Fig. 6
The spectral energy distribution of object 1 (left panel) and 2 (right panel). The Kurucz model for a B0 star is shown for object 1. The de-reddened slope of the (photospheric) SINFONI spectra provides an additional consistency check for the classification method and the derived extinction. The SOFI, 2MASS and IRAC detections are marked with triangles, squares and crosses respectively.
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