DiFX-2: A More Flexible, Efficient, Robust, and Powerful Software Correlator

被引:364
作者
Deller, A. T. [1 ,2 ]
Brisken, W. F. [1 ]
Phillips, C. J. [3 ]
Morgan, J. [4 ]
Alef, W. [5 ]
Cappallo, R. [6 ]
Middelberg, E. [7 ]
Romney, J. [1 ]
Rottmann, H. [5 ]
Tingay, S. J. [4 ]
Wayth, R. [4 ]
机构
[1] Natl Radio Astron Observ, Socorro, NM 87801 USA
[2] Univ Calif Berkeley, Berkeley, CA 94720 USA
[3] CSIRO Astron & Space Sci, Australia Telescope Natl Facil, Epping, NSW, Australia
[4] Curtin Univ, Int Ctr Radio Astron Res, Perth, WA, Australia
[5] Max Planck Inst Radioastron, D-53010 Bonn, Germany
[6] MIT, Haystack Observ, Westford, MA 01886 USA
[7] Ruhr Univ Bochum, Astron Inst, D-44801 Bochum, Germany
关键词
D O I
10.1086/658907
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
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.
引用
收藏
页码:275 / 287
页数:13
相关论文
共 17 条
[1]  
[Anonymous], INTERFEROMETRY SYNTH
[2]   A 6 X 320-MHZ 1024-CHANNEL FFT CROSS-SPECTRUM ANALYZER FOR RADIO ASTRONOMY [J].
CHIKADA, Y ;
ISHIGURO, M ;
HIRABAYASHI, H ;
MORIMOTO, M ;
MORITA, KI ;
KANZAWA, T ;
IWASHITA, H ;
NAKAZIMA, K ;
ISHIKAWA, SI ;
TAKAHASHI, T ;
HANDA, K ;
KASUGA, T ;
OKUMURA, S ;
MIYAZAWA, T ;
NAKAZURU, T ;
MIURA, K ;
NAGASAWA, S .
PROCEEDINGS OF THE IEEE, 1987, 75 (09) :1203-1210
[3]   DiFX: A software correlator for very long baseline interferometry using multiprocessor computing environments [J].
Deller, A. T. ;
Tingay, S. J. ;
Bailes, M. ;
West, C. .
PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF THE PACIFIC, 2007, 119 (853) :318-336
[4]  
DELLER AT, 2010, POS IN PRESS
[5]   A deep, high-resolution survey of the low-frequency radio sky [J].
Lenc, E. ;
Garrett, M. A. ;
Wucknitz, O. ;
Anderson, J. M. ;
Tingay, S. J. .
ASTROPHYSICAL JOURNAL, 2008, 673 (01) :78-95
[6]  
MACQUART JPR, 2010, P ISKAF2010 SCI M TR
[7]  
MIDDELBERG E, 2010, A A UNPUB
[8]  
MORGAN JS, 2010, A A UNPUB
[9]   Radio frequency interference excision using spectral-domain statistics [J].
Nita, Gelu M. ;
Gary, Dale E. ;
Liu, Zhiwei ;
Hurford, Gordon J. ;
White, Stephen M. .
PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF THE PACIFIC, 2007, 119 (857) :805-827
[10]   Detection of compact radio emission from Circinus X-1 with the first Southern hemisphere e-VLBI experiment [J].
Phillips, C. J. ;
Deller, A. ;
Amy, S. W. ;
Tingay, S. J. ;
Tzioumis, A. K. ;
Reynolds, J. E. ;
Jauncey, D. L. ;
Stevens, J. ;
Ellingsen, S. P. ;
Dickey, J. ;
Fender, R. P. ;
Tudose, V. ;
Nicolson, G. D. .
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2007, 380 (01) :L11-L14