Fig. 15
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Examples of ALMA images of CO(5−4) and [CII] emission from high-z star-forming galaxies PACS-787 (top) and HZ7 (bottom). Left: ALMA dirty image. Right: residual map with the primary disk component modeled by a single Spergel profile subtracted. The image size is 3.5″ × 3.5″. The synthesized beam (0.15″ × 0.14″ and 0.36″ × 0.35″ for PACS-787 and HZ7, respectively) is presented in the bottom left of the left panels. Contours start from ±2σ and increase by a factor of 1.5.
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