Fetching the paper…
Reading the bibliography…
The Diffuse Gamma-Ray Background (DGB) above 100 GeV at high-latitudes is expected to be produced by unresolved extragalactic objects such as active galactic nuclei, isotropic Galactic gamma-rays, and possible emission from dark matter annihilations or decays in the Galactic dark matter halo.
C. E. Fichtel, R. C. Hartman, D. A. Kniffen, D. J. Thompson, G. F. Bignami, H. Ögelman, M. E. Özel, and T. Tümer, Astrophys. J
1975
Earlier work this paper cites.
CASA-MIA
1997
Earlier work this paper cites.
GRAPES-3
2009
Earlier work this paper cites.
K. N. Abazajian, S. Blanchet, and J. P. Harding, Phys. Rev
2012
Cited alongside, same era.
Fermi-LAT
2015
Cited alongside, same era.
A. U. Abeysekara et al., Astrophys. J
2017
Cited alongside, same era.
Talk at the 35th International Cosmic Ray Conference (ICRC), Busan, Korea
D. Kerszberg et al., The cosmic-ray electron spectrum measured with H.E.S.S · 2017
Later among the works it cites.
https://www.mpi-hd.mpg.de/hfm/HESS/pages/home/som/2017/09/
HESS · 2017
Later among the works it cites.
O. Adriani et al., Phys. Rev. Lett
2018
Later among the works it cites.
alphaXiv searches the wider corpus for related work and actual follow-ups.
alphaXiv is searching for related work…