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From the Etna volcano to the Chilean Andes: ASTRI end-to-end telescopes for the Cherenkov Telescope Array

机译:从埃特纳火山到智利安第斯山脉:阿斯特蒂终端望远镜为Cherenkov望远镜阵列

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The Cherenkov Telescope Array (CTA) will be the largest ground-based very high-energy gamma-ray detection observatory in the world with more than one hundred telescopes located in the Northern and Southern Hemispheres (La Palma, Canary Islands and currently proposed at Paranal, Chile). The energy coverage, in the southern CTA array, will extend up to 300TeV thanks to a large number (up to 70) of small size telescopes, with their primary mirrors of about 4meters in diameter and large field of view of the order of 9 degrees. It is proposed that one of the first set of CTA small size telescopes will be represented by the ASTRI mini-array which includes (at least) nine ASTRI telescopes whose end-to-end prototype, named the ASTRI SST-2M, is installed in Italy and is now entering in its commissioning and science verification phase. During this phase, that includes scientific observations of known sources such as the Crab Nebula and a few blazars, the prototype performance will be crosschecked with the predictions of Monte Carlo simulations. ASTRI telescopes are characterized by an optical system based on a dual-mirror Schwarzschild-Couder design and by a curved focal plane covered by silicon photomultiplier (SiPM) sensors managed by a fast front-end electronics. The telescope prototype, developed by the Italian National Institute for Astrophysics, INAF, follows an end-to-end approach that includes the internal and external calibration systems, control/acquisition hardware and software, data reduction and analysis software, and the data archiving system. All these sub-systems are developed following the CTA requirements for the SSTs. A collaborative effort is ongoing, led by INAF within CTA, in synergy with the Universidade de Sao Paulo (Brazil), and the North-West University (South Africa) and the Italian National Institute for Nuclear Physics (INFN). In this contribution, we will describe the main features of the ASTRI telescopes, the latest news on the prototype activities and the ASTRI mini-array technological and scientific expectations.
机译:切伦科夫望远镜阵列(CTA)将是最大的地面非常高能量伽马射线检测在世界上与位于南北半球(拉帕尔马,加那利群岛一百多个望远镜观测站,目前在巴拉那建议,智利)。能量覆盖范围,南部CTA阵列中,将一直延伸到的小尺寸的望远镜感谢300TeV到大量(高达70),与他们的直径约4米和视的9度的量级的大视场主镜的。所以建议第一组CTA小尺寸的望远镜中的一个将被ASTRI小型阵列,其包括(至少)9个科院望远镜,其端至端原型,命名为科院SST-2M表示,被安装在意大利,现在进入了试运行和科学验证阶段。在此阶段,其包括已知的来源如蟹状星云和几个耀变科学观察,原型性能将与Monte Carlo模拟的预测进行交叉检查。科院望远镜通过基于双镜施瓦兹希尔德-Couder设计的光学系统,并通过由硅光电倍增器(SiPM的)通过快速前端电子管理传感器所覆盖的弯曲焦面特征。望远镜原型,由意大利国家天体物理研究所,INAF,开发了如下的端至端的方法,其包括内部和外部的校准系统,控制/采集硬件和软件,数据缩减和分析软件,以及数据存档系统。所有这些子系统的开发下的海表温度的CTA要求。合作努力正在进行中,CTA内通过国家天体物理研究所的带领下,在与圣保罗大学(巴西)和西北大学(南非)和意大利国家核物理研究所(INFN)的协同作用。在这方面的贡献,我们将描述科院望远镜,在原型活动的最新消息和ASTRI小型阵列技术和科学预期的主要特点。

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