SoUthern Cluster sCale Extended Source Survey (SUCCESS): a GMRT and Meerkat study of nine massive galaxy clusters

• Published in: Monthly Notices of the Royal Astronomical Society
• Main Authors: Kale, R, Parekh, V, Rahaman, M, Joshi, D C, Venturi, T, Kolokythas, K, Chibueze, J O, Sikhosana, S, Pillay, D, Knowles, K
• Other Authors: Department of Atomic Energy, Government of India, National Aeronautics and Space Administration, Goddard Space Flight Center, Department of Science and Technology, DST, Ministry of Science and Technology of Taiwan, MOST, Ministero degli Affari Esteri e della Cooperazione Internazionale, National Research Foundation, NRF, SPS, Tata Institute of Fundamental Research, NED, Jet Propulsion Laboratory, California Institute of Technology
• Format: Article in Journal/Newspaper
• Language: English
• Published: Oxford University Press (OUP) 2022
• Subjects: South pole
• Online Access: http://dx.doi.org/10.1093/mnras/stac1649; https://academic.oup.com/mnras/advance-article-pdf/doi/10.1093/mnras/stac1649/44112437/stac1649.pdf; https://academic.oup.com/mnras/article-pdf/514/4/5969/44858369/stac1649.pdf

ABSTRACT We aim to carry out a radio study of the SoUthern Cluster sCale Extended Source Survey (SUCCESS) sample consisting of 20 massive (M500 > 5 × 1014 M⊙), nearby (redshift <0.3) and southern (−50° < δ < −30°) galaxy clusters detected by the Planck satellite and the South Pole Telescope. Here, we report targeted GMRT observations (325/610 MHz) for a subsample of nine clusters. We also use the first data release of MeerKAT Galaxy Cluster Legacy Survey (1283 MHz) for five of these nine clusters. The properties of the mini-halo in RXC J0528.9-3927, a candidate mini-halo in A3322, the radio halo and candidate double relics in A3399, and the radio halo in RXC J0232.2-4420 are presented. We also report a detection of candidate radio relics at distances 1 and 1.9 Mpc from the centre of RXC J0232.2-4420. The southeast relic of A3399 is consistent with the radio power–mass scaling relation for radio relics, while the candidate relics around RXC J0232.2-4420 are outliers. This indicates an origin of the candidate relics near RXC J0232.2-4420 to be independent of this cluster and a cluster merger-shock origin for the relic in A3399. In this subsample of clusters, 1/9 hosts a radio halo and double relics, 1/9 hosts a radio halo and 2/9 host mini-haloes. The dynamical states based on X-ray morphology show that A3399 is a disturbed cluster; however, the radio halo cluster RXC J0232.2-4420 is relaxed, and the mini-halo clusters have intermediate morphologies, adding to the cases of the less commonly found associations.