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{\'a}sp{\'a}r {\'A}. Bakos and Joel D. Hartman and Guillermo Torres and Bence B'eky and David W. Latham and Lars A. Buchhave and Zolt{\'a}n Csubry and G. Kov'acs and Allyson Bieryla and Samuel N. Quinn and T. Szklen'ar and Gilbert A. Esquerdo and Avi Shporer and Robert W. Noyes and D. A. Fischer and J. A. Johnson and Andrew W. Howard and Geoffrey W. Marcy and Bun’ei Sato and Kaloyan Penev and Mark E. Everett and Dimitar D. Sasselov and G. Fur'esz and Robert P. Stefanik and J'ozsef L'az'ar and Istv{\'a}n Papp and Planetary Sciences and P. S'ari Princeton University and Harvard--Smithsonian Center for Astrophysics and Niels Bohr Institute and University of Copenhagen and Konkoly Observatory and Lcogt and Astronomy Department and Yale and Caltech and Department of Theoretical Astrophysics and Department of Physics Astronomy and Uc Berkeley and Department of Earth and Planetary Sciences and Tokyo Institute of Technology and Hungarian Astronomical Association},
  journal={The Astronomical Journal},
  year={2012},
  volume={144}
}
We report the discovery of four transiting extrasolar planets (HAT-P-34b–HAT-P-37b) with masses ranging from 1.05 to 3.33 MJ 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 MJ), 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 that… 
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