1.1k citations · 2.9k across the 9 of their papers we have counts for
23 papers
Deep U band and R imaging of GOODS-South: Observations,data reduction and first results
M. Nonino, M. Dickinson, P. Rosati +9
We present deep imaging in the {\em U} band covering an area of 630 arcmin centered on the southern field of the Great Observatories Origins Deep Survey (GOODS). The data wer…
A submillimetre galaxy at z=4.76 in the LABOCA survey of the Extended Chandra Deep Field South
Kristen Coppin, Ian Smail, David M. Alexander +30
We report on the identification of the highest redshift submm-selected source currently known: LESSJ033229.4-275619. This source was detected in the Large Apex BOlometer CAmera (LA…
Reliable Identification of Compton-thick Quasars at z~2: Spitzer Mid-IR spectroscopy of HDF-oMD49
D. M. Alexander, R. R. Chary, A. Pope +6
Many models that seek to explain the origin of the unresolved X-ray background predict that Compton-thick Active Galactic Nuclei (AGNs) are ubiquitious at high redshift. However, f…
Multi-Wavelength Constraints on the Cosmic Star Formation History from Spectroscopy: the Rest-Frame UV, H-alpha, and Infrared Luminosity Functions at Redshifts 1.9<z<3.4
Naveen A. Reddy, Charles C. Steidel, Max Pettini +4
We use a sample of rest-frame UV selected and spectroscopically observed galaxies at redshifts 1.9<z<3.4, combined with ground-based spectroscopic H-alpha and Spitzer MIPS 24 micro…
Morphologies of Galaxies in and around a Protocluster at z=2.300
Annika H. G. Peter, Alice E. Shapley, David R. Law +4
We present results from the first robust investigation of galaxy morphology as a function of environment at z>1.5. Our study is motivated by the fact that star-forming galaxies con…
The Physical Nature of Rest-UV Galaxy Morphology During the Peak Epoch of Galaxy Formation
David R. Law, Charles C. Steidel, Dawn K. Erb +5
Motivated by the irregular and little-understood morphologies of z ~ 2 - 3 galaxies, we use non-parametric coefficents to quantify the morphologies of 216 galaxies which have been…