An end-to-end calibration of the Mini-EUSO detector in space

IF 4.2 3区 物理与天体物理 Q1 ASTRONOMY & ASTROPHYSICS
M. Battisti , M. Bertaina , E. Parizot , M. Abrate , D. Barghini , A. Belov , F. Bisconti , C. Blaksley , S. Blin , F. Capel , M. Casolino , I. Churilo , A.G. Coretti , M. Crisconio , C. De La Taille , T. Ebisuzaki , F. Fenu , M.A. Franceschi , C. Fuglesang , S. Gallian , M. Zotov
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引用次数: 0

Abstract

Mini-EUSO is a wide Field-of-View (44×44) telescope currently in operation from a nadir-facing Ultra-Violet (UV) transparent window in the Russian Zvezda module on the International Space Station (ISS). Mini-EUSO has been designed as a scaled-down version of the original JEM-EUSO telescope to raise its instrumentation’s technological readiness level and demonstrate its observational principle, while performing multidisciplinary studies on different fields such as atmospheric science and planetology. One of Mini-EUSO main goals is the study of the UV background for future space missions employing the same concept as the original JEM-EUSO telescope, which requires an absolute calibration of the Mini-EUSO instrument. During the past years, a few observational campaigns have been completed, employing a ground-based UV flasher to perform an end-to-end calibration of the instrument. In this paper, we present the assembled UV flasher system, the operation of the field campaign and the analysis of the obtained data. The results are interpreted by the means of a parametrization of the Mini-EUSO photon counts. The end-to-end efficiency of several pixels has been obtained, taking into account different parameters such as the atmospheric attenuation, the optics efficiency and the multi-anode photomultiplier detection efficiency.
空间微型 EUSO 探测器的端对端校准
Mini-EUSO 是一台宽视场(44∘×44∘)望远镜,目前正在国际空间站(ISS)俄罗斯 Zvezda 舱的一个面向天底的紫外线(UV)透明窗口中运行。迷你 EUSO 是作为原始 JEM-EUSO 望远镜的缩小版而设计的,目的是提高其仪器的技术就绪水平并展示其观测原理,同时对大气科学和行星学等不同领域进行多学科研究。Mini-EUSO 的主要目标之一是为未来的空间任务研究紫外线背景,采用与最初的 JEM-EUSO 望远镜相同的概念,这需要对 Mini-EUSO 仪器进行绝对校准。在过去几年中,已经完成了一些观测活动,利用地面紫外线闪烁器对仪器进行了端对端校准。在本文中,我们介绍了组装好的紫外线闪烁器系统、实地活动的运行情况以及对所获数据的分析。我们通过对迷你 EUSO 光子计数的参数化来解释结果。考虑到大气衰减、光学效率和多阳极光电倍增管探测效率等不同参数,获得了多个像素的端到端效率。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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来源期刊
Astroparticle Physics
Astroparticle Physics 地学天文-天文与天体物理
CiteScore
8.00
自引率
2.90%
发文量
41
审稿时长
79 days
期刊介绍: Astroparticle Physics publishes experimental and theoretical research papers in the interacting fields of Cosmic Ray Physics, Astronomy and Astrophysics, Cosmology and Particle Physics focusing on new developments in the following areas: High-energy cosmic-ray physics and astrophysics; Particle cosmology; Particle astrophysics; Related astrophysics: supernova, AGN, cosmic abundances, dark matter etc.; Gravitational waves; High-energy, VHE and UHE gamma-ray astronomy; High- and low-energy neutrino astronomy; Instrumentation and detector developments related to the above-mentioned fields.
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