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@INPROCEEDINGS{Pelicci:906370,
author = {Pelicci, Luca},
title = {{D}ata analysis strategy used for the detection of {CNO}
solar neutrinos with {B}orexino},
journal = {Journal of physics / Conference Series},
volume = {2156},
number = {1},
issn = {1742-6588},
address = {Bristol},
publisher = {IOP Publ.},
reportid = {FZJ-2022-01399},
pages = {012200},
year = {2021},
abstract = {Borexino is a large liquid scintillator experiment located
at the underground INFN Laboratori Nazionali del Gran Sasso,
in Italy. It was designed and built with the primary goal of
real-time detection of low energy solar neutrinos, and in
more than ten years of data taking it has measured all the
neutrino fluxes produced in the proton-proton chain, i.e.
the main fusion process accounting for $99\%$ of the energy
production in the Sun. Recently, after improvements and
developments in both hardware and software, Borexino has
provided the first observation of solar neutrinos emitted
from the subdominant Carbon-Nitrogen-Oxygen (CNO) fusion
cycle. All the crucial steps of the analysis strategy
adopted to disentangle the signal of CNO neutrinos from
backgrounds present in the detector will be described in
this article.},
month = {Aug},
date = {2021-08-26},
organization = {17th International Conference on
Topics in Astroparticle and Underground
Physics, Valencia (online) (Spain), 26
Aug 2021 - 3 Sep 2021},
cin = {IKP-2},
ddc = {530},
cid = {I:(DE-Juel1)IKP-2-20111104},
pnm = {612 - Cosmic Matter in the Laboratory (POF4-612)},
pid = {G:(DE-HGF)POF4-612},
typ = {PUB:(DE-HGF)16 / PUB:(DE-HGF)8},
doi = {10.1088/1742-6596/2156/1/012200},
url = {https://juser.fz-juelich.de/record/906370},
}