MORPHOLOGIES OF HIGH-REDSHIFT, DUST-OBSCURED GALAXIES FROM KECK LASER GUIDE STAR ADAPTIVE OPTICS

@article{Melbourne2008MORPHOLOGIESOH,
  title={MORPHOLOGIES OF HIGH-REDSHIFT, DUST-OBSCURED GALAXIES FROM KECK LASER GUIDE STAR ADAPTIVE OPTICS},
  author={J. Melbourne and V. Desai and L. Armus and A. Dey and K. Brand and D. Thompson and B. Soifer and K. Matthews and B. Jannuzi and J. R. H. C. I. O. Technology and Spitzer Science Center and National Optical Astronomy Observatory and S. Institute and U. O. Arizona and C. University},
  journal={The Astronomical Journal},
  year={2008},
  volume={136},
  pages={1110-1117}
}
Spitzer MIPS images in the Bootes field of the NOAO Deep Wide-Field Survey have revealed a class of extremely dust-obscured galaxy (DOG) at z ~ 2. The DOGs are defined by very red optical to mid-infrared (IR; observed-frame) colors, R – [24 μm] > 14 mag, i.e. f_ν(24 μm)/f_ν(R) > 1000. They are ultra-luminous infrared galaxies with L_(8-1000 μm) > 10^(12)-10^(14) L⊙, but typically have very faint optical (rest-frame UV) fluxes. We imaged three DOGs with the Keck laser guide star adaptive optics… Expand
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