Journal article
Characterizing the performance of high-speed data converters for RFSoC-based radio astronomy receivers
- Abstract:
- RF system-on-chip (RFSoC) devices provide the potential for implementing a complete radio astronomy receiver on a single board, but performance of the integrated analogue-to-digital converters (ADCs) is critical. We have evaluated the performance of the data converters in the Xilinx ZU28DR RFSoC, which are 12-bit, 8-fold interleaved converters with a maximum sample speed of 4.096 Giga-sample per second (GSPS). We measured the spurious-free dynamic range (SFDR), signal-to-noise and distortion (SINAD), effective number of bits (ENOB), intermodulation distortion (IMD), and cross-talk between adjacent channels over the bandwidth of 2.048 GHz. We both captured data for off-line analysis with floating-point arithmetic, and implemented a real-time integer arithmetic spectrometer on the RFSoC. The performance of the ADCs is sufficient for radio astronomy applications and close to the vendor specifications in most of the scenarios. We have carried out spectral integrations of up to 100 s and stability tests over tens of hours and find thermal noise-limited performance over these time-scales.
- Publication status:
- Published
- Peer review status:
- Peer reviewed
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                        (Preview, Accepted manuscript, 3.2MB, Terms of use)
 
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- Publisher copy:
- 10.1093/mnras/staa3895
Authors
- Publisher:
- Oxford University Press
- Journal:
- Monthly Notices of the Royal Astronomical Society More from this journal
- Volume:
- 501
- Issue:
- 4
- Pages:
- 5096-5104
- Publication date:
- 2020-12-21
- Acceptance date:
- 2020-12-14
- DOI:
- EISSN:
- 
                    1365-2966
- ISSN:
- 
                    0035-8711
- Language:
- 
                    English
- Keywords:
- Pubs id:
- 
                  1146380
- Local pid:
- 
                    pubs:1146380
- Deposit date:
- 
                    2021-02-17
Terms of use
- Copyright holder:
- Liu et al.
- Copyright date:
- 2021
- Rights statement:
- © 2020 The Author(s) Published by Oxford University Press on behalf of Royal Astronomical Society
- Notes:
- This is the accepted manuscript version of the article. The final version is available from Oxford University Press at: https://doi.org/10.1093/mnras/staa3895
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