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Fig. 17

image

Detection limits versus stellar inclination for the correlation-based (four top panels) and the LPA (four bottom panels) methods. The detection limits are displayed for different samplings and for different noise levels (black: no added noise, red: 0.01 m s-1 noise, green: 0.05 m s-1 noise and blue: 0.1 m s-1 noise). Solid line: detection limits computed in case 2. Dashed line: detection limits computed in case 1.

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