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Status and progress of China SKA Regional Centre prototype 被引量:1
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作者 Tao An Xiaocong Wu +5 位作者 Baoqiang Lao Shaoguang Guo Zhijun Xu Weijia Lv yingkang zhang Zhongli zhang 《Science China(Physics,Mechanics & Astronomy)》 SCIE EI CAS CSCD 2022年第12期72-90,共19页
The Square Kilometre Array(SKA)project consists of delivering two largest radio telescope arrays being built by the SKA Observatory(SKAO),which is an intergovernmental organization bringing together nations from aroun... The Square Kilometre Array(SKA)project consists of delivering two largest radio telescope arrays being built by the SKA Observatory(SKAO),which is an intergovernmental organization bringing together nations from around the world with China being one of the major member countries.The computing resources needed to process,distribute,curate and use the vast amount of data that will be generated by the SKA telescopes are too large for the SKAO to manage on its own.To address this challenge,the SKAO is working with the international community to create a shared,distributed data,computing and networking capability called the SKA Regional Centre Alliance.In this model,the SKAO will be supported by a global network of SKA Regional Centres(SRCs)distributed around the world in its member countries to build an end-to-end science data system that will provide astronomers with high-quality science products.SRCs undertake deep processing,scientific analysis,and long-term storage of the SKA data,as well as user support.China has been actively participating in and promoting the construction of SRCs.This paper introduces the international cooperation and ongoing prototyping of the global SRC network,the basis for the construction of the China SRC and describes in detail the progress of the China SRC prototype.The paper also presents examples of scientific applications of SKA precursor and pathfinder telescopes performed using resources from the China SRC prototype.Finally,the future prospects of the China SRC are presented. 展开更多
关键词 Square Kilometre Array SKA Regional Centre radio astronomy science pipeline
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在红移4.72的耀变体中发现快速喷流
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作者 张迎康 安涛 Sándor Frey 《Science Bulletin》 SCIE EI CAS CSCD 2020年第7期525-530,M0003,共7页
耀变体由星系中央超大黑洞供应强大的能源,由于相对论性束流效应,其喷流的亮度被放大,从而比同等距离的其他天体显得更加明亮,耀变体也由此成为贯穿宇宙漫长演化历程的"灯塔",成为人类解开宇宙奥秘的一把钥匙.即便有增亮的加... 耀变体由星系中央超大黑洞供应强大的能源,由于相对论性束流效应,其喷流的亮度被放大,从而比同等距离的其他天体显得更加明亮,耀变体也由此成为贯穿宇宙漫长演化历程的"灯塔",成为人类解开宇宙奥秘的一把钥匙.即便有增亮的加持,观测宇宙极早期耀变体的难度仍然很高,导致人们对第一代耀变体的认识极为有限.本文利用甚长基线干涉测量技术成功观测到一颗编号为J1430+4204的耀变体,并结合历史数据测量了喷流的运动.该天体生活在约等于宇宙十分之一年龄的时期,记录着宇宙早期的宝贵信息.对J1430+4204以及其他宇宙早期耀变体的研究有助于理解第一代超大黑洞的活动性及其对宿主星系的反馈. 展开更多
关键词 耀变体 宇宙早期 喷流 黑洞 演化历程 数据测量 相对论性 甚长基线干涉测量技术
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东亚VLBI网观测高能伽马暴190114C的余辉辐射
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作者 安涛 Om Sharan Salafia +7 位作者 张迎康 Giancarlo Ghirlanda Gabriele GiovanniniGiovannini Marcello Giroletti Kazuhiro Hada Giulia Migliori Monica Orienti Bong Won Sohn 《Science Bulletin》 SCIE EI CAS CSCD 2020年第4期267-271,共5页
GRB190114C是人类首次在TeV波段观测到的伽马暴,最高光子能量超过以往事例的10倍,是宇宙中最耀眼的闪光.在甚高能伽马射线被探测到之后,多个波段的望远镜立即对其余辉辐射开展了联测.它是为数不多在全部电磁波段均有探测的伽马暴,为研... GRB190114C是人类首次在TeV波段观测到的伽马暴,最高光子能量超过以往事例的10倍,是宇宙中最耀眼的闪光.在甚高能伽马射线被探测到之后,多个波段的望远镜立即对其余辉辐射开展了联测.它是为数不多在全部电磁波段均有探测的伽马暴,为研究高能光子辐射起源和机制提供了难得机会.本文作者协调组织了东亚VLBI网的观测,在该伽马暴爆发后的第6、15和32天完成了三次观测.这是在流量下降期的唯一射电数据.在三次观测中,目标源对应的天区中均没有发现该天体(通常认为高于5倍背景噪声的信号为可靠探测).由此作者得出结论,GRB190114C的流量已经快速下降.该观测给出GRB190114C在三个时间点的射电亮度上限,以此为参考对理论模型的参数空间进行了限制. 展开更多
关键词 GRB 伽马暴
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