activity
20072009
most citedNew constraints on the Mid-IR EBL from the HESS discovery of VHE gamma rays from 1ES 0229+200

261 citations · 868 across the 11 of their papers we have counts for

collaborators
Showing astro-ph.HEShow all

6 papers · 1 filter

astro-ph.HE2009219 cited

Detection of Gamma Rays From a Starburst Galaxy

The HESS Collaboration, F. Acero

Starburst galaxies exhibit in their central regions a highly increased rate of supernovae, the remnants of which are thought to accelerate energetic cosmic rays up to energies of ~…

astro-ph.HE20091 cited

Correlation between the synchrotron and the inverse-Compton components, in the longterm light curve of GeV blazars

Bagmeet Behera, Marcus Hauser, Stefan J. Wagner

To explore the correlation in the GeV band (i.e. the inverse-Compton component) with the optical band (i.e. the synchrotron component) of blazars that are bright in high energies,…

astro-ph.HE2009

A new strategy to select candidate blazars for VHE observation

Bagmeet Behera, Stefan J. Wagner

A new strategy to select candidate blazars for VHE observations, that gives an inherently complete sample from an all-sky compilation (excluding a narrow region around the galactic…

astro-ph.HE2009173 cited

Simultaneous observations of PKS 2155-304 with H.E.S.S., Fermi, RXTE and ATOM: spectral energy distributions and variability in a low state

H. E. S. S., Fermi-LAT collaborations

We report on the first simultaneous observations that cover the optical, X-ray, and high energy gamma-ray bands of the BL Lac object PKS 2155-304. The gamma-ray bands were observed…

astro-ph.HE200959 cited

H.E.S.S. observations of gamma-ray bursts in 2003-2007

F. Aharonian

Very-high-energy (VHE; >~100 GeV) gamma-rays are expected from gamma-ray bursts (GRBs) in some scenarios. Exploring this photon energy regime is necessary for understanding the ene…

astro-ph.HE20091 cited

Spectral trends in the Very High Energy blazar sample due to EBL absorption

B. Behera, S. J. Wagner

The absorption of gamma-rays in the intergalactic medium due to the EBL (Extragalactic Background Light) causes the observed blazar spectrum to be fainter and softer than their int…