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19 April 2024

» arxiv » 0807.2469

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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 ; 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. Geisbüsch ; R. Génova-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. Rodríguez-Gonzálvez ; 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. Velić ; E. M. Waldram ; S. West ;
Date:	16 Jul 2008
Abstract:	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.
Source:	arXiv, 0807.2469
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