  The Cygnus Loop is a nearby supernova remnant (SNR) observed across the
electromagnetic spectrum. With the analysis of 6 years of Fermi/LAT data we
find that, what previous studies had considered a single source, consists of an
extended source plus a point-like source south-east of the SNR. The extended
gamma-ray emission is well correlated with the thermal X-ray emission of the
SNR, and the energy spectrum displays a pronounced maximum at $\sim0.6$\,GeV.
However, in a region where the radio emission is strongly and distinctly
polarized, the gamma-ray spectrum shows no sign of a break. Therefore, the
spatially resolved gamma-ray emission permits the study of different
interaction conditions of the SNR and the surrounding medium.
