Fig. 16
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Mono and multi-epoch 5σ contrast curves of the IRDIS (left) and IFS (right) datasets of HR 8799 in ASDI mode with flat spectral priors. The multi-epoch contrast is computed as a function of the separation assuming face-on circular orbits and a source flux constant over the epochs. The 5σ contrasts found in Wahhaj et al. (2021) were extracted and overplotted for comparison.
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