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 4.
GLS periodogram for the different data sets. The horizontal gray lines represent the 0.1%, 1%, and 10% FAP values. The red vertical line depicts the orbital period of planet b, whereas the gray line marks its 1 day alias.