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| Hauptseite > Publikationsdatenbank > Data selection strategy for solar neutrino analysis with Borexino > print |
| Hauptseite > Publikationsdatenbank > Data selection strategy for solar neutrino analysis with Borexino > print |
| 001 | 890237 | ||
| 005 | 20250813203210.0 | ||
| 024 | 7 | _ | |a 10.1088/1742-6596/1342/1/012110 |2 doi |
| 024 | 7 | _ | |a Caprioli:2020dal |2 INSPIRETeX |
| 024 | 7 | _ | |a inspire:1776468 |2 inspire |
| 024 | 7 | _ | |a 1742-6588 |2 ISSN |
| 024 | 7 | _ | |a 1742-6596 |2 ISSN |
| 024 | 7 | _ | |a 2128/27069 |2 Handle |
| 024 | 7 | _ | |a WOS:001432953400110 |2 WOS |
| 037 | _ | _ | |a FZJ-2021-00824 |
| 082 | _ | _ | |a 530 |
| 100 | 1 | _ | |a Caprioli, S. |0 S.Caprioli.1 |b 0 |
| 111 | 2 | _ | |a 15th International Conference on Topics in Astroparticle and Underground Physics |g TAUP 2017 |c Sudbury |d 2017-07-24 - 2017-07-28 |w Canada |
| 245 | _ | _ | |a Data selection strategy for solar neutrino analysis with Borexino |
| 260 | _ | _ | |a Bristol |c 2020 |b IOP Publ.87703 |
| 264 | _ | 1 | |3 print |2 Crossref |b IOP Publishing |c 2020-01-01 |
| 264 | _ | 1 | |3 print |2 Crossref |b IOP Publishing |c 2020-01-01 |
| 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 1754992034_31401 |2 PUB:(DE-HGF) |
| 520 | _ | _ | |a The Borexino collaboration has recently released the first simultaneous measurement of the interaction rates of pp, 7Be and pep solar neutrinos. This result was made possible by the unprecedented low background of the scintillator during Phase-II, together with new data analysis techniques. We present the data selection strategy of the Borexino solar neutrino analysis: we describe how we select the neutrino-like scintillation events according to event-based cuts which eliminate most of the external and cosmogenic backgrounds. We describe also how the spatial distribution of events and a β+/β− pulse shape discrimination variable are used in a multivariate fit approach to additionally constrain the residual cosmogenic 11C and external backgrounds. |
| 536 | _ | _ | |a 612 - Cosmic Matter in the Laboratory (POF3-612) |0 G:(DE-HGF)POF3-612 |c POF3-612 |f POF III |x 0 |
| 542 | _ | _ | |i 2020-01-01 |2 Crossref |u http://creativecommons.org/licenses/by/3.0/ |
| 542 | _ | _ | |i 2020-01-01 |2 Crossref |u https://iopscience.iop.org/info/page/text-and-data-mining |
| 588 | _ | _ | |a Dataset connected to CrossRef, INSPIRE |
| 650 | _ | 7 | |a neutrino: solar |2 INSPIRE |
| 650 | _ | 7 | |a background: low |2 INSPIRE |
| 650 | _ | 7 | |a Borexino |2 INSPIRE |
| 650 | _ | 7 | |a scintillation counter |2 INSPIRE |
| 650 | _ | 7 | |a data analysis method |2 INSPIRE |
| 650 | _ | 7 | |a shape analysis |2 INSPIRE |
