Table 3: Heliocentric velocities and line widths (FWHM) (separated by |) in km s^-1 as well as mean d-parameter as derived from d-Lorentz fits for the central row.
line ESO 103-G035 TXS 2226-184 IC 1481

H $\beta$ 4011|479 7498|446 6138|445

[O III] $\lambda$ 5007 4045|539 7553|397 6123|405

[O I] $\lambda$ 6300 4063|584 7564|676 6087|405

H $\alpha$ 4046|504 7486|327 6098|392

[N II] $\lambda$ 6583 4046|443 7486|526 6097|416

[S II] $\lambda$ 6731 4059|411 7515|389 6107|363^a

mean $4045\pm8 \vert 493\pm26$ $7517\pm14 \vert 460\pm51$ $6108\pm7 \vert 404\pm11$

mean d $1.6\pm0.2$ $1.1\pm0.1$ $1.4\pm0.3$

^a [S II] $\lambda$ 6731 was truncated by telluric absorption bands and thus, [S II] $\lambda$ 6716 was used instead.

**Table 3:** Heliocentric velocities and line widths (*FWHM*) (separated by |) in km s^-1 as well as mean d-parameter as derived from d-Lorentz fits for the central row.
line	ESO 103-G035	TXS 2226-184	IC 1481
H $\beta$	4011\|479	7498\|446	6138\|445
[O III] $\lambda$ 5007	4045\|539	7553\|397	6123\|405
[O I] $\lambda$ 6300	4063\|584	7564\|676	6087\|405
H $\alpha$	4046\|504	7486\|327	6098\|392
[N II] $\lambda$ 6583	4046\|443	7486\|526	6097\|416
[S II] $\lambda$ 6731	4059\|411	7515\|389	6107\|363^a
mean	$4045\pm8 \vert 493\pm26$	$7517\pm14 \vert 460\pm51$	$6108\pm7 \vert 404\pm11$
mean d	$1.6\pm0.2$	$1.1\pm0.1$	$1.4\pm0.3$

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