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20022006
most citedFast variability of TeV gamma-rays from the radio galaxy M 87

342 citations · 741 across the 4 of their papers we have counts for

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6 papers · 1 filter

astro-ph2006189 cited

H.E.S.S. observations of the supernova remnant RX J0852.0-4622: shell-type morphology and spectrum of a widely extended VHE gamma-ray source

HESS Collaboration, F. A. Aharonian

The shell-type supernova remnant RX J0852.0-4622 was observed with the High Energy Stereoscopic System (H.E.S.S.) of Atmospheric Cherenkov Telescopes between December 2004 and May…

astro-ph2006342 cited

Fast variability of TeV gamma-rays from the radio galaxy M 87

HESS Collaboration, F. A. Aharonian

The detection of fast variations of the TeV (10^12 eV) gamma-ray flux, on time-scales of days, from the nearby radio galaxy M 87 is reported. These variations are ~10 times faster…

astro-ph2006328 cited

Primary particle acceleration above 100 TeV in the shell-type Supernova Remnant RX J1713.7-3946 with deep H.E.S.S. observations

The HESS Collaboration, F. Aharonian

We present deep H.E.S.S. observations of the supernova remnant (SNR) RX J1713.7-3946. Combining data of three years - from 2003 to 2005 - we obtain significantly increased statisti…

astro-ph200619 cited

Mrk 421, Mrk 501, and 1ES 1426+428 at 100 GeV with the CELESTE Cherenkov Telescope

D. A. Smith, E. Brion, R. Britto +18

We have measured the gamma-ray fluxes of the blazars Mrk 421 and Mrk 501 in the energy range between 50 and 350 GeV (1.2 to 8.3 x 10^25 Hz). The detector, called CELESTE, used firs…

astro-ph200636 cited

Study of time lags in HETE-2 Gamma-Ray Bursts with redshift: search for astrophysical effects and Quantum Gravity signature

J. Bolmont, J. -L. Atteia, A. Jacholkowska +2

The study of time lags between spikes in Gamma-Ray Burst light curves in different energy bands as a function of redshift may lead to the detection of effects due to Quantum Gravit…

astro-ph2006

Indirect Search for Dark Matter in M31 with the CELESTE Experiment

J. Lavalle, H. Manseri, A. Jacholkowska +13

If dark matter is made of neutralinos, annihilation of such Majorana particles should produce high energy cosmic rays, especially in galaxy halo high density regions like galaxy ce…