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A 16 Myr Super-Neptune in Upper Centaurus Lupus and a Preliminary Survey of Transiting Planets in Sco-Cen with TESS

Authors: Sydney Vach, George Zhou, Andrew W. Mann, Madyson G. Barber, Tyler R. Fairnington, Chelsea X. Huang, James G. Rogers, Luke G. Bouma, Joachim Krüger, Duncan Wright, Annabelle E. Niblett, Jack M. Nelson, Samuel N. Quinn, David W. Latham, Allyson Bieryla, Karen A. Collins, Michelle Kunimoto, Cristilyn N. Watkins, Richard P. Schwarz, Kevin I. Collins, Ramotholo Sefako, Keith Horne, Steve B. Howell, Catherine A. Clark, Colin Littlefield, Jessie L. Christiansen, Zahra Essack, Joshua N. Winn

Sydney Vach et al 2025 The Astronomical Journal 170 .

Provider: AAS Journals

Caption: Figure 4.

Galactic coordinates (l, b) of literature Sco-Cen (gray) members (see K. L. Luhman 2022, and references within). TIC 88785435 (red star) is a member of the classically defined UCL subpopulation. S. Ratzenböck et al. (2023b) identified TIC 88785435 as a high-confidence candidate member of the kinematically distinct ϕ Lup substructure (salmon circles) primarily within UCL. ϕ Lup candidate members outlined in black are rotationally and photometrically validated members of the Sco-Cen population (L. M. Rebull et al. 2018, 2022).

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