Get access

The Arcminute Microkelvin Imager

Authors


  • We request that any reference to this paper cites ‘AMI Consortium: Zwart et al. 2008’.

Issuing author: jtlz2@mrao.cam.ac.uk

Present address: Kavli Institute for Cosmological Physics, University of Chicago, 5640 South Ellis Avenue, Chicago, IL 60637, USA.

Present address: The University Chemical Laboratory, Lensfield Road, Cambridge CB2 1EW.

Present address: Instituto de Astrofísica de Canarias, 38200 La Laguna, Tenerife, Canary Islands, Spain.

Present address: Department of Physics, Columbia University, 538 W. 120th Street, New York, NY 10027, USA.

Present address: Joint ALMA Office, Av El Golf 40, Piso 18, Santiago, Chile.

Present address: Astrophysics Group, Department of Physics, Denys Wilkinson Building, Keble Road, Oxford OX1 3RH.

Present address: MPI für Radioastronomie, Auf dem Hügel 69, D-53121 Bonn, Germany.

Present address: Astrophysics Group, H. H. Wills Physics Laboratory, Royal Fort, Tyndall Avenue, Bristol BS8 1TL.

Present address: UC Santa Barbara, Santa Barbara, CA 93106, USA.

Present address: NRAO Technology Center, 1180 Boxwood Estate Road, Charlottesville, VA 22903, USA.

Present address: Spatial Technology Ltd, 1 Quayside, Cambridge CB5 8AB.

ABSTRACT

The Arcminute Microkelvin Imager is a pair of interferometer arrays operating with six frequency 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 of 30 mJy s−1/2 and the Large Array has a sensitivity of 3 mJy s−1/2. 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.

Ancillary