KMT-2016-BLG-1836Lb: A Super-Jovian Planet From A High-Cadence Microlensing Field

@article{Yang2019KMT2016BLG1836LbAS,
  title={KMT-2016-BLG-1836Lb: A Super-Jovian Planet From A High-Cadence Microlensing Field},
  author={H. Yang and X. Zhang and Kyu-Ha Hwang and W. Zang and A. Gould and T. Wang and S. Mao and M. Albrow and Sun-Ju Chung and C. Han and Y. K. Jung and Yoon-Hyun Ryu and In-gu Shin and Y. Shvartzvald and J. Yee and W. Zhu and M. Penny and P. Fouqu'e and Sang-Mok Cha and D. Kim and Hyounwoo Kim and S. Kim and C. Lee and D. Lee and Y. Lee and Byeong-Gon Park and R. W. Pogge},
  journal={arXiv: Earth and Planetary Astrophysics},
  year={2019}
}
  • H. Yang, X. Zhang, +24 authors R. W. Pogge
  • Published 2019
  • Physics
  • arXiv: Earth and Planetary Astrophysics
  • We report the discovery of a super-Jovian planet in the microlensing event KMT-2016-BLG-1836, which was found by the Korea Microlensing Telescope Network's high-cadence observations (\Gamma ~ 4~{hr}^{-1}). The planet-host mass ratio q ~ 0.004. A Bayesian analysis indicates that the planetary system is composed of a super-Jovian M_{planet} = 2.2_{-1.1}^{+1.9} M_{J} planet orbiting an M or K dwarf M_{\rm host} = 0.49_{-0.25}^{+0.38} M_{Sun}, at a distance of D_{L} = 7.1_{-2.4}^{+0.8} kpc. The… CONTINUE READING
    1 Citations
    OGLE-2015-BLG-1771Lb: A Microlens Planet Orbiting an Ultracool Dwarf?
    • 1
    • PDF

    References

    SHOWING 1-10 OF 76 REFERENCES
    KMT-2018-BLG-1990Lb: A Nearby Jovian Planet From A Low-Cadence Microlensing Field
    • 1
    • PDF
    KMT-2017-BLG-0165Lb: A Super-Neptune mass planet Orbiting a Sun-like Host Star
    • 10
    • PDF
    Two Jupiter-Mass Planets Discovered by the KMTNet Survey in 2017
    • 4
    • PDF
    KMT-2018-BLG-0029Lb: A Very Low Mass-Ratio Spitzer Microlens Planet
    • 6
    • PDF
    KMT-2016-BLG-1107: A New Hollywood-Planet Close/Wide Degeneracy
    • 6
    • PDF
    Kmt-2016-blg-1397b: Kmtnet-only discovery of a microlens giant planet
    • 5
    • PDF