UCL Energy Institute


The Arcminute Microkelvin Imager


1 January 2008

The Arcminute Microkelvin Imager is a pair of interferometer arrays operating with six frequency channels spanning 13.9-18.2 GHz, with very high sensitivity to angular scales 30''-10'. The telescope is aimed principally at Sunyaev-Zel'dovich imaging of clusters of galaxies. We discuss the design of the telescope and describe and explain its electronic and mechanical systems.

The Arcminute Microkelvin Imager. 10.1111/j.1365-2966.2008.13953.x.

Consortium, AMI; Zwart, JTL; Barker, RW; Biddulph, P; Bly, D; Boysen, RC; ... Yassin, G; + view all (2008)