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@ARTICLE{Agostini:872788,
      author       = {Agostini, M. and Altenmüller, K. and Appel, S. and
                      Atroshchenko, V. and Bagdasarian, Z. and Basilico, D. and
                      Bellini, G. and Benziger, J. and Bonfini, G. and Bravo, D.
                      and Caccianiga, B. and Calaprice, F. and Caminata, A. and
                      Cappelli, L. and Caprioli, S. and Carlini, M. and
                      Cavalcante, P. and Cavanna, F. and Chepurnov, A. and Choi,
                      K. and Collica, L. and D’Angelo, D. and Davini, S. and
                      Derbin, A. and Ding, X. F. and Di Ludovico, A. and Di Noto,
                      L. and Drachnev, I. and Fomenko, K. and Formozov, A. and
                      Franco, D. and Gabriele, F. and Galbiati, C. and Gschwender,
                      M. and Ghiano, C. and Giammarchi, M. and Goretti, A. and
                      Gromov, M. and Guffanti, D. and Houdy, T. and Hungerford, E.
                      and Ianni, Aldo and Ianni, Andrea and Jany, A. and Jeschke,
                      D. and Kumaran, S. and Kobychev, V. and Korga, G. and
                      Lachenmaier, T. and Laubenstein, M. and Litvinovich, E. and
                      Lombardi, P. and Ludhova, L. and Lukyanchenko, G. and
                      Lukyanchenko, L. and Machulin, I. and Manuzio, G. and
                      Marcocci, S. and Maricic, J. and Martyn, J. and Meroni, E.
                      and Meyer, M. and Miramonti, L. and Misiaszek, M. and
                      Muratova, V. and Neumair, B. and Nieslony, M. and Orekhov,
                      V. and Oberauer, L. and Ortica, F. and Pallavicini, M. and
                      Papp, L. and Penek, Ömer and Pietrofaccia, L. and
                      Pilipenko, N. and Pocar, A. and Porcelli, A. and Raikov, G.
                      and Ranucci, G. and Razeto, A. and Re, A. and Redchuk,
                      Mariia and Romani, A. and Rossi, N. and Rottenanger, S. and
                      Schönert, S. and Semenov, D. and Skorokhvatov, M. and
                      Smirnov, O. and Sotnikov, A. and Stokes, L. F. F. and
                      Suvorov, Y. and Tartaglia, R. and Testera, G. and Unzhakov,
                      E. and Thurn, J. and Villante, F. and Vishneva, A. and
                      Vogelaar, R. B. and von Feilitzsch, F. and Weinz, S. and
                      Wojcik, M. and Wurm, M. and Zaimidoroga, O. and Zavatarelli,
                      S. and Zuber, K. and Zuzel, G.},
      title        = {{S}imultaneous precision spectroscopy of p p , {B}e 7 , and
                      p e p solar neutrinos with {B}orexino {P}hase-{II}},
      journal      = {Physical review / D},
      volume       = {100},
      number       = {8},
      issn         = {2470-0010},
      address      = {Melville, NY},
      publisher    = {Inst.812068},
      reportid     = {FZJ-2020-00260},
      pages        = {082004},
      year         = {2019},
      abstract     = {We present the simultaneous measurement of the interaction
                      rates Rpp, RBe, Rpep of pp, 7Be, and pep solar neutrinos
                      performed with a global fit to the Borexino data in an
                      extended energy range (0.19–2.93) MeV with particular
                      attention to details of the analysis methods. This result
                      was obtained by analyzing 1291.51 days of Borexino Phase-II
                      data, collected after an extensive scintillator purification
                      campaign. Using counts per day (cpd)/100 ton as unit, we
                      find Rpp=134±10(stat)+6−10(sys),
                      RBe=48.3±1.1(stat)+0.4−0.7(sys); and
                      RHZpep=2.43±0.36(stat)+0.15−0.22(sys) assuming the
                      interaction rate RCNO of CNO-cycle (Carbon, Nitrogen,
                      Oxigen) solar neutrinos according to the prediction of the
                      high metallicity standard solar model, and
                      RLZpep=2.65±0.36(stat)+0.15−0.24(sys) according to that
                      of the low metallicity model. An upper limit
                      RCNO<8.1 cpd/100 ton $(95\%$ C.L.) is obtained by
                      setting in the fit a constraint on the ratio Rpp/Rpep
                      (47.7±0.8 cpd/100 ton or 47.5±0.8cpd/100 ton according
                      to the high or low metallicity hypothesis).},
      cin          = {IKP-2 / JARA-HPC},
      ddc          = {530},
      cid          = {I:(DE-Juel1)IKP-2-20111104 / $I:(DE-82)080012_20140620$},
      pnm          = {612 - Cosmic Matter in the Laboratory (POF3-612) / Solar
                      and Geo-neutrino Analysis with Borexino $(jikp20_20190501)$},
      pid          = {G:(DE-HGF)POF3-612 / $G:(DE-Juel1)jikp20_20190501$},
      typ          = {PUB:(DE-HGF)16},
      UT           = {WOS:000492976700001},
      doi          = {10.1103/PhysRevD.100.082004},
      url          = {https://juser.fz-juelich.de/record/872788},
}