Please use this identifier to cite or link to this item: https://dspace.iiti.ac.in/handle/123456789/10826
Title: SoUthern Cluster sCale Extended Source Survey (SUCCESS): a GMRT and Meerkat study of nine massive galaxy clusters
Authors: Rahaman, Majidul;
Keywords: Galaxies; Morphology; Acceleration of particles; Cluster scale; Galaxies clusters; Galaxies: clusters: individual: Virgo; Galaxies: clusters: intracluster mediums; Galaxy:cluster:individual: a3322, a3396, a3343, a3399, a3937, RXC j0232.2-4420, RXC j0528.9-3927, RXC j1358.9-4750, PSZ1 g313.85 + 19.21; Radiation mechanisms: nonthermal; Radio continuum: galaxies; Radio halo; X-rays galaxies clusters; Surveys
Issue Date: 2022
Publisher: Oxford University Press
Citation: Kale, R., Parekh, V., Rahaman, M., Joshi, D. C., Venturi, T., Kolokythas, K., . . . Knowles, K. (2022). SoUthern cluster sCale extended source survey (SUCCESS): A GMRT and meerkat study of nine massive galaxy clusters. Monthly Notices of the Royal Astronomical Society, 514(4), 5969-5986. doi:10.1093/mnras/stac1649
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. © 2022 The Author(s).
URI: https://doi.org/10.1093/mnras/stac1649
https://dspace.iiti.ac.in/handle/123456789/10826
ISSN: 0035-8711
Type of Material: Journal Article
Appears in Collections:Department of Astronomy, Astrophysics and Space Engineering

Files in This Item:
There are no files associated with this item.


Items in DSpace are protected by copyright, with all rights reserved, unless otherwise indicated.

Altmetric Badge: