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@INPROCEEDINGS{Cantatore:316753,
      author       = {Cantatore, G. and Gardikiotis, A. and Hoffmann, D. H. H.
                      and Karuza, M. and Semertzidis, Y. K. and Zioutas, K.},
      title        = {{R}ecent {P}rogress with the {KWISP} {F}orce {S}ensor},
      address      = {Hamburg},
      publisher    = {Verlag Deutsches Elektronen-Synchrotron},
      reportid     = {PUBDB-2017-00151},
      isbn         = {978-3-935702-43-0},
      series       = {DESY-PROC},
      pages        = {153-156},
      year         = {2015},
      comment      = {Cantatore, G. "Recent Progress with the KWISP Force Sensor"
                      in Proceedings, 11th Patras Workshop on Axions, WIMPs and
                      WISPs (Axion-WIMP 2015) / Irastorza, Igor G., Redondo,
                      Javier, Carmona, José Manuel, Cebrian, Susana, Dafni,
                      Theopisti, Iguaz, Francisco J., Luzon, Gloria (eds.), Verlag
                      Deutsches Elektronen-Synchrotron : 2015 ; AXION-WIMP 2015 :
                      11th Patras Workshop on Axions, WIMPs and WISPs, 2015-06-22
                      - 2015-06-26, Zaragoza},
      booktitle     = {Cantatore, G. "Recent Progress with
                       the KWISP Force Sensor" in Proceedings,
                       11th Patras Workshop on Axions, WIMPs
                       and WISPs (Axion-WIMP 2015) /
                       Irastorza, Igor G., Redondo, Javier,
                       Carmona, José Manuel, Cebrian, Susana,
                       Dafni, Theopisti, Iguaz, Francisco J.,
                       Luzon, Gloria (eds.), Verlag Deutsches
                       Elektronen-Synchrotron : 2015 ;
                       AXION-WIMP 2015 : 11th Patras Workshop
                       on Axions, WIMPs and WISPs, 2015-06-22
                       - 2015-06-26, Zaragoza},
      abstract     = {The KWISP opto-mechanical force sensor has been built and
                      calibrated in the INFN Trieste optics laboratory and is now
                      under off-beam commissioning at CAST. It is designed to
                      detect the pressure exerted by a flux of solar Chameleons on
                      a thin (100 nm) Si$_3$N$_4$ micromembrane thanks to their
                      direct coupling to matter. A thermally-limited force
                      sensitivity of $1.5 \cdot
                      10^{-14}~\mbox{N}/\sqrt{\mbox{Hz}}$, corresponding to $7.5
                      \cdot 10^{-16}~\mbox{m}/\sqrt{\mbox{Hz}}$ in terms of
                      displacement, has been obtained. An originally developed
                      prototype chameleon chopper has been used in combination
                      with the KWISP force sensor to conduct preliminary searches
                      for solar chamaleons.},
      month         = {Jun},
      date          = {2015-06-22},
      organization  = {11th Patras Workshop on Axions, WIMPs
                       and WISPs, Zaragoza (Spain), 22 Jun
                       2015 - 26 Jun 2015},
      typ          = {PUB:(DE-HGF)8 / PUB:(DE-HGF)7},
      doi          = {10.3204/DESY-PROC-2015-02/cantatore_giovanni},
      url          = {https://bib-pubdb1.desy.de/record/316753},
}