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    The Arcminute Microkelvin Imager

    Access Status
    Fulltext not available
    Authors
    Zwart, J.
    Barker, R.
    Biddulph, P.
    Bly, D.
    Boysen, R.
    Brown, A.
    Clementson, C.
    Crofts, M.
    Culverhouse, T.
    Czeres, J.
    Dace, R.
    Davies, M.
    D’Alessandro, R.
    Doherty, P.
    Duggan, K.
    Ely, J.
    Felvus, M.
    Feroz, F.
    Flynn, W.
    Franzen, Thomas
    Geisbusch, J.
    Genova-Santos, R.
    Grainge, K.
    Grainger, W.
    Hammett, D.
    Hills, R.
    Hobson, M.
    Holler, C.
    Hurley-Walker, Natasha
    Jilley, R.
    Jones, M.
    Kaneko, T.
    Kneissl, R.
    Lancaster, K.
    Lasenby, A.
    Marshall, P.
    Newton, F.
    Norris, O.
    Northrop, I.
    Odell, D.
    Petencin, G.
    Pober, J.
    Pooley, G.
    Pospieszalski, M.
    Quy, V.
    Rodriguez-Gonzalvez, C.
    Saunders, R.
    Scaife, A.
    Schofield, J.
    Scott, P.
    Shaw, C.
    Shimwell, T.
    Smith, H.
    Taylor, A.
    Titterington, D.
    Velic, M.
    Waldram, E.
    West, S.
    Wood, B.
    Yassin, G.
    Date
    2008
    Type
    Journal Article
    
    Metadata
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    Citation
    Zwart, J. and Barker, R. and Biddulph, P. and Bly, D. and Boysen, R. and Brown, A. and Clementson, C. et al. 2008. The Arcminute Microkelvin Imager. Monthly Notices of the Royal Astronomical Society. 391: pp. 1545-1558.
    Source Title
    Monthly Notices of the Royal Astronomical Society
    Additional URLs
    http://mnras.oxfordjournals.org/content/391/4/1545.full.pdf+html
    ISSN
    0035-8711
    URI
    http://hdl.handle.net/20.500.11937/11596
    Collection
    • Curtin Research Publications
    Abstract

    The Arcminute Microkelvin Imager is a pair of interferometer arrays operating with sixfrequency channels spanning 13.9–18.2 GHz, for observations on angular scales of 30 arcsec–10 arcmin and for declinations greater than -15?; the Small Array has a sensitivity of30 mJy s-1/2 and the Large Array has a sensitivity of 3mJy s-1/2. The telescope is aimedprincipally at Sunyaev–Zel’dovich imaging of clusters of galaxies. We discuss the design ofthe telescope and describe and explain its electronic and mechanical systems.

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