Fig. 7

Fitting of the TPN spectra with ISL model spectrum. The upper panel
is for the bright rim. The observed spectrum is shown as a histogram (thick
black line). The upper and the lower continuous thin line in black show ISL model
spectra for the bright rim and the sky positions, respectively. Their difference,
the red continuous line, is the fit. The parameters used for the model spectrum were
mag and
C5000 = 0.66. The residuals observation-minus-fit are
shown as histogram (in red), shifted down by 20 units. The lower panel
shows the core. Same as for the rim but the parameters used for the model
fit were
mag and
C5000 = 0.33.
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