activity
19982005
most citedImpZ: a new photometric redshift code for galaxies and quasars

90 citations · 91 across the 5 of their papers we have counts for

collaborators

23 papers

astro-ph2005

Morphological Studies of the SWIRE Galaxy Population in the UGC 10214 HST/ACS field

E. Hatziminaoglou, P. Cassata, G. Rodighiero +16

We present results of a morphological analysis of a small subset of the Spitzer Wide-area InfraRed Extragalactic survey (SWIRE) galaxy population. The analysis is based on public A…

astro-ph20051 cited

The 24 micron Luminosity Function of spectroscopic SWIRE sources from the Lockman validation field

N. Onyett, S. Oliver, G. Morrison +4

A spectroscopic follow-up of SWIRE sources from the Lockman Validation Field has allowed the determination of the SWIRE 24 micron Luminosity Function (LF). The spectroscopic sample…

astro-ph2004

Sloan Digital Sky Survey Quasars in the SWIRE ELAIS N1 Field: Properties and Spectral Energy Distributions

E. Hatziminaoglou, I. Perez-Fournon, M. Polletta +16

We present a mid-infrared analysis of 35 quasars with spectroscopic redshifts selected from the Spitzer Wide-area InfraRed Extragalactic Survey (SWIRE). We discuss their optical an…

astro-ph200490 cited

ImpZ: a new photometric redshift code for galaxies and quasars

T. S. R Babbedge, M. Rowan-Robinson, E. Gonzalez-Solares +7

We present a combined galaxy-quasar approach to template-fitting photometric redshift techniques and show the method to be a powerful one. The code (ImpZ) is presented, developed a…

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-ph2001

HST imaging of hyperluminous infrared galaxies

D. Farrah, A. Verma, S. Oliver +2

We present HST WFPC2 I band imaging for a sample of 9 Hyperluminous Infrared Galaxies spanning a redshift range 0.45 < z < 1.34. Three of the sample have morphologies showing evide…