Fig. B.1
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Noise-free simulations of isolated objects with FWHM0=15 arcsec and different aspect ratios AR. From left to right: AR=1 (core), 2, 5, and ∞ (infinite filament). From top to bottom: Reference model (panel A), and simulated ALMA 12 m-alone (panel B), ALMA 12m + 7m (panel C), ALMA Feather (panel D), ALMA MACF (panel E), and ALMA 12 m + IRAM-30 m MACF (panel F) observations, respectively.
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