Protoplanetary disk insights from the first ERIS/vAPP survey at 4 μm

Open Access

Fig. D.21

Recovered flux from aperture photometry for the six outer synthetic planets ( $1_{\cdot}^{''} 0$ $\[1^{\prime\prime}_\cdot0\]$ ) and the four inner planets ( $0_{\cdot}^{''} 25$ $\[0^{\prime\prime}_\cdot25\]$ ). The vertical gray bands indicate the transition regions for the PDS 70 observations. The colors represent different analysis techniques: blue for cADI, green for ADI-PCA with three subtracted PCs, and red for ADI-PCA with five subtracted PCs.

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