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Validation of a Third Earth-sized Planet in the TOI-2267 Binary System

  • Authors: Michael Greklek-McKeon, Jonathan Gomez Barrientos, Heather A. Knutson, Sebastián Zúñiga-Fernández, Francisco J. Pozuelos, Morgan Saidel, W. Garrett Levine, Renyu Hu, Fei Dai, Tansu Daylan, John P. Doty, David R. Rodriguez, Joseph D. Twicken, David W. Latham, Jon M. Jenkins, Richard P. Schwarz

Michael Greklek-McKeon et al 2026 The Astronomical Journal 171 .

  • Provider: AAS Journals

Caption: Figure 2.

Empirical stellar density constraints derived from our transit shape analysis (red) compared to the stellar density measurements from the SED fitting of ZP25 (blue), for the primary (top) and secondary star (bottom) fits. Our empirical constraints on the stellar density are not precise enough to conclusively rule out either star as the host of TOI-2267 d.

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