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Fig. 6

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SPHERE total-intensity reduction of the H- and K-band data sets (with ADI and iRDI as in the previous figure). Total intensity observations are sensitive to thermal emission of embedded planets. We show the ALMA continuum data from Sierra et al. (2024) as the contour overlay (3σ, 4σ, and 10σ contours shown). The yellow arrows indicate tentative point sources detected with SPHERE in the H and K bands. Both detections are directly adjacent to a 3σ compact continuum signal detected with ALMA in the disk gap.

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