activity
20072020
most citedDesign Concepts for the Cherenkov Telescope Array

902 citations · 8.6k across the 102 of their papers we have counts for

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Showing 2012Show all

9 papers · 1 filter

astro-ph.HE2012

CTA and cosmic-ray diffusion in molecular clouds

G. Pedaletti, D. F. Torres, S. Gabici +3

Molecular clouds act as primary targets for cosmic-ray interactions and are expected to shine in gamma-rays as a by-product of these interactions. Indeed several detected gamma-ray…

astro-ph.IM2012★ 236 cited

Monte Carlo design studies for the Cherenkov Telescope Array

K. Bernlöhr, A. Barnacka, Y. Becherini +36

The Cherenkov Telescopes Array (CTA) is planned as the future instrument for very-high-energy (VHE) gamma-ray astronomy with a wide energy range of four orders of magnitude and an…

astro-ph.HE2012★ 28 cited

Binaries with the eyes of CTA

J. M. Paredes, W. Bednarek, P. Bordas +20

The binary systems that have been detected in gamma rays have proven very useful to study high-energy processes, in particular particle acceleration, emission and radiation reproce…

astro-ph.HE2012★ 30 cited

Gamma-ray signatures of cosmic ray acceleration, propagation, and confinement in the era of CTA

F. Acero, A. Bamba, S. Casanova +11

Galactic cosmic rays are commonly believed to be accelerated at supernova remnants via diffusive shock acceleration. Despite the popularity of this idea, a conclusive proof for its…

astro-ph.IM2012★ 37 cited

Prospects for Observations of Pulsars and Pulsar Wind Nebulae with CTA

E. de Ona Wilhelmi, B. Rudak, J. A. Barrio +11

The last few years have seen a revolution in very-high gamma-ray astronomy (VHE; E>100 GeV) driven largely by a new generation of Cherenkov telescopes (namely the H.E.S.S. telescop…

astro-ph.HE2012★ 39 cited

Discovery of VHE emission towards the Carina arm region with the H.E.S.S. telescope array: HESS J1018-589

HESS Collaboration, A. Abramowski, F. Acero +195

The observational coverage with HESS of the Carina region in VHE gamma-rays benefits from deep exposure (40 h) of the neighboring open cluster Westerlund 2. The observations have r…