activity
20062008
most citedA synchrotron self-Compton scenario for the very high energy gamma-ray emission of the radiogalaxy M87

86 citations · 86 across the 5 of their papers we have counts for

collaborators

6 papers

astro-ph2008

SSC scenario for VHE emission from 2 radiogalaxies: M 87 and Cen A

Jean-Philippe Lenain, Catherine Boisson, Hélène Sol

M 87 is the first extragalactic source detected in the Very High Energy (VHE; E > 100 GeV) gamma-ray domain that is not a blazar, its large scale jet not being aligned to the line…

astro-ph200786 cited

A synchrotron self-Compton scenario for the very high energy gamma-ray emission of the radiogalaxy M87

Jean-Philippe Lenain, Catherine Boisson, Hélène Sol +1

M87 is the first extragalactic source detected in the TeV range that is not a blazar. With the increasing performances of ground-based Cherenkov telescopes, we can now probe the va…

astro-ph2007

Predictions of Very High Energy gamma-ray fluxes for three Active Galactic Nuclei

Jean-Philippe Lenain

M87 is the first extragalactic source detected at the TeV that is not a blazar. To account for the recent observations of M87 made by the High Energy Stereoscopic System (H.E.S.S.)…

astro-ph2007

Modeling of the multiwavelength emission of M87 with H.E.S.S. observations

Jean-Philippe Lenain

M87 is the first extragalactic source detected in the TeV range that is not a blazar. The large scale jet of M87 is not aligned with the line of sight. Modification of standard emi…

astro-ph2007

Multiwavelength modeling of TeV AGN observed by HESS

Jean-Philippe Lenain

The High Energy Stereoscopic System (H.E.S.S.) experiment, a ground-based gamma-ray Cherenkov telescope array located in Namibia, has now detected many extragalactic objects, which…

astro-ph2006

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…