Next Generation Radio Astronomy Receiver Systems
Matthew A. Morgan, J. Richard Fisher

TL;DR
This paper proposes a comprehensive redesign of radio astronomy receiver systems, leveraging modern digital and optical technologies to enhance sensitivity, reduce costs, and improve reliability for large-scale astronomical observations.
Contribution
It introduces an integrated receiver architecture that combines RF to digital conversion, analog to digital, and copper to fiber transitions within a single module, optimizing performance and cost.
Findings
Enhanced receiver sensitivity approaching fundamental limits
Reduced system cost and complexity through integration
Improved reliability and reproducibility of receiver systems
Abstract
Radio astronomy observations in the coming decade will require new levels of sensitivity while mapping large regions of space with much greater efficiency than is achieved with current telescopes. This requires new instrumentation with the greatest achievable sensitivity, dynamic range, and field of view. Receiver noise is quickly approaching fundamental limits at most radio wavelengths, so significant gains in sensitivity can only be made by increasing collecting area. Jointly, these requirements suggest using large arrays of smaller antennas, or many moderate-size antennas equipped with multi-beam arrays. The challenge is to develop receivers and wide bandwidth data transport systems which are lower cost, more compact, more reliable, lower weight, and more reproducible than the best current systems, with no compromise to performance. This can be achieved with a greater degree of…
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Taxonomy
TopicsRadio Astronomy Observations and Technology · Astronomy and Astrophysical Research · Superconducting and THz Device Technology
