**Table 5:** IC 5117 fluxes and equivalent widths.
Wavelength	Ion	log [Flux]	log [ EW]	Number of
(Å)		(erg cm^-2 s^-1)	(Å)	observations
3705.00	HeI	$-13.661\pm0.155$	$0.810\pm0.211$	2
3712.75	HeII	$-13.656\pm0.032$	$0.806\pm0.122$	2
3726.19	[OII]	$-12.337\pm0.004$	$1.768\pm0.023$	2
3734.37	H₁₃	$-13.340\pm0.088$	$0.493\pm0.261$	2
3750.15	H₁₂	$-13.254\pm0.021$	$1.217\pm0.179$	2
3770.63	H₁₁	$-13.156\pm0.053$	$1.502\pm0.051$	2
3797.90	H₁₀	$-13.014\pm0.005$	$1.651\pm0.175$	2
3819.70	HeI $^{\star}$	$-13.700\pm0.001$	$0.846\pm0.019$	2
3835.38	H₉	$-12.836\pm0.015$	$1.767\pm0.016$	2
3868.71	[NeIII]	$-11.503\pm0.002$	$2.871\pm0.071$	4
3889.05	H₈	$-12.482\pm0.013$	$1.955\pm0.098$	3
3967.41	[NeIII]	$-11.844\pm0.003$	$2.781\pm0.100$	4
4068.91	CIII	$-12.991\pm0.002$	$1.382\pm0.063$	2
4101.74	H $\delta$	$-12.179\pm0.012$	$2.387\pm0.134$	4
4340.47	H $\gamma$	$-11.876\pm0.003$	$2.581\pm0.112$	4
4363.21	[OIII]	$-12.191\pm0.010$	$2.262\pm0.077$	4
4387.93	HeI	$-13.878\pm0.152$	$0.637\pm0.111$	2
4471.68	HeI	$-12.798\pm0.001$	$1.783\pm0.024$	2
4634.14	NIII	$-13.576\pm0.036$	$0.695\pm0.333$	4
4640.64	NIII	$-13.215\pm0.013$	$0.947\pm0.291$	4
4685.71	HeII	$-12.359\pm0.001$	$2.106\pm0.075$	4
4713.38	HeI $^{\star}$	$-13.036\pm0.003$	$1.419\pm0.082$	4
4724.30	[NeIV]	$-14.154\pm0.057$	$0.270\pm0.163$	4
4740.18	[ArIV]	$-12.661\pm0.001$	$1.813\pm0.029$	4
4861.20	H $\beta$	$-11.380\pm0.020$	$3.032\pm0.006$	6
4921.93	HeI	$-13.180\pm0.050$	$1.019\pm0.063$	4
4958.52	[OIII]	$-10.629\pm0.023$	$3.270\pm0.124$	5
5007.57	[OIII]	$-10.131\pm0.017$	$3.743\pm0.026$	2
5191.80	[ArIII]	$-14.152\pm0.159$	$0.151\pm0.004$	4
5197.90	[NI]	$-13.852\pm0.019$	$0.488\pm0.116$	4
5411.52	HeII	$-13.276\pm0.042$	$1.107\pm0.019$	4
5517.72	[ClIII]	$-14.084\pm0.025$	$0.209\pm0.072$	4
5537.89	[ClIII]	$-13.544\pm0.005$	$0.801\pm0.007$	4
5754.59	[NII]	$-12.653\pm0.006$	$1.650\pm0.005$	2
5875.97	HeI	$-11.909\pm0.024$	$2.325\pm0.109$	9 $\dagger$
6300.30	[OI]	$-12.177\pm0.026$	$1.881\pm0.050$	8 $\dagger$
6312.10	[SIII]	$-12.606\pm0.039$	$1.437\pm0.011$	9 $\dagger$
6363.77	[OI]	$-12.656\pm0.024$	$1.453\pm0.038$	9 $\dagger$
6548.05	[NII]	$-11.733\pm0.032$	$1.612\pm0.116$	9 $\dagger$
6562.85	H $\alpha$	$-10.524\pm0.002$	$2.887\pm0.223$	3 $\dagger$
6583.45	[NII]	$-11.272\pm0.008$	$2.312\pm0.184$	7 $\dagger$
6678.15	HeI	$-12.366\pm0.003$	$1.743\pm0.007$	9 $\dagger$
6716.47	[SII]	$-12.958\pm0.006$	$1.151\pm0.015$	9 $\dagger$
6730.85	[SII]	$-12.612\pm0.008$	$1.495\pm0.037$	9 $\dagger$
7065.71	HeI	$-11.860\pm0.009$	$2.200\pm0.044$	9 $\dagger$

$\textstyle \parbox{10cm}{ $^\star$\space HeI lines are a double blend.\\ $\dagger$\space Measured values were determined from two nights of observation. }$

Source LaTeX | All tables | In the text

	1 Introduction
	2 Observations and reduction
	3 Morphology and sizes
	4 Analysis
	5 Discussion and conclusions
	References