Search engine for discovering works of Art, research articles, and books related to Art and Culture
ShareThis
Javascript must be enabled to continue!

KM3NeT Online Multi-Messenger Results

View through CrossRef
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 energy sensitivity ranging from MeV to PeV. The infrastructure is well suited to detect astrophysical neutrinos thanks to a wide field of view and high duty cycle. In the context of multi-messenger astronomy, KM3NeT aims at quickly reconstructing data to identify neutrino candidates, both to search for coincidences after external triggering and to send alerts. This contribution reports on the online analysis framework status, allowing follow-up of alerts from partner experiments and operational since late 2022.
Title: KM3NeT Online Multi-Messenger Results
Description:
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 energy sensitivity ranging from MeV to PeV.
The infrastructure is well suited to detect astrophysical neutrinos thanks to a wide field of view and high duty cycle.
In the context of multi-messenger astronomy, KM3NeT aims at quickly reconstructing data to identify neutrino candidates, both to search for coincidences after external triggering and to send alerts.
This contribution reports on the online analysis framework status, allowing follow-up of alerts from partner experiments and operational since late 2022.

Related Results

The KM3NeT online processing for multi-messenger alerts
The KM3NeT online processing for multi-messenger alerts
KM3NeT is a deep-sea research infrastructure under construction in the Mediterranean Sea. It consists of two water-Cherenkov neutrino telescopes: ARCA (Italy), designed to identify...
Development of multi-messenger real-time analyses for the KM3NeT neutrino telescope
Development of multi-messenger real-time analyses for the KM3NeT neutrino telescope
Développement d'analyses multi-messager en temps réels pour le télescope à neutrino KM3NeT Parmi les développements récents de l'astronomie multi-messagers, les tél...
KM3NeT sensitivity to low energy astrophysical neutrinos
KM3NeT sensitivity to low energy astrophysical neutrinos
Abstract KM3NeT, a new generation of neutrino telescope, is currently being deployed in the Mediterranean Sea. While its two sites, ORCA and ARCA, were respectively ...
 KM3NeT/ARCA Optical Network 
 KM3NeT/ARCA Optical Network 
   Laboratori Nazionali del Sud dell’INFN owns and manages a deep sea infrastructure situated in Portopalo di Capo Passero where theARCA KM3NeT infrastr...
Multi-messenger observations with the KM3NeT telescope : search for high energy neutrinos coinciding with fast radio transients
Multi-messenger observations with the KM3NeT telescope : search for high energy neutrinos coinciding with fast radio transients
Observations multi-messagers avec le télescope à neutrinos KM3NeT : recherche de neutrinos de haute énergie en coïncidence avec des transitoires radio rapides À l’è...
The KM3NeT project: status and perspectives
The KM3NeT project: status and perspectives
Abstract. KM3NeT is an international consortium involving more than 300 scientists from 10 EU countries. Its main objective is the construction of a multi-km3 high-energy neutrino ...
The KM3NeT project: status and perspectives
The KM3NeT project: status and perspectives
Abstract. KM3NeT is an international consortium involving more than 300 scientists from 10 EU countries. Its main objective is the construction of a multi-km3 high-energy neutrino ...
Core-Collapse Supernova neutrino detection with KM3NeT
Core-Collapse Supernova neutrino detection with KM3NeT
Core Collapse Supernovae (CCSNe) are explosive phenomena that may occur at the end of the life of massive stars, releasing over 99% of the energy through neutrino emission. While t...

Back to Top