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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 | ||
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| 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% | |
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| 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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