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The host star is an F star with $T_{\\rm eff}=6206\\pm75$ K, $\\log g=4.108\\pm0.014$, $\\left[{\\rm Fe}/{\\rm H}\\right]=-0.116_{-0.069}^{+0.065}$, ${\\rm M_*}=1.201_{-0.061}^{+0.067} \\ {\\rm M}_{\\odot}$, and ${\\rm R_*}=1.610_{-0.068}^{+0.078} \\ {\\rm R}_{\\odot}$. The best-fit linear ephemeris is $\\rm {BJD_{TDB}} = 2456193.29157 \\pm 0.00021 + E\\left(2.9895936 \\pm 0.0000048\\right)$. With a magnitude of $V\\sim10$, a planetary radius of $1.699_{-0.045}^{+0.046} ","authors_text":"Allyson Bieryla, Andrew Gould, Andrew W. Howard, Benjamin J. Fulton, Bo Ma, B. Scott Gaudi, David W. Latham, D. L. DePoy, Erica J. Gonzales, Eric L. N. Jensen, Gilbert A. Esquerdo, Jason D. Eastman, Jennifer L. Marshall, Jian Ge, Ji Wang, Joao Gregorio, John Asher Johnson, John F. Kielkopf, Joseph M. O. Antognini, Joshua Pepper, Justin R. Crepp, Kaloyan Penev, Karen Collins, Keivan G. Stassun, Kim K. McLeod, Knicole D. Colon, Lars A. Buchhave, Mark Manner, Mark Trueblood, Matthew T. Penny, Michael L. 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