Astrophysics Group

Cavendish Laboratory

AMI Publications

This page contains links to papers containing AMI data that have been published in, or submitted to, refereed journals.

2011

Further Sunyaev-Zel’dovich observations of two Planck ERCSC clusters with the Arcminute Microkelvin Imager
AMI Consortium: Hurley-Walker N. et al., 2011, preprint (arXiv:1103.0947)

Bayesian analysis of weak-gravitational-lensing and Sunyaev-Zel’dovich data for six galaxy clusters
AMI Consortium: Hurley-Walker N. et al., 2011, preprint (arXiv:1101.5912)

Sunyaev-Zel’dovich observations of LoCuSS clusters with the Arcminute Microkelvin Imager: high X-ray luminosity sample
AMI Consortium: Shimwell T. W. et al., 2011, preprint (arXiv:1101.5590)

Sunyaev-Zel’dovich observations of LoCuSS clusters with the Arcminute Microkelvin Imager: moderate X-ray luminosity sample
AMI Consortium: Rodriguez-Gonzalvez C. et al., 2011, preprint (arXiv:1101.5589)

AMI-LA radio continuum observations of Spitzer c2d small clouds and cores: Perseus region
AMI Consortium: Scaife A. M. M. et al., 2011, preprint (arXiv:1101.5514)

AMI Large Array radio continuum observations of Spitzer c2d small clouds and cores
AMI Consortium: Scaife A. M. M. et al., 2011, MNRAS, 410, 2662

The doubling of the superorbital period of Cyg X-1
Zdziarski A. A., Pooley G. G. and Skinner G. K., 2011, MNRAS, no. doi: 10.1111/j.1365-2966.2010.18034.x

Planck Early Results: The all-sky Early Sunyaev-Zeldovich cluster sample
Planck Collaboration: Ade P. A. R. et al., 2011, preprint (arXiv:1101.2024)


2010

Parameterization Effects in the analysis of Sunyaev-Zel’dovich Observations
AMI Consortium: Olamaie M. et al., 2010, preprint (arXiv:1012.4996)

A blind detection of a large, complex, Sunyaev–Zel’dovich structure
AMI Consortium: Shimwell T. W. et al., 2010, preprint (arXiv:1012.4441)

10C Survey of Radio Sources at 15.7 GHz: II – First Results
AMI Consortium: Davies et al., 2010, preprint (arXiv:1012.3659)

10C Survey of Radio Sources at 15.7 GHz: I – Observing, mapping and source extraction
AMI Consortium: Franzen et al., 2010, preprint (arXiv:1012.3711)

Understanding Cygnus X-3 Through Multi-Wavelength Studies
McCollough M., Koljonen K., Hannikainen D., Pooley G., Trushkin S. A., Steeghs D., Tavani M., Droulans R., 2010, preprint (arXiv:1012.3378)

A tale of two GRB-SNe at a common redshift of z = 0.54
Cano Z. et al., 2010, preprint (arXiv:1012.1466)

Sunyaev-Zel’dovich observation of the Bullet-like cluster A2146 with the Arcminute Microkelvin Imager
AMI Consortium: Rodriguez-Gonzalvez C. et al., 2010, preprint (arXiv:1011.0325)

GRB 090313 and the Origin of Optical Peaks in Gamma-ray Burst Light Curves: Implications for Lorentz Factors and Radio Flares
Melandri A. et al., 2010, ApJ, 723, 1331

Magic Constraints on gamma-ray Emission from Cygnus X-3
Aleksic J. et al., 2010, ApJ, 721, 843

Sunyaev-Zel’dovich observations of galaxy clusters out to the virial radius with the Arcminute Microkelvin Imager
AMI Consortium: Zwart et al., 2010, preprint (arXiv:1008.0443)

Microwave observations of spinning dust emission in NGC6946
AMI Consortium: Scaife A. M. M. et al., 2010, MNRAS, 406, 45

High-resolution AMI Large Array imaging of spinning dust sources: spatially correlated 8μm emission and evidence of a stellar wind in L675
AMI Consortium: Scaife A. M. M. et al., 2010, MNRAS, 403, 46

A change in the optical polarization associated with a gamma-ray flare in the blazar 3C279
Abdo A. A. et al., 2010, Natur, 463, 919

The first blind cluster detected in the AMI survey data (see AMI Consortium: Shimwell T. W. et al. 2010).


2009

Modulated High-Energy Gamma-Ray Emission from the Microquasar Cygnus X-3
Fermi LAT Collaboration: Abdo A. A. et al., 2009, Sci, 326, 1512

Extreme particle acceleration in the microquasar Cygnus X-3
Tavani M. et al., 2009, Natur, 462, 620

AMI observations of Lynds dark nebulae: further evidence for anomalous cm-wave emission
AMI Consortium: Scaife A. M. M., MNRAS, 400, 1394

Follow-up observations at 16 and 33GHz of extragalactic sources from WMAP 3-yr data: II – Flux density variability
AMI Consortium: Franzen T. M. O. et al., 2009, MNRAS, 400, 995

Follow-up observations at 16 and 33GHz of extragalactic sources from WMAP 3-yr data: I – Spectral properties
AMI Consortium: Davies M. L. et al., 2009, MNRAS, 400, 984

G64.5+0.9: a new shell supernova remnant with unusual central emission
AMI Consortium: Hurley-Walker N. et al., 2009, MNRAS, 398, 249

AMI observations of northern supernova remnants at 14-18GHz
AMI Consortium: Hurley-Walker N. et al., 2009, MNRAS, 396, 365

An excess of emission in the dark cloud LDN1111 with the Arcminute Microkelvin Imager
AMI Consortium: Scaife A. M. M., MNRAS, 2009, 394, 46

An unusual ‘feature’ in VLA archive-data was confirmed to be a new supernova remnant, G64.5+0.9, using AMI (see AMI Consortium: Hurley-Walker N. et al. 2009).


2008 and earlier

The Arcminute Microkelvin Imager
AMI Consortium: Zwart J. T. L. et al., 2008, MNRAS, 391, 1545

AMI limits on 15-GHz excess emission in northern HII regions
AMI Consortium: Scaife A. M. M. et al., 2008, MNRAS, 385, 809

High-significance Sunyaev-Zel’dovich measurement: Abell 1914 seen with the Arcminute Microkelvin Imager
AMI Consortium: Barker R. et al., 2006, MNRAS, 369, 1

AMI Consortium: Zwart et al. J. T. L. (2008) gives a detailed description of AMI. (Photograph by kind permission of Ross Nieuwburg© 2011.)