A Real-time Monitor for TeV Gamma-Ray Flare with the LHAASO-WCDA Detector

Abstract With its high duty cycle, wide field of view and high detection sensitivity, Water Chereknov Detector Array as one of sub-arrays of Large High Altitude Air Shower Observatory is a promising facility to monitor transient phenomena in the very high energy gamma-ray band. In this work, a real-time monitor for selected TeV extragalactic sources is introduced, this flare monitor is developed to detect very high energy flare events and for further studying the power-providing mechanism of blazar relativistic jets. The detailed information such as the searching method and sensitivity of this real-time flare monitor is also presented. In the end, successful multi-wavelength and multi-messenger observation of 1ES 1959+650 and IC 310 also confirms the capabilities and reliability of the monitoring system.

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Publication Details

Journal
Research in Astronomy and Astrophysics
Published
2024-10-24
DOI
https://doi.org/10.1088/1674-4527/ad8b0d
Primary Topic
Astrophysics and Cosmic Phenomena
Type
article
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article

A Real-time Monitor for TeV Gamma-Ray Flare with the LHAASO-WCDA Detector

M. Zha, Yi Xing, Guangman Xiang, J. N. Zhou
Research in Astronomy and Astrophysics
Astrophysics and Cosmic Phenomena
article

A Real-time Monitor for TeV Gamma-Ray Flare with the LHAASO-WCDA Detector

M. Zha, Yi Xing, Guangman Xiang, J. N. Zhou
article en

Abstract

Abstract With its high duty cycle, wide field of view and high detection sensitivity, Water Chereknov Detector Array as one of sub-arrays of Large High Altitude Air Shower Observatory is a promising facility to monitor transient phenomena in the very high energy gamma-ray band. In this work, a real-time monitor for selected TeV extragalactic sources is introduced, this flare monitor is developed to detect very high energy flare events and for further studying the power-providing mechanism of blazar relativistic jets. The detailed information such as the searching method and sensitivity of this real-time flare monitor is also presented. In the end, successful multi-wavelength and multi-messenger observation of 1ES 1959+650 and IC 310 also confirms the capabilities and reliability of the monitoring system.

Research in Astronomy and AstrophysicsVol. 24(12)
Chinese Academy of Sciences (CN), Shanghai Astronomical Observatory (CN), Institute of High Energy Physics (CN), University of Chinese Academy of Sciences (CN)
Openalex Percentile: Top 95%
Astrophysics and Cosmic Phenomena
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