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Fig. 9

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Reconstructed properties of isolated Gaussian filaments. Top: Percentage of emission recovered along the entire radial profile vs. FWHM0 Different colors are used for the different data combination methods used: blue for the ALMA 12 m-alone, orange for the 12 m + 7 m, pink for the ALMA Feather, green for the ALMA MACF, and black for the ALMA 12 m + IRAM-30 m MACF. The grey dotted and dashed lines show θres(12m) and θMRS(12m), respectively. Middle: Intensity peak estimated from the Gaussian fit vs. FWHM0. Bottom: FWHM estimated from the Gaussian fit vs. FWHM0. The grey solid line shows the theoretical expectation. For comparison, the results for the radial profile shown in Fig. 8 with FWHM0 = 30 arcsec correspond to values close to θMRS(12 m).

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