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$\textit{TESS}$ Giants Transiting Giants I: A Non-inflated Hot Jupiter Orbiting a Massive Subgiant

Authors :
Saunders, Nicholas
Grunblatt, Samuel K.
Huber, Daniel
Collins, Karen A.
Jensen, Eric L. N.
Vanderburg, Andrew
Brahm, Rafael
Jordán, Andrés
Espinoza, Néstor
Henning, Thomas
Hobson, Melissa J.
Quinn, Samuel N.
Zhou, George
Butler, R. Paul
Crause, Lisa
Kuhn, Rudi B.
Mogotsi, K. Moses
Hellier, Coel
Angus, Ruth
Hattori, Soichiro
Chontos, Ashley
Ricker, George R.
Jenkins, Jon M.
Tenenbaum, Peter
Latham, David W.
Seager, Sara
Vanderspek, Roland K.
Winn, Joshua N.
Stockdale, Chris
Cloutier, Ryan
Publication Year :
2021

Abstract

While the population of confirmed exoplanets continues to grow, the sample of confirmed transiting planets around evolved stars is still limited. We present the discovery and confirmation of a hot Jupiter orbiting TOI-2184 (TIC 176956893), a massive evolved subgiant ($M_\star= 1.53 \pm 0.12 M_\odot$, $R_\star= 2.90 \pm 0.14 R_\odot$) in the $\textit{TESS}$ Southern Continuous Viewing Zone. The planet was flagged as a false positive by the $\textit{TESS}$ Quick-Look Pipeline due to periodic systematics introducing a spurious depth difference between even and odd transits. Using a new pipeline to remove background scattered light in $\textit{TESS}$ Full Frame Image (FFI) data, we combine space-based $\textit{TESS}$ photometry, ground-based photometry, and ground-based radial velocity measurements to report a planet radius of $R_p= 1.017 \pm 0.051 R_J$ and mass of $M_p= 0.65 \pm 0.16 M_J$. For a planet so close to its star, the mass and radius of TOI-2184b are unusually well matched to those of Jupiter. We find that the radius of TOI-2184b is smaller than theoretically predicted based on its mass and incident flux, providing a valuable new constraint on the timescale of post-main-sequence planet inflation. The discovery of TOI-2184b demonstrates the feasibility of detecting planets around faint ($\textit{TESS}$ magnitude $>12$) post-main sequence stars and suggests that many more similar systems are waiting to be detected in the $\textit{TESS}$ FFIs, whose confirmation may elucidate the final stages of planetary system evolution.<br />Comment: 20 pages, 13 figures

Details

Database :
arXiv
Publication Type :
Report
Accession number :
edsarx.2108.02294
Document Type :
Working Paper
Full Text :
https://doi.org/10.3847/1538-3881/ac38a1