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A Submillimetre Imaging Polarimeter at the James Clerk Maxwell Telescope

J. S. Greaves·W. S. Holland·T. Jenness·A. Chrysostomou·D. S. Berry·A. G. Murray·M. Tamura·E. I. Robson·P. A. R. Ade·R. Nartallo·J. A. Stevens·M. Momose·J. -I. Morino·G. Moriarty-Schieven·F. Gannaway·C. V. Haynes
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Abstract

A polarimeter has been built for use with the Submillimetre Common-User Bolometer Array (SCUBA), on the James Clerk Maxwell Telescope (JCMT) in Hawaii. SCUBA is the first of a new generation of highly sensitive submillimetre cameras, and the UK/Japan Polarimeter adds a polarimetric imaging/photometry capability in the wavelength range 350 to 2000 microns. Early science results range from measuring the synchrotron polarization of the black hole candidate Sgr A* to mapping magnetic fields inferred from polarized dust emission in Galactic star-forming clouds. We describe the instrument design, performance, observing techniques and data reduction processes, along with an assessment of the current and future scientific capability.

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J. S. Greaves, W. S. Holland, T. Jenness, A. Chrysostomou, D. S. Berry, A. G. Murray, M. Tamura, E. I. Robson, P. A. R. Ade, R. Nartallo, J. A. Stevens, M. Momose, J. -I. Morino, G. Moriarty-Schieven, F. Gannaway, C. V. Haynes. 2003-02-28. A Submillimetre Imaging Polarimeter at the James Clerk Maxwell Telescope. https://doi.org/10.1046/j.1365-8711.2003.06230.x

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