Figure C5.
Distribution of the best-fitting GP hyperprameters obtained by modelling 270-d chunks of HARPS-N solar RV. The dotted blue line in the top panel shows the best-fitting parabola to the GP amplitudes. The three seasons defined in Table 2 (i.e. end of Cycle 24, solar minimum and start of Cycle 25) are delimited by the vertical dashed lines.

Distribution of the best-fitting GP hyperprameters obtained by modelling 270-d chunks of HARPS-N solar RV. The dotted blue line in the top panel shows the best-fitting parabola to the GP amplitudes. The three seasons defined in Table 2 (i.e. end of Cycle 24, solar minimum and start of Cycle 25) are delimited by the vertical dashed lines.

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