TY - JOUR
T1 - Implementation and first results of the KM3NeT real-time core-collapse supernova neutrino search
AU - KM3NeT Collaboration
AU - Aiello, S.
AU - Albert, A.
AU - Alshamsi, M.
AU - Alves Garre, S.
AU - Aly, Z.
AU - Ambrosone, A.
AU - Ameli, F.
AU - Andre, M.
AU - Androulakis, G.
AU - Anghinolfi, M.
AU - Anguita, M.
AU - Ardid, M.
AU - Ardid, S.
AU - Aublin, J.
AU - Bagatelas, C.
AU - Baret, B.
AU - Pree, S. Basegmez du
AU - Bendahman, M.
AU - Benfenati, F.
AU - Berbee, E.
AU - Berg, A. M.van den
AU - Bertin, V.
AU - Biagi, S.
AU - Boettcher, M.
AU - Cabo, M. Bou
AU - Boumaaza, J.
AU - Bouta, M.
AU - Bouwhuis, M.
AU - Bozza, C.
AU - Brânzaş, H.
AU - Bruijn, R.
AU - Brunner, J.
AU - Bruno, R.
AU - Buis, E.
AU - Buompane, R.
AU - Busto, J.
AU - Caiffi, B.
AU - Calvo, D.
AU - Campion, S.
AU - Capone, A.
AU - Carretero, V.
AU - Castaldi, P.
AU - Celli, S.
AU - Chabab, M.
AU - Chau, N.
AU - Chen, A.
AU - Cherubini, S.
AU - Chiarella, V.
AU - Chiarusi, T.
AU - Razzaque, S.
N1 - Publisher Copyright:
© 2022, The Author(s).
PY - 2022/4
Y1 - 2022/4
N2 - The KM3NeT research infrastructure is unconstruction in the Mediterranean Sea. KM3NeT will study atmospheric and astrophysical neutrinos with two multi-purpose neutrino detectors, ARCA and ORCA, primarily aimed at GeV–PeV neutrinos. Thanks to the multi-photomultiplier tube design of the digital optical modules, KM3NeT is capable of detecting the neutrino burst from a Galactic or near-Galactic core-collapse supernova. This potential is already exploitable with the first detection units deployed in the sea. This paper describes the real-time implementation of the supernova neutrino search, operating on the two KM3NeT detectors since the first months of 2019. A quasi-online astronomy analysis is introduced to study the time profile of the detected neutrinos for especially significant events. The mechanism of generation and distribution of alerts, as well as the integration into the SNEWS and SNEWS 2.0 global alert systems, are described. The approach for the follow-up of external alerts with a search for a neutrino excess in the archival data is defined. Finally, an overview of the current detector capabilities and a report after the first two years of operation are given.
AB - The KM3NeT research infrastructure is unconstruction in the Mediterranean Sea. KM3NeT will study atmospheric and astrophysical neutrinos with two multi-purpose neutrino detectors, ARCA and ORCA, primarily aimed at GeV–PeV neutrinos. Thanks to the multi-photomultiplier tube design of the digital optical modules, KM3NeT is capable of detecting the neutrino burst from a Galactic or near-Galactic core-collapse supernova. This potential is already exploitable with the first detection units deployed in the sea. This paper describes the real-time implementation of the supernova neutrino search, operating on the two KM3NeT detectors since the first months of 2019. A quasi-online astronomy analysis is introduced to study the time profile of the detected neutrinos for especially significant events. The mechanism of generation and distribution of alerts, as well as the integration into the SNEWS and SNEWS 2.0 global alert systems, are described. The approach for the follow-up of external alerts with a search for a neutrino excess in the archival data is defined. Finally, an overview of the current detector capabilities and a report after the first two years of operation are given.
UR - http://www.scopus.com/inward/record.url?scp=85130983084&partnerID=8YFLogxK
U2 - 10.1140/epjc/s10052-022-10137-y
DO - 10.1140/epjc/s10052-022-10137-y
M3 - Article
AN - SCOPUS:85130983084
SN - 1434-6044
VL - 82
JO - European Physical Journal C
JF - European Physical Journal C
IS - 4
M1 - 317
ER -