Table 1: Summary of the Lorentzian coefficients and integrated flux resulting from fitting Lorentzian profiles to a pixel (Labelled D) on the head of $\Pi _1$.
Emission Line Peak Wavelength Peak flux FWHM Intensity
$\lambda$ ($\mu $m) $\lambda$ ($\mu $m) (Jy) ($\delta$$\lambda$) (W m-2)
UIB 6.2 6.26 $4.4\times 10$-1 $2.9 \times 10^{-1}$ $2.0\times 10^{-27}$
[ArII] 7.0 6.95 $ 1.7 \times 10^{-1}$ $2.2 \times 10^{-1}$ $6.0 \times 10^{-28}$
UIB 7.7 7.69 $8.1 \times 10^{-1}$ $6.5 \times 10^{-1}$ $8.25 \times 10 ^{-27}$
UIB 8.6 8.57 $3.4 \times 10^{-1}$ $5.7 \times 10^{-1}$ $3.05 \times 10 ^{-27}$
[ArIII] 9.0 9.01 $9.0\times 10^{-2}$ $1.6 \times 10^{-1}$ $2.5 \times 10^{-28}$
UIB 11.3 11.30 $8.6\times 10^{-1}$ $3.9 \times 10^{-1}$ $5.25\times 10^{-27}$
UIB & [NeII] 12.8 12.81 $10.1 \times 10^{-1}$ $3.7 \times 10^{-1}$ $5.85 \times 10^{-27}$
[NeIII] 15.6 15.56 $6.6 \times 10^{-1}$ $4.5 \times 10^{-1}$ $4.65 \times10^{-27}$


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