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@INPROCEEDINGS{Lozza:315080,
      author       = {Lozza, Valentina},
      collaboration = {SNO+{ Collaboration}},
      title        = {{T}he {SNO}+ experiment: current status and future
                      prospects},
      address      = {Hamburg},
      publisher    = {Verlag Deutsches Elektronen-Synchrotron},
      reportid     = {PUBDB-2016-05615},
      isbn         = {978-3-945931-08-0},
      series       = {DESY-PROC},
      pages        = {87-94},
      year         = {2016},
      comment      = {Lozza, Valentina "The SNO+ experiment: current status and
                      future prospects" in Proceedings, Magellan Workshop:
                      Connecting Neutrino Physics and Astronomy / Dahmke, Stefan
                      K.G., Meyer, Mikko, Vanhoefer, Laura (eds.), Deutsches
                      Elektronen-Synchrotron, DESY : 2016 ; Magellan Workshop,
                      2016-03-17 - 2016-03-18, Hamburg},
      booktitle     = {Lozza, Valentina "The SNO+ experiment:
                       current status and future prospects" in
                       Proceedings, Magellan Workshop:
                       Connecting Neutrino Physics and
                       Astronomy / Dahmke, Stefan K.G., Meyer,
                       Mikko, Vanhoefer, Laura (eds.),
                       Deutsches Elektronen-Synchrotron, DESY
                       : 2016 ; Magellan Workshop, 2016-03-17
                       - 2016-03-18, Hamburg},
      abstract     = {SNO+ is a multi-purpose neutrino experiment whose main
                      physics goal is the search for the neutrinoless double-beta
                      ($0\nu\beta\beta$) decay of $^{130}$Te. With an initial
                      loading of 0.5\\% (by weight) of natural tellurium SNO+ is
                      expected to reach a sensitivity on the $0\nu\beta\beta$
                      lifetime of the order of 10$^{26}$ years at 90\\% C.L. in a
                      5-year run. Along with the $0\nu\beta\beta$ decay search,
                      SNO+ has the capability to measure the low energy solar
                      neutrinos, like pep and CNO neutrinos. It has also an
                      extraordinary opportunity to do the first measurement of the
                      supernova $\nu_x$ energy spectrum.},
      month         = {Mar},
      date          = {2016-03-17},
      organization  = {Magellan Workshop, Hamburg (Germany),
                       17 Mar 2016 - 18 Mar 2016},
      typ          = {PUB:(DE-HGF)8 / PUB:(DE-HGF)7},
      doi          = {10.3204/DESY-PROC-2016-05/5},
      url          = {https://bib-pubdb1.desy.de/record/315080},
}