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2015

Fornasa, Mattia, Sanchez-Conde, Miguel A.

We review the current understanding of the diffuse gamma-ray background (DGRB).

The DGRB is what remains of the total measured gamma-ray emission after the subtraction of the resolved sources and of the diffuse Galactic foregrounds.
It is interpreted as the cumulative emission of sources that are not bright enough to be detected individually.
Yet, its exact composition remains unveiled.

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