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      https://www.ias.ac.in/article/fulltext/joaa/038/01/0011

    • Keywords

       

      Radio astronomy: radio telescope; receiver system; space weather watch: solar wind transients; cosmology: large scale structure of the Universe; fast radio bursts.

    • Abstract

       

      The legacy Ooty Radio Telescope (ORT) is being reconfigured as a 264-element synthesis telescope, called the Ooty Wide Field Array (OWFA). Its antenna elements are the contiguous 1.92 m sections of the parabolic cylinder. It will operate in a 38-MHz frequency band centred at 326.5 MHz and will be equipped with a digital receiver including a 264-element spectral correlator with a spectral resolution of 48 kHz. OWFA is designed to retain the benefits of equatorial mount, continuous 9-hour tracking ability and large collecting area of the legacy telescope and use of modern digital techniques to enhance the instantaneous field-of-view by more than an order of magnitude. OWFA has unique advantages for contemporary investigations related to large scale structure, transient events and space weather watch. In this paper, we describe the RF subsystems, digitizers and fibre optic communication of OWFA and highlight some specific aspects of the system relevant for the observations planned during the initial operation.

    • Author Affiliations

       

      C. R. Subrahmanya1 P. Prasad1 B. S. Girish1 R. Somashekar1 P. K. Manoharan2 A. K. Mittal2

      1. Raman Research Institute, C.V. Raman Avenue, Sadashivnagar, Bengaluru 560 080, India.
      2. Radio Astronomy Centre, NCRA-TIFR, P.O. Box 8, Ooty 643 001, India.
    • Dates

       
  • Journal of Astrophysics and Astronomy | News

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