Fig. 1

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SPHERE-IRDIS observations of the disk around HD 129590. Left panel: DI-sNMF total intensity reduction. The detection of the birth ring and the presence of a faint arc are highlighted by two arrows in the left panel. The inset in the left panel also shows the DI-sNMF reduction with the birth ring (best-fit from Olofsson et al. 2022b) and the arc highlighted. Top-right panel: PCA total intensity reduction. Bottom-right panel: Qϕ polarized intensity reduction. The location of the birth ring is shown in the Qϕ image as a solid black line. For each image, the central mask has a radius of 0.125′′, and the color scale is linear. North is up, east is left, and the pixel scale is of 12.26 mas.
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