activity
19972026
most citedVariable VHE gamma-ray emission from Markarian 501

547 citations · 15.3k across the 263 of their papers we have counts for

collaborators
Showing 2009Show all

20 papers · 1 filter

astro-ph.HE2009★ 21 cited

Simultaneous multi-frequency observation of the unknown redshift blazar PG 1553+113 in March-April 2008

MAGIC Collaboration, J. Aleksić, H. Anderhub +161

The blazar PG 1553+113 is a well known TeV gamma-ray emitter. In this paper, we determine its spectral energy distribution using simultaneous multi-frequency data in order to study…

astro-ph.HE2009★ 56 cited

Correlated X-ray and Very High Energy emission in the gamma-ray binary LS I +61 303

The MAGIC Collaboration, H. Anderhub, L. A. Antonelli +153

The discovery of very high energy (VHE) gamma-ray emitting X-ray binaries has triggered an intense effort to better understand the particle acceleration, absorption, and emission m…

astro-ph.HE2009★ 59 cited

Simultaneous Multiwavelength observation of Mkn 501 in a low state in 2006

The MAGIC Collaboration, H. Anderhub, R. Sato +4

We present results of the multiwavelength campaign on the TeV blazar Mkn 501 performed in 2006 July, including MAGIC for the VHE gamma-ray band and Suzaku for the X-ray band. A VHE…

astro-ph.HE2009★ 5 cited

JEM-EUSO Science Objectives

Gustavo Medina-Tanco, K. Asano, D. Cline +10

JEM-EUSO, on board of the Japanese Exploration Module of the International Space Station, is being proposed as the first space observatory devoted to UHECR. Its privileged position…

astro-ph.HE2009

Hadron-gamma discrimination from an orbital UHECR observatory

A. D. Supanitsky, G. Medina-Tanco, K. Asano +10

The identification of very high energy photons is of great importance for the understanding of the origin of extreme energy cosmic rays (EECR). Several can be the sources of high e…

astro-ph.HE2009

Development of neutrino initiated cascades at mid and high altitudes in the atmosphere

A. D. Supanitsky, G. Medina-Tanco, K. Asano +9

Neutrinos are a very promising messenger at tens of EeV and above. They can be produced by several channels, namely as by products of hadronic interactions at the sources, as the m…