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20002023
most citedThe energy spectrum of cosmic-ray electrons at TeV energies

638 citations · 18k across the 223 of their papers we have counts for

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50 papers · 1 filter

astro-ph2008★ 104 cited

Study of the Spectral and Temporal Characteristics of X-Ray Emission of the Gamma-Ray Binary LS 5039 with Suzaku

T. Takahashi, T. Kishishita, Y. Uchiyama +6

We report on the results from Suzaku broadband X-ray observations of the galactic binary source LS5039. The Suzaku data, which have continuous coverage of more than one orbital per…

astro-ph2008★ 638 cited

The energy spectrum of cosmic-ray electrons at TeV energies

H. E. S. S. Collaboration, :, F. Aharonian

The very large collection area of ground-based gamma-ray telescopes gives them a substantial advantage over balloon/satellite based instruments in the detection of very-high-energy…

astro-ph2008★ 113 cited

Limits on an Energy Dependence of the Speed of Light from a Flare of the Active Galaxy PKS 2155-304

H. E. S. S. Collaboration, :, F. Aharonian

In the past few decades, several models have predicted an energy-dependence of the speed of light in the context of quantum gravity. For cosmological sources such as active galaxie…

astro-ph2008★ 112 cited

Discovery of gamma-ray emission from the shell-type supernova remnant RCW 86 with H.E.S.S

HESS Collaboration, F. Aharonian

The shell-type supernova remnant (SNR) RCW 86, possibly associated with the historical supernova SN 185, with its relatively large size (about 40' in diameter) and the presence of…

astro-ph2008★ 113 cited

HESS J0632+057 : A new gamma-ray binary?

J. A. Hinton, J. L. Skilton, S. Funk +8

The High Energy Stereoscopic System (HESS) survey of the Galactic plane has established the existence of a substantial number (~40) of Galactic TeV gamma-ray sources, a large fract…

astro-ph2008★ 33 cited

H.E.S.S. upper limits for Kepler's supernova remnant

HESS Collaboration, F. Aharonian

Observations of Kepler's supernova remnant (G4.5+6.8) with the H.E.S.S. telescope array in 2004 and 2005 with a total live time of 13 h are presented. Stereoscopic imaging of Chere…