Background rejection using image residuals from large telescopes in imaging atmospheric cherenkov telescope arrays

HIGHLIGHTS

• who: L. Olivera-Nieto from the Max-Planck-Institut fu00fcr Kernphysik, POBox, Heidelberg, Germany have published the research work: Background rejection using image residuals from large telescopes in imaging atmospheric Cherenkov telescope arrays, in the Journal: Eur. Phys. J. C
• what: The authors show that in the case of the H.E.S.S. array of five telescopes this approach results in background rejection improvements at all energies above 1 TeV. Note that since the goal of this paper is to demonstrate the the datasets with and without ABRIR (solid lines) and as the ratio . . .
  

   

  

  If you want to have access to all the content you need to log in!

  Thanks :)

  Username or Email

  Password

  Remember me

  Lost your password?

  If you don't have an account, you can create one here.