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Fig. A.2


Spectral energy distribution of our program stars compared to the final, reddened models (red graphs). Models of WD 0111+002, and PG 0109+111 were normalized to the 2MASS H magnitude and that of PG 1707+427 to the SDSSz magnitude. Magnitudes from GALEX, SDSS, and 2MASS are plotted in blue with their error bars.

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