With high duty cycle and wide aperture, the Large High Altitude Air Shower Observatory
- Water Cherenkov Detector Array (LHAASO-WCDA) can conduct an unbiased gammaray
sky survey in the energy range from a few hundred GeV to 100 TeV. The sensitivity
of WCDA is as high as a few percent of Crab units, which allow us to monitor the VHE
variability of blazars. Once a flare exceeding the threshold is detected, an alert will be
generated and follow-up analysis could be carried out. In this paper the candidate sources,
the methods and current status of the monitors as well as some prospects of alert issues
in the future will be presented.
A REAL-TIME MONITOR FOR TEV TRANSIENTS WITH LHAASO-WCDA
Full text:
Not available
Abstract
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
Copyright owned by the author(s) under the term of the Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International License.
Copyright owned by the author(s) under the term of the Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International License.