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Fig. 4

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Band 7 (0.9 mm, top panels) and Band 4 (2.1 mm, bottom panels) comparison between dust continuum images from the ALMA observation and our synthetic observations obtained from the simulation with a final planet mass of 2.0 MJup after 4 × 104 yr, along with their residuals. The synthesized beam (0.050″ × 0.034″ for Band 7, 0.048″ × 0.032″ for Band 4, FWHMs) is shown in the bottom-left corner of each image. The contours in the residuals represent the 5σ and −5σ flux levels, respectively, for Band 7 and Band 4.

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