activity
20052026
most citedVariable Very High Energy Gamma-ray Emission from the Microquasar LS I +61 303

405 citations · 578 across the 15 of their papers we have counts for

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astro-ph2006★ 405 cited

Variable Very High Energy Gamma-ray Emission from the Microquasar LS I +61 303

MAGIC Collaboration, J. Albert

Microquasars are binary star systems with relativistic radio-emitting jets. They are potential sources of cosmic rays and laboratories for elucidating the physics of relativistic j…

astro-ph2006★ 59 cited

Observation of VHE Gamma Radiation from HESS J1834-087/W41 with the MAGIC Telescope

J. Albert et al.

Recently, the HESS array has reported the detection of gamma-ray emission above a few hundred GeV from eight new sources located close to the Galactic Plane. The source HESS J1834-…

astro-ph2006★ 43 cited

Flux upper limit of gamma-ray emission by GRB050713a from MAGIC Telescope observations

J. Albert, E. Aliu, H. Anderhub +127

The long-duration GRB050713a was observed by the MAGIC Telescope, 40 seconds after the burst onset, and followed up for 37 minutes, until twilight. The observation, triggered by a…

astro-ph2005★ 41 cited

MAGIC observations of very high energy gamma-rays from HESS J1813-178

J. Albert, MAGIC collaboration

Recently, the HESS collaboration has reported the detection of gamma-ray emission above a few hundred GeV from eight new sources located close to the Galactic Plane. The source HES…

astro-ph2005★ 11 cited

Using the photons from the Crab Nebula seen by GLAST to calibrate MAGIC and the Imaging Air Cherenkov Telescopes

D. Bastieri, C. Bigongiari, E. Bisesi +14

In this article we discuss the possibility of using the observations by GLAST of standard gamma sources, as the Crab Nebula, to calibrate Imaging Air Cherenkov detectors, MAGIC in…

astro-ph2005

Contribution of pulsars to the gamma-ray background and their observation with the space telescopes GLAST and AGILE

E. Bisesi

Luminosities and uxes of the expected population of galactic gamma-ray pulsars become foreseeable if physical distributions at birth and evolutive history are assigned. In this wor…