299- G07 269 30 - - - 128 24 21

299- G20 269 33 13 - 5.0 139 22 20

303- G14 79 13 - 11 7.6 48 11 7.6

340- G07 6.0 - - - 6.9 9.0 - -

341- G32 4.8 - - - - - - -

345- G49 11 -2.0 - - - 4.4 - -

**Table 6:** Fluxes of the most prominent emission lines of the galaxies in the comparison sample. The unit is 10^-19 W m^-2. Positive numbers are emission lines and negative are absorption lines. Only galaxies with detected emission lines are included.
ESO-nr	H $\alpha$	H $\beta$	H $\gamma$	[OII]	[O III]	[N II]	[S II]	[S II]
	6563	4861	4340	3727	5007	6584	6717	6731
015- G05	9.9	-5.1	-2.3	-	-	23	-	-
026- G04	-	-1.1	-	-	-	11	-	-
027- G14	35	5.4	-	-	-	14	3.9	1.9
048- G25	7.9	-	-	-	-	1.2	-	-
074- G26	17	-	-	-	-	6.8	-	-
106- G08	10	-	-	-	-	5.5	-	-
151- G43	2.8	-	-	-	-	0.3	-	-
153- G33	3.5	-	-	-	-	2.9	1.1	0.8
201- G12	13	-	-	-	-	-	-	-
200- G36	22	-4.6	-	-	-	12	4.3	2.9
240- G12	21	3.6	-	14	5.9	7.0	7.6	2.7
287- G21	8.7	-	-	-	-	-	-	-
293- G04	11	-	-8.1	24	3.1	3.3	2.5	1.9
299- G07	269	30	-	-	-	128	24	21
299- G20	269	33	13	-	5.0	139	22	20
303- G14	79	13	-	11	7.6	48	11	7.6
340- G07	6.0	-	-	-	6.9	9.0	-	-
341- G32	4.8	-	-	-	-	-	-	-
345- G49	11	-2.0	-	-	-	4.4	-	-

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