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@INPROCEEDINGS{Saleev:335254,
      author       = {Saleev, Artem and Pretz, Joerg and Shmakova, Vera and
                      Lenisa, Paolo and Rathmann, Frank},
      title        = {{S}pin {T}une {R}esponse to {V}ertical {O}rbit {C}orrection
                      at {COSY}},
      volume       = {37},
      publisher    = {Journal of the Physical Society of Japan},
      reportid     = {GSI-2023-00380},
      pages        = {020702},
      year         = {2022},
      note         = {"This article is published by the Physical Society of Japan
                      under the terms of the Creative Commons Attribution 4.0
                      License. Any further distribution of this work must maintain
                      attribution to the author(s) and the title of the article,
                      journal citation, and DOI."},
      comment      = {Proceedings of the 24th International Spin Symposium
                      (SPIN2021) - Journal of the Physical Society of Japan, 2022.
                      - ISBN 4-89027-150-3 - doi:10.7566/JPSCP.37.020702},
      booktitle     = {Proceedings of the 24th International
                       Spin Symposium (SPIN2021) - Journal of
                       the Physical Society of Japan, 2022. -
                       ISBN 4-89027-150-3 -
                       doi:10.7566/JPSCP.37.020702},
      abstract     = {Searches of electric dipole moments (EDM) of charged
                      particles in pure magnetic rings, such as COSY, or
                      electrostatic and hybrid magnetic-electric storage rings,
                      planned in the future, require new methods to disentangle
                      the EDM signal from the large background produced by
                      magnetic dipole moments. In these experiments, the sources
                      of systematic background are in-plane magnetic fields. It is
                      important to distinguish the origins of the in-plane
                      magnetic fields, which could be produced intentionally by
                      vertical orbit correction to keep the beam on a closed path,
                      or unintentionally due to the alignment errors of the
                      magnets. We propose to use the method of spin tune mapping
                      to determine the relative importance of those two origins.
                      At the first stage, the model of COSY should be verified for
                      the spin tune shifts when vertical three-steerer
                      closed-orbit bumps are applied. At the second stage, the
                      spin tune response to vertical orbit correction in the arcs
                      will testify its contribution to the systematic background.},
      month         = {Oct},
      date          = {2021-10-18},
      organization  = {Proceedings of the 24th International
                       Spin Symposium (SPIN2021), Matsue
                       (Japan (Hybrid)), 18 Oct 2021 - 22 Oct
                       2021},
      cin          = {FFN},
      cid          = {I:(DE-Ds200)FFN-20210302OR452},
      pnm          = {899 - ohne Topic (POF4-899)},
      pid          = {G:(DE-HGF)POF4-899},
      experiment   = {$EXP:(DE-Ds200)External_experiment-20200803$},
      typ          = {PUB:(DE-HGF)8 / PUB:(DE-HGF)7},
      doi          = {10.7566/JPSCP.37.020702},
      url          = {https://repository.gsi.de/record/335254},
}