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arxiv: 0807.2469 · v1 · pith:QECLFOBDnew · submitted 2008-07-15 · 🌌 astro-ph

The Arcminute Microkelvin Imager

AMI Consortium: J. T. L. Zwart , R. W. Barker , P. Biddulph , D. Bly , R. C. Boysen , A. R. Brown , C. Clementson , M. Crofts
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T. L. Culverhouse J. Czeres R. J. Dace M. L. Davies R. D'Alessandro P. Doherty K. Duggan J. A. Ely M. Felvus F. Feroz W. Flynn T. M. O. Franzen J. Geisb\"usch R. G\'enova-Santos K. J. B. Grainge W. F. Grainger D. Hammett R. E. Hills M. P. Hobson C. M. Holler N. Hurley-Walker R. Jilley M. E. Jones T. Kaneko R. Kneissl K. Lancaster A. N. Lasenby P. J. Marshall F. Newton O. Norris I. Northrop D. M. Odell J. C. Pober G. G. Pooley V. Quy C. Rodr\'iguez-Gonz\'alvez R. D. E. Saunders A. M. Scaife J. Schofield P. F. Scott C. Shaw T. W. Shimwell H. Smith A. C. Taylor D. J. Titterington M. Veli\'c E. M. Waldram S. West B. A. Wood G. Yassin (Astrophysics Group Cavendish Laboratory Cambridge UK)
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keywords arcminuteimagermicrokelvintelescopeaimedangulararrayschannels
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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.

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