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Table 2

Flux loss from two fake planets after ADI reduction. The flux loss is computed by aperture photometry with a radius of 0.75 × FWHM. mcADI is a technique introduced and commented on Sect. 6.2.

Δθ = 77.5° Δθ = 23°
cADI mcADI rADI Nδ = 1.5 rADI Nδ = 3 cADI mcADI rADI Nδ = 1.5 rADI Nδ = 3

Planet 1 without disk 0.2% 0.3% 1.4% 0.2% 8.5% NA 2.7% 2.6%
with disk 27.1% 4.3% 100% 23.5% 100% NA 100% 99.7%

Planet 2 without disk 0.1% 0.3% 1.4% 1.2% 3.1% 12.9% 2.7% 0.7%
with disk 4.4% 1.8% 100% 100% 63.0% 21.1% 45.0% 100%

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