Figure 2 from Search for Nearby Earth Analogs. II. Detection of Five New Planets, Eight Planet Candidates, and Confirmation of Three Planets around Nine Nearby M Dwarfs

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Search for Nearby Earth Analogs. II. Detection of Five New Planets, Eight Planet Candidates, and Confirmation of Three Planets around Nine Nearby M Dwarfs

Authors: Fabo Feng, R. Paul Butler, Stephen A. Shectman, Jeffrey D. Crane, Steve Vogt, John Chambers, Hugh R. A. Jones, Sharon Xuesong Wang, Johanna K. Teske, Jenn Burt, Matías R. Díaz, and Ian B. Thompson

2020 The Astrophysical Journal Supplement Series 246 11.

Provider: AAS Journals

Caption: Figure 2.

Phase curves and corresponding residuals for all planet candidates are shown. The instruments are encoded by different colors and are shown on top of all panels. The error bars show the error-weighted average RVs in 10 evenly separated time bins. The best orbital solution is determined by the MAP values of orbital parameters. The rms of the residual RVs after subtracting all signals is shown in each panel.

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