Offline performance studies and first real-time results on Core-Collapse Supernova neutrino searches with the KM3NeT neutrino detectors

• Published in: Proceedings of 36th International Cosmic Ray Conference — PoS(ICRC2019)
• Main Authors: Colomer Molla, Marta, Coleiro, Alexis, Dornic, Damien, Kulikovskiy, Vladimir, Lincetto, Massimiliano
• Other Authors: AstroParticule et Cosmologie (APC (UMR_7164)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université de Paris (UP), Centre de Physique des Particules de Marseille (CPPM), Aix Marseille Université (AMU)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), KM3NeT
• Format: Conference Object
• Language: English
• Published: HAL CCSD 2019
• Subjects: KM3NeT; numerical calculations; neutrino; supernova; [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]; Orca
• Online Access: https://hal.archives-ouvertes.fr/hal-02507604; https://hal.archives-ouvertes.fr/hal-02507604/document; https://hal.archives-ouvertes.fr/hal-02507604/file/PoS-ICRC2019-857.pdf; https://doi.org/10.22323/1.358.0857

International audience The KM3NeT collaboration has started the construction of the ARCA and ORCA neutrino telescopes in the Mediterranean Sea. With the most recent data from the deployed lines, the detection technique for Core-Collapse Supernova neutrino bursts has been refined. The real time trigger was implemented and verified to be robust and effective. %The first results are presented here.The study of the resolution to fast-time variation in the neutrino light-curve is also presented exploiting two different methods, with estimates from real data and state-of-the-art Core-Collapse Supernova simulations.Finally, the mean energy of the incoming neutrinos can be estimated through the correlation between the number of photo-multipliers detecting light in coincidence and the mean energy of the incoming neutrinos.