Abstract
An experimental survey of ultra-high-energy γ-ray sources in the Magellanic Clouds is described. Results of the survey may be used to study the intergalactic magnetic field.
Full Text 
Sign-in/Register to access full text options
Sign-in/Register to access full text options 
Paper version not known
Talk to us
Join us for a 30 min session where you can share your feedback and ask us any queries you have
Schedule a call
