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Fig. 5.


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SED of VPMS J1708+4332 based on reddening corrected photometric data from VPMS, SDSS, 2MASS, and WISE (symbols). The error bars are usually smaller than the symbol size. The downward error is an upper limit from Galex in the near-UV. The SWIRE template for bright quasars (Polletta et al. 2007) has been over plotted (blue), redshifted into the observer frame, and scaled to the observed SED in the near-IR.

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