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TOI-2494 c and TOI-5143 c: A Hot Saturn and a Hot Jupiter with Interior Planetary Companions

  • Authors: Samuel N. Quinn, Joseph E. Rodriguez, Karen A. Collins, Allyson Bieryla, W. J. Brennom, Jiayin Dong, Kyle Hixenbaugh, David W. Latham, Brandon T. Radzom, Andrew Vanderburg, Songhu Wang, Samuel W. Yee, George Zhou, Isabelle Boisse, Ilaria Carleo, Pia Cortés-Zuleta, Xavier Delfosse, Thierry Forveille, Davide Gandolfi, Elisa Goffo, Guillaume Hébrard, Neda Heidari, Flavien Kiefer, Eder Martioli, Grzegorz Nowak, Enric Palle, Rafael Brahm, Thomas Henning, Melissa J. Hobson, Matias Jones, Andrés Jordán, Chelsea X. Huang, Lizhou Sha, Alton Spencer, Ashley Ashiku, Khalid Barkaoui, Zouhair Benkhaldoun, Perry Berlind, Michael L. Calkins, Kevin I. Collins, Dennis M. Conti, Gilbert A. Esquerdo, Phil Evans, Mark E. Everett, Mourad Ghachoui, Michaël Gillon, Elisabeth Heldridge, Keith Horne, Steve B. Howell, Emmanuël Jehin, Christopher R. Mann, Adam Popowicz, Francisco J. Pozuelos, Justus J. Randolph, Howard M. Relles, Boris Safonov, Richard P. Schwarz, Jonathan J. Swift, Thiam-Guan Tan, Mathilde Timmermans, Cristilyn N. Watkins, Roberto Zambelli, Carl Ziegler, Jessie L. Christiansen, Tansu Daylan, Martin Paegert, Eric B. Ting, Jon M. Jenkins, George R. Ricker, Sara Seager, Roland K. Vanderspek, Joshua N. Winn

Samuel N. Quinn et al 2026 The Astronomical Journal 171 .

  • Provider: AAS Journals

Caption: Figure 2.

The TESS 30 minute cadence (orange), 2 minute cadence (blue), and TFOP SG1 follow-up transits of TOI-2494 b (left), TOI-2494 c (middle), and TOI-5143 c (right). The EXOFASTv2 model for each transit observation is shown by the red solid line.

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