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20072009
most citedA Significant Population of Very Luminous Dust-Obscured Galaxies at Redshift z ~ 2

303 citations · 642 across the 6 of their papers we have counts for

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astro-ph200823 cited

Morphologies of High Redshift, Dust Obscured Galaxies from Keck Laser Guide Star Adaptive Optics

J. Melbourne, V. Desai, Lee Armus +7

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 op…

astro-ph200819 cited

Spitzer Mid-Infrared Spectroscopy of Distant X-ray Luminous AGN

Kate Brand, Dan W. Weedman, Vandana Desai +7

We present mid-infrared spectroscopy of a sample of 16 optically faint infrared luminous galaxies obtained with the Infrared Spectrograph (IRS) on the Spitzer Space Telescope. Thes…

astro-ph2008303 cited

A Significant Population of Very Luminous Dust-Obscured Galaxies at Redshift z ~ 2

Arjun Dey, B. T. Soifer, Vandana Desai +12

Observations with Spitzer Space Telescope have recently revealed a significant population of high-redshift z~2 dust-obscured galaxies (DOGs) with large mid-IR to UV luminosity rati…

astro-ph200744 cited

Lens Galaxy Properties of SBS1520+530: Insights from Keck Spectroscopy and AO Imaging

M. W. Auger, C. D. Fassnacht, K. C. Wong +3

We report on an investigation of the SBS 1520+530 gravitational lens system and its environment using archival HST imaging, Keck spectroscopic data, and Keck adaptive-optics imagin…

astro-ph200718 cited

Spitzer Mid-Infrared Spectroscopy of 70um-Selected Distant Luminous Infrared Galaxies

Kate Brand, Dan W. Weedman, Vandana Desai +7

We present mid-infrared spectroscopy obtained with the Spitzer Space Telescope of a sample of 11 optically faint, infrared luminous galaxies selected from a Spitzer MIPS 70um imagi…

astro-ph2007266 cited

High resolution mid-infrared spectroscopy of ultraluminous infrared galaxies

D. Farrah, J. Bernard-Salas, H. W. W. Spoon +8

(Abridged) We present R~600, 10-37um spectra of 53 ULIRGs at z<0.32, taken using the IRS on board Spitzer. All of the spectra show fine structure emission lines of Ne, O, S, Si and…