activity
20052009
most citedWhat do we learn from IRAC observations of galaxies at 2 < z < 3.5?

367 citations · 444 across the 4 of their papers we have counts for

collaborators

8 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.CO200910 cited

The Deep Optical Imaging of the Extended Groth Strip

Ying-He Zhao, Jia-Sheng Huang, M. L. N. Ashby +2

We present optical images taken with the MMT/Megacam and the Subaru/Suprime of the Extended Groth Strip survey. The total survey covers an area of about degree

astro-ph.CO20096 cited

A New Era in Extragalactic Background Light Measurements: The Cosmic History of Accretion, Nucleosynthesis and Reionization

Asantha Cooray, Alexandre Amblard, Charles Beichman +52

(Brief Summary) What is the total radiative content of the Universe since the epoch of recombination? The extragalactic background light (EBL) spectrum captures the redshifted ener…

astro-ph2006367 cited

What do we learn from IRAC observations of galaxies at 2 < z < 3.5?

Stijn Wuyts, Ivo Labbe, Marijn Franx +9

We analyze very deep HST, VLT and Spitzer photometry of galaxies at 2<z<3.5 in the Hubble Deep Field South. The sample is selected from the deepest public K-band imaging currently…

astro-ph2005

Star Formation in Distant Red Galaxies: Spitzer observations in the Hubble Deep Field South

Tracy Webb, Pieter van Dokkum, Eiichi Egami +12

We present Spitzer 24micron imaging of 1.5 < z < 2.5 Distant Red Galaxies (DRGs) in the 10arcmin by 10arcmin Extended Hubble Deep Field South of the Multiwavelength Survey by Yale-…

astro-ph2005

Spitzer view on the evolution of star-forming galaxies from z=0 to z~3

Pablo G. Perez-Gonzalez, George H. Rieke, Eiichi Egami +11

We use a 24 micron selected sample containing more than 8,000 sources to study the evolution of star-forming galaxies in the redshift range from z=0 to z~3. We obtain photometric r…