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19952009
most citedThe Mass-Metallicity Relation at z~2

1.1k citations · 4.2k across the 29 of their papers we have counts for

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Showing 2004Show all

11 papers · 1 filter

astro-ph2004

The Spatial Clustering of Star-forming Galaxies at Redshifts 1.4<z<3.5

K. L. Adelberger, C. C. Steidel, M. Pettini +3

We analyzed the spatial distribution of 28500 photometrically selected galaxies with AB magnitude 23.5<R<25.5 and redshift 1.4<z<3.5 in 21 fields with a total area of 0.81 square d…

astro-ph2004

Spectral Modelling of Star-Forming Regions in the Ultraviolet: Stellar Metallicity Diagnostics for High Redshift Galaxies

Samantha A. Rix, Max Pettini, Claus Leitherer +3

The chemical composition of high redshift galaxies is an important property which gives clues to their past history and future evolution and yet is difficult to measure with curren…

astro-ph2004

The Number Density of 0.6 < z < 1.7 MgII Systems from CORALS: Observational Biases at Intermediate Redshift

Sara L. Ellison, Chris W. Churchill, Samantha A. Rix +1

The goal of the Complete Optical and Radio Absorption Line System (CORALS) survey is to quantify the potential impact on QSO absorber statistics from dust in intervening galaxies.…

astro-ph2004

Deep mid-infrared observations of Lyman-break galaxies

P. Barmby, J. -S. Huang, G. G Fazio +15

As part of the In-Orbit Checkout activities for the Spitzer Space Telescope, the IRAC team carried out a deep observation (average integration time ~8 hours) of a field surrounding…

astro-ph2004

Evidence for Solar Metallicities in Massive Star-forming Galaxies at z>~2

A. E. Shapley, D. K. Erb, M. Pettini +2

We present results of near-IR spectroscopic measurements of 7 star-forming galaxies at 2.1<z<2.5. Drawn from a large spectroscopic survey of galaxies photometrically pre-selected b…

astro-ph2004

The Kinematics of Morphologically Selected z~2 Galaxies in the GOODS-N Field

Dawn K. Erb, Charles C. Steidel, Alice E. Shapley +2

We present near-IR spectra of H-alpha emission from 13 galaxies at z~2 in the GOODS-N field. The galaxies were selected primarily because they appear to have elongated morphologies…