Fig. B.1
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Top: Image reconstruction of the 2.2 μm continuum towards G282.2988, G287.3716, G301.8147, and G034.8211 using WISARD. Bottom: Image reconstruction of the 2.2 μm emission towards G034.8211 using three different algorithms (WISARD, BSMEM, and MIRA). In addition, we present the image resulted independently by applying a simple geometric model (bottom left). The white contours represent the reconstructed image of the calibrator star for evaluation of the achieved spatial resolution.
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