activity
20042008
most citedFast variability of TeV gamma-rays from the radio galaxy M 87

342 citations · 1.1k across the 15 of their papers we have counts for

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11 papers · 1 filter

astro-ph20071 cited

A particle acceleration site in the Coma cluster?

D. Eckert, N. Produit, A. Neronov +1

We present the results of a deep (1.1 Ms) observation of the Coma cluster of galaxies in the 18-30 keV band with the IBIS/ISGRI imager on board the INTEGRAL satellite. We show that…

astro-ph200722 cited

Can one detect passage of small black hole through the Earth?

I. B. Khriplovich, A. A. Pomeransky, N. Produit +1

The energy losses of a small black hole passing through the Earth are examined. In particular, we investigate the excitations in the frequency range accessible to modern acoustic d…

astro-ph200725 cited

South-West extension of the hard X-ray emission from the Coma cluster

D. Eckert, A. Neronov, T. J. -L. Courvoisier +1

We explore the morphology of hard (18-30 keV) X-ray emission from the Coma cluster of galaxies. We analyze a deep (1.1 Ms) observation of the Coma cluster with the ISGRI imager on…

astro-ph200799 cited

A description of sources detected by INTEGRAL during the first 4 years of observations

A. Bodaghee, T. J. -L. Courvoisier, J. Rodriguez +6

Parameters from the literature, such as positions, photoelectric absorption (nH), spin and orbital periods, and distances or redshifts, were collected for all ~500 sources detected…

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…