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TOI-4010: A System of Three Large Short-period Planets with a Massive Long-period Companion

Authors: Michelle Kunimoto, Andrew Vanderburg, Chelsea X. Huang, M. Ryleigh Davis, Laura Affer, Andrew Collier Cameron, David Charbonneau, Rosario Cosentino, Mario Damasso, Xavier Dumusque, A. F. Martnez Fiorenzano, Adriano Ghedina, R. D. Haywood, Florian Lienhard, Mercedes López-Morales, Michel Mayor, Francesco Pepe, Matteo Pinamonti, Ennio Poretti, Jesús Maldonado, Ken Rice, Alessandro Sozzetti, Thomas G. Wilson, Stéphane Udry, Jay Baptista, Khalid Barkaoui, Juliette Becker, Paul Benni, Allyson Bieryla, Pau Bosch-Cabot, David R. Ciardi, Karen A. Collins, Kevin I. Collins, Elise Evans, Trent J. Dupuy, Maria V. Goliguzova, Pere Guerra, Adam Kraus, Jack J. Lissauer, Daniel Huber, Felipe Murgas, Enric Palle, Samuel N. Quinn, Boris S. Safonov, Richard P. Schwarz, Avi Shporer, Keivan G. Stassun, Jon M. Jenkins, David W. Latham, George R. Ricker, Sara Seager, Roland Vanderspek, Joshua Winn, Zahra Essack, Hannah M. Lewis, Mark E. Rose

Michelle Kunimoto et al 2023 The Astronomical Journal 166 .

Provider: AAS Journals

Caption: Figure 11.

Top: HARPS-N RV time series, which has a long-term trend best explained by an outer giant planet. The four-planet model is overplotted in red, and the residuals after subtracting the model are in the lower panel. Bottom: RV phase diagram for the long-period giant planet TOI-4010 e with the signals of the other three planets removed, in the same format as in Figure 10. The Keplerian model is plotted in purple. The gap in the phase diagram reflects the fact that the RV observing baseline is shorter than the estimated orbital period of the planet.

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