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Fig. 5


Four examples of results from experiment 3. The continuous line shows the best (mode) TLUSTY SED output from CHORIZOS and the green stars are the associated synthetic photometry (from right to left, F336W, F438W, F555W, F656N, F814W, J, H, and Ks). The blue points with error bars (horizontal for indicative filter extent, vertical for uncertainty) show the input photometry used for the fit. The red points with error bars show the input F656N filter (not used for the fit). The vertical axes are in AB magnitudes (Laidler et al. 2005).

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