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The Arcminute Microkelvin Imager (2008) |
- Barker, R. W.,
- Biddulph, P.,
- Bly, D.,
- Boysen, R. C.,
- Brown, A. R.,
- Clementson, C.,
- Crofts, M.,
- Culverhouse, T. L.,
- Czeres, J.,
- Dace, R. J.,
- Davies, M. L.,
- D'Alessandro, R.,
- Doherty, P.,
- Duggan, K.,
- Ely, J. A.,
- Felvus, M.,
- Feroz, F.,
- Flynn, W.,
- Franzen, T. M. O.,
- Geisbüsch, J.,
- Génova-Santos, R.,
- Grainge, K. J. B.,
- Grainger, W. F.,
- Hammett, D.,
- Hills, R. E.,
- Hobson, M. P.,
- Holler, C. M.,
- Hurley-Walker, N.,
- Jilley, R.,
- Jones, M. E.,
- Kaneko, T.,
- Kneissl, R.,
- Lancaster, K.,
- Lasenby, A. N.,
- Marshall, P. J.,
- Newton, F.,
- Norris, O.,
- Northrop, I.,
- Odell, D. M.,
- Pober, J. C.,
- Pooley, G. G.,
- Quy, V.,
- Rodríguez-Gonzálvez, C.,
- Saunders, R. D. E.,
- Scaife, A. M.,
- Schofield, J.,
- Scott, P. F.,
- Shaw, C.,
- Shimwell, T. W.,
- Smith, H.,
- Taylor, A. C.,
- Titterington, D. J.,
- Velić, M.,
- Waldram, E. M.,
- West, S.,
- Wood, B. A.,
- Yassin, G.
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Abstract |
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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..
Comment: 15 pages, 13 figures. Submitted to MNRAS |
Publication details |
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