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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 Journal 164 .

Provider: AAS Journals

Caption: Figure 6.

Photometric observations for TOI-3757 b. (a) the TESS-phased plot shows the detrended light curve phase-folded to the best-fit orbital period; (b) ground-based observations for TOI-3757 b from RBO. The raw photometry is shown in gray, with the best-fit transit solution in blue, along with the 1σ confidence interval shown in lighter blue. The data behind Figure 6(b) are available.

(The data used to create this figure are available.)

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