Fig. 3
Top panel: precise optical Doppler measurements of GJ 1148 from HIRES (blue triangles) and CARMENES (red circles) modeled with a two-planet model. Bottom panels: phase-folded planetary signals fitted to the data. Compared to Trifonov et al. (2018a), there are 24 additional CARMENES RVs, and the HIRES data were corrected for small systematics.The data uncertainties include the estimated RV jitter.
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