Title:	Software data-processing pipeline for transient detection
Authors:	Chennamangalam, J. Maan, Yogesh Deshpande, A.A.
Issue Date:	Sep-2009
Publisher:	Astronomical Society of the Pacific
Citation:	ASP Conference Series, 2009, Vol.407, p442
Abstract:	Although several existing and upcoming telescopes have imaging as their primary mode, they also have a sensitive phased-array mode 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 pulsars and 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.
Description:	Restricted Access. An open-access version is available at the alternative location.
URI:	http://hdl.handle.net/2289/4125
Alternative Location:	http://adsabs.harvard.edu/abs/2009ASPC..407..442C http://arxiv.org/abs/0905.0888
Copyright:	2009 Astronomical Society of the Pacific.
Additional information:	Proceedings of the conference held 8-12 December 2008, at National Centre for Radio Astrophysics (NCRA), TIFR, Pune, India. Edited by D. J. Saikia, D. A. Green, Y. Gupta, and T. Venturi. San Francisco: Astronomical Society of the Pacific.
Appears in Collections:	Research Papers (A&A)

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