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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References

SHOWING 1-10 OF 49 REFERENCES

KELT-2Ab: A HOT JUPITER TRANSITING THE BRIGHT (V = 8.77) PRIMARY STAR OF A BINARY SYSTEM

We report the discovery of KELT-2Ab, a hot Jupiter transiting the bright (V = 8.77) primary star of the HD 42176 binary system. The host is a slightly evolved late F-star likely in the very

KELT-1b: A STRONGLY IRRADIATED, HIGHLY INFLATED, SHORT PERIOD, 27 JUPITER-MASS COMPANION TRANSITING A MID-F STAR

We present the discovery of KELT-1b, the first transiting low-mass companion from the wide-field Kilodegree Extremely Little Telescope-North (KELT-North) transit survey. A joint analysis of the

TrES-1: The Transiting Planet of a Bright K0 V Star

We report the detection of a transiting Jupiter-sized planet orbiting a relatively bright (V = 11.79) K0 V star. We detected the transit light-curve signature in the course of the TrES multisite

HAT-P-16b: A 4 MJ PLANET TRANSITING A BRIGHT STAR ON AN ECCENTRIC ORBIT,

We report the discovery of HAT-P-16b, a transiting extrasolar planet orbiting the V = 10.8 mag F8 dwarf GSC 2792-01700, with a period P = 2.775960 ± 0.000003 days, transit epoch Tc = 2455027.59293 ±

HAT-P-1b: A Large-Radius, Low-Density Exoplanet Transiting One Member of a Stellar Binary

Using small automated telescopes in Arizona and Hawaii, the HATNet project has detected an object transiting one member of the double star system ADS 16402. This system is a pair of G0 main-sequence

A Transiting Planet of a Sun-like Star

A planet transits an 11th magnitude, G1 V star in the constellation Corona Borealis. We designate the planet XO-1b and the star XO-1, also known as GSC 02041-01657. XO-1 lacks a trigonometric

Deep MMT Transit Survey of the Open Cluster M37. II. Variable Stars

We have conducted a deep (15≲ r≲ 23), 20 night survey for transiting planets in the intermediate-age (~550 Myr) open cluster M37 (NGC 2099) using the Megacam wide-field mosaic CCD camera on the 6.5 m

THE TRANSIT LIGHT CURVE PROJECT. XIII. SIXTEEN TRANSITS OF THE SUPER-EARTH GJ 1214b

We present optical photometry of 16 transits of the super-Earth GJ 1214b, allowing us to refine the system parameters and search for additional planets via transit timing. Starspot-crossing events

DETECTING TRANSITS OF PLANETARY COMPANIONS TO GIANT STARS

Of the approximately 350 extrasolar planets currently known, of order 10% orbit evolved stars with radii R* ≳ 2.5 R☉. These planets are of particular interest because they tend to orbit more massive

JUPITER WILL BECOME A HOT JUPITER: CONSEQUENCES OF POST-MAIN-SEQUENCE STELLAR EVOLUTION ON GAS GIANT PLANETS

When the Sun ascends the red giant branch (RGB), its luminosity will increase and all the planets will receive much greater irradiation than they do now. Jupiter, in particular, might end up more