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@INPROCEEDINGS{Gerbier:395476,
      author       = {Gerbier, G.},
      collaboration = {{NEWS Collaboration}},
      title        = {{S}earch for low-mass {WIMP}s with {S}pherical {D}etectors
                      : {NEWS}-{LSM} and {NEWS}-{SNO}},
      address      = {Hamburg},
      publisher    = {Verlag Deutsches Elektronen-Synchrotron},
      reportid     = {PUBDB-2017-12141, DESY-PROC-2016-03},
      isbn         = {978-3-945931-06-6},
      series       = {DESY-PROC},
      pages        = {43-47},
      year         = {2017},
      comment      = {Gerbier, G. "Search for low-mass WIMPs with Spherical
                      Detectors : NEWS-LSM and NEWS-SNO" in 12th "Patras" Workshop
                      on Axions, WIMPs and WISPs, PATRAS 2016 / Kim, Younglm,
                      Lindner, Axel, Semertzidis, Yannis K. (eds.), Verlag
                      Deutsches Elektronen-Synchrotron : 2017 ; PATRAS 2016 : 12th
                      "Patras" Workshop on Axions, WIMPs and WISPs, 2016-06-20 -
                      2016-06-24, Jeju Island},
      booktitle     = {Gerbier, G. "Search for low-mass WIMPs
                       with Spherical Detectors : NEWS-LSM and
                       NEWS-SNO" in 12th "Patras" Workshop on
                       Axions, WIMPs and WISPs, PATRAS 2016 /
                       Kim, Younglm, Lindner, Axel,
                       Semertzidis, Yannis K. (eds.), Verlag
                       Deutsches Elektronen-Synchrotron : 2017
                       ; PATRAS 2016 : 12th "Patras" Workshop
                       on Axions, WIMPs and WISPs, 2016-06-20
                       - 2016-06-24, Jeju Island},
      abstract     = {The technique of spherical gaseous detectors has been used
                      for the first time in the Laboratoire Souterrain de Modane
                      to search for WIMP signal. Some details on the used 60 cm
                      diameter detector, operating conditions and preliminary
                      results are given. Thanks to a low energy threshold of 150
                      eV and the use of Neon target, anticipated sensitivity has
                      been calculated for WIMP masses as low as 0.7 GeV with a
                      Boosted Decision Tree method. Final analysis of this data
                      set is under way. A larger size detector of 140 cm diameter
                      to be installed in SNOLAB is currently under design and
                      planned to be operated end 2017.},
      month         = {Jun},
      date          = {2016-06-20},
      organization  = {12th Patras Workshop on Axions, WIMPs
                       and WISPs, Jeju Island (South Korea),
                       20 Jun 2016 - 24 Jun 2016},
      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-2009-03/Gerbier_Gilles},
      url          = {https://bib-pubdb1.desy.de/record/395476},
}