Prospects for joint reconstruction of imaging air Cherenkov Telescope array and extensive air shower array

Fuente: arXiv
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Auteurs principaux: Zhang, Zhipeng, Yang, Ruizhi, Zhang, Shoushan, Yin, Liqiao, Liu, Jiali, Wang, Yudong, Ma, Lingling, Cao, Zhen
Format: Preprint
Publié: 2024
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author Zhang, Zhipeng
Yang, Ruizhi
Zhang, Shoushan
Yin, Liqiao
Liu, Jiali
Wang, Yudong
Ma, Lingling
Cao, Zhen
author_facet Zhang, Zhipeng
Yang, Ruizhi
Zhang, Shoushan
Yin, Liqiao
Liu, Jiali
Wang, Yudong
Ma, Lingling
Cao, Zhen
contents In this paper we proposed a joint reconstruction of \gray events using both extensive air array (EAS) and Imaging air Cherenkov Telescope array (IACT). We considered eight Cherenkov telescopes to be built on the LHAASO (Large High Altitude Air Shower Observatory) site and investigate the improvement in differential sensitivity when combining the information from both IACT and Moun detectors of LHAASO-KM2A. We found that due to the higher cosmic ray background rejection power and higher gamma ray retention ratio provided by muon detectors of LHAASO, such a joint reconstruction can significantly improve the sensitivity of IACTs, especially for extended sources and long exposure time. In this article, we have shown the performance of an eight-telescopes mini array, and our results indicate that above $10~\rm TeV$, the sensitivity can be improved by muon detector from $25\% - 60\%$ in different energy ranges.
format Preprint
id arxiv_https___arxiv_org_abs_2402_11286
institution arXiv
publishDate 2024
record_format arxiv
spellingShingle Prospects for joint reconstruction of imaging air Cherenkov Telescope array and extensive air shower array
Zhang, Zhipeng
Yang, Ruizhi
Zhang, Shoushan
Yin, Liqiao
Liu, Jiali
Wang, Yudong
Ma, Lingling
Cao, Zhen
High Energy Astrophysical Phenomena
Instrumentation and Methods for Astrophysics
In this paper we proposed a joint reconstruction of \gray events using both extensive air array (EAS) and Imaging air Cherenkov Telescope array (IACT). We considered eight Cherenkov telescopes to be built on the LHAASO (Large High Altitude Air Shower Observatory) site and investigate the improvement in differential sensitivity when combining the information from both IACT and Moun detectors of LHAASO-KM2A. We found that due to the higher cosmic ray background rejection power and higher gamma ray retention ratio provided by muon detectors of LHAASO, such a joint reconstruction can significantly improve the sensitivity of IACTs, especially for extended sources and long exposure time. In this article, we have shown the performance of an eight-telescopes mini array, and our results indicate that above $10~\rm TeV$, the sensitivity can be improved by muon detector from $25\% - 60\%$ in different energy ranges.
title Prospects for joint reconstruction of imaging air Cherenkov Telescope array and extensive air shower array
topic High Energy Astrophysical Phenomena
Instrumentation and Methods for Astrophysics
url https://arxiv.org/abs/2402.11286