Two efficient, new techniques for detecting dispersed radio pulses with interferometers: The Chirpolator and The Chimageator
arXiv:1109.3186 · doi:10.1088/0067-0049/196/2/16
Abstract
Searching for dispersed radio pulses in interferometric data is of great scientific interest, but poses a formidable computational burden. Here we present two efficient, new antenna-coherent solutions: The Chirpolator and The Chimageator. We describe the equations governing both techniques and propose a number of novel optimizations. We compare the implementation costs of our techniques with classical methods using three criteria: the operations rates (1) before and (2) after the integrate-and-dump stage, and (3) the data rate directly after the integrate-and-dump stage. When compared with classical methods, our techniques excel in the regime of sparse arrays, where they both require substantially lower data rates, and The Chirpolator requires a much lower post-integrator operations rate. In general, our techniques require more pre-integrator operations than the classical ones. We argue that the data and operations rates required by our techniques are better matched to future supercomputer architectures, where the arithmetic capability is outstripping the bandwidth capability. Our techniques are, therefore, viable candidates for deploying on future interferometers such as the Square Kilometer Array.
Accepted for publication in ApJS. 14 figures, 2 tables
References in corpus (11)
- Shapiro delay measurement of a two solar mass neutron star
- A bright millisecond radio burst of extragalactic origin
- Tests of general relativity from timing the double pulsar
- The Parkes multibeam pulsar survey: VI. Discovery and timing of 142 pulsars and a Galactic population analysis
- On the birthrates of Galactic neutron stars
- Modeling the Magnetic Field in the Galactic Disk using New Rotation Measure Observations from the Very Large Array
- Radio Bursts with Extragalactic Spectral Characteristics Show Terrestrial Origins
- V-FASTR: The VLBA Fast Radio Transients Experiment
- Discovery and timing of the first 8gr8 Cygnus survey pulsars
- Detection Rates for Surveys for Fast Transients with Next Generation Radio Arrays
- Source detection in interferometric visibility data. I. Fundamental estimation limits
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