Table 7: Parity forbidden lines observed in AG Peg.
Spectrum Ionization $\lambda_{\rm lab}$ (vac). Shifta Width Transition Aij    Noteb
  (eV) (Å) (km s-1) (km s-1)   (s-1)     
[Fe VI] 75.01 1957.28 bl bl 3d3 2G7/2-3d3 2D15/2 0.91     $\uparrow$
    1944.30 17 20 3d3 2G7/2-3d3 2D13/2 12         $\uparrow$
[Mg V] 109.25 2928.0  bl bl 2p4 3P1-2p4 1D2 0.55     $\uparrow$
    2783.50 bl bl 2p4 3P2-2p4 1D2 1.90     $\uparrow$
    1324.45 45 20 2p4 3P1-2p4 1S0 23         $\uparrow$
[Ne V] 97.08 2975.66 152 51 2p2 1D2-2p2 1S0 2.60     $\uparrow$
    1575.18 124 84 2p2 3P1-2p2 1S0 4.20     $\uparrow$
[Ar V] 59.81 2692.02 41 40 3p2 3P1-3p2 1S0 6.80     $\uparrow$
[Ne IV] 63.46 2425.23 -6 18 2p3 4S3/2-2p3 2D5/2 0.00018 $\leftrightarrow$
    2422.60 -7 17 2p3 4S3/2-2p3 2D3/2 0.0053  $\leftrightarrow$
    1601.67 bl bl 2p3 4S3/2-2p3 2P1/2 0.53     $\leftrightarrow$
    1601.50 bl bl 2p3 4S3/2-2p3 2P3/2 1.33     $\leftrightarrow$
[Ne III] 40.96 1814.63 21 40 2p4 3P1-2p4 1S0 2.20     $\leftrightarrow$
[O III] 35.12 2321.66 49 25 2p2 3P1-2p2 1S0 0.22     $\downarrow$
a $\frac{\lambda_{\rm lab} - \lambda_{\rm obs}}{\lambda_{\rm lab}} \cdot 3 \times 10^{5}$; b $\downarrow$ = Only observed before 1986, $\leftrightarrow$ = observed throughout 1978 to 1995, $\uparrow$ = only observed after 1986,
bl = blend.

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