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| Hauptseite > Publikationsdatenbank > Data analysis strategy used for the detection of CNO solar neutrinos with Borexino > print |
| Hauptseite > Publikationsdatenbank > Data analysis strategy used for the detection of CNO solar neutrinos with Borexino > print |
| 001 | 906370 | ||
| 005 | 20251027132718.0 | ||
| 024 | 7 | _ | |a 10.1088/1742-6596/2156/1/012200 |2 doi |
| 024 | 7 | _ | |a 1742-6588 |2 ISSN |
| 024 | 7 | _ | |a 1742-6596 |2 ISSN |
| 024 | 7 | _ | |a 2128/30762 |2 Handle |
| 024 | 7 | _ | |a WOS:001432940800200 |2 WOS |
| 037 | _ | _ | |a FZJ-2022-01399 |
| 082 | _ | _ | |a 530 |
| 100 | 1 | _ | |a Pelicci, Luca |0 P:(DE-Juel1)186943 |b 0 |e Corresponding author |
| 111 | 2 | _ | |a 17th International Conference on Topics in Astroparticle and Underground Physics |g TAUP 2021 |c Valencia (online) |d 2021-08-26 - 2021-09-03 |w Spain |
| 245 | _ | _ | |a Data analysis strategy used for the detection of CNO solar neutrinos with Borexino |
| 260 | _ | _ | |a Bristol |c 2021 |b IOP Publ. |
| 264 | _ | 1 | |3 print |2 Crossref |b IOP Publishing |c 2021-12-01 |
| 264 | _ | 1 | |3 print |2 Crossref |b IOP Publishing |c 2021-12-01 |
| 300 | _ | _ | |a 5 |
| 336 | 7 | _ | |a CONFERENCE_PAPER |2 ORCID |
| 336 | 7 | _ | |a Conference Paper |0 33 |2 EndNote |
| 336 | 7 | _ | |a Journal Article |0 PUB:(DE-HGF)16 |2 PUB:(DE-HGF) |m journal |
| 336 | 7 | _ | |a INPROCEEDINGS |2 BibTeX |
| 336 | 7 | _ | |a conferenceObject |2 DRIVER |
| 336 | 7 | _ | |a Output Types/Conference Paper |2 DataCite |
| 336 | 7 | _ | |a Contribution to a conference proceedings |b contrib |m contrib |0 PUB:(DE-HGF)8 |s 1645535054_26051 |2 PUB:(DE-HGF) |
| 520 | _ | _ | |a 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. |
| 536 | _ | _ | |a 612 - Cosmic Matter in the Laboratory (POF4-612) |0 G:(DE-HGF)POF4-612 |c POF4-612 |f POF IV |x 0 |
| 542 | _ | _ | |i 2021-12-01 |2 Crossref |u http://creativecommons.org/licenses/by/3.0/ |
| 542 | _ | _ | |i 2021-12-01 |2 Crossref |u https://iopscience.iop.org/info/page/text-and-data-mining |
| 588 | _ | _ | |a Dataset connected to CrossRef, Journals: juser.fz-juelich.de |
| 773 | 1 | 8 | |a 10.1088/1742-6596/2156/1/012200 |b IOP Publishing |d 2021-12-01 |n 1 |p 012200 |3 journal-article |2 Crossref |t Journal of Physics: Conference Series |v 2156 |y 2021 |x 1742-6588 |
| 773 | _ | _ | |a 10.1088/1742-6596/2156/1/012200 |g Vol. 2156, no. 1, p. 012200 - |0 PERI:(DE-600)2166409-2 |n 1 |p 012200 |t Journal of physics / Conference Series |v 2156 |y 2021 |x 1742-6588 |
| 856 | 4 | _ | |u https://juser.fz-juelich.de/record/906370/files/Data%20analysis%20strategy%20used%20for%20the%20detection%20of%20CNO%20solar%20neutrinos%20with%20Borexino.pdf |y OpenAccess |
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| 910 | 1 | _ | |a Forschungszentrum Jülich |0 I:(DE-588b)5008462-8 |k FZJ |b 0 |6 P:(DE-Juel1)186943 |
| 913 | 1 | _ | |a DE-HGF |b Forschungsbereich Materie |l Matter and the Universe |1 G:(DE-HGF)POF4-610 |0 G:(DE-HGF)POF4-612 |3 G:(DE-HGF)POF4 |2 G:(DE-HGF)POF4-600 |4 G:(DE-HGF)POF |v Cosmic Matter in the Laboratory |x 0 |
| 914 | 1 | _ | |y 2022 |
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| 999 | C | 5 | |1 Agostini |2 Crossref |o Agostini |
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| 999 | C | 5 | |1 Ludhova |y 2021 |2 Crossref |o Ludhova 2021 |
| 999 | C | 5 | |1 Penek |y 2021 |2 Crossref |o Penek 2021 |
| 999 | C | 5 | |1 Porcelli |y 2021 |2 Crossref |o Porcelli 2021 |
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