activity
20012019
most citedMonte Carlo studies for the optimisation of the Cherenkov Telescope Array layout

72 citations · 104 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.IM2019★ 72 cited

Monte Carlo studies for the optimisation of the Cherenkov Telescope Array layout

A. Acharyya, I. Agudo, E. O. Angüner +467

The Cherenkov Telescope Array (CTA) is the major next-generation observatory for ground-based very-high-energy gamma-ray astronomy. It will improve the sensitivity of current groun…

astro-ph.HE2017★ 3 cited

Cherenkov Telescope Array Contributions to the 35th International Cosmic Ray Conference (ICRC2017)

F. Acero, B. S. Acharya, V. Acín Portella +1137

List of contributions from the Cherenkov Telescope Array Consortium presented at the 35th International Cosmic Ray Conference, July 12-20 2017, Busan, Korea.

astro-ph.HE2016★ 1 cited

Contributions of the Cherenkov Telescope Array (CTA) to the 6th International Symposium on High-Energy Gamma-Ray Astronomy (Gamma 2016)

The CTA Consortium, :, A. Abchiche +1387

List of contributions from the Cherenkov Telescope Array (CTA) Consortium presented at the 6th International Symposium on High-Energy Gamma-Ray Astronomy (Gamma 2016), July 11-15,…

nucl-th2009

High Momentum Probes of Nuclear Matter

Rainer J. Fries

We discuss how the chemical composition of QCD jets is altered by final state interactions in surrounding nuclear matter. We describe this process through conversions of leading je…

astro-ph2002★ 21 cited

BL Lac Identification for the Ultraluminous X-ray Source Observed in the Direction of NGC 4698

L. Foschini, L. C. Ho, N. Masetti +11

We report the identification of the optical and radio counterparts of the ultraluminous X-ray (ULX) source XMMU J124825.9+083020 (NGC4698-ULX1). The optical spectrum taken with the…

astro-ph2001★ 7 cited

On the Origin of the FeK Line in the Seyfert 2 Galaxy NGC 7172

M. Dadina, L. Bassani, M. Cappi +6

The Seyfert 2 Galaxy NGC 7172 was observed twice by BeppoSAX narrow field instruments approximately one year apart. As found in previous observations, the source is variable on sho…