HAT-P-34b-HAT-P-37b: Four Transiting Planets More Massive than Jupiter Orbiting Moderately Bright Stars

@article{Bakos2012HATP34bHATP37bFT,
  title={HAT-P-34b-HAT-P-37b: Four Transiting Planets More Massive than Jupiter Orbiting Moderately Bright Stars},
  author={G. Bakos and J. Hartman and G. Torres and B. B'eky and D. Latham and L. Buchhave and Z. Csubry and G. Kov'acs and A. Bieryla and S. Quinn and T. Szklenar and G. Esquerdo and A. Shporer and R. Noyes and D. Fischer and J. Johnson and A. Howard and G. Marcy and B. Sato and K. Penev and M. Everett and D. Sasselov and G. Fur'esz and R. Stefanik and J. L'az'ar and I. Papp and P. Sciences and P. University and H. F. Astrophysics and N. B. Institute and U. O. Copenhagen and K. Observatory and Lcogt and A. Department and Yale and Caltech. and Dep. of Astrophysics and D. O. Astronomy and UC Berkeley and D. O. Earth and Tokyo Institute of Technology and Hungarian Astronomical Association},
  journal={The Astronomical Journal},
  year={2012},
  volume={144},
  pages={19}
}
We report the discovery of four transiting extrasolar planets (HAT-P-34b–HAT-P-37b) with masses ranging from 1.05 to 3.33 M_J and periods from 1.33 to 5.45 days. These planets orbit relatively bright F and G dwarf stars (from V = 10.16 to V = 13.2). Of particular interest is HAT-P-34b which is moderately massive (3.33 M_J), has a high eccentricity of e = 0.441 ± 0.032 at a period of P = 5.452654 ± 0.000016 days, and shows hints of an outer component. The other three planets have properties… Expand
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