%0 Journal Article
%T HAT-P-34b -- HAT-P-37b: Four Transiting Planets More Massive Than Jupiter Orbiting Moderately Bright Stars
%A G. ¨¢. Bakos
%A J. D. Hartman
%A G. Torres
%A B. B¨¦ky
%A D. W. Latham
%A L. A. Buchhave
%A Z. Csubry
%A G. Kov¨¢cs
%A A. Bieryla
%A S. Quinn
%A T. Szklen¨¢r
%A G. A. Esquerdo
%A A. Shporer
%A R. W. Noyes
%A D. A. Fischer
%A J. A. Johnson
%A A. W. Howard
%A G. W. Marcy
%A B. Sato
%A K. Penev
%A M. Everett
%A D. D. Sasselov
%A G. F¨¹r¨¦sz
%A R. P. Stefanik
%A J. L¨¢z¨¢r
%A I. Papp
%A P. S¨¢ri
%J Physics
%D 2012
%I arXiv
%R 10.1088/0004-6256/144/1/19
%X 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 P = 5.4526540+/-0.000016 d period, and shows hints of an outer component. The other three planets have properties that are typical of hot Jupiters.
%U http://arxiv.org/abs/1201.0659v2