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A Warm Massive Pair of Planets around TOI-1232 Revealed with Transit-timing Variations and Doppler Spectroscopy

  • Authors: Deyan P. Mihaylov, Jan Eberhardt, Trifon Trifonov, Rafael Brahm, Thomas Henning, Andrés Jordán, Denitza Stoeva, Matías I. Jones, Lorena Acuña-Aguirre, Stefan Stefanov, M. Tala Pinto, Melissa J. Hobson, Nestor Espinoza, Felipe I. Rojas, Martin Schlecker, Vladimir Bozhilov, Tristan Guillot, Amaury H. M. J. Triaud, Jack J. Lissauer, Judith Korth, Hannu Parviainen, Laura Kreidberg, Philippe Bendjoya, Olga Suarez, Carl Ziegler, Pamela Rowden, Alexander Rudat, Veselin Kostov, Joshua N. Winn, Jon M. Jenkins, Karen A. Collins, Cristilyn N. Watkins, Don J. Radford, Chris Stockdale, Tianjun Gan

Deyan P. Mihaylov et al 2026 The Astronomical Journal 171 .

  • Provider: AAS Journals

Caption: Figure 8.

The top panel shows the RVs of TOI-1232 from the FEROS spectrograph together with the RV component of the RV + TTV joint N-body model. The model is consistent with two massive planets with an additional RV linear trend component, suggesting a likely third substellar body in the system. The bottom subpanel shows the RV residuals after the model contribution has been subtracted. The bottom left and right panels show a phase-folded representation of the model and RV data.

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