HARPS-N and HPF RVs of GJ 1151. In panel (a), we show the Bayes factor periodogram of the combined HARPS-N+HPF RV series, along with the corresponding window function. The section of the periodogram near the 2.02-day peak is detailed in panel (b). In panel (c), we show the time-series RVs with the Keplerian model to the planet overlaid. The five earliest HPF RVs are not shown to facilitate visibility. In panel (d), we show all RVs phased to the 2.018-day period of the planet. The planet model is shown as a black curve, with 1σ, 2σ, and 3σ uncertainty regions shaded in gray. RVs and associated activity indicators are available in machine-readable format.
(The data used to create this figure are available.)