activity
20062026
most citedDesign Concepts for the Cherenkov Telescope Array

902 citations · 5k across the 37 of their papers we have counts for

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astro-ph2008★ 21 cited

MAGIC Observations of PG 1553+113 during a Multiwavelength Campaign in July 2006

MAGIC Collaboration, Albert

The active galactic nucleus PG 1553+113 was observed by the MAGIC telescope in July 2006 during a multiwavelength campaign, in which telescopes in the optical, X-ray, and very high…

astro-ph2008★ 125 cited

Improving the performance of the single-dish Cherenkov telescope MAGIC through the use of signal timing

MAGIC Collaboration

The Cherenkov light flashes produced by Extensive Air Showers are very short in time. A high bandwidth and fast digitizing readout, therefore, can minimize the influence of the bac…

astro-ph2008★ 108 cited

Very High Energy Gamma-Ray Observations of a Strong Flaring Activity in M87 in 2008 February

MAGIC Collaboration, J. Albert

M87 is the only known non blazar radio galaxy to emit very high energy (VHE) gamma-rays. During a monitoring program of M87, a rapid flare in VHE gamma-rays was detected by the MAG…

astro-ph2008★ 84 cited

MAGIC observations of the unidentified TeV gamma-ray source TeV J2032+4130

J. Albert

We observed the first known very high energy (VHE) gamma-ray emitting unidentified source, TeV J2032+4130, for 94 hours with the MAGIC telescope. The source was detected with a sig…

astro-ph2008★ 57 cited

Multi-wavelength (radio, X-ray and gamma-ray) observations of the gamma-ray binary LS I +61 303

MAGIC Collaboration, J. Albert

We present the results of the first multiwavelength observing campaign on the high-mass X-ray binary LS I +61 303 comprising observations at the TeV regime with the MAGIC telescope…

astro-ph2007★ 246 cited

Very High Energy Gamma-ray Radiation from the Stellar-mass Black Hole Cygnus X-1

MAGIC Collaboration, J. Albert

We report on the results from the observations in very high energy band (VHE, E_gamma > 100 GeV) of the black hole X-ray binary (BHXB) Cygnus X-1. The observations were performed w…