Spectral and spatial variations of the diffuse γ-ray background in the vicinity of the Galactic plane and possible nature of the feature at 130 GeV

We study the properties of the diffuse γ-ray background around the Galactic plane at energies 20–200 GeV. We find that the spectrum of this emission possesses significant spacial variations with respect to the average smooth component. The positions and shapes of these spectral features change with the direction on the sky. We therefore argue that the spectral feature around 130 GeV, found in several regions around the Galactic Center and in the Galactic plane in Bringmann et al. (2012) [1], Weniger (2012) [2], Tempel et al. (2012) [3], and Su and Finkbeiner (2012) [4], cannot be interpreted with confidence as a γ-ray line, but may be a component of the diffuse background and can be of instrumental or astrophysical origin. Therefore, the dark matter origin of this spectral feature becomes dubious.