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@INPROCEEDINGS{Knirck:395482,
      author       = {Knirck, Stefan and Jaeckel, Joerg},
      title        = {{D}ish {A}ntenna {S}earches for {WISP}y {D}ark {M}atter:
                      {D}irectional {R}esolution {S}mall {M}ass {L}imitations},
      address      = {Hamburg},
      publisher    = {Verlag Deutsches Elektronen-Synchrotron},
      reportid     = {PUBDB-2017-12147, DESY-PROC-2016-03},
      isbn         = {978-3-945931-06-6},
      series       = {DESY-PROC},
      pages        = {78-81},
      year         = {2017},
      comment      = {Knirck, Stefan "Dish Antenna Searches for WISPy Dark
                      Matter: Directional Resolution Small Mass Limitations" 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     = {Knirck, Stefan "Dish Antenna Searches
                       for WISPy Dark Matter: Directional
                       Resolution Small Mass Limitations" 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     = {Hidden photon and axion-like dark matter may be detected
                      using spherical reflective surfaces such as dish antenna
                      setups converting some of the dark matter particles into
                      photons and concentrating them on a detector. These setups
                      may be used to perform directional searches measuring the
                      dark matter momentum distribution. We briefly review the
                      photon distribution one expects to detect with such an
                      antenna and directional resolution in ray approximation.
                      Furthermore we consider the regime $m_{DM} \lesssim
                      (R_{sp}\,v_{DM})^{-1}$ where this approximation does not
                      hold anymore due to photon wavelengths exceeding the
                      expected distribution widths. We discuss how this affects
                      the expected distributions and experimental implications.},
      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/Knirck_Stefan},
      url          = {https://bib-pubdb1.desy.de/record/395482},
}