We review the statistical properties of the main populations of radio sources, as emerging
from radio and millimeter sky surveys. Recent determinations of local luminosity functions …

We present the first all-sky sample of galaxy clusters detected blindly by the Planck satellite
through the Sunyaev-Zeldovich (SZ) effect from its six highest frequencies. This early SZ …

Abstract The Arcminute Microkelvin Imager is a pair of interferometer arrays operating with
six frequency channels spanning 13.9–18.2 GHz, for observations on angular scales of 30 …

We present the scaling relation between Sunyaev-Zeldovich (SZ) signal and stellar mass for
almost 260,000 locally brightest galaxies (LBGs) selected from the Sloan Digital Sky Survey …

A technological milestone for experiments employing transition edge sensor bolometers
operating at sub-Kelvin temperature is the deployment of detector arrays with 100s–1000s of …

We present a sample of 29 galaxy clusters from the XMM-LSS survey over an area of some
5 deg2 out to a redshift of z= 1.05. The sample clusters, which represent about half of the X …

We make use of the Planck all-sky survey to derive number counts and spectral indices of
extragalactic sources–infrared and radio sources–from the Planck Early Release Compact …

ABSTRACT The Spitzer Adaptation of the Red-sequence Cluster Survey (SpARCS) is a z'-
passband imaging survey of the 50 deg 2 Spitzer SWIRE Legacy fields, designed with the …

We present the Sunyaev-Zeldovich (SZ) signal-to-richness scaling relation (Y 500− N 200)
for the MaxBCG cluster catalogue. Employing a multi-frequency matched filter on the Planck …

We investigate the utility of a new, self-similar pressure profile for fitting Sunyaev–Zel'dovich
(SZ) effect observations of galaxy clusters. Current SZ imaging instruments–such as the …