Determination of the point-spread function for the fermi large area telescope from on-orbit data and limits on pair halos of active galactic nuclei
The Large Area Telescope (LAT) on the Fermi Gamma-ray Space Telescope is a pair-conversion telescope designed to detect photons with energies from ≈20 MeV to >300 GeV. The pre-launch response functions of the LAT were determined through extensive Monte Carlo simulations and beam tests. The point-...
Guardado en:
| Autor principal: | Ackermann, M. |
|---|---|
| Formato: | JOUR |
| Materias: | |
| Acceso en línea: | http://hdl.handle.net/20.500.12110/paper_0004637X_v765_n1_p_Ackermann |
| Aporte de: |
Ejemplares similares
-
Determination of the point-spread function for the fermi large area telescope from on-orbit data and limits on pair halos of active galactic nuclei
Publicado: (2013) -
Distribution of the high-velocity clouds in the Galactic halo
por: Olano, Carlos Alberto
Publicado: (2008) -
Low-metallicity stellar halo populations as tracers of dark matter haloes
Publicado: (2014) -
Low-metallicity stellar halo populations as tracers of dark matter haloes
por: Tissera, P.B., et al. -
The Three Hundred project: A large catalogue of theoretically modelled galaxy clusters for cosmological and astrophysical applications
Publicado: (2018)