论文标题

南部群集量表扩展源调查(成功):九个大型星系簇的GMRT和Meerkat研究

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

论文作者

Kale, R., Parekh, V., Rahaman, M., Joshi, D. C., Venturi, T., Kolokythas, K., Chibueze, J. O., Sikhosana, S., Pillay, D., Knowles, K.

论文摘要

我们的目标是对南部集群量表扩展源调查(成功)样本进行无线电研究,该样本由二十个(m $ _ {500}> 5 \ times10^{14} $ m $ _ {\ odot} $),附近(redshift $ <0.3 $)和Southern($ -50^^cluse cluse cluse)普朗克卫星和南极望远镜。在这里,我们报告了针对9个簇的子样本的针对性GMRT观测值(325/610 MHz)。我们还使用Meerkat Galaxy群集遗产调查(1283 MHz)的第一个数据发布,其中五个群集中有五个。介绍了RXC J0528.9-3927中的迷你山地,A3322中的候选小型山洛,A3399中的无线电晕和候选列表以及RXC J0232.2-4420的无线电晕。我们还报告了距RXC J0232.2-4420中心1和1.9 MPC的候选无线电遗迹的检测。 A3399的东南遗物与无线电储物的无线电功率 - 质量扩展关系一致,而RXC J0232.2-4420围绕的候选遗物是异常值。这表明RXC J0232.2-4420附近的候选遗物的起源独立于该集群,并且在A3399中为遗物的集群合并震动起源。在这个集群1/9的子样本中,有一个无线电光环和双文物,1/9主持了无线电光环和2/9主机Mini-Halos。基于X射线形态的动力状态表明,A3399是一个受干扰的群集。然而,无线电晕圈RXC J0232.2-4420放松,而迷你挂起簇具有中间形态,这增加了较不常见的关联的情况。

We aim to carry out a radio study of the SoUthern Cluster sCale Extended Source Survey (SUCCESS) sample consisting of twenty massive (M$_{500} > 5\times10^{14}$ M$_{\odot}$), nearby (redshift $<0.3$) and southern ($-50^{\circ} < δ< -30^\circ$) galaxy clusters detected by the Planck satellite and the South Pole Telescope. Here we report targeted GMRT observations (325/610 MHz) for a sub-sample 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 detection of candidate radio relics at distances 1 and 1.9 Mpc from the center 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 sub-sample of clusters 1/9 hosts a radio halo and double relics, 1/9 hosts a radio halo and 2/9 host mini-halos. 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.

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