Fig. 5
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Fluxes of hypothetical 2RIo moons around e Eridani b. The black lines are the 10 σ and 10 000 s detection limits for MIRI (Glasse et al. 2015). The planet model (Spiegel & Burrows 2012) is shown in gray. The red and purple lines correspond to the black bodies of a 270 and 470 K 2 × RIo exomoon, and the yellow dashed line corresponds to the black body of the star.
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