activity
19992025
most citedCosmological parameter estimation and Bayesian model comparison using VSA data

52 citations · 250 across the 12 of their papers we have counts for

collaborators

12 papers

astro-ph.GA2025

Spectral Properties of Anomalous Microwave Emission in 144 Galactic Clouds

Roke Cepeda-Arroita, J. A. Rubiño-Martín, R. T. Génova-Santos +23

Anomalous Microwave Emission (AME) is a diffuse microwave component thought to arise from spinning dust grains, yet remains poorly understood. We analyze AME in 144 Galactic clouds…

astro-ph.IM2013★ 30 cited

The C-Band All-Sky Survey (C-BASS): Design and implementation of the northern receiver

O. G. King, Michael E. Jones, E. J. Blackhurst +12

The C-Band All-Sky Survey (C-BASS) is a project to map the full sky in total intensity and linear polarization at 5 GHz. The northern component of the survey uses a broadband singl…

astro-ph.CO2011★ 7 cited

The Cosmic Background Imager 2

Angela C. Taylor, Michael E. Jones, James R. Allison +14

We describe an upgrade to the Cosmic Background Imager instrument to increase its surface brightness sensitivity at small angular scales. The upgrade consisted of replacing the thi…

astro-ph.GA2011★ 36 cited

Dust-correlated cm-wavelength continuum emission on translucent clouds ζ Oph and LDN 1780

M. Vidal, S. Casassus, C. Dickinson +17

The diffuse cm-wave IR-correlated signal, the "anomalous" CMB foreground, is thought to arise in the dust in cirrus clouds. We present Cosmic Background Imager (CBI) cm-wave data o…

astro-ph.CO2010★ 14 cited

A parametric physical model for the intracluster medium and its use in joint SZ/X-ray analyses of galaxy clusters

J. R. Allison, A. C. Taylor, M. E. Jones +2

We present a parameterized model of the intra-cluster medium that is suitable for jointly analysing pointed observations of the Sunyaev-Zel'dovich (SZ) effect and X-ray emission in…

astro-ph.GA2010★ 14 cited

A 33 GHz VSA survey of the Galactic plane from 27 to 46 degrees

M. Todorović, R. D. Davies, C. Dickinson +17

The Very Small Array (VSA) has been used to survey the l = 27 to 46 deg, |b|<4 deg region of the Galactic plane at a resolution of 13 arcmin. The survey consists of 44 pointings of…