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Observational and Dynamical Constraints on an Unseen Outer Perturber in the GJ 436 Hot Neptune System

  • Authors: Haedam Im, 해담 임, Tiger Lu, 均 陆, Malena Rice, Quang H. Tran, Gongjie Li, Smadar Naoz

Haedam Im et al 2026 The Astrophysical Journal 1003 .

  • Provider: AAS Journals

Caption: Figure 1.

RV measurements and our best-fitting model of the GJ 436 system. Panel (a) shows the RV data with the best-fit model over the 19 yr baseline. Panel (b) displays the RV residuals. Panel (c) presents the phased data and model based on the best-fit orbital parameters. Each instrument is plotted with a different color, and the Keplerian model is shown in black.

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