TOI-3757 b: A Low-density Gas Giant Orbiting a Solar-metallicity M Dwarf
Authors: Shubham Kanodia, Jessica Libby-Roberts, Caleb I. Cañas, Joe P. Ninan, Suvrath Mahadevan, Gudmundur Stefansson, Andrea S. J. Lin, Sinclaire Jones, Andrew Monson, Brock A. Parker, Henry A. Kobulnicky, Tera N. Swaby, Luke Powers, Corey Beard, Chad F. Bender, Cullen H. Blake, William D. Cochran, Jiayin Dong, Scott A. Diddams, Connor Fredrick, Arvind F. Gupta, Samuel Halverson, Fred Hearty, Sarah E. Logsdon, Andrew J. Metcalf, Michael W. McElwain, Caroline Morley, Jayadev Rajagopal, Lawrence W. Ramsey, Paul Robertson, Arpita Roy, Christian Schwab, Ryan C. Terrien, John Wisniewski, Jason T. Wright
Shubham Kanodia et al
2022 The Astronomical Journal164.
Provider: AAS Journals
Caption: Figure 7.
HPF + NEID RV observations phase-folded on the best-fit orbital period from the joint fit from Section 4.1. The best-fit model is shown in the solid line, whereas the 1σ confidence intervals are shown in lighter blue.