Fig. 4
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High temperature cases: minimum integration times necessary for detection against the planet’s emission temperature. The dashed lines represent the results for a Solar-sized star at 1 AU, while the solid lines are for M-dwarfs at 0.13 AU. The associations are respectively at distances of 37 pc (β Pictoris, red), 53 pc (TW Hydrae, blue), and 94 pc (η Chamaeleontis, green).
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