The detectability of WCDA to TeV-sources
July 22, 2019
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).
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.