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@INPROCEEDINGS{McAllister:395490,
      author       = {McAllister, Ben T. and Parker, Stephen R. and Ivanov,
                      Eugene N. and Tobar, Michael E.},
      title        = {{H}igh and low mass {A}xion {H}aloscopes at {UWA}},
      address      = {Hamburg},
      publisher    = {Verlag Deutsches Elektronen-Synchrotron},
      reportid     = {PUBDB-2017-12155, DESY-PROC-2016-03},
      isbn         = {978-3-945931-06-6},
      series       = {DESY-PROC},
      pages        = {116-120},
      year         = {2017},
      comment      = {McAllister, Ben T. "High and low mass Axion Haloscopes at
                      UWA" 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     = {McAllister, Ben T. "High and low mass
                       Axion Haloscopes at UWA" 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     = {We consider the design of a haloscope experiment (ORGAN) to
                      probe for axions at 26.6 GHz. The motivation for this search
                      is to perform the first direct test of a result which claims
                      a possible axion signal at this frequency. There are many
                      technical issues and optimisations that must be considered
                      in the design of a high mass axion haloscope. We discuss the
                      current status of the ORGAN experiment, as well as its
                      future. We also discuss low mass axion haloscopes employing
                      lumped 3D LC resonators.},
      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/McAllister_Ben},
      url          = {https://bib-pubdb1.desy.de/record/395490},
}