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

261 citations · 524 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph200880 cited

Exploring a SNR/Molecular Cloud Association Within HESS J1745-303

HESS Collaboration, F. Aharonian

HESS J1745-303 is an extended, unidentified VHE (very high energy) gamma-ray source discovered using HESS in the Galactic Plane Survey. Since no obvious counterpart has previously…

astro-ph200865 cited

Discovery of VHE gamma-rays from the high-frequency-peaked BL Lac object RGB J0152+017

HESS Collaboration, F. Aharonian

Aims: The BL Lac object RGB J0152+017 (z=0.080) was predicted to be a very high-energy (VHE; > 100 GeV) gamma-ray source, due to its high X-ray and radio fluxes. Our aim is to unde…

astro-ph200740 cited

Upper Limits from HESS AGN Observations in 2005-2007

HESS Collaboration, F. Aharonian

AIMS: Very high energy (VHE; E>100 GeV) gamma-ray studies were performed for 18 active galactic nuclei (AGN) from a variety of AGN classes. METHODS: VHE observations of a sample of…

astro-ph200775 cited

The modulation of the gamma-ray emission from the binary LS 5039

G. Dubus, B. Cerutti, G. Henri

Gamma-ray binaries, composed of a massive star and compact object, have been established as a new class of sources of very high energy (VHE) photons. The gamma-rays are produced by…

astro-ph20073 cited

A Spectacular VHE Gamma-Ray Outburst from PKS 2155-304 in 2006

W. Benbow, C. Boisson, L. Costamante +10

Since 2002 the VHE (>100 GeV) gamma-ray flux of the high-frequency peaked BL Lac PKS 2155-304 has been monitored with the High Energy Stereoscopic System (HESS). An extreme gamma-r…

astro-ph2007261 cited

New constraints on the Mid-IR EBL from the HESS discovery of VHE gamma rays from 1ES 0229+200

HESS Collaboration, F. Aharonian

AIMS: To investigate the very high energy (VHE: >100 GeV) gamma-ray emission from the high-frequency peaked BL Lac 1ES 0229+200. METHODS: Observations of 1ES 0229+200 at energies a…