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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:用于切伦科夫望远镜阵列的应科院端对端望远镜

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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)将成为世界上最大的地面超高能伽马射线探测天文台,在北半球和南半球(加那利群岛的拉帕尔玛岛,目前提议在帕拉纳尔,智利)。南部CTA阵列的能量覆盖范围将扩大到300TeV,这要归功于大量(多达70个)小型望远镜,它们的主镜直径约为4米,大视场约为9度。建议将第一套CTA小型望远镜用ASTRI微型阵列表示,该阵列包括(至少)九个ASTRI望远镜,其端对端原型安装在ASTRI SST-2M中。意大利,目前正进入调试和科学验证阶段。在此阶段,其中包括对已知来源(如蟹状星云和一些大火星)的科学观察,原型性能将与蒙特卡洛模拟的预测相互核对。应科院望远镜的特点是基于双镜Schwarzschild-Couder设计的光学系统,以及由快速前端电子设备管理的硅光电倍增管(SiPM)传感器覆盖的弯曲焦平面。由意大利国家天体物理研究所(INAF)开发的望远镜原型遵循端到端方法,包括内部和外部校准系统,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。所有这些子系统都是根据SST的CTA要求开发的。由CAF的INAF领导,巴西圣保罗大学,西北大学(南非)和意大利国家核物理研究所(INFN)的协同合作正在进行中。在本文中,我们将介绍应科院望远镜的主要功能,有关原型活动的最新消息以及应科院微型阵列的技术和科学期望。

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