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View article: Probing neutrino yield from different gamma-ray burst populations using the entire ANTARES data set
Probing neutrino yield from different gamma-ray burst populations using the entire ANTARES data set Open
While the evidence of high-energy neutrinos was established a decade ago and confirmed independently by the observation of an ultra-high-energy neutrino recently announced, the origin of these neutrinos is not yet fully identified. Gamma-r…
View article: Search for quantum decoherence in neutrino oscillations with six detection units of KM3NeT/ORCA
Search for quantum decoherence in neutrino oscillations with six detection units of KM3NeT/ORCA Open
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 phenome…
View article: First searches for dark matter with the KM3NeT neutrino telescopes
First searches for dark matter with the KM3NeT neutrino telescopes Open
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…
View article: Search for non-standard neutrino interactions with the first six detection units of KM3NeT/ORCA
Search for non-standard neutrino interactions with the first six detection units of KM3NeT/ORCA Open
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…
Constraints on the energy spectrum of the diffuse cosmic neutrino flux from the ANTARES neutrino telescope Open
The high-purity all-flavour neutrino sample collected with the ANTARES neutrino telescope over 15 years of data taking in the Mediterranean Sea, from 2007 to 2022, has been used to search for a diffuse cosmic neutrino signal. No statistica…
View article: KM3NeT Online Multi-Messenger Results
KM3NeT Online Multi-Messenger Results Open
KM3NeT is a Cherenkov-light based neutrino telescope located in the Mediterranean Sea, comprising two detectors ARCA (Sicily, It) and ORCA (Var, Fr). Currently at ∼15% of its total deployment, with completion expected by 2029, it has an en…
Management of the data processing & Run-by-Run simulations in KM3NeT Open
The KM3NeT collaboration is constructing two underwater neutrino detectors in the Mediterranean Sea: ARCA, optimized for the observation of astrophysical neutrinos, and ORCA, designed to determine the neutrino mass hierarchy by detecting a…
View article: Search for quantum decoherence in neutrino oscillations with six detection units of KM3NeT/ORCA
Search for quantum decoherence in neutrino oscillations with six detection units of KM3NeT/ORCA Open
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…
View article: Results of the follow-up of ANTARES neutrino alerts
Results of the follow-up of ANTARES neutrino alerts Open
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 …
View article: Constraints on the energy spectrum of the diffuse cosmic neutrino flux from the ANTARES neutrino telescope
Constraints on the energy spectrum of the diffuse cosmic neutrino flux from the ANTARES neutrino telescope Open
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…
View article: Constraints on the energy spectrum of the diffuse cosmic neutrino flux from the ANTARES neutrino telescope
Constraints on the energy spectrum of the diffuse cosmic neutrino flux from the ANTARES neutrino telescope Open
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…
View article: Acoustic Positioning for Deep Sea Neutrino Telescopes with a System of Piezo Sensors Integrated into Glass Spheres
Acoustic Positioning for Deep Sea Neutrino Telescopes with a System of Piezo Sensors Integrated into Glass Spheres Open
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…
View article: Searches for Neutrinos in the Direction of Radio-bright Blazars with the ANTARES Telescope
Searches for Neutrinos in the Direction of Radio-bright Blazars with the ANTARES Telescope Open
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…
View article: Results of the follow-up of ANTARES neutrino alerts
Results of the follow-up of ANTARES neutrino alerts Open
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 …
Embedded software of the KM3NeT central logic board Open
The KM3NeT Collaboration is building and operating two deep sea neutrino telescopes at the bottom of the Mediterranean Sea. The telescopes consist of latices of photomultiplier tubes housed in pressure-resistant glass spheres, called digit…
View article: Studying bioluminescence flashes with the <scp>ANTARES</scp> deep‐sea neutrino telescope
Studying bioluminescence flashes with the <span>ANTARES</span> deep‐sea neutrino telescope Open
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…
View article: Searches for neutrinos in the direction of radio-bright blazars with the ANTARES telescope
Searches for neutrinos in the direction of radio-bright blazars with the ANTARES telescope Open
Active galaxies, especially blazars, are among the most promising neutrino source candidates. To date, ANTARES searches for these objects considered GeV-TeV $γ$-ray bright blazars. Here, a statistically complete radio-bright blazar sample …
View article: Review of the online analyses of multi-messenger alerts and electromagnetic transient events with the ANTARES neutrino telescope
Review of the online analyses of multi-messenger alerts and electromagnetic transient events with the ANTARES neutrino telescope Open
By constantly monitoring a very large portion of the sky, neutrino telescopes are well-designed to detect neutrinos emitted by transient astrophysical events. Real-time searches with the ANTARES telescope have been performed to look for ne…
View article: Follow-up of O3 gravitational wave events with neutrinos in ANTARES and KM3NeT telescopes
Follow-up of O3 gravitational wave events with neutrinos in ANTARES and KM3NeT telescopes Open
Astrophysical neutrinos may be produced during the coalescence of compact objects, in particular those involving neutron stars. Such mergers have been identified through gravitational wave detections by the LIGO and Virgo collaborations an…
View article: Hint for a TeV neutrino emission from the Galactic Ridge with the ANTARES telescope
Hint for a TeV neutrino emission from the Galactic Ridge with the ANTARES telescope Open
The central region of our Galaxy (Galactic Ridge) is expected to produce a neutrino flux comparable to the one detected in $\gamma$ rays by Fermi, assuming these result from hadronic collisions of cosmic rays within the interstellar medium…
First observation of the cosmic ray shadow of the Moon and the Sun with KM3NeT/ORCA Open
This article reports the first observation of the Moon and the Sun shadows in the sky distribution of cosmic-ray induced muons measured by the KM3NeT/ORCA detector. The analysed data-taking period spans from February 2020 to November 2021,…