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
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.