| 650 | _ | 7 | |a carbon: nuclide |2 INSPIRE |
| 700 | 1 | _ | |a Ghiano, C. |0 C.Ghiano.1 |b 1 |
| 700 | 1 | _ | |a Re, A. |0 A.Re.1 |b 2 |
| 700 | 1 | _ | |a Redchuk, Mariia |0 P:(DE-Juel1)171322 |b 3 |e Corresponding author |
| 700 | 1 | _ | |a BOREXINO Collaboration |0 P:(DE-HGF)0 |b 4 |
| 773 | 1 | 8 | |a 10.1088/1742-6596/1342/1/012110 |b IOP Publishing |d 2020-01-01 |n 1 |p 012110 |3 journal-article |2 Crossref |t Journal of Physics: Conference Series |v 1342 |y 2020 |x 1742-6588 |
| 773 | _ | _ | |a 10.1088/1742-6596/1342/1/012110 |g Vol. 1342, no. 1, p. 012110 - |0 PERI:(DE-600)2166409-2 |n 1 |p 012110 |t Journal of physics / Conference Series |v 1342 |y 2020 |x 1742-6588 |
| 856 | 4 | _ | |u https://juser.fz-juelich.de/record/890237/files/Caprioli_2020_J._Phys.%20_Conf._Ser._1342_012110.pdf |y OpenAccess |
| 909 | C | O | |o oai:juser.fz-juelich.de:890237 |p openaire |p open_access |p VDB |p driver |p dnbdelivery |
| 910 | 1 | _ | |a Forschungszentrum Jülich |0 I:(DE-588b)5008462-8 |k FZJ |b 3 |6 P:(DE-Juel1)171322 |
| 913 | 1 | _ | |a DE-HGF |b Forschungsbereich Materie |l Materie und Universum |1 G:(DE-HGF)POF3-610 |0 G:(DE-HGF)POF3-612 |3 G:(DE-HGF)POF3 |2 G:(DE-HGF)POF3-600 |4 G:(DE-HGF)POF |v Cosmic Matter in the Laboratory |x 0 |
| 914 | 1 | _ | |y 2020 |
| 915 | _ | _ | |a Creative Commons Attribution CC BY 3.0 |0 LIC:(DE-HGF)CCBY3 |2 HGFVOC |
| 915 | _ | _ | |a DBCoverage |0 StatID:(DE-HGF)0200 |2 StatID |b SCOPUS |
| 915 | _ | _ | |a DBCoverage |0 StatID:(DE-HGF)0300 |2 StatID |b Medline |
| 915 | _ | _ | |a OpenAccess |0 StatID:(DE-HGF)0510 |2 StatID |
| 920 | 1 | _ | |0 I:(DE-Juel1)IKP-2-20111104 |k IKP-2 |l Experimentelle Hadrondynamik |x 0 |
| 980 | _ | _ | |a contrib |
| 980 | _ | _ | |a VDB |
| 980 | _ | _ | |a journal |
| 980 | _ | _ | |a I:(DE-Juel1)IKP-2-20111104 |
| 980 | _ | _ | |a UNRESTRICTED |
| 980 | 1 | _ | |a FullTexts |
| 999 | C | 5 | |a 10.1016/j.nima.2008.11.076 |9 -- missing cx lookup -- |1 Alimonti |p 568 - |2 Crossref |t Nuclear Instruments and Methods A |v 600 |y 2009 |
| 999 | C | 5 | |1 Agostini |y 2017 |2 Crossref |o Agostini 2017 |
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| 999 | C | 5 | |a 10.1088/1748-0221/6/05/P05005 |9 -- missing cx lookup -- |1 Bellini |p 05005 - |2 Crossref |t Journal of instrumentation |v 6 |y 2011 |
| 999 | C | 5 | |a 10.1103/PhysRevD.89.112007 |1 Bellini |9 -- missing cx lookup -- |2 Crossref |t Physical Review D |v 89 |y 2014 |
| 999 | C | 5 | |a 10.1103/PhysRevC.71.055805 |1 Galbiati |9 -- missing cx lookup -- |2 Crossref |t Physical Review C |v 71 |y 2005 |
| 999 | C | 5 | |a 10.1103/PhysRevC.83.015504 |1 Franco |9 -- missing cx lookup -- |2 Crossref |t Physical Review C |v 83 |y 2011 |
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