Comparison of FUSE and HST (STIS and NICMOS) observations with our final model. A reddening of EB − V = 0.0005 is applied. The low-resolution (LR) STIS+NICMOS observation vanishes behind the model SED due to the line width. Therefore, we plotted the observed spectrum twice, one shifted by Δlog fλ = −0.2 for clarity. U,R,I (Landolt & Uomoto 2007), B,V (Høg et al. 2000), J,H, and K (Cutri et al. 2003) fluxes (converted from brightnesses using values given by Heber et al. 2002) are shown for comparison.
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