KELT-3b: A HOT JUPITER TRANSITING A V = 9.8 LATE-F STAR

@article{Pepper2013KELT3bAH,
  title={KELT-3b: A HOT JUPITER TRANSITING A V = 9.8 LATE-F STAR},
  author={Joshua A. Pepper and Robert J. Siverd and Thomas G. Beatty and B. Scott Gaudi and Keivan G. Stassun and Jason D. Eastman and Karen A. Collins and David W. Latham and Allyson Bieryla and Lars A. Buchhave and Eric L. N. Jensen and Mark Manner and Kaloyan Penev and Justin R. Crepp and Phillip A. Cargile and Saurav Dhital and M. Calkins and Gilbert A. Esquerdo and Perry L. Berlind and Benjamin J. Fulton and Rachel A. Street and Bo Ma and Jian Ge and Ji Wang and Qingqing Mao and Alexander J. W. Richert and Andrew P. Gould and Darren Lee Depoy and John F. Kielkopf and Jennifer L. Marshall and Richard W. Pogge and Robert P. Stefanik and Mark H. Trueblood and Patricia Trueblood},
  journal={The Astrophysical Journal},
  year={2013},
  volume={773}
}
We report the discovery of KELT-3b, a moderately inflated transiting hot Jupiter with a mass of , radius of 1.345 ± 0.072 RJ, and an orbital period of 2.7033904 ± 0.000010 days. The host star, KELT-3, is a V = 9.8 late F star with , , K, , and [Fe/H] = , and has a likely proper motion companion. KELT-3b is the third transiting exoplanet discovered by the KELT survey, and is orbiting one of the 20 brightest known transiting planet host stars, making it a promising candidate for detailed… 

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