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Fig. 4


Theoretical fitting of the Albus SEDs. Solid lines represent the Kurucz models that best fits the observational data. Filled (blue) and open (red) circles indicate the photometric data used for the fit and the synthetic GRIZ photometry data used for control, respectively. The thin (green) line in the second panel depicts the ultraviolet FUSE spectra of Albus 5.

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