activity
20012009
most citedThe All-wavelength Extended Groth Strip International Survey (AEGIS) Data Sets

595 citations · 1.8k across the 20 of their papers we have counts for

collaborators

31 papers

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.CO2009145 cited

Mid-IR Luminosities and UV/Optical Star Formation Rates at z<1.4

Samir Salim, Mark Dickinson, R. Michael Rich +15

UV continuum and mid-IR emission constitute two widely used star formation indicators at intermediate and high redshifts. We study 2430 galaxies with z<1.4 in the Extended Groth St…

astro-ph.CO20094 cited

The Morphological Type Dependence of K-band Luminosity Functions

Nick Devereux, Paul Hriljac, S. P. Willner +2

Differential 2.2um (K-band) luminosity functions are presented for a complete sample of 1570 nearby Vgsr < 3000 km/s, where Vgsr is the velocity measured with respect to the Galact…

astro-ph2008124 cited

The Physical Scale of the Far-Infrared Emission in the Most Luminous Submillimeter Galaxies

Joshua D. Younger, Giovanni G. Fazio, David J. Wilner +10

We present high resolution submillimeter interferometric imaging of two of the brightest high-redshift submillimeter galaxies known: GN20 and AzTEC1 at 0.8 and 0.3 arcsec resolutio…

astro-ph200835 cited

AEGIS: Radio and Mid-Infrared Selection of Obscured AGN Candidates

S. Q. Park, P. Barmby, G. G. Fazio +10

The application of multi-wavelength selection techniques is crucial for discovering a complete and unbiased set of Active Galactic Nuclei (AGNs). Here, we select a sample of 72 AGN…