Table 2: Observed wavelengths, equivalent widths, and FWHM of all identified emission lines in the 2002 and 2003 spectrum of TV Ret. For 2003 the line flux is also given. Note that the uncertainty of the line flux describes the uncertainty of the relative flux in the line and does not include the photometric error. The line flux has been dereddened using the reddening laws for H II regions and for AGNs (see text for details).
  September 2003         November 2004
Transition $\lambda_{\rm obs}$ [nm] -W [nm] F [10-18 W m-2] $F_{\rm SB~dered}$ $F_{\rm AGN~dered}$ $ 100\cdot F_{\rm SB~dered} / F_{\rm H\beta}$   $\lambda_{\rm obs}$ [nm] -W [nm]

H$_\alpha$		 719.47 46.0 3.51(3) 4.55 3.85 285(10)   719.42 46.1
H$_\beta$ 532.97 10.5 1.08(2) 1.60 1.24 100(4)   533.16 9.0
H$_\gamma$ 475.97 3.5 0.46(2) 0.72 0.54 45(3)   476.14 3.4
H$_\delta$ 449.76 1.8 0.26(5) 0.42 0.31 26(6)   450.01 1.4
H$_\epsilon$ 434.94 1.8 0.26(2) 0.42 0.31 26(3)   435.48 1.2
H8 425.83             426.68  
[S II]: 673.1 737.81 3.1 0.24(2)     15(2)   737.58  
[S II]: 671.7 736.36 3.7 0.29(2) 0.68 0.58 18(2)   736.20 6.8
[N II]: 658.4 721.70 3.6 0.28(3) 0.36 0.31 23(3)   721.64 3.9
[O I]: 630.0(1) 691.20 2.3 0.17(2) 0.22 0.19 14(2)     1.6
He I: 587.56 644.12 2.2 0.20(2) 0.27 0.22 17(2)   644.20 2.0
[O III]: 500.7 548.95 47.2 5.23(2) 7.61 5.97 477(15)   549.04 50.4
[O III]: 495.9 543.69 16.0 1.73(2) 2.53 1.98 159(6)   543.82 17.1
[O III]: 436.3 478.53 0.6 0.07(1) 0.11 0.08 7(1)   478.57 0.5
[Ne III]: 386.8 423.44 3.1 0.48(3) 0.78 0.57 49(4)   424.42 3.0
[O II]: 372.7           169(15)   408.93 16.2
$\textstyle \parbox{17.5cm}{ (1): Blend of several O~I lines.}$

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