Fig. A.1.
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Same as Fig. 3, but for SDSS J1020+6023. Dust emission with T ∼ 1700 K (dashed blue line) is added to the near-IR magnitudes to better match the composite because the near-IR composite from Glikman et al. (2006) has a stronger IR emission than SDSS J1020+6023. The correctional multi-band magnitudes of SDSS J1020+6023 from the 2MASS and WISE surveys are presented by open orange squares.
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