PoS - Proceedings of Science
Volume 358 - 36th International Cosmic Ray Conference (ICRC2019) - CRI - Cosmic Ray Indirect
The detectability of WCDA to TeV-sources
Y. Guo*, X. Chang, H. Hu, Z. Yao  on behalf of the LHAASO Collaboration
Full text: pdf
Pre-published on: July 22, 2019
Published on: July 02, 2021
The Large High Altitude Air Shower Observatory (LHAASO) as a new generation of cosmic ray experiment with unprecedented sensitivity is under construction, and the Water Cherenkov Detector Array (WCDA) is one major component aiming at TeV $\gamma$ rays. In order to sufficiently understand the prospect of searching for TeV $\gamma$-ray sources with WCDA, one-year observing ability of WCDA to TeV $\gamma$-ray sources in TeVCat is presented in this paper. There are 56 out of 128 $\gamma$-ray sources in the $45^\circ$ view of WCDA would be observed at the middle energy of 1 TeV. Most of them are galactic sources, and the extragalactic sources are mainly active galactic nuclei (AGNs).
DOI: https://doi.org/10.22323/1.358.0277
How to cite

Metadata are provided both in "article" format (very similar to INSPIRE) as this helps creating very compact bibliographies which can be beneficial to authors and readers, and in "proceeding" format which is more detailed and complete.

Open Access
Creative Commons LicenseCopyright owned by the author(s) under the term of the Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International License.