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Fig. 2


Time series of each physical RV component in our L 98-59 models. Left column: raw RVs (top panel), RV activity (second panel), three L 98-59 planets (third, fourth, and fifth panels), and RV residuals (bottom panel). The RV activity model depicted is the mean GP function along with its ± 1σ uncertainty in the surrounding shaded region. The L 98-59c and d planet curves are their MAP Keplerian orbital solutions while the L 98-59b curve is its median Keplerian orbit. Right column: the GLSP corresponding to each RV component.

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