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No Giant Planets in the Eta Cassiopeiae System: Dynamical Implications of a Wide Binary Companion

  • Authors: Stephen R. Kane, Zhexing Li, Michelle L. Hill, Skylar D'Angiolillo, Benjamin J. Fulton, Andrew W. Howard

Stephen R. Kane et al 2025 The Astronomical Journal 170 .

  • Provider: AAS Journals

Caption: Figure 3.

Results of the injection-recovery test to assess the sensitivity of our RV data to planetary signatures as a function of planetary mass (﹩{M}_{p}\sin i﹩) and semimajor axis (a). The blue dots indicate successfully recovered injected planetary signatures and the red dots indicate unrecovered planets. The color scale corresponding to the probability contours of detecting a planet of a given mass and semimajor axis is shown on the right vertical axis.

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