output
19922020
most citedGATE : a simulation toolkit for PET and SPECT

2.2k citations

Showing 2018 · astro-ph.HEShow all

6 papers · 2 filters

astro-ph.HE2018★ 293 cited

The Giant Radio Array for Neutrino Detection (GRAND): Science and Design

GRAND Collaboration, Jaime Alvarez-Muniz, Rafael Alves Batista +48

The Giant Radio Array for Neutrino Detection (GRAND) is a planned large-scale observatory of ultra-high-energy (UHE) cosmic particles, with energies exceeding 10^8 GeV. Its goal is…

astro-ph.HE2018★ 92 cited

Joint constraints on Galactic diffuse neutrino emission from ANTARES and IceCube

A. Albert, M. André, M. Anghinolfi +454

The existence of diffuse Galactic neutrino production is expected from cosmic ray interactions with Galactic gas and radiation fields. Thus, neutrinos are a unique messenger offeri…

astro-ph.HE2018★ 20 cited

The cosmic ray shadow of the Moon observed with the ANTARES neutrino telescope

A. Albert, M. André, M. Anghinolfi +124

One of the main objectives of the ANTARES telescope is the search for point-like neutrino sources. Both the pointing accuracy and the angular resolution of the detector are importa…

astro-ph.HE2018★ 29 cited

Search for neutrinos from TXS 0506+056 with the ANTARES telescope

A. Albert, M. Andrè, M. Anghinolfi +124

The results of three different searches for neutrino candidates, associated with the IceCube-170922A event or from the direction of TXS 0506+056, by the ANTARES neutrino telescope…

astro-ph.HE2018★ 13 cited

Search for high-energy neutrinos in coincidence with Fast Radio Bursts with the ANTARES neutrino telescope

A. Albert, M. André, M. Anghinolfi +125

In the past decade, a new class of bright transient radio sources with millisecond duration has been discovered. The origin of these so-called Fast Radio Bursts (FRBs) is still a g…

astro-ph.HE2018★ 12 cited

Understanding Type Ia supernovae through their U-band spectra

J. Nordin, G. Aldering, P. Antilogus +39

Context. Observations of Type Ia supernovae (SNe Ia) can be used to derive accurate cosmological distances through empirical standardization techniques. Despite this success neithe…