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Fig. 9

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Comparison between the 400 mas contrast predictions made by the model of this work vs. the current (as of the publication of this paper) ETC on the ESO website. The ETC options were set to match the observed mode of the model developed here: DBH23 filter with coronagraph. Both the ETC and model were set with no neutral densities, exptime ~64 s, DIT ≤ 64 s, without differential imaging and considered a spectral type of around GV2.

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