G. Ferrara YOU? Author Swipe

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Deep Learning Framework for Enhanced Neutrino Reconstruction of Single-line Events in the ANTARES Telescope Open

A. Albert, Sofia Giusti Alves, M. Ardid, S. Ardid, B. Baret , et al. · 2025

We present the $N$-fit algorithm designed to improve the reconstruction of neutrino events detected by a single line of the ANTARES underwater telescope, usually associated with low energy neutrino events ($\sim$ 100 GeV). $N$-Fit is a neu…

KM3NeT constraint on Lorentz-violating superluminal neutrino velocity Open

О. Адриани, S. Aiello, A.R Alhebsi, M. Alshamsi, A. Ambrosone , et al. · 2025

Lorentz invariance is a fundamental symmetry of spacetime and foundational to modern physics. One of its most important consequences is the constancy of the speed of light. This invariance, together with the geometry of spacetime, implies …

Search for magnetic monopoles with the complete ANTARES dataset Open

A. Albert, S. Alves, M. André, M. Ardid, S Ardid , et al. · 2025

Tests and calibration of detector strings for the KM3NeT/ARCA neutrino telescope Open

S. Mastroianni, F. Badaracco, Francesca Gualandi, G. Ferrara, V. Kulikovskiy , et al. · 2025

Investigating Cherenkov Telescope Array Observatory capability to detect gamma-ray emission from simulated neutrino sources identified by KM3NeT Open

Gloria Maria Cicciari, G. Ferrara, M. Mallamaci, G. Marsella, O. Sergijenko , et al. · 2025

The ANTARES detector: two decades of neutrino searches in the Mediterranean Sea Open

Maurizio Spurio, S. Alves, M. André, M. Ardid, S Ardid , et al. · 2025

Interest for studying cosmic neutrinos using deep-sea detectors has increase after the discovery of a diffuse flux of cosmic neutrinos by the IceCube collaboration and the possibility of wider multi-messenger studies with the observations …

Constraining gamma-ray burst parameters with the first ultra-high energy neutrino event KM3-230213A Open

O. Adriani, A. Albert, A.R Alhebsi, S Alshalloudi, M. Alshamsi , et al. · 2025

Context: The detection of the highest energy neutrino observed to date by KM3NeT, with an estimated energy of 220 PeV, opens up new possibilities for the study and identification of the astrophysical sources responsible for a diffuse flux …

gSeaGen code by KM3NeT: An efficient tool to propagate muons simulated with CORSIKA Open

S. Aiello, A. Albert, A.R Alhebsi, M. Alshamsi, S. Alves Garre , et al. · 2025

The ANTARES detector: Two decades of neutrino searches in the Mediterranean Sea Open

A. Albert, S. Alves, M. André, M. Ardid, S. Ardid , et al. · 2025

Probing invisible neutrino decay with the first six detection units of KM3NeT/ORCA Open

S. Aiello, A. Albert, A.R Alhebsi, M. Alshamsi, S. Alves Garre , et al. · 2025

First searches for dark matter with the KM3NeT neutrino telescopes Open

S. Aiello, A. Albert, A.R Alhebsi, M. Alshamsi, S. Alves Garre , et al. · 2025

Indirect dark matter detection methods are used to observe the products of dark matter annihilations or decays originating from astrophysical objects where large amounts of dark matter are thought to accumulate. With neutrino telescopes, a…

Study of tau neutrinos and non-unitary neutrino mixing with the first six detection units of KM3NeT/ORCA Open

S. Aiello, A. Albert, A.R Alhebsi, M. Alshamsi, S. Alves Garre , et al. · 2025

Oscillations of atmospheric muon and electron neutrinos produce tau neutrinos with energies in the GeV range, which can be observed by the ORCA detector of the KM3NeT neutrino telescope in the Mediterranean Sea. First measurements with ORC…

Search for non-standard neutrino interactions with the first six detection units of KM3NeT/ORCA Open

S. Aiello, A. Albert, A.R Alhebsi, M. Alshamsi, S. Alves Garre , et al. · 2025

KM3NeT/ORCA is an underwater neutrino telescope under construction in the Mediterranean Sea. Its primary scientific goal is to measure the atmospheric neutrino oscillation parameters and to determine the neutrino mass ordering. ORCA can co…

Acoustic positioning for deep sea neutrino telescopes with a system of piezo sensors integrated into glass spheres Open

A. Albert, S. Alves, M. André, M. Ardid, S. Ardid , et al. · 2025

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

S. Aiello, A. Albert, A.R Alhebsi, M. Alshamsi, S. Alves Garre , et al. · 2024

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 coherence along the propagation of the neutrino $-$ a pheno…

Results of the follow-up of ANTARES neutrino alerts Open

A. Albert, Sofia Giusti Alves, M. André, M. Ardid, S. Ardid , et al. · 2024

High-energy neutrinos could be produced in the interaction of charged cosmic rays with matter or radiation surrounding astrophysical sources. To look for transient sources associated with neutrino emission, a follow-up program of neutrino …

Measurement of neutrino oscillation parameters with the first six detection units of KM3NeT/ORCA Open

S. Aiello, A. Albert, A.R Alhebsi, M. Alshamsi, S. Alves Garre , et al. · 2024

KM3NeT/ORCA is a water Cherenkov neutrino detector under construction and anchored at the bottom of the Mediterranean Sea. The detector is designed to study oscillations of atmospheric neutrinos and determine the neutrino mass ordering. Th…

