Allen Telescope Array digital processing requirements driven by radio frequency interference concerns

Author:

Harp G. R.1

Affiliation:

1. Allen Telescope Array; SETI Institute; Mountain View; California; USA

Publisher

American Geophysical Union (AGU)

Subject

Electrical and Electronic Engineering,General Earth and Planetary Sciences,Condensed Matter Physics

Reference29 articles.

1. A new approach to interference excision in radio astronomy: Real time adaptive filtering;Barnbaum;Astron. J.,1998

2. Benson , J. F. Owen 2000 Scientific requirements for the EVAL real-time system EVLA Memo 15 Expanded Very Large Array Socorro, N. M. http://www.aoc.nrao.edu/evla/geninfo/memoseries/evlamemo15.ps.gz

3. The S2 VLBI correlator: A correlator for space VLBI and geodetic signal processing;Carlson;Publ. Astron. Soc. Pac.,1999

4. D'Addario , L. R. 2001 Notes on delay and phase tracking for the ATA ATA Memo Ser. 27 Allen Telescope Array Mountain View, Calif. http://astron.berkeley.edu/ral/ata/memos/memo27.pdf

5. D'Addario , L. R. 2001 Processing architectures for complex gain tracking ATA Memo Ser. 40 Allen Telescope Array Mountain View, Calif. http://astron.berkeley.edu/ral/ata/memos/memo40.pdf

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1. Parallel Implementation of SUMPLE Algorithm in Large-Scale Antenna Array;Lecture Notes in Electrical Engineering;2019-08-14

2. StarWatch 3.0: Visualizing Wave Patterns of Phased Array Radio Telescopes;2017 International Conference on Cyberworlds (CW);2017-09

3. StarWatch 2.0: RFI Filter for SETI Signals;2016 International Conference on Cyberworlds (CW);2016-09

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