activity
19972011
most citedA Significant Population of Very Luminous Dust-Obscured Galaxies at Redshift z ~ 2

303 citations · 1.5k across the 24 of their papers we have counts for

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Showing 2009Show all

6 papers · 1 filter

astro-ph.CO200961 cited

Strong PAH Emission from z~2 ULIRGs

Vandana Desai, B. T. Soifer, Arjun Dey +15

Using the Infrared Spectrograph on board the Spitzer Space Telescope, we present low-resolution (64 < lambda / dlambda < 124), mid-infrared (20-38 micron) spectra of 23 high-redshi…

astro-ph.CO2009210 cited

The Spitzer Deep, Wide-Field Survey

M. L. N. Ashby, D. Stern, M. Brodwin +30

The Spitzer Deep, Wide-Field Survey (SDWFS) is a four-epoch infrared survey of ten square degrees in the Bootes field of the NOAO Deep Wide-Field Survey using the IRAC instrument o…

astro-ph.CO20091 cited

The Pedigrees of DOGs (Dust-Obscured Galaxies)

Arjun Dey, the NDWFS/MIPS Collaboration

A simple mid-infrared-to-optical color criterion of R-[24]>14 Vega mag results in a robust selection of approximately half of the redshift 2 ultraluminous infrared galaxy (ULIRG) p…

astro-ph.CO200961 cited

BigBOSS: The Ground-Based Stage IV Dark Energy Experiment

David J. Schlegel, Chris Bebek, Henry Heetderks +18

The BigBOSS experiment is a proposed DOE-NSF Stage IV ground-based dark energy experiment to study baryon acoustic oscillations (BAO) and the growth of structure with an all-sky ga…

astro-ph.CO200931 cited

High Redshift Dust Obscured Galaxies, A Morphology-SED Connection Revealed by Keck Adaptive Optics

J. Melbourne, S. Bussman, K. Brand +7

A simple optical to mid-IR color selection, R-[24] > 14, i.e. f_nu(24) / f_nu(R) > 1000, identifies highly dust obscured galaxies (DOGs) with typical redshifts of z~2 +/- 0.5. Extr…

astro-ph.CO20092 cited

Understanding the Astrophysics of Galaxy Evolution: the role of spectroscopic surveys in the next decade

Eric Bell, Marc Davis, Arjun Dey +24

Over the last decade optical spectroscopic surveys have characterized the low redshift galaxy population and uncovered populations of star-forming galaxies back to z ~ 7. This work…