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GATE V6: a major enhancement of the GATE simulation platform enabling modelling of CT and radiotherapy.
TLDR
This paper presents an overview of the main additions and improvements implemented in GATE since the publication of the initial GATE paper since 2001 and first publicly released in 2004. Expand
The ANTARES optical module
The ANTARES collaboration is building a deep sea neutrino telescope in the Mediterranean Sea. This detector will cover a sensitive area of typically 0.1 km-squared and will be equipped with aboutExpand
A Deep Sea Telescope for High Energy Neutrinos
The ANTARES Collaboration proposes to construct a large area water Cherenkov detector in the deep Mediterranean Sea, optimised for the detection of muons from high-energy astrophysical neutrinos.Expand
Background light in potential sites for the ANTARES undersea neutrino telescope
Abstract The ANTARES collaboration has performed a series of in-situ measurements to study the background light for a planned undersea neutrino telescope. Such background can be caused by 40 K decaysExpand
The chorus experiment to search for νμ → ντ oscillation
Abstract A new experimental apparatus, designed principally for a high sensitivity search for ν μ → ν τ oscillation, has been successlly constructed and made operational by the CHORUS CollaborationExpand
Monte Carlo studies for the optimisation of the Cherenkov Telescope Array layout
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 ground-based instrumentsExpand
Pre-construction estimates of the Cherenkov Telescope Array sensitivity to a dark matter signal from the Galactic centre
We provide an updated assessment of the power of the Cherenkov Telescope Array (CTA) to search for thermally produced dark matter at the TeV scale, via the associated gamma-ray signal fromExpand
The CHORUS experiment
The Chorus experiment, which aims at a search for v μ → v τ oscillations using the neutrino beam of the CERN-SPS, has successfully taken data in 1994 and 1995. The detection technique will beExpand
Development of K-edge spectral tomography using XPAD3 composite pixels
TLDR
We investigate the capability to perform K-edge imaging by using the hybrid pixel camera XPAD3 with 500,000 pixels of (130 × 130) μm2 integrated in the micro-CT demonstrator. Expand
Sensitivity of the Cherenkov Telescope Array to a dark matter signal from the Galactic centre
We provide an updated assessment of the power of the Cherenkov Telescope Array (CTA) to search for thermally produced dark matter at the TeV scale, via the associated gamma-ray signal fromExpand
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