Table 1: Fluxes (in units of 10^-15 erg s^-1 cm^-2) of the emission lines detected in the spectrum acquired in Loiano. Values are corrected for Galactic absorption.
Line Flux

[O II] $\lambda$ 3727 $1.51 \pm 0.15$

H $_\beta$ $1.1 \pm 0.2$

[O III] $\lambda$ 5007 $0.35 \pm 0.09$

[N II] $\lambda$ 6548 $0.90 \pm 0.18$

H $_\alpha$ $6.4 \pm 0.3$

[N II] $\lambda$ 6583 $2.90 \pm 0.15$

[S II] $\lambda$ 6716 $0.63 \pm 0.13$

[S II] $\lambda$ 6731 $0.86 \pm 0.17$

**Table 1:** Fluxes (in units of 10^-15 erg s^-1 cm^-2) of the emission lines detected in the spectrum acquired in Loiano. Values are corrected for Galactic absorption.
Line	Flux
[O II] $\lambda$ 3727	$1.51 \pm 0.15$
H $_\beta$	$1.1 \pm 0.2$
[O III] $\lambda$ 5007	$0.35 \pm 0.09$
[N II] $\lambda$ 6548	$0.90 \pm 0.18$
H $_\alpha$	$6.4 \pm 0.3$
[N II] $\lambda$ 6583	$2.90 \pm 0.15$
[S II] $\lambda$ 6716	$0.63 \pm 0.13$
[S II] $\lambda$ 6731	$0.86 \pm 0.17$

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