Fig. 5

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Extracted MIRI fluxes for the new object, shown together with STM predictions for two different η-values, which also correspond to different best-fit r, ∆, α observing geometries. The red line shows the η = 0.756 (pV = 0.05, Deff =km), the blue line the η = 1.0 (pV = 0.25, Deff = km) STM solution, and the green envelope all orbit solutions with χ2 < 1.55. The flux scale is given in μJy.
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