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Results with the Extended MERLIN

Published online by Cambridge University Press:  19 July 2016

R. D. Davies
Affiliation:
Nuffield Radio Astronomy Laboratories, Jodrell Bank, Macclesfield, Cheshire SK11 9DL, UK

Extract

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A major enhancement of MERLIN completed in 1992 has led to a transformation of its capabilities. The seventh telescope added to the array is a 32-m telescope at Cambridge which provides high sensitivity on all the longest baselines where extra collecting area is especially beneficial. The 32-m telescope is a shaped primary-Cassegrain configuration which achieves an 80 percent aperture efficiency. A change from frequency to amplitude modulation in the microwave links increased the effective bandwidth from 9 to 30 MHz. This broadbanding enables the two hands of circular polarization to be transmitted simultaneously, each in a 15 MHz bandwidth. A further improvement in the system sensitivity was achieved by cryogenically cooling the low noise amplifiers in the front-end receivers.

Type
Imaging Results: Radio and Millimeter Waves
Copyright
Copyright © Kluwer 1994 

References

Patnaik, A.R. et al. 1992a. M.N.R.A.S., 254, 665.CrossRefGoogle Scholar
Patnaik, A.R. et al. 1992b. M.N.R.A.S., 259, 1P.Google Scholar
Patnaik, A.R. et al. 1992c. M.N.R.A.S., in press.Google Scholar
Pavelin, P.E. et al. 1992. Nature, submitted,Google Scholar
Pedlar, A. et al. 1992. M.N.R.A.S. submitted.Google Scholar