Fig. 8
The azimuthally averaged intensity profile of G310.0135 (upper circles) compared to a PSF standard (lower circles) and the models that fit the SED of this object from Mottram et al. (2011, dashed lines). The solid line is the radial profile of the model of Kraus et al. (2010). The error bars represent the rms within a given annuli and thus represent an upper limit on the uncertainty in the flux distribution.
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