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@INPROCEEDINGS{DreylingEschweiler:315505,
      author       = {Dreyling-Eschweiler, Jan},
      collaboration = {ALPS-{II Collaboration}},
      title        = {{F}irst sensitivity limits of the {ALPS} {TES} detector},
      address      = {Hamburg},
      publisher    = {Verlag Deutsches Elektronen-Synchrotron},
      reportid     = {PUBDB-2016-05912, DESY-14-165. arXiv:1409.6992.
                      DESY-14-165},
      isbn         = {978-3-935702-59-1},
      series       = {DESY-PROC},
      pages        = {63-66},
      year         = {2014},
      note         = {4 pages, 1 figure; proceedings of 10th Patras Workshop on
                      Axions, WIMPs, and WISPs, Geneva, CERN, 29 June to 4 July
                      2014},
      comment      = {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     = {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     = {The Any Light Particle Search II (ALPS II) requires a
                      sensitive detection of 1064~nm photons. Thus, a low dark
                      count rate ($DC$) and a high detection efficiency ($DE$) is
                      needed. ALPS has set up a transition-edge sensor (TES)
                      detector system, namely the ALPS TES detector. It is found
                      that thermal photons from room temperature surfaces are the
                      main contribution of dark counts for 1064~nm photon signals.
                      Furthermore, the current setup of the ALPS TES detector
                      shows an improvement compared to using the ALPS I detector.},
      month         = {Jun},
      date          = {2014-06-29},
      organization  = {10th Patras Workshop on Axions, WIMPs
                       and WISPs, Geneva (Switzerland), 29 Jun
                       2014 - 4 Jul 2014},
      keywords     = {photon: thermal (INSPIRE) / temperature: surface (INSPIRE)
                      / ALPS (INSPIRE) / sensitivity (INSPIRE) / efficiency
                      (INSPIRE) / photon: detector (INSPIRE) / detector:
                      superconductivity (INSPIRE)},
      cin          = {ATLAS},
      cid          = {I:(DE-H253)ATLAS-20120731},
      pnm          = {514 - Theoretical Particle Physics (POF2-514)},
      pid          = {G:(DE-HGF)POF2-514},
      experiment   = {EXP:(DE-H253)ALPS-20150101},
      typ          = {PUB:(DE-HGF)8 / PUB:(DE-HGF)7},
      eprint       = {1409.6992},
      howpublished = {arXiv:1409.6992},
      archivePrefix = {arXiv},
      SLACcitation = {$\%\%CITATION$ = $arXiv:1409.6992;\%\%$},
      doi          = {10.3204/DESY-PROC-2014-03/dreyling-eschweiler_jan},
      url          = {https://bib-pubdb1.desy.de/record/315505},
}