Constraints on the energy spectrum of the diffuse cosmic neutrino flux from the ANTARES neutrino telescope Open

A. Albert, S. Alves, M. André, M. Ardid, S. Ardid , et al. · 2024

High-significance evidences of the existence of a high-energy diffuse flux of cosmic neutrinos have emerged in the last decade from several observations by the IceCube Collaboration. The ANTARES neutrino telescope took data for 15 years in…

Constraints on the energy spectrum of the diffuse cosmic neutrino flux from the ANTARES neutrino telescope Open

A. Albert, Sofia Giusti Alves, M. André, M. Ardid, S Ardid , et al. · 2024

High-significance evidences of the existence of a high-energy diffuse flux of cosmic neutrinos have emerged in the last decade from several observations by the IceCube Collaboration. The ANTARES neutrino telescope took data for 15 years in…

Differential Sensitivity of the KM3NeT/ARCA detector to a diffuse neutrino flux and to point-like source emission: Exploring the case of the Starburst Galaxies Open

S. Aiello, A. Albert, M. Alshamsi, S. Alves Garre, Z. Aly , et al. · 2024

Acoustic Positioning for Deep Sea Neutrino Telescopes with a System of Piezo Sensors Integrated into Glass Spheres Open

A. Albert, Sofia Giusti Alves, M. André, M. Ardid, Salva Ardid , et al. · 2024

Position calibration in the deep sea is typically done by means of acoustic multilateration using three or more acoustic emitters installed at known positions. Rather than using hydrophones as receivers that are exposed to the ambient pres…

Search for Neutrino Emission from GRB 221009A using the KM3NeT ARCA and ORCA detectors Open

S. Aiello, A. Albert, M. Alshamsi, S. Alves Garre, Antonio Ambrosone , et al. · 2024

Gamma-ray bursts are promising candidate sources of high-energy astrophysical neutrinos. The recent GRB 221009A event, identified as the brightest gamma-ray burst ever detected, provides a unique opportunity to investigate hadronic emissio…

Searches for neutrino counterparts of gravitational waves from the LIGO/Virgo third observing run with KM3NeT Open

S. Aiello, A. Albert, S. Alves Garre, Z. Aly, Antonio Ambrosone , et al. · 2024

The KM3NeT neutrino telescope is currently being deployed at two different sites in the Mediterranean Sea. First searches for astrophysical neutrinos have been performed using data taken with the partial detector configuration already in o…

Searches for Neutrinos in the Direction of Radio-bright Blazars with the ANTARES Telescope Open

A. Albert, Sofia Giusti Alves, M. André, M. Ardid, Salva Ardid , et al. · 2024

Active galaxies, especially blazars, are among the most promising extragalactic candidates for high-energy neutrino sources. To date, ANTARES searches included these objects and used GeV–TeV γ -ray flux to select blazars. Here, a statistic…

Results of the follow-up of ANTARES neutrino alerts Open

A. Albert, S. Alves, M. André, M. Ardid, Salva Ardid , et al. · 2024

High-energy neutrinos could be produced in the interaction of charged cosmic rays with matter or radiation surrounding astrophysical sources. To look for transient sources associated with neutrino emission, a follow-up program of neutrino …

KM3NeT real-time analysis framework Open

Massimo Mastrodicasa, S. Aiello, A. Albert, M. Alshamsi, S. Alves Garre , et al. · 2024

Track: Astrophysical neutrinos

Prospects for combined analyses of hadronic emission from $$\gamma $$-ray sources in the Milky Way with CTA and KM3NeT Open

Tim Unbehaun, L. Mohrmann, S. Funk, S. Aiello, A. Albert , et al. · 2024

The Cherenkov Telescope Array and the KM3NeT neutrino telescopes are major upcoming facilities in the fields of $$\gamma $$ -ray and neutrino astronomy, respectively. Possible simultaneous production of $$\gamma $$ rays and neutrinos i…

Searches for neutrino counterparts of gravitational waves from the LIGO/Virgo third observing run with KM3NeT Open

KM NeT Collaboration, S. Aiello, A. Albert, S. Alves Garre, Z. Aly , et al. · 2023

The KM3NeT neutrino telescope is currently being deployed at two different sites in the Mediterranean Sea. First searches for astrophysical neutrinos have been performed using data taken with the partial detector configuration already in o…

Studying bioluminescence flashes with the <span>ANTARES</span> deep‐sea neutrino telescope Open

Nico Reeb, Sebastian Hutschenreuter, Philipp Zehetner, T. A. Enßlin, A. Albert , et al. · 2023

We develop a novel technique to exploit the extensive data sets provided by underwater neutrino telescopes to gain information on bioluminescence in the deep sea. The passive nature of the telescopes gives us the unique opportunity to infe…

Observations of the Crab Nebula and Pulsar with the Large-sized Telescope Prototype of the Cherenkov Telescope Array Open

Hidetarô Abe, K. Abe, S. Abe, Arnau Aguasca-Cabot, I. Agudo , et al. · 2023

The Cherenkov Telescope Array (CTA) is a next-generation ground-based observatory for gamma-ray astronomy at very high energies. The Large-Sized Telescope prototype (LST-1) is located at the CTA-North site, on the Canary Island of La Palma…

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