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@INPROCEEDINGS{Dafni:402226,
      author       = {Dafni, Theopisti and Aznar, F. and Castel, J. F. and
                      Cebrián, S. and Coarasa, I. and Galán, J. and Garza, J. G.
                      and Iguaz, F. J. and Irastorza, I. G. and Luzón, G. and
                      Mirallas, H. and Ortiz de Solórzano, A. and Ruiz-Chóliz,
                      E. and Villar, J. A.},
      title        = {{L}ooking for {L}ow-{M}ass {WIMP}s with {TREX}-{DM}},
      address      = {Hamburg},
      publisher    = {Verlag Deutsches Elektronen-Synchrotron},
      reportid     = {PUBDB-2018-01755, DESY-PROC-2017-02},
      isbn         = {978-3-945931-17-2},
      series       = {DESY-PROC},
      pages        = {122-125},
      year         = {2018},
      comment      = {Dafni, Theopisti "Looking for Low-Mass WIMPs with TREX-DM"
                      in Proceedings of the 13th "Patras" Workshop on Axions,
                      WIMPs and WISPs, PATRAS 2017 / Maroudas, Marios (eds.),
                      Verlag Deutsches Elektronen-Synchrotron : 2018 ; Patras 2017
                      : 13th Patras Workshop on Axions, WIMPs and WISPs,
                      2017-05-15 - 2017-05-19, Thessaloniki},
      booktitle     = {Dafni, Theopisti "Looking for Low-Mass
                       WIMPs with TREX-DM" in Proceedings of
                       the 13th "Patras" Workshop on Axions,
                       WIMPs and WISPs, PATRAS 2017 /
                       Maroudas, Marios (eds.), Verlag
                       Deutsches Elektronen-Synchrotron : 2018
                       ; Patras 2017 : 13th Patras Workshop on
                       Axions, WIMPs and WISPs, 2017-05-15 -
                       2017-05-19, Thessaloniki},
      abstract     = {TREX-DM is a low-mass WIMP detector: a gas time projection
                      chamber (TPC) equipped with novel micromesh gas structures
                      (Micromegas) readout planes. In the fiducial volume of
                      $\sim$20 litres and a pressure of 10$\;$bar, there will be
                      approx. 0.160$\;$kg of Ne, or alternatively 0.300$\;$kg of
                      Ar. The energy threshold foreseen is well below 0.4~keVee
                      and the expected background level is better than 10 counts
                      keV$^{-1}$kg$^{-1}$d$^{-1}$, and could give competitive
                      results in the search for low-mass WIMPs. The experiment has
                      recently been approved by the Laboratorio Subterráneo de
                      Canfranc and is expected to be commissioned by the end of
                      the current year. We report on the status of the project.},
      month         = {May},
      date          = {2017-05-15},
      organization  = {13th Patras Workshop on Axions, WIMPs
                       and WISPs, Thessaloniki (Greece), 15
                       May 2017 - 19 May 2017},
      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-2017-02/dafni_theopisti},
      url          = {https://bib-pubdb1.desy.de/record/402226},
}