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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 2.

5σ contrast curve for TOI-3757 observed from NESSI in the Sloan ${r}^{{\prime} }$ filter showing no bright companions within 1.″2 from the host star. The ${r}^{{\prime} }$ image is shown as an inset 1″ across.

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