activity
19962009
most citedThe stellar mass assembly of galaxies from z=0 to z=4. Analysis of a sample selected in the rest-frame near-infrared with Spitzer

614 citations · 2.7k across the 31 of their papers we have counts for

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Showing 2008 · astro-phShow all

5 papers · 2 filters

astro-ph200811 cited

Observations of the Gas Reservoir around a Star Forming Galaxy in the Early Universe

Brenda L. Frye, David. V. Bowen, Mairead Hurley +8

We present a high signal-to-noise spectrum of a bright galaxy at z = 4.9 in 14 h of integration on VLT FORS2. This galaxy is extremely bright, i_850 = 23.10 +/- 0.01, and is strong…

astro-ph2008274 cited

An Infrared Survey of Brightest Cluster Galaxies. II: Why are Some Brightest Cluster Galaxies Forming Stars?

Christopher P. O'Dea, Stefi A. Baum, George Privon +12

Quillen et al.(2007) presented an imaging survey with the {\it Spitzer Space Telescope} of 62 brightest cluster galaxies with optical line emission located in the cores of X-ray lu…

astro-ph2008110 cited

A Hubble & Spitzer Space Telescope Survey for Gravitationally-Lensed Galaxies: Further Evidence for a Significant Population of Low Luminosity Galaxies beyond Redshift Seven

Johan Richard, Daniel P. Stark, Richard S. Ellis +4

We present the results of a systematic search for gravitationally-lensed continuum Lyman break `drop-outs' beyond a redshift 7 conducted via very deep imaging through six foregroun…

astro-ph200896 cited

The SCUBA HAlf Degree Extragalactic Survey (SHADES) - VII. Optical/IR photometry and stellar masses of sub-millimeter galaxies

Simon Dye, S. A. Eales, I. Aretxaga +21

We present estimates of the photometric redshifts, stellar masses and star formation histories of sources in the SCUBA HAlf Degree Extragalactic Survey (SHADES). This paper describ…

astro-ph2008105 cited

Strong Lensing in Abell 1703: Constraints on the Slope of the Inner Dark Matter Distribution

M. Limousin, J. Richard, J. -P. Kneib +9

In this article, we apply strong lensing techniques in Abell 1703, a massive X-ray luminous galaxy cluster at z=0.28. Our analysis is based on imaging data both from space and grou…