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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 5.

Panel (a) overlays an 11 ×11 pixel footprint from TESS Sector 19 (blue grid) on a POSS-I red image from 1953.1. TOI-3757 has a small proper motion as can be seen while comparing panels (a) and (b). The TESS aperture is outlined in red, and we highlight TOI-3757 with a star. No bright targets are present inside the TESS aperture with Δ G RP < 3. Panel (b) is similar to panel (a) but with a background image from ZTF zr (5600–7316 Å) from 2019 (Masci et al. 2019).

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