activity
20022026
most citedAn Exceptional VHE Gamma-Ray Flare of PKS 2155-304

816 citations · 15.8k across the 233 of their papers we have counts for

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Showing 2010 · astro-ph.HEShow all

6 papers · 2 filters

astro-ph.HE2010★ 27 cited

Discovery and follow-up studies of the extended, off-plane, VHE gamma-ray source HESS J1507-622

H. E. S. S. Collaboration, F. Acero, F. Aharonian +167

Context: The detection of gamma-rays in the very-high-energy (VHE) range (100 GeV-100 TeV) offers the possibility of studying the parent population of ultrarelativistic particles f…

astro-ph.HE2010★ 78 cited

Revisiting the Westerlund 2 Field with the H.E.S.S. Telescope Array

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

Aims. Previous observations with the H.E.S.S. telescope array revealed the existence of extended very-high-energy (VHE; E>100 GeV) γ-ray emission, HESS J1023-575, coincident with t…

astro-ph.HE2010★ 36 cited

Discovery of VHE gamma-rays from the BL Lac object PKS 0548-322

H. E. S. S. collaboration, :, F. Aharonian +168

PKS 0548-322 (z=0.069) is a ``high-frequency-peaked'' BL Lac object and a candidate very high energy (VHE, E>100 GeV) gamma-ray emitter, due to its high X-ray and radio flux. Obser…

astro-ph.HE2010

Active Galactic Nuclei and gamma rays

Berrie Giebels, Felix Aharonian, Hélène Sol

The supermassive black holes harboured in active galactic nuclei are at the origin of powerful jets which can emit copious amounts of gamma-rays. The exact interplay between the in…

astro-ph.HE2010★ 46 cited

Multi-wavelength Observations of H 2356-309

HESS Collaboration, A. Abramowski, F. Acero +184

AIMS: The properties of the broad-band emission from the high-frequency peaked BL Lac H 2356-309 (z=0.165) are investigated. METHODS: Very High Energy (VHE; E > 100 GeV) observatio…

astro-ph.HE2010★ 171 cited

First detection of VHE gamma-rays from SN 1006 by H.E.S.S

HESS Collaboration, F. Acero, F. Aharonian +175

Recent theoretical predictions of the lowest very high energy (VHE) luminosity of SN 1006 are only a factor 5 below the previously published H.E.S.S. upper limit, thus motivating f…