SIMBAD references

2008MNRAS.391.1545Z - Mon. Not. R. Astron. Soc., 391, 1545-1558 (2008/December-3)

The Arcminute Microkelvin Imager AMI Consortium:.

ZWART J.T.L., 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., GEISBUSCH J., GENOVA-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., PETENCIN G., POBER J.C., POOLEY G.G., POSPIESZALSKI M.W., QUY V., RODRIGUEZ-GONZALVEZ C., SAUNDERS R.D.E., SCAIFE A.M.M., SCHOFIELD J., SCOTT P.F., SHAW C., SHIMWELL T.W., SMITH H., TAYLOR A.C., TITTERINGTON D.J., VELIC M., WALDRAM E.M., WEST S., WOOD B.A. and YASSIN G.

Abstract (from CDS):

The Arcminute Microkelvin Imager is a pair of interferometer arrays operating with six frequency channels spanning 13.9-18.2GHz, for observations on angular scales of 30arcsec-10arcmin and for declinations greater than -15°; the Small Array has a sensitivity of 30mJy s–1/2 and the Large Array has a sensitivity of 3mJys–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.

Abstract Copyright: © 2008 The Authors. Journal compilation © 2008 RAS

Journal keyword(s): instrumentation: interferometers - telescopes - galaxies: clusters: general - cosmic microwave background - cosmology: observations - radio continuum: general

Simbad objects: 2

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