Radial velocity measurements of TOI-2095 taken with CARMENES. (a): RV time series and best-fitting model (blue line) including red noise. The plotted RV model was computed using the median values of the posterior distribution for each fitted parameter. The shaded area around the blue line represent the 1σ uncertainty levels of the fitted model. (b): residuals of the fit after subtracting the two planet models. (c) and (d): phase-folded RV measurements after subtracting the red noise and best-fit model (blue line).