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19962009
most citedA Significant Population of Very Luminous Dust-Obscured Galaxies at Redshift z ~ 2

303 citations · 1.8k across the 23 of their papers we have counts for

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Showing 2006Show all

8 papers · 1 filter

astro-ph2006

Evidence for merging or disruption of red galaxies from the evolution of their clustering

Martin White, Zheng Zheng, Michael J. I. Brown +2

The formation and evolution of massive red galaxies form a crucial test of theories of galaxy formation based on hierarchical assembly. In this letter we use observations of the cl…

astro-ph200624 cited

The association between gas and galaxies II: The 2-point correlation function

R. J. Wilman, S. L. Morris, B. T. Jannuzi +2

We measure the 2-point correlation function, xi(AG), between galaxies and quasar absorption line systems at z<1, using the dataset of Morris & Jannuzi (2006; paper I) on 16 lines o…

astro-ph2006157 cited

Photometric Redshifts in the IRAC Shallow Survey

M. Brodwin, M. J. I. Brown, M. L. N. Ashby +16

Accurate photometric redshifts are calculated for nearly 200,000 galaxies to a 4.5 micron flux limit of ~13 uJy in the 8.5 deg^2 Spitzer/IRAC Shallow survey. Using a hybrid photome…

astro-ph200664 cited

Spitzer IRS Spectra of Optically Faint Infrared Sources with Weak Spectral Features

D. W. Weedman, B. T. Soifer, Lei Hao +15

Spectra have been obtained with the low-resolution modules of the Infrared Spectrograph (IRS) on the Spitzer Space Telescope (Spitzer) for 58 sources having f(24 micron) > 0.75…

astro-ph200663 cited

The Discovery of Three New z>5 Quasars in the AGN and Galaxy Evolution Survey

Richard J. Cool, Christopher S. Kochanek, Daniel J. Eisenstein +15

We present the discovery of three z>5 quasars in the AGN and Galaxy Evolution Survey (AGES) spectroscopic observations of the NOAO Deep Wide-Field Survey (NDWFS) Bootes Field. Thes…

astro-ph200658 cited

ChaMP Serendipitous Galaxy Cluster Survey

W. A. Barkhouse, P. J. Green, A. Vikhlinin +12

We present a survey of serendipitous extended X-ray sources and optical cluster candidates from the Chandra Multi-wavelength Project (ChaMP). Our main goal is to make an unbiased c…