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000890237 0247_ $$2ISSN$$a1742-6588
000890237 0247_ $$2ISSN$$a1742-6596
000890237 0247_ $$2Handle$$a2128/27069
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000890237 1001_ $$0S.Caprioli.1$$aCaprioli, S.$$b0
000890237 1112_ $$a15th International Conference on Topics in Astroparticle and Underground Physics$$cSudbury$$d2017-07-24 - 2017-07-28$$gTAUP 2017$$wCanada
000890237 245__ $$aData selection strategy for solar neutrino analysis with Borexino
000890237 260__ $$aBristol$$bIOP Publ.87703$$c2020
000890237 264_1 $$2Crossref$$3print$$bIOP Publishing$$c2020-01-01
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000890237 3367_ $$0PUB:(DE-HGF)8$$2PUB:(DE-HGF)$$aContribution to a conference proceedings$$bcontrib$$mcontrib$$s1754992034_31401
000890237 520__ $$aThe Borexino collaboration has recently released the first simultaneous measurement of the interaction rates of pp, 7Be and pep solar neutrinos. This result was made possible by the unprecedented low background of the scintillator during Phase-II, together with new data analysis techniques. We present the data selection strategy of the Borexino solar neutrino analysis: we describe how we select the neutrino-like scintillation events according to event-based cuts which eliminate most of the external and cosmogenic backgrounds. We describe also how the spatial distribution of events and a β+/β− pulse shape discrimination variable are used in a multivariate fit approach to additionally constrain the residual cosmogenic 11C and external backgrounds.
000890237 536__ $$0G:(DE-HGF)POF3-612$$a612 - Cosmic Matter in the Laboratory (POF3-612)$$cPOF3-612$$fPOF III$$x0
000890237 542__ $$2Crossref$$i2020-01-01$$uhttp://creativecommons.org/licenses/by/3.0/
000890237 542__ $$2Crossref$$i2020-01-01$$uhttps://iopscience.iop.org/info/page/text-and-data-mining
000890237 588__ $$aDataset connected to CrossRef, INSPIRE
000890237 650_7 $$2INSPIRE$$aneutrino: solar
000890237 650_7 $$2INSPIRE$$abackground: low
000890237 650_7 $$2INSPIRE$$aBorexino
000890237 650_7 $$2INSPIRE$$ascintillation counter
000890237 650_7 $$2INSPIRE$$adata analysis method
000890237 650_7 $$2INSPIRE$$ashape analysis
000890237 650_7 $$2INSPIRE$$acarbon: nuclide
000890237 7001_ $$0C.Ghiano.1$$aGhiano, C.$$b1
000890237 7001_ $$0A.Re.1$$aRe, A.$$b2
000890237 7001_ $$0P:(DE-Juel1)171322$$aRedchuk, Mariia$$b3$$eCorresponding author
000890237 7001_ $$0P:(DE-HGF)0$$aBOREXINO Collaboration$$b4
000890237 77318 $$2Crossref$$3journal-article$$a10.1088/1742-6596/1342/1/012110$$bIOP Publishing$$d2020-01-01$$n1$$p012110$$tJournal of Physics: Conference Series$$v1342$$x1742-6588$$y2020
000890237 773__ $$0PERI:(DE-600)2166409-2$$a10.1088/1742-6596/1342/1/012110$$gVol. 1342, no. 1, p. 012110 -$$n1$$p012110$$tJournal of physics / Conference Series$$v1342$$x1742-6588$$y2020
000890237 8564_ $$uhttps://juser.fz-juelich.de/record/890237/files/Caprioli_2020_J._Phys.%20_Conf._Ser._1342_012110.pdf$$yOpenAccess
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000890237 9141_ $$y2020
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