Left: ESPRESSO RVs (blue dots), model components (GP: red, Keplerian: grey), and median model (black) for the juliet 2c model. The error bars show the RV errors and jitter added in quadrature. The instrumental systemic velocity has been subtracted. The GP fit to the FWHM is also shown (dotted green line) for comparison. Centre and right: phase-folded RVs and median Keplerian model for the inner candidate planet TOI-2322.02 (centre) and outer candidate planet TOI-2322.01 (right).