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Fig. 6

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Detection limits in the SPIRou RV time series. Left panels: upper limits in m s−1 of the semiamplitude K of the sinusoidal signal. Right panels: upper limits in terms of the projected mass m sin(i). Objects with a projected mass above the limit are ruled out by the observed GLS periodogram with 99% (light blue) and 75% (dark blue) confidence levels (see text for details). Upper panels: upper limits for periods from 0.8 to 1000 days. Lower panels: zoom on the 0.8 to 10 day range. The red star indicates the location of the 0.24 MJ (76 M) planet in corotation claimed by Tuomi et al. (2018). The blue triangle shows the planet-mass equivalent (27 M) of the stable RV component in Kossakowski et al. (2022). Both are ruled out by the SPIRou data with a confidence higher than 99%.

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