Experiments with calibrated digital sideband separating downconversion
arXiv:1001.5422 · doi:10.1086/651525
Abstract
This article reports on the first step in a focused program to re-optimize radio astronomy receiver architecture to better take advantage of the latest advancements in commercial digital technology. Specifically, an L-Band sideband-separating downconverter has been built using a combination of careful (but ultimately very simple) analog design and digital signal processing to achieve wideband downconversion of an RFI-rich frequency spectrum to baseband in a single mixing step, with a fixed-frequency Local Oscillator and stable sideband isolation exceeding 50 dB over a 12 degree C temperature range.
10 pages, 12 figures, to be published in PASP
Cited by in corpus (5)
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- Unformatted Digital Fiber-Optic Data Transmission for Radio Astronomy Front-Ends
- Digital compensation of the side-band-rejection ratio in a fully analog 2SB sub-millimeter receiver