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Fig. 6.

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Spatially resolved outputs of Bagpipes run obtained by fixing redshift of all pixels in the system at z = 5.7. The segmentation map obtained from SEP is used to identify the physical regions associated with each of the three main components (A, B, and C) identified in Fig. 2. In the three plots, from left to right, we report the spatial distribution of stellar mass, SFR, and AV, respectively. The pixel size used in this map accounts for the convolution with the PSF in each NIRCam band. In this figure, we adopt the F444W PSF as a reference. In each panel, we report the integrated values of the physical properties obtained for the three separate components. Contours of the F444W flux emission are reported as solid lines in each plot.

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