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@INPROCEEDINGS{Lewis:395484,
      author       = {Lewis, Samantha M.},
      collaboration = {ADMX-{HF Collaboration}},
      title        = {{S}tatus of the {ADMX}-{HF} {E}xperiment},
      address      = {Hamburg},
      publisher    = {Verlag Deutsches Elektronen-Synchrotron},
      reportid     = {PUBDB-2017-12149, DESY-PROC-2016-03},
      isbn         = {978-3-945931-06-6},
      series       = {DESY-PROC},
      pages        = {86-89},
      year         = {2017},
      comment      = {Lewis, Samantha M. "Status of the ADMX-HF Experiment" 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     = {Lewis, Samantha M. "Status of the
                       ADMX-HF Experiment" 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 axion is a leading dark matter candidate particle.
                      Haloscope-type experiments search for the axion using its
                      resonant conversion to a photon in the presence of a strong
                      magnetic field, enhancing the signal through the use of
                      resonant microwave cavities and quantum-limited amplifiers.
                      The Axion Dark Matter eXperiment -- High Frequency (ADMX-HF)
                      is an operating experiment taking a first look at data in
                      the 20--100 $\mu$eV ($\sim$~4--25 GHz) range. This paper
                      discusses the newly completed data run as well as research
                      and development underway that will further the reach of the
                      experiment.},
      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/Lewis_Samantha},
      url          = {https://bib-pubdb1.desy.de/record/395484},
}