Extended Data Fig. 2: Radial velocity data modeled with Keplerian planet signal and stellar activity with Gaussian Process.
From: An adolescent and near-resonant planetary system near the end of photoevaporation
(a) An overview of RV analysis of TOI-2076 with a Gaussian process (GP) activity model over the combined HIRES (orange triangle), APF (blue circle), and HARPS (green diamond) RV series of TOI-2076, overlaid with mean prediction from GP activity model (black line). The dark and light gray region show the 1σ and 2σ uncertainty band of GP model. (b)RV residuals after subtracting the activity and planetary signals. Legends are the same as those in panel a. (c-d) zoom-in view of GP model at two observing seasons. Legends are the same as those in panel a.
