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The Very Small Array - status report

Michael E. Jones·P. F. Scott
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Abstract

We are contructing an interferometric telescope, the Very Small Array, to study the cosmic microwave background on angular scales 0.2--4.5 degrees. The physical layout and electronic design of the telescope are optimised to give maximum protection from systematic effects, while still providing sufficient sensitivity to make high signal-to-noise images. A prototype single baseline is currently being tested, with scientific results expected during 2000.

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Michael E. Jones, P. F. Scott. 1998-04-17. The Very Small Array - status report. https://arxiv.org/abs/astro-ph/9804175

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