tokens: ACKNOWLEDGEMENTS We thank the anonymous referee for critical comments that have improved this paper. RK acknowledges support through the DST-INSPIRE Faculty Award by the Government of India. We thank the staff of the GMRT that made these observations possible. GMRT is run by the National Centre for Radio Astrophysics of the Tata Institute of Fundamental Research. This research has made use of the NASA/IPAC Extragalactic Database (NED) which is operated by the Jet Propulsion Laboratory, California Institute of Technology, under contract with the National Aeronautics and Space Administration. This research made use of Astropy, a community-developed core python package for Astronomy (Astropy Collaboration, 2018). The scientific results reported in this article are based in part on data obtained from the Chandra Data Archive.
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