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

Author:

Kale R1ORCID,Parekh V23ORCID,Rahaman M45ORCID,Joshi D C1,Venturi T6,Kolokythas K7ORCID,Chibueze J O78ORCID,Sikhosana S910,Pillay D910,Knowles K2ORCID

Affiliation:

1. National Centre for Radio Astrophysics, Tata Institute of Fundamental Research , S. P. Pune University Campus, Ganeshkhind, Pune 411007, India

2. Centre for Radio Astronomy Techniques and Technologies, Department of Physics and Electronics, Rhodes University , PO Box 94, Makhanda, 6140, South Africa

3. South African Radio Astronomy Observatory (SARAO) , 2 Fir Street, Black River Park, Observatory, Cape Town 7925, South Africa

4. Department of Astronomy, Astrophysics and Space Engineering, Indian Institute of Technology Indore , Indore 453552, India

5. Institute of Astronomy, National Tsing Hua University , Hsinchu 300, Taiwan

6. INAF , Istituto di Radioastronomia Via Gobetti 101, I-40129 Bologna, Italy

7. Centre for Space Research, North-West University , Potchefstroom 2520, South Africa

8. Department of Physics and Astronomy, Faculty of Physical Sciences, University of Nigeria , Carver Building, 1 University Road, Nsukka 410105, Nigeria

9. Astrophysics Research Centre, University of KwaZulu-Natal , Durban 4041, South Africa

10. School of Mathematics, Statistics, and Computer Science, University of KwaZulu-Natal , Westville 3696, South Africa

Abstract

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.

Funder

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

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

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