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Warm Jupiters in TESS Full-frame Images: A Catalog and Observed Eccentricity Distribution for Year 1

Dong, JY; Huang, CX; Dawson, RI; Foreman-Mackey, D; Collins, KA; Quinn, SN; Lissauer, JJ; Beatty, T; Quarles, B; Sha, LZ; Shporer, A; Guo, Z; Kane, SR; Abe, L; Barkaoui, K; Benkhaldoun, Z; Brahm, R; Bouchy, F; Carmichael, TW; Collins, KI; Conti, DM; Crouzet, N; Dransfield, G; Evans, P; Gan, TJ; Ghachoui, M; Gillon, M; Grieves, N; Guillot, T; Hellier, C; Jehin, E; Jensen, ELN; Jordan, A; Kamler, J; Kielkopf, JF; Mekarnia, D; Nielsen, LD; Pozuelos, FJ; Radford, DJ; Schmider, FX; Schwarz, RP; Stockdale, C; Tan, TG; Timmermans, M; Triaud, AHMJ; Wang, G; Ricker, G; Vanderspek, R; Latham, DW; Seager, S; Winn, JN; Jenkins, JM; Mireles, I; Yahalomi, DA; Morgan, EH; Vezie, M; Quintana, EV; Rose, ME; Smith, JC; Shiao, B

Dong, JY (corresponding author), Penn State Univ, Dept Astron & Astrophys, University Pk, PA 16802 USA.; Dong, JY (corresponding author), Penn State Univ, Ctr Exoplanets & Habitable Worlds, 525 Davey Lab, University Pk, PA 16802 USA.; Dong, JY (corresponding author), Flatiron Inst, Ctr Computat Astrophys, 162 Fifth Ave, New York, NY 10010 USA.

ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES, 2021; 255 (1):

Abstract

Warm Jupiters-defined here as planets larger than 6 Earth radii with orbital periods of 8-200 days-are a key missing piece in our understanding of how......

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