DiFX-2: A More Flexible, Efficient, Robust, and Powerful Software Correlator
dc.contributor.author | Deller, A. T. | |
dc.contributor.author | Brisken, W. F. | |
dc.contributor.author | Phillips, C. J. | |
dc.contributor.author | Morgan, John | |
dc.contributor.author | Alef, W. | |
dc.contributor.author | Cappallo, R. | |
dc.contributor.author | Middelberg, E. | |
dc.contributor.author | Romney, J. | |
dc.contributor.author | Rottmann, H. | |
dc.contributor.author | Tingay, Steven | |
dc.contributor.author | Wayth, Randall | |
dc.date.accessioned | 2017-01-30T13:30:40Z | |
dc.date.available | 2017-01-30T13:30:40Z | |
dc.date.created | 2012-03-12T20:01:09Z | |
dc.date.issued | 2011 | |
dc.identifier.citation | Deller, A. T. and Brisken, W. F. and Phillips, C. J. and Morgan, J. and Alef, W. and Cappallo, R. and Middelberg, E. et al. DiFX-2: A More Flexible, Efficient, Robust, and Powerful Software Correlator. Publications of the Astronomical Society of the Pacific. 123 (901): pp. 275-287. | |
dc.identifier.uri | http://hdl.handle.net/20.500.11937/32383 | |
dc.identifier.doi | 10.1086/658907 | |
dc.description.abstract |
Software correlation, where a correlation algorithm written in a high-level language such as C++ is run on commodity computer hardware, has become increasingly attractive for small-to medium-sized and/or bandwidth-constrained radio interferometers. In particular, many long-baseline arrays (which typically have fewer than 20 elements and are restricted in observing bandwidth by costly recording hardware and media) have utilized software correlators for rapid, cost-effective, correlator upgrades to allow compatibility with new, wider-bandwidth, recording systems and to improve correlator flexibility. The DiFX correlator, made publicly available in 2007, has been a popular choice in such upgrades and is now used for production correlation by a number of observatories and research groups worldwide. Here, we describe the evolution in the capabilities of the DiFX correlator over the past three years, including a number of new capabilities, substantial performance improvements, and a large amount of supporting infrastructure to ease use of the code. New capabilities include the ability to correlate a large number of phase centers in a single correlation pass, the extraction of phase-calibration tones, correlation of disparate but overlapping sub-bands, the production of rapidly sampled filter-bank and kurtosis data at minimal cost, and many more. The latest version of the code is at least 15% faster than the original (and in certain situations, many times this value). Finally, we also present detailed test results validating the correctness of the new code. | |
dc.publisher | University of Chicago Press | |
dc.subject | Astronomical Instrumentation | |
dc.title | DiFX-2: A More Flexible, Efficient, Robust, and Powerful Software Correlator | |
dc.type | Journal Article | |
dcterms.source.volume | 123 | |
dcterms.source.number | 901 | |
dcterms.source.startPage | 275 | |
dcterms.source.endPage | 287 | |
dcterms.source.issn | 0004-6280 | |
dcterms.source.title | Publications of the Astronomical Society of the Pacific | |
curtin.department | Curtin Institute of Radio Astronomy | |
curtin.accessStatus | Open access |