activity
19992002
collaborators

15 papers

astro-ph2002

A search for TeV gamma-ray emission from SNRs, pulsars and unidentified GeV sources in the Galactic plane in the longitude range between -2 deg and 85 deg

HEGRA-Collaboration, F. A. Aharonian

Using the HEGRA system of imaging atmospheric Cherenkov telescopes, one quarter of the Galactic plane (-2 deg < l < 85 deg) was surveyed for TeV gamma-ray emission from point sourc…

astro-ph2002

On the Potential of the Imaging Atmospheric Cherenkov Technique for Study of the Mass Composition of Primary Cosmic Radiation in the Energy Region above 30 TeV

F. A. Aharonian, V. V. Bugayov, J. Kettler +2

We suggest a new approach to study the cosmis ray (CR) mass composition in the energy region from 30 TeV/nucleus up to the "knee" region, i.e. up to a few PeV/nucleus, using an arr…

astro-ph2002

An unidentified TeV source in the vicinity of Cygnus OB2

F. A. Aharonian, A. Akhperjanian, M. Beilicke +2

Deep observation (~113 hrs) of the Cygnus region at TeV energies using the HEGRA stereoscopic system of air Cerenkov telescopes has serendipitously revealed a signal positionally i…

astro-ph2002

Variations of the TeV energy spectrum at different flux levels of Mkn 421 observed with the HEGRA system of Cherenkov telescopes

HEGRA Collaboration, F. Aharonian

The nearby BL Lacertae (BL Lac) object Markarian~421 (Mkn~421) at a red shift z=0.031 was observed to undergo strong TeV Gamma-ray outbursts in the observational periods from Decem…

astro-ph2002

The Composition of Cosmic Rays at the Knee

S. P. Swordy, L. F. Fortson, J. Hinton +21

The observation of a small change in spectral slope, or 'knee' in the fluxes of cosmic rays near energies 10^15 eV has caused much speculation since its discovery over 40 years ago…

astro-ph2001

A study of Tycho's SNR at TeV energies with the HEGRA CT-System

F. A. Aharonian, A. G. Akhperjanian, J. A. Barrio +1

Tycho's supernova remnant (SNR) was observed during 1997 and 1998 with the HEGRA Cherenkov Telescope System in a search for gamma-ray emission at energies above ~1 TeV. An analysis…