• DOI:10.1088/0004-637X/796/2/115
Corpus ID: 44031425

Characterization of the atmosphere of the hot Jupiter HAT-P-32Ab and the M-Dwarf companion HAT-P-32B

@article{Zhao2014CharacterizationOT,
  title={Characterization of the atmosphere of the hot Jupiter HAT-P-32Ab and the M-Dwarf companion HAT-P-32B},
  author={Ming Zhao and J. O’Rourke and J. Wright and H. Knutson and A. Burrows and J. Fortney and Henry Ngo and B. Fulton and C. Baranec and R. Riddle and N. Law and P. Muirhead and S. Hinkley and A. Showman and J. Curtis and Rick Burruss Pennsylvania State University and Center for Exoplanets and Habitable Worlds and California Institute of Technology. and P. University and U. S. California and S. Cruz and University of Hawaii at Manoa and University of North Carolina at Chapel Hill and B. University and T. U. O. Arizona and J. P. Laboratory},
  journal={The Astrophysical Journal},
  year={2014},
  volume={796},
  pages={115}
}

Ming Zhao, J. O’Rourke, +24 authors J. P. Laboratory

Published 2014

Physics

The Astrophysical Journal

We report secondary eclipse photometry of the hot Jupiter HAT-P-32Ab, taken with Hale/Wide-field Infra-Red Camera (WIRC) in H and K_S bands and with Spitzer/IRAC at 3.6 and 4.5 μm. We carried out adaptive optics imaging of the planet host star HAT-P-32A and its companion HAT-P-32B in the near-IR and the visible. We clearly resolve the two stars from each other and find a separation of 2."923 ± 0."004 and a position angle 110.o64 ± 0.o12. We measure the flux ratios of the binary in g'r'i'z' and… CONTINUE READING

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