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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 1.

Top: Difference images for TOI-4010.01, 4010.02, and 4010.03, made using 20 × 20 pixel cutouts of the Sector 25 TESS FFIs. Bottom: Close-up of the central 5 × 5 pixels. The fourth column shows the average of out-of-transit images, which should represent a direct image of the field near the target star. The color bars show the average pixel flux in electrons per second. The target TIC-352682207 is indicated with a pink star, while nearby stars up to ΔT = 4 mag fainter are plotted as white circles with sizes scaled by brightness. The difference images for all three planet candidates indicate the transit sources are co-located with the target star.

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