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NEID Reveals That the Young Warm Neptune TOI-2076 b Has a Low Obliquity

  • Authors: Robert C. Frazier, Gudmundur Stefánsson, Suvrath Mahadevan, Samuel W. Yee, Caleb I. Cañas, Joshua N. Winn, Jacob Luhn, Fei Dai, Lauren Doyle, Heather Cegla, Shubham Kanodia, Paul Robertson, John Wisniewski, Chad F. Bender, Jiayin Dong, Arvind F. Gupta, Samuel Halverson, Suzanne Hawley, Leslie Hebb, Rae Holcomb, Adam Kowalski, Jessica Libby-Roberts, Andrea S. J. Lin, Michael W. McElwain, Joe P. Ninan, Cristobal Petrovich, Arpita Roy, Christian Schwab, Ryan C. Terrien, Jason T. Wright

Robert C. Frazier et al 2023 The Astrophysical Journal Letters 944 .

  • Provider: AAS Journals

Caption: Figure 1.

TESS lightcurves of TOI-2076 from (A) Sector 16, (B) Sector 23, and (C) Sector 50. The top row shows the TESS photometry (blue points) with along with a transit model for TOI-2076 b + GP model (red) to account for stellar activity. The middle panel shows the photometry after subtracting the quasi-periodic GP model, revealing the TOI-2076 b transits. Panel (D) shows the phase-folded TESS photometry phased to the orbital period of TOI-2076 b, with the transit model overlaid.

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