Fig. B.11

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Comparison of dust emission maps between the perfect resolution scenario and a case that accounts for the PSFs of the respective instruments for the limited filter configuration used in Section 4.3. The red circle in the bottom row panels indicates the FWHM of the respective PSFs. We note that this example is based on the assumption that all considered telescopes share the same pixel size, matching our simulation resolution at a query distance of d = 397 pc.
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