activity
20082020
most citedSearch for a Dark Matter annihilation signal from the Galactic Center halo with H.E.S.S

270 citations · 5k across the 79 of their papers we have counts for

collaborators
Showing 2010Show all

6 papers · 1 filter

astro-ph.HE2010★ 102 cited

H.E.S.S. constraints on Dark Matter annihilations towards the Sculptor and Carina Dwarf Galaxies

HESS Collaboration, A. Abramowski, F. Acero +192

The Sculptor and Carina Dwarf spheroidal galaxies were observed with the H.E.S.S. Cherenkov telescope array between January 2008 and December 2009. The data sets consist of a total…

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★ 165 cited

The Crab Nebula as a standard candle in very high-energy astrophysics

M. Meyer, D. Horns, H. -S. Zechlin

The continuum high-energy gamma-ray emission between 1 GeV and 100 TeV from the Crab Nebula has been measured for the first time in overlapping energy bands by the Fermi large-area…

astro-ph.HE2010★ 126 cited

VHE gamma-ray emission of PKS 2155-304: spectral and temporal variability

HESS Collaboration, A. Abramowski, F. Acero +185

Observations of very high energy gamma-rays from blazars provide information about acceleration mechanisms occurring in their innermost regions. Studies of variability in these obj…

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.GA2010★ 2 cited

Locating the VHE source in the Galactic Centre with milli-arcsecond accuracy

A. Abramowski, S. Gillessen, D. Horns +1

Very high-energy gamma-rays (VHE; E>100 GeV) have been detected from the direction of the Galactic Centre up to energies E>10 TeV. Up to now, the origin of this emission is unknown…