NEAR-INFRARED SPECTROSCOPY OF THE EXTRASOLAR PLANET HR 8799 b

@article{Bowler2010NEARINFRAREDSO,
  title={NEAR-INFRARED SPECTROSCOPY OF THE EXTRASOLAR PLANET HR 8799 b},
  author={Brendan P. Bowler and Michael C. Liu and Trent J. Dupuy and Michael C. Cushing},
  journal={The Astrophysical Journal},
  year={2010},
  volume={723},
  pages={850 - 868}
}
We present 2.12–2.23 μm high contrast integral field spectroscopy of the extrasolar planet HR 8799 b. Our observations were obtained with OSIRIS on the Keck II telescope and sample the 2.2 μm CH4 feature, which is useful for spectral classification and as a temperature diagnostic for ultracool objects. The spectrum of HR 8799 b is relatively featureless, with little or no methane absorption, and does not exhibit the strong CH4 seen in T dwarfs of similar absolute magnitudes. The spectrum is… 
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