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Fig. 4.
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Distributions in NPIC (PLATO noise from the PIC1.1.0, in ppm h1/2) of MS stars with M ≤ 1.2 M⊙ from the P5 sample with an expected positive detection of solar-like oscillations with a probability higher than 99% assuming 730 days of observations. Conditions are (1 LOP, δνenv = νmax/2), BOL (blue), EOL(red).
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