## More than a decade after its discovery, the Fermi GeV excess is still an exciting subject of research.

A multi-wavelength search for bulge millisecond pulsars

## The radio filaments trace a population of pulsars also responsible for the Fermi GeV excess produced by the Inverse Compton scattering by the pulsar wind particles.

On the nature of radio filaments near the Galactic Centre

## Statistical evidence has previously suggested that the Galactic Center GeV Excess (GCE) originates largely from point sources, and not from annihilating dark matter.

Dark Matter Strikes Back at the Galactic Center

## Statistical evidence has previously suggested that the galactic center GeV excess (GCE) originates largely from point sources, and not from annihilating dark matter.

Revival of the Dark Matter Hypothesis for the Galactic Center Gamma-Ray Excess.

10.22323/1.395.0681

## More than a decade after its discovery, the Fermi GeV excess is still an exciting subject of research.

A multi-wavelength search for bulge millisecond pulsars

10.3390/sym13081432

## This in turn changes the ratio between various emission components at those energies and may potentially absorb the GeV excess by a simple renormalization of key components.

On a Possible Origin of the Gamma-ray Excess around the Galactic Center

10.22323/1.395.0645

## In our analysis the GeV excess component has been taken into account and the resulting $\gamma$-ray spectrum as well as the intensity gradient are consistent with that measured by the Imaging Atmospheric Cherenkov Telescopes.

A new GeV-TeV particle component and the barrier of cosmic-ray sea in the CMZ region

10.1093/mnrasl/slz124

## The radio filaments trace a population of pulsars also responsible for the Fermi GeV excess produced by the Inverse Compton scattering by the pulsar wind particles.

On the nature of radio filaments near the Galactic Centre

10.1103/PhysRevD.99.123020

## The leading theory postulates that this GeV excess is the aggregate emission from a large number of faint millisecond pulsars (MSPs).

Inverse-Compton emission from Millisecond Pulsars in the Galactic bulge

10.1103/PhysRevLett.123.241101

## Statistical evidence has previously suggested that the Galactic Center GeV Excess (GCE) originates largely from point sources, and not from annihilating dark matter.

Dark Matter Strikes Back at the Galactic Center

10.1103/PHYSREVLETT.123.241101

## Statistical evidence has previously suggested that the galactic center GeV excess (GCE) originates largely from point sources, and not from annihilating dark matter.

Revival of the Dark Matter Hypothesis for the Galactic Center Gamma-Ray Excess.