activity
19942023
most citedDiscovery of a Supernova Explosion at Half the Age of the Universe and its Cosmological Implications

2.5k citations · 57.7k across the 311 of their papers we have counts for

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Showing 2003Show all

19 papers · 1 filter

astro-ph2003★ 93 cited

The 2dF Galaxy Redshift Survey: Wiener Reconstruction of the Cosmic Web

Pirin Erdogdu, Ofer Lahav, Saleem Zaroubi +27

We reconstruct the underlying density field of the 2 degree Field Galaxy Redshift Survey (2dFGRS) for the redshift range 0.035<z<0.200 using the Wiener Filtering method. The Wiener…

astro-ph2003

The Relationship between Stellar and Halo Masses of Disk Galaxies at z = 0.2 - 1.2

Christopher J. Conselice, Kevin Bundy, Richard S. Ellis +2

We present the results of a study to determine the co-evolution of the virial and stellar masses for a sample of 83 disk galaxies between redshifts z = 0.2 - 1.2. The virial masses…

astro-ph2003★ 104 cited

A Slow Merger History of Field Galaxies Since z~1

Kevin Bundy, Masataka Fukugita, Richard S. Ellis +2

Using deep infrared observations conducted with the CISCO imager on the Subaru Telescope, we investigate the field-corrected pair fraction and the implied merger rate of galaxies i…

astro-ph2003★ 65 cited

The 2dF Galaxy Redshift Survey: Clustering properties of radio galaxies

Manuela Magliocchetti, Steve J. Maddox, Ed Hawkins +24

The clustering properties of local, S_{1.4 GHz} > 1 mJy, radio sources are investigated for a sample of 820 objects drawn from the joint use of the FIRST and 2dF Galaxy Redshift su…

astro-ph2003★ 500 cited

Galaxy ecology: groups and low-density environments in the SDSS and 2dFGRS

Michael Balogh, Vince Eke, Chris Miller +34

We analyse the observed correlation between galaxy environment and H-alpha emission line strength, using volume-limited samples and group catalogues of 24968 galaxies drawn from th…

astro-ph2003★ 311 cited

The Dark Matter Distribution in the Central Regions of Galaxy Clusters

D. J. Sand, T. Treu, G. P. Smith +1

Cosmological N-body simulations predict that dark matter halos should have a universal shape characterized by a steep, cuspy inner profile. Here we report on a spectroscopic study…