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Gev Excess sentence examples within Fermi Gev Excess

Fermi Gev Excess

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

Fermi Gev Excess

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

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Gev Excess sentence examples within Center Gev Excess

Center Gev Excess

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

Center Gev Excess

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.

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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

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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

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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

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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

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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

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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

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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.

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Gev Excess
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What is/are Gev Excess?

Gev Excess - More than a decade after its discovery, the Fermi GeV excess is still an exciting subject of research. [1] 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. [2] 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. [3] 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. [4] The leading theory postulates that this GeV excess is the aggregate emission from a large number of faint millisecond pulsars (MSPs). [5] Statistical evidence has previously suggested that the Galactic Center GeV Excess (GCE) originates largely from point sources, and not from annihilating dark matter. [6] Statistical evidence has previously suggested that the galactic center GeV excess (GCE) originates largely from point sources, and not from annihilating dark matter. [7]

Fermi Gev Excess

More than a decade after its discovery, the Fermi GeV excess is still an exciting subject of research. [1] 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. [2]

Center Gev Excess

Statistical evidence has previously suggested that the Galactic Center GeV Excess (GCE) originates largely from point sources, and not from annihilating dark matter. [1] Statistical evidence has previously suggested that the galactic center GeV excess (GCE) originates largely from point sources, and not from annihilating dark matter. [2]