Software Data-Processing Pipeline for Transient Detection
2009
Although several existing and upcoming telescopes have imaging as their primary mode, they also have a sensitive
phased-arraymode with a multiple-beam forming capability enabling high time resolution studies of several types of objects, including
pulsars. For example, the potentially wide coverage in frequency, combined with its collecting area, makes the MWA-LFD a unique instrument for low-frequency detection and studies of
pulsarsand transients. A software data-processing pipeline is being developed by the Raman Research Institute for this purpose. We describe the various issues relevant to the detection strategies, illustrated with real data at low radio frequencies.
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