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@INPROCEEDINGS{Priel:315499,
      author       = {Priel, Nadav},
      collaboration = {{XENON Collaboration}},
      title        = {{XENON}100 {R}esults on {WIMP} and non-{WIMP} {S}earches},
      address      = {Hamburg},
      publisher    = {Verlag Deutsches Elektronen-Synchrotron},
      reportid     = {PUBDB-2016-05906},
      isbn         = {978-3-935702-59-1},
      series       = {DESY-PROC},
      pages        = {37-40},
      year         = {2014},
      comment      = {Priel, Nadav "XENON100 Results on WIMP and non-WIMP
                      Searches" in Proceedings, 10th Patras Workshop on Axions,
                      WIMPs and WISPs (AXION-WIMP 2014) / Tsesmelis, Emmanuel,
                      Maroudas, Marios (eds.), Verlag Deutsches
                      Elektronen-Synchrotron : 2014 ; AXION-WIMP 2014 : 10th
                      Patras Workshop on Axions, WIMPs and WISPs, 2014-06-29 -
                      2014-07-04, Geneva},
      booktitle     = {Priel, Nadav "XENON100 Results on WIMP
                       and non-WIMP Searches" in Proceedings,
                       10th Patras Workshop on Axions, WIMPs
                       and WISPs (AXION-WIMP 2014) /
                       Tsesmelis, Emmanuel, Maroudas, Marios
                       (eds.), Verlag Deutsches
                       Elektronen-Synchrotron : 2014 ;
                       AXION-WIMP 2014 : 10th Patras Workshop
                       on Axions, WIMPs and WISPs, 2014-06-29
                       - 2014-07-04, Geneva},
      abstract     = {XENON100 is the second phase of the XENON direct Dark
                      Matter search program. It consists of an ultra-low
                      background double phase (liquid-gas) xenon filled time
                      projection chamber, and is installed at the Laboratori
                      Nazionali del Gran Sasso. The results from the 224.6 live
                      days of data taken between March 2011 and April 2012 are
                      reported. The experiment sets one of the most stringent
                      limits on the WIMP-nucleon spin-independent cross section,
                      and the most stringent limit on the spin-dependent
                      WIMP-neutron interaction. With the same dataset, XENON100
                      sets the best limit to date on the axion coupling to
                      electrons for solar and for galactic axions.},
      month         = {Jun},
      date          = {2014-06-29},
      organization  = {10th Patras Workshop on Axions, WIMPs
                       and WISPs, Geneva (Switzerland), 29 Jun
                       2014 - 4 Jul 2014},
      typ          = {PUB:(DE-HGF)8 / PUB:(DE-HGF)7},
      doi          = {10.3204/DESY-PROC-2014-03/priel_nadav},
      url          = {https://bib-pubdb1.desy.de/record/315499},
}