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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 7.

Lithium (left) and Hα (right) equivalent widths of TIC 88785435 (red), ϕ Lup candidate members (salmon), and literature established Sco-Cen members (gray). We plot the EAGLES (R. D. Jeffries et al. 2023) lithium distribution curve calculated for the age of UCL (16 Myr). Positive values denote the feature was observed in absorption, and negative values indicate emission. TIC 88785435 exhibited strong Hα emission and Li absorption supporting membership to Sco-Cen.

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