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DC Field | Value | Language |
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dc.contributor.author | Rahaman, Majidul; | en_US |
dc.date.accessioned | 2022-11-03T19:42:26Z | - |
dc.date.available | 2022-11-03T19:42:26Z | - |
dc.date.issued | 2022 | - |
dc.identifier.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 | en_US |
dc.identifier.issn | 0035-8711 | - |
dc.identifier.other | EID(2-s2.0-85135173343) | - |
dc.identifier.uri | https://doi.org/10.1093/mnras/stac1649 | - |
dc.identifier.uri | https://dspace.iiti.ac.in/handle/123456789/10826 | - |
dc.description.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). | en_US |
dc.language.iso | en | en_US |
dc.publisher | Oxford University Press | en_US |
dc.source | Monthly Notices of the Royal Astronomical Society | en_US |
dc.subject | 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 | en_US |
dc.title | SoUthern Cluster sCale Extended Source Survey (SUCCESS): a GMRT and Meerkat study of nine massive galaxy clusters | en_US |
dc.type | Journal Article | en_US |
dc.rights.license | All Open Access, Green | - |
Appears in Collections: | Department of Astronomy, Astrophysics and Space Engineering |
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