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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 5.

Left: Time series of activity indicators from HARPS-N spectra. Right: GLS periodograms of activity indicators. The horizontal lines mark 1% (dotted line) and 0.1% (dashed–dotted line) false-alarm probability levels, while vertical lines mark the orbital periods of the three planets. The line at P = 762 days marks the possible orbital period of the fourth planet that was uncovered in our later RV analysis (see Section 4.2).

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