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.
Authors
- M. Zha
- Yi Xing (ORCID: https://orcid.org/0000-0002-5818-0732)
- Guangman Xiang
- J. N. Zhou
Institutions
- Chinese Academy of Sciences (CN)
- Shanghai Astronomical Observatory (CN)
- Institute of High Energy Physics (CN)
- University of Chinese Academy of Sciences (CN)
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
- Field-Weighted Citation Impact
- 0.00