activity
19982008
most citedXMM-LSS discovery of a z=1.22 galaxy cluster

65 citations · 258 across the 10 of their papers we have counts for

collaborators
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6 papers · 1 filter

astro-ph200713 cited

Clustering of galaxies at 3.6 microns in the Spitzer Wide-area Infrared Extragalactic legacy survey

I. Waddington, S. J. Oliver, T. S. R. Babbedge +11

We investigate the clustering of galaxies selected in the 3.6 micron band of the Spitzer Wide-area Infrared Extragalactic (SWIRE) legacy survey. The angular two-point correlation f…

astro-ph200751 cited

The discovery of a massive supercluster at z=0.9 in the UKIDSS DXS

A. M. Swinbank, A. Edge, I. Smail +19

We analyse the first publicly released deep field of the UKIDSS Deep eXtragalactic Survey (DXS) to identify candidate galaxy over-densities at z~1 across ~1 sq. degree in the ELAIS…

astro-ph2007

Ultraluminous Infrared Galaxies at 1.5<z<3 occupy dark matter haloes of mass ~6x10^13 solar masses

D. Farrah, C. J. Lonsdale, C. Borys +9

We present measurements of the spatial clustering of ultraluminous infrared galaxies in two redshift intervals, 1.5<z<2.0 and 2<z<3. Both samples cluster strongly, with r_0=14.40+/…

astro-ph2004

Angular Clustering of Galaxies at 3.6 micron from the SWIRE survey

Seb Oliver, Ian Waddington, Eduardo Gonzalez-Solares +11

We present the first analysis of large-scale clustering from the Spitzer Wide-area InfraRed Extragalactic legacy survey: SWIRE. We compute the angular correlation function of galax…

astro-ph1999

A Complete Sample of Millijansky Radio Sources

I. Waddington

The results of an optical and infrared investigation of a radio sample drawn from the 1.4 GHz Leiden-Berkeley Deep Survey are presented. This is believed to be the most comprehensi…

astro-ph1998

Near-Infrared Imaging of a Group or Cluster of Galaxies at a Redshift of 2.39

Ian Waddington

At z=2.39, the cluster around 53W002 is one of the most distant groups or clusters of galaxies known to date. At this redshift the 4000A-break falls between the J and H bands, thus…