The Arcminute Microkelvin Imager
AMI Consortium, JTL Zwart, RW Barker… - arXiv preprint arXiv …, 2008 - arxiv.org
AMI Consortium, JTL Zwart, RW Barker, P Biddulph, D Bly, RC Boysen, AR Brown…
arXiv preprint arXiv:0807.2469, 2008•arxiv.orgThe 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.
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 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.
arxiv.org