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@INPROCEEDINGS{Bernabei:408355,
      author       = {Bernabei, R. and Belli, P. and Cappella, F. and Caracciolo,
                      V. and Castellano, S. and Cerulli, R. and Dai, C. J. and
                      d’Angelo, A. and d’Angelo, S. and Di Marco, A. and He,
                      H. L. and Incicchitti, A. and Ma, X. H. and Montecchia, F.
                      and Sheng, X. D. and Wang, R. G. and Ye, Z. P.},
      title        = {{R}esults from {DAMA}/{LIBRA} and perspectives},
      address      = {Hamburg},
      publisher    = {Verlag Deutsches Elektronen-Synchrotron},
      reportid     = {PUBDB-2018-02808, DESY-PROC-2013-04},
      isbn         = {978-3-935702-83-6},
      series       = {DESY-PROC},
      pages        = {179-183},
      year         = {2013},
      comment      = {Bernabei, R. "Results from DAMA/LIBRA and perspectives" in
                      Proceedings, 9th Patras Workshop on Axions, WIMPs and WISPs
                      (AXION-WIMP 2013) / Oberlack, Uwe, Sissol, Pierre (eds.),
                      2013 ; AXION-WIMP 2013 : 9th Patras Workshop on Axions,
                      WIMPs and WISPs , 2013-06-23 - 2013-06-28, Mainz},
      booktitle     = {Bernabei, R. "Results from DAMA/LIBRA
                       and perspectives" in Proceedings, 9th
                       Patras Workshop on Axions, WIMPs and
                       WISPs (AXION-WIMP 2013) / Oberlack,
                       Uwe, Sissol, Pierre (eds.), 2013 ;
                       AXION-WIMP 2013 : 9th Patras Workshop
                       on Axions, WIMPs and WISPs , 2013-06-23
                       - 2013-06-28, Mainz},
      abstract     = {The DAMA/LIBRA experiment (about 250 kg of highly radiopure
                      NaI(Tl)) is in operation at the Gran Sasso National
                      Laboratory of the INFN. The main aim of the experiment is to
                      further investigate the Dark Matter (DM) particles in the
                      Galactic halo by exploiting the model independent DM annual
                      modulation signature. At the time of this Workshop, the
                      DAMA/LIBRA experiment and the former DAMA/NaI one (the first
                      generation experiment having an exposed mass of about 100
                      kg) have released results corresponding to a total exposure
                      of 1.17 ton × yr over 13 annual cycles; they have provided
                      a model independent evidence of the presence of DM particles
                      in the galactic halo at 8.9 $σ$ C.L.. The results of a
                      further annual cycle, concluding the DAMA/LIBRA–phase1,
                      have been released after this Workshop and are not included
                      here. After the upgrade at fall 2010 when all the PMTs have
                      been replaced with new ones having higher quantum
                      efficiency, the feasibility to decrease the software energy
                      threshold has been demonstrated and the setup is running in
                      this new configuration, named DAMA/LIBRA–phase2.},
      month         = {Jun},
      date          = {2013-06-24},
      organization  = {9th Patras Workshop on Axions, WIMPs
                       and WISPs, Mainz (Germany), 24 Jun 2013
                       - 28 Jun 2013},
      keywords     = {Hypothetisches Teilchen (gnd)},
      cin          = {L},
      cid          = {I:(DE-H253)L-20120731},
      pnm          = {899 - ohne Topic (POF3-899)},
      pid          = {G:(DE-HGF)POF3-899},
      experiment   = {EXP:(DE-MLZ)NOSPEC-20140101},
      typ          = {PUB:(DE-HGF)29 / PUB:(DE-HGF)8 / PUB:(DE-HGF)7},
      doi          = {10.3204/DESY-PROC-2013-04/cerulli_riccardo},
      url          = {https://bib-pubdb1.desy.de/record/408355},
}