Prospects for the detection of very-high-energy pulsars with LHAASO and SWGO
Author:
Affiliation:
1. Key Laboratory of Space Science and Astronomy, Purple Mountain Observatory, Chinese Academy of Sciences , Nanjing 210023 , China
2. School of Astronomy and Space Science, University of Science and Technology of China , Hefei 230026 China
Abstract
Funder
National Natural Science Foundation of China
Chinese Academy of Sciences
Publisher
Oxford University Press (OUP)
Link
https://academic.oup.com/mnras/advance-article-pdf/doi/10.1093/mnras/stae1497/58257720/stae1497.pdf
Reference46 articles.
1. MILAGRO OBSERVATIONS OF MULTI-TeV EMISSION FROM GALACTIC SOURCES IN THE FERMI BRIGHT SOURCE LIST
2. THE SECOND FERMI LARGE AREA TELESCOPE CATALOG OF GAMMA-RAY PULSARS
3. Extended gamma-ray sources around pulsars constrain the origin of the positron flux at Earth
4. Probing the extent of the non-thermal emission from the Vela X region at TeV energies with H.E.S.S.
5. Search for VHE gamma-ray emission from Geminga pulsar and nebula with the MAGIC telescopes
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