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Please use this identifier to cite or link to this item: http://hdl.handle.net/2289/4125
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dc.contributor.authorChennamangalam, J.-
dc.contributor.authorMaan, Yogesh-
dc.contributor.authorDeshpande, A.A.-
dc.date.accessioned2011-08-23T09:52:18Z-
dc.date.available2011-08-23T09:52:18Z-
dc.date.issued2009-09-
dc.identifier.citationASP Conference Series, 2009, Vol.407, p442en
dc.identifier.urihttp://hdl.handle.net/2289/4125-
dc.descriptionRestricted Access. An open-access version is available at the alternative location.en
dc.description.abstractAlthough 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.en
dc.language.isoenen
dc.publisherAstronomical Society of the Pacificen
dc.relation.urihttp://adsabs.harvard.edu/abs/2009ASPC..407..442Cen
dc.relation.urihttp://arxiv.org/abs/0905.0888en
dc.rights2009 Astronomical Society of the Pacific.en
dc.titleSoftware data-processing pipeline for transient detectionen
dc.typeArticleen
dc.additionalProceedings 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.en
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