Using multiple-accumulator CMACs to improve efficiency of the X part of an input-buffered FX correlator

Author:

Lapshev Stepan,Hasan S. M. Rezaul

Publisher

Springer Science and Business Media LLC

Subject

Space and Planetary Science,Astronomy and Astrophysics

Reference9 articles.

1. D’Addario, L., Wang, D.: An integrated circuit for radio astronomy correlators supporting large arrays of antennas. In: Journal of Astronomical Instrumentation, vol. 5, no. 2, 26 pages. (2016)

2. Chikada, Y., Ishiguro, M., Hirabayashi, H.: A digital FFT spectro-correlator for radio astronomy. In: Roberts, J.A. (ed.) Indirect imaging. Measurement and processing for indirect imaging. Cambridge University Press, Cambridge (1984)

3. Romney J.: Cross correlators. In: Astronomical Society of the Pacific Conference Series, vol. 180, pp. 57–78. (1999)

4. Lapshev, S., Hasan, R.: On the architecture for the X part of a very large FX correlator using two-accumulator CMACs. In: Experimental Astronomy, vol. 41, pp. 259–270. (2016)

5. D’Addario L.: Low-power correlator architecture for the mid-frequency SKA. SKA Memo 133, 2011 March 21. Available at http://www.skatelescope.org/memos

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