2009/05/06 by Jayanth Chennamangalam, Yogesh Maan, Chennamangalam, Jayanth +4
Biochemistry, Genetics and Molecular Biology · Physics and Astronomy · #Astronomy and Astrophysical Research #FOS: Physical sciences #Instrumentation and Methods for Astrophysics (astro-ph.IM) #Pulsars and Gravitational Waves Research #Spectroscopy Techniques in Biomedical and Chemical Research #astro-ph.IM
paper · pdf · doi:10.48550/arxiv.0905.0888
4 pages, 2 figures, The Low-Frequency Radio Universe, Proceedings of a conference held at NCRA-TIFR, Pune, 8-12 December 2008, ASP Conference Series, Vol. 407, 2009, Eds: D. J. Saikia, D. A. Green, Y. Gupta and T. Venturi
openalex publication_date 2009/05/06 · arxiv created 2010/01/29 · arxiv updated 2010/02/08 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28
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.