activity
20002024
most citedThe Phase II Murchison Widefield Array: Design Overview

240 citations · 372 across the 6 of their papers we have counts for

collaborators

6 papers

hep-ex2024

Search for quantum decoherence in neutrino oscillations with six detection units of KM3NeT/ORCA

S. Aiello, A. Albert, A. R. Alhebsi +259

Neutrinos described as an open quantum system may interact with the environment which introduces stochastic perturbations to their quantum phase. This mechanism leads to a loss of…

astro-ph.HE2024★ 23 cited

Spectrum and extension of the inverse-Compton emission of the Crab Nebula from a combined Fermi-LAT and H.E.S.S. analysis

F. Aharonian, F. Ait Benkhali, J. Aschersleben +158

The Crab Nebula is a unique laboratory for studying the acceleration of electrons and positrons through their non-thermal radiation. Observations of very-high-energy rays from…

physics.ins-det2019★ 37 cited

Dependence of atmospheric muon flux on seawater depth measured with the first KM3NeT detection units

KM3NeT Collaboration, M. Ageron, S. Aiello +262

KM3NeT is a research infrastructure located in the Mediterranean Sea, that will consist of two deep-sea Cherenkov neutrino detectors. With one detector (ARCA), the KM3NeT Collabora…

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.IM2018★ 240 cited

The Phase II Murchison Widefield Array: Design Overview

Randall B. Wayth, Steven J. Tingay, Cathryn M. Trott +26

We describe the motivation and design details of the "Phase II" upgrade of the Murchison Widefield Array (MWA) radio telescope. The expansion doubles to 256 the number of antenna t…

astro-ph2000

XMM-Newton EPIC Observation of SMC SNR 0102-72.3

M. Sasaki, T. F. X. Stadlbauer, F. Haberl +2

Results from observations of the young oxygen-rich supernova remnant SNR 0102-72.3 in the Small Magellanic Cloud during the calibration phase of the XMM-Newton Observatory are pres…