activity
20002019
most citedThe European Large Area ISO Survey I: Goals, Definition and Observation

221 citations · 866 across the 10 of their papers we have counts for

collaborators

10 papers

astro-ph.CO2019★ 43 cited

Stellar mass as a galaxy cluster mass proxy: application to the Dark Energy Survey redMaPPer clusters

A. Palmese, J. Annis, J. Burgad +82

We introduce a galaxy cluster mass observable, , based on the stellar masses of cluster members, and we present results for the Dark Energy Survey (DES) Year 1 observation…

astro-ph.CO2011★ 125 cited

Planck Early Results: Statistical properties of extragalactic radio sources in the Planck Early Release Compact Source Catalogue

Planck Collaboration, P. A. R. Ade, N. Aghanim +201

The data reported in Planck's Early Release Compact Source Catalogue (ERCSC) are exploited to measure the number counts (dN/dS) of extragalactic radio sources at 30, 44, 70, 100, 1…

astro-ph.IM2009★ 29 cited

Archiving multi-epoch data and the discovery of variables in the near infrared

N. J. G. Cross, R. S. Collins, N. C. Hambly +5

We present a description of the design and usage of a new synoptic pipeline and database model for time series photometry in the VISTA Data Flow System (VDFS). All UKIRT-WFCAM data…

astro-ph2005★ 25 cited

Properties of FIRBACK-ELAIS 175 um sources in the ELAIS N2 region

E. L. Taylor, R. G. Mann, A. N. Efstathiou +15

We report on a search for the optical counterparts of 175 um - selected sources from the Far-Infrared Background (FIRBACK) survey in the European Large Area ISO Survey (ELAIS) N2 f…

astro-ph2003★ 146 cited

The European Large Area ISO Survey (ELAIS): The Final Band-merged Catalogue

ELAIS Consortium, :, M. Rowan-Robinson +16

We present the final band-merged ELAIS catalogue at 6.7, 15, 90, and 175 m, and the associated data at u,g,r,i,z,J,H,K, and 20cm. The origin of the survey, infrared and radio ob…

astro-ph2002★ 34 cited

Obscured AGN from the ELAIS Deep X-ray Survey

C. J. Willott, C. Simpson, O. Almaini +13

The sources discovered in deep hard X-ray surveys with 2-8 keV fluxes of 10^-14 erg cm^-2 s^-1 make up the bulk of the X-ray background at these energies. We present here detailed…