Fig. D.7.
Results of BeeP analysis for 3C 273. See the caption of Fig. 7 for a full description. As in the previous figure, this is a non-thermal source, and BeeP also obtains very poor results (though not as extreme as in the previous case). The flux density of the source in the IRIS map is highly anomalous, but also has very low S/N ratio with respect to the well-determined background.
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