activity
20042026
most citedAn Exceptional VHE Gamma-Ray Flare of PKS 2155-304

816 citations · 11.8k across the 149 of their papers we have counts for

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Showing 2011 · astro-ph.HEShow all

10 papers · 2 filters

astro-ph.HE2011★ 29 cited

Simultaneous multi-wavelength campaign on PKS 2005-489 in a high state

The H. E. S. S. Collaboration, the Fermi LAT Collaboration, : +345

The high-frequency peaked BL Lac object PKS 2005-489 was the target of a multi-wavelength campaign with simultaneous observations in the TeV gamma-ray (H.E.S.S.), GeV gamma-ray (Fe…

astro-ph.HE2011★ 116 cited

Discovery of extended VHE γ-ray emission from the vicinity of the young massive stellar cluster Westerlund 1

HESS Collaboration, A. Abramowski, F. Acero +198

Results obtained in very-high-energy (VHE; E > 100 GeV) γ-ray observations performed with the H.E.S.S. telescope array are used to investigate particle acceleration processes in th…

astro-ph.HE2011★ 41 cited

Discovery of the source HESS J1356-645 associated with the young and energetic PSR J1357-6429

HESS Collaboration, A. Abramowski, F. Acero +195

Several newly discovered very-high-energy (VHE; E > 100 GeV) gamma-ray sources in the Galaxy are thought to be associated with energetic pulsars. Among them, middle-aged (> 1E+4 yr…

astro-ph.HE2011★ 54 cited

Very-high-energy gamma-ray emission from the direction of the Galactic globular cluster Terzan 5

HESS Collaboration, A. Abramowski, F. Acero +194

The H.E.S.S. very-high-energy (VHE, E > 0.1 TeV) gamma-ray telescope system has discovered a new source, HESS J1747-248. The measured integral flux is (1.2 +/- 0.3) \times 10^-12 c…

astro-ph.HE2011★ 83 cited

A new SNR with TeV shell-type morphology: HESS J1731-347

HESS Collaboration, A. Abramowski, F. Acero +195

The recent discovery of the radio shell-type supernova remnant (SNR), G353.6-0.7, in spatial coincidence with the unidentified TeV source HESS J1731-347 has motivated further obser…

astro-ph.HE2011★ 2 cited

The very-high-energy gamma-ray view of the Galactic Centre as of early 2010

Christopher van Eldik

Progress in the Imaging Atmospheric Cherenkov Technique has enabled first sensitive observations of the innermost few 100 pc of the Milky Way in Very High Energy (VHE; >100 GeV) ga…