activity
19982026
most citedObservation of a Large-scale Anisotropy in the Arrival Directions of Cosmic Rays above eV

409 citations · 6.4k across the 159 of their papers we have counts for

collaborators
Showing 2009Show all

14 papers · 1 filter

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★ 1 cited

Studying individual UHECR sources with high statistics

Gustavo Medina-Tanco

One of the main impacts of the JEM-EUSO mission will come from its unprecedented exposure. This feature creates, for the first time in the field, the possibility of studying indivi…

astro-ph.IM2009★ 1 cited

BATATA: A device to characterize the punch-through observed in underground muon detectors and to operate as a prototype for AMIGA

Gustavo Medina-Tanco

BATATA is a hodoscope comprising three X-Y planes of plastic scintillation detectors. This system of buried counters is complemented by an array of 3 water-Cherenkov detectors, loc…

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

On the statistical effects of multiple reusing of simulated air showers in detector simulations

A. D. Supanitsky, G. Medina-Tanco

The simulations of extensive air showers as well as the detectors involved in their detection play a fundamental role in the study of the high energy cosmic rays. At the highest en…

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…