Optical and Infrared Diagnostics of SDSS galaxies in the SWIRE Survey (2006)
Davoodi, Payam, Pozzi, Francesca, Oliver, Seb, Polletta, Mari, Afonso-Luis, Alejandro, Farrah, Duncan, ...
We present the rest-frame optical and infrared colours of a complete sample of 1114 z
Parametric modelling of the 3.6um to 8um colour distributions of galaxies in the SWIRE Survey (2006)
Davoodi, Payam, Oliver, Seb, Polletta, Maria Del Carmen, Rowan-Robinson, Michael, Savage, Richard S., Waddington, Ian, ...
We fit a parametric model comprising a mixture of multi-dimensional Gaussian functions to the 3.6 to 8um colour and optical photo-z distribution of galaxy populations in the ELAIS-N1 and Lockman...
The spatial clustering of ultraluminous infrared galaxies over 1.5 (2006)
Farrah, Duncan, Lonsdale, Carol, Borys, Colin, Fang, Fan, Waddington, Ian, Oliver, Seb, ...
We present measurements of the spatial clustering of galaxies with stellar masses >10^11Msun, infrared luminosities >10^12 Lsun, and star formation rates >200Msun per year in two redshift intervals;...
The IRAC galaxy correlation functions from SWIRE (2005)
Waddington, Ian, Team, For The SWIRE
We present an analysis of large-scale structure from the Spitzer Wide-area Infrared Extragalactic legacy survey, SWIRE. The two-point angular correlation functions were computed for galaxies detected...
Angular Clustering of Galaxies at 3.6 micron from the SWIRE survey (2004)
Oliver, Seb, Waddington, Ian, Gonzalez-Solares, Eduardo, Surace, Jason, Fang, Fan, Shupe, Dave, ...
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 galaxies selected to...
HST Imaging of a z=1.55 Old Galaxy Group (2002)
Bunker, Andrew, Spinrad, Hyron, McLure, Ross, Dey, Arjun, Dunlop, James, Peacock, John, ...
We present high-resolution imaging in the rest-frame optical of the weak radio source LBDS53W091. Previous optical spectroscopy has shown that this object has an evolved stellar population of age...
Evidence for Large-Scale Structure at z=2.4 From Lyman-alpha Imaging (1999)
Keel, William C., Cohen, Seth H., Windhorst, Rogier A., Waddington, Ian
We present deep wide-field medium-band imaging in redshifted Lyman alpha of fields surrounding HST detections of faint emitters, to characterize their larger-scale environment. The radio galaxy...
Evolution of the 1.4 GHz Radio Luminosity Function (1999)
The results of an optical and infrared investigation of a complete sub-sample of the Leiden-Berkeley Deep Survey (flux > 1 mJy at 1.4 GHz) are presented. Optical counterparts have been identified for...
Faint Radio Sources and Star Formation History (1999)
Haarsma, Deborah B., Partridge, R. Bruce, Waddington, Ian, Windhorst, Rogier A.
Faint extragalactic radio sources provide important information about the global history of star formation. Sensitive radio observations of the Hubble Deep Field and other fields have found that...
Near-Infrared Imaging of a Group or Cluster of Galaxies at a Redshift of 2.39 (1998)
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 our infrared...