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Fig. 10

image

Planet detection regions for a star of the sample derived using the RV rms analysis. Red area: the rms of the simulated RV values is more than three times higher than the real measurement error, thus all potential planets can be detected. Blue ruled area: the rms of the simulated RV values is lower than three times the real measurement errors. Potential planets in this mass-period range cannot be detected with our observations.

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