To gain further insight on the origin of diffuse radio sources in galaxy clusters and their connection with cluster merger processes, we performed GMRT low frequency observations of the radio halos, relics and new candidates belonging to the GMRT Radio Halo Cluster Sample first observed at 610MHz. Our main aim was to investigate their observational properties and integrated spectrum at frequencies below 610MHz.
Cone search capability for table J/A+A/551/A24/table1 (Clusters observed with the GMRT)
Cone search capability for table J/A+A/551/A24/table3 (Properties of the discrete radio sources)