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The Arcminute Microkelvin Imager

publications

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.聽.

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