Speaker
世聪 胡
(高能所)
Description
With emission extending beyond 100 TeV, the gamma ray source MGRO J1908+06 is one of the Galactic PeVatron candidates. The nature of MGRO J1908+06 remains unrevealed and a single accelerator cannot explain the whole set of multiwavelength data. We observed the MGRO J1908+06 using LHAASO. A significant excess of gamma ray excesses above 100 TeV is detected with 30σ. The measured energy spectrum can be extend to 500 TeV. Using the results, the emission mechanisms is discussed.
Primary author
世聪 胡
(高能所)
Co-author
Dr
Sha Wu
