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Fig. 7

image

Left: detection probabilities of planets around β Pictoris using all available HCI data and RV pulsation-subtracted data. Right: detection probabilities of planets around β Pictoris using allavailable HCI data and RV data which were pulsation-subtracted and corrected from β Pictoris b and c. Various levels of probabilities are considered. The two known planets are indicated.

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