论文标题

Merghers Pilot:Meerkat发现了从ACT中发现的9个巨大的Sunyaev-Zel'Dovich选择的星系簇

MERGHERS Pilot: MeerKAT discovery of diffuse emission in nine massive Sunyaev-Zel'dovich-selected galaxy clusters from ACT

论文作者

Knowles, K., Pillay, D. S., Amodeo, S., Baker, A. J., Basu, K., Crichton, D., de Gasperin, F., Devlin, M., Ferrari, C., Hilton, M., Huffenberger, K. M., Hughes, J. P., Koopman, B. J., Moodley, K., Mroczkowski, T., Naess, S., Nati, F., Newburgh, L. B., Oozeer, N., Page, L., Partridge, B., Pfrommer, C., Salatino, M., Schillaci, A., Sifón, C., Smirnov, O., Sikhosana, S. P., Wollack, E. J., Xu, Z.

论文摘要

Meerkat探索文物,巨型光环和玛格拉术无线电来源(Merghers)调查是一个计划的项目,旨在研究使用Meerkat天文台研究的大型星系簇样本。在这里,我们介绍了一个16小时的试点项目的结果,该项目响应于2019年的Meerkat共享风险建议电话,以测试使用Short(0.2----2.1 \,小时)整合时间使用Meerkat进行大型聚类研究的可行性。该飞行员的重点是1.28 \,GHz观察13个大型,低到中间的红移($ 0.22 <z <0.65 $),来自Sunyaev-Zel'Dovich选择的Atacama Cosmology telescope(ACT)DR5 Catalog drd Catalog the Multiiwavellength指示动态干扰的指示。这项试点研究以70%的检测率(9/13簇)验证了我们提出的观察策略的拟议梅尔格斯,并提供了十二种扩散排放的检测,其中有11个是新的,这表明Meerkat的强度用于此类研究。概述(信噪比$ \ gtrsim6 $)总结如下:两个系统主机同时使用遗物和一个巨大的无线电晕,五个系统主机无线电晕和两个具有候选无线电晕。假设$α= -1.3 \ pm 0.4 $的基准频谱指数与已知的无线电晕和遗物缩放关系一致,则功率值,$ k $校正至1.4 GHz。

The MeerKAT Exploration of Relics, Giant Halos, and Extragalactic Radio Sources (MERGHERS) survey is a planned project to study a large statistical sample of galaxy clusters with the MeerKAT observatory. Here we present the results of a 16--hour pilot project, observed in response to the 2019 MeerKAT Shared Risk proposal call, to test the feasibility of using MeerKAT for a large cluster study using short (0.2--2.1\,hour) integration times. The pilot focuses on 1.28\,GHz observations of 13 massive, low-to-intermediate redshift ($0.22 < z < 0.65$) clusters from the Sunyaev-Zel'dovich-selected Atacama Cosmology Telescope (ACT) DR5 catalogue that show multiwavelength indications of dynamical disturbance. With a 70 per cent detection rate (9/13 clusters), this pilot study validates our proposed MERGHERS observing strategy and provides twelve detections of diffuse emission, eleven of them new, indicating the strength of MeerKAT for such types of studies. The detections (signal-to-noise ratio $\gtrsim6$) are summarised as follows: two systems host both relic(s) and a giant radio halo, five systems host radio halos, and two have candidate radio halos. Power values, $k$-corrected to 1.4 GHz assuming a fiducial spectral index of $α= -1.3 \pm 0.4$, are consistent with known radio halo and relic scaling relations.

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