activity
20042013
most citedDesign Concepts for the Cherenkov Telescope Array

902 citations · 5.6k across the 48 of their papers we have counts for

collaborators

48 papers

astro-ph.HE2013★ 7 cited

CTA contributions to the 33rd International Cosmic Ray Conference (ICRC2013)

The CTA Consortium, :, O. Abril +1102

Compilation of CTA contributions to the proceedings of the 33rd International Cosmic Ray Conference (ICRC2013), which took place in 2-9 July, 2013, in Rio de Janeiro, Brazil

astro-ph.IM2010★ 902 cited

Design Concepts for the Cherenkov Telescope Array

The CTA Consortium

Ground-based gamma-ray astronomy has had a major breakthrough with the impressive results obtained using systems of imaging atmospheric Cherenkov telescopes. Ground-based gamma-ray…

astro-ph.HE2010★ 58 cited

Magic constraints on Gamma-ray emission from Cygnus X-3

J. Aleksić, L. A. Antonelli, P. Antoranz +156

Cygnus X-3 is a microquasar consisting of an accreting compact object orbiting around a Wolf-Rayet star. It has been detected at radio frequencies and up to high-energy gamma rays…

astro-ph.HE2010★ 17 cited

MAGIC observation of the GRB080430 afterglow

MAGIC Collaboration, J. Aleksić, H. Anderhub +151

Context: Gamma-ray bursts are cosmological sources emitting radiation from the gamma-rays to the radio band. Substantial observational efforts have been devoted to the study of gam…

astro-ph.HE2010★ 66 cited

Search for an extended VHE gamma-ray emission from Mrk 421 and Mrk 501 with the MAGIC Telescope

MAGIC Collaboration, J. Aleksić, L. A. Antonelli +148

Context: Part of the very high energy -ray radiation coming from extragalactic sources is absorbed through the pair production process on the extragalactic background light phot…

astro-ph.HE2010★ 26 cited

Gamma-ray excess from a stacked sample of high- and intermediate-frequency peaked blazars observed with the MAGIC telescope

MAGIC Collaboration, J. Aleksić, L. A. Antonelli +147

Between 2004 and 2009 a sample of 28 X-ray selected high- and intermediate-frequency peaked blazars with a X-ray flux larger than 2 uJy at 1 keV in the redshift range from 0.018 to…