Fig. A.1.
Large-scale ALMA 1.3 mm continuum emission maps of NGC 1365 with a field of view of 25″×25″ (upper panel) and NGC 1808 with a field of view of 15″×15″ (lower panel). The contours are shown in a linear scale. The filled cyan ellipses represent the synthesized beam sizes and orientations. We show the tentative identification of some mid-IR emitting sources detected by Galliano et al. (2005).
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