activity
20012022
most citedThe ANTARES Optical Module

208 citations · 1.8k across the 35 of their papers we have counts for

collaborators

35 papers

astro-ph.HE2022★ 5 cited

Limits on the nuclearite flux using the ANTARES neutrino telescope

ANTARES Collaboration, A. Albert, S. Alves +143

In this work, a search for nuclearites of strange quark matter by using nine years of ANTARES data taken in the period 2009-2017 is presented. The passage through matter of these p…

astro-ph.HE2022★ 9 cited

Search for secluded dark matter towards the Galactic Centre with the ANTARES neutrino telescope

A. Albert, S. Alves, M. Andre +146

Searches for dark matter (DM) have not provided any solid evidence for the existence of weakly interacting massive particles in the GeV-TeV mass range. Coincidentally, the scale of…

hep-ex2021★ 24 cited

Measurement of the atmospheric and energy spectra with the ANTARES neutrino telescope

A. Albert, S. Alves, M. André +139

This letter presents a combined measurement of the energy spectra of atmospheric and in the energy range between 100 GeV and 50 TeV with the ANTARES neutrin…

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.HE2017★ 192 cited

The SUrvey for Pulsars and Extragalactic Radio Bursts II: New FRB discoveries and their follow-up

S. Bhandari, E. F. Keane, E. D. Barr +47

We report the discovery of four Fast Radio Bursts (FRBs) in the ongoing SUrvey for Pulsars and Extragalactic Radio Bursts (SUPERB) at the Parkes Radio Telescope: FRBs 150610, 15120…

astro-ph.HE2017★ 53 cited

New Constraints on all flavour Galactic diffuse neutrino emission with the ANTARES telescope

A. Albert, M. André, M. Anghinolfi +126

The flux of very high-energy neutrinos produced in our Galaxy by the interaction of accelerated cosmic rays with the interstellar medium is not yet determined. The characterization…