activity
20072012
most citedThe Large Area Telescope on the Fermi Gamma-ray Space Telescope Mission

4.1k citations · 6k across the 16 of their papers we have counts for

collaborators

16 papers

astro-ph.HE2012★ 239 cited

Fermi LAT Search for Dark Matter in Gamma-ray Lines and the Inclusive Photon Spectrum

LAT Collaboration, M. Ackermann, M. Ajello +117

Dark matter particle annihilation or decay can produce monochromatic gamma-ray lines and contribute to the diffuse gamma-ray background. Flux upper limits are presented for gamma-r…

astro-ph.HE2010★ 69 cited

Fermi LAT observations of the Geminga pulsar

LAT Collaboration, A. A. Abdo

We report on the \textit{Fermi}-LAT observations of the Geminga pulsar, the second brightest non-variable GeV source in the -ray sky and the first example of a radio-quiet -r…

astro-ph.CO2010★ 193 cited

Constraints on Cosmological Dark Matter Annihilation from the Fermi-LAT Isotropic Diffuse Gamma-Ray Measurement

LAT collaboration, A. A. Abdo, M. Ackermann +147

The first published Fermi large area telescope (Fermi-LAT) measurement of the isotropic diffuse gamma-ray emission is in good agreement with a single power law, and is not showing…

astro-ph.GA2010★ 39 cited

Fermi Large Area Telescope observations of PSR J1836+5925

The Fermi LAT Collaboration

The discovery of the gamma-ray pulsar PSR J1836+5925, powering the formerly unidentified EGRET source 3EG J1835+5918, was one of the early accomplishments of the Fermi Large Area T…

astro-ph.CO2010★ 198 cited

Constraints on Dark Matter Annihilation in Clusters of Galaxies with the Fermi Large Area Telescope

LAT Collaboration

Nearby clusters and groups of galaxies are potentially bright sources of high-energy gamma-ray emission resulting from the pair-annihilation of dark matter particles. However, no s…

astro-ph.HE2010★ 199 cited

Fermi LAT Search for Photon Lines from 30 to 200 GeV and Dark Matter Implications

The Fermi LAT Collaboration, A. A. Abdo, M. Ackermann +160

Dark matter (DM) particle annihilation or decay can produce monochromatic -rays readily distinguishable from astrophysical sources. -ray line limits from 30 GeV to 200 GeV ob…