DETECTION OF FAST RADIO TRANSIENTS WITH MULTIPLE STATIONS: A CASE STUDY USING THE VERY LONG BASELINE ARRAY

Recent investigations reveal an important new class of transient radio phenomena that occur on submillisecond timescales. Often, transient surveys' data volumes are too large to archive exhaustively. Instead, an online automatic system must excise impulsive interference and detect candidate events in real time. This work presents a case study using data from multiple geographically distributed stations to perform simultaneous interference excision and transient detection. We present several algorithms that incorporate dedispersed data from multiple sites, and report experiments with a commensal real-time transient detection system on the Very Long Baseline Array. We test the system using observations of pulsar B0329+54. The multiple-station algorithms enhanced sensitivity for detection of individual pulses. These strategies could improve detection performance for a future generation of geographically distributed arrays such as the Australian Square Kilometre Array Pathfinder and the Square Kilometre Array.

[1]  Alan E. E. Rogers,et al.  The Murchison Widefield Array: Design Overview , 2009, Proceedings of the IEEE.

[2]  R. Ekers,et al.  RADIO BURSTS WITH EXTRAGALACTIC SPECTRAL CHARACTERISTICS SHOW TERRESTRIAL ORIGINS , 2010, 1009.5392.

[3]  Alexei V. Filippenko,et al.  Submillijansky Transients in Archival Radio Observations , 2007, 0705.3158.

[4]  D. Werthimer,et al.  ERRATUM: “THE ALLEN TELESCOPE ARRAY TWENTY-CENTIMETER SURVEY—A 690 DEG2, 12 EPOCH RADIO DATA SET. I. CATALOG AND LONG-DURATION TRANSIENT STATISTICS” (2010, ApJ, 719, 45) , 2010 .

[5]  J. van Paradijs,et al.  The many faces of neutron stars , 1998 .

[6]  A. Hopkins,et al.  Science with ASKAP , 2008, 0810.5187.

[7]  P. A. Fridman,et al.  A method of detecting radio transients , 2010, 1008.3152.

[8]  Justin L. Jonas,et al.  MeerKAT—The South African Array With Composite Dishes and Wide-Band Single Pixel Feeds , 2009, Proceedings of the IEEE.

[9]  Radford M. Neal Pattern Recognition and Machine Learning , 2007, Technometrics.

[10]  J. Karvanen,et al.  Trimmed estimators for robust averaging of event-related potentials , 2005, Journal of Neuroscience Methods.

[11]  M. Popov,et al.  Analysis of the scintillation pattern of the pulsar PSR B0329+54 based on VLBI data at 1650 MHz , 2004 .

[12]  Berkeley,et al.  New SETI Sky Surveys for Radio Pulses , 2008, 0811.3046.

[13]  J. Mclaughlin Searches for Fast Radio Transients , 2003, astro-ph/0304364.

[14]  Michael S. Warren,et al.  The Commensal Real-Time ASKAP Fast-Transients (CRAFT) Survey , 2010, Publications of the Astronomical Society of Australia.

[15]  R. N. Manchester,et al.  Transient radio bursts from rotating neutron stars , 2005, Nature.

[16]  A. T. Deller,et al.  DiFX: A Software Correlator for Very Long Baseline Interferometry Using Multiprocessor Computing Environments , 2007, astro-ph/0702141.

[17]  R. Rosenfeld Nature , 2009, Otolaryngology--head and neck surgery : official journal of American Academy of Otolaryngology-Head and Neck Surgery.

[18]  J. van Leeuwen,et al.  The Radio Sky on Short Timescales with LOFAR: Pulsars and Fast Transients , 1984 .

[19]  Dipankar Bhattacharya Detection of Radio Emission from Pulsars , 1998 .

[20]  B. J. Rickett,et al.  Radio propagation through the turbulent interstellar plasma. , 1990 .

[21]  T. Joseph W. Lazio,et al.  The dynamic radio sky , 2004 .

[22]  S. Ellingson Rfi Mitigation And The Ska , 2004 .

[23]  J. Cordes,et al.  ARECIBO PULSAR SURVEY USING ALFA: PROBING RADIO PULSAR INTERMITTENCY AND TRANSIENTS , 2008, 0811.2532.

[24]  David R. Thompson,et al.  V-FASTR: THE VLBA FAST RADIO TRANSIENTS EXPERIMENT , 2011, 1104.4908.

[25]  R. Davies,et al.  Astronomical Society of the Pacific Conference Series , 2010 .

[26]  M. Mclaughlin,et al.  A Bright Millisecond Radio Burst of Extragalactic Origin , 2007, Science.

[27]  Stergios B. Fotopoulos,et al.  All of Nonparametric Statistics , 2007, Technometrics.

[28]  Detection of a radio counterpart to the 27 December 2004 giant flare from SGR 1806–20 , 2005, Nature.