activity
19992021
most citedDesign Concepts for the Cherenkov Telescope Array

902 citations · 12.2k across the 122 of their papers we have counts for

collaborators
Showing 2005Show all

6 papers · 1 filter

astro-ph2005★ 59 cited

Multiwavelength Observations of the Blazar Mrk 421 in December 2002 and January 2003

P. Rebillot, M. Aller, H. Aller +5

We report on a multiwavelength campaign on the TeV gamma-ray blazar Markarian (Mrk) 421 performed during December 2002 and January 2003. These target of opportunity observations we…

astro-ph2005★ 286 cited

A new population of very high energy gamma-ray sources in the Milky Way

F. A. Aharonian

Very high energy gamma-rays probe the long-standing mystery of the origin of cosmic rays. Produced in the interactions of accelerated particles in astrophysical objects, they can b…

astro-ph2005★ 36 cited

Upper limits to the SN1006 multi-TeV gamma-ray flux from H.E.S.S. observations

F. Aharonian

Observations of the shell-type supernova remnant SN1006 have been carried out with the H.E.S.S. system of Cherenkov telescopes during 2003 (18.2h with two operating telescopes) and…

astro-ph2005★ 125 cited

The unidentified TeV source (TeVJ2032+4130) and surrounding field: Final HEGRA IACT-System results

HEGRA Collaboration, F. Aharonian

The unidentified TeV source in Cygnus is now confirmed by follow-up observations from 2002 with the HEGRA stereoscopic system of Cherenkov Telescopes. Using all data (1999 to 2002)…

astro-ph2005★ 15 cited

Search for TeV emission from the region around PSR B1706-44 with the H.E.S.S. experiment

H. E. S. S. Collaboration, :, F. Aharonian

The region around PSR B1706-44 has been observed with the H.E.S.S. imaging atmospheric Cherenkov telescopes in 2003. No evidence for gamma-ray emission in the TeV range was found a…

astro-ph2005★ 139 cited

Very high energy gamma rays from the composite SNR G0.9+0.1

H. E. S. S. Collaboration, :, F. Aharonian

Very high energy (> 100 GeV) gamma-ray emission has been detected for the first time from the composite supernova remnant G0.9+0.1 using the H.E.S.S. instrument. The source is dete…