论文标题

从ASKAP-EMU PILOT调查中发现大量合并群集SPT-CL 2023-5535中的无线电遗物

Discovery of a Radio Relic in the Massive Merging Cluster SPT-CL 2023-5535 from the ASKAP-EMU PILOT SURVEY

论文作者

HyeongHan, Kim, Jee, M. James, Rudnick, Lawrence, Parkinson, David, Finner, Kyle, Yoon, Mijin, Lee, Wonki, Brunetti, Gianfranco, Brüggen, Marcus, Collier, Jordan D., Hopkins, Andrew M., Michałowski, Michał J., Norris, Ray P., Riseley, Chris

论文摘要

ASKAP-EMU调查是一项深层广播连续调查,旨在覆盖整个南部的天空,而北方天空的很大一部分则达到$+30^{\ circ} $。在这里,我们报告了从askap-emu Pilot 300平方deg调查(800-1088 MHz)合并群集SPT-CL 2023-5535中发现的无线电遗物。深层高分辨率数据显示,$ \ sim2 $ mpc尺度的无线电光环在东西方向延伸,与群内气体一致。无线电遗物位于该电台光环的西部边缘,在南北方向上延伸了$ \ sim0.5 $ MPC。狭窄带宽内无线电遗物的集成光谱索引为$α^{\ scriptStyle \ rm 1088〜mhz} _ {\ scriptStyle \ rm 800〜mhz} = -0.76 \ pm pm 0.06 $。我们的弱镜头分析表明,系统是巨大的($ m_ {200} = 1.04 \ pm0.36 \ times 10^{15} m _ {\ odot} $),并且至少由三个子观点组成。我们建议一种场景,其中无线电特征是由于东部和中间子场所之间的碰撞引起的。我们的发现说明了ASKAP-EMU调查在检测星系簇中扩散排放的有效性,完成后,调查将大大增加与弥散无线电排放的合并群集检测的数量。

The ASKAP-EMU survey is a deep wide-field radio continuum survey designed to cover the entire southern sky and a significant fraction of the northern sky up to $+30^{\circ}$. Here, we report a discovery of a radio relic in the merging cluster SPT-CL 2023-5535 at z=0.23 from the ASKAP-EMU pilot 300 sq. deg survey (800-1088 MHz). The deep high-resolution data reveal a $\sim2$ Mpc-scale radio halo elongated in the east-west direction, coincident with the intracluster gas. The radio relic is located at the western edge of this radio halo stretched $\sim0.5$ Mpc in the north-south orientation. The integrated spectral index of the radio relic within the narrow bandwidth is $α^{\scriptstyle \rm 1088~MHz}_{\scriptstyle \rm 800~MHz}=-0.76 \pm 0.06$. Our weak-lensing analysis shows that the system is massive ($M_{200}=1.04\pm0.36\times 10^{15} M_{\odot}$) and composed of at least three subclusters. We suggest a scenario, wherein the radio features arise from the collision between the eastern and middle subclusters. Our discovery illustrates the effectiveness of the ASKAP-EMU survey in detecting diffuse emissions in galaxy clusters and when completed, the survey will greatly increase the number of merging cluster detections with diffuse radio emissions.